Far-infrared surveys of galaxy evolution

Abstract

Roughly half of the radiation from evolving galaxies in the early universe reaches us in the far-infrared and submillimeter wavelength range. Recent major advances in observing capabilities, in particular the launch of the Herschel Space Observatory in 2009, have dramatically enhanced our ability to use this information in the context of multiwavelength studies of galaxy evolution. Near its peak, three quarters of the cosmic infrared background is now resolved into individually detected sources. The use of far-infrared diagnostics of dust-obscured star formation and of interstellar medium conditions has expanded from rare extreme high-redshift galaxies to more typical main sequence galaxies and hosts of active galactic nuclei, out to z>~2. These studies shed light on the evolving role of steady equilibrium processes and of brief starbursts, at and since the peak of cosmic star formation and black hole accretion. This review presents a selection of recent far-infrared studies of galaxy evolution, with an emphasis on Herschel results

arXiv commentReview for Annual Review Astronomy Astrophysics vol. 52 (2014)

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• The stellar masses and specific star-formation rates of submillimetre galaxies
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• The Herschel-ATLAS: Extragalactic Number Counts from 250 to 500 Microns
• Sub-millimetre galaxies reside in dark matter halos with masses greater than 3x10^11 solar masses
• The Herschel Lensing Survey (HLS): overview
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• Herschel PEP: The star-formation rates of 1.5<z<2.5 massive galaxies
• A Comprehensive View of a Strongly Lensed Planck-Associated Submillimeter Galaxy
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• The redshift-evolution of the distribution of star formation among dark matter halos as seen in the infrared
• The Molecular Gas Content of z = 3 Lyman Break Galaxies; Evidence of a non Evolving Gas Fraction in Main Sequence Galaxies at z > 2
• The Detection of Crystalline Silicates in Ultra-Luminous Infrared Galaxies
• Variations of the spectral index of dust emissivity from Hi-GAL observations of the Galactic plane
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• The impact of evolving infrared spectral energy distributions of galaxies on star formation rate estimates
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• Supermassive Black Hole Growth in Starburst Galaxies over Cosmic Time: Constraints from the Deepest Chandra Fields
• Strong [CII] emission at high redshift
• The dust content of high-z submillimeter galaxies revealed by Herschel
• Herschel-ATLAS: The far-infrared--radio correlation at z<0.5
• Can dust emission be used to map the interstellar medium in high-redshift galaxies? Results from the Herschel Reference Survey
• A backward evolution model for infrared surveys: the role of AGN- and Color-L_TIR distributions
• Confusion in the infrared: Spitzer and beyond
• HerMES: Unveiling obscured star formation - the far infrared luminosity function of ultraviolet-selected galaxies at z~1.5
• The Relation Between Cool Cluster Cores and Herschel-Detected Star Formation in Brightest Cluster Galaxies
• Size bias and differential lensing of strongly lensed, dusty galaxies identified in wide-field surveys
• A New Population of High Redshift, Dusty Lyman-Alpha Emitters and Blobs Discovered by WISE
• Herschel-ATLAS: towards a sample of ~1000 strongly-lensed galaxies
• Connecting stellar mass and star-formation rate to dark matter halo mass out to z ~ 2
• H2O emission in high-z ultra-luminous infrared galaxies
• The Herschel Virgo Cluster Survey: I. Luminosity functions
• Herschel-ATLAS/GAMA: a census of dust in optically selected galaxies from stacking at submillimetre wavelengths
• The Herschel Virgo Cluster Survey - VIII. The Bright Galaxy Sample
• Mid-Infrared Determination of Total Infrared Luminosity and Star Formation Rates of Local and High-Redshift Galaxies
• PEP: first Herschel probe of dusty galaxy evolution up to z~3
• Far-infrared properties of submillimeter and optically faint radio galaxies
• Measurements of CO redshifts with Z-Spec for lensed submillimeter galaxies discovered in the H-ATLAS survey
• Multi-Wavelength SEDs of Herschel Selected Galaxies in the COSMOS Field
• Herschel reveals a T_dust-unbiased selection of z~2 ULIRGs
• Spitzer and Herschel-based SEDs of 24um-bright z~0.3-3.0 starbursts and obscured quasars
• Herschel-ATLAS: The link between accretion luminosity and star formation in quasar host galaxies
