Cloud structure of brown dwarfs from spectroscopic variability observations
Cloud Structure of the Nearest Brown Dwarfs: Spectroscopic Variability of Luhman 16AB from the Hubble Space Telescope
Maps of Evolving Cloud Structures in Luhman 16AB from HST Time-resolved Spectroscopy
The JWST weather report from the nearest brown dwarfs I: multiperiod JWST NIRSpec + MIRI monitoring of the benchmark binary brown dwarf WISE 1049AB
Instrument
WFC3, WFC3/IR
Temporal Coverage
2013-11-08T06:34:52Z/2014-06-07T00:17:39Z
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, Buenzli et al., 2015, 'Evolution of heterogeneous cloud structure through the T dwarf sequence', 1.0, European Space Agency, https://doi.org/10.5270/esa-mhohfhe