activity
19952023
most citedFirst-year Sloan Digital Sky Survey-II (SDSS-II) Supernova Results: Hubble Diagram and Cosmological Parameters

696 citations · 4.8k across the 98 of their papers we have counts for

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60 papers · 1 filter

astro-ph2008★ 66 cited

The comet 17P/Holmes 2007 outburst: the early motion of the outburst material

M. Montalto, A. Riffeser, U. Hopp +2

Context. On October 24, 2007 the periodic comet 17P/Holmes underwent an astonishing outburst that increased its apparent total brightness from magnitude V\sim17 up to V\sim2.5 in r…

astro-ph2007★ 23 cited

A deep i-selected multi-waveband galaxy catalogue in the COSMOS field

A. Gabasch, Y. Goranova, U. Hopp +2

In this paper we present a deep and homogeneous i-band selected multi-waveband catalogue in the COSMOS field covering an area of about 0.7 square-degree. Our catalogue with a forma…

astro-ph2007★ 8 cited

Photometric study of the IC 65 group of galaxies

J. Vennik, U. Hopp

We carry out a photometric study of a poor group of late-type galaxies around IC 65, with the aim: (a) to search for new dwarf members and to measure their photometric characterist…

astro-ph2006★ 14 cited

Integrated specific star formation rates of galaxies, groups, and clusters: A continuous upper limit with stellar mass?

Georg Feulner, Ulrich Hopp, Christine S. Botzler

Aims: We investigate the build-up of stellar mass through star formation in field galaxies, galaxy groups, and clusters in order to better understand the physical processes regulat…

astro-ph2006★ 66 cited

The evolution of the mass function split by morphology up to redshift 1 in the FORS Deep and the GOODS-S Fields

M. Pannella, U. Hopp, R. P. Saglia +5

We study the evolution of the stellar mass density for the separate families of bulge-dominated and disk-dominated galaxies over the redshift range 0.25 < z < 1.15. We derive quant…

astro-ph2006

Tracing the Mass-Assembly History of Galaxies with Deep Surveys

Georg Feulner, Armin Gabasch, Yuliana Goranova +2

We use the optical and near-infrared galaxy samples from the Munich Near-Infrared Cluster Survey (MUNICS), the FORS Deep Field (FDF) and GOODS-S to probe the stellar mass assembly…