Big Three Dragons: A N II 122 mm Constraint and New Dust-continuum Detection of a z = 7.15 Bright Lyman-break Galaxy with ALMA
Big Three Dragons: A z = 7.15 Lyman-break galaxy detected in O III 88 mm, C II 158 mm, and dust continuum with ALMA
Big Three Dragons: Molecular Gas in a Bright Lyman-break Galaxy at z = 7.15
Dual constraints with ALMA: new O III 88-mm and dust-continuum observations reveal the ISM conditions of luminous LBGs at z 7
From peculiar morphologies to Hubble-type spirals: the relation between galaxy dynamics and morphology in star-forming galaxies at z ~ 1.5
Normal, dust-obscured galaxies in the epoch of reionization
Obscured star formation in bright z 7 Lyman-break galaxies
Spatially resolved Kennicutt-Schmidt relation at z 7 and its connection with the interstellar medium properties
The discovery of rest-frame UV colour gradients and a diversity of dust morphologies in bright z 7 Lyman-break galaxies
The Roles of Morphology and Environment on the Star Formation Rate-Stellar Mass Relation in COSMOS from 0 < z < 3.5
Unveiling the nature of bright z 7 galaxies with the Hubble Space Telescope
Instrument
WFC3, WFC3/IR
Temporal Coverage
2014-11-18T17:55:51Z/2015-12-08T03:05:17Z
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, Bowler comma Rebecca A A, 2016, 'Unveiling the merger fraction, sizes and morphologies of the brightest z ~ 7 galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-skzzvh2