Speckle interferometry at SOAR in 2016 and 2017
arXiv:1804.10553 · doi:10.3847/1538-3881/aabf8d
Abstract
The results of speckle interferometric observations at the 4.1 m SOAR telescope in 2016 and 2017 are given, totaling 2483 measurements of 1570 resolved pairs and 609 non-resolutions. We describe briefly recent changes in the instrument and observing method and quantify the accuracy of the pixel scale and position angle calibration. Comments are given on 44 pairs resolved here for the first time. Orbital motion of the newly resolved subsystem BU~83 Aa,Ab roughly agrees with its 36 year astrometric orbit proposed by J.~Dommanget. Most Tycho binaries examined here turned out to be spurious.
Accepted by AJ. 11 pages, 5 figures. Electronic tables 3,4 are available from the 1st author
References in corpus (9)
- Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties
- Speckle interferometry at SOAR in 2012 and 2013
- Ten years of speckle interferometry at SOAR
- SOAR Adaptive Module (SAM): seeing improvement with a UV laser
- Dancing twins: stellar hierarchies that formed sequentially?
- Orbits for eighteen visual binaries and two double-line spectroscopic binaries observed with HRCAM on the CTIO SOAR 4m telescope, using a new Bayesian orbit code based on Markov Chain Monte Carlo
- New orbits based on speckle interferometry at SOAR. II
- Speckle interferometry of secondary components in nearby visual binaries
- New binaries in the epsilon Cha association
Cited by in corpus (24)
- How to Constrain Your M dwarf II: the mass-luminosity-metallicity relation from 0.075 to 0.70
- TOI-1338: TESS' First Transiting Circumbinary Planet
- The TESS-Keck Survey II: An Ultra-Short Period Rocky Planet and its Siblings Transiting the Galactic Thick-Disk Star TOI-561
- Speckle interferometry at SOAR in 2018
- Speckle interferometry at SOAR in 2019
- Speckle Interferometry at SOAR in 2021
- TOI-132 b: A short-period planet in the Neptune desert transiting a G-type star
- TOI-1231 b: A Temperate, Neptune-Sized Planet Transiting the Nearby M3 Dwarf NLTT 24399
- Spectroscopic orbits of nearby stars
- Binary stars in Upper Scorpius
- Speckle Interferometry at SOAR in 2020
- Spectroscopic orbits of subsystems in multiple stars. III
- Observations of Binary Stars with the Differential Speckle Survey Instrument. VIII. Measures of Metal-Poor Stars and Triple Stars from 2015 to 2018
- Speckle observations and orbits of multiple stars
- New binaries from the SHINE survey
- Orbital and physical parameters of eclipsing binaries from the All-Sky Automated Survey catalogue - X. Three high-contrast systems with secondaries detected with IR spectroscopy
- Spectroscopic orbits of subsystems in multiple stars. IV. Double-lined pairs
- Yes, multi-periodic dwarfs in Upper Scorpius are binaries
- Young and eccentric: the quadruple system HD 86588
- Discovery of a substellar companion in the TESS light curve of the Scuti/ Doradus hybrid pulsator HD 31221
- Towards a consistent model of the hot quadruple system HD 93206 = QZ Carinae - I. Observations and their initial analyses
- On the correctness of orbital solutions obtained from a small set of points. Orbit of HIP 53731
- CD-27 11535: Evidence for a Triple System in the Pictoris Moving Group
- Hubble Space Telescope Snapshot Survey for Resolved Companions of Galactic Cepheids: Final Results