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description Publicationkeyboard_double_arrow_right Article , Review , Other literature type 2021 Italy, Belgium, Italy, Switzerland, Italy, Italy, Italy, Italy, Italy, Italy, Italy, Italy, Italy, Italy, Italy, Italy, Italy, Italy, Italy, Italy, Italy, Belgium, Italy, Italy, Italy, Italy, Italy, France, Italy, Italy, ItalyPublisher:Taylor & Francis Klionsky D. J.; Abdel-Aziz A. K.; Abdelfatah S.; Abdellatif M.; Abdoli A.; Abel S.; Abeliovich H.; Abildgaard M. H.; Abudu Y. P.; Acevedo-Arozena A.; Adamopoulos I. E.; Adeli K.; Adolph T. E.; Adornetto A.; Aflaki E.; Agam G.; Agarwal A.; Aggarwal B. B.; Agnello M.; Agostinis P.; Agrewala J. N.; Agrotis A.; Aguilar P. V.; Ahmad S. T.; Ahmed Z. M.; Ahumada-Castro U.; Aits S.; Aizawa S.; Akkoc Y.; Akoumianaki T.; Akpinar H. A.; Al-Abd A. M.; Al-Akra L.; Al-Gharaibeh A.; Alaoui-Jamali M. A.; Alberti S.; Alcocer-Gomez E.; Alessandri C.; Ali M.; Alim Al-Bari M. A.; Aliwaini S.; Alizadeh J.; Almacellas E.; Almasan A.; Alonso A.; Alonso G. D.; Altan-Bonnet N.; Altieri D. C.; Alvarez E. M. C.; Alves S.; Alves da Costa C.; Alzaharna M. M.; Amadio M.; Amantini C.; Amaral C.; Ambrosio S.; Amer A. O.; Ammanathan V.; An Z.; Andersen S. U.; Andrabi S. A.; Andrade-Silva M.; Andres A. M.; Angelini S.; Ann D.; Anozie U. C.; Ansari M. Y.; Antas P.; Antebi A.; Anton Z.; Anwar T.; Apetoh L.; Apostolova N.; Araki T.; Araki Y.; Arasaki K.; Araujo W. L.; Araya J.; Arden C.; Arevalo M. -A.; Arguelles S.; Arias E.; Arikkath J.; Arimoto H.; Ariosa A. R.; Armstrong-James D.; Arnaune-Pelloquin L.; Aroca A.; Arroyo D. S.; Arsov I.; Artero R.; Asaro D. M. L.; Aschner M.; Ashrafizadeh M.; Ashur-Fabian O.; Atanasov A. G.; Au A. K.; Auberger P.; Auner H. W.; Aurelian L.; Autelli R.; Avagliano L.; Avalos Y.; Aveic S.; Aveleira C. A.; Avin-Wittenberg T.; Aydin Y.; Ayton S.; Ayyadevara S.; Azzopardi M.; Baba M.; Backer J. M.; Backues S. K.; Bae D. -H.; Bae O. -N.; Bae S. H.; Baehrecke E. H.; Baek A.; Baek S. -H.; Baek S. H.; Bagetta G.; Bagniewska-Zadworna A.; Bai H.; Bai J.; Bai X.; Bai Y.; Bairagi N.; Baksi S.; Balbi T.; Baldari C. T.; Balduini W.; Ballabio A.; Ballester M.; Balazadeh S.; Balzan R.; Bandopadhyay R.; Banerjee S.; Banerjee S.; Banreti A.; Bao Y.; Baptista M. S.; Baracca A.; Barbati C.; Bargiela A.; Barila D.; Barlow P. G.; Barmada S. J.; Barreiro E.; Barreto G. E.; Bartek J.; Bartel B.; Bartolome A.; Barve G. R.; Basagoudanavar S. H.; Bassham D. C.; Bast R. C.; Basu A.; Batoko H.; Batten I.; Baulieu E. E.; Baumgarner B. L.; Bayry J.; Beale R.; Beau I.; Beaumatin F.; Bechara L. R. G.; Beck G. R.; Beers M. F.; Begun J.; Behrends C.; Behrens G. M. N.; Bei R.; Bejarano E.; Bel S.; Behl C.; Belaid A.; Belgareh-Touze N.; Bellarosa C.; Belleudi F.; Bello Perez M.; Bello-Morales R.; Beltran J. S. D. O.; Beltran S.; Benbrook D. M.; Bendorius M.; Benitez B. A.; Benito-Cuesta I.; Bensalem J.; Berchtold M. W.; Berezowska S.; Bergamaschi D.; Bergami M.; Bergmann A.; Berliocchi L.; Berlioz-Torrent C.; Bernard A.; Berthoux L.; Besirli C. G.; Besteiro S.; Betin V. M.; Bezbradica J. S.; Biden T. J.; Boeuf P.; Boland B.; Bomont P.; Bonaldo P.; Bonam S. R.; Bornhauser B. C.; Bourke N. M.; Bozhkov P. V.; Bozkurt T. O.; Bronson P. G.; Brown C. N.; Bruno D.; Budak H.; Bultynck G.; Burgoyne J. R.; Cadwell K.; Call J. A.; Calvani R.; Calvo-Rubio Barrera M.; Camara N. O. S.; Canti C.; Carames B.; Cardoso S. M.; Carle G. F.; Carloni S.; Casas C.; Castillo-Lluva S.; Cavadas C.; Cechowska-Pasko M.; Cerutti J. M.; Chamilos G.; Chan D. W.; Chan E. Y. W.; Charlet-Berguerand N.; Chauhan S.; Checler F.; Cheetham M. E.; Chen L. L.; Chen L.; Chen L.; Chen M.; Chen W.; Cherry S.; Cheung C. F. R.; Chevet E.; Chi R. J.; Chiaradonna F.; Chiariello M.; Chua J. P.; Ciechomska I. A.; Cinque L.; Clarke R.; Codogno P.; Colasanti T.; Colell A.; Collins M. O.; Costelli P.; Csizmadia T.; Cui B.; Cui J.; Cumino A. C.; da Silva J. A.; Dafsari H. S.; Dalla Valle L.; Dallenga T.; Das H.; Dasari S. K.; Dauphinee A. N.; De Meyer G. R. Y.; De Nunzio C.; De Palma C.; De Virgilio C.; De Zio D.; Dehay B.; Dengjel J.; Devuyst O.; di Bernardo D.; Di Cristina M.; Di Domenico F.; Di Fazio P.; Diao J.; Dickinson J. M.; Diederich M.; Dieude M.; Dinic J.; Dinkova-Kostova A. T.; Dong B.; Dong X.; Dowaidar M.; Du A.; Du C.; Efferth T.; Ejarque M.; El-Naggar S.; Engelsen A. S. T.; Fang E. F.; Fang Y.; Filadi R.; Filigheddu N.; Fimia G. M.; Fineschi V.; Finetti F.; Fisher E. A.; Florey O.; Follo C.; Fortini P.; Fulda S.; Furic L.; Garcia-Del Portillo F.; Garcia-Garcia A.; Garofalo T.; Ghavami S.; Ghigo A.; Gluschko A.; Goder V.; Golab J.; Golebiewska A.; Gomez R.; Gonzalez-Hernandez T.; Gorojod R. M.; Gregory S. L.; Guerri C.; Gunst J.; Guo C.; Guo C.; Gupta P.; Gupta S. K.; Hamacher-Brady A.; Haucke V.; He R. -R.; Herb M.; Hernandez A.; Hernandez C.; Hernandez-Diaz S.; Hilfiker S.; Ho E. A.; Hoet P. H. M.; Huang C.; Hummer G.; Ikeda F.; Imbriano C.; Inman D. M.; Itakura E.; Jacquin E.; Jakobsson J.; Jessen N.; Jimenez-Sanchez M.; Joffre C.; Judith D.; Jung C. H.; Jungbluth H.; Kalia M.; Kaludercic N.; Kalvari I.; Kang C.; Kaniyappan S.; Karmakar P.; Kho W.; Kimchi A.; Kimura T.; Kjaerulff O.; Koch I.; Korkmaz G.; Kou Y.; Krasnodembskaya A. D.; Kuenen S.; Kukar T.; Kumar A.; Ladoire S.; Lafont F.; Laird A. S.; Langer R.; Lee C.; Lee E. B.; Lee E. F.; Lee G. M.; Lefebvre C.; Lenoir O.; Letellier E.; Leung P. S.; Lewis P. A.; Li B.; Li J.; Liang C.; Lindner P.; Liu C.; LLeonart M. E.; Lo C. H.; Lossi L.; Luftig M. A.; Lund A. H.; Lund V. K.; Luu L.; Lyakhovich A.; MacIntosh G. C.; Madeo F.; Madrigal-Matute J.; Maiani E.; Marchetti S.; Mardente S.; Marinelli S.; Martin-Rincon M.; Martinez A.; Martins D. O.; Martins J. O.; Marzetti E.; Mashek D. G.; Masuelli L.; Mattar P.; Maycotte P.; McKenna S. L.; Meng D.; Mercier A. E.; Merighi A.; Meyer C.; Micale L.; Milczarek M.; Mirzaei H.; Misasi R.; Mogensen T. H.; Mollereau B.; Montagna C.; Morishita H.; Morleo M.; Morselli E.; Motori E.; Mukherjee A.; Nandi S. S.; Nanni M.; Nassif M.; Naveiras O.; Nazarko T. Y.; Nazio F.; Neisch A. L.; Neutzner A.; Ni Cheallaigh C.; Noda T.; Novoa B.; Nylandsted J.; Ogier-Denis E.; Oikonomou V.; Olivan S.; Oliveira J. M. A.; Olzmann J. A.; Onnis A.; Ortiz-Gonzalez X. R.; Pahari S.; Palmisano G.; Panasyuk G.; Pandya V.; Paneni F.; Papademetrio D. L.; Papp D.; Park E. C.; Passos J. F.; Pedrozo Z.; Pei G.; Pellegrini J. M.; Pelletier J.; Penna F.; Pennuto M.; Pfirrmann T.; Pierre P.; Pierrefite-Carle V.; Pierzynowska K.; Pietruczuk M.; Pinar M.; Pircs K.; Pizzo P.; Pocock R.; Poletti A.; Popova B.; Prahlad V.; Proikas-Cezanne T.; Puyal J.; Raimundo N.; Ramachandra Rao S.; Rao H.; Reggiori F.; Reigada D.; Renga G.; Richardson D. R.; Rizza S.; Rizzuto R.; Robinson K. J.; Rocchi S.; Romanello V.; Romano A.; Rosenfeldt M. T.; Roussel B. D.; Rozieres A.; Rudolf E.; Sachse C.; Salekdeh G. H.; Sanchez-Vera V.; Sandri M.; Sargeant T. J.; Sarkar C.; Sarkar S.; Sathyanarayanan R.; Schapira A. H. V.; Scharl M.; Schiaffino M. V.; Schmitz I.; Schwamborn J. C.; Schwarten M.; Sciarretta S.; Scott M. J.; Sebastian D.; Sebti S.; Serra-Moreno R.; Shah J. A.; Sharkey L. M.; Shen H.; Shimozawa M.; Shoji I.; Shukla A. K.; Shutt T. E.; Sirko A.; Sirohi K.; Skendros P.; Somarelli J. A.; Staiano L.; Stalnecker C. A.; Stankov M. V.; Stefan K.; Sterneckert J.; Su H.; Sue C. M.; Sze S. C. W.; Szewczyk N. J.; Tafani M.; Takahashi Y.; Tettamanti G.; Thedieck K.; Thumm M.; Timmerman V.; Tomaipitinca L.; Tong C.; Torii S.; Torriglia A.; Ugun-Klusek A.; Uhlig H. H.; Vahsen B. F.; Valdor R.; Valverde A. M.; van Loosdregt J.; van Wijk S. J. L.; Vanhorebeek I.; Varga M.; Verdier M.; Vervliet T.; Vervoorts J.; Victor V. M.; Vigano S.; Villalobo A.; Vincent O.; Voitsekhovskaja O. V.; Wandosell F. G.; Wang B.; Wang C.; Wang C.; Wang C.; Wang D.; Watchon M.; Wei H.; Weiskirchen R.; Weykopf B.; Woehlbier U.; Xia H.; Xiao B.; Yang C.; Yang H.; Yao H.; Yu B.; Yuan J.; Yue J.; Zambelli V. O.; Zanella I.; Zang Q. S.; Zanivan S.; Zhang M.; Zheng G.; Zhong Q.; Zhou A.; Zhou B.; Zhu B.; Ziviani E.; Zoladek T.; Zou W.; Zuryn S.;doi: 10.48350/155081
handle: 11379/542024 , 11392/2442540 , 11564/765957 , 11591/444669 , 2318/1785276 , 11587/453716 , 11391/1490255 , 11568/1104102 , 10807/173406 , 21.11116/0000-000D-4E66-A , 21.11116/0000-000D-4E68-8 , 2434/844005 , 10067/1756630151162165141 , 11590/385750 , 11380/1244073 , 11383/2112326 , 11588/855085 , 11577/3390116 , 11581/450344 , 11388/248298 , 11576/2685604 , 11573/1688011 , 20.500.11770/313778 , 11562/1037826
pmid: 33634751
pmc: PMC7996087
doi: 10.48350/155081
handle: 11379/542024 , 11392/2442540 , 11564/765957 , 11591/444669 , 2318/1785276 , 11587/453716 , 11391/1490255 , 11568/1104102 , 10807/173406 , 21.11116/0000-000D-4E66-A , 21.11116/0000-000D-4E68-8 , 2434/844005 , 10067/1756630151162165141 , 11590/385750 , 11380/1244073 , 11383/2112326 , 11588/855085 , 11577/3390116 , 11581/450344 , 11388/248298 , 11576/2685604 , 11573/1688011 , 20.500.11770/313778 , 11562/1037826
pmid: 33634751
pmc: PMC7996087
