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Infant-phase reddening by surface Fe-peak elements in a normal type Ia supernova
Indexado
WoS WOS:000757130000001
Scopus SCOPUS_ID:85124749249
DOI 10.1038/S41550-022-01603-4
Año 2022
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



Very early observations of a type Ia supernova-from within one hour of explosion-show a red colour that develops and rapidly disappears. These data provide information on the initial explosion mechanism: surface nuclear burning on the white dwarf or extreme mixing of the nuclear burning process.

Revista



Revista ISSN
Nature Astronomy 2397-3366

Métricas Externas



PlumX Altmetric Dimensions

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Disciplinas de Investigación



WOS
Astronomy & Astrophysics
Scopus
Sin Disciplinas
SciELO
Sin Disciplinas

Muestra la distribución de disciplinas para esta publicación.

Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



Muestra la distribución de colaboración, tanto nacional como extranjera, generada en esta publicación.


Autores - Afiliación



Ord. Autor Género Institución - País
1 Ni, Yuan Qi - UNIV TORONTO - Canadá
University of Toronto - Canadá
2 Moon, Dae-Sik Hombre UNIV TORONTO - Canadá
University of Toronto - Canadá
3 Drout, Maria R. Mujer UNIV TORONTO - Canadá
University of Toronto - Canadá
4 Polin, A. Mujer Observ Carnegie Inst Sci - Estados Unidos
CALTECH - Estados Unidos
Observatorio Las Campanas - Estados Unidos
California Institute of Technology - Estados Unidos
5 Sand, David J. Hombre UNIV ARIZONA - Estados Unidos
The University of Arizona - Estados Unidos
6 Gonzalez-Gaitan, S. Hombre Univ Lisbon - Portugal
Instituto Superior Técnico - Portugal
7 Ree, Chang H. Hombre Korea Astron & Space Sci Inst - Corea del Sur
Korea Univ Sci & Technol - Corea del Sur
Korea Astronomy and Space Science Institute - Corea del Sur
University of Science and Technology (UST) - Corea del Sur
8 Lee, Youngdae Hombre Korea Astron & Space Sci Inst - Corea del Sur
Chungnam Natl Univ - Corea del Sur
Korea Astronomy and Space Science Institute - Corea del Sur
Chungnam National University - Corea del Sur
9 Park, Hong Soo Hombre Korea Astron & Space Sci Inst - Corea del Sur
Korea Univ Sci & Technol - Corea del Sur
Korea Astronomy and Space Science Institute - Corea del Sur
University of Science and Technology (UST) - Corea del Sur
10 Howell, D. Andrew - UNIV CALIF SANTA BARBARA - Estados Unidos
Las Cumbres Observ - Estados Unidos
University of California, Santa Barbara - Estados Unidos
Las Cumbres Observatory Global Telescope Network, Inc - Estados Unidos
11 Nugent, Peter Hombre UNIV CALIF BERKELEY - Estados Unidos
Lawrence Berkeley Natl Lab - Estados Unidos
Texas A&M Univ - Estados Unidos
University of California, Berkeley - Estados Unidos
Lawrence Berkeley National Laboratory - Estados Unidos
12 Piro, Anthony L. Hombre Observ Carnegie Inst Sci - Estados Unidos
Observatorio Las Campanas - Estados Unidos
13 Brown, Peter J. Hombre George P & Cynthia Woods Mitchell Inst Fundamenta - Estados Unidos
Texas A&M University - Estados Unidos
14 Frohmaier, C. Hombre UNIV AUTONOMA BARCELONA - España
Inst Estudis Espacials Catalunya IEEC - España
15 Burke, Jamison Hombre UNIV CALIF SANTA BARBARA - Estados Unidos
Las Cumbres Observ - Estados Unidos
University of California, Santa Barbara - Estados Unidos
Las Cumbres Observatory Global Telescope Network, Inc - Estados Unidos
16 Hiramatsu, D. Hombre UNIV CALIF SANTA BARBARA - Estados Unidos
Las Cumbres Observ - Estados Unidos
Ctr Astrophys Harvard & Smithsonian - Estados Unidos
NSF Al Inst Artificial Intelligence & Fundamental - Estados Unidos
University of California, Santa Barbara - Estados Unidos
Las Cumbres Observatory Global Telescope Network, Inc - Estados Unidos
Harvard-Smithsonian Center for Astrophysics - Estados Unidos
