The CHIME/FRB Discovery of the Extremely Active Fast Radio Burst Source FRB 20240114A
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arXiv
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| Natura: | Preprint |
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2025
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| author | Shin, Kaitlyn Curtin, Alice Fine, Maxwell Pandhi, Ayush Andrew, Shion Bhardwaj, Mohit Chatterjee, Shami Cook, Amanda M. Fonseca, Emmanuel Gaensler, B. M. Hessels, Jason Jain, Naman Kaspi, Victoria M. Kharel, Bikash Lanman, Adam E. Lazda, Mattias Leung, Calvin Main, Robert Masui, Kiyoshi W. Michilli, Daniele Ng, Mason Nimmo, Kenzie Pearlman, Aaron B. Pen, Ue-Li Pleunis, Ziggy Rafiei-Ravandi, Masoud Sammons, Mawson Sand, Ketan R. Scholz, Paul Smith, Kendrick Stairs, Ingrid |
| author_facet | Shin, Kaitlyn Curtin, Alice Fine, Maxwell Pandhi, Ayush Andrew, Shion Bhardwaj, Mohit Chatterjee, Shami Cook, Amanda M. Fonseca, Emmanuel Gaensler, B. M. Hessels, Jason Jain, Naman Kaspi, Victoria M. Kharel, Bikash Lanman, Adam E. Lazda, Mattias Leung, Calvin Main, Robert Masui, Kiyoshi W. Michilli, Daniele Ng, Mason Nimmo, Kenzie Pearlman, Aaron B. Pen, Ue-Li Pleunis, Ziggy Rafiei-Ravandi, Masoud Sammons, Mawson Sand, Ketan R. Scholz, Paul Smith, Kendrick Stairs, Ingrid |
| contents | Among the thousands of observed fast radio bursts (FRBs), a few sources exhibit exceptionally high burst activity observable by many telescopes across a broad range of radio frequencies. Almost all of these highly active repeaters have been discovered by CHIME/FRB, due to its daily observations of the entire Northern sky as a transit radio telescope. FRB 20240114A is a source discovered and reported by CHIME/FRB to the community in January 2024; given its low declination, even the detection of a few bursts hints at a high burst rate. Following the community announcement of this source as a potentially active repeater, it was extensively followed up by other observatories and has emerged as one of the most prolific FRB repeaters ever observed. This paper presents the five bursts CHIME/FRB observed from FRB 20240114A, with channelized raw voltage data saved for two bursts. We do not observe changes in the DM of the source greater than ~1.3 pc cm$^{-3}$ in our observations over nearly a year baseline. We find an RM of ~ +320 rad m$^{-2}$. We do not find evidence for scattering at the level of < 0.3 ms in the bursts, and we find no evidence for astrophysical scintillation. In our observations of FRB 20240114A, we see a burst rate ~49x higher than the median burst rate of apparent non-repeaters also discovered by CHIME/FRB. Each discovery of highly active FRBs provides a valuable opportunity to investigate whether there is a fundamental difference between repeating and apparently non-repeating sources. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2505_13297 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | The CHIME/FRB Discovery of the Extremely Active Fast Radio Burst Source FRB 20240114A Shin, Kaitlyn Curtin, Alice Fine, Maxwell Pandhi, Ayush Andrew, Shion Bhardwaj, Mohit Chatterjee, Shami Cook, Amanda M. Fonseca, Emmanuel Gaensler, B. M. Hessels, Jason Jain, Naman Kaspi, Victoria M. Kharel, Bikash Lanman, Adam E. Lazda, Mattias Leung, Calvin Main, Robert Masui, Kiyoshi W. Michilli, Daniele Ng, Mason Nimmo, Kenzie Pearlman, Aaron B. Pen, Ue-Li Pleunis, Ziggy Rafiei-Ravandi, Masoud Sammons, Mawson Sand, Ketan R. Scholz, Paul Smith, Kendrick Stairs, Ingrid High Energy Astrophysical Phenomena Among the thousands of observed fast radio bursts (FRBs), a few sources exhibit exceptionally high burst activity observable by many telescopes across a broad range of radio frequencies. Almost all of these highly active repeaters have been discovered by CHIME/FRB, due to its daily observations of the entire Northern sky as a transit radio telescope. FRB 20240114A is a source discovered and reported by CHIME/FRB to the community in January 2024; given its low declination, even the detection of a few bursts hints at a high burst rate. Following the community announcement of this source as a potentially active repeater, it was extensively followed up by other observatories and has emerged as one of the most prolific FRB repeaters ever observed. This paper presents the five bursts CHIME/FRB observed from FRB 20240114A, with channelized raw voltage data saved for two bursts. We do not observe changes in the DM of the source greater than ~1.3 pc cm$^{-3}$ in our observations over nearly a year baseline. We find an RM of ~ +320 rad m$^{-2}$. We do not find evidence for scattering at the level of < 0.3 ms in the bursts, and we find no evidence for astrophysical scintillation. In our observations of FRB 20240114A, we see a burst rate ~49x higher than the median burst rate of apparent non-repeaters also discovered by CHIME/FRB. Each discovery of highly active FRBs provides a valuable opportunity to investigate whether there is a fundamental difference between repeating and apparently non-repeating sources. |
| title | The CHIME/FRB Discovery of the Extremely Active Fast Radio Burst Source FRB 20240114A |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2505.13297 |