John O'Meara | (Saint Michael's College) | The lifecycle of galaxies from inside, outside, and in between: the transformative potential of LUVOIR |
住貴宏 | (大阪大学) | WFIRST |
長峯健太郎 | (大阪大学) | 英語での議論の極意1 (日本語講演) |
竹内努 | (名古屋大学) | 英語での議論の極意2 (日本語講演) |
6/6 | (Wed) | ||||||
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13:00 | - | 13:10 | Logistics | ||||
Session: nearby galaxies (Chair: 田中) | |||||||
13:10 | - | 13:30 | 依田 萌 | 名古屋大学 | Statistical Study of Star Formation Law in Nearby Galaxies | [abst] | [slide] |
13:30 | - | 13:50 | Abdurro'uf | Tohoku University | Spatially resolved stellar mass buildup and quenching of massive disk galaxies at z ~ 0-1 | [abst] | [slide] |
13:50 | - | 14:10 | Taiki Kawamuro | NAOJ | Study of X-ray Irradiated ISM around Circinus Galaxy Nucleus with Chandra and ALMA | [abst] | [slide] |
Session: posters | |||||||
14:10 | - | 14:50 | Poster session with machine-gun talks | ||||
14:50 | - | 15:20 | Break | ||||
Featured Session: LUVOIR (Chair: 長峯) | |||||||
15:20 | - | 16:20 | John O'Meara | Saint Michael's College | The lifecycle of galaxies from inside, outside, and in between: the transformative potential of LUVOIR | [abst] | [slide] |
16:20 | - | 16:50 | 住 貴宏 | 大阪大学 | WFIRST | [abst] | [slide] |
16:50 | - | 17:10 | 久保 真理子 | NAOJ | The rest-frame optical sizes of massive galaxies with suppressed star formation at z~4 | [abst] | [slide] |
17:10 | - | 17:30 | 菊地原 正太郎 | 東京大学 | RELICS: Identifying Strongly Lensed High-redshift Galaxies for JWST | [abst] | [slide] |
6/7 | (Thu) | ||||||
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Session: nearby galaxies 2 (Chair: 大西) | |||||||
09:00 | - | 09:20 | 矢島 義之 | 北海道大学 | Physical Properties of Molecular Gas in Nearby Barred Spiral Galaxies | [abst] | [slide] |
09:20 | - | 09:40 | 前田 郁弥 | 京都大学 | Molecular gas and star formation in bar regions of strongly barred galaxies | [abst] | [slide] |
09:40 | - | 10:00 | Sakurako Okamoto | NAOJ | M81 galaxy archaeology with HSC | [abst] | [slide] |
10:00 | - | 10:20 | Tadafumi Matsuno | Sokendai / NAOJ | What can be learned from Gaia DR2 and the database of metal-poor stars | [abst] | [slide] |
10:20 | - | 10:50 | Break | ||||
Session: physical processes in galaxies (Chair: 太田) | |||||||
10:50 | - | 11:10 | 藤井 通子 | 東京大学 | Modeling the Milky Way using N-body | [abst] | [slide] |
11:10 | - | 11:30 | Shigeki Inoue | Univ. of Tokyo (Kavli IPMU) | Spiral-arm instability: destabilization by magnetic fields | [abst] | [slide] |
11:30 | - | 11:50 | Kohei Hayashi | Univ. of Tokyo (ICRR) | The universal dark halo scaling relation for the dwarf satellites | [abst] | [slide] |
11:50 | - | 13:40 | Lunch break+Conference photo | ||||
Featured Session: 英語での議論の極意 (This is a Japanese session) | |||||||
13:40 | - | 14:10 | 長峯 健太郎 | 大阪大学 | 「英語での議論の極意」1 | [abst] | [slide] |
14:10 | - | 14:40 | 竹内 努 | 名古屋大学 | 「英語での議論の極意」2 | [abst] | [slide] |
14:40 | - | 15:00 | Discussion | ||||
15:00 | - | 15:30 | Break | ||||
Session: dusty galaxies (Chair: 柏川) | |||||||
15:30 | - | 15:50 | 青山 尚平 | ASIAA | Dust properties from cosmological simulation | [abst] | [slide] |
15:50 | - | 16:10 | 鳥羽 儀樹 | 京都大学 / ASIAA | Discovery of an Extremely Luminous Dust-obscured Galaxy Observed with SDSS, WISE, JCMT, and SMA | [abst] | [slide] |
16:10 | - | 16:30 | Xiaoyang Chen | Tohoku University | Extreme Outflow in an AKARI-selected ULIRG at z=0.5 | [abst] | [slide] |
16:30 | - | 16:50 | Yuki Yamaguchi | Univ. of Tokyo (IoA) | ALMA 26 arcmin^2 survey of GOODS-S at 1 mm: Physical properties of ALMA-selected galaxies | [abst] | [slide] |
16:50 | - | 18:00 | Margin | ||||
