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J/A+A/312/745    SSRS groups of galaxies redshift neighbourhood (Ramella+, 1996)

The redshift-space neighbourhoods of 13 SSRS groups of galaxies Ramella M., Focardi P., Geller M.J. <Astron. Astrophys. 312, 745 (1996)> =1996A&A...312..745R (SIMBAD/NED BibCode)
ADC_Keywords: Redshifts ; Clusters, galaxy Keywords: galaxies: general - galaxies: clusters of - galaxies: redshifts Description: The Southern Sky Redshift Survey (SSRS) includes 13 groups of 5 or more members with velocities ≥2000km/s. By measuring redshifts and accumulating data from the literature, we increase the total number of known group members from 89 to 218. We also measured new redshifts for 59 foreground/background galaxies superimposed on the group neighborhoods. The velocity dispersions of the groups are remarkably stable. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 35 227 The groups redshift neighborhood table2.tex 71 370 TeX version of table2 table3.dat 35 59 New redshifts in the fore/backgrounds of groups table3.tex 71 98 TeX version of table3
Byte-by-byte Description of file: table2.dat table3.dat
Bytes Format Units Label Explanations
1- 2 I2 --- Group ? Group number (only in table2) 4- 5 I2 h RAh Right Ascension 1950 (hours) 7- 8 I2 min RAm Right Ascension 1950 (minutes) 10- 13 F4.1 s RAs Right Ascension 1950 (seconds) 15 A1 --- DE- Declination 1950 (sign) 16- 17 I2 deg DEd Declination 1950 (degrees) 19- 20 I2 arcmin DEm Declination 1950 (minutes) 22- 23 I2 arcsec DEs Declination 1950 (seconds) 25- 29 I5 km/s cz Heliocentric velocity 31- 33 I3 km/s e_cz ?=0 Mean error on cz 35 A1 --- r_cz Reference for cz (1)
Note (1) : The references are: M = Maia et al. (MdCL), 1989, Ap.J.S. 69,809 =1989ApJS...69..809M 0 = from ZCAT (Huchra, see Cat. VII/193) 1 = this work, RV from absorption lines in a low resolution spectrum 2 = this work, RV from absorption lines in a high resolution spectrum 3 = this work, RV from absorption lines (average of low and high respective spectrum) 4 = this work, RV from emission lines in a low resolution spectrum 5 = this work, RV from emission lines in a high resolution spectrum 6 = this work, RV from emission lines (average of low and high respective spectrum) Courtesy: P. Focardi <pfocardi(at)astbo4.bo.astro.it>
(End) Patricia Bauer [CDS] 18-Mar-1996
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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