Limits on Simultaneous and Delayed Optical Emission from Well-localized Fast Radio Bursts

被引：10

作者：

Hiramatsu, Daichi ^{[1
,2
]}

Berger, Edo ^{[1
,2
]}

Metzger, Brian D. D. ^{[3
,4
,5
]}

Gomez, Sebastian ^{[6
]}

Bieryla, Allyson ^{[1
]}

Arcavi, Iair ^{[7
,8
]}

Howell, D. Andrew ^{[9
,10
]}

Mckinven, Ryan ^{[11
]}

Tominaga, Nozomu

机构：

[1] Harvard & Smithsonian, Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA

[2] NSF AI Inst Artificial Intelligence & Fundamental, Cambridge, MA 02138 USA

[3] Columbia Univ, Dept Phys, 538 West 120th St, New York, NY 10027 USA

[4] Columbia Univ, Columbia Astrophys Lab, 538 West 120th St, New York, NY 10027 USA

[5] Flatiron Inst, Ctr Computat Astrophys, New York, NY 10010 USA

[6] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA

[7] Tel Aviv Univ, Sch Phys & Astron, IL-69978 Tel Aviv, Israel

[8] CIFAR Azrieli Global Scholars program, CIFAR, 661 Univ Ave, Toronto, ON M5G 1M1, Canada

[9] Las Cumbres Observ, 6740 Cortona Dr,Suite 102, Goleta, CA 93117 USA

[10] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA

[11] McGill Univ, Dept Phys, 3600 Rue Univ, Montreal, PQ H3A 2T8, Canada

来源：

ASTROPHYSICAL JOURNAL LETTERS | 2023年 / 947卷 / 02期

基金：

以色列科学基金会; 欧洲研究理事会;

关键词：

FREQUENCY-DEPENDENT POLARIZATION; SYNCHROTRON MASER EMISSION; HOST GALAXY PROPERTIES; SIMULTANEOUS X-RAY; FRB; 121102; MULTIWAVELENGTH OBSERVATIONS; SNR G57.2+0.8; GAMMA-RAY; MAGNETAR; TELESCOPE;

D O I：

10.3847/2041-8213/acae98

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the largest compilation to date of optical observations during and following fast radio bursts (FRBs). The data set includes our dedicated simultaneous and follow-up observations, as well as serendipitous archival survey observations, for a sample of 15 well-localized FRBs: eight repeating and seven one-off sources. Our simultaneous (and nearly simultaneous with a 0.4 s delay) optical observations of 13 (1) bursts from the repeating FRB 20220912A provide the deepest such limits to date for any extragalactic FRB, reaching a luminosity limit of nu L ( nu ) less than or similar to 10(42) erg s(-1) (less than or similar to 2 x 10(41) erg s(-1)) with 15-400 s exposures; an optical-flux-to-radio-fluence ratio of f (opt)/F (radio) less than or similar to 10(-7) ms(-1) (less than or similar to 10(-8) ms(-1)); and a flux ratio of f (opt)/f (radio) less than or similar to 0.02-less than or similar to 2 x 10(-5) (less than or similar to 10(-6)) on millisecond to second timescales. These simultaneous limits provide useful constraints in the context of FRB emission models, such as the pulsar magnetosphere and pulsar nebula models. Interpreting all available optical limits in the context of the synchrotron maser model, we find that they constrain the flare energies to less than or similar to 10(43)-10(49) erg (depending on the distances of the various repeating FRBs, with less than or similar to 10(39) erg for the Galactic SGR 1935+2154). These limits are generally at least an order of magnitude larger than those inferred from the FRBs themselves, although in the case of FRB 20220912A our simultaneous and rapid follow-up observations severely restrict the model parameter space. We conclude by exploring the potential of future simultaneous and rapid-response observations with large optical telescopes.

引用

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