The Solar Neighborhood. XIII. Parallax Results from the CTIOPI 0.9 Meter Program: Stars with μ ≥ 10 yr−1 (MOTION Sample)

@article{Jao2005TheSN,
  title={The Solar Neighborhood. XIII. Parallax Results from the CTIOPI 0.9 Meter Program: Stars with $\mu$ ≥ 10 yr−1 (MOTION Sample)},
  author={W. C. Jao and Todd J. Henry and John P. Subasavage and Misty A. Brown and Philip Anthony Ianna and Jennifer Lynn Bartlett and Edgardo Costa and Rene Mendz Georgia State University and University of Virginia and Universidad Catolica de Chile},
  journal={The Astronomical Journal},
  year={2005},
  volume={129},
  pages={1954 - 1967}
}
We present the first set of definitive trigonometric parallaxes and proper motions from the Cerro Tololo Inter-American Observatory Parallax Investigation. Full astrometric reductions for the program are discussed, including methods of reference star selection, differential color refraction corrections, and conversion of relative to absolute parallax. Using data acquired at the 0.9 m telescope at CTIO, full astrometric solutions and VRIJHKs photometry are presented for 36 red and white dwarf… 

Tables from this paper

The Solar Neighborhood. 22. Parallax Results from the CTIOPI 0.9 m Program: Trigonometric Parallaxes of 64 Nearby Systems With 0.5 or = mu or = 1.0 yr-1 (SLOWMO Sample)
We present trigonometric parallaxes of 64 stellar systems with proper motions between 0.″5 yr−1 and 1.″0 yr−1 from the ongoing Research Consortium On Nearby Stars parallax program at the Cerro Tololo
THE SOLAR NEIGHBORHOOD. XVI. PARALLAXES FROM CTIOPI: FINAL RESULTS FROM THE 1.5 m TELESCOPE PROGRAM
Trigonometric parallaxes, proper motions and VJ(RI)KC photometry are given for 25 stars (of which one is a zero-parallax control field) targeted by the Cerro Tololo Inter-American Observatory
The Solar Neighborhood. XIV. Parallaxes from the Cerro Tololo Inter-American Observatory Parallax Investigation-First Results from the 1.5 m Telescope Program
Trigonometric parallaxes, proper motions, and VJ(RI)KC photometry are presented for 31 stars targeted by the Cerro Tololo Inter-American Observatory Parallax Investigation (CTIOPI), a program of wide
THE SOLAR NEIGHBORHOOD. XXIV. PARALLAX RESULTS FROM THE CTIOPI 0.9 m PROGRAM: STARS WITH μ ⩾ 1.″0 yr–1 (MOTION SAMPLE) AND SUBDWARFS
We present 41 trigonometric parallaxes of 37 stellar systems, most of which have proper motions greater than 1.″0 yr−1. These are the first trigonometric parallaxes for 24 systems. Overall, there are
The Solar Neighborhood. XXXX. Parallax Results from the CTIOPI 0.9 m Program: New Young Stars Near the Sun
As a step toward completing and characterizing the census of the solar neighborhood, we present astrometric, photometric, and spectroscopic observations of 32 systems observed with the Cerro Tololo
THE SOLAR NEIGHBORHOOD. XXXVIII. RESULTS FROM THE CTIO/SMARTS 0.9 m: TRIGONOMETRIC PARALLAXES FOR 151 NEARBY M DWARF SYSTEMS
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 0.9 m
THE SOLAR NEIGHBORHOOD. XXXIII. PARALLAX RESULTS FROM THE CTIOPI 0.9 m PROGRAM: TRIGONOMETRIC PARALLAXES OF NEARBY LOW-MASS ACTIVE AND YOUNG SYSTEMS
We present basic observational data and association membership analysis for 45 young and active low-mass stellar systems from the ongoing Research Consortium On Nearby Stars photometry and astrometry
The Solar Neighborhood. XXXIX. Parallax Results from the CTIOPI and NOFS Programs: 50 New Members of the 25 parsec White Dwarf Sample
We present 114 trigonometric parallaxes for 107 nearby white dwarf (WD) systems from both the Cerro Tololo Inter-American Observatory Parallax Investigation (CTIOPI) and the U. S. Naval Observatory
The Solar Neighborhood. XLII. Parallax Results from the CTIOPI 0.9 m Program—Identifying New Nearby Subdwarfs Using Tangential Velocities and Locations on the H–R Diagram
Parallaxes, proper motions, and optical photometry are presented for 51 systems consisting of 37 cool subdwarf and 14 additional high proper motion systems. Thirty-seven systems have parallaxes
THE SOLAR NEIGHBORHOOD. XXI. PARALLAX RESULTS FROM THE CTIOPI 0.9 m PROGRAM: 20 NEW MEMBERS OF THE 25 PARSEC WHITE DWARF SAMPLE
We present accurate trigonometric parallaxes for 20 new members of the 25 pc white dwarf (WD) sample as part of the Discovery and Evalution of Nearby Stellar Embers (DENSE) project.77
...
...

