525 datasets found

Keywords: trigonometric parallax

Filter Results
  • Ultracool and brown dwarf candidates

    Ultracool and brown dwarf candidates (d_{sun}<=125pc, |b|>8deg) were identified via multiband and astrometric data from CatWISE (W1, W2), 2MASS (J, H, Ks), and Gaia DR3...
  • Astrometry & phot. of Gaia DR3 open cluster Cepheids

    Classical Cepheids (CCs) in Galactic open clusters (OCs) provide essential observational constraints for calibrating the period-age relation (PAR) and the period-Wesenheit...
  • MiMO: 1232 Gaia DR3 open clusters param. & mass funct.

    We present a homogeneous catalog of 1232 open clusters with precisely determined ages, metallicities, distances, extinctions, and stellar mass function (MF) slopes, derived from...
  • Stellar encounters kinematics with beta Pic

    beta Pictoris is an A-type star that hosts a complex planetary system with two massive gas giants and a prominent debris disc. Variable absorption lines in its stellar spectrum...
  • Kinematic groups in USco with GaiaEDR3

    The improved astrometry precision of Gaia-eDR3 allows us to perform a detailed study of the Upper Scorpius OB association and revisit its spatial, kinematic, and age...
  • SB1s properties from GaiaDR3/TESS/ASAS-SN

    Gaia Data Release 3 (DR3) provides >181000 radial velocity (RV) solutions for single-lined spectroscopic binaries (SB1s) that can be used to search for non-interacting...
  • Classifying cool dwarfs

    Low-mass stars and brown dwarfs-spectral types (SpTs) M0 and later-play a significant role in studying stellar and substellar processes and demographics, reaching down to...
  • Photometry & RVs of YSOs in Messier 16

    We present a kinematic study of young stars in Messier 16 (M16) using the Gaia Data Release 3 and high-resolution spectra. A total of 345 stars are selected as genuine members...
  • NESSI: resolving wide binaries in Gaia & SUPERWIDE

    Stellar systems consisting of three or more stars are not an uncommon occurrence in the Galaxy. Nearly 50% of solar-type wide binaries with separations >1000AU are actually...
  • The value-added cat. of OB stars in LAMOST DR7

    In this work, we update the catalog of OB stars based on the Large Sky Area Multi-Object Fiber Spectroscopic Telescope data release 7 and modify the OB stars' selection criteria...
  • BSS in distant open clusters

    We identified blue straggler stars (BSSs) in 53 open clusters utilizing data from Gaia DR3. Most of these clusters are situated in the outer regions of the Galactic disk,...
  • 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...
  • California-Kepler Survey (CKS). II. Properties

    We present stellar and planetary properties for 1305 Kepler Objects of Interest hosting 2025 planet candidates observed as part of the California-Kepler Survey. We combine...
  • Velocity dispersion evolution in Sco-Cen OB

    We study how the stellar velocity dispersion within the Scorpius-Centaurus OB association (Sco-Cen) has evolved over approximately 20 million years, from its formation to the...
  • Catalog of Stellar Flares in 219 M-dwarfs

    We present a study of the relationship between Galactic kinematics, flare rates, chromospheric activity, and rotation periods for a volume-complete, nearly all-sky sample of 219...
  • Milky Way field giants from Gaia & APASS I-band

    The calibration of the tip of the red giant branch (TRGB) in the I-band has a direct role in determinations of the Hubble constant, a subject of recent interest due to the...
  • Gaia Focused Product Release (Gaia FPR)

    The Gaia Focused Product Release builds partly on the data period that went into Gaia's Data Release 3 but in case of the Solar System objects extends the stretch of time that...
  • Gaia DR3 Part 1. Main source

    Gaia Data Release 3 (Gaia DR3) will be released on 13 June 2022. The Gaia DR3 catalogue builds upon the Early Data Release 3 (released on 3 December 2020) and combines, for the...
  • Gaia EDR3

    Gaia DR3 data (both Gaia EDR3 and the full Gaia DR3) are based on data collected between 25 July 2014 (10:30 UTC) and 28 May 2017 (08:44 UTC), spanning a period of 34 months. As...
  • Gaia DR2

    Gaia Data Release 2. Summary of the contents and survey properties: We present the second Gaia data release, Gaia DR2, consisting of astrometry, photometry, radial velocities,...
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