In 2008, we published the first set of guidelines for standardizing research in autophagy. Since then, this topic has received increasing attention, and many scientists have entered the field. Our knowledge base and relevant new technologies have also been expanding. Thus, it is important to formulate on a regular basis updated guidelines for monitoring autophagy in different organisms. Despite numerous reviews, there continues to be confusion regarding acceptable methods to evaluate autophagy, especially in multicellular eukaryotes. Here, we present a set of guidelines for investigators to select and interpret methods to examine autophagy and related processes, and for reviewers to provide realistic and reasonable critiques of reports that are focused on these processes. These guidelines are not meant to be a dogmatic set of rules, because the appropriateness of any assay largely depends on the question being asked and the system being used. Moreover, no individual assay is perfect for every situation, calling for the use of multiple techniques to properly monitor autophagy in each experimental setting. Finally, several core components of the autophagy machinery have been implicated in distinct autophagic processes (canonical and noncanonical autophagy), implying that genetic approaches to block autophagy should rely on targeting two or more autophagy-related genes that ideally participate in distinct steps of the pathway. Along similar lines, because multiple proteins involved in autophagy also regulate other cellular pathways including apoptosis, not all of them can be used as a specific marker for bona fide autophagic responses. Here, we critically discuss current methods of assessing autophagy and the information they can, or cannot, provide. Our ultimate goal is to encourage intellectual and technical innovation in the field. doi: 10.1080/15548627.2020.1797280 ispartof: Autophagy vol:17 issue:1 pages:1-382 ispartof: location:United States status: published
BOA - Bicocca Open A... arrow_drop_down Archivio della Ricerca - Università di PisaArticle . 2021Data sources: Archivio della Ricerca - Università di PisaArchivio Istituzionale (AperTO)Article . 2021Full-Text: https://iris.unito.it/bitstream/2318/1785276/1/Klionsky%20et%20al_Guidelines_2020_Post-print.docxData sources: Archivio Istituzionale (AperTO)Recolector de Ciencia Abierta, RECOLECTAReview . 2021Data sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAReview . 2021Data sources: Recolector de Ciencia Abierta, RECOLECTAIRIS - Università degli Studi di VeronaArticle . 2021Data sources: IRIS - Università degli Studi di VeronaArchivio della ricerca- Università di Roma La SapienzaArticle . 2021Data sources: Archivio della ricerca- Università di Roma La SapienzaArchiMer - Institutional Archive of IfremerOther literature type . 2021Data sources: ArchiMer - Institutional Archive of IfremerArchivio della Ricerca - Università di PisaArticle . 2021Data sources: Archivio della Ricerca - Università di PisaRecolector de Ciencia Abierta, RECOLECTAReview . 2021Data sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAReview . Article . 2021Data sources: Recolector de Ciencia Abierta, RECOLECTAInfoscience - EPFL scientific publicationsOther literature typeData sources: Infoscience - EPFL scientific publicationsHAL-Inserm; Hal-DiderotArticle . 2021IRIS - Università degli Studi di VeronaArticle . 2021Data sources: IRIS - Università degli Studi di VeronaArchivio della ricerca- Università di Roma La SapienzaArticle . 2021Data sources: Archivio della ricerca- Università di Roma La SapienzaArchivio Istituzionale dell'Università della CalabriaArticle . 2021Data sources: Archivio Istituzionale dell'Università della Calabriaadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.48350/155081&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eu613 citations 613 popularity Top 0.01% influence Top 1% impulse Top 0.01% Powered by BIP!more_vert BOA - Bicocca Open A... arrow_drop_down Archivio della Ricerca - Università di PisaArticle . 2021Data sources: Archivio della Ricerca - Università di PisaArchivio Istituzionale (AperTO)Article . 2021Full-Text: https://iris.unito.it/bitstream/2318/1785276/1/Klionsky%20et%20al_Guidelines_2020_Post-print.docxData sources: Archivio Istituzionale (AperTO)Recolector de Ciencia Abierta, RECOLECTAReview . 2021Data sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAReview . 2021Data sources: Recolector de Ciencia Abierta, RECOLECTAIRIS - Università degli Studi di VeronaArticle . 2021Data sources: IRIS - Università degli Studi di VeronaArchivio della ricerca- Università di Roma La SapienzaArticle . 2021Data sources: Archivio della ricerca- Università di Roma La SapienzaArchiMer - Institutional Archive of IfremerOther literature type . 2021Data sources: ArchiMer - Institutional Archive of IfremerArchivio della Ricerca - Università di PisaArticle . 2021Data sources: Archivio della Ricerca - Università di PisaRecolector de Ciencia Abierta, RECOLECTAReview . 2021Data sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAReview . Article . 2021Data sources: Recolector de Ciencia Abierta, RECOLECTAInfoscience - EPFL scientific publicationsOther literature typeData sources: Infoscience - EPFL scientific publicationsHAL-Inserm; Hal-DiderotArticle . 2021IRIS - Università degli Studi di VeronaArticle . 2021Data sources: IRIS - Università degli Studi di VeronaArchivio della ricerca- Università di Roma La SapienzaArticle . 2021Data sources: Archivio della ricerca- Università di Roma La SapienzaArchivio Istituzionale dell'Università della CalabriaArticle . 2021Data sources: Archivio Istituzionale dell'Università della Calabriaadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.48350/155081&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2020 FrancePublisher:EDP Sciences Funded by:ANR | Amidex, ANR | OCEVU, EC | CONCERTOANR| Amidex ,ANR| OCEVU ,EC| CONCERTOLagache, G.; Béthermin, M.; Montier, L.; Serra, P.; Tucci, M.;One of the main goals of Cosmology is to search for the imprint of primordial gravitational waves in the CMB polarisation field, to probe inflationary theories. One of the obstacles toward the detection of the primordial signal is to extract the B-mode polarisation from astrophysical contaminations. We present a complete analysis of extragalactic foreground contamination due to polarised emission of radio and dusty star-forming galaxies. We update or use up-to-date models that are validated using the most recent measurements. We predict the flux limit (confusion noise) for the future CMB space or balloon experiments (IDS, PIPER, SPIDER, LiteBIRD, PICO), as well as ground-based experiments (C-BASS, NEXT-BASS, QUIJOTE, AdvACTPOL, BICEP3+Keck, BICEPArray, CLASS, SO, SPT3G, S4). Telescope aperture size (and frequency) is the main characteristic impacting the level of confusion noise. Using the flux limits and assuming constant polarisation fractions for radio and dusty galaxies, we compute the B-mode power spectra of the three extragalactic foregrounds (radio source shot noise, dusty galaxy shot noise and clustering), discuss their relative levels and compare their amplitudes to that of the primordial tensor modes parametrized by the tensor-to-scalar ratio r. At the reionization bump (l=5), contamination by extragalactic foregrounds is negligible. At the recombination peak (l=80), while the contamination is much lower than the targeted sensitivity on r for large-aperture telescopes, it is at comparable level for some of the medium- and small-aperture telescope experiments. For example, the contamination is at the level of the 68 per cent confidence level uncertainty on the primordial r for the LiteBIRD and PICO space experiments. Finally we also provide some useful unit conversion factors and give some predictions for the SPICA B-BOP experiment. Abridged Comment: A&A in press. Match published version
Astronomy and Astrop... arrow_drop_down https://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: DataciteHAL - UPEC / UPEM; HAL-Pasteur; HAL-InsermPreprint . 2019add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1051/0004-6361/201937147&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 20 citations 20 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert Astronomy and Astrop... arrow_drop_down https://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: DataciteHAL - UPEC / UPEM; HAL-Pasteur; HAL-InsermPreprint . 2019add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1051/0004-6361/201937147&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2020 FrancePublisher:MDPI AG Funded by:EC | GlassRoutesEC| GlassRoutesAuthors: Nadine Schibille; Cristina Boschetti; Miguel Ángel Valero Tévar; Emmanuel Veron; +1 AuthorsNadine Schibille; Cristina Boschetti; Miguel Ángel Valero Tévar; Emmanuel Veron; Jorge de Juan Ares;doi: 10.3390/min10030272
International audience; Excavations at the Roman villa of Noheda (Spain) revealed the remains of an exceptionally elaborate fourth-century floor mosaic that contains a surprisingly large number of glass tesserae, representing a broad spectrum of colors. This paper presents the results of the chemical (LA-ICP-MS) and microstructural analyses (SEM-EDS, XRPD) of 420 glass tesserae from these mosaics. The high number of data allowed us to establish the compositional variability and to elucidate questions of supply in relation to a large-scale artistic campaign. The tesserae from Noheda were almost exclusively made from recycled mixed Roman Mn and Sb base glass, thus demonstrating that recycling of Roman base glasses was common practice in the fourth century, occurring on a near industrial scale. It also suggests that the workshops specializing in the production of mosaic tesserae might have been in the western Mediterranean. A limited number of coloring and opacifying additives (Mn, Co, Cu, Sb, Pb) were identified, which resulted in a wide range of hues. These were differentially associated with various trace elements, which implies the use of different raw materials. A subset of red, green, and orange tesserae reflect distinct base glass characteristics as well as coloring technologies that point to an Egyptian provenance.
