High-redshift star formation in the ALMA era

Abstract

The Atacama Large Millimetre/submillimetre Array (ALMA) is currently in the process of transforming our view of star-forming galaxies in the distant ($z\gtrsim 1$) universe. Before ALMA, most of what we knew about dust-obscured star formation in distant galaxies was limited to the brightest submillimetre sources$-$the so-called submillimetre galaxies (SMGs)$-$and even the information on those sources was sparse, with resolved (i.e., sub-galactic) observations of the obscured star formation and gas reservoirs typically restricted to the most extreme and/or strongly lensed sources. Starting with the beginning of early science operations in 2011, the last nine years of ALMA observations have ushered in a new era for studies of high-redshift star formation. With its long baselines, ALMA has allowed observations of distant dust-obscured star formation with angular resolutions comparable to$-$or even far surpassing$-$the best current optical telescopes. With its bandwidth and frequency coverage, it has provided an unprecedented look at the associated molecular and atomic gas in these distant galaxies through targeted follow-up and serendipitous detections/blind line scans. Finally, with its leap in sensitivity compared to previous (sub-)millimetre arrays, it has enabled the detection of these powerful dust/gas tracers much further down the luminosity function through both statistical studies of color/mass-selected galaxy populations and dedicated deep fields. We review the main advances ALMA has helped bring about in our understanding of the dust and gas properties of high-redshift ($z\gtrsim 1$) star-forming galaxies during these first nine years of its science operations, and we highlight the interesting questions that may be answered by ALMA in the years to come.

arXiv commentInvited Review for Royal Society Open Science, Published version (+ table of contents)

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• Assessing Radiation Pressure as a Feedback Mechanism in Star-Forming Galaxies
• An ALMA Survey of Submillimeter Galaxies in the Extended Chandra Deep Field South: The AGN Fraction and X-ray Properties of Submillimeter Galaxies
• ALMA Long Baseline Observations of the Strongly Lensed Submillimeter Galaxy HATLAS J090311.6+003906 at z=3.042
• Deep 1.1 mm-wavelength imaging of the GOODS-South field by AzTEC/ASTE -- II. Redshift distribution and nature of the submillimetre galaxy population
• PHIBSS2: survey design and z=0.5-0.8 results. Molecular gas reservoirs during the winding-down of star formation
• Dust production 680-850 million years after the Big Bang
• Cold Molecular Gas in Merger Remnants: I. Formation of Molecular Gas Disks
• Shock-Enhanced C+ Emission and the Detection of H2O from Stephan's Quintet's Group-Wide Shock using Herschel
• Simulating galactic dust grain evolution on a moving mesh
• An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: High-resolution dust continuum morphologies and the link between sub-millimetre galaxies and spheroid formation
• Dust continuum emission as a tracer of gas mass in galaxies
• Discovery of a dark, massive, ALMA-only galaxy at z~5-6 in a tiny 3-millimeter survey
• Demonstrating A New Census of INfrared Galaxies with ALMA (DANCING-ALMA). I. FIR Size and Luminosity Relation at z = 0-6 Revealed with 1034 ALMA Sources
• Planck's Dusty GEMS: Gravitationally lensed high-redshift galaxies discovered with the Planck survey
• Are high redshift Galaxies hot? - Temperature of z > 5 Galaxies and Implications on their Dust Properties
• The Properties of Sub-mm Galaxies in Hierarchical Models
• The Spatially Resolved [CII] Cooling Line Deficit in Galaxies
• The Origins of [CII] Emission in Local Star-forming Galaxies
• CI emission in Ultra Luminous Infrared Galaxies as a molecular gas mass tracer
• The IRX-Beta Dust Attenuation Relation in Cosmological Galaxy Formation Simulations
• Dust origin in late-type dwarf galaxies: ISM growth vs. type II supernovae
• The Cosmic Decline in the H2/HI-Ratio in Galaxies
• A dusty star-forming galaxy at z=6 revealed by strong gravitational lensing
• ALMA Observation of 158 micron [CII] Line and Dust Continuum of a z=7 Normally Star-forming Galaxy in the Epoch of Reionization
• The SCUBA-2 Cosmology Legacy Survey: the nature of bright submm galaxies from 2 deg2 of 850-um imaging
• SHINING, A Survey of Far Infrared Lines in Nearby Galaxies. II: Line-Deficit Models, AGN impact, [CII]-SFR Scaling Relations, and Mass-Metallicity Relation in (U)LIRGS
• The evolution of CNO isotopes: the impact of massive stellar rotators
• Dense Gas Tracers and Star Formation Laws in Active Galaxies: APEX Survey of HCN J=4-3, HCO+ J=4-3, and CS J=7-6
• ALMACAL I: First dual-band number counts from a deep and wide ALMA submm survey, free from cosmic variance
• The SCUBA-2 Cosmology Legacy Survey: blank-field number counts of 450um-selected galaxies and their contribution to the cosmic infrared background
• HerMES: ALMA Imaging of Herschel-selected Dusty Star-forming Galaxies
• Revealing the complex nature of the strong gravitationally lensed system H-ATLAS J090311.6+003906 using ALMA
• Alma Twenty-six Arcmin^2 Survey Of Goods-s At One-millimeter (asagao): Source Catalog And Number Counts
• Gas Fraction and Depletion Time of Massive Star Forming Galaxies at z~3.2: No Change in Global Star Formation Process out to z>3
• Discovery of a Multiply-Lensed Submillimeter Galaxy in Early HerMES Herschel/SPIRE Data
• ALMA reveals metals yet no dust within multiple components in CR7
• Cosmological simulation with dust formation and destruction
• Is atomic carbon a good tracer of molecular gas in metal-poor galaxies?
