Galaxy masses from different tracers: how much mass there is in stars, gas, and dark matter, and how it is distributed
Galaxy assembly as traced from the kinematic structure: what the motions of stars and gas tell us about the structure of the galaxies
Galaxy assembly as traced through the stellar population content: how, when, and where did stars form throughout the history of the galaxies
CALIFA data are made public through regular releases (DR). DR1, containing 200 data cubes of 100 galaxies, was released 1 November 2012.[1] DR2, containing 400 data cubes of 200 galaxies, was released on 1 October 2014.[2]
"CALIFA, the Calar Alto Legacy Integral Field Area survey. I. Survey presentation"; S. F. Sánchez et al.; Astronomy & Astrophysics, Volume 538, id.A8, 31 pp. February 2012; doi:10.1051/0004-6361/201117353; Bibcode:2012A&A...538A...8S;
"CALIFA, the Calar Alto Legacy Integral Field Area survey. II. First public data release"; B. Husemann et al.; Astronomy & Astrophysics, Volume 549, id.A87, 25 pp. January 2013; doi:10.1051/0004-6361/201220582; Bibcode:2013A&A...549A..87H;
"CALIFA, the Calar Alto Legacy Integral Field Area survey. III. Second public data release"; R. García-Benito et al.; September 2014; Bibcode:2014arXiv1409.8302G; arXiv:1409.8302;
