› A Historical Overview of Galaxy Surveys - Sadanori Okamura, Executive Management Program, University of Tokyo
09:45-10:25 (40min)
› The physical ingredients for panchromatic modeling - Stephane Charlot, Institut d'Astrophysique de Paris / CNRS-Sorbonne Université
10:25-11:05 (40min)
› ALPINE: The large ALMA Program to Study the Interstellar Medium of High Redshift Galaxies - Andreas Faisst, Infrared Processing and Analysis Center
11:35-11:55 (20min)
› ALMA unveils a large population of massive galaxies at z>3 that are hidden from HST - Tao Wang, University of Tokyo
11:55-12:15 (20min)
› 18-band SED fitting in mid-infrared in the AKARI NEP field. - Tomotsugu Goto, National Tsing Hua University
12:15-12:35 (20min)
› The averaged FIR SED of protoclusters at z=4 - Mariko Kubo, NAOJ
12:35-12:55 (20min)
› The spectral energy distributions of active galactic nuclei - Michael Brown, Monash University
12:55-13:15 (20min)
› A revised picture of galaxy stellar mass assembly from panchromatic SED fitting of the 3D-HST survey - Joel Leja, Harvard- Smithsonian Center for Astrophysics
16:40-17:00 (20min)
› HELP - a dreamed-of multiwavelength dataset for SED fitting: a new approach to select peculiar galaxies, the prediction of Ldust and the influence of used models for the main physical properties of galaxies. - Katarzyna Malek, Laboratoire dÁstrophysique de Marseille, National Center for Nuclear Research
17:00-17:20 (20min)
› Are SMGs on the Main Sequence of galaxies? - Laia Barrufet, ESAC / RAL Space
17:20-17:40 (20min)
› Modeling the emission of passive galaxies at z~3 - Chiara D'Eugenio, CEA Saclay, Université Paris Diderot, Irfu/SAp
17:40-18:00 (20min)
› Evolution histories of massive galaxies at z~2 over the past 3Gyr - Takahiro Morishita, Space Telescope Science Institute
18:00-18:20 (20min)
› Study of the spatially resolved stellar mass buildup and quenching in massive disk galaxies over the last 10 Gyrs using spatially resolved SED fitting - Abdurrouf Abdurrouf, Tohoku University/ASIAA
09:25-09:45 (20min)
› Probing star formation quenching in galaxies with resolved optical and radio data - Lihwai Lin, Academia Sinica Institute of Astronomy and Astrophysics
09:45-10:05 (20min)
› Exploring the Star Formation Histories of Galaxies in Different Environments from MaNGA Spectra - Maria Argudo Fernandez, Center of Astronomy of the University of Antofagasta
10:05-10:25 (20min)
› High-resolution, 3D radiative transfer modeling of barred galaxies - Angelos Nersesian, Ghent University, IAASARS, National Observatory of Athens
10:25-10:45 (20min)
› Which dust attenuation law(s) for star forming galaxies? - Veronique Buat, Laboratoire dÁstrophysique de Marseille
11:35-11:55 (20min)
› Dust attenuation on and off the galaxy Main Sequence at z>1 - Annagrazia Puglisi, CEA-Saclay
11:55-12:15 (20min)
› Spatially resolved dust-to-gas mass ratio in nearby galaxies - Basilio Solis-Castillo, Max Planck Institute for Radio Astronomy, University of Bonn
12:15-12:35 (20min)
› A MUSE multi-wavelength analysis of the Abell 2667 BCG - Edoardo Iani, University of Padova
12:35-12:55 (20min)
Pushing the technical frontier: from overwhelming large datasets to machine learning
Katarzyna Malek
› Pushing the technical frontier from large datasets to machine learning - Viviana Acquaviva, New York City College of Technology
14:30-15:10 (40min)
› Modeling with the Crowd: Optimizing the Human-Machine Partnership with Zooniverse - Hugh Dickinson, University of Minnesota - Twin Cities
15:10-15:30 (20min)
› Deep Learning for Galaxy Mergers in the Galaxy Main Sequence - William Pearson, Kapteyn Astronomical Institute, SRON Netherlands Institute for Space Research
15:30-15:50 (20min)
Pushing the technical frontier: from overwhelming large datasets to machine learning
Maarten Baes
› Automatic classification of sources in large astronomical catalogues - Agnieszka Pollo, National Centre for Nuclear Research AND Jagiellonian University
16:40-17:00 (20min)
› The infrared emission of galaxies via machine learning techniques - Wouter Dobbels, Ghent University
17:00-17:20 (20min)
› Modelling the Structure of GAMA Galaxies with PROFIT - Amanda Moffett, Vanderbilt University
17:20-17:40 (20min)
› Spatially-Resolved Stellar Populations and Star-Formation Histories with Pixel Color-Magnitude Diagrams - Ben Cook, Harvard-Smithsonian Center for Astrophysics
17:40-18:00 (20min)
› Spatially-resolved Stellar Population Structure of Nearby Galaxies and Real-time Analysis of Multi-wavelength Pixel-SEDs - Chang Hee Ree, Korea Astronomy and Space Science Institute
18:00-18:20 (20min)
