Cosmological constraints from HII starburst galaxy apparent magnitude and other cosmological measurements

Abstract

We use HII starburst galaxy apparent magnitude measurements to constrain cosmological parameters in six cosmological models. A joint analysis of HII galaxy, quasar angular size, baryon acoustic oscillations peak length scale, and Hubble parameter measurements result in relatively model-independent and restrictive estimates of the current values of the non-relativistic matter density parameter ${\Omega }_{{\mathrm{m}}_0}$ and the Hubble constant $H_0$. These estimates favor a 2.0$\sigma$ to 3.4$\sigma$ (depending on cosmological model) lower $H_0$ than what is measured from the local expansion rate. The combined data are consistent with dark energy being a cosmological constant and with flat spatial hypersurfaces, but do not strongly rule out mild dark energy dynamics or slightly non-flat spatial geometries.

arXiv comment16 pages, 6 figures, MNRAS, in press. Removed observational data that will appear in Gonzalez-Moran's PhD thesis (in preparation) and added comments about early-Universe and late-Universe Hubble constant determinations

References in corpus (107)

• emcee: The MCMC Hammer
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
• The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample
• Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
• A Quantitative Comparison of SMC, LMC, and Milky Way UV to NIR Extinction Curves
• Everything You Always Wanted To Know About The Cosmological Constant Problem (But Were Afraid To Ask)
• The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch
• Cosmological implications of baryon acoustic oscillation (BAO) measurements
• The Stellar, Gas and Dynamical Masses of Star-Forming Galaxies at z~2
• The Expansion of the Universe is Faster than Expected
• Calibration of the Tip of the Red Giant Branch (TRGB)
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: First measurement of Baryon Acoustic Oscillations between redshift 0.8 and 2.2
• Dark Energy Survey Year 1 Results: Constraints on Extended Cosmological Models from Galaxy Clustering and Weak Lensing
• Hubble parameter measurement constraints on the cosmological deceleration-acceleration transition redshift
• Gamma-Ray Bursts as a Probe of the Very High Redshift Universe
• Gamma-Ray Bursts as a Probe of the Very High Redshift Universe
• Hubble parameter measurement constraints on the redshift of the deceleration-acceleration transition, dynamical dark energy, and space curvature
• Hubble Parameter and Baryon Acoustic Oscillation Measurement Constraints on the Hubble Constant, the Deviation from the Spatially-Flat $\Lambda$cdm Model, The Deceleration-Acceleration Transition Redshift, and Spatial Curvature
• Setting the Stage for Cosmic Chronometers. II. Impact of Stellar Population Synthesis Models Systematics and Full Covariance Matrix
• Dark Energy Survey Year 1 Results: A Precise H0 Measurement from DES Y1, BAO, and D/H Data
• Distance measures in cosmology
• $H_0$ from cosmic chronometers and Type Ia supernovae, with Gaussian Processes and the novel Weighted Polynomial Regression method
• Baryon acoustic oscillations at z = 2.34 from the correlations of Ly$\alpha$ absorption in eBOSS DR14
• A Hubble Diagram for Quasars
• Confirmation of a Star Formation Bias in Type Ia Supernova Distances and its Effect on Measurement of the Hubble Constant
• Median Statistics, H_0, and the Accelerating Universe
• The evidence for a spatially flat Universe
• Physical Properties of Emission-Line Galaxies at z ~ 2 from Near-Infrared Spectroscopy with Magellan FIRE
• The BAO+BBN take on the Hubble tension
• Baryon Acoustic Oscillations and the Hubble Constant: Past, Present and Future
• Dark Energy Survey Year 1 Results: Measurement of the Baryon Acoustic Oscillation scale in the distribution of galaxies to redshift 1
• Measuring the Hubble constant with Type Ia supernovae as near-infrared standard candles
• General Cosmography Model with Spatial Curvature
• Possible signals of vacuum dynamics in the Universe
• Median statistics and the Hubble constant
• An improved model-independent assessment of the late-time cosmic expansion
• A blinded determination of $H_0$ from low-redshift Type Ia supernovae, calibrated by Cepheid variables
• Determining the Hubble constant from Hubble parameter measurements
• The Nature of Extreme Emission Line Galaxies at z=1-2: Kinematics and Metallicities from Near-Infrared Spectroscopy
• Baryon acoustic oscillation, Hubble parameter, and angular size measurement constraints on the Hubble constant, dark energy dynamics, and spatial curvature
• Setting the Stage for Cosmic Chronometers. I. Assessing the Impact of Young Stellar Populations on Hubble Parameter Measurements
• Ultra-compact structure in intermediate-luminosity radio quasars: building a sample of standard cosmological rulers and improving the dark energy constraints up to $z\sim 3$
• Low Redshift Baryon Acoustic Oscillation Measurement from the Reconstructed 6-degree Field Galaxy Survey
• Using the tilted flat-$\Lambda$CDM and the untilted non-flat $\Lambda$CDM inflation models to measure cosmological parameters from a compilation of observational data
• The $L-\sigma$ relation for massive bursts of star formation
• Constraints on dark energy dynamics and spatial curvature from Hubble parameter and baryon acoustic oscillation data
