Decoding the Mystery of FRB 20121102
Researchers investigate the repeating fast radio bursts from a distant galaxy.
C. Gouiffés, C. Ng, I. Cognard, M. Dennefeld, N. Devaney, V. S. Dhillon, J. Guilet, P. Laurent, E. Le Floc'h, A. J. Maury, K. Nimmo, A. Shearer, L. G. Spitler, P. Zarka, S. Corbel
― 5 min read
Table of Contents
- What Are Fast Radio Bursts?
- Why Are We Observing FRB 20121102?
- The Friendly Neighborhood Telescopes
- Nançay Radio Telescope
- INTEGRAL Satellite
- Observatoire de Haute Provence
- Campaigns to Catch the Bursts
- What Did They Find?
- Learning More About the Host Galaxy
- Theories About What’s Happening
- The Search for Counterparts
- Conclusion
- Original Source
- Reference Links
Fast Radio Bursts (FRBs) are like the cosmic equivalent of loud fireworks, appearing for just a brief moment but making a big noise in the universe. These bursts come from very far away, and we're still trying to figure out what causes them. Some people think they might be linked to exploding stars or other exciting cosmic events. One specific FRB that has captured a lot of attention is FRB 20121102. It’s been the focus of a long-term monitoring effort using various telescopes and observatories.
What Are Fast Radio Bursts?
FRBs are bright bursts of radio waves that last just a few milliseconds. They were first discovered in 2007 and have since puzzled scientists. Most FRBs look like one-time events, but FRB 20121102 is a special case. It likes to repeat itself, which has led scientists to get a bit more excited about it. The bursts from this particular FRB can be seen across a variety of radio frequencies, which suggests that they're coming from a very energetic source.
Why Are We Observing FRB 20121102?
To figure out what FRB 20121102 is, researchers have been on the lookout for its "relatives" in other types of light, such as X-rays and optical light. Collecting data across different wavelengths helps scientists piece together the story of this enigmatic burst. The idea is that by monitoring it closely, they can learn more about its nature and possibly even its origins.
The Friendly Neighborhood Telescopes
Nançay Radio Telescope
In France, the Nançay Radio Telescope (NRT) is like the local watchtower for FRB 20121102. This radio telescope has been busy keeping tabs on the FRB from 2016 to 2020. It's a big radio dish that captures signals from space, allowing researchers to observe radio bursts effectively.
INTEGRAL Satellite
Meanwhile, the INTEGRAL satellite is floating above us, watching the sky for high-energy light. It was launched way back in 2002 and has been collecting data ever since. INTEGRAL can capture very high-energy photons, which might help find counterparts to the radio bursts.
Observatoire de Haute Provence
There's also the Observatoire de Haute Provence, which has been set up with multiple telescopes to look for any possible optical light associated with FRB 20121102. They have fancy cameras that can take super-fast pictures, increasing the chances of spotting something fleeting.
Campaigns to Catch the Bursts
Between 2017 and 2019, campaigns were organized to gather data on FRB 20121102. In 2017, the plan was to observe simultaneously with INTEGRAL and other ground-based telescopes. However, things didn’t go as expected, and FRB 20121102 decided to take a break during the campaign. So, no radio bursts were detected, and the researchers were left in the dark - no fireworks that year!
In 2019, they tried a different approach. They decided to conduct "Target of Opportunity" observations. If the NRT detected a burst, it would send up a flare (figuratively speaking), and INTEGRAL would then aim its instruments at FRB 20121102. This time around, they managed to detect bursts and had a successful campaign!
What Did They Find?
After all those observations, the researchers didn’t find much in terms of X-ray emissions alongside the radio bursts. It’s a bit like expecting to find a shadow at night with no light - sometimes, things just don’t match up. The NRT detected multiple radio bursts, which helped to better understand the periodic window of activity of this FRB. They figured out that FRB 20121102 has a pattern, or a “cycle,” of activity that lasts for about 154 days.
Learning More About the Host Galaxy
FRB 20121102 is located inside a faint dwarf galaxy. This galaxy has very low metallicity, which means it’s not filled with a lot of heavy elements. Such environments are often where energetic events like gamma-ray bursts occur, which could give more clues about what FRBs are.
