Dusty star forming galaxies at high redshift

Abstract

The global star formation rate in high redshift galaxies, based on optical surveys, shows a strong peak at a redshift of z=1.5, which implies that we have already seen most of the formation. High redshift galaxies may, however, emit most of their energy at submillimeter wavelengths if they contain substantial amounts of dust. The dust would absorb the starlight and reradiate it as far-infrared light, which would be redshifted to the submillimeter range. Here we report a deep survey of two blank regions of sky performed at submillimeter wavelengths (450 and 850-micron). If the sources we detect in the 850-micron band are powered by star formation, then each must be converting more than 100 solar masses of gas per year into stars, which is larger than the maximum star formation rates inferred for most optically-selected galaxies. The total amount of high redshift star formation is essentially fixed by the level of background light, but where the peak occurs in redshift for the submillimeter is not yet established. However, the background light contribution from only the sources detected at 850-micron is already comparable to that from the optically-selected sources. Establishing the main epoch of star formation will therefore require a combination of optical and submillimeter studies.

10 pages + 2 Postscript figures, under embargo at Nature

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• The e-MERLIN Galaxy Evolution Survey (e-MERGE): Overview and Survey Description
• Herschel-PACS observations of [OI]63um towards submillimetre galaxies at z~1
• SCUBA-2 Ultra Deep Imaging Eao Survey (Studies) III: Multi-wavelength properties, luminosity functions and preliminary source catalog of 450-$\mu$m-selected galaxies
• Tracing the evolution of dust-obscured activity using sub-millimetre galaxy populations from STUDIES and AS2UDS
• A machine-learning method for identifying multi-wavelength counterparts of submillimeter galaxies: training and testing using AS2UDS and ALESS
• A LABOCA survey of the Extended Chandra Deep Field South - submillimeter properties of near-IR selected galaxies
• Submillimeter observations of IC 10: the dust properties and neutral carbon content of a low metallicity starburst
• The European Large Area ISO Survey IV: the preliminary 90 micron luminosity function
• Millimetre observations of a sample of high-redshift obscured quasars
• A new look at local ultraluminous infrared galaxies: the atlas and radiative transfer models of their complex physics
• Theoretical predictions on the clustering of SCUBA galaxies and implications for small-scale fluctuations at sub-mm wavelengths
• HST Observations of the Host Galaxy of GRB970508
• Early Science with the Large Millimeter Telescope: Observations of dust continuum and CO emission lines of cluster-lensed submillimetre galaxies at z=2.0-4.7
• An ALMA survey of CO in submillimetre galaxies: companions, triggering, and the environment in blended sources
• The ALMA Frontier Fields Survey - II. Multiwavelength Photometric analysis of 1.1mm continuum sources in Abell 2744, MACSJ0416.1-2403 and MACSJ1149.5+2223
• Statistical lensing by galactic discs
• Impact of Future Submillimeter and Millimeter Large Facilities on the Studies of Galaxy Formation and Evolution
• Inverse stellar population age gradients of post-starburst galaxies at z=0.8 with LEGA-C
• Environment of MAMBO galaxies in the COSMOS field
• ALMACAL II: Extreme star-formation-rate densities in a pair of dusty starbursts at $z=3.442$ revealed by ALMA 20-milliarcsec resolution imaging
• A SCUBA-2 850 micron survey of protoplanetary discs in the sigma Orionis cluster
• An Evolutionary Paradigm for Dusty Active Galaxies at Low Redshift
• Submillimeter Galaxy Number Counts and Magnification by Galaxy Clusters
• Modeling of the HERMES J105751.1+573027 submillimeter source lensed by a dark matter dominated foreground group of galaxies
• The Infrared Properties of Submillimeter Galaxies: Clues From Ultra-Deep 70 Micron Imaging
• A deep 6.7um survey in the SSA13 field with ISO
• Mid-Infrared Identifications of SCUBA Galaxies in the CUDSS 14-Hour Field with the Spitzer Space Telescope
