Flux densities of 235 pulsars at 102.5MHz (Malofeev+, 2000)

Details Flux densities of 235 pulsars at 102.5MHz (Malofeev+, 2000) Flux densities of 235 pulsars at 102.5MHz (Malofeev+, 2000)

Nov 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ycat..80770499m&link_type=abstract

VizieR On-line Data Catalog: J/AZh/77/499. Originally published in: 2000AZh....77..499M; 2000ARep...44..436M

Physics

Pulsars, Radio Sources

Scientific paper

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. (1 data file).

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