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Article
Astronomy & Astrophysics
J. N. Jahns et al.
Summary: We discovered 849 new bursts from FRB 20121102A using the 305-m Arecibo Telescope, with a burst rate of up to 218 per hour, the highest observed so far. The times between consecutive bursts show a bimodal distribution and a Poisson process with varying rate best describes the arrival times with separations > 0.1 s. The spectro-temporal structure of the bursts reveals a linear relationship between the sub-burst's drift and its duration, which is consistent with the sad-trombone effect.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
K. Nimmo et al.
Summary: The repeating fast radio burst source FRB 20200120E is associated with a globular cluster and exhibits a burst storm with 53 bursts occurring within 40 minutes. The burst storm shows steep energy distribution and a bimodal wait-time distribution.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Yuan-Pei Yang et al.
Summary: Recently, it was found that fast radio burst (FRB) repeaters display complex variations of Faraday rotation measures (RMs), indicating a magnetized environment that evolves dynamically. Several astrophysical processes were investigated to explain the RM variations, including supernova remnants, binary systems, pair plasma from neutron stars, and outflows from massive black holes. The results suggest that young supernova remnants or massive star companions are more likely to cause the observed RM variations, while scenarios involving low-mass star flares or pair plasma can be ruled out. The presence of a massive black hole in the vicinity of the FRB source could also explain the large RM variations.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Bridget Andersen et al.
Summary: We have discovered 25 new repeating fast radio burst (FRB) sources using a clustering algorithm that identifies colocated events with similar dispersion measures (DMs). The repeaters have DMs ranging from approximately 220 to 1700 pc cm(-3), with as few as two bursts and as many as twelve. We observe a significant difference in DM and extragalactic DM distributions between repeating and nonrepeating sources, with repeaters showing lower mean values. The repeater fraction tends to stabilize at 2.6% over our total time-on-sky.
ASTROPHYSICAL JOURNAL
(2023)
Article
Astronomy & Astrophysics
R. Mckinven et al.
Summary: Fast radio burst (FRB) source FRB 20180916B exhibits a 16.33-day periodicity in its burst activity. The polarization properties of 44 bursts from FRB 20180916B detected by CHIME/FRB show significant variations in the Faraday rotation measure (RM), as well as an apparent secular increase in RM accompanied by a possible drift of the emitting band to lower frequencies. This suggests that the observed RM evolution is likely produced from coherent changes in the Faraday-active medium's magnetic field.
ASTROPHYSICAL JOURNAL
(2023)
Article
Astronomy & Astrophysics
Z. Y. Zhao et al.
Summary: Recent observations have found that some repeating fast radio bursts (FRBs) exhibit complex variations and reversals in Faraday rotation measures (RMs), suggesting they originate from magnetized environments. One possible explanation is that pulsars in binary systems, particularly those with high-mass companions and strong stellar outflows, generate these repeating FRBs. In this study, the researchers investigate the RM variations caused by stellar winds and a potential stellar disk, suggesting that by monitoring long-term RM changes, the environments of repeating FRBs can be revealed.
ASTROPHYSICAL JOURNAL
(2023)
Review
Physics, Multidisciplinary
Bing Zhang
Summary: This review discusses the phenomenology and underlying physics of Fast radio bursts (FRBs). It covers topics such as observational data, basic plasma physics, constraints on FRB models from the data, radiation mechanisms, source and environment models, propagation effects, as well as the potential of FRBs as cosmological probes. The paper also addresses current pressing problems and future prospects.
REVIEWS OF MODERN PHYSICS
(2023)
Article
Astronomy & Astrophysics
R. Mckinven et al.
Summary: Repeating fast radio bursts (FRBs) exhibit a wide range of burst properties and host-galaxy associations. By monitoring 12 repeating sources over multiple years using the Canadian Hydrogen Intensity Mapping Experiment (CHIME), significant rotation measure (RM) variations were observed from several sources, including changes of several hundred radians per square meter over month timescales. The findings suggest that repeating FRBs and pulsars occupy distinct magnetoionic environments.
ASTROPHYSICAL JOURNAL
(2023)
Article
Astronomy & Astrophysics
Pravir Kumar et al.
Summary: The study of impulsive astrophysical radio emission allows us to investigate the plasma between the emission source and the Earth. The circular propagating wave modes in cold electron-ion plasmas affect the linear polarization plane, while in relativistic plasmas, the wave modes can convert linearly polarized emission into circular and vice versa. Fast radio bursts (FRBs) provide an opportunity to study the intergalactic and magneto-ionic medium. This article presents the polarimetric analysis of a repeat burst from the FRB 20201124A source, which displays a unique frequency-dependent circular polarization. The observed circular polarization can be explained by the propagation of a linearly polarized burst signal through a relativistic plasma along the line of sight from the progenitor.
