Fast radio burst
In radio astronomy, a fast radio burst (FRB) is a transient radio pulse of length ranging from a fraction of a millisecond to a few milliseconds, caused by some high-energy astrophysical process not yet understood. While extremely energetic at their source, the strength of the signal reaching Earth has been described as 1,000 times less than from a mobile phone on the Moon. The first FRB was discovered by Duncan Lorimer and his student David Narkevic in 2007 when they were looking through archival pulsar survey data, and it is therefore commonly referred to as the Lorimer Burst. Many FRBs have since been recorded, including three that repeat. Although the exact origin and cause is uncertain, they are almost definitely extragalactic.
When the FRBs are polarized, it indicates that they are emitted from a source contained within an extremely powerful magnetic field. The origin of the FRBs has yet to be identified; proposals for their origin range from a rapidly rotating neutron star and a black hole, to extraterrestrial intelligence.
The localization and characterization in 2012 of FRB 121102, one of the three repeating sources, has improved the understanding of the source class. FRB 121102 is identified with a galaxy at a distance of approximately 3 billion light-years, well outside the Milky Way, and is embedded in an extreme environment. The first host galaxy identified for a non-repeating burst, FRB 180924, was identified in 2019 and is a much larger and more ordinary galaxy, nearly the size of the Milky Way. In August 2019, astronomers reported the detection of eight more repeating FRB signals.
- 1 Detection
- 2 Features
- 3 Bursts observed
- 4 Origin hypotheses
- 5 List of bursts
- 6 References
- 7 External links
The first fast radio burst to be described, the Lorimer Burst FRB 010724, was detected in 2007 in archived data recorded by the Parkes Observatory on 24 July 2001. Since then, most known FRBs have been found in previously recorded data. On 19 January 2015, astronomers at Australia's national science agency (CSIRO) reported that a fast radio burst had been observed for the first time live, by the Parkes Observatory.
Fast radio bursts are bright, unresolved (pointsource-like), broadband (spanning a large range of radio frequencies), millisecond flashes found in parts of the sky outside the Milky Way. Unlike many radio sources, the signal from a burst is detected in a short period of time with enough strength to stand out from the noise floor. The burst usually appears as a single spike of energy without any change in its strength over time. The bursts last for several milliseconds (thousandths of a second). The bursts come from all over the sky, and are not concentrated on the plane of the Milky Way. Known FRB locations are biased by the parts of the sky that the observatories can image.
Many have radio frequencies detected around 1400 MHz; a few have been detected at lower frequencies in the range of 400–800 MHz. The component frequencies of each burst are delayed by different amounts of time depending on the wavelength. This delay is described by a value referred to as a dispersion measure (DM). This results in a received signal that sweeps rapidly down in frequency, as longer wavelengths are delayed more.
The interferometer UTMOST has put a lower limit of 10,000 kilometers for the distance to the FRBs it has detected, supporting the case for an astronomical, rather than terrestrial, origin (because signal sources on Earth are ruled out as being closer than this limit). This limit can be determined from the fact that closer sources would have a curved wave front that could be detected by the multiple antennas of the interferometer.
Fast radio bursts have pulse dispersion measurements > 100 pc cm−3, much larger than expected for a source inside the Milky Way galaxy and consistent with propagation through an ionized plasma. Furthermore, their distribution is isotropic (not especially coming from the galactic plane);:fig 3 consequently they are conjectured to be of extragalactic origin.
Fast radio bursts are named by the date the signal was recorded, as "FRB YYMMDD".
2007 (Lorimer Burst)
The first FRB detected, the Lorimer Burst FRB 010724, was discovered in 2007 when Duncan Lorimer assigned his student David Narkevic to look through archival data taken in 2001 by the Parkes radio dish in Australia. Analysis of the survey data found a 30-jansky dispersed burst which occurred on 24 July 2001, less than 5 milliseconds in duration, located 3° from the Small Magellanic Cloud. The reported burst properties argue against a physical association with the Milky Way galaxy or the Small Magellanic Cloud. The burst became known as the Lorimer Burst. The discoverers argue that current models for the free electron content in the Universe imply that the burst is less than 1 gigaparsec distant. The fact that no further bursts were seen in 90 hours of additional observations implies that it was a singular event such as a supernova or merger of relativistic objects. It is suggested that hundreds of similar events could occur every day and, if detected, could serve as cosmological probes.
In 2010 there was a report of 16 similar pulses, clearly of terrestrial origin, detected by the Parkes radio telescope and given the name perytons. In 2015 perytons were shown to be generated when microwave oven doors were opened during a heating cycle, with detected emission being generated by the microwave oven's magnetron tube as it was being powered off.
In 2015, FRB 110523 was discovered in archival data collected in 2011 from the Green Bank Telescope. It was the first FRB for which linear polarization was detected (allowing a measurement of Faraday rotation). Measurement of the signal's dispersion delay suggested that this burst was of extragalactic origin, possibly up to 6 billion light-years away.
An observation in 2012 of a fast radio burst (FRB 121102) in the direction of Auriga in the northern hemisphere using the Arecibo radio telescope confirmed the extragalactic origin of fast radio pulses by an effect known as plasma dispersion.
In November 2015, astronomer Paul Scholz at McGill University in Canada, found ten non-periodically repeated fast radio pulses in archival data gathered in May and June 2015 by the Arecibo radio telescope. The ten bursts have dispersion measures and sky positions consistent with the original burst FRB 121102, detected in 2012. Like the 2012 burst, the 10 bursts have a plasma dispersion measure that is three times larger than possible for a source in the Milky Way Galaxy. The team thinks that this finding rules out self-destructive, cataclysmic events that could only occur once, such as the explosion of a black hole or the collision between two neutron stars. According to the scientists, the data support an origin in a young rotating neutron star (pulsar), or in a highly magnetized neutron star (magnetar), or from highly magnetized pulsars travelling through asteroid belts, or from an intermittent Roche lobe overflow in a neutron star-white dwarf binary.