The NSF AI Institute for Artificial Intelligence and Fundamental Interactions - Estados Unidos
17 de Wasseige, G. Hombre UNIV ARIZONA - Estados Unidos
The University of Arizona - Estados Unidos
18 Valenti, S. Hombre UNIV CALIF DAVIS - Estados Unidos
University of California, Davis - Estados Unidos
19 Afsariardchi, Niloufar Mujer UNIV TORONTO - Canadá
University of Toronto - Canadá
20 Andrews, Jennifer E. Mujer UNIV ARIZONA - Estados Unidos
The University of Arizona - Estados Unidos
21 Antoniadis, John Hombre Univ Crete - Grecia
Wax Planck Inst Radioastron - Alemania
Argelander Inst Astron - Alemania
Foundation for Research and Technology-Hellas - Grecia
Max Planck Institute for Radio Astronomy - Alemania
Universität Bonn - Alemania
22 Arcavi, Iair - Tel Aviv Univ - Israel
Canadian Inst Adv Res CIfAR - Canadá
Tel Aviv University - Israel
Canadian Institute for Advanced Research - Canadá
23 Beaton, R. L. Mujer Observ Carnegie Inst Sci - Estados Unidos
Princeton Univ - Estados Unidos
Observatorio Las Campanas - Estados Unidos
Princeton University - Estados Unidos
24 Fox, O. Hombre UNIV WASHINGTON - Estados Unidos
University of Washington - Estados Unidos
25 Carlberg, Raymond G. Hombre UNIV TORONTO - Canadá
University of Toronto - Canadá
26 Cenko, S. B. Hombre NASA - Estados Unidos
UNIV MARYLAND - Estados Unidos
NASA Goddard Space Flight Center - Estados Unidos
University of Maryland, College Park - Estados Unidos
27 Cha, Sang-Mok - Korea Astron & Space Sci Inst - Corea del Sur
Kyung Hee Univ - Corea del Sur
Korea Astronomy and Space Science Institute - Corea del Sur
Kyung Hee University - Corea del Sur
27 Cha, Sang Mok - Korea Astronomy and Space Science Institute - Corea del Sur
Kyung Hee University - Corea del Sur
27 Cha, Sang-Mok - Korea Astron & Space Sci Inst - Corea del Sur
Kyung Hee Univ - Corea del Sur
28 Dong, Y. - UNIV CALIF DAVIS - Estados Unidos
University of California, Davis - Estados Unidos
29 Gal-Yam, Avishay Hombre Weizmann Inst Sci - Israel
Weizmann Institute of Science Israel - Israel
30 Haislip, Joshua Hombre UNIV N CAROLINA - Estados Unidos
The University of North Carolina at Chapel Hill - Estados Unidos
College of Arts & Sciences - Estados Unidos
31 Holoien, Thomas W. -S. Hombre Observ Carnegie Inst Sci - Estados Unidos
Observatorio Las Campanas - Estados Unidos
32 Johnson, Sean Hombre Princeton Univ - Estados Unidos
Princeton University - Estados Unidos
33 Kouprianov, V. Hombre UNIV N CAROLINA - Estados Unidos
Russian Acad Sci - Rusia
The University of North Carolina at Chapel Hill - Estados Unidos
Pulkovo Observatory of the Russian Academy of Sciences - Rusia
College of Arts & Sciences - Estados Unidos
34 Lee, Yongseok Hombre Korea Astron & Space Sci Inst - Corea del Sur
Kyung Hee Univ - Corea del Sur
Korea Astronomy and Space Science Institute - Corea del Sur
Kyung Hee University - Corea del Sur
35 Matzner, Christopher D. Hombre UNIV TORONTO - Canadá
University of Toronto - Canadá
36 MORRELL, NIDIA IRENE Mujer Observatorio Las Campanas - Chile
Las Campanas Observatory - Chile
Carnegie Observ - Chile
37 McCully, Curtis - UNIV CALIF SANTA BARBARA - Estados Unidos
Las Cumbres Observ - Estados Unidos
38 Nicholl, M. Hombre Universidad Nacional Andrés Bello - Chile
Instituto Milenio de Astrofísica - Chile
39 Reichart, Daniel E. Hombre UNIV N CAROLINA - Estados Unidos
The University of North Carolina at Chapel Hill - Estados Unidos
College of Arts & Sciences - Estados Unidos
40 Rich, J. A. Hombre Observ Carnegie Inst Sci - Estados Unidos
Observatorio Las Campanas - Estados Unidos
41 Ryder, Stuart D. Hombre Macquarie Univ - Australia
Macquarie University - Australia
42 Smith, N. Hombre UNIV ARIZONA - Estados Unidos
The University of Arizona - Estados Unidos
43 Wyatt, Samuel Hombre UNIV ARIZONA - Estados Unidos
The University of Arizona - Estados Unidos
44 Yang, S. - Stockholm Univ - Suecia
Stockholms universitet - Suecia

