The ALPINE-ALMA [CII] Survey: data processing, catalogs, and statistical source properties

Abstract

The ALPINE-ALMA large program targets the [CII] 158 $\mu$m line and the far-infrared continuum in 118 spectroscopically confirmed star-forming galaxies between z=4.4 and z=5.9. It represents the first large [CII] statistical sample built in this redshift range. We present details of the data processing and the construction of the catalogs. We detected 23 of our targets in the continuum. To derive accurate infrared luminosities and obscured star formation rates, we measured the conversion factor from the ALMA 158 $\mu$m rest-frame dust continuum luminosity to the total infrared luminosity (L${}_{\mathrm{IR}}$) after constraining the dust spectral energy distribution by stacking a photometric sample similar to ALPINE in ancillary single-dish far-infrared data. We found that our continuum detections have a median L${}_{\mathrm{IR}}$ of 4.4$\times 10^{11}$ L${}_{\odot }$. We also detected 57 additional continuum sources in our ALMA pointings. They are at lower redshift than the ALPINE targets, with a mean photometric redshift of 2.5$\pm$0.2. We measured the 850 $\mu$m number counts between 0.35 and 3.5 mJy, improving the current interferometric constraints in this flux density range. We found a slope break in the number counts around 3 mJy with a shallower slope below this value. More than 40 % of the cosmic infrared background is emitted by sources brighter than 0.35 mJy. Finally, we detected the [CII] line in 75 of our targets. Their median [CII] luminosity is 4.8$\times$10${}^8$ L${}_{\odot }$ and their median full width at half maximum is 252 km/s. After measuring the mean obscured SFR in various [CII] luminosity bins by stacking ALPINE continuum data, we find a good agreement between our data and the local and predicted SFR-L${}_{[\mathrm{CII}]}$ relations of De Looze et al. (2014) and Lagache et al. (2018).

44 pages, 29 figures, 14 tables, accepted by A&A, ALPINE products released at https://cesam.lam.fr/a2c2s/, luminosities in table B2 corrected

References in corpus (114)

• Astropy: A Community Python Package for Astronomy
• Cosmic Star Formation History
• Binary companions of evolved stars in APOGEE DR14: Search method and catalog of ~5,000 companions
• Herschel Space Observatory - An ESA facility for far-infrared and submillimetre astronomy
• CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey
• CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey - The Hubble Space Telescope Observations, Imaging Data Products and Mosaics
• The COSMOS2015 Catalog: Exploring the 1<z<6 Universe with half a million galaxies
• GOODS-Herschel: an infrared main sequence for star-forming galaxies
• Cool Gas in High Redshift Galaxies
• The Structure and Kinematics of the Circum-Galactic Medium from Far-UV Spectra of z~2-3 Galaxies
• The Herschel view of the dominant mode of galaxy growth from z=4 to the present day
• The Herschel Multi-tiered Extragalactic Survey: HerMES
• The 3D-HST Survey: Hubble Space Telescope WFC3/G141 grism spectra, redshifts, and emission line measurements for $\sim 100,000$ galaxies
• A Dust-Obscured Massive Maximum-Starburst Galaxy at a Redshift of 6.34
• The Evolving Interstellar Medium of Star Forming Galaxies Since z=2 as Probed by Their Infrared Spectral Energy Distributions
• The Cosmic Infrared Background Resolved by Spitzer. Contributions of Mid-Infrared Galaxies to the Far-Infrared Background
• PACS Evolutionary Probe (PEP) - A Herschel Key Program
• The Interstellar Medium In Galaxies Seen A Billion Years After The Big Bang
• The applicability of FIR fine-structure lines as Star Formation Rate tracers over wide ranges of metallicities and galaxy types
• Evidence of strong quasar feedback in the early Universe
• The Herschel PEP/HerMES Luminosity Function. I: Probing the Evolution of PACS selected Galaxies to z~4
• The SCUBA HAlf Degree Extragalactic Survey (SHADES) -- II. Submillimetre maps, catalogue and number counts