Article
Astronomy & Astrophysics
Shivani Bhandari et al.
Summary: This study presents the localization and host galaxies of one repeating and two apparently nonrepeating fast radio bursts (FRBs). The results show that there are no significant differences in the host properties of repeating and apparently nonrepeating FRBs. The host galaxies of FRBs are moderately star forming and have global properties similar to core-collapse supernovae and short gamma-ray bursts hosts.
ASTRONOMICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
Di Xiao et al.
Summary: The total number of observed fast radio burst (FRB) events is increasing rapidly due to the improvement of existing radio telescopes and the introduction of new facilities. A recent study found a bimodal distribution in the bursts, leading to a reevaluation of the definition of FRBs. The study proposes using brightness temperature to distinguish between two subtypes of FRBs, with classical FRBs exhibiting a tight pulse width-fluence relation and atypical FRBs potentially originating from a different type of physical process.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
S. Hutschenreuter et al.
Summary: This work updates the reconstruction of the Galactic Faraday rotation sky using the latest Faraday rotation data sets. The results show a thinner and more pronounced Galactic disc with small-scale structures exceeding several thousand rad m(-2). The improved resolution and handling of noisy and incomplete data contribute to these findings.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Brian D. Metzger et al.
Summary: This article introduces a toy model to describe the time-frequency structure of fast radio bursts. By varying a parameter in the model, the burst's duration and frequency bandwidth can be transformed, potentially providing insights into the external environment differences of different FRB sources.
ASTROPHYSICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
Paz Beniamini et al.
Summary: This article describes the relationship between the observed polarization properties of an astronomical object and its intrinsic polarization properties, as well as the finite temporal and spectral resolutions of the observing device. It also discusses the impact of a scattering screen with a non-zero magnetic field on the observed polarization properties. The findings highlight the importance of the observing bandwidth, coherence bandwidth, and temporal resolution in determining the polarization properties.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
V. R. Marthi et al.
Summary: Observations of FRB20201124A using uGMRT revealed interesting phenomena such as intense radio bursts, persistent radio emission, and a high number of bursts detected. Analysis of the brightest burst led to determination of a dispersion measure and the finding that waiting times between bursts follow an exponential distribution. Additionally, measurements were made of spectro-temporal drift rates and an upper limit on scattering time.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Review
Astronomy & Astrophysics
E. Petroff et al.
Summary: Since the discovery of the first fast radio burst (FRB) in 2007, the study of FRBs has expanded rapidly. Recent observations have provided a wealth of information about FRBs, including their abundance, repeaters, host galaxies, and source activity. Surprising discoveries, such as the connection between FRBs and magnetars and the localization of FRBs to specific clusters, have also been made.
ASTRONOMY AND ASTROPHYSICS REVIEW
(2022)
Article
Astronomy & Astrophysics
Stella Koch Ocker et al.
Summary: The repeating fast radio burst FRB 20190520B is localized to a nearby galaxy. The observed dispersion measure and scattering phenomena provide support for a novel technique for estimating FRB redshifts and are consistent with previous findings.
ASTROPHYSICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
Casey J. Law et al.
Summary: The researchers discovered a second radio source (PRS) associated with a fast radio burst (FRB), but the relationship between FRBs and PRS is still unclear. They proposed a practical definition for PRS and modeled the probability distribution of FRBs with PRS, finding no strong evidence for a preferential association between repeating FRBs and PRS. They discussed how FRB/PRS sources can be distinguished through active repetition and excess dispersion measure. Using observations, they also estimated the average repetition rate and the density of FRB-emitting sources in the local universe. They found that the density and phenomenology of PRS are similar to off-nuclear wandering active galactic nuclei (AGN), suggesting that some PRS may have been misidentified as AGN.
ASTROPHYSICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
Adam E. Lanman et al.
Summary: This paper reports on the bursts detected by CHIME/FRB from the repeating FRB 20201124A, including their morphologies, fluences, and arrival times. The observations show a significant change in the event rate before and after discovery. Through maximum-likelihood estimation, we find a best-fit index for a power-law luminosity function that is consistent with other repeating FRBs.
ASTROPHYSICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
Sibasish Laha et al.
