A High Space Density of Luminous Lyman Alpha Emitters at z ~ 6.5
Beyond the Local Volume. II. Population Scaleheights and Ages of Ultracool Dwarfs in Deep HST/WFC3 Parallel Fields
HST Grism-derived Forecasts for Future Galaxy Redshift Surveys
Hubble Space Telescope Grism Spectroscopy of Extreme Starbursts across Cosmic Time: The Role of Dwarf Galaxies in the Star Formation History of the Universe
Low Masses and High Redshifts: The Evolution of the Mass-Metallicity Relation
Physical Properties of Emission-line Galaxies at z ~ 2 from Near-infrared Spectroscopy with Magellan FIRE
Predicting the Redshift 2 Ha Luminosity Function Using OIII Emission Line Galaxies
Proper Motions and Orbits of Distant Local Group Dwarf Galaxies from a Combination of Gaia and Hubble Data
WFC3 Infrared Spectroscopic Parallel (WISP) survey: photometric and emission-line data release
Instrument
WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2012-10-16T21:03:22Z/2014-03-20T14:07:57Z
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, Malkan et al., 2014, 'WFC3 Infrared Spectroscopic Parallel Survey WISP: A Survey of Star Formation Across Cosmic Time', 1.0, European Space Agency, https://doi.org/10.5270/esa-4bbvlio