output
19942026
Showing 2017 · astro-ph.GAShow all

27 papers · 2 filters

astro-ph.GA2017★ 88 cited

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…

astro-ph.GA2017★ 33 cited

Group quenching and galactic conformity at low redshift

M. Treyer, K. Kraljic, S. Arnouts +13

We quantify the quenching impact of the group environment using the spectroscopic survey Galaxy and Mass Assembly (GAMA) to z=0.2. The fraction of red (quiescent) galaxies, whether…

astro-ph.GA2017★ 258 cited

Galaxy And Mass Assembly (GAMA): the G02 field, Herschel-ATLAS target selection and Data Release 3

I. K. Baldry, J. Liske, M. J. I. Brown +39

We describe data release 3 (DR3) of the Galaxy And Mass Assembly (GAMA) survey. The GAMA survey is a spectroscopic redshift and multi-wavelength photometric survey in three equator…

astro-ph.GA2017★ 39 cited

Simulating and interpreting deep observations in the Hubble Ultra Deep Field with the JWST/NIRSpec low-resolution 'prism'

Jacopo Chevallard, Emma Curtis-Lake, Stephane Charlot +16

The James Webb Space Telescope (JWST) will enable the detection of optical emission lines in galaxies spanning a broad range of luminosities out to redshifts z>10. Measurements of…

astro-ph.GA2017★ 126 cited

SILVERRUSH. V. Census of Lya, [OIII]5007, Ha, and [CII]158um Line Emission with ~1000 LAEs at z=4.9-7.0 Revealed with Subaru/HSC

Yuichi Harikane, Masami Ouchi, Takatoshi Shibuya +23

We investigate Lya, [OIII]5007, Ha, and [CII]158um emission from 1124 galaxies at z=4.9-7.0. Our sample is composed of 1092 Lya emitters (LAEs) at z=4.9, 5.7, 6.6, and 7.0 identifi…

astro-ph.GA2017★ 87 cited

CANDELS: Elevated Black Hole Growth in the Progenitors of Compact Quiescent Galaxies at z~2

Dale D. Kocevski, Guillermo Barro, S. M. Faber +31

We examine the fraction of massive (), compact star-forming galaxies (cSFGs) that host an active galactic nucleus (AGN) at . These cSFGs are likely…