3D-HST: A wide-field grism spectroscopic survey with the Hubble Space Telescope

Abstract

We present 3D-HST, a near-infrared spectroscopic Treasury program with the Hubble Space Telescope for studying the processes that shape galaxies in the distant Universe. 3D-HST provides rest-frame optical spectra for a sample of ~7000 galaxies at 1<z<3.5, the epoch when 60% of all star formation took place, the number density of quasars peaked, the first galaxies stopped forming stars, and the structural regularity that we see in galaxies today must have emerged. 3D-HST will cover 3/4 (625 sq.arcmin) of the CANDELS survey area with two orbits of primary WFC3/G141 grism coverage and two to four parallel orbits with the ACS/G800L grism. In the IR these exposure times yield a continuum signal-to-noise of ~5 per resolution element at H~23.1 and a 5sigma emission line sensitivity of 5x10-17 erg/s/cm2 for typical objects, improving by a factor of ~2 for compact sources in images with low sky background levels. The WFC3/G141 spectra provide continuous wavelength coverage from 1.1-1.6 um at a spatial resolution of ~0."13, which, combined with their depth, makes them a unique resource for studying galaxy evolution. We present the preliminary reduction and analysis of the grism observations, including emission line and redshift measurements from combined fits to the extracted grism spectra and photometry from ancillary multi-wavelength catalogs. The present analysis yields redshift estimates with a precision of sigma(z)=0.0034(1+z), or sigma(v)~1000 km/s. We illustrate how the generalized nature of the survey yields near-infrared spectra of remarkable quality for many different types of objects, including a quasar at z=4.7, quiescent galaxies at z~2, and the most distant T-type brown dwarf star known. The CANDELS and 3D-HST surveys combined will provide the definitive imaging and spectroscopic dataset for studies of the 1<z<3.5 Universe until the launch of the James Webb Space Telescope.

Replacement reflects version now accepted by ApJS. A preliminary data release intended to provide a general illustration of the WFC3 grism data is available at http://3dhst.research.yale.edu/

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• Are star formation rates of galaxies bimodal?
• RUBIES: A Spectroscopic Census of Little Red Dots; All V-Shaped Point Sources Have Broad Lines
• Caught in the act: gas and stellar velocity dispersions in a fast quenching compact star-forming galaxy at z~1.7
• GOODS-ALMA 2.0: Starbursts in the main sequence reveal compact star formation regulating galaxy evolution prequenching
• The Differential Size Growth of Field and Cluster Galaxies at z=2.1 Using the ZFOURGE Survey
• Evolution of the galaxy stellar mass function: evidence for an increasing $M^{\ast }$ from $z=2$ to the present day
• Cluster and field elliptical galaxies at z~1.3. The marginal role of the environment and the relevance of the galaxy central regions
• Overturning the Case for Gravitational Powering in the Prototypical Cooling Lyman-alpha Nebula
• Nature versus nurture: what regulates star formation in satellite galaxies?
• Color gradients and half-mass radii of galaxies out to $z=2$ in the CANDELS/3D-HST fields: further evidence for important differences in the evolution of mass-weighted and light-weighted sizes
• A New View of the Size-Mass Distribution of Galaxies: Using $r_{20}$ and $r_{80}$ instead of $r_{50}$
• The MOSDEF survey: the prevalence and properties of galaxy-wide AGN-driven outflows at $z\sim 2$
• Photometric Redshift Calibration Requirements for WFIRST Weak Lensing Cosmology: Predictions from CANDELS
• The HDUV Survey: Six Lyman Continuum Emitter Candidates at z~2 Revealed by HST UV Imaging
• Mass calibration of distant SPT galaxy clusters through expanded weak lensing follow-up observations with HST, VLT & Gemini-South
• Constraining Lyman-alpha spatial offsets at $3<z<5.5$ from VANDELS slit spectroscopy
• Predicting Ly$\alpha$ Emission from Galaxies via Empirical Markers of Production and Escape in the KBSS
• HST Grism Observations of a Gravitationally Lensed Redshift 10 Galaxy
• The Dust Attenuation Curve versus Stellar Mass for Emission Line Galaxies at z ~ 2
• Evolution of Star-formation Properties of High-redshift Cluster Galaxies since $z=2$
• High gas fraction in a CO-selected main-sequence galaxy at $z>3$
• The IRAM/GISMO two-millimeter survey in the COSMOS field
• Simulating and interpreting deep observations in the Hubble Ultra Deep Field with the JWST/NIRSpec low-resolution 'prism'
• A 16 deg${}^2$ survey of emission-line galaxies at z<1.5 in HSC-SSP PDR1
• The Grism Lens-Amplified Survey from Space (GLASS). IX. The dual origin of low-mass cluster galaxies as revealed by new structural analyses
• The [OIII]$\lambda 5007$ equivalent width distribution at z $\sim 2$: The redshift evolution of the extreme emission line galaxies
• HST Grism Confirmation of Two $z\sim 2$ Structures from the Clusters Around Radio-Loud AGN (CARLA) Survey
• One Plane for All: Massive Star-Forming and Quiescent Galaxies Lie on the Same Mass Fundamental Plane at z~0 and z~0.7
• Diagnosing DASH: A Catalog of Structural Properties for the COSMOS-DASH Survey
• A Comprehensive Bayesian Discrimination of the Simple Stellar Population Model, Star Formation History and Dust Attenuation Law in the Spectral Energy Distribution Modeling of Galaxies
• The kinematics of massive quiescent galaxies at $1.4<z<2.1$: dark matter fractions, IMF variation, and the relation to local early-type galaxies
• The Ages of Passive Galaxies in a z=1.62 Protocluster
• Are LGRBs biased tracers of star formation? Clues from the host galaxies of the Swift/BAT6 complete sample of bright LGRBs. II: star formation rates and metallicities at z < 1
• The e-MERLIN Galaxy Evolution Survey (e-MERGE): Overview and Survey Description
• Milky Way Red Dwarfs in the BoRG Survey; Galactic scale-height and the distribution of dwarfs stars in WFC3 imaging
• Galaxy Merger Candidates in High-Redshift Cluster Environments
• The Number Density Evolution of Extreme Emission Line Galaxies in 3D-HST: Results from a Novel Automated Line Search Technique for Slitless Spectroscopy
• The Impact of Strong Gravitational Lensing on Observed Lyman-Break Galaxy Numbers at 4<z<8 in the GOODS and the XDF Blank Fields
• Galaxy Merger Fractions in Two Clusters at $z\sim 2$ Using the Hubble Space Telescope
• Completing the Census of AGN in GOODS-S/HUDF: New Ultra-Deep Radio Imaging and Predictions for JWST
• Quenching and the UVJ diagram in the SIMBA cosmological simulation
• A panchromatic spatially-resolved analysis of nearby galaxies -- I. Sub-kpc scale Main Sequence in grand-design spirals
• Luminosity Dependence and Redshift Evolution of Strong Emission-line Diagnostics in Star-Forming Galaxies
• The Team Keck Redshift Survey 2: MOSFIRE Spectroscopy of the GOODS-North Field
• The ALPINE-ALMA [CII] survey: dust attenuation curves at z=4.4-5.5
• Blue Rest-Frame UV-Optical Colors in z~8 Galaxies from GREATS: Very Young Stellar Populations at ~650 Myr of Cosmic Time
• The Grism lens-amplified survey from space (GLASS). VII. The diversity of the distribution of star formation in cluster and field galaxies at 0.3<z<0.7
• The Lyman Continuum Escape Fraction of Galaxies and AGN in the GOODS Fields
• Evidence for Inside-Out Galaxy Growth and Quenching of a z~2 Compact Galaxy from High-Resolution Molecular Gas Imaging
• HST Emission Line Galaxies at z ~ 2: The Mystery of Neon
• Discovery of a Quadruple Lens in CANDELS with a Record Lens Redshift z=1.53
• Limits to Rest-Frame Ultraviolet Emission From Far-Infrared-Luminous z~6 Quasar Hosts
• Nature of Faint Radio Sources in GOODS-North and GOODS-South Fields - I. Spectral Index and Radio-FIR Correlation
• The Super Eight Galaxies: Properties of a Sample of Very Bright Galaxies at $7<z<8$
• Near-infrared emission line diagnostics for AGN from the local Universe to redshift 3
• From Nuclear to Circumgalactic: Zooming in on AGN-Driven Outflows at z~2.2 with SINFONI
• The kiloparsec-scale gas kinematics in two star-forming galaxies at $z\sim 1.47$ seen with ALMA and VLT-SINFONI
• The Fundamental Plane of massive quiescent galaxies out to z~2
• A Bayesian Population Model for the Observed Dust Attenuation in Galaxies
• The Geometry of Cold, Metal-Enriched Gas Around Galaxies at $z\sim 1.2$
• Quasar Sightline and Galaxy Evolution (QSAGE) Survey - I. The Galaxy Environment of OVI Absorbers up to z=1.4 around PKS 0232-04
• Identification of galaxies that experienced a recent major drop of star formation
• The Kinematics and Dark Matter Fractions of TNG50 Galaxies at z=2 from an Observational Perspective
