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J/AZh/77/499        Flux densities of 235 pulsars at 102.5MHz (Malofeev+, 2000)

Flux densities of 235 pulsars at 102.5 MHz Malofeev V.M., Malov O.I., Shchegoleva N.V. <Astron. Zh. 77, 499 (2000)> =2000AZh....77..499M =2000ARep...44..436M
ADC_Keywords: Pulsars ; Radio sources Description: 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. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 44 238 Flux densities of Pulsars at 102.5 MHz
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
2- 11 A10 --- PSR Name of pulsar (1) 13- 14 A2 --- Rem Remarks: MP - main impulse, IP - intermediate impulse 15 A1 --- l_Flux ? Limit symbol on flux 16- 20 I5 mJy Flux Flux density at 102.5MHz 21 A1 --- u_Flux Uncertainty flag on Flux 23- 26 I4 mJy e_Flux ? Mean error on Flux 27 A1 --- ueFlux Uncertainty flag on e_Flux 29- 33 F5.1 10+3 Nper Number of summed periods of pulsar 37- 38 I2 --- Nobs Number of observation days 40 A1 --- l_Sp-Index ? Limit flag on alpha 41- 44 F4.1 --- Sp-Index ? Spectral index in the frequency range of 102-408MHz ( - dLogFlux/dlogν )
Note (1): Taylor et al., 1993, Cat. VII/156

(End) Veta Avedisova [INASAN] 12-Dec-1998
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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