Program
Monday, November 12, 2018
| Time |
Event |
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08:30 - 09:25
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Registration open - Registration desk is open throughout the week. |
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09:25 - 09:45
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Welcoming remarks |
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09:45 - 11:05
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State-of-the-art panchromatic surveys and studies - Mederic Boquien |
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| 09:45 - 10:25 |
› A Historical Overview of Galaxy Surveys - Sadanori Okamura, Executive Management Program, University of Tokyo |
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| 10:25 - 11:05 |
› The physical ingredients for panchromatic modeling - Stephane Charlot, Institut d'Astrophysique de Paris / CNRS-Sorbonne Université |
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11:05 - 11:35
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Poster session and Break |
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11:35 - 13:15
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State-of-the-art panchromatic surveys and studies - Veronique Buat |
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| 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 |
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| 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 |
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| 12:15 - 12:35 |
› 18-band SED fitting in mid-infrared in the AKARI NEP field. - Tomotsugu Goto, National Tsing Hua University |
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| 12:35 - 12:55 |
› The averaged FIR SED of protoclusters at z=4 - Mariko Kubo, NAOJ |
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| 12:55 - 13:15 |
› The spectral energy distributions of active galactic nuclei - Michael Brown, Monash University |
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13:15 - 14:30
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Lunch |
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14:30 - 15:50
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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 |
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| 15:30 - 15:50 |
› A New Frontier of Globular Cluster Studies - Alexa Villaume, UC Santa Cruz |
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15:50 - 16:10
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Flash poster presentations #1 |
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16:10 - 16:40
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Poster session and Break |
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16:40 - 18:20
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State-of-the-art panchromatic surveys and studies - Agnieszka Pollo |
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| 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 |
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| 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 |
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| 17:40 - 18:00 |
› Modeling the emission of passive galaxies at z~3 - Chiara D'Eugenio, CEA Saclay, Université Paris Diderot, Irfu/SAp |
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| 18:00 - 18:20 |
› Evolution histories of massive galaxies at z~2 over the past 3Gyr - Takahiro Morishita, Space Telescope Science Institute |
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Tuesday, November 13, 2018
| Time |
Event |
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08:45 - 09:25
|
Registration open - Registration is open throughout the week |
|
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09:25 - 10:45
|
State-of-the-art panchromatic surveys and studies - Sadanori Okamura |
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| 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 |
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| 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 |
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| 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 |
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| 10:25 - 10:45 |
› High-resolution, 3D radiative transfer modeling of barred galaxies - Angelos Nersesian, Ghent University, IAASARS, National Observatory of Athens |
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10:45 - 11:05
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Flash poster presentations #2 |
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11:05 - 11:35
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Poster session and Break |
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11:35 - 12:55
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State-of-the-art panchromatic surveys and studies - Maud Galametz |
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| 11:35 - 11:55 |
› Which dust attenuation law(s) for star forming galaxies? - Veronique Buat, Laboratoire dÁstrophysique de Marseille |
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| 11:55 - 12:15 |
› Dust attenuation on and off the galaxy Main Sequence at z>1 - Annagrazia Puglisi, CEA-Saclay |
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| 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 |
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| 12:35 - 12:55 |
› A MUSE multi-wavelength analysis of the Abell 2667 BCG - Edoardo Iani, University of Padova |
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12:55 - 13:15
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IAU Commission J1 (SED of galaxies) Report |
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13:15 - 14:30
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Lunch |
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14:30 - 15:50
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Pushing the technical frontier: from overwhelming large datasets to machine learning - Katarzyna Malek |
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| 14:30 - 15:10 |
› Pushing the technical frontier from large datasets to machine learning - Viviana Acquaviva, New York City College of Technology |
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| 15:10 - 15:30 |
› Modeling with the Crowd: Optimizing the Human-Machine Partnership with Zooniverse - Hugh Dickinson, University of Minnesota - Twin Cities |
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| 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 |
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15:50 - 16:10
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Flash poster presentations #3 |
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16:10 - 16:40
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Poster session and Break |
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16:40 - 18:20
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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 |
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| 17:00 - 17:20 |
› The infrared emission of galaxies via machine learning techniques - Wouter Dobbels, Ghent University |
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| 17:20 - 17:40 |
› Modelling the Structure of GAMA Galaxies with PROFIT - Amanda Moffett, Vanderbilt University |
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| 17:40 - 18:00 |
› Spatially-Resolved Stellar Populations and Star-Formation Histories with Pixel Color-Magnitude Diagrams - Ben Cook, Harvard-Smithsonian Center for Astrophysics |
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| 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 |
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Wednesday, November 14, 2018
| Time |
Event |
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09:05 - 09:25
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Registration open - Registration desk is open throughout the week |
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09:25 - 11:05
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Pushing the technical frontier: from overwhelming large datasets to machine learning - Kentaro Nagamine |
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| 09:25 - 09:45 |
› Integration of Semi Analytic Model with SED Modelling Platforms - Dian Triani, Swinburne University of Technology |
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| 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 |
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| 10:05 - 10:25 |
› Dust extinction and emission properties in a cosmological simulation - Shohei Aoyama, ASIAA |
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| 10:25 - 10:45 |
› Simulating Galaxy Spectra with the FIRE Simulations - Tova Yoast-Hull, Canadian Institute for Theoretical Astrophysics |
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| 10:45 - 11:05 |
