scholarly article | Q13442814 |
P819 | ADS bibcode | 2012A&A...539A.155M |
P818 | arXiv ID | 1202.0761 |
P356 | DOI | 10.1051/0004-6361/201118312 |
P5875 | ResearchGate publication ID | 221661802 |
P50 | author | Asantha Cooray | Q2866314 |
Reinhard Genzel | Q65807 | ||
James Scott Dunlop | Q24051741 | ||
Albrecht Poglitsch | Q30116440 | ||
Rob Ivison | Q44376416 | ||
David Elbaz | Q49693247 | ||
Douglas Scott | Q53953423 | ||
Roberto Maiolino | Q53953487 | ||
Georgios Magdis | Q56421223 | ||
Bruno Altieri | Q56421224 | ||
Duncan Farrah | Q58492776 | ||
Ian Smail | Q56547452 | ||
Emanuele Daddi | Q56547981 | ||
Helmut Dannerbauer | Q56549282 | ||
Matthieu Béthermin | Q56550610 | ||
Paola Santini | Q56550798 | ||
Giulia Rodighiero | Q56550799 | ||
Paola Andreani | Q58916811 | ||
Frank Bertoldi | Q59674796 | ||
Stefano Berta | Q59675173 | ||
Mara Salvato | Q59676296 | ||
Dieter Lutz | Q62520019 | ||
Peter Capak | Q62629908 | ||
Eduardo Ibar Plasser | Q63191748 | ||
A. M. Swinbank | Q56557116 | ||
Amélie Saintonge | Q56907097 | ||
Benjamin Magnelli | Q57079160 | ||
David Rosario | Q57430161 | ||
Hervé Aussel | Q58375065 | ||
Natascha M. Förster Schreiber | Q72044124 | ||
Emeric Le Floc'h | Q112583617 | ||
Francesca Pozzi | Q112767807 | ||
P2093 | author name string | L. Wang | |
L. J. Tacconi | |||
S. Chapman | |||
M. Albrecht | |||
J. Cepa | |||
S. J. Oliver | |||
A. Bongiovanni | |||
A. Cimatti | |||
A. L. R. Danielson | |||
H. S. Hwang | |||
I. Valtchanov | |||
E. Sturm | |||
P. Popesso | |||
L. Riguccini | |||
R. Nordon | |||
S. Wuyts | |||
I. Roseboom | |||
M. Sanchez-Portal | |||
A. Pérez García | |||
P2860 | cites work | The Multiband Imaging Photometer forSpitzer(MIPS) | Q55451216 |
High-redshift star formation in the Hubble Deep Field revealed by a submillimetre-wavelength survey | Q55883245 | ||
The nature of a gravitationally lensed submillimetre arc in MS0451.6−0305: two interacting galaxies at z∼ 2.9? | Q58489963 | ||
COLD GASS, an IRAM legacy survey of molecular gas in massive galaxies - II. The non-universality of the molecular gas depletion time-scale | Q58492533 | ||
Infrared Emission from Interstellar Dust. IV. The Silicate‐Graphite‐PAH Model in the Post‐SpitzerEra | Q58898193 | ||
Star formation and mass assembly in high redshift galaxies | Q58907872 | ||
The K20 survey. VI. The distribution of the stellar masses in galaxies up to z=~2 | Q58907971 | ||
Galaxy structure and mode of star formation in the SFR-mass plane from z ~ 2.5 to z ~ 0.1 | Q58908687 | ||
The star formation history of mass-selected galaxies in the COSMOS field | Q58908730 | ||
The VLA-COSMOS survey. IV. Deep data and joint catalog | Q58908793 | ||
The VLA-COSMOS perspective on the infrared-radio relation. I. New constraints on selection biases and the non-evolution of the Infrared/Radio properties of star-forming and active galactic nucleus galaxies at intermediate and high redshift | Q58908816 | ||
DEEPSPITZER24 μm COSMOS IMAGING. I. THE EVOLUTION OF LUMINOUS DUSTY GALAXIES—CONFRONTING THE MODELS | Q58908859 | ||
COSBO: The MAMBO 1.2 Millimeter Imaging Survey of the COSMOS Field | Q58908921 | ||
Multiwavelength Study of Massive Galaxies at z ∼ 2. II. Widespread Compton‐thick Active Galactic Nuclei and the Concurrent Growth of Black Holes and Bulges | Q58909663 | ||
Multiwavelength Study of Massive Galaxies at z∼2. I. Star Formation and Galaxy Growth | Q58909666 | ||
A 1200-μm MAMBO survey of the GOODS-N field: a significant population of submillimetre dropout galaxies | Q58909976 | ||
Star Formation in AEGIS Field Galaxies since z = 1.1: The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-forming Galaxies | Q58910042 | ||
The Hubble Deep Field North SCUBA Super-map - III. Optical and near-infrared properties of submillimetre galaxies | Q58910127 | ||
Can the faint submillimetre galaxies be explained in the Λ cold dark matter model? | Q58910144 | ||
The lesser role of starbursts in star formation at z = 2 | Q58910727 | ||
GMASS ultradeep spectroscopy of galaxies at z ~ 2 II. Superdense passive galaxies: how did they form and evolve? | Q58910766 | ||