• A dusty, normal galaxy in the epoch of reionization
• A deep ALMA image of the Hubble Ultra Deep Field
• A 158 Micron [CII] Line Survey of Galaxies at z ~ 1 to 2: An Indicator of Star Formation in the Early Universe
• The VIMOS Ultra-Deep Survey: ~10,000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2<z<~6
• The SCUBA-2 Cosmology Legacy Survey: 850um maps, catalogues and number counts
• Evolution of the dust emission of massive galaxies up to z=4 and constraints on their dominant mode of star formation
• An ALMA [CII] survey of 27 quasars at z>5.94
• HerMES: The SPIRE confusion limit
• The Intense Starburst HDF850.1 in a Galaxy Overdensity at z=5.2 in the Hubble Deep Field
• ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Infrared Excess of UV-selected z=2-10 galaxies as a function of UV-continuum Slope and Stellar Mass
• An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: High resolution 870um source counts
• Explaining the [CII]158um Deficit in Luminous Infrared Galaxies - First Results from a Herschel/PACS Study of the GOALS Sample
• The evolution of the dust temperatures of galaxies in the SFR$-M_{\ast }$ plane up to $z$$\sim$$2$
• Herschel-ATLAS: Rapid evolution of dust in galaxies in the last 5 billion years
• ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Survey Description
• The [C II] emission as a molecular gas mass tracer in galaxies at low and high redshift
• A unified empirical model for infrared galaxy counts based on observed physical evolution of distant galaxies
• The DEIMOS 10k spectroscopic survey catalog of the COSMOS field
• HerMES: deep number counts at 250, 350, and 500 microns in the COSMOS and GOODS-N fields and the build-up of the cosmic infrared background
• Dust temperature and mid-to-total infrared color distributions for star-forming galaxies at 0<z<4
• How neutral is the intergalactic medium surrounding the redshift z=7.085 quasar ULAS J1120+0641?
• The ALPINE-ALMA [CII] Survey: The nature, luminosity function and star formation history of dusty galaxies up to z~6
• The [CII] 158 micron line emission in high-redshift galaxies
• On the [CII]-SFR relation in high redshift galaxies
• The impact of clustering and angular resolution on far-infrared and millimeter continuum observations
• The SCUBA-2 Cosmology Legacy Survey: ALMA resolves the bright-end of the sub-millimeter number counts
• Panchromatic spectral energy distributions of Herschel sources
• Characterisation of SCUBA-2 450um and 850um-selected Galaxies in the COSMOS Field
• Large Structures and Galaxy Evolution in COSMOS at z < 1.1
• The ALPINE-ALMA [CII] survey. Little to no evolution in the [CII]-SFR relation over the last 13 Gyr
• The ALPINE-ALMA [CII] survey: Star-formation-driven outflows and circumgalactic enrichment in the early Universe
• The nature of the [CII] emission in dusty star-forming galaxies from the SPT survey
• The evolving SFR-M_star relation and sSFR since z~5 from the VUDS spectroscopic survey
• 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
• The ALPINE-ALMA [CII] Survey: Multi-Wavelength Ancillary Data and Basic Physical Measurements
• Kiloparsec-scale gaseous clumps and star formation at $z=5-7$
• The Herschel census of infrared SEDs through cosmic time
• AzTEC millimeter survey of the COSMOS field - III. Source catalog over 0.72 sq. deg. and plausible boosting by large-scale structure
• The redshift distribution of dusty star forming galaxies from the SPT survey
• The ALPINE-ALMA [CII] Survey: Size of Individual Star-Forming Galaxies at z=4-6 and their Extended Halo Structure
• ISM properties of a Massive Dusty Star-Forming Galaxy discovered at z ~ 7
• Deep into the structure of the first galaxies: SERRA views
• ALMA Census of Faint 1.2 mm Sources Down to ~0.02 mJy: Extragalactic Background Light and Dust-Poor High-z Galaxies
• The SCUBA-2 Cosmology Legacy Survey: Multi-wavelength Properties of ALMA-identified Submillimeter Galaxies in UKIDSS-UDS