Minerals arrow_drop_down MineralsOther literature type . Article . 2020 . Peer-reviewedLicense: CC BYFull-Text: https://www.mdpi.com/2075-163X/10/3/272/pdfMémoires en Sciences de l'Information et de la CommunicationArticle . 2020Full-Text: https://hal.science/hal-02511142/documentadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3390/min10030272&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesgold 18 citations 18 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert Minerals arrow_drop_down MineralsOther literature type . Article . 2020 . Peer-reviewedLicense: CC BYFull-Text: https://www.mdpi.com/2075-163X/10/3/272/pdfMémoires en Sciences de l'Information et de la CommunicationArticle . 2020Full-Text: https://hal.science/hal-02511142/documentadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3390/min10030272&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2020 FrancePublisher:American Geophysical Union (AGU) Funded by:EC | PoroFracEC| PoroFracAuthors: Thibault Duretz; René de Borst; Philippe Yamato; Laetitia Le Pourhiet;Thibault Duretz; René de Borst; Philippe Yamato; Laetitia Le Pourhiet;doi: 10.1029/2019gl086027
AbstractStrain localization is a fundamental characteristic of plate tectonics. The resulting deformation structures shape the margins of continents and the internal structure of tectonic plates. To model the occurrence of faulting, geodynamic models generally rely on frictional plasticity. Frictional plasticity is normally embedded in visco‐plastic (V‐P) or visco‐elasto‐plastic (V‐E‐P) rheologies. This poses some fundamental issues, such as the difficulty, or often inability, to obtain a converged equilibrium state and a severe grid sensitivity. Here, we study shear banding at crustal‐scale using a visco‐elasto‐viscoplastic (V‐E‐VP) model. We show that this rheology allows to accurately satisfy equilibrium, leads to shear band patterns that converge upon mesh refinement, and preserves characteristic shear band angles. Moreover, a comparison with analytic models and laboratory data reveals that V‐E‐VP rheology captures first‐order characteristics of frictional plasticity. V‐E‐VP models thus overcomes limitations of V‐P and V‐E‐P models and appears as an attractive alternative for geodynamic modeling.
CORE (RIOXX-UK Aggre... arrow_drop_down Geophysical Research LettersOther literature type . Article . 2020 . Peer-reviewedLicense: Wiley Online Library User AgreementHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2020add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1029/2019gl086027&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesbronze 12 citations 12 popularity Top 10% influence Average impulse Top 10% Powered by BIP!visibility 4visibility views 4 download downloads 53 Powered bymore_vert CORE (RIOXX-UK Aggre... arrow_drop_down Geophysical Research LettersOther literature type . Article . 2020 . Peer-reviewedLicense: Wiley Online Library User AgreementHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2020add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1029/2019gl086027&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2020 FrancePublisher:Copernicus GmbH Funded by:EC | ESCAPEEC| ESCAPET. J. Fauchez; T. J. Fauchez; T. J. Fauchez; M. Turbet; M. Turbet; E. T. Wolf; E. T. Wolf; I. Boutle; M. J. Way; M. J. Way; A. D. Del Genio; N. J. Mayne; K. Tsigaridis; K. Tsigaridis; R. K. Kopparapu; R. K. Kopparapu; J. Yang; F. Forget; A. Mandell; A. Mandell; S. D. Domagal Goldman; S. D. Domagal Goldman;Upcoming telescopes such as the James Webb Space Telescope (JWST), or the Extremely Large Telescope (ELTs), may soon be able to characterize, through transmission, emission or reflection spectroscopy, the atmospheres of rocky exoplanets orbiting nearby M dwarfs. One of the most promising candidates is the late M dwarf system TRAPPIST-1 which has seven known transiting planets for which Transit Timing Variation (TTV) measurements suggest that they are terrestrial in nature, with a possible enrichment in volatiles. Among these seven planets, TRAPPIST-1e seems to be the most promising candidate to have habitable surface conditions, receiving ~66 % of the Earth's incident radiation, and thus needing only modest greenhouse gas inventories to raise surface temperatures to allow surface liquid water to exist. TRAPPIST-1e is therefore one of the prime targets for JWST atmospheric characterization. In this context, the modeling of its potential atmosphere is an essential step prior to observation. Global Climate Models (GCMs) offer the most detailed way to simulate planetary atmospheres. However, intrinsic differences exist between GCMs which can lead to different climate prediction and thus observability of gas and/or cloud features in transmission and thermal emission spectra. Such differences should preferably be known prior to observations. In this paper we present a protocol to inter-compare planetary GCMs. Four testing cases are considered for TRAPPIST-1e but the methodology is applicable to other rocky exoplanets in the Habitable Zone. The four test cases included two land planets composed with a modern Earth and pure CO2 atmospheres, respectively, and two aqua planets with the same atmospheric compositions. Currently, there are four participating models (LMDG, ROCKE-3D, ExoCAM, UM), however this protocol is intended to let other teams participate as well. Comment: Accepted and published in Geoscientific Model Development (GMD)
Geoscientific Model ... arrow_drop_down Geoscientific Model DevelopmentOther literature type . Article . 2020 . Peer-reviewedLicense: CC BYhttps://doi.org/10.48550/arxiv...Article . 2020License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.5194/gmd-13-707-2020&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 52 citations 52 popularity Top 1% influence Average impulse Top 1% Powered by BIP!more_vert Geoscientific Model ... arrow_drop_down Geoscientific Model DevelopmentOther literature type . Article . 2020 . Peer-reviewedLicense: CC BYhttps://doi.org/10.48550/arxiv...Article . 2020License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.5194/gmd-13-707-2020&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Other literature type 2020 FrancePublisher:Elsevier BV Funded by:SNSF | SeaO2 - Past changes in S..., ARC | Discovery Early Career Re..., EC | ACCLIMATE +1 projectsSNSF| SeaO2 - Past changes in Southern Ocean overturning circulation - implications for the partitioning of carbon and oxygen between the ocean and the atmosphere ,ARC| Discovery Early Career Researcher Award - Grant ID: DE150100107 ,EC| ACCLIMATE ,UKRI| The bi-polar seesaw and CO2: Is there anything special about 'Terminal seesaw events'?Julia Gottschalk; Luke C Skinner; Samuel L Jaccard; Laurie Menviel; Christoph Nehrbass-Ahles; Claire Waelbroeck;International audience; Past millennial-scale changes in atmospheric CO2 (CO2,atm) concentrations have often been attributed to variations in the overturning timescale of the ocean that result in changes in the marine carbon inventory. Yet, there remains a paucity of proxy evidence that documents changes in marine carbon storage globally, and that links them to abrupt climate variability in the northern hemisphere associated with perturbations of the Atlantic Meridional Overturning Circulation (AMOC). The last two glacial periods were suggested to differ in the spatial extent of the AMOC and its sensitivity to perturbations. This provides an opportunity to compare the nature of marine carbon cycle-climate feedbacks between them. Here, we reconstruct variations in respired carbon storage (via oxygenation) and the AMOC “geometry” (via carbonate ion saturation) in the deep South Atlantic. We infer decreases in deep South Atlantic respired carbon levels at times of weakened AMOC and rising CO2,atm concentrations during both glacial periods. These findings suggest a consistent pattern of increased Southern Ocean convection and/or air-sea CO2 fluxes during northern-hemisphere stadials accompanying AMOC perturbations and promoting a rise in CO2,atm levels. We find that net ocean carbon loss, and hence the magnitude of CO2,atm rise, is largely determined by the stadial duration. North Atlantic climate anomalies therefore affect Southern Ocean carbon cycling in a consistent manner, through oceanic (e.g., ventilation seesaw) and/or atmospheric processes (e.g., Ekman pumping).