On 16 December 2016 six new FRBs were reported in the same direction (one having been received on 13 November 2015, four on 19 November 2015, and one on 8 December 2015).:Table 2 As of January 2019[update] this is one of only two instances in which these signals have been found twice in the same location in space. FRB 121102 is located at least 1150 AU from Earth, excluding the possibility of a human-made source, and is almost certainly extragalactic in nature.
As of April 2018, FRB 121102 is thought to be co-located in a dwarf galaxy about three billion light-years from Earth with a low-luminosity active galactic nucleus, or a previously unknown type of extragalactic source, or a young neutron star energising a supernova remnant.
On 26 August 2017, astronomers using data from the Green Bank Telescope detected 15 additional repeating FRBs coming from FRB 121102 at 5 to 8 GHz. The researchers also noted that FRB 121102 is presently in a "heightened activity state, and follow-on observations are encouraged, particularly at higher radio frequencies". The waves are highly polarized, meaning "twisting" transverse waves, that could only have formed when passing through hot plasma with an extremely strong magnetic field. FRB 121102's radio bursts are about 500 times more twisted (polarized) than those from any other FRB to date. Since it is a repeating FRB source, it suggests that it does not come from some one-time cataclysmic event, so one hypothesis, first advanced in January 2018, proposes that these particular repeating bursts may come from a dense stellar core called a neutron star near an extremely powerful magnetic field, such as one near a massive black hole, or one embedded in a nebula.
In April 2018, it was reported that FRB 121102 consisted of 21 bursts spanning one hour. In September 2018, an additional 72 bursts spanning five hours had been detected using a convolutional neural network. In September 2019, more repeating signals, 20 pulses on 3 September 2019, were reported to have been detected from FRB 121102 by the Five-hundred-meter Aperture Spherical Telescope (FAST).
In 2013, four bursts were identified that supported the likelihood of extragalactic sources.
Fast radio bursts discovered up until 2015 had dispersion measures that were close to multiples of 187.5 pc cm−3. However subsequent observations do not fit this pattern.
On 18 April 2015, FRB 150418 was detected by the Parkes observatory and within hours, several telescopes including the Australia Telescope Compact Array caught an apparent radio "afterglow" of the flash, which took six days to fade. The Subaru telescope was used to find what was thought to be the host galaxy and determine its redshift and the implied distance to the burst.
However, the association of the burst with the afterglow was soon disputed, and by April 2016 it was established that the "afterglow" originates from an active galactic nucleus that is powered by a supermassive black hole with dual jets blasting outward from the black hole. It was also noted that what was thought to be an "afterglow", did not fade away as would be expected, meaning that the variable AGN is unlikely to be associated with the actual fast radio burst.
The upgraded Molonglo Observatory Synthesis Telescope (UTMOST), near Canberra (Australia), reported finding three more FRBs. A 180-day three-part survey in 2015 and 2016 found three FRBs at 843 MHz. Each FRB located with a narrow elliptical 'beam'; the relatively narrow band 828–858 MHz gives a less precise dispersion measure (DM).
According to Anastasia Fialkov and Abraham Loeb, FRB's could be occurring as often as once per second. Earlier research could not identify the occurrence of FRB's to this degree.
The unusual CHIME (Canadian Hydrogen Intensity Mapping Experiment) radio telescope, operational from September 2018, will be used to detect "hundreds" of fast radio bursts as a secondary objective to its cosmological observations. FRB 180725A was reported by CHIME as the first detection of a FRB under 700 MHz – as low as 580 MHz.
In October 2018, astronomers reported 19 more new non-repeating FRB bursts detected by the Australian Square Kilometre Array Pathfinder (ASKAP). These included three with dispersion measure (DM) smaller than seen before.
FRB 181112 was mysteriously unaffected after believed to have passed through the Halo of an intervening galaxy. 
On 9 January 2019, astronomers announced the discovery of a second repeating FRB source, named FRB 180814, by CHIME. Six bursts were detected between August and October 2018, "consistent with originating from a single position on the sky". The detection was made during CHIME's pre-commissioning phase, during which it operated intermittently, suggesting a "substantial population of repeating FRBs", and that the new telescope would make more detections.
Some news media reporting of the discovery speculated that the repeating FRB could be evidence of extraterrestrial intelligence, a possibility explored in relation to previous FRBs by some scientists, but not raised by the discoverers of FRB 180814.
FRB 180924 is the first non-repeating FRB to be traced to its source. The source is a galaxy 3.6 billion light-years away. The galaxy is nearly as large as the Milky Way and about 1000 times larger than the source of FRB 121102. While the latter is an active site of star formation and a likely place for magnetars, the source of FRB 180924 is an older and less active galaxy.
Because the source was nonrepeating, the astronomers had to scan large areas with the 36 telescopes of ASKAP. Once a signal was found, they used the Very Large Telescope, the Gemini Observatory in Chile, and the W. M. Keck Observatory in Hawaii to identify its host galaxy and determine its distance. Knowing the distance and source galaxy properties, enables a study of the composition of the intergalactic medium.
On 28 June 2019, Russian astronomers reported the discovery of nine FRB events (FRB 121029, FRB 131030, FRB 140212, FRB 141216, FRB 151125.1, FRB 151125.2, FRB 160206, FRB 161202, FRB 180321), which include FRB 151125, the third repeating one ever detected, from the direction of the M 31 (Andromeda Galaxy) and M 33 (Triangulum Galaxy) galaxies during the analysis of archive data (July 2012 to December 2018) produced by the BSA/LPI large phased array radio telescope at the Pushchino Radio Astronomy Observatory.
On 2 July 2019, astronomers reported that FRB 190523, a non-repeating FRB, has been discovered and, notably, localized to a few-arcsecond region containing a single massive galaxy at a redshift of 0.66, nearly 8 billion light-years away from Earth.
