J/MNRAS/328/17ivo://CDS.VizieR/J/MNRAS/328/17doi:10.26093/cds/vizier.73280017CDSManchester R.N.Lyne A.G.Camilo F.Bell J.F.Kaspi V.M.D'Amico N.,McKay N.P.F.Crawford F.Stairs I.H.Possenti A.Kramer M.,Sheppard D.C.2024-06-27T20:17:47Z2006-02-26T21:34:49ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frpulsarsThe Parkes multi-beam pulsar survey is a sensitive survey of a strip along the Galactic plane with |b|<5{deg} and l=260{deg} to l=50{deg}. It uses a 13-beam receiver on the 64-m Parkes radio telescope, receiving two polarizations per beam over a 288-MHz bandwidth centred on 1374MHz. The receiver and data acquisition systems are described in some detail. For pulsar periods in the range 0.1-2s and dispersion measures of less than 300cm^-3^pc, the nominal limiting flux density of the survey is about 0.2mJy. At shorter or longer periods or higher dispersions, the sensitivity is reduced. Timing observations are carried out for pulsars discovered in the survey for 12-18 months after confirmation to obtain accurate positions, spin parameters, dispersion measures, pulse shapes and mean flux densities. The survey is proving to be extremely successful, with more than 600 pulsars discovered so far. We expect that, when complete, this one survey will come close to finding as many pulsars as all previous pulsar surveys put together. The newly discovered pulsars tend to be young, distant and of high radio luminosity. They will form a valuable sample for studies of pulsar emission properties, the Galactic distribution and evolution of pulsars, and as probes of interstellar medium properties. This paper reports the timing and pulse shape parameters for the first 100 pulsars timed at Parkes, including three pulsars with periods of less than 100ms which are members of binary systems. These results are briefly compared with the parameters of the previously known population.2001MNRAS.328...17Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/328/17CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/MNRAS/335/275 : Parkes Multi-Beam Pulsar Survey. II. (Morris+, 2002)J/MNRAS/342/1299 : Parkes Multi-Beam Pulsar Survey. III. (Kramer+, 2003)J/MNRAS/352/1439 : Parkes Multi-Beam Pulsar Survey. IV. (Hobbs+, 2004)J/MNRAS/372/777 : Parkes Multibeam Pulsar Survey. VI. (Lorimer+, 2006)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/328/17https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/328/17http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/328/17https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/328/17https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/328/17http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/328/17GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/328/17/psr (Pulsars discovered in the Parkes Multi-Beam Pulsar Survey)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/328/17/psr?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/328/17/psr?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/328/17/psr?GETtext/xml+votable180.050000true128.762833333-37.1309722220.0055555555555555566/37364 37372 37374 37717 37721 37758 37873 37895 37901 37903 37906 37915 37923-37924 37946 38020 39283 39294 41595 41597 41645 41652-41654 41657 41660 41671-41672 41677 41679 41681 41683-41686 41696 41701 41712 41768-41769 41772 41778 41781 41796 41799 41809 41811 41813 41816 41818 41840 41857 42157 42159 42168-42169 42172-42173 42203 42214 42216-42218 42232 42378 42383 42401 42438 42442 42445 42447 42449-42451 42456-42457 42460 42496-42497 42500-42501 42513 43019-43020 43022 43024https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/328/17?format=asciiRadiodefaultJ/MNRAS/328/17/psrPulsars discovered in the Parkes Multi-Beam Pulsar SurveyPSRJPulsar namecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRAJ2000Right ascension (J2000)pos.eq.ra;meta.maine_RAsrms uncertainty on RAsfloatDEJ2000Declination (J2000)pos.eq.dec;meta.maine_DEsrms uncertainty on DEarcsecfloatGLONGalactic longitudedegGLATGalactic latitudedegfloatBeamBeam in which the pulsar was detectedintbDistRadial distance of the pulsar from the beam centre in units of the beam radiusfloatS/NSignal-to-noise ratio of the discovery observation from the final time-domain folding in the search processfloatS1400MHzMean flux density at 1400MHzmJyfloate_S1400MHzrms uncertainty on S1400MHz0.01mJyintW50Pulse width at 50% of the peak of the mean pulse profilemsfloatW10? Pulse width at 10% of the peak of the mean pulse profilemsintnullablePerPeriodsdoublee_Perrms uncertainty on PersdoubledP/dtPeriod derivativedoublee_dP/dtrms uncertainty on dP/dtdoubleEpochJD of the epoch of the perioddfloatNTOANumber of time-of-arrival in the timing solutionintObsBegMJD range covered by the timing observationsdintObsEndMJD range covered by the timing observationsdintResResidual rms timing residual (in {mu}s)usintDMDispersion measurepc.cm**-3floate_DMrms uncertainty on DMpc.cm**-3floatl_log(tauc)Limit flag on log(tauc)charlog(tauc)Characteristic age, tauc = P/2(dP/dt)log(yr)floatl_log(Bs)Limit flag on log(Bs)charlog(Bs)Surface dipole magnetic field, Bs=3.2*10^19^[(P.dP/dt)^1/2^]log(0.0001T)floatl_log(dE/dt)Limit flag on log(dE/dt)charlog(dE/dt)Rate of loss of rotational energy (1)log(1e-07W)floatl_DistLimit flag on DistcharDistDistancekpcfloatl_ZLimit flag on ZcharZGalactic Z-distancekpcfloatl_L1400MHzLimit flag on L1400MHzcharL1400MHzRadio luminosity at L1400MHzmJy.kpc**-2floatSimbadSimbad column added by the CDSchar