TY  - GEN
TI  - On the derivation of an X-ray temperature function without reference to mass and the prediction of weak-lensing number counts from the statistics of Gaussian random fields
Y1  - 2011///
UR  - https://archiv.ub.uni-heidelberg.de/volltextserver/12197/
ID  - heidok12197
KW  - Röntgenastronomie 
KW  -  kosmologische Parameter 
KW  -  analytische Methodencosmology 
KW  -  cosmological parameters 
KW  -  analytical methods 
KW  -  galaxy clusters 
KW  -  X-ray astronomy
N2  - We present a novel approach for the derivation of the X-ray temperature function for galaxy clusters, which is based on the statistics of Gaussian random fields applied to the cosmic gravitational potential. It invokes only locally defined quantities so that no reference to the cluster's mass is made. To relate linear and non-linear potential and to take into account only structures that have collapsed, we include either spherical- or ellipsoidal-collapse dynamics and compare both resulting models to temperature functions derived from a numerical simulation. Since deviations from the theoretical prediction are found in the simulation for high redshifts, we develop an analytic model to include the effects of mergers in our formalism. We jointly determine the cosmological parameters Omega_m0 and sigma_8 from two different cluster samples for different temperature definitions and find good agreement with constraints from WMAP5. Introducing theoretically a refined detection definition based on the upcrossing criterion, we reformulate our analytic approach for 2D and use it to predict the number density of spurious detections caused by large-scale structure and shot noise in filtered weak-lensing convergence maps. Agreement with a numerical simulation is found at the expected level.
A1  - Angrick, Christian
AV  - public
ER  -