papers

Publications (7)

astro-ph.GA2023

Directly constraining the spatial coherence of the circumgalactic medium

A. Afruni, S. Lopez, P. Anshul +9

One of the biggest puzzles regarding the circumgalactic medium (CGM) is the structure of its cool ( K) gas phase. While the kinematics of quasar absorption systems sugge…

astro-ph.IM2010

ACTPol: A polarization-sensitive receiver for the Atacama Cosmology Telescope

M. D. Niemack, P. A. R. Ade, J. Aguirre +39

The six-meter Atacama Cosmology Telescope (ACT) in Chile was built to measure the cosmic microwave background (CMB) at arcminute angular scales. We are building a new polarization…

astro-ph.GA2021

Telltale signs of metal recycling in the circumgalactic medium of a galaxy

N. Tejos, S. López, C. Ledoux +15

We present gravitational-arc tomography of the cool-warm enriched circumgalactic medium (CGM) of an isolated galaxy (``G1'') at . Combining VLT/MUSE adaptive-optics…

astro-ph.GA2018

The ALMA Frontier Fields Survey - IV. Lensing-corrected 1.1 mm number counts in Abell 2744, MACSJ0416.1-2403 and MACSJ1149.5+2223

A. M. Muñoz Arancibia, J. González-López, E. Ibar +15

[abridged] Characterizing the number counts of faint, dusty star-forming galaxies is currently a challenge even for deep, high-resolution observations in the FIR-to-mm regime. They…

astro-ph.CO2013

Larger sizes of massive quiescent early-type galaxies in clusters than in the field at 0.8 < z < 1.5

L. Delaye, M. Huertas-Company, S. Mei +13

[abridged] The mass-size relation of early-type galaxies (ETGs) has been largely studied in the last years to probe the mass assembly of the most massive objects in the Universe. I…

astro-ph.CO2011

Scaling Relations and Overabundance of Massive Clusters at z>~1 from Weak-Lensing Studies with HST

M. J. Jee, K. S. Dawson, H. Hoekstra +22

We present weak gravitational lensing analysis of 22 high-redshift (z >~1) clusters based on Hubble Space Telescope images. Most clusters in our sample provide significant lensing…

astro-ph.GA2024

A lack of LAEs within 5Mpc of a luminous quasar in an overdensity at z=6.9: potential evidence of quasar negative feedback at protocluster scales

Trystan S. Lambert, R. J. Assef, C. Mazzucchelli +13

High-redshift quasars are thought to live in the densest regions of space which should be made evident by an overdensity of galaxies around them. However, campaigns to identify the…