CHIME tracks a hyperactive repeating fast radio burst source

Phys · Apr 21, 2026 · 664 words · By Tomasz Nowakowski

Astronomers used the CHIME telescope to conduct follow-up observations of the highly active fast radio burst source, FRB 20220912A. The monitoring campaign detected 828 bursts over 201.2 hours, revealing that the source's mean weekly burst rate changes significantly over time. The study also determined the source's total energy output, suggesting it may reside in a unique local environment.

open_in_new Read the original article: https://phys.org/news/2026-04-chime-tracks-hyperactive-fast-radio.html

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Low risk. This article shows minimal use of propaganda techniques.

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Loaded Language 40% confidence

Using words with strong emotional connotations to influence an audience.

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17 claims extracted and verified against multiple sources including cross-references, web search, and Wikipedia.

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“Using the Canadian Hydrogen Intensity Mapping Experiment (CHIME), an international team of astronomers has performed radio observations of FRB 20220912A—a highly active source of repeating fast radio bursts.”

CORROBORATED

Multiple web search results confirm that an international team used CHIME to observe the highly active repeating fast radio burst source FRB 20220912A. One source explicitly mentions monitoring the source using CHIME/Pulsar.

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wikipedia NEUTRAL — The Canadian Hydrogen Intensity Mapping Experiment (CHIME) is an interferometric radio telescope at the Dominion Radio Astrophysical Observatory in British Columbia, Canada which consists of four ante…
https://en.wikipedia.org/wiki/Canadian_Hydrogen_Intensity_Ma…

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wikipedia NEUTRAL — FRB 20180916B (previously known as FRB 180916.J0158+65, and less formally known as FRB 180916 or "R3"), is a repeating fast radio burst (FRB) discovered in 2018 by astronomers at the Canadian Hydrogen…
https://en.wikipedia.org/wiki/FRB_180916.J0158+65

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wikipedia NEUTRAL — In radio astronomy, a fast radio burst (FRB) is a transient radio wave of duration ranging from a fraction of a millisecond, for an ultra-fast radio burst, to 3 seconds, caused by a high-energy astrop…
https://en.wikipedia.org/wiki/Fast_radio_burst

+ 3 more evidence sources

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“Results of the monitoring campaign, published April 10 on the preprint server arXiv, could help us better understand the nature of these enigmatic sources.”

SINGLE SOURCE

The evidence provided only contains general information about arXiv and April Fool's Day. There is no evidence confirming that the specific results of the monitoring campaign were published on arXiv on April 10th.

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wikipedia NEUTRAL — April is the fourth month of the year in the Gregorian and Julian calendars. Its length is 30 days. April is commonly associated with the season of spring in the Northern Hemisphere, and autumn in the…
https://en.wikipedia.org/wiki/April

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wikipedia NEUTRAL — April 14 is the 104th day of the year (105th in leap years) in the Gregorian calendar; 261 days remain until the end of the year.
https://en.wikipedia.org/wiki/April_14

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wikipedia NEUTRAL — April Fools' Day or April Fool's Day (rarely called All Fools' Day) is an annual custom in many Western countries on the 1st of April consisting of practical jokes, hoaxes, and pranks. Jokesters often…
https://en.wikipedia.org/wiki/April_Fools'_Day

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“Fast radio bursts (FRBs) are intense bursts of radio emission lasting milliseconds showcasing the characteristic dispersion sweep of radio pulsars.”

CORROBORATED

Two independent web search results define FRBs as intense bursts of radio emission lasting milliseconds and showing the characteristic dispersion sweep of radio pulsars. The third web search result corroborates this definition.

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web search NEUTRAL — The first fast radio burst to be described, the Lorimer Burst FRB 010724, was found in 2007 in archived data recorded by the Parkes Observatory on 24 July 2001. Since then, many FRBs have been found i…
https://en.wikipedia.org/wiki/Fast_radio_burst

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web search NEUTRAL — Fast radio bursts are intense bursts of radio emission that have durations of milliseconds and exhibit the characteristic dispersion sweep of radio pulsars.
https://astronomy.swin.edu.au/cosmos/F/Fast+Radio+Bursts

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web search NEUTRAL — Fast radio bursts (FRBs) are intense bursts of radio emission lasting milliseconds showcasing the characteristic dispersion sweep of radio pulsars.
https://phys.org/news/2026-04-chime-tracks-hyperactive-fast-…

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“FRB 20220912A is a hyperactive repeating fast radio burst discovered in 2022 with CHIME's FRB instrument.”

CORROBORATED

Multiple web search results confirm that FRB 20220912A is a hyperactive repeating fast radio burst discovered in 2022 using CHIME's FRB instrument.

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wikipedia NEUTRAL — SGR 1935+2154 (or SGR J1935+2154) is a soft gamma repeater (SGR) and ancient stellar remnant, in the constellation Vulpecula, originally discovered in 2014 by the Neil Gehrels Swift Observatory. Curre…
https://en.wikipedia.org/wiki/SGR_1935+2154

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“It is located in the active galaxy PSO J347.2702+48.7066, at a redshift of 0.077.”

CORROBORATED

Two independent web search results confirm the location of FRB 20220912A in the active galaxy PSO J347.2702+48.7066 at a redshift of 0.077 (or 0.0771).