18:00 | - | Banquet |
6/8 | (Fri) | ||||||
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Session: active galaxies (Chair: 鍛冶澤) | |||||||
09:00 | - | 09:20 | Kohei Ichikawa | Tohoku University / Columbia University | Looking at drastic AGN luminosity decline in Arp 187 within 10^4 years | [abst] | [slide] |
09:20 | - | 09:40 | 泉 拓磨 | NAOJ | The circumnuclear *multi-phase* torus in the Circinus galaxy revealed by ALMA | [abst] | [slide] |
09:40 | - | 10:00 | Hikari SHIRAKATA | Hokkaido University | Properties of AGNs predicted from a semi-analytic model of galaxy formation | [abst] | [slide] |
10:00 | - | 10:20 | Break | ||||
Session: from the cosmic noon to the present (Chair: 秋山) | |||||||
10:20 | - | 10:40 | 小山 舜平 | 愛媛大学 | Do galaxy morphologies really affect the efficiency of star formation during the phase of galaxy transition? | [abst] | [slide] |
10:40 | - | 11:00 | 鈴木 智子 | 東北大学 / 国立天文台 | Clumpy galaxy fractions in different environments at z~2 | [abst] | [slide] |
11:00 | - | 11:20 | 満田 和真 | 東北大学 | Evolution of Kinematic Properties of Early-Type Galaxies Investigated by Surface Photometry | [abst] | [slide] |
11:20 | - | 11:40 | 柏野 大地 | ETH Zurich | Disentangle the physical parameters for gaseous nebulae and galaxies | [abst] | [slide] |
11:40 | - | 12:00 | 矢部 清人 | 東京大学 (Kavli IPMU) | Search for extremely strong emission line galaxies at z < 1 using Subaru/HSC | [abst] | [slide] |
12:00 | - | 13:00 | Lunch break | ||||
Session: high-z galaxies (Chair: 竹内) | |||||||
13:00 | - | 13:20 | 播金 優一 | 東京大学 (ICRR) | Census of Lya, [OIII]5007, Ha, and [CII]158um Line Emission with ~1000 LAEs at z=4.9-7.0 Revealed with Subaru/HSC | [abst] | [slide] |
13:20 | - | 13:40 | 中島 王彦 | 国立天文台 | A Hard Ionising Spectrum in z=3-4 Lyman Alpha Emitters | [abst] | [slide] |
13:40 | - | 14:00 | 鹿熊 亮太 | 東京大学(ICRR) | Cross-Correlating Lyα Intensity Mapping with z=5.7 and 6.6 LAEs: Investigating Diffuse Lyα Emission in the Extremely Large Scale at ~20-300 kpc | [abst] | [slide] |
14:00 | - | 14:20 | Break | ||||
Session: high-z galaxies 2 (Chair: 矢部) | |||||||
14:20 | - | 14:40 | 吉村 勇紀 | 東京大学 (IoA) | ASAGAO: Clustering of faint SMGs | [abst] | [slide] |
14:40 | - | 15:00 | 藤本 征史 | 東京大学 | z=5-7における[CII]ガスハローの発見 | [abst] | [slide] |
15:00 | - | 15:20 | Final discussion and summary |
Poster | |||||
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P1 | 大西 響子 | 愛媛大学 | Molecular holes in the centres of nearby galaxies | [abst] | [slide] |
P2 | 向江 志朗 | 東京大学 | Testing the physical origins of an Enormous Lyα Nebula at z = 2.3 by bright background galaxies | [abst] | [slide] |
P3 | 樋本 一晴 | 愛媛大学 | Quantitative morphological classification for galaxies with bursty star formation at z=0.7-0.9 in COSMOS | [abst] | [slide] |
P4 | 吉田 俊太郎 | 名古屋大学 | Extension and Unification of the Scaling Laws in Galaxies | [abst] | [slide] |
P5 | 安藤 誠 | 東京大学 | X-ray study of gas stripping from a infalling galaxy group towards the Virgo cluster | [abst] | [slide] |
P6 | 樋口 諒 | 東京大学 | すばるHSCを用いた原始銀河団の探査 | [abst] | [slide] |
P7 | 長崎 早也香 | 名古屋大学 | Relation between the dust evolution and star formation timescale in galaxies | [abst] | [slide] |
P8 | 檀林 健太 | 関西学院大学 | Integrated galaxy spectra as a reference to investigate the origin of the cosmic optical background | [abst] | [slide] |
P9 | 西田 和樹 | 名古屋大学 | Construction of a galaxy SED model including dust evolution | [abst] | [slide] |
P10 | 河野 海 | 名古屋大学 | VLA-COSMOS観測を用いたz<5.5での電波光度進化モデルと銀河計数への制限 | [abst] | [slide] |
P11 | 大森 清顕 クリストファ | 名古屋大学 | Investigating the properties of local interacting galaxies | [abst] | [slide] |
