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The need for ultra high resolution X-ray imaging

This paper discusses the broad science case for obtaining milliarcsecond to microarcsecond astronomical imaging resolution in the soft to medium-energy X-ray band (∼0.5 to ∼8 keV). Astronomy across much of the electromagnetic spectrum has been fundamentally transformed with a rapid increase in groun...

Täydet tiedot

Tallennettuna:
Päätekijät: Kimberly A. Weaver, Jenna M. Cann, Ryan Pfeifle, Miranda McCarthy, Laura D. Vega, Ronald S. Gamble, Teresa Monsue, Kyla Mullaney, Mainak Singha, Erini Lambrides, Jeffrey McKaig, Isabella Carlton, Kelly Whalen, Emma Kleiner, Atul Mohan, Subhajeet Karmakar, Ann E. Hornschemeier, Herbert Ortiz, Claudio Ricci, Lynne Valencic, Brandon Coleman, Kaylee DeGennaro, Ruchi Pandey
Aineistotyyppi: Artigo
Kieli:Inglês
Julkaistu: Frontiers Media S.A. 2026-06-01
Sarja:Frontiers in Astronomy and Space Sciences
Aiheet:
active galactic nucleus
astrophysics
black holes
dual AGN
interferometry
jets
Linkit:https://www.frontiersin.org/articles/10.3389/fspas.2026.1790876/full
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