• Predicted future fate of COSMOS galaxy protoclusters over 11 Gyr with constrained simulations
• Ages of massive galaxies at $0.5<z<2.0$ from 3D-HST rest-frame optical spectroscopy
• CO Emission, Molecular Gas, and Metallicity in Main-Sequence Star-Forming Galaxies at $z\sim 2.3$
• BIRTH of the COSMOS Field: Primordial and Evolved Density Reconstructions During Cosmic High Noon
• Ly$\alpha$ Emitters with Very Large Ly$\alpha$ Equivalent Widths, EW${}_0$(Ly$\alpha$) $\simeq 200-400$ Å, at $z\sim 2$
• Simulating JWST deep extragalactic imaging surveys and physical parameter recovery
• The Missing Satellite Problem in 3D
• The angular momentum of disc galaxies at z=1
• HST Emission Line Galaxies at z ~ 2: The Ly-alpha Escape Fraction
• Large-Scale Star Formation-Driven Outflows at 1<z<2 in the 3D-HST Survey
• COSMOS2020: Manifold Learning to Estimate Physical Parameters in Large Galaxy Surveys
• The NIRSpec Wide GTO Survey
• Young, Star-forming Galaxies and their local Counterparts: the Evolving Relationship of Mass-SFR-Metallicity since z ~ 2.1
• A large, deep 3 deg${}^2$ survey of H$\alpha$, [OIII], and [OII] emitters from LAGER: constraining luminosity functions
• The GOGREEN survey: Dependence of galaxy properties on halo mass at z > 1 and implications for environmental quenching
• Growth of bulges in disc galaxies since $z\sim 1$
• PHIBSS: Exploring the Dependence of the CO-H${}_2$ Conversion Factor on Total Mass Surface Density at $z<1.5$
• Leveraging 3D-HST Grism Redshifts to Quantify Photometric Redshift Performance
• Massive quiescent galaxies at $z\sim 3$: a comparison of selection, stellar population and structural properties with simulation predictions
• The Relation between Dynamical Mass-to-Light Ratio and Color for Massive Quiescent Galaxies out to z~2 and Comparison with Stellar Population Synthesis Models
• Resolved Star Formation on Sub-galactic Scales in a Merger at z=1.7
• The average dust attenuation curve at z~1.3 based on HST grism surveys
• The definition of environment and its relation to the quenching of galaxies at z=1-2 in a hierarchical Universe
• 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
• Compact Star-Forming Galaxies as Old Starbursts Becoming Quiescent
• Stellar Mass Growth of Brightest Cluster Galaxy Progenitors in COSMOS Since z ~ 3
• A NOEMA molecular line scan of the Hubble Deep Field North: Improved constraints on the CO luminosity functions and cosmic density of molecular gas
• Changing physical conditions in star-forming galaxies between redshifts 0 < z < 4: [OIII]/Hb evolution
• Passive galaxies as tracers of cluster environments at z~2
• A First Look at Spatially Resolved Star Formation at $4.8<z<6.5$ with JWST FRESCO NIRCam Slitless Spectroscopy
• Lyman Continuum Escape Fraction from Low-mass Starbursts at z=1.3
• The Spitzer/IRAC Legacy over the GOODS Fields: Full-Depth 3.6, 4.5, 5.8 and 8.0um Mosaics and Photometry for > 9000 Galaxies at z~3.5-10 from the GOODS Re-ionization Era wide-Area Treasury from Spitzer (GREATS)
• CLEAR: The Evolution of Spatially Resolved Star Formation in Galaxies between $0.5\lesssim z\lesssim 1.7$ using H$\alpha$ Emission Line Maps
• Recent Star-formation in a Massive Slowly-Quenched Lensed Quiescent Galaxy at z=1.88
• THE MOSDEF SURVEY: The Nature of Mid-Infrared Excess Galaxies and a Comparison of IR and UV Star Formation Tracers at z~2
• The KMOS Cluster Survey (KCS) II - The Effect of Environment on the Structural Properties of Massive Cluster Galaxies at Redshift $1.39<z<1.61$
• Exploring the chemical link between local ellipticals and their high-redshift progenitors
• Starburst galaxies in the COSMOS field: clumpy star-formation at redshift 0 < z < 0.5
• HST Grism-derived Forecasts for Future Galaxy Redshift Surveys
• No More Active Galactic Nuclei in Clumpy Disks Than in Smooth Galaxies at z~2 in CANDELS / 3D-HST
• CLEAR: Survey Overview, Data Analysis and Products
• First Infrared-based implications for the dust attenuation and star formation of typical Ly$\alpha$ emitters
• REQUIEM-2D: Spatially Resolved Stellar Populations from HST 2D Grism Spectroscopy
• Morphology and the Color-Mass Diagram as Clues to Galaxy Evolution at z~1
• Infrared luminosity functions and dust mass functions in the EAGLE simulation
• Are the host galaxies of Long Gamma-Ray Bursts more compact than star-forming galaxies of the field?