Because of the isolated nature of the observed phenomenon, the nature of the source remains speculative. As of 2019[update], there is no generally accepted explanation. The sources are thought to be a few hundred kilometers or less in size, as the bursts last for only a few milliseconds, and if the bursts come from cosmological distances, their sources must be very energetic, generating as much energy in a millisecond burst as the Sun does in 80 years.
One possible explanation would be a collision between very dense objects like merging black holes or neutron stars. It has been suggested that there is a connection to gamma-ray bursts. Some have speculated that these signals might be artificial in origin, that they may be signs of extraterrestrial intelligence. Analogously, when the first pulsar was discovered, it was thought that the fast, regular pulses could possibly originate from a distant civilization, and the source nicknamed "LGM-1" (for "little green men").
In 2007, just after the publication of the e-print with the first discovery, it was proposed that fast radio bursts could be related to hyperflares of magnetars. In 2015 three studies supported the magnetar hypothesis.
Especially energetic supernovae could be the source of these bursts. Blitzars were proposed in 2013 as an explanation. In 2014 it was suggested that following dark matter-induced collapse of pulsars, the resulting expulsion of the pulsar magnetospheres could be the source of fast radio bursts. In 2015 it was suggested that FRBs are caused by explosive decays of axion miniclusters. Another exotic possible source are cosmic strings that produced these bursts as they interacted with the plasma that permeated the early Universe. In 2016 the collapse of the magnetospheres of Kerr–Newman black holes were proposed to explain the origin of the FRBs' "afterglow" and the weak gamma-ray transient 0.4 s after GW 150914. It has also been proposed that if fast radio bursts originate in black hole explosions, FRBs would be the first detection of quantum gravity effects. In early 2017, it was proposed that the strong magnetic field near a supermassive black hole could destabilize the current sheets within a pulsar's magnetosphere, releasing trapped energy to power the FRBs.
Repeated bursts of FRB 121102 have initiated multiple origin hypotheses. A coherent emission phenomenon known as superradiance, which involves large-scale entangled quantum mechanical states possibly arising in environments such as active galactic nuclei, has been proposed to explain these and other associated observations with FRBs (e.g. high event rate, variable intensity profiles).
Nonetheless, in July 2019, astronomers reported that non-repeating Fast Radio Bursts (FRB)s may not be one-off events, but actually FRB repeaters with repeat events that have gone undetected and, further, that FRBs may be formed by events that have not yet been seen or considered.
List of bursts
|Name||Date and time (UTC) for 1581.804688 MHz||RA
|FRB 010621||2001-06-21 13:02:10.795||18h 52m||−08° 29′||746||7.8||0.4|
|FRB 010724||2001-07-24 19:50:01.63||01h 18m||−75° 12′||375||4.6||30||"Lorimer Burst"|
|FRB 011025||2001-10-25 00:29:13.23||19h 07m||−40° 37′||790||9.4||0.3|
|FRB 090625||2009-06-25 21:53:52.85||03h 07m||−29° 55′||899.6||<1.9||>2.2|
|FRB 110220||2011-02-20 01:55:48.957||22h 34m||−12° 24′||944.38||5.6||1.3|
|FRB 110523 ||2011-05-23||21h 45m||−00° 12′||623.30||1.73||0.6||700–900 MHz at Green Bank radio telescope, detection of both circular and linear polarization.|
|FRB 110627||2011-06-27 21:33:17.474||21h 03m||−44° 44′||723.0||<1.4||0.4|
|FRB 110703||2011-07-03 18:59:40.591||23h 30m||−02° 52′||1103.6||<4.3||0.5|
|FRB 120127||2012-01-27 08:11:21.723||23h 15m||−18° 25′||553.3||<1.1||0.5|
|FRB 121002||2012-10-02 13:09:18.402||18h 14m||−85° 11′||1628.76||2.1; 3.7||0.35||double pulse 5.1 ms apart|
|FRB 121002||2012-10-02 13:09:18.50||18h 14m||−85° 11′||1629.18||<0.3||>2.3|
|FRB 121102||2012-11-02 06:35:53.244||05h 32m||+33° 05′||557||3.0||0.4||by Arecibo radio telescope|
|FRB 130626||2013-06-26 14:56:00.06||16h 27m||−07° 27′||952.4||<0.12||>1.5|
|FRB 130628||2013-06-28 03:58:00.02||09h 03m||+03° 26′||469.88||<0.05||>1.2|
|FRB 130729||2013-07-29 09:01:52.64||13h 41m||−05° 59′||861||<4||>3.5|
|FRB 131104||2013-11-04 18:04:01.2||06h 44m||−51° 17′||779.0||<0.64||1.12||'near' Carina Dwarf Spheroidal Galaxy|
|FRB 140514||2014-05-14 17:14:11.06||22h 34m||−12° 18′||562.7||2.8||0.47||21 ± 7 per cent (3σ) circular polarization|
|FRB 150215||2015-02-15 20:41:41.714||18h 17m 27s||−04° 54′ 15″||1105.6||2.8||0.7||43% linear, 3% circular polarized. Low galactic latitude. Low/zero rotation measure. Detected in real time. Not detected in follow up observations of gamma rays, X-rays, neutrinos, IR etc.|
