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The core radius is defined as that where the optical surface brightness is half its central value.
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The 442-ms pulsar J1748-2444 was initially identified as Ter 5 B (B1744-24B) but is now known to be a foreground pulsar unrelated to Terzan 5 (20).
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in preparation
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13644268835
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These comparisons assume a typical pulsar spectral index of -1.6 (32).
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29
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13644252537
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Ter 5 E was a candidate (i.e., unconfirmed) pulsar in (21).
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32
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1950,min is about 8 μJy for P ∼ 2- to 4-ms isolated or long orbital period MSPs.
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13644258572
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The Tempo program is available online at http://pulsar.princeton.edu/ tempo.
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48
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13644260837
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note
-
We thank F. Rasio, S. Sigurdsson, and M. van Kerkwijk for extremely useful discussions and J. Herrnstein, L. Greenhill, D. Manchester, A. Lyne, and N. D'Amico for providing or aiding with the Parkes data from 1998 and 2000. J.W.T.H. is a Natural Sciences and Engineering Research Council of Canada (NSERC) Post-Graduate Scholarship-Doctoral fellow. I.H.5. holds an NSERC University Faculty Award and is supported by a Discovery grant and University of British Columbia start-up funds. F.C. thanks support from NSF. V.M.K. holds a Canada Research Chair and is supported by an NSERC Discovery Grant and Steacie Fellowship Supplement, by the Fonds Québécois de la recherche sur la nature et les technologies and Canadian Institute for Advanced Research, and by a New Opportunities Grant from the Canada Foundation for Innovation. D.L.K. is a Pappalardo Fellow.
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