A Census of Photometrically Selected Little Red Dots at 4 < z < 9 in JWST Blank Fields
A Large-scale Ring Galaxy at z = 2.2 Revealed by JWST/NIRCam: Kinematic Observations and Analytical Modelling
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 PAH deficit in the starburst core of a distant spiral galaxy
COSMOS-DASH: The Evolution of the Galaxy Size-Mass Relation since z ~ 3 from New Wide-field WFC3 Imaging Combined with CANDELS/3D-HST
Dust in Little Red Dots
Morphology of Galaxies in JWST Fields: Initial Distribution and Evolution of Galaxy Morphology
Relation between colour gradient and central asymmetric features for post-starburst galaxies at z ~ 0.8
Stellar Mass Growth of Brightest Cluster Galaxy Progenitors in COSMOS Since z ~ 3
The ALMA-CRISTAL survey: Resolved kinematic studies of main sequence star-forming galaxies at 4 < z < 6
The ALMA-CRISTAL Survey: Spatially Resolved Star Formation Activity and Dust Content in 4 < z < 6 Star-forming Galaxies
The impact of satellite trails on Hubble Space Telescope observations
The PANORAMIC Survey: Pure Parallel Wide Area Legacy Imaging with JWST/NIRCam
The Roles of Morphology and Environment on the Star Formation Rate-Stellar Mass Relation in COSMOS from 0 < z < 3.5
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR
Temporal Coverage
2014-11-18T22:42:28Z/2015-10-19T23:29:06Z
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, Kartaltepe et al., 2016, 'Probing the Most Luminous Galaxies in the Universe at the Peak of Galaxy Assembly', 1.0, European Space Agency, https://doi.org/10.5270/esa-pcnk2rv