The host galaxies and progenitors of Fast Radio Bursts localized with the Australian Square Kilometre Array Pathfinder.

@article{Bhandari2020TheHG,
  title={The host galaxies and progenitors of Fast Radio Bursts localized with the Australian Square Kilometre Array Pathfinder.},
  author={Shivani Bhandari and Elaine M Sadler and J. Xavier Prochaska and Sunil Simha and Stuart D. Ryder and Lachlan Marnoch and Keith W. Bannister and Jean-Pierre Macquart and Chris Flynn and Ryan M. Shannon and Nicolas Tejos and Felipe Corro-Guerra and Cherie K.Day and Adam T.Deller and R D Ekers and Sebasti{\'a}n L{\'o}pez and Elizabeth K. Mahony and Consuelo Nunez and Chris Phillips},
  journal={arXiv: Astrophysics of Galaxies},
  year={2020}
}
The Australian SKA Pathfinder (ASKAP) telescope has started to localize Fast Radio Bursts (FRBs) to arcsecond accuracy from the detection of a single pulse, allowing their host galaxies to be reliably identified. We discuss the global properties of the host galaxies of the first four FRBs localized by ASKAP, which lie in the redshift range $0.11<z<0.48$. All four are massive galaxies (log( $M_{*}/ M_{\odot}$) $\sim 9.4 -10.4$) with modest star-formation rates of up to $2M_{\odot}$yr$^{-1… Expand

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References

SHOWING 1-10 OF 84 REFERENCES
A fast radio burst in the direction of the Virgo cluster
The rate of fast radio bursts (FRBs) in the direction of nearby galaxy clusters is expected to be higher than the mean cosmological rate if intrinsically faint FRBs are numerous. In this paper, weExpand
A fast radio burst localized to a massive galaxy
TLDR
Use of a specially built radio interferometer shows that a non-repeating fast radio burst is localized to a few-arcsecond region containing a single massive galaxy, and is perhaps derived from an old stellar population. Expand
The Host Galaxy and Redshift of the Repeating Fast Radio Burst FRB 121102
The precise localization of the repeating fast radio burst (FRB 121102) has provided the first unambiguous association (chance coincidence probability p ≲ 3 × 10‑4) of an FRB with an optical andExpand
HOST-GALAXY PROPERTIES of 32 LOW-REDSHIFT SUPERLUMINOUS SUPERNOVAE from the PALOMAR TRANSIENT FACTORY
We present ultraviolet through near-infrared photometry and spectroscopy of the host galaxies of all superluminous supernovae (SLSNe) discovered by the Palomar Transient Factory prior to 2013 andExpand
Fast Radio Bursts: An Extragalactic Enigma.
We summarize our understanding of millisecond radio bursts from an extragalactic population of sources. FRBs occur at an extraordinary rate, thousands per day over the entire sky with radiationExpand
A repeating fast radio burst source localized to a nearby spiral galaxy
TLDR
Only one repeating fast radio burst has been localized, to an irregular dwarf galaxy; now another is found to come from a star-forming region of a nearby spiral galaxy, suggesting that repeating FRBs may have a wide range of luminosities, and originate from diverse host galaxies and local environments. Expand
A survey of the Galactic plane for dispersed radio pulses with the Australian Square Kilometre Array Pathfinder
We report the results from a survey of the Galactic plane for dispersed single pulses using the Australian SKA Pathfinder (ASKAP). We searched for rare bright dispersed radio pulses comprising 160Expand
Host galaxies of merging compact objects: mass, star formation rate, metallicity, and colours
Characterizing the properties of the host galaxies of merging compact objects provides essential clues to interpret current and future gravitational-wave detections. Here, we investigate the stellarExpand
The low density and magnetization of a massive galaxy halo exposed by a fast radio burst
TLDR
The detection of a fast radio burst (FRB 181112), localized with arcsecond precision, that passes through the halo of a foreground galaxy implies predominantly diffuse gas in massive galactic halos, even those hosting active supermassive black holes, contrary to some previous results. Expand
A direct localization of a fast radio burst and its host
TLDR
The authors' observations are inconsistent with the fast radio burst having a Galactic origin or its source being located within a prominent star-forming galaxy, and the source appears to be co-located with a low-luminosity active galactic nucleus or a previously unknown type of extragalactic source. Expand
...
1
2
3
4
5
...