Quaternary Science R... arrow_drop_down HAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2020add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.quascirev.2019.106067&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesbronze 18 citations 18 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert Quaternary Science R... arrow_drop_down HAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2020add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.quascirev.2019.106067&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Other literature type 2020 France, GermanyPublisher:Elsevier BV Sepideh Esmaeilirad; Alexandra Lai; Gülcin Abbaszade; Juergen Schnelle-Kreis; Ralf Zimmermann; Gaëlle Uzu; Kaspar R. Daellenbach; Francesco Canonaco; Hossein Hassankhany; Mohammad Arhami; Urs Baltensperger; André S. H. Prévôt; James J. Schauer; Jean-Luc Jaffrezo; Vahid Hosseini; Imad El Haddad;pmid: 31835192
International audience; With over 8 million inhabitants and 4 million motor vehicles on the streets, Tehran is one of the most crowded and polluted cities in the Middle East. Frequent exceedances of national daily PM2.5 limit have been reported in this city during the last decade, yet, the chemical composition and sources of fine particles are poorly determined. In the present study, 24-hour PM2.5 samples were collected at two urban sites during two separate campaigns, a one-year period from 2014 to 2015 and another three-month period at the beginning of 2017. Concentrations of organic carbon (OC), elemental carbon (EC), inorganic ions, trace metals and specific organic molecular markers were measured by chemical analysis of filter samples. The dominant mass components were organic matter (OM), sulfate and EC. With a 20% water-soluble organic carbon (WSOC) fraction, the predominance of primary anthropogenic sources (i.e. fossil fuel combustion) was anticipated. A positive matrix factorization (PMF) analysis using the ME-2 (Multilinear Engine-2) solver was then applied to this dataset. 5 factors were identified by Marker-PMF, named as traffic exhaust (TE), biomass burning (BB), industries (Ind.), nitrate-rich and sulfate-rich. Another 4 factors were identified by Metal-PMF, including, dust, vehicles (traffic non-exhaust, TNE), industries (Ind.) and heavy fuel combustion (HFC). Traffic exhaust was the dominant source with 44.5% contribution to total quantified PM2.5 mass. Sulfate-rich (24.2%) and nitrate-rich (18.4%) factors were the next major contributing sources. Dust (4.4%) and biomass burning (6.7%) also had small contributions while the total share of all other factors was < 2%. Investigating the correlations of different factors between the two sampling sites showed that traffic emissions and biomass burning were local, whereas dust, heavy fuel combustion and industrial sources were regional. Results of this study indicate that gas- and particle-phase pollutants emitted from fossil fuel combustion (mobile and stationary) are the principal origin of both primary and secondary fine aerosols in Tehran.
Horizon / Pleins tex... arrow_drop_down Publication Server of Helmholtz Zentrum München (PuSH)Article . 2020Data sources: Publication Server of Helmholtz Zentrum München (PuSH)The Science of The Total EnvironmentArticle . 2020 . Peer-reviewedLicense: Elsevier TDMData sources: CrossrefHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2020add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.scitotenv.2019.135330&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesbronze 35 citations 35 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert Horizon / Pleins tex... arrow_drop_down Publication Server of Helmholtz Zentrum München (PuSH)Article . 2020Data sources: Publication Server of Helmholtz Zentrum München (PuSH)The Science of The Total EnvironmentArticle . 2020 . Peer-reviewedLicense: Elsevier TDMData sources: CrossrefHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2020add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.scitotenv.2019.135330&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2020 FrancePublisher:MDPI AG Funded by:NSF | GeoSoilEnviroCARS: A Nati...NSF| GeoSoilEnviroCARS: A National Resource for Earth, Planetary, Soil and Environmental Science Research at the APSZhicheng Jing; Tony Yu; Man Xu; Julien Chantel; Yanbin Wang;doi: 10.3390/min10020126
s interior. Unlike their solid counterparts, these properties of liquids pose great technical challenges to high-pressure measurements and are poorly constrained. Here we present the technical developments that have been made at the GSECARS beamline 13-ID-D of the Advanced Photon Source for the past several years for determination of sound velocity of liquids using the ultrasonic techniques in a 1000-ton Kawai-type multianvil apparatus. Temperature of the sound velocity measurements has been extended to ~2400 K at 4 GPa and ~2000 K at 8 GPa to enable studies of liquids with very high melting temperatures, such as the silicate liquids. Sound velocity and equation of state of liquids provide important constraints on the generation, presence, and transport of silicate and metallic melts in the Earth&rsquo
Minerals arrow_drop_down MineralsOther literature type . Article . 2020 . Peer-reviewedLicense: CC BYFull-Text: http://www.mdpi.com/2075-163X/10/2/126/pdfadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3390/min10020126&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesgold 11 citations 11 popularity Top 10% influence Average impulse Top 10% Powered by BIP!visibility 16visibility views 16 download downloads 68 Powered bymore_vert Minerals arrow_drop_down MineralsOther literature type . Article . 2020 . Peer-reviewedLicense: CC BYFull-Text: http://www.mdpi.com/2075-163X/10/2/126/pdfadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3390/min10020126&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Other literature type 2020 Italy, France, ItalyPublisher:Elsevier BV Funded by:EC | TRUE DEPTHS, EC | ZIPEC| TRUE DEPTHS ,EC| ZIPGilio M.[1; 2]; Scambelluri M.[1]; Agostini S.[3]; Godard M.[4]; Pettke T.[5]; Agard P.[6]; Locatelli M.[6]; Angiboust S.[7];handle: 11567/990872
International audience; The Lago Superiore Unit (LSU, Monviso Massif, Italian Western Alps) is a section of fossil oceanic lithosphere equilibrated to eclogite facies conditions (550 °C – 2.8 GPa) during Alpine subduction (45–40 Ma). It is cut by two major shear zones, namely the Intermediate (ISZ) and Lower Shear Zone (LSZ), mostly consisting of serpentinite. The lowermost, serpentine-rich, section of the Lago Superiore Unit, the Basal Serpentinite, separates the HP ophiolite domain from the underlying continental Dora-Maira Unit.Here we show that the LSZ and the Basal Serpentinite were active at different stages of the subduction and exhumation history of the complex. Most of retrograde deformation and mineral re-equilibration were localized in the LSZ. Channelized fluids percolating during this phase chemically homogenized the LSZ serpentinites, that preserved their HP mineralogy only locally; the best-preserved relicts of the eclogite-facies high pressure stage within the LSZ serpentinite are nodules of magnesite (representing former veins) and eclogite blocks. Differently, the underlying Basal Serpentinite largely escaped the exhumation-related processes and still records the prograde chemical and petrological history of the LSU serpentinite, from ocean-floor hydration to HP metamorphic conditions.The Lago Superiore Unit thus represents a snapshot of major Alpine metamorphic and shearing events, from prograde subduction to exhumation. Its km-scale thickness, and the oriented antigorite fabric in the Lower Shear Zone and Basal Serpentinite makes it a good seismic reflector. This HP ophiolite complex can thus be used as proxy of a deep (70–80 km) Alpine-type subduction zone, and to better constrain and interpret seismic images of present-day convergent margins.
