Pith. sign in

REVIEW

New Pulsars from Arecibo Drift-Scan Searches

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv astro-ph/0211261 v1 pith:ALW3FXJV submitted 2002-11-12 astro-ph

M. A. McLaughlin , D. R. Lorimer , Z. Arzoumanian , D. C. Backer , J. M. Cordes , A. Fruchter , A. N. Lommen K. Xilouris This is my paper
classification astro-ph
keywords pulsarsarecibopulsardatadiscovereddrift-scanperiodprocessing
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

We 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.

Discussion (0). Sign in to comment.

Pith tools