• The Brightest Galaxies in the Dark Ages: Galaxies' Dust Continuum Emission During the Reionization Era
• Dusty galaxies in the Epoch of Reionization: simulations
• Interpreting ALMA Observations of the ISM During the Epoch of Reionisation
• ALMA spectroscopic survey in the Hubble Ultra Deep Field: CO luminosity functions and the evolution of the cosmic density of molecular gas
• The ALPINE-ALMA [CII] survey: Dust attenuation properties and obscured star formation at z~4.4-5.8
• Recovering the systemic redshift of galaxies from their Lyman-alpha line profile
• The ALPINE-ALMA [CII] survey: Molecular gas budget in the Early Universe as traced by [CII]
• Molecular Gas in a Submillimeter Galaxy at z=4.5: Evidence for a Major Merger at 1 Billion Years after the Big Bang
• Are high redshift Galaxies hot? - Temperature of z > 5 Galaxies and Implications on their Dust Properties
• Kinematics of $z\ge 6$ galaxies from [CII] line emission
• A dusty star-forming galaxy at z=6 revealed by strong gravitational lensing
• A physical model for [CII] line emission from galaxies
• ALMACAL I: First dual-band number counts from a deep and wide ALMA submm survey, free from cosmic variance
• HerMES: ALMA Imaging of Herschel-selected Dusty Star-forming Galaxies
• Alma Twenty-six Arcmin^2 Survey Of Goods-s At One-millimeter (asagao): Source Catalog And Number Counts
• SIGAME simulations of the [CII], [OI] and [OIII] line emission from star forming galaxies at z ~ 6
• 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
• ALMA constraints on the faint millimetre source number counts and their contribution to the cosmic infrared background
• An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: number counts of submillimeter galaxies
• The ALMA Spectroscopic Survey in the HUDF: CO emission lines and 3 mm continuum sources
• Resolved UV and [CII] structures of luminous galaxies within the epoch of reionisation
• 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
• ALMA suggests outflows in z~5.5 galaxies
• Spatially unassociated galaxies contribute significantly to the blended submillimetre galaxy population: predictions for follow-up observations of ALMA sources
• Spectroscopic properties of luminous Lyman-α emitters at $z\approx 6-7$ and comparison to the Lyman-break population
• Physical Characterization of an Unlensed Dusty Star-Forming Galaxy at $z=5.85$
• The ALMA Frontier Fields survey I: 1.1 mm continuum detections in Abell 2744, MACSJ0416.1-2403 and MACSJ1149.5+2223
• Dust properties of Lyman break galaxies at $z\sim 3$
• ALMA detection of extended [CII] emission in Himiko at z=6.6
• The influence of wavelength, flux, and lensing selection effects on the redshift distribution of dusty, star-forming galaxies
• The Dust Attenuation of Star-forming Galaxies at $z\sim 3$ and Beyond: New Insights from ALMA Observations
• Rest-UV Absorption Lines as Metallicity Estimator: the Metal Content of Star-Forming Galaxies at z~5
• The history of star formation from the cosmic infrared background anisotropies
• Faint Submillimter Galaxy Counts at 450 micron
• The ALPINE-ALMA [CII] survey: Small Lya-[CII] velocity offsets in main-sequence galaxies at 4.4 < z < 6
• The Hawaii SCUBA-2 Lensing Cluster Survey: Number Counts and Submillimeter Flux Ratios
• The Redshift Evolution of Rest-UV Spectroscopic Properties to z~5
• The ALPINE-ALMA [CII] Survey: A Triple Merger at z~4.56
• The multiplicity of 250-$\mu$m Herschel sources in the COSMOS field
• Lyα emission from galaxies in the Epoch of Reionization
• The ALPINE-ALMA [CII] Survey: On the nature of an extremely obscured serendipitous galaxy
• Determination of the Cosmic Infrared Background from COBE/FIRAS and Planck HFI Observations
• A Model Connecting Galaxy Masses, Star Formation Rates, and Dust Temperatures Across Cosmic Time
• How to Find Variable Active Galactic Nuclei with Machine Learning
• On the existence of bright IR galaxies at z>2: tension between Herschel and SCUBA-2 results?
