881 citations
- D. Schaile11 profiles112 · h 87
- A. Quadt11 profiles95 · h 86
- N. Wermes9 profiles95 · h 88
- A. Harel11 profiles94 · h 107
- F. Fiedler4 profiles94 · h 87
- G. Wilson3 profiles94 · h 62
- P. Mättig12 profiles94 · h 88
- P. Renkel12 profiles94 · h 51
- R. Ströhmer11 profiles94 · h 93
- F. Guo6 profiles93 · h 49
- K. M. Chan2 profiles93
- M. Verzocchi14 profiles93 · h 86
- Joint Institute for Nuclear ResearchRU110 papers
- University of FreiburgDE108 papers
- Ludwig-Maximilians-Universität MünchenDE105 papers
- University of ArizonaUS104 papers
- Columbia UniversityUS103 papers
- Johannes Gutenberg University MainzDE103 papers
- University of Maryland, College ParkUS102 papers
- Charles UniversityCZ99 papers
- Princeton UniversityUS99 papers
- Fermi National Accelerator LaboratoryUS98 papers
- Lomonosov Moscow State UniversityRU98 papers
- University of ManchesterGB98 papers
36 papers · 1 filter
Weak lensing measurements of dark matter halos of galaxies from COMBO-17
M. Kleinheinrich, P. Schneider, H. -W. Rix +8
We present a measurement of mass estimates for dark matter halos around galaxies from the COMBO-17 survey using weak gravitational lensing. COMBO-17 is particularly useful for this…
Spectral projections for the twisted Laplacian
Herbert Koch, Fulvio Ricci
The twisted Laplacian in the d=2n dimensional Euclidean space has the spectrum n+2k, k a nonnegative integer. We find sharp asymptotic bounds of the norm of the projection to the e…
The galaxy-dark matter bias in the Garching-Bonn Deep Survey
Patrick Simon, Peter Schneider, Thomas Erben +3
We measured the bias and correlation factor of galaxies with respect to the dark matter using the aperture statistics including the aperture mass from weak gravitational lensing. T…
Bottom Up Meets Heterotic Strings
Stefan Forste, Akin Wingerter
In this talk we argue that a certain class of heterotic orbifolds can be the underlying fundamental theory for recently studied field theory GUTs. In addition we demonstrate that s…
IMF variations and their implications for Supernovae numbers
C. Weidner, P. Kroupa
The stellar initial mass function (IMF) integrated over an entire galaxy is an integral over all separate star-formation events. Since most stars form in star clusters with differe…
How star clusters could survive low star formation efficiencies
M. Fellhauer, P. Kroupa
After the stars of a new, embedded star cluster have formed they blow the remaining gas out of the cluster. Especially winds of high mass stars and definitely the on-set of the fir…