A deep ALMA image of the Hubble Ultra Deep Field

Abstract

We present the results of the first, deep ALMA imaging covering the full 4.5 sq arcmin of the Hubble Ultra Deep Field (HUDF) as previously imaged with WFC3/IR on HST. Using a mosaic of 45 pointings, we have obtained a homogeneous 1.3mm image of the HUDF, achieving an rms sensitivity of 35 microJy, at a resolution of 0.7 arcsec. From an initial list of ~50 >3.5sigma peaks, a rigorous analysis confirms 16 sources with flux densities S(1.3) > 120 microJy. All of these have secure galaxy counterparts with robust redshifts (<z> = 2.15), and 12 are also detected at 6GHz in new deep JVLA imaging. Due to the wealth of supporting data in this unique field, the physical properties of the ALMA sources are well constrained, including their stellar masses (M*) and UV+FIR star-formation rates (SFR). Our results show that stellar mass is the best predictor of SFR in the high-z Universe; indeed at z > 2 our ALMA sample contains 7 of the 9 galaxies in the HUDF with M* > 2 x 10^10 Msun and we detect only one galaxy at z > 3.5, reflecting the rapid drop-off of high-mass galaxies with increasing redshift. The detections, coupled with stacking, allow us to probe the redshift/mass distribution of the 1.3-mm background down to S(1.3) ~ 10 micro-Jy. We find strong evidence for a steep `main sequence' for star-forming galaxies at z ~ 2, with SFR \propto M* and a mean specific SFR = 2.2 /Gyr. Moreover, we find that ~85% of total star formation at z ~ 2 is enshrouded in dust, with ~65% of all star formation at this epoch occurring in high-mass galaxies (M* > 2 x 10^10 Msun), for which the average obscured:unobscured SF ratio is ~200. Finally, we combine our new ALMA results with the existing HST data to revisit the cosmic evolution of star-formation rate density; we find that this peaks at z ~ 2.5, and that the star-forming Universe transits from primarily unobscured to primarily obscured thereafter at z ~ 4.

26 pages, 15 figures, updated to match version accepted for publication in MNRAS

References in corpus (37)

• Cosmic Star Formation History
• 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
• A Highly Consistent Framework for the Evolution of the Star-Forming "Main Sequence" from z~0-6
• UV Luminosity Functions at redshifts z~4 to z~10: 10000 Galaxies from HST Legacy Fields
• 3D-HST WFC3-selected Photometric Catalogs in the Five CANDELS/3D-HST Fields: Photometry, Photometric Redshifts and Stellar Masses
• The Hubble Ultra Deep Field
• Constraining the Low-Mass Slope of the Star Formation Sequence at 0.5<z<2.5
• The Herschel view of the dominant mode of galaxy growth from z=4 to the present day
• An Objective Definition for the Main Sequence of Star-Forming Galaxies
• A dusty, normal galaxy in the epoch of reionization
• Mid-Infrared Spectral Diagnosis of Submillimeter Galaxies
• Faint AGNs at z>4 in the CANDELS GOODS-S field: looking for contributors to the reionization of the Universe
• The 0.4 < z < 1.3 star formation history of the Universe as viewed in the far-infrared
• The SCUBA HAlf Degree Extragalactic Survey (SHADES) - III. Identification of radio and mid-infrared counterparts to submillimetre galaxies
• An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: High resolution 870um source counts
• The SCUBA-2 Cosmology Legacy Survey: ALMA resolves the rest-frame far-infrared emission of sub-millimeter galaxies
• AzTEC Millimetre Survey of the COSMOS Field: I. Data Reduction and Source Catalogue
• ALMA Imaging and Gravitational Lens Models of South Pole Telescope-Selected Dusty, Star-Forming Galaxies at High Redshifts
• Star Formation at $4<z<6$ From the Spitzer Large Area Survey with Hyper-Suprime-Cam (SPLASH)
• The SCUBA-2 Cosmology Legacy Survey: ALMA resolves the bright-end of the sub-millimeter number counts
• Over half of the far-infrared background light comes from galaxies at z >= 1.2
• Deep U band and R imaging of GOODS-South: Observations,data reduction and first results
• New redshift z ~ 9 galaxies in the Hubble Frontier Fields: Implications for early evolution of the UV luminosity density
• VLA and ALMA Imaging of Intense, Galaxy-Wide Star Formation in z ~ 2 Galaxies
