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Challenges in Panchromatic Modelling with Next Generation Facilities (IAU S341).
・ISBN 978-1-108-47147-3 hard GB£ 125.00
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| 著者・編者 | Boquien, Mederic / Lusso, Elisabeta / Gruppioni, Carlotta / Tissera, Patricia (eds.), |
|---|---|
| シリーズ | (Proceedings of the International Astronomical Union Symposia and Colloquia) |
| 出版社 | (Cambridge University Press, UK) |
| 出版年月 | 2020 |
| ページ数 | 346 pp. |
| 言語 | ENG |
| ニュース番号 | ＜A00-8651＞ |
解説
Over the past decade, modelling the panchromatic emission of galaxies has become one of the key tools in measuring their properties. As new and next-generation facilities progressively herald a new era in observational astronomy, we face new and specific challenges: LSST (recently named the Vera C. Rubin Observatory) and SKA will provide us with an avalanche of data; the advent of e-ROSITA and the preparation for Athena make it ever more pressing to include X-ray emission into the standard UV to radio panchromatic models; JWST will observe the first galaxies with extreme stellar populations; and, in the meantime, ALMA is already starting to provide us with remarkable dust and metal observations at high redshift. The proceedings of IAU Symposium 341 offer a broad overview of the state of the field from theoreticians, modellers, and observers to present and discuss the current frontier in the panchromatic modelling of galaxies.