Photometric metallicity and distance estimates for 136,000 RR Lyrae stars from Gaia DR3
arXiv:2206.07668 · doi:10.3847/1538-4357/acadd5
Abstract
We present a sample of 135,873 RR Lyrae stars (RRLs) with precise photometric-metallicity and distance estimates from our newly calibrated [Fe/H]/[Fe/H] and band absolute magnitude-metallicity relations. The [Fe/H] and [Fe/H] relations for type RRab and type RRc stars are obtained from nearly 2700 Gaia-identified RRLs with precise and measurements from the light curves and metallicity estimates from spectroscopy. Using 236 nearby RRLs with accurate distances estimated from parallax measurements with Gaia EDR3, new band absolute magnitude-metallicity relations and near-infrared period-absolute magnitude-metallicity relations are constructed. External checks, using other high-resolution spectroscopic sample of field RRLs and RRL members of globular clusters (GCs), show that the typical uncertainties in our photometric-metallicity estimates are about 0.24 and 0.16 dex for type RRab/c stars, respectively, without significant systematic bias with respect to high-resolution spectroscopic metallicity measurements. The accuracies of these metallicity estimates are much improved, especially for RRab stars, when compared to those provided by the Gaia DR3 release. Validations of our distance estimates, again by using members of GCs, show that the typical distance errors are only 3-4%. The distance modulus mag for the LMC and mag for the SMC are estimated from our RRab sample, respectively, and are in excellent agreement with previous measurements. The mean metallicities of the LMC and SMC derived in this work are also consistent with the previous determinations. Using our sample, a steep metallicity gradient of dex/kpc is found for the LMC, while a negligible metallicity gradient is obtained for the SMC.
16 pages, 18 figures and 6 tables, accepted by ApJ, the RRL catalog will be available at http://doi.org/10.5281/zenodo.6731860
References in corpus (29)
- Gaia Early Data Release 3: Parallax bias versus magnitude, colour, and position
- A distance to the Large Magellanic Cloud that is precise to one per cent
- Gaia EDR3 view on Galactic globular clusters
- The Catalina Surveys Periodic Variable Star Catalog
- A distance determination to the Small Magellanic Cloud with an accuracy of better than 2 percent based on late-type eclipsing binary stars
- Clustering of Local Group distances: publication bias or correlated measurements? I. The Large Magellanic Cloud
- Clustering of Local Group distances: publication bias or correlated measurements? III. The Small Magellanic Cloud
- The RR Lyrae Period - K Luminosity relation for Globular Clusters: an observational approach
- New near-infrared period-luminosity-metallicity relations for RR Lyrae stars and the outlook for Gaia
- Evidence for an Overluminosity of the Variable Star RR Lyr, and a Revised Distance to the LMC
- Standard Galactic Field RR Lyrae II: A Gaia DR2 calibration of the period-Wesenheit-metallicity relation
- The Parallax Zero-Point of Gaia Early Data Release 3 from LAMOST Primary Red Clump Stars
- The infrared JHK light curves of RR Lyr
- Gaia EDR3 Parallax Zero-point Offset based on W Ursae Majoris-type Eclipsing Binaries
- On the Use of Field RR Lyrae as Galactic Probes. II. A new S calibration to estimate their metallicity
- Chemical abundances of solar neighborhood RR Lyrae stars
- Milky Way Tomography with the SkyMapper Southern Survey. II. Photometric Re-calibration of SMSS DR2
- Metallicity of Galactic RR Lyrae from Optical and Infrared Light Curves: I. Period-Fourier-Metallicity Relations for Fundamental Mode RR Lyrae
- Probing the Galactic Halo with RR Lyrae Stars. II. The Substructures of the Milky Way
- Morphology and metallicity of the Small Magellanic Cloud using RRab stars
- Correction to the photometric magnitudes of the Gaia Early Data Release 3
- Probing the Galactic halo with RR Lyrae stars III. The chemical and kinematic properties of the stellar halo
- Discovery of A candidate Hypervelocity star originated from the Sagittarius Dwarf Spheroidal galaxy
- Kinematics and Multi Band Period-Luminosity-Metallicity Relation of RR Lyrae Stars via Statistical Parallax
- Metallicity of Galactic RR Lyrae from Optical and Infrared Light Curves: II. Period-Fourier-Metallicity Relations for First Overtone RR Lyrae
- Blazhko Effect in the first overtone RR Lyrae stars of the OGLE Galactic bulge collection
- Palomar Transient Factory and RR Lyrae: Metallicity-Light Curve Relation Based on ab-Type RR Lyrae in Kepler Field
- Metallicity dependence of the Blazhko effect
- A spatially dependent correction of Gaia EDR3 parallax zero-point offset based on 0.3 million LAMOST DR8 giant stars
Cited by in corpus (22)
- RR Lyrae From Binary Evolution: Abundant, Young and Metal-Rich
- RR Lyrae mid-infrared Period-Luminosity-Metallicity and Period-Wesenheit-Metallicity relations based on Gaia DR3 parallaxes
- Photometric metallicity for 694233 Galactic giant stars from Gaia DR3 synthetic Stromgren photometry. Metallicity distribution functions of halo sub-structures
- The SPHEREx Target List of Ice Sources (SPLICES)
- A Pristine-UNIONS view on the Galaxy: Kinematics of the distant spur feature of the Sagittarius stream traced by Blue Horizontal Branch stars
- Probing the Galactic halo with RR Lyrae stars -- IV. On the Oosterhoff dichotomy of RR Lyrae stars
- Photometric-Metallicity and Distance Estimates for 70,000 RR Lyrae Stars from the Zwicky Transient Facility
- RR Lyrae Stars in Intermediate-age Magellanic Clusters: Membership Probabilities and Delay Time Distribution
- RR Lyrae stars trace the Milky Way warp
- Determining the Scale Length and Height of the Milky Way's Thick Disc Using RR~Lyrae
- Discovery of the shell structure via break radii in the outer halo of the Milky Way
- Give to Ursa Minor what is Ursa Minor's: an updated census of the RR Lyrae population in the Ursa Minor dwarf galaxy based on Gaia DR3
- Rare Find: Discovery and chemo-dynamical properties of two s-process enhanced RR Lyrae stars
- A joint 1% calibration of the RR Lyrae & type-II Cepheid Leavitt laws yields homogeneous distances to 93 Galactic globular clusters
- Connections between the cycle-to-cycle light curve and O-C variations of the non-Blazhko RR Lyrae stars
- Toward more accurate RR Lyrae metallicities
- Exploring the Sagittarius stream with RR Lyrae Stars from Gaia Data Release 3
- First direct detection of an RR Lyrae star conclusively associated with an intermediate-age cluster
- Decoding RR Lyrae light curves with deep learning for accurate absolute magnitude estimation
- Probing the Milky Way Halo with RR Lyrae Stars from Gaia Data Release 3
- rrlfe: Software for Generating and Applying Metallicity Calibrations for RR Lyrae Variable Stars Across a Wide Range of Phases and Temperatures
- Epicyclic Density Variations in the Indus Stellar Stream