Relativistic corrections for measuring Hubble's constant to 1% using stellar standard candles
arXiv:2108.09067 · doi:10.1051/0004-6361/202141644
Abstract
Relativistic corrections are estimated for classical Cepheids and the Tip of the Red Giant Branch (TRGB stars), to enable future unbiased 1% measurements of Hubble's constant, . We considered four effects: corrections, time-dilation, the apparent change of host dust extinction due to non-comoving reference frames, and the change of observed color due to redshift. Extinction-dependent corrections were computed using stellar atmosphere models applicable to giant stars for in HST, JWST, and 2MASS filters. The optical-NIR Wesenheit function advantageously combines filters with oppositely signed corrections and avoids complications due to host extinction. For TRGB stars, the JWST/NIRCAM F277W filter combines insensitivity to reddening with corrections % at Coma cluster distances. Missing corrections for host extinction due to circumgalactic or circumstellar material are discussed as potential systematics for TRGB distances although their impacts are insufficient to explain differences between based on Cepheid or TRGB supernova calibrations. All stellar standard candles require relativistic corrections to achieve an unbiased 1% measurement in the future. The combined relativistic correction involving , redshift-Leavitt bias, and the redshift-dependence of the Wesenheit function yield an increase of the Cepheid-based by km/s/Mpc to km/s/Mpc and raises the tension with the {\it Planck} value from to . For TRGB stars, we estimate a increase of reported by Freedman et al. (to km/s/Mpc) and a small decrease by for reported by Anand et al. (to km/s/Mpc). The opposite sign of these corrections is due to different reddening systematics and reduces the difference between the studies by km/s/Mpc.[abridged]
arXiv commentA&A in press (accepted: 2021-11-08). 21 pages, 10 figures, 6 tables
References in corpus (86)
- SciPy 1.0--Fundamental Algorithms for Scientific Computing in Python
- Array Programming with NumPy
- Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
- Astropy: A Community Python Package for Astronomy
- Measuring Reddening with SDSS Stellar Spectra and Recalibrating SFD
- PARSEC: stellar tracks and isochrones with the PAdova and TRieste Stellar Evolution Code
- Binary companions of evolved stars in APOGEE DR14: Search method and catalog of ~5,000 companions
- Correcting for the Effects of Interstellar Extinction
- A 2.4% Determination of the Local Value of the Hubble Constant
- In the Realm of the Hubble tension a Review of Solutions
- Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
- Grids of stellar models with rotation - I. Models from 0.8 to 120 Msun at solar metallicity (Z = 0.014)
- Observational Probes of Cosmic Acceleration
- Tensions between the Early and the Late Universe
- The Circumgalactic Medium
- The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch
- Cosmic Distances Calibrated to 1% Precision with Gaia EDR3 Parallaxes and Hubble Space Telescope Photometry of 75 Milky Way Cepheids Confirm Tension with LambdaCDM
- Cosmicflows-2: The Data
- Milky Way Cepheid Standards for Measuring Cosmic Distances and Application to Gaia DR2: Implications for the Hubble Constant
- Measurements of the Hubble Constant: Tensions in Perspective
- Gaseous Galaxy Halos
- The Expansion of the Universe is Faster than Expected
- Calibration of the Tip of the Red Giant Branch (TRGB)
- Tip of the Red Giant Branch Distances. II. Zero-Point Calibration
- Asteroseismology of old open clusters with Kepler: direct estimate of the integrated RGB mass loss in NGC6791 and NGC6819
- Testing a Predictive Theoretical Model for the Mass Loss Rates of Cool Stars
- K-corrections and Extinction Corrections for Type Ia Supernovae
- An Improved Distance to NGC 4258 and its Implications for the Hubble Constant
- AGB Variables and the Mira Period-Luminosity Relation
- A New Version of Reimers' law of Mass Loss Based on a Physical Approach
- The Extragalactic Distance Database: Color-Magnitude Diagrams
- The second and third parameters of the Horizontal Branch in Globular Clusters
- Hubble Space Telescope Observations of Mira Variables in the Type Ia Supernova Host NGC 1559: An Alternative Candle to Measure the Hubble Constant
- A Generalized correction for Type Ia Supernovae: Comparing R-band Photometry Beyond z=0.2 with B, V, and R-band Nearby Photometry
- Tip of the Red Giant Branch Distances. I. Optimization of a Maximum Likelihood Algorithm
- On the Effect of Rotation on Populations of Classical Cepheids II. Pulsation Analysis for Metallicities 0.014, 0.006, and 0.002
- YBC, a stellar bolometric corrections database with variable extinction coefficients: an application to PARSEC isochrones
