Clumpy Galaxies in CANDELS. II. Physical Properties of UV-bright Clumps at 0.5 <= z < 3
Clumpy Galaxies in CANDELS. I. The Definition of UV Clumps and the Fraction of Clumpy Galaxies at 0.5 < z < 3
Clustering dependence on Lya luminosity from MUSE surveys at 3 < z < 6
Constraining the cosmic UV background at z > 3 with MUSE Lyman-a emission observations
First gas-phase metallicity gradients of 0.1 z 0.8 galaxies with MUSE
The contribution of faint Lyman-a emitters to extended Lyman-a halos constrained by MUSE clustering measurements
The impact of satellite trails on Hubble Space Telescope observations
The MUSE Extremely Deep Field: Evidence for SFR-induced cores in dark-matter dominated galaxies at z 1
The MUSE eXtremely deep field: first panoramic view of an Mg II emitting intragroup medium
The MUSE Hubble Ultra Deep Field Survey. III. Testing photometric redshifts to 30th magnitude
The MUSE Hubble Ultra Deep Field Survey. II. Spectroscopic redshifts and comparisons to color selections of high-redshift galaxies
The MUSE Hubble Ultra Deep Field Survey. XIII. Spatially resolved spectral properties of Lyman a haloes around star-forming galaxies at z > 3
The MUSE Hubble Ultra Deep Field Survey. XII. Mg II emission and absorption in star-forming galaxies
UVUDF: Ultraviolet Through Near-infrared Catalog and Photometric Redshifts of Galaxies in the Hubble Ultra Deep Field
Instrument
WFC3, WFC3/UVIS
Temporal Coverage
2013-10-25T04:34:12Z/2014-09-12T15:07:29Z
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, Guo comma Yicheng, 2014, 'UV Snapshot of Low-redshift Massive Star-forming Galaxies: Searching for the Analogs of High-redshift Clumpy Galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-tie048h