• The VLA 1.4GHz Survey of the Extended Chandra Deep Field South: First Data Release
• The Hawk-I UDS and GOODS Survey (HUGS): Survey design and deep K-band number counts
• The SCUBA-2 Cosmology Legacy Survey: the nature of bright submm galaxies from 2 deg2 of 850-um imaging
• The SCUBA HAlf Degree Extragalactic Survey (SHADES) - IV: Radio-mm-FIR photometric redshifts
• The VLA Survey of the Chandra Deep Field South: I. Overview of the Radio Data
• Evolution of cosmic star formation in the SCUBA-2 Cosmology Legacy Survey
• A systematic search for very massive galaxies at z > 4
• A combined re-analysis of existing blank-field SCUBA surveys: comparative 850-micron source lists, combined number counts, and evidence for strong clustering of the bright sub-mm galaxy population
• SXDF-ALMA 2 arcmin${}^2$ Deep Survey: 1.1-mm Number Counts
• A WFC3 Grism Emission Line Redshift Catalog in the GOODS-South Field
• A Deep 1.2 mm Map of the Lockman Hole North Field
• The SCUBA-2 Cosmology Legacy Survey: the submillimetre properties of Lyman break galaxies at z=3-5
• The Mass Distribution of the Strong Lensing Cluster SDSS J1531+3414

Cited by in corpus (285)

• PHIBSS: Unified Scaling Relations of Gas Depletion Time and Molecular Gas Fractions
• The Evolution of the Star-forming Interstellar Medium across Cosmic Time
• The MUSE Hubble Ultra Deep Field Survey: I. Survey description, data reduction and source detection
• The Main Sequence of star-forming galaxies across cosmic times
• Full-Data Results of Hubble Frontier Fields: UV Luminosity Functions at $z\sim 6-10$ and a Consistent Picture of Cosmic Reionization
• An ALMA survey of the SCUBA-2 CLS UDS field: Physical properties of 707 Sub-millimetre Galaxies
• The dust content of galaxies from z = 0 to z = 9
• The ALPINE-ALMA [CII] Survey: data processing, catalogs, and statistical source properties
• "Big Three Dragons": a z = 7.15 Lyman BreakGalaxy Detected in [OIII] 88 $\mu$m, [CII] 158 $\mu$m, and Dust Continuum with ALMA
• The [C II] emission as a molecular gas mass tracer in galaxies at low and high redshift
• Galaxy Formation and Reionization: Key Unknowns and Expected Breakthroughs by the James Webb Space Telescope
• The HDUV Survey: A Revised Assessment of the Relationship between UV Slope and Dust Attenuation for High-Redshift Galaxies
• Rotation in [CII]-emitting gas in two galaxies at a redshift of 6.8
• The Star Formation Main Sequence in the Hubble Space Telescope Frontier Fields
• The VANDELS survey: the star-formation histories of massive quiescent galaxies at 1.0 < z < 1.3
• High-redshift star formation in the ALMA era
• The ALPINE-ALMA [CII] Survey: The nature, luminosity function and star formation history of dusty galaxies up to z~6
• An extreme proto-cluster of luminous dusty starbursts in the early Universe
• "Super-deblended" Dust Emission in Galaxies: II. Far-IR to (sub)millimeter photometry and high redshift galaxy candidates in the full COSMOS field
• The extragalactic background light revisited and the cosmic photon-photon opacity
• The Constant Average Relationship between Dust-obscured Star Formation and Stellar Mass from $z=0$ to $z=2.5$
• The Evolution of the IR Luminosity Function and Dust-obscured Star Formation in the Last 13 Billion Years
• JADES NIRSpec Initial Data Release for the Hubble Ultra Deep Field: Redshifts and Line Fluxes of Distant Galaxies from the Deepest JWST Cycle 1 NIRSpec Multi-Object Spectroscopy
• Starbursts in and out of the star-formation main sequence
• The ALMA Spectroscopic Survey in the HUDF: CO luminosity functions and the molecular gas content of galaxies through cosmic history
• The VLA-COSMOS 3 GHz Large Project: The cosmic star formation history since z~5
• "Super-deblended" Dust Emission in Galaxies: I. The GOODS-North Catalog and the Cosmic Star Formation Rate Density out to Redshift 6
• Galaxy Stellar Mass Functions from z~10 to z~6 using the Deepest Spitzer/IRAC Data: No Significant Evolution in the Stellar-to-Halo Mass Ratio of Galaxies in the First Gyr of Cosmic Time
• ALMA spectroscopic survey in the Hubble Ultra Deep Field: Continuum number counts, resolved 1.2-mm extragalactic background, and properties of the faintest dusty star forming galaxies
