We present the discoveries of WISEA J041451.67−585456.7 and WISEA J181006.18−101000.5, two low-temperature (1200–1400 K), high proper motion T-type subdwarfs. Both objects were discovered via their high proper motion (>0".5 yr⁻¹); WISEA J181006.18−101000.5 as part of the NEOWISE proper motion survey and WISEA J041451.67−585456.7 as part of the citizen science project Backyard Worlds; Planet 9. We have confirmed both as brown dwarfs with follow-up near-infrared spectroscopy. Their spectra and near-infrared colors are unique among known brown dwarfs, with some colors consistent with L-type brown dwarfs and other colors resembling those of the latest-type T dwarfs. While no forward model consistently reproduces the features seen in their near-...
WISE1810-10 is the brightest metal-poor T-type object reported by Schneider et al. (2020) in a WISE ...
We present the discovery of seven ultracool brown dwarfs identified with the Wide-field Infrared Sur...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society....
We present the discoveries of WISEA J041451.67−585456.7 and WISEA J181006.18−101000.5, two low-tempe...
International audienceMapping out the populations of thick disk and halo brown dwarfs is important f...
Schneider et al. (2020) presented the discovery of WISEA J041451.67-585456.7 and WISEA J181006.18-10...
We report the discovery of ULAS J131610.28+075553.0, an sdT6.5 dwarf in the UKIDSS Large Area Survey...
International audienceWe have conducted a search for L subdwarf candidates within the photometric ca...
Aims. WISE provides an infrared all-sky survey that aims at completing our knowledge on the possibly...
International audienceWe report the discovery of an esdL3 subdwarf, ULAS J020858.62+020657.0, and a ...
We present the discovery of five late-type T dwarfs identified with the Wide-field Infrared Survey E...
Continued follow-up of WISEA J153429.75−104303.3, announced in Meisner et al., has proven it to have...
We report the discovery of the first new ultra-cool brown dwarf (BDs) found with the Wide-field Infr...
We report the discovery of 87 new T dwarfs uncovered with the Wide-field Infrared Survey Explorer (W...
We report the discovery of the L dwarf WISE J174102.78–464225.5, which was discovered as part of a s...
WISE1810-10 is the brightest metal-poor T-type object reported by Schneider et al. (2020) in a WISE ...
We present the discovery of seven ultracool brown dwarfs identified with the Wide-field Infrared Sur...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society....
We present the discoveries of WISEA J041451.67−585456.7 and WISEA J181006.18−101000.5, two low-tempe...
International audienceMapping out the populations of thick disk and halo brown dwarfs is important f...
Schneider et al. (2020) presented the discovery of WISEA J041451.67-585456.7 and WISEA J181006.18-10...
We report the discovery of ULAS J131610.28+075553.0, an sdT6.5 dwarf in the UKIDSS Large Area Survey...
International audienceWe have conducted a search for L subdwarf candidates within the photometric ca...
Aims. WISE provides an infrared all-sky survey that aims at completing our knowledge on the possibly...
International audienceWe report the discovery of an esdL3 subdwarf, ULAS J020858.62+020657.0, and a ...
We present the discovery of five late-type T dwarfs identified with the Wide-field Infrared Survey E...
Continued follow-up of WISEA J153429.75−104303.3, announced in Meisner et al., has proven it to have...
We report the discovery of the first new ultra-cool brown dwarf (BDs) found with the Wide-field Infr...
We report the discovery of 87 new T dwarfs uncovered with the Wide-field Infrared Survey Explorer (W...
We report the discovery of the L dwarf WISE J174102.78–464225.5, which was discovered as part of a s...
WISE1810-10 is the brightest metal-poor T-type object reported by Schneider et al. (2020) in a WISE ...
We present the discovery of seven ultracool brown dwarfs identified with the Wide-field Infrared Sur...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society....