VizieR Online Data Catalog: ALMA observations of GKM stars in Upper Sco (Barenfeld+, 2016)
Abstract
ALMA observations were obtained in Cycle 0 and Cycle 2 using the 12m array. Twenty sources were observed in Cycle 0 between 2012 August and 2012 December. Eighty-seven sources were observed in 2014 June and 2014 July. All observations used band 7 with the correlator configured to record dual polarization. Spectral windows for Cycle 2 were centered at 334.2, 336.1, 346.2, and 348.1GHz for a mean frequency of 341.1GHz (0.88mm). The bandwidth of each window is 1.875GHz. Cycle 0 observations used between 17 and 28 antennas with maximum baselines of ~400m, for an angular resolution of ~0.55". Cycle 2 observations used between 34 and 36 antennas with baselines extending out to 650m, corresponding to an angular resolution of 0.34".
(3 data files).- Publication:
-
VizieR Online Data Catalog
- Pub Date:
- November 2016
- DOI:
- 10.26093/cds/vizier.18270142
- Bibcode:
- 2016yCat..18270142B
- Keywords:
-
- Stars: masses;
- Spectral types;
- Effective temperatures;
- Millimetric/submm sources;
- Extinction