Calibrated fits cubes can be downloaded from this link. When you use the data, we strongly recommend you to contact us. We note that new data with more sophisticated reduction from JVO in NAOJ is uploaded.
When you publish any result obtained from our data, we kindly request you to include the following acknowledgement, and cite the paper below.
"This publication made use of data from COMING, CO Multi-line Imaging of Nearby Galaxies, a legacy project of the Nobeyama 45-m radio telescope."
Reference: Sorai, K., et al. 2019, PASJ, 71, S14
(October 3, 2019)
Cubes of the following 19 galaxies were replaced because of our further reduction. Arp 283, NGC 628, NGC 660, NGC1022, NGC2339, NGC2976, NGC3077, NGC3169, NGC4030, NGC4041, NGC4045, NGC4085, NGC4527, NGC4559, NGC4579, NGC4632, NGC5676, NGC5713, and NGC5907. The number of emission channels of the revised data is 3 -13 channels larger than the previous one. The total intensity integrated over the whole cubes becomes 1.7 times larger than the previous one in NGC 4559, 1.6 times in NGC 3077 in 12CO. The absolute differences are much smaller in 13CO and C18O data, but their relative differences are much larger. We also make public baseline-emission identifying cubes for the whole data. In the cubes, 0 represents emission channel and 1 represents baseline channel.
Last modified: February 5, 2020