VizieR Online Data Catalog: Molecular gas distribution and star formation (Chown+, 2019)
Abstract
CARMA EDGE (Bolatto et al. 2017ApJ...846..159B, Cat. J/ApJ/846/159) is a survey of CO emission in 126 nearby galaxies carried out using the CARMA interferometer (Bock et al. 2006SPIE.6267E..13B). The CARMA EDGE sample was selected from the CALIFA sample with high fluxes in the 22um band from the Wide-field Spectroscopic Explorer (WISE) survey. The requirement for high mid-infrared flux means that the sample is mainly gas-rich and actively star-forming, given the correlation between the mid-infrared luminosities from WISE and the molecular gas mass (e.g. Jiang et al. 2015ApJ...799...92J). The sample consists of galaxies imaged in 12CO and 13CO with sensitivity. We use the publicly available 12CO J=1-0 integrated flux maps from CARMA EDGE.
We use optical IFU data from the 3rd data release (DR3) of the CALIFA survey (Sanchez et al. 2012A&A...538A...8S). The CALIFA survey consists of about 600 galaxies observed with the PMAS/PPak integral-field spectrograph at the Calar Alto Observatory (Roth et al. 2005PASP..117..620R; Kelz et al. 2006PASP..118..129K). The CALIFA datacubes are available in three spectral setups: (1) a low-resolution setup with 6Å spectral resolution (V500), (2) a medium-resolution setup with 2.3Å resolution (V1200), and (3) the combination of V500 and V1200 cubes (called COMBO). We used the COMBO data cubes from CALIFA DR3 where available. (2 data files).- Publication:
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VizieR Online Data Catalog
- Pub Date:
- September 2022
- Bibcode:
- 2022yCat..74845192C
- Keywords:
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- Galaxies;
- Molecular data;
- Star Forming Region;
- Equivalent widths;
- Carbon monoxide