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J/MNRAS/273/411     Multifrequency fluxes of 280 pulsars     (Lorimer+ 1995)

Multifrequency flux density measurements of 280 pulsars. Lorimer D.R., Yates J.A., Lyne A.G., Gould D.M. <Mon. Not. R. Astron. Soc. 273, 411 (1995)> =1995MNRAS.273..411L (SIMBAD/NED BibCode)
ADC_Keywords: Pulsars ; Radio sources Keywords: Pulsars: general - radio continuum: stars. Description: Table3 contains the flux density measurements of pulsars made at radio frequencies centred around 408, 606, 925, 1408 and 1606MHz using the 76-m Lowell telescope at Jodrell Bank. The observations have been made over a period of more than 3 years and concern 280 pulsars. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table3.dat 109 280 Fluxes for the 280 pulsars spectra.ps 132 19926 Postscript spectra (completed Figure 1)
See also: VII/156 : Catalog of pulsars (Taylor+, 1993) J/A+AS/147/195 : Pulsar spectra of radio emission (Maron+, 2000) http://www.mpifr-bonn.mpg.de/pulsar : MPIfR pulsar group Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 8 A8 --- PSRB Name of pulsar as in Taylor cat. VII/156 11- 13 I3 ms W50 *? Pulse width at 50% of pulse peak 16- 18 I3 ms W10 *? Pulse width at 10% of pulse peak 20 A1 --- l_S408 Limit flag on S408 21- 26 F6.1 mJy S408 ? Flux density at 408MHz 27- 31 F5.1 mJy e_S408 ? Mean error on S408 33 A1 --- l_S606 Limit flag on S606 34- 39 F6.1 mJy S606 ? Flux density at 606MHz 40- 44 F5.1 mJy e_S606 ? Mean error on S606 46 A1 --- l_S925 Limit flag on S925 48- 52 F5.1 mJy S925 ? Flux density at 925MHz 53- 57 F5.1 mJy e_S925 ? Mean error on S925 59 A1 --- l_S1408 Limit flag on S1408 61- 65 F5.1 mJy S1408 ? Flux density at 1408MHz 66- 70 F5.1 mJy e_S1408 ? Mean error on S1408 72 A1 --- l_S1606 Limit flag on S1606 74- 78 F5.1 mJy S1606 ? Flux density at 1606MHz 79- 83 F5.1 mJy e_S1606 ? Mean error on S1606 85 A1 --- l_SI Limit flag on SI 87- 91 F5.1 --- SI ? Spectral index (F(nu) prop.to. (nu)**(SI)) 93- 96 F4.1 --- e_SI ? Limit flag on SI
Note on W50, W10: the pulse widths are taken mainly from the 408MHz profile data.
Acknowledgements: The table was kindly supplied by Dunc Lorimer in January 1998.
(End) Francois Ochsenbein [CDS] 26-Jan-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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