• Cosmography and flat $\Lambda$CDM tensions at high redshift
• The Beginning and Evolution of the Universe
• Using quasar X-ray and UV flux measurements to constrain cosmological model parameters
• Non-Gaussian Error Distribution of Hubble Constant Measurements
• An independent determination of the local Hubble constant
• A new measurement of the Hubble constant and matter content of the Universe using extragalactic background light $\gamma$-ray attenuation
• Observational constraints on the tilted spatially-flat and the untilted nonflat $\varphi$CDM dynamical dark energy inflation models
• Planck 2015 constraints on the non-flat $\Lambda$CDM inflation model
• Quasar X-ray and UV flux, baryon acoustic oscillation, and Hubble parameter measurement constraints on cosmological model parameters
• Cosmological Constraints from Compact Radio Source Angular Size versus Redshift Data
• Dynamical dark energy: scalar fields and running vacuum
• Binned Hubble parameter measurements and the cosmological deceleration-acceleration transition
• Measuring the Hubble constant and spatial curvature from supernova apparent magnitude, baryon acoustic oscillation, and Hubble parameter data
• New Model-independent Method to Test the Curvature of the Universe
• Constraining cosmic curvature by using age of galaxies and gravitational lenses
• Constraining the Dark Energy Equation of State with HII Galaxies
• Determining the Hubble constant using Giant extragalactic HII regions and HII galaxies
• Constraints on non-flat cosmologies with massive neutrinos after Planck 2015
• HII Galaxies as deep cosmological probes
• Using SPTpol, Planck 2015, and non-CMB data to constrain tilted spatially-flat and untilted non-flat $\Lambda$CDM, XCDM, and $\varphi$CDM dark energy inflation cosmologies
• Independent Cosmological Constraints from high-z HII Galaxies
• Nonflat time-variable dark energy cosmology
• Planck 2015 constraints on the non-flat $\varphi$CDM inflation model
• Hubble parameter data constraints on dark energy
• Model-independent Curvature Determination from Gravitational-Wave Standard Sirens and Cosmic Chronometers
• Constraining dark energy with gamma-ray bursts
• An evaluation of cosmological models from expansion and growth of structure measurements
• Towards a Precision Cosmology from Starburst Galaxies at z>2
• Observational constraints on the tilted flat-XCDM and the untilted nonflat XCDM dynamical dark energy inflation parameterizations
• Constraints on Scalar-Field Dark Energy from Galaxy Cluster Gas Mass Fraction versus Redshift
• A Strategy to Measure the Dark Energy Equation of State using the HII galaxy Hubble Relation & X-ray AGN Clustering: Preliminary Results
• Primordial power spectra for curved inflating universes
• CMB tensions with low-redshift $H_0$ and $S_8$ measurements: impact of a redshift-dependent type-Ia supernovae intrinsic luminosity
• Planck 2015 constraints on the non-flat XCDM inflation model
• Cosmological model-independent constraints on spatial curvature from strong gravitational lensing and type Ia supernova observations
• Observational constraints on non-flat dynamical dark energy cosmological models
• Planck 2015 constraints on spatially-flat dynamical dark energy models
• Constraints on dark energy from H II starburst galaxy apparent magnitude versus redshift data
• The HII Galaxy Hubble Diagram Strongly Favors $R_{\mathrm{h}}=ct$ over $\Lambda$CDM
• Multiple measurements of quasars acing as standard probes: exploring the cosmic distance duality relation at higher redshift
• A Bayesian interpretation of inconsistency measures in cosmology
• Low redshift observational constraints on tachyon models of dark energy
• CMB distance priors revisited: effects of dark energy dynamics, spatial curvature, primordial power spectrum, and neutrino parameters
• Constraints on dark energy from the lookback time versus redshift test
• Galaxy cluster number count data constraints on cosmological parameters
• Reconstruction of the HII Galaxy Hubble Diagram using Gaussian Processes
• Exploring Parameter Constraints on Quintessential Dark Energy: the Inverse Power Law Model
• Using spatial curvature with HII galaxies and cosmic chronometers to explore the tension in $H_0$
• Exploring the "$L$--$\sigma$" relation of HII galaxies and giant extragalactic HII regions acting as standard candles
• Kinematic Constraints on Spatial Curvature from Supernovae Ia and Cosmic Chronometers
• Galaxy Cluster Gas Mass Fraction and Hubble Parameter versus Redshift Constraints on Dark Energy
• Observational constraints on quintessence models of dark energy
• Using the Extragalactic Gamma-Ray Background to Constrain the Hubble Constant and Matter Density of the Universe
• The L - σ relation for HII galaxies in green
• Alternative High-z Cosmic Tracers and the Dark Energy Equation of State
• Testing the $R_{\mathrm{h}}=ct$ Universe Jointly with the Redshift-dependent Expansion rate and Angular-diameter and Luminosity Distances
• The Dark Energy Equation of State using Alternative High-z Cosmic Tracers
• Spatial Curvature in Cosmology Revisited
• A Model-Independent Measurement of the Spatial Curvature using Cosmic Chronometers and the HII Hubble Diagram
• Prospects of high redshift constraints on dark energy models with the Ep- Eiso correlation in long Gamma Ray Bursts
• Measuring $H_0$ from low-$z$ datasets