• GBT Zpectrometer CO(1-0) Observations of the Strongly-Lensed Submillimeter Galaxies from the Herschel ATLAS
• Ultra-deep Spitzer Mid-Infrared Spectroscopy of LIRGs and ULIRGs at z ~ 1-2
• The evolution of the star formation activity per halo mass up to redshift ~ 1.6 as seen by Herschel
• The Spectral Energy Distributions and Infrared Luminosities of z \approx 2 Dust Obscured Galaxies from Herschel and Spitzer
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• The Atacama Cosmology Telescope: Dusty Star-Forming Galaxies and Active Galactic Nuclei in the Southern Survey
• The HerMES SPIRE submillimeter local luminosity function
• Inferring the mass of sub-millimetre galaxies by exploiting their gravitational magnification of background galaxies
• Observation of H2O in a strongly lensed Herschel-ATLAS source at z=2.3
• Herschel-SPIRE, Far-Infrared Properties of Millimetre-Bright and -Faint Radio Galaxies
• First results from HerMES on the evolution of the submillimetre luminosity function
• The effect of environment on star forming galaxies at redshift 1 - First insight from PACS
• Complete infrared spectral energy distributions of mm detected quasars at z>5
• H-ATLAS: The cosmic abundance of dust from the far-infrared background power spectrum
• Dust emission from the lensed Lyman break galaxy cB58
• GOODS-Herschel: the impact of galaxy-galaxy interactions on the far-infrared properties of galaxies
• The Far-Infrared, UV and Molecular Gas Relation in Galaxies up to z=2.5
• Dust in the wind: Crystalline silicates, corundum and periclase in PG 2112+059
• GOODS-Herschel A population of 24micron dropout sources at z < 2
• Star formation histories, extinction, and dust properties of strongly lensed z~1.5-3 star-forming galaxies from the Herschel Lensing Survey
• SPT 0538-50: Physical conditions in the ISM of a strongly lensed dusty star-forming galaxy at z=2.8
• Reversal or no reversal: the evolution of the star formation rate-density relation up to z~1.6
• The local FIR Galaxy Colour-Luminosity distribution: A reference for BLAST, and Herschel/SPIRE sub-mm surveys
• Redshift Determination and CO Line Excitation Modeling for the Multiply-Lensed Galaxy HLSW-01
• Herschel Observations of Far-Infrared Cooling Lines in intermediate Redshift (Ultra)-luminous Infrared Galaxies
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• Herschel Detection of Dust Emission from UV-Luminous Star-Forming Galaxies at 3.3<z<4.3
• The far-infrared/submillimeter properties of galaxies located behind the Bullet cluster
• FIR-detected Lyman break galaxies at z ~ 3: Dust attenuation and dust correction factors at high redshift
• Measures of star formation rates from Infrared (Herschel) and UV (GALEX) emissions of galaxies in the HerMES fields
• Herschel ATLAS: The cosmic star formation history of quasar host galaxies
• A Population of Dust-Rich Quasars at z ~ 1.5
• Herschel-PACS observations of [OI]63um towards submillimetre galaxies at z~1
• Molecular gas mass functions of normal star forming galaxies since z~3
• GAMA/H-ATLAS: The ultraviolet spectral slope and obscuration in galaxies
• Cosmic Evolution of Star-Formation Enhancement in Close Major-Merger Galaxy Pairs Since z = 1
• What triggers black-hole growth? Insights from star formation rates
• Comparison of star formation rates from Halpha and infrared luminosities as seen by Herschel
• HerMES: Lyman Break Galaxies individually detected at 0.7 < z < 2.0 in GOODS-N with Herschel/SPIRE
• Contribution of Lensed SCUBA Galaxies to the Cosmic Infrared Background
• Extreme host galaxy growth in powerful early-epoch radio galaxies
• HerMES: SPIRE/Sub-millimetre Emission from Radio Selected AGN
• The PEP survey: clustering of infrared-selected galaxies and structure formation at z~2 in the GOODS South
• Constraining the Lyman Alpha Escape Fraction with Far-Infrared Observations of Lyman Alpha Emitters
• Herschel deep far-infrared counts through the Abell 2218 cluster-lens
• PACS-Herschel FIR detections of Lyman-alpha emitters at 2.0<z<3.5
• Extreme star formation in the host galaxies of the fastest growing super-massive black holes at z=4.8
• HerMES: Herschel-SPIRE observations of Lyman Break Galaxies
• The environment and characteristics of low redshift galaxies detected by the Herschel-ATLAS
• HerMES: A Statistical Measurement of the Redshift Distribution of Herschel-SPIRE Sources Using the Cross-correlation Technique
• Herschel-ATLAS: the far-infrared properties and star-formation rates of broad absorption line quasi-stellar objects
• Discovery of "Warm Dust" Galaxies in Clusters at z~0.3: Evidence for Stripping of Cool Dust in the Dense Environment?
