2025
Standardizing a larger, higher-quality, homogeneous sample of reverberation-mapped Hβ active galactic nuclei using the broad-line region radius-luminosity relation
CAO, Shulei; Amit Kumar MANDAL; Michal ZAJAČEK a Bharat RATRAZákladní údaje
Originální název
Standardizing a larger, higher-quality, homogeneous sample of reverberation-mapped Hβ active galactic nuclei using the broad-line region radius-luminosity relation
Autoři
CAO, Shulei; Amit Kumar MANDAL; Michal ZAJAČEK a Bharat RATRA
Vydání
Physical review D, American Physical Society, 2025, 2470-0010
Další údaje
Jazyk
angličtina
Typ výsledku
Článek v odborném periodiku
Obor
10308 Astronomy
Stát vydavatele
Spojené státy
Utajení
není předmětem státního či obchodního tajemství
Odkazy
Impakt faktor
Impact factor: 5.300 v roce 2024
Označené pro přenos do RIV
Ano
Organizační jednotka
Přírodovědecká fakulta
UT WoS
EID Scopus
Klíčová slova anglicky
Cosmological parameters; Cosmology; Dark energy; Galactic nuclei and quasars
Příznaky
Mezinárodní význam, Recenzováno
Změněno: 28. 1. 2026 11:41, Mgr. Marie Novosadová Šípková, DiS.
Anotace
V originále
We present a high-quality, homogeneous sample of 157 H𝛽 reverberation-mapped active galactic nuclei (AGNs) spanning redshifts 0.00308 ≤𝑧 ≤0.8429, which is approximately 3.8 times larger than the previously available high-quality homogeneous sample. Using the broad-line region radius-luminosity relation (𝑅 −𝐿), which involves the broad H𝛽 line time delay and the monochromatic luminosity at 5100 Å, we show that the sample is standardizable by using six spatially flat and nonflat cosmological models. The inferred cosmological model parameters are consistent within 2𝜎 uncertainties with those from better established baryon acoustic oscillation and Hubble parameter measurements, with the exception of two nonflat models that are ruled out by other data. The 𝑅 −𝐿 relation slope is found to be flatter (𝛾 =0.428 ±0.025 in the flat ΛCDM model) than the slope of 0.5 expected from a simple photoionization model as well as the slope found previously for the smaller homogeneous sample. In addition, we find a mild dependence of H𝛽 𝑅 −𝐿 relation parameters as well as its intrinsic scatter on the Eddington ratio by comparing the 𝑅 −𝐿 relations for low- and high-accreting equal-sized subsamples. A future analysis of a larger homogeneous sample containing a broader range of luminosities and Eddington ratios is necessary to confirm the standardizability of H𝛽 AGNs.
Návaznosti
| GF23-04053L, projekt VaV |
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