Gaia EDR3 Parallax Zero-point Offset based on W Ursae Majoris-type Eclipsing Binaries
arXiv:2103.16096 · doi:10.3847/2041-8213/abf359
Abstract
We independently determine the zero-point offset of the Gaia early Data Release-3 (EDR3) parallaxes based on W Ursae Majoris (EW)-type eclipsing binary systems. EWs cover almost the entire sky and are characterized by a relatively complete coverage in magnitude and color. They are an excellent proxy for Galactic main-sequence stars. We derive a -band Period-Luminosity relation with a distance accuracy of , which we use to anchor the Gaia parallax zero-point. The final, global parallax offsets are as and as (before correction) and as and as (after correction) for the five- and six-parameter solutions, respectively. The total systematic uncertainty is as. The spatial distribution of the parallax offsets shows that the bias in the corrected Gaia EDR3 parallaxes is less than 10 as across of the sky. Only of the sky is characterized by a parallax offset greater than 30 as. Thus, we have provided independent evidence that the parallax zero-point correction provided by the Gaia team significantly reduces the prevailing bias. Combined with literature data, we find that the overall Gaia EDR3 parallax offsets for Galactic stars are as and 4-10 as, respectively, before and after correction. For specific regions, an additional deviation of about 10 as is found.
arXiv comment7 pages, 4 figures. Accepted for publication in The Astrophysical Journal Letters
References in corpus (23)
- Gaia Data Release 2. Summary of the contents and survey properties
- The Gaia mission
- A 3D Dust Map Based on Gaia, Pan-STARRS 1 and 2MASS
- Gaia Early Data Release 3: The astrometric solution
- Cosmic Distances Calibrated to 1% Precision with Gaia EDR3 Parallaxes and Hubble Space Telescope Photometry of 75 Milky Way Cepheids Confirm Tension with LambdaCDM
- Gaia Data Release 1: Astrometry - one billion positions, two million proper motions and parallaxes
- The Optical to Mid-Infrared Extinction Law Based on the APOGEE, Gaia DR2, Pan-STARRS1, SDSS, APASS, 2MASS and WISE Surveys
- The ASAS-SN Catalog of Variable Stars I: The Serendipitous Survey
- Gaia Early Data Release 3 -- Catalogue validation
- A First Catalog of Variable Stars Measured by the Asteroid Terrestrial-impact Last Alert System (ATLAS)
- The Zwicky Transient Facility Catalog of Periodic Variable Stars
- Parallax Systematics and Photocenter Motions of Benchmark Eclipsing Binaries in Gaia EDR3
- Confirmation of the DR2 parallax zero-point offset using asteroseismology and spectroscopy in the field
- Absolute Magnitude Calibration for the W UMa-type Systems Based on Hipparcos Data
- Contact Binaries with Additional Components. II. A Spectroscopic Search for Faint Tertiaries
- Wide-field Infrared Survey Explorer (WISE) Catalog of Periodic Variable Stars
- Evidence for a systematic offset of 0.25 mas in the Gaia DR1 parallaxes
- The Parallax Zero-Point of Gaia Early Data Release 3 from LAMOST Primary Red Clump Stars
- Optical-Mid-Infrared Period-Luminosity Relations for W UMa-type Contact Binaries Based on Gaia DR 1: 8% Distance Accuracy
- Contact Binaries as Viable Distance Indicators: New, Competitive (V)JHKs Period-Luminosity Relations
- Distance Dependent Offsets between Parallaxes for Nearby Stars and Gaia DR1 Parallaxes
- Absolute Magnitude Calibration for W UMa-Type Systems Based on Gaia Data
- Eclipsing Binary Populations across the Northern Galactic Plane from the KISOGP survey
Cited by in corpus (35)
- Gaia Data Release 3: Summary of the content and survey properties
- The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
- Distance estimates for AGB stars from parallax measurements
- The parallax zero point offset from Gaia EDR3 data
- A 0.9% Calibration of the Galactic Cepheid luminosity scale based on Gaia DR3 data of open clusters and Cepheids
- Photometric metallicity and distance estimates for 136,000 RR Lyrae stars from Gaia DR3
- The value-added catalogue for LAMOST DR8 low-resolution spectra
- Substructure in the stellar halo near the Sun. II. Characterisation of independent structures
- Investigation of the Orbital Period and Mass Relations for W UMa-type Contact Systems
- The period--luminosity relation for Mira variables in the Milky Way using Gaia DR3: a further distance anchor for
- J-PLUS: Spectral evolution of white dwarfs by PDF analysis
- Stars that approach within one parsec of the Sun: New and more accurate encounters identified in Gaia Data Release 3
- Extremely low-mass white dwarf stars observed in Gaia DR2 and LAMOST DR8
- Cepheid metallicity in the Leavitt law (C-MetaLL) survey -- III. Simultaneous derivation of the Gaia parallax offset and Period-Luminosity-Metallicity coefficients
- Asteroseismology of overmassive, undermassive, and potential past members of the open cluster NGC6791
- Exploring the stellar rotation of early-type stars in the LAMOST Medium-Resolution Survey. I. Catalog
- The use of double-mode RR Lyrae stars as robust distance and metallicity indicators
- A Gaia Data Release 3 View on the Tip of the Red Giant Branch Luminosity
- Investigating Gaia EDR3 parallax systematics using asteroseismology of Cool Giant Stars observed by Kepler, K2, and TESS II. Deciphering Gaia parallax systematics using red clump stars
- A spatially dependent correction of Gaia EDR3 parallax zero-point offset based on 0.3 million LAMOST DR8 giant stars
- The Photo-Astrometric Vertical Tracer Density of the Milky Way II: Results from Gaia
- HD144941: The most extreme helium-strong star
- Investigating Gaia EDR3 parallax systematics using asteroseismology of Cool Giant Stars observed by Kepler, K2, and TESS I. Asteroseismic distances to 12,500 red-giant stars
- 3D Parameter Maps of Red Clump Stars in the Milky Way -- Absolute Magnitudes and Intrinsic Colors
- The lightcurve intrinsic variability in 47 Kepler contact binary stars
- Probing galactic double-mode RR Lyrae stars against Gaia EDR3
- A Geometric Calibration of the Tip of the Red Giant Branch in the Milky Way using Gaia DR3
- Physical Properties of 29 sdB+dM Eclipsing Binaries in Zwicky Transient Facility
- Gaia EDR3 parallaxes of type I X-ray bursters and their implications on the models of type I X-ray bursts: a generic approach to the Gaia parallax zero-point and its uncertainty
- Galaxy Rotation Parameters from OB2 Stars with Proper Motions and Parallaxes from the Gaia EDR3 Catalog
- Link between the Optical and Radio Frames from Gaia DR3 Data and VLBI Measurements
- Orbital parallax of binary systems compared to GAIA DR3 and the parallax zero-point offset at bright magnitudes
- The Environments around W Serpentis Systems: Independent Limits on System Masses and Extended Envelopes
- Kinematics of the Galaxy from Young Open Star Clusters with Data from the Gaia EDR3 Catalogue
- The First Photometric Study of AH Mic Contact Binary System