485 citations · 6.9k across the 247 of their papers we have counts for
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An alternate approach to measure specific star formation rates at 2<z<7
Iary Davidzon, Olivier Ilbert, Andreas L. Faisst +2
We trace the specific star formation rate (sSFR) of massive star-forming galaxies () from to 7. Our method is substantially different…
SPLASH-SXDF Multi-wavelength Photometric Catalog
Vihang Mehta, Claudia Scarlata, Peter Capak +19
We present a multi-wavelength catalog in the Subaru-XMM Deep Field (SXDF) as part of the Spitzer Large Area Survey with Hyper-Suprime-Cam (SPLASH). We include the newly acquired op…
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…
Empirical Modeling of the Redshift Evolution of the [NII]/H-ratio for Galaxy Redshift Surveys
Andreas L. Faisst, Daniel Masters, Yun Wang +4
We present an empirical parameterization of the [NII]/H flux ratio as a function of stellar mass and redshift valid at 0 < z < 2.7 and 8.5 < log(M) < 11.0. This description can…
Predicting Hα emission line galaxy counts for future galaxy redshift surveys
Alexander Merson, Yun Wang, Andrew Benson +4
Knowledge of the number density of H emitting galaxies is vital for assessing the scientific impact of the Euclid and WFIRST missions. In this work we present predictions from a…
Are high redshift Galaxies hot? - Temperature of z > 5 Galaxies and Implications on their Dust Properties
Andreas L. Faisst, Peter L. Capak, Lin Yan +6
Recent studies have found a significant evolution and scatter in the IRX- relation at z > 4, suggesting different dust properties of these galaxies. The total far-infrared (FIR)…