Cited by in corpus (48)

• Challenges for $\Lambda$CDM: An update
• Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0{w}_a$CDM cosmological parameterization result
• Using Pantheon and DES supernova, baryon acoustic oscillation, and Hubble parameter data to constrain the Hubble constant, dark energy dynamics, and spatial curvature
• Do gamma-ray burst measurements provide a useful test of cosmological models?
• Determining the range of validity of quasar X-ray and UV flux measurements for constraining cosmological model parameters
• Standardizing Platinum Dainotti-correlated gamma-ray bursts, and using them with standardized Amati-correlated gamma-ray bursts to constrain cosmological model parameters
• Brans-Dicke cosmology with a $\Lambda$- term: a possible solution to $\Lambda$CDM tensions
• 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
• 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
• Barrow Entropy Cosmology: an observational approach with a hint of stability analysis
• $H_0=69.8\pm 1.3$ $\mathrm{km}{\mathrm{s}}^{-1}\mathrm{Mp}{\mathrm{c}}^{-1}$, ${\Omega }_{m0}=0.288\pm 0.017$, and other constraints from lower-redshift, non-CMB, expansion-rate data
• Cosmological constraints from higher-redshift gamma-ray burst, HII starburst galaxy, and quasar (and other) data
• Gamma-ray burst data strongly favor the three-parameter fundamental plane (Dainotti) correlation relation over the two-parameter one
• Metastable dark energy models in light of Planck 2018: Alleviating the $H_0$ tension
• Probing modified gravity theories with multiple measurements of high-redshift quasars
• Standardizing reverberation-measured C IV time-lag quasars, and using them with standardized Mg II quasars to constrain cosmological parameters
• Is the $w_0{w}_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck CMB anisotropy data?
• Observational constraints and predictions of the interacting dark sector with field-fluid mapping
• Cosmological constraints from HII starburst galaxy, quasar angular size, and other measurements
• Revising the Hubble constant, spatial curvature and dark energy dynamics with the latest observations of quasars
• Quasar UV/X-ray relation luminosity distances are shorter than reverberation-measured radius-luminosity relation luminosity distances
• Effects of type Ia supernovae absolute magnitude priors on the Hubble constant value
• 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?
• Gaussian Processes Reconstruction of the Dark Energy Potential
• 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
• Revisiting Chaplygin gas cosmologies with the recent observations of high-redshfit quasars
• A hybrid model of viscous and Chaplygin gas to tackle the Universe acceleration
• Cosmological Constraints on the Coupling Model from Observational Hubble Parameter and Baryon Acoustic Oscillation Measurements
• Effect of extinction on quasar luminosity distances determined from UV and X-ray flux measurements
• Redshift-evolutionary X-ray and UV luminosity relation of quasars from Gaussian copula
• Effects of heterogeneous data sets and time-lag measurement techniques on cosmological parameter constraints from MgII and CIV reverberation-mapped quasar data
• Testing the standardizability of, and deriving cosmological constraints from, a new Amati-correlated gamma-ray burst data compilation
• Constraints on power law cosmology from cosmic chronometer, standard ruler, and standard candle data
• Potentialities of Hubble parameter and expansion rate function data to alleviate Hubble tension
• Revisiting Friedmann-like cosmology with torsion: newest constraints from high-redshift observations
• Low- and high-redshift H II starburst galaxies obey different luminosity-velocity dispersion relations
• Tilted non-spatially-flat inflation
• Reconstruction of the scalar field potential in nonmetricity gravity through Gaussian processes
• Updated observational constraints on $\varphi$CDM dynamical dark energy cosmological models
• Implications of Dynamical Dark Energy in the expansion of the Universe and the Structure Formation
• Standardizing reverberation-measured Mg II time-lag quasars, by using the radius-luminosity relation, and constraining cosmological model parameters
• Testing the consistency of new Amati-correlated gamma-ray burst dataset cosmological constraints with those from better-established cosmological data
• Constraints on Multicomponent Dark Energy from Cosmological Observations
• Bayesian Model Comparison of $R_h=ct$ versus $\Lambda$CDM using HII galaxy Hubble diagram