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THE CARNEGIE-CHICAGO HUBBLE PROGRAM. VII. THE DISTANCE TO M 101 VIA THE OPTICAL TIP OF THE RED GIANT BRANCH METHOD
THE CARNEGIE-CHICAGO HUBBLE PROGRAM. VII. THE DISTANCE TO M 101 VIA THE OPTICAL TIP OF THE RED GIANT BRANCH METHOD
2019
Rachael L. Beaton
Mark Seibert
Dylan Hatt
Wendy L. Freedman
Taylor J. Hoyt
In-Sung Jang
Myung Gyoon Lee
Barry F. Madore
Andrew J. Monson
Jillian R. Neeley
Jeffrey A. Rich
Victoria Scowcroft
Keywords:
Physics
Astrophysics
Astronomy
Red-giant branch
Correction
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