A Deep Hubble Space Telescope Search for Escaping Lyman Continuum Flux at z ~ 1.3: Evidence for an Evolving Ionizing Emissivity
Expanding the Search for Galaxies at z ~ 7-10 with New NICMOS Parallel Fields
Exploring new emission line diagnostics for accreting compact objects
Far-ultraviolet Number Counts of Field Galaxies
The Stellar Mass Density and Specific Star Formation Rate of the Universe at z ~ 7
UV Continuum Slope and Dust Obscuration from z ~ 6 to z ~ 2: The Star Formation Rate Density at High Redshift
z ~ 7-10 Galaxies in the HUDF and GOODS Fields: UV Luminosity Functions
z ~ 7 Galaxy Candidates from NICMOS Observations Over the HDF-South and the CDF-South and HDF-North Goods Fields
Instrument
ACS, ACS/SBC, NICMOS, NICMOS/NIC3
Temporal Coverage
2006-09-18T14:32:58Z/2008-09-23T09:34:54Z
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, Teplitz comma Harry, 2009, 'Lyman Continuum Emission in Galaxies at z=1.2', 1.0, European Space Agency, https://doi.org/10.5270/esa-11xrd4k