Building the cosmic infrared background brick by brick with Herschel/PEP | Q58911970 | ||
PACS Evolutionary Probe (PEP) – A Herschel key program | Q58911973 | ||
Unveiling far-infrared counterparts of bright submillimeter galaxies using PACS imaging | Q58911991 | ||
Dissecting the cosmic infra-red background with Herschel/PEP | Q58911995 | ||
Far-infrared properties of submillimeter and optically faint radio galaxies | Q58911999 | ||
The first Herschel view of the mass-SFR link in high-z galaxies | Q58912008 | ||
The star-formation rates of 1.5 < z < 2.5 massive galaxies | Q58912010 | ||
Different star formation laws for disks versus starbursts at low and high redshifts | Q58912021 | ||
Imaging the molecular gas in a submillimeter galaxy at z = 4.05: cold mode accretion or a Major merger? | Q58912024 | ||
A CO emission line from the optical and near-IR undetected submillimeter galaxy GN10 | Q58912048 | ||
Two bright submillimeter galaxies in a z = 4.05 protocluster in GOODS-North, and accurate radio-infrared photometric redshifts | Q58912051 | ||
Vigorous Star Formation with Low Efficiency in Massive Disk Galaxies at z = 1.5 | Q58912065 | ||
The reversal of the star formation-density relation in the distant universe | Q58912075 | ||
The Hubble Deep Field-North SCUBA Super-map - IV. Characterizing submillimetre galaxies using deep Spitzer imaging | Q58912084 | ||
Evidence for a Population of High‐Redshift Submillimeter Galaxies from Interferometric Imaging | Q58916059 | ||
A Monte Carlo approach to evolution of the far-infrared luminosity function with BLAST | Q58916383 | ||
Herschel-SPIRE, far-infrared properties of millimetre-bright and -faint radio galaxies | Q58916426 | ||
On the X-ray properties of sub-mm-selected galaxies | Q58916440 | ||
Mid‐Infrared Spectral Diagnosis of Submillimeter Galaxies | Q58916502 | ||
The Hubble Deep Field North SCUBA Super-map - I. Submillimetre maps, sources and number counts | Q58916556 | ||
Submillimetre sources in rich cluster fields: source counts, redshift estimates and cooling flow limits | Q58916573 | ||
SCUBA: a common-user submillimetre camera operating on the James Clerk Maxwell Telescope | Q56485793 | ||
TheHerschel-SPIRE instrument and its in-flight performance | Q56506362 | ||
A joint analysis of BLAST 250-500 μm and LABOCA 870 μm observations in the Extended Chandra Deep Field-South | Q56551095 | ||
Luminous starbursts in the redshift desert at z∼ 1-2: star formation rates, masses and evidence for outflows | Q56551299 | ||
Molecular gas in submillimetre-faint, star-forming ultraluminous galaxies at z > 1 | Q56551385 | ||
On the evolution of the molecular gas fraction of star-forming galaxies | Q56551468 | ||
The stellar mass content of submillimeter-selected galaxies | Q56551960 | ||
The LABOCA survey of the Extended Chandra Deep Field-South - radio and mid-infrared counterparts to submillimetre galaxies | Q56552002 | ||
The potential influence of far-infrared emission lines on the selection of high-redshift galaxies | Q56552347 | ||
AzTEC half square degree survey of the SHADES fields â I. Maps, catalogues and source counts | Q56553142 | ||
BLAST: the far-infrared/radio correlation in distant galaxies | Q56553249 | ||
Deep multi-frequency radio imaging in the Lockman Hole — II. The spectral index of submillimetre galaxies | Q56553484 | ||
The Photodetector Array Camera and Spectrometer (PACS) on the HerschelSpace Observatory | Q56553510 | ||
Mid-infrared spectroscopy of candidate active galactic nuclei-dominated submillimeter galaxies | Q56554006 | ||
Most submillimeter galaxies are major mergers | Q56554092 | ||
A mid-infrared imaging survey of submillimeter-selected galaxies with the Spitzer Space Telescope | Q56555430 | ||
Confirming a population of hot-dust dominated, star-forming, ultraluminous galaxies at high redshift | Q56555820 | ||
Mid-infrared spectroscopy of submillimeter galaxies: extended star formation in massive high-redshift galaxies | Q56555870 | ||
The Large Apex BOlometer Camera survey of the Extended Chandra Deep Field South | Q56555921 | ||
