The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method
Author:
Funder
NASA
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ab4263/pdf
Reference87 articles.
1. Ground-Based Discovery of Cepheids and Miras in M101
2. A Robust Tip of the Red Giant Branch Distance to the Fireworks Galaxy (NGC 6946)
3. Old-Aged Primary Distance Indicators
4. THE CARNEGIE-CHICAGO HUBBLE PROGRAM. I. AN INDEPENDENT APPROACH TO THE EXTRAGALACTIC DISTANCE SCALE USING ONLY POPULATION II DISTANCE INDICATORS
5. PERFECTING THE PHOTOMETRIC CALIBRATION OF THE ACS CCD CAMERAS
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1. CHAOS. VIII. Far-ultraviolet Spectra of M101 and the Impact of Wolf–Rayet Stars*;The Astrophysical Journal;2024-08-01
2. Erratum: “Systematics in the Cepheid and TRGB Distance Scales: Metallicity Sensitivity of the Wesenheit Leavitt Law” (2024, ApJ, 961, 166);The Astrophysical Journal;2024-07-31
3. The SN 2023ixf Progenitor in M101. II. Properties;The Astrophysical Journal;2024-06-01
4. Resolved Near-infrared Stellar Photometry from the Magellan Telescope for 13 Nearby Galaxies: J-region Asymptotic Giant Branch Method Distances;The Astrophysical Journal;2024-05-01
5. Tip of the Red Giant Branch Distances with JWST: An Absolute Calibration in NGC 4258 and First Applications to Type Ia Supernova Hosts;The Astrophysical Journal;2024-04-26
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