- OGLE-ing the Magellanic System: Optical Reddening Maps of the Large and Small Magellanic Cloud from Red Clump Stars
- The "Tip" of the Red Giant Branch as a distance indicator: results from evolutionary models
- Mass loss on the red giant branch: the value and metallicity dependence of Reimers' η in globular clusters
- 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
- Comparing Tip of the Red Giant Branch Distance Scales: An Independent Reduction of the Carnegie-Chicago Hubble Program and the Value of the Hubble Constant
- Large Magellanic Cloud Near-Infrared Synoptic Survey. I. Cepheid variables and the calibration of the Leavitt Law
- The HST Key Project on the Extragalactic Distance Scale. XV. A Cepheid Distance to the Fornax Cluster and Its Implications
- The Extragalactic Distance Database: The Color-Magnitude Diagrams and Tip of the Red Giant Branch Distances Catalog
- The brightness of the Red Giant Branch tip: Theoretical framework, a set of reference models, and predicted observables
- VLT/FLAMES spectroscopy of red giant branch stars in the Fornax dwarf spheroidal galaxy
- The Red Giant Branch in Near-Infrared Colour-Magnitude Diagrams. II: The luminosity of the Bump and the Tip
- Dust in the Circumgalactic Medium of Low-Redshift Galaxies
- The Cepheid period -- luminosity -- metallicity relation based on Gaia DR2 data
- A Near-Infrared Period-Luminosity Relation for Miras in NGC 4258, an Anchor for a New Distance Ladder
- The X-Shooter Spectral Library (XSL): Data Release 2
- The parallax zero point offset from Gaia EDR3 data
- The Milky Way Cepheid Leavitt law based on Gaia DR2 parallaxes of companion stars and host open cluster populations
- Infrared Tip of the Red Giant Branch and Distances to the Maffei/IC 342 Group
- The effect of metallicity on Cepheid Period-Luminosity relations from a Baade-Wesselink analysis of Cepheids in the Milky Way and Magellanic Clouds
- Fundamental parameters, integrated RGB mass loss and dust production in the Galactic globular cluster 47 Tucanae
- Fast Winds and Mass Loss from Metal-Poor Field Giants
- Empirical calibration of the reddening maps in the Magellanic Clouds
- The influence of metallicity on the Leavitt Law from geometrical distances of Milky Way and Magellanic Clouds Cepheids
- The Carnegie-Chicago Hubble Program. IX. Calibration of the Tip of the Red Giant Branch Method in the Mega-Maser Host Galaxy, NGC4258 (M106)
- The circumstellar envelopes of the Cepheids L Car and RS Pup - Comparative study in the infrared with Spitzer, VLT/VISIR and VLTI/MIDI
- Characterizing the abundance, properties, and kinematics of the cool circumgalactic medium of galaxies in absorption with SDSS DR16
- Large Magellanic Cloud Near-Infrared Synoptic Survey. V. Period-Luminosity Relations of Miras
- The Accuracy of the Hubble Constant Measurement Verified through Cepheid Amplitudes
- Infrared Light Curves of Mira Variable Stars from COBE DIRBE Data
- Astrophysical Distance Scale The JAGB Method: I. Calibration and a First Application
- The need for accurate redshifts in supernova cosmology
- On the red giant branch mass loss in 47 Tucanae: Constraints from the horizontal branch morphology
- Using the Tip of the Red Giant Branch as a Distance Indicator in the Near Infrared
- Extended envelopes around Galactic Cepheids IV. T Monocerotis and X Sagittarii from mid-infrared interferometry with VLTI/MIDI
- On Cepheid Distance Scale Bias due to Stellar Companions and Cluster Populations
- The Hubble constant and new discoveries in cosmology
- A Direct Stellar Metallicity Determination in the Disk of the Maser Galaxy NGC4258
- A thin shell of ionized gas explaining the IR excess of classical Cepheids
- Inspecting the Cepheid distance ladder: The Hubble Space Telescope distance to the SNIa host galaxy NGC 5584
- An Overview of the Rotational Behavior of Metal--Poor Stars
- On a new and homogeneous metallicity scale for Galactic classical Cepheids - I. Physical parameters
- Empirical determination of the integrated red giant and horizontal branch stellar mass loss in omega Centauri
- Analysing the spectral energy distributions of Galactic classical Cepheids
- Mass loss law for red giant stars in simple population globular clusters
- Mira Variable Stars From LAMOST DR4 Data: Emission Features, Temperature Types, and Candidate Selection
- On the Color-Metallicity Relation of the Red Clump and the Reddening Toward the Magellanic Clouds
- Towards a 1% Measurement of the Hubble Constant: Accounting for Time Dilation in Variable Star Light Curves
- Stellar-Encounter Driven Red-Giant Star Mass-Loss in Globular Clusters
- Multi-Wavelength, Optical (VI) and Near-Infrared (JHK) Calibration of the Tip of the Red Giant Branch Method based on Milky Way Globular Clusters