› 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)