3D-DASH: The Evolution of Size, Shape, and Intrinsic Scatter in Populations of Young and Old Quiescent Galaxies at 0.5 < z < 3
3D-DASH: The Widest Near-infrared Hubble Space Telescope Survey
A Census of Photometrically Selected Little Red Dots at 4 < z < 9 in JWST Blank Fields
Age and metal gradients in massive quiescent galaxies at 0.6 z 1.0: implications for quenching and assembly histories
A Large-scale Ring Galaxy at z = 2.2 Revealed by JWST/NIRCam: Kinematic Observations and Analytical Modelling
ALMA Measures Rapidly Depleted Molecular Gas Reservoirs in Massive Quiescent Galaxies at z ~ 1.5
A Mass-dependent Slope of the Galaxy Size-Mass Relation out to z ~ 3: Further Evidence for a Direct Relation between Median Galaxy Size and Median Halo Mass
A New Approach to Constraining Properties of Active Galactic Nucleus Host Galaxies by Combining Image and Spectral Energy Distribution Decomposition: Testing upon the MBH-M Relation
A New Method for Wide-field Near-IR Imaging with the Hubble Space Telescope
COSMOS-DASH: The Evolution of the Galaxy Size-Mass Relation since z ~ 3 from New Wide-field WFC3 Imaging Combined with CANDELS/3D-HST
Counterparts of candidate dusty starbursts at z > 6
Diagnosing DASH: A Catalog of Structural Properties for the COSMOS-DASH Survey
Dust in Little Red Dots
Euclid preparation - XXIII. Derivation of galaxy physical properties with deep machine learning using mock fluxes and H-band images
Morphological Evolution of the Hosts of Far-infrared/Submillimeter Galaxies
Rapid Quenching of Galaxies at Cosmic Noon
Relation between colour gradient and central asymmetric features for post-starburst galaxies at z ~ 0.8
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
The ALMA-CRISTAL survey: Resolved kinematic studies of main sequence star-forming galaxies at 4 < z < 6
The ALMA-CRISTAL Survey: Spatial extent of CII line emission in star-forming galaxies at z = 4-6
The ALMA REBELS Survey: discovery of a massive, highly star-forming, and morphologically complex ULIRG at z = 7.31
The Brightest z 8 Galaxies over the COSMOS UltraVISTA Field
The Classification of Galaxy Morphology in the H Band of the COSMOS-DASH Field: A Combination-based Machine-learning Clustering Model
The Effect of Environment on the Properties of the Most Massive Galaxies at 0.5 < z < 2.5 in the COSMOS-DASH Field
The Heavy Metal Survey: Star Formation Constraints and Dynamical Masses of 21 Massive Quiescent Galaxies at z = 1.3-2.3
The Number Densities and Stellar Populations of Massive Galaxies at 3 < z < 6: A Diverse, Rapidly Forming Population in the Early Universe
The PANORAMIC Survey: Pure Parallel Wide Area Legacy Imaging with JWST/NIRCam
Uncovering a Massive z 7.7 Galaxy Hosting a Heavily Obscured Radio-loud Active Galactic Nucleus Candidate in COSMOS-Web
Instrument
WFC3, WFC3/IR
Temporal Coverage
2015-10-15T01:04:37Z/2017-06-05T06:09:10Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, van Dokkum et al., 2017, 'A Wide-Field WFC3 Imaging Survey in the COSMOS Field', 1.0, European Space Agency, https://doi.org/10.5270/esa-zuz2s12