Pushing the technical frontier: from overwhelming large datasets to machine learning
Kentaro Nagamine
› Integration of Semi Analytic Model with SED Modelling Platforms - Dian Triani, Swinburne University of Technology
09:25-09:45 (20min)
› Variations of the stellar initial mass function in semi-analytical models: implications for the mass assembly of galaxies in the GAEA model. - Fabio Fontanot, Astronomical Observatory of Trieste
09:45-10:05 (20min)
› Dust extinction and emission properties in a cosmological simulation - Shohei Aoyama, ASIAA
10:05-10:25 (20min)
› Simulating Galaxy Spectra with the FIRE Simulations - Tova Yoast-Hull, Canadian Institute for Theoretical Astrophysics
10:25-10:45 (20min)
› Modeling the panchromatic emission of galaxies with CIGALE - Médéric Boquien, Universidad de Antofagasta
10:45-11:05 (20min)
Pushing the technical frontier: from overwhelming large datasets to machine learning
Fangting Yuan
› Advanced panchromatic spectral modelling and fitting with BAGPIPES - Adam Carnall, Royal Observatory Edinburgh
11:35-11:55 (20min)
› FortesFit: Flexible SED modelling with a Bayesian backbone - David Rosario, Department of Physics, Durham University
11:55-12:15 (20min)
› Going beyond Galaxy Ages with Dense Basis Star Formation History Reconstruction - Kartheik Iyer, Rutgers, The State University of New Jersey
12:15-12:35 (20min)
› A Dust Spectral Energy Distribution Model with Hierarchical Bayesian Inference and Its Application to the Nearby Universe - Frédéric Galliano, UMR Astrophysique, Instrumentation-Modelisation, à Paris-Saclay
12:35-12:55 (20min)
› Bayesian discrimination of the panchromatic spectral energy distribution modelings of galaxies - Yunkun Han, Yunnan Observatories, CAS
12:55-13:15 (20min)
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)
Pushing the redshift frontier: modeling the first galaxies
Fumi Egusa
› Pushing the redshift frontier with future ground-based and space-borne facilities - Toru Yamada, JAXA/ISAS
09:25-10:05 (40min)
› Census of Lya, [OIII]5007, Ha, and [CII]158um line emission with ~1000 galaxies at z=4.9-7.0 revealed with Subaru/HSC, Spitzer, and ALMA - Yuichi Harikane, The University of Tokyo
10:05-10:25 (20min)
› ALMA Detections of the Far-infrared [OIII] and Dust Emission in a Galaxy at z = 8.312: Early Metal Enrichment in the Heart of the Reionization Era - Yoichi Tamura, Nagoya University
10:25-10:45 (20min)
› Dust mass and dust production efficiency on the redshift frontier - Hiroyuki Hirashita, ASIAA
10:45-11:05 (20min)
Pushing the redshift frontier: modeling the first galaxies
Erik Zackrisson
› The onset of star formation 250 million years after the Big Bang - Takuya Hashimoto, Osaka Sangyo University/NAOJ
11:35-11:55 (20min)
› Modeling the sources of cosmic reionisation and low-z analogs - Daniel Schaerer, CNRS & Universite de Geneve
11:55-12:15 (20min)
› Extreme variations in star formation activity in the first galaxies - Christian Binggeli, Uppsala University
12:15-12:35 (20min)
› Improving Our View of the z>6 Universe with Dust Laws, Lensed Galaxies, and a Candidate Spatially Resolved Arc at z~10 - Brett Salmon, Space Telescope Science Institute
12:35-12:55 (20min)
› Hi-z SMGs, Hi-z LBGs and low-zZ galaxies - Denis Burgarella, Laboratoire d'Astrophysique de Marseille
12:55-13:15 (20min)
Pushing the redshift frontier: modeling the first galaxies
Viviana Acquaviva
› Subaru/HSC Identifications of Protocluster Candidates at z~6-7: Implications for Cosmic Reionization - Ryo Higuchi, The University of Tokyo, ICRR (Institute for Cosmic Ray Research)
14:30-14:50 (20min)
› Probing the ISM of HeII1640 emitters at z=2-4 via MUSE - Themiya Nanayakkara, Leiden Observatory
14:50-15:10 (20min)
› Panchromatic study of the first galaxies in cosmological simulations - Hidenobu Yajima, University of Tsukuba
15:10-15:30 (20min)
› FirstLight: Cosmological simulations of first galaxies from redshifts 5-15 - Daniel Ceverino, Heidelberg University
15:30-15:50 (20min)
› The distribution and physical properties of high-redshift [OIII] emitters in a cosmological hydrodynamics simulation - Kana Moriwaki, Department of Physics, The University of Tokyo
15:50-16:10 (20min)
Pushing the redshift frontier: modeling the first galaxies
Andrea Merloni
› Formation of the First Galaxies - Li-Hsin Chen, National Taiwan University, Academia Sinica Institute of Astronomy and Astrophysics (ASIAA)
16:40-17:00 (20min)
› How the First Supernovae Regulated Star Formation in the First Galaxies - Ke-Jung Chen, National Astronomical Observatory of Japan, Academia Sinica Institute of Astronomy and Astrophysics (ASIAA)
17:00-17:20 (20min)
