A 5% measurement of the Hubble constant from Type II supernovae

Abstract

The most stringent local measurement of the Hubble-Lemaître constant from Cepheid-calibrated Type Ia supernovae (SNe~Ia) differs from the value inferred via the cosmic microwave background radiation ({\it Planck}$+\Lambda$CDM) by $\sim 5\sigma$. This so-called "Hubble tension" has been confirmed by other independent methods, and thus does not appear to be a possible consequence of systematic errors. Here, we continue upon our prior work of using Type II supernovae to provide another, largely-independent method to measure the Hubble-Lemaître constant. From 13 SNe~II with geometric, Cepheid, or tip of the red giant branch (TRGB) host-galaxy distance measurements, we derive H${}_0=75.4_{-3.7}^{+3.8}$\,km\,s${}^{-1}$\,Mpc${}^{-1}$ (statistical errors only), consistent with the local measurement but in disagreement by $\sim 2.0\sigma$ with the {\it Planck}$+\Lambda$CDM value. Using only Cepheids ($N=7$), we find H${}_0=77.6_{-4.8}^{+5.2}$\,km\,s${}^{-1}$\,Mpc${}^{-1}$, while using only TRGB ($N=5$), we derive H${}_0=73.1_{-5.3}^{+5.7}$\,km\,s${}^{-1}$\,Mpc${}^{-1}$. Via 13 variants of our dataset, we derive a systematic uncertainty estimate of 1.5\,km\,s${}^{-1}$\,Mpc${}^{-1}$. The median value derived from these variants differs by just 0.3\,km\,s${}^{-1}$\,Mpc${}^{-1}$ from that produced by our fiducial model. Because we only replace SNe~Ia with SNe~II -- and we do not find statistically significant difference between the Cepheid and TRGB H${}_0$ measurements -- our work reveals no indication that SNe~Ia or Cepheids could be the sources of the "H${}_0$ tension." We caution, however, that our conclusions rest upon a modest calibrator sample; as this sample grows in the future, our results should be verified.

arXiv comment10 pages, 4 figures, 2 tables. Accepted for publication by MNRAS. arXiv admin note: text overlap with arXiv:2006.03412

References in corpus (68)

