A 30 kpc Spatially Extended Clumpy and Asymmetric Galactic Outflow at z 1.7
A clumpy and anisotropic galaxy halo at redshift 1 from gravitational-arc tomography
ALMA Resolves the Molecular Gas in a Young Low-metallicity Starburst Galaxy at z = 1.7
A Magnified View of the Kinematics and Morphology of RCSGA 032727-132609: Zooming in on a Merger at z = 1.7
Dissecting a 30 kpc galactic outflow at z 1.7
Resolved Star Formation on Sub-galactic Scales in a Merger at z = 1.7
Source-plane Reconstruction of the Bright Lensed Galaxy RCSGA 032727-132609
Spatially resolved galactic wind in lensed galaxy RCSGA 032727-132609
The impact of satellite trails on Hubble Space Telescope observations
The Magellan Evolution of Galaxies Spectroscopic and Ultraviolet Reference Atlas (MegaSaura). I. The Sample and the Spectra
The missing light of the Hubble Ultra Deep Field
Instrument
WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2011-03-01T03:39:20Z/2011-03-01T09:11:24Z
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, Rigby et al., 2012, 'Dissecting star formation, extinction, and stellar populations in the brightest lensed galaxy', 1.0, European Space Agency, https://doi.org/10.5270/esa-37ffsj1