We closed the Q&A page on 31 Jan.2023.
We closed the poster session page on 31 Jan. 2023.
Link to the poster session
|1||CO(J=1-0) mapping survey of 64 galaxies in the Fornax cluster with the ALMA Morita array||Kana Morokuma (The University of Tokyo)|
|2||Nobeyama 45-m CO J=1-0 observations of type 1 AGNs at z ∼ 0.3||Tomonari Michiyama (Osaka University / NAOJ)|
|3||Relationship between SFE and physical state of molecular gas in NGC 3627||Kazuki Shibata (University of Tsukuba)|
|4||Quantitative and statistical analysis of the molecular gas morphology in the nearby star-forming galaxies||Takashi Yamamoto (University of Tsukuba)|
|5||Giant molecular clouds and their Type classifications in M74||Fumika Demachi (Nagoya university)|
|6||ALMA Super-resolution Imaging of Star- and Planet-forming Regions Using Sparse Modeling||Ayumu Shoshi (Kyushu University)|
|7||Cluster formation by fragmentations of 1000 AU-scale filaments in Corona Australis||Naofumi Fukaya (Nagoya University)|
|8||30-34 GHz Line Survey toward the Starless Core Serpens South with the eQ Receiver||Kotomi Taniguchi (NAOJ)|
|9||CI and CO gas properties studied with ASTE Band 10 SV data||Kengo Tachihara (Nagoya University)|
|10||Using ALMA to observe C and CO gas in debris disks||Gianni Cataldi (NAOJ / The University of Tokyo)|
|11||Launch and management of an astronomy laboratory at Tokyo Denki University||Aya Higuchi (Tokyo Denki University)|
|12||FINER: Far-Infrared Nebular Emission Receiver for LMT based on the ALMA 2 receiver technology||Yoichi Tamura (Nagoya University)|
|13||Design method of a broadband planar magic-T: a 6-14GHz scaled model for mm/submm camera||Shuhei Inoue (The University of Tokyo)|