• Evolution of the UV LF from z~15 to z~8 Using New JWST NIRCam Medium-Band Observations over the HUDF/XDF
• The Hubble Legacy Field GOODS-S Photometric Catalog
• The ALPINE-ALMA [CII] Survey: Multi-Wavelength Ancillary Data and Basic Physical Measurements
• ALMA uncovers the [CII] emission and warm dust continuum in a z = 8.31 Lyman break galaxy
• Kiloparsec-scale gaseous clumps and star formation at $z=5-7$
• The ALMA Spectroscopic Survey Large Program: The Infrared Excess of z=1.5-10 UV-selected Galaxies and the Implied High-Redshift Star Formation History
• Main sequence of star forming galaxies beyond the Herschel confusion limit
• Extended ionised and clumpy gas in a normal galaxy at z=7.1 revealed by ALMA
• On the dust temperatures of high redshift galaxies
• First Identification of 10-kpc Scale [CII] 158um Halos around Star-Forming Galaxies at z=5-7
• VLA and ALMA Imaging of Intense, Galaxy-Wide Star Formation in z ~ 2 Galaxies
• An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: Spectroscopic redshifts
• The SCUBA-2 Cosmology Legacy Survey: Multi-wavelength Properties of ALMA-identified Submillimeter Galaxies in UKIDSS-UDS
• Dust attenuation in 2<z<3 star-forming galaxies from deep ALMA observations of the Hubble Ultra Deep Field
• The Brightest Galaxies in the Dark Ages: Galaxies' Dust Continuum Emission During the Reionization Era
• Dust attenuation, dust emission, and dust temperature in galaxies at z>=5: a view from the FIRE-2 simulations
• The VANDELS ESO public spectroscopic survey
• An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: Source catalogue and properties
• Molecular gas in the Herschel-selected strongly lensed submillimeter galaxies at z~2-4 as probed by multi-J CO lines
• The ALMA REBELS Survey: Dust Continuum Detections at z > 6.5
• The ALMA Spectroscopic Survey in the HUDF: CO Excitation and Atomic Carbon in Star-Forming Galaxies at $z=1-3$
• The MUSE Hubble Ultra Deep Field surveys: Data release II
• Semi-analytic forecasts for JWST -- II. physical properties and scaling relations for galaxies at z = 4-10
• 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
• z~2-9 Galaxies Magnified by the Hubble Frontier Field Clusters II: Luminosity Functions and Constraints on a Faint-End Turnover
• Discovery of a dark, massive, ALMA-only galaxy at z~5-6 in a tiny 3-millimeter survey
• The IRX-Beta Dust Attenuation Relation in Cosmological Galaxy Formation Simulations
• The SCUBA-2 Cosmology Legacy Survey: the nature of bright submm galaxies from 2 deg2 of 850-um imaging
• The Lyman-alpha luminosity function at z=5.7-6.6 and the steep drop of the faint end: implications for reionization
• The ALMA Spectroscopic Survey in the HUDF: Multi-band constraints on line luminosity functions and the cosmic density of molecular gas
• Alma Twenty-six Arcmin^2 Survey Of Goods-s At One-millimeter (asagao): Source Catalog And Number Counts
• The ALMA REBELS Survey: The Dust-obscured Cosmic Star Formation Rate Density at Redshift 7
• ALMA reveals metals yet no dust within multiple components in CR7
• Jekyll & Hyde: quiescence and extreme obscuration in a pair of massive galaxies 1.5 Gyr after the Big Bang
• Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) VIII. A less biased view of the early co-evolution of black holes and host galaxies
• The ALPINE-ALMA [CII] Survey: Obscured Star Formation Rate Density and Main Sequence of star-forming galaxies at z>4
• CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope
• 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
• Star formation in galaxies at z~4-5 from the SMUVS survey: a clear starburst/main-sequence bimodality for Halpha emitters on the SFR-M* plane
• Colours, Star formation Rates, and Environments of Star forming and Quiescent Galaxies at the Cosmic Noon
• An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: number counts of submillimeter galaxies
• Carbonaceous dust grains seen in the first billion years of cosmic time
• Detailed dust modelling in the L-Galaxies semi-analytic model of galaxy formation
• ALMA [CII] detection of a redshift 7 lensed galaxy behind RXJ1347.1-1145
