J/MNRAS/342/1299ivo://CDS.VizieR/J/MNRAS/342/1299doi:10.26093/cds/vizier.73421299CDSKramer M.Bell J.F.Manchester R.N.Lyne A.G.Camilo F.Stairs I.H.,D'Amico N.Kaspi V.M.Hobbs G.Morris D.J.Crawford F.Possenti A.,Joshi B.C.McLaughlin M.A.Lorimer D.R.Faulkner A.J.2024-06-28T20:17:20Z2004-09-16T06:56:30ZCDS support team

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

cds-question@unistra.frpulsarsradio-astronomygamma-ray-astronomyThe Parkes Multibeam Pulsar Survey has unlocked vast areas of the Galactic plane, which were previously invisible to earlier low-frequency and less-sensitive surveys. The survey has discovered more than 600 new pulsars so far, including many that are young and exotic. In this paper we report the discovery of 200 pulsars for which we present positional and spin-down parameters, dispersion measures, flux densities and pulse profiles. A large number of these new pulsars are young and energetic, and we review possible associations of {gamma}-ray sources with the sample of about 1300 pulsars for which timing solutions are known. Based on a statistical analysis, we estimate that about 19+/-6 associations are genuine. The survey has also discovered 12 pulsars with spin properties similar to those of the Vela pulsar, nearly doubling the known population of such neutron stars. Studying the properties of all known 'Vela-like' pulsars, we find their radio luminosities to be similar to normal pulsars, implying that they are very inefficient radio sources. Finally, we review the use of the newly discovered pulsars as Galactic probes and discuss the implications of the new NE2001 Galactic electron density model for the determination of pulsar distances and luminosities.2003MNRAS.342.1299Khttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/342/1299CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toVII/189 : Catalog of Pulsars (Taylor+ 1995)J/ApJS/123/79 : Third EGRET catalog (3EG) (Hartman+, 1999)J/MNRAS/328/17 : Parkes Multi-Beam Pulsar Survey. I. (Manchester+, 2001)J/MNRAS/335/275 : Parkes Multi-Beam Pulsar Survey. II. (Morris+, 2002)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/342/1299https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/342/1299http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/342/1299https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/342/1299https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/342/1299http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/342/1299GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/342/1299/table1 (*Positions, flux densities and widths for 200 pulsars discovered in the Parkes Multibeam Pulsar Survey (PMPS))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/342/1299/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/342/1299/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/342/1299/table1?GETtext/xml+votable180.050000true127.885125-44.103305560.0055555555555555566/28730 28800 29130 29525 29556 30211 30428 30430 30505 30606 37207 37215 37236 37244 37317 37331-37332 37339 37343 37360-37361 37365 37863 37874 37891-37892 37902 37904 37909 37919 37921-37922 37929 37931 37963 37984 38406 38436 39243 39269 41454 41466 41578 41585 41594 41615 41628 41647 41650 41656 41660 41671 41674 41679 41682 41684-41685 41687 41695 41697-41698 41704 41706 41713 41743 41755-41756 41758 41763 41765 41771 41773 41777-41778 41781 41788-41789 41793 41798-41799 41803-41804 41806 41810 41812-41813 41815-41816 41820-41821 41828-41829 41833 41840-41841 41844 41859 41865 42126 42143 42147 42156 42158 42162 42170 42187 42193 42200 42206 42209 42214-42215 42217 42219-42220 42223 42225-42228 42231 42237 42301 42348 42363 42368 42374-42375 42378-42382 42384 42386 42389 42394 42396-42397 42399 42401 42405 42432-42433 42435 42437-42438 42441-42442 42445 42468 42504 42510 42514 42517 42529 42533 42560 43013 43015 43017 43025 43040 43044 43065 43137 431409.276497240453405e-25 9.276497240453405e-25https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/342/1299?format=asciiGamma-rayRadiodefaultJ/MNRAS/342/1299/table1*Positions, flux densities and widths for 200 pulsars discovered in the Parkes Multibeam Pulsar Survey (PMPS)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintPSRJPSR J denominationmeta.id;meta.maincharprimaryn_PSRJ[J] J: pulsars that have also been timed at Jodrell Bankmeta.notecharRAJ2000Right ascension (J2000)pos.eq.ra;meta.maine_RAJ2000rms uncertainty on right ascensionsstat.error;pos.eq.rafloatDEJ2000Declination (J2000)pos.eq.dec;meta.maine_DEJ2000rms