List of fast radio bursts

Last updated

This is a list of fast radio bursts . Items are listed here if information about the fast radio burst has been published. Although there could be thousands of detectable events per day, only detected ones are listed.

NameDate and time (UTC) for 1581.804688 MHz RA
(J2000)		 Decl.
(J2000)		 DM
(pc.cm−3)
[note 1] 		Width
(ms)		Peak flux
(Jy)		Maximum
estimated
comoving
distance (Gly)
[note 1] 		Observed
comoving
distance (Gly)
[note 1] 		Notes
FRB 0103122001-03-12 11:06:47.9805h 27m−64° 56′1187±1424.3±1.30.2±0.0510.14±0.15—
FRB 010621 [1] 2001-06-21 13:02:11.3018h 52m−08° 30′748±38+4
−2.3		0.53+0.26
−0.09		2.41±0.03—
FRB 010724 [2] 2001-07-24 19:50:01.6901h 18m−75° 12′375±313+5
−11		30+10
−10		3.42±0.05—"Lorimer Burst"
FRB 011025 [3] 2001-01-25 00:29:15.7919h 07m−40° 37′790.3±39.4±0.20.54+0.11
−0.07		6.62±0.10—Announced in 2014 as FRB 011025 (from data archived in 2001).
FRB 090625 [4] 2009-06-25 21:53:52.8503h 07m−29° 55′899.55±0.011.9+0
−1.9		1.14+0.42
−0.21		8.22±0.12—
FRB 1102142011-02-14 07:14:10.35301h 21m−49° 47′168.9±0.51.9±0.927+1028
−0		1.79±0.02—
FRB 110220 [5] 2011-02-20 01:55:48.09622h 35m−12° 24′944.38±0.055.6±0.11.38.48±0.12—
FRB 110523 [6] [7] [8] 2011-05-23 15:06:19.721h 45m−00° 10′623.30±0.061.73±0.170.65.77±0.09—700–900 MHz at Green Bank radio telescope, detection of both circular and linear polarization.
FRB 110626 [5] 2011-06-26 21:33:17.47721h 04m−44° 44′723.0±0.31.41+1.22
−0.45		0.63+1.22
−0.12		6.62±0.10—
FRB 110703 [5] 2011-07-03 18:59:40.60723h 31m−02° 52′1103.6±0.73.9+2.24
−1.85		0.48+0.28
−0.10		9.72±0.14—
FRB 120127 [5] 2012-01-27 08:11:21.72523h 15m−18° 26′553.3±0.31.21+0.64
−0.25		0.62+0.35
−0.10		5.25±0.09—
FRB 121002.1 [9] [4] 2012-10-02 13:09:18.40218h 15m−85° 12′1629.18±0.025.44+3.5
−1.2		0.3912.82±0.17—double burst 5.1 ms apart
FRB 121002.2 [4] 2012-10-02 13:09:18.460.43+0.33
−0.06
FRB 1210292012-10-29 16:06:26.000h 12m+42° 04′732±5320±400.346.46±0.10—
FRB 121102 [10] 2012-11-02 06:35:53.24405h 31m 58.7s+33° 08′ 52.6″557±23.0±0.50.4+0.4
−0.1		3.85±0.06—by Arecibo radio telescope
FRB 130626 [4] 2013-06-26 14:55:59.77116h 27m−07° 28′952.4±0.11.98+1.2
−0.44		0.74+0.49
−0.11		8.22±0.12—
FRB 130628 [4] 2013-06-28 03:58:00.17809h 03m+03° 26′469.88±0.010.64±0.131.91+0.29
−0.23		4.30±0.08—
FRB 130729 [4] 2013-07-29 09:01:51.1913h 41m−06° 00′861±215.61+9.98
−6.27		0.22+0.17
−0.046		7.80±0.11—
FRB 1310302013-10-30 16:13:15.0000h 25m+39° 59′203±4530±400.241.50±0.02—
FRB 131104 [11] 2013-11-04 18:04:01.206h 44m−51° 17′779±12.37+0.89
−0.45		1.16+0.35
−0.126		6.88±0.10—'near' Carina Dwarf Spheroidal Galaxy
FRB 1402122014-02-12 10:31:14.0001h 31m+30° 32′910±4390±400.268.15±0.12—
FRB 140514 [12] 2014-05-14 17:14:11.0622h 34m−12° 19′562.7±0.62.8+3.5
−0.7		0.47+0.099
−0.136		5.32±0.08—21 ± 7 per cent (3σ) circular polarization
FRB 1411132014-11-13 07:42:55.2206h 13m+18° 47′400.320.0391.96±0.02—
FRB 1412162014-12-16 13:03:24.0000h 14m+41° 38′545±5870±400.234.83±0.09—
FRB 150215 [13] 2015-02-15 20:41:41.71418h 17m−04° 54′1105.6±0.82.88+1.2
−0.57		0.7+0.28
−0.095		6.72±0.10—43% linear 3% circular polarized
FRB 1504182015-04-18 04:29:06.65707h 17m−19° 01′776.2±0.50.8±0.32.2+0.6
−0.3		5.84±0.09—Detection of linear polarization. The origin of the burst is disputed. [14] [15] [16] [17]
FRB 150517.12015-05-17 17:42:08.71205h 31m 58.7s+33° 08′ 52.6″560±43.8±0.40.033.85±0.06—10 repeat bursts at FRB 121102 location: 2 bursts on May 17 and 8 bursts on June 2 [18] [19]
