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The Fraction of Active Galactic Nuclei in the USS 1558–003 Protocluster at z = 2.53

  • Authors: Michael Macuga, Paul Martini, Eric D. Miller, Mark Brodwin, Masao Hayashi, Tadayuki Kodama, Yusei Koyama, Roderik A. Overzier, Rhythm Shimakawa, Ken-ichi Tadaki, and Ichi Tanaka

2019 The Astrophysical Journal 874 54.

  • Provider: AAS Journals

Caption: Figure 1.

An ﹩r﹩-band image from Subaru of the USS 1558−003 protocluster. The large, black box shows the 6′ × 6′ field of view of MODS. The large blue circles show three overdense clumps within USS 1558−003 that were identified by Hayashi et al. (2012). The small, black circles are the HAEs from the Hayashi et al. (2016) catalog, and the small magenta ellipses are the X-ray sources from Chandra. The red rectangles mark the five galaxies with confirmed spectroscopic redshifts from our LBT observations. The two members are the ApID 10 (4C-00.62) and ApID 13.

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