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 ∼1 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.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 826-830 |
| Number of pages | 5 |
| Journal | Astrophysical Journal |
| Volume | 454 |
| Issue number | 2 |
| DOIs | |
| State | Published - Dec 1 1995 |
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All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science
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A high galactic latitude pulsar survey of the Arecibo sky. / Foster, R. S.; Cadwell, B. J.; Wolszczan, Alexander; Anderson, S. B.
In: Astrophysical Journal, Vol. 454, No. 2, 01.12.1995, p. 826-830.Research output: Contribution to journal › Article
TY - JOUR
T1 - A high galactic latitude pulsar survey of the Arecibo sky
AU - Foster, R. S.
AU - Cadwell, B. J.
AU - Wolszczan, Alexander
AU - Anderson, S. B.
PY - 1995/12/1
Y1 - 1995/12/1
N2 - 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 ∼1 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.
AB - 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 ∼1 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.
UR - http://www.scopus.com/inward/record.url?scp=11944267607&partnerID=8YFLogxK
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U2 - 10.1086/176535
DO - 10.1086/176535
M3 - Article
VL - 454
SP - 826
EP - 830
JO - Astrophysical Journal
JF - Astrophysical Journal
SN - 0004-637X
IS - 2
ER -