|FRB 150418||2015-04-18 04:29||07h 16m||−19° 00′||776.2||0.8||2.4||Detection of linear polarization. The origin of the burst is disputed.|
|05h 31m 58s (average)||+33° 08′ 04″ (average)||559 (average)||0.02–0.31||2.8–8.7||10 repeat bursts at FRB 121102 location: 2 bursts on May 17 and 8 bursts on June 2 |
and 1 on 13 Nov 2015, 4 on 19 Nov 2015, and 1 on 8 Dec 2015
|FRB 150610||2015-06-10 05:26:59.396||10:44:26||−40:05:23||1593.9(±0.6)||2(±1)||0.7(±0.2)|
|FRB 150807||2015-08-07 17:53:55.7799||22:40:23||– 55:16||266.5||0.35±0.05||120±30||80% linearly polarised, Galactic latitude −54.4°, Decl ±4 arcmin, RA ±1.5 arcmin, highest peak flux|
|FRB 151206||2015-12-06 06:17:52.778||19:21:25||−04:07:54||1909.8(±0.6)||3.0(±0.6)||0.3(±0.04)|
|FRB 151230||2015-12-30 16:15:46.525||09:40:50||−03:27:05||960.4(±0.5)||4.4(±0.5)||0.42(±0.03)|
|FRB 160102||2016-01-02 08:28:39.374||22:38:49||−30:10:50||2596.1(±0.3)||3.4(±0.8)||0.5(±0.1)|
|FRB 160317||2016-03-17 09:00:36.530||07:53:47||−29:36:31||1165(±11)||21||>3.0||UTMOST, Decl ± 1.5°:Table A1|
|FRB 160410||2016-04-10 08:33:39.680||08:41:25||+06:05:05||278(±3)||4||>7.0||UTMOST, Decl ± 1.5°:Table A1|
|FRB 160608||2016-06-08 03:53:01.088||07:36:42||−40:47:52||682(±7)||9||>4.3||UTMOST, Decl ± 1.5°:Table A1|
|FRB 170107||2017-01-07 20:05:45.1397||11:23||– 05:01||609.5(±0.5)||2.6||27±4||first by ASKAP, high fluence ~58 Jy ms. In Leo. Galactic latitude 51°, Distance 3.1 Gpc, isotropic energy ~3 x 1034 J|
|unnamed||2017-08-26 13:51:44||05h 32m||+33° 08′||558(approx)||?||?||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.|
|FRB 170827||2017-08-27 16:20:18||00h 49m 18.66s||−65° 33′ 02.3″||176.4||0.395||low DM|
|FRB 170922||2017-09-22 11:23:33.4||21h 29m 50.61s||−07° 59′ 40.49″||1111||26||extreme scattering (long pulse)|
|FRB 171020||2017-10-20 10:27:58.598||22:15||– 19:40||114.1±0.2||3.2||ASKAP s/n=19.5 G-Long'=29.3 G-lat'=-51.3 Lowest DM so far.|
|FRB 171209||2017-12-09 20:34:23.5||15h 50m 25s||−46° 10′ 20″||1458||2.5||2.3|
|FRB 180301||2018-03-01 07:34:19.76||06h 12m 43.4s||+04° 33′ 44.8″||520||3||0.5||positive spectrum, from Breakthrough Listen|
|FRB 180309||2018-03-09 02:49:32.99||21h 24m 43.8s||−33° 58′ 44.5″||263.47||0.576||12|
|FRB 180311||2018-03-11 04:11:54.80||21h 31m 33.42s||−57° 44′ 26.7″||1575.6||12||2.4|
|FRB 180725A||2018-07-25 17:59:43.115||06h 13m 54.7s||+67° 04′ 00.1″||716.6||2||first detection of an FRB at radio frequencies below 700 MHz|
Realtime detection by CHIME.
|FRB 180814||Detected by CHIME. Second repeating FRB to be discovered and first since 2012.|
|FRB 180924||2018-09-24 16:23:12.6265||21h 44m 25.26s||−40° 54′ 0.1″||361.42||1.3||16||first non-repeating FRB whose source has been localized|
FRBs are also cataloged at frbcat.
- Duncan Lorimer (West Virginia University, USA); Matthew Bailes (Swinburne University); Maura McLaughlin (West Virginia University, USA); David Narkevic (West Virginia University, USA); et al. (October 2007). "A bright millisecond radio burst of extragalactic origin". Australia Telescope National Facility. Retrieved 2010-06-23.
- Lee Billings (9 July 2013). "A Brilliant Flash, Then Nothing: New "Fast Radio Bursts" Mystify Astronomers". Scientific American.
- Mann, Adam (28 March 2017). "Core Concept: Unraveling the enigma of fast radio bursts". Proc Natl Acad Sci U S A. 114 (13): 3269–3271. Bibcode:2017PNAS..114.3269M. doi:10.1073/pnas.1703512114. PMC 5380068. PMID 28351957.
- 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. Retrieved 30 August 2017.
- Osbourne, Hannah (30 August 2017). "FRBS:Repeating Radio Signals Coming From Distant Galaxy Detected By Astronomers". Newsweek. Retrieved 30 August 2017.
- Overbye, Dennis (10 January 2018). "Magnetic Secrets of Mysterious Radio Bursts in a Faraway Galaxy". The New York Times. Retrieved 11 January 2018.
- 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.
- Fedorova, V.A.; et al. (29 June 2019). "Detection of nine new Fast Radio Bursts in the direction of the galaxy M31 and M33 at the frequency 111 MHz at the radio telescope BSA LPI". The Astronomer's Telegram. Retrieved 4 July 2019.
- Staff (28 June 2019). "Search Fast Radio Burst at the frequency 111 MHz - News About Our Project". Pushchino Radio Astronomy Observatory. Retrieved 3 July 2019.
- Mack, Eric. "More mysterious signals from deep space detected - New fast radio bursts from beyond our galaxy have been recorded, adding more data to help solve one of the universe's most recent puzzles". Retrieved 3 July 2019.
- Michilli, D.; Seymour, A.; Hessels, J. W. T.; Spitler, L. G.; Gajjar, V.; Archibald, A. M.; Bower, G. C.; Chatterjee, S.; Cordes, J. M.; et al. (11 January 2018). "An extreme magneto-ionic environment associated with the fast radio burst source FRB 121102". Nature. 553 (7687): 182–185. arXiv:1801.03965. Bibcode:2018Natur.553..182M. doi:10.1038/nature25149. ISSN 0028-0836. PMID 29323297.