• The ALMA Spectroscopic Survey in the HUDF: CO emission lines and 3 mm continuum sources
• An ALMA survey of the brightest sub-millimetre sources in the SCUBA-2 COSMOS field
• Predictions for the spatial distribution of the dust continuum emission in 1<z<5 star-forming galaxies
• The LOFAR Two-metre Sky Survey Deep Fields Data Release 1: V. Survey description, source classifications and host galaxy properties
• GOODS-ALMA 2.0: Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxies
• Timing the earliest quenching events with a robust sample of massive quiescent galaxies at 2 < z < 5
• The evolving far-IR galaxy luminosity function and dust-obscured star-formation rate density out to z~5
• A Submillimeter Perspective on the GOODS Fields (SUPER GOODS) - I. An Ultradeep SCUBA-2 Survey of the GOODS-N
• A kiloparsec view of a typical star-forming galaxy when the Universe was ~1 Gyr old. Part I. Outflow, halo, and interstellar medium properties
• Evolution of cosmic star formation in the SCUBA-2 Cosmology Legacy Survey
• The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Evolution of the molecular gas in CO-selected galaxies
• Obscured star-formation in bright z ~ 7 Lyman-break galaxies
• ALMA 200-parsec Resolution Imaging of Smooth Cold Dusty Disks in Typical $z\sim 3$ Star-Forming Galaxies
• Cold dust and stellar emissions in dust-rich galaxies observed with ALMA: a challenge for SED-fitting techniques
• The ALMA Spectroscopic Survey in the HUDF: Deep 1.2 mm continuum number counts
• The Dramatic Size and Kinematic Evolution of Massive Early-Type Galaxies
• The First Billion Years project: constraining the dust attenuation law of star-forming galaxies at z $\simeq$ 5
• The nature of sub-millimeter and highly star-forming galaxies in the EAGLE simulation
• Mapping Obscuration to Reionization with ALMA (MORA): 2mm Efficiently Selects the Highest-Redshift Obscured Galaxies
• Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) III. Star formation properties of the host galaxies at $z\gtrsim 6$ studied with ALMA
• ALMA twenty-six arcmin${}^2$ survey of GOODS-S at one-millimeter (ASAGAO): Near-infrared-dark faint ALMA sources
• An ALMA survey of the S2CLS UDS field: Optically invisible submillimetre galaxies
• Illuminating the dark side of cosmic star formation two billion years after the Big Bang
• A Submillimeter Perspective on the GOODS Fields (SUPER GOODS). III. A Large Sample of ALMA Sources in the GOODS-S
• The ALMA Spectroscopic Survey in the HUDF: The Cosmic Dust and Gas Mass Densities in Galaxies up to $z\sim 3$
• The ALMA Redshift 4 Survey (AR4S): I. The massive end of the z=4 main sequence of galaxies
• Planck's dusty GEMS. VI. Multi-J CO excitation and interstellar medium conditions in dusty starburst galaxies at z=2-4
• The ionising photon production efficiency at z~6 for Lyman-alpha emitters using JEMS and MUSE
• The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The nature of the faintest dusty star-forming galaxies
• Significant Dust-Obscured Star Formation in Luminous Lyman-break Galaxies at $z$$\sim$$7$$-$$8$
• ALMA Lensing Cluster Survey: $HST$ and $Spitzer$ Photometry of 33 Lensed Fields Built with CHArGE
• The ALMA Spectroscopic Survey in the HUDF: Nature and physical properties of gas-mass selected galaxies using MUSE spectroscopy
• The SCUBA-2 Cosmology Legacy Survey: The EGS deep field I - Deep number counts and the redshift distribution of the recovered Cosmic Infrared Background at 450 and 850 um
• Knocking on giants' doors: I. The evolution of the dust-to-stellar mass ratio in distant dusty galaxies
• CO emission in distant galaxies on and above the main sequence
• SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES): Faint-End Counts at 450 um
• 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 ($n\simeq 1$)
• ALMA view of a massive spheroid progenitor: a compact rotating core of molecular gas in an AGN host at z=2.226
• The discovery of rest-frame UV colour gradients and a diversity of dust morphologies in bright z ~ 7 Lyman-break galaxies
• The Dust Attenuation of Star-forming Galaxies at $z\sim 3$ and Beyond: New Insights from ALMA Observations
• ALMA reveals extended cool gas and hot ionized outflows in a typical star-forming galaxy at $z=7.13$
