Bulk Flows

This project is devoted to measuring large scale bulk flows from cosmic microwave background radiation and X-ray cluster data. The method uses kinematic Sunyaev Zeldovich effect on known X-ray clusters. The project is supported by NASA grants (PI - A. Kashlinsky). The team includes A. Kashlinsky (Goddard) , F. Atrio-Barandela (Salamanca, Spain) and H. Ebeling (Hawaii, USA).

Site under construction.