Nondetection of CHIME/Fast Radio Burst Sources with the Arecibo Observatory

被引：3

作者：

Good, Deborah C. ^{[1
,2
]}

Chawla, Pragya ^{[3
,4
,5
]}

Fonseca, Emmanuel ^{[3
,4
,6
,7
]}

Kaspi, Victoria ^{[3
,4
]}

Meyers, B. W. ^{[8
,9
]}

Pleunis, Ziggy ^{[10
]}

Sand, Ketan R. ^{[3
,4
]}

Scholz, Paul ^{[10
]}

Stairs, I. H. ^{[9
]}

Tendulkar, Shriharsh P. ^{[11
,12
]}

机构：

[1] Univ Connecticut, Dept Phys, Storrs, CT 06269 USA

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

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

[4] McGill Univ, McGill Space Inst, Rue Univ 3550, Montreal, PQ H3A 2A7, Canada

[5] Univ Amsterdam, Anton Pannekoek Inst Astron, Sci Pk 904, NL-1098 XH Amsterdam, Netherlands

[6] West Virginia Univ, Dept Phys & Astron, POB 6315, Morgantown, WV 26506 USA

[7] West Virginia Univ, Ctr Gravitat Waves & Cosmol, Chestnut Ridge Res Bldg, Morgantown, WV 26505 USA

[8] Curtin Univ, Int Ctr Radio Astron Res, Bentley, WA 6102, Australia

[9] Univ British Columbia, Dept Phys & Astron, 6224 Agr Rd, Vancouver, BC V6T 1Z1, Canada

[10] Univ Toronto, Dunlap Inst Astron & Astrophys, 50 St George St, Toronto, ON M5S 3H4, Canada

[11] Tata Inst Fundamental Res, Dept Astron & Astrophys, Mumbai 400005, India

[12] Natl Ctr Radio Astrophys, Post Bag 3, Pune 411007, India

来源：

ASTROPHYSICAL JOURNAL | 2023年 / 944卷 / 01期

基金：

加拿大自然科学与工程研究理事会; 加拿大创新基金会;

关键词：

POPULATION; REPETITION; PULSAR; LIMITS; MHZ;

D O I：

10.3847/1538-4357/acb139

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In this work, we present follow-up observations of two known repeating fast radio bursts (FRBs) and seven nonrepeating FRBs with complex morphology discovered with the CHIME/FRB project. These observations were conducted with the Arecibo Observatory 327 MHz receiver. We detected no additional bursts from these sources, nor did CHIME/FRB detect any additional bursts from these sources during our follow-up program. Based on these nondetections, we provide constraints on the repetition rate for all nine sources. We calculate repetition rates above 1 Jy using both a Poisson distribution of repetition and the Weibull distribution of repetition presented by Oppermann et al. For both distributions we find repetition upper limits of the order lambda = 10(-2)-10(-1) hr(-1) for all sources. These rates are much lower than those published for notable repeating FRBs like FRB 20121102A and FRB 20201124A, suggesting the possibility of a low-repetition subpopulation.

引用

页数：10

共 50 条

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