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20032007
most citedDynamical modelling of luminous and dark matter in 17 Coma early-type galaxies

190 citations · 353 across the 4 of their papers we have counts for

collaborators

8 papers

astro-ph2007190 cited

Dynamical modelling of luminous and dark matter in 17 Coma early-type galaxies

J. Thomas, R. P. Saglia, R. Bender +5

Dynamical models for 17 Coma early-type galaxies are presented. The galaxy sample consists of flattened, rotating as well as non-rotating early-types including cD and S0 galaxies w…

astro-ph200694 cited

X-ray monitoring of optical novae in M31 from July 2004 to February 2005

W. Pietsch, F. Haberl, G. Sala +9

Optical novae have recently been identified as the major class of supersoft X-ray sources in M31 based on ROSAT and early XMM-Newton and Chandra observations. This paper reports on…

astro-ph200639 cited

Lyman Break Galaxies Under a Microscope: The Small Scale Dynamics and Mass of an Arc in the Cluster 1E0657-56

N. P. H. Nesvadba, M. D. Lehnert, F. Eisenhauer +8

Using the near-infrared integral-field spectrograph SPIFFI on the VLT, we have studied the spatially-resolved dynamics in the z=3.2 strongly lensed galaxy 1E0657-56 ``arc+core''. T…

astro-ph200630 cited

Lyman-alpha emission galaxies at a redshift of z = 5.7 in the FORS Deep Field

C. Tapken, I. Appenzeller, A. Gabasch +7

We present the results of a search for Lyman-alpha emission galaxies at z~ 5.7 in the FORS Deep Field. The objective of this study is to improve the faint end of the luminosity fun…

astro-ph2005

Microlensing toward crowded fields: Theory and applications to M31

A. Riffeser, J. Fliri, S. Seitz +1

We present a comprehensive treatment of the pixel-lensing theory and apply it to lensing experiments and their results toward M31. Using distribution functions for the distances, v…

astro-ph2004

SPIFFI observations of the starburst SMMJ14011+0252: Already old, fat, and rich by z = 2.565

M. Tecza, A. J. Baker, R. I. Davies +10

Using the SPectrometer for Infrared Faint Field Imaging (SPIFFI) on the ESO VLT, we have obtained J, H, and K band integral field spectroscopy of the z = 2.565 luminous submillimet…