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
Is NGC 300 a pure exponential disk galaxy?
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 impact of satellite trails on Hubble Space Telescope observations
WFC3 Infrared Spectroscopic Parallel (WISP) survey: photometric and emission-line data release
Instrument
WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2015-11-30T15:11:42Z/2017-04-27T15:34:00Z
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., 2017, 'WFC3 Infrared Spectroscopic Parallel Survey: The WISP Deep Fields', 1.0, European Space Agency, https://doi.org/10.5270/esa-fxfxijw