Submillimeter Galaxies atz∼ 2: Evidence for Major Mergers and Constraints on Lifetimes, IMF, and CO‐H2Conversion Factor | Q56556101 | ||
The properties of submm galaxies in hierarchical models | Q56556194 | ||
Mid-Infrared Spectroscopy of High-Redshift Submillimeter Galaxies: First Results | Q56556322 | ||
The SCUBA HAlf Degree Extragalactic Survey - III. Identification of radio and mid-infrared counterparts to submillimetre galaxies | Q56556406 | ||
An ultradeep submillimetre map: beneath the SCUBA confusion limit with lensing and robust source extraction | Q56556538 | ||
High‐Resolution Millimeter Imaging of Submillimeter Galaxies | Q56556598 | ||
SHARC‐2 350 μm Observations of Distant Submillimeter‐selected Galaxies | Q56556650 | ||
The SCUBA Half-Degree Extragalactic Survey - II. Submillimetre maps, catalogue and number counts | Q56556702 | ||
The link between submillimetre galaxies and luminous ellipticals: near-infrared IFU spectroscopy of submillimetre galaxies | Q56556722 | ||
First redshift determination of an optically/ultraviolet faint submillimeter galaxy using CO emission lines | Q58922276 | ||
The VLA 1.4 GHz Survey of the Extended Chandra Deep Field–South: First Data Release | Q58923594 | ||
Cold streams in early massive hot haloes as the main mode of galaxy formation | Q59069187 | ||
The merger-driven evolution of warm infrared luminous galaxies | Q59710069 | ||
What does a submillimeter galaxy selection actually select? the dependence of submillimeter flux density on star formation rate and dust mass | Q59710073 | ||
Selection of ULIRGs in infrared and submm surveys | Q59713766 | ||
SpitzerMid‐ to Far‐Infrared Flux Densities of Distant Galaxies | Q59714176 | ||
The physical scale of the far-infrared emission in the most luminous submillimetre galaxies - II. Evidence for merger-driven star formation | Q59753513 | ||
The formation of high-redshift submillimetre galaxies | Q59783692 | ||
AzTEC millimetre survey of the COSMOS field – I. Data reduction and source catalogue | Q59787916 | ||
Balancing the energy budget between star formation and active galactic nuclei in high-redshift infrared luminous galaxies | Q59812749 | ||
The AzTEC mm-wavelength camera | Q59823079 | ||
The impact of cold gas accretion above a mass floor on galaxy scaling relations | Q59851173 | ||
Cosmic evolution of submillimeter galaxies and their contribution to stellar mass assembly | Q59942697 | ||
A Three‐dimensional Decomposition of the Infrared Emission from Dust in the Milky Way | Q59950866 | ||
SMA observations of GOODS 850-11 and GOODS 850-13: first examples of multiple submillimeter sources resolved by an interferometer | Q60028820 | ||
HerschelSpace Observatory | Q60306078 | ||
Physical conditions in the interstellar medium of intensely star-forming galaxies at redshift~2 | Q63370677 | ||
The Canada-United Kingdom deep submillimeter survey. II. First identifications, redshifts, and implications for galaxy evolution | Q66470360 | ||
A Redshift Survey of the Submillimeter Galaxy Population | Q56556773 | ||
The X‐Ray Spectral Properties of SCUBA Galaxies | Q56557108 | ||
A multiply imaged, submillimetre-selected ultraluminous infrared galaxy in a galaxy group atz∼ 2.5 | Q56557160 | ||
A Population of Hot, Dusty Ultraluminous Galaxies atz≈ 2 | Q56557179 | ||
Near-Infrared Colors of Submillimeter-selected Galaxies | Q56557279 | ||
The Rest‐Frame Optical Spectra of SCUBA Galaxies | Q56557348 | ||
Deep radio imaging of the SCUBA 8-mJy survey fields: submillimetre source identifications and redshift distribution | Q56557762 | ||
Submillimeter galaxies | Q56557950 | ||
The nature of faint submillimetre-selected galaxies | Q56558059 | ||
Radio Constraints on the Identifications and Redshifts of Submillimeter Galaxies | Q56558667 | ||
The diversity of SCUBA-selected galaxies | Q56558735 | ||
Redshift Distribution of the Faint Submillimeter Galaxy Population | Q56558909 | ||
A hyperluminous galaxy at z = 2.8 found in a deep submillimetre survey | Q56559164 | ||
A Deep Submillimeter Survey of Lensing Clusters: A New Window on Galaxy Formation and Evolution | Q56559432 | ||
