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WISE J085510.83-071442.5 was recently discovered as the coldest known brown dwarf based on four epochs of images from the Wide-field Infrared Survey Explorer and the Spitzer Space Telescope. We have improved the accuracy of its parallax…

Astrophysics of Galaxies · Physics 2015-06-22 K. L. Luhman , T. L. Esplin

We present initial results from a wide-field (30,000 deg^2) search for L/T transition brown dwarfs within 25 pc using the Pan-STARRS1 and WISE surveys. Previous large-area searches have been incomplete for L/T transition dwarfs, because…

We report the discovery of a bright (V ~ 13.7), extremely low-mass white dwarf in a close double degenerate system. We originally selected GALEX J171708.5+675712 for spectroscopic follow-up among a group of white dwarf candidates in an…

Solar and Stellar Astrophysics · Physics 2011-08-02 S. Vennes , J. R. Thorstensen , A. Kawka , P. Nemeth , J. N. Skinner , A. Pigulski , M. Steslicki , Z. Kolaczkowski , P. Srodka

We present the Late-Type Extension to the Motion Verified Red Stars (LaTE-MoVeRS) catalog, containing 46,463 photometric late-type ($>$ M5) dwarfs within the Sloan Digital Sky Survey (SDSS) footprint. Proper motions were computed for…

Solar and Stellar Astrophysics · Physics 2017-02-08 Christopher A. Theissen , Andrew A. West , Guillaume Shippe , Adam J. Burgasser , Sarah J. Schmidt

We present a parallax solution for WISE J135501.90-825838.9, a spectral binary with spectral types L7+T7.5 and candidate AB Doradus member. Using $WISE$ astrometry, we obtain a distance of $d = 16.7\pm5.3$ pc. This preliminary parallax…

Solar and Stellar Astrophysics · Physics 2020-05-15 C. A. Theissen , D. C. Bardalez Gagliuffi , J. K. Faherty , J. Gagne , A. J. Burgasser

We have monitored the position of the cool Y dwarf WISEPA J182831.08+265037.8 using a combination of ground- and space-based telescopes and have determined its distance to be 11.2$_{-1.0}^{+1.3}$ pc. Its absolute H magnitude,…

We present the serendipitous discovery of a late T-type brown dwarf candidate in JWST NIRCam observations of the Early Release Science Abell 2744 parallel field. The discovery was enabled by the sensitivity of JWST at 4~$\mu$m wavelengths…

We present a search for new planetary-mass members of nearby young moving groups (YMGs) using astrometry for 694 T and Y dwarfs, including 447 objects with parallaxes, mostly produced by recent large parallax programs from UKIRT and…

Earth and Planetary Astrophysics · Physics 2021-04-14 Zhoujian Zhang , Michael C. Liu , William M. J. Best , Trent J. Dupuy , Robert J. Siverd

We present new near-infrared photometry for seven late-type T dwarfs and nine Y-type dwarfs, and lower limit magnitudes for a tenth Y dwarf, obtained at Gemini Observatory. We also present a reanalysis of H-band imaging data from the Keck…

Solar and Stellar Astrophysics · Physics 2015-06-23 S. K. Leggett , Caroline V. Morley , M. S. Marley , D. Saumon

Using Keck laser guide star adaptive optics imaging, we have found that the T9 dwarf WISE J1217+1626 and T8 dwarf WISE J1711+3500 are exceptional binaries, with unusually wide separations (~0.8 arcsec, 8-15 AU), large near-IR flux ratios…

Solar and Stellar Astrophysics · Physics 2015-06-05 Michael C. Liu , Trent J. Dupuy , Brendan P. Bowler , S. K. Leggett , William M. J. Best

In this paper we present our project that aims at determining accurate distances and proper motions for the Y brown dwarf population using the Hubble Space Telescope. We validate the program with our first results, using a single new epoch…

Solar and Stellar Astrophysics · Physics 2020-12-09 Clemence Fontanive , Luigi R. Bedin , Daniella C. Bardalez Gagliuffi

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…

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.…

We report resolved near-infrared spectroscopy and photometry of the recently identified brown dwarf binary WISE J104915.57-531906.1AB, located 2.02+/-0.15 pc from the Sun. Low-resolution spectral data from Magellan/FIRE and IRTF/SpeX reveal…

Solar and Stellar Astrophysics · Physics 2015-06-15 Adam J. Burgasser , Scott S. Sheppard , K. L. Luhman

We analyze the spectrum of an unusually-low mass white dwarf, SDSSJ123410.37-022802.9 (0335-264-52000), found in our recent, white dwarf catalog from the SDSS DR1 data release. Two independent, model atmosphere fits result in an accurate…

We have measured high-precision parallaxes for a large sample of candidate young (~10-100 Myr) and intermediate-age (~100-600 Myr) ultracool dwarfs, with spectral types ranging from M8 to T2.5. These objects are compelling benchmarks for…

Solar and Stellar Astrophysics · Physics 2015-06-15 Michael C. Liu , Trent J. Dupuy , Katelyn N. Allers

We report the discovery of a close binary J0606+2132 (Gaia DR3 3423365496448406272) with $P_{\rm obs}=2.77$ days containing a possible massive white dwarf or a neutron star using the LAMOST spectroscopic data. By a joint fitting of the…

Solar and Stellar Astrophysics · Physics 2024-11-14 Xinlin Zhao , Song Wang , Pengfei Wang , Chuanjie Zheng , Haibo Yuan , Jifeng Liu

We present a Hubble Space Telescope/Wide-Field Camera 3 near infrared spectrum of the archetype Y dwarf WISEP 182831.08+265037.8. The spectrum covers the 0.9-1.7 um wavelength range at a resolving power of lambda/Delta lambda ~180 and is a…

The Backyard Worlds: Planet 9 citizen science project uses data from the Wide-field Infrared Survey Explorer to detect infrared objects with significant motion. In this work, we present the majority of the L and T dwarf candidates…

We present results from a Hubble Space Telescope imaging search for low-mass binary and planetary companions to 33 nearby brown dwarfs with spectral types of T8-Y1. Our survey provides new photometric information for these faint systems,…

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