• Unbiased Cosmological Parameter Estimation from Emission Line Surveys with Interlopers
• An Updated Dust-to-Star Geometry: Dust Attenuation Does Not Depend on Inclination in $1.3\le z\le 2.6$ Star-Forming Galaxies from MOSDEF
• Extending empirical constraints on the SZ-mass scaling relation to higher redshifts via HST weak lensing measurements of nine clusters from the SPT-SZ survey at $z\gtrsim 1$
• Across the Green Valley with HST grisms: colour evolution, crossing time-scales and the growth of the red sequence at $z=1.0-1.8$
• ZFIRE: Similar Stellar Growth in H$\alpha$-emitting Cluster and Field Galaxies at z~2
• MIRI Deep Imaging Survey (MIDIS) of the Hubble Ultra Deep Field
• Resolving Ambiguities in the Inferred Star Formation Histories of Intense [O III] Emitters in the Reionisation Era
• Stellar populations and star formation histories of the most extreme [OIII] emitters at $z=1.3-3.7$
• AGN Feedback in Quiescent Galaxies at Cosmic Noon Traced by Ionized Gas Emission
• The Grism lens-amplified survey from space (GLASS). VIII. The influence of the cluster properties on Halpha emitter galaxies at 0.3<z<0.7
• Quiescent galaxies in a virialized cluster at redshift 2: Evidence for accelerated size-growth
• The Relation Between [OIII]/H$\beta$ and Specific Star Formation Rate in Galaxies at $z\sim 2$
• The complex case of MACSJ0717.5+3745 and its extended filament: intra-cluster light, galaxy luminosity function, and galaxy orientations
• Studying the Physical Properties of Tidal Features I. Extracting Morphological Substructure in CANDELS Observations and VELA Simulations
• A spatially resolved analysis of star-formation burstiness by comparing UV and H$\alpha$ in galaxies at z$\sim$1 with UVCANDELS
• Lyman Continuum Galaxy Candidates in COSMOS
• A Local Leaky-box Model for the Local Stellar Surface Density - Gas Surface Density - Gas Phase Metallicity Relation
• 3D-HST Emission Line Galaxies at z ~ 2: Discrepancies in the Optical/UV Star Formation Rates
• The faint end of the red sequence galaxy luminosity function: unveiling surface brightness selection effects with the CLASH clusters
• Neural Networks Optimized by Genetic Algorithms in Cosmology
• Outside the Lyman-break box: detecting Lyman continuum emitters at $3.5<z<5.1$ with CLAUDS
• The Evolution of Sizes and Specific Angular Momenta in Hierarchical Models of Galaxy Formation and Evolution
• Redshifting galaxies from DESI to JWST CEERS: Correction of biases and uncertainties in quantifying morphology
• Beyond the Local Volume. I. Surface Densities of Ultracool Dwarfs in Deep HST/WFC3 Parallel Fields
• AGN accretion and black hole growth across compact and extended galaxy evolution phases
• The Obscured Fraction of Quasars at Cosmic Noon
• Mapping the Morphology and Kinematics of a Lyman-alpha-selected Nebula at z=3.15 with MUSE
• Ubiquitous [OII] Emission in Quiescent Galaxies at z ~ 0.85
• A Comparison of Rest-frame Ultraviolet and Optical Emission-Line Diagnostics in the Lensed Galaxy SDSS J1723+3411 at Redshift z=1.3293
• Early galaxy growth: mergers or gravitational instability?
