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Cited article:

Environment of 1 ≤ z ≤ 2 MIR selected obscured and unobscured AGNs in the Extended Chandra Deep Field South

Carlos Guillermo Bornancini, Mónica Silvia Taormina, Diego García Lambas

A&A, 605 (2017) A10

Published online: 2017-08-31

DOI: https://doi.org/10.1051/0004-6361/201629326

This article has been cited by the following article(s):

Properties of IR-selected active galactic nuclei

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The Effect of the Morphological Quenching Mechanism on Star Formation Activity at 0.5 < z < 1.5 in 3D-HST/CANDELS

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The Astrophysical Journal 913 (2) 81 (2021)
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Host galaxy and orientation differences between different AGN types

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Astronomy & Astrophysics 650 A75 (2021)
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The Compact Star-forming Galaxies at 2 < z < 3 in 3D-HST/CANDELS: AGN and Non-AGN Physical Properties

Shiying Lu, Yizhou Gu, Guanwen Fang, et al.
Publications of the Astronomical Society of the Pacific 132 (1014) 084101 (2020)
https://doi.org/10.1088/1538-3873/ab9b70

Host galaxy properties and environment of obscured and unobscured X-ray selected active galactic nuclei in the COSMOS survey

D García Lambas and C Bornancini
Monthly Notices of the Royal Astronomical Society 494 (1) 1189 (2020)
https://doi.org/10.1093/mnras/staa723

Active galactic nuclei at high redshifts: properties and environment of Type 1 and 2 AGNs

C Bornancini and D García Lambas
Monthly Notices of the Royal Astronomical Society 479 (2) 2308 (2018)
https://doi.org/10.1093/mnras/sty1659