- Devlin, Hannah (10 January 2018). "Astronomers may be closing in on source of mysterious fast radio bursts". The Guardian.
- Strickland, Ashley (January 10, 2018). "What's sending mysterious repeating fast radio bursts in space?". CNN.
- Chatterjee, S.; Law, C. J.; Wharton, R. S.; Burke-Spolaor, S.; Hessels, J. W. T.; Bower, G. C.; Cordes, J. M.; Tendulkar, S. P.; Bassa, C. G. (January 2017). "A direct localization of a fast radio burst and its host". Nature. 541 (7635): 58–61. arXiv:1701.01098. Bibcode:2017Natur.541...58C. doi:10.1038/nature20797. ISSN 1476-4687. PMID 28054614.
- Starr, Michelle (14 August 2018). "Astronomers Have Detected a Whopping 8 New Repeating Signals From Deep Space". Science Alert.com. Retrieved 14 August 2019.
- Andersen, B.C.; et al. (9 August 2019). "CHIME/FRB Detection of Eight New Repeating Fast Radio Burst Sources". arXiv:1908.03507v1 [astro-ph.HE].
- "Cosmic radio burst caught red-handed". Royal Astronomical Society. 19 January 2015.
- News, Mike Wall 2019-01-09T18:55:23Z. "Scientists Find 13 Mysterious Deep-Space Flashes, Including 2nd Known 'Repeater'". Space.com. Retrieved 2019-03-03.
- D. R. Lorimer; M. Bailes; M. A. McLaughlin; D. J. Narkevic; et al. (27 September 2007). "A Bright Millisecond Radio Burst of Extragalactic Origin". Science. 318 (5851): 777–780. arXiv:0709.4301. Bibcode:2007Sci...318..777L. doi:10.1126/science.1147532. PMID 17901298. Retrieved 2010-06-23.
- 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.
- 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.
- Masui, Kiyoshi; Lin, Hsiu-Hsien; Sievers, Sievers; et al. (24 December 2015). "Dense magnetized plasma associated with a fast radio burst". Nature. 528 (7583): 523–525. arXiv:1512.00529. Bibcode:2015Natur.528..523M. doi:10.1038/nature15769. PMID 26633633.
- McKee, Maggie (27 September 2007). "Extragalactic radio burst puzzles astronomers". New Scientist. Retrieved 2015-09-18.
- Chiao, May (2013). "No flash in the pan". Nature Physics. 9 (8): 454. Bibcode:2013NatPh...9..454C. doi:10.1038/nphys2724.
- Sarah Burke-Spolaor; Matthew Bailes; Ronald Ekers; Jean-Pierre Macquart; Fronefield Crawford III (2010). "Radio Bursts with Extragalactic Spectral Characteristics Show Terrestrial Origins". The Astrophysical Journal. 727 (1): 18. arXiv:1009.5392. Bibcode:2011ApJ...727...18B. doi:10.1088/0004-637X/727/1/18.
- Petroff, E.; Keane, E. F.; Barr, E. D.; Reynolds, J. E.; Sarkissian, J.; Edwards, P. G.; Stevens, J.; Brem, C.; Jameson, A.; Burke-Spolaor, S.; Johnston, S.; Bhat, N. D. R.; Kudale, P. Chandra S.; Bhandari, S. (9 April 2015). "Identifying the source of perytons at the Parkes radio telescope". Monthly Notices of the Royal Astronomical Society. 451 (4): 3933–3940. arXiv:1504.02165. Bibcode:2015MNRAS.451.3933P. doi:10.1093/mnras/stv1242.
- Carnegie Mellon University (2 December 2015). "Team finds detailed record of mysterious fast radio burst". Phys.org. Retrieved 11 January 2019.
- "Radio-burst discovery deepens astrophysics mystery". Max Planck Institute. 10 July 2014.
- Chipello, Chris (2 March 2016). "Mysterious cosmic radio bursts found to repeat". McGill University News. Retrieved 2016-03-05.
- Woo, Marcus (7 June 2016). "There a re weird bursts of energy coming from deep space". BBC News. Retrieved 2016-06-07.
- 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.
- Draka, Nadia (2 March 2016). "Astronomers Discover a New Kind of Radio Blast From Space". National Geographic News. Retrieved 2016-03-03.
- G., Dai, Z.; S., Wang, J.; F., Wu, X.; F., Huang, Y. (2016-03-27). "Repeating Fast Radio Bursts from Highly Magnetized Pulsars Travelling through Asteroid Belts". The Astrophysical Journal. 829 (1): 27. arXiv:1603.08207. Bibcode:2016ApJ...829...27D. doi:10.3847/0004-637X/829/1/27.
- Gu, Wei-Min; Dong, Yi-Ze; Liu, Tong; Ma, Renyi; Wang, Junfeng (2016). "A Neutron Star-White Dwarf Binary Model for Repeating Fast Radio Burst 121102". The Astrophysical Journal. 823 (2): L28. arXiv:1604.05336. Bibcode:2016ApJ...823L..28G. doi:10.3847/2041-8205/823/2/l28.
- Scholz, P.; Spitler, L. G.; Hessels, J. W. T.; Chatterjee, S.; Cordes, J. M.; Kaspi, V. M.; Wharton, R. S.; Bassa, C. G.; Bogdanov, S. (2016-12-16). "The repeating Fast Radio Burst FRB 121102: Multi-wavelength observations and additional bursts". The Astrophysical Journal. 833 (2): 177. arXiv:1603.08880. Bibcode:2016ApJ...833..177S. doi:10.3847/1538-4357/833/2/177. ISSN 1538-4357.
- Overbye, Dennis (4 January 2017). "Radio Bursts Traced to Faraway Galaxy, but Caller Is Probably 'Ordinary Physics'". New York Times. Retrieved 4 January 2017.
