Dataset 20220606
Data version: 20220606 (included all ALMA data in COSMOS and GOODS-South being public before date 2022-06-06)
Number of pointings/images: (beam_maj > 0.1 arcsec)
3232 in COSMOS
723 in GOODS-South
Number of ALMA projects:
173 in COSMOS
74 in GOODS-South
Data Release:
https://drive.google.com/drive/folders/1mlrgsicK_cbIr5WlwpAtX18B_R_JqCr8?usp=sharing
Two photometry catalogs per field:
The blind photometry catalog A-COSMOS_blind*.fits contains blindly extracted ALMA sources with a peak flux signal-to-noise ratio of 5.4 or higher. The catalog also contains a column with a flag for sources which are identified as blended.
The prior photometry catalog A-COSMOS_prior*.fits contains prior fitting of known optical/near-infrared/mid-infrared/radio sources in our COSMOS Master Catalog. Flux density information is provided only for sources above the detection threshold (peak flux signal-to-noise ratio of 4.35). For undetected sources, information on image noise and beam sizes is provided so that upper limits can be determined.
One galaxy property catalog per field:
The value-added galaxy catalog A-COSMOS_Robust_Galaxy_Catalog*.fits contains only robustly detected galaxies with optical/near-infrared detections, so that each galaxy has a reasonably constrained, consistently fitted stellar mass, star formation rate and redshift.
Other files available upon request:
The catalog datatable_ID_RA_Dec_z_Mstar_SFR_sSFR_with_deltaGas.fits contains the galaxies in the Robust Galaxy Catalog with more columns including the molecular and total gas masses computed using the Hughes+2017 calibration ('Mgas' column) and other calibration methods.
The catalog datatable_ID_RA_Dec_z_Mstar_SFR_sSFR_with_SED_fluxes.fits contains one or multiple ALMA fluxes for each galaxy. FOBS and FSED are the observed and SED predicted fluxes at each ALMA wavelength.
Meta tables in FITS format for our ALMA images. This is useful to check whether a source is in the spatial coverage of our dataset.
Our A3COSMOS/GOODSS Master Catalog, combining optical, near-IR, sub-mm and radio catalogs so as to identify unique sources for our prior-position-based photometry.
Notes:
The column names may be slightly different from our published ones, just let us know if you have any question.
There are a number of other very useful data:
Continuum images will be released soon at the COSMOS IRSA website: https://irsa.ipac.caltech.edu/data/COSMOS/overview.html or https://irsa.ipac.caltech.edu/data/COSMOS/images/a3cosmos/ (depending on IRSA schedule)
Galaxy SEDs (optical-to-mm-radio) are available upon request.
The dust and dust-inferred molecular gas mass of each galaxy in the Robust Galaxy Catalog are available upon request.
In addition, after the setup of the COSMOS IRSA repository, we will release a Python package to easily make cutouts and query sources.