• Contribution of Lensed SCUBA Galaxies to the Cosmic Infrared Background
• Investigating the nature of the z~2.8 submillimeter selected galaxy SMM J02399-0136 with VLT spectropolarimetry
• Dust Emission from High Redshift QSOs
• A Ks and IRAC Selection of High-Redshift Extremely Red Objects
• Star formation properties of UCM galaxies
• Interferometric CO Observations of submillimeter-faint, radio-selected starburst galaxies at z~2
• Sub-millimeter detections of Spitzer Space Telescope galaxy populations
• Atacama Cosmology Telescope: Dusty star-forming galaxies and active galactic nuclei in the equatorial survey
• Blank field submm sources, failed stars, and the dark matter
• Collision-induced galaxy formation: semi-analytical model and multi-wavelength predictions
• An ALMA Survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS Field: The Far-infrared/Radio correlation for High-redshift Dusty Star-forming Galaxies
• A New interpretation of chain galaxies at high redshift
• An ALMA Spectroscopic Survey of the Brightest Submillimeter Galaxies in the SCUBA-2-COSMOS Field (AS2COSPEC): Physical Properties of z=2-5 Ultra- and Hyperluminous Infrared Galaxies
• Multi-wavelength properties of radio and machine-learning identified counterparts to submillimeter sources in S2COSMOS
• Unveiling the Nature of Submillimeter Galaxy SXDF850.6
• Millimetre/submillimetre-wave emission line searches for high-redshift galaxies
• The extraordinary mid-infrared spectral properties of FeLoBAL Quasars
• Identification of two bright z>3 submillimeter galaxy candidates in the COSMOS field
• The DEEP2 Redshift Survey: Lyman Alpha Emitters in the Spectroscopic Database
• Where are the Cosmic Metals at z~3?
• Studying clusters with Planck
• The Canada-UK Deep Submillimetre Survey VIII: Source Identifications in the 3-hour field
• Submillimetre galaxies in two massive protoclusters at z = 2.24: witnessing the enrichment of extreme starbursts in the outskirts of HAE density peaks
• Stellar and Dust Properties of a Complete Sample of Massive Dusty Galaxies at $1\le z\le 4$ from MAGPHYS Modeling of UltraVISTA DR3 and Herschel Photometry
• The clustering of submillimeter galaxies detected with ALMA
• From starburst to quiescence: post-starburst galaxies and their large-scale clustering over cosmic time
• The Subillimeter Properties of Extremely Red Objects in the CUDSS Fields
• Extremely red galaxies: dust attenuation and classification
• GOODS-ALMA: Using IRAC and VLA to probe fainter millimeter galaxies
• Submillimetre surveys: The prospects for Herschel
• Optical identification of ISO far-infrared sources in the Lockman Hole using a deep VLA 1.4 GHz continuum survey
• Quasars in the MAMBO blank field survey
• Dusty ERO Search behind Two Massive Clusters
• Predicting sub-millimeter flux densities from global galaxy properties
• The Discovery of a New Massive Molecular Gas Component Associated with the Submillimeter Galaxy SMM J02399-0136
• Emission from Dust in Galaxies: Metallicity Dependence
• The IRIS Far-Infrared Galaxy Survey : Expected Number Count, Redshift, and Perspective
• Dust-to-gas ratios in the starburst regions of luminous infrared galaxies
• ISOCAM 15um Search for Distant Infrared Galaxies Lensed by Clusters
• (Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies - II. The spatial extent of the radio-emitting regions
• SCUBA sub-millimeter observations of gamma-ray bursters: II. GRB 991208, 991216, 000301C, 000630, 000911, 000926
• (Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies IV. Physical properties derived from spectral energy distributions
• A Submillimeter Perspective on the GOODS Fields (SUPER GOODS). V. Deep 450 Micron Imaging
• X-ray observations of sub-mm LABOCA galaxies in the eCDFS
• The JCMT SCUBA-2 Survey of the James Webb Space Telescope North Ecliptic Pole Time-Domain Field
• Using SCUBA to place upper limits on arcsecond scale CMB anisotropies at 850 microns
• ALMACAL IX: multi-band ALMA survey for dusty star-forming galaxies and the resolved fractions of the cosmic infrared background
• Gigamasers: the key to the dust-obscured star-formation history of the Universe?
