HTRU-North pulsar survey. III Virtual Observatory Resource

Authors
  1. Houben L.J.M.
  2. Falcke H.
  3. Spitler L.G.
  4. Barr E.D.
  5. Berezina M.,Champion D.J.
  6. Karuppusamy R.
  7. Kramer M.
  8. Published by
    CDS
Abstract

We continued the search for single pulses (SPs) in the northern part of the all-sky High Time Resolution Universe survey, whose aim is to detect pulsars and other radio transients. This search is now about 21% complete and yielded the first discovery of a fast radio burst (FRB) with the 100m Effelsberg Radio Telescope. FRB 20110220A is detected with an S/N optimised dispersion measure of 501.0pc/cm^3^ and width of 11.9+/-3.5ms giving it a fluence of 0.6+/-0.1Jy.ms. We obtained the first the first L-band detection of the rotating radio transient (RRAT) J2028+28, from which upper limits on the source's period and burst rate are obtained, as well as an improved position. The discovery of a new RRAT, J0404+53, is reported previously identified as an isolated SP candidate by Houben et al. (2026A&A.707A..10H, Cat. J/A+A/707/A10). Eight new SP trains and 272 faint isolated SP candidates were detected. The latter could be used to show the presence of a Galactic latitude and longitude dependence on the all-sky detection rates of the isolated SP candidates. This direction dependence suggests the existence of a faint Galactic SP population.

Keywords
  1. radio-sources
  2. pulsars
Bibliographic source Bibcode
2026A&A...708A.199H
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/708/A199
IVOA Identifier IVOID
ivo://CDS.VizieR/J/A+A/708/A199

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History

2026-04-09T17:19:37Z
Resource record created
2026-04-09T17:19:37Z
Created
2026-05-04T07:43:19Z
Updated

Contact

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CDS support team
Postal Address
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