Kirkpatrick, A.A.KirkpatrickHall, K.K.HallNyland, K.K.NylandLacy, M.M.LacyPRANDONI, ISABELLAISABELLAPRANDONI2020-10-062020-10-062018978-1-58381-919-71050-3390http://hdl.handle.net/20.500.12386/27612The next generation Very Large Array (ngVLA) will have unprecedented sensitivities and mapping speeds at 1.2-8 GHz. We discuss how the active galactic nuclei (AGN) community can benefit from a wide-area, medium depth ngVLA survey. We propose a 10 deg<SUP>2</SUP> survey in the Stripe 82 field using the 8 GHz band with an rms depth of 1 μJy beam<SUP>-1</SUP>. We will detect ∼130,000 galaxies, including radio-quiet AGN out to z ∼ 7. We can measure the luminosity and space density evolution of radio-quiet and radio-loud AGN. We can also measure AGN evolution through clustering of both populations using cross-correlation functions. A wide area ngVLA survey will benefit from existing multiwavelength AGN populations, particularly in the Stripe 82 field, as well as new information from next-generation optical and infrared survey instruments such as LSST and WFIRST.STAMPAenConference paperhttp://aspbooks.org/custom/publications/paper/517-0639.html2018ASPC..517..639KFIS/05 - ASTRONOMIA E ASTROFISICAERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation