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Related papers: Trigonometric parallaxes of ten ultracool subdwarf…

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We present trigonometric parallax and proper motion measurements for two T-type brown dwarfs. We derive our measurements from infrared laser guide star adaptive optics observations spanning five years from the ShaneAO/SHARCS and…

Solar and Stellar Astrophysics · Physics 2021-08-25 Jayke Nguyen , S. Mark Ammons , Kaitlin Dennison , E. Victor Garcia , Jessica R. Lu , Stephen McMillan , Maissa Salama

We report on the analysis of ~22,000 M dwarfs using a statistical parallax method. This technique employs a maximum-likelihood formulation to simultaneously solve for the absolute magnitude, velocity ellipsoid parameters and reflex solar…

Solar and Stellar Astrophysics · Physics 2010-12-17 Suzanne L. Hawley , John J. Bochanski , Andrew A. West

We present 160 new trigonometric parallaxes for 151 M dwarf systems from the REsearch Consortium On Nearby Stars (RECONS) group's long-term astrometry/photometry program at the CTIO/SMARTS 0.9m telescope. Most systems (124 or 82%) are found…

The A5V star Alcor has an M3-M4 dwarf companion, as evidenced by a novel astrometric technique. Imaging spectroscopy combined with adaptive optics coronagraphy allowed for the detection and spectrophotometric characterization of the point…

We report parallax measurements for 70 ultracool dwarfs (UCDs). Using both literature values and our sample, we report new polynomial relations between spectral type and M$_{JHK}$. Including resolved L/T transition binaries in the…

The photometry from 2MASS, UCAC3 and SuperCosmos catalogues together with the proper motions from the Tycho-2, XPM and UCAC3 catalogues are used to select the all-sky samples of 34 white dwarfs, 1996 evolved and 7769 unevolved subdwarfs…

Solar and Stellar Astrophysics · Physics 2015-05-18 George A. Gontcharov , Anisa T. Bajkova , Peter N. Fedorov , Vladimir S. Akhmetov

We report new parallax measurements for ten L and early T type dwarfs, five of which have no previous published values, using observations over 3 years at the robotic Liverpool Telescope. The resulting parallaxes and proper motions have…

Solar and Stellar Astrophysics · Physics 2018-05-23 Y. Wang , R. L. Smart , Z. Shao , H. R. A Jones , F. Marocco , A. Luo , A. Burgasser , J. Zhong , B. Du

We present optical spectroscopy and near-infrared photometry of 126 cool white dwarfs in the Sloan Digital Sky Survey (SDSS). Our sample includes high proper motion targets selected using the SDSS and USNO-B astrometry and a dozen…

Using the Wide Field Camera 3 (WFC3) on the Hubble Space Telescope (HST), we have obtained a direct trigonometric parallax for the nearest metal-poor globular cluster, NGC 6397. Although trigonometric parallaxes have been previously…

Solar and Stellar Astrophysics · Physics 2018-04-04 T. M. Brown , S. Casertano , J. Strader , A. Riess , D. A. VandenBerg , D. R. Soderblom , J. Kalirai , R. Salinas

We present an all-sky catalog of M dwarf stars with apparent infrared magnitude J<10. The 8,889 stars are selected from the ongoing SUPERBLINK survey of stars with proper motion >40 mas/yr, supplemented on the bright end with the TYCHO-2…

Solar and Stellar Astrophysics · Physics 2015-05-30 Sébastien Lépine , Eric Gaidos

Three ongoing microlensing experiments have found more candidate events than expected from the known stars. These experiments measure only one parameter of the massive compact halo objects (machos), the magnification time scale of the…

Astrophysics · Physics 2009-10-28 Thomas Boutreux , Andrew Gould

We present the discovery of seven new T dwarfs identified in the Two Micron All Sky Survey. Low-resolution (R$\sim$150) 0.8--2.5 micron spectroscopy obtained with the IRTF SpeX instrument reveal the characteristic H$_2$O and CH$_4$ bands in…

We present a catalog of 9888 M, L and T dwarfs detected in the Pan-STARRS1 3$\pi$ Survey (PS1), covering three-quarters of the sky. Our catalog contains nearly all known objects of spectral types L0-T2 in the PS1 field, with objects as…

We present a new luminosity-colour relation based on trigonometric parallaxes for thin disc main-sequence stars in SDSS photometry. We matched stars from the newly reduced Hipparcos catalogue with the ones taken from 2MASS All-Sky Catalogue…

Astrophysics of Galaxies · Physics 2015-05-13 S. Bilir , S. Karaali , S. Ak , K. B. Coskunoglu , E. Yaz , A. Cabrera-Lavers

We present the first results from our high-precision infrared (IR) astrometry program at the Canada-France-Hawaii Telescope. We measure parallaxes for 83 ultracool dwarfs (spectral types M6--T9) in 49 systems, with a median uncertainty of…

Solar and Stellar Astrophysics · Physics 2015-06-03 Trent J. Dupuy , Michael C. Liu

We present a new sample of M subdwarfs compiled from the 7th data release of the Sloan Digital Sky Survey. With 3517 new subdwarfs, this new sample significantly increases the number of spectroscopically confirmed low-mass subdwarfs. This…

Solar and Stellar Astrophysics · Physics 2015-06-22 Antonia Savcheva , Andrew A. West , John J. Bochanski

We aim at developing an efficient method to search for late-type subdwarfs (metal-depleted dwarfs with spectral types >M5) to improve the current statistics. Our objectives are: improve our knowledge of metal-poor low-mass dwarfs, bridge…

Solar and Stellar Astrophysics · Physics 2017-02-08 N. Lodieu , M. Espinoza Contreras , M. R. Zapatero Osorio , E. Solano , M. Aberasturi , E. L. Martin , C. Rodrigo

We have combined 2MASS and POSS II data in a search for nearby ultracool (later than M6.5) dwarfs with K_s<12. Spectroscopic follow-up observations identify 53 M7 to M9.5 dwarfs and seven L dwarfs. The observed space density is 0.0045 +-…

Trigonometric parallax astrometry and BVI photometry are presented for two late-type subdwarf candidates, LSR1425+71 (sdM8.0) and LSR1610-00 (sd?M6pec). For the former we measure an absolute parallax of 13.37+/-0.51 mas yielding…

We report the parallax and proper motion of five L dwarfs obtained with observations from the robotic Liverpool Telescope. Our derived proper motions are consistent with published values and have considerably smaller errors. Based on our…