1,456 datasets found

The Cluster Lensing And Supernova survey with Hubble (CLASH) Multi-Cycle Treasury program (PI: Marc Postman) completed its Hubble Space Telescope (HST) multiwavelength...

The Frontier Fields is a Spitzer and HST Director's Discretionary program of six deep fields centered on strong lensing galaxy clusters in parallel with six deep "blank fields"....

The Cluster Lensing And Supernova survey with Hubble (CLASH) is an HST Multi-Cycle Treasury program (PI: Marc Postman) to survey 25 massive galaxy clusters at 16 wavelengths...

The Spitzer Reionization Lensing Cluster Survey (SRELICS, PI: Bradac) is the Spitzer counterpart to the RELICS HST Treasury program (PI: Coe) to survey 41 massive galaxy clusters.

This is a deep optical mosaic of the Fornax cluster’s core, covering 1.6 square degrees. The data were acquired with ESO/MPG 2.2m/WFI, using a transparent filter that nearly...

150 lines of sight through the volume of a simulated galaxy cluster at z=0, produced by F.Vazza et al. running ENZO-MHD on the Jureca supercluster in Juelich. Each line is...

3D dimensional dataset (256^3 cells) in HDF5 format, of a high-resolution MHD cosmological simulations obtained with the ENZO code (Bryan et al. 2015). The data are mapped onto...

3D dimensional dataset (256^3 cells) in HDF5 format, of a high-resolution MHD cosmological simulations obtained with the ENZO code (Bryan et al. 2015), employing 4 or 5 levels...

The two .tar files contain maps along X,Y,Z of all M>10^13 Msol simulated galaxy clusters in the CUR1 box of Vazza et al. 2014...

3D dimensional dataset (256^3 cells) in HDF5 format, of a high-resolution MHD cosmological simulations obtained with the ENZO code (Bryan et al. 2015). The data are mapped onto...

3D dimensional dataset (256^3 cells) in HDF5 format, of a high-resolution MHD cosmological simulations obtained with the ENZO code (Bryan et al. 2015), employing 6 levels of...

The two .tar files contain maps along X,Y,Z of all M>10^13 Msol simulated galaxy clusters in the CUR1 box of Vazza et al. 2014...

Fits datacube of 256 x 256 pixels and 100 frequency channels, for the simulated synchrotron radio emission from a galaxy cluster at z=0.05. Each pixel is 34 kpc, and has values...

3-D distribution of gas density, dark matter density, temperature, and 3-components of velocity field for cluster IT90_0 (relaxed) at z=0, simulated with the ENZO code (Bryan...

Hdf5 monolitic 256^3 files for a simulated galaxy cluster at z=0, using with ENZO-AMR. The uniform resolution is 34kpc everywhere. The data belongs to the simulations by Vazza...

With the aim of distinguishing between possible physical mechanisms acting on galaxies when they fall into clusters, we study the properties of the gas and the stars in a sample...