Muestra la afiliación y género (detectado) para los co-autores de la publicación.

Financiamiento



Fuente
National Science Foundation
Fundação para a Ciência e a Tecnologia
FCT
National Research Foundation of Korea
European Commission
Ministerio de Ciencia e Innovación
University of California
European Social Fund
NSF
European Research Council
U.S. Department of Energy
NASA
Natural Sciences and Engineering Research Council of Canada
Millennium Science Initiative
National Aeronautics and Space Administration
W. M. Keck Foundation
University of Toronto
Office of Science
Canada Research Chairs program
German-Israeli Foundation for Scientific Research and Development
Heising-Simons Foundation
NASA through Hubble Fellowship - Space Telescope Science Institute
Space Telescope Science Institute
Agencia Estatal de Investigación
Korea Astronomy and Space Science Institute
Israel Science Foundation
ISF GW excellence center
Veronika A. Rabl Physics Discretionary Fund
Benoziyo Endowment Fund for the Advancement of Science
Horizon 2020 Framework Programme
Canada Foundation for Innovation
United States-Israel Binational Science Foundation
Stavros Niarchos Foundation
Canadian Institute for Advanced Research
Dunlap Institute at the University of Toronto
Leading Edge Fund from the Canadian Foundation for Innovation
Ministry of Science, ICT and Future Planning
NASA's Astrophysics Data Analysis Program
United States - Israel Binational Science Foundation (BSF)
Agencia Estatal de Investigacion (AEI)
Scleroderma Society of Ontario
Hellenic Foundation for Research and Innovation
Swift GI program
Canadian Institute for Advanced Research (CIFAR)
CTIO
Helen and Martin Kimmel Award for Innovative Investigation
MCIN
SAAO
Deloro Institute for Advanced Research in Space and Optics
United States - Israel Binational Science Foundation
Israeli Council for Higher Education Alon Fellowship
National Energy Research Scientific Computing Center, a Department of Energy Office of Science User Facility
Stavros Niarchos Foundation (SNF)
Centro Superior de Investigaciones Cientificas (CSIC) under the PIE project
European Union via ERC
United States Department of Energy's Science Office of High Energy Physics
HOSTFLOWS project
IMOS space infrastructure grant
Gravity and the Extreme Universe Program
Spanish Ministerio de Ciencia e Innovacion (MCIN)
WIS-CIT joint research grant
Hellenic Foundation for Research and Innovation (HFRI) under the 2nd Call of 'Science and Society' Action 'Always strive for excellence - Theodoros Papazoglou'
BSF/Transformative and GIF grants
National Research Foundation (NRF) of Korea - Korean government (MSIT, Ministry of Science and ICT)
K-GMT Science Program of KASI
Yeda-Sela Center for Basic Research
European Social Fund (ESF) 'Investing in your future' under the 2019 Ramon y Cajal program
Centro Superior de Investigaciones Científicas
WIS-CIT
Swift GI

