“Supernovae Ia Twins” in the Hubble Flow, and the Determination of H0
We have applied our approach of using “supernovae (SNe) Ia twins” in the Hubble flow to obtain distances to SNe Ia at z > 0.015 and derive H _0 . Our results, taking a single step between the low- z domain and the Hubble flow, validate the three-rung classical method. We find, however, that the ful...
Tallennettuna:
| Päätekijät: | , , , |
|---|---|
| Aineistotyyppi: | Artigo |
| Kieli: | Inglês |
| Julkaistu: |
IOP Publishing
2026-01-01
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| Sarja: | The Astrophysical Journal |
| Aiheet: | |
| Linkit: | https://doi.org/10.3847/1538-4357/ae632a |
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