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Related papers: Four new T dwarfs identified in PanSTARRS 1 commis…

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We present near-infrared parallax and proper motion astrometry for 74 L-dwarfs and 99 T-dwarfs, as single objects or in binary systems, obtained with the ASTROCAM astrometric imager on the USNO, Flagstaff Station 1.55-m telescope over two…

We present the discovery of a very cold, very low mass, nearby brown dwarf using data from the NASA Wide-field Infrared Survey Explorer (WISE). The object, WISE J064723.23-623235.5, has a very red WISE color of W1-W2 > 3.77 mag and a very…

Studies of brown dwarfs as a distinct galactic population have been largely pioneered by dedicated, vast-area surveys at deep optical and near-infrared wavebands. The Two Micron All Sky Survey has, because of its full-sky coverage and…

Astrophysics · Physics 2007-05-23 J. Davy Kirkpatrick

We report the results of a deep photometric search for planets and brown dwarfs in the nearby young OB Upper Scorpius association. We obtained optical (I) and near-infrared (JKs) images around nine very low-mass stars and brown dwarf member…

Astrophysics · Physics 2009-11-11 M. T. Costado , V. J. S. Bejar , J. A. Caballero , R. Rebolo , J. Acosta-Pulido , A. Manchado

In our effort to complete the census of low-mass stars and brown dwarfs in the immediate Solar Neighborhood, we present spectra, photometry, proper motions, and distance estimates for forty-two low-mass star and brown dwarf candidates…

Brown dwarf spectra are rich in information revealing of the chemical and physical processes operating in their atmospheres. We apply a recently developed atmospheric retrieval tool to an ensemble of late T-dwarf (600-800K) near infrared…

Young brown dwarfs share many properties with directly imaged giant extrasolar planets. They therefore provide unique laboratories for investigating the full range of temperature and mass encompasses by the growing collection of planets…

Solar and Stellar Astrophysics · Physics 2017-04-12 Adam C. Schneider , James Windsor , Michael C. Cushing , J. Davy Kirkpatrick

How confident are we that all of the nearest white dwarfs (WDs) have been identified? In an effort to answer this question, we have begun an initiative to identify and characterize new nearby WDs, particularly in the southern hemisphere. We…

We present the first X-ray detections of ultracool dwarfs (UCDs) from the first all-sky survey of the extended ROentgen Survey with an Imaging Telescope Array (eROSITA) onboard the Russian Spektrum-Roentgen-Gamma (SRG) mission. We use three…

Solar and Stellar Astrophysics · Physics 2022-05-25 B. Stelzer , A. Klutsch , M. Coffaro , E. Magaudda , M. Salvato

We explore the spectral and atmospheric properties of brown dwarfs cooler than the latest known T dwarfs. Our focus is on the yet-to-be-discovered free-floating brown dwarfs in the \teff range from $\sim$800 K to $\sim$130 K and with masses…

Astrophysics · Physics 2008-11-26 Adam Burrows , David Sudarsky , Jonathan Lunine

We present Spitzer 5-15 micron spectroscopy of one cool white dwarf and 3.6-8 micron photometry of 51 cool white dwarfs with T_eff < 6000 K. The majority of our targets have accurate BVRIJHK photometry and trigonometric parallax…

Solar and Stellar Astrophysics · Physics 2011-02-11 Mukremin Kilic , Piotr M. Kowalski , William T. Reach , Ted von Hippel

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

One of the main scientific drivers of the Space InfraRed Telescope Facility (SIRTF) is the search for brown dwarfs and extrasolar superplanets. We discuss observational strategies for identification of these objects, and conclude that an…

Brown dwarfs are compact objects that do not reach temperatures high enough to produce sustained hydrogen fusion. Consequently, they cool over time, gradually evolving through later spectral types. In fact, three new spectral types (L, T,…

Solar and Stellar Astrophysics · Physics 2026-05-20 A. R. Callen , I. H. Bustos Fierro , M. Gómez

Large area observations of extragalactic deep fields with the James Webb Space Telescope (JWST) have provided a wealth of candidate low-mass L- and T-class brown dwarfs. The existence of these sources, which are at derived distances of…

Ultracool dwarfs (UCDs) are objects with spectral types equal or later than M7. Most of them have been discovered using wide-field imaging surveys. The Virtual Observatory (VO) has proven to be of great utility to efficiently exploit these…

We review the available near- and mid- infrared photometry data sets for white dwarfs from the Two Micron All-Sky Survey (2MASS) Point Source Catalog and the Spitzer Space Telescope. These data sets have been widely used to search for white…

Astrophysics · Physics 2007-05-23 P. -E. Tremblay , P. Bergeron

We present the results of a search for cool white dwarfs in the United Kingdom InfraRed Telescope (UKIRT) Infrared Deep Sky Survey (UKIDSS) Large Area Survey (LAS). The UKIDSS LAS photometry was paired with the Sloan Digital Sky Survey…

Solar and Stellar Astrophysics · Physics 2015-05-27 S. K. Leggett , N. Lodieu , P. -E. Tremblay , P. Bergeron , A. Nitta

By selecting astrometric and photometric data from the Sloan Digital Sky Survey (SDSS), the L{\'e}pine & Shara Proper Motion North Catalog (LSPM-North), the Two Micron All Sky Survey (2MASS), and the USNO-B1.0 catalog, we use a succession…

Solar and Stellar Astrophysics · Physics 2015-06-04 Conor Sayres , John P. Subasavage , P. Bergeron , P. Dufour , James R. A. Davenport , Yusra AlSayyad , Benjamin M. Tofflemire

We present spectra of 59 nearby stars candidates, M dwarfs and white dwarfs, previously identified using high proper motion catalogues and the DENIS database. We review the existing spectral classification schemes and spectroscopic parallax…

Astrophysics · Physics 2009-11-11 C. Reyle , R. -D. Scholz , M. Schultheis , A. C. Robin , M. Irwin
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