Evolution of dust temperature of galaxies through cosmic time as seen by Herschel | Q56583655 | ||
HerMES: The SPIRE confusion limit | Q56584847 | ||
Herschel unveils a puzzling uniformity of distant dusty galaxies | Q56585269 | ||
The Herschel Multi-Tiered Extragalactic Survey: source extraction and cross-identifications in confusion-dominated SPIRE images | Q56586238 | ||
The far-infrared/radio correlation as probed by Herschel | Q56586358 | ||
A study of the gas-star formation relation over cosmic time | Q56915230 | ||
High molecular gas fractions in normal massive star-forming galaxies in the young Universe | Q56915386 | ||
An AzTEC 1.1 mm survey of the GOODS-N field - II. Multiwavelength identifications and redshift distribution | Q57088427 | ||
An AzTEC 1.1 mm survey of the GOODS-N field - I. Maps, catalogue and source statistics | Q57088432 | ||
The SCUBA HAlf Degree Extragalactic Survey (SHADES) – VII. Optical/IR photometry and stellar masses of submillimetre galaxies | Q57088435 | ||
Planck early results. XVI. The Planck view of nearby galaxies | Q57549175 | ||
High-resolution radio observations of submillimetre galaxies | Q57640584 | ||
A catalogue of Jy radio sources in northern legacy fields | Q57640601 | ||
GOODS–Herschel: an infrared main sequence for star-forming galaxies | Q57710922 | ||
THE zCOSMOS-SINFONI PROJECT. I. SAMPLE SELECTION AND NATURAL-SEEING OBSERVATIONS | Q58035554 | ||
The effect of Line-of-Sight temperature variation and noise on dust continuum observations | Q58049653 | ||
The impact of evolving infrared spectral energy distributions of galaxies on star formation rate estimates | Q58217207 | ||
Herschel reveals a Tdust-unbiased selection of z∼ 2 ultraluminous infrared galaxies | Q58217281 | ||
Far-infrared properties of Spitzer-selected luminous starbursts | Q58217367 | ||
Star formation and dust obscuration at z {approx} 2: galaxies at the dawn of downsizing | Q58489833 | ||
Mid‐Infrared Spectroscopy of Lensed Galaxies at 1 Q58489855 | | ||
Probing the submillimetre number counts at f850 μm< 2 mJy | Q58489864 | ||
Galaxy-galaxy gravitational lensing in the millimetre /submillimetre waveband | Q68268226 | ||
The infrared spectral energy distribution of normal star-forming galaxies | Q68291251 | ||
Properties of millimeter galaxies: constraints from K-band blank fields | Q68335554 | ||
The spectral distribution of normal star-forming galaxies: calibration at far-infrared and submillimeter wavelengths | Q68338876 | ||
The galactic disk mass function: reconciliation of the Hubble Space Telescope and nearby determinations | Q68348812 | ||
IRAS observations of galaxies in the Virgo cluster area | Q68396561 | ||
The evolution of cluster radio galaxies from z = 0 to z = 0.8 | Q68429149 | ||
Mapping the evolution of high-redshift dusty galaxies with submillimeter observations of a radio-selected sample | Q68429995 | ||
Strong dusty bursts of star formation in galaxies falling into the cluster RX J0152.7-1357 | Q68465815 | ||
A mid-infrared spectroscopic study of submillimeter galaxies: luminous starbursts at high redshift | Q68467087 | ||
IR observations of MS 1054-03: star formation and its evolution in rich galaxy clusters | Q68467873 | ||
Far-infrared spectral energy distributions and photometric redshifts of dusty galaxies | Q68483160 | ||
An evolutionary model for submillimeter galaxies | Q68484610 | ||
Luminous infrared galaxies with the submillimeter array. II. Comparing the CO (3-2) sizes and luminosities of local and high-redshift luminous infrared galaxies | Q68487075 | ||
Constraints on the relationship between stellar mass and halo mass at low and high redshift | Q68491610 | ||
Submillimetre-wavelength detection of dusty star-forming galaxies at high redshift | Q68631207 | ||
The 0.4 < z < 1.3 star formation history of the universe as viewed in the far-infrared | Q68675402 | ||
The SCUBA Local Universe Galaxy Survey - II. 450-{mu}m data: evidence for cold dust in bright IRAS galaxies | Q68697911 | ||
