activity
20002023
most citedThe wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation

211 citations · 2.8k across the 74 of their papers we have counts for

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Showing 2015Show all

6 papers · 1 filter

astro-ph.GA2015★ 41 cited

Early Science with the Large Millimeter Telescope: COOL BUDHIES I - a pilot study of molecular and atomic gas at z~0.2

Ryan Cybulski, Min S. Yun, Neal Erickson +20

An understanding of the mass build-up in galaxies over time necessitates tracing the evolution of cold gas (molecular and atomic) in galaxies. To that end, we have conducted a pilo…

astro-ph.GA2015★ 13 cited

Shapley Supercluster Survey: Construction of the Photometric Catalogues and i-band Data Release

A. Mercurio, P. Merluzzi, G. Busarello +10

The Shapley Supercluster Survey is a multi-wavelength survey covering an area of ~23 deg^2 (~260 Mpc^2 at z=0.048) around the supercluster core, including nine Abell and two poor c…

astro-ph.GA2015★ 33 cited

A Herschel Study of 24 micron-Selected AGNs and Their Host Galaxies

Lei Xu, G. H. Rieke, E. Egami +3

We present a sample of 290 24-micron-selected active galactic nuclei (AGNs) mostly at z ~ 0.3 -- 2.5, within 5.2 square degrees distributed as 25' X 25' fields around each of 30 ga…

astro-ph.GA2015★ 49 cited

The Relation between Luminous AGNs and Star Formation in Their Host Galaxies

Lei Xu, G. H. Rieke, E. Egami +3

We study the relation of active galactic nuclei (AGNs) to star formation in their host galaxies. Our sample includes 205 Type-1 and 85 Type-2 AGNs, 162 detected with Herschel, from…

astro-ph.GA2015★ 16 cited

LoCuSS: Exploring the selection of faint blue background galaxies for cluster weak-lensing

Felicia Ziparo, Graham P. Smith, Nobuhiro Okabe +3

Cosmological constraints from galaxy clusters rely on accurate measurements of the mass and internal structure of clusters. An important source of systematic uncertainty in cluster…

astro-ph.GA2015★ 13 cited

GLACE survey: OSIRIS/GTC Tuneable Filter H imaging of the rich galaxy cluster ZwCl 0024.0+1652 at z = 0.395. Part I -- Survey presentation, TF data reduction techniques and catalogue

Miguel Sánchez-Portal, Irene Pintos-Castro, Ricardo Pérez-Martínez +35

The cores of clusters at 0 z 1 are dominated by quiescent early-type galaxies, whereas the field is dominated by star-forming late-type ones. Galaxy propertie…