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.
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![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.](https://content.cld.iop.org/journals/0004-637X/865/2/160/revision1/apjaadb43f15_hr.jpg?Expires=1710006986&Signature=rpS3auAZGABokMVG0E6IHkbmp6avZS9cUcLZe421ZoLGYy5743RpL1mLKK3jNoH0OuO5DVFHRjQS9Ed8DM3ih6rzLq1mF~1ctlzpXyDuLjtRjeqQ1jTqk6vVQ2Vgg0Aar0m~qDTq2uIXkbaVDBLnqX~AgQlL2xfTvFPw00rYzcEBGnvbJH6MpeDKevREOQ2Fzd-Zwjr-M9YbnMBtkRL7a2NlTGqKoCVkBxSjmCfL15Zq7jKPaN6aZFWY918t-mrqizJmzVcFFdCDNW0XukypdgBNQ5emmLrHbTMn5uEWuNJ380Du8se8h-wJ5~jJUoekNYOHbCoH15OJzCE4FweSVQ__&Key-Pair-Id=KL1D8TIY3N7T8)
The GeMS/GSAOI Galactic Globular Cluster Survey (G4CS). I. A Pilot Study of the Stellar Populations in NGC 2298 and NGC 3201 - IOPscience
Galpy, PDF, Parameter (Computer Programming)
![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.](https://www.researchgate.net/publication/371662970/figure/fig1/AS:11431281168606829@1687034557121/An-example-of-the-result-of-the-adaptive-Voronoi-binning-method-Cappellari-Copin_Q320.jpg)
PDF) The Absolute Age of M92
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Reaction rate ratio of the present reaction rate to the rate compiled
![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.](https://content.cld.iop.org/journals/0004-637X/838/2/162/revision1/apjaa6574f3_hr.jpg)
Absolute Ages and Distances of 22 GCs Using Monte Carlo Main-sequence Fitting - IOPscience
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The Physics of Star Cluster Formation and Evolution
![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.](https://image.slidesharecdn.com/2211-221217114351-8377cc66/85/the-hubble-tension-and-early-dark-energy-4-320.jpg?cb=1671277775)
The Hubble Tension and Early Dark Energy
![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.](https://ar5iv.labs.arxiv.org/html/2211.12684/assets/x16.png)
2211.12684] Isochrone fitting of Galactic globular clusters – IV. NGC 6362 and NGC 6723
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Unveiling the Universe with emerging cosmological probes
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Environmental and Internal Controls on Lagrangian Transitions from Closed Cell Mesoscale Cellular Convection over Subtropical Oceans in: Journal of the Atmospheric Sciences Volume 78 Issue 8 (2021)
![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.](https://content.cld.iop.org/journals/0004-637X/865/2/160/revision1/apjaadb43f8_hr.jpg?Expires=1710006986&Signature=NuBdjejIeH-ivzFGq6DJaRHafFZtOsklNIYdfzf9sRj1ngyZzOV6m1l7Vq51c~yx0-zaHxswudEMb83Orax36Zk-FD6HwJyJrEmQxpPOwSzMUnxXFsRJYpBQmWu~5wcjapEPxe9cmhPlaWWnLXFkVJtRVsQOa4p1-M-3Qu8OGrolDDSKwTp-zIFt~ueKYNzup5wvo4TBogpdY9MUWOJ0SFPpXnU96StqrLp~WZgOWKRL0cMvhvS8QAp5ZAuF~4xny4aVTjeQ7jCS4kzaI8uGXcGCZ2BpzpSJlxFNNOVsfcsKZMyBUoRTI1wraFLEJS4RnABgQhi9cbjPOplBdMri0Q__&Key-Pair-Id=KL1D8TIY3N7T8)
The GeMS/GSAOI Galactic Globular Cluster Survey (G4CS). I. A Pilot Study of the Stellar Populations in NGC 2298 and NGC 3201 - IOPscience
![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.](https://content.cld.iop.org/journals/0004-637X/891/1/37/revision1/apjab6f76f16_hr.jpg?Expires=1708128594&Signature=csh0iH0Ycx5WBeZbo1OyLJgDNjb-G32vNHEwxzgEgVYb06ei4yJx8wAjQBzz4Yd5pc3Dliu96Vv8g3szqRXIpAvsm97lBjoldD8DtBtzIXubs5FoVadCIMOk87kqbU-emLXVs7JeF4hsadOm46OUZ8zr661xXoevg5R91xC5uQCZWwZ-6AGbsPyauF3MIDyeoN49NwcT1IM0y57HJr~NzSd6bxorW7TK6Io~eEUOu0GS4LhY7nbxnh5ZvyT8j2W8TXpPJDsmn8JVJIlXpOse~ne-alLsv4tqiqYRdX~rrlLymnvEuxD5FjnPvE8fwLXy6kRf3gU0~pYBDuyypNuMpw__&Key-Pair-Id=KL1D8TIY3N7T8)
The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XX. Ages of Single and Multiple Stellar Populations in Seven Bulge Globular Clusters - IOPscience
![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.](https://ar5iv.labs.arxiv.org/html/2211.12684/assets/x9.png)
2211.12684] Isochrone fitting of Galactic globular clusters – IV. NGC 6362 and NGC 6723
![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.](https://image.slidesharecdn.com/2211-221217114351-8377cc66/85/the-hubble-tension-and-early-dark-energy-21-320.jpg?cb=1671277775)
The Hubble Tension and Early Dark Energy
![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.](https://www.researchgate.net/publication/51891502/figure/fig2/AS:342259527634944@1458612438281/sochrones-for-a-cluster-of-stars-with-masses-between-07-M-and-35-M-that-evolved-in-a.png)
Isochrones for a cluster of stars with masses between 0.7 M☉ and 3.5 M☉
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