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Title: A Dark Energy Camera Search for an Optical Counterpart to the First Advanced LIGO Gravitational Wave Event GW150914

Journal Article · · Astrophys.J.Lett.
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  1. Fermilab
  2. Chicago U., KICP
  3. Harvard-Smithsonian Ctr. Astrophys.
  4. Pennsylvania U.
  5. Illinois U., Urbana, Astron. Dept.; Illinois U., Urbana
  6. Fermilab; Chicago U., KICP
  7. Johns Hopkins U.
  8. Sao Paulo, IFT
  9. Cerro-Tololo InterAmerican Obs.
  10. University Coll. London; Rhodes U.
  11. Princeton U.
  12. Cambridge U., Inst. of Astron.; Cambridge U., KICC
  13. Paris, Inst. Astrophys.; University Coll. London
  14. Carnegie Inst. Observ.
  15. Paris, Inst. Astrophys.
  16. Syracuse U.
  17. KIPAC, Menlo Park; SLAC
  18. Portsmouth U., ICG
  19. LIneA, Rio de Janeiro; Rio de Janeiro Observ.
  20. Barcelona, IEEC; Barcelona, IFAE
  21. Barcelona, IEEC
  22. NASA, Goddard; Maryland U.
  23. Ohio U.
  24. Portsmouth U., ICG; Southampton U.
  25. Munich, Tech. U., Universe; Munich U.
  26. Pennsylvania U.; Caltech
  27. U. Michigan, Dept. Astron.; Michigan U.
  28. Cardiff U.
  29. Barcelona, IFAE
  30. Arizona U.
  31. Penn State U.
  32. Los Alamos
  33. Madrid, CIEMAT
  34. Michigan U.
  35. UC, Berkeley; LBL, Berkeley
  36. Ohio State U., CCAPP; Ohio State U.
  37. Illinois U., Urbana
  38. Australia, CSIRO, North Ryde
  39. University Coll. London
  40. Texas A-M
  41. Sao Paulo U.; LIneA, Rio de Janeiro
  42. New York U., CCPP
  43. Ohio State U., CCAPP; Ohio State U., Dept. Astron.
  44. NOAO, Tucson
  45. Columbia U.
  46. ICREA, Barcelona; Barcelona, IFAE
  47. Munich, Tech. U., Universe; Munich U.; Garching, Max Planck Inst., MPE
  48. Caltech
  49. UC, Berkeley
  50. Sussex U.
  51. SLAC
  52. Madrid, CIEMAT; Illinois U., Urbana, Astron. Dept.
  53. Brookhaven
  54. Southampton U.
  55. LBL, Berkeley
  56. Argonne
  57. Stanford U., Phys. Dept.; KIPAC, Menlo Park; SLAC
  58. 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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