Reference health
Determining the range of validity of quasar X-ray and UV flux measurements for constraining cosmological model parameters
111/111 checkable references clean · checked 2026-07-24
Every reference with a DOI in the deposited reference list resolved to a known work in Crossref or DataCite at the dated check, and none carried a retraction, withdrawal, or removal notice.
19 without a DOI — not checked. A reference deposited without a DOI is never matched by title or guessed at; it stays outside the checked set, and this line discloses that.
The 111 checked references that resolve
resolves10.1134/S0202289320040106
Constraints from Observational Data for a Running Cosmological Constant and Warm Dark Matter with Curvature
resolves10.1093/mnras/stx721
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
resolves10.1093/mnrasl/slz056
Addressing the circularity problem in the <i>E</i>p−<i>E</i>iso correlation of gamma-ray bursts
resolves10.1093/mnras/stx2630
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
resolves10.3847/2041-8213/ab8012
Could Quasar Lensing Time Delays Hint to a Core Component in Halos, Instead of H<sub>0</sub> Tension?
resolves10.1051/0004-6361/202038633
The Milky Way Cepheid Leavitt law based on <i>Gaia</i> DR2 parallaxes of companion stars and host open cluster populations
resolves10.1140/epjc/s10052-012-2218-4
Galaxy cluster number count data constraints on cosmological parameters
resolves10.1051/0004-6361/201730551
Ultra-compact structure in intermediate-luminosity radio quasars: building a sample of standard cosmological rulers and improving the dark energy constraints up to <i>z </i>~ 3
resolves10.1093/mnras/staa2190
Cosmological constraints from H <scp>ii</scp> starburst galaxy apparent magnitude and other cosmological measurements
resolves10.1093/mnras/sty2405
Low redshift baryon acoustic oscillation measurement from the reconstructed 6-degree field galaxy survey
resolves10.1086/344786
Cosmological Constraints from Compact Radio Source Angular Size versus Redshift Data
resolves10.3847/0004-637X/829/2/61
CONSTRAINTS ON NON-FLAT COSMOLOGIES WITH MASSIVE NEUTRINOS AFTER PLANCK 2015
resolves10.3847/1538-4357/835/1/86
DETERMINING THE HUBBLE CONSTANT FROM HUBBLE PARAMETER MEASUREMENTS
resolves10.1088/1475-7516/2019/10/044
Baryon Acoustic Oscillations and the Hubble constant: past, present and future
resolves10.1093/mnras/sty1939
Dark Energy Survey Year 1 Results: A Precise H0 Estimate from DES Y1, BAO, and D/H Data
resolves10.1103/PhysRevD.99.123505
Dark Energy Survey year 1 results: Constraints on extended cosmological models from galaxy clustering and weak lensing
resolves10.1093/mnras/sty3351
Dark Energy Survey Year 1 results: measurement of the baryon acoustic oscillation scale in the distribution of galaxies to redshift 1
resolves10.1051/0004-6361/201731501
Measuring the Hubble constant with Type Ia supernovae as near-infrared standard candles
resolves10.3847/1538-4357/abd242
A Backscattering-dominated Prompt Emission Model for the Prompt Phase of Gamma-Ray Bursts
resolves10.3847/1538-4357/ab4a0e
A New Measurement of the Hubble Constant and Matter Content of the Universe Using Extragalactic Background Light γ-Ray Attenuation
resolves10.3847/1538-4357/abb085
The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations with Lyα Forests
resolves10.3847/1538-4357/ab4e11
Spectral Analysis of Fermi-LAT Gamma-Ray Bursts with Known Redshift and their Potential Use as Cosmological Standard Candles
resolves10.1088/2041-8205/766/1/L7
HUBBLE PARAMETER MEASUREMENT CONSTRAINTS ON THE COSMOLOGICAL DECELERATION-ACCELERATION TRANSITION REDSHIFT
resolves10.1016/j.physletb.2013.08.078
Binned Hubble parameter measurements and the cosmological deceleration–acceleration transition