• A gravitationally unstable gas disk of a starburst galaxy 12 billion years ago
• ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Search for [CII] line and dust emission in 6<z<8 galaxies
• [CII] and 12CO(1-0) Emission Maps in HLSJ091828.6+514223: A Strongly Lensed Interacting System at z=5.24
• Discovery of four apparently cold dusty galaxies at z=3.62-5.85 in the COSMOS field: direct evidence of CMB impact on high-redshift galaxy observables
• Witnessing the birth of the red sequence: ALMA high-resolution imaging of [CII] and dust in two interacting ultra-red starbursts at z = 4.425
• SIGAME simulations of the [CII], [OI] and [OIII] line emission from star forming galaxies at z ~ 6
• A spatially resolved study of cold dust, molecular gas, HII regions, and stars in the $z=2.12$ submillimeter galaxy ALESS67.1
• Using [CI] to probe the Interstellar Medium in z~2.5 Sub-Millimeter Galaxies
• Molecular gas content in strongly-lensed z~1.5-3 star-forming galaxies with low IR luminosities
• Automated Mining of the ALMA Archive in the COSMOS Field (A3COSMOS): I. Robust ALMA Continuum Photometry Catalogs and Stellar Mass and Star Formation Properties for ~700 Galaxies at z=0.5-6
• ALMA constraints on the faint millimetre source number counts and their contribution to the cosmic infrared background
• The Nature of Sub-millimetre Galaxies in Cosmological Hydrodynamic Simulations
• The AzTEC/SMA Interferometric Imaging Survey of Submillimeter-Selected High-Redshift Galaxies
• PHIBSS: molecular gas, extinction, star formation and kinematics in the z=1.5 star forming galaxy EGS13011166
• A lower fragmentation mass scale in high redshift galaxies and its implications on giant clumps: a systematic numerical study
• The dust and [CII] morphologies of redshift ~4.5 sub-millimeter galaxies at ~200pc resolution: The absence of large clumps in the interstellar medium of high-redshift galaxies
• An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: number counts of submillimeter galaxies
• Molecular clouds in the Cosmic Snake normal star-forming galaxy 8 billion years ago
• Deep multi-frequency radio imaging in the Lockman Hole using the GMRT and VLA: II. The spectral index of submillimetre galaxies
• The problematic growth of dust in high redshift galaxies
• Exploring the physical properties of local star-forming ULIRGs from the ultraviolet to the infrared
• Large turbulent reservoirs of cold molecular gas around high-redshift starburst galaxies
• Dissecting the IRX - $\beta$ dust attenuation relation: exploring the physical origin of observed variations in galaxies
• ALMA Deep Field in SSA22: Source Catalog and Number Counts
• From the far-ultraviolet to the far-infrared -- galaxy emission at $0\le z\le 10$ in the Shark semi-analytic model
• Resolving the Cosmic Far-Infrared Background at 450 and 850 Microns with SCUBA-2
• Size bias and differential lensing of strongly lensed, dusty galaxies identified in wide-field surveys
• Rise of the Titans: A Dusty, Hyper-Luminous "870 micron Riser" Galaxy at z~6
• Reexamination of the Infrared Excess-Ultraviolet Slope Relation of Local Galaxies
• Measures of galaxy dust and gas mass with Herschel photometry and prospects for ALMA
• SMAObservations of GOODS 850-11 and GOODS 850-13 - First Examples of Multiple Submillimeter Sources Resolved by an Interferometer
• Molecules in galaxies
• Excitation Mechanisms for HCN (1-0) and HCO+ (1-0) in Galaxies from the Great Observatories All-sky LIRG Survey
• The LABOCA survey of the Extended Chandra Deep Field South - radio and mid-infrared counterparts to submillimetre galaxies
• Predictions for the spatial distribution of the dust continuum emission in 1<z<5 star-forming galaxies
• Simulated observations of sub-millimetre galaxies: the impact of single-dish resolution and field variance
• H2O emission in high-z ultra-luminous infrared galaxies
• Evolution of the atomic and molecular gas content of galaxies in dark matter haloes
• ALMA reveals a chemically evolved submillimeter galaxy at z=4.76
• ALMA maps the Star-Forming Regions in a Dense Gas Disk at z~3
• New constraints on dust emission and UV attenuation of z=6.5-7.5 galaxies from millimeter observations
• Hidden in plain sight: a massive, dusty starburst in a galaxy protocluster at z=5.7 in the COSMOS field
• Is There a Maximum Star Formation Rate in High-Redshift Galaxies?
