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Target-of-opportunity Observations of Gravitational-wave Events with Vera C. Rubin Observatory
Indexado
WoS WOS:000794984400001
Scopus SCOPUS_ID:85131351937
DOI 10.3847/1538-4365/AC617C
Año 2022
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



The discovery of the electromagnetic counterpart to the binary neutron star (NS) merger GW170817 has opened the era of gravitational-wave multimessenger astronomy. Rapid identification of the optical/infrared kilonova enabled a precise localization of the source, which paved the way to deep multiwavelength follow-up and its myriad of related science results. Fully exploiting this new territory of exploration requires the acquisition of electromagnetic data from samples of NS mergers and other gravitational-wave sources. After GW170817, the frontier is now to map the diversity of kilonova properties and provide more stringent constraints on the Hubble constant, and enable new tests of fundamental physics. The Vera C. Rubin Observatory’s Legacy Survey of Space and Time can play a key role in this field in the 2020s, when an improved network of gravitational-wave detectors is expected to reach a sensitivity that will enable the discovery of a high rate of merger events involving NSs (∼tens per year) out to distances of several hundred megaparsecs. We design comprehensive target-of-opportunity observing strategies for follow-up of gravitational-wave triggers that will make the Rubin Observatory the premier instrument for discovery and early characterization of NS and other compact-object mergers, and yet unknown classes of gravitational-wave events.

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Disciplinas de Investigación



WOS
Astronomy & Astrophysics
Scopus
Sin Disciplinas
SciELO
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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