• Blending bias impacts the host halo masses derived from a cross-correlation analysis of bright sub-millimetre galaxies
• The Close AGN Reference Survey (CARS). Discovery of a global [CII] 158 $\mu$m line excess in AGN HE1353-1917

Cited by in corpus (173)

• GA-NIFS: A massive black hole in a low-metallicity AGN at $z\sim 5.55$ revealed by JWST/NIRSpec IFS
• Reionization Era Bright Emission Line Survey: Selection and Characterization of Luminous Interstellar Medium Reservoirs in the z>6.5 Universe
• 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
• Tracing the total molecular gas in galaxies: [CII] and the CO-dark gas
• The ALPINE-ALMA [CII] survey. Little to no evolution in the [CII]-SFR relation over the last 13 Gyr
• The REBELS ALMA Survey: cosmic dust temperature evolution out to z $\sim$ 7
• The ALPINE-ALMA [CII] survey: Dust attenuation properties and obscured star formation at z~4.4-5.8
• The ALPINE-ALMA [CII] survey: Molecular gas budget in the Early Universe as traced by [CII]
• 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 ALPINE-ALMA [CII] Survey: Obscured Star Formation Rate Density and Main Sequence of star-forming galaxies at z>4
• A kiloparsec view of a typical star-forming galaxy when the Universe was ~1 Gyr old. Part I. Outflow, halo, and interstellar medium properties
• Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XIII. Large-scale Feedback and Star Formation in a Low-Luminosity Quasar at z = 7.07 on the Local Black Hole to Host Mass Relation
• Accurate dust temperature determination in a $z=7.13$ galaxy
• The ALPINE-ALMA [CII] Survey: Kinematic Diversity & Rotation in Massive Star Forming Galaxies at z~4.4-5.9
• A wide field-of-view low-resolution spectrometer at APEX: instrument design and science forecast
• Reproducing sub-millimetre galaxy number counts with cosmological hydrodynamic simulations
• Illuminating the dark side of cosmic star formation two billion years after the Big Bang
• Dust temperature in ALMA $\hbox{[C $\scriptstyle\rm II $]}$-detected high-$z$ galaxies
• The VIMOS Ultra Deep Survey: The reversal of the star-formation rate $-$ density relation at $2<z<5$
• 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
• Dynamical characterization of galaxies up to $z\sim 7$
• The ALPINE-ALMA [CII] survey: The contribution of major mergers to the galaxy mass assembly at z~5
• The Nature of High ${[\mathrm{OIII}]}_{88\mu \mathrm{m}}$/${[\mathrm{CII}]}_{158\mu \mathrm{m}}$ Galaxies in the Epoch of Reionization: Low Carbon Abundance and a Top-Heavy IMF?
• ALMA Lensing Cluster Survey: Bright [CII] 158 $\mu$m Lines from a Multiply Imaged Sub-$L^{\star }$ Galaxy at $z=6.0719$
• CONCERTO: High-fidelity simulation of millimeter line emissions of galaxies and [CII] intensity mapping
• The gas and stellar content of a metal-poor galaxy at $z=8.496$ as revealed by JWST and ALMA
• 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
• A new estimate of the cosmic star formation density from a radio-selected sample, and the contribution of $H$-dark galaxies at $z\ge 3$
• The ALMA REBELS Survey: Efficient Ly$\alpha$ Transmission of UV-Bright z$\simeq$7 Galaxies from Large Velocity Offsets and Broad Line Widths
• Probing Cosmic Reionization and Molecular Gas Growth with TIME
• Ubiquitous Molecular Outflows in z > 4 Massive, Dusty Galaxies I. Sample Overview and Clumpy Structure in Molecular Outflows on 500pc Scales
• The Interstellar Medium of Quiescent Galaxies and its Evolution With Time
• The assembly of dusty galaxies at $z\ge 4$: the build-up of stellar mass and its scaling relations with hints from early JWST data
• COALAS: I. ATCA CO(1-0) survey and luminosity function in the Spiderweb protocluster at z=2.16
• An empirical representation of a physical model for the ISM [CII], CO, and [CI] emission at redshift $1\le z\le 9$
• The ALPINE-ALMA [CII] survey: Small Lya-[CII] velocity offsets in main-sequence galaxies at 4.4 < z < 6
• ALMA hints at the presence of turbulent disk galaxies at z > 5