FRB 150517.22015-05-17 17:51:40.921566±103.3±0.40.03
FRB 150602.12015-06-02 16:38:07.575555±34.6±0.30.04
FRB 150602.22015-06-02 16:47:36.484558±108.7±1.50.02
FRB 150602.32015-06-02 17:49:18.627559±102.8±0.40.02
FRB 150602.42015-06-02 17:49:41.319—6.1±1.40.02
FRB 150602.52015-06-02 17:50:39.298556.5±3.76.6±0.10.14
FRB 150602.62015-06-02 17:53:45.528557.4±3.76.0±0.30.05
FRB 150602.72015-06-02 17:56:34.787558.7±4.98.0±0.50.05
FRB 150602.82015-06-02 17:57:32.020556.5±1.13.06±0.040.31
FRB 1506102015-06-10 05:26:59.39610h 44m−40° 05′1593.9±0.62±10.7±0.212.17±0.16—
FRB 1508072015-08-07 17:53:55.8322h 43m−55° 05′266.5±0.10.35±0.05128±52.45±0.03—
FRB 151018.12015-10-18 01:05:48.0005h 31m 58.7s+33° 08′ 52.6″570±5650+0
−650		1.43.85±0.06—double burst 2.5 seconds apart at FRB121102 location
FRB 151018.22015-10-18 01:05:50.50400+0
−400
FRB 1511132015-11-13 08:32:42.375559.9±7.16.73±1.120.045 repeat bursts at FRB121102 location: 1 burst on November 13 and 4 bursts on November 19
FRB 151119.12015-11-19 10:44:40.524565.1±5.26.1±0.570.06
FRB 151119.22015-11-19 10:51:34.957568.8±6.66.14±10.04
FRB 151119.32015-11-19 10:58:56.234—4.3±1.40.02
FRB 151119.42015-11-19 11:05:52.492560.0±6.45.97±0.350.09
FRB 1511252015-11-25 15:42:36.0001h 32m+30° 59′273±41680±400.542.38±0.03—
FRB 1512062015-12-06 06:17:52.7819h 21m−04° 08′1909.8±0.63±0.60.3±0.0414.29±0.20—
FRB 1512082015-12-08 04:54:40.2605h 31m 58.7s+33° 08′ 52.6″558.6±1.72.5±0.230.033.85±0.06—at FRB121102 location
FRB 1512302015-12-30 16:15:46.52509h 41m−03° 27′960.4±0.54.4±0.50.42±0.038.90±0.13—
FRB 1601022016-01-02 08:28:39.37422h 39m−30° 11′2596.1±0.33.4±0.80.5±0.117.81±0.27—
FRB 1602062016-02-06 10:26:50.0001h 01m+41° 38′1262±51590±400.2610.67±0.15—
FRB 160317 [20] 2016-03-17 09:00:36.5307h 54m−29° 37′1165±1121±738.09±0.11—First FRB observed by the interferometer UTMOST
FRB 160410 [20] 2016-04-10 08:33:39.6808h 41m+06° 05′278±34±172.35±0.03—
FRB 160608 [20] 2016-06-08 03:53:01.08807h 37m−40° 48′682±79±64.34.60±0.09—
FRB 1608232016-08-23 17:51:23.92105h 31m 58.7s+33° 08′ 52.6″567±22—3.85±0.06—at FRB121102 location
FRB 1609202016-09-20 03:05:43.0005h 34m+41° 45′1767±450000.2212.23±0.16—
FRB 1612022016-12-02 13:24:54.0023h 44m+40° 48′291±4810±400.292.38±0.03—
FRB 170107 [21] 2017-01-07 20:05:08.13911h 23m−05° 00′609.5±0.52.4±0.224.15.81±0.09—first by ASKAP, high fluence ~58 Jy ms. In Leo. Galactic latitude 51°, Distance 3.1 Gpc, isotropic energy ~3 x 1034 J [21]
FRB 1704162017-04-16 23:11:12.79922h 13m−55° 02′523.2±0.25±0.619.44.92±0.09—
FRB 1704282017-04-28 18:02:34.70021h 47m−41° 51′991.7±0.94.4±0.57.78.84±0.13—
FRB 1706062017-06-06 10:03:27.0005h 34m+41° 45′247±533000.54——
FRB 1707072017-07-07 06:17:34.35402h 59m−57° 16′235.2±0.63.5±0.514.82.15±0.02—
FRB 1707122017-07-12 13:22:17.39422h 36m−60° 57′312.79±0.071.4±0.337.82.94±0.04—
FRB 170826.1-152017-08-26 13:52:01.25205h 31m 58.7s+33° 08′ 52.6″565±51.740.383.85±0.06—15 more bursts at the location of FRB 121102 detected by Green Bank Telescope over a 24-minute interval, bringing the total received bursts from this location to 34. [22]
FRB 170827 [23] 2017-08-27 16:20:1800h 49m−65° 33′176.80±0.040.40±0.0160±201.57±0.02—low DM
FRB 1709062017-09-06 13:06:56.48822h 00m−19° 57′390.3±0.42.5±0.329.63.69±0.05—
FRB 170922 [24] 2017-09-22 11:23:33.421h 30m−08° 00′1111±134.1+2.6
