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Major Merging History in CANDELS. I. Evolution of the Incidence of Massive Galaxy-Galaxy Pairs from z=3 to z~0
Kameswara Bharadwaj Mantha, Daniel H. McIntosh, Ryan Brennan +37
The rate of major galaxy-galaxy merging is theoretically predicted to steadily increase with redshift during the peak epoch of massive galaxy development (). We us…
Clumpy Galaxies in CANDELS. II. Physical Properties of UV-bright Clumps at
Yicheng Guo, Marc Rafelski, Eric F. Bell +20
Studying giant star-forming clumps in distant galaxies is important to understand galaxy formation and evolution. At present, however, observers and theorists have not reached a co…
FIGS -- Faint Infrared Grism Survey: Description and Data Reduction
Norbert Pirzkal, Sangeeta Malhotra, Russell E. Ryan +26
The Faint Infrared Grism Survey (FIGS) is a deep Hubble Space Telescope (HST) WFC3/IR (Wide Field Camera 3 Infrared) slitless spectroscopic survey of four deep fields. Two fields a…
The intrinsic characteristics of galaxies on the SFR-stellar mass plane at 1.2<z<4: I. the correlation between stellar age, central density and position relative to the main sequence
Bomee Lee, Mauro Giavalisco, Katherine Whitaker +12
We use the deep CANDELS observations in the GOODS North and South fields to revisit the correlations between stellar mass (), star--formation rate (SFR) and morphology, and to…