Implications for the origin of GRB 070201 from LIGO observations

被引：129

作者：

Abbott, B. ^{[1
]}

Abbott, R. ^{[1
]}

Adhikari, R. ^{[1
]}

Agresti, J. ^{[1
]}

Ajith, P. ^{[2
]}

Allen, B. ^{[2
,3
]}

Amin, R. ^{[4
]}

Anderson, S. B. ^{[1
]}

Anderson, W. G. ^{[3
]}

Arain, M. ^{[5
]}

Araya, M. ^{[1
]}

Armandula, H. ^{[1
]}

Ashley, M. ^{[6
]}

Aston, S. ^{[7
]}

Aufmuth, P. ^{[8
]}

Aulbert, C. ^{[9
]}

Babak, S. ^{[9
]}

Ballmer, S. ^{[1
]}

Bantilan, H. ^{[10
]}

Barish, B. C. ^{[1
]}

Barker, C. ^{[11
]}

Barker, D. ^{[11
]}

Barr, B. ^{[12
]}

Barriga, P. ^{[13
]}

Barton, M. A. ^{[12
]}

Bayer, K. ^{[14
]}

Betzwieser, J. ^{[14
]}

Beyersdorf, P. T. ^{[15
]}

Bhawal, B. ^{[1
]}

Bilenko, I. A. ^{[16
]}

Billingsley, G. ^{[1
]}

Biswas, R. ^{[3
]}

Black, E. ^{[1
]}

Blackburn, K. ^{[1
]}

Blackburn, L. ^{[14
]}

Blair, D. ^{[13
]}

Bland, B. ^{[11
]}

Bogenstahl, J. ^{[12
]}

Bogue, L. ^{[17
]}

Bork, R. ^{[1
]}

Boschi, V. ^{[1
]}

Bose, S. ^{[18
]}

Brady, P. R. ^{[3
]}

Braginsky, V. B. ^{[16
]}

Brau, J. E. ^{[19
]}

Brinkmann, M. ^{[2
]}

Brooks, A. ^{[20
]}

Brown, D. A. ^{[1
,21
]}

Bullington, A. ^{[22
]}

Bunkowski, A. ^{[2
]}

机构：

[1] LIGO Calif Inst Technol, Pasadena, CA 91125 USA

[2] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-30167 Hannover, Germany

[3] Univ Wisconsin, Milwaukee, WI 53201 USA

[4] Louisiana State Univ, Baton Rouge, LA 70803 USA

[5] Univ Florida, Gainesville, FL 32611 USA

[6] Australian Natl Univ, Canberra, ACT 0200, Australia

[7] Univ Birmingham, Birmingham B15 2TT, England

[8] Leibniz Univ Hannover, D-30167 Hannover, Germany

[9] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-14476 Golm, Germany

[10] Carleton Coll, Northfield, MN 55057 USA

[11] LIGO Hanford Observ, Richland, WA 99352 USA

[12] Univ Glasgow, Glasgow G12 8QQ, Lanark, Scotland

[13] Univ Western Australia, Crawley, WA 6009, Australia

[14] LIGO Massachusetts Inst Technol, Cambridge, MA 02139 USA

[15] San Jose State Univ, San Jose, CA 95192 USA

[16] Moscow MV Lomonosov State Univ, Moscow 119992, Russia

[17] LIGO Livingston Observ, Livingston, LA 70754 USA

[18] Washington State Univ, Pullman, WA 99164 USA

[19] Univ Oregon, Eugene, OR 97403 USA

[20] Univ Adelaide, Adelaide, SA 5005, Australia

[21] CALTECH, CaRT, Pasadena, CA USA

[22] Stanford Univ, Stanford, CA 94305 USA

[23] Univ Maryland, College Pk, MD 20742 USA

[24] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA

[25] Univ Sannio Benevento, I-82100 Benevento, Italy

[26] Charles Sturt Univ, Wagga Wagga, NSW 2678, Australia

[27] Univ Salerno, I-84084 Fisciano, Salerno, Italy

[28] Cardiff Univ, Cardiff CF24 3AA, England

[29] Syracuse Univ, Syracuse, NY 13244 USA

[30] Univ Michigan, Ann Arbor, MI 48109 USA

[31] Penn State Univ, University Pk, PA 16802 USA

[32] Inter Univ Ctr Astron & Astrophys, Pune 411007, Maharashtra, India

[33] Univ Texas Brownsville, Brownsville, TX 78520 USA

[34] So Univ, Baton Rouge, LA 70813 USA

[35] Columbia Univ, New York, NY 10027 USA

[36] Univ Rochester, Rochester, NY 14627 USA

[37] Rutherford Appleton Lab, Didcot OX11 0QX, Oxon, England

[38] Embry Riddle Aeronaut Univ, Prescott, AZ 86301 USA

[39] Univ Southampton, Southampton SO17 1BJ, Hants, England

[40] NW Univ, Evanston, IL 60208 USA

[41] Natl Astron Observ Japan, Tokyo 1818588, Japan

[42] Univ Strathclyde, Glasgow G1 1XQ, Lanark, Scotland

[43] Loyola Univ, New Orleans, LA 70118 USA

[44] Hobart & William Smith Coll, Geneva, NY 14456 USA

[45] Univ Illes Balears, E-07122 Palma de Mallorca, Spain

[46] Rochester Inst Technol, Rochester, NY 14623 USA

[47] Andrews Univ, Berrien Springs, MI 49104 USA

[48] Trinity Univ, San Antonio, TX 78212 USA

[49] SE Louisiana Univ, Hammond, LA 70402 USA

[50] Louisiana Tech Univ, Ruston, LA 71272 USA

来源：

ASTROPHYSICAL JOURNAL | 2008年 / 681卷 / 02期

基金：

美国国家科学基金会; 英国科学技术设施理事会;

关键词：

gamma rays : bursts; gravitational waves; methods : data analysis;

D O I：

10.1086/587954

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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-circle dot < m(1) < 3 M-circle dot and 1 M-circle dot < m(2) < 40 M-circle dot, 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; 10(-4) M(circle dot)c(2) (7.9 x 10(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 approximate to 150 Hz). This upper limit does not exclude current models of SGRs at the M31 distance.

引用

页码：1419 / 1430

页数：12

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