Quasars as high-redshift standard candles

被引:1
|
作者
Risaliti, G. [1 ,2 ]
Lusso, E. [1 ,2 ]
Nardini, E. [2 ]
Bargiacchi, G. [3 ,4 ]
Bisogni, S. [5 ]
Sacchi, A. [6 ]
Signorini, M. [1 ,2 ]
Trefoloni, B. [1 ,2 ]
机构
[1] Univ Florence, Dept Phys & Astron, Via G Sansone 1, I-50019 Sesto Fiorentino, FI, Italy
[2] INAF Arcetri Astrophys Observ, Largo E Fermi 5 Firenze, I-50125 Florence, Italy
[3] Scuola Super Meridionale, Largo S Marcellino 10, I-80138 Naples, Italy
[4] INFN, Sez Napoli, Via Cinthia 9, I-80126 Naples, Italy
[5] INAF Ist Astrofis Spaziale & Fis Cosm Milano, Via Corti 12, I-20133 Milan, Italy
[6] Ist Univ Studi Superiori IUSS, Piazza Vittoria 15, I-27100 Pavia, Italy
关键词
Cosmology; extra-galactic astronomy;
D O I
10.1002/asna.20230054
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In the past few years, we built a Hubble diagram of quasars up to redshift z similar to 7, based on the nonlinear relation between quasars' x-ray and UV luminosities. Such a Hubble diagram shows a > 4sdeviation from the standard flat Delta CDM model at z > 1.5. Given the important consequences of this result, it is fundamental to rule out any systematic effect in the selection of the sample and/or in the flux measurements, and to investigate possible redshift dependences of the relation, that would invalidate the use of quasars as standard candles. Here we review all the observational results supporting our method: the match of the Hubble diagram of quasars with that of supernovae in the common redshift range, the constant slope of the relation at all redshifts, the redshift non-evolution of the spectral properties of our sources both in the x-rays and in the UV. An independent test of our results requires the observation of other standard candles at high redshift. In particular, we expect that future observations of supernovas at z > 2 will confirm the deviation from the concordance model found with the Hubble diagram of quasars.
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页数:5
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