activity
19992016
most citedThe Canadian Cluster Comparison Project: detailed study of systematics and updated weak lensing masses

411 citations · 4.2k across the 42 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

17 papers · 1 filter

astro-ph.CO2016★ 30 cited

Constraints on the Mass, Concentration, and Nonthermal Pressure Support of Six CLASH Clusters from a Joint Analysis of X-ray, SZ, and Lensing Data

Seth R. Siegel, Jack Sayers, Andisheh Mahdavi +17

We present a joint analysis of Chandra X-ray observations, Bolocam thermal Sunyaev-Zel'dovich (SZ) effect observations, Hubble Space Telescope (HST) strong lensing data, and HST an…

astro-ph.CO2015★ 411 cited

The Canadian Cluster Comparison Project: detailed study of systematics and updated weak lensing masses

Henk Hoekstra, Ricardo Herbonnet, Adam Muzzin +4

Masses of clusters of galaxies from weak gravitational lensing analyses of ever larger samples are increasingly used as the reference to which baryonic scaling relations are compar…

astro-ph.CO2014★ 1 cited

CFHTLenS: Weak lensing calibrated scaling relations for low mass clusters of galaxies

K. Kettula, S. Giodini, E. van Uitert +24

We present weak lensing and X-ray analysis of 12 low mass clusters from the CFHTLenS and XMM-CFHTLS surveys. We combine these systems with high-mass systems from CCCP and low-mass…

astro-ph.CO2014★ 17 cited

Scaling Relations and X-ray Properties of Moderate-Luminosity Galaxy Clusters from 0.3 < z < 0.6 with XMM-Newton

Thomas Connor, Megan Donahue, Ming Sun +4

We present new X-ray temperatures and improved X-ray luminosity estimates for 15 new and archival XMM-Newton observations of galaxy clusters at intermediate redshift with mass and…

astro-ph.CO2014★ 130 cited

CLASH-X: A Comparison of Lensing and X-ray Techniques for Measuring the Mass Profiles of Galaxy Clusters

Megan Donahue, G. Mark Voit, Andisheh Mahdavi +35

We present profiles of temperature (Tx), gas mass, and hydrostatic mass estimated from new and archival X-ray observations of CLASH clusters. We compare measurements derived from X…

astro-ph.CO2014★ 81 cited

Hubble Space Telescope/Advanced Camera for Surveys Confirmation of the Dark Substructure in A520

M. James Jee, Henk Hoekstra, Andisheh Mahdavi +1

We present the results from a weak gravitational lensing study of the merging cluster A520 based on the analysis of Hubble Space Telescope/Advanced Camera for Surveys (ACS) data. T…

astro-ph.CO2012★ 243 cited

Joint Analysis of Cluster Observations: II. Chandra/XMM-Newton X-ray and Weak Lensing Scaling Relations for a Sample of 50 Rich Clusters of Galaxies

A. Mahdavi, H. Hoekstra, A. Babul +3

We present a study of multiwavelength X-ray and weak lensing scaling relations for a sample of 50 clusters of galaxies. Our analysis combines Chandra and XMM-Newton data using an e…

astro-ph.CO2012★ 159 cited

The Canadian Cluster Comparison Project: weak lensing masses and SZ scaling relations

Henk Hoekstra, Andisheh Mahdavi, Arif Babul +1

The Canadian Cluster Comparison Project is a comprehensive multi-wavelength survey targeting 50 massive X-ray selected clusters of galaxies to examine baryonic tracers of cluster m…

astro-ph.CO2012★ 49 cited

A Giant Metrewave Radio Telescope/Chandra view of IRAS 09104+4109: A type 2 QSO in a cooling flow

Ewan O'Sullivan, Simona Giacintucci, Arif Babul +8

IRAS 09104+4109 is a rare example of a dust enshrouded type 2 QSO in the centre of a cool-core galaxy cluster. Previous observations of this z=0.44 system showed that as well as po…

astro-ph.CO2012★ 123 cited

CLASH: Mass Distribution in and around MACS J1206.2-0847 from a Full Cluster Lensing Analysis

Keiichi Umetsu, Elinor Medezinski, Mario Nonino +45

We derive an accurate mass distribution of the galaxy cluster MACS J1206.2-0847 (z=0.439) from a combined weak-lensing distortion, magnification, and strong-lensing analysis of wid…

astro-ph.CO2012★ 104 cited

A Study of the Dark Core in A520 with Hubble Space Telescope: The Mystery Deepens

M. J. Jee, A. Mahdavi, H. Hoekstra +4

We present a Hubble Space Telescope/Wide Field Planetary Camera 2 weak-lensing study of A520, where a previous analysis of ground-based data suggested the presence of a dark mass c…

astro-ph.CO2012★ 27 cited

Evolution of the Red Sequence Giant to Dwarf Ratio in Galaxy Clusters out to z ~ 0.5

C. Bildfell, H. Hoekstra, A. Babul +9

We analyze deep g' and r' band data of 97 galaxy clusters imaged with MegaCam on the Canada-France-Hawaii telescope. We compute the number of luminous (giant) and faint (dwarf) gal…

astro-ph.CO2012★ 157 cited

CLASH: Precise New Constraints on the Mass Profile of Abell 2261

Dan Coe, Keiichi Umetsu, Adi Zitrin +43

We precisely constrain the inner mass profile of Abell 2261 (z=0.225) for the first time and determine this cluster is not "over-concentrated" as found previously, implying a forma…

astro-ph.CO2011★ 46 cited

The Multi-Epoch Nearby Cluster Survey: type Ia supernova rate measurement in z~0.1 clusters and the late-time delay time distribution

David J. Sand, Melissa L. Graham, Chris Bildfell +8

We describe the Multi-Epoch Nearby Cluster Survey (MENeaCS), designed to measure the cluster Type Ia supernova (SN Ia) rate in a sample of 57 X-ray selected galaxy clusters, with r…

astro-ph.CO2011★ 8 cited

Model-Independent Limits on the Line-of-Sight Depth of Clusters of Galaxies Using X-ray and Sunyaev-Zel'dovich Data

A. Mahdavi, W. Chang

We derive a model-independent expression for the minimum line-of-sight extent of the hot plasma in a cluster of galaxies. The only inputs are the 1-5 keV X-ray surface brightness a…

astro-ph.CO2009★ 408 cited

The role of black holes in galaxy formation and evolution

A. Cattaneo, S. M. Faber, J. Binney +14

Virtually all massive galaxies, including our own, host central black holes ranging in mass from millions to billions of solar masses. The growth of these black holes releases vast…

astro-ph.CO2009★ 3 cited

The Evolution of Galaxy Clusters Across Cosmic Time

M. Arnaud, H. Bohringer, C. Jones +40

The large scale structure of the present Universe is determined by the growth of dark matter density fluctuations and by the dynamical action of dark energy and dark matter. While…