VizieR Online Data Catalog: Observation of 148 young stars toward NGC 1980 (Kounkel+, 2017)

We conducted observations using the Inamori-Magellan Areal Camera and Spectrograph (IMACS) on the Magellan Baade telescope. Observations were done using the f/2 camera with the 300 line grism at a blaze angle of 17.5° and slit width of 0.6". In this configuration, the typical resolution is 4Å, and the spectral coverage is approximately 4000-9000Å.

We observed four fields toward NGC1980 using the multi-slit mode on 2016 January 7. We targeted 280 sources identified by Bouy et al. 2014 (Cat. J/A+A/564/A29) with r<21mag, of which 212 sources had probabilities of membership (P) greater than 50%. The exposure time was 5*10 minutes per field for the first three fields, and the last field had the exposure time of 8*10 minutes. The weather conditions deteriorated rapidly over the course of the night, therefore, while the first field had the full sensitivity, the last field, even with the increased exposure time, yielded little in terms of the number of sources detected. Partially because of this, we have detected only 148 sources (see Table1).

(1 data file).