2020年3月17日(火)午前(09:30-11:30) [A会場] |
09:30 | | Introduction and Scope of this Session
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09:36 | Z101r | Galaxy formation and evolution seen by ALMA and Subaru UMEHATA, Hideki(RIKEN) |
10:06 | Z102a | Numerical simulations of multi–wavelength radiative properties of galaxies in the epoch of reionization 荒田翔平(大阪大学) |
10:18 | Z103a | Molecular gas reservoirs of cluster galaxies at cosmic noon 林将央(国立天文台) |
10:30 | Z104a | New insights into the environmental dependence of massive galaxy formation from a panchromatic view of the first galaxy clusters WANG, Tao(The University of Tokyo/NAOJ) |
10:42 | Z105a | ALMA lensing cluster survey (ALCS) and follow-up observations using SUBARU KOHNO, Kotaro(The University of Tokyo) |
10:54 | Z106a | ALMA Reveals the Internal Structure in a z $\sim $ 3 Submillimeter Galaxy 小山紗桜(新潟大学) |
11:06 | Z107a | The low dust content of massive, quiescent galaxies at $z\sim 2$ Masayuki Tanaka(NAOJ) |
11:18 | Z108a | Star-formation rates of two GRB host galaxies at $z\sim 2$ and a [C II] deficit observed with ALMA Tetsuya Hashimoto(National Tsing Hua University) |
2020年3月17日(火)午後(13:00-15:00) [A会場] |
13:00 | Z109a | Detection of a CO emission line counterpart of a $z=3.3$ damped Ly$\alpha $ system 井上昭雄(早稲田大学) |
13:12 | Z110a | Rapid co-evolution into quiescence? Subaru + ALMA view on $z > 6$ low-luminosity quasars Takuma Izumi(NAOJ) |
13:24 | Z111r | The Evolving Landscape In and Around the Field of Nearby Galaxy Studies 幸田仁(Stony Brook University) |
13:54 | Z112a | Connecting molecules with the others in cosmological simulations 井上茂樹(筑波大学 / 国立天文台) |
14:06 | Z113a | Star-formation and molecular cloud properties in a low metallicity environment: Subaru/HSC-ALMA-ASTE observations of NGC 6822 TOSAKI, Tomoka(Joetsu University of Education) |
14:18 | Z114a | ALMA CO Observations of a Giant Molecular Cloud in M33: Evidence for High-Mass Star Formation Triggered by Cloud-Cloud Collisions Hidetoshi Sano(Nagoya University) |
14:30 | Z115a | Multiphase properties of ISM in a nearby radio galaxy, NGC 1316 Kana Morokuma(The University of Tokyo) |
14:42 | | Summary
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