• Merging Rates of Compact Binaries in Galaxies: Perspectives for Gravitational Wave Detections
• On the Gas Content, Star Formation Efficiency, and Environmental Quenching of Massive Galaxies in Proto-Clusters at z~2.0-2.5
• UVI colour gradients of 0.4<z<1.4 star-forming main sequence galaxies in CANDELS: dust extinction and star formation profiles
• High Equivalent Width of Hα+[N II] Emission in z~8 Lyman-break Galaxies from IRAC 5.8μm Observations: Evidence for Efficient Lyman-continuum Photon production in the Epoch of Re-ionization
• EGG: hatching a mock Universe from empirical prescriptions
• A${}^3$COSMOS: The Dust Attenuation of Star-Forming Galaxies at $z=2.5-4.0$ from the COSMOS-ALMA Archive
• KASHz: No evidence for ionised outflows instantaneously suppressing star formation in moderate luminosity AGN at $z$$\sim$$1.4$-$2.6$
• A new estimate of the cosmic star formation density from a radio-selected sample, and the contribution of $H$-dark galaxies at $z\ge 3$
• GOODS-ALMA: The slow downfall of star-formation in $z$ = 2-3 massive galaxies
• Convergence of Lobatto-type Runge-Kutta methods for partitioned differential-algebraic systems of index 2
• GOODS-ALMA: 1.1 mm galaxy survey - I. Source catalogue and optically dark galaxies
• The missing light of the Hubble Ultra Deep Field
• A direct calibration of the IRX-β relation in Lyman-break Galaxies at z=3-5
• Molecular gas properties of a lensed star-forming galaxy at z~3.6: a case study
• The main sequence of star forming galaxies II. A non evolving slope at the high mass end
• Evolution of Galaxy Star Formation and Metallicity: Impact on Double Compact Objects Mergers
• Dust and gas content of high-redshift galaxies hosting obscured AGN in the CDF-S
• COALAS: I. ATCA CO(1-0) survey and luminosity function in the Spiderweb protocluster at z=2.16
• AstroSat detection of Lyman continuum emission from a z=1.42 galaxy
• The SCUBA-2 Cosmology Legacy Survey: The EGS deep field - II. Morphological transformation and multi-wavelength properties of faint submillimetre galaxies
• ALMA Twenty-six arcmin${}^2$ Survey of GOODS-S at One-millimeter (ASAGAO): X-ray AGN Properties of Millimeter-Selected Galaxies
• Exploring galaxies-gravitational waves cross-correlations as an astrophysical probe
• An imperfectly passive nature: Bright sub-millimeter emission from dust-obscured star formation in the z=3.717 "passive" system, ZF20115
• The VANDELS survey: Dust attenuation in star-forming galaxies at $\mathbf{z}=3-4$
• New Analytic Solutions for Galaxy Evolution: Gas, Stars, Metals and Dust in local Early-Type Galaxies and in their high-z Starforming Progenitors
• Dust attenuation evolution in $z\sim 2$-$12$ JWST 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
• 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
• Constraining the volume density of Dusty Star-Forming Galaxies through the first 3mm Number Counts from ALMA
• CO, H2O, H2O+ line and dust emission in a z = 3.63 strongly lensed starburst merger at sub-kiloparsec scales
• Submillimetre galaxies in cosmological hydrodynamical simulations -- an opportunity for constraining feedback models
• The Far Infrared Emission of the First Massive Galaxies
• The ALMA REBELS Survey: The First Infrared Luminosity Function Measurement at $\mathbf{z \sim 7}
• Panchromatic SED modelling of spatially-resolved galaxies
• The Structure of Massive Star-Forming Galaxies from JWST and ALMA: Dusty, High Redshift Disk Galaxies
• A gravitationally-boosted MUSE survey for emission-line galaxies at z>~5 behind the massive cluster RCS 0224
• Dust Obscured Star Forming Galaxies in the Early Universe
• A Comparison of the Stellar, CO and Dust-Continuum Emission from Three, Star-Forming HUDF Galaxies at $z\sim 2$
• Resolving a dusty, star-forming SHiZELS galaxy at z=2.2 with HST, ALMA and SINFONI on kiloparsec scales
• The LOFAR Two-metre Sky Survey: the radio view of the cosmic star formation history
• The IRX-$\beta$ relation of high-redshift galaxies
• ALMA Lensing Cluster Survey: ALMA-Herschel Joint Study of Lensed Dusty Star-Forming Galaxies across $z\simeq 0.5-6$
