VizieR Online Data Catalog: Linking ice and gas. Serpens SVS4 (Perotti+, 2020)

The observations of the Serpens SVS 4 cluster were done with the Submillimeter Array (SMA), Mauna Kea, Hawaii, program code: 2016B-S022; with the Atacama Pathfinder EXperiment (APEX), Llano Chajnantor, Chile, program code: 099.F-9316(A) and with the Very Large Telescope (VLT), Paranal, Chile, under European Southern Observatory (ESO) programmes 075.C-0384(A) and 077.C-0363(A). The calibration and imaging were done in CASA and CLASS. The datacubes are 6 FITS files that correspond to 4 spectral windows for each sideband (lower and upper) and each receiver (230 and 240GHz). The VLT spectra are 20 ascii files.

(4 data files).