Challenges in Panchromatic Modelling with Next Generation Facilities

Mon. 12

Tue. 13

Wed. 14

Thu. 15

Fri. 16

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09:00

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21:00

Registration open

8:30 - 9:25 (55min)

Registration open

Registration desk is open throughout the week.

Welcoming remarks

9:25 - 9:45 (20min)

Welcoming remarks

State-of-the-art panchromatic surveys and studies

9:45 - 11:05 (1h20)

State-of-the-art panchromatic surveys and studies

Mederic Boquien

› 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)

Poster session and Break

11:05 - 11:35 (30min)

Poster session and Break

State-of-the-art panchromatic surveys and studies

11:35 - 13:15 (1h40)

State-of-the-art panchromatic surveys and studies

Veronique Buat

› 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)

Lunch

13:15 - 14:30 (1h15)

Lunch

State-of-the-art panchromatic surveys and studies

14:30 - 15:50 (1h20)

State-of-the-art panchromatic surveys and studies

Stephane Charlot

› Panchromatic codes and modeling techniques - Maarten Baes, Universiteit Gent 14:30-15:10 (40min)

› Population Synthesis models with binary stars - Fenghui Zhang, Yunnan Observatories, Chinese Academy of Sciences 15:10-15:30 (20min)

› A New Frontier of Globular Cluster Studies - Alexa Villaume, UC Santa Cruz 15:30-15:50 (20min)

Flash poster presentations #1

15:50 - 16:10 (20min)

Flash poster presentations #1

Poster session and Break

16:10 - 16:40 (30min)

Poster session and Break

State-of-the-art panchromatic surveys and studies

16:40 - 18:20 (1h40)

State-of-the-art panchromatic surveys and studies

Agnieszka Pollo

› 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)

Registration open

8:45 - 9:25 (40min)

Registration open

Registration is open throughout the week

State-of-the-art panchromatic surveys and studies

9:25 - 10:45 (1h20)

State-of-the-art panchromatic surveys and studies

Sadanori Okamura

› 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)

Flash poster presentations #2

10:45 - 11:05 (20min)

Flash poster presentations #2

Poster session and Break

11:05 - 11:35 (30min)

Poster session and Break

State-of-the-art panchromatic surveys and studies

11:35 - 12:55 (1h20)

State-of-the-art panchromatic surveys and studies

Maud Galametz

› 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)

IAU Commission J1 (SED of galaxies) Report

12:55 - 13:15 (20min)

IAU Commission J1 (SED of galaxies) Report

Lunch

13:15 - 14:30 (1h15)

Lunch

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

14:30 - 15:50 (1h20)

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)

Flash poster presentations #3

15:50 - 16:10 (20min)

Flash poster presentations #3

Poster session and Break

16:10 - 16:40 (30min)

Poster session and Break

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

16:40 - 18:20 (1h40)

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)

Registration open

9:05 - 9:25 (20min)

Registration open

Registration desk is open throughout the week

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

9:25 - 11:05 (1h40)

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)

Poster session and Break

11:05 - 11:35 (30min)

Poster session and Break

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

11:35 - 13:15 (1h40)

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)

Free afternoon

13:15 - 18:00 (4h45)

Free afternoon

Banquet

19:00 - 21:00 (2h)

Banquet

Registration open

9:05 - 9:25 (20min)

Registration open

Registration desk is open throughout the week

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

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)

Poster session and Break

11:05 - 11:35 (30min)

Poster session and Break

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

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)

Lunch

13:15 - 14:30 (1h15)

Lunch

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

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)

Poster award presentation

15:50 - 16:10 (20min)

Poster award presentation

Poster session and Break

16:10 - 16:40 (30min)

Poster session and Break

Pushing the redshift frontier: modeling the first galaxies

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)

Registration open

9:05 - 9:25 (20min)

Registration open

Registration desk is open throughout the week

Pushing the redshift frontier: modeling the first galaxies

9:25 - 11:05 (1h40)

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)

Break and poster viewing

11:05 - 11:35 (30min)

Break and poster viewing

Pushing the redshift frontier: modeling the first galaxies

11:35 - 13:15 (1h40)

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)

Lunch

13:15 - 14:30 (1h15)

Lunch

Pushing the redshift frontier: modeling the first galaxies

14:30 - 16:10 (1h40)

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)

Poster session and Break

16:10 - 16:40 (30min)

Poster session and Break

Pushing the redshift frontier: modeling the first galaxies

16:40 - 17:20 (40min)

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)

Concluding remarks and discussion: the next steps

17:20 - 18:00 (40min)

Concluding remarks and discussion: the next steps