Observations favor the redshift-evolutionary $L_X$-$L_{UV}$ relation of quasars from copula
Bao Wang, Yang Liu, Hongwei Yu, Puxun Wu

TL;DR
This study compares different $L_X$-$L_{UV}$ relations of quasars, finding strong observational support for a redshift-evolutionary relation constructed via copula, which better aligns with cosmic background data than the standard relation.
Contribution
It introduces and tests a redshift-evolutionary $L_X$-$L_{UV}$ relation of quasars using copula, demonstrating its consistency and superiority over the standard relation with observational data.
Findings
Redshift-evolutionary relations are consistent across low and high redshift data.
Observations support the redshift-evolutionary relation at more than 3 sigma.
Statistical criteria favor the copula-based redshift-evolutionary relation over the standard relation.
Abstract
We compare, with data from the quasars, the Hubble parameter measurements, and the Pantheon+ type Ia supernova, three different relations between X-ray luminosity () and ultraviolet luminosity () of quasars. These three relations consist of the standard and two redshift-evolutionary - relations which are constructed respectively by considering a redshift dependent correction to the luminosities of quasars and using the statistical tool called copula. By employing the PAge approximation for a cosmological-model-independent description of the cosmic background evolution and dividing the quasar data into the low-redshift and high-redshift parts, we find that the constraints on the PAge parameters from the low-redshift and high-redshift data, which are obtained with the redshift-evolutionary relations, are consistent with each other, while they are not when the…
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Taxonomy
TopicsStatistical and numerical algorithms · Advanced Statistical Methods and Models
