Observation results by the TAMA300 detector on gravitational wave bursts from stellar-core collapses

被引：21

作者：

Ando, M ^{[1
]}

Arai, K

Aso, Y

Beyersdorf, P

Hayama, K

Iida, Y

Kanda, N

Kawamura, S

Kondo, K

Mio, N

Miyoki, S

Moriwaki, S

Nagano, S

Numata, K

Sato, S

Somiya, K

Tagoshi, H

Takahashi, H

Takahashi, R

Tatsumi, D

Tsunesada, Y

Zhu, ZH

Akutsu, T

Araya, A

Asada, H

Barton, MA

Fujiki, Y

Fujimoto, MK

Fujita, R

Fukushima, M

Futamase, T

Hamuro, Y

Haruyama, T

Hayakawa, H

Heinzel, G

Horikoshi, G

Iguchi, H

Ioka, K

Ishitsuka, H

Kamikubota, N

Kaneyama, T

Karasawa, Y

Kasahara, K

Kasai, T

Katsuki, M

Kawabe, K

Kawamura, M

Kawashima, N

Kawazoe, F

机构：

[1] Univ Tokyo, Dept Phys, Bunkyo Ku, Tokyo 1130033, Japan

[2] Natl Astron Observ, Tokyo 1818588, Japan

[3] Univ Tokyo, Dept Astron, Bunkyo Ku, Tokyo 1130033, Japan

[4] Osaka City Univ, Grad Sch Sci, Sumiyoshi Ku, Osaka 5588585, Japan

[5] Univ Tokyo, Inst Cosm Ray Res, Chiba 2778582, Japan

[6] Univ Tokyo, Dept Adv Mat Sci, Chiba 2778561, Japan

[7] Natl Inst Informat & Commun Technol, Tokyo 1848795, Japan

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

[9] Osaka Univ, Grad Sch Sci, Osaka 5600043, Japan

[10] Niigata Univ, Fac Sci, Niigata 9502102, Japan

[11] Univ Tokyo, Earthquake Res Inst, Bunkyo Ku, Tokyo 1130032, Japan

[12] Hirosaki Univ, Fac Sci & Technol, Hirosaki, Aomori 0368561, Japan

[13] Tohoku Univ, Grad Sch Sci, Sendai, Miyagi 9808578, Japan

[14] High Energy Accelerator Res Org, Tsukuba, Ibaraki 3050801, Japan

[15] Max Planck Inst Gravitat Phys, D-30167 Hannover, Germany

[16] Tokyo Inst Technol, Meguro Ku, Tokyo 1528551, Japan

[17] Penn State Univ, Dept Phys, University Pk, PA 16802 USA

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

[19] Kyoto Univ, Fac Sci, Sakyo Ku, Kyoto 6068502, Japan

[20] Kinki Univ, Osaka 5778502, Japan

[21] Ochanomizu Univ, Bunkyo Ku, Tokyo 1128610, Japan

[22] Hiroshima Univ, Dept Phys, Hiroshima 7398526, Japan

[23] Univ Tokyo, Dept Phys, Theoret Astrophys Grp, Bunkyo Ku, Tokyo 1130033, Japan

[24] Tokyo Denki Univ, Chiyoda Ku, Tokyo 1018457, Japan

[25] Miyagi Univ Educ, Dept Phys, Sendai, Miyagi 9800845, Japan

[26] CALTECH, Pasadena, CA 91125 USA

[27] Univ Electrocommun, Inst Laser Sci, Tokyo 1828585, Japan

[28] Kyoto Univ, Yukawa Inst Theoret Phys, Sakyo Ku, Kyoto 6068502, Japan

[29] Tokai Univ, Fac Engn, Div Precis Engn, Kanagawa 2591292, Japan

[30] Waseda Univ, Shinjyuku Ku, Tokyo 1698555, Japan

[31] Univ Tokyo, Grad Sch Arts & Sci, Meguro Ku, Tokyo 1538902, Japan

[32] RIKEN, Wako, Saitaka 3510198, Japan

[33] Univ Illinois, Dept Phys, Urbana, IL 61801 USA

[34] Natl Inst Adv Ind Sci & Technol, Tsukuba, Ibaraki 3058563, Japan

[35] ISAS, JAXA, Kanagawa 2298510, Japan

来源：

PHYSICAL REVIEW D | 2005年 / 71卷 / 08期

关键词：

D O I：

10.1103/PhysRevD.71.082002

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present data-analysis schemes and results of observations with the TAMA300 gravitational wave detector, targeting burst signals from stellar-core collapse events. In analyses for burst gravitational waves, the detection and fake-reduction schemes are different from well-investigated ones for a chirp wave analysis, because precise waveform templates are not available. We used an excess -power filter for the extraction of gravitational wave candidates, and developed two methods for the reduction of fake events caused by nonstationary noises of the detector. These analysis schemes were applied to real data from the TAMA300 interferometric gravitational wave detector. As a result, fake events were reduced by a factor of about 1000 in the best cases. In addition, in order to interpret the event candidates from an astronomical viewpoint, we performed a Monte-Carlo simulation with an assumed Galactic event distribution model and with burst waveforms obtained from numerical simulations of stellar-core collapses. We set an upper limit of 5.0x10(3) events/sec on the burst gravitational wave event rate in our Galaxy with a confidence level of 90%. This work shows prospects on the search for burst gravitational waves, by establishing an analysis scheme for the observation data from an interferometric gravitational wave detector.

引用

页码：1 / 17

页数：17

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