CO(J=2-1) Survey of the Milky Way (Sakamoto+, 1995)

Details CO(J=2-1) Survey of the Milky Way (Sakamoto+, 1995) CO(J=2-1) Survey of the Milky Way (Sakamoto+, 1995)

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ycat..21000125s&link_type=abstract

VizieR On-line Data Catalog: J/ApJS/100/125. Originally published in: 1995ApJS..100..125S

Physics

Milky Way, Co, Radio Sources

Scientific paper

This extensive survey of the first quadrant of the Galaxy (GLON from 20 to 60 degrees, GLAT from -1 to +1 degrees) was taken with the 60-cm submillimiter-wave telescope of the University of Tokyo-Nobeyama Radio Observatory. The HPBW (half-power beam width) is 9+/-1 arcmin at 230GHz, and the intensity scale of the data is stable within typical fluctuations of 5%. It was carried out between December 1992 and May 1993. The survey gives the main-beam brightness temperatures (sensitivity of 0.4K) on a grid spaced every 15' (0.25 deg) in GLON and GLAT, and velocities spaced every 0.65km/s between -13 and 153 km/s (velocity resolution of 0.3km/s) (9 data files).

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