A HUBBLE DIAGRAM FOR QUASARS
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[1] J. Baldwin,et al. Quasars as Cosmological Probes: The Ionizing Continuum, Gas Metallicity, and the Wλ-L Relation , 1998, astro-ph/9805338.
[2] M. Elvis,et al. THE X-RAY ENERGY DEPENDENCE OF THE RELATION BETWEEN OPTICAL AND X-RAY EMISSION IN QUASARS , 2009, 0911.0474.
[3] Richard G. McMahon,et al. A luminous quasar at a redshift of z = 7.085 , 2011, Nature.
[4] G. Risaliti,et al. THE TIGHT RELATION BETWEEN X-RAY AND ULTRAVIOLET LUMINOSITY OF QUASARS , 2016, 1602.01090.
[5] S. Bianchi. A new cosmological distance measure using AGN X-ray variability , 2014 .
[6] G. Risaliti,et al. Cosmology with AGN: can we use quasars as standard candles? , 2016, 1612.02838.
[7] D. Valls-Gabaud,et al. Super-Eddington accreting massive black holes as long-lived cosmological standards. , 2013, Physical review letters.
[8] C. Firmani,et al. Gamma-ray bursts as standard candles to constrain the cosmological parameters , 2006, astro-ph/0610248.
[9] Christopher F. McKee,et al. Reverberation mapping of the emission line regions of Seyfert galaxies and quasars. , 1982 .
[10] The X-Ray-to-Optical Properties of Optically Selected Active Galaxies over Wide Luminosity and Redshift Ranges , 2006, astro-ph/0602407.
[11] James Liebert,et al. X-ray studies of quasars with the Einstein observatory , 1979 .
[12] P. Marziani,et al. Highly accreting quasars: sample definition and possible cosmological implications , 2014, 1405.2727.
[13] M. Salvato,et al. The X-ray to optical-UV luminosity ratio of X-ray selected type 1 AGN in XMM-COSMOS , 2009, 0912.4166.
[14] G. Richards,et al. A CATALOG OF QUASAR PROPERTIES FROM SLOAN DIGITAL SKY SURVEY DATA RELEASE 7 , 2011, 2209.03987.
[15] Bradley M. Peterson,et al. REVERBERATION MAPPING OF ACTIVE GALACTIC NUCLEI , 1993 .
[16] J. Baldwin. Luminosity Indicators in the Spectra of Quasi-Stellar Objects , 1977 .
[17] T. Davis,et al. A NEW COSMOLOGICAL DISTANCE MEASURE USING ACTIVE GALACTIC NUCLEI , 2011, 1109.4632.
[18] M. Sullivan,et al. Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples , 2014, 1401.4064.
[19] F. J. Carrera,et al. The XMM-Newton serendipitous survey - VII. The third XMM-Newton serendipitous source catalogue , 2015, 1504.07051.
[20] G. Risaliti,et al. Quasars as standard candles. I. The physical relation between disc and coronal emission , 2017, 1703.05299.
[21] D. Schneider,et al. Baryon acoustic oscillations from the complete SDSS-III Ly$\alpha$-quasar cross-correlation function at $z=2.4$ , 2017, 1708.02225.
[22] Elisabeta Lusso,et al. A Hubble Diagram for Quasars , 2015 .
[23] D. Raine,et al. Determining the cosmological parameters from the linewidths of active galaxies , 1999, astro-ph/9905165.
[24] Jean-Luc Starck,et al. Astronomical Data Analysis , 2007 .
[25] B. Peterson,et al. ON THE SCATTER IN THE RADIUS–LUMINOSITY RELATIONSHIP FOR ACTIVE GALACTIC NUCLEI , 2014, 1411.2977.
[26] A. Myers,et al. The Sloan Digital Sky Survey Quasar Catalog: Twelfth data release , 2016, 1608.06483.
[27] E. Branchini,et al. A NEW COSMOLOGICAL DISTANCE MEASURE USING ACTIVE GALACTIC NUCLEUS X-RAY VARIABILITY , 2014, 1404.2607.
[28] Margarita Karovska,et al. Quasar Parallax: A Method for Determining Direct Geometrical Distances to Quasars , 2002 .
[29] Bradley M. Peterson,et al. A NEW DIRECT METHOD FOR MEASURING THE HUBBLE CONSTANT FROM REVERBERATING ACCRETION DISCS IN ACTIVE GALAXIES , 1999 .