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...
I tiakina i:
| Ngā kaituhi matua: | , , , , |
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| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
IOP Publishing
2023-01-01
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| Rangatū: | The Astrophysical Journal Letters |
| Ngā marau: | |
| Urunga tuihono: | https://doi.org/10.3847/2041-8213/acdef6 |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
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