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J/other/AuJPA/14.77    408MHz galactic radio sources         (Shaver+ 1970)

Galactic radio sources. II. High resolution 408 MHz observations Shaver P.A., Goss W.M. <Australian J. Phys. Astrophys. Suppl., 14, 77 (1970)> =1970AuJPA..14...77S (SIMBAD/NED BibCode)
ADC_Keywords: Radio sources Abstract: Contour maps of 58 regions are presented showing 408 MHz radioisophotes for over 200 galactic radio sources. Positions and integrated flux densities are listed for all the sources. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 121 253 Source positions and integrated flux densities
Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 11 A11 --- [GS70] Galactic source name (GLLL.l+BB.b) 12 A1 --- n_[GS70] [*+] Note on [GS70] (1) 14- 20 F7.3 deg GLON Source peak galactic longitude 22- 27 F6.3 deg GLAT Source peak galactic latitude 30- 31 I2 h RAh Source peak right ascension (1950) 33- 34 I2 min RAm Source peak right ascension (1950) 36- 39 F4.1 s RAs Source peak right ascension (1950) 41 A1 --- DE- Source peak declination sign (1950) 42- 43 I2 deg DEd Source peak declination (1950) 45- 46 I2 arcmin DEm Source peak declination (1950) 48- 49 I2 arcsec DEs Source peak declination (1950) 50- 51 A2 --- n_Tb Groups designation (2) 53- 55 I3 K Tb ? Individual base brightness temperature 58- 63 F6.1 Jy S408MHz ? Individual flux density at 408MHz 64 A1 --- n_Tbc [a-k] Groups designation (3) 66- 68 I3 K Tbc ? Composite base brightness temperature 70- 74 F5.1 Jy S408MHzc ? Composite flux density at 408MHz 76- 77 I2 --- Fig Countour map in which the source appears 79-121 A43 --- Name Other names
Note (1): * Galactic source number is different in Part I (Shaver & Goss, 1970AuJPA..14....1S) due to positional measuring error and/or real shifts in position with frequency. + G25.4-0.2 has often been mistakenly identified as W42 Note (2): For a group, same n_Tb, from a to ag, the values Tb, S, Tbc, Sc, Fig and Name concern those of the group. They are repeated in each line of the group members. Note (3): For a group, same n_Tbc, the values Tbc, Sc, Fig and Name concern those of the group. They are repeated in each line of the group members.
History: Prepared via OCR at CDS, and proof-read by H. Andernach References: Shaver & Goss, Paper I. 1970AuJPA..14....1S Shaver & Goss, Paper III. 1970AuJPA..14..133S
(End) James Marcout, Patricia Bauer [CDS] 18-Jan-1999
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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