Lithos arrow_drop_down Lithos; Archivio istituzionale della ricerca - Università di GenovaArticle . 2020 . Peer-reviewedLicense: Elsevier TDMadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.lithos.2019.105308&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesbronze 9 citations 9 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert Lithos arrow_drop_down Lithos; Archivio istituzionale della ricerca - Università di GenovaArticle . 2020 . Peer-reviewedLicense: Elsevier TDMadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.lithos.2019.105308&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2019 United Kingdom, Netherlands, United States, Netherlands, Netherlands, FrancePublisher:American Astronomical Society Funded by:EC | CSINEUTRONSTAREC| CSINEUTRONSTARSlavko Bogdanov; Sebastien Guillot; Paul S. Ray; Michael T. Wolff; Deepto Chakrabarty; Wynn C. G. Ho; Matthew Kerr; Frederick K. Lamb; Andrea N. Lommen; Renee M. Ludlam; Reilly Milburn; Sergio Montano; M. Coleman Miller; Michi Baubock; Feryal Özel; Dimitrios Psaltis; Ronald A. Remillard; Thomas E. Riley; James F. Steiner; Tod E. Strohmayer; Anna L. Watts; Kent S. Wood; Jesse Zeldes; Teruaki Enoto; Takashi Okajima; James W. Kellogg; Charles Baker; Craig B. Markwardt; Zaven Arzoumanian; Keith C. Gendreau;We present the set of deep Neutron Star Interior Composition Explorer (NICER) X-ray timing observations of the nearby rotation-powered millisecond pulsars PSRs J0437-4715, J0030+0451, J1231-1411, and J2124-3358, selected as targets for constraining the mass-radius relation of neutron stars and the dense matter equation of state via modeling of their pulsed thermal X-ray emission. We describe the instrument, observations, and data processing/reduction procedures, as well as the series of investigations conducted to ensure that the properties of the data sets are suitable for parameter estimation analyses to produce reliable constraints on the neutron star mass-radius relation and the dense matter equation of state. We find that the long-term timing and flux behavior and the Fourier-domain properties of the event data do not exhibit any anomalies that could adversely affect the intended measurements. From phase-selected spectroscopy, we find that emission from the individual pulse peaks is well described by a single-temperature hydrogen atmosphere spectrum, with the exception of PSR J0437-4715, for which multiple temperatures are required. Comment: 28 pages, 9 figures; accepted for publication in the Astrophysical Journal Letters
NARCIS; The Astrophy... arrow_drop_down The Astrophysical Journal LettersOther literature type . Article . 2019 . Peer-reviewedLicense: IOP Copyright Policieshttps://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: DataciteHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2019add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3847/2041-8213/ab53eb&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 108 citations 108 popularity Top 1% influence Top 10% impulse Top 1% Powered by BIP!visibility 5visibility views 5 download downloads 8 Powered bymore_vert NARCIS; The Astrophy... arrow_drop_down The Astrophysical Journal LettersOther literature type . Article . 2019 . Peer-reviewedLicense: IOP Copyright Policieshttps://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: DataciteHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2019add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3847/2041-8213/ab53eb&type=result"></script>'); --> </script>
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description Publicationkeyboard_double_arrow_right Article , Review , Other literature type 2021 Italy, Belgium, Italy, Switzerland, Italy, Italy, Italy, Italy, Italy, Italy, Italy, Italy, Italy, Italy, Italy, Italy, Italy, Italy, Italy, Italy, Italy, Belgium, Italy, Italy, Italy, Italy, Italy, France, Italy, Italy, ItalyPublisher:Taylor & Francis Klionsky D. J.; Abdel-Aziz A. K.; Abdelfatah S.; Abdellatif M.; Abdoli A.; Abel S.; Abeliovich H.; Abildgaard M. H.; Abudu Y. P.; Acevedo-Arozena A.; Adamopoulos I. E.; Adeli K.; Adolph T. E.; Adornetto A.; Aflaki E.; Agam G.; Agarwal A.; Aggarwal B. B.; Agnello M.; Agostinis P.; Agrewala J. N.; Agrotis A.; Aguilar P. V.; Ahmad S. T.; Ahmed Z. M.; Ahumada-Castro U.; Aits S.; Aizawa S.; Akkoc Y.; Akoumianaki T.; Akpinar H. A.; Al-Abd A. M.; Al-Akra L.; Al-Gharaibeh A.; Alaoui-Jamali M. A.; Alberti S.; Alcocer-Gomez E.; Alessandri C.; Ali M.; Alim Al-Bari M. A.; Aliwaini S.; Alizadeh J.; Almacellas E.; Almasan A.; Alonso A.; Alonso G. D.; Altan-Bonnet N.; Altieri D. C.; Alvarez E. M. C.; Alves S.; Alves da Costa C.; Alzaharna M. M.; Amadio M.; Amantini C.; Amaral C.; Ambrosio S.; Amer A. O.; Ammanathan V.; An Z.; Andersen S. U.; Andrabi S. A.; Andrade-Silva M.; Andres A. M.; Angelini S.; Ann D.; Anozie U. C.; Ansari M. Y.; Antas P.; Antebi A.; Anton Z.; Anwar T.; Apetoh L.; Apostolova N.; Araki T.; Araki Y.; Arasaki K.; Araujo W. L.; Araya J.; Arden C.; Arevalo M. -A.; Arguelles S.; Arias E.; Arikkath J.; Arimoto H.; Ariosa A. R.; Armstrong-James D.; Arnaune-Pelloquin L.; Aroca A.; Arroyo D. S.; Arsov I.; Artero R.; Asaro D. M. L.; Aschner M.; Ashrafizadeh M.; Ashur-Fabian O.; Atanasov A. G.; Au A. K.; Auberger P.; Auner H. W.; Aurelian L.; Autelli R.; Avagliano L.; Avalos Y.; Aveic S.; Aveleira C. A.; Avin-Wittenberg T.; Aydin Y.; Ayton S.; Ayyadevara S.; Azzopardi M.; Baba M.; Backer J. M.; Backues S. K.; Bae D. -H.; Bae O. -N.; Bae S. H.; Baehrecke E. H.; Baek A.; Baek S. -H.; Baek S. H.; Bagetta G.; Bagniewska-Zadworna A.; Bai H.; Bai J.; Bai X.; Bai Y.; Bairagi N.; Baksi S.; Balbi T.; Baldari C. T.; Balduini W.; Ballabio A.; Ballester M.; Balazadeh S.; Balzan R.; Bandopadhyay R.; Banerjee S.; Banerjee S.; Banreti A.; Bao Y.; Baptista M. S.; Baracca A.; Barbati C.; Bargiela A.; Barila D.; Barlow P. G.; Barmada S. J.; Barreiro E.; Barreto G. E.; Bartek J.; Bartel B.; Bartolome A.; Barve G. R.; Basagoudanavar S. H.; Bassham D. C.; Bast R. C.; Basu A.; Batoko H.; Batten I.; Baulieu E. E.; Baumgarner B. L.; Bayry J.; Beale R.; Beau I.; Beaumatin F.; Bechara L. R. G.; Beck G. R.; Beers M. F.; Begun J.; Behrends C.; Behrens G. M. N.; Bei R.; Bejarano E.; Bel S.; Behl C.; Belaid A.; Belgareh-Touze N.; Bellarosa C.; Belleudi F.; Bello Perez M.; Bello-Morales R.; Beltran J. S. D. O.; Beltran S.; Benbrook D. M.; Bendorius M.; Benitez B. A.; Benito-Cuesta I.; Bensalem J.; Berchtold M. W.; Berezowska S.; Bergamaschi D.; Bergami M.; Bergmann A.; Berliocchi L.; Berlioz-Torrent C.; Bernard A.; Berthoux L.; Besirli C. G.; Besteiro S.; Betin V. M.; Bezbradica J. S.; Biden T. J.; Boeuf P.; Boland B.; Bomont P.; Bonaldo P.; Bonam S. R.; Bornhauser B. C.; Bourke N. M.; Bozhkov P. V.; Bozkurt T. O.; Bronson P. G.; Brown C. N.; Bruno D.; Budak H.; Bultynck G.; Burgoyne J. R.; Cadwell K.; Call J. A.; Calvani R.; Calvo-Rubio Barrera M.; Camara N. O. S.; Canti C.; Carames B.; Cardoso S. M.; Carle G. F.; Carloni S.; Casas C.; Castillo-Lluva S.; Cavadas C.; Cechowska-Pasko M.; Cerutti J. M.; Chamilos G.; Chan D. W.; Chan E. Y. W.; Charlet-Berguerand N.; Chauhan S.; Checler F.; Cheetham M. E.; Chen L. L.; Chen L.; Chen L.; Chen M.; Chen W.; Cherry S.; Cheung C. F. R.; Chevet E.; Chi R. J.; Chiaradonna F.; Chiariello M.; Chua J. P.; Ciechomska I. A.; Cinque L.; Clarke R.; Codogno P.; Colasanti T.; Colell A.; Collins M. O.; Costelli P.; Csizmadia T.; Cui B.; Cui J.; Cumino A. C.; da Silva J. A.; Dafsari H. S.; Dalla Valle L.; Dallenga T.; Das H.; Dasari S. K.; Dauphinee A. N.; De Meyer G. R. Y.; De Nunzio C.; De Palma C.; De Virgilio C.; De Zio D.; Dehay B.; Dengjel J.; Devuyst O.; di Bernardo D.; Di Cristina M.; Di Domenico F.; Di Fazio P.; Diao J.; Dickinson J. M.; Diederich M.; Dieude M.; Dinic J.; Dinkova-Kostova A. T.; Dong B.; Dong X.; Dowaidar M.; Du A.; Du C.; Efferth T.; Ejarque M.; El-Naggar S.; Engelsen A. S. T.; Fang E. F.; Fang Y.; Filadi R.; Filigheddu N.; Fimia G. M.; Fineschi V.; Finetti F.; Fisher E. A.; Florey O.; Follo C.; Fortini P.; Fulda S.; Furic L.; Garcia-Del Portillo F.; Garcia-Garcia A.; Garofalo T.; Ghavami S.; Ghigo A.; Gluschko A.; Goder V.; Golab J.; Golebiewska A.; Gomez R.; Gonzalez-Hernandez T.; Gorojod R. M.; Gregory S. L.; Guerri C.; Gunst J.; Guo C.; Guo C.; Gupta P.; Gupta S. K.; Hamacher-Brady A.; Haucke V.; He R. -R.; Herb M.; Hernandez A.; Hernandez C.; Hernandez-Diaz S.; Hilfiker S.; Ho E. A.; Hoet P. H. M.; Huang C.; Hummer G.; Ikeda F.; Imbriano C.; Inman D. M.; Itakura E.; Jacquin E.; Jakobsson J.; Jessen N.; Jimenez-Sanchez M.; Joffre C.; Judith D.; Jung C. H.; Jungbluth H.; Kalia M.; Kaludercic N.; Kalvari I.; Kang C.; Kaniyappan S.; Karmakar P.; Kho W.; Kimchi A.; Kimura T.; Kjaerulff O.; Koch I.; Korkmaz G.; Kou Y.; Krasnodembskaya A. D.; Kuenen S.; Kukar T.; Kumar A.; Ladoire S.; Lafont F.; Laird A. S.; Langer R.; Lee C.; Lee E. B.; Lee E. F.; Lee G. M.; Lefebvre C.; Lenoir O.; Letellier E.; Leung P. S.; Lewis P. A.; Li B.; Li J.; Liang C.; Lindner P.; Liu C.; LLeonart M. E.; Lo C. H.; Lossi L.; Luftig M. A.; Lund A. H.; Lund V. K.; Luu L.; Lyakhovich A.; MacIntosh G. C.; Madeo F.; Madrigal-Matute J.; Maiani E.; Marchetti S.; Mardente S.; Marinelli S.; Martin-Rincon M.; Martinez A.; Martins D. O.; Martins J. O.; Marzetti E.; Mashek D. G.; Masuelli L.; Mattar P.; Maycotte P.; McKenna S. L.; Meng D.; Mercier A. E.; Merighi A.; Meyer C.; Micale L.; Milczarek M.; Mirzaei H.; Misasi R.; Mogensen T. H.; Mollereau B.; Montagna C.; Morishita H.; Morleo M.; Morselli E.; Motori E.; Mukherjee A.; Nandi S. S.; Nanni M.; Nassif M.; Naveiras O.; Nazarko T. Y.; Nazio F.; Neisch A. L.; Neutzner A.; Ni Cheallaigh C.; Noda T.; Novoa B.; Nylandsted J.; Ogier-Denis E.; Oikonomou V.; Olivan S.; Oliveira J. M. A.; Olzmann J. A.; Onnis A.; Ortiz-Gonzalez X. R.; Pahari S.; Palmisano G.; Panasyuk G.; Pandya V.; Paneni F.; Papademetrio D. L.; Papp D.; Park E. C.; Passos J. F.; Pedrozo Z.; Pei G.; Pellegrini J. M.; Pelletier J.; Penna F.; Pennuto M.; Pfirrmann T.; Pierre P.; Pierrefite-Carle V.; Pierzynowska K.; Pietruczuk M.; Pinar M.; Pircs K.; Pizzo P.; Pocock R.; Poletti A.; Popova B.; Prahlad V.; Proikas-Cezanne T.; Puyal J.; Raimundo N.; Ramachandra Rao S.; Rao H.; Reggiori F.; Reigada D.; Renga G.; Richardson D. R.; Rizza S.; Rizzuto R.; Robinson K. J.; Rocchi S.; Romanello V.; Romano A.; Rosenfeldt M. T.; Roussel B. D.; Rozieres A.; Rudolf E.; Sachse C.; Salekdeh G. H.; Sanchez-Vera V.; Sandri M.; Sargeant T. J.; Sarkar C.; Sarkar S.; Sathyanarayanan R.; Schapira A. H. V.; Scharl M.; Schiaffino M. V.; Schmitz I.; Schwamborn J. C.; Schwarten M.; Sciarretta S.; Scott M. J.; Sebastian D.; Sebti S.; Serra-Moreno R.; Shah J. A.; Sharkey L. M.; Shen H.; Shimozawa M.; Shoji I.; Shukla A. K.; Shutt T. E.; Sirko A.; Sirohi K.; Skendros P.; Somarelli J. A.; Staiano L.; Stalnecker C. A.; Stankov M. V.; Stefan K.; Sterneckert J.; Su H.; Sue C. M.; Sze S. C. W.; Szewczyk N. J.; Tafani M.; Takahashi Y.; Tettamanti G.; Thedieck K.; Thumm M.; Timmerman V.; Tomaipitinca L.; Tong C.; Torii S.; Torriglia A.; Ugun-Klusek A.; Uhlig H. H.; Vahsen B. F.; Valdor R.; Valverde A. M.; van Loosdregt J.; van Wijk S. J. L.; Vanhorebeek I.; Varga M.; Verdier M.; Vervliet T.; Vervoorts J.; Victor V. M.; Vigano S.; Villalobo A.; Vincent O.; Voitsekhovskaja O. V.; Wandosell F. G.; Wang B.; Wang C.; Wang C.; Wang C.; Wang D.; Watchon M.; Wei H.; Weiskirchen R.; Weykopf B.; Woehlbier U.; Xia H.; Xiao B.; Yang C.; Yang H.; Yao H.; Yu B.; Yuan J.; Yue J.; Zambelli V. O.; Zanella I.; Zang Q. S.; Zanivan S.; Zhang M.; Zheng G.; Zhong Q.; Zhou A.; Zhou B.; Zhu B.; Ziviani E.; Zoladek T.; Zou W.; Zuryn S.;doi: 10.48350/155081
