VizieR Online Data Catalog: Cold molecular gas in merger remnants. II. (Ueda+, 2021)

Multiline observations toward 28 merger remnants were carried out using the Large Millimeter Telescope (LMT) between 2014 October and 2015 May in its early science phase (frequency range 73-111GHz with a spectral resolution of 31.25MHz).

We also used the CO(1-0) data of six sources (Arp 187, AM 0956-282, NGC 3597, AM 1300-233, AM 2055-425, and NGC 7252) obtained with the Atacama Large Millimeter/submillimeter Array (ALMA) 12m array and the Atacama Compact Array (ACA: 7m array + Total Power (TP) array) as part of 2011.0.00099.S, 2016.2.00006.S, and 2017.1.01003.S. In addition, we used the CO(1-0) data of NGC 3256 obtained with the ALMA 12m (TM2) array and the ACA 7m array as part of 2016.2.00042.S, 2016.2.00094.S, and 2018.1.00223.S.

(3 data files).