Comparing Tip of the Red Giant Branch Distance Scales: An Independent Reduction of the Carnegie-Chicago Hubble Program and the Value of the Hubble Constant
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Abstract The tip of the red giant branch has been used to measure distances to 500 nearby galaxies with the Hubble Space Telescope (HST) which are available in the Color–Magnitude Diagrams and Tip of the Red Giant Branch (CMDs/TRGB) catalog on the Extragalactic Distance Database (EDD). Our established methods are employed to perform an independent reduction of the targets presented by the Carnegie-Chicago Hubble Program (CCHP) in the series of papers culminating in Freedman (2021). Our distinct methodology involves modeling the observed luminosity function of red giant branch and asymptotic giant branch stars, which differs from the edge-detection algorithms employed by the CCHP. We find excellent agreement between distances for 11 hosts with new imaging, all at D < 20 Mpc. However, we are unable to measure the TRGB for four hosts that use archival data designed to measure distances with Cepheids, all at D > 23 Mpc. With two new HST observations taken in the halo of the megamaser host NGC 4258, the first with the same ACS F606W and F814W filters and state of the electronics used for SN Ia hosts, we then calibrate our TRGB distance scale to the geometric megamaser distance. Using our TRGB distances, we find a value of the Hubble Constant of H 0 = 71.5 ± 1.8 km s−1 Mpc−1 when using either the Pantheon or Carnegie Supernova Project (CSP) samples of supernovae. In the future, the James Webb Space Telescope will extend measurements of the TRGB to additional hosts of SN Ia and surface-brightness fluctuation measurements for separate paths to H 0.
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The CCHP reanalysis of targets is shifted more in agreement with the SH0ES value.
“the new independent reanalysis of the targets presented by the Carnegie-Chicago Hubble Program (CCHP) performed in [36] that is shifted more in agreement with the SH0ES value.”
From Challenges of the Standard Cosmological Model (2022) · cites this paper as [36]
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Tang, Y., Anand, G. S., Romanowsky, A. J., van Dokkum, P., & Bundy, K. A. (2026) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/ae77ef · Cited by 1 · see citing works
Self-citation“Supernovae Ia Twins” in the Hubble Flow, and the Determination of H 0
Ruiz-Lapuente, P., Quintana, A., Hernández, J. I. G., & Pastorello, A. (2026) · The Astrophysical Journal · doi:10.3847/1538-4357/ae632a · Cited by 1 · see citing works
The Tip of the Red Giant Branch as a Cosmological Tool
Lee, M. G. (2022) · Proceedings of the International Astronomical Union · doi:10.1017/s1743921323002685 · Cited by 1 · see citing works
- Authors
- Anand, G. S., Tully, R. B., Rizzi, L., Riess, A. G., & Yuan, W.
- Affiliations
- University of Hawaiʻi at Mānoa (US)
- W.M. Keck Observatory (US)
- Space Telescope Science Institute (US)
- Johns Hopkins University (US)
- Corresponding author
- Anand, Gagandeep S.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2022-06-01
- Volume
- 932
- Issue
- 1
- Pages
- 15
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W3187894162
- Cited by
- 109
- References
- 72
- Citations by year
- 2026: 16 · 2025: 23 · 2024: 27 · 2023: 22 · 2022: 18 · 2021: 3
- FWCI
- 9.00
- Type
- journal article
- Language
- en
- Open access
- gold
- doi.org
- Licence
- Locations
- The Astrophysical Journal (publishedVersion, cc-by)
- arXiv (Cornell University) (submittedVersion)
- arXiv (Cornell University)
- Funders
- HST (SNAP-15922)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Keywords
- tip of the red giant branch, Hubble constant, asymptotic giant branch stars, Type Ia supernovae, Pantheon sample, Carnegie Supernova Project, surface brightness fluctuations, Hubble Space Telescope imaging
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