The Arizona Molecular ISM Survey with the SMT: Survey Overview and Public Data Release
Ryan P. Keenan, Daniel P. Marrone, Garrett K. Keating, Evan C. Mayer,, Kevin Bays, John Downey, Lochlann C. Dunn, Joanne C. Flores, Thomas W., Folkers, David C. Forbes, Blythe C. Guvenen, Christian Holmstedt, Robert M., Moulton, Patrick Sullivan

TL;DR
This survey calibrates higher J CO lines as tracers of molecular gas in galaxies, providing a comprehensive dataset and analysis of line ratios to improve understanding of molecular gas properties across galaxy populations.
Contribution
The paper introduces the AMISS survey, providing calibrated CO(2-1) and CO(3-2) line data for a representative galaxy sample, enabling better use of higher J CO lines as molecular gas tracers.
Findings
Median CO(2-1)/CO(1-0) ratio is 0.71
Median CO(3-2)/CO(1-0) ratio is 0.39
CO disk sizes are on average equal to optical sizes
Abstract
The CO(1-0) line has been carefully calibrated as a tracer of molecular gas mass. However, recent studies often favor higher J transitions of the CO molecule which are brighter and accessible for redshift ranges where CO(1-0) is not. These lines are not perfect analogues for CO(1-0), owing to their more stringent excitation conditions, and must be calibrated for use as molecular gas tracers. Here we introduce the Arizona Molecular ISM Survey with the SMT (AMISS), a multi-CO line survey of z~0 galaxies conducted to calibrate the CO(2-1) and CO(3-2) lines. The final survey includes CO(2-1) spectra of 176 galaxies and CO(3-2) spectra for a subset of 45. We supplement these with archival CO(1-0) spectra from xCOLD GASS for all sources and additional CO(1-0) observations with the Kitt Peak 12m Telescope. Targets were selected to be representative of the galaxy population in the stellar mass…
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Taxonomy
TopicsDiverse Educational Innovations Studies · Survey Methodology and Nonresponse · Various Chemistry Research Topics