• The nature of the interstellar medium of the starburst low-metallicity galaxy Haro11: a multi-phase model of the infrared emission
• An ALMA survey of submillimeter galaxies in the COSMOS field: Multiwavelength counterparts and redshift distribution
• The Mid-IR and X-ray Selected QSO Luminosity Function
• The essential signature of a massive starburst in a distant galaxy
• Spatially unassociated galaxies contribute significantly to the blended submillimetre galaxy population: predictions for follow-up observations of ALMA sources
• Prediction of the Cosmic Evolution of the CO-Luminosity Functions
• Fast Molecular Outflow from a Dusty Star-Forming Galaxy in the Early Universe
• Obscured star-formation in bright z ~ 7 Lyman-break galaxies
• Dust production scenarios in galaxies at z ~ 6-8.3
• The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Evolution of the molecular gas in CO-selected galaxies
• The far-infrared emitting region in local galaxies and QSOs: Size and scaling relations
• ALMA reveals starburst-like interstellar medium conditions in a compact star-forming galaxy at z ~ 2 using [CI] and CO
• The ALMA Frontier Fields survey I: 1.1 mm continuum detections in Abell 2744, MACSJ0416.1-2403 and MACSJ1149.5+2223
• Physical Characterization of an Unlensed Dusty Star-Forming Galaxy at $z=5.85$
• Faint End of 1.3 mm Number Counts Revealed by ALMA
• AzTEC/ASTE 1.1-mm Survey of the AKARI Deep Field South: source catalogue and number counts
• Rotating starburst cores in massive galaxies at z=2.5
• ALMA 200-parsec Resolution Imaging of Smooth Cold Dusty Disks in Typical $z\sim 3$ Star-Forming Galaxies
• Relationship between star formation rate and black hole accretion at z=2: The different contributions in quiescent, normal and starburst galaxies
• The ALMA Spectroscopic Survey in the HUDF: Deep 1.2 mm continuum number counts
• An Alternative Accurate Tracer of Molecular Clouds: The "$X_{\mathrm{CI}}$-Factor"
• The anatomy of an extreme starburst within 1.3Gyr of the Big Bang revealed by ALMA
• Towards a resolved Kennicutt-Schmidt law at high redshift
• ALMA detection of extended [CII] emission in Himiko at z=6.6
• ALMA Reveals Weak [NII] Emission in "Typical" Galaxies and Intense Starbursts at z=5-6
• The Herschel Virgo Cluster Survey. IX. Dust-to-gas mass ratio and metallicity gradients in four Virgo spiral galaxies
• Early Science with the Large Millimeter Telescope: Observations of Extremely Luminous High-z Sources Identified by Planck
• The nature of sub-millimeter and highly star-forming galaxies in the EAGLE simulation
• The EDGE-CALIFA survey: Variations in the Molecular Gas Depletion Time in Local Galaxies
• CO(1-0) line imaging of massive star-forming disc galaxies at z=1.5-2.2
• Starbursting [O III] emitters and quiescent [C II] emitters in the reionization era
• An ALMA survey of submillimetre galaxies in the COSMOS field: Physical properties derived from energy balance spectral energy distribution modelling
• ALMA twenty-six arcmin${}^2$ survey of GOODS-S at one-millimeter (ASAGAO): Near-infrared-dark faint ALMA sources
• Giant galaxy growing from recycled gas: ALMA maps the circumgalactic molecular medium of the Spiderweb in [CI]
• Faint Submillimeter Galaxies Revealed by Multifield Deep ALMA Observations: Number Counts, Spatial Clustering, and A Dark Submillimeter Line Emitter
• The Absence of [CII] 158$\mu$m Emission in Spectroscopically-Confirmed Galaxies at $z>8$
• The ALMA Spectroscopic Survey in the HUDF: The Cosmic Dust and Gas Mass Densities in Galaxies up to $z\sim 3$
• A Submillimeter Perspective on the GOODS Fields (SUPER GOODS). III. A Large Sample of ALMA Sources in the GOODS-S
• VLA-ALMA Spectroscopic Survey in the Hubble Ultra Deep Field (VLASPECS): Total Cold Gas Masses and CO Line Ratios for z=2-3 "Main Sequence" Galaxies
• FIR line emission from high redshift galaxies
• Strong FUV fields drive the [CII]/FIR deficit in z~3 dusty, star-forming galaxies
• Neutral carbon and CO in 76 (U)LIRGs and starburst galaxy centers A method to determine molecular gas properties in luminous galaxies
• Sub-mm Emission Line Deep Fields: CO and [CII] Luminosity Functions out to z = 6
• Multiple CO lines in SMM J16359+6612 -- Further evidence for a merger
• The ALMA Redshift 4 Survey (AR4S): I. The massive end of the z=4 main sequence of galaxies
• SXDF-ALMA 2 arcmin${}^2$ Deep Survey: 1.1-mm Number Counts
• The Evolution of the Ultraluminous Infrared Galaxy Population from Redshift 0 to 1.5
• The faint counterparts of MAMBO mm sources near the NTT Deep Field
• High-resolution spectroscopic imaging of CO in a z=4.05 proto-cluster
• EVLA observations of a proto-cluster of molecular gas rich galaxies at z = 4.05
• Reproducing the assembly of massive galaxies within the hierarchical cosmogony
• Deceptively cold dust in the massive starburst galaxy GN20 at $z\sim 4$
• The Multiple Merger Assembly of a Hyper-luminous Obscured Quasar at redshift 4.6
• Revealing the Stellar Mass and Dust Distributions of Submillimeter Galaxies at Redshift 2
• Submillimeter H2O and H2O+ emission in lensed ultra- and hyper-luminous infrared galaxies at z ~ 2-4
• Physical properties of z>4 submillimeter galaxies in the COSMOS field
• Neutral Carbon Emission in luminous infrared galaxies The \CI\ Lines as Total Molecular Gas Tracers
• Near-Infrared MOSFIRE Spectra of Dusty Star-Forming Galaxies at 0.2<z<4
• Water vapor emission reveals a highly obscured, star forming nuclear region in the QSO host galaxy APM08279+5255 at z=3.9
• A New Probe of Dense Gas at High Redshift: Detection of HCO+(5-4) Line Emission in APM 08279+5255
• Far-infrared Herschel SPIRE spectroscopy of lensed starbursts reveals physical conditions of ionised gas
• Confirming Herschel candidate protoclusters from ALMA/VLA CO observations
• The ALMA Spectroscopic Survey in the HUDF: Nature and physical properties of gas-mass selected galaxies using MUSE spectroscopy
• Dynamical Structure of the Molecular Interstellar Medium in an Extremely Bright, Multiply Lensed z~3 Submillimeter Galaxy Discovered with Herschel