• Far-IR Emission From Dust-Obscured Galaxies
• ASTRO-F - Super IRAS - The All Sky Infra-Red Survey
• Prospects for ACT: simulations, power spectrum, and non-Gaussian analysis
• Correlations between bright submillimetre sources and low-redshift galaxies
• SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES) IV: Spatial clustering and halo masses of 450-$\mu$m-selected sub-millimeter galaxies
• Lyman$\alpha$ Emitters beyond Redshift 5:The Dawn of Galaxy Formation
• FIR-luminous [CII] emitters in the ALMA-SCUBA-2 COSMOS survey (AS2COSMOS): The nature of submillimeter galaxies in a 10 comoving Mpc-scale structure at z~4.6
• X-raying the Star Formation History of the Universe
• Formation and evolution of dusty starburst galaxies I. A new method for deriving spectral energy distribution
• Radio counterpart of the lensed sub-mm emission in the cluster MS0451.6-0305: new evidence for the merger scenario
• NIKA2 Cosmological Legacy Survey: Survey Description and Galaxy Number Counts
• A Multiwavelength Study of ELAN Environments (AMUSE${}^2$): Ubiquitous dusty star-forming galaxies associated with enormous Ly$\alpha$ nebulae on megaparsec scales
• Interstellar Silicate Dust in the z=0.89 Absorber Towards PKS 1830-211: Crystalline Silicates at High Redshift?
• First Constraints on Source Counts at 350 Microns
• Centimeter searches for molecular line emission from high-redshift galaxies
• Modelling the dusty universe II: The clustering of submillimetre-selected galaxies
• Morphological and photometric evolution of ultra-luminous infrared galaxies: Nature of faint SCUBA sources
• Arp 220: New Observational Insights into the Structure and Kinematics of the Nuclear Molecular Disks and Surrounding Gas
• SXDF-ALMA 2 Arcmin^2 Deep Survey: Resolving and Characterizing the Infrared Extragalactic Background Light Down to 0.5 mJy
• A hyper luminous starburst at z=4.72 magnified by a lensing galaxy pair at z=1.48
• A Long Stream of Metal-Poor Cool Gas around a Massive Starburst Galaxy at z = 2.67
• Dust Properties of 870 Micron Selected Galaxies in the GOODS-S
• Herschel-ATLAS Data Release III: Near-infrared counterparts in the South Galactic Pole field -- Another 100,000 submillimetre galaxies
• Mid Infrared Polarisation of Ultraluminous Infrared Galaxies
• The Circumgalactic Medium of Submillimeter Galaxies. I. First Results from a Radio-Identified Sample
• The Cosmic Infrared Background Radiation, Star Formation Rate, and Metallicity
• A broadband spectroscopic search for CO line emission in HDF850.1: the brightest submillimetre object in the Hubble Deep Field North
• A multi-wavelength approach to the properties of Extremely Red Galaxy populations: I - Contribution to the Star Formation Rate density and AGN content
• A Bright Submillimeter Source in the Bullet Cluster (1E0657--56) Field Detected with BLAST
• Measurements of the Cross Spectra of the Cosmic Infrared and Microwave Backgrounds from 95 to 1200 GHz
• Multi-wavelength properties of 850-$\mu$m selected sources from the North Ecliptic Pole SCUBA-2 survey
• Submillimetre Source Counts in the Fields of High-Redshift Galaxy Clusters
• Numerical simulations on the relative importance of starbursts and AGN in ultra-luminous infrared galaxies
• Sub-millimeter brightness of early star-forming galaxies
• NGC 6240 Supermassive Black Hole Binary dynamical evolution based on Chandra data
• Source structure and molecular gas properties from high-resolution CO imaging of SPT-selected dusty star-forming galaxies
• The Atacama Cosmology Telescope: CO(J = 3 - 2) mapping and lens modeling of an ACT-selected dusty star-forming galaxy
• Excitation Conditions in the Multi-component Submillimeter Galaxy SMM J00266+1708
• VLA 1.4 GHz Catalogs of the Abell 370 and Abell 2390 Cluster Fields
• A high redshift population of galaxies at the North Ecliptic Pole: unveiling the main sequence of dusty galaxies
• Submm/mm Galaxy Counterpart Identification Using a Characteristic Density Distribution
• The contribution of AGN to the sub-mm population
• Three Dusty Star Forming Galaxies at $z\sim 1.5$: Mergers and Disks on the Main Sequence