- Strauss, Mark (4 January 2017). "Strange Radio Bursts Seen Coming From a Galaxy Far, Far Away". National Geographic Society. Retrieved 4 January 2017.
- Marcote, B.; Paragi, Z.; Hessels, J. W. T.; Keimpema, A.; Langevelde, H. J. van; Huang, Y.; Bassa, C. G.; S. Bogdanov; Bower, G. C. (2017-01-01). "The Repeating Fast Radio Burst FRB 121102 as Seen on Milliarcsecond Angular Scales". The Astrophysical Journal Letters. 834 (2): L8. arXiv:1701.01099. Bibcode:2017ApJ...834L...8M. doi:10.3847/2041-8213/834/2/L8. ISSN 2041-8205.
- Govert Schilling (4 January 2017). "Mysterious radio bursts originate outside the Milky Way". Science.
- Seth Shostak (23 April 2018). "FRB 121102: Radio Calling Cards from a Distant Civilization?". SETI Institute. Retrieved 9 January 2019.
- Wilford, Greg (2 September 2017). "Mysterious signals from distant galaxy spark row over whether they could be from aliens". The Independent. Retrieved 2 September 2017.
- Researchers Probe Origin of Superpowerful Radio Blasts from Space. Charles Qoi, Space.com. 10 January 2018.
- Light shed on mystery space radio pulses. Paul Rincon, BBC News. 10 January 2018.
- Gajjar, V.; Siemion, A. P. V.; Price, D. C.; Law, C. J.; Michilli, D.; Hessels, J. W. T.; Chatterjee, S.; Archibald, A. M.; Bower, G. C. (2018-08-06). "Highest-frequency detection of FRB 121102 at 4–8 GHz using the Breakthrough Listen Digital Backend at the Green Bank Telescope". The Astrophysical Journal. 863 (1): 2. arXiv:1804.04101. Bibcode:2018ApJ...863....2G. doi:10.3847/1538-4357/aad005. ISSN 1538-4357.
- Zhang, Yunfan Gerry; Gajjar, Vishal; Foster, Griffin; Siemion, Andrew; Cordes, James; Law, Casey; Wang, Yu (9 September 2018). "Fast Radio Burst 121102 Pulse Detection and Periodicity: A Machine Learning Approach". The Astrophysical Journal. 866 (2): 149. arXiv:1809.03043. Bibcode:2018ApJ...866..149Z. doi:10.3847/1538-4357/aadf31.
- Wall, Mike (11 September 2018). "Mysterious Light Flashes Are Coming from Deep Space, and AI Just Found More of Them". Space.com. Retrieved 11 September 2018.
- Starr, Michelle (11 September 2018). "Astronomers Have Detected an Astonishing 72 New Mystery Radio Bursts From Space – We still have no idea what these signals are". ScienceAlert.com. Retrieved 11 September 2018.
- Nield, David (10 September 2019). "Giant Radio Telescope in China Just Detected Repeating Signals From Across Space". ScienceAlert.com. Retrieved 10 September 2019.
- 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.
- Hippke, Michael; Domainko, Wilfried F.; Learned, John G. (30 March 2015). "Discrete steps in dispersion measures of Fast Radio Bursts". arXiv:1503.05245 [astro-ph.HE].
- Webb, Jonathan (24 February 2016). "Radio flash tracked to faraway galaxy". BBC News. Retrieved 2016-02-24.
- Keane, E. F.; Johnston, S.; et al. (25 February 2016). "The host galaxy of a fast radio burst". Nature. 530 (7591): 453–461. arXiv:1602.07477. Bibcode:2016Natur.530..453K. doi:10.1038/nature17140. PMID 26911781.
- Plait, Phil (24 February 2016). "Astronomers Solve One Mystery of Fast Radio Bursts and Find Half the Missing Matter in the Universe". Bad Astronomy – Slate. Retrieved 2016-02-24.
- "New Fast Radio Burst Discovery Finds Missing Matter in the Universe". Subaru Telescope. Space Ref. 24 February 2016. Retrieved 2016-02-25.
- "Cosmological Origin for FRB 150418? Not So Fast" (PDF).
- "ATel #8752: Radio brightening of FRB 150418 host galaxy candidate". ATel. Retrieved 2016-03-03.
- says, Franko (2016-02-29). "That Blast of Radio Waves Produced By Colliding Dead Stars? Not So Fast". Phenomena. Retrieved 2016-03-03.
- "Fast Radio Burst Afterglow Was Actually a Flickering Black Hole". Harvard-Smithsonian Center for Astrophysics (HSCFA). SpaceRef. April 4, 2016. Retrieved 2016-04-05.
- Born-again Australian telescope solves mystery of intergalactic Fast Radio Bursts. April 2017
- Australian telescope spies its first burst from beyond the galaxy, many more expected. 2017
- Fialkov, Anastasia; Loeb, Abraham (2017). "A Fast Radio Burst Occurs Every Second throughout the Observable Universe". The Astrophysical Journal Letters. 846 (2): L27. arXiv:1706.06582. Bibcode:2017ApJ...846L..27F. doi:10.3847/2041-8213/aa8905. ISSN 2041-8205.
- "Enigmatic radio burst illuminates a galaxy's tranquil halo". www.eso.org. Retrieved 27 September 2019.
- Strongest Fast Radio Burst Signal From Space Captured In Australi March 2018
- FRB catalog
- Castelvecchi, Davide (29 July 2015). "'Half-pipe' telescope will probe dark energy in teen Universe". Nature. 523 (7562): 514–515. Bibcode:2015Natur.523..514C. doi:10.1038/523514a. PMID 26223607.
- MacDonald, Fiona (6 August 2018). "Astronomers Have Detected an Intense And Mysteriously Low Frequency Radio Signal Coming From Space". ScienceAlert.com. Retrieved 6 August 2018.