resolves10.1007/s10509-015-2319-2
Observational constraints on non-flat dynamical dark energy cosmological models
resolves10.3847/1538-4357/835/1/26
HUBBLE PARAMETER MEASUREMENT CONSTRAINTS ON THE REDSHIFT OF THE DECELERATION–ACCELERATION TRANSITION, DYNAMICAL DARK ENERGY, AND SPACE CURVATURE
resolves10.1088/1674-4527/20/9/151
Investigating the relationship between cosmic curvature and dark energy models with the latest supernova sample
resolves10.1088/1475-7516/2018/04/051
<i>H</i><sub>0</sub>from cosmic chronometers and Type Ia supernovae, with Gaussian Processes and the novel Weighted Polynomial Regression method
resolves10.1093/mnras/staa3426
Kinematic constraints on spatial curvature from supernovae Ia and cosmic chronometers
resolves10.1093/mnras/staa101
Quasar X-ray and UV flux, baryon acoustic oscillation, and Hubble parameter measurement constraints on cosmological model parameters
resolves10.1093/mnras/staa1855
Using quasar X-ray and UV flux measurements to constrain cosmological model parameters
resolves10.1093/mnras/staa2779
Constraints on cosmological parameters from gamma-ray burst peak photon energy and bolometric fluence measurements and other data
resolves10.3847/1538-4357/abbd97
Determination of the Local Hubble Constant from Virgo Infall Using TRGB Distances
resolves10.1088/1475-7516/2020/10/040
Probing alternative cosmologies through the inverse distance ladder
resolves10.1051/0004-6361/202038264
Kinematic constraints beyond <i>z</i> ≃ 0 using calibrated GRB correlations
resolves10.3847/1538-4357/aba756
H<sub>0</sub> Reconstruction with Type Ia Supernovae, Baryon Acoustic Oscillation and Gravitational Lensing Time Delay
resolves10.1016/j.physletb.2012.07.011
Constraints on dark energy from H II starburst galaxy apparent magnitude versus redshift data
resolves10.1016/j.crhy.2012.04.008
Everything you always wanted to know about the cosmological constant problem (but were afraid to ask)
resolves10.3390/sym11080986
CMB Tensions with Low-Redshift H0 and S8 Measurements: Impact of a Redshift-Dependent Type-Ia Supernovae Intrinsic Luminosity
resolves10.1140/epjc/s10052-020-8221-2
Does $$\varLambda $$CDM really be in tension with the Hubble diagram data?
resolves10.3390/sym12071118
A Confront between Amati and Combo Correlations at Intermediate and Early Redshifts
resolves10.1007/s10509-019-3663-4
Planck 2015 constraints on spatially-flat dynamical dark energy models
resolves10.3847/1538-4357/aae82d
Observational Constraints on the Tilted Spatially Flat and the Untilted Nonflat ϕCDM Dynamical Dark Energy Inflation Models
resolves10.1007/s10509-019-3567-3
Observational constraints on the tilted flat-XCDM and the untilted nonflat XCDM dynamical dark energy inflation parameterizations
resolves10.1007/s10509-019-3627-8
Measuring the Hubble constant and spatial curvature from supernova apparent magnitude, baryon acoustic oscillation, and Hubble parameter data
resolves10.3847/1538-4357/ab3641
Using the Tilted flat-ΛCDM and the Untilted Non-flat ΛCDM Inflation Models to Measure Cosmological Parameters from a Compilation of Observational Data
resolves10.1103/PhysRevD.101.083508
Using SPT polarization,
<i>Planck</i>
2015, and non-CMB data to constrain tilted spatially-flat and untilted nonflat
<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi mathvariant="normal">Λ</mml:mi><mml:mi>CDM</mml:mi></mml:math>
, XCDM, and
<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>ϕ</mml:mi><mml:mi>CDM</mml:mi></mml:math>
dark energy inflation cosmologies
resolves10.1088/1475-7516/2020/05/032
Combining full-shape and BAO analyses of galaxy power spectra: a 1.6% CMB-independent constraint on<i>H</i><sub>0</sub>
resolves10.1088/1742-6596/189/1/012032