• SCUBA-2 Ultra Deep Imaging Eao Survey (Studies) III: Multi-wavelength properties, luminosity functions and preliminary source catalog of 450-$\mu$m-selected galaxies
• GOODS-ALMA: Optically dark ALMA galaxies shed light on a cluster in formation at z = 3.5
• ALMA Deep Field in SSA22: Survey Design and Source Catalog of a 20 arcmin^2 Survey at 1.1mm
• JWST's PEARLS: A JWST/NIRCam view of ALMA sources
• A multi-wavelength de-blended Herschel view of the statistical properties of dusty star-forming galaxies across cosmic time
• A machine-learning method for identifying multi-wavelength counterparts of submillimeter galaxies: training and testing using AS2UDS and ALESS
• The ALMA Spectroscopic Survey in the HUDF: A model to explain observed 1.1 and 0.85 millimeter dust continuum number counts
• ALMA pin-points a strong over-density of U/LIRGs in the massive cluster XCS J2215 at z=1.46
• Molecular gas in distant galaxies from ALMA studies
• Intensity and anisotropies of the stochastic Gravitational Wave background from merging compact binaries in galaxies
• Blue Rest-Frame UV-Optical Colors in z~8 Galaxies from GREATS: Very Young Stellar Populations at ~650 Myr of Cosmic Time
• The ALMA Frontier Fields Survey - II. Multiwavelength Photometric analysis of 1.1mm continuum sources in Abell 2744, MACSJ0416.1-2403 and MACSJ1149.5+2223
• Nature of Faint Radio Sources in GOODS-North and GOODS-South Fields - I. Spectral Index and Radio-FIR Correlation
• 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
• ALMA Deep Field in SSA22: A near-infrared-dark submillimeter galaxy at z=4.0
• The ALMA-CRISTAL survey: Widespread dust-obscured star formation in typical star-forming galaxies at z=4-6
• The First Robust Constraints on the Relationship Between Dust-to-Gas Ratio and Metallicity in Luminous Star-forming Galaxies at High Redshift
• The evolution of the UV-to-mm extragalactic background light: evidence for a top-heavy initial mass function?
• ALMA Deep Field in SSA22: Blindly Detected CO Emitters and [CII] Emitter Candidates
• Strong stellar-driven outflows shape the evolution of galaxies at cosmic dawn
• 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
• X-shooting GRBs at high redshift: probing dust production history
• 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
• A Model Connecting Galaxy Masses, Star Formation Rates, and Dust Temperatures Across Cosmic Time
• Multi-wavelength properties of radio and machine-learning identified counterparts to submillimeter sources in S2COSMOS
• Modelling the M*-SFR relation at high redshift: untangling factors driving biases in the intrinsic scatter measurement
• Rapid build-up of the stellar content in the protocluster core SPT2349$-$56 at $z=4.3$
• Early Science with the Large Millimeter Telescope: Detection of dust emission in multiple images of a normal galaxy at $z>4$ lensed by a Frontier Fields cluster
• ALMA observations of a metal-rich damped Lyα absorber at z = 2.5832: evidence for strong galactic winds in a galaxy group
• A census of optically dark massive galaxies in the early Universe from magnification by lensing galaxy clusters
• JWST and ALMA imaging of dust-obscured, massive substructures in a typical $z\sim 3$ star-forming disk galaxy
• Using ALMA to resolve the nature of the early star-forming large-scale structure PLCK G073.4-57.5
• Stellar Mass Function of Active and Quiescent Galaxies via the Continuity Equation
• High-resolution ALMA study of CO (2-1) line and dust continuum emissions in cluster galaxies at z = 1.46
• GOODS-ALMA: Using IRAC and VLA to probe fainter millimeter galaxies
• Missing Giants: Predictions on Dust-Obscured Galaxy Stellar Mass Assembly Throughout Cosmic Time
• The ALMA Frontier Fields Survey - IV. Lensing-corrected 1.1 mm number counts in Abell 2744, MACSJ0416.1-2403 and MACSJ1149.5+2223
• Unveiling the nature of 11 dusty star-forming galaxies at the peak of cosmic star formation history
• The ALMA REBELS Survey: Discovery of a massive, highly star-forming and morphologically complex ULIRG at $z=7.31$
• Predicting sub-millimeter flux densities from global galaxy properties
• On the existence of bright IR galaxies at z>2: tension between Herschel and SCUBA-2 results?
