368 citations · 1.8k across the 43 of their papers we have counts for
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Cluster Cosmology Constraints from the 2500 deg SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope
S. Bocquet, J. P. Dietrich, T. Schrabback +77
We derive cosmological constraints using a galaxy cluster sample selected from the 2500~deg SPT-SZ survey. The sample spans the redshift range and contains 343 c…
A Detailed Study of the Most Relaxed SPT-Selected Galaxy Clusters: Cool Core and Central Galaxy Properties
M. McDonald, S. W. Allen, J. Hlavacek-Larrondo +14
We present a multi-wavelength analysis of the four most relaxed clusters in the South Pole Telescope 2500 deg^2 survey, which lie at 0.55 < z < 0.75. This study, which utilizes new…
Galaxy populations in the most distant SPT-SZ clusters - I. Environmental quenching in massive clusters at
V. Strazzullo, M. Pannella, J. J. Mohr +25
We present first results from a galaxy population study in the highest redshift galaxy clusters identified in the 2500 deg South Pole Telescope Sunyaev Zel'dovich effect (SPT-S…
X-ray Properties of SPT Selected Galaxy Clusters at 0.2<z<1.5 Observed with XMM-Newton
Esra Bulbul, I-Non Chiu, Joseph J. Mohr +22
We present measurements of the X-ray observables of the intra-cluster medium (ICM), including luminosity , ICM mass , emission-weighted mean temperature , and in…
Spectroscopic Confirmation of Five Galaxy Clusters at z > 1.25 in the 2500 sq. deg. SPT-SZ Survey
G. Khullar, L. E. Bleem, M. B. Bayliss +29
We present spectroscopic confirmation of five galaxy clusters at , discovered in the deg South Pole Telescope Sunyaev-Zel'dovich (SPT-SZ) surv…
CLUMP-3D. Testing CDM with galaxy cluster shapes
Mauro Sereno, Keiichi Umetsu, Stefano Ettori +5
The CDM model of structure formation makes strong predictions on concentration and shape of DM (dark matter) halos, which are determined by mass accretion processes. Comparison…