• The MUSE Ultra Deep Field (MUDF). III. Hubble Space Telescope WFC3 Grism Spectroscopy and Imaging
• LINEAR: A Novel Algorithm for Reconstructing Slitless Spectroscopy from HST/WFC3
• The ALPINE-ALMA [CII] Survey: the population of [CII]-undetected galaxies and their role in the ${\mathrm{L}}_{[\mathrm{CII}]}$-SFR relation
• The Environment of z >1 3CR Radio Galaxies and QSOs: From Proto-Clusters to Clusters of Galaxies?
• High Redshift Massive Quiescent Galaxies are as Flat as Star Forming Galaxies: The Flattening of Galaxies and the Correlation with Structural Properties in CANDELS/3D-HST
• The Spatial Extent and Distribution of Star Formation in 3D-HST Mergers at z~1.5
• The Subaru FMOS Galaxy Redshift Survey (FastSound). II. The Emission Line Catalog and Properties of Emission Line Galaxies
• The HETDEX Survey: The Ly$\alpha$ Escape Fraction from 3D-HST Emission Line Galaxies at $z\sim 2$
• Deep ugrizY Imaging and DEEP2/3 Spectroscopy: A Photometric Redshift Testbed for LSST and Public Release of Data from the DEEP3 Galaxy Redshift Survey
• The Grism Lens-Amplified Survey from Space (GLASS). V. Extent and spatial distribution of star formation in z~0.5 cluster galaxies
• Similarities and uniqueness of Ly$\alpha$ emitters among star-forming galaxies at z=2.5
• The IllustrisTNG Simulations: Public Data Release
• Galaxy morphologies at cosmic noon with JWST: A foundation for exploring gas transport with bars and spiral arms
• Spatially resolved mass-metallicity relation at z~0.26 from the MUSE-Wide Survey
• Growing up in a megalopolis: Environmental effects on galaxy evolution in a supercluster at z~0.65 in UKIDSS UDS
• The Lyman Continuum Escape Fraction of Star-forming Galaxies at $2.4\lesssim z\lesssim 3.0$ from UVCANDELS
• Lyα Halos around [O III]-Selected Galaxies in HETDEX
• The MOSDEF Survey: No Significant Enhancement in Star Formation or Deficit in Metallicity in Merging Galaxy Pairs at 1.5<=z<=3.5
• Evidence for a low Lyman Continuum Escape fraction in three Massive, UV-bright galaxies at z > 7
• Morphology & Environment's Role on the Star Formation Rate -- Stellar Mass Relation in COSMOS from 0 < z < 3.5
• More is better: Strong constraints on the stellar properties of LEGA-C z ~ 1 galaxies with Prospector
• Properties of LBGs with [OIII] detection at z $\sim$ 3.5: The importance of including nebular emission data in SED fitting
• Connecting Galactic Outflows and Star Formation: Inferences from H-alpha Maps and Absorption Line Spectroscopy at 1 < z < 1.5
• The MOSDEF Survey: Differences in SFR and Metallicity for Morphologically-Selected Mergers at z~2
• COLDz: Deep 34 GHz Continuum Observations and Free-free Emission in High-redshift Star-forming Galaxies
• ODIN: Improved Narrowband Ly$\alpha$ Emitter Selection Techniques for $z$ = 2.4, 3.1, and 4.5
• Imaging Spectroscopy of Ionized Gaseous Nebulae around Optically Faint AGN at Redshift z ~ 2
• Physical properties of compact star-forming galaxies at $z\sim 2-3$
• Solution to the conflict between the resolved and unresolved galaxy stellar mass estimation from the perspective of JWST
• Compact galaxies and the size-mass galaxy distribution from a colour-selected sample at 0.04 < z < 0.15 supplemented by ugrizYJHK photometric redshifts
• Bimodal morphologies of massive galaxies at the core of a protocluster at z=3.09 and the strong size growth of a brightest cluster galaxy
• Euclid preparation. XXX. Performance assessment of the NISP Red-Grism through spectroscopic simulations for the Wide and Deep surveys
• Star-forming galaxies at low-redshift in the SHARDS survey
• JADES: Rest-frame UV-to-NIR Size Evolution of Massive Quiescent Galaxies from Redshift z=5 to z=0.5
• The Shape and Scatter of The Galaxy Main Sequence for Massive Galaxies at Cosmic Noon
• The OTELO survey as a morphological probe. Last ten Gyr of galaxy evolution. The mass--size relation up to z=2
• Correlations between H$\alpha$ Equivalent Width and Galaxy Properties at $z=0.47$: Physical or Selection-driven?
