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Hsiao, Francesco Taddia, Gast\\'on Folatelli, Jacqueline Ser\\'on, Jing Lu, Jorge Anais, Joseph P. Anderson, Kevin Krisciunas, Lifan Wang, Llu\\'is Galbany, Luis Busta, Mansi Kasliwal, Mario Hamuy, Mark M. Phillips, Maximilian Stritzinger, Melissa Shahbandeh, Miguel Roth, Nicholas B. Suntzeff, Nidia Morrell, Peter E. Nugent, Peter Hoeflich, Peter J. Brown, Sahana Kumar, Saul Perlmutter, Scott Davis, S. E. Persson, Sergio Castell\\'on, Simon Holmbo, Sim\\'on Torres, Stuart D. Ryder, Syed A. Uddin, Tiara Diamond, Wendy L. Freedman","submitted_at":"2023-08-03T17:05:32Z","abstract_excerpt":"We present an analysis of Type Ia Supernovae (SNe~Ia) from both the Carnegie Supernova Project~I (CSP-I) and II (CSP-II), and extend the Hubble diagram from the optical to the near-infrared wavelengths ($uBgVriYJH$). We calculate the Hubble constant, $H_0$, using various distance calibrators: Cepheids, Tip of the Red Giant Branch (TRGB), and Surface Brightness Fluctuations (SBF). 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