Flux densities of 235 pulsars at 102.5MHz

The flux densities of 235 mostly faint pulsars at 102.5MHz are presented. The observations were carried out on the very sensitive Large Phased Array of the Lebedev Institute of Physics in 1994-1998. The procedure used for the observations and data processing is described in detail, and estimates of probable errors, including the effect of interstellar scintillations, are given. The mean spectral indices at 102-408MHz for normal and millisecond pulsars are calculated and compared with information from higher frequency data. There is a deficit of pulsars at distances of less than 3 kpc.

Cone search capability for table J/AZh/77/499/table2 (Flux densities of Pulsars at 102.5 MHz)

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/AZh/77/499
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AZh/77/499
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AZh/77/499
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/AZh/77/499
Provenance
Creator Malofeev V.M.; Malov O.I.; Shchegoleva N.V.
Publisher CDS
Publication Year 2001
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; Cosmology; Natural Sciences; Physics; Stellar Astronomy