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Stellar parameters in Ophiuchus Stream with MMT
We present new kinematic data for the Ophiuchus stellar stream. Spectra have been taken of member candidates at the Multiple Mirror Telescope (MMT) using Hectospec, Hectochelle,... -
Gaia-Kepler stellar properties catalog.I. KIC stars
An accurate and precise Kepler Stellar Properties Catalog is essential for the interpretation of the Kepler exoplanet survey results. Previous Kepler Stellar Properties Catalogs... -
Hawaii IR parallax program. IV. L0-T8 BDs with UKIRT
We present parallaxes, proper motions, and J-band photometry for 348 L and T dwarfs measured using the wide-field near-infrared camera (WFCAM) on the United Kingdom Infrared... -
Young stellar objects in Lupus star-forming region
The identification and characterization of stellar members within a star-forming region are critical to many aspects of star formation, including formalization of the initial... -
Cataclysmic variables in the ZTF 1st-yr (2018-2019)
Using selection criteria based on amplitude, time, and color, we have identified 329 objects as known or candidate cataclysmic variables (CVs) during the first year of testing... -
Binary stars in Upper Scorpius
To address the statistics of binary stars in the 8 Myr old Upper Scorpius (USco) star formation region, we conducted a speckle interferometric survey of 614 association members... -
Low-mass stars from the first two TESS sectors
Continuous data releases throughout the Transiting Exoplanet Survey Satellite (TESS) primary mission will provide unique opportunities for the exoplanet community at large to... -
Stellar parameters of M and K dwarfs
Empirical correlations between stellar parameters such as rotation or radius and magnetic activity diagnostics require estimates of the effective temperatures and the stellar... -
RR Lyrae members of the Pal 5 stellar stream
Thin stellar streams, formed from the tidal disruption of globular clusters, are important gravitational tools, sensitive to both global and small-scale properties of dark... -
Spectrophotometric parallaxes with linear models
With contemporary infrared spectroscopic surveys like APO Galactic Evolution Experiment (APOGEE), red-giant stars can be observed to distances and extinctions at which Gaia... -
Local structure & star formation history of the MW
Gaia DR2 (Cat. I/345) provides unprecedented precision in measurements of the distance and kinematics of stars in the solar neighborhood. Through applying unsupervised machine... -
IR photometry of field RR Lyrae variable stars
We present multi-epoch infrared photometry in the K_s_-band for 74 bright RR Lyrae variable stars tied directly to the Two-Micron All-Sky Survey (2MASS) photometric system. We... -
Cloud Atlas: HST/WFC3 NIR spectral library
Bayesian atmospheric retrieval tools can place constraints on the properties of brown dwarfs' and hot Jupiters' atmospheres. To fully exploit these methods, high signal-to-noise... -
APOGEE and Gaia DR2 analysis of IC 166
IC 166 is an intermediate-age open cluster (OC) (~1 Gyr) that lies in the transition zone of the metallicity gradient in the outer disk. Its location, combined with our very... -
APOGEE-2 survey of Orion Complex. II.
We present an analysis of spectroscopic and astrometric data from APOGEE-2 and Gaia DR2 (Cat. I/345) to identify structures toward the Orion Complex. By applying a hierarchical... -
The solar neighborhood. XLIII. New nearby stars
We have conducted a novel search of most of the southern sky for nearby red dwarfs having low proper motions, with specific emphasis on those with {mu}<0.18"/yr, the lower... -
Orbits of subsystems in six multiple stars. III.
Spectroscopic orbits are computed for inner pairs in six nearby hierarchical multiple systems (HIP 35733, 95106/95110, 105441, 105585/105569, 105947, and 109951). Radial... -
The stellar membership of the Taurus SFR
The high-precision astrometry from the second data release of the Gaia mission (Cat. I/345) has made it possible to greatly improve the census of members of nearby clusters and... -
California-Kepler Survey. VII. Planet radius gap
The distribution of planet sizes encodes details of planet formation and evolution. We present the most precise planet size distribution to date based on Gaia parallaxes, Kepler... -
Stellar properties for M dwarfs in MEarth-South
Stellar rotation periods are valuable both for constraining models of angular momentum loss and for understanding how magnetic features impact inferences of exoplanet...
