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arXiv · 1310.7582

Tracing the Mass Growth and Star Formation Rate Evolution of Massive Galaxies from z~6 to z~1 in the Hubble Ultra-Deep Field

Britt F. Lundgren·Pieter van Dokkum·Marijn Franx·Ivo Labbe·Michele Trenti·Rychard Bouwens·Valentino Gonzalez·Garth Illingworth·Daniel Magee·Pascal Oesch·Massimo Stiavelli
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Abstract

We present an analysis of $\sim$1500 H160-selected photometric galaxies detected to a limiting magnitude of 27.8 in the HUDF, using imaging from the HST WFC3/IR camera in combination with archival UV, optical, and NIR imaging. We fit photometric redshifts and stellar population estimates for all galaxies with well-determined Spitzer IRAC fluxes, allowing for the determination of the cumulative mass function within the range $1 4$.

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Britt F. Lundgren, Pieter van Dokkum, Marijn Franx, Ivo Labbe, Michele Trenti, Rychard Bouwens, Valentino Gonzalez, Garth Illingworth, Daniel Magee, Pascal Oesch, Massimo Stiavelli. 2013-10-28. Tracing the Mass Growth and Star Formation Rate Evolution of Massive Galaxies from z~6 to z~1 in the Hubble Ultra-Deep Field. https://doi.org/10.1088/0004-637x%2F780%2F1%2F34

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