4.6 Article

CRAFTS for Fast Radio Bursts: Extending the Dispersion-Fluence Relation with New FRBs Detected by FAST

期刊

ASTROPHYSICAL JOURNAL LETTERS
卷 909, 期 1, 页码 -

出版社

IOP Publishing Ltd
DOI: 10.3847/2041-8213/abe7f0

关键词

Radio transient sources; Radio astronomy; Radio bursts; Astronomical object identification

资金

  1. National Key R&D Program of China [2017YFA0402600]
  2. National Natural Science Foundation of China [11988101, 11725313, 12041303, 11873067]
  3. Strategic Priority Research Program of the Chinese Academy of Sciences [XDB23000000]
  4. National SKA Program of China [2020SKA0120200]
  5. FAST Fellowship
  6. Cultivation Project for FAST Scientific Payoff and Research Achievement of CAMS-CAS
  7. CAS-MPG LEGACY project

向作者/读者索取更多资源

FAST discovered three new FRBs through the CRAFTS survey, showing similar characteristics to previously reported FRBs but with some new features, providing new insights for FRB research.
We report three new FRBs discovered by the Five-hundred-meter Aperture Spherical radio Telescope (FAST), namely FRB 181017.J0036+11, FRB 181118, and FRB 181130, through the Commensal Radio Astronomy FAST Survey (CRAFTS). Together with FRB 181123, which was reported earlier, all four FAST-discovered FRBs share the same characteristics of low fluence (<= 0.2 Jy ms) and high dispersion measure (DM, >1000 pc cm(-3)), consistent with the anticorrelation between DM and fluence of the entire FRB population. FRB 181118 and FRB 181130 exhibit band-limited features. FRB 181130 is prominently scattered (tau(s) 8 ms) at 1.25 GHz. FRB 181017.J0036+11 has full-bandwidth emission with a fluence of 0.042 Jy ms, which is one of the faintest FRB sources detected so far. CRAFTS has started to build a new sample of FRBs that fills the region for more distant and fainter FRBs in the fluence-DME diagram, previously out of reach of other surveys. The implied all-sky event rate of FRBs is 1.24(-0.90)(+1.94) x 5 sky(-1) day(-1) at the 95% confidence interval above 0.0146 Jy ms. We also demonstrate here that the probability density function of CRAFTS FRB detections is sensitive to the assumed intrinsic FRB luminosity function and cosmological evolution, which may be further constrained with more discoveries.

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