VizieR Online Data Catalog: ATOMS I Description and a first look at G9.62+0.19 (Liu+, 2020)

The ATOMS sample of 146 sources was selected from the CS J=2-1 survey of Bronfman, Nyman & May (1996A&AS..115...81B, Cat. J/A+AS/115/81), a complete and homogenous molecular line survey of UC HII region candidates in the Galactic plane. The sample of our 146 targets is complete for protoclusters with bright CS J=2-1 emission (T_b>2K), indicative of reasonably dense gas. It is also complete for the longitude range observable by SEST as well as ALMA (Faundez et al. 2004A&A...426...97F, Cat. J/A+A/426/97). Table A1 lists the basic parameters of this sample, including source IDs in observations, IRAS names, coordinates, systemic velocities, distances from the sun, Galactocentric distances, effective radii, dust temperature, bolometric luminosity, and clump masses. There are 122 clumps with ATLASGAL and HiGAL counterparts, which have been analysed in detail by Urquhart, Konig & Giannetti (2018MNRAS.473.1059U, Cat. J/MNRAS/473/1059). The basic parameters for these 122 clumps are adopted from Urquhart et al. (2018MNRAS.473.1059U, Cat. J/MNRAS/473/1059). The basic parameters for the remaining clumps are adopted from Faundez et al. (2004A&A...426...97F, Cat. J/A+A/426/97).

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