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.

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

Isochrone - an overview

The Hubble Tension and Early Dark Energy

Reaction rate ratio of the present reaction rate to the rate compiled

PDF) The Absolute Age of M92

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

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

PDF) Estimating Distance from Parallaxes. IV. Distances to 1.33 Billion Stars in Gaia Data Release 2

R-matrix fit to the S(E) data for the R,DC→0.0 transition. The solid

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

The Hubble Tension and Early Dark Energy

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