• The ALMA Spectroscopic Survey in the HUDF: A Search for [CII] Emitters at $6\le z\le 8$
• ALMA 1.3 mm Survey of Lensed Submillimeter Galaxies (SMGs) Selected by Herschel: Discovery of Spatially Extended SMGs and Implications
• ALMACAL IX: multi-band ALMA survey for dusty star-forming galaxies and the resolved fractions of the cosmic infrared background
• The dust-to-gas mass ratio of luminous galaxies as a function of their metallicity at cosmic noon
• An ALMA view of 11 Dusty Star Forming Galaxies at the peak of Cosmic Star Formation History
• SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES) IV: Spatial clustering and halo masses of 450-$\mu$m-selected sub-millimeter galaxies
• The ALPINE-ALMA [CII] Survey: the population of [CII]-undetected galaxies and their role in the ${\mathrm{L}}_{[\mathrm{CII}]}$-SFR relation
• Probing the High-Redshift Universe with SPICA: Toward the Epoch of Reionization and Beyond
• A multi-wavelength study of a massive, active galaxy at $z\sim 2$: coupling the kinematics of the ionized and molecular gas
• A complete distribution of redshifts for sub-millimetre galaxies in the SCUBA-2 Cosmology Legacy Survey UDS field
• The intrinsic SFRF and sSFRF of galaxies: comparing SDSS observation with IllustrisTNG simulation
• z-GAL -- A NOEMA spectroscopic redshift survey of bright Herschel galaxies: [III] Physical properties
• Evolution of the Gas Mass Fraction of Progenitors to Today's Massive Galaxies: ALMA Observations in the CANDELS GOODS-S Field
• Gamma-ray Bursts and the Early Star-formation History
• JWST's PEARLS: resolved study of the stellar and dust components in starburst galaxies at cosmic noon
• Significant Molecular Gas Deficiencies in Star-forming Cluster Galaxies at $z\sim 1.4$
• An ultra-deep multi-band VLA survey of the faint radio sky (COSMOS-XS): New constraints on the cosmic star formation history
• Measuring the average molecular gas content of star-forming galaxies at $z=3-4$
• 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
• Tracing the evolution of dust obscured star-formation and accretion back to the reionisation epoch with SPICA
• Optical Transient from an Explosion Close to the Stellar Surface
• Is a top-heavy initial mass function needed to reproduce the submillimeter galaxy number counts?
• An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: Dust attenuation in high-redshift Lyman break Galaxies
• A minimal empirical model for the cosmic far-infrared background anisotropies
• A Submillimeter Perspective on the GOODS Fields (SUPER GOODS). IV. The Submillimeter Properties of X-ray Sources in the CDF-S
• ALMA resolves the first strongly-lensed Optical/NIR-dark galaxy
• Cospatial Star Formation and Supermassive Black Hole Growth in $z\sim 3$ Galaxies: Evidence for In-situ Co-evolution
• SXDF-ALMA 2-arcmin^2 Deep Survey: Stacking of Rest-Frame Near-Infrared Selected Objects
• A high redshift population of galaxies at the North Ecliptic Pole: unveiling the main sequence of dusty galaxies
• The LOFAR Two Metre Sky Survey Data Release 2: Probabilistic Spectral Source Classifications and Faint Radio Source Demographics
• ALMA 26 arcmin${}^2$ survey of GOODS-S at one-millimeter (ASAGAO): millimeter properties of stellar mass selected galaxies
• Deep Spitzer/IRAC Data for z~10 galaxies Reveal Blue Balmer Break Colors: Young Stellar Populations at ~500 Myr of Cosmic Time
• 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
• Maximising the power of deep extragalactic imaging surveys with the James Webb Space Telescope
• The ALPINE-ALMA [C II] survey: the luminosity function of serendipitous [C II] line emitters at $z\sim 5$
• PRIMER & JADES reveal an abundance of massive quiescent galaxies at 2 < z < 5
• The ALMA Frontier Fields survey V: ALMA Stacking of Lyman-Break Galaxies in Abell 2744, Abell 370, Abell S1063, MACSJ0416.1-2403 and MACSJ1149.5+2223
• ASW${}^2$DF: Census of the obscured star formation in a galaxy cluster in formation at $z=2.2$
• A deep radio view of the evolution of the cosmic star-formation rate density from a stellar-mass selected sample in VLA-COSMOS
• The slippery slope of dust attenuation curves: Correlation of dust attenuation laws with star-to-dust compactness up to z = 4
• Correct estimate of the probability of false detection of the matched filter in weak-signal detection problems. III (Peak distribution method versus the Gumbel distribution method)
• ALMACAL VII: First Interferometric Number Counts at 650 $\mu$m
• The far-infrared/radio correlation for a sample of strongly lensed dusty star-forming galaxies detected by Herschel
• GalaPy, the highly optimised C++/Python spectral modelling tool for galaxies -- I. Library presentation and photometric fitting
• ALMA Lensing Cluster Survey: A spectral stacking analysis of [CII] in lensed $z\sim 6$ galaxies
• Multi-band Optical and Near-infrared Properties of Faint Submillimeter Galaxies with Serendipitous ALMA Detections
• Multiwavelength dissection of a massive heavily dust-obscured galaxy and its blue companion at z $\sim$2
• Emergence of Galactic Morphologies at Cosmic Dawn: Input from Numerical Modeling
• A puzzling non-detection of [O III] and [C II] from a $z\approx 7.7$ galaxy observed with ALMA
• 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
• 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
• Local starburst conditions and formation of GRB 980425 / SN 1998bw within a collisional ring
• JWST PRIMER: A deep JWST study of all ALMA-detected galaxies in PRIMER COSMOS -- dust-obscured star-formation history back to z $\simeq$ 7
• 2mm Observations and the Search for High-Redshift Dusty Star-forming Galaxies
• Dynamical Properties of Molecular-forming Gas Clumps in Galaxies at the Epoch of Reionization
• Herschel and ALMA Observations of Massive SZE-selected Clusters
• The Hawaii SCUBA-2 Lensing Cluster Survey: Are Low-luminosity Submillimeter Galaxies Detected in the Rest-frame UV?
