activity
20132016
most citedALMA redshifts of millimeter-selected galaxies from the SPT survey: The redshift distribution of dusty star-forming galaxies

295 citations · 1.1k across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2016★ 11 cited

Early Quenching of Massive Protocluster Galaxies Around z=2.2 Radio Galaxies

Kate Husband, Malcolm N. Bremer, John P. Stott +1

Radio galaxies are among the most massive galaxies in the high redshift universe and are known to often lie in protocluster environments. We have studied the fields of seven z = 2.…

astro-ph.CO2015★ 272 cited

The XXL Survey: I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme

M. Pierre, F. Pacaud, C. Adami +89

We present the XXL Survey, the largest XMM programme totaling some 6.9 Ms to date and involving an international consortium of roughly 100 members. The XXL Survey covers two extrag…

astro-ph.GA2015★ 19 cited

Dissecting the complex environment of a distant quasar with MUSE

K. Husband, M. N. Bremer, E. R. Stanway +1

High redshift quasars can be used to trace the early growth of massive galaxies and may be triggered by galaxy-galaxy interactions. We present MUSE science verification data on one…

astro-ph.GA2015★ 170 cited

The nature of the [CII] emission in dusty star-forming galaxies from the SPT survey

Bitten Gullberg, Carlos De Breuck, Joaquin Vieira +24

We present [CII] observations of 20 strongly lensed dusty star forming galaxies at 2.1 < z < 5.7 using APEX and Herschel. The sources were selected on their 1.4 mm flux (S_1.4mm >…

astro-ph.GA2014★ 144 cited

The Rest-Frame Submillimeter Spectrum of High-Redshift, Dusty, Star-Forming Galaxies

J. S. Spilker, D. P. Marrone, J. E. Aguirre +28

We present the average rest-frame spectrum of high-redshift dusty, star-forming galaxies from 250-770GHz. This spectrum was constructed by stacking ALMA 3mm spectra of 22 such sour…

astro-ph.CO2013★ 4 cited

Identifying clustering at high redshift through actively star-forming galaxies

L. J. M. Davies, M. N. Bremer, E. R. Stanway +3

Identifying galaxy clustering at high redshift (i.e. z > 1) is essential to our understanding of the current cosmological model. However, at increasing redshift, clusters evolve co…

astro-ph.CO2013★ 68 cited

Are z~5 QSOs found in the most massive high redshift over-densities?

K. Husband, M. N. Bremer, E. R. Stanway +3

Luminous high-redshift QSOs are thought to exist within the most massive dark matter haloes in the young Universe. As a consequence they are likely to be markers for biased, over-d…

astro-ph.CO2013★ 295 cited

ALMA redshifts of millimeter-selected galaxies from the SPT survey: The redshift distribution of dusty star-forming galaxies

A. Weiss, C. De Breuck, D. P. Marrone +64

Using the Atacama Large Millimeter/submillimeter Array (ALMA), we have conducted a blind redshift survey in the 3 mm atmospheric transmission window for 26 strongly lensd dusty sta…

astro-ph.CO2013★ 135 cited

ALMA Observations of SPT-Discovered, Strongly Lensed, Dusty, Star-Forming Galaxies

Y. D. Hezaveh, D. P. Marrone, C. D. Fassnacht +64

We present Atacama Large Millimeter/submillimeter Array (ALMA) 860 micrometer imaging of four high-redshift (z=2.8-5.7) dusty sources that were detected using the South Pole Telesc…