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相关论文: Characterization of High Proper Motion Objects fro…

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The photometry data base of the second phase of the OGLE microlensing experiment, OGLE-II, is a rich source of information about the kinematics and structure of the Galaxy. In this work we use the OGLE-II proper motion catalogue to identify…

天体物理学 · 物理学 2009-11-13 Nicholas J. Rattenbury , Shude Mao

Our aim is to compile a catalog of white dwarfs within 40 parsecs of the Sun, in which newly discovered objects would significantly increase the completeness of the current census. White dwarf candidates are identified from the SUPERBLINK…

太阳与恒星天体物理 · 物理学 2015-05-20 M. -M. Limoges , P. Bergeron , Sebastien Lepine

The aim of the project is to improve our current knowledge of the density of T dwarfs and the shape of the substellar initial mass function by identifying a magnitude-limited sample of T dwarfs in the full southern sky. We present the…

We present two confirmed wide separation L-dwarf common proper motion companions to nearby stars and one candidate identified from the Two Micron All Sky Survey. Spectral types from optical spectroscopy are L0 V, L2.5 V, and L8 V.…

天体物理学 · 物理学 2009-11-07 J. C. Wilson , J. Davy Kirkpatrick , J. E. Gizis , M. F. Skrutskie , D. G. Monet , J. R. Houck

Although many new brown dwarf (BD) neighbours have recently been discovered thanks to new sky surveys in the mid- and near-infrared (MIR, NIR), their numbers are still more than five times lower than those of stars in the same volume. Our…

太阳与恒星天体物理 · 物理学 2015-06-16 Gabriel Bihain , Ralf-Dieter Scholz , Jesper Storm , Olivier Schnurr

The Wide-field Infrared Survey Explorer (WISE) is a powerful tool for finding nearby brown dwarfs and searching for new planets in the outer solar system, especially with the incorporation of NEOWISE and NEOWISE-Reactivation data. So far,…

We present results from the PARallaxes of Southern Extremely Cool objects (PARSEC) program, an observational program begun in April 2007 to determine parallaxes for 122 L and 28 T southern hemisphere dwarfs using the Wide Field Imager on…

The aim of the Degenerate Objects around Degenerate Objects (DODO) survey is to search for very low mass brown dwarfs and extrasolar planets in wide orbits around white dwarfs via direct imaging. The direct detection of such companions…

地球与行星天体物理 · 物理学 2011-03-17 E. Hogan , M. R. Burleigh , F. J. Clarke

We present a new Y dwarf, WISE J030449.03-270508.3, confirmed from a candidate sample designed to pick out low temperature objects from the WISE database. The new object is typed Y0pec following a visual comparison with spectral standards,…

We present the discovery and spectroscopic follow-up of a nearby late-type L dwarf (2M0614+3950), and two extremely wide very-low-mass binary systems (2M0525-7425AB and 2M1348-1344AB), resulting from our search for common proper motion…

Five new objects with proper motions between 1.0 arcsec/yr and 2.6 arcsec/yr have been discovered via a new RECONS search for high proper motion stars utilizing the SuperCOSMOS Sky Survey. The first portion of the search, discussed here, is…

天体物理学 · 物理学 2009-11-10 N. C. Hambly , T. J. Henry , J. Subasavage , M. Brown , W. -C. Jao

The comparison of optical and 2MASS near-infrared photometry for large samples of catalogued proper motion stars has the potential to discover previously unrecognized nearby objects of rare type. In this paper we present the discovery of…

天体物理学 · 物理学 2009-11-07 Patrick J. Lowrance , J. Davy Kirkpatrick , I. Neill Reid , Kelle L. Cruz , James Liebert

We report the discovery of 182 new southern stars with proper motion larger than 0.45''/yr. The stars were found in an expansion of the SUPERBLINK proper motion survey to 8,980 square degrees south of Decl.=-30. The new high proper motion…

天体物理学 · 物理学 2008-11-26 Sebastien Lepine

We present the results of a search of infrared excess candidates in a comprehensive (29\,000 stars) magnitude limited sample of dwarf stars, spanning the spectral range F2-K0, and brighter than V$=$15 mag. We searched the sample within the…

太阳与恒星天体物理 · 物理学 2015-06-17 Fernando Cruz-Saenz de Miera , Miguel Chavez , Emanuele Bertone , Olga Vega

While quality checking a new motion-aware co-addition of all 12.5 months of WISE data, the source WISE J070720.48+170533.0 was found to have moved 0.9 arc-sec in 6 months. Backtracking this motion allowed us to identify this source as 2MASS…

Mapping out the populations of thick disk and halo brown dwarfs is important for understanding the metallicity dependence of low-temperature atmospheres and the substellar mass function. Recently, a new population of cold and metal-poor…

太阳与恒星天体物理 · 物理学 2023-07-19 A. M. Meisner , S. K. Leggett , S. E. Logsdon , A. C. Schneider , P. Tremblin , M. Phillips

We report the discovery of 14 low-mass binary systems containing mid-M to mid-L dwarf companions with separations larger than 250 AU. We also report the independent discovery of 9 other systems with similar characteristics that were…

We report near-infrared spectral model fits to seven distant L- and T-type dwarfs observed with the JWST Near Infrared Spectrograph (NIRSpec) as part of the Red Unknowns: Bright Infrared Extragalactic Survey (RUBIES). Comparison of 0.9-2.5…

太阳与恒星天体物理 · 物理学 2025-11-13 Sara J. Morrissey , Adam J. Burgasser , Anna de Graaff , Ian McConachie , Gabriel Brammer

The interpretation of high proper motion white dwarfs detected by Oppenheimer et al (2001) was the start of a lively controversy. While the discoverers identify a large fraction of their findings as dark halo members, others interpret the…

天体物理学 · 物理学 2009-11-07 Celine Reyle , Annie C. Robin , Michel Creze

Three nearby star candidates were selected as bright 2MASS point sources without associated optical sources, i.e. with potentially large proper motions, subsequently confirmed by multi-epoch optical data from the SuperCOSMOS Sky Surveys.…

天体物理学 · 物理学 2016-08-16 R. -D. Scholz , G. Lo Curto , R. A. Méndez , V. Hambaryan , E. Costa , T. J. Henry , A. D. Schwope