A High Galactic Latitude Pulsar Survey of the Arecibo Sky
1995; IOP Publishing; Volume: 454; Linguagem: Inglês
10.1086/176535
ISSN1538-4357
AutoresRoger S. Foster, B. J. Cadwell, A. Wolszczan, S. B. Anderson,
Tópico(s)Geophysics and Gravity Measurements
Resumoview Abstract Citations (59) References (27) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS A High Galactic Latitude Pulsar Survey of the Arecibo Sky Foster, R. S. ; Cadwell, B. J. ; Wolszczan, A. ; Anderson, S. B. Abstract The results of a 1355 square degree survey of high Galactic latitudes conducted from 1990 to 1995 with the Arecibo radio telescope are presented. The majority of the survey was performed at 430 MHz with a 32 channel × 250 kHz filter bank sampled at 4 kHz. A 7 σ sensitivity of ∼31 mJy was obtained for pulsars with periods down to ∼3 ms. This survey yielded five millisecond or recycled pulsars and 14 slow period pulsars. In addition, one millisecond pulsar and four slow period pulsar candidates have been identified but are as yet unconfirmed. One of the new slow period pulsars appears to be associated with the supernova remnant S147 located toward the Galactic anticenter. Publication: The Astrophysical Journal Pub Date: December 1995 DOI: 10.1086/176535 Bibcode: 1995ApJ...454..826F Keywords: STARS: PULSARS: GENERAL; ISM: INDIVIDUAL ALPHANUMERIC: S147; SURVEYS full text sources ADS | data products SIMBAD (26)
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