Extrapolation of Type Ia Supernova Spectra into the Near-infrared Using Principal Component Analysis
We present a method of extrapolating the spectroscopic behavior of Type Ia supernovae (SNe Ia) in the near-infrared (NIR) wavelength regime up to 2.30 μ m using optical spectroscopy. Such a process is useful for accurately estimating K-corrections and other photometric quantities of SNe Ia in the NI...
Збережено в:
| Автори: | , , , , , , , , , , , , , , , , |
|---|---|
| Формат: | Artigo |
| Мова: | Inglês |
| Опубліковано: |
IOP Publishing
2024-01-01
|
| Серія: | The Astrophysical Journal |
| Предмети: | |
| Онлайн доступ: | https://doi.org/10.3847/1538-4357/ad3c45 |
| Теги: |
Немає тегів, Будьте першим, хто поставить тег для цього запису!
|
