The VLA-COSMOS 3 GHz Large Project: Evolution of specific star formation rates out to $z\sim5$
| العنوان: | The VLA-COSMOS 3 GHz Large Project: Evolution of specific star formation rates out to $z\sim5$ |
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| المؤلفون: | Sarah K. Leslie, Yingjie Peng, G. Zamorani, Brent Groves, Mladen Novak, Eleni Vardoulaki, Alexander Karim, Iary Davidzon, Ghassem Gozaliasl, A. J. Battisti, Vernesa Smolčić, Mark Sargent, E. F. Jiménez-Andrade, Daizhong Liu, Philipp Lang, H. S. B. Algera, Benjamin Magnelli, Eva Schinnerer, Mattia Vaccari, Jeyhan S. Kartaltepe |
| المصدر: | The Astrophysical Journal, 899(1), 58 The Astrophysical Journal Leslie, S K, Schinnerer, E, Liu, D, Magnelli, B, Algera, H, Karim, A, Davidzon, I, Gozaliasl, G, Jiménez-Andrade, E F, Lang, P, Sargent, M T, Novak, M, Groves, B, Smolčić, V, Zamorani, G, Vaccari, M, Battisti, A, Vardoulaki, E, Peng, Y & Kartaltepe, J 2020, ' The VLA-COSMOS 3 GHz Large Project : Evolution of Specific Star Formation Rates out to z ∼ 5 ', Astrophysical Journal, vol. 899, no. 1, 58 . https://doi.org/10.3847/1538-4357/aba044 |
| سنة النشر: | 2020 |
| مصطلحات موضوعية: | Stellar mass, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, Extragalactic radio sources, Galaxy evolution, 0103 physical sciences, Galaxy formation and evolution, Astrophysics::Solar and Stellar Astrophysics, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, Galaxy bulges, Physics, 010308 nuclear & particles physics, Star formation, Astronomy, Astronomy and Astrophysics, Galaxy environments, Astrophysics - Astrophysics of Galaxies, Interstellar medium, Radio continuum emission, Space and Planetary Science, Galaxy quenching, Astrophysics of Galaxies (astro-ph.GA), Cosmos (category theory), Astrophysics::Earth and Planetary Astrophysics |
| الوصف: | We provide a coherent, uniform measurement of the evolution of the logarithmic star formation rate (SFR) - stellar mass ($M_*$) relation, called the main sequence of star-forming galaxies (MS), for galaxies out to $z\sim5$. We measure the MS using mean stacks of 3 GHz radio continuum images to derive average SFRs for $\sim$200,000 mass-selected galaxies at $z>0.3$ in the COSMOS field. We describe the MS relation adopting a new model that incorporates a linear relation at low stellar mass (log($M_*$/M$_\odot$)$ Comment: 48 pages (main paper 25 pages, 15 figures). Accepted for publication in The Astrophysical Journal |
| وصف الملف: | application/pdf |
| اللغة: | English |
| تدمد: | 0004-637X 0067-0049 0004-6361 1538-3881 1017-0405 1538-3873 0035-8711 |
| URL الوصول: | https://explore.openaire.eu/search/publication?articleId=doi_dedup___::17ef975c195f865825c7ad3d2d655bbe http://arxiv.org/abs/2006.13937 |
| حقوق: | OPEN |
| رقم الأكسشن: | edsair.doi.dedup.....17ef975c195f865825c7ad3d2d655bbe |
| قاعدة البيانات: | OpenAIRE |
| تدمد: | 0004637X 00670049 00046361 15383881 10170405 15383873 00358711 |
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