Large scale Structures: catalogues
L3S delivers data and services on multiwavelength galaxy clusters, proto-clusters and galaxies. You can query the SZ cluster database (SZDB) to get properties from clusters observed by Planck, SPT, ACT, AMI, CARMA. You can provide a (list of) positions in the sky and find out if it matches with a known cluster, obtain stamped maps in SZ and Xray, and/or run a detection algorithm in Optical data with the MAGYC portal. Herschel cluster and proto-clusters observations are also availbale through the HESIOD database. Finally, GAL-P offers galaxy properties obtained with machine learning around your prefered sky position in our 3D visualisation of DTFE galaxy overdensity.