• The HSC-SSP Transient Survey: Implications from Early Photometry and Rise Time of Normal Type Ia Supernovae
• Quasar Sightline and Galaxy Evolution (QSAGE) survey -- II. Galaxy overdensities around UV luminous quasars at z=1-2
• K-CLASH: Strangulation and Ram Pressure Stripping in Galaxy Cluster Members at 0.3 < z < 0.6
• Testing the accuracy of 3D-HST photometric redshift estimates as reference samples for deep weak lensing studies
• Differential attenuation in star-forming galaxies at 0.3 $\lesssim$ $z$ $\lesssim$ 1.5 in the SHARDS/CANDELS field
• Substellar and low-mass dwarf identification with near-infrared imaging space observatories
• Timescales for Hi consumption and SFR depletion of satellite galaxies in groups
• Abundant Serendipitous Emission Line Sources with JWST/NIRSpec
• COLDz: Probing Cosmic Star Formation With Radio Free-free Emission
• JWST reveals a high fraction of disk breaks at $1\le z\le 3$
• Angular momentum evolution of stellar disks at high redshifts
• FORECAST: a flexible software to forward model cosmological hydrodynamical simulations mimicking real observations
• The MOSDEF-LRIS Survey: Probing ISM/CGM Structure of Star-Forming Galaxies at z~2 Using Rest-UV Spectroscopy
• Beyond the Local Volume. II. Population Scaleheights and Ages of Ultracool Dwarfs in Deep HST/WFC3 Parallel Fields
• MAGIC: Muse gAlaxy Groups In Cosmos -- A survey to probe the impact of environment on galaxy evolution over the last 8 Gyr
• Not In Our Backyard: Spectroscopic Support for the CLASH z=11 Candidate MACS0647-JD
• Galaxies of the $z\sim 2$ Universe. I. Grism-Selected Rest-Frame Optical Emission Line Galaxies
• HETDEX [OIII] Emitters I: A spectroscopically selected low-redshift population of low-mass, low-metallicity galaxies
• The Impact of Black Hole Scaling Relation Assumptions on the Mass Density of Black Holes
• The ALPINE-ALMA [CII] survey: double stellar population and AGN activity in a galaxy at $z\sim 5.5$
• The MOSDEF Survey: An Improved Voronoi Binning Technique on Spatially Resolved Stellar Populations at z~2
• Surface brightness profiles of blue compact dwarf galaxies in the GOODS-N and GOODS-S field
• Dust Temperature of Compact Star-forming Galaxies at $z\sim 1-3$ in 3D-{\it HST}/CANDELS
• The ALPINE-ALMA [C II] survey: the luminosity function of serendipitous [C II] line emitters at $z\sim 5$
• Formation of disc galaxies around z~2
• A Catalog of Emission-Line Galaxies from the Faint Infrared Grism Survey: Studying Environmental Influence on Star Formation
• The MOSDEF Survey: The Dependence of H$\alpha$-to-UV SFR Ratios on SFR and Size at $z\sim 2$
• MOSEL Survey: Tracking the Growth of Massive Galaxies at 2<z<4 using Kinematics and the IllustrisTNG Simulation
• Revealing the host galaxy of a quasar 2175 Å dust absorber at z = 2.12
• Identification of single spectral lines through supervised machine learning in a large HST survey (WISP): a pilot study for Euclid and WFIRST
• SEEDisCS I. Molecular gas in galaxy clusters and their large scale structure: the case of CL1411.1$-$1148 at $z\sim 0.5$
• Exploring the Correlation between $\mathrm{H}\alpha$-to-UV Ratio and Burstiness for Typical Star-forming Galaxies at $z\sim 2$
• Influence of star-forming galaxy selection on the galaxy main sequence
• Near-infrared spectroscopy of 5 ultra-massive galaxies at 1.7 < z < 2.7