Summary: In this study, multiwavelength observations were conducted on FRB 180301, detecting five bright radio bursts with no coincident X-ray emission. The upper limits on X-ray flux were determined to be <7.64 x 10(-12) erg cm(-2) s(-1) for persistent flux and <2 x 10(-11) erg cm(-2) for 5 ms fluence, showing a consistency with magnetospheric models and synchrotron maser models involving relativistic shocks. The estimated radio efficiency also supports these models, with an estimated value greater than or similar to 10^(-8).
ASTROPHYSICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
P. Kumar et al.
Summary: The mechanism and emission properties of repeating fast radio burst (FRB) sources are not well understood. In this study, observations of the FRB source 20201124A were conducted using the Australian Square Kilometre Array Pathfinder (ASKAP) and the Ultra-wideband Low (UWL) receiver at the Parkes 64-m radio telescope. The results show significant findings, including the brightest burst ever observed from a repeating FRB source with ASKAP, highly polarized bursts from UWL, and evidence of circular polarization in one of the UWL bursts.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
A. Plavin et al.
Summary: This study investigates the properties of the persistent radio counterpart to FRB 121102 and a bright burst. The observations reveal the highest burst Faraday rotation measure to date, consistent with a decreasing trend. The width of the burst environment and the fractional polarization can be reconciled, suggesting possible non-uniformities or effects in the emitting region itself. The size of the persistent source is barely consistent with a young supernova scenario, and the flux variability and fractional polarization of the faint persistent source challenge other interpretations.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Multidisciplinary Sciences
F. Kirsten et al.
Summary: The fast radio burst FRB 20200120E is reported to originate from a globular cluster in the galaxy M81, which challenges previous models that invoke young magnetars as the source of FRBs. Instead, it is proposed that FRB 20200120E may come from a highly magnetized neutron star formed through the collapse of a white dwarf or the merger of compact stars in a binary system.
Article
Multidisciplinary Sciences
Yi Feng et al.
Summary: Observations of five repeating FRBs revealed a trend of lower polarization at lower frequencies. This behavior can be modeled as multipath scattering, characterized by the rotation measure (RM) scatter. Sources with higher RM scatter have higher RM magnitude and scattering time scales. Furthermore, the two sources with the highest RM scatter are associated with compact persistent radio sources.
Article
Astronomy & Astrophysics
K. Nimmo et al.
Summary: Recent observational measurements of the nearby fast radio burst FRB 20200120E connect these extreme extragalactic transients with studies of Galactic neutron stars. The observational results of FRB suggest that FRB 20200120E bridges the gap between known Galactic young pulsars and magnetars and the more distant extragalactic FRBs, indicating a common magnetically powered emission mechanism across various timescales and luminosities.
Article
Astronomy & Astrophysics
Ketan R. Sand et al.
Summary: This study presents a multiband analysis of the repeating source FRB 20180916B, revealing its burst characteristics and periodicity. The study reports the detection of bursts at different frequencies and provides the first-ever detection of the source in the 800-1000 MHz range. The findings also show the presence of unique structures at lower frequencies and indicate a correlation between the source's activity and frequency variations.
ASTROPHYSICAL JOURNAL
(2022)
Editorial Material
Multidisciplinary Sciences
Yi Feng et al.
Article
Multidisciplinary Sciences
C-H Niu et al.
Summary: The dispersive sweep of fast radio burstsreveals the ionized baryon content of intergalactic medium. The detection and localization of repeating FRB 20190520B with a persistent radio source co-located suggests caution in inferring redshifts for FRBs without accurate host-galaxy identifications.
Article
Multidisciplinary Sciences
H. Xu et al.
Summary: This study reports the continuous observations of FRB 20201124A, revealing the irregular time variation and circular polarization of its radio bursts. These features provide evidence for the immediate environment around the source and its location in a low-stellar-density interarm region at the center of the galaxy. This finding is significant for understanding the origin of cosmological FRBs.
Article
Astronomy & Astrophysics
D. J. Zhou et al.
Summary: We report the properties of more than 600 bursts detected from the repeating FRB source FRB 20201124A. Detailed morphological study reveals different drifting patterns and spectral characteristics of the bursts.
RESEARCH IN ASTRONOMY AND ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Jin-Chen Jiang et al.
Summary: In this study, we report the statistical properties of radio bursts from the repeating FRB source FRB 20201124A. We found that the RM values of the bursts varied within a small range during the observation period, and the bursts exhibited high degrees of polarization with certain variations in polarization angles.
RESEARCH IN ASTRONOMY AND ASTROPHYSICS
(2022)
Article
Multidisciplinary Sciences
F. Y. Wang et al.
Summary: Fast radio bursts (FRBs) are cosmic sources emitting millisecond-duration radio bursts, and their physical nature and central engine are still unclear. Recent observations on FRB 20201124A show a significant variation in rotation measure on a daily timescale. Researchers propose a physical model that explains these observations, suggesting that the repeating signal comes from a binary system containing a magnetar and a Be star.
