A Gaia Data Release 3 View on the Tip of the Red Giant Branch Luminosity
arXiv:2304.06695 · doi:10.3847/1538-4357/accd69
Abstract
The tip of the red giant branch (TRGB) is a standard candle that can be used to help refine the determination of the Hubble constant. Data Release 3 (DR3) provides synthetic photometry constructed from low-resolution BP/RP spectra for Milky Way field stars that can be used to directly calibrate the luminosity of the TRGB in the Johnson-Cousins I band, where the TRGB is least sensitive to metallicity. We calibrate the TRGB luminosity using a two-dimensional maximum likelihood algorithm with field stars and synthetic photometry and parallaxes. For a high-contrast and low-contrast break (characterized by the values of the contrast parameter or the magnitude of the break ), we find = and mag respectively, or a midpoint of (sys) (stat) mag. This measurement improves upon the TRGB measurement from Li et al. (2022), as the higher precision photometry based on DR3 allows us to constrain two additional free parameters of the luminosity function. We also investigate the possibility of using DR3 synthetic photometry to calibrate the TRGB luminosity with Centauri, but find evidence of blending within the inner region for cluster member photometry that precludes accurate calibration with DR3 photometry. We instead provide an updated TRGB measurement of = mag in Centauri using ground-based photometry from the most recent version of the database described in Stetson et al. (2019), which gives = (stat) 0.10 (sys) mag when tied to the EDR3 parallax distance from the consensus of Vasiliev & Baumgardt (2021), Soltis et al. (2021), and Maíz Apellániz et al. (2022a).
17 pages, 10 figures, 3 tables. Accepted by ApJ
References in corpus (21)
- The Gaia mission
- A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team
- Gaia Early Data Release 3: Parallax bias versus magnitude, colour, and position
- Gaia Early Data Release 3: Photometric content and validation
- Gaia EDR3 view on Galactic globular clusters
- Accurate distances to Galactic globular clusters through a combination of Gaia EDR3, HST and literature data
- Distances to PHANGS Galaxies: New Tip of the Red Giant Branch Measurements and Adopted Distances
- Tip of the Red Giant Branch Distances. I. Optimization of a Maximum Likelihood Algorithm
- Cluster Cepheids with High Precision Gaia Parallaxes, Low Zeropoint Uncertainties, and Hubble Space Telescope Photometry
- Homogeneous photometry VII. Globular clusters in the Gaia era
- The Parallax of Omega Centauri Measured from Gaia EDR3 and a Direct, Geometric Calibration of the Tip of the Red Giant Branch and the Hubble Constant
- The Extragalactic Distance Database: The Color-Magnitude Diagrams and Tip of the Red Giant Branch Distances Catalog
- The Tip of the Red Giant Branch Distances to Type Ia Supernova Host Galaxies. IV. Color Dependence and Zero-Point Calibration
- Sharpening the Tip of the Red Giant Branch
- The parallax zero point offset from Gaia EDR3 data
- The Parallax Zero-Point of Gaia Early Data Release 3 from LAMOST Primary Red Clump Stars
- An estimation of the Gaia EDR3 parallax bias from stellar clusters and Magellanic Clouds data
- Gaia EDR3 Parallax Zero-point Offset based on W Ursae Majoris-type Eclipsing Binaries
- Bayesian Mass Estimates of the Milky Way II: The dark and light sides of parameter assumptions
- Relative distances of Omega Centauri and 47 Tucanae
- A Maximum Likelihood Calibration of the Tip of the Red Giant Branch Luminosity from High Latitude Field Giants using Gaia Early Data Release 3 Parallaxes
Cited by in corpus (5)
- The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
- Tip of the Red Giant Branch Distances with JWST. II. I-band Measurements in a Sample of Hosts of 10 SN Ia Match HST Cepheids
- The red giant branch tip in the SDSS, PS1, JWST, NGRST and Euclid photometric systems. Calibration in optical passbands using Gaia DR3 synthetic photometry
- Automated Identification of the Tip of the Red Giant Branch in Globular Clusters with Gaia Data
- Calibrating the Tip of the Red Giant Branch and measuring Magellanic Cloud distances to 2% exclusively with Gaia