- Boyle, P. J. (1 August 2018). "ATel #11901: First detection of fast radio bursts between 400 and 800 MHz by CHIME/FRB". ATel. Retrieved 2018-08-04.
- Wall, Mike (10 October 2018). "Mysterious Deep-Space Flashes: 19 More 'Fast Radio Bursts' Found". Space.com. Retrieved 10 October 2018.
- Shannon, R.M.; et al. (10 October 2018). "The dispersion–brightness relation for fast radio bursts from a wide-field survey". Nature. 562 (7727): 386–390. Bibcode:2018Natur.562..386S. doi:10.1038/s41586-018-0588-y. PMID 30305732.
- Overbye, Dennis (10 January 2019). "Broadcasting from Deep Space, a Mysterious Series of Radio Signals". The New York Times. Retrieved 11 January 2019.
- Busby, Mattha (9 January 2019). "Mysterious fast radio bursts from deep space 'could be aliens'". The Guardian. Retrieved 10 January 2019.
- Rice, Doyle (10 January 2019). "Alien signals? More bizarre 'fast radio bursts' detected from outer space". USA Today. Retrieved 10 January 2019.
- Lingam, Manasvi; Loeb, Abraham (8 March 2017). "Fast Radio Bursts from Extragalactic Light Sails". The Astrophysical Journal. 837 (2): L23. arXiv:1701.01109. Bibcode:2017ApJ...837L..23L. doi:10.3847/2041-8213/aa633e. ISSN 2041-8213.
- "Could Fast Radio Bursts Be Powering Alien Probes?". Harvards & Smithsonian Center for Astrophysics. Cambridge, Massachusetts. 8 March 2017. Retrieved 10 January 2019.
- Bannister, K. W.; Deller, A. T.; Phillips, C.; Macquart, J.-P.; Prochaska, J. X.; Tejos, N.; Ryder, S. D.; Sadler, E. M.; Shannon, R. M.; Simha, S.; Day, C. K.; McQuinn, M.; North-Hickey, F. O.; Bhandari, S.; Arcus, W. R.; Bennert, V. N.; Burchett, J.; Bouwhuis, M.; Dodson, R.; Ekers, R. D.; Farah, W.; Flynn, C.; James, C. W.; Kerr, M.; Lenc, E.; Mahony, E. K.; O’Meara, J.; Osłowski, S.; Qiu, H.; Treu, T.; U, V.; Bateman, T. J.; Bock, D. C.-J.; Bolton, R. J.; Brown, A.; Bunton, J. D.; Chippendale, A. P.; Cooray, F. R.; Cornwell, T.; Gupta, N.; Hayman, D. B.; Kesteven, M.; Koribalski, B. S.; MacLeod, A.; McClure-Griffiths, N. M.; Neuhold, S.; Norris, R. P.; Pilawa, M. A.; Qiao, R.-Y.; Reynolds, J.; Roxby, D. N.; Shimwell, T. W.; Voronkov, M. A.; Wilson, C. D. (27 June 2019). "A single fast radio burst localized to a massive galaxy at cosmological distance". Science. 365 (6453): 565–570. arXiv:1906.11476. Bibcode:2019Sci...365..565B. doi:10.1126/science.aaw5903. PMID 31249136.
- O'Callaghan, Jonathan (27 June 2019). "Mysterious Outburst's Quiet Cosmic Home Yields More Questions Than Answers". Scientific American. Retrieved 29 June 2019.
- Clery, Daniel (27 June 2019). "Baffling radio burst traced to a galaxy 3.6 billion light-years away". Science. doi:10.1126/science.aay5459.
- Ravi, V.; et al. (2 July 2019). "A fast radio burst localized to a massive galaxy". Nature. 572 (7769): 352–354. Bibcode:2019Natur.572..352R. doi:10.1038/s41586-019-1389-7. PMID 31266051.
- Mack, Eric (2 July 2019). "Another mysterious deep space signal traced to the other side of the universe - Fast radio bursts suddenly seem to be everywhere in the news, but they're still coming from very far away". CNET. Retrieved 3 July 2019.
- Totani, Tomonori (25 October 2013). "Cosmological Fast Radio Bursts from Binary Neutron Star Mergers". Publications of the Astronomical Society of Japan. 65 (5): L12. arXiv:1307.4985. Bibcode:2013PASJ...65L..12T. doi:10.1093/pasj/65.5.L12.
- Wang, Jie-Shuang; Yang, Yuan-Pei; Wu, Xue-Feng; Dai, Zi-Gao; Wang, Fa-Yin (22 April 2016). "Fast Radio Bursts from the Inspiral of Double Neutron Stars". The Astrophysical Journal. 822 (1): L7. arXiv:1603.02014. Bibcode:2016ApJ...822L...7W. doi:10.3847/2041-8205/822/1/L7.
- B. Zhang (10 January 2014). "A Possible Connection between Fast Radio Bursts and Gamma-Ray Bursts". The Astrophysical Journal Letters. 780 (2): L21. arXiv:1310.4893. Bibcode:2014ApJ...780L..21Z. doi:10.1088/2041-8205/780/2/L21.
- V. Ravi; P. D. Lasky (20 May 2014). "The birth of black holes: neutron star collapse times, gamma-ray bursts and fast radio bursts". Monthly Notices of the Royal Astronomical Society. 441 (3): 2433–2439. arXiv:1403.6327. Bibcode:2014MNRAS.441.2433R. doi:10.1093/mnras/stu720.
- Scoles, Sarah (31 March 2015). "Is this ET? Mystery of strange radio bursts from space". New Scientist. Retrieved 17 September 2015.
- Scoles, Sarah (4 April 2015). "Cosmic radio plays an alien tune". New Scientist. 226 (3015): 8–9. doi:10.1016/S0262-4079(15)30056-7.
- Calla Cofield (28 November 2017). "Little Green Men? Pulsars Presented a Mystery 50 Years Ago". Space.com. Retrieved 10 January 2019.
