CAO, Shulei, Michal ZAJAČEK, Bożena CZERNY, Swayamtrupta PANDA and Bharat RATRA. Effects of heterogeneous data sets and time-lag measurement techniques on cosmological parameter constraints from Mg II and C IV reverberation-mapped quasar data. Monthly Notices of the Royal Astronomical Society. Oxford University Press, 2024, vol. 528, No 4, p. 6444-6469. ISSN 0035-8711. Available from: https://dx.doi.org/10.1093/mnras/stae433.
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Basic information
Original name Effects of heterogeneous data sets and time-lag measurement techniques on cosmological parameter constraints from Mg II and C IV reverberation-mapped quasar data
Authors CAO, Shulei, Michal ZAJAČEK (703 Slovakia, guarantor, belonging to the institution), Bożena CZERNY, Swayamtrupta PANDA and Bharat RATRA.
Edition Monthly Notices of the Royal Astronomical Society, Oxford University Press, 2024, 0035-8711.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher United Kingdom of Great Britain and Northern Ireland
Confidentiality degree is not subject to a state or trade secret
WWW URL URL
Impact factor Impact factor: 4.800 in 2022
Organization unit Faculty of Science
Doi http://dx.doi.org/10.1093/mnras/stae433
UT WoS 001169271500018
Keywords in English cosmological parameters; cosmology: observations; dark energy; quasars: emission lines
Tags rivok
Tags International impact, Reviewed
Changed by Changed by: Mgr. Marie Šípková, DiS., učo 437722. Changed: 25/4/2024 11:05.
Abstract
Previously, we demonstrated that Mg II and C IV reverberation-mapped quasars (RM QSOs) are standardizable and that the cosmological parameters inferred using the broad-line region radius-luminosity (R-L) relation are consistent with those determined from better-established cosmological probes. With more data expected from ongoing and future spectroscopic and photometric surveys, it is imperative to examine how new QSO data sets of varied quality, with their own specific luminosity and time-delay distributions, can be best used to determine more restrictive cosmological parameter constraints. In this study, we test the effect of adding 25 OzDES Mg II RM QSOs as well as 25 lower quality SDSS RM C IV QSOs, which increases the previous sample of RM QSOs by ∼36 per cent. Although cosmological parameter constraints become tighter for some cosmological models after adding these new QSOs, the new combined data sets have increased differences between R-L parameter values obtained in different cosmological models and thus a lower standardizability for the larger Mg II + C IV compilation. Different time-delay methodologies, particularly the ICCF and CREAM methods used for inferring time delays of SDSS RM QSOs, slightly affect cosmological and R-L relation parameter values, however, the effect is negligible for (smaller) compilations of robust time-delay detections. Our analysis indicates that increasing the sample size is not sufficient for tightening cosmological constraints and a quality cut is necessary to obtain a standardizable RM QSO sample.
Links
GM24-10599M, research and development projectName: Hvězdy v galaktických jádrech: vzájemný vztah s masivními černými dírami
Investor: Czech Science Foundation, Stars in galactic nuclei: interrelation with massive black holes
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