• Cosmic star formation history associated with QSO activity: an approach using the black hole to bulge mass correlation
• The AGN fraction of submm-selected galaxies and contributions to the submm/mm-wave extragalactic background light
• High Sensitivity Array Observations of the z=1.87 Sub-Millimeter Galaxy GOODS 850-3
• ALMA 26 arcmin${}^2$ survey of GOODS-S at one-millimeter (ASAGAO): millimeter properties of stellar mass selected galaxies
• Principal Component Analysis and Radiative Transfer modelling of Spitzer IRS Spectra of Ultra Luminous Infrared Galaxies
• Evolution of Dust-Obscured Star Formation and Gas to z=2.2 from HiZELS
• SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES) II: Structural Properties and Near-Infrared Morphologies of Faint Submillimeter Galaxies
• Cosmology with the Planck cluster sample
• A New View of Galaxy Evolution from Submillimeter Surveys with SCUBA
• The SCUBA-2 Large eXtragalactic Survey: 850um map, catalogue and the bright-end number counts of the XMM-LSS field
• An Orientation Bias in Observations of Submillimetre Galaxies
• Flat Rotation Curves found in Merging Dusty Starbursts at $z=2.3$ through Tilted-Ring Modeling
• Spitzer Imaging of Strongly-Lensed Herschel-Selected Dusty Star Forming Galaxies
• Early Science with the Large Millimeter Telescope: a 1.1 mm AzTEC Survey of Red-$Herschel$ dusty star-forming galaxies
• Cosmic Sands: The Origin of Dusty, Star-forming Galaxies in the Epoch of Reionization
• A panchromatic study of BLAST counterparts: total star-formation rate, morphology, AGN fraction and stellar mass
• High-z dusty star-forming galaxies: a top-heavy initial mass function?
• JADES Ultra-red Flattened Objects: Morphologies and Spatial Gradients in Color and Stellar Populations
• Improved Templates for Photometric Redshifts of Submm Sources
• Deep Submillimeter Surveys: Luminous Infrared Galaxies at High Redshift
• JWST/MIRI unveils the stellar component of the GN20 dusty galaxy overdensity at $z$=4.05
• ALMACAL VII: First Interferometric Number Counts at 650 $\mu$m
• ALMACAL. XI. Over-densities as signposts to proto-clusters? A cautionary tale
• On the discovery of the first 350 micron-selected galaxy
• A submillimetre-bright z~3 overdensity behind a z~1 supercluster revealed by SCUBA-2 and Herschel
• A Submillimeter Survey of Faint Galaxies Behind Ten Strong Lensing Clusters
• The nature of sub-millimetre galaxies I: A comparison of AGN and star-forming galaxy SED fits
• ASCA observations of deep ROSAT fields V. The X-ray spectrum of hard X-ray selected QSOs
• Multi-band Optical and Near-infrared Properties of Faint Submillimeter Galaxies with Serendipitous ALMA Detections
• [NII] fine-structure emission at 122 and 205um in a galaxy at z=2.6: a globally dense star-forming interstellar medium
• Cosmological History of Stars and Metals
• Environments of a sample of AzTEC submillimetre galaxies in the COSMOS field
• Mid-Infrared Identification of Faint Submillimeter Sources
• Low-frequency radio spectra of submillimetre galaxies in the Lockman Hole
• The SCUBA-2 Cosmology Legacy Survey: The EGS deep field -- III. The evolution of faint submillimeter galaxies at $z<4$
• Radio and X-ray properties of submillimeter galaxies in the A2125 field
• Understanding galaxy formation with ISO deep surveys
• Classification of local ultraluminous infrared galaxies and quasars with kernel principal component analysis
• On the fate of gas in ultraluminous galaxies at low and high redshift
• SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). V. Confusion-limited Submillimeter Galaxy Number Counts at 450 $\mu$m and Data Release for the COSMOS Field
• Identification of a Complete 160 micron Flux-Limited Sample of Infrared Galaxies in the ISO Lockman Hole 1-Deg^2 Deep Fields: Source Properties and Evidence for Strong Evolution in the FIR Luminosity Function for ULIRGs
• Effects of a burst of formation of first-generation stars on the evolution of galaxies
• Constraints on the galaxy "main sequence" at z>5: the stellar mass of HDF850.1
