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

Table of Contents

• 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
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