−2.8		2.3±0.59.03±0.13—extreme scattering (long pulse)
FRB 1710032017-10-03 04:07:23.78112h 30m−14° 07′463.2±1.22.0±0.240.54.37±0.08—
FRB 1710042017-10-04 03:23:39.25011h 58m−11° 54′304.0±0.32.0±0.3222.84±0.04—
FRB 1710192017-10-19 13:26:40.09722h 18m−08° 35′460.8±1.15.4±0.340.54.37±0.08—repeating FRB
FRB 1710202017-10-20 10:27:58.59822h 15m−19° 40′114.1±0.23.2±0.5117.60.85±0.01—
FRB 1711162017-11-16 14:59:33.30503h 31m−17° 14′618.5±0.53.2±0.519.65.87±0.09—
FRB 171209 [25] 2017-12-09 20:34:23.515h 50m−46° 10′1457.4±0.032.51.4814.71±0.21—
FRB 1712132017-12-13 14:22:40.46703h 39m−10° 56′158.6±0.21.5±0.288.61.34±0.02—
FRB 1712162017-12-16 17:59:10.82203h 28m−57° 04′203.1±0.51.9±0.3211.79±0.02—
FRB 1801102018-01-10 07:34:34.95921h 53m−35° 27′715.7±0.23.2±0.2128.16.69±0.10—
FRB 1801192018-01-19 12:24:40.74703h 29m−12° 44′402.7±0.72.7±0.540.73.85±0.06—
FRB 180128.12018-01-28 00:59:38.61713h 56m−06° 43′441.4±0.22.9±0.317.54.24±0.07—
FRB 180128.22018-01-28 04:53:26.79622h 22m−60° 15′495.9±0.72.3±0.228.74.73±0.09—
FRB 1801302018-01-30 04:55:29.99321h 52m−38° 34′343.5±0.44.1±123.13.23±0.05—
FRB 1801312018-01-31 05:45:04.32021h 50m−40° 41′657.7±0.54.5±0.422.26.16±0.09—
FRB 1802122018-02-12 23:45:04.39914h 21m−03° 35′167.5±0.51.81±0.06531.47±0.02—
FRB 180301 [26] 2018-03-01 07:34:19.7606h 13m+04° 34′52030.5——positive spectrum, from Breakthrough Listen
FRB 180309 [27] 2018-03-09 02:49:32.9921h 25m−33° 59′263.42±0.010.47527.62.41±0.03—
FRB 180311 [28] 2018-03-11 04:11:54.8021h 32m−57° 44′1570.9±0.513.40.1516.86±0.25—
FRB 1803152018-03-15 05:05:30.98519h 35m−26° 50′479±0.42.4±0.323.34.57±0.09—
FRB 1803212018-03-21 07:05:54.0000h 33m+42° 02′594±51670±400.545.35±0.09—
FRB 1803242018-03-24 09:31:46.70606h 16m−34° 47′431±0.44.3±0.516.53.78±0.06—
FRB 1804172018-04-17 13:18:31.0012h 25m+14° 13′474.82.5221.84.63±0.09—
FRB 1804302018-04-30 10:00:35.7006h 51m−09° 57′264.1±0.51.2147.5±3.31.08±0.01—
FRB 1805152018-05-15 21:57:26.48523h 13m−42° 15′355.2±0.51.9±0.424.22.58±0.04—
FRB 1805252018-05-25 15:19:06.51514h 40m−02° 12′388.1±0.33.8±0.178.93.72±0.05—
FRB 1805282018-05-28 04:24:00.906h 39m−49° 54′899.3±0.62.0±0.215.759.75±0.14—
FRB 1807142018-07-14 10:00:08.717h 46m−11° 46′1467.92±0.32.90.614.87±0.21—
FRB 180725 [29] 2018-07-25 17:59:32.81306h 13m+67° 04′715.98±0.020.31+0.08
−0.07		396.43±0.10—first detection of an FRB at radio frequencies below 700 MHz
realtime detection by CHIME
FRB 1807272018-07-27 00:52:04.47413h 11m+26° 26′642.07±0.030.78±0.16186.20±0.10—
FRB 180729.12018-07-29 00:48:19.23813h 16m+55° 32′109.61±0.0020.12±0.012830.85±0.01—
FRB 180729.22018-07-29 17:28:18.25805h 58m+56° 30′317.37±0.010.081132.38±0.03—
FRB 1807302018-07-30 03:37:25.93703h 53m+87° 12′849.047±0.0020.42±0.041197.66±0.11—
FRB 1808012018-08-01 08:47:14.79321h 30m+72° 43′656.2±0.030.51±0.09555.71±0.09—
FRB 1808062018-08-06 14:13:03.10715h 15m+75° 38′739.98±0.030.69356.91±0.11—
FRB 180810.12018-08-10 17:28:54.61406h 46m+34° 52′414.95±0.020.27413.29±0.05—
FRB 180810.22018-08-10 22:40:42.49311h 59m+83° 07′169.134±0.0020.28±0.03611.34±0.02—
FRB 1808122018-08-12 11:45:32.87201h 12m+80° 47′802.57±0.041.25+0.49
−0.47		147.08±0.11—
FRB 180814.12018-08-14 14:20:14.44015h 54m+74° 01′238.32±0.010.181392.12±0.02—
FRB 180814.2 [30] 2018-08-14 14:49:48.02204h 22m 22s+73° 40′189.38±0.092.6±0.28.11.11±0.01—Detected by CHIME. Second repeating FRB to be discovered and first since 2012.
