The evolution of obscured AGN across cosmic time -- A large quasar survey for the 2040s

  • Tanya Urrutia
  • , Darshan Kakkad
  • , Paula Sánchez-Sáez
  • , Mojtaba Raouf
  • , Swayamtrupta Panda
  • , Sarah E. I. Bosman
  • , Francisco Pozo Nunez
  • , Annagrazia Puglisi
  • , Sophia Flury
  • , Dragana Ilic
  • , Andjelka B. Kovacevic
  • , Mamta Pandey-Pommier
  • , Giustina Vietri
  • , Sarath Satheesh-Sheeba
  • , Francesco Salvestrini
  • , Susanna Bisogni
  • , Eduardo Bañados
  • , Ana Monreal Ibero
  • , Sabine Thater
  • , Pratika Dayal
  • Filippo D'Ammando, José Afonso, Paramita Barai, Valentin Ivanov

Research output: Other contribution

Abstract

We propose a large quasar demographic optical multi-object spectroscopic (MOS) survey targeting over 50 million AGN candidates up to the highest redshifts possible in the optical (z~6.5), with repeat visits, using a variety of selection criteria available by 2040. A large MOS survey combining all AGN selection methods is the only way to unify a diverse range of different obscured AGN populations within a single, variability- and spectroscopy-based framework, rather than as disjoint classes selected by different methods.
Original languageUndefined/Unknown
Publication statusPublished - 20 Dec 2025

Keywords

  • astro-ph.GA

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