• Probing galaxy evolution from $z=0$ to $z\simeq 10$ through galaxy scaling relations in three L-Galaxies flavours
• A selection of Hα emitters at z = 2.1-2.5 using the Ks-band photometry of ZFOURGE
• An empirical approach to selecting the first growing black hole seeds with JWST/NIRCam
• Galaxy populations in the most distant SPT-SZ clusters -- II. Galaxy structural properties in massive clusters at 1.4<z<1.7
• Astrobotics: Swarm Robotics for Astrophysical Studies
• The Hα Luminosity Function of Galaxies at z {\sim} 4.5
• The mass-dependent UVJ diagram at cosmic noon: A challenge for galaxy evolution models and dust radiative transfer
• The Grism Lens-Amplified Survey from Space (GLASS). XIII. G800L optical spectra from the parallel fields
• The PAU Survey: Photometric redshift estimation in deep wide fields
• High dense gas fraction in a gas-rich star-forming galaxy at z = 1.2
• The Direct-Method Oxygen Abundance of Typical Dwarf Galaxies at Cosmic High-Noon
• A Synthetic Roman Space Telescope High-Latitude Time-Domain Survey: Supernovae in the Deep Field
• The Grism Lens-Amplified Survey from Space (GLASS). XII. Spatially Resolved Galaxy Star Formation Histories and True Evolutionary Paths at z > 1
• NOEMA reveals the true nature of luminous red JWST z>10 galaxy candidates
• DESI Massive Post-Starburst Galaxies at $\mathbf{z}\sim 1.2$ have compact structures and dense cores
• Forward modeling of galaxy kinematics in slitless spectroscopy
• The GLASS-JWST Early Release Science Programme: The NIRISS Spectroscopic Catalogue
• JWST PRIMER: A deep JWST study of all ALMA-detected galaxies in PRIMER COSMOS -- dust-obscured star-formation history back to z $\simeq$ 7
• Measuring Stellar Masses of Emission Line Galaxies at 1.2<z<1.9
• Unresolved z~8 point sources and their impact on the bright end of the galaxy luminosity function
• Using Multiple Emission Line Ratios to Constrain the Slope of the Dust Attenuation Law
• Improved Measurements of Galaxy Star Formation Stochasticity from the Intrinsic Scatter of Burst Indicators
• Stellar, Gas, and Dust Emission of Star Forming Galaxies out to z~2
• HELLO project: High-$z$ Evolution of Large and Luminous Objects
• Stellar populations of galaxies in the ALHAMBRA survey up to $z\sim 1$. III. The stellar content of the quiescent galaxy population during the last $8$ Gyr
• Bright Compact Bulges (BCBs) at intermediate redshifts
• HETDEX Pilot Survey. VI. [OIII] Emitters and Expectations for a Local Sample of Star Forming Galaxies in HETDEX
• Empirical Dust Attenuation Model Leads to More Realistic UVJ Diagram for TNG100 Galaxies
• The H$\alpha$ and [O III] $\lambda 5007$ Luminosity Functions of $1.2<z<1.9$ Emission-Line Galaxies from HST Grism Spectroscopy
• JWST Reveals Bulge-dominated Star-forming Galaxies at Cosmic Noon
• Evidence for non-stellar rest-frame near-IR emission associated with increased star formation in galaxies at $z\sim 1$
• The Chandra Deep Field South as a test case for Global Multi Conjugate Adaptive Optics
• Dark Matter Fraction in Disk-Like Galaxies Over the Past 10 Gyr
• The Differential Assembly History of the Centers and Outskirts of Main Sequence Galaxies at $z\sim 2.3$
• How accurate are infrared luminosities from monochromatic photometric extrapolation?
