/ftp/cats/III/172



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III/172     Radial Velocities from Objective Prism Plates (Stock 1992)
The following files can be converted to FITS (extension .fit .fit.Z .fgz)
	table3 table4
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=III/172
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drwxr-xr-x 259 cats archive 8192 Dec 5 19:00 [Up] drwxr-xr-x 2 cats archive 231 Jul 25 2023 [TAR file] -rw-r--r-- 1 cats archive 457 Dec 19 2022 .message -r--r--r-- 1 cats archive 3257 Jul 22 1996 ReadMe -rw-r--r-- 1 cats archive 1053 Feb 26 2013 +footg5.gif -rw-r--r-- 1 cats archive 2605 Feb 26 2013 +footg8.gif -r--r--r-- 1 cats archive 61636 Jul 20 1993 table3 -r--r--r-- 1 cats archive 37316 Jul 20 1993 table4
Beginning of ReadMe : III/172 Radial Velocities from Objective Prism Plates (Stock 1992) ================================================================================ Radial Velocities from Objective Prism Plates Stock J. <Rev. Mex. Astron. Astrofis., 24, 45 (1992)> =1992RMxAA..24...45S ================================================================================ ADC_Keywords: Galactic plane ; Galactic pole, south ; Spectral types ; Radial velocities Description: Accurate positions and radial velocities are determined from 32 objective-prism plates for two areas. Each field is observed twice with opposite dispersion, allowing adjustment of coordinates for spectra not at the plate centers. From the adjusted coordinates and plate overlap, positions are determined with average mean errors: 0.0135 s in RA and 0.177 arcsec in Dec for Area I (near the South Galactic Pole); 0.0315 s in RA, 0.144 arcsec in Dec for Area II (near the galactic plane). Observations were taken by J.D. MacConnell and G. Araya with a six degree prism on the Curtis Schmidt telescope at Cerro Tololo.