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The Carnegie–Chicago Hubble Program. V. The Distances to NGC 1448 and NGC 1316 via the Tip of the Red Giant Branch

  • Authors: Dylan Hatt, Wendy L. Freedman, Barry F. Madore, In Sung Jang, Rachael L. Beaton, Taylor J. Hoyt, Myung Gyoon Lee, Andrew J. Monson, Jeffrey A. Rich, Victoria Scowcroft, and Mark Seibert

2018 The Astrophysical Journal 866 145.

  • Provider: AAS Journals

Caption: Figure 4.

TRGB edge detection for NGC 1448 and NGC 1316. Panels (a) and (d) display the CMDs. A red arrow in each plot shows the location of the measured TRGB. Panels (b) and (e) show the binned luminosity functions in 0.01 mag intervals in gray and the GLOESS-smoothed luminosity functions in solid green. Panels (c) and (f) show the response function of the [−1, 0, +1] kernel on the smoothed luminosity functions. These functions are scaled so that their peaks align. A dashed line passes through the location of the greatest change in the luminosity functions.

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