Theories About What’s Happening
There are many theories about the causes of FRBs, and FRB 20121102 is no exception. Some scientists propose that Magnetars - a type of neutron star - are behind these bursts. Magnetars have super-strong magnetic fields and can produce a variety of emissions. Think of them as the rebellious teenagers of the star world - full of energy and unpredictability.
The Search for Counterparts
Researchers are on the lookout for any other types of light that could be connected to FRB 20121102. They’ve scoured the optical and X-ray realms to see if they can spot what’s going on around this FRB. So far, their results have given them upper limits of energy emissions in those wavelengths. It’s like looking for a needle in a haystack, and so far, they’ve found only the edges.
Conclusion
The pursuit of understanding FRB 20121102 continues, and researchers remain eager to collect more data. They hope that as technology improves and more observations are made, they’ll finally pinpoint what's causing this cosmic mystery. Until then, FRB 20121102 will remain a fascinating puzzle, keeping astronomers busy and curious about the broader universe. Who knew that chasing after some radio bursts could lead to such a thrilling cosmic adventure?
Title: Long term monitoring of FRB~20121102 with the Nan\c{c}ay Radio Telescope and multi-wavelength campaigns including INTEGRAL
Abstract: The origin(s) of Fast Radio Bursts (FRBs), mysterious radio bursts coming from extragalactic distances, remains unknown. Multi-wavelength observations are arguably the only way to answer this question unambiguously. We attempt to detect hard X-ray/soft gamma-ray counterparts to one of the most active FRB sources, FRB20121102, as well as improve understanding of burst properties in radio through a long-term monitoring campaign using the Nan\c{c}ay Radio Telescope (NRT). Multi-wavelength campaigns involving the International Gamma-ray Astrophysics Laboratory (INTEGRAL) satellite, the Nan\c{c}ay Radio Observatory, the optical telescopes at the Observatoire de Haute Provence as well as Arecibo were conducted between 2017 and 2019. In 2017, the telescopes were scheduled to observe simultaneously between Sept 24-29. We specifically used the Fast Response Enhanced CCDs for the optical observations to ensure a high time resolution. In 2019, we changed the strategy to instead conduct ToO observations on INTEGRAL and other available facilities upon positive detection triggers from the NRT. In the 2017 campaign, FRB20121102 was not in its burst activity window. We obtain a 5-sigma optical flux limit of 12 mJy ms using the GASP and a 3-sigma limit from OHP T120cm R-band image of R=22.2 mag of any potential persistent emission not associated to radio bursts. In the 2019 campaign, we have simultaneous INTEGRAL data with 11 radio bursts from the NRT and Arecibo. We obtain a 5-sigma upper limit of 2.7e-7 erg/cm2 in the 25-400 keV energy range for contemporary radio and high energy bursts, and a 5-sigma upper limit of 3.8e-11 erg/cm2 for permanent emission in the 25-100 keV energy range. In addition, we report on the regular observations from NRT between 2016-2020, which accounts for 119 additional radio bursts from FRB20121102. We present an updated fit of the periodic active window of 154+/-2 days.
Authors: C. Gouiffés, C. Ng, I. Cognard, M. Dennefeld, N. Devaney, V. S. Dhillon, J. Guilet, P. Laurent, E. Le Floc'h, A. J. Maury, K. Nimmo, A. Shearer, L. G. Spitler, P. Zarka, S. Corbel
Last Update: 2024-11-25 00:00:00
Language: English
Source URL: https://arxiv.org/abs/2411.16419
Source PDF: https://arxiv.org/pdf/2411.16419
Licence: https://creativecommons.org/licenses/by/4.0/
Changes: This summary was created with assistance from AI and may have inaccuracies. For accurate information, please refer to the original source documents linked here.
Thank you to arxiv for use of its open access interoperability.
Reference Links
- https://www.overleaf.com/project/651a9fe1edcf5172ff02a379
- https://www.overleaf.com/project/651a9fe1edcf5172ff02a379structured
- https://www.isdc.unige.ch/integral/analysis
- https://github.com/scottransom/presto
- https://nenufar.obs-nancay.fr/en/astronomer/
- https://www.jb.man.ac.uk/~pulsar/crab.html
- https://chimefrb.github.io/fitburst/installation/