Alternative high-<i>z</i>cosmic tracers and the dark energy equation of state
resolves10.3847/2041-8213/abc6a8
Recombination-independent Determination of the Sound Horizon and the Hubble Constant from BAO
resolves10.1088/1475-7516/2017/03/028
Constraining cosmic curvature by using age of galaxies and gravitational lenses
resolves10.3847/1538-4357/aba517
A Cosmography Approach to Dark Energy Cosmologies: New Constraints Using the Hubble Diagrams of Supernovae, Quasars, and Gamma-Ray Bursts
resolves10.3847/1538-4357/ab1422
Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics beyond ΛCDM
resolves10.1088/0004-637X/802/1/20
CONFIRMATION OF A STAR FORMATION BIAS IN TYPE Ia SUPERNOVA DISTANCES AND ITS EFFECT ON THE MEASUREMENT OF THE HUBBLE CONSTANT
resolves10.1038/s41550-018-0657-z
Cosmological constraints from the Hubble diagram of quasars at high redshifts
resolves10.1093/mnras/sty1922
Constraints on dark energy dynamics and spatial curvature from Hubble parameter and baryon acoustic oscillation data
resolves10.1093/mnras/stz1966
Baryon acoustic oscillation, Hubble parameter, and angular size measurement constraints on the Hubble constant, dark energy dynamics, and spatial curvature
resolves10.1016/j.physletb.2010.07.057
Constraints on dark energy from the lookback time versus redshift test
resolves10.3847/1538-4357/aab9bb
The Complete Light-curve Sample of Spectroscopically Confirmed SNe Ia from Pan-STARRS1 and Cosmological Constraints from the Combined Pantheon Sample
resolves10.1111/j.1365-2966.2004.08539.x
Towards a precision cosmology from starburst galaxies at<i>z</i>> 2
resolves10.1088/1475-7516/2019/04/047
Low redshift observational constraints on tachyon models of dark energy
resolves10.3847/1538-4357/abd4df
Eppur è piatto? The Cosmic Chronometers Take on Spatial Curvature and Cosmic Concordance
resolves10.1140/epjc/s10052-020-08785-z
The growth factor parametrization versus numerical solutions in flat and non-flat dark energy models
resolves10.1103/PhysRevD.101.043502
Is the Hubble diagram of quasars in tension with concordance cosmology?
resolves10.1051/0004-6361/201526485
Measuring dark energy with the<i>E</i><sub>iso</sub>–<i>E</i><sub>p</sub>correlation of gamma-ray bursts using model-independent methods
resolves10.3847/1538-4357/ab5e7d
Model-independent Distance Calibration and Curvature Measurement Using Quasars and Cosmic Chronometers
resolves10.3847/1538-4357/aae696
Model-independent Curvature Determination from Gravitational-wave Standard Sirens and Cosmic Chronometers
resolves10.1103/PhysRevD.79.103004
Exploring parameter constraints on quintessential dark energy: The inverse power law model
resolves10.3847/0004-637X/828/2/85
NEW MODEL-INDEPENDENT METHOD TO TEST THE CURVATURE OF THE UNIVERSE
resolves10.3847/1538-4357/aab0a2
Hubble Parameter and Baryon Acoustic Oscillation Measurement Constraints on the Hubble Constant, the Deviation from the Spatially Flat ΛCDM Model, the Deceleration–Acceleration Transition Redshift, and Spatial Curvature
resolves10.3847/1538-4357/ab35e3
Using the Extragalactic Gamma-Ray Background to Constrain the Hubble Constant and Matter Density of the Universe
resolves10.3847/1538-4357/aa9888
An Evaluation of Cosmological Models from the Expansion and Growth of Structure Measurements
resolves10.1088/1475-7516/2020/07/009
CMB distance priors revisited: effects of dark energy dynamics, spatial curvature, primordial power spectrum, and neutrino parameters
resolves10.1093/mnras/stx1600
A blinded determination of H0 from low-redshift Type Ia supernovae, calibrated by Cepheid variables
resolves10.3847/1538-4357/ab7995
Multiple Measurements of Quasars Acting as Standard Probes: Exploring the Cosmic Distance Duality Relation at Higher Redshift
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