• High [OIII]/[CII] surface brightness ratios trace early starburst galaxies
• A new look at the infrared properties of z $\sim$ 5 galaxies
• High redshift JWST predictions from IllustrisTNG: III. Infrared luminosity functions, obscured star formation and dust temperature of high-redshift galaxies
• The ALPINE-ALMA [CII] survey: Dust mass budget in the early Universe
• The Evolving Interstellar Medium of Star-Forming Galaxies, as traced by $\text{Stardust}$
• Impact of polarised extragalactic sources on the measurement of CMB B-mode anisotropies
• The ALMA REBELS Survey: The Cosmic HI Gas Mass Density in Galaxies at $z\approx 7$
• Multitracer cosmological line intensity mapping mock lightcone simulation
• The ALMA REBELS Survey: The First Infrared Luminosity Function Measurement at $\mathbf{z \sim 7}
• The early Universe was dust-rich and extremely hot
• The ALPINE-ALMA [C II] Survey: [C II]158micron Emission Line Luminosity Functions at $z\sim 4-6$
• Kinematics and Star Formation of High-Redshift Hot Dust-Obscured Quasars as Seen by ALMA
• The ALPINE-ALMA [CII] survey: dust attenuation curves at z=4.4-5.5
• Optical and mid-infrared line emission in nearby Seyfert galaxies
• [CII] line intensity mapping the epoch of reionization with the Prime-Cam on FYST
• The ALMA-CRISTAL survey: Widespread dust-obscured star formation in typical star-forming galaxies at z=4-6
• ALMA reveals a stable rotating gas disk in a paradoxical low-mass, ultra-dusty galaxy at z = 4.274
• No [CII] or dust detection in two Little Red Dots at z${}_{\mathrm{spec}}$ > 7
• Two Modes of LyC Escape From Bursty Star Formation: Implications for [C II] Deficits and the Sources of Reionization
• GA-NIFS: Multi-phase analysis of a star-forming galaxy at $z\sim 5.5$
• UNCOVERing the contribution of black holes to reionization in the JWST era
• [CII] halos in ALPINE galaxies: smoking-gun of galactic outflows?
• An extended [CII] halo around a massive star-forming galaxy at z = 5.3
• A${}^3$COSMOS and A${}^3$GOODSS: Continuum Source Catalogues and Multi-band Number Counts
• Rapid build-up of the stellar content in the protocluster core SPT2349$-$56 at $z=4.3$
• Star-formation driven outflows in local dwarf galaxies as revealed from [CII] observations by Herschel
• Chaotic and Clumpy Galaxy Formation in an Extremely Massive Reionization-Era Halo
• 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
• Probing cold gas in a massive, compact star-forming galaxy at z=6
• Simulating the infrared sky with a Spritz
• Constraints on the [CII] luminosity of a proto-globular cluster at z~6 obtained with ALMA
• The ALMA-CRISTAL Survey: Spatial extent of [CII] line emission in star-forming galaxies at $z=4-6$
• Synergising semi-analytical models and hydrodynamical simulations to interpret JWST data from the first billion years
• The ALMA REBELS Survey: Discovery of a massive, highly star-forming and morphologically complex ULIRG at $z=7.31$
• The ALMA-CRISTAL survey. Discovery of a 15 kpc-long gas plume in a $z=4.54$ Lyman-$\alpha$ blob
• ALMACAL IX: multi-band ALMA survey for dusty star-forming galaxies and the resolved fractions of the cosmic infrared background
• The Size and Pervasiveness of Ly$\alpha$-UV Spatial Offsets in Star-Forming Galaxies at $z\sim 6$
• The ALPINE-ALMA [CII] Survey: the population of [CII]-undetected galaxies and their role in the ${\mathrm{L}}_{[\mathrm{CII}]}$-SFR relation
• HYPERION. Coevolution of supermassive black holes and galaxies at $z>6$ and the build-up of massive galaxies
• Atomic and molecular gas as traced by [C II] emission
• To see or not to see a $z\sim 13$ galaxy, that is the question
• NIKA2 Cosmological Legacy Survey: Survey Description and Galaxy Number Counts
• Unveiling Luminous Ly$\alpha$ Emitters at $z\approx 6$ through JWST/NIRCam Imaging in the COSMOS Field
• Measuring the average molecular gas content of star-forming galaxies at $z=3-4$
• The COSMOS-Web ring: in-depth characterization of an Einstein ring lensing system at z~2
• High resolution spectral imaging of CO(7-6), [CI](2-1) and continuum of three high-z lensed dusty star-forming galaxies using ALMA
