854 citations · 7.6k across the 93 of their papers we have counts for
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Photometric redshifts for the CFHTLS-Wide
Fabrice Brimioulle, Michael Lerchster, Stella Seitz +2
We want to derive bias free, accurate photometric redshifts for those fields of the CFHTLS-Wide data which are covered in the u*, g', r', i' and z' filters and are public on Januar…
SDSS J120923.7+264047: A new massive galaxy cluster with a bright giant arc
Eran O. Ofek, Stella Seitz, Felix Klein
Highly magnified lensed galaxies allow us to probe the morphological and spectroscopic properties of high-redshift stellar systems in great detail. However, such objects are rare,…
Intense Star-formation and Feedback at High Redshift: Spatially-resolved Properties of the z=2.6 Submillimeter Galaxy SMMJ14011+0252
N. P. H. Nesvadba, M. D. Lehnert, R. Genzel +9
We present a detailed analysis of the spatially-resolved properties of the lensed submillimeter galaxy SMMJ14011+0252 at z=2.56, combining deep near-infrared integral-field data ob…
The Wendelstein Calar Alto Pixellensing Project (WeCAPP): The M31 Variable Star Catalogue
Juergen Fliri, Arno Riffeser, Stella Seitz +1
In this paper we present the WeCAPP variable star catalogue towards the bulge of M31. The observations of the WeCAPP microlensing survey (optical R and I bands) during three years…
The star formation rate history in the FORS Deep and GOODS South Fields
A. Gabasch, M. Salvato, R. P. Saglia +8
We measure the star formation rate (SFR) as a function of redshift z up to z \~4.5, based on B, I and (I+B) selected galaxy catalogues from the FORS Deep Field (FDF) and the K-sele…
The evolution of the luminosity functions in the FORS Deep Field from low to high redshift: I. The blue bands
A. Gabasch, R. Bender, S. Seitz +13
We use the very deep and homogeneous I-band selected dataset of the FORS Deep Field (FDF) to trace the evolution of the luminosity function over the redshift range 0.5 < z < 5.0. W…