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Cited article:

Spectral Connection between Far UV and Soft X-Ray Emission from Active Galactic Nuclei Using AstroSat

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Revealing the burning and soft heart of the bright bare active galactic nucleus ESO 141-G55: X-ray broadband and SED analysis

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Far-ultraviolet Spectroscopy of Active Galactic Nuclei with ASTROSAT/UVIT

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The Astrophysical Journal 950 (2) 90 (2023)
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A broad-band X-ray spectral study of the Seyfert 1 galaxy ESO 141–G055 with XMM–Newton and NuSTAR

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Monthly Notices of the Royal Astronomical Society 497 (4) 4213 (2020)
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The subarcsecond mid-infrared view of local active galactic nuclei – II. The mid-infrared–X-ray correlation

D. Asmus, P. Gandhi, S. F. Hönig, A. Smette and W. J. Duschl
Monthly Notices of the Royal Astronomical Society 454 (1) 766 (2015)
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The X-ray to [Ne V]3426 flux ratio: discovering heavily obscured AGN in the distant Universe

R. Gilli, C. Vignali, M. Mignoli, et al.
Astronomy and Astrophysics 519 A92 (2010)
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The mid IR – hard X-ray correlation in AGN and its implications for dusty torus models

H. Horst, P. Gandhi, A. Smette and W. J. Duschl
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The nature and origin of Seyfert warm absorbers

A. J. Blustin, M. J. Page, S. V. Fuerst, G. Branduardi-Raymont and C. E. Ashton
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The relation between AGN hard X-ray emission and mid-infrared continuum from ISO spectra: Scatter and unification aspects

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Astronomy & Astrophysics 418 (2) 465 (2004)
https://doi.org/10.1051/0004-6361:20035838