JWST PRIMER: a lack of outshining in four normal z = 4 - 6 galaxies from the ALMA-CRISTAL Survey
On the nature and physical conditions of the luminous Ly a emitter CR7 and its rest-frame UV components
The ALMA-CRISTAL survey: Resolved kinematic studies of main sequence star-forming galaxies at 4 < z < 6
The ALMA-CRISTAL Survey: Spatially Resolved Star Formation Activity and Dust Content in 4 < z < 6 Star-forming Galaxies
The nature of CR7 revealed with MUSE: a young starburst powering extended Ly a emission at z = 6.6
The Roles of Morphology and Environment on the Star Formation Rate-Stellar Mass Relation in COSMOS from 0 < z < 3.5
Instrument
WFC3/IR
Temporal Coverage
2017-03-14T08:53:18Z/2017-11-21T19:59:39Z
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, Fan et al., 2018, 'Is Lyman Alpha Emitter CR7 Powered by a Direct Collapse Black Hole?', 1.0, European Space Agency, https://doi.org/10.5270/esa-feuaqni
Rights
Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.