830 citations · 10.9k across the 176 of their papers we have counts for
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ALFALFA HI Data Stacking III. Comparison of environmental trends in HI gas mass fraction and specific star formation rate
Silvia Fabello, Guinevere Kauffmann, Barbara Catinella +3
It is well known that both the star formation rate and the cold gas content of a galaxy depend on the local density out to distances of a few Megaparsecs. In this paper, we compare…
The impact of interactions, bars, bulges, and AGN on star formation efficiency in local massive galaxies
A. Saintonge, L. J. Tacconi, S. Fabello +10
Using observations from the GASS and COLD GASS surveys and complementary data from SDSS and GALEX, we investigate the nature of variations in gas depletion time observed across the…
The GALEX Arecibo SDSS Survey. VI. Second Data Release and Updated Gas Fraction Scaling Relations
Barbara Catinella, David Schiminovich, Guinevere Kauffmann +7
We present the second data release from the GALEX Arecibo SDSS Survey (GASS), an ongoing large Arecibo program to measure the HI properties for an unbiased sample of ~1000 galaxies…
Quantifying the role of bars in the build-up of central mass concentrations in disk galaxies
Jing Wang, Guinevere Kauffmann, Roderik Overzier +7
We analyze the role of bars in the build-up of central mass concentrations in massive, disk galaxies. Our parent sample consists of 3757 face-on disk galaxies with redshifts betwee…
COLD GASS, an IRAM Legacy Survey of Molecular Gas in Massive Galaxies: III. Comparison with semi-analytic models of galaxy formation
Guinevere Kauffmann, Cheng Li, Jian Fu +7
We compare the semi-analytic models of galaxy formation of Fu et al. (2010), which track the evolution of the radial profiles of atomic and molecular gas in galaxies, with gas frac…
The clustering of galaxies as a function of their photometrically-estimated atomic gas content
Cheng Li, Guinevere Kauffmann, Jian Fu +5
We introduce a new photometric estimator of the HI mass fraction (M_HI/M_*) in local galaxies, which is a linear combination of four parameters: stellar mass, stellar surface mass…