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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 8.

Each pair of panels gives the F606W AB magnitude histograms and success fractions for one of the four HALO7D fields. The top panels give magnitude histograms for the whole target sample (white), the sample with usable extracted spectra (red), and the sample with good redshift fits (blue). The bottom panels give the success fractions as a function of magnitude. The red dashed line is the fraction of usable spectra out of the target sample in a given magnitude bin. The solid blue line gives the fraction of spectra with good redshift fits out of the total target sample.

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