<mets:mets LABEL="Eprints Item" xsi:schemaLocation="http://www.loc.gov/METS/ http://www.loc.gov/standards/mets/mets.xsd http://www.loc.gov/mods/v3 http://www.loc.gov/standards/mods/v3/mods-3-0.xsd" xmlns:xlink="http://www.w3.org/1999/xlink" OBJID="oai:utas.edu.au:4047" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:mods="http://www.loc.gov/mods/v3" xmlns:mets="http://www.loc.gov/METS/"><mets:metsHdr CREATEDATA="2009-01-08T04:58:04Z"><mets:agent TYPE="ORGANIZATION" ROLE="CUSTODIAN"><mets:name>UTas ePrints</mets:name></mets:agent></mets:metsHdr><mets:dmdSec ID="DMD_oai:utas.edu.au:4047_mods"><mets:mdWrap MDTYPE="mods"><mets:xmlData><mods:titleInfo><mods:title>Discovery of Five Recycled Pulsars in a High Galactic Latitude Survey</mods:title></mods:titleInfo><mods:name type="personal"><mods:namePart type="given">BA</mods:namePart><mods:namePart type="family">Jacoby</mods:namePart><mods:role><mods:roleTerm type="text">author</mods:roleTerm></mods:role></mods:name><mods:name type="personal"><mods:namePart type="given">M</mods:namePart><mods:namePart type="family">Bailes</mods:namePart><mods:role><mods:roleTerm type="text">author</mods:roleTerm></mods:role></mods:name><mods:name type="personal"><mods:namePart type="given">SM</mods:namePart><mods:namePart type="family">Ord</mods:namePart><mods:role><mods:roleTerm type="text">author</mods:roleTerm></mods:role></mods:name><mods:name type="personal"><mods:namePart type="given">HS</mods:namePart><mods:namePart type="family">Knight</mods:namePart><mods:role><mods:roleTerm type="text">author</mods:roleTerm></mods:role></mods:name><mods:name type="personal"><mods:namePart type="given">AW</mods:namePart><mods:namePart type="family">Hotan</mods:namePart><mods:role><mods:roleTerm type="text">author</mods:roleTerm></mods:role></mods:name><mods:abstract>We present five recycled pulsars discovered during a 21 cm survey of approximately 4150 deg2 between 15 and&#13;
30 from the Galactic plane using the Parkes radio telescope. One new pulsar, PSR J15283146, has a 61 ms spin&#13;
period and a massive white dwarf companion. Like many recycled pulsars with heavy companions, the orbital&#13;
eccentricity is relatively high (0.0002), consistent with evolutionary models that predict less time for circularization.&#13;
The four remaining pulsars have short spin periods (3 ms &lt; P &lt; 6 ms); three of these have probable white&#13;
dwarf binary companions and one (PSR J20101323) is isolated. PSR J16003053 is relatively bright for its&#13;
dispersion measure of 52.3 pc cm3 and promises good timing precision thanks to an intrinsically narrow feature in its&#13;
pulse profile, resolvable through coherent dedispersion. In this survey, the recycled pulsar discovery rate was 1 per 4 days&#13;
of telescope time or 1 per 600 deg2 of sky. The variability of these sources implies that there are more millisecond&#13;
pulsars that might be found by repeating this survey.</mods:abstract><mods:classification authority="lcc">240101 Astronomy and Astrophysics</mods:classification><mods:originInfo><mods:dateIssued encoding="iso8061">2007</mods:dateIssued></mods:originInfo><mods:originInfo><mods:publisher>University of Chicago Press</mods:publisher></mods:originInfo><mods:genre>Article</mods:genre></mets:xmlData></mets:mdWrap></mets:dmdSec><mets:amdSec ID="TMD_oai:utas.edu.au:4047"><mets:rightsMD ID="rights_oai:utas.edu.au:4047_mods"><mets:mdWrap MDTYPE="mods"><mets:xmlData><mods:useAndReproduction>
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