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Autores - Afiliación



Ord. Autor Género Institución - País
1 Andreoni, I. Hombre University of Maryland, College Park - Estados Unidos
NASA Goddard Space Flight Center - Estados Unidos
UNIV MARYLAND - Estados Unidos
NASA Goddard Space Flight Ctr - Estados Unidos
2 Margutti, R. Mujer University of California, Berkeley - Estados Unidos
UNIV CALIF BERKELEY - Estados Unidos
3 Salafia, O. S. Hombre Osservatorio Astronomico di Brera - Italia
Istituto Nazionale di Fisica Nucleare, Sezione di Milano-Bicocca - Italia
Istituto Nazionale di Astrofisica - Italia
Ist Nazl Fis Nucl - Italia
INAF Osservatorio Astron Brera - Italia
4 Parazin, B. - Northeastern University - Estados Unidos
Northeastern Univ - Estados Unidos
5 Villar, A. - Pennsylvania State University - Estados Unidos
PENN STATE UNIV - Estados Unidos
6 Coughlin, Michael W. Hombre University of Minnesota Twin Cities - Estados Unidos
Univ Minnesota - Estados Unidos
College of Science and Engineering - Estados Unidos
7 Yoachim, Peter Hombre University of Washington - Estados Unidos
UNIV WASHINGTON - Estados Unidos
8 Mortensen, Kris Hombre University of California, Davis - Estados Unidos
UNIV CALIF DAVIS - Estados Unidos
9 Brethauer, D. Hombre University of California, Berkeley - Estados Unidos
UNIV CALIF BERKELEY - Estados Unidos
10 Smartt, Stephen J. Hombre Queen's University Belfast - Reino Unido
Queens Univ Belfast - Reino Unido
11 Kasliwal, M. M. - California Institute of Technology - Estados Unidos
CALTECH - Estados Unidos
California Institute of Technology Division of Engineering and Applied Science - Estados Unidos
12 Alexander, K. D. Mujer Northwestern University - Estados Unidos
NORTHWESTERN UNIV - Estados Unidos
13 Anand, Shreya Mujer California Institute of Technology - Estados Unidos
CALTECH - Estados Unidos
California Institute of Technology Division of Engineering and Applied Science - Estados Unidos
14 Berger, E. - Harvard-Smithsonian Center for Astrophysics - Estados Unidos
Ctr Astrophys Harvard & Smithsonian - Estados Unidos
15 Bernardini, Maria Grazia Mujer Osservatorio Astronomico di Brera - Italia
Istituto Nazionale di Astrofisica - Italia
INAF Osservatorio Astron Brera - Italia
16 Bianco, Federica B. Mujer University of Delaware - Estados Unidos
New York University - Estados Unidos
Univ Delaware - Estados Unidos
NYU - Estados Unidos
17 Blanchard, P. K. Hombre Northwestern University - Estados Unidos
NORTHWESTERN UNIV - Estados Unidos
18 Bloom, J. Hombre University of California, Berkeley - Estados Unidos
Lawrence Berkeley National Laboratory - Estados Unidos
UNIV CALIF BERKELEY - Estados Unidos
Lawrence Berkeley Natl Lab - Estados Unidos
19 Brocato, Enzo Hombre Osservatorio Astronomico di Roma - Italia
Istituto Nazionale Di Astrofisica, Rome - Italia
Istituto Nazionale di Astrofisica - Italia
Teramo - Italia
Osservatorio Astronomico di Brera - Italia
INAF Osservatorio Astron Roma - Italia
INAF Osservatorio Astron Brera - Italia
20 Bulla, M. Hombre Stockholms universitet - Suecia
Stockholm Univ - Suecia
21 CARTIER-UGARTE, REGIS ANDRE Hombre Gemini ObservatorySouthern Operations Center - Chile
NSFs Natl Opt Infrared Astron Res Lab - Chile
NOIRLab - Estados Unidos
22 Cenko, S. B. Hombre University of Maryland, College Park - Estados Unidos
NASA Goddard Space Flight Center - Estados Unidos
UNIV MARYLAND - Estados Unidos
NASA Goddard Space Flight Ctr - Estados Unidos
23 Chornock, R. Hombre University of California, Berkeley - Estados Unidos
UNIV CALIF BERKELEY - Estados Unidos
24 Copperwheat, Christopher M. Hombre Liverpool John Moores University - Reino Unido
Liverpool John Moores Univ - Reino Unido
25 Corsi, Alessandra Mujer Texas Tech University - Estados Unidos
TEXAS TECH UNIV - Estados Unidos
26 D'Ammando, F. Hombre Istituto Di Radioastronomia, Bologna - Italia
INAF Ist Radioastron - Italia
27 D'Avanzo, P. Hombre Osservatorio Astronomico di Brera - Italia
Istituto Nazionale di Astrofisica - Italia
INAF Osservatorio Astron Brera - Italia
28 da Costa, L. N. Hombre University of Glasgow - Reino Unido
Univ Glasgow - Reino Unido
29 Foley, R. J. Hombre University of California, Santa Cruz - Estados Unidos
Univ Calif Santa Cruz - Estados Unidos
30 Ghirlanda, G. Hombre Osservatorio Astronomico di Brera - Italia
Istituto Nazionale di Astrofisica - Italia
INAF Osservatorio Astron Brera - Italia
31 Goobar, Ariel Hombre Stockholms universitet - Suecia
Purdue Univ - Estados Unidos
32 Grindlay, Jonathan Hombre Harvard-Smithsonian Center for Astrophysics - Estados Unidos
Ctr Astrophys Harvard & Smithsonian - Estados Unidos
33 Hajela, A. - Northwestern University - Estados Unidos
NORTHWESTERN UNIV - Estados Unidos
34 Holz, D. E. Hombre Department of Physics, The University of Chicago - Estados Unidos
UNIV CHICAGO - Estados Unidos
35 Karambelkar, Viraj - California Institute of Technology - Estados Unidos
CALTECH - Estados Unidos
California Institute of Technology Division of Engineering and Applied Science - Estados Unidos
36 Kool, Erik Hombre Stockholms universitet - Suecia
Stockholm Univ - Suecia
37 Lamb, Gavin P. Hombre University of Leicester - Reino Unido
Univ Leicester - Reino Unido
38 Laskar, T. - Radboud Universiteit - Países Bajos
Radboud Univ Nijmegen - Países Bajos
39 Levan, A. J. Hombre Radboud Universiteit - Países Bajos
Faculty of Science, Engineering and Medicine - Reino Unido
Radboud Univ Nijmegen - Países Bajos
Univ Warwick - Reino Unido
40 Maguire, K. Mujer Trinity College Dublin - Irlanda
Univ Dublin - Irlanda
41 May, Morgan Hombre Columbia University - Estados Unidos
Columbia Univ - Estados Unidos
The Fu Foundation School of Engineering and Applied Science - Estados Unidos
42 Melandri, A. Mujer Osservatorio Astronomico di Brera - Italia
Istituto Nazionale di Astrofisica - Italia
INAF Osservatorio Astron Brera - Italia
43 Milisavljevic, D. Hombre College of Science - Estados Unidos
Purdue Univ - Estados Unidos
44 Miller, A. Hombre Northwestern University - Estados Unidos
NORTHWESTERN UNIV - Estados Unidos
45 Nicholl, M. Hombre University of Birmingham - Reino Unido
Univ Birmingham - Reino Unido
46 Nissanke, Samaya M. - Universiteit van Amsterdam - Países Bajos
Univ Amsterdam - Países Bajos
47 Palmese, A. Mujer University of California, Berkeley - Estados Unidos
UNIV CALIF BERKELEY - Estados Unidos
48 Piranomonte, S. Mujer Osservatorio Astronomico di Roma - Italia
Istituto Nazionale di Astrofisica - Italia
Osservatorio Astronomico di Brera - Italia
INAF Osservatorio Astron Roma - Italia
INAF Osservatorio Astron Brera - Italia
49 Rest, A. Hombre Space Telescope Science Institute - Estados Unidos
Johns Hopkins University - Estados Unidos
Space Telescope Sci Inst - Estados Unidos
Johns Hopkins Univ - Estados Unidos
50 Sagues Carracedo, A. - Stockholms universitet - Suecia
Stockholm Univ - Suecia
51 Siellez, Karelle Mujer CNRS Centre National de la Recherche Scientifique - Francia
CNRS - Francia
52 Singer, L. P. Hombre NASA Goddard Space Flight Center - Estados Unidos
NASA Goddard Space Flight Ctr - Estados Unidos
53 Smith, Matthew Hombre Université Claude Bernard Lyon 1 - Francia
Univ Lyon - Francia
54 Steeghs, D. Hombre Faculty of Science, Engineering and Medicine - Reino Unido
ARC Centre of Excellence for Gravitational Wave Discovery - Australia
Univ Warwick - Reino Unido
OzGrav ARC Ctr Excellence Gravitat Wave Discovery - Australia
55 Tanvir, Nial Hombre University of Leicester - Reino Unido
Univ Leicester - Reino Unido

