CASASOLA, VIVIANAVIVIANACASASOLA0000-0002-3879-6038HUNT, Leslie KippLeslie KippHUNT0000-0001-9162-2371Combes, F.F.CombesGarcia-Burillo, S.S.Garcia-Burillo2020-03-312020-03-312015http://hdl.handle.net/20.500.12386/23767<SUP>12</SUP>CO(1-0) and <SUP>12</SUP>CO(2-1) line intensity maps are p survey. NUGA observations have been carried out with 6 antennas of the PdBI in the ABCD configuration of the array and with the IRAM 30m single dish telescope. <P />For NGC 4569 and NGC 4826, we have also <SUP>12</SUP>CO(3-2) line intensity maps obtained with the Submillimeter Array (SMA) in its compact configuration with seven working antennas. <P />We retrieved Hα emission-line images from the Hubble Legacy Archive (HLA) that makes available HST WFPC2 observations of our galaxy sample. (2 data files).enDatabasehttps://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/577/A135&-to=32015yCat..35770135CFIS/05 - ASTRONOMIA E ASTROFISICA