• Discovery of Radio Jets in Phoenix Galaxy Cluster Center
• The ALPINE-ALMA [CII] Survey: Unveiling the baryon evolution in the ISM of $z\sim 5$ star-forming galaxies
• Evolving beyond z=0: insights about the future of stars and the intergalactic medium
• A [CII]-158-micron Survey of DLA galaxies at z~4: Observations of Dense and Metal-Enriched Neutral Gas within the Circumgalactic Medium of Star-Forming Galaxies
• Exploring the multiband gravitational wave background with a semi-analytic galaxy formation model
• ALMA Lensing Cluster Survey: Properties of Millimeter Galaxies Hosting X-ray Detected Active Galactic Nuclei
• Modeling submillimeter galaxies in cosmological simulations: Contribution to the cosmic star formation density and predictions for future surveys
• Even redder than we knew: color and $A_{\mathrm{V}}$ evolution up to $z=2.5$ from JWST/NIRCam photometry
• Internal structure of molecular gas in a main sequence galaxy with a UV clump at z = 1.45
• Strength in Numbers: Red Galaxies Bolster the Cosmic Star Formation Rate Density at z > 3
• The JWST Emission Line Survey (JELS): The sizes and merger fraction of star-forming galaxies during the Epoch of Reionization
• Interrelations between Astrochemistry and Galactic Dynamics
• Tracing obscured galaxy build-up at high redshift using deep radio surveys
• SEMPER I. Radio Predictions for Star-Forming Galaxies at $0<z<5$
• Simultaneously Modelling Dusty Star Forming Galaxies and Massive Quiescents: A Calibration Framework for Galaxy Formation Models
• A mock redshift catalogue of the dusty star-forming galaxy population with intrinsic clustering and lensing for deep millimetre surveys
• Measuring the gas reservoirs in $10^8<$ M${}_{\star }<10^{11}$ M${}_{\odot }$ galaxies at $1\le z\le 3$
• Simulating infrared spectro-photometric surveys with a SPRITZ
• Evolution of the infrared luminosity function and its corresponding dust-obscured star formation rate density out to z~6
• Searching Far and Long I: Pilot ALMA 2mm Follow-up of Bright Dusty Galaxies as a Redshift Filter
• Extended H$\alpha$ over compact far-infrared continuum in dusty submillimeter galaxies -- Insights into dust distributions and star-formation rates at $z\sim 2$
• Astro2020 Science White Paper: Exploration and characterization of the earliest epoch of galaxy formation: beyond the re-ionization era
• A deep ALMA Band 3 survey of HDFS/MUSE3D: Survey description and initial results
• The ALMA View of High-Redshift Galaxy Formation
• The Evolution of the SFR-M_* relation at 0.1<z<4: Environmental and Morphological Dependencies
• Spatial disconnection between stellar and dust emissions: the test of the Antennae Galaxies (Arp 244)
• The NIKA2 cosmological legacy survey at 2 mm: catalogs, colors, redshift distributions, and implications for deep surveys
• Implications of the cosmological 21-cm absorption profile for high-redshift star formation and deep JWST surveys
• The interstellar medium content of galaxies in the ALMA era
• Near-IR Spectroscopic Studies of Galaxies at z~1-3