activity
20062015
most citedVariable VHE gamma-ray emission from Markarian 501

547 citations · 2.7k across the 22 of their papers we have counts for

collaborators

22 papers

astro-ph.CO2015★ 2 cited

Environment-based selection effects of Planck clusters

Ralf Kosyra, Daniel Gruen, Stella Seitz +5

We investigate whether the large scale structure environment of galaxy clusters imprints a selection bias on Sunyaev Zel'dovich (SZ) catalogs. Such a selection effect might be caus…

astro-ph.IM2014★ 27 cited

The 64 Mpixel wide field imager for the Wendelstein 2m Telescope: Design and Calibration

Ralf Kosyra, Claus Goessl, Ulrich Hopp +4

The Wendelstein Observatory of Ludwig Maximilians University of Munich has recently been upgraded with a modern 2m robotic telescope. One Nasmyth port of the telescope has been equ…

astro-ph.CO2013★ 119 cited

Weak lensing analysis of SZ-selected clusters of galaxies from the SPT and Planck surveys

D. Gruen, S. Seitz, F. Brimioulle +8

We present the weak lensing analysis of the Wide-Field Imager SZ Cluster of galaxy (WISCy) sample, a set of 12 clusters of galaxies selected for their Sunyaev-Zel'dovich (SZ) effec…

astro-ph2008★ 21 cited

MAGIC Observations of PG 1553+113 during a Multiwavelength Campaign in July 2006

MAGIC Collaboration, Albert

The active galactic nucleus PG 1553+113 was observed by the MAGIC telescope in July 2006 during a multiwavelength campaign, in which telescopes in the optical, X-ray, and very high…

astro-ph2008★ 84 cited

MAGIC observations of the unidentified TeV gamma-ray source TeV J2032+4130

J. Albert

We observed the first known very high energy (VHE) gamma-ray emitting unidentified source, TeV J2032+4130, for 94 hours with the MAGIC telescope. The source was detected with a sig…

astro-ph2008★ 100 cited

Simultaneous multiwavelength observations of the blazar 1ES1959+650 at a low TeV flux

G. Tagliaferri, L. Foschini, G. Ghisellini +7

We present the results from a multiwavelength campaign on the TeV blazar 1ES 1959+650, performed in May, 2006. Data from the optical, UV, soft- and hard-X-ray and very high energy…