The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. I. Discovery of the Optical Counterpart Using the Dark Energy Camera
Fermi National Accelerator Laboratory · Brandeis University · +63 more institutions
Abstract
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 deg 2 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 from the nucleus of NGC 4993 at redshift z = 0.0098, consistent (for km s −1 Mpc −1 ) with the distance of 40 ± 8 Mpc reported by the LIGO Scientific Collaboration…
Citation impact
- FWCI
- 50.06
- Percentile
- 100%
- References
- 66
Authors
146Topics & keywords
- Physics
- Kilonova
- Astrophysics
- LIGO
- Neutron star
- Gravitational wave
- Astronomy
- Absolute magnitude
Funding
- NSNational Science FoundationAwards: 1518052, FPA2015-68048, PHY-1151836, AYA2015-71825, AST-1518052, 1536171, 1708081, AST-1536171, SEV-2016-0597, 1125897, DE-AC02-07CH11359, 1411763, 1714498, 1151836, CAREER, MDM-2015-0509, PHY-1125897, 1138766, AST-1138766, AST-1714498
- UDU.S. Department of EnergyAwards: DE-AC02-07CH11359, AC02-07CH11359, DE-AC02, DE-AC02-
- NANational Aeronautics and Space AdministrationAwards: NNX16AC22G, NNX15AE50G
- APAlfred P. Sloan Foundation
- GAGordon and Betty Moore Foundation
- UOUniversity of California, Santa Cruz
- UOUniversity of Pennsylvania
- OSOhio State University
- UOUniversity of ChicagoAward: PHY-1125897
- UOUniversity of Portsmouth
- NCNational Centre for Supercomputing Applications
- UCUniversity College London
- UOUniversity of Sussex
- NRNational Research Foundation
- DFDeutsche ForschungsgemeinschaftAwards: DE-AC02-07CH11359, SEV-2016-0597, AST-1536171, AST-1138766
- DGDanmarks Grundforskningsfond
- ETEidgenössische Technische Hochschule Zürich
- MDMinisterio de Economía y CompetitividadAwards: -2015-0509, SEV-2016-0597, SEV-2012-0234, AYA2015-71825, ESP2015-88861, FPA2015-68048, MDM-2015-0509
- CNConselho Nacional de Desenvolvimento Científico e TecnológicoAward: SEV-2016-0597
- FCFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro
- FDFinanciadora de Estudos e Projetos
- MDMinisterio de Ciencia e InnovaciónAwards: SEV-2012-0234, FPA2015-68048, FPA2015-, MDM-2015-0509, AYA2015-71825, SEV-2016-0597, ESP2015-88861
- ACARC Centre of Excellence for All-Sky AstrophysicsAward: CE110001020
- IDInstitut de Física d'Altes Energies
- UOUniversity of Illinois at Urbana-Champaign
- OOOffice of ScienceAwards: DE-AC02, DE-AC02-07CH11359
- 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, DE-AC02-07CH11359, ST/L006529/1, ST/L000652/1, ST/H001581/1, ST/N001087/1, ST/M003574/1, ST/M001334/1
- CDCentro de Investigaciones Energéticas, Medioambientales y TecnológicasAward: MDM-2015-0509
- HEHigh Energy Physics
- IEIntegrated Electronics Engineering Center, Binghamton University
- ANArgonne National LaboratoryAward: DE-AC02
- FFermilab
- LBLawrence Berkeley National LaboratoryAward: DE-AC02-07CH11359
- SNSLAC National Accelerator Laboratory