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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 10.

Top: photometric redshifts z p (primarily from CANDELS, Dahlen et al. 2013; EGS/IRAC, Barro et al. 2011a, 2011b; and COSMOS/UltraVista, Muzzin et al. 2013) compared to the redshift from HALO7D spectra z h7, colored by the stellar mass. Bottom: the difference in redshift between z h7 and z p , colored by the stellar mass. The solid black points show the median difference as a function of z h7.

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