4.6 Article

Periodicity Search on X-Ray Bursts of SGR J1935+2154 Using 8.5 yr of Fermi/GBM Data

期刊

ASTROPHYSICAL JOURNAL LETTERS
卷 923, 期 2, 页码 -

出版社

IOP Publishing Ltd
DOI: 10.3847/2041-8213/ac3759

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资金

  1. Fundamental Research Funds for the Central Universities [14380046]
  2. National Key Research and Development Programs of China [2018YFA0404204]
  3. National Natural Science Foundation of China [11833003, U2038105, 12121003, U1831207]
  4. China Manned Space Project [CMS-CSST-2021B11]
  5. Program for Innovative Talents, Entrepreneur in Jiangsu

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The study systematically searched for X-ray bursts of SGR J1935+2154 using Fermi Gamma-ray Burst Monitor data, identifying 8 bursting phases and 353 individual bursts. Analysis revealed bursts exhibiting a 238-day period with a 63.2% duty cycle. Predictions of two upcoming active windows of X-ray bursts were made based on the analysis, with the first prediction confirmed by ongoing X-ray activities of SGR J1935+2154 since July 2021.
We performed a systematic search for X-ray bursts of the SGR J1935+2154 using the Fermi Gamma-ray Burst Monitor continuous data dated from 2013 January to 2021 October. Eight bursting phases, which consist of a total of 353 individual bursts, are identified. We further analyze the periodic properties of our sample using the Lomb-Scargle periodogram. The result suggests that those bursts exhibit a period of similar to 238 days with a similar to 63.2% duty cycle. Based on our analysis, we further predict two upcoming active windows of the X-ray bursts. Since 2021 July, the beginning date of our first prediction has been confirmed by the ongoing X-ray activities of the SGR J1935+2154.

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