FRB 1808172018-08-17 01:49:20.20215h 33m+42° 12′1006.84±0.0020.37709.20±0.14—
FRB 1809062018-09-06 01:17:47.38004h 22m 22s+73° 40′191±33.95.41.11±0.01—at FRB 180814.2 location
FRB 1809112018-09-11 12:59:13.733189.8±0.97.90.43
FRB 180916 2018-09-16 10:15:19.80301h 58m 00.75s+65° 43′ 00.5″349.2±0.41.4±0.071.4±0.61.63±0.020.45±0.02repeating FRB localized to a nearby spiral galaxy
FRB 1809172018-09-17 00:46:35.35904h 22m 22s+73° 40′189.5±0.1631.01.11±0.01—at FRB 180814.2 location
FRB 1809192018-09-19 12:36:09.141190±0.1160.75
FRB 180924 [31] 2018-09-24 16:23:12.626521h 44m 25.26s−40° 54′ 00.1″361.42±0.061.3±0.09164.26±0.073.99±0.06first non-repeating FRB whose source has been localized
FRB 1810162018-10-16 04:16:56.3015h 46m−25° 25′1982.8±2.88.6+0.7
−0.8		10.1917.78±0.27—
FRB 181017.12018-10-17 10:24:37.4022h 06m−08° 51′239.97±0.030.33902.54±0.04—
FRB 181017.22018-10-17 23:26:11.8617h 05m+68° 17′1281.9±0.413.4±0.10.4±0.310.89±0.15—repeating FRB
FRB 1810192018-10-19 08:13:22.7501h 58m 00.75s+65° 43′ 00.5″349.0±0.64.1±0.30.6±0.31.63±0.020.45±0.02burst at FRB 180916 location
FRB 1810282018-10-28 10:12:31.47704h 22m 22s+73° 40′188.9±0.5420.291.11±0.01—at FRB 180814.2 location
FRB 181030.12018-10-30 04:13:13.02510h 54m+73° 44′103.5±0.70.59±0.083.2±1.70.68±0.010.088±0.003repeating FRB, most likely originating from NGC 3403.
FRB 181030.22018-10-30 04:16:21.654103.5±0.31.43±0.083.1±1.4
FRB 181104.12018-11-04 06:57:18.58501h 58m 00.75s+65° 43′ 00.5″349.5±0.31.37±0.071.4±0.51.63±0.020.45±0.02burst at FRB 180916 location
FRB 181104.22018-11-04 07:07:01.591349.6±0.26.3±1.10.4±0.2
FRB 1811122018-11-12 17:31:15.48321h 49m−52° 58′589.27±0.032.1±0.2124.96±0.095.81±0.10localized to a small galaxy
FRB 1811192018-11-19 16:49:03.19112h 42m+65° 08′364.2±16.3±0.60.3±0.23.49±0.05—repeating FRB
FRB 1811202018-11-20 05:56:06.23201h 58m 00.75s+65° 43′ 00.5″349.9±0.61.1±0.091.1±0.51.63±0.020.45±0.02burst at FRB 180916 location
FRB 1811282018-11-28 08:27:41.74004h 56m+63° 23′450.2±0.32.43±0.160.5±0.33.56±0.05—repeating FRB
FRB 1812192018-12-19 07:04:41.678450.8±0.35.5±0.70.3±0.2
FRB 1812222018-12-22 03:59:23.20801h 58m 00.75s+65° 43′ 00.5″349.1±0.14.95±0.014.9±1.81.63±0.020.45±0.02burst at FRB 180916 location
FRB 1812232018-12-23 03:51:28.960349.7±0.71.06±0.051.7±0.6
FRB 1812252018-12-25 03:53:03.926348.9±0.71.3±0.30.4±0.2
FRB 1812262018-12-26 03:43:30.107348.8±0.20.87±0.031.6±0.6
FRB 1812282018-12-28 13:48:50.1006h 09m−45° 58′354.2±0.91.24+0.13
−0.15		19.233.78±0.06—
FRB 1901032019-01-03 13:47:23.32212h 42m+65° 08′364.0±0.32.66±0.10.6±0.33.49±0.05—burst at FRB 181119 location
FRB 190116.12019-01-16 13:07:33.83312h 49m+27° 09′444.0±0.64.0±0.50.3±0.24.37±0.08—repeating FRB
FRB 190116.22019-01-16 13:08:20.412443.6±0.81.5±0.30.4±0.2
FRB 1901262019-01-26 01:32:45.32801h 58m 00.75s+65° 43′ 00.5″349.8±0.52.53±0.130.7±0.31.63±0.02—
