A population of luminous accreting black holes with hidden mergers
Bright z ~ 9 Galaxies in Parallel: The Bright End of the Rest-frame UV Luminosity Function from HST Parallel Programs
Gaseous nebulae and massive stars in the giant H I ring in Leo
SuperBoRG: Exploration of Point Sources at z ~ 8 in HST Parallel Fields
SuperBoRG: Search for the Brightest of Reionizing Galaxies and Quasars in HST Parallel Imaging Data
The impact of satellite trails on Hubble Space Telescope observations
The missing light of the Hubble Ultra Deep Field
The Physical Properties of Luminous z 8 Galaxies and Implications for the Cosmic Star Formation Rate Density from 0.35 deg2 of (Pure-)Parallel HST Observations
The Proper-motion Field along the Magellanic Bridge: A New Probe of the LMC-SMC Interaction
The UV luminosity functions of bright z > 8 galaxies: determination from 0.41 deg2 of HST observations along 300 independent sightlines
The VMC survey. XXXVIII. Proper motion of the Magellanic Bridge
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2010-10-05T22:09:49Z/2012-01-03T15:15:53Z
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, Yan comma Haojing, 2012, 'Hubble Infrared Pure Parallel Imaging Extragalactic Survey {HIPPIES}', 1.0, European Space Agency, https://doi.org/10.5270/esa-i1s5uzs