Cosmological constraints from HII starburst galaxy, quasar angular size, and other measurements

Abstract

We compare the constraints from two (2019 and 2021) compilations of HII starburst galaxy (HIIG) data and test the model-independence of quasar angular size (QSO) data using six spatially flat and non-flat cosmological models. We find that the new 2021 compilation of HIIG data generally provides tighter constraints and prefers lower values of cosmological parameters than those from the 2019 HIIG data. QSO data by themselves give relatively model-independent constraints on the characteristic linear size, $l_{\mathrm{m}}$, of the QSOs within the sample. We also use Hubble parameter ($H(z)$), baryon acoustic oscillation (BAO), Pantheon Type Ia supernova (SN Ia) apparent magnitude (SN-Pantheon), and DES-3yr binned SN Ia apparent magnitude (SN-DES) measurements to perform joint analyses with HIIG and QSO angular size data, since their constraints are not mutually inconsistent within the six cosmological models we study. A joint analysis of $H(z)$, BAO, SN-Pantheon, SN-DES, QSO, and the newest compilation of HIIG data provides almost model-independent summary estimates of the Hubble constant, $H_0=69.7\pm 1.2\mathrm{km}{\mathrm{s}}^{-1}\mathrm{Mp}{\mathrm{c}}^{-1}$, the non-relativistic matter density parameter, ${\Omega }_{{\mathrm{m}}_0}=0.293\pm 0.021$, and $l_{\mathrm{m}}=10.93\pm 0.25$ pc.

13 pages, 6 figures, reference updated, MNRAS accepted version. arXiv admin note: text overlap with arXiv:2101.08817

References in corpus (29)

• Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z$\sim$2
• Cosmic Distances Calibrated to 1% Precision with Gaia EDR3 Parallaxes and Hubble Space Telescope Photometry of 75 Milky Way Cepheids Confirm Tension with LambdaCDM
• Measurements of the Hubble Constant: Tensions in Perspective
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Baryon acoustic oscillations with Lyman-$\alpha$ forests
• Hubble parameter measurement constraints on the redshift of the deceleration-acceleration transition, dynamical dark energy, and space curvature
• Eppur è piatto? The cosmic chronometer take on spatial curvature and cosmic concordance
• Measuring the Hubble constant with Type Ia supernovae as near-infrared standard candles
• A blinded determination of $H_0$ from low-redshift Type Ia supernovae, calibrated by Cepheid variables
• Ultra-compact structure in intermediate-luminosity radio quasars: building a sample of standard cosmological rulers and improving the dark energy constraints up to $z\sim 3$
• Using Pantheon and DES supernova, baryon acoustic oscillation, and Hubble parameter data to constrain the Hubble constant, dark energy dynamics, and spatial curvature
• The $L-\sigma$ relation for massive bursts of star formation
• An independent determination of the local Hubble constant
• Determining the range of validity of quasar X-ray and UV flux measurements for constraining cosmological model parameters
• A Lockdown Perspective on the Hubble Tension (with comments from the SH0ES team)
• Recombination-independent determination of the sound horizon and the Hubble constant from BAO
• Constraining cosmic curvature by using age of galaxies and gravitational lenses
• Constraining the Dark Energy Equation of State with HII Galaxies
• Standardized long gamma-ray bursts as a cosmic distance indicator
• Spectral analysis of Fermi-LAT gamma-ray bursts with known redshift and their potential use as cosmological standard candles
• Do quasar X-ray and UV flux measurements provide a useful test of cosmological models?
• Independent cosmological constraints from high-z HII galaxies: new results from VLT-KMOS data
• Independent Cosmological Constraints from high-z HII Galaxies
• Measuring cosmological parameters with a luminosity-time correlation of gamma-ray bursts
• Cosmological constraints from HII starburst galaxy apparent magnitude and other cosmological measurements
• Generalized tracker quintessence models for dark energy
• Probing modified gravity theories with multiple measurements of high-redshift quasars
• A 4% measurement of $H_0$ using the cumulative distribution of strong-lensing time delays in doubly-imaged quasars
• Cosmological Constraints using the newest VLT-KMOS HII Galaxies and the full Planck CMB spectrum
• Standardizing reverberation-measured Mg II time-lag quasars, by using the radius-luminosity relation, and constraining cosmological model parameters

Cited by in corpus (26)

• Challenges for $\Lambda$CDM: An update
• Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension
• Robust Preference for Dynamical Dark Energy in DESI BAO and SN Measurements
• Standardizing Platinum Dainotti-correlated gamma-ray bursts, and using them with standardized Amati-correlated gamma-ray bursts to constrain cosmological model parameters
• The state of the dark energy equation of state circa 2023
• Standardizing Dainotti-correlated gamma-ray bursts, and using them with standardized Amati-correlated gamma-ray bursts to constrain cosmological model parameters
• Revealing the effects of curvature on the cosmological models
• $H_0=69.8\pm 1.3$ $\mathrm{km}{\mathrm{s}}^{-1}\mathrm{Mp}{\mathrm{c}}^{-1}$, ${\Omega }_{m0}=0.288\pm 0.017$, and other constraints from lower-redshift, non-CMB, expansion-rate data
• Gamma-ray burst data strongly favor the three-parameter fundamental plane (Dainotti) correlation relation over the two-parameter one
• Inflation, the Hubble Tension and Early Dark Energy: an alternative overview
• Standardizing reverberation-measured C IV time-lag quasars, and using them with standardized Mg II quasars to constrain cosmological parameters
• Quasar UV/X-ray relation luminosity distances are shorter than reverberation-measured radius-luminosity relation luminosity distances
• Current data are consistent with flat spatial hypersurfaces in the $\Lambda$CDM cosmological model but favor more lensing than the model predicts
• Do reverberation-measured H$\beta$ quasars provide a useful test of cosmology?
• Consistency study of high- and low-accreting Mg ii quasars: No significant effect of the Fe ii to Mg ii flux ratio on the radius-luminosity relation dispersion
• Observational Constraints on Dynamical Dark Energy Models
• Effect of extinction on quasar luminosity distances determined from UV and X-ray flux measurements
• Testing the standardizability of, and deriving cosmological constraints from, a new Amati-correlated gamma-ray burst data compilation
• Effects of heterogeneous data sets and time-lag measurement techniques on cosmological parameter constraints from MgII and CIV reverberation-mapped quasar data
• Potentialities of Hubble parameter and expansion rate function data to alleviate Hubble tension
• Low- and high-redshift H II starburst galaxies obey different luminosity-velocity dispersion relations
• Tilted non-spatially-flat inflation
• Beyond Fisher Forecasting for Cosmology
• Testing the consistency of new Amati-correlated gamma-ray burst dataset cosmological constraints with those from better-established cosmological data
• Updated neutrino mass constraints from galaxy clustering and CMB lensing-galaxy cross-correlation measurements
• Bayesian Model Comparison of $R_h=ct$ versus $\Lambda$CDM using HII galaxy Hubble diagram