• Far-IR Emission From Dust-Obscured Galaxies
• The Herschel-PEP survey: evidence for downsizing in the hosts of dusty star-forming systems
• The Herschel view of the environment of the radio galaxy 4C+41.17 at z = 3.8
• The UV to FIR spectral energy distribution of star-forming galaxies in the redshift desert
• Unveiling Far-Infrared Counterparts of Bright Submillimeter Galaxies Using PACS Imaging
• Extragalactic number counts at 100 um, free from cosmic variance
• Herschel-ATLAS/GAMA: spatial clustering of low-redshift sub-mm galaxies
• The detection of FIR emission from high redshift star-forming galaxies in the ECDF-S
• {\em Herschel}-ATLAS/GAMA: The Environmental Density of Far-Infrared Bright Galaxies at $z\le 0.5$
• Lyman break and UV-selected galaxies at z ~ 1: II. PACS-100um/160um FIR detections
• Herschel-ATLAS/GAMA: What determines the far-infrared properties of radio-galaxies?
• Physical properties of Lyman-alpha emitters at $z\sim 0.3$ from UV-to-FIR measurements
• Herschel FIR counterparts of selected Ly-alpha emitters at z~2.2. Fast evolution since z~3 or missed obscured AGNs?
• Which halos host Herschel-ATLAS galaxies in the local Universe?
• FIR measurements of Ly-$\alpha$ emitters at z$\lesssim$1.0: dust attenuation from PACS-\emph{Herschel}
• Photometric Redshifts of Submillimeter Galaxies

Cited by in corpus (70)

• Cosmic Star Formation History
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• Understanding Galaxy Evolution through Emission Lines
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• Cosmic X-ray Surveys of Distant Active Galaxies: The Demographics, Physics, and Ecology of Growing Supermassive Black Holes
• The Main Sequence of star-forming galaxies across cosmic times
• Star-Forming Galaxies at Cosmic Noon
• A remarkably flat relationship between the average star formation rate and AGN luminosity for distant X-ray AGN
• On the dust temperatures of high redshift galaxies
• Automated Mining of the ALMA Archive in the COSMOS Field (A3COSMOS): II. Cold Molecular Gas Evolution out to Redshift 6
• A New Star-Formation Rate Calibration from Polycyclic Aromatic Hydrocarbon Emission Features and Application to High Redshift Galaxies
• The infrared-radio correlation of star-forming galaxies is strongly M${}_{\star }$-dependent but nearly redshift-invariant since z$\sim$4
• ALMA Long Baseline Observations of the Strongly Lensed Submillimeter Galaxy HATLAS J090311.6+003906 at z=3.042
• CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope
• The mean star formation rates of unobscured QSOs: searching for evidence of suppressed or enhanced star formation
• Star formation properties of sub-mJy radio sources
• The far-infrared emitting region in local galaxies and QSOs: Size and scaling relations
• The reversal of the SF-density relation in a massive, X-ray selected galaxy cluster at z=1.58: results from Herschel
• A physical model for the [CII]-FIR deficit in luminous galaxies
• Star formation in z>1 3CR host galaxies as seen by Herschel
• Powderday: Dust Radiative Transfer for Galaxy Simulations
• The fraction of bolometric luminosity absorbed by dust in DustPedia galaxies
• The Intrinsic Far-infrared Continua of Type-1 Quasars
• The multiwavelength properties of red QSOs -- Evidence for dusty winds as the origin of QSO reddening
• The Contribution of Host Galaxies to the Infrared Energy Output of $z\gtrsim 5.0$ QUASARS
• The main sequence of star forming galaxies II. A non evolving slope at the high mass end
• The Relation between Luminous AGNs and Star Formation in Their Host Galaxies
• Spectral Energy Distributions in Three Deep-Drilling Fields of the Vera C. Rubin Observatory Legacy Survey of Space and Time: Source Classification and Galaxy Properties
• Molecular Gas, Dust and Star Formation in Galaxies: II. Dust properties and scalings in \sim\ 1600 nearby galaxies
• Herschel Survey of the Palomar-Green QSOs at Low Redshift
