Constraining C III Emission in a Sample of Five Luminous z = 5.7 Galaxies
Direct Gas-phase Metallicities, Stellar Properties, and Local Environments of Emission-line Galaxies at Redshifts below 0.90
Keck Spectroscopy of Lyman-break Galaxies and Its Implications for the UV-continuum and Lya Luminosity Functions at z > 6
Physical Properties of Spectroscopically Confirmed Galaxies at z >= 6. III. Stellar Populations from SED Modeling with Secure Lya Emission and Redshifts
Physical Properties of Spectroscopically Confirmed Galaxies at z >= 6. I. Basic Characteristics of the Rest-frame UV Continuum and Lya Emission
Physical Properties of Spectroscopically Confirmed Galaxies at z >= 6. II. Morphology of the Rest-frame UV Continuum and Lya Emission
The missing light of the Hubble Ultra Deep Field
Instrument
NICMOS, NICMOS/NIC3, WFC3, WFC3/IR
Temporal Coverage
2008-02-15T13:34:31Z/2010-08-14T07:23:25Z
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, Egami comma Eiichi, 2011, 'Characterizing the Stellar Populations in Lyman-Alpha Emitters and Lyman Break Galaxies at 5.7https://doi.org/10.5270/esa-28r1z70