Challenges in Panchromatic Modelling with Next Generation Facilities (IAU S341)

IAU S341 offers a broad overview of the state of this observational field from, and for, theoreticians, modellers, and observers,

Médéric Boquien (Edited by), Elisabeta Lusso (Edited by), Carlotta Gruppioni (Edited by), Patricia Tissera (Edited by)

9781108471473, Cambridge University Press

Hardback, published 30 July 2020

346 pages
25.4 x 18 x 1.7 cm, 0.71 kg

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 Ma?ek, 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 Ma?ek
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, Ma?gorzata 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

Subject Areas: Astrophysics [PHVB], Astronomical observation: observatories, equipment & methods [PGG], Astronomy, space & time [PG]