NATURE COMMUNICATIONS
(2022)
Article
Astronomy & Astrophysics
M. Cruces et al.
Summary: Detections from the repeating fast radio burst FRB 121102 show clustering in time, potentially indicating periodic activity rather than randomness. Extensive multiwavelength observations provided important data on burst behavior, with the potential to reveal the underlying activity patterns of the source.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Editorial Material
Astronomy & Astrophysics
Shami Chatterjee
ASTRONOMY & GEOPHYSICS
(2021)
Article
Astronomy & Astrophysics
Ziggy Pleunis et al.
Summary: This study presents a synthesis of fast radio burst (FRB) morphology detected in the 400-800 MHz frequency range by the CHIME/FRB project, identifying four observed archetypes of burst morphology and discussing the implications of these differences for using FRBs as astrophysical tools. The researchers confirm that bursts from repeating sources have larger widths on average and are narrower in bandwidth, potentially due to beaming or propagation effects.
ASTROPHYSICAL JOURNAL
(2021)
Article
Astronomy & Astrophysics
Maxim Lyutikov
Summary: The article introduces a model for the generation of coherent radio emission in the Crab pulsar, magnetars, and fast radio bursts, which successfully explains several observed features such as the frequency dependence, broadband emission, presence of emission bands, and correlated polarization properties. The model is robust to plasma parameters and reproduces subtle observed features effectively.
ASTROPHYSICAL JOURNAL
(2021)
Article
Astronomy & Astrophysics
Z. Y. Zhao et al.
Summary: FRB 190520B, discovered by the Five-hundred-meter Aperture Spherical radio Telescope (FAST), has the largest extragalactic dispersion measure (DM) and is associated with a compact persistent radio source (PRS). The study suggests that this fast radio burst may be powered by a young magnetar, with specific ranges of magnetic field and age.
ASTROPHYSICAL JOURNAL LETTERS
(2021)
Article
Astronomy & Astrophysics
Kshitij Aggarwal
Summary: Recent observations have shown that repeating fast radio bursts exhibit band-limited emission, leading to incompleteness across the observing band. It is recommended to model burst spectra to estimate the intrinsic fluence and bandwidth robustly, and to use bursts primarily within the observing band for energy distribution analyses.
ASTROPHYSICAL JOURNAL LETTERS
(2021)
Article
Astronomy & Astrophysics
Mandana Amiri et al.
Summary: This study presents a catalog of 536 fast radio bursts detected by the CHIME/FRB Project over a one-year period, providing insights into the FRB population. The research shows consistency in sky locations and dispersion measures between repeaters and apparent nonrepeaters, while also highlighting differences in intrinsic temporal width and spectral bandwidth. Additionally, the study reveals the population properties of FRBs and conducts an absolute calibration of selection effects.
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
(2021)
Article
Astronomy & Astrophysics
G. H. Hilmarsson et al.
Summary: FRB 20201124A, a highly active repeating fast radio burst (FRB) source, shows clear frequency drift and polarization characteristics. The variation in rotation measure (RM), circular polarization, and estimated magnetic field strength are similar to magnetospheric emission from pulsars and other repeating sources.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Multidisciplinary Sciences
D. Li et al.
Summary: The observation of FRB 121102 reveals a bimodal burst rate energy distribution, the absence of detectable periodicity or quasi-periodicity, challenging models involving a single rotating compact object.
Article
Astronomy & Astrophysics
Z. Pleunis et al.
Summary: The study reports detections of 18 bursts from the well-studied FRB 20180916B, providing insights into its nature and offering stronger constraints on the optical depth in the source's local environment. Additionally, it is found that the burst activity is systematically delayed by about 3 days at lower frequencies, which may have implications for the source's activity cycle.
ASTROPHYSICAL JOURNAL LETTERS
(2021)
Article
Astronomy & Astrophysics
M. Bhardwaj et al.
Summary: We report the discovery of FRB 20200120E, a repeating fast radio burst with a low dispersion measure, detected by the Canadian Hydrogen Intensity Mapping Experiment FRB project. The FRB is located near the spiral galaxy M81 at a distance of 3.6 Mpc. Several cataloged M81 sources and a radio point source have been found within the localization region of the FRB.
ASTROPHYSICAL JOURNAL LETTERS
(2021)
Review
Astronomy & Astrophysics
Manisha Caleb et al.
