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Open AccessJournal ArticleDOI

A Bright Millisecond Radio Burst of Extragalactic Origin

Duncan R. Lorimer, +4 more
- 02 Nov 2007 - 
- Vol. 318, Iss: 5851, pp 777-780
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TLDR
A 30-jansky dispersed burst, less than 5 milliseconds in duration, located 3° from the Small Magellanic Cloud is found, which implies that it was a singular event such as a supernova or coalescence of relativistic objects.
Abstract
Pulsar surveys offer a rare opportunity to monitor the radio sky for impulsive burst-like events with millisecond durations. We analyzed archival survey data and found a 30-jansky dispersed burst, less than 5 milliseconds in duration, located 3 degrees from the Small Magellanic Cloud. The burst properties argue against a physical association with our Galaxy or the Small Magellanic Cloud. Current models for the free electron content in the universe imply that the burst is less than 1 gigaparsec distant. No further bursts were seen in 90 hours of additional observations, which implies that it was a singular event such as a supernova or coalescence of relativistic objects. Hundreds of similar events could occur every day and, if detected, could serve as cosmological probes.

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Journal ArticleDOI

Future Cosmological Constraints From Fast Radio Bursts

TL;DR: In this paper, the authors consider the possible observation of fast radio bursts (FRBs) with planned future radio telescopes, and investigate how well the dispersions and redshifts of these signals might constrain cosmological parameters.
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Periodicity in recurrent fast radio bursts and the origin of ultralong period magnetars

TL;DR: In this paper, the authors make a connection to the 6.7 hour period of the Galactic magnetar candidate, 1E 161348--5055, and explore three physical mechanisms that could lead to the creation of ultra long period magnetars: (i) enhanced spin-down due to episodic mass-loaded charged particle winds (e.g. as may accompany giant flares), (ii) angular momentum kicks from giant flares and (iii) fallback leading to long lasting accretion disks).
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On the FRB luminosity function - - II. Event rate density

TL;DR: In this article, the authors measured the FRB luminosity function using 46 known FRBs and found that the expected FRB event rate density at the upper cut-off luminosity is 2.9.
References
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Book

Handbook of Pulsar Astronomy

TL;DR: In this paper, theoretical background for pulsar observations is described. But pulsars as physical tools are not used as a physical tool for the measurement of pulsar properties.
Journal ArticleDOI

Hyperleda. I. Identification and designation of galaxies

TL;DR: In this paper, the authors presented a new catalog of principal galaxies (PGC2003), which constitutes the framework of the HYPERLEDA database that supersedes the LEDA one, with more data and more capabilities.
Journal ArticleDOI

The Parkes multi-beam pulsar survey - I. Observing and data analysis systems, discovery and timing of 100 pulsars

TL;DR: The survey is proving to be extremely successful, with more than 600 pulsars discovered so far as discussed by the authors, and the number of newly discovered pulsars tend to be young, distant and of high radio luminosity, which is a valuable sample for studies of pulsar emission properties, the Galactic distribution and evolution of pulsars, and as probes of interstellar medium properties.
Journal ArticleDOI

Transient radio bursts from rotating neutron stars

TL;DR: A search for radio sources that vary on much shorter timescales, finding eleven objects characterized by single, dispersed bursts having durations between 2 and 30 ms, suggesting origins in rotating neutron stars.
Journal ArticleDOI

The large‐scale HI structure of the Small Magellanic Cloud

TL;DR: In this paper, Parkes telescope observations of neutral hydrogen (Hi) in the Small Magellanic Cloud (SMC) were combined with an Australia Telescope Compact Array (ATCA) aperture synthesis mosaic to obtain a set of images sensitive to all angular (spatial) scales between 98 arcsec (30 pc) and 4° (4 kpc).
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