Implications for the Origin of GRB 070201 from LIGO Observations
- LIGO California Institute of Technology, Pasadena, CA 91125 (United States)
- Albert-Einstein-Institut, Max-Planck-Institut fuer Gravitationsphysik, D-30167 Hannover (Germany)
- Louisiana State University, Baton Rouge, LA 70803 (United States)
- University of Wisconsin, Milwaukee, WI 53201 (United States)
- University of Florida, Gainesville, FL 32611 (United States)
- Australian National University, Canberra, ACT 0200 (Australia)
- University of Birmingham, Birmingham B15 2TT (United Kingdom)
- Universitaet Hannover, D-30167 Hannover (Germany)
- Albert-Einstein-Institut, Max-Planck-Institut fuer Gravitationsphysik, D-14476 Golm (Germany)
- Carleton College, Northfield, MN 55057 (United States)
We analyzed the available LIGO data coincident with GRB 070201, a short-duration, hard-spectrum {gamma}-ray burst (GRB) whose electromagnetically determined sky position is coincident with the spiral arms of the Andromeda galaxy (M31). Possible progenitors of such short, hard GRBs include mergers of neutron stars or a neutron star and a black hole, or soft {gamma}-ray repeater (SGR) flares. These events can be accompanied by gravitational-wave emission. No plausible gravitational-wave candidates were found within a 180 s long window around the time of GRB 070201. This result implies that a compact binary progenitor of GRB 070201, with masses in the range 1 M{sub sun} < m{sub 1} < 3 M{sub sun} and 1 M{sub sun} < m{sub 2} < 40 M{sub sun}, located in M31 is excluded at >99% confidence. If the GRB 070201 progenitor was not in M31, then we can exclude a binary neutron star merger progenitor with distance D < 3.5 Mpc, assuming random inclination, at 90% confidence. The result also implies that an unmodeled gravitational-wave burst from GRB 070201 most probably emitted less than 4.4 x 10{sup -4} M{sub sun}c{sup 2} (7.9 x 10{sup 50} ergs) in any 100 ms long period within the signal region if the source was in M31 and radiated isotropically at the same frequency as LIGO's peak sensitivity (f {approx} 150 Hz). This upper limit does not exclude current models of SGRs at the M31 distance.
- OSTI ID:
- 21255759
- Journal Information:
- Astrophysical Journal, Vol. 681, Issue 2; Other Information: DOI: 10.1086/587954; Country of input: International Atomic Energy Agency (IAEA); ISSN 0004-637X
- Country of Publication:
- United States
- Language:
- English
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