• Galaxy evolution studies with the SPace IR telescope for Cosmology and Astrophysics (SPICA): the power of IR spectroscopy
• The IRX-$\beta$ relation of high-redshift galaxies
• Local SDSS galaxies in the Herschel Stripe82 survey: A critical assessment of optically-derived star-formation rates
• A multi-wavelength de-blended Herschel view of the statistical properties of dusty star-forming galaxies across cosmic time
• Tracing the evolution of dust-obscured activity using sub-millimetre galaxy populations from STUDIES and AS2UDS
• The infra-red luminosities of ~332,000 SDSS galaxies predicted from artificial neural networks and the Herschel Stripe 82 survey
• ALMA Observations of Quasar Host Galaxies at $z\simeq 4.8$
• Towards a census of high-redshift dusty galaxies with $Herschel$: A selection of "500 $\mu$m-risers"
• Uncovering the stellar structure of the dusty star-forming galaxy GN20 at z=4.055 with MIRI/JWST
• Continuous Mid-Infrared Star Formation Rate Indicators: Diagnostics for 0<z<3 Star Forming Galaxies
• 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
• ALMA resolves extended star formation in high-z AGN host galaxies
• A census of radio-selected AGN on the COSMOS field and of their FIR properties
• The PEP Survey: evidence for intense star-forming activity in the majority of radio-selected AGN at z>~1
• On the existence of bright IR galaxies at z>2: tension between Herschel and SCUBA-2 results?
• Revisiting Attenuation Curves: the Case of NGC 3351
• ZFIRE: Similar Stellar Growth in H$\alpha$-emitting Cluster and Field Galaxies at z~2
• Spectral Distortion of the CMB by the Cumulative CO Emission from Galaxies throughout Cosmic History
• Identification of AKARI infrared sources by Deep HSC Optical Survey: Construction of New Band-Merged Catalogue in the NEP-Wide field
• The Star Formation Reference Survey-V: the effect of extinction, stellar mass, metallicity, and nuclear activity on star-formation rates based on H$\alpha$ emission
• Starbursts and dusty tori in distant 3CR radio galaxies
• Identification of z~>2 Herschel 500 micron sources using color-deconfusion
• Tracing the evolution of dust obscured star-formation and accretion back to the reionisation epoch with SPICA
• A minimal empirical model for the cosmic far-infrared background anisotropies
• Super-resolving Herschel imaging: a proof of concept using Deep Neural Networks
• GOODS-$Herschel$: identification of the individual galaxies responsible for the 80-290$\mu$m cosmic infrared background
• Panchromatic Photometry of Low-redshift, Massive Galaxies Selected from SDSS Stripe 82
• SXDF-ALMA 2-arcmin^2 Deep Survey: Stacking of Rest-Frame Near-Infrared Selected Objects
• The ALMA Spectroscopic Survey in the HUDF: Constraining the Molecular Content at $\log (M_{\ast }/M_{\odot })\sim 9.5$ with CO stacking of MUSE detected $z\sim 1.5$ Galaxies
• Optimizing future experiments of cosmic far-infrared background: a principal component approach
• The Herschel Virgo Cluster Survey. XIX. Physical properties of low luminosity FIR sources at $z<$ 0.5
• The spectral energy distribution of galaxies at z > 2.5: Implications from the Herschel/SPIRE color-color diagram
• The dust and cold gas content of local star forming galaxies
• Star-dust geometry main determinant of dust attenuation in galaxies
• Exploring the evolution of star formation and dwarf galaxy properties with JWST/MIRI serendipitous spectroscopic surveys
• Cosmic X-ray surveys of Active Galactic Nuclei: synergy between X-ray and infrared observations
• A High-resolution Far-infrared Survey to Probe Black Hole-Galaxy Co-evolution
• Image Stacking Analysis of SDSS Galaxies with AKARI Far-Infrared Surveyor Maps at 65μm, 90μm, and 140μm
• The Herschel-SPIRE Dark Field I: The deepest Herschel image of the submillimetre Universe
• Understanding galaxy formation and evolution through an all-sky submillimetre spectroscopic survey