Gilligan And O Malley, The isochrones that fit the calibration
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![](https://www.researchgate.net/publication/371662970/figure/tbl1/AS:11431281168615163@1687034557530/Monte-Carlo-Input-Parameters_Q320.jpg)
PDF) The Absolute Age of M92
![](https://ar5iv.labs.arxiv.org/html/2211.12684/assets/x12.png)
2211.12684] Isochrone fitting of Galactic globular clusters – IV. NGC 6362 and NGC 6723
![](https://www.researchgate.net/publication/371662970/figure/fig3/AS:11431281168622537@1687034557403/The-empirical-ch-2-distribution-is-shown-in-red-while-the-ch-2-values-determined-from_Q320.jpg)
PDF) The Absolute Age of M92
![](https://media.springernature.com/m685/springer-static/image/art%3A10.1007%2Fs41114-022-00040-z/MediaObjects/41114_2022_40_Fig7_HTML.png)
Unveiling the Universe with emerging cosmological probes
![](https://www.researchgate.net/publication/317378228/figure/fig1/AS:502452001492992@1496805300366/Left-aluminum-transmission-spectrum-measured-by-Davidson-et-al-27-on-HELEN-laser_Q320.jpg)
R-matrix fit to the S(E) data for the R,DC→0.0 transition. The solid
![](https://d3i71xaburhd42.cloudfront.net/429459fceec24e1a0c3b3538ec89518406e6f092/24-Figure9-1.png)
PDF] Accurate distances to Galactic globular clusters through a combination of Gaia EDR3, HST, and literature data
![](https://content.cld.iop.org/journals/0004-637X/865/2/160/revision1/apjaadb43f17_hr.jpg?Expires=1710006986&Signature=vXcI0wxHry3mTdTv-9bHvtFHXkJQTWLITAIAVMJwRwZoqMLjXQhmwHo9WIeEAAexn53PLp~gAkijCJIK6BrX5kOdW5sdU5XA2b12q0LZof~epJQDUBXV5QPgxA5NA0~2e1Z2Hn9CxmfZvm2KM73vWuBFPtBpjfbmCwCWAUfKEAQ1ZYfk232bACrFNx75tGApo2xlby8Xpr0S7WWIQKzKc4TMlsMmab5XoZ1K9BLWsY07XtYvn2iAH~XCLV9zYNFq6ajnI68pBPcYqzIF2iVJBjOgFEpk6yT5ehVP5q0nnfmeoIPhVhJqNubSrKS0DVV-Ax4sxtdQA7nt9gDdHxyItA__&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
![](https://content.cld.iop.org/journals/0004-637X/856/1/10/revision1/apjaab200f3_lr.jpg?Expires=1708966482&Signature=c15ExVwAWixfIo93r8QBrSKAFTqBdkOmyBhLDG-bqRe~oErY1zek46Yg1Vif0j3IaE-BqDQcOrfirV3x6Y7xb9DGGZvKNCSOnVbyAi35eu2Yj2JlErXvBez2GjWrxSWOWR7Gf-F6ZDlyNndiMb56BcRk2NVCVS3eoVN7v~9Ahb9u~s9PDh9HrARJGl1wSqBPW~N01UfQf9Wo7VtYL9C75Qgy3-EfUo4HVxVBaz2l2GFMkgdnFot0X4QcC0XQRwJEhVf6dmj9EMp0eH6-VTFliygSR7CYwGgJPbi9KUR4ETQ261VjGBL69rV0SK~7DHJYh1O9I9ugEUZPva8DVB4JaQ__&Key-Pair-Id=KL1D8TIY3N7T8)
Not All Stars Are the Sun: Empirical Calibration of the Mixing Length for Metal-poor Stars Using One-dimensional Stellar Evolution Models - IOPscience
![](https://www.researchgate.net/publication/317378228/figure/fig5/AS:502452002582530@1496805300654/Iron-transmission-spectrum-measured-by-Bailey-et-al-33-on-the-SNL-Z-facility_Q320.jpg)
Reaction rate ratio of the present reaction rate to the rate compiled
![](https://media.springernature.com/lw685/springer-static/image/art%3A10.1007%2Fs41114-022-00040-z/MediaObjects/41114_2022_40_Fig3_HTML.png)
Unveiling the Universe with emerging cosmological probes
![](https://ar5iv.labs.arxiv.org/html/2211.12684/assets/x5.png)
2211.12684] Isochrone fitting of Galactic globular clusters – IV. NGC 6362 and NGC 6723
![](https://www.researchgate.net/profile/Pavel-Usachev-2/publication/354893680/figure/fig3/AS:1073024895811585@1632840479252/The-distribution-of-stars-selected-within-187-arcmin-of-the-NGC-362-centre-on-the_Q320.jpg)
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