Dancing in the Dark: New Brown Dwarf Binaries from Kernel Phase Interferometry
Direct measurements of the fundamental properties of low-mass stars and brown dwarfs
L-Dwarf Binaries in the 20-Parsec Sample
Long-term 4.6 mm Variability in Brown Dwarfs and a New Technique for Identifying Brown Dwarf Binary Candidates
Meeting the Cool Neighbors. X. Ultracool Dwarfs from the 2MASS All-Sky Data Release
NICMOS Kernel-phase Interferometry. I. Catalogue of Brown Dwarfs Observed in F110W and F170M
NICMOS Kernel-phase Interferometry. II. Demographics of Nearby Brown Dwarfs
Super resolution from diffraction limited images with kernel-phases
Instrument
NICMOS, NICMOS/NIC1
Temporal Coverage
2006-07-04T04:54:30Z/2007-05-09T17:35:29Z
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, Reid comma I. Neill, 2008, 'A search for planetary-mass companions to the nearest L dwarfs - completing the survey', 1.0, European Space Agency, https://doi.org/10.5270/esa-r7eok8k