On the Interpretation of the Fermi-GBM Transient Observed in Coincidence with LIGO Gravitational-wave Event GW150914

被引:33
作者
Connaughton, V. [1 ]
Burns, E. [2 ,17 ]
Goldstein, A. [1 ,3 ]
Blackburn, L. [4 ]
Briggs, M. S. [5 ,6 ]
Christensen, N. [7 ,8 ]
Hui, C. M. [9 ]
Kocevski, D. [9 ]
Littenberg, T. [9 ]
McEnery, J. E. [2 ]
Racusin, J. [2 ]
Shawhan, P. [10 ]
Veitch, J. [11 ]
Wilson-Hodge, C. A. [9 ]
Bhat, P. N. [6 ]
Bissaldi, E. [12 ]
Cleveland, W. [1 ]
Giles, M. M. [13 ]
Gibby, M. H. [13 ]
von Kienlin, A. [14 ]
Kippen, R. M. [15 ]
McBreen, S. [16 ]
Meegan, C. A. [6 ]
Paciesas, W. S. [1 ]
Preece, R. D. [5 ]
Roberts, O. J. [1 ]
Stanbro, M. [5 ]
Veres, P. [6 ]
机构
[1] Univ Space Res Assoc, 320 Sparkman Dr, Huntsville, AL 35805 USA
[2] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[3] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
[4] MIT, LIGO, 77 Massachusetts Ave, Cambridge, MA 02139 USA
[5] Univ Alabama, Dept Space Sci, 320 Sparkman Dr, Huntsville, AL 35805 USA
[6] Univ Alabama, CSPAR, 320 Sparkman Dr, Huntsville, AL 35805 USA
[7] Carleton Coll, Phys & Astron, Northfield, MN USA
[8] Univ Cote Azur, Observ Cote Azur, CNRS, Artemis, CS 34229, F-06304 Nice 4, France
[9] NASA, Astrophys Off, Marshall Space Flight Ctr, ST12, Huntsville, AL 35812 USA
[10] Univ Maryland, Dept Phys, College Pk, MD 20742 USA
[11] Ist Nazl Fis Nucl, Sez Bari, I-70126 Bari, Italy
[12] Politecn Bari, Dipartimento Fis, I-70125 Bari, Italy
[13] Jacobs Technol Inc, Huntsville, AL USA
[14] Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany
[15] Los Alamos Natl Lab, Los Alamos, NM 87545 USA
[16] Univ Coll Dublin, Sch Phys, Stillorgan Rd, Dublin 4, Ireland
[17] USRA, Mountain View, CA USA
关键词
gamma-ray burst: individual (GW150914-GBM); gravitational waves; methods: data analysis; stars: black holes;
D O I
10.3847/2041-8213/aaa4f2
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The weak transient detected by the Fermi Gamma-ray Burst Monitor (GBM) 0.4. s after GW150914 has generated much speculation regarding its possible association with the black hole binary merger. Investigation of the GBM data by Connaughton et al. revealed a source location consistent with GW150914 and a spectrum consistent with a weak, short gamma-ray burst. Greiner et al. present an alternative technique for fitting background-limited data in the low-count regime, and call into question the spectral analysis and the significance of the detection of GW150914-GBM presented in Connaughton et al. The spectral analysis of Connaughton et al. is not subject to the limitations of the low-count regime noted by Greiner et al. We find Greiner et al. used an inconsistent source position and did not follow the steps taken in Connaughton et al. to mitigate the statistical shortcomings of their software when analyzing this weak event. We use the approach of Greiner et al. to verify that our original spectral analysis is not biased. The detection significance of GW150914-GBM is established empirically, with a false-alarm rate (FAR) of similar to 10(-4) Hz. A post-trials false-alarm probability (FAP) of 2.2 x 10(-3) (2.9 sigma) of this transient being associated with GW150914 is based on the proximity in time to the gravitational-wave event of a transient with that FAR. The FAR and the FAP are unaffected by the spectral analysis that is the focus of Greiner et al.
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页数:9
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