handle: 11379/542024 , 11392/2442540 , 11564/765957 , 11591/444669 , 2318/1785276 , 11587/453716 , 11391/1490255 , 11568/1104102 , 10807/173406 , 21.11116/0000-000D-4E66-A , 21.11116/0000-000D-4E68-8 , 2434/844005 , 10067/1756630151162165141 , 11590/385750 , 11380/1244073 , 11383/2112326 , 11588/855085 , 11577/3390116 , 11581/450344 , 11388/248298 , 11576/2685604 , 11573/1688011 , 20.500.11770/313778 , 11562/1037826
pmid: 33634751
pmc: PMC7996087
doi: 10.48350/155081
handle: 11379/542024 , 11392/2442540 , 11564/765957 , 11591/444669 , 2318/1785276 , 11587/453716 , 11391/1490255 , 11568/1104102 , 10807/173406 , 21.11116/0000-000D-4E66-A , 21.11116/0000-000D-4E68-8 , 2434/844005 , 10067/1756630151162165141 , 11590/385750 , 11380/1244073 , 11383/2112326 , 11588/855085 , 11577/3390116 , 11581/450344 , 11388/248298 , 11576/2685604 , 11573/1688011 , 20.500.11770/313778 , 11562/1037826
pmid: 33634751
pmc: PMC7996087
In 2008, we published the first set of guidelines for standardizing research in autophagy. Since then, this topic has received increasing attention, and many scientists have entered the field. Our knowledge base and relevant new technologies have also been expanding. Thus, it is important to formulate on a regular basis updated guidelines for monitoring autophagy in different organisms. Despite numerous reviews, there continues to be confusion regarding acceptable methods to evaluate autophagy, especially in multicellular eukaryotes. Here, we present a set of guidelines for investigators to select and interpret methods to examine autophagy and related processes, and for reviewers to provide realistic and reasonable critiques of reports that are focused on these processes. These guidelines are not meant to be a dogmatic set of rules, because the appropriateness of any assay largely depends on the question being asked and the system being used. Moreover, no individual assay is perfect for every situation, calling for the use of multiple techniques to properly monitor autophagy in each experimental setting. Finally, several core components of the autophagy machinery have been implicated in distinct autophagic processes (canonical and noncanonical autophagy), implying that genetic approaches to block autophagy should rely on targeting two or more autophagy-related genes that ideally participate in distinct steps of the pathway. Along similar lines, because multiple proteins involved in autophagy also regulate other cellular pathways including apoptosis, not all of them can be used as a specific marker for bona fide autophagic responses. Here, we critically discuss current methods of assessing autophagy and the information they can, or cannot, provide. Our ultimate goal is to encourage intellectual and technical innovation in the field. doi: 10.1080/15548627.2020.1797280 ispartof: Autophagy vol:17 issue:1 pages:1-382 ispartof: location:United States status: published
BOA - Bicocca Open A... arrow_drop_down Archivio della Ricerca - Università di PisaArticle . 2021Data sources: Archivio della Ricerca - Università di PisaArchivio Istituzionale (AperTO)Article . 2021Full-Text: https://iris.unito.it/bitstream/2318/1785276/1/Klionsky%20et%20al_Guidelines_2020_Post-print.docxData sources: Archivio Istituzionale (AperTO)Recolector de Ciencia Abierta, RECOLECTAReview . 2021Data sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAReview . 2021Data sources: Recolector de Ciencia Abierta, RECOLECTAIRIS - Università degli Studi di VeronaArticle . 2021Data sources: IRIS - Università degli Studi di VeronaArchivio della ricerca- Università di Roma La SapienzaArticle . 2021Data sources: Archivio della ricerca- Università di Roma La SapienzaArchiMer - Institutional Archive of IfremerOther literature type . 2021Data sources: ArchiMer - Institutional Archive of IfremerArchivio della Ricerca - Università di PisaArticle . 2021Data sources: Archivio della Ricerca - Università di PisaRecolector de Ciencia Abierta, RECOLECTAReview . 2021Data sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAReview . Article . 2021Data sources: Recolector de Ciencia Abierta, RECOLECTAInfoscience - EPFL scientific publicationsOther literature typeData sources: Infoscience - EPFL scientific publicationsHAL-Inserm; Hal-DiderotArticle . 2021IRIS - Università degli Studi di VeronaArticle . 2021Data sources: IRIS - Università degli Studi di VeronaArchivio della ricerca- Università di Roma La SapienzaArticle . 2021Data sources: Archivio della ricerca- Università di Roma La SapienzaArchivio Istituzionale dell'Università della CalabriaArticle . 2021Data sources: Archivio Istituzionale dell'Università della Calabriaadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eu613 citations 613 popularity Top 0.01% influence Top 1% impulse Top 0.01% Powered by BIP!more_vert BOA - Bicocca Open A... arrow_drop_down Archivio della Ricerca - Università di PisaArticle . 2021Data sources: Archivio della Ricerca - Università di PisaArchivio Istituzionale (AperTO)Article . 2021Full-Text: https://iris.unito.it/bitstream/2318/1785276/1/Klionsky%20et%20al_Guidelines_2020_Post-print.docxData sources: Archivio Istituzionale (AperTO)Recolector de Ciencia Abierta, RECOLECTAReview . 2021Data sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAReview . 2021Data sources: Recolector de Ciencia Abierta, RECOLECTAIRIS - Università degli Studi di VeronaArticle . 2021Data sources: IRIS - Università degli Studi di VeronaArchivio della ricerca- Università di Roma La SapienzaArticle . 2021Data sources: Archivio della ricerca- Università di Roma La SapienzaArchiMer - Institutional Archive of IfremerOther literature type . 2021Data sources: ArchiMer - Institutional Archive of IfremerArchivio della Ricerca - Università di PisaArticle . 2021Data sources: Archivio della Ricerca - Università di PisaRecolector de Ciencia Abierta, RECOLECTAReview . 2021Data sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAReview . Article . 2021Data sources: Recolector de Ciencia Abierta, RECOLECTAInfoscience - EPFL scientific publicationsOther literature typeData sources: Infoscience - EPFL scientific publicationsHAL-Inserm; Hal-DiderotArticle . 2021IRIS - Università degli Studi di VeronaArticle . 2021Data sources: IRIS - Università degli Studi di VeronaArchivio della ricerca- Università di Roma La SapienzaArticle . 2021Data sources: Archivio della ricerca- Università di Roma La SapienzaArchivio Istituzionale dell'Università della CalabriaArticle . 2021Data sources: Archivio Istituzionale dell'Università della Calabriaadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.48350/155081&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2020 FrancePublisher:EDP Sciences Funded by:ANR | Amidex, ANR | OCEVU, EC | CONCERTOANR| Amidex ,ANR| OCEVU ,EC| CONCERTOLagache, G.; Béthermin, M.; Montier, L.; Serra, P.; Tucci, M.;One of the main goals of Cosmology is to search for the imprint of primordial gravitational waves in the CMB polarisation field, to probe inflationary theories. One of the obstacles toward the detection of the primordial signal is to extract the B-mode polarisation from astrophysical contaminations. We present a complete analysis of extragalactic foreground contamination due to polarised emission of radio and dusty star-forming galaxies. We update or use up-to-date models that are validated using the most recent measurements. We predict the flux limit (confusion noise) for the future CMB space or balloon experiments (IDS, PIPER, SPIDER, LiteBIRD, PICO), as well as ground-based experiments (C-BASS, NEXT-BASS, QUIJOTE, AdvACTPOL, BICEP3+Keck, BICEPArray, CLASS, SO, SPT3G, S4). Telescope aperture size (and frequency) is the main characteristic impacting the level of confusion noise. Using the flux limits and assuming constant polarisation fractions for radio and dusty galaxies, we compute the B-mode power spectra of the three extragalactic foregrounds (radio source shot noise, dusty galaxy shot noise and clustering), discuss their relative levels and compare their amplitudes to that of the primordial tensor modes parametrized by the tensor-to-scalar ratio r. At the reionization bump (l=5), contamination by extragalactic foregrounds is negligible. At the recombination peak (l=80), while the contamination is much lower than the targeted sensitivity on r for large-aperture telescopes, it is at comparable level for some of the medium- and small-aperture telescope experiments. For example, the contamination is at the level of the 68 per cent confidence level uncertainty on the primordial r for the LiteBIRD and PICO space experiments. Finally we also provide some useful unit conversion factors and give some predictions for the SPICA B-BOP experiment. Abridged Comment: A&A in press. Match published version
Astronomy and Astrop... arrow_drop_down https://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: DataciteHAL - UPEC / UPEM; HAL-Pasteur; HAL-InsermPreprint . 2019add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 20 citations 20 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert Astronomy and Astrop... arrow_drop_down https://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: DataciteHAL - UPEC / UPEM; HAL-Pasteur; HAL-InsermPreprint . 2019add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2020 FrancePublisher:MDPI AG Funded by:EC | GlassRoutesEC| GlassRoutesAuthors: Nadine Schibille; Cristina Boschetti; Miguel Ángel Valero Tévar; Emmanuel Veron; +1 AuthorsNadine Schibille; Cristina Boschetti; Miguel Ángel Valero Tévar; Emmanuel Veron; Jorge de Juan Ares;doi: 10.3390/min10030272
International audience; Excavations at the Roman villa of Noheda (Spain) revealed the remains of an exceptionally elaborate fourth-century floor mosaic that contains a surprisingly large number of glass tesserae, representing a broad spectrum of colors. This paper presents the results of the chemical (LA-ICP-MS) and microstructural analyses (SEM-EDS, XRPD) of 420 glass tesserae from these mosaics. The high number of data allowed us to establish the compositional variability and to elucidate questions of supply in relation to a large-scale artistic campaign. The tesserae from Noheda were almost exclusively made from recycled mixed Roman Mn and Sb base glass, thus demonstrating that recycling of Roman base glasses was common practice in the fourth century, occurring on a near industrial scale. It also suggests that the workshops specializing in the production of mosaic tesserae might have been in the western Mediterranean. A limited number of coloring and opacifying additives (Mn, Co, Cu, Sb, Pb) were identified, which resulted in a wide range of hues. These were differentially associated with various trace elements, which implies the use of different raw materials. A subset of red, green, and orange tesserae reflect distinct base glass characteristics as well as coloring technologies that point to an Egyptian provenance.
