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We have carried out a search for late-type T dwarfs in the UKIDSS Galactic Plane Survey 6th Data Release. The search yielded two persuasive candidates, both of which have been confirmed as T dwarfs. The brightest, UGPS J0521+3640 has been…

We present the first results of the ongoing Canada-France Brown Dwarfs Survey-InfraRed, hereafter CFBDSIR, a Near InfraRed extension to the optical wide-field survey CFBDS. Our final objectives are to constrain ultracool atmosphere physics…

Solar and Stellar Astrophysics · Physics 2015-05-18 P. Delorme , L. Albert , T. Forveille , E. Artigau , X. Delfosse , C. Reylé , C. J. Willott , E. Bertin , S. M. Wilkins , F. Allard , D. Arzoumanian

We have used blue near-infrared colours to select a group of 12 spectroscopically-confirmed UKIDSS T dwarfs later than T4. From amongst these we identify the first two kinematic halo T-dwarf candidates. Blue near-infrared colours have been…

We selected brown dwarf candidates from the seventh Data Release of the Sloan Digital Sky Survey (SDSS DR7) with new photometric selectioncriteria based on a parameteriaztion of well-known L and T dwarfs. Then we confirmed their status with…

Astrophysics of Galaxies · Physics 2010-01-21 Z. H. Zhang , H. R. A. Jones , D. J. Pinfield , R. S. Pokorny , Z. Han

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 arcsec…

We present the discovery of two brown dwarfs in the UKIRT Infrared Deep Sky Survey (UKIDSS) Deep Extragalactic Survey (DXS) Data Release 2. Both objects were selected photometrically from six square degrees in DXS for their blue J-K colour…

Astrophysics of Galaxies · Physics 2009-11-13 N. Lodieu , P. D. Dobbie , N. R. Deacon , B. P. Venemans , M. Durant

Context. Nearby isolated planetary mass objects are beginning to be discovered, but their individual properties are poorly constrained because their low surface temperatures and strong molecular self-absorption make them extremely faint.…

Aims. We try to identify ultra-cool dwarfs from the seventh Data Release of the Sloan Digital Sky Survey (SDSS DR7) with SDSS i-z and r-z colors. We also obtain proper motion data from SDSS, 2MASS, and UKIDSS and improve spectral typing…

Astrophysics of Galaxies · Physics 2009-08-18 Z. H. Zhang , R. S. Pokorny , H. R. A. Jones , D. J. Pinfield , P. S. Chen , Z. Han , D. Chen , M. C. Gálvez-Ortiz , B. Burningham

We have combined multi-epoch images from the Infrared Side Port Imager on the CTIO 4-meter telescope to derive a 3-sigma limit of J=21.7 for the ultra cool brown dwarf companion to WD 0806-661 (GJ 3483). We find that J-[4.5]>4.95, redder…

Solar and Stellar Astrophysics · Physics 2015-05-27 David R. Rodriguez , Ben Zuckerman , Carl Melis , Inseok Song

In recent years brown dwarfs have been extended to a new Y-dwarf class with effective temperatures colder than 500K and masses in the range 5-30 Jupiter masses. They fill a crucial gap in observable atmospheric properties between the much…

Solar and Stellar Astrophysics · Physics 2015-06-23 C. G. Tinney , Jacqueline K. Faherty , J. Davy Kirkpatrick , Mike Cushing , Caroline V. Morley , Edward L. Wright

We present deep VLT/NACO infrared imaging and spectroscopic observations of the brown dwarf 2MASSWJ1207334-393254, obtained during our on-going adaptive optics survey of southern young, nearby associations. This 25 MJup brown dwarf, located…

Astrophysics · Physics 2010-04-06 G. Chauvin , A. -M. Lagrange , C. Dumas , B. Zuckerman , D. Mouillet , I. Song , J. -L. Beuzit , P. Lowrance

We report the discovery of two L dwarfs (the new spectral class defined for dwarfs cooler than the M type) in a two-epoch CCD proper motion survey of 413 square degrees, complemented by infrared photometry from DENIS. One of them has a…

Astrophysics · Physics 2012-08-27 B. Goldman , X. Delfosse , T. Forveille , C. Afonso et al , : , the EROS collaboration

We report the identification of LSR J0745+2627 in the United Kingdom InfraRed Telescope Infrared Deep Sky Survey (UKIDSS) Large Area Survey (LAS) as a cool white dwarf with kinematics and age compatible with the thick-disk/halo population.…

We present new JHKL'M' photometry on the MKO system for a large sample of L and T dwarfs identified from SDSS and 2MASS and classified according to the scheme of Geballe et al. (2002). We have compiled a sample of 105 L and T dwarfs that…

Astrophysics · Physics 2007-05-23 D. A. Golimowski , S. K. Leggett , M. S. Marley , X. Fan. T. R. Geballe , G. R. Knapp

We present astrometric measurements of eleven nearby ultracool brown dwarfs of spectral types Y and late-T, based on imaging observations from a variety of space-based and ground-based telescopes. These measurements have been used to…

We identify new Y- and T-type brown dwarfs from the WISE All Sky data release using images obtained in filters that divide the traditional near-infrared H and J bands into two halves -- specifically CH4s & CH4l in the H and J2 & J3 in the…

The coolest known brown dwarfs are our best analogs to extrasolar gas-giant planets. The prolific detections of such cold substellar objects in the past two years has spurred intensive followup, but the lack of accurate distances is a key…

Solar and Stellar Astrophysics · Physics 2015-06-17 Trent J. Dupuy , Adam L. Kraus

We present near-infrared (1.15-2.50 microns) medium-resolution (R = 1700) spectroscopy of a sample of 23 brown dwarf candidates in the young Upper Sco association. We confirm membership of 21 brown dwarfs based on their spectral shape,…

Astrophysics · Physics 2009-11-13 N. Lodieu , N. C. Hambly , R. F. Jameson , S. T. Hodgkin

We present i and z photometry for 25 T dwarfs and one L dwarf. Combined with published photometry, the data show that the i - z, z - Y and z - J colors of T dwarfs are very red, and continue to increase through to the late-type T dwarfs,…

We report the discovery of an esdL3 subdwarf, ULAS J020858.62+020657.0, and a usdL4.5 subdwarf, ULAS J230711.01+014447.1. They were identified as L subdwarfs by optical spectra obtained with the Gran Telescopio Canarias, and followed up by…