scispace - formally typeset
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
Reads0
Chats0
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.

read more

Citations
More filters
Journal ArticleDOI

Detection of Radio Emission from Fireballs

TL;DR: In this article, the Prototype All-Sky Imager (PASI) was used as a backend correlator of the first station of the Long Wavelength Array (LWA1), which has recorded over 11,000 hours of all-sky images at frequencies between 25 and 75 MHz.
Journal ArticleDOI

A search for highly dispersed fast radio bursts in three Parkes multibeam surveys

TL;DR: In this paper, the Parkes multibeam 14 GHz surveys for the presence of fast radio bursts (FRBs) out to a dispersion measure (DM) of 5000 pc cm$^{-3}$ were searched.
Journal ArticleDOI

Classifying RRATs and FRBs

TL;DR: In this article, the authors consider the fact that the simple criterion used to label fast radio transient events as either fast radio bursts (FRBs) or rotating radio transients (RRATs, thought to be Galactic neutron stars) is uncertain.
Journal ArticleDOI

Radio-interferometric monitoring of FRB 131104: A coincident AGN flare, but no evidence for a cosmic fireball

TL;DR: In this paper, the authors report on radio-continuum imaging observations of the original localization region of the fast radio burst (FRB) beginning three days after the event and comprising 25 epochs over 2.5 yr.
References
More filters
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).
Related Papers (5)