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19962025
most citedPHIBSS: molecular gas content and scaling relations in z~1-3 normal star forming galaxies

948 citations · 18.1k across the 214 of their papers we have counts for

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66 papers · 1 filter

astro-ph.CO2020★ 34 cited

Close-up view of a luminous star-forming galaxy at z=2.95

S. Berta, A. J. Young, P. Cox +35

(Abridged) Exploiting the sensitivity and broad band width of NOEMA, we have studied the molecular gas and dust in the galaxy HerBS-89a, at z=2.95. High angular resolution images r…

astro-ph.CO2018★ 38 cited

Spitzer Planck Herschel Infrared Cluster (SPHerIC) survey: Candidate galaxy clusters at 1.3 < z < 3 selected by high star-formation rate

C. Martinache, A. Rettura, H. Dole +17

There is a lack of large samples of spectroscopically confirmed clusters and protoclusters at high redshifts, 1.5. Discovering and characterizing distant (proto-)clusters is im…

astro-ph.CO2013★ 208 cited

The suppression of star formation by powerful active galactic nuclei

M. J. Page, M. Symeonidis, J. D. Vieira +75

The old, red stars which constitute the bulges of galaxies, and the massive black holes at their centres, are the relics of a period in cosmic history when galaxies formed stars at…

astro-ph.CO2013★ 103 cited

[CII] and 12CO(1-0) Emission Maps in HLSJ091828.6+514223: A Strongly Lensed Interacting System at z=5.24

T. D. Rawle, E. Egami, R. S. Bussmann +25

We present Submillimeter Array (SMA) [CII] 158um and Jansky Very Large Array (JVLA) CO(1-0) line emission maps for the bright, lensed, submillimeter source at beh…

astro-ph.CO2013★ 36 cited

An extended Herschel drop-out source in the center of AS1063, a 'normal' dusty galaxy at z=6.1 or SZ substructures?

F. Boone, B. Clément, J. Richard +23

In the course of our 870um APEX/LABOCA follow up of the Herschel Lensing Survey we have detected a source in AS1063 (RXC J2248.7-4431), that has no counterparts in any of the Hersc…

astro-ph.CO2013★ 153 cited

The rapid assembly of an elliptical galaxy of 400 billion solar masses at a redshift of 2.3

Hai Fu, Asantha Cooray, C. Feruglio +41

Stellar archeology shows that massive elliptical galaxies today formed rapidly about ten billion years ago with star formation rates above several hundreds solar masses per year (M…

astro-ph.CO2013★ 609 cited

A Dust-Obscured Massive Maximum-Starburst Galaxy at a Redshift of 6.34

Dominik A. Riechers, C. M. Bradford, D. L. Clements +61

Massive present-day early-type (elliptical and lenticular) galaxies probably gained the bulk of their stellar mass and heavy elements through intense, dust-enshrouded starbursts -…

astro-ph.CO2013★ 154 cited

The Herschel census of infrared SEDs through cosmic time

Myrto Symeonidis, M. Vaccari, S. Berta +57

Using Herschel data from the deepest SPIRE and PACS surveys (HerMES and PEP) in COSMOS and GOODS (N+S), we examine the dust properties of IR-luminous (L_IR>10^10 L_sun) galaxies at…

astro-ph.CO2013★ 185 cited

Herschel-ATLAS: a binary HyLIRG pinpointing a cluster of starbursting proto-ellipticals

R. J. Ivison, A. M. Swinbank, Ian Smail +48

Panchromatic observations of the best candidate HyLIRG from the widest Herschel extragalactic imaging survey have led to the discovery of at least four intrinsically luminous z=2.4…

astro-ph.CO2013★ 393 cited

Star Formation and Gas Kinematics of Quasar Host Galaxies at z~6: New insights from ALMA

Ran Wang, Jeff Wagg, Chris L. Carilli +13

We present ALMA observations of the [C II] 158 micron fine structure line and dust continuum emission from the host galaxies of five redshift 6 quasars. We also report complementar…

astro-ph.CO2013★ 130 cited

Redshift 6.4 host galaxies of 10^8 solar mass black holes: low star formation rate and dynamical mass

Chris J. Willott, Alain Omont, Jacqueline Bergeron

We present ALMA observations of rest-frame far-infrared continuum and [CII] line emission in two z=6.4 quasars with black hole masses of ~10^8 M_sun. CFHQS J0210-0456 is detected i…

astro-ph.CO2013★ 31 cited

The Canada-France High-z Quasar Survey: 1.2mm Observations

A. Omont, C. J. Willott, A. Beelen +3

We report 250 GHz (1.2 mm) observations of a sample of 20 QSOs at redshifts 5.8<z<6.5 from the the Canada-France High-z Quasar Survey (CFHQS), using the Max-Planck Millimeter Bolom…

astro-ph.CO2012★ 948 cited

PHIBSS: molecular gas content and scaling relations in z~1-3 normal star forming galaxies

