activity
20062011
most citedThe UDF05 Follow-up of the HUDF: I. The Faint-End Slope of the Lyman-Break Galaxy Population at z~5

103 citations · 438 across the 10 of their papers we have counts for

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astro-ph200821 cited

Where can we really find the First Stars' Remnants today?

M. Trenti, M. R. Santos, M. Stiavelli

A number of recent numerical investigations concluded that the remnants of rare structures formed at very high redshift, such as the very first stars and bright redshift z~6 QSOs,…

astro-ph200888 cited

The UDF05 Follow-up of the HUDF: II. Constraints on Reionization from z-dropout Galaxies

P. A. Oesch, C. M. Carollo, M. Stiavelli +12

[Abridged] We detect three (plus one less certain) z-dropout sources in two separate fields of our UDF05 HST NICMOS images. These z~7 Lyman-Break Galaxy (LBG) candidates allow us t…

astro-ph2007

The very first Pop III stars and their relation to bright z~6 quasars

M. Trenti, M. Stiavelli

We discuss the link between dark matter halos hosting the first PopIII stars formed at redshift z > 40 and the rare, massive, halos that are generally considered to host bright z~6…

astro-ph2007103 cited

The UDF05 Follow-up of the HUDF: I. The Faint-End Slope of the Lyman-Break Galaxy Population at z~5

P. A. Oesch, M. Stiavelli, C. M. Carollo +14

We present the UDF05 project, a HST Large Program of deep ACS (F606W, F775W, F850LP) and NICMOS (F110W, F160W) imaging of three fields, two of which coincide with the NICP1-4 NICMO…

astro-ph200730 cited

Distribution of the very first PopIII stars and their relation to bright z~6 quasars

M. Trenti, M. Stiavelli

We discuss the link between dark matter halos hosting the first PopIII stars and the rare, massive, halos that are generally considered to host bright quasars at high redshift z~6.…

astro-ph20063 cited

Dust absorption along the line of sight for high-redshift objects

M. Trenti, M. Stiavelli

We estimate the optical depth distribution of dust present in absorption systems along the line of sight of high redshift galaxies and the resulting reddening. We characterize the…