VizieR Online Data Catalog: CORE high-mass star-forming regions (Gieser+, 2021)

Physical and chemical properties of 120 positions toward 18 high-mass star-forming regions of the CORE sample. Table A shows the position (given by the region name and position number); coordinates (J2000); systemic velocity determined by the C¹⁸O line; noise in the spectrum; kinetic temperature determined by CH₃CN, if detected, or H₂CO; 1.37mm continuum intensity; continuum optical depth; and the molecular hydrogen column density. Table E shows the column densities of ¹³CO, C¹⁸O, SO, OCS, SO₂, DCN, H₂CO, HNCO, HC₃N, HC₃N v7=1, HC₃N v7=2, CH₃OH, CH₃OH vt=1, and CH₃CN derived with XCLASS toward the 120 positions. Lower and upper column density error estimates are given as well. If no lower and upper column density error is shown, the derived column density is an upper limit.

The reduced images and data cubes are all available at https://www2.mpia-hd.mpg.de/core/DATA/www

(2 data files).