FRB 1902092019-02-09 08:20:20.97709h 37m+77° 40′424.6±0.63.7±0.50.4±0.23.95±0.07—repeating FRB
FRB 1902102019-02-10 08:17:13.907425.2±0.59.4±1.40.6±0.4
FRB 1902162019-02-16 15:26:58.02917h 05m+68° 17′1281.0±0.620.2±1.70.4±0.210.89±0.15—burst at FRB 181017.2 location
FRB 1902222019-02-22 18:46:01.36720h 52m+69° 50′460.6±0.12.97±0.901.9±0.63.91±0.07—repeating FRB
FRB 1903012019-03-01 18:03:02.479459.8±0.42.44±0.81.4±0.5
FRB 1903132019-03-13 09:21:46.72512h 42m+65° 08′364.2±0.61.5±0.20.4±0.23.49±0.05—burst at FRB 181119 location
FRB 1905232019-05-23 06:05:55.81513h 48m 15.6s+72° 28′ 11″760.8±0.60.42±0.056707.08±0.117.51±0.06localized to only 5 arcseconds
FRB 1907112019-07-11 01:53:41.09321h 56m−80° 23′593±2————
FRB 1907142019-07-14 05:17:12.90112h 16m−13° 00′504±2————
FRB 1908052019-08-05 09:21:0822h 18m−08° 35′460.4±0.26±2———burst at FRB 171019 location
FRB 1908062019-08-06 17:07:58.000h 02m−07° 35′388.5————
FRB 1909062019-09-06 00:08:4605h 31m 58.7s33° 08′ 52.6″—————burst at FRB 121102 location
FRB 190910.1-122019-09-1212 bursts detected at FRB 121102 location in a 3-hour timespan
FRB 1910012019-10-01 16:55:35.97121h 32m−54° 40′506.92±0.04——4.37±0.08—
FRB 1911072019-11-07 18:55:36.708h 02m−13° 44′714.25————
FRB 1912232019-12-23 04:55:31.220h 34m−75° 09′665————
FRB 1912282019-12-28 09:16:16.44422h 57m−29° 46′297.9±0.5————
FRB 200120 [32] 2020-01-20———————
FRB 200428 2020-04-2819h 35m+21° 54′332.8————
FRB 201124 2020-11-24
08:50:41		05h 08m+26° 11′413.52±0.05————very high repeating burst activity reported to have begun 23 March 2021; includes "extremely bright" 15 April 2021 [33] [34] [35] [36] [37] [38] [39] [40] [41]
FRB 210401 2021-04-01 11:33:01.66(1)05h 07m+25° 53′412±3————
FRB 210402 2021-04-02 05:48:59.114(1)05h 08m+26° 02′414±3————
FRB 20240304BThe farthest FRB detected as of August 2025 [42]

Notes

  1. 1 2 3 The dispersion measure (DM) measures how much dust a radio signal had to pass through, as higher frequencies penetrate dust more quickly than lower frequencies, creating a delayed signal across different radio frequencies.
    If one compares the DM of a radio burst to the amount of known dust in the Milky Way in that direction, as well as the density of dust in intergalactic space, a very rough distance can be inferred.
    In reality, the actual distance is usually shorter, as fast radio bursts appear to originate inside galaxies with their own concentrated dust clouds, dispersing the signal even more and making it appear much further from the Milky Way than it truly is.

References

  1. ↑ Keane, E. F.; Stappers, B. W.; Kramer, M.; Lyne, A. G. (September 2012). "On the origin of a highly dispersed coherent radio burst". Monthly Notices of the Royal Astronomical Society: Letters. 425 (1): L71 –L75. arXiv: 1206.4135 . Bibcode:2012MNRAS.425L..71K. doi: 10.1111/j.1745-3933.2012.01306.x . S2CID   118594059.