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

Financiamiento



Fuente
National Science Foundation
NSF
European Research Council
NASA
Swedish Research Council
STFC
Gordon and Betty Moore Foundation
Science and Technology Facilities Council
National Aeronautics and Space Administration
David and Lucile Packard Foundation
Agenzia Spaziale Italiana
European Research Council (ERC) under the European Union
Heising-Simons Foundation
Horizon 2020
Vetenskapsradet
Italian Space Agency
Gordon & Betty Moore Foundation
Alan Turing Institute
Wenner-Gren Foundation
EU H2020 ERC
Wenner-Gren Foundations
Future Investigators in NASA Earth and Space Science and Technology (FINESST) Award
PRIN-MIUR 2017
LSST Corporation
FINESST
NASA Earth and Space Science and Technology
Preparing for Astrophysics with LSST Program - Heising Simons Foundation
G. R.E.A.T research environment - Vetenskapsradet, the Swedish Research Council
Vera C. Rubin Legacy Survey of Space and Time Transient and Variable Stars Science Collaboration

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos



Agradecimiento
Finally, we plan to reevaluate the ToO triggering criteria and observing strategies proposed here at the end of O4 and on a yearly base after the start of Rubin operations. The authors acknowledge the support of the Vera C. Rubin Legacy Survey of Space and Time Transient and Variable Stars Science Collaboration, which provided opportunities for collaboration and exchange of ideas and knowledge, and of Rubin Observatory in the creation and implementation of this work. The authors acknowledge the support of the LSST Corporation, which enabled the organization of many workshops and hackathons throughout the cadence optimization process by directing private funding to these activities.
We thank Lynne Jones for her work on LSST strategy simulations. This paper was created in the nursery of the Rubin LSST Transient and Variable Star Science Collaboration.53 The authors acknowledge the support of the Vera C. Rubin Legacy Survey of Space and Time Transient and Variable Stars Science Collaboration, which provided opportunities for collaboration and exchange of ideas and knowledge, and of Rubin Observatory in the creation and implementation of this work. The authors acknowledge the support of the LSST Corporation, which enabled the organization of many workshops and hackathons throughout the cadence optimization process by directing private funding to these activities. R.M. acknowledges support from the National Science Foundation under grant No. AST-1909796 and AST-1944985, and by the Heising-Simons foundation. M.W.C. acknowledges support from the National Science Foundation with grant Nos. PHY-2010970 and OAC-2117997. A.C. acknowledges support from the NSF award AST #1907975. S.J.S. acknowledges funding from STFC grants ST/T000198/1 and ST/S006109/1. D.M. acknowledges NSF support from grants PHY-1914448 and AST-2037297 K.M. acknowledges support from EU H2020 ERC grant No. 758638. A.H. is partially supported by a Future Investigators in NASA Earth and Space Science and Technology (FINESST) award No. 80NSSC19K1422. M.N. acknowledges support from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program (grant agreement No. 948381) and a Fellowship from the Alan Turing Institute. P.D.'A. acknowledges support from PRIN-MIUR 2017 (grant 20179ZF5KS) and from the Italian Space Agency, contract ASI/INAF No. I/004/11/4. E.C.K. and A.G. acknowledge support from the G. R.E.A.T research environment funded by Vetenskapsradet, the Swedish Research Council, under project No. 2016-06012, and support from The Wenner-Gren Foundations. M.B. acknowledges support from the Swedish Research Council (Reg. No. 2020-03330). The UCSC team is supported in part by NASA grant NNG17PX03C, NSF grant AST-1815935, the Gordon & Betty Moore Foundation, the Heising-Simons Foundation, and by a fellowship from the David and Lucile Packard Foundation to R.J.F. This work was supported by the Preparing for Astrophysics with LSST Program, funded by the Heising Simons Foundation through grant 2021-2975, and administered by Las Cumbres Observatory.

Muestra la fuente de financiamiento declarada en la publicación.