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Discovery of millisecond pulsars in radio searches of southern Fermi Large Area Telescope sources

Identifieur interne : 007038 ( Main/Merge ); précédent : 007037; suivant : 007039

Discovery of millisecond pulsars in radio searches of southern Fermi Large Area Telescope sources

Auteurs : M. J. Keith [Australie] ; S. Johnston [Australie] ; P. S. Ray [États-Unis] ; E. C. Ferrara [États-Unis] ; P. M. Saz Parkinson [États-Unis] ; Ö. Celik [États-Unis] ; A. Belfiore [États-Unis, Italie] ; D. Donato [États-Unis] ; C. C. Cheung [États-Unis] ; A. A. Abdo [États-Unis] ; F. Camilo [États-Unis] ; P. C. C. Freire [Allemagne] ; L. Guillemot [Allemagne] ; A. K. Harding [États-Unis] ; M. Kramer [Allemagne, Royaume-Uni] ; P. F. Michelson [États-Unis] ; S. M. Ransom [États-Unis] ; R. W. Romani [États-Unis] ; D. A. Smith [France] ; D. J. Thompson [États-Unis] ; P. Weltevrede [Royaume-Uni] ; K. S. Wood [États-Unis]

Source :

RBID : Pascal:11-0287659

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English descriptors

Abstract

Using the Parkes Radio Telescope, we have carried out deep observations of 11 unassociated gamma-ray sources. Periodicity searches of these data have discovered two millisecond pulsars, PSRJ1103-5403 (1FGLJ1103.9-5355) and PSRJ2241-5236 (1FGLJ2241.9-5236), and a long-period pulsar, PSRJ1604-44 (1FGLJ1604.7-4443). In addition, we searched for but did not detect any radio pulsations from six gamma-ray pulsars discovered by the Fermi satellite to a level of ˜0.04 mJy (for pulsars with a 10 per cent duty cycle). The timing of the millisecond pulsar PSRJ1103-5403 has shown that its position is 9 arcmin from the centroid of the gamma-ray source. Since these observations were carried out, independent evidence has shown that 1FGL J1103.9-5355 is associated with the flat spectrum radio source PKS 1101-536. It appears certain that the pulsar is not associated with the gamma-ray source, despite the seemingly low probability of a chance detection of a radio millisecond pulsar. We consider that PSRJ1604-44 is a chance discovery of a weak, long-period pulsar and is unlikely to be associated with 1FGL J1604.7-4443. PSR J2241-5236 has a spin period of 2.2 ms and orbits a very low mass companion with a 3.5-h orbital period. The relatively high flux density and low dispersion measure of PSR J2241-5236 make it an excellent candidate for high precision timing experiments. The gamma rays of 1FGL J2241.9-5236 have a spectrum that is well modelled by a power law with an exponential cut-off, and phase binning with the radio ephemeris results in a multipeaked gamma-ray pulse profile. Observations with Chandra have identified a coincident X-ray source within 0.1 arcsec of the position of the pulsar obtained by radio timing.

