作者: M. A. McLaughlin , D. R. Lorimer , D. J. Champion , K. Xilouris , Z. Arzoumanian
DOI: 10.1017/S0074180900180763
关键词:
摘要: We report new pulsars discovered in drift-scan data taken by two collaborations (Berkeley/Cornell and STScI/NAIC) during the latter stages of Arecibo upgrade period. The were with Penn State Pulsar Machine are being processed on COBRA cluster at Jodrell Bank. Processing is roughly 70% complete has resulted detection 10 31 known pulsars, addition to a number pulsar candidates. include one spin-period 55 ms another spin period 5.8 ms. At completion processing, we expect have 20 pulsars. All subjected program followup observations determine astrometric parameters.