• 13CO and C18O emission from a dense gas disk at z=2.3: abundance variations, cosmic rays and the initial conditions for star formation
• An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: radio properties and the far-infrared/radio correlation
• The influence of wavelength, flux, and lensing selection effects on the redshift distribution of dusty, star-forming galaxies
• ALMA 26 Arcmin${}^2$ Survey of GOODS-S at One-millimeter (ASAGAO): Average Morphology of High-$z$ Dusty Star-Forming Galaxies is an Exponential-Disk ($n\simeq 1$)
• Dust Properties of [CII] Detected z $\sim$ 5.5 Galaxies: New HST/WFC3 Near-IR Observations
• A spectacular giant arc in the massive cluster lens MACSJ1206.2-0847
• The SCUBA-2 Cosmology Legacy Survey: galaxies in the deep 850-micron survey, and the star-forming `main sequence'
• Observation of H2O in a strongly lensed Herschel-ATLAS source at z=2.3
• Sub-kiloparsec Imaging of Cool Molecular Gas in Two Strongly Lensed Dusty, Star-Forming Galaxies
• The bias of the submillimetre galaxy population: SMGs are poor tracers of the most massive structures in the z ~ 2 Universe
• The Dust Attenuation of Star-forming Galaxies at $z\sim 3$ and Beyond: New Insights from ALMA Observations
• No evidence for enhanced [OIII] 88um emission in a z~6 quasar compared to its companion starbursting galaxy
• The Molecular Gas Reservoirs of $z\sim 2$ Galaxies: A comparison of CO(1-0) and dust-based molecular gas masses
• A 33 GHz Survey of Local Major Mergers: Estimating the Sizes of the Energetically Dominant Regions from High Resolution Measurements of the Radio Continuum
• An Analysis of ALMA Deep Fields and the Perceived Dearth of High-z Galaxies
• New places and phases of CO-poor/CI-rich molecular gas in the Universe
• ALMA imaging of SDP.81 - II. A pixelated reconstruction of the CO emission lines
• Modelling SCUBA sources in a Lambda-CDM cosmology: hot starbursts or cold extended galactic dust?
• Varying [CII]/[NII] line ratios in the interacting system BR1202-0725 at z=4.7
• Near-Infrared Colors of Submillimeter-Selected Galaxies
• Spatially Resolved [CII] Emission in SPT0346-52: A Hyper-Starburst Galaxy Merger at z~5.7
• A Detailed Gravitational Lens Model Based on Submillimeter Array and Keck Adaptive Optics Imaging of a Herschel-ATLAS Sub-millimeter Galaxy at z=4.243
• Interpreting the evolution of galaxy colours from $z=8$ to $z=5$
• The infrared-dark dust content of high redshift galaxies
• Detection of HNC and tentative detection of CN at z=3.9
• Galaxy simulation with the evolution of grain size distribution
• The Star Formation Rate - Dense Gas Relation in Galaxies as Measured by HCN (3-2) Emission
• Molecular clouds photoevaporation and FIR line emission
• Testing Star Formation Laws in a Starburst Galaxy At Redshift 3 Resolved with ALMA
• VLA Mapping of the CO(1-0) Line in SMM J14011+0252
• High dense gas fraction in intensely star-forming dusty galaxies at high redshift
• GOODS-ALMA: 1.1 mm galaxy survey - I. Source catalogue and optically dark galaxies
• The GISMO 2-millimeter Deep Field in GOODS-N
• A direct calibration of the IRX-β relation in Lyman-break Galaxies at z=3-5
• First Detection of HCO+ Emission at High Redshift
• VALES: III. The calibration between the dust continuum and interstellar gas content of star-forming galaxies
• A reassessment of the redshift distribution and physical properties of luminous (sub-)millimetre galaxies
• Modelling high resolution ALMA observations of strongly lensed highly star forming galaxies detected by Herschel
• Evolution of the extinction curves in galaxies
• Resolved neutral carbon emission in nearby galaxies: [CI] Lines as Total Molecular Gas Tracers
• The Role of Merger Stage on Galaxy Radio Spectra in Local Infrared-Bright Starburst Galaxies
• Millimeter mapping at z~1: dust-obscured bulge building and disk growth
• Dense Molecular Gas Excitation in Nuclear Starbursts at High Redshift: HCN, HNC, and HCO+(J=6-5) Emission in the z=3.91 Quasar Host of APM08279+5255
• Empirical predictions for (sub-)millimeter line and continuum deep fields
• Clumpy and Extended Starbursts in the Brightest Unlensed Submillimeter Galaxies
• SXDF-ALMA 1.5 arcmin^2 deep survey. A compact dusty star-forming galaxy at z=2.5
• Radiative equilibrium estimates of dust temperature and mass in high-redshift galaxies
• Full of Orions: a 200-pc mapping of the interstellar medium in the redshift-3 lensed dusty star-forming galaxy SDP.81
• Faint Submillimeter Galaxies identified through their optical/near-infrared colours I: spatial clustering and halo masses
• Weak 13CO in the Cloverleaf Quasar: evidence for a young, early generation starburst
• Search for [CII] emission in z=6.5-11 star-forming galaxies
• The high redshift SFR-M* relation is sensitive to the employed star formation rate and stellar mass indicators: Towards addressing the tension between observations and simulations
• ALMA will determine the spectroscopic redshift z>8 with FIR [O III] emission lines
• The differential magnification of high-redshift ultraluminous infrared galaxies
• (Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies - I. Multiwavelength identifications and redshift distribution
• Constraining the volume density of Dusty Star-Forming Galaxies through the first 3mm Number Counts from ALMA
• The ALPINE-ALMA [CII] Survey: A Triple Merger at z~4.56
• Planck's dusty GEMS. IV. Star formation and feedback in a maximum starburst at z=3 seen at 60-pc resolution
• Evolution of grain size distribution in high-redshift dusty quasars: Integrating large amounts of dust and unusual extinction curves
• CO, H2O, H2O+ line and dust emission in a z = 3.63 strongly lensed starburst merger at sub-kiloparsec scales
• ALMACAL VI: Molecular gas mass density across cosmic time via a blind search for intervening molecular absorbers
• Radiative transfer meets Bayesian statistics: where does a galaxy's [CII] emission come from?
