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
Dust Extinction from Balmer Decrements of Star-forming Galaxies at 0.75 <= z <= 1.5 with Hubble Space Telescope/Wide-Field-Camera 3 Spectroscopy from the WFC3 Infrared Spectroscopic Parallel Survey
HST Grism-derived Forecasts for Future Galaxy Redshift Surveys
HST/WFC3 Near-infrared Spectroscopy of Quenched Galaxies at z ~ 1.5 from the WISP Survey: Stellar Population Properties
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
Spectroscopically Identified Emission Line Galaxy Pairs in the WISP Survey
The average dust attenuation curve at z 1.3 based on HST grism surveys
The missing light of the Hubble Ultra Deep Field
WFC3 Infrared Spectroscopic Parallel (WISP) survey: photometric and emission-line data release
Instrument
WFC3, WFC3/IR
Temporal Coverage
2011-10-29T06:06:35Z/2014-01-23T00:23:02Z
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 comma Matthew A., 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-2vacij9