학술논문

Searching the Gamma-ray Sky for Counterparts to Gravitational Wave Sources: Fermi GBM and LAT Observations of LVT151012 and GW151226
Document Type
Working Paper
Author
Racusin, J. L.Burns, E.Goldstein, A.Connaughton, V.Wilson-Hodge, C. A.Jenke, P.Blackburn, L.Briggs, M. S.Broida, J.Camp, J.Christensen, N.Hui, C. M.Littenberg, T.Shawhan, P.Singer, L.Veitch, J.Bhat, P. N.Cleveland, W.Fitzpatrick, G.Gibby, M. H.von Kienlin, A.McBreen, S.Mailyan, B.Meegan, C. A.Paciesas, W. S.Preece, R. D.Roberts, O. J.Stanbro, M.Veres, P.Zhang, B. -B.Ackermann, M.Albert, A.Atwood, W. B.Axelsson, M.Baldini, L.Ballet, J.Barbiellini, G.Baring, M. G.Bastieri, D.Bellazzini, R.Bissaldi, E.Blandford, R. D.Bloom, E. D.Bonino, R.Bregeon, J.Bruel, P.Buson, S.Caliandro, G. A.Cameron, R. A.Caputo, R.Caragiulo, M.Caraveo, P. A.Cavazzuti, E.Charles, E.Chiang, J.Ciprini, S.Costanza, F.Cuoco, A.Cutini, S.D'Ammando, F.de Palma, F.Desiante, R.Digel, S. W.Di Lalla, N.Di Mauro, M.Di Venere, L.Drell, P. S.Favuzzi, C.Ferrara, E. C.Focke, W. B.Fukazawa, Y.Funk, S.Fusco, P.Gargano, F.Gasparrini, D.Giglietto, N.Gill, R.Giroletti, M.Glanzman, T.Granot, J.Green, D.Grove, J. E.Guillemot, L.Guiriec, S.Harding, A. K.Jogler, T.Johannesson, G.Kamae, T.Kensei, S.Kocevski, D.Kuss, M.Larsson, S.Latronico, L.Li, J.Longo, F.Loparco, F.Lubrano, P.Magill, J. D.Maldera, S.Malyshev, D.McEnery, J. E.Michelson, P. F.Mizuno, T.Morselli, A.Moskalenko, I. V.Negro, M.Nuss, E.Omodei, N.Orienti, M.Orlando, E.Ormes, J. F.Paneque, D.Perkins, J. S.Pesce-Rollins, M.Piron, F.Pivato, G.Porter, T. A.Principe, G.Raino, S.Rando, R.Razzano, M.Razzaque, S.Reimer, A.Reimer, O.Parkinson, P. M. SazScargle, J. D.Sgro, C.Simone, D.Siskind, E. J.Smith, D. A.Spada, F.Spinelli, P.Suson, D. J.Tajima, H.Thayer, J. B.Torres, D. F.Troja, E.Uchiyama, Y.Vianello, G.Wood, K. S.Wood, M.
Source
Subject
Astrophysics - High Energy Astrophysical Phenomena
Language
Abstract
We present the Fermi Gamma-ray Burst Monitor (GBM) and Large Area Telescope (LAT) observations of the LIGO binary black hole merger event GW151226 and candi- date LVT151012. No candidate electromagnetic counterparts were detected by either the GBM or LAT. We present a detailed analysis of the GBM and LAT data over a range of timescales from seconds to years, using automated pipelines and new techniques for char- acterizing the upper limits across a large area of the sky. Due to the partial GBM and LAT coverage of the large LIGO localization regions at the trigger times for both events, dif- ferences in source distances and masses, as well as the uncertain degree to which emission from these sources could be beamed, these non-detections cannot be used to constrain the variety of theoretical models recently applied to explain the candidate GBM counterpart to GW150914.
Comment: 27 pages, 1 table, 11 figures, Submitted to ApJ