Challenges in Panchromatic Modelling with Next Generation Facilities (IAU S341)
Cambridge University Press (Verlag)
978-1-108-47147-3 (ISBN)
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.
Preface; Editors; Participants; A historical overview of galaxy surveys Sadanori Okamura; Panchromatic study of the first galaxies with large ALMA programs A. Faisst, M. Béthermin, P. Capak, et al.; The average FIR SED of proto-clusters at z = 4 Mariko Kubo, Jun Toshikawa, Nobunari Kashikawa, et al.; The spectral energy distributions of active galactic nuclei M. J. I. Brown, K. J. Duncan, H. Landt, et al.; Panchromatic SED fitting codes and modelling techniques Maarten Baes; Evolutionary Population Synthesis model with binary stars – Yunnan-II model F. Zhang, Z. Han and L. Li; HELP project – a dreamed-of multiwavelength dataset for SED fitting Katarzyna Małek, Veronique Buat, Denis Burgarella, et al.; Modelling the emission of passive galaxy candidates at z ∼ 3 C. D'Eugenio, E. Daddi, R. Gobat, et al.; Evolution histories of massive galaxies at z ∼ 2 over the past 3 Gyr T. Morishita, L. E. Abramson, T. Treu, et al.; Spatially resolved stellar mass buildup and quenching in massive disk galaxies over the last 10 Gyr revealed with spatially resolved SED fitting Abdurro'uf and Masayuki Akiyama; Exploring the star formation histories of galaxies in different environments from MaNGA spectra Maria Argudo-Fernández, Médéric Boquien, Shiyin Shen, et al.; High-resolution radiation transfer modelling of barred galaxies A. Nersesian, S. Verstocken, S. Viaene and M. Baes; Which attenuation curves for star-forming galaxies? Véronique Buat, David Corre, Médéric Boquien and Katarzyna Małek; Dust attenuation on and off the galaxy Main Sequence at z ≥ 1 Annagrazia Puglisi; Spatially resolved dust-to-gas mass ratios in nearby galaxies Basilio Solís-Castillo and Marcus Albrecht; A MUSE inquiry into the physical processes taking place within the Abell 2667 Brightest Cluster Galaxy E. Iani, G. Rodighiero, J. Fritz, et al.; Pushing the technical frontier: From overwhelmingly large data sets to machine learning Viviana Acquaviva; Modeling with the crowd: Optimizing the human-machine partnership with Zooniverse Hugh Dickinson, Lucy Fortson, Claudia Scarlata, et al.; Deep learning for galaxy mergers in the galaxy main sequence William J. Pearson, Lingyu Wang, James Trayford, et al.; Automatic classification of sources in large astronomical catalogs Agnieszka Pollo, Aleksandra Solarz, Małgorzata Siudek, et al.; Predicting the global far-infrared emission of galaxies Wouter Dobbels and Maarten Baes; Mentari: A pipeline to model the galaxy SED using semi analytic models Dian Triani, Darren Croton and Manodeep Sinha; Variations of the stellar Initial Mass Function in semi-analytic models Fabio Fontanot; Modeling the panchromatic emission of galaxies with CIGALE M. Boquien, D. Burgarella, Y. Roehlly, et al.; Going beyond galaxy ages with dense basis star formation history reconstruction Kartheik G. Iyer and Eric Gawiser; A hierarchical Bayesian dust SED model and its application to the nearby universe Frédéric Galliano; Bayesian discrimination of the panchromatic spectral energy distribution modelings of galaxies Yunkun Han, Zhanwen Han and Lulu Fan; Stellar population synthesis of galaxies with chemical evolution model Shiyin Shen and Jun Yin; A new galaxy Spectral Energy Distribution model with the evolution of dust consistent with chemical evolution Kazuki Y. Nishida, Tsutomu T. Takeuchi, Takuma Nagata, et al.; The Spitzer Extragalactic Representative Volume Survey – measuring photometric redshifts for ∼4 million galaxies Janine Pforr; Probing the building blocks of galaxies: Sub-galactic scaling relations between X-ray luminosity, SFR and stellar mass K. Kouroumpatzakis, A. Zezas, P. Sell, et al.; Tips learned from panchromatic modeling of AGNs Y. Sophia Dai; X-ray – Infrared relation of AGNs and search for highly obscured accretion in the AKARI NEP Field Takamitsu Miyaji and AKARI NEP Survey Team; The Diagnostic power of radio spectra from star
| Erscheinungsdatum | 16.11.2020 |
|---|---|
| Reihe/Serie | Proceedings of the International Astronomical Union Symposia and Colloquia |
| Zusatzinfo | Worked examples or Exercises |
| Verlagsort | Cambridge |
| Sprache | englisch |
| Maße | 180 x 254 mm |
| Gewicht | 710 g |
| Themenwelt | Naturwissenschaften ► Physik / Astronomie ► Astronomie / Astrophysik |
| ISBN-10 | 1-108-47147-1 / 1108471471 |
| ISBN-13 | 978-1-108-47147-3 / 9781108471473 |
| Zustand | Neuware |
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