Minerals arrow_drop_down MineralsOther literature type . Article . 2020 . Peer-reviewedLicense: CC BYFull-Text: https://www.mdpi.com/2075-163X/10/3/272/pdfMémoires en Sciences de l'Information et de la CommunicationArticle . 2020Full-Text: https://hal.science/hal-02511142/documentadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess Routesgold 18 citations 18 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert Minerals arrow_drop_down MineralsOther literature type . Article . 2020 . Peer-reviewedLicense: CC BYFull-Text: https://www.mdpi.com/2075-163X/10/3/272/pdfMémoires en Sciences de l'Information et de la CommunicationArticle . 2020Full-Text: https://hal.science/hal-02511142/documentadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2020 FrancePublisher:American Geophysical Union (AGU) Funded by:EC | PoroFracEC| PoroFracAuthors: Thibault Duretz; René de Borst; Philippe Yamato; Laetitia Le Pourhiet;Thibault Duretz; René de Borst; Philippe Yamato; Laetitia Le Pourhiet;doi: 10.1029/2019gl086027
AbstractStrain localization is a fundamental characteristic of plate tectonics. The resulting deformation structures shape the margins of continents and the internal structure of tectonic plates. To model the occurrence of faulting, geodynamic models generally rely on frictional plasticity. Frictional plasticity is normally embedded in visco‐plastic (V‐P) or visco‐elasto‐plastic (V‐E‐P) rheologies. This poses some fundamental issues, such as the difficulty, or often inability, to obtain a converged equilibrium state and a severe grid sensitivity. Here, we study shear banding at crustal‐scale using a visco‐elasto‐viscoplastic (V‐E‐VP) model. We show that this rheology allows to accurately satisfy equilibrium, leads to shear band patterns that converge upon mesh refinement, and preserves characteristic shear band angles. Moreover, a comparison with analytic models and laboratory data reveals that V‐E‐VP rheology captures first‐order characteristics of frictional plasticity. V‐E‐VP models thus overcomes limitations of V‐P and V‐E‐P models and appears as an attractive alternative for geodynamic modeling.
CORE (RIOXX-UK Aggre... arrow_drop_down Geophysical Research LettersOther literature type . Article . 2020 . Peer-reviewedLicense: Wiley Online Library User AgreementHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2020add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1029/2019gl086027&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesbronze 12 citations 12 popularity Top 10% influence Average impulse Top 10% Powered by BIP!visibility 4visibility views 4 download downloads 53 Powered bymore_vert CORE (RIOXX-UK Aggre... arrow_drop_down Geophysical Research LettersOther literature type . Article . 2020 . Peer-reviewedLicense: Wiley Online Library User AgreementHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2020add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1029/2019gl086027&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2020 FrancePublisher:Copernicus GmbH Funded by:EC | ESCAPEEC| ESCAPET. J. Fauchez; T. J. Fauchez; T. J. Fauchez; M. Turbet; M. Turbet; E. T. Wolf; E. T. Wolf; I. Boutle; M. J. Way; M. J. Way; A. D. Del Genio; N. J. Mayne; K. Tsigaridis; K. Tsigaridis; R. K. Kopparapu; R. K. Kopparapu; J. Yang; F. Forget; A. Mandell; A. Mandell; S. D. Domagal Goldman; S. D. Domagal Goldman;Upcoming telescopes such as the James Webb Space Telescope (JWST), or the Extremely Large Telescope (ELTs), may soon be able to characterize, through transmission, emission or reflection spectroscopy, the atmospheres of rocky exoplanets orbiting nearby M dwarfs. One of the most promising candidates is the late M dwarf system TRAPPIST-1 which has seven known transiting planets for which Transit Timing Variation (TTV) measurements suggest that they are terrestrial in nature, with a possible enrichment in volatiles. Among these seven planets, TRAPPIST-1e seems to be the most promising candidate to have habitable surface conditions, receiving ~66 % of the Earth's incident radiation, and thus needing only modest greenhouse gas inventories to raise surface temperatures to allow surface liquid water to exist. TRAPPIST-1e is therefore one of the prime targets for JWST atmospheric characterization. In this context, the modeling of its potential atmosphere is an essential step prior to observation. Global Climate Models (GCMs) offer the most detailed way to simulate planetary atmospheres. However, intrinsic differences exist between GCMs which can lead to different climate prediction and thus observability of gas and/or cloud features in transmission and thermal emission spectra. Such differences should preferably be known prior to observations. In this paper we present a protocol to inter-compare planetary GCMs. Four testing cases are considered for TRAPPIST-1e but the methodology is applicable to other rocky exoplanets in the Habitable Zone. The four test cases included two land planets composed with a modern Earth and pure CO2 atmospheres, respectively, and two aqua planets with the same atmospheric compositions. Currently, there are four participating models (LMDG, ROCKE-3D, ExoCAM, UM), however this protocol is intended to let other teams participate as well. Comment: Accepted and published in Geoscientific Model Development (GMD)
Geoscientific Model ... arrow_drop_down Geoscientific Model DevelopmentOther literature type . Article . 2020 . Peer-reviewedLicense: CC BYhttps://doi.org/10.48550/arxiv...Article . 2020License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.5194/gmd-13-707-2020&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 52 citations 52 popularity Top 1% influence Average impulse Top 1% Powered by BIP!more_vert Geoscientific Model ... arrow_drop_down Geoscientific Model DevelopmentOther literature type . Article . 2020 . Peer-reviewedLicense: CC BYhttps://doi.org/10.48550/arxiv...Article . 2020License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.5194/gmd-13-707-2020&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Other literature type 2020 FrancePublisher:Elsevier BV Funded by:SNSF | SeaO2 - Past changes in S..., ARC | Discovery Early Career Re..., EC | ACCLIMATE +1 projectsSNSF| SeaO2 - Past changes in Southern Ocean overturning circulation - implications for the partitioning of carbon and oxygen between the ocean and the atmosphere ,ARC| Discovery Early Career Researcher Award - Grant ID: DE150100107 ,EC| ACCLIMATE ,UKRI| The bi-polar seesaw and CO2: Is there anything special about 'Terminal seesaw events'?Julia Gottschalk; Luke C Skinner; Samuel L Jaccard; Laurie Menviel; Christoph Nehrbass-Ahles; Claire Waelbroeck;International audience; Past millennial-scale changes in atmospheric CO2 (CO2,atm) concentrations have often been attributed to variations in the overturning timescale of the ocean that result in changes in the marine carbon inventory. Yet, there remains a paucity of proxy evidence that documents changes in marine carbon storage globally, and that links them to abrupt climate variability in the northern hemisphere associated with perturbations of the Atlantic Meridional Overturning Circulation (AMOC). The last two glacial periods were suggested to differ in the spatial extent of the AMOC and its sensitivity to perturbations. This provides an opportunity to compare the nature of marine carbon cycle-climate feedbacks between them. Here, we reconstruct variations in respired carbon storage (via oxygenation) and the AMOC “geometry” (via carbonate ion saturation) in the deep South Atlantic. We infer decreases in deep South Atlantic respired carbon levels at times of weakened AMOC and rising CO2,atm concentrations during both glacial periods. These findings suggest a consistent pattern of increased Southern Ocean convection and/or air-sea CO2 fluxes during northern-hemisphere stadials accompanying AMOC perturbations and promoting a rise in CO2,atm levels. We find that net ocean carbon loss, and hence the magnitude of CO2,atm rise, is largely determined by the stadial duration. North Atlantic climate anomalies therefore affect Southern Ocean carbon cycling in a consistent manner, through oceanic (e.g., ventilation seesaw) and/or atmospheric processes (e.g., Ekman pumping).