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Pascal:11-0287659

Le document en format XML

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<title xml:lang="en" level="a">Discovery of millisecond pulsars in radio searches of southern Fermi Large Area Telescope sources</title>
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<author>
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<s1>Department of Physics and Center for Space Sciences and Technology, University of Maryland Baltimore County</s1>
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<sZ>6 aut.</sZ>
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<s1>Departments of Physics and Gastronomy, University of Maryland</s1>
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<s1>Columbia Astrophysics Laboratory Columbia University</s1>
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<s3>USA</s3>
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</inist:fA14>
<country>États-Unis</country>
<wicri:noRegion>Columbia Astrophysics Laboratory Columbia University</wicri:noRegion>
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<name sortKey="Freire, P C C" sort="Freire, P C C" uniqKey="Freire P" first="P. C. C." last="Freire">P. C. C. Freire</name>
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<s1>Max-Planck-Institut für Radioastronomie, Auf dem Hiigel 69</s1>
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<country>Allemagne</country>
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<region type="land" nuts="1">Rhénanie-du-Nord-Westphalie</region>
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<name sortKey="Guillemot, L" sort="Guillemot, L" uniqKey="Guillemot L" first="L." last="Guillemot">L. Guillemot</name>
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<inist:fA14 i1="12">
<s1>Max-Planck-Institut für Radioastronomie, Auf dem Hiigel 69</s1>
<s2>53121 Bonn</s2>
<s3>DEU</s3>
<sZ>12 aut.</sZ>
<sZ>13 aut.</sZ>
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<country>Allemagne</country>
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<region type="land" nuts="1">Rhénanie-du-Nord-Westphalie</region>
<region type="district" nuts="2">District de Cologne</region>
<settlement type="city">Bonn</settlement>
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<name sortKey="Harding, A K" sort="Harding, A K" uniqKey="Harding A" first="A. K." last="Harding">A. K. Harding</name>
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<s1>NASA Goddard Space Flight Center</s1>
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<sZ>4 aut.</sZ>
<sZ>6 aut.</sZ>
<sZ>14 aut.</sZ>
<sZ>20 aut.</sZ>
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<country>États-Unis</country>
<wicri:noRegion>NASA Goddard Space Flight Center</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Kramer, M" sort="Kramer, M" uniqKey="Kramer M" first="M." last="Kramer">M. Kramer</name>
<affiliation wicri:level="3">
<inist:fA14 i1="12">
<s1>Max-Planck-Institut für Radioastronomie, Auf dem Hiigel 69</s1>
<s2>53121 Bonn</s2>
<s3>DEU</s3>
<sZ>12 aut.</sZ>
<sZ>13 aut.</sZ>
<sZ>15 aut.</sZ>
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<country>Allemagne</country>
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<region type="land" nuts="1">Rhénanie-du-Nord-Westphalie</region>
<region type="district" nuts="2">District de Cologne</region>
<settlement type="city">Bonn</settlement>
</placeName>
</affiliation>
<affiliation wicri:level="4">
<inist:fA14 i1="13">
<s1>Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester</s1>
<s2>Manchester M13 9PL</s2>
<s3>GBR</s3>
<sZ>15 aut.</sZ>
<sZ>21 aut.</sZ>
</inist:fA14>
<country>Royaume-Uni</country>
<placeName>
<settlement type="city">Manchester</settlement>
<region type="nation">Angleterre</region>
<region nuts="2" type="region">Grand Manchester</region>
</placeName>
<orgName type="university">Université de Manchester</orgName>
</affiliation>
</author>
<author>
<name sortKey="Michelson, P F" sort="Michelson, P F" uniqKey="Michelson P" first="P. F." last="Michelson">P. F. Michelson</name>
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<inist:fA14 i1="14">
<s1>W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University</s1>
<s2>Stanford, CA 94305</s2>
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<sZ>16 aut.</sZ>
<sZ>18 aut.</sZ>
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<wicri:noRegion>Stanford, CA 94305</wicri:noRegion>
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<author>
<name sortKey="Ransom, S M" sort="Ransom, S M" uniqKey="Ransom S" first="S. M." last="Ransom">S. M. Ransom</name>
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<inist:fA14 i1="15">
<s1>National Radio Astronomy Observatory (NRAO)</s1>
<s2>Charlottesville, VA 22903</s2>
<s3>USA</s3>
<sZ>17 aut.</sZ>
</inist:fA14>
<country>États-Unis</country>
<wicri:noRegion>National Radio Astronomy Observatory (NRAO)</wicri:noRegion>
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<author>
<name sortKey="Romani, R W" sort="Romani, R W" uniqKey="Romani R" first="R. W." last="Romani">R. W. Romani</name>
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<inist:fA14 i1="14">
<s1>W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University</s1>
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<s3>USA</s3>
<sZ>16 aut.</sZ>
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<name sortKey="Smith, D A" sort="Smith, D A" uniqKey="Smith D" first="D. A." last="Smith">D. A. Smith</name>
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<inist:fA14 i1="16">
<s1>Centre, d'Études Nucléaires de Bordeaux Gradignan, Université Bordeaux 1, CNRS/IN2p3</s1>
<s2>33175 Gradignan</s2>
<s3>FRA</s3>
<sZ>19 aut.</sZ>
</inist:fA14>
<country>France</country>
<wicri:noRegion>33175 Gradignan</wicri:noRegion>
