output
20032026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations

Showing 2014 · astro-ph.GAShow all

107 papers · 2 filters

astro-ph.GA2014★ 12 cited

Star Formation in High-Redshift Cluster Ellipticals

Cory R. Wagner, Mark Brodwin, Gregory F. Snyder +11

We measure the star formation rates (SFRs) of massive () early-type galaxies (ETGs) in a sample of 11 high-redshift () galaxy clusters…

astro-ph.GA2014★ 149 cited

ZFOURGE/CANDELS: On the Evolution of M* Galaxy Progenitors from z=3 to 0.5

Casey Papovich, I. Labbé, R. Quadri +38

Galaxies with stellar masses near M* contain the majority of stellar mass in the universe, and are therefore of special interest in the study of galaxy evolution. The Milky Way (MW…

astro-ph.GA2014★ 5 cited

Modeling Warm Absorption in HST/COS Spectrum of Mrk 290 with XSTAR

S. N. Zhang, L. Ji, T. R. Kallman +4

We present a new method to model a HST/COS spectrum, aimed to analyze intrinsic UV absorption from the outflow of Mrk 290, a Seyfert I galaxy. We use newly updated XSTAR to generat…

astro-ph.GA2014★ 47 cited

Frontier Fields : Combining HST, VLT and Spitzer data to explore the 8 Universe behind the lensing cluster MACS04162403

N. Laporte, A. Streblyanska, S. Kim +7

(Abridged) The HST Frontier Fields project started at the end of 2013 with the aim of providing extremely deep images of 6 massive galaxy clusters. One of the main goals of this pr…

astro-ph.GA2014★ 282 cited

Stellar masses from the CANDELS survey: the GOODS-South and UDS fields

P. Santini, H. C. Ferguson, A. Fontana +35

We present the public release of the stellar mass catalogs for the GOODS-S and UDS fields obtained using some of the deepest near-IR images available, achieved as part of the Cosmi…

astro-ph.GA2014★ 26 cited

The Cepheid distance to the maser-host galaxy NGC 4258: Studying systematics with the Large Binocular Telescope

M. M. Fausnaugh, C. S. Kochanek, J. R. Gerke +3

We identify and phase a sample of 81 Cepheids in the maser-host galaxy NGC 4258 using the Large Binocular Telescope (LBT), and obtain calibrated mean magnitudes in up to 4 filters…