A complex multiphase DLA associated with a compact group at z = 2.431 traces accretion, outflows, and tidal streams
ALMA Reveals Metals yet No Dust within Multiple Components in CR7
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
Cold gas disks in main-sequence galaxies at cosmic noon: Low turbulence, flat rotation curves, and disk-halo degeneracy
COSMOS-DASH: The Evolution of the Galaxy Size-Mass Relation since z ~ 3 from New Wide-field WFC3 Imaging Combined with CANDELS/3D-HST
Detecting direct collapse black holes: making the case for CR7
Dust Attenuation, Bulge Formation, and Inside-out Quenching of Star Formation in Star-forming Main Sequence Galaxies at z ~ 2
Evidence for Large-scale, Rapid Gas Inflows in z 2 Star-forming Disks
Evidence for mature bulges and an inside-out quenching phase 3 billion years after the Big Bang
Evidence for PopIII-like Stellar Populations in the Most Luminous Lyman-a Emitters at the Epoch of Reionization: Spectroscopic Confirmation
High dust content of a quiescent galaxy at z 2 revealed by deep ALMA observation
No evidence for Population III stars or a Direct Collapse Black Hole in the z = 6.6 Lyman-a emitter CR7
Normal, dust-obscured galaxies in the epoch of reionization
Obscured star formation in bright z 7 Lyman-break galaxies
On the nature and physical conditions of the luminous Ly a emitter CR7 and its rest-frame UV components
SINS/zC-SINF Survey of z ~ 2 Galaxy Kinematics: Rest-frame Morphology, Structure, and Colors from Near-infrared Hubble Space Telescope Imaging
The nature of CR7 revealed with MUSE: a young starburst powering extended Ly a emission at z = 6.6
The Roles of Morphology and Environment on the Star Formation Rate-Stellar Mass Relation in COSMOS from 0 < z < 3.5
The Sins/zC-Sinf Survey of z ~ 2 Galaxy Kinematics: Evidence for Powerful Active Galactic Nucleus-Driven Nuclear Outflows in Massive Star-Forming Galaxies
The SINS/zC-SINF Survey of z ~ 2 Galaxy Kinematics: SINFONI Adaptive Optics-assisted Data and Kiloparsec-scale Emission-line Properties
Unveiling the nature of bright z 7 galaxies with the Hubble Space Telescope
Instrument
WFC3, WFC3/IR
Temporal Coverage
2012-03-02T16:52:21Z/2012-11-13T05:04:57Z
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, Forster Schreiber et al., 2013, 'Constraints on the Mass Assembly and Early Evolution of z~2 Galaxies: Witnessing the Growth of Bulges and Disks', 1.0, European Space Agency, https://doi.org/10.5270/esa-dg4271q