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 z = 1.85 galaxy group in CEERS: Evolved, dustless, massive intra-halo light and a brightest group galaxy in the making
COSMOS-DASH: The Evolution of the Galaxy Size-Mass Relation since z ~ 3 from New Wide-field WFC3 Imaging Combined with CANDELS/3D-HST
Extremely Low Molecular Gas Content in a Compact, Quiescent Galaxy at z = 1.522
Morphology of Galaxies in JWST Fields: Initial Distribution and Evolution of Galaxy Morphology
Near-IR Weak-lensing (NIRWL) Measurements in the CANDELS Fields. I. Point-spread Function Modeling and Systematics
Stellar Kinematics of z ~ 2 Galaxies and the Inside-out Growth of Quiescent 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 missing light of the Hubble Ultra Deep Field
The Roles of Morphology and Environment on the Star Formation Rate-Stellar Mass Relation in COSMOS from 0 < z < 3.5
The Stellar Velocity Dispersion of a Compact Massive Galaxy at z = 1.80 Using X-Shooter: Confirmation of the Evolution in the Mass-Size and Mass-Dispersion Relations
Instrument
WFC3, WFC3/IR
Temporal Coverage
2010-10-22T04:09:54Z/2011-11-07T03:48:16Z
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, Franx et al., 2012, 'Resolving the Matter of Massive Quiescent Galaxies at z=1.5-2', 1.0, European Space Agency, https://doi.org/10.5270/esa-v0upuo4