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  3. ↑ Burke-Spolaor, Sarah; Bannister, Keith W. (11 August 2014). "The Galactic Position Dependence of Fast Radio Bursts and the Discovery of FRB011025". The Astrophysical Journal. 792 (1): 19. arXiv: 1407.0400 . Bibcode:2014ApJ...792...19B. doi:10.1088/0004-637X/792/1/19. S2CID   118545823.
  4. 1 2 3 4 5 6 Champion, D. J.; Petroff, E.; Kramer, M.; Keith, M. J.; Bailes, M.; Barr, E. D.; Bates, S. D.; Bhat, N. D. R.; Burgay, M.; Burke-Spolaor, S.; Flynn, C. M. L.; Jameson, A.; Johnston, S.; Ng, C.; Levin, L.; Possenti, A.; Stappers, B. W.; van Straten, W.; Tiburzi, C.; Lyne, A. G. (24 November 2015). "Five new Fast Radio Bursts from the HTRU high latitude survey: first evidence for two-component bursts". Monthly Notices of the Royal Astronomical Society: Letters. 460 (1): L30. arXiv: 1511.07746 . Bibcode:2016MNRAS.460L..30C. doi: 10.1093/mnrasl/slw069 . S2CID   3500618. D. J. Champion, E. Petroff, M. Kramer, M. J. Keith, M. Bailes, E. D. Barr, S. D. Bates, N. D. R. Bhat, M. Burgay, S. Burke-Spolaor, C. M. L. Flynn, A. Jameson, S. Johnston, C. Ng, L. Levin, A. Possenti, B. W. Stappers, W. van Straten, C. Tiburzi, A. G. Lyne
  5. 1 2 3 4 D. Thornton; B. Stappers; M. Bailes; B. Barsdell; et al. (5 July 2013). "A Population of Fast Radio Bursts at Cosmological Distances". Science. 341 (6141): 53–6. arXiv: 1307.1628 . Bibcode:2013Sci...341...53T. doi:10.1126/science.1236789. PMID   23828936. S2CID   206548502.
  6. ↑ K. Masui; et al. (3 December 2015). "Dense magnetized plasma associated with a fast radio burst". Nature. 528 (7580): 523–5. arXiv: 1512.00529 . Bibcode:2015Natur.528..523M. doi:10.1038/nature15769. PMID   26633633. S2CID   4470819.
  7. ↑ "Team finds detailed record of mysterious fast radio burst".
  8. ↑ Masui, K; Lin, HH; Sievers, J; Anderson, CJ; Chang, TC; Chen, X; Ganguly, A; Jarvis, M; Kuo, CY; Li, YC; Liao, YW; McLaughlin, M; Pen, UL; Peterson, JB; Roman, A; Timbie, PT; Voytek, T; Yadav, JK (2015). "Dense magnetized plasma associated with a fast radio burst". Nature. 528 (7583): 523–5. arXiv: 1512.00529 . Bibcode:2015Natur.528..523M. doi:10.1038/nature15769. PMID   26633633. S2CID   4470819.
  9. ↑ Dan Thornton (September 2013). The High Time Resolution Radio Sky (PDF) (Thesis). Manchester. p. 140-147.
  10. ↑ Spitler, L. G.; Cordes, J. M.; Hessels, J. W. T.; Lorimer, D. R.; McLaughlin, M. A.; Chatterjee, S.; Crawford, F.; Deneva, J. S.; Kaspi, V. M.; Wharton, R. S.; et al. (1 August 2014). "Fast Radio Burst Discovered in the Arecibo Pulsar Alfa Survey". The Astrophysical Journal. 790 (2): 101. arXiv: 1404.2934 . Bibcode:2014ApJ...790..101S. doi:10.1088/0004-637X/790/2/101. S2CID   8812299.
  11. ↑ Ravi, V.; Shannon, R. M.; Jameson, A. (14 January 2015). "A Fast Radio Burst in the Direction of the Carine Dwarf Spheroildal Galaxy". The Astrophysical Journal. 799 (1): L5. arXiv: 1412.1599 . Bibcode:2015ApJ...799L...5R. doi:10.1088/2041-8205/799/1/L5. S2CID   53708003.
  12. ↑ Petroff, E.; Bailes, M.; Barr, E. D.; Barsdell, B. R.; Bhat, N. D. R.; Bian, F.; Burke-Spolaor, S.; Caleb, M.; Champion, D.; Chandra, P.; Da Costa, G.; Delvaux, C.; Flynn, C.; Gehrels, N.; Greiner, J.; Jameson, A.; Johnston, S.; Kasliwal, M. M.; Keane, E. F.; Keller, S.; Kocz, J.; Kramer, M.; Leloudas, G.; Malesani, D.; Mulchaey, J. S.; Ng, C.; Ofek, E. O.; Perley, D. A.; Possenti, A.; et al. (19 January 2015). "A real-time fast radio burst: polarization detection and multiwavelength follow-up". Monthly Notices of the Royal Astronomical Society. 447 (1): 246–255. arXiv: 1412.0342 . Bibcode:2015MNRAS.447..246P. doi: 10.1093/mnras/stu2419 . S2CID   27470464.