• SciPy 1.0--Fundamental Algorithms for Scientific Computing in Python
• Array Programming with NumPy
• Astropy: A Community Python Package for Astronomy
• emcee: The MCMC Hammer
• Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
• Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
• The Supernova Legacy Survey: Measurement of Omega_M, Omega_Lambda and w from the First Year Data Set
• The Zwicky Transient Facility: System Overview, Performance, and First Results
• 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
• The Cosmic Microwave Background Spectrum from the Full COBE/FIRAS Data Set
• A 3% Solution: Determination of the Hubble Constant with the Hubble Space Telescope and Wide Field Camera 3
• Gaia Early Data Release 3: The astrometric solution
• The Hyper Suprime-Cam SSP Survey: Overview and Survey Design
• The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch
• A Redetermination of the Hubble Constant with the Hubble Space Telescope from a Differential Distance Ladder
• Cosmic Distances Calibrated to 1% Precision with Gaia EDR3 Parallaxes and Hubble Space Telescope Photometry of 75 Milky Way Cepheids Confirm Tension with LambdaCDM
• A distance to the Large Magellanic Cloud that is precise to one per cent
• 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
• New Parallaxes of Galactic Cepheids from Spatially Scanning the Hubble Space Telescope: Implications for the Hubble Constant
• Cosmology from Maxima-1, Boomerang and COBE/DMR CMB Observations
• The Sloan Digital Sky Survey-II Supernova Survey: Technical Summary
• The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
• The Hubble Constant
• The Hubble Constant: A Summary of the HST Program for the Luminosity Calibration of Type Ia Supernovae by Means of Cepheids
• Toward a New Geometric Distance to the Active Galaxy NGC 4258. III. Final Results and the Hubble Constant
• The Carnegie Supernova Project: The Low-Redshift Survey
• An Improved Distance to NGC 4258 and its Implications for the Hubble Constant
• AGB Variables and the Mira Period-Luminosity Relation
• Cosmological parameters from the comparison of peculiar velocities with predictions from the 2M++ density field
• Type II Supernovae as Standardized Candles
• First Cosmological Results using Type Ia Supernovae from the Dark Energy Survey: Measurement of the Hubble Constant
• Hubble Space Telescope Observations of Mira Variables in the Type Ia Supernova Host NGC 1559: An Alternative Candle to Measure the Hubble Constant
• Consistent Calibration of the Tip of the Red Giant Branch in the Large Magellanic Cloud on the Hubble Space Telescope Photometric System and a Re-determination of the Hubble Constant
• Distance determinations using type II supernovae and the expanding photosphere method
• The Carnegie Supernova Project: Absolute Calibration and the Hubble Constant
• Supernova Simulations and Strategies For the Dark Energy Survey
• A Study of the Type II-Plateau Supernova 1999gi, and the Distance to its Host Galaxy, NGC 3184
• The Hubble Constant from Infrared Surface Brightness Fluctuation Distances
• Measuring the Hubble constant with Type Ia supernovae as near-infrared standard candles
• Improved Standardization of Type II-P Supernovae: Application to an Expanded Sample
• The Standardized Candle Method for Type II Plateau Supernovae
• The Cepheid Distance to NGC 1637: A Direct Test of the EPM Distance to SN 1999em
• A measurement of the Hubble constant from Type II supernovae
• 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
• 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 Type II-Plateau Supernova 2017eaw in NGC 6946 and Its Red Supergiant Progenitor
• Type II-P Supernovae from the SDSS-II Supernova Survey and the Standardized Candle Method
• The Berkeley sample of Type II supernovae: BVRI light curves and spectroscopy of 55 SNe II
• A Robust Tip of the Red Giant Branch Distance to the Fireworks Galaxy (NGC 6946)
• The extra-galactic Cepheid distance scale from LMC and Galactic period-luminosity relations
• Determining the Hubble Constant without the Sound Horizon Scale: Measurements from CMB Lensing
• Spectral modeling of type II supernovae. I. Dilution factors
• The Cepheid Distance to the Seyfert 1 Galaxy NGC 4151
• A Hubble diagram from Type II Supernovae based solely on photometry: the Photometric-Colour Method
• Spectral modeling of type II supernovae II. A machine learning approach to quantitative spectroscopic analysis
• Peculiar velocities in the local Universe: comparison of different models and the implications for $H_0$ and dark matter
• A Type II Supernova Hubble diagram from the CSP-I, SDSS-II, and SNLS surveys
• SN 2016jhj at redshift 0.34: extending the Type II supernova Hubble diagram using the standard candle method
• A supernova distance to the anchor galaxy NGC 4258
• Cosmicflows-4: The Baryonic Tully-Fisher Relation Providing ~10,000 Distances
• Studying Type II supernovae as cosmological standard candles using the Dark Energy Survey
• Type II Supernovae as Distance Indicators at Near-IR Wavelengths
• The effects of peculiar velocities in SN Ia environments on the local $H_0$ measurement

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• The Local Distance Network: a community consensus report on the measurement of the Hubble constant at 1% precision
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• Thermal Friction as a Solution to the Hubble and Large-Scale Structure Tensions
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• The Hubble constant from two sibling Type Ia supernovae in the nearby galaxy NGC 4414: SN 1974G and SN 2021J
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• Two Dynamical Scenarios for Binned Master Sample Interpretation
• A New Window on Dynamical Dark Energy: Combining DESI-DR2 BAO with future Gravitational Wave Observations
• Application of the FRADO model of BLR formation to the Seyfert galaxy NGC 5548 and the first step toward determining the Hubble constant
• One Extension to Explain Them All, One Scale-Invariant Spectrum to Test Them All, and in One Model Bind Them
• ParamANN: A Neural Network to Estimate Cosmological Parameters for $\Lambda$CDM Universe Using Hubble Measurements
• An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$
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• Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: ${\Lambda }_{\mathrm{s}}$CDM versus $\Lambda$CDM
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