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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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Citations
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Journal ArticleDOI

Emission from a Pulsar Wind Nebula: Application to the Persistent Radio Counterpart of FRB 121102

TL;DR: In this paper, a pulsar wind nebula powered by a magnetar without surrounding supernova ejecta was proposed as a radio counterpart of fast radio bursts (FRBs) and the model parameters were constrained by the spectrum of the counterpart emission, the size of the nebula, and the large but decreasing rotation measure (RM) of the repeating bursts.
Dissertation

A Dedicated Search for Low Frequency Radio Transient Astrophysical Events using ETA

K. Deshpande
TL;DR: In this article, the results of a search campaign using ETA, namely, a Crab giant pulse (CGP) search, were described and a software toolchain was developed for the analysis of data that includes calibration, radio frequency interference (RFI) mitigation, and incoherent dedispersion.
Journal ArticleDOI

Limits on Absorption from a 332-MHz survey for Fast Radio Bursts

TL;DR: In this article, the authors present results from a fast radio burst (FRB) survey conducted at the Jodrell Bank Observatory at 332 MHz with the 76m Lovell telescope for a total of 58 days.
Journal ArticleDOI

Cosmic Anisotropy and Fast Radio Bursts

TL;DR: In this paper, the authors tried to test the possible cosmic anisotropy with simulated FRBs and found that at least 2800, 190, 100 FRBs are competent to find the cosmic dipole with amplitude 0.01, 0.03, and 0.05, respectively.
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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