J-GEM optical and near-infrared follow-up of gravitational wave events during LIGO's and Virgo's third observing run

被引:6
|
作者
Sasada, Mahito [1 ,2 ]
Utsumi, Yousuke [3 ]
Itoh, Ryosuke [4 ]
Tominaga, Nozomu [5 ,6 ]
Tanaka, Masaomi [7 ]
Morokuma, Tomoki [8 ]
Yanagisawa, Kenshi [1 ,9 ]
Kawabata, Koji S. [1 ]
Ohgami, Takayuki [5 ]
Yoshida, Michitoshi [10 ]
Abe, Fumio [11 ]
Adachi, Ryo [12 ]
Akitaya, Hiroshi [1 ]
Chong, Yang [13 ]
Daikuhara, Kazuki [7 ,14 ]
Hamasaki, Ryo [5 ]
Honda, Satoshi [15 ]
Hosokawa, Ryohei [12 ]
Iida, Kota [12 ]
Imazato, Fumiya [13 ]
Ishioka, Chihiro [16 ]
Iwasaki, Takumi [5 ]
Jian, Mingjie [17 ]
Kamei, Yuhei [11 ]
Kanai, Takahiro [14 ]
Kaneda, Hidehiro [18 ]
Kaneko, Ayane [5 ,13 ]
Katoh, Noriyuki [15 ]
Kawai, Nobuyuki [12 ]
Kubota, Keiichiro [14 ,19 ]
Kubota, Yuma [16 ]
Mamiya, Hideo [12 ]
Matsubayashi, Kazuya [20 ]
Morihana, Kumiko [18 ,21 ]
Murata, Katsuhiro L. [12 ]
Nagayama, Takahiro [22 ]
Nakamura, Noriatsu [12 ]
Nakaoka, Tatsuya [1 ]
Niino, Yuu [8 ,23 ]
Nishinaka, Yuki [13 ]
Niwano, Masafumi [12 ]
Nogami, Daisaku [19 ]
Oasa, Yumiko [16 ,24 ]
Oeda, Miki [12 ]
Ogawa, Futa [12 ]
Ohsawa, Ryou [8 ]
Ohta, Kouji [19 ]
Oide, Kohei [16 ]
Onozato, Hiroki [15 ]
Sako, Shigeyuki [8 ]
机构
[1] Hiroshima Univ, Hiroshima Astrophys Sci Ctr, 1-3-1 Kagamiyama, Higashihiroshima, Hiroshima 7398526, Japan
[2] Natl Astron Observ Japan, Mizusawa VLBI Observ, 2-12 Hoshigaoka, Oshu, Iwate 0230861, Japan
[3] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol KIPAC, SLAC Natl Accelerator Lab, 2575 Sand Hill Rd, Menlo Pk, CA 94025 USA
[4] Bisei Astron Observ, 1723-70 Ookura,Bisei Cho, Ibara, Okayama 7141411, Japan
[5] Konan Univ, Fac Sci & Engn, Dept Phys, 8-9-1 Okamoto, Kobe, Hyogo 6588501, Japan
[6] Univ Tokyo, Kavli Inst Phys & Math Universe WPI, 5-1-5 Kashiwanoha, Kashiwa, Chiba 2778583, Japan
[7] Tohoku Univ, Astron Inst, Sendai, Miyagi 9808578, Japan
[8] Univ Tokyo, Grad Sch Sci, Inst Astron, 2-21-1 Osawa, Mitaka, Tokyo 1810015, Japan
[9] Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan
[10] Natl Astron Observ Japan, Subaru Telescope, 650 North AaLTMohoku Pl, Hilo, HI 96720 USA
[11] Nagoya Univ, Inst Space Earth Environm Res, Chikusa Ku, Nagoya, Aichi 4648601, Japan
[12] Tokyo Inst Technol, Dept Phys, Meguro Ku, 2-12-1 Ookayama, Tokyo 1528551, Japan
[13] Hiroshima Univ, Dept Phys Sci, Kagamiyama 1-3-1, Higashihiroshima 7398526, Japan
[14] Toho Univ, Fac Sci, Dept Phys, 2-2-1 Miyama, Funabashi, Chiba 2748510, Japan
[15] Univ Hyogo, Ctr Astron, Nishi Harima Astron Observ, 407-2 Nishi Gaichi, Sayo, Hyogo 6795313, Japan
[16] Saitama Univ, Fac Educ, Sakura Ku, Simo Okubo 255, Saitama 3388570, Japan
[17] Univ Tokyo, Sch Sci, Dept Astron, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan
[18] Nagoya Univ, Grad Sch Sci, Chikusa Ku, Nagoya, Aichi 4648602, Japan
[19] Kyoto Univ, Grad Sch Sci, Dept Astron, Sakyo Ku, Kitashirakawa Oiwake Cho, Kyoto, Kyoto 6068502, Japan
[20] Kyoto Univ, Okayama Observ, 3037-5 Honjo,Kamogata Cho, Asakuchi, Okayama 7190232, Japan
[21] Nagoya Univ, Inst Liberal Arts & Sci, Chikusa Ku, Furo Cho, Nagoya, Aichi 4648601, Japan
[22] Kagoshima Univ, Grad Sch Sci & Engn, 1-21-40 Korimoto, Kagoshima, Kagoshima 8900065, Japan
[23] Univ Tokyo, Res Ctr Early Universe, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan
[24] Saitama Univ, Grad Sch Sci & Engn, Sakura Ku, Simo Okubo 255, Saitama 3388570, Japan
[25] Univ Tokyo, Sch Sci, Dept Phys, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan
[26] Osaka Univ, Grad Sch Sci, Dept Earth & Space Sci, 1-1 Machikaneyama, Toyonaka, Osaka 5600043, Japan
[27] NINS, Astrobiol Ctr, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan
来源
基金
美国国家航空航天局; 美国国家科学基金会; 日本学术振兴会;
关键词
NEUTRON-STAR MERGER; ELECTROMAGNETIC COUNTERPART; GW170817; KILONOVA; LIGHT CURVES; RAY-EMISSION; GAMMA-RAYS; SKY SURVEY; X-RAY; SEARCH; GROWTH;
D O I
10.1093/ptep/ptab007
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The Laser Interferometer Gravitational-wave Observatory Scientific Collaboration and Virgo Collaboration (LVC) sent out 56 gravitational-wave (GW) notices during the third observing run (O3). The Japanese Collaboration for Gravitational wave ElectroMagnetic follow-up (J-GEM) performed optical and near-infrared observations to identify and observe an electromagnetic (EM) counterpart. We constructed a web-based system that enabled us to obtain and share information on candidate host galaxies for the counterpart, and the status of our observations. Candidate host galaxies were selected from the GLADE catalog with a weight based on the 3D GW localization map provided by LVC. We conducted galaxy-targeted and wide-field blind surveys, real-time data analysis, and visual inspection of observed galaxies. We performed galaxy-targeted follow-ups to 23 GW events during O3, and the maximum probability covered by our observations reached 9.8%. Among these, we successfully started observations for 10 GW events within 0.5 days after the detection. This result demonstrates that our follow-up observation has the potential to constrain EM radiation models for a merger of binary neutron stars at a distance of up to similar to 100 Mpc with a probability area of <= 500 deg(2).
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页数:23
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