SCUBA observations of galaxies with metallicity measurements: a new method for determining the relation between submillimetre luminosity and dust mass | Q68700336 | ||
Submillimetre and far-infrared spectral energy distributions of galaxies: the luminosity-temperature relation and consequences for photometric redshifts | Q68701346 | ||
A census of metals at high and low redshift and the connection between submillimetre sources and spheroid formation | Q68702423 | ||
Stellar population synthesis at the resolution of 2003 | Q68703757 | ||
A 1200-{mu}m MAMBO survey of ELAISN2 and the Lockman Hole - I. Maps, sources and number counts | Q68707311 | ||
High-resolution studies of radio sources in the Hubble Deep and flanking fields | Q68708877 | ||
The Parkes selected regions : powerful radio galaxies and quasars at high redshifts | Q68804475 | ||
Inverse temperature dependence of the dust submillimeter spectral index | Q68845807 | ||
The radio-to-submillimeter spectral index as a redshift indicator | Q68871637 | ||
Interpreting the cosmic infrared background: constraints on the evolution of the dust-enshrouded star formation rate | Q68879509 | ||
The bivariate luminosity-color distribution of IRAS galaxies and implications for the high-redshift universe | Q68884815 | ||
Mid-infrared spectroscopy of two luminous submillimeter galaxies at {\em z} ~ 2.8 | Q68890660 | ||
Very Large Array 1.4 GHz observations of the GOODS-North field: data reduction and analysis | Q68955566 | ||
The submillimetre properties of ultraluminous infrared galaxies | Q68990268 | ||
Evolution of the dusty infrared luminosity function from z=0. to z=2.3 using observations from Spitzer | Q68997723 | ||
Galaxy evolution in cosmological simulations with outflows -- II. Metallicities and gas fractions | Q69020635 | ||
P407 | language of work or name | English | Q1860 |
P304 | page(s) | 155–155 | |
P577 | publication date | 2012-03-01 | |
P1433 | published in | Astronomy and Astrophysics | Q752075 |
P1476 | title | A Herschel view of the far-infrared properties of submillimetre galaxies | |
P478 | volume | 539 |
Q58910645 | (Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies. II. The spatial extent of the radio-emitting regions |
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Q58898112 | Calibration of the total infrared luminosity of nearby galaxies from Spitzer and Herschel bands |
Q58911782 | Characterizing elusive, faint dusty star-forming galaxies: a lensed, optically undetected ALMA galaxy atz ~ 3.3 |
Q56914358 | Combined CO and dust scaling relations of depletion time and molecular gas fractions with cosmic time, specific star-formation rate, and stellar mass |
Q58911853 | Dust and gas in luminous proto-cluster galaxies at z = 4.05: the case for different cosmic dust evolution in normal and starburst galaxies |
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Q56550131 | Early Science with the Large Millimeter Telescope: observations of dust continuum and CO emission lines of cluster-lensed submillimetre galaxies atz=2.0–4.7 |
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Q58908689 | Herschelobservations of gamma-ray burst host galaxies: implications for the topology of the dusty interstellar medium |
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Q56550172 | Mapping the dynamics of a giant Ly α halo at z = 4.1 with MUSE: the energetics of a large-scale AGN-driven outflow around a massive, high-redshift galaxy |
Q68688044 | Measures of galaxy dust and gas mass with Herschel photometry and prospects for ALMA |
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Q57633598 | Planck intermediate results XXXIX. The Planck list of high-redshift source candidates |
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Q57640483 | Strongly star-forming rotating disks in a complex merging system atz= 4.7 as revealed by ALMA |
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Q69058854 | Validation of the equilibrium model for galaxy evolution to z ~ 3 through molecular gas and dust observations of lensed star-forming galaxies |
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