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New Pulsars from Arecibo Drift Scan SearchesWe report new pulsars discovered in drift-scan data taken by two collaborations (Berkeley/Cornell and STScI/NAIC) during the latter stages of the Arecibo upgrade period. The data were taken with the Penn State Pulsar Machine and are being processed on the COBRA cluster at Jodrell Bank. Processing is roughly 70% complete and has resulted in the detection of 10 new and 31 known pulsars, in addition to a number of pulsar candidates. The 10 new pulsars include one pulsar with a spin-period of 55 ms and another with a spin period of 5.8 ms. At the completion of the processing, we expect to have discovered roughly 20 new pulsars. All new pulsars are being subjected to a program of followup observations at Arecibo to determine spin and astrometric parameters.
Document ID
20030025737
Acquisition Source
Goddard Space Flight Center
Document Type
Preprint (Draft being sent to journal)
Authors
McLaughlin, M. A.
(Manchester Univ. United Kingdom)
Lorimer, D. R.
(Manchester Univ. United Kingdom)
Arzoumanian, Z.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Backer, D. C.
(California Univ. Berkeley, CA, United States)
Cordes, J. M.
(Cornell Univ. Ithaca, NY, United States)
Fruchter, A.
(Space Telescope Science Inst. Baltimore, MD, United States)
Lommen, A. N.
(Amsterdam Univ. Netherlands)
Xilouris, K.
(Virginia Univ. Charlottesville, VA, United States)
Date Acquired
August 21, 2013
Publication Date
January 1, 2003
Subject Category
Astronomy
Distribution Limits
Public
Copyright
Public Use Permitted.
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