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The Dwarf Galaxy Population at z ∼ 0.7: A Catalog of Emission Lines and Redshifts from Deep Keck Observations

  • Authors: John Pharo, Yicheng Guo, Guillermo Barro Calvo, Timothy Carleton, S. M. Faber, Puragra Guhathakurta, Susan A. Kassin, David C. Koo, Jack Lonergan, Teja Teppala, Weichen Wang, Hassen M. Yesuf, Fuyan Bian, Romeel Davé, John C. Forbes, Dusan Keres, Pablo Perez-Gonzalez, Alec Martin, A. J. Puleo, Lauryn Williams, Benjamin Winningham

John Pharo et al 2022 The Astrophysical Journal Supplement Series 261 .

  • Provider: AAS Journals

Caption: Figure 3.

RGB images of example HALO7D galaxies matching the three categories of target described in Figure 2. The photometric bands used are F606W (blue), F814W/F850LP (green), and F160W (red), taken from CANDELS (Guo et al. 2013; Barro et al. 2019) and 3D-HST (Skelton et al. 2014). Each image has a diameter of 60 HST pixels, for a diameter of 3.″6. Dashed lines indicate the placement of spectroscopic slits.

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