Summary: Fast radio bursts (FRBs) have been a subject of excitement and controversy since their discovery in 2007, with various theories proposed for their origin. Recent observations of FRB-like pulses from Galactic magnetars have led to magnetar engine models emerging as the leading theory in understanding these mysterious phenomena. Overall, FRB pulses offer unique characteristics for probing magnetic field strengths, interstellar media inhomogeneities, and plasma turbulence, making them important tools for studying the Universe.
Article
Astronomy & Astrophysics
K. Nimmo et al.
Summary: High-time-resolution observations of four 1.7 GHz bursts from the repeating fast radio burst source FRB 20180916B reveal highly linearly polarized emissions with subtle changes in polarization position angle on short timescales, indicating an origin in the source magnetosphere.
Article
Astronomy & Astrophysics
Alexandra G. Mannings et al.
Summary: Observations of eight fast radio burst host galaxies with the Hubble Space Telescope show that they are typically located in fainter regions of their host galaxies but overall follow a certain pattern, distinct from other transient populations with known progenitors. Most of the FRBs are not in regions of elevated star formation rates or stellar mass surface densities. Additionally, five out of eight FRB hosts exhibit clear spiral arm features.
ASTROPHYSICAL JOURNAL
(2021)
Article
Astronomy & Astrophysics
Walid A. Majid et al.
Summary: The translation discusses the detection of a bright radio burst from FRB 20200120E using NASA's Deep Space Network, noting its potential association with a globular cluster in the M81 galactic system. The burst exhibits high time resolution, low scattering, and a narrow component structure similar to microstructure in pulsars.
ASTROPHYSICAL JOURNAL LETTERS
(2021)
Article
Astronomy & Astrophysics
E. Platts et al.
Summary: The study revealed a complex time-frequency structure of FRB 121102 bursts, with differences in dispersion measures possibly caused by plasma lensing effects. Other factors like Faraday delay may also contribute to the observed frequency dependence. Exercise caution when considering individual bursts is advised.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Multidisciplinary Sciences
Ines Pastor-Marazuela et al.
Summary: Fast radio burst FRB 20180916B repeats with a periodicity of 16 days and emits down to a frequency of 120 MHz, showing a frequency-dependent activity window. The results suggest that some FRBs are found in 'clean' environments without absorption of low-frequency radiation, indicating possible scenarios of low-frequency FRB emission escaping local medium.
Article
Astronomy & Astrophysics
Mohammed A. Chamma et al.
Summary: By studying the spectro-temporal characteristics of repeating fast radio bursts, we found a universal physical phenomenon that may be responsible for the emission of signals from these bursts, as predicted by a previous model. The behavior observed in all sources suggests a common underlying mechanism and potentially a distinct subclass among repeating FRBs.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
D. C. Price et al.
Summary: Galactic electron density distribution models are crucial for estimating the impact of the ionised interstellar medium on radio pulsars and fast radio bursts. The prevailing models, YMW16 and NE2001, show differences in predicting DM values in different directions. Both models have outliers, suggesting a need for future models to consider the Galactic halo component and focus on discrepancies in pulsar distance measurements for better estimates.
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA
(2021)
Article
Astronomy & Astrophysics
G. H. Hilmarsson et al.
Summary: Monitoring of the RM variations of FRB 121102 shows a decreasing trend, although not linear. Additionally, significant short-term RM fluctuations were observed, potentially explained by the presence of a neutron star in a supernova remnant or near a massive black hole.
ASTROPHYSICAL JOURNAL LETTERS
(2021)
Article
Astronomy & Astrophysics
Z. Y. Zhao et al.
Summary: Magnetars have been identified as a potential energy source for fast radio bursts (FRBs), potentially formed by core-collapse explosions and compact binary mergers. The expansion of merger ejecta can produce time-evolving dispersion measure and rotation measure to probe local environments of FRBs. Research has shown that in the binary neutron star merger scenario, the age of the FRB source is estimated to be around 9-10 years, with an ambient medium density of approximately 2.5-3.1 cm(-3).
ASTROPHYSICAL JOURNAL
(2021)
Article
Astronomy & Astrophysics
P. Kumar et al.
Summary: The study found a repeating fast radio burst (FRB) from a specific source, but did not detect any other emissions in the remaining band. This highlights the unique emission mechanism of the source and the importance of sub-banded search methods in detecting FRBs.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
L. C. Oostrum et al.
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(2020)
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V Morello et al.
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(2020)
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B. Marcote et al.
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K. M. Rajwade et al.
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(2020)
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L. Connor et al.
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(2020)
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Cherie K. Day et al.
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(2020)
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Hao Qiu et al.
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(2020)
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