References

SHOWING 1-10 OF 51 REFERENCES
The Solar Neighborhood. XII. Discovery of New High Proper Motion Stars with μ ≥ 04 yr−1 between Declinations −90° and −47°
We report the discovery of 141 new high proper motion systems (μ ≥ 0.″4 yr-1) in the southern sky (δ = -90° to -47°) brighter than UKST plate R59F = 16.5 via our SuperCOSMOS-RECONS search. When
The Solar Neighborhood. VII. Discovery and Characterization of Nearby Multiples in the CTIO Parallax Investigation
We report the discovery of eight new multiple star systems among 191 stellar systems targeted for parallax determinations in the RECONS (Research Consortium on Nearby Stars) southern parallax
Preliminary Parallaxes of 40 L and T Dwarfs from the US Naval Observatory Infrared Astrometry Program
We present preliminary trigonometric parallaxes and proper motions for 22 L dwarfs and 18 T dwarfs measured using the ASTROCAM infrared imager on the US Naval Observatory (USNO) 1.55 m Strand
The Solar Neighborhood. VIII. Discovery of New High Proper Motion Nearby Stars Using the SuperCOSMOS Sky Survey
Five new objects with proper motions between 1.″0 and 2.″6 yr-1 have been discovered via a new Research Consortium on Nearby Stars (RECONS) search for high proper motion stars using the SuperCOSMOS
Infrared Parallaxes for Methane T Dwarfs
We report final results from our 2.5 yr infrared parallax program carried out with the European Southern Observatory 3.5 m New Technology Telescope and the SOFI infrared camera. Our program targeted
Interferometric Astrometry of Proxima Centauri and Barnard's Star Using HUBBLE SPACE TELESCOPE Fine Guidance Sensor 3: Detection Limits for Substellar Companions
We report on a substellar-companion search utilizing interferometric fringe-tracking astrometry acquired with Fine Guidance Sensor 3 on the Hubble Space Telescope. Our targets were Proxima Centauri
Revised Coordinates and Proper Motions of the Stars in the Luyten Half-Second Catalog
We present refined coordinates and proper-motion data for the high proper-motion (HPM) stars in the Luyten Half-Second (LHS) catalog. The positional uncertainty in the original Luyten catalog is
The Solar Neighborhood. X. New Nearby Stars in the Southern Sky and Accurate Photometric Distance Estimates for Red Dwarfs
Photometric (VJRCIC) and spectroscopic (6000–9500 Å) observations of high–proper-motion stars discovered during the first phase of the SuperCOSMOS RECONS (SCR) search are used to estimate accurate
U.S. Naval Observatory CCD parallaxes of faint stars. I - Program description and first results
The U.S. Naval Observatory CCD trigonometric parallax program is described in detail, including the instrumentation employed, observing procedures followed, and reduction procedures applied.
The faintest stars: trigonometric CCD parallaxes
First results are presented from a trigonometric parallax program being carried out with a CCD detector on the 60» telescope at Palomar Mountain. New parallaxes for six extremely late M-dwarfs (M bol
...
...