Absorption-line Spectroscopy of Gravitationally Lensed Galaxies: Further Constraints on the Escape Fraction of Ionizing Photons at High Redshift
A Magnified View of Star Formation at z = 0.9 From Two Lensed Galaxies
Hubble Space Telescope Ha imaging of star-forming galaxies at z 1-1.5: evolution in the size and luminosity of giant H II regions
Kinematics, turbulence, and star formation of z ~ 1 strongly lensed galaxies seen with MUSE
SMA Observations on Faint Submillimeter Galaxies with S 850 < 2 mJy: Ultra Dusty Low-luminosity Galaxies at High Redshift
The Density Profiles of Massive, Relaxed Galaxy Clusters. I. The Total Density Over Three Decades in Radius
The Hawaii SCUBA-2 Lensing Cluster Survey: Are Low-luminosity Submillimeter Galaxies Detected in the Rest-frame UV?
The missing light of the Hubble Ultra Deep Field
X-ray bright active galactic nuclei in massive galaxy clusters - III. New insights into the triggering mechanisms of cluster AGN
Instrument
WFC3, WFC3/IR
Temporal Coverage
2010-09-02T11:17:01Z/2010-09-02T13:40:21Z
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 comma Jane R., 2011, 'Resolved H alpha star formation in two lensed galaxies at z=0.9', 1.0, European Space Agency, https://doi.org/10.5270/esa-mg5zcim