• The IRAM/GISMO two-millimeter survey in the COSMOS field
• AzTEC half square degree survey of the SHADES fields - II. Identifications, redshifts, and evidence for large-scale structure
• Measuring Star-formation Rate and Far-Infrared Color in High-redshift Galaxies Using the CO (7-6) and [NII] 205 micron Lines
• High-resolution SMA imaging of bright submillimetre sources from the SCUBA-2 Cosmology Legacy Survey
• An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: Identifying candidate z~4.5 [CII] emitters
• SMA observations on faint Submillimeter Galaxies with S${}_{850}$ < 2 mJy: Ultra Dusty Low-Luminosity Galaxies at High Redshift
• CNO emission of an unlensed submillimeter galaxy at z=4.3
• The [CII] Deficit in LIRGs and ULIRGs is Due to High-Temperature Saturation
• ALMA Deep Field in SSA22: Survey Design and Source Catalog of a 20 arcmin^2 Survey at 1.1mm
• The ALMA Spectroscopic Survey in the HUDF: A model to explain observed 1.1 and 0.85 millimeter dust continuum number counts
• A machine-learning method for identifying multi-wavelength counterparts of submillimeter galaxies: training and testing using AS2UDS and ALESS
• The Nature of the Second Parameter in the IRX-beta Relation for Local Galaxies
• Constraints on the Cosmic-Ray Ionization Rate in the $z\sim 2.3$ Lensed Galaxies SMM J2135$-$0102 and SDP 17b from Observations of OH${}^{+}$ and H${}_2$O${}^{+}$
• Molecular gas mass functions of normal star forming galaxies since z~3
• Herschel reveals a molecular outflow in a z = 2.3 ULIRG
• An ALMA survey of CO in submillimetre galaxies: companions, triggering, and the environment in blended sources
• Imaging the Molecular Interstellar Medium in a Gravitationally Lensed Star-forming Galaxy at z=5.7
• Up to 100,000 reliable strong gravitational lenses in future dark energy experiments
• Dense Molecular Gas Excitation at High Redshift: Detection of HCO+(J=4-3) Emission in the Cloverleaf Quasar
• Similar Scaling Relations for the Gas Content of Galaxies across Environments to z ~ 3.5
• The redshift distribution of submillimetre galaxies at different wavelengths
• ALMACAL II: Extreme star-formation-rate densities in a pair of dusty starbursts at $z=3.442$ revealed by ALMA 20-milliarcsec resolution imaging
• The cosmic abundance of cold gas in the local Universe
• ALMA constraints on star-forming gas in a prototypical z=1.5 clumpy galaxy: the dearth of CO(5-4) emission from UV-bright clumps
• Atomic carbon as a powerful tracer of molecular gas in the high-redshift Universe: perspectives for ALMA
• The relationship between dust and [CI] at z=1 and beyond
• Observational constraints on the physical nature of submillimetre source multiplicity: chance projections are common
• An ALMA survey of submillimetre galaxies in the COSMOS field: The extent of the radio-emitting region revealed by 3 GHz imaging with the Very Large Array
• Testing Star Formation Laws on Spatially Resolved Regions in a $z\approx 4.3$ Starburst Galaxy
• A Ks and IRAC Selection of High-Redshift Extremely Red Objects
• The ALMA Frontier Fields Survey III: 1.1 mm Emission Line Identifications in Abell 2744, MACSJ0416.1-2403, MACSJ1149.5+2223, Abell 370, and Abell S1063
• Resolved Molecular Gas and Star Formation Properties of the Strongly Lensed z=2.26 Galaxy SDSS J0901+1814
• ALMA Deep Field in SSA22: Blindly Detected CO Emitters and [CII] Emitter Candidates
• Extreme conditions in the molecular gas of lensed star-forming galaxies at z~3
• Radio spectra and sizes of ALMA-identified submillimetre galaxies: evidence of age-related spectral curvature and cosmic ray diffusion?