• The Contribution of Faint Blue Galaxies to the Sub-mm Counts and Background
• Cosmic happenstance: 24-$\mu$m selected, multi-component Herschel sources are line-of-sight projections
• Contribution of starburst mergers at z~1 to the strong evolution of infrared and submillimeter deep surveys
• Extending PLE models into the mid-IR, far-IR & sub-mm
• Gas and Dust in Protogalaxies
• Faint 6.7um Galaxies and their Contributions to the Stellar Mass Density in the Universe
• On the abundance of gravitational arcs produced by submillimeter galaxies at radio and submm wavelengths
• The ALPINE-ALMA [CII] Survey: Unveiling the baryon evolution in the ISM of $z\sim 5$ star-forming galaxies
• Multiwavelength characterisation of an ACT-selected, lensed dusty star-forming galaxy at z=2.64
• A Massive Molecular Gas Reservoir in the z=2.221 Type-2 Quasar Host Galaxy SMM J0939+8315 Lensed by the Radio Galaxy 3C220.3
• Vigorous star formation in a bulge-dominated ERO at z = 1.34
• Interpreting the statistical properties of high-z extragalactic sources detected by the South Pole Telescope survey
• Resolving a merger in a hyper-luminous submillimeter galaxy at z=2.82
• Lensing-Induced Structure of Submillimeter Sources: Implications for the Microwave Background
• An EVLA search for water megamaser emission in the submm galaxy SMM J16359+6612 at z=2.5
• Modeling submillimeter galaxies in cosmological simulations: Contribution to the cosmic star formation density and predictions for future surveys
• Deep Submillimetre and Radio Observations in the SSA22 Field. II. Sub-millimetre source catalogue and number counts
• Graph Theoretical Analysis of local ultraluminous infrared galaxies and quasars
• Detection of H-alpha emission from z>3.5 submillimetre luminous galaxies with AKARI-FUHYU spectroscopy
• Constraints on the presence of water megamaser emission in z~2.5 ultraluminous infrared starburst galaxies
• Do sub-mm sources and quasars form an evolutionary sequence?
• On the nature of the first galaxies selected at 350 microns
• Submillimeter galaxy overdensities around physically associated quasar pairs
• The Hawaii SCUBA-2 Lensing Cluster Survey: Radio-detected Submillimeter Galaxies in the HST Frontier Fields
• Identifying and Characterizing the Most Heavily Dust-Obscured Galaxies at $1\le z\le 4$
• A mock redshift catalogue of the dusty star-forming galaxy population with intrinsic clustering and lensing for deep millimetre surveys
• Instruments on large optical telescopes -- A case study
• Simultaneously Modelling Dusty Star Forming Galaxies and Massive Quiescents: A Calibration Framework for Galaxy Formation Models
• LRG J0239-0134: A Ring Galaxy or a Pair of Superbubbles at z=1 ?
• Gravitational Lensing Limits on the Average Redshift of Submillimeter Sources
• Disclosing Submillimeter Galaxy Formation: Mergers or Secular Evolution?
• Interstellar Medium in Extremely High Star-Formation Regions: A Prospect of Observations on the Millimetron Space Observatory
• Probing Cool and Warm Infrared Galaxies using Photometric and Structural Measures
• Cosmic magnification on high-redshift submillimeter galaxies
• A comparative study of ultraluminous infrared galaxies in the IRAS and SDSS Surveys
• Investigating the role of turbulence in the interstellar medium in $z\sim 3$ dusty star-forming galaxies using kpc-resolution ALMA dust and gas maps
• The Atacama Cosmology Telescope: Extragalactic Point Sources in the Southern Surveys at 150, 220 and 280 GHz observed between 2008-2010
• Licking the plate: dusty star-forming galaxies buried in the ALMA calibration data
• The Nature of Hyperluminous Infrared Galaxies
• The LMT 2 Millimeter Receiver System (B4R). I. Overview and Results of Science Demonstration
• Implementing Remote Observing at the JCMT
• Millimeter-Wave Spectroscopy and Mapping of Quasar Hosts, and the Status of ULIRGs as Quasar 2s
• The nature of sub-millimetre galaxies II: an ALMA comparison of SMG dust heating mechanisms
• Understanding galaxy formation and evolution through an all-sky submillimetre spectroscopic survey