Templates for Fitting Photometry of Ultra-high-redshift Galaxies
Recent data from the James Webb Space Telescope allow a first glimpse of galaxies at z ≳ 11. The most successful tool for identifying ultra-high-redshift candidates and inferring their properties is photometric template fitting. However, current methods rely on templates derived from much lower-reds...
Wedi'i Gadw mewn:
| Prif Awduron: | , , , , |
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| Fformat: | Artigo |
| Iaith: | Inglês |
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IOP Publishing
2023-01-01
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| Cyfres: | The Astrophysical Journal Letters |
| Pynciau: | |
| Mynediad Ar-lein: | https://doi.org/10.3847/2041-8213/acdef6 |
| Tagiau: |
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