• PHIBSS: Exploring the Dependence of the CO-H${}_2$ Conversion Factor on Total Mass Surface Density at $z<1.5$
• Multi-wavelength properties of radio and machine-learning identified counterparts to submillimeter sources in S2COSMOS
• Molecular absorptions in high-z objects
• Spatially Resolved Water Emission from Gravitationally Lensed Dusty Star Forming Galaxies at z $\sim$ 3
• The clustering of submillimeter galaxies detected with ALMA
• On the Interpretation of Far-infrared Spectral Energy Distributions. I: The 850 $\mu$m Molecular Mass Estimator
• The ISM Properties and Gas Kinematics of a Redshift 3 Massive Dusty Star-forming Galaxy
• Blind millimeter line emitter search using ALMA data toward gravitational lensing clusters
• The Clustering Evolution of Dusty Star-Forming Galaxies
• The ALMA Development Roadmap
• Detection of Emission from the CN Radical in the Cloverleaf Quasar at z=2.56
• The ALMA Frontier Fields Survey - IV. Lensing-corrected 1.1 mm number counts in Abell 2744, MACSJ0416.1-2403 and MACSJ1149.5+2223
• The Discovery of a New Massive Molecular Gas Component Associated with the Submillimeter Galaxy SMM J02399-0136
• (Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies - II. The spatial extent of the radio-emitting regions
• (Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies IV. Physical properties derived from spectral energy distributions
• Resolving Star Formation on Sub-Kiloparsec Scales in the High-Redshift Galaxy SDP.11 Using Gravitational Lensing
• ALMA [NII] 205 micron Imaging Spectroscopy of the Interacting Galaxy System BRI 1202-0725 at Redshift 4.7
• Stacked Average Far-Infrared Spectrum of Dusty Star-Forming Galaxies from the Herschel/SPIRE Fourier Transform Spectrometer
• SXDF-ALMA 2 Arcmin^2 Deep Survey: Resolving and Characterizing the Infrared Extragalactic Background Light Down to 0.5 mJy
• The Astrochemical Impact of Cosmic Rays in Protoclusters II: CI-to-H${}_2$ and CO-to-H${}_2$ Conversion Factors
• Is a top-heavy initial mass function needed to reproduce the submillimeter galaxy number counts?
• SXDF-ALMA 2-arcmin^2 Deep Survey: Stacking of Rest-Frame Near-Infrared Selected Objects
• "Zombie" or active? An alternative explanation to the properties of star-forming galaxies at high redshift
• A resolved warm/dense gas Schmidt-Kennicutt relationship in a binary HyLIRG at $z=2.41$

Cited by in corpus (131)

• Reionization Era Bright Emission Line Survey: Selection and Characterization of Luminous Interstellar Medium Reservoirs in the z>6.5 Universe
• Photodissociation and X-Ray Dominated Regions
• The REBELS ALMA Survey: cosmic dust temperature evolution out to z $\sim$ 7
• The ALMA REBELS Survey: Dust Continuum Detections at z > 6.5
• The ALMA REBELS Survey: the dust content of $z\sim 7$ Lyman Break Galaxies
• Low-J CO Line Ratios From Single Dish CO Mapping Surveys and PHANGS-ALMA
• Supermassive Black Holes at High Redshift are Expected to be Obscured by their Massive Host Galaxies' Inter Stellar Medium
• The ALMA REBELS Survey: The Dust-obscured Cosmic Star Formation Rate Density at Redshift 7
• The ALMA REBELS Survey. Epoch of Reionization giants: properties of dusty galaxies at $z\approx 7$
• An ALMA/NOEMA survey of the molecular gas properties of high-redshift star-forming galaxies
• RUBIES: a complete census of the bright and red distant Universe with JWST/NIRSpec
• CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope
• Turbulent Gas in Lensed Planck-selected Starbursts at redshifts 1-3.5
• JWST reveals a population of ultra-red, flattened disk galaxies at 2<z<6 previously missed by HST
• GOODS-ALMA 2.0: Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxies
• Dual constraints with ALMA: new [O III] 88 $\mu$m and dust-continuum observations reveal the ISM conditions of luminous LBGs at $z\sim 7$
• The dust-continuum size of TNG50 galaxies at $z=1-5$: a comparison with the distribution of stellar light, stars, dust and H${}_2$
• Regular rotation and low turbulence in a diverse sample of z ~ 4.5 galaxies observed with ALMA
• Reproducing sub-millimetre galaxy number counts with cosmological hydrodynamic simulations
• Dust temperature in ALMA $\hbox{[C $\scriptstyle\rm II $]}$-detected high-$z$ galaxies
• Significant Dust-Obscured Star Formation in Luminous Lyman-break Galaxies at $z$$\sim$$7$$-$$8$
• The discovery of rest-frame UV colour gradients and a diversity of dust morphologies in bright z ~ 7 Lyman-break galaxies
• ALMA measures rapidly depleted molecular gas reservoirs in massive quiescent galaxies at z~1.5
• ALMA reveals extended cool gas and hot ionized outflows in a typical star-forming galaxy at $z=7.13$
• Measurements of the dust properties in z~1-3 SMGs with ALMA
• Molecular gas in z~6 quasar host galaxies
• The evolution of CNO elements in galaxies
• An ALMA Spectroscopic Survey of the Brightest Submillimeter Galaxies in the SCUBA-2-COSMOS field (AS2COSPEC): Survey Description and First Results
• Early results from GLASS-JWST XVI: Discovering a bluer z~4-7 Universe through UV slopes
• Sub-millimetre compactness as a critical dimension to understand the Main Sequence of star-forming galaxies
• The Evolving Interstellar Medium of Star-Forming Galaxies, as traced by $\text{Stardust}$
• The ALPINE-ALMA [CII] survey: Dust mass budget in the early Universe
• GOODS-ALMA 2.0: Starbursts in the main sequence reveal compact star formation regulating galaxy evolution prequenching
• No Redshift Evolution of Dust Temperatures from $0<z<2$
• The Structure of Massive Star-Forming Galaxies from JWST and ALMA: Dusty, High Redshift Disk Galaxies
• The ALMA REBELS Survey: The First Infrared Luminosity Function Measurement at $\mathbf{z \sim 7}
• Resolving a dusty, star-forming SHiZELS galaxy at z=2.2 with HST, ALMA and SINFONI on kiloparsec scales
• ALMA Lensing Cluster Survey: ALMA-Herschel Joint Study of Lensed Dusty Star-Forming Galaxies across $z\simeq 0.5-6$
• JWST CEERS probes the role of stellar mass and morphology in obscuring galaxies
• Sub-Millimetre Galaxies with Webb: Near-Infrared Counterparts and Multi-wavelength Morphology
• Close-up view of a luminous star-forming galaxy at z=2.95
• High Molecular-Gas to Dust Mass Ratios Predicted in Most Quiescent Galaxies
• A High-Resolution Investigation of the Multi-Phase ISM in a Galaxy during the First Two Billion Years
• The Bright Extragalactic ALMA Redshift Survey (BEARS) I: redshifts of bright gravitationally-lensed galaxies from the Herschel ATLAS
• PDFchem: A new fast method to determine ISM properties and infer environmental parameters using probability distributions
• [CII] halos in ALPINE galaxies: smoking-gun of galactic outflows?
