We report on an observational research program aimed at studying the physical properties, the environment and the cosmological relevance of high-redshift quasars. We have been awarded the largest XMM-Newton AO16 program (1.05 Msec) to study z>3 quasars, and a large (500 ks) Chandra program to investigate the environment of a z=6.31 quasar. Our objectives were: -use quasars as standard candles in the Hubble Diagram of quasars, in order to constrain the cosmological model at high redshift; - investigate quasar variability at all redshifts and luminosities with unprecedented detail; - characterize the multiwavelength emission of z=6 quasars, and their environment; obtain an unbiased and complete census of high-z blazars....

Quasars at High-Redshift: Physics and Cosmology

RisalitI, G.;Gilli, R.;Amati, L.;Dallacasa, D.;Ighina, L.;Lusso, E.;Marchesi, S.
Writing – Review & Editing
;
Nanni, R.;Signorini, M.;Spingola, C.;
2022

Abstract

We report on an observational research program aimed at studying the physical properties, the environment and the cosmological relevance of high-redshift quasars. We have been awarded the largest XMM-Newton AO16 program (1.05 Msec) to study z>3 quasars, and a large (500 ks) Chandra program to investigate the environment of a z=6.31 quasar. Our objectives were: -use quasars as standard candles in the Hubble Diagram of quasars, in order to constrain the cosmological model at high redshift; - investigate quasar variability at all redshifts and luminosities with unprecedented detail; - characterize the multiwavelength emission of z=6 quasars, and their environment; obtain an unbiased and complete census of high-z blazars....
2022
RisalitI, G.; Caccianiga, A.; Gilli, R.; Paolillo, M.; Amati, L.; Bargiacchi, G.; Belladitta, S.; Dallacasa, D.; Diana, A.; Di Girolamo, T.; Haardt, F.; Ighina, L.; Lusso, E.; Marchesi, S.; Moretti, A.; Nanni, R.; Nardini, E.; Peca, A.; Piedipalumbo, E.; Sacchi, A.; Sbarrato, T.; Severgnini, P.; Signorini, M.; Spingola, C.; Trefoloni, B.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/957392
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