/ftp/cats/viii/39



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VIII/39          Composite CO Survey of the Milky Way    (Dame+ 1987)
The following files can be converted to FITS (extension .fit or fit.gz)
	files.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=VIII/39
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drwxr-xr-x 112 cats archive 4096 Nov 7 15:27 [Up] drwxr-xr-x 3 cats archive 303 Jan 13 2023 [TAR file] -rw-r--r-- 1 cats archive 450 Dec 19 2022 .message -r--r--r-- 1 cats archive 2937 Dec 28 2016 ReadMe -r--r--r-- 1 cats archive 15120 Sep 29 2010 files.dat [txt] [txt.gz] [fits] [fits.gz] [html] drwxr-xr-x 2 cats archive 20480 Dec 28 2016 fits -rw-r--r-- 1 cats archive 1920 Mar 20 2017 saada.ant.err -rw-r--r-- 1 cats archive 186943 Mar 20 2017 tmp.log
Beginning of ReadMe : VIII/39 Composite CO Survey of the Milky Way (Dame+ 1987) ================================================================================ Composite CO Survey of the Milky Way Dame T.M., Ungerechts H., Cohen R.S., de Geus E., Grenier I.A., May J., Murphy D.C., Nyman L.-A., Thaddeus P. <Astrophys. J., 322, 706 (1987)> =1987ApJ...322..706D ================================================================================ ADC_Keywords: Radio sources; Surveys; Carbon monoxide; Galactic plane Description: This survey consists of CO(J=1-0) (115 GHz) spectra for the entire Galactic plane. The latitude coverage varies with longitude and in some regions extends from -25 degrees to +25 degrees. The observations were made with the Columbia/GISS 1.2m telescope in New York City, and a twin telescope on Cerro Tololo in Chile. The angular resolution of the survey is 30' (square), the velocity resolution is 1.3km/s and the sensitivity ranges from about 0.1K/chan to 0.35K/chan. The survey is presented as 720 latitude-velocity maps in FITS format, one for each 30' of longitude from -180.0 deg to +179.5 deg, and one velocity-integrated map covering the entire plane. The velocity range of each file is -300 km/s to +300 km/s. The survey has been updated to include some additional data, more careful reprojections of the regions that were originally mapped in equatorial coordinates, and improved estimates of the absolute calibration of the CO intensities (Digel and Dame 1995, unpublished).