Monday, November 12, 2018

Time Event  
08:30 - 09:25 Registration open - Registration desk is open throughout the week.  
09:25 - 09:45 Welcoming remarks  
09:45 - 11:05 State-of-the-art panchromatic surveys and studies - Mederic Boquien  
09:45 - 10:25 › A Historical Overview of Galaxy Surveys - Sadanori Okamura, Executive Management Program, University of Tokyo  
10:25 - 11:05 › The physical ingredients for panchromatic modeling - Stephane Charlot, Institut d'Astrophysique de Paris / CNRS-Sorbonne Université  
11:05 - 11:35 Poster session and Break  
11:35 - 13:15 State-of-the-art panchromatic surveys and studies - Veronique Buat  
11:35 - 11:55 › ALPINE: The large ALMA Program to Study the Interstellar Medium of High Redshift Galaxies - Andreas Faisst, Infrared Processing and Analysis Center  
11:55 - 12:15 › ALMA unveils a large population of massive galaxies at z>3 that are hidden from HST - Tao Wang, University of Tokyo  
12:15 - 12:35 › 18-band SED fitting in mid-infrared in the AKARI NEP field. - Tomotsugu Goto, National Tsing Hua University  
12:35 - 12:55 › The averaged FIR SED of protoclusters at z=4 - Mariko Kubo, NAOJ  
12:55 - 13:15 › The spectral energy distributions of active galactic nuclei - Michael Brown, Monash University  
13:15 - 14:30 Lunch  
14:30 - 15:50 State-of-the-art panchromatic surveys and studies - Stephane Charlot  
14:30 - 15:10 › Panchromatic codes and modeling techniques - Maarten Baes, Universiteit Gent  
15:10 - 15:30 › Population Synthesis models with binary stars - Fenghui Zhang, Yunnan Observatories, Chinese Academy of Sciences  
15:30 - 15:50 › A New Frontier of Globular Cluster Studies - Alexa Villaume, UC Santa Cruz  
15:50 - 16:10 Flash poster presentations #1  
16:10 - 16:40 Poster session and Break  
16:40 - 18:20 State-of-the-art panchromatic surveys and studies - Agnieszka Pollo  
16:40 - 17:00 › A revised picture of galaxy stellar mass assembly from panchromatic SED fitting of the 3D-HST survey - Joel Leja, Harvard- Smithsonian Center for Astrophysics  
17:00 - 17:20 › 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  
17:20 - 17:40 › Are SMGs on the Main Sequence of galaxies? - Laia Barrufet, ESAC / RAL Space  
17:40 - 18:00 › Modeling the emission of passive galaxies at z~3 - Chiara D'Eugenio, CEA Saclay, Université Paris Diderot, Irfu/SAp  
18:00 - 18:20 › Evolution histories of massive galaxies at z~2 over the past 3Gyr - Takahiro Morishita, Space Telescope Science Institute  