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos



Agradecimiento
13039/501100011033, the European Social Fund (ESF) 'Investing in your future' under the 2019 Ramon y Cajal program RYC2019-027683-I and the PID2020-115253GA-I00 HOSTFLOWS project, as well as from the Centro Superior de Investigaciones Cientificas (CSIC) under the PIE project 20215AT016. G.P. acknowledges support from the Millennium Science Initiative through grant no. IC120009. J.A. is supported by the Stavros Niarchos Foundation (SNF) and the Hellenic Foundation for Research and Innovation (HFRI) under the 2nd Call of 'Science and Society' Action 'Always strive for excellence - Theodoros Papazoglou' (project no. 01431).
13039/501100011033, the European Social Fund (ESF) 'Investing in your future' under the 2019 Ramon y Cajal program RYC2019-027683-I and the PID2020-115253GA-I00 HOSTFLOWS project, as well as from the Centro Superior de Investigaciones Cientificas (CSIC) under the PIE project 20215AT016. G.P. acknowledges support from the Millennium Science Initiative through grant no. IC120009. J.A. is supported by the Stavros Niarchos Foundation (SNF) and the Hellenic Foundation for Research and Innovation (HFRI) under the 2nd Call of 'Science and Society' Action 'Always strive for excellence - Theodoros Papazoglou' (project no. 01431).
This research has made use of the KMTNet system operated by the Korea Astronomy and Space Science Institute (KASI), and the data were obtained at the three host sites of CTIO in Chile, SAAO in South Africa and SSO in Australia. The Gemini South observations were obtained under the K-GMT Science Program (PID GS-2018A-Q-117 and GS-2018B-Q-121) of KASI. The Swift observations were triggered through the Swift GI program 80NSSC19K0316. SOUSA is supported by NASA’s Astrophysics Data Analysis Program through grant no. NNX13AF35G. Some of the data presented here were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California and NASA. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation. The Computational HEP program in the United States Department of Energy’s Science Office of High Energy Physics provided simulation resources through grant no. KA2401022. This research used resources of the National Energy Research Scientific Computing Center, a Department of Energy Office of Science User Facility operated under contract no. DE-AC02-05CH11231. D.-S.M., M.R.D. and C.D.M. are supported by Discovery Grants from the Natural Sciences and Engineering Research Council of Canada. D.-S.M. was supported in part by a Leading Edge Fund from the Canadian Foundation for Innovation (project no. 30951). M.R.D. was supported in part by the Canada Research Chairs Program, the Canadian Institute for Advanced Research (CIFAR) and the Dunlap Institute at the University of Toronto. D.J.S. acknowledges support by NSF grant nos. AST-1821987, 1821967 and 1908972 and from the Heising–Simons Foundation under grant no. 2020-1864. S.G.-G. acknowledges support by FCT under project CRISP PTDC/FIS-AST-31546 and project UIDB/00099/2020. H.S.P. was supported in part by a National Research Foundation (NRF) of Korea grant funded by the Korean government (MSIT, Ministry of Science and ICT; no. NRF-2019R1F1A1058228). P.J.B. acknowledges support from the Swift GI program 80NSSC19K0316. S.V., Y.D. and K.A.B. acknowledge support by NSF grant nos. AST-1813176 and AST-2008108. C.M. acknowledges support by NSF grant AST-1313484. I.A. is a CIFAR Azrieli Global Scholar in the Gravity and the Extreme Universe Program and acknowledges support from that program, from the Israel Science Foundation (grant nos. 2108/18 and 2752/19), from the United States – Israel Binational Science Foundation (BSF) and from an Israeli Council for Higher Education Alon Fellowship. R.L.B. acknowledges support by NASA through Hubble Fellowship grant no. 51386.01 awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA under contract no. NAS 5-26555. A.G.-Y. acknowledges support from the European Union via ERC grant no. 725161, the ISF GW Excellence Center, an IMOS space infrastructure grant and BSF/Transformative and GIF grants, as well as from the Benoziyo Endowment Fund for the Advancement of Science, the Deloro Institute for Advanced Research in Space and Optics, the Veronika A. Rabl Physics Discretionary Fund, P. and T. Gardner, the Yeda-Sela Center for Basic Research and a WIS-CIT joint research grant. A.G.-Y. is the recipient of the Helen and Martin Kimmel Award for Innovative Investigation. L.G. acknowledges financial support from the Spanish Ministerio de Ciencia e Innovación (MCIN), the Agencia Estatal de Investigación (AEI) 10.13039/501100011033, the European Social Fund (ESF) ‘Investing in your future’ under the 2019 Ramón y Cajal program RYC2019-027683-I and the PID2020-115253GA-I00 HOSTFLOWS project, as well as from the Centro Superior de Investigaciones Científicas (CSIC) under the PIE project 20215AT016. G.P. acknowledges support from the Millennium Science Initiative through grant no. IC120009. J.A. is supported by the Stavros Niarchos Foundation (SNF) and the Hellenic Foundation for Research and Innovation (HFRI) under the 2nd Call of ‘Science and Society’ Action ‘Always strive for excellence – Theodoros Papazoglou’ (project no. 01431).

Muestra la fuente de financiamiento declarada en la publicación.