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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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TL;DR: In this paper, the relationship between the dispersion measures (DMs) and redshifts of fast radio bursts (FRBs) is investigated, accounting for uncertainties due to their extragalactic DM components, redshift dependences, and progenitor scenarios.
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Constraining the mass of the photon with gamma-ray bursts

TL;DR: In this article, the upper limits of the photon mass with cosmological gamma-ray bursts (GRBs) early time radio afterglow observations as well as multi-band radio peaks were derived.
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The Northern Cross fast radio burst project - I. Overview and pilot observations at 408 MHz

TL;DR: In this article, the authors describe the upgrade of the Northern Cross radio telescope, operating in the 400-416~MHz frequency band, with the ultimate goal of turning the array into a dedicated instrument to survey the sky for fast radio bursts.
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The High Time and Frequency Resolution Capabilities of the Murchison Widefield Array

TL;DR: In this article, the authors describe the system that records the 100 micro-second and 10 kHz resolution voltage data from the Murchison Widefield Array (MWA) and demonstrate that this capability is critical for science applications.
References
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Book

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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

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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

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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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