New calibrated models for the tip of the red giant branch luminosity and a thorough analysis of theoretical uncertainties

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F22%3A00567137" target="_blank" >RIV/68378271:_____/22:00567137 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1093/mnras/stac1546" target="_blank" >https://doi.org/10.1093/mnras/stac1546</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1093/mnras/stac1546" target="_blank" >10.1093/mnras/stac1546</a>

Result language
angličtina
Original language name
New calibrated models for the tip of the red giant branch luminosity and a thorough analysis of theoretical uncertainties
Original language description
The luminosity of TRGB stars is key for the determination of the Hubble parameter. We presented the most complete analysis up to date of the theoretical uncertainties on of the luminosity of these stars. Our analysis produced the largest database of TRGB models in the literature which will enhance greatly future works in the field.
Czech name
—
Czech description
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Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)

Project
<a href="/en/project/GM21-16583M" target="_blank" >GM21-16583M: New avenues in the hunt for dark energy</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2022
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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