• VLA Legacy Survey of Molecular Gas in Massive Star-forming Galaxies at High Redshift
• z-GAL -- A NOEMA spectroscopic redshift survey of bright Herschel galaxies: [I] Overview
• The ALMA-CRISTAL survey: Gas, dust, and stars in star-forming galaxies when the Universe was ~1 Gyr old I. Survey overview and case studies
• Submillimetre galaxies in two massive protoclusters at z = 2.24: witnessing the enrichment of extreme starbursts in the outskirts of HAE density peaks
• Atomic and molecular gas from the epoch of reionization down to redshift 2
• A solar metallicity galaxy at $z>$ 7? Possible detection of the [N II] 122 $\mu$m and [O III] 52 $\mu$m lines
• High-resolution ALMA study of CO (2-1) line and dust continuum emissions in cluster galaxies at z = 1.46
• Predicting sub-millimeter flux densities from global galaxy properties
• Unveiling the nature of 11 dusty star-forming galaxies at the peak of cosmic star formation history
• The GADOT Galaxy Survey: Dense Gas and Feedback in Herschel-Selected Starburst Galaxies at Redshifts 2 to 6
• The interplay between feedback, accretion, transport and winds in setting gas-phase metal distribution in galaxies
• The ALMA REBELS Survey: Discovery of a massive, highly star-forming and morphologically complex ULIRG at $z=7.31$
• z-GAL -- A NOEMA spectroscopic redshift survey of bright Herschel galaxies: [II] Dust properties
• Metal and dust evolution in ALMA REBELS galaxies: insights for future JWST observations
• JWST's PEARLS: TN J1338-1942 -- I. Extreme jet triggered star-formation in a $z=4.11$ luminous radio galaxy
• ALMACAL IX: multi-band ALMA survey for dusty star-forming galaxies and the resolved fractions of the cosmic infrared background
• PRUSSIC I - a JVLA survey of HCN/HCO+/HNC (1-0) emission in z$\sim$3 dusty galaxies: Low dense-gas fractions in high-redshift star-forming galaxies
• Rise of the Titans: Gas Excitation and Feedback in a Binary Hyper-Luminous Dusty Starburst Galaxy at z~6
• The JCMT SCUBA-2 Survey of the James Webb Space Telescope North Ecliptic Pole Time-Domain Field
• ALMA 1.3 mm Survey of Lensed Submillimeter Galaxies (SMGs) Selected by Herschel: Discovery of Spatially Extended SMGs and Implications
• z-GAL -- A NOEMA spectroscopic redshift survey of bright Herschel galaxies: [III] Physical properties
• NIKA2 Cosmological Legacy Survey: Survey Description and Galaxy Number Counts
• Extreme Variation in Star Formation Efficiency Across a Compact, Starbursting Disk Galaxy
• Resolved CO(1-0) emission and gas properties in luminous dusty star forming galaxies at z=2-4
• An ultra-deep multi-band VLA survey of the faint radio sky (COSMOS-XS): New constraints on the cosmic star formation history
• The observed cosmic star formation rate density has an evolution which resembles a Γ(a, bt) distribution and can be described successfully by only 2 parameters
• SUNRISE: The rich molecular inventory of high-redshift dusty galaxies revealed by broadband spectral line surveys
• Gravitational lensing in LoTSS DR2 -- Extremely faint 144-MHz radio emission from two highly magnified quasars
• Dust Properties of 870 Micron Selected Galaxies in the GOODS-S
• Estimating Dust Temperature and Far-IR Luminosity of High-Redshift Galaxies using ALMA Single-Band Continuum Observations
• Where infall meets outflows: turbulent dissipation probed by CH${}^{+}$ and Ly$\alpha$ in the starburst/AGN galaxy group SMM J02399$-$0136 at z$\sim$2.8
• Large gas inflow driven by a matured galactic bar in the early Universe
• The ALMA-CRISTAL survey: Dust temperature and physical conditions of the interstellar medium in a typical galaxy at z=5.66
• COLDz: Probing Cosmic Star Formation With Radio Free-free Emission
• Diagnosing the interstellar medium of galaxies with far-infrared emission lines II. [C II], [O I], [O III], [N II] and [N III] up to z=6
• The ALPINE-ALMA [CII] Survey: Dust emission effective radius up to 3 kpc in the Early Universe
• ALMACAL VIII: A pilot survey for untargeted extragalactic CO emission lines in deep ALMA calibration data
• Updated measurements of [O III] 88 $\mu$m, [C II] 158 $\mu$m, and Dust Continuum Emission from a z=7.2 Galaxy
• 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
• ASW${}^2$DF: Census of the obscured star formation in a galaxy cluster in formation at $z=2.2$
