An Improved Distance to NGC 4258 and Its Implications for the Hubble Constant
Close Binary Stars. VI: New Research Methods
Measurements of the Hubble Constant: Tensions in Perspective
Metallicity-corrected Tip of the Red Giant Branch Distance to NGC 4258
Sharpening the Tip of the Red Giant Branch
Standardized Luminosity of the Tip of the Red Giant Branch Utilizing Multiple Fields in NGC 4258 and the CATs Algorithm
The Carnegie-Chicago Hubble Program. I. An Independent Approach to the Extragalactic Distance Scale Using Only Population II Distance Indicators
The Carnegie-Chicago Hubble Program. IX. Calibration of the Tip of the Red Giant Branch Method in the Megamaser Host Galaxy, NGC 4258 (M106)
The impact of satellite trails on Hubble Space Telescope observations
The Tip of the Red Giant Branch Distances to Type Ia Supernova Host Galaxies. IV. Color Dependence and Zero-point Calibration
Tip of the Red Giant Branch Distances. II. Zero-Point Calibration
Instrument
ACS, ACS/HRC, ACS/WFC
Temporal Coverage
2003-05-05T12:49:24Z/2003-05-05T16:42:55Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Madore et al., 2004, 'TRGB Distance to the Maser Galaxy NGC4258', 1.0, European Space Agency, https://doi.org/10.5270/esa-7cpu3fc
