2MASS J22521073-1730134: A Resolved L/T Binary at 14 Parsecs
A Search for Binary Systems among the Nearest L Dwarfs
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
Individual Dynamical Masses of Ultracool Dwarfs
Large-amplitude Variations of an L/T Transition Brown Dwarf: Multi-wavelength Observations of Patchy, High-contrast Cloud Features
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
Star Formation via the Little Guy: A Bayesian Study of Ultracool Dwarf Imaging Surveys for Companions
Super resolution from diffraction limited images with kernel-phases
The Hawaii Infrared Parallax Program. I. Ultracool Binaries and the L/T Transition
Instrument
NICMOS, NICMOS/NIC1
Temporal Coverage
2004-09-07T09:25:58Z/2006-06-29T11:35:02Z
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, 2007, 'Ultracool companions to the nearest L dwarfs', 1.0, European Space Agency, https://doi.org/10.5270/esa-cdvu4ce