- S. B. Popov; K. A. Postnov (2007). "Hyperflares of SGRs as an engine for millisecond extragalactic radio bursts". arXiv:0710.2006 [astro-ph].
- "Those Blasts of Radio Waves from Deep Space? Not Aliens". Phenomena. Retrieved 2015-12-03.
- "Fast Radio Bursts Mystify Experts—for Now". www.scientificamerican.com. Retrieved 2015-12-04.
- 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–L34. arXiv:1511.07746. Bibcode:2016MNRAS.460L..30C. doi:10.1093/mnrasl/slw069. 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
- Kulkarni, S. R.; Ofek, E. O.; Neill, J. D. (29 November 2015). "The Arecibo Fast Radio Burst: Dense Circum-burst Medium". arXiv:1511.09137 [astro-ph.HE].
- Lorimer, Duncan; McLaughlin, Maura (Apr 2018). "Flashes in the Night". Scientific American.
- Bramante, Joseph; Linden, Tim (2014). "Detecting Dark Matter with Imploding Pulsars in the Galactic Center". Physical Review Letters. 113 (19): 191301. arXiv:1405.1031. Bibcode:2014PhRvL.113s1301B. doi:10.1103/PhysRevLett.113.191301. PMID 25415895.
- Fuller, Jim; Ott, Christian (2015). "Dark Matter-induced Collapse of Neutron Stars: A Possible Link Between Fast Radio Bursts and the Missing Pulsar Problem". Monthly Notices of the Royal Astronomical Society: Letters. 450 (1): L71–L75. arXiv:1412.6119. Bibcode:2015MNRAS.450L..71F. doi:10.1093/mnrasl/slv049.
- Tkachev, Igor I. (2015). "Fast radio bursts and axion miniclusters". JETP Letters. 101 (1): 1–6. arXiv:1411.3900. Bibcode:2015JETPL.101....1T. doi:10.1134/S0021364015010154.
- Liu, Tong; Romero, Gustavo E.; Liu, Mo-Lin; Li, Ang (2016). "Fast Radio Bursts and Their Gamma-Ray or Radio Afterglows as Kerr–Newman Black Hole Binaries". The Astrophysical Journal. 826 (1): 82. arXiv:1602.06907. Bibcode:2016ApJ...826...82L. doi:10.3847/0004-637x/826/1/82.
- Zhang, Bing (2016). "Mergers of Charged Black Holes: Gravitational-Wave Events, Short Gamma-Ray Bursts, and Fast Radio Bursts". The Astrophysical Journal. 827 (2): L31. arXiv:1602.04542. Bibcode:2016ApJ...827L..31Z. doi:10.3847/2041-8205/827/2/l31.
- A. Barrau; C. Rovelli & F. Vidotto (2014). "Fast radio bursts and white hole signals". Physical Review D. 90 (12): 127503. arXiv:1409.4031. Bibcode:2014PhRvD..90l7503B. doi:10.1103/PhysRevD.90.127503.
- Zhang, Fan (7 February 2017). "Pulsar magnetospheric convulsions induced by an external magnetic field". Astronomy & Astrophysics. 598 (2017): A88. arXiv:1701.01209. Bibcode:2017A&A...598A..88Z. doi:10.1051/0004-6361/201629254. ISSN 0004-6361.
- "A Cosmic Burst Repeats, Deepening a Mystery | Quanta Magazine". www.quantamagazine.org. Retrieved 2017-04-19.
- Houde, M.; Mathews, A.; Rajabi, F. (12 December 2017). "Explaining fast radio bursts through Dicke's superradiance". Monthly Notices of the Royal Astronomical Society. 475 (1): 514. arXiv:1710.00401. Bibcode:2018MNRAS.475..514H. doi:10.1093/mnras/stx3205.
- Crane, Leah (15 July 2019). "There aren't enough space explosions to explain strange radio bursts". New Scientist. Retrieved 16 July 2019.
- Ravi, Vikram (15 July 2019). "The prevalence of repeating fast radio bursts". Nature Astronomy: 405. arXiv:1907.06619. Bibcode:2019NatAs.tmp..405R. doi:10.1038/s41550-019-0831-y. Retrieved 16 July 2019.
- 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.
- 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.
- Dan Thornton (September 2013). The High Time Resolution Radio Sky (PDF) (Thesis). Manchester. pp. 140–147.
- 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.
- Ravi, V.; Shannon, R. M.; Jameson, A. (14 January 2015). "A Fast Radio Burst in the Direction of the Carina Dwarf Spheroidal Galaxy". The Astrophysical Journal. 799 (1): L5. arXiv:1412.1599. Bibcode:2015ApJ...799L...5R. doi:10.1088/2041-8205/799/1/L5.
- 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.
- 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.
- FRBs: New Mystery Space Signal from Unknown Cosmic Source Leaves Scientists Baffled. Hannah Osbourne, Newsweek. 11 May 2017.
- The magnetic field and turbulence of the cosmic web measured using a brilliant fast radio burst. Science. 17 Nov 2016arxiv pre-pub
- Farah, W. (2 September 2017). "ATel #10697: Real-time detection of a Fast Radio Burst at the Molonglo Radio Telescope". ATel.
- Farah, W. "ATel #10867: Detection of a highly scattered Fast Radio Burst at the Molonglo Radio Telescope". ATel.
- 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.
- Price, Danny C. "ATel #11376: Detection of a new fast radio burst during Breakthrough Listen observations". ATel.
- 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.
- 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". ATel. Retrieved 20 March 2018.
- First detection of fast radio bursts between 400 and 800 MHz by CHIME/FRB. (PDF). CHIME/FRB Collaboration. 1 August 2018. Accessed: 19 August 2018.
- "AA-ALERT". www.frbcat.org. Retrieved 2018-04-16.
- "FRB Catalogue". Swinburne University of Technology.