Quaternary Science R... arrow_drop_down HAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2020add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.quascirev.2019.106067&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesbronze 18 citations 18 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert Quaternary Science R... arrow_drop_down HAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2020add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.quascirev.2019.106067&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Other literature type 2020 France, GermanyPublisher:Elsevier BV Sepideh Esmaeilirad; Alexandra Lai; Gülcin Abbaszade; Juergen Schnelle-Kreis; Ralf Zimmermann; Gaëlle Uzu; Kaspar R. Daellenbach; Francesco Canonaco; Hossein Hassankhany; Mohammad Arhami; Urs Baltensperger; André S. H. Prévôt; James J. Schauer; Jean-Luc Jaffrezo; Vahid Hosseini; Imad El Haddad;pmid: 31835192
International audience; With over 8 million inhabitants and 4 million motor vehicles on the streets, Tehran is one of the most crowded and polluted cities in the Middle East. Frequent exceedances of national daily PM2.5 limit have been reported in this city during the last decade, yet, the chemical composition and sources of fine particles are poorly determined. In the present study, 24-hour PM2.5 samples were collected at two urban sites during two separate campaigns, a one-year period from 2014 to 2015 and another three-month period at the beginning of 2017. Concentrations of organic carbon (OC), elemental carbon (EC), inorganic ions, trace metals and specific organic molecular markers were measured by chemical analysis of filter samples. The dominant mass components were organic matter (OM), sulfate and EC. With a 20% water-soluble organic carbon (WSOC) fraction, the predominance of primary anthropogenic sources (i.e. fossil fuel combustion) was anticipated. A positive matrix factorization (PMF) analysis using the ME-2 (Multilinear Engine-2) solver was then applied to this dataset. 5 factors were identified by Marker-PMF, named as traffic exhaust (TE), biomass burning (BB), industries (Ind.), nitrate-rich and sulfate-rich. Another 4 factors were identified by Metal-PMF, including, dust, vehicles (traffic non-exhaust, TNE), industries (Ind.) and heavy fuel combustion (HFC). Traffic exhaust was the dominant source with 44.5% contribution to total quantified PM2.5 mass. Sulfate-rich (24.2%) and nitrate-rich (18.4%) factors were the next major contributing sources. Dust (4.4%) and biomass burning (6.7%) also had small contributions while the total share of all other factors was < 2%. Investigating the correlations of different factors between the two sampling sites showed that traffic emissions and biomass burning were local, whereas dust, heavy fuel combustion and industrial sources were regional. Results of this study indicate that gas- and particle-phase pollutants emitted from fossil fuel combustion (mobile and stationary) are the principal origin of both primary and secondary fine aerosols in Tehran.
Horizon / Pleins tex... arrow_drop_down Publication Server of Helmholtz Zentrum München (PuSH)Article . 2020Data sources: Publication Server of Helmholtz Zentrum München (PuSH)The Science of The Total EnvironmentArticle . 2020 . Peer-reviewedLicense: Elsevier TDMData sources: CrossrefHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2020add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.scitotenv.2019.135330&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesbronze 35 citations 35 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert Horizon / Pleins tex... arrow_drop_down Publication Server of Helmholtz Zentrum München (PuSH)Article . 2020Data sources: Publication Server of Helmholtz Zentrum München (PuSH)The Science of The Total EnvironmentArticle . 2020 . Peer-reviewedLicense: Elsevier TDMData sources: CrossrefHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2020add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.scitotenv.2019.135330&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2020 FrancePublisher:MDPI AG Funded by:NSF | GeoSoilEnviroCARS: A Nati...NSF| GeoSoilEnviroCARS: A National Resource for Earth, Planetary, Soil and Environmental Science Research at the APSZhicheng Jing; Tony Yu; Man Xu; Julien Chantel; Yanbin Wang;doi: 10.3390/min10020126
s interior. Unlike their solid counterparts, these properties of liquids pose great technical challenges to high-pressure measurements and are poorly constrained. Here we present the technical developments that have been made at the GSECARS beamline 13-ID-D of the Advanced Photon Source for the past several years for determination of sound velocity of liquids using the ultrasonic techniques in a 1000-ton Kawai-type multianvil apparatus. Temperature of the sound velocity measurements has been extended to ~2400 K at 4 GPa and ~2000 K at 8 GPa to enable studies of liquids with very high melting temperatures, such as the silicate liquids. Sound velocity and equation of state of liquids provide important constraints on the generation, presence, and transport of silicate and metallic melts in the Earth&rsquo
Minerals arrow_drop_down MineralsOther literature type . Article . 2020 . Peer-reviewedLicense: CC BYFull-Text: http://www.mdpi.com/2075-163X/10/2/126/pdfadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3390/min10020126&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesgold 11 citations 11 popularity Top 10% influence Average impulse Top 10% Powered by BIP!visibility 16visibility views 16 download downloads 68 Powered bymore_vert Minerals arrow_drop_down MineralsOther literature type . Article . 2020 . Peer-reviewedLicense: CC BYFull-Text: http://www.mdpi.com/2075-163X/10/2/126/pdfadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3390/min10020126&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Other literature type 2020 Italy, France, ItalyPublisher:Elsevier BV Funded by:EC | TRUE DEPTHS, EC | ZIPEC| TRUE DEPTHS ,EC| ZIPGilio M.[1; 2]; Scambelluri M.[1]; Agostini S.[3]; Godard M.[4]; Pettke T.[5]; Agard P.[6]; Locatelli M.[6]; Angiboust S.[7];handle: 11567/990872
International audience; The Lago Superiore Unit (LSU, Monviso Massif, Italian Western Alps) is a section of fossil oceanic lithosphere equilibrated to eclogite facies conditions (550 °C – 2.8 GPa) during Alpine subduction (45–40 Ma). It is cut by two major shear zones, namely the Intermediate (ISZ) and Lower Shear Zone (LSZ), mostly consisting of serpentinite. The lowermost, serpentine-rich, section of the Lago Superiore Unit, the Basal Serpentinite, separates the HP ophiolite domain from the underlying continental Dora-Maira Unit.Here we show that the LSZ and the Basal Serpentinite were active at different stages of the subduction and exhumation history of the complex. Most of retrograde deformation and mineral re-equilibration were localized in the LSZ. Channelized fluids percolating during this phase chemically homogenized the LSZ serpentinites, that preserved their HP mineralogy only locally; the best-preserved relicts of the eclogite-facies high pressure stage within the LSZ serpentinite are nodules of magnesite (representing former veins) and eclogite blocks. Differently, the underlying Basal Serpentinite largely escaped the exhumation-related processes and still records the prograde chemical and petrological history of the LSU serpentinite, from ocean-floor hydration to HP metamorphic conditions.The Lago Superiore Unit thus represents a snapshot of major Alpine metamorphic and shearing events, from prograde subduction to exhumation. Its km-scale thickness, and the oriented antigorite fabric in the Lower Shear Zone and Basal Serpentinite makes it a good seismic reflector. This HP ophiolite complex can thus be used as proxy of a deep (70–80 km) Alpine-type subduction zone, and to better constrain and interpret seismic images of present-day convergent margins.
Lithos arrow_drop_down Lithos; Archivio istituzionale della ricerca - Università di GenovaArticle . 2020 . Peer-reviewedLicense: Elsevier TDMadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.lithos.2019.105308&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesbronze 9 citations 9 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert Lithos arrow_drop_down Lithos; Archivio istituzionale della ricerca - Università di GenovaArticle . 2020 . Peer-reviewedLicense: Elsevier TDMadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.lithos.2019.105308&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2019 United Kingdom, Netherlands, United States, Netherlands, Netherlands, FrancePublisher:American Astronomical Society Funded by:EC | CSINEUTRONSTAREC| CSINEUTRONSTARSlavko Bogdanov; Sebastien Guillot; Paul S. Ray; Michael T. Wolff; Deepto Chakrabarty; Wynn C. G. Ho; Matthew Kerr; Frederick K. Lamb; Andrea N. Lommen; Renee M. Ludlam; Reilly Milburn; Sergio Montano; M. Coleman Miller; Michi Baubock; Feryal Özel; Dimitrios Psaltis; Ronald A. Remillard; Thomas E. Riley; James F. Steiner; Tod E. Strohmayer; Anna L. Watts; Kent S. Wood; Jesse Zeldes; Teruaki Enoto; Takashi Okajima; James W. Kellogg; Charles Baker; Craig B. Markwardt; Zaven Arzoumanian; Keith C. Gendreau;We present the set of deep Neutron Star Interior Composition Explorer (NICER) X-ray timing observations of the nearby rotation-powered millisecond pulsars PSRs J0437-4715, J0030+0451, J1231-1411, and J2124-3358, selected as targets for constraining the mass-radius relation of neutron stars and the dense matter equation of state via modeling of their pulsed thermal X-ray emission. We describe the instrument, observations, and data processing/reduction procedures, as well as the series of investigations conducted to ensure that the properties of the data sets are suitable for parameter estimation analyses to produce reliable constraints on the neutron star mass-radius relation and the dense matter equation of state. We find that the long-term timing and flux behavior and the Fourier-domain properties of the event data do not exhibit any anomalies that could adversely affect the intended measurements. From phase-selected spectroscopy, we find that emission from the individual pulse peaks is well described by a single-temperature hydrogen atmosphere spectrum, with the exception of PSR J0437-4715, for which multiple temperatures are required. Comment: 28 pages, 9 figures; accepted for publication in the Astrophysical Journal Letters
NARCIS; The Astrophy... arrow_drop_down The Astrophysical Journal LettersOther literature type . Article . 2019 . Peer-reviewedLicense: IOP Copyright Policieshttps://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: DataciteHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2019add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3847/2041-8213/ab53eb&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 108 citations 108 popularity Top 1% influence Top 10% impulse Top 1% Powered by BIP!visibility 5visibility views 5 download downloads 8 Powered bymore_vert NARCIS; The Astrophy... arrow_drop_down The Astrophysical Journal LettersOther literature type . Article . 2019 . Peer-reviewedLicense: IOP Copyright Policieshttps://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: DataciteHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2019add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3847/2041-8213/ab53eb&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eu