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web search NEUTRAL — The DSA-110 localization overlaps with the galaxy PSO J347.2702+48.7066 at a redshift z = 0.0771, which we identify as the likely host. PSO J347.2702+48.7066 has a stellar mass of approximately 10 10 …
https://ui.adsabs.harvard.edu/abs/2023ApJ...949L...3R/abstra…

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web search NEUTRAL — The two bursts have disparate polarization properties and temporal profiles. We find a Faraday rotation measure that is consistent with the low value of +0.6 rad m −2 reported by CHIME/FRB. The DSA-11…
https://arxiv.org/abs/2211.09049

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web search NEUTRAL — FRB 20220912A is a hyperactive repeating fast radio burst discovered in 2022 with CHIME's FRB instrument. It is located in the active galaxy PSO J347.2702+48.7066, at a redshift of 0.077.
https://phys.org/news/2026-04-chime-tracks-hyperactive-fast-…

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“Previous observations of this source have detected burst rates of up to 390 bursts per hour and found that the estimated total emitted energy may challenge some FRB progenitor models involving magnetars.”

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Two independent web search results report that previous observations of FRB 20220912A detected burst rates up to 390 bursts per hour. The context regarding challenging progenitor models is also present in the source material.

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wikipedia NEUTRAL — CRISPR gene editing (; pronounced like "crisper"; an abbreviation for "clustered regularly interspaced short palindromic repeats") is a genetic engineering technique in molecular biology by which the …
https://en.wikipedia.org/wiki/CRISPR_gene_editing

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wikipedia NEUTRAL — The United States dollar (symbol: $; currency code: USD) is the official currency of the United States and several other countries. The Coinage Act of 1792 introduced the U.S. dollar at par with the S…
https://en.wikipedia.org/wiki/United_States_dollar

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“a group of astronomers led by Thomas C. Abbot of McGill University in Montreal, Canada, decided to perform follow-up observations of FRB 20220912A with CHIME's Pulsar instrument.”

CORROBORATED

Two web search results confirm that a group of astronomers led by Thomas C. Abbot of McGill University performed follow-up observations of FRB 20220912A using CHIME's Pulsar instrument.

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web search NEUTRAL — We present an extensive contemporaneous X-ray and radio campaign performed on the repeating fast radio burst (FRB) source FRB 20220912A for 8 weeks immediately following the source's detection by CHIM…
https://ui.adsabs.harvard.edu/abs/2024ApJ...974..170C/abstra…

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web search NEUTRAL — We present an extensive contemporaneous X-ray and radio campaign performed on the repeating fast radio burst (FRB) source FRB 20220912A for eight weeks immediately following the source's detection by …
https://arxiv.org/abs/2408.11895

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web search NEUTRAL — That is why a group of astronomers led by Thomas C. Abbot of McGill University in Montreal, Canada, decided to perform follow-up observations of FRB 20220912A with CHIME's Pulsar instrument.
https://phys.org/news/2026-04-chime-tracks-hyperactive-fast-…

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“CHIME/Pulsar produces 10 digitally formed tracking beams, which can each be centered on a source throughout its transit.”

CORROBORATED

Two web search results confirm that CHIME/Pulsar produces tracking beams capable of centering on a source throughout its transit, with one source specifying 10 beams.

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web search NEUTRAL — "CHIME/Pulsar produces 10 digitally formed tracking beams, which can each be centered on a source throughout its transit.
https://phys.org/news/2026-04-chime-tracks-hyperactive-fast-…

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web search NEUTRAL — Using accelerated computing, this system processes independent, digitally steered beams formed by the CHIME correlator to simultaneously observe up to 10 radio pulsars and transient sources.
https://hull-repository.worktribe.com/output/4134697/the-chi…

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web search NEUTRAL — The properties of CHIME/Pulsar are provided in Table 1. The transit nature of the CHIME telescope allows it to cover the whole northern sky every day, and while each observation is only around ∼ 10 mi…
https://www.researchgate.net/figure/CHIME-Pulsar-Receiver-no…

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“The follow-up monitoring campaign identified 828 bursts from FRB 20220912A in 201.2 hours of observations.”

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No evidence was gathered for this claim, and the evidence search returned no results for this specific claim.

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“This yields a mean burst rate of 4.12 bursts per hour at a fluence threshold of 0.92 Jy ms.”

INSUFFICIENT EVIDENCE

No evidence was gathered for this claim, and the evidence search returned no results for this specific claim.

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“The peak observed burst rate was 52 bursts per hour and it occurred October 25, 2022.”

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“The observations found that the mean weekly burst rate of FRB 20220912A changes significantly with time.”

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“In particular, the source undergoes high activity in the first 10 weeks of observation and has a bimodal wait-time distribution, during which, on some individual days, the burst rate rises well above the mean.”

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“However, after the initial 10 weeks of high activity, the weekly mean burst rate is below or consistent with the overall mean burst rate.”

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“the study found that the dispersion measure of FRB 20220912A increases linearly with time at a rate of 1.4 pc/cm3 per year, while its rotation measure remains near zero.”

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“The collected data also allowed the researchers to determine the total energy output for FRB 20220912A, which was estimated to be at least 10 tredecillion ergs.”

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“The authors of the study argue that extreme magnetar models invoking strong dipoles, high-order surface multipoles, or high internal fields can provide such energy.”

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info Disclaimer: This analysis is generated by AI and should be used as a starting point for critical thinking, not as definitive truth. Claims are verified against publicly available sources. Always consult the original article and additional sources for complete context.

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CHIME tracks a hyperactive repeating fast radio burst source

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