Challenges in Panchromatic Modelling with Next Generation Facilities

›9:05 (20min)

Registration open

9:05 - 9:25 (20min)

Registration open

Registration desk is open throughout the week

›9:25 (1h40)

Pushing the technical frontier: from overwhelming large datasets to machine learning
Denis Burgarella

9:25 - 11:05 (1h40)

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)

›11:05 (30min)

Poster session and Break

11:05 - 11:35 (30min)

Poster session and Break

›11:35 (1h40)

Pushing the wavelength frontier: extending models towards X-rays and radio
Elisabeta Lusso

11:35 - 13:15 (1h40)

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)

›13:15 (1h15)

Lunch

13:15 - 14:30 (1h15)

Lunch

›14:30 (1h20)

Pushing the wavelength frontier: extending models towards X-rays and radio
Tohru Nagao

14:30 - 15:50 (1h20)

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)

›15:50 (20min)

Poster award presentation

15:50 - 16:10 (20min)

Poster award presentation

›16:10 (30min)

Poster session and Break

16:10 - 16:40 (30min)

Poster session and Break

›16:40 (1h40)

Pushing the redshift frontier: modeling the first galaxies
Hiroyuki Hirashita

16:40 - 18:20 (1h40)

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)