Add to ORKGWe perform a joint analysis of X-ray and Sunyaev-Zel'dovich effect data using an analytic model that describes the gas properties of galaxy clusters. The joint analysis allows the measurement of the cluster gas mass fraction profile and Hubble constant independent of cosmological parameters. Weak cosmological priors are used to calculate the overdensity radius within which the gas mass fractions are reported. Such an analysis can provide direct constraints on the evolution of the cluster gas mass fraction with redshift. We validate the model and the joint analysis on high signal-to-noise data from the Chandra X-ray Observatory and the Sunyaev-Zel'dovich Array for two clusters, A2631 and A2204
We report measurements of the Sunyaev-Zel'dovich (SZ) effect in three high-redshift (0.89 ≤ z ≤ 1.03...
We present a technique to constrain galaxy cluster pressure profiles by jointly fitting Sunyaev-Zeld...
We present two non-parametric deprojection methods aimed at recovering the three-dimensional density...
We perform a joint analysis of X-ray and Sunyaev-Zel'dovich effect data using an analytic model that...
Future data from galaxy redshift surveys, combined with high-resolutions maps of the cosmic microwav...
We provide a new framework for the joint analysis of cluster observations (JACO) using simultaneous ...
We have performed a combined analysis of X-ray and Sunyaev-Zel'dovich data in the direction of the d...
We present Sunyaev-Zel'dovich Effect (SZE) scaling relations for 38 massive galaxy clusters at redsh...
We present gas constraints from Sunyaev-Zel'dovich (SZ) effect measurements in a sample of 11 X-ray ...
We present gas mass fractions of 38 massive galaxy clusters spanning redshifts from 0.14 to 0.89, de...
Using sensitive centimeter-wave receivers mounted on the Owens Valley Radio Observatory and Berkeley...
We present Sunyaev-Zel'dovich Effect (SZE) scaling relations for 38 massive galaxy clusters at redsh...
We present an analysis of observations made with the Arcminute Microkelvin Imager (AMI) and the Cana...
We present gas mass fractions of 38 massive galaxy clusters at redshifts 0.14 ≤ z ≤ 0.89, derived fr...
We jointly analyse the Bolocam Sunyaev–Zel’dovich (SZ) effect and Chandra X-ray data for a set of 45...
We report measurements of the Sunyaev-Zel'dovich (SZ) effect in three high-redshift (0.89 ≤ z ≤ 1.03...
We present a technique to constrain galaxy cluster pressure profiles by jointly fitting Sunyaev-Zeld...
We present two non-parametric deprojection methods aimed at recovering the three-dimensional density...
We perform a joint analysis of X-ray and Sunyaev-Zel'dovich effect data using an analytic model that...
Future data from galaxy redshift surveys, combined with high-resolutions maps of the cosmic microwav...
We provide a new framework for the joint analysis of cluster observations (JACO) using simultaneous ...
We have performed a combined analysis of X-ray and Sunyaev-Zel'dovich data in the direction of the d...
We present Sunyaev-Zel'dovich Effect (SZE) scaling relations for 38 massive galaxy clusters at redsh...
We present gas constraints from Sunyaev-Zel'dovich (SZ) effect measurements in a sample of 11 X-ray ...
We present gas mass fractions of 38 massive galaxy clusters spanning redshifts from 0.14 to 0.89, de...
Using sensitive centimeter-wave receivers mounted on the Owens Valley Radio Observatory and Berkeley...
We present Sunyaev-Zel'dovich Effect (SZE) scaling relations for 38 massive galaxy clusters at redsh...
We present an analysis of observations made with the Arcminute Microkelvin Imager (AMI) and the Cana...
We present gas mass fractions of 38 massive galaxy clusters at redshifts 0.14 ≤ z ≤ 0.89, derived fr...
We jointly analyse the Bolocam Sunyaev–Zel’dovich (SZ) effect and Chandra X-ray data for a set of 45...
We report measurements of the Sunyaev-Zel'dovich (SZ) effect in three high-redshift (0.89 ≤ z ≤ 1.03...
We present a technique to constrain galaxy cluster pressure profiles by jointly fitting Sunyaev-Zeld...
We present two non-parametric deprojection methods aimed at recovering the three-dimensional density...