Astrometric information of the 135 spectroscopic OB stars in the regions NGC 6334 and NGC 6357. For each star spectral type, equatorial coordinates, V and G magnitudes, GAIA...

Observational tests of stellar and Galactic chemical evolution call for the joint knowledge of a star's physical parameters, detailed element abundances, and precise age. For...

We extended the sample of 35 eclipsing binaries compiled by Graczyk+ (2017ApJ...837....7G) by searching for detached systems in the literature suitable for a precise distance...

We obtained near infra-red (NIR) spectra for 58 of our 62 nearby binary targets using the SpeX spectrograph on the NASA Infrared Telescope Facility (IRTF) atop Maunakea....

The sample of stars used for this study is comprised of known OB members of Cygnus OB2 within a radius of 1{deg} of the coordinates l=79.8 and b=+0.8. This produced a sample of...

The twin method is applied to determine parallaxes for stars in the RAVE survey. The method is based on the proposition that if two stars have the same spectra (hence twins)...

The TIC is used to help identify two-minute cadence target selection for the Transiting Exoplanet Survey Satellite (TESS) mission, and to calculate physical and observational...

In this paper we compile and derive lists of members for 2017 open clusters. We employ an artificial neural network to estimate cluster parameters (extinction Av, distance...

United States Naval Observatory (USNO) Robotic Astrometric Telescope (URAT) Parallax Catalog south (UPCs) and north (UPCn). These data are based on the accepted paper for the...

UFMG clusters parameters and memberlists.

A source list of objects toward the Lupus star-forming region is constructed from archived Infrared Array Camera (IRAC) images in the Spitzer Heritage Archive. These images span...

The Zwicky Transient Facility (ZTF) is a northern all-sky survey that uses the Palomar 48 inch telescope equipped with a 47deg^2^ field-of-view camera (Bellm+,...

The full best matches catalogue (Table B.1) is given, containing the highest reliability matches from Gaia DR2 for all true, likely, and possible PNe in HASH, for which the...

In this paper, we present a survey of those very low-proper-motion stars, along with astrometric, photometric, and spectroscopic follow-up observations for selected...

Table A.1 lists the properties of the 283 Taurus stars analysed in the paper. The stars were selected from the catalogue of spectroscopically confirmed members by Esplin &...

We present the Star cluster Hunting Pipeline (SHiP) that can identify star clusters in Gaia second data release (DR2) data and establish a star cluster catalog for the Galactic...

The VVV Infrared Astrometric Catalog (VIRAC) collects the proper motion measurements based on the VISTA Variables in the Via Lactea (VVV) survey data. It provides ZYJHKs...

We have obtained high resolution spectra for a volume-limited sample of 118 field M dwarfs. From these observations we derive projected rotational velocities and fluxes in the...

NIR high-resolution spectral observations of stars toward the Orion Complex were conducted with the Apache Point Observatory Galactic Evolution Experiment (APOGEE) spectrograph,...

Our sample of subgiants consists of 245 stars that have been continuously monitored by the Lick and Keck subgiant planet surveys since 2004 and 2007, respectively (see Table 1)....