Pushing the technical frontier: from overwhelming large datasets to machine learning
Denis Burgarella
› A new stellar population fitting algorithm based on chemical evolution models - Shiyin Shen, Shanghai Astronomical Observatory, Chinese Academy of Sciences
09:25-09:45 (20min)
› A new galaxy spectral energy distribution model with the evolution of dust consistent with chemical evolution - Kazuki Nishida, Nagoya University
09:45-10:05 (20min)
› AGN mocks for Euclid - Elisabeta Lusso, Durham University
10:05-10:25 (20min)
› The Spitzer Extragalactic Representative Volume Survey (SERVS): measuring photometric redshifts for ~4 million galaxies – challenges and ways forward - Janine Pforr, European Space Research and Technology Centre
10:25-10:45 (20min)
› Galaxy photometric and dynamical modelling in the era of all-sky multiwavelength surveys - Dan Taranu, Princeton University
10:45-11:05 (20min)
Pushing the wavelength frontier: extending models towards X-rays and radio
Elisabeta Lusso
› eROSITA: Mapping the Hot Universe - Andrea Merloni, Max-Planck-Institut für Extraterrestrische Physik
11:35-12:15 (40min)
› Probing the building blocks of galaxies: sub-galactic scaling relations between X-ray luminosity, SFR and stellar mass. - Konstantinos Kouroumpatzakis, University of Crete, Institute of Electronic Structure and Laser
12:15-12:35 (20min)
› Importance and tips learned from panchromatic modeling of AGNs - Y.Sophia Dai, National Astronomical Observatories
12:35-12:55 (20min)
› X-ray - Infrared relation of AGNs and search for highly obscured accretion in the AKARI NEP Field - Takamitsu Miyaji, Universidad Nacional Autónoma de México, Instituto de Astronomía Ensenada
12:55-13:15 (20min)
Pushing the wavelength frontier: extending models towards X-rays and radio
Tohru Nagao
› Modeling the Energetic Processes Powering Radio Continuum Emission from Galaxies - Eric Murphy, National Radio Astronomy Observatory
14:30-15:10 (40min)
› Panchromatic characterisation of AGN and star-forming galaxies- From the radio to the X-rays - Gabriela Calistro-Rivera, Leiden Observatory
15:10-15:30 (20min)
› Characterization of dusty galaxies uncovered by ALMA 26 arcmin^2 survey of GOODS-S at one-millimeter (ASAGAO) - Kotaro Kohno, The University of Tokyo
15:30-15:50 (20min)
Pushing the redshift frontier: modeling the first galaxies
Hiroyuki Hirashita
› Modelling challenges in the rest-frame UV/optical at the high-redshift frontier - Erik Zackrisson, Uppsala University
16:40-17:20 (40min)
› Systematic errors in high-redshift dust mass fits: the role of dust opacity - Lapo Fanciullo, Academia Sinica, Institute of Astronomy and Astrophysics
17:20-17:40 (20min)
› Properties of LBGs with [OIII] detections at z > 3: The importance of including nebular emission data in SED fitting - Fangting Yuan, Laboratoire dÁstrophysique de Marseille, Shanghai Astronomical Observatory
17:40-18:00 (20min)
› Modeling the dust content and dust-absorbed SED of galaxies in the early Universe - Gergö Popping, MPIA
18:00-18:20 (20min)