The Arizona Molecular ISM Survey with the SMT: Full Data Release

The Arizona Molecular ISM Survey with the SMT (AMISS) is an extra-galactic survey of the CO(1-0), CO(2-1) and CO(3-2) spectral lines designed to constrain molecular gas properties of redshift zero galaxies by emperically calibrating the relationship between the CO spectral lines and molecular gas mass, temperature, and density.

Details of the survey can be found in the paper "The Arizona Molecular ISM Survey with the SMT: Survey Overview and Public Data Release" by Ryan P. Keenan, Daniel P. Marrone, Garret K. Keating et al. 

This data release contains the following files:

• amiss_spectra_data.tar.gz - compressed folder containing all CO(1-0), CO(2-1) and CO(3-2) spectra observed by AMISS. Files are named following the convetion AMISS.{ID}_CO{line} where ID is replaced with the AMISS survey ID number of each target and {line} is replaced by 10, 21, or 32 for CO(1-0), CO(2-1) and CO(3-2) respectively
• amiss_figure_gallery.tar.gz - plots showing the SDSS images and all available CO spectra of each target. These are also available as an online figure set in the published survey paper.
• amiss_catalog.txt - machine readable table (MRT) of basic galaxy properties, CO luminosities, and CO line ratios for each target (Table 6 in the accepted manuscript).

All redshift information comes from Saintonge, A. et al.  (2017) [2017ApJS..233...22S]; also available in the associated VizieR table (J/ApJS/233/22). All redshifts are spectroscopic. For sources where the CO(1-0) line is detected the value is the redshift derived from that line (column zCO in J/ApJS/233/22). Otherwise they are optical redshifts from SDSS (column zSDSS in J/ApJS/233/22).