The Arecibo 430-MHz Intermediate Galactic Latitude Survey: Discovery of Nine Radio Pulsars

dc.creatorNavarro, Jose
dc.creatorAnderson, Stuart
dc.creatorFreire, Paulo C.
dc.date2003-06-21
dc.date.accessioned2026-07-07T11:29:09Z
dc.date.available2026-07-07T11:29:09Z
dc.descriptionWe have used the Arecibo Radio Telescope to search for millisecond pulsars in two intermediate Galactic latitude regions (7 deg < | b | < 20 deg) accessible to this telescope. For these latitudes the useful millisecond pulsar search volume achieved by Arecibo's 430-MHz beam is predicted to be maximal. Searching a total of 130 square degrees, we have discovered nine new pulsars and detected four previously known objects. We compare the results of this survey with those of other 430-MHz surveys carried out at Arecibo and of an intermediate latitude survey made at Parkes that included part of our search area; the latter independently found two of the nine pulsars we have discovered. At least six of our discoveries are isolated pulsars with ages between 5 and 300 Myr; one of these, PSR J1819+1305, exhibits very marked and periodic nulling. We have also found a recycled pulsar, PSR J2016+1948. With a rotational period of 65 ms, this is a member of a binary system with a 635-day orbital period. We discuss some of the the properties of this system in detail, and indicate its potential to provide a test of the Strong Equivalence Principle. This pulsar and PSR J0407+16, a similar system now being timed at Arecibo, are by far the best systems known for such a test.
dc.descriptionAccepted for publication in ApJ Referee format: 22 pages, 7 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0306432
dc.identifierhttp://arxiv.org/abs/astro-ph/0306432
dc.identifierAstrophys.J.594:943-951,2003
dc.identifierdoi:10.1086/377153
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/196622
dc.subjectAstrophysics
dc.titleThe Arecibo 430-MHz Intermediate Galactic Latitude Survey: Discovery of Nine Radio Pulsars
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