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Slow pulsars from the STScI/NAIC drift scan search

Published online by Cambridge University Press:  12 April 2016

K. M. Xilouris ,
A. Fruchter ,
D.R. Lorimer ,
J. Eder  and
A. Vazquez
K. M. Xilouris
Affiliation:
Center Development Lab, NRAO, Charlottesville, VA 22903, USA
A. Fruchter
Affiliation:
Space Telescope Science Institute, Baltimore, MD 21218, USA
D.R. Lorimer
Affiliation:
Arecibo Observatory, HC3 Box 53995, Arecibo, PR 00612, USA
J. Eder
Affiliation:
Arecibo Observatory, HC3 Box 53995, Arecibo, PR 00612, USA
A. Vazquez
Affiliation:
Arecibo Observatory, HC3 Box 53995, Arecibo, PR 00612, USA

Abstract

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The unique sensitivity of the Arecibo telescope at 430 MHz motivated a drift scan search of the visible sky divided up into eight declination strips. Based on an analysis of the data collected in the region assigned to us, eight new long-period pulsars have so far been discovered.

Type
Part 1. Searching for Pulsars
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 21 - 22
Copyright
Copyright © Astronomical Society of the Pacific 2000