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19992018
most citedExtremely compact massive galaxies at z~1.4

244 citations · 1.3k across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.GA2018★ 36 cited

The stellar populations of the central region of M31

R. P. Saglia, M. Opitsch, M. H. Fabricius +3

We continue the analysis of the dataset of our spectroscopic observation campaign of M31, by deriving simple stellar population properties (age metallicity and alpha-elements overa…

astro-ph2008★ 63 cited

First-Year Spectroscopy for the SDSS-II Supernova Survey

Chen Zheng, Roger W. Romani, Masao Sako +77

This paper presents spectroscopy of supernovae discovered in the first season of the Sloan Digital Sky Survey-II Supernova Survey. This program searches for and measures multi-band…

astro-ph2007★ 10 cited

The Munich Near-Infrared Cluster Survey (MUNICS) - IX. Galaxy Evolution to z ~ 2 From Optically Selected Catalogues

Georg Feulner, Yuliana Goranova, Ulrich Hopp +4

(Abridged) We present B, R, and I-band selected galaxy catalogues based on the Munich Near-Infrared Cluster Survey (MUNICS) which, together with the K-selected sample, serve as an…

astro-ph2006★ 151 cited

The Kormendy relation of massive elliptical galaxies at z~1.5. Evidence for size evolution ?

M. Longhetti, P. Saracco, P. Severgnini +6

We present the morphological analysis based on HST-NIC2 (0.075 arcsec/pixel) images in the F160W filter of a sample of 9 massive field (> 10^{11} M_\odot) galaxies spectroscopicall…

astro-ph2006★ 244 cited

Extremely compact massive galaxies at z~1.4

I. Trujillo, G. Feulner, Y. Goranova +9

The optical rest-frame sizes of 10 of the most massive (~5x10^{11}h_{70}^{-2}M_sun) galaxies found in the near-infrared MUNICS survey at 1.2<z<1.7 are analysed. Sizes were estimate…

astro-ph2005★ 65 cited

The evolution of the luminosity functions in the FORS Deep Field from low to high redshift: II. The red bands

A. Gabasch, U. Hopp, G. Feulner +12

We present the redshift evolution of the restframe galaxy luminosity function (LF) in the red r', i', and z' bands as derived from the FORS Deep Field (FDF). Using the deep and hom…