J/A+A/674/A163       Type I quasars luminosity distances          (Huang+, 2023)

A measure of cosmological distance using the CIV Baldwin effect in quasars. Huang L., Wang H., Gao Z., Zeng X., Chang Z. <Astron. Astrophys. 674, A163 (2023)> =2023A&A...674A.163H 2023A&A...674A.163H (SIMBAD/NED BibCode)
ADC_Keywords: QSOs ; Radio sources ; Stars, distances Keywords: dark energy - quasars: emission lines - quasars: general - distance scale Abstract: We use the anticorrelation between the equivalent width (EW) of the CIV 1549Å emission line and the continuum luminosity in the quasars rest frame (Baldwin effect) to measure their luminosity distance as well as estimate cosmological parameters. We obtain a sample of 471 Type I quasars with the UV-optical spectra and EW (CIV) measurements in the redshift range of 2.3<z<7.1 including 25 objects at 5<z<7.1, which can be used to investigate the CIV Baldwin effect and determine cosmological luminosity distance. The relation EW(CIV)~(λLλ)γ can be applied to check the inverse correlation between the CIV EW and Lλ of quasars and give their distance, and the data suggest that the EW of CIV is inversely correlated with continuum monochromatic luminosities. On the other hand, we also consider dividing the Type I quasar sample into various redshift bins, which can be used to check if the CIV EW-luminosity relation depends on the redshift. Finally, we apply a combination of Type I quasars and Type Ia supernovae (SNIa) of the Pantheon sample to test the property of dark energy concerning whether or not its density deviates from the constant, and give the statistical results Description: The properties of the 471 Type I quasars with the UV-optical spectra and EW (CIV) measurements, which can be used to investigate the CIV Baldwin effect and measure these cosmological luminosity distances. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 114 471 The properties of the Type I quasars -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 18 A18 --- Name SDSS name of Type I quasars (HHMMSS.ss+DDMMSS.s) 20- 27 F8.6 --- z Redshift 29- 34 F6.3 mag rmag SDSS r magnitude 36- 40 F5.3 mag e_rmag Error on r magnitude 42- 48 F7.4 0.1nm EW(CIV) Equivalent width of the CIV 1549Å emission line 50- 58 E9.7 0.1nm e_EW(CIV) Error on EW(C IV) 60- 71 F12.8 10-7W/Hz/m2 F2500 Rest-frame flux at 2500Å 73- 78 F6.4 10-7W/Hz/m2 e_F2500 Error on Rest-frame flux at 2500Å 80- 90 F11.9 --- GammaUV UV-optical power-law index 92-102 F11.8 --- DM Distance modulus 104-114 F11.9 --- e_DM Error on distance modulus -------------------------------------------------------------------------------- Acknowledgements: Long Huang, huanglong20122021(at)163.com
(End) Patricia Vannier [CDS] 08-Jun-2023
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line