• A comprehensive study of H$\alpha$ emitters at $z\sim$ 0.62 in the DAWN survey: the need for deep and wide regions
• Multiple emission lines of H$\alpha$ emitters at $z\sim 2.3$ from the broad and medium-band photometry in the ZFOURGE Survey
• Spectrophotometric Redshifts In The Faint Infrared Grism Survey: Finding Overdensities Of Faint Galaxies
• Search for extended Lyman-$\alpha$ emission around 9k quasars at z=2-3
• Decoupled Black Hole Accretion and Quenching: The Relationship Between BHAR, SFR, and Quenching in Milky Way and Andromeda-mass Progenitors Since z = 2.5
• HST Hα grism spectroscopy of ROLES: a flatter low-mass slope for the z~1 SSFR--mass relation
• The H$\alpha$ luminosity and stellar mass dependent clustering of star-forming galaxies at $0.7<z<1.5$ with 3D-HST
• Local galaxies with compact cores as the possible descendants of massive compact quiescent galaxies at high redshift
• Spectroscopy of an extreme [OIII] emitting active galactic nucleus at $z=3.212$: implications for the reionisation era
• A Morphology Catalog of Galaxies in CEERS: Evolution in the Size and Color Gradients of Galaxies Since Cosmic Dawn
• Self-Similar Buildup and Inside-Out Growth: Tracing the Evolution of Intermediate to High-Mass Star-Forming Galaxies Since $z=2$
• Quasars Have Fewer Close Companions than Normal Galaxies
• The average structural evolution of massive galaxies can be reliably estimated using cumulative galaxy number densities
• Spectrophotometric redshifts for $\mathrm{z}\sim 1$ galaxies and predictions for number densities with WFIRST and Euclid
• The $z\sim 2$ $[\mathrm{O}\mathrm{III}]$ Luminosity Function of Grism-selected Emission-line Galaxies
• Near-IR narrow-band imaging with CIRCE at the Gran Telescopio Canarias: Searching for Ly$\alpha$-emitters at $z\sim 9.3$
• The MOSDEF Survey: Probing Resolved Stellar Populations at $z\sim 2$ Using a New Bayesian-defined Morphology Metric Called Patchiness
• Exploring high-z galaxies with the E-ELT
• X-ray Unveiling Events in a z~1.6 Active Galactic Nucleus in the 7 Ms Chandra Deep Field-South
• Brighter and More Massive Galaxies in the Vicinity of Lyman-alpha Nebulae
• Spatially Extended Low Ionization Emission Regions (LIERs) at $z\sim 0.9$
• The JWST Emission Line Survey (JELS): The sizes and merger fraction of star-forming galaxies during the Epoch of Reionization
• GalaxyGenius: Mock galaxy image generator for various telescopes from hydrodynamical simulations
• Observing galaxy mergers at the epoch of reionization
• Simulating continuum-based redshift measurement in the \textit{Roman's} High Latitude Spectroscopy Survey
• Through the fog: a complementary optical galaxy classification scheme for 'intermediate' redshifts
• Disentangling AGN and Star Formation Activity at High Redshift Using Hubble Space Telescope Grism Spectroscopy
• From Exoplanets to Quasars: Detection of Potential Damped Lyman Alpha Absorbing Galaxies Using Angular Differential Imaging
• Enhanced AGN Activity in Overdense Galactic Environments at $2<z<4$
• The HST-Hyperion Survey: Companion Fraction and Overdensity in a z ~ 2.5 Proto-supercluster
• The stellar host in star-forming low-mass galaxies: Evidence for two classes
• Exploring the X-ray-radio connection for AGN via measurements of the multi-dimensional luminosity function
• SKYSURF. X. A Novel Method for Measuring Integrated Galaxy Light
• Compact [OIII] emission-line regions ("Green Seeds") in $\mathrm{H}\alpha$ emitters at Cosmic Noon from JWST Observations
• Flexible Simulation Based Inference for Galaxy Photometric Fitting with Synthesizer
• LATIS Data Release: $\sim 4200$ Spectra of $z\sim 2-3$ Galaxies, Redshifts, and Intergalactic Medium Tomography Maps
• SpecZoo: An AI-Powered Platform for Spectral Analysis and Visualization in Science and Education
• COSMOS-Web: Galaxy Size and Surface Brightness Evolution at Rest-Frame 1.22 $\mu$m Since $z=3$
• Near-IR Spectroscopic Studies of Galaxies at z~1-3
• Structural and morphological properties of ultraluminous infrared galaxies at $1<z<3$
• Introducing the FLAMINGOS-2 Split-K Medium Band Filters: The Impact on Photometric Selection of High-z Galaxies in the FENIKS-pilot survey
• Initial Investigations of the Outskirts of XLSSC 122
• Lack of influence of the environment in the earliest stages of massive galaxy formation