/ftp/cats/8/47
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VIII/47 Galactic 21-cm line Survey (Westerhout+ 1982)
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drwxr-xr-x 112 cats archive 4096 Nov 7 15:27 [Up]
drwxr-xr-x 2 cats archive 4096 Jan 12 2023 [TAR file]
-rw-r--r-- 1 cats archive 220 Aug 27 1998 .message
-r--r--r-- 1 cats archive 7566 Aug 27 1998 ReadMe
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Beginning of ReadMe :
VIII/47 Galactic 21-cm line Survey (Westerhout+ 1982)
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The Maryland-Green Bank Galactic 21-cm line survey
Westerhout G., Wendlandt H.U.
<Astron. Astrophys. Suppl. 49, 137 (1982)>
=1982A&AS...49..137W
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ADC_Keywords: H I data; Surveys; Galactic plane; Atlases
Description:
This catalog presents a completely sampled survey of 21-cm line
profiles extending from Galactic longitude 11 to 235 degrees and
nominally covering a range between latitude +2 and -2 degrees. It was
observed in 1971-72 with the newly resurfaced 92-m (300-foot)
telescope of the National Radio Astronomy Observatory (NRAO) in Green
Bank, W.V. The spatial resolution is 0.22 degrees (13 arcmin), and the
velocity resolution is 2 km/s. The line profiles have 260 values of
Brightness Temperature at 1 km/s intervals, and at spacings of 0.1
degree in longitude and 0.1 degree in latitude. The r.m.s per data
point varies from 1.0K at low declinations to 0.5K at high
declinations. The maps at constant Galactic longitude published in the
printed version are at intervals of 0.2 degrees in longitude; the
spectra in this catalog are therefore spatially twice as dense. The
catalog is arranged in two forms: as FITS data cubes, and as FITS
binary tables. The cubes contain three-dimensional arrays of spectra
for various longitude ranges. The binary tables contain spectra at
constant Galactic latitude, along with coordinate and velocity
information necessary for the interpretation of individual spectra.
A detailed description of the telescope beam characteristics and the
derivation of the temperature scale is given by Westerhout, G., Mader,
G.L., and Harten, R.H. (Astron. and Astrophys. Suppl. 49, 137-141,
1982). Temperature scales of this and several other 21-cm line surveys
were compared by Harten, R.H., Westerhout, G., and Kerr, F.J.
(Astron.J. 80, 307-310, 1975) and found to agree to within 5 %.