Long-term timing observations of 374 pulsars

DOI

We present pulsar timing solutions for 374 pulsars. Each ephemeris was obtained by analysing archival data stored at Jodrell Bank Observatory. This data archive contains over 5600yr of pulsar rotational history with individual data-spans of up to 34yr. A new method has been developed to mitigate the effects of timing noise by whitening the pulsar timing residuals.

Cone search capability for table J/MNRAS/353/1311/pulsars (Rotational slowdown and astrometrical parameters for the 374 pulsars)

Identifier
DOI http://doi.org/10.26093/cds/vizier.73531311
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/353/1311
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/353/1311
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/353/1311
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/353/1311
Provenance
Creator Hobbs G.; Lyne A.G.; Kramer M.; Martin C.E.; Jordan C.
Publisher CDS
Publication Year 2008
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysical Processes; Astrophysics and Astronomy; Galactic and extragalactic Astronomy; Natural Sciences; Physics; Stellar Astronomy