activity
20042026
most citedImproved constraints on dark energy from Chandra X-ray observations of the largest relaxed galaxy clusters

634 citations · 6.2k across the 103 of their papers we have counts for

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Showing 2017Show all

8 papers · 1 filter

astro-ph.CO2017★ 19 cited

The XXL Survey: XXIII. The Mass Scale of XXL Clusters from Ensemble Spectroscopy

A. Farahi, V. Guglielmo, A. E. Evrard +34

An X-ray survey with the XMM-Newton telescope, XMM-XXL, has identified hundreds of galaxy groups and clusters in two 25 deg fields. Combining spectroscopic and X-ray observatio…

astro-ph.IM2017★ 45 cited

Global 21-cm signal extraction from foreground and instrumental effects I: Pattern recognition framework for separation using training sets

Keith Tauscher, David Rapetti, Jack O. Burns +1

The sky-averaged (global) highly redshifted 21-cm spectrum from neutral hydrogen is expected to appear in the VHF range of MHz and its spectral shape and strength are…

astro-ph.CO2017★ 114 cited

Baryon Content in a Sample of 91 Galaxy Clusters Selected by the South Pole Telescope at 0.2 < z < 1.25

I. Chiu, J. J. Mohr, M. McDonald +89

We estimate total mass (), intracluster medium (ICM) mass () and stellar mass () in a Sunyaev-Zel'dovich effect (SZE) selected sample of 91 ga…

astro-ph.CO2017★ 99 cited

The Splashback Feature around DES Galaxy Clusters: Galaxy Density and Weak Lensing Profiles

C. Chang, E. Baxter, B. Jain +82

Splashback refers to the process of matter that is accreting onto a dark matter halo reaching its first orbital apocenter and turning around in its orbit. The cluster-centric radiu…

astro-ph.CO2017★ 50 cited

A Measurement of CMB Cluster Lensing with SPT and DES Year 1 Data

E. J. Baxter, S. Raghunathan, T. M. Crawford +118

Clusters of galaxies gravitationally lens the cosmic microwave background (CMB) radiation, resulting in a distinct imprint in the CMB on arcminute scales. Measurement of this effec…

astro-ph.IM2017★ 58 cited

A Space-Based Observational Strategy for Characterizing the First Stars and Galaxies Using the Redshifted 21-cm Global Spectrum

Jack O. Burns, Richard Bradley, Keith Tauscher +19

The redshifted 21-cm monopole is expected to be a powerful probe of the epoch of the first stars and galaxies (). The global 21-cm signal is sensitive to the thermal and i…