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20112025
most citedWide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report

1k citations · 8.3k across the 79 of their papers we have counts for

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Showing 2017 · astro-ph.GAShow all

6 papers · 2 filters

astro-ph.GA2017★ 52 cited

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…

astro-ph.GA2017★ 45 cited

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…

astro-ph.GA2017★ 44 cited

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…

astro-ph.GA2017★ 113 cited

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)…

astro-ph.GA2017★ 348 cited

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.…

astro-ph.GA2017★ 113 cited

The COSMOS2015 galaxy stellar mass function: 13 billion years of stellar mass assembly in 10 snapshots

I. Davidzon, O. Ilbert, C. Laigle +21

We measure the stellar mass function (SMF) of galaxies in the COSMOS field up to . We select them in the near-IR bands of the COSMOS2015 catalogue, which includes ultra-dee…