Tuesday, November 13, 2018

Time Event  
08:45 - 09:25 Registration open - Registration is open throughout the week  
09:25 - 10:45 State-of-the-art panchromatic surveys and studies - Sadanori Okamura  
09:25 - 09:45 › 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  
09:45 - 10:05 › Probing star formation quenching in galaxies with resolved optical and radio data - Lihwai Lin, Academia Sinica Institute of Astronomy and Astrophysics  
10:05 - 10:25 › Exploring the Star Formation Histories of Galaxies in Different Environments from MaNGA Spectra - Maria Argudo Fernandez, Center of Astronomy of the University of Antofagasta  
10:25 - 10:45 › High-resolution, 3D radiative transfer modeling of barred galaxies - Angelos Nersesian, Ghent University, IAASARS, National Observatory of Athens  
10:45 - 11:05 Flash poster presentations #2  
11:05 - 11:35 Poster session and Break  
11:35 - 12:55 State-of-the-art panchromatic surveys and studies - Maud Galametz  
11:35 - 11:55 › Which dust attenuation law(s) for star forming galaxies? - Veronique Buat, Laboratoire dÁstrophysique de Marseille  
11:55 - 12:15 › Dust attenuation on and off the galaxy Main Sequence at z>1 - Annagrazia Puglisi, CEA-Saclay  
12:15 - 12:35 › Spatially resolved dust-to-gas mass ratio in nearby galaxies - Basilio Solis-Castillo, Max Planck Institute for Radio Astronomy, University of Bonn  
12:35 - 12:55 › A MUSE multi-wavelength analysis of the Abell 2667 BCG - Edoardo Iani, University of Padova  
12:55 - 13:15 IAU Commission J1 (SED of galaxies) Report  
13:15 - 14:30 Lunch  
14:30 - 15:50 Pushing the technical frontier: from overwhelming large datasets to machine learning - Katarzyna Malek  
14:30 - 15:10 › Pushing the technical frontier from large datasets to machine learning - Viviana Acquaviva, New York City College of Technology  
15:10 - 15:30 › Modeling with the Crowd: Optimizing the Human-Machine Partnership with Zooniverse - Hugh Dickinson, University of Minnesota - Twin Cities  
15:30 - 15:50 › Deep Learning for Galaxy Mergers in the Galaxy Main Sequence - William Pearson, Kapteyn Astronomical Institute, SRON Netherlands Institute for Space Research  
15:50 - 16:10 Flash poster presentations #3  
16:10 - 16:40 Poster session and Break  
16:40 - 18:20 Pushing the technical frontier: from overwhelming large datasets to machine learning - Maarten Baes  
16:40 - 17:00 › Automatic classification of sources in large astronomical catalogues - Agnieszka Pollo, National Centre for Nuclear Research AND Jagiellonian University  
17:00 - 17:20 › The infrared emission of galaxies via machine learning techniques - Wouter Dobbels, Ghent University  
17:20 - 17:40 › Modelling the Structure of GAMA Galaxies with PROFIT - Amanda Moffett, Vanderbilt University  
17:40 - 18:00 › Spatially-Resolved Stellar Populations and Star-Formation Histories with Pixel Color-Magnitude Diagrams - Ben Cook, Harvard-Smithsonian Center for Astrophysics  
18:00 - 18:20 › 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  

Wednesday, November 14, 2018

Time Event  
09:05 - 09:25 Registration open - Registration desk is open throughout the week  
09:25 - 11:05 Pushing the technical frontier: from overwhelming large datasets to machine learning - Kentaro Nagamine  
09:25 - 09:45 › Integration of Semi Analytic Model with SED Modelling Platforms - Dian Triani, Swinburne University of Technology  
09:45 - 10:05 › 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  
10:05 - 10:25 › Dust extinction and emission properties in a cosmological simulation - Shohei Aoyama, ASIAA  
10:25 - 10:45 › Simulating Galaxy Spectra with the FIRE Simulations - Tova Yoast-Hull, Canadian Institute for Theoretical Astrophysics  
10:45 - 11:05 › Modeling the panchromatic emission of galaxies with CIGALE - Médéric Boquien, Universidad de Antofagasta  
11:05 - 11:35 Poster session and Break  
11:35 - 13:15 Pushing the technical frontier: from overwhelming large datasets to machine learning - Fangting Yuan  
11:35 - 11:55 › Advanced panchromatic spectral modelling and fitting with BAGPIPES - Adam Carnall, Royal Observatory Edinburgh  
11:55 - 12:15 › FortesFit: Flexible SED modelling with a Bayesian backbone - David Rosario, Department of Physics, Durham University  
12:15 - 12:35 › Going beyond Galaxy Ages with Dense Basis Star Formation History Reconstruction - Kartheik Iyer, Rutgers, The State University of New Jersey  
12:35 - 12:55 › 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  
12:55 - 13:15 › Bayesian discrimination of the panchromatic spectral energy distribution modelings of galaxies - Yunkun Han, Yunnan Observatories, CAS  
13:15 - 18:00 Free afternoon  
19:00 - 21:00 Banquet  