• A hide-and-seek game: Looking for Population III stars during the Epoch of Reionization through the HeII$\lambda$1640 line
• JWST PRIMER: A lack of outshining in four normal z =4-6 galaxies from the ALMA-CRISTAL Survey
• On estimating the cosmic molecular gas density from CO Line Intensity Mapping observations
• Dead or Alive? How Bursty Star Formation and Patchy Dust Can Cause Temporary Quiescence in High Redshift Galaxies
• Estimating Dust Temperature and Far-IR Luminosity of High-Redshift Galaxies using ALMA Single-Band Continuum Observations
• The ALMA-CRISTAL survey: Resolved kinematic studies of main sequence star-forming galaxies at 4<z<6
• The ALPINE-ALMA [CII] Survey: Investigation of 10 Galaxies at $z\sim 4.5$ with [OII] and [CII] Line Emission $-$ ISM Properties and [OII]$-$SFR Relation
• Multi-Phase ISM in the z = 5.7 Hyperluminous Starburst SPT0346-52
• Diagnosing the interstellar medium of galaxies with far-infrared emission lines I. The [C II] 158 microns line at z~0
• The cold interstellar medium of a normal sub-$L^{\star }$ galaxy at the end of reionization
• ColdSIM predictions of [C II] emission in primordial galaxies
• The rate and contribution of mergers to mass assembly from NIRCam observations of galaxy candidates up to 13.3 billion years ago
• The interstellar medium of high-redshift galaxies: Gathering clues from C III] and [C II] lines
• The nature of H{\sc i}-absorption-selected galaxies at $z\approx 4$
• Evidence for extended gaseous reservoirs around AGN at cosmic noon from ALMA CO(3-2) observations
• 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 ALMA-ALPINE [CII] survey: sub-kpc morphology of 3 main-sequence galaxy systems at z~4.5 revealed by ALMA
• A Dusty Dawn: Galactic Dust Buildup at $z\gtrsim 5$
• Dense and warm neutral gas in BR1202-0725 at z = 4.7 as traced by the [O I] 145 um line
• IR characteristic emission and dust properties of star-forming galaxies at 4.5 $<$ z $<$ 6.2
• Evidence of extended [CII] and dust emission in local dwarf galaxies
• The archival discovery of a strong Lyman-$\alpha$ and [CII] emitter at z = 7.677
• Synergizing 21 cm and sub-millimetre surveys during reionization: new empirical insights
• The ALPINE-ALMA [CII] Survey: Dust emission effective radius up to 3 kpc in the Early Universe
• MOSEL Survey: Extremely weak outflows in EoR analogues at z=3-4
• A${}^3$COSMOS: Measuring the cosmic dust-attenuated star formation rate density at $4<z<5$
• The ALPINE-ALMA [C II] survey: the luminosity function of serendipitous [C II] line emitters at $z\sim 5$
• Dust in High-Redshift Galaxies: Reconciling UV Attenuation and IR Emission
• A [C II] 158$\mu$m Emitter Associated with an OI Absorber at the End of the Reionization Epoch
• The ALPINE-ALMA [CII] survey: double stellar population and AGN activity in a galaxy at $z\sim 5.5$
• ALMACAL. XI. Over-densities as signposts to proto-clusters? A cautionary tale
• Kinematic analysis of $\mathbf{z}=4.3$ galaxies in the SPT2349$-$56 protocluster core
• Spectroscopic confirmation of a gravitationally lensed Lyman break galaxy at z${}_{[CII]}$ = 6.827 using NOEMA
• Carbon envelopes around merging galaxies at z ~ 4.5
• The ALPINE-CRISTAL-JWST Survey: Revealing Less Massive Black Holes in High-Redshift Galaxies
• Analytic models of dust temperature in high-redshift galaxies
• ALMA Lensing Cluster Survey: A spectral stacking analysis of [CII] in lensed $z\sim 6$ galaxies
• Multiwavelength dissection of a massive heavily dust-obscured galaxy and its blue companion at z $\sim$2
• Compact [C II] emitters around a C IV absorption complex at redshift 5.7
• Spatially resolved dust properties over 50 kpc in a hyperluminous galaxy merger at $z=4.6$
• Challenging interferometric imaging: Machine learning-based source localization from uv-plane observations
• Spatially resolved [CII]-gas conversion factor in early galaxies
• A puzzling non-detection of [O III] and [C II] from a $z\approx 7.7$ galaxy observed with ALMA
