The inferred evolution of the cold gas properties of CANDELS galaxies at 0.5 < z < 3.0

Bibliographic Details
Title: The inferred evolution of the cold gas properties of CANDELS galaxies at 0.5 < z < 3.0
Authors: Popping, G., Caputi, K. I., Trager, S. C., Somerville, R. S., Dekel, A., Kassin, S. A., Kocevski, D. D., Koekemoer, A. M., Faber, S. M., Ferguson, H. C., Galametz, A., Grogin, N. A., Guo, Y., Lu, Y., van der Wel, A., Weiner, B. J.
Publication Year: 2015
Collection: Astrophysics
Subject Terms: Astrophysics - Astrophysics of Galaxies
More Details: We derive the total cold gas, atomic hydrogen, and molecular gas masses of approximately 24 000 galaxies covering four decades in stellar mass at redshifts 0.5 < z < 3.0, taken from the CANDELS survey. Our inferences are based on the inversion of a molecular hydrogen based star formation law, coupled with a prescription to separate atomic and molecular gas. We find that: 1) there is an increasing trend between the inferred cold gas (HI and H2), HI, and H2 mass and the stellar mass of galaxies down to stellar masses of 10^8 Msun already in place at z = 3; 2) the molecular fractions of cold gas increase with increasing stellar mass and look-back time; 3) there is hardly any evolution in the mean HI content of galaxies at fixed stellar mass; 4) the cold gas fraction and relative amount of molecular hydrogen in galaxies decrease at a relatively constant rate with time, independent of stellar mass; 5) there is a large population of low-stellar mass galaxies dominated by atomic gas. These galaxies are very gas rich, but only a minor fraction of their gas is molecular; 6) the ratio between star-formation rate (SFR) and inferred total cold gas mass (HI + H2) of galaxies (i.e., star-formation efficiency; SFE) increases with star-formation at fixed stellar masses. Due to its simplicity, the presented approach is valuable to assess the impact of selection biases on small samples of directly-observed gas masses and to extend scaling relations down to stellar mass ranges and redshifts that are currently difficult to probe with direct measurements of gas content.
Comment: Accepted for publication in MNRAS. 22 pages, 18 figures. Data products are available at http://www.eso.org/~gpopping/Gergo_Poppings_Homepage/Data.html
Document Type: Working Paper
DOI: 10.1093/mnras/stv2136
Access URL: http://arxiv.org/abs/1509.04720
Accession Number: edsarx.1509.04720
Database: arXiv
More Details
DOI:10.1093/mnras/stv2136