<wicri:noRegion>CNRS/IN2p3</wicri:noRegion>
<wicri:noRegion>33175 Gradignan</wicri:noRegion>
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</author>
<author>
<name sortKey="Thompson, D J" sort="Thompson, D J" uniqKey="Thompson D" first="D. J." last="Thompson">D. J. Thompson</name>
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<inist:fA14 i1="03">
<s1>NASA Goddard Space Flight Center</s1>
<s2>Greenbelt, MD 20771</s2>
<s3>USA</s3>
<sZ>4 aut.</sZ>
<sZ>6 aut.</sZ>
<sZ>14 aut.</sZ>
<sZ>20 aut.</sZ>
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<country>États-Unis</country>
<wicri:noRegion>NASA Goddard Space Flight Center</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Weltevrede, P" sort="Weltevrede, P" uniqKey="Weltevrede P" first="P." last="Weltevrede">P. Weltevrede</name>
<affiliation wicri:level="4">
<inist:fA14 i1="13">
<s1>Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester</s1>
<s2>Manchester M13 9PL</s2>
<s3>GBR</s3>
<sZ>15 aut.</sZ>
<sZ>21 aut.</sZ>
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<country>Royaume-Uni</country>
<placeName>
<settlement type="city">Manchester</settlement>
<region type="nation">Angleterre</region>
<region nuts="2" type="region">Grand Manchester</region>
</placeName>
<orgName type="university">Université de Manchester</orgName>
</affiliation>
</author>
<author>
<name sortKey="Wood, K S" sort="Wood, K S" uniqKey="Wood K" first="K. S." last="Wood">K. S. Wood</name>
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<inist:fA14 i1="02">
<s1>Space Science Division, Naval Research Laboratory</s1>
<s2>Washington, DC 20375</s2>
<s3>USA</s3>
<sZ>3 aut.</sZ>
<sZ>22 aut.</sZ>
</inist:fA14>
<country>États-Unis</country>
<wicri:noRegion>Washington, DC 20375</wicri:noRegion>
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<series>
<title level="j" type="main">Monthly Notices of the Royal Astronomical Society</title>
<title level="j" type="abbreviated">Mon. Not. R. Astron. Soc.</title>
<idno type="ISSN">0035-8711</idno>
<imprint>
<date when="2011">2011</date>
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<title level="j" type="main">Monthly Notices of the Royal Astronomical Society</title>
<title level="j" type="abbreviated">Mon. Not. R. Astron. Soc.</title>
<idno type="ISSN">0035-8711</idno>
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</fileDesc>
<profileDesc>
<textClass>
<keywords scheme="KwdEn" xml:lang="en">
<term>Dispersion measure</term>
<term>Flux density</term>
<term>Gamma radiation</term>
<term>Gamma ray source</term>
<term>High density</term>
<term>Millisecond pulsar</term>
<term>Orbits</term>
<term>Periodicity</term>
<term>Positions</term>
<term>Power law</term>
<term>Probability</term>
<term>Pulse shape</term>
<term>Radio pulsation</term>
<term>Radio spectrum</term>
<term>Radiopulsar</term>
<term>Timing</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr">
<term>Pulsar milliseconde</term>
<term>Pulsar radio</term>
<term>Source Rγ</term>
<term>Périodicité</term>
<term>Pulsation radio</term>
<term>Rayonnement gamma</term>
<term>Timing</term>
<term>Position</term>
<term>Spectre radio</term>
<term>Probabilité</term>
<term>Orbite</term>
<term>Densité élevée</term>
<term>Densité flux</term>
<term>Mesure dispersion</term>
<term>Loi puissance</term>
<term>Forme impulsion</term>
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<front>
<div type="abstract" xml:lang="en">Using the Parkes Radio Telescope, we have carried out deep observations of 11 unassociated gamma-ray sources. Periodicity searches of these data have discovered two millisecond pulsars, PSRJ1103-5403 (1FGLJ1103.9-5355) and PSRJ2241-5236 (1FGLJ2241.9-5236), and a long-period pulsar, PSRJ1604-44 (1FGLJ1604.7-4443). In addition, we searched for but did not detect any radio pulsations from six gamma-ray pulsars discovered by the Fermi satellite to a level of ˜0.04 mJy (for pulsars with a 10 per cent duty cycle). The timing of the millisecond pulsar PSRJ1103-5403 has shown that its position is 9 arcmin from the centroid of the gamma-ray source. Since these observations were carried out, independent evidence has shown that 1FGL J1103.9-5355 is associated with the flat spectrum radio source PKS 1101-536. It appears certain that the pulsar is not associated with the gamma-ray source, despite the seemingly low probability of a chance detection of a radio millisecond pulsar. We consider that PSRJ1604-44 is a chance discovery of a weak, long-period pulsar and is unlikely to be associated with 1FGL J1604.7-4443. PSR J2241-5236 has a spin period of 2.2 ms and orbits a very low mass companion with a 3.5-h orbital period. The relatively high flux density and low dispersion measure of PSR J2241-5236 make it an excellent candidate for high precision timing experiments. The gamma rays of 1FGL J2241.9-5236 have a spectrum that is well modelled by a power law with an exponential cut-off, and phase binning with the radio ephemeris results in a multipeaked gamma-ray pulse profile. Observations with Chandra have identified a coincident X-ray source within 0.1 arcsec of the position of the pulsar obtained by radio timing.</div>
</front>
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<li>District de Cologne</li>
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<li>Bonn</li>
<li>College Park (Maryland)</li>
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<name sortKey="Weltevrede, P" sort="Weltevrede, P" uniqKey="Weltevrede P" first="P." last="Weltevrede">P. Weltevrede</name>
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<country name="France">
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<name sortKey="Smith, D A" sort="Smith, D A" uniqKey="Smith D" first="D. A." last="Smith">D. A. Smith</name>
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