1k citations · 8.3k across the 79 of their papers we have counts for
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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…
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)…
The Complete Calibration of the Color-Redshift Relation (C3R2) Survey: Survey Overview and Data Release 1
Daniel Masters, Daniel Stern, Judith Cohen +4
A key goal of the Stage IV dark energy experiments Euclid, LSST and WFIRST is to measure the growth of structure with cosmic time from weak lensing analysis over large regions of t…
Evolution of Interstellar Medium, Star Formation, and Accretion at High Redshift
N. Scoville, N. Lee, P. Vanden Bout +20
ALMA observations of the long wavelength dust continuum are used to estimate the interstellar medium (ISM) masses in a sample of 708 galaxies at z = 0.3 to 4.5 in the COSMOS field.…