2021
Standardizing reverberation-measured Mg II time-lag quasars, by using the radius–luminosity relation, and constraining cosmological model parameters
KHADKA, Narayan, Zhefu YU, Michal ZAJAČEK, Mary Loli MARTINEZ-ALDAMA, Bożena CZERNY et. al.Základní údaje
Originální název
Standardizing reverberation-measured Mg II time-lag quasars, by using the radius–luminosity relation, and constraining cosmological model parameters
Autoři
KHADKA, Narayan (garant), Zhefu YU, Michal ZAJAČEK (703 Slovensko, domácí), Mary Loli MARTINEZ-ALDAMA, Bożena CZERNY a Bharat RATRA
Vydání
Monthly Notices of the Royal Astronomical Society, Oxford University Press, 2021, 0035-8711
Další údaje
Jazyk
angličtina
Typ výsledku
Článek v odborném periodiku
Obor
10308 Astronomy
Stát vydavatele
Velká Británie a Severní Irsko
Utajení
není předmětem státního či obchodního tajemství
Odkazy
Impakt faktor
Impact factor: 5.235
Kód RIV
RIV/00216224:14310/21:00119315
Organizační jednotka
Přírodovědecká fakulta
UT WoS
000715897400004
Klíčová slova anglicky
cosmological parameters; cosmology: observations; dark energy; quasars: emission lines
Štítky
Příznaky
Mezinárodní význam, Recenzováno
Změněno: 29. 11. 2021 09:24, Mgr. Marie Šípková, DiS.
Anotace
V originále
We use 78 reverberation-measured Mg II time-lag quasars (QSOs) in the redshift range 0.0033 ≤ z ≤ 1.89 to constrain cosmological parameters in six different cosmological models. The basis of our method is the use of the radius–luminosity or R−L relation to standardize these 78 Mg II QSOs. In each cosmological model, we simultaneously determine R−L relation and cosmological model parameters, thus avoiding the circularity problem. We find that the R−L relation parameter values are independent of the cosmological model used in the analysis, thus, establishing that current Mg II QSOs are standardizable candles. Cosmological constraints obtained using these QSOs are significantly weaker than, but consistent with, those obtained from a joint analysis of baryon acoustic oscillation (BAO) observations and Hubble parameter [H(z)] measurements. So, we also analyse these QSOs in conjunction with the BAO + H(z) data and find cosmological constraints consistent with the standard spatially flat ΛCDM model as well as with mild dark energy dynamics and a little spatial curvature. A larger sample of higher quality reverberation-measured QSOs should have a smaller intrinsic dispersion and so should provide tighter constraints on cosmological parameters.
Návaznosti
GX21-13491X, projekt VaV |
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