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Five New Millisecond Pulsars From a Radio Survey of 14 Unidentified Fermi-LAT Gamma-ray Sources

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arxiv 1201.5160 v1 pith:53C4U6AZ submitted 2012-01-25 astro-ph.HE astro-ph.GAastro-ph.SR

classification astro-ph.HEastro-ph.GAastro-ph.SR
keywords gammamspsradiosourcesfermi-latfivej0101-6422millisecond
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We have discovered five millisecond pulsars (MSPs) in a survey of 14 unidentified Fermi-LAT sources in the southern sky using the Parkes radio telescope. PSRs J0101-6422, J1514-4946, and J1902-5105 reside in binaries, while PSRs J1658-5324 and J1747-4036 are isolated. Using an ephemeris derived from timing observations of PSR J0101-6422 (P =2.57 ms, DM=12 pc cm-3), we have detected {\gamma}-ray pulsations and measured its proper motion. Its {\gamma}-ray spectrum (a power law of {\Gamma} = 0.9 with a cutoff at 1.6 GeV) and efficiency are typical of other MSPs, but its radio and {\gamma}-ray light curves challenge simple geometric models of emission. The high success rate of this survey-enabled by selecting {\gamma}-ray sources based on their detailed spectral characteristics-and other similarly successful searches indicate that a substantial fraction of the local population of MSPs may soon be known.

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  1. Fingerprints of Individual Supermassive Black Hole Binaries in Pulsar Timing Arrays

    astro-ph.HE 2026-03 conditional novelty 6.0 of 10

    A single supermassive black hole binary imprints a deterministic, direction-dependent correlation fingerprint on pulsar timing arrays, enabling identification via cross-correlations.

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