Polarimetry of 600 pulsars from 1.4GHz obs.

Over the past 13yr, the Parkes radio telescope has observed a large number of pulsars using digital filter bank backends with high time and frequency resolution and the capability for Stokes recording. Here, we use archival data to present polarimetry data at an observing frequency of 1.4GHz for 600 pulsars with spin-periods ranging from 0.036 to 8.5s. We comment briefly on some of the statistical implications from the data and highlight the differences between pulsars with high and low spin-down energy. The data set, images and table of properties for all 600 pulsars are made available in a public data archive maintained by the CSIRO.

Cone search capability for table J/MNRAS/474/4629/table2 (Pulsar polarization properties at 1.4 GHz)

Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/474/4629
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/474/4629
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/474/4629
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/474/4629
Creator Johnston S.; Kerr M.
Publisher CDS
Publication Year 2021
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Resource Type Dataset; AstroObjects
Discipline Astrophysical Processes; Astrophysics and Astronomy; Cosmology; Exoplanet Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy