An Atlas of Color-selected Quiescent Galaxies at z > 3 in Public JWST Fields
A Tentative Detection of an Emission Line at 1.6 mm for the z ~ 12 Candidate UDFj-39546284
A z = 1.85 galaxy group in CEERS: Evolved, dustless, massive intra-halo light and a brightest group galaxy in the making
Delving deep: A population of extremely dusty dwarfs observed by JWST
HALO7D II: The Halo Velocity Ellipsoid and Velocity Anisotropy with Distant Main-sequence Stars
Harnessing the Hubble Space Telescope Archives: A Catalog of 21,926 Interacting Galaxies
Morphology of Galaxies in JWST Fields: Initial Distribution and Evolution of Galaxy Morphology
PHIBSS: exploring the dependence of the CO-H2 conversion factor on total mass surface density at z<1.5
Sunyaev-Zeldovich effect and X-ray scaling relations from weak lensing mass calibration of 32 South Pole Telescope selected galaxy clusters
The 3D-HST Survey: Hubble Space Telescope WFC3/G141 Grism Spectra, Redshifts, and Emission Line Measurements for ~ 100,000 Galaxies
The impact of satellite trails on Hubble Space Telescope observations
The missing light of the Hubble Ultra Deep Field
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR
Temporal Coverage
2011-10-25T11:21:49Z/2013-02-27T01:22:38Z
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, Cooper comma Michael, 2013, 'Measuring the Star-Formation Efficiency of Galaxies at z > 1 with Sizes and SFRs from HST Grism Spectroscopy', 1.0, European Space Agency, https://doi.org/10.5270/esa-xpj5mit