Thursday, November 15, 2018

Time Event  
09:05 - 09:25 Registration open - Registration desk is open throughout the week  
09:25 - 11:05 Pushing the technical frontier: from overwhelming large datasets to machine learning - Denis Burgarella  
09:25 - 09:45 › A new stellar population fitting algorithm based on chemical evolution models - Shiyin Shen, Shanghai Astronomical Observatory, Chinese Academy of Sciences  
09:45 - 10:05 › A new galaxy spectral energy distribution model with the evolution of dust consistent with chemical evolution - Kazuki Nishida, Nagoya University  
10:05 - 10:25 › AGN mocks for Euclid - Elisabeta Lusso, Durham University  
10:25 - 10:45 › 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  
10:45 - 11:05 › Galaxy photometric and dynamical modelling in the era of all-sky multiwavelength surveys - Dan Taranu, Princeton University  
11:05 - 11:35 Poster session and Break  
11:35 - 13:15 Pushing the wavelength frontier: extending models towards X-rays and radio - Elisabeta Lusso  
11:35 - 12:15 › eROSITA: Mapping the Hot Universe - Andrea Merloni, Max-Planck-Institut für Extraterrestrische Physik  
12:15 - 12:35 › 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  
12:35 - 12:55 › Importance and tips learned from panchromatic modeling of AGNs - Y.Sophia Dai, National Astronomical Observatories  
12:55 - 13:15 › 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  
13:15 - 14:30 Lunch  
14:30 - 15:50 Pushing the wavelength frontier: extending models towards X-rays and radio - Tohru Nagao  
14:30 - 15:10 › Modeling the Energetic Processes Powering Radio Continuum Emission from Galaxies - Eric Murphy, National Radio Astronomy Observatory  
15:10 - 15:30 › Panchromatic characterisation of AGN and star-forming galaxies- From the radio to the X-rays - Gabriela Calistro-Rivera, Leiden Observatory  
15:30 - 15:50 › Characterization of dusty galaxies uncovered by ALMA 26 arcmin^2 survey of GOODS-S at one-millimeter (ASAGAO) - Kotaro Kohno, The University of Tokyo  
15:50 - 16:10 Poster award presentation  
16:10 - 16:40 Poster session and Break  
16:40 - 18:20 Pushing the redshift frontier: modeling the first galaxies - Hiroyuki Hirashita  
16:40 - 17:20 › Modelling challenges in the rest-frame UV/optical at the high-redshift frontier - Erik Zackrisson, Uppsala University  
17:20 - 17:40 › Systematic errors in high-redshift dust mass fits: the role of dust opacity - Lapo Fanciullo, Academia Sinica, Institute of Astronomy and Astrophysics  
17:40 - 18:00 › 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  
18:00 - 18:20 › Modeling the dust content and dust-absorbed SED of galaxies in the early Universe - Gergö Popping, MPIA  

Friday, November 16, 2018

Time Event  
09:05 - 09:25 Registration open - Registration desk is open throughout the week  
09:25 - 11:05 Pushing the redshift frontier: modeling the first galaxies - Fumi Egusa  
09:25 - 10:05 › Pushing the redshift frontier with future ground-based and space-borne facilities - Toru Yamada, JAXA/ISAS  
10:05 - 10:25 › 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  
10:25 - 10:45 › 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  
10:45 - 11:05 › Dust mass and dust production efficiency on the redshift frontier - Hiroyuki Hirashita, ASIAA  
11:05 - 11:35 Break and poster viewing  
11:35 - 13:15 Pushing the redshift frontier: modeling the first galaxies - Erik Zackrisson  
11:35 - 11:55 › The onset of star formation 250 million years after the Big Bang - Takuya Hashimoto, Osaka Sangyo University/NAOJ  
11:55 - 12:15 › Modeling the sources of cosmic reionisation and low-z analogs - Daniel Schaerer, CNRS & Universite de Geneve  
12:15 - 12:35 › Extreme variations in star formation activity in the first galaxies - Christian Binggeli, Uppsala University  
12:35 - 12:55 › 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  
12:55 - 13:15 › Hi-z SMGs, Hi-z LBGs and low-zZ galaxies - Denis Burgarella, Laboratoire d'Astrophysique de Marseille  
13:15 - 14:30 Lunch  
14:30 - 16:10 Pushing the redshift frontier: modeling the first galaxies - Viviana Acquaviva  
14:30 - 14:50 › 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)  
14:50 - 15:10 › Probing the ISM of HeII1640 emitters at z=2-4 via MUSE - Themiya Nanayakkara, Leiden Observatory  
15:10 - 15:30 › Panchromatic study of the first galaxies in cosmological simulations - Hidenobu Yajima, University of Tsukuba  
15:30 - 15:50 › FirstLight: Cosmological simulations of first galaxies from redshifts 5-15 - Daniel Ceverino, Heidelberg University  
15:50 - 16:10 › The distribution and physical properties of high-redshift [OIII] emitters in a cosmological hydrodynamics simulation - Kana Moriwaki, Department of Physics, The University of Tokyo  
16:10 - 16:40 Poster session and Break  
16:40 - 17:20 Pushing the redshift frontier: modeling the first galaxies - Andrea Merloni  
16:40 - 17:00 › Formation of the First Galaxies - Li-Hsin Chen, National Taiwan University, Academia Sinica Institute of Astronomy and Astrophysics (ASIAA)  
17:00 - 17:20 › 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)  
17:20 - 18:00 Concluding remarks and discussion: the next steps