• Tracing the evolutionary pathways of dust and cold gas in high-z quiescent galaxies with SIMBA
• Spectroscopic confirmation of a gravitationally lensed Lyman break galaxy at z${}_{[CII]}$ = 6.827 using NOEMA
• ALMACAL. XI. Over-densities as signposts to proto-clusters? A cautionary tale
• Molecular gas budget and characterization of intermediate-mass star-forming galaxies at $z\approx 2-3$
• Effects of dust sources on dust attenuation properties in IllustrisTNG galaxies at $z\sim 7$
• GalaPy, the highly optimised C++/Python spectral modelling tool for galaxies -- I. Library presentation and photometric fitting
• The mass-dependent UVJ diagram at cosmic noon: A challenge for galaxy evolution models and dust radiative transfer
• The ALMA Frontier Fields Survey. VI. Lensing-corrected 1.1mm number counts in Abell 2744, MACSJ0416.1-2403, MACSJ1149.5+2223, Abell 370 and Abell S1063
• A nuclear spiral in a dusty star-forming galaxy at $z=2.78$
• The [C II] line emission as an interstellar medium probe in the MARIGOLD galaxies
• $\text{slick}$: Modeling a Universe of Molecular Line Luminosities in Hydrodynamical Simulations
• A Large Molecular Gas Reservoir in the Protocluster SPT2349$-$56 at $z=4.3$
• Potential contributions of Pop III and intermediate-mass Pop II stars to cosmic chemical enrichment
• PRUSSIC II -- ALMA imaging of dense-gas tracers in SDP.81: Evidence for low mechanical heating and a sub-solar metallicity in a z=3.04 dusty galaxy
• Ultra-faint [CII] emission in a redshift = 2 gravitationally-lensed metal-poor dwarf galaxy
• ALMACAL XIII. Evolution of the CO luminosity function and the molecular gas mass density out to $z$ ~ 6
• The ALPINE-ALMA [CII] Survey: Unveiling the baryon evolution in the ISM of $z\sim 5$ star-forming galaxies
• CO(1--0) imaging reveals 10-kiloparsec molecular gas reservoirs around star-forming galaxies at high redshift
• DESHIMA 2.0: Rapid redshift surveys and multi-line spectroscopy of dusty galaxies
• Molecular gas in a gravitationally lensed galaxy group at $z=2.9$
• Water emission tracing active star formation from the Milky Way to high-$z$ galaxies
• Resolving a merger in a hyper-luminous submillimeter galaxy at z=2.82
• Millimeter-wave observations of Euclid Deep Field South using the South Pole Telescope: A data release of temperature maps and catalogs
• PRUSSIC III -- ALMA and NOEMA survey of dense gas in high-redshift star-forming galaxies
• Internal structure of molecular gas in a main sequence galaxy with a UV clump at z = 1.45
• JWST reveals extended stellar disks for ALMA-bright dusty star-forming galaxies in the Spiderweb protocluster
• Vz-GAL: Probing Cold Molecular Gas in Dusty Star-forming Galaxies at z=1-6
• Bright [CII]158$\mu$m Streamers as a Beacon for Giant Galaxy Formation in SPT2349$-$56 at $z=4.3$
• A High-resolution Far-infrared Survey to Probe Black Hole-Galaxy Co-evolution
• ALMA discovery of Punctum -- a highly polarized mm source in nuclear starburst galaxy NGC 4945
• A PAH deficit in the starburst core of a distant spiral galaxy
• Simultaneously Modelling Dusty Star Forming Galaxies and Massive Quiescents: A Calibration Framework for Galaxy Formation Models
• ADF22+: a declining faint end in the far-infrared luminosity function in the SSA22 protocluster at z=3.09
• ALMA Lensing Cluster Survey: Dust mass measurements as a function of redshift, stellar-mass and star formation rate, from z=1 to z=5
• 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
• Direct detection of cool molecular gas in a star-forming galaxy at $z=7.31$
• Do Unusually Cold Starburst Galaxies Exist? A Case Study
• Candidate cosmic filament in the GJ526 field, mapped with the NIKA2 camera
• A scaling relation in [C II]-detected galaxies and its likely application in cosmology
• First Light And Reionisation Epoch Simulations (FLARES) III: The properties of massive dusty galaxies at cosmic dawn
• The ALMA View of High-Redshift Galaxy Formation
• Extensive Lensing Survey of Optical and Near-Infrared Dark Objects (El Sonido): HST H-Faint Galaxies behind 101 Lensing Clusters
• The NIKA2 cosmological legacy survey at 2 mm: catalogs, colors, redshift distributions, and implications for deep surveys
• Kiloparsec-scale imaging of the CO(1-0)-traced cold molecular gas reservoir in a z~3.4 submillimeter galaxy