L. J. Tacconi, R. Neri, R. Genzel +21

We present PHIBSS, the IRAM Plateau de Bure high-z blue sequence CO 3-2 survey of the molecular gas properties in normal star forming galaxies (SFGs) near the cosmic star formation…

astro-ph.CO2012★ 1 cited

Star Formation in Quasar Host Galaxies at Redshift 6: Millimeter Surveys and New Insights from ALMA

Ran Wang, Jeff Wagg, Chris L. Carilli +9

We have been carrying out a systematic survey of the star formation and ISM properties in the host galaxies of z~6 quasars. Our 250 GHz observations, together with available data f…

astro-ph.CO2012★ 168 cited

HerMES: Cosmic Infrared Background Anisotropies and the Clustering of Dusty Star-Forming Galaxies

M. P. Viero, L. Wang, M. Zemcov +51

We present measurements of the auto- and cross-frequency power spectra of the cosmic infrared background (CIB) at 250, 350, and 500um (1200, 860, and 600 GHz) from observations tot…

astro-ph.CO2012★ 44 cited

BR1202-0725: An Extreme Multiple Merger at z = 4.7

P. Salome, M. Guelin, D. Downes +5

The radio-quiet quasar BR1202-0725 (z=4.695) is a remarkable source with a bright Northwest (NW) companion detected at submm and radio wavelengths but invisible in the optical. In…

astro-ph.CO2012★ 8 cited

Limits on dust emission from z~5 LBGs and their local environments

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

We present 1.2mm MAMBO-2 observations of a field which is over-dense in Lyman Break Galaxies (LBGs) at z~5. The field includes seven spectroscopically-confirmed LBGs contained with…

astro-ph.CO2012★ 37 cited

A Population of Dust-Rich Quasars at z ~ 1.5

Y. Sophia Dai, Jacqueline Bergeron, Martin Elvis +19

We report Herschel SPIRE (250, 350, and 500 micron) detections of 32 quasars with redshifts 0.5 < z < 3.6 from the Herschel Multi-tiered Extragalactic Survey. These sources are fro…

astro-ph.CO2012★ 180 cited

HerMES: Candidate Gravitationally Lensed Galaxies and Lensing Statistics at Submillimeter Wavelengths

Julie L. Wardlow, Asantha Cooray, Francesco De Bernardis +83

We present a list of 13 candidate gravitationally lensed submillimeter galaxies (SMGs) from 95 square degrees of the Herschel Multi-tiered Extragalactic Survey, a surface density o…

astro-ph.CO2012★ 40 cited

Ionized nitrogen at high redshift

R. Decarli, F. Walter, R. Neri +11

We present secure [NII[ detections in two mm-bright, strongly lensed objects at high redshift, APM08279+5255 (z=3.911) and MM18423+5938 (z=3.930), using the IRAM Plateau de Bure In…

astro-ph.CO2012★ 800 cited

The Herschel Multi-tiered Extragalactic Survey: HerMES

HerMES Collaboration, S. J. Oliver, J. Bock +102

The Herschel Multi-tiered Extragalactic Survey, HerMES, is a legacy program designed to map a set of nested fields totalling ~380 deg^2. Fields range in size from 0.01 to ~20 deg^2…

astro-ph.CO2012★ 220 cited

HerMES: deep number counts at 250, 350, and 500 microns in the COSMOS and GOODS-N fields and the build-up of the cosmic infrared background

M. Béthermin, E. Le Floc'h, O. Ilbert +58

ABRIGED Herschel/SPIRE has provided confusion limited maps of deep fields at 250, 350, and 500um, as part of the HerMES survey. Due to confusion, only a small fraction of the Cosmi…

astro-ph.CO2012★ 56 cited

Molecular Gas in Infrared Ultraluminous QSO Hosts

X. Y. Xia, Y. Gao, C. -N. Hao +6

We report CO detections in 17 out of 19 infrared ultraluminous QSO (IR QSO) hosts observed with the IRAM 30m telescope. The cold molecular gas reservoir in these objects is in a ra…

astro-ph.CO2011★ 113 cited

The Herschel Multi-Tiered Extragalactic Survey: SPIRE-mm Photometric Redshifts

I. G. Roseboom, R. J. Ivison, T. R. Greve +78

We investigate the potential of submm-mm and submm-mm-radio photometric redshifts using a sample of mm-selected sources as seen at 250, 350 and 500 μm by the SPIRE instrument on He…