uncertainty on declinationarcsecstat.error;pos.eq.decfloatGLONGalactic longitudedegpos.galactic.lonGLATGalactic latitudedegpos.galactic.latfloatBeamBeam in which the pulsar was detectedmeta.id;instrintDistRadial distance of the pulsar from the beam centre in units of beam radius (~7')pos.cartesian;instr.detfloatS/NSignal-to-noise ratio of the discovery observation from the final time-domain folding in the search processobs.param;obsfloatS1400MHzMean flux density at 1400MHzmJyphot.flux.density;em.radio.750-1500MHzfloate_S1400MHzrms uncertainty on S1400MHzmJystat.errorfloatW50Pulse width at 50% of the peak of the mean pulse profilemssrc.var.pulsefloatW10? Pulse width at 10% of the peak of the mean pulse profilemssrc.var.pulseintnullableJ/MNRAS/342/1299/table2Periods, period derivatives and dispersion measures for 200 pulsars discovered in the PMPSrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintPSRJPSR J designationmeta.id;meta.maincharn_PSRJ[B] B: binary pulsarmeta.notecharf_PSRJ[*] Note (1)meta.codecharPerPeriodstime.perioddoublee_Perrms uncertainty on Persstat.errordoubledPer/dtPeriod derivativemeta.notedoublee_dPer/dtrms uncertainty on dPer/dtstat.errordoubleObsMJDModified Julan date of observation (MJD)dtime.epochintNtANumber of time of arrivalsmeta.numberintSpan1Range covered, MJD of beginningdtime.epochintSpan2Range covered, MJD of endingdtime.epochintResrms of the post-fit residualmsstat.fit.residualfloatDMDispersion measurecm**3.pc**-1phys.dispMeasure;instr.dispersionfloate_DMrms uncertainty on DMcm**3.pc**-1stat.errorfloatJ/MNRAS/342/1299/table3Derived parameters for 200 pulsars discovered in the Parkes Multibeam Pulsar SurveyrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintPSRJPSR J designationmeta.id;meta.maincharlogTcCharacteristic agelog(yr)time.agefloatlogBsSurface magnetic dipole field strengthlog(0.0001T)phys.magField;phys.atmol.collStrengthfloatlog(Edot)Rate of rotational energy losslog(1e-07W)phys.energy;phys.mol.rotationfloatDistDistance derived from the DM and the Taylor & Cordes (1993ApJ...411..674T) modelkpcpos.distance;pos.heliocentricfloatZInferred Z-height (over the Galactic plane)kpcpos.cartesian.z;pos.galacticfloatL1400MHzRadio luminosity at 1400MHz corresponding to ZmJy.kpc**-2phot.flux.density;em.radio.750-1500MHzfloatJ/MNRAS/342/1299/table4EGRET point sources as listed in the 3EG catalogue (Hartman et al., 1999, <J/ApJS/123/79>) and radio pulsars positionally coincident with their error boxesn_DistTC[*] *: Distance obtained by independent estimate, used for (Edot)/d^2^meta.notecharl_DistLimit flag on Distmeta.code.errorcharDistDistance from new NE2001, Cordes & Lazio (2002, astro-ph/0207156) (3)kpcpos.distance;pos.heliocentricfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint3EGJ3EG J denomination (<J/ApJS/123/79>)meta.id;meta.maincharID[PAG?] Identification listed in the 3EG catalog (1)meta.idcharFluxFlux for E>100MeV, in 10^-10^erg/s/cm^2^1e-13W.m**-2phot.flux.density;em.gamma.hardfloate_Fluxrms uncertainty on Flux1e-13W.m**-2stat.error;phot.fluxfloatVarVariability index, from McLaughlin (2001, PhD thesis, Cornell Univ.)src.var.indexfloatTheta95Size of the 95 per cent error-boxdegphys.angSizefloatPSRAssociated pulsar (2)meta.id.crosscharn_PSR[+] +: Name and parameters based on preliminary timing solutionmeta.notecharDPosRelative positional differencepos.angDistancefloatDistTCTaylor & Cordes, 1993ApJ...411..674T model dispersion measure distancekpcpos.angDistancefloatTcCharacteristic agekyrtime.agedoublelog(Edot)Spin-down luminosity Edot=dE/dt (3)log(1e-07W)phys.energyfloatlog(Edot/d2)Spin-down flux value (3)log(1e-07W.kpc**-2)phys.energyfloatetaGamma-ray efficiency for a beaming fraction of 1/4{pi}%phys.electron.degen;arith.ratiodoubleQLikelihood of a genuine association (+, -, +? or ?)meta.codecharRefsReferences to the pulsar and/or already proposed associations, in refs.dat filemeta.ref;pos.framecharJ/MNRAS/342/1299/table5Young pulsars with spin parameters similar to the Vela pulsarrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintPSRPSR designationmeta.id;meta.maincharPerPeriodmstime.periodfloatTcCharacteristic age, 10<-Tc<-100kyrkyrtime.ageintEdotSpin-down luminosity (10^36^erg/s)1e+29Wphys.energyfloatRefsReferences, detailed in refs.dat filemeta.ref;pos.framecharNotesNotes (1)meta.notecharJ/MNRAS/342/1299/refsReferencesComCommentsmeta.notecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRefReference numbermeta.id;meta.maincharBibCodeBibCodemeta.bib.bibcodecharAutAuthor's namemeta.bib.authorchar