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Supernova quasar
Supernova quasar











supernova quasar supernova quasar

For this reason they have always been considered as potential candidates for extending the distance ladder in a redshift range well beyond the limit imposed by the supernovae ( z ~ 1.4). Quasars are among the brightest sources in the universe, by now observable up to redshift z ~ 7 ( Mortlock et al., 2011). The application of this method to forthcoming, larger quasar samples, will also provide tight constraints on the dark energy equation of state and its possible evolution with time. The analysis of the quasar Hubble Diagram, when used in combination with supernovae, provides robust constraints on the matter and energy content in the cosmos. We built a sample of ~1,900 quasars with available UV and X-ray observations, and produced a Hubble Diagram up to z ~ 5. Here we introduce a new method to measure the cosmological parameters: we show that quasars can be used as “standard candles” by employing the non-linear relation between their intrinsic UV and X-ray emission as an absolute distance indicator. The cosmological model is at present not tested between the redshift of the farthest observed supernovae ( z ~ 1.4) and that of the Cosmic Microwave Background ( z ~ 1,100).

  • 4Centre for Extragalactic Astronomy, Department of Physics, Durham University, Durham, United Kingdom.
  • 3Dipartimento di Fisica e Astronomia, Università degli Studi di Firenze, Firenze, Italy.
  • 2INAF, Osservatorio Astrofisico di Arcetri, Firenze, Italy.
  • supernova quasar

  • 1Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States.
  • Susanna Bisogni 1,2 *, Guido Risaliti 2,3 and Elisabeta Lusso 4













    Supernova quasar