The cosmological model is at present not tested between the redshift of the farthest observed supernovae (z similar to 1.4) and that of the Cosmic Microwave Background (z similar to 1,100). 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. We built a sample of similar to 1,900 quasars with available UV and X-ray observations, and produced a Hubble Diagram up to z similar to 5. 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. 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.

A Hubble Diagram for Quasars / Bisogni, Susanna; Risaliti, Guido; Lusso, Elisabeta. - In: FRONTIERS IN ASTRONOMY AND SPACE SCIENCES. - ISSN 2296-987X. - ELETTRONICO. - 4:(2018), pp. 68-75. [10.3389/fspas.2017.00068]

A Hubble Diagram for Quasars

Bisogni, Susanna;Risaliti, Guido;Lusso, Elisabeta
2018

Abstract

The cosmological model is at present not tested between the redshift of the farthest observed supernovae (z similar to 1.4) and that of the Cosmic Microwave Background (z similar to 1,100). 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. We built a sample of similar to 1,900 quasars with available UV and X-ray observations, and produced a Hubble Diagram up to z similar to 5. 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. 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.
2018
4
68
75
Bisogni, Susanna; Risaliti, Guido; Lusso, Elisabeta
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Utilizza questo identificatore per citare o creare un link a questa risorsa: https://hdl.handle.net/2158/1157203
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