Figure 4 from The Next Generation Fornax Survey (NGFS). V. Discovery of a Dwarf–Dwarf Galaxy Pair at z = 0.30 and Its Characterization Using Deep VLT/MUSE Observations

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The Next Generation Fornax Survey (NGFS). V. Discovery of a Dwarf–Dwarf Galaxy Pair at z = 0.30 and Its Characterization Using Deep VLT/MUSE Observations

Authors: Evelyn J. Johnston, Paul Eigenthaler, Thomas H. Puzia, Yasna Ordenes-Briceño, Matthew A. Taylor, Karla Alamo-Martínez, Patrick Côté, Gaspar Galaz, Eva K. Grebel, Michael Hilker, Ariane Lançon, Steffen Mieske, Ruben Sánchez-Janssen, and Yu Rong

2019 The Astrophysical Journal 873 59.

Provider: AAS Journals

Caption: Figure 4.

A histogram showing the distribution of spectroscopic redshifts for all targets shown in Figure 3. The globular clusters from Mentz et al. (2016), for which redshifts could not be obtained with the MUSE data, were assigned a redshift of z = 0.003 to match NGC 1396.

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