A Dark Energy Camera Search for an Optical Counterpart to the First Advanced LIGO Gravitational Wave Event GW150914
- Fermilab
- Chicago U., KICP
- Harvard-Smithsonian Ctr. Astrophys.
- Pennsylvania U.
- Illinois U., Urbana, Astron. Dept.; Illinois U., Urbana
- Fermilab; Chicago U., KICP
- Johns Hopkins U.
- Sao Paulo, IFT
- Cerro-Tololo InterAmerican Obs.
- University Coll. London; Rhodes U.
- Princeton U.
- Cambridge U., Inst. of Astron.; Cambridge U., KICC
- Paris, Inst. Astrophys.; University Coll. London
- Carnegie Inst. Observ.
- Paris, Inst. Astrophys.
- Syracuse U.
- KIPAC, Menlo Park; SLAC
- Portsmouth U., ICG
- LIneA, Rio de Janeiro; Rio de Janeiro Observ.
- Barcelona, IEEC; Barcelona, IFAE
- Barcelona, IEEC
- NASA, Goddard; Maryland U.
- Ohio U.
- Portsmouth U., ICG; Southampton U.
- Munich, Tech. U., Universe; Munich U.
- Pennsylvania U.; Caltech
- U. Michigan, Dept. Astron.; Michigan U.
- Cardiff U.
- Barcelona, IFAE
- Arizona U.
- Penn State U.
- Los Alamos
- Madrid, CIEMAT
- Michigan U.
- UC, Berkeley; LBL, Berkeley
- Ohio State U., CCAPP; Ohio State U.
- Illinois U., Urbana
- Australia, CSIRO, North Ryde
- University Coll. London
- Texas A-M
- Sao Paulo U.; LIneA, Rio de Janeiro
- New York U., CCPP
- Ohio State U., CCAPP; Ohio State U., Dept. Astron.
- NOAO, Tucson
- Columbia U.
- ICREA, Barcelona; Barcelona, IFAE
- Munich, Tech. U., Universe; Munich U.; Garching, Max Planck Inst., MPE
- Caltech
- UC, Berkeley
- Sussex U.
- SLAC
- Madrid, CIEMAT; Illinois U., Urbana, Astron. Dept.
- Brookhaven
- Southampton U.
- LBL, Berkeley
- Argonne
- Stanford U., Phys. Dept.; KIPAC, Menlo Park; SLAC
- Munich, Tech. U., Universe; Garching, Max Planck Inst., MPE; Munich U.
We report the results of a deep search for an optical counterpart to the gravitational wave (GW) event GW150914, the first trigger from the Advanced LIGO GW detectors. We used the Dark Energy Camera (DECam) to image a 102 deg(2) area, corresponding to 38% of the initial trigger high-probability sky region and to 11% of the revised high-probability region. We observed in the i and z bands at 4–5, 7, and 24 days after the trigger. The median 5σ point-source limiting magnitudes of our search images are i = 22.5 and z = 21.8 mag. We processed the images through a difference-imaging pipeline using templates from pre-existing Dark Energy Survey data and publicly available DECam data. Due to missing template observations and other losses, our effective search area subtends 40 deg(2), corresponding to a 12% total probability in the initial map and 3% in the final map. In this area, we search for objects that decline significantly between days 4–5 and day 7, and are undetectable by day 24, finding none to typical magnitude limits of i = 21.5, 21.1, 20.1 for object colors (i − z) = 1, 0, −1, respectively. Our search demonstrates the feasibility of a dedicated search program with DECam and bodes well for future research in this emerging field.
- Research Organization:
- Portsmouth U., ICG; Illinois U., Urbana; Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States); Ohio State U., Dept. Astron.; Ohio State U.; NASA, Goddard; Princeton U.; U. Michigan, Dept. Astron.; Brookhaven National Laboratory (BNL), Upton, NY (United States); LIneA, Rio de Janeiro; Southampton U.; Cardiff U.; Paris, Inst. Astrophys.; Sao Paulo, IFT; Barcelona, IFAE; Cambridge U., KICC; Cambridge U., Inst. of Astron.; Maryland U.; Ohio State U., CCAPP; Stanford U., Phys. Dept.; Texas A-M; Los Alamos National Laboratory (LANL), Los Alamos, NM (United States); NOAO, Tucson; Madrid, CIEMAT; ICREA, Barcelona; Illinois U., Urbana, Astron. Dept.; Ohio U.; Argonne National Laboratory (ANL), Argonne, IL (United States); Harvard-Smithsonian Ctr. Astrophys.; Cerro-Tololo InterAmerican Obs.; Rio de Janeiro Observ.; New York U., CCPP; Arizona U.; Columbia U.; Barcelona, IEEC; Penn State U.; Chicago U., KICP; Johns Hopkins U.; Garching, Max Planck Inst., MPE; UC, Berkeley; Pennsylvania U.; Sussex U.; Syracuse U.; Sao Paulo U.; Caltech; Rhodes U.; Australia, CSIRO, North Ryde; Michigan U.; Munich U.; Carnegie Inst. Observ.; Munich, Tech. U., Universe; Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); University Coll. London
- Sponsoring Organization:
- US Department of Energy
- Grant/Contract Number:
- AC02-07CH11359
- OSTI ID:
- 1253580
- Report Number(s):
- FERMILAB-PUB-16-031-AE-PPD; oai:inspirehep.net:1421418; arXiv:1602.04198
- Journal Information:
- Astrophys.J.Lett., Journal Name: Astrophys.J.Lett. Journal Issue: 2 Vol. 823
- Country of Publication:
- United States
- Language:
- English
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