  13. ↑ Petroff, E.; Burke-Spolaor, S.; Keane, E. F.; McLaughlin, M. A.; Miller, R.; Andreoni, I.; Bailes, M.; Barr, E. D.; Bernard, S. R.; Bhandari, S.; Bhat, N. D. R.; Burgay, M.; Caleb, M.; Champion, D.; Chandra, P.; Cooke, J.; Dhillon, V. S.; Farnes, J. S.; Hardy, L. K.; Jaroenjittichai, P.; Johnston, S.; Kasliwal, M.; Kramer, M.; Littlefair, S. P.; MacQuart, J. P.; Mickaliger, M.; Possenti, A.; Pritchard, T.; Ravi, V.; et al. (2017). "A polarized fast radio burst at low Galactic latitude". Monthly Notices of the Royal Astronomical Society. 469 (4): 4465. arXiv: 1705.02911 . Bibcode:2017MNRAS.469.4465P. doi: 10.1093/mnras/stx1098 . S2CID   211141701.
  14. ↑ "Cosmological Origin for FRB 150418? Not So Fast" (PDF).
  15. ↑ "ATel #8752: Radio brightening of FRB 150418 host galaxy candidate". ATel. Retrieved 2016-03-03.
  16. ↑ says, Franko (29 February 2016). "That Blast of Radio Waves Produced By Colliding Dead Stars? Not So Fast". Phenomena. Archived from the original on March 1, 2016. Retrieved 2016-03-03.
  17. ↑ "Fast Radio Burst Afterglow Was Actually a Flickering Black Hole". Harvard-Smithsonian Center for Astrophysics (HSCFA). SpaceRef. April 4, 2016. Retrieved 2016-04-05.
  18. ↑ Spitler, L. G.; Scholz, P.; Hessels, J. W. T.; Bogdanov, S.; Brazier, A.; Camilo, F.; Chatterjee, S.; Cordes, J. M.; Crawford, F. (2016-03-02). "A repeating fast radio burst". Nature. 531 (7593): 202–205. arXiv: 1603.00581 . Bibcode:2016Natur.531..202S. doi:10.1038/nature17168. ISSN   1476-4687. PMID   26934226. S2CID   205247994.
  19. ↑ Draka, Nadia (2 March 2016). "Astronomers Discover a New Kind of Radio Blast From Space". National Geographic News. Archived from the original on March 3, 2016. Retrieved 2016-03-03.
  20. 1 2 3 Caleb, M.; Flynn, C.; Bailes, M.; Barr, E. D.; Bateman, T.; Bhandari, S.; Campbell-Wilson, D.; Farah, W.; Green, A. J.; Hunstead, R. W.; Jameson, A.; Jankowski, F.; Keane, E. F.; Parthasarathy, A.; Ravi, V.; Rosado, P. A.; van Straten, W.; Venkatraman Krishnan, V. (2017). "The first interferometric detections of Fast Radio Bursts". Monthly Notices of the Royal Astronomical Society. 468 (3): 3746. arXiv: 1703.10173 . Bibcode:2017MNRAS.468.3746C. doi: 10.1093/mnras/stx638 . S2CID   54836555.
  21. 1 2 Bannister, K. W.; Shannon, R. M.; Macquart, J.-P.; Flynn, C.; Edwards, P. G.; O’Neill, M.; Osłowski, S.; Bailes, M.; Zackay, B.; Clarke, N.; D’Addario, L. R.; Dodson, R.; Hall, P. J.; Jameson, A.; Jones, D.; Navarro, R.; Trinh, J. T.; Allison, J.; Anderson, C. S.; Bell, M.; Chippendale, A. P.; Collier, J. D.; Heald, G.; Heywood, I.; Hotan, A. W.; Lee-Waddell, K.; Madrid, J. P.; Marvil, J.; McConnell, D.; Popping, A.; Voronkov, M. A.; Whiting, M. T.; Allen, G. R.; Bock, D. C.-J.; Brodrick, D. P.; Cooray, F.; DeBoer, D. R.; Diamond, P. J.; Ekers, R.; Gough, R. G.; Hampson, G. A.; Harvey-Smith, L.; Hay, S. G.; Hayman, D. B.; Jackson, C. A.; Johnston, S.; Koribalski, B. S.; McClure-Griffiths, N. M.; Mirtschin, P.; Ng, A.; Norris, R. P.; Pearce, S. E.; Phillips, C. J.; Roxby, D. N.; Troup, E. R.; Westmeier, T. (22 May 2017). "The Detection of an Extremely Bright Fast Radio Burst in a Phased Array Feed Survey". The Astrophysical Journal. 841 (1): L12. arXiv: 1705.07581 . Bibcode:2017ApJ...841L..12B. doi: 10.3847/2041-8213/aa71ff . S2CID   55643060.
  22. ↑ Gajjar, Vishal; et al. (29 August 2017). "FRB 121102: Detection at 4–8 GHz band with Breakthrough Listen backend at Green Bank". Astronomer's Telegram . 10675: 1. Bibcode:2017ATel10675....1G . Retrieved 30 August 2017.