› Modeling the panchromatic emission of galaxies with CIGALE - Médéric Boquien, Universidad de Antofagasta |
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11:05 - 11:35
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Poster session and Break |
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11:35 - 13:15
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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 |
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| 11:55 - 12:15 |
› FortesFit: Flexible SED modelling with a Bayesian backbone - David Rosario, Department of Physics, Durham University |
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| 12:15 - 12:35 |
› Going beyond Galaxy Ages with Dense Basis Star Formation History Reconstruction - Kartheik Iyer, Rutgers, The State University of New Jersey |
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| 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 |
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| 12:55 - 13:15 |
› Bayesian discrimination of the panchromatic spectral energy distribution modelings of galaxies - Yunkun Han, Yunnan Observatories, CAS |
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13:15 - 18:00
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Free afternoon |
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19:00 - 21:00
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Banquet |
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Thursday, November 15, 2018
| Time |
Event |
|
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09:05 - 09:25
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Registration open - Registration desk is open throughout the week |
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09:25 - 11:05
|
Pushing the technical frontier: from overwhelming large datasets to machine learning - Denis Burgarella |
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| 09:25 - 09:45 |
› A new stellar population fitting algorithm based on chemical evolution models - Shiyin Shen, Shanghai Astronomical Observatory, Chinese Academy of Sciences |
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| 09:45 - 10:05 |
› A new galaxy spectral energy distribution model with the evolution of dust consistent with chemical evolution - Kazuki Nishida, Nagoya University |
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| 10:05 - 10:25 |
› AGN mocks for Euclid - Elisabeta Lusso, Durham University |
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| 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 |
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| 10:45 - 11:05 |
› Galaxy photometric and dynamical modelling in the era of all-sky multiwavelength surveys - Dan Taranu, Princeton University |
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11:05 - 11:35
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Poster session and Break |
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11:35 - 13:15
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Pushing the wavelength frontier: extending models towards X-rays and radio - Elisabeta Lusso |
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| 11:35 - 12:15 |
› eROSITA: Mapping the Hot Universe - Andrea Merloni, Max-Planck-Institut für Extraterrestrische Physik |
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| 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 |
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| 12:35 - 12:55 |
› Importance and tips learned from panchromatic modeling of AGNs - Y.Sophia Dai, National Astronomical Observatories |
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| 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 |
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13:15 - 14:30
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Lunch |
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14:30 - 15:50
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Pushing the wavelength frontier: extending models towards X-rays and radio - Tohru Nagao |
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| 14:30 - 15:10 |
› Modeling the Energetic Processes Powering Radio Continuum Emission from Galaxies - Eric Murphy, National Radio Astronomy Observatory |
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| 15:10 - 15:30 |
› Panchromatic characterisation of AGN and star-forming galaxies- From the radio to the X-rays - Gabriela Calistro-Rivera, Leiden Observatory |
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| 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 |
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15:50 - 16:10
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Poster award presentation |
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16:10 - 16:40
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Poster session and Break |
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16:40 - 18:20
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Pushing the redshift frontier: modeling the first galaxies - Hiroyuki Hirashita |
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| 16:40 - 17:20 |
› Modelling challenges in the rest-frame UV/optical at the high-redshift frontier - Erik Zackrisson, Uppsala University |
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| 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 |
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| 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 |
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Friday, November 16, 2018
| Time |
Event |
|
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09:05 - 09:25
|
Registration open - Registration desk is open throughout the week |
|
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09:25 - 11:05
|
Pushing the redshift frontier: modeling the first galaxies - Fumi Egusa |
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| 09:25 - 10:05 |
› Pushing the redshift frontier with future ground-based and space-borne facilities - Toru Yamada, JAXA/ISAS |
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| 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 |
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| 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 |
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| 10:45 - 11:05 |
› Dust mass and dust production efficiency on the redshift frontier - Hiroyuki Hirashita, ASIAA |
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11:05 - 11:35
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Break and poster viewing |
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11:35 - 13:15
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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 |
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| 11:55 - 12:15 |
› Modeling the sources of cosmic reionisation and low-z analogs - Daniel Schaerer, CNRS & Universite de Geneve |
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| 12:15 - 12:35 |
› Extreme variations in star formation activity in the first galaxies - Christian Binggeli, Uppsala University |
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| 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 |
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| 12:55 - 13:15 |
› Hi-z SMGs, Hi-z LBGs and low-zZ galaxies - Denis Burgarella, Laboratoire d'Astrophysique de Marseille |
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13:15 - 14:30
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Lunch |
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14:30 - 16:10
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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) |
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| 14:50 - 15:10 |
› Probing the ISM of HeII1640 emitters at z=2-4 via MUSE - Themiya Nanayakkara, Leiden Observatory |
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| 15:10 - 15:30 |
› Panchromatic study of the first galaxies in cosmological simulations - Hidenobu Yajima, University of Tsukuba |
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| 15:30 - 15:50 |
› FirstLight: Cosmological simulations of first galaxies from redshifts 5-15 - Daniel Ceverino, Heidelberg University |
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| 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 |
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16:10 - 16:40
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Poster session and Break |
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16:40 - 17:20
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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) |
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| 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) |
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17:20 - 18:00
|
Concluding remarks and discussion: the next steps |
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