Gilligan And O Malley, The isochrones that fit the calibration stars best were then used to determine the distances and ages of 22 GCs with metallicities ranging from −2.

Absolute Ages and Distances of 22 GCs Using Monte Carlo Main-sequence Fitting - IOPscience

Unveiling the Universe with emerging cosmological probes

The GeMS/GSAOI Galactic Globular Cluster Survey (G4CS). I. A Pilot Study of the Stellar Populations in NGC 2298 and NGC 3201 - IOPscience

Unveiling the Universe with emerging cosmological probes

Galpy, PDF, Parameter (Computer Programming)

PDF) The Absolute Age of M92

Grids of stellar models with rotation. I. Models from 0.8 to 120 M_⊙ at solar metallicity (Z = 0.014) - NASA/ADS

2211.12684] Isochrone fitting of Galactic globular clusters – IV. NGC 6362 and NGC 6723

The Physics of Star Cluster Formation and Evolution

PDF) The Absolute Age of M92

The Hubble Tension and Early Dark Energy

The Hubble Tension and Early Dark Energy

Absolute Ages and Distances of 22 GCs Using Monte Carlo Main-sequence Fitting - IOPscience

Unveiling the Universe with emerging cosmological probes

Solved Part 2. Calibration Curves, Squares of the