  23. ↑ Farah, W. (2 September 2017). "ATel #10697: Real-time detection of a Fast Radio Burst at the Molonglo Radio Telescope". The Astronomer's Telegram.
  24. ↑ Farah, W. "ATel #10867: Detection of a highly scattered Fast Radio Burst at the Molonglo Radio Telescope". The Astronomer's Telegram.
  25. ↑ Shannon, R. M. "ATel #11046: Real-time detection of a low-latitude Fast Radio Burst during observations of PSR J1545-4550". ATel. Retrieved 20 March 2018.
  26. ↑ Price, Danny C. "ATel #11376: Detection of a new fast radio burst during Breakthrough Listen observations". The Astronomer's Telegram.
  27. ↑ Oslowski, S. "ATel #11385: Real-time detection of an extremely high signal-to-noise ratio fast radio burst during observations of PSR J2124-3358". ATel. Retrieved 20 March 2018.
  28. ↑ Oslowski (11 March 2018). "ATel #11396: A second fast radio burst discovered with Parkes Telescope within 50 hours: FRB180311 in the direction of PSR J2129-5721". The Astronomer's Telegram. Retrieved 20 March 2018.
  29. ↑ Boyle, P. J. (1 August 2018). "ATel #11901: First detection of fast radio bursts between 400 and 800 MHz by CHIME/FRB". The Astronomer's Telegram. Retrieved 2018-08-04.
  30. ↑ The CHIME/FRB Collaboration (9 January 2019). "A second source of repeating fast radio bursts". Nature . 566 (7743): 235–238. arXiv: 1901.04525 . Bibcode:2019Natur.566..235C. doi:10.1038/s41586-018-0864-x. PMID   30653190. S2CID   186244363.
  31. ↑ Bannister, K. W.; Deller, A. T.; Phillips, C.; Macquart, J.-P.; et al. (27 June 2019). "A single fast radio burst localized to a massive galaxy at cosmological distance". Science Magazine. 364 (6447): 565–570. arXiv: 1906.11476 . Bibcode:2019Sci...365..565B. doi:10.1126/science.aaw5903. hdl: 1959.3/450579 . PMID   31249136. S2CID   195699409.
  32. ↑ Andreoni, Igor; et al. (27 May 2021). "ATel #14666: ZTF optical observations of FRB 20200120E in M81". The Astronomer's Telegram . Retrieved 28 May 2021.
  33. ↑ CHIME/FRB Collaboration (31 March 2021). "ATel #14497:Recent high activity from a repeating Fast Radio Burst discovered by CHIME/FRB". The Astronomer's Telegram . Retrieved 2 April 2021.
  34. ↑ Kumar, Pravir; et al. (2 April 2021). "ATel #14502: ASKAP detection of a repeat burst from the FRB 20201124A source". The Astronomer's Telegram . Retrieved 2 April 2021.
  35. ↑ Kumar, Pravir (3 April 2021). "ATel #14508: A second fast radio burst from the source of FRB 201124A detected by ASKAP". The Astronomer's Telegram . Retrieved 3 April 2021.
  36. ↑ Kumar, Pravir; et al. (4 April 2021). "ATel #14509: Correction to ATel #14508". The Astronomer's Telegram . Retrieved 4 April 2021.
  37. ↑ Xu, Heng; et al. (6 April 2021). "ATel #145218: FAST detection and localization of FRB20201124A". The Astronomer's Telegram . Retrieved 7 April 2021.
  38. ↑ Pearlman, Aaron B.; et al. (7 April 2021). "ATel #14519: High Frequency Radio Observations of FRB 20201124A at 2.26 GHz using the Deep Space Network". The Astronomer's Telegram . Retrieved 7 April 2021.
  39. ↑ Campana, Sergio; et al. (7 April 2021). "ATel #14523: Swift observations of FRB20201124A". The Astronomer's Telegram . Retrieved 7 April 2021.
  40. ↑ Ricci, Roberto; et al. (14 April 2021). "ATel #14549: Detection of a persistent radio source at the location of FRB20201124A with VLA". The Astronomers Telegram . Retrieved 16 April 2021.
  41. ↑ Herrmann, Wolfgang (16 April 2021). "ATel #14556: Extremely bright pulse from FRB20201124A observed with the 25-m Stockert Radio Telescope". The Astronomer's Telegram . Retrieved 17 April 2021.
  42. ↑ Caleb, Manisha; Nanayakkara, Themiya; Stappers, Benjamin; Pastor-Marazuela, Inés; Khrykin, Ilya S.; Glazebrook, Karl; Tejos, Nicolas; Prochaska, J. Xavier; Rajwade, Kaustubh (2025-08-03), A fast radio burst from the first 3 billion years of the Universe, arXiv, doi:10.48550/arXiv.2508.01648, arXiv:2508.01648, retrieved 2025-08-12
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