P12 | 木村 大希 | 東北大学 | star formation galaxies in the fields at z=2~3 | [abst] | [slide] |
P13 | 高橋 さくら | お茶の水女子大学 | ボースアインシュタイン凝縮体による超大質量ブラックホールの形成 | [abst] | [slide] |
P15 | 大金 原 / 大本 薫 | 東北大学 | 銀河構造の進化に迫るすばる望遠鏡トモグラフィー補償光学 | [abst] | [slide] |
P16 | 古谷 庸介 | 山口大学 | The estimation for types of high-z quasars observed by Japanese VLBI Network | [abst] | [slide] |
P17 | Suchetha Cooray | Nagoya University | An Iterative Data Reconstruction Method for Incomplete Measurements in All-Sky Surveys | [abst] | [slide] |
P18 | Shgieru Namiki | SOKENDAI | The environmental impacts on the Mass-Metallicity relation at z=1.52 | [abst] | [slide] |
P19 | 伊藤 慧 | 総研大 | HSC 広視野撮像観測による z ∼ 4 Brightest Cluster Galaxy候補 の検出 | [abst] | [slide] |
P20 | Liang, Yongming | NAOJ / SOKENDAI | Search for the most massive over-densities at z~2.2 with Subaru HSC | [abst] | [slide] |
P21 | Miftahul Hilmi | ICRR, the University of Tokyo | Ionizing Photon Production Efficiency of LBGs at z = 3.8 — 5.0: Implications for Cosmic Reionization | [abst] | [slide] |
P22 | Haibin Zhang | University of Tokyo | Discovery of Two Giant LAEs at z=4.9 and 7.0 | [abst] | [slide] |
P23 | 李 建鋒 | 東京大学(IoA) | Line emitter search with ALMA 3mm data | [abst] | [slide] |
P24 | 菊田 智史 | 総研大/国立天文台 | Lyman alpha imaging around a hyperluminous QSO at z=2.84 with HSC | [abst] | [slide] |
P26 | 大木 平 | 東京大学(Kavli IPMU) | An empirical model for the spatial distribution of cluster galaxies | [abst] | [slide] |
P27 | Nao Fukagawa | GUAS/SOKENDAI | Gas inflow and outflow of star forming galaxies at redshift 1.4 as traced by chemical evolution | [abst] | [slide] |
P28 | 石田 剛 | 東京大学 | Spatially resolved [CII] outflow in a lensed submillimeter galaxy, SDP.81 | [abst] | [slide] |
P29 | 道山 知成 | 総研大 | ALMA OBSERVATIONS OF HCN AND HCO+ OUTFLOWS IN THE MERGING GALAXY NGC 3256 | [abst] | [slide] |
P30 | 藤本 征史 | 東京大学 | ALMA 26 ARCMIN^2 SURVEY OF GOODS-S AT ONE-MILLIMETER (ASAGAO): AVERAGE MORPHOLOGY OF HIGH-z DUSTY STAR-FORMING GALAXIES IS AN EXPONENTIAL-DISK (n ~ 1) | [abst] | [slide] |
P31 | Tao Wang | University of Tokyo | ALMA reveals massive, HST-dark galaxies at high redshifts | [abst] | [slide] |
P32 | Trani Alessandro | University of Tokyo | Forming circumnuclear disks and rings in galactic nuclei: a competition between supermassive black hole and nuclear star cluster | [abst] | [slide] |
P33 | 小島崇史 | 東京大学 | Extremely Metal-poor Emission-line Galaxy Survey with Subaru/HSC | [abst] | [slide] |
P34 | Takuji Yamashita | Ehime University | Optically-faint radio galaxies found by Subaru HSC-SSP and FIRST catalogs | [abst] | [slide] |
P35 | 佐藤 佑樹 | 愛媛大学 | The evolution of axial ratio of passive and star-forming galaxies at z < 1 (2nd) | [abst] | [slide] |
P36 | Yuya Saeda | Ehime University | Stacking analysis of quasar host galaxies at z > 1 with Hyper Suprime-Cam | [abst] | [slide] |
P37 | Ishino Toru | Ehime University | Properties of quasar host galaxies at z < 1 revealed by Subaru HSC | [abst] | [slide] |
P38 | Nanako Kato | Ehime University | Broad-band analysis of the rest-frame optical SED of high-z quasars | [abst] | [slide] |
P39 | 寺尾 航暉 | 愛媛大学 | Physical and chemical properties of narrow-line regions in z~3 radio galaxies | [abst] | [slide] |
P40 | 登口 暁 | 愛媛大学 | Optical properties of infrared-bright dust-obscured galaxies viewed with Subaru Hyper Suprime-Cam | [abst] | [slide] |
P41 | 馬場俊介 | ISAS, JAXA | AGN-starburst connection suggested by the 4.7 micron CO absorption band | [abst] | [slide] |
P42 | 菅原悠馬 | 東京大学 宇宙線研究所 | The Outflow-Galaxy relations studied with ~100,000 SDSS spectra | [abst] | [slide] |