期刊论文、会议论文

英文

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES

0067-0049

2022

260

2

24

00670049

Astrophys. J. Suppl. Ser.

10.3847/1538-4365/ac6172

We thank the anonymous reviewer for very helpful comments and suggestions. We are grateful to Shri Kulkarni for suggesting the 1-month observation after the initial ToO of SGR J1935+2154. This work is supported by the National Key R&D Program of China (2021YFA0718500), the Strategic Priority Research Program on Space Science, the Chinese Academy of Sciences (grant Nos. XDA15360300, XDA15052700, XDB23040400), and the National Natural Science Foundation of China (under grant Nos. U1838113, U2038106, U1938201, 12133007, 11961141013). This work made use of the data from the Insight-HXMT mission, a project funded by the China National Space Administration (CNSA) and the Chinese Academy of Sciences (CAS).

本校为其他机构

Magnetars are neutron stars with an extreme magnetic field and sometimes manifest as soft gamma-ray repeaters (SGRs). SGR J1935+2154 is one of the most prolific bursters and the first confirmed source of a fast radio burst (FRB; i.e., FRB 200428). Encouraged by the discovery of the first X-ray counterpart of FRBs, the Insight-Hard X-ray Modulation Telescope (Insight-HXMT) implemented a dedicated 33-day-long Target of Opportunity observation of SGR J1935+2154 since 2020 April 28. With the HE, ME, and LE telescopes, Insight-HXMT provides a thorou...