Aeolus: A Markov Chain Monte Carlo Code for Mapping Ultracool Atmospheres. An Application on Jupiter and Brown Dwarf HST Light Curves
Cloud Atlas: Hubble Space Telescope Near-infrared Spectral Library of Brown Dwarfs, Planetary-mass Companions, and Hot Jupiters
Cloud structure of brown dwarfs from spectroscopic variability observations
HST Rotational Spectral Mapping of Two L-type Brown Dwarfs: Variability in and out of Water Bands indicates High-altitude Haze Layers
HST Spectral Mapping of L/T Transition Brown Dwarfs Reveals Cloud Thickness Variations
Informed Systematic Method to Identify Variable Mid- and Late-T Dwarfs
Revealing the Vertical Cloud Structure of a Young Low-mass Brown Dwarf, an Analog to the b-Pictoris b Directly Imaged Exoplanet, through Keck I/MOSFIRE Spectrophotometric Variability
Vertical Atmospheric Structure in a Variable Brown Dwarf: Pressure-dependent Phase Shifts in Simultaneous Hubble Space Telescope-Spitzer Light Curves
Instrument
WFC3, WFC3/IR
Temporal Coverage
2010-10-21T08:02:32Z/2011-10-10T20:47:23Z
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, Apai et al., 2012, 'Mapping Brown Dwarfs: The Evolution of Cloud Properties Through the L/T Transition', 1.0, European Space Agency, https://doi.org/10.5270/esa-f2vxvrv