• Radio-astronomical Image Reconstruction with Conditional Denoising Diffusion Model
• Simulated [CII] in high-z galaxies
• 2mm Observations and the Search for High-Redshift Dusty Star-forming Galaxies
• 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
• 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
• The ALMA-CRISTAL survey: Extended [CII] emission in an interacting galaxy system at z ~ 5.5
• ALPINE: A Large Survey to Understand Teenage Galaxies
• CEERS: Forging the First Dust Grains in the Universe? A Population of Galaxies with spectroscopically-derived Extremely Low Dust Attenuation (GELDA) at 4.0<z<11.4
• The [C II] line emission as an interstellar medium probe in the MARIGOLD galaxies
• ALMA 360 pc high-frequency observations reveal warm dust in the center of a $z=6.9$ quasar
• The ALPINE-ALMA [CII] Survey: Unveiling the baryon evolution in the ISM of $z\sim 5$ star-forming galaxies
• The ALPINE-ALMA [CII] Survey: Modelling ALMA and JWST lines to constrain the interstellar medium of $z\sim 5$ galaxies
• Dust emission from the bulk of galaxies at the Epoch of Reionization
• The [NII] 205 $\mu$m line emission from high-z SMGs and QSOs
• Ultra-faint [CII] emission in a redshift = 2 gravitationally-lensed metal-poor dwarf galaxy
• CONCERTO at APEX -- On-sky performance in continuum
• 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
• Searching for [CII] Emission from the First Sample of $z\sim 6$ OI Absorption-Associated Galaxies with ALMA
• Dust-UV offsets in high-redshift galaxies in the Cosmic Dawn III simulation
• The ALPINE-CRISTAL-JWST survey: spatially resolved star formation relations at $z\sim 5$
• Predictions of the 21cm global signal in the JWST and ALMA era
• The ALPINE-ALMA [CII] survey: The infrared-radio correlation and AGN fraction of star-forming galaxies at z $\sim$ 4.4-5.9
• Discovery of a Unique Close Quasar-DSFG Pair Linked by a [C II] Bridge at $z=5.63$
• [CII] luminosity models and large-scale image cubes based on COSMOS 2020 and ALPINE-ALMA [CII] data back to the epoch of reionisation
• ADF22+: a declining faint end in the far-infrared luminosity function in the SSA22 protocluster at z=3.09
• ALMA survey of a massive node of the Cosmic Web at $z\sim 3$. II. A dynamically cold and massive disk galaxy in the proximity of a hyperluminous quasar
• Bright [CII]158$\mu$m Streamers as a Beacon for Giant Galaxy Formation in SPT2349$-$56 at $z=4.3$
• The slope and scatter of the star forming main sequence at z~5 : reconciling observations with simulations
• A mock redshift catalogue of the dusty star-forming galaxy population with intrinsic clustering and lensing for deep millimetre surveys
• The early Universe with JWST and ALMA
• A High-resolution Far-infrared Survey to Probe Black Hole-Galaxy Co-evolution
• ALMA Lensing Cluster Survey: Dust mass measurements as a function of redshift, stellar-mass and star formation rate, from z=1 to z=5
• Measuring the HI content of individual galaxies out to the epoch of reionization with [CII]
• The ALPINE-CRISTAL-JWST Survey: Gas-phase abundance gradients of main sequence star-forming galaxies and their kinematics at $4<z<6$
• First Light And Reionisation Epoch Simulations (FLARES) III: The properties of massive dusty galaxies at cosmic dawn
• Gas-Poor Hosts and Gas-Rich Companions of $z\approx$3.5 Radio Active Galactic Nuclei: ALMA Insights into Jet Triggering and Feedback
• Multi-wavelength properties of $z\gtrsim 6$ LISA detectable events
• A scaling relation in [C II]-detected galaxies and its likely application in cosmology
• Constraining the [CII] luminosity function from the power spectrum of line-intensity maps at redshift 3.6
• Probing the warm dark matter mass with [C II] intensity mapping
• Resolving circumgalactic gas flows around a z$\approx$3.6 quasar using MUSE and ALMA
• The NIKA2 cosmological legacy survey at 2 mm: catalogs, colors, redshift distributions, and implications for deep surveys
• The ALMA View of High-Redshift Galaxy Formation
• Evaluating star formation rates at z = 5