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2013ApJ...776...91L - Astrophys. J., 776, 91 (2013/October-3)
The contribution of halos with different mass ratios to the overall growth of cluster-sized halos.
LEMZE D., POSTMAN M., GENEL S., FORD H.C., BALESTRA I., DONAHUE M., KELSON D., NONINO M., MERCURIO A., BIVIANO A., ROSATI P., UMETSU K., SAND D., KOEKEMOER A., MENEGHETTI M., MELCHIOR P., NEWMAN A.B., BHATTI W.A., VOIT G.M., MEDEZINSKI E., ZITRIN A., ZHENG W., BROADHURST T., BARTELMANN M., BENITEZ N., BOUWENS R., BRADLEY L., COE D., GRAVES G., GRILLO C., INFANTE L., JIMENEZ-TEJA Y., JOUVEL S., LAHAV O., MAOZ D., MERTEN J., MOLINO A., MOUSTAKAS J., MOUSTAKAS L., OGAZ S., SCODEGGIO M. and SEITZ S.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): dark matter - galaxies: clusters: individual (Abell 611, Abell 963, Abell 1423, Abell 2261, MACS J1206.2-0848, RX J2129.7+0005, CL 2130.4-0000) - galaxies: kinematics and dynamics
VizieR on-line data: <Available at CDS (J/ApJ/776/91): table1.dat table2.dat>
Simbad objects: 1544