التفاصيل البيبلوغرافية
| العنوان: |
Characterizing the Average Interstellar Medium Conditions of Galaxies at $z\sim$ 5.6-9 with UV and Optical Nebular Lines |
| المؤلفون: |
Hu, Weida, Papovich, Casey, Dickinson, Mark, Kennicutt, Robert, Shen, Lu, Amorín, Ricardo O., Haro, Pablo Arrabal, Bagley, Micaela B., Bhatawdekar, Rachana, Cleri, Nikko J., Cole, Justin W., Dekel, Avishai, de la Vega, Alexander, Finkelstein, Steven L., Grogin, Norman A., Hathi, Nimish P., Hirschmann, Michaela, Holwerda, Benne W., Hutchison, Taylor A., Jung, Intae, Koekemoer, Anton M., Kartaltepe, Jeyhan S., Lucas, Ray A., Llerena, Mario, Mascia, S., Mobasher, Bahram, Napolitano, L., Newman, Jeffrey A., Pentericci, Laura, Pérez-González, Pablo G., Trump, Jonathan R., Wilkins, Stephen M., Yung, L. Y. Aaron |
| سنة النشر: |
2024 |
| المجموعة: |
Astrophysics |
| مصطلحات موضوعية: |
Astrophysics - Astrophysics of Galaxies |
| الوصف: |
Ultraviolet (UV; rest-frame $\sim1200-2000$ A) spectra provide a wealth of diagnostics to characterize fundamental galaxy properties, such as their chemical enrichment, the nature of their stellar populations, and their amount of Lyman-continuum (LyC) radiation. In this work, we leverage publicly released JWST data to construct the rest-frame UV-to-optical composite spectrum of a sample of 63 galaxies at $5.6Comment: 21 pages, 7 figures, 4 tables. Submitted. Comments are welcome |
| نوع الوثيقة: |
Working Paper |
| URL الوصول: |
http://arxiv.org/abs/2401.12402 |
| رقم الانضمام: |
edsarx.2401.12402 |
| قاعدة البيانات: |
arXiv |