The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. II. UV, Optical, and Near-infrared Light Curves and Comparison to Kilonova Models
Center for Astrophysics Harvard & Smithsonian · Columbia University · +61 more institutions
Abstract
We present the Dark Energy Camera (DECam) discovery of the optical counterpart of the first binary neutron star merger detected through gravitational-wave emission, GW170817. Our observations commenced 10.5 hr post-merger, as soon as the localization region became accessible from Chile. We imaged 70 deg2 in the i and z bands, covering 93% of the initial integrated localization probability, to a depth necessary to identify likely optical counterparts (e.g., a kilonova). At 11.4 hr post-merger we detected a bright optical transient located 10.6 from the nucleus of NGC 4993 at redshift z=0.0098, consistent (for H0 = 70 km s−1 Mpc−1) with the distance of 40±8 Mpc reported by the LIGO Scientific Collaboration and…
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- 88.09
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- 100%
- References
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Authors
144Topics & keywords
- Physics
- Kilonova
- Astrophysics
- Neutron star
- LIGO
- Photometry (optics)
- Light curve
- Spectral energy distribution
Funding
- NSNational Science FoundationAwards: 1518052, PHY-1707954, AST-1518052, DGE 1144152, 1707954, 1411763, 1714498, 1144152, AST-1714498
- UDU.S. Department of Energy
- NANational Aeronautics and Space AdministrationAwards: NNX16AC22G, NNX15AE50G
- APAlfred P. Sloan Foundation
- GAGordon and Betty Moore FoundationAward: GBMF5076
- UOUniversity of California, Santa Cruz
- UOUniversity of Pennsylvania
- OSOhio State University
- UOUniversity of Portsmouth
- NCNational Centre for Supercomputing Applications
- UCUniversity College London
- UOUniversity of Sussex
- NRNational Research Foundation
- DFDeutsche Forschungsgemeinschaft
- DGDanmarks Grundforskningsfond
- ETEidgenössische Technische Hochschule Zürich
- MDMinisterio de Ciencia, Tecnología e Innovación Productiva
- MDMinistério da Ciência, Tecnologia e Inovação
- CNConselho Nacional de Desenvolvimento Científico e Tecnológico
- FCFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro
- FDFinanciadora de Estudos e Projetos
- IDInstitut de Física d'Altes Energies
- UOUniversity of Illinois at Urbana-Champaign
- CFCenter for Cosmology and Astroparticle Physics, Ohio State University
- KIKavli Institute for Cosmological Physics, University of Chicago
- SAScience and Technology Facilities CouncilAwards: ST/I000976/1, ST/N000668/1, ST/P000525/1, ST/N000927/1, ST/L006529/1, ST/L000652/1, ST/H001581/1, ST/N001087/1, ST/M003574/1, ST/M001334/1
- CNComisión Nacional de Investigación Científica y Tecnológica
- CDCentro de Investigaciones Energéticas, Medioambientales y Tecnológicas
- IEIntegrated Electronics Engineering Center, Binghamton University
- ANArgonne National Laboratory
- FFermilab
- LBLawrence Berkeley National Laboratory
- SNSLAC National Accelerator Laboratory