Program

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Program

Day1 | 3 Mar 2021 (Wed)

9:00-10:45	Business Session 09:00 - 09:30 [o01] Director’s report Michitoshi Yoshida 09:30 - 09:40 [o02] FY2020 Subaru Science Operation Report Tae-Soo Pyo 09:40 - 09:55 [o03] Status of Existing Facility Instruments Takashi Hattori 09:55 - 10:05 [o04] Status of full remote observations Kentaro Aoki 10:05 - 10:15 [o05] Database Aya Higuchi 10:15 - 10:30 [o06] SAC report Naoki Yasuda 10:30 - 10:45 [o07] TAC report Kentaro Motohara
10:45 - 11:00	Break
11:00-12:00	Maunakea Observatories 11:00 - 11:15 [o08] CFHT Doug Simons 11:15 - 11:30 [o09] Gemini Andy Adamson 11:30 - 11:45 [o10] Keck Hilton Lewis 11:45 - 12:00 [o11] UH Karen Meech
12:00 - 13:00	Break
13:00 - 13:30	Poster flash talks
13:30 - 14:10	Current Status of Future Instruments 13:30 - 13:50 [o12] PFS Naoyuki Tamura 13:50 - 14:10 [o13] ULTIMATE [ 1 2 ] Yosuke Minowa/Yusei Koyama
14:10 - 15:05	SSP and Intensive Programs 1 14:10 - 14:30 [o14] Status report of HSC-SSP [HSC SSP] Satoshi Miyazaki 14:30 - 14:50 [o15] Search for Planets like Earth around Late-M Dwarfs: Precise Radial Velocity Survey with IRD [IRD SSP] Bunei Sato 14:50 - 15:05 [o16] Subaru Intensive Searches for the Most Distant Quasars [S18B-011I] Yoshiki Matsuoka

Day2 | 4 Mar 2021 (Thu)

9:00-10:30	SSP and Intensive Programs 2 09:00 - 09:15 [o17] An intermediate report on microlensing PBH search from HSC observation of M31 [S18B-093I] Masahiro Takada 09:15 - 09:30 [o18] Subaru Near Field Cosmology Survey [S19A-060I] [ png ] Sakurako Okamoto 09:30 - 09:45 [o19] Subaru IRD TESS Intensive Follow-up Project [S19A-069I & S20B-088I] Norio Narita 09:45 - 10:00 [o20] Progress report of FOSSIL survey [S20A-096I] Fumi Yoshida 10:00 - 10:15 [o21] Wide Imaging with Subaru HSC of the Euclid Sky (WISHES) [S20B-097I] Masamune Oguri 10:15 - 10:30 [o22] New Targets for NASA’s New Horizons: a new collaboration with Subaru JJ Kavelaars
10:30 - 10:45	Break
10:45 - 12:15	Science Session 1 10:45 - 11:00 [o23] High-resolution spectroscopy of halo stars with asteroseismic information [Invited] Tadafumi Matsuno 11:00 - 11:15 [o24] Abundance analysis of individual elements for nearby M dwarfs based on high-resolution near-infrared spectra obtained by IRD-SSP Hiroyuki Ishikawa 11:15 - 11:30 [o25] Solving the nature of dark matter from dwarf satellites: ultimate goal of Subaru/PFS Masashi Chiba 11:30 - 11:45 [o26] Lyman-alpha halos of Lyman-alpha emitters across environments at z=2.84 [Invited] [ png ] Satoshi Kikuta 11:45 - 12:00 [o27] Initial results from Subaru/HSC-eROSITA AGN collaboration Yoshiki Toba 12:00 - 12:15 [o28] Overview of AO activities at Subaru telescope Yoshito Ono
12:15 -13:00	Break
13:00 - 14:00	Discussion Session 1 (in Japanese) 13:00 - 14:00 [d01]PFS [ 1 2 3 ]
14:00 - 14:15	Break
14:15 - 15:15	Discussion Session 1 (in Japanese) 14:15 - 15:15 [d02] LSST and Euclid

Day3 | 5 Mar 2021 (Fri)

9:00-11:10	Discussion Session 2 09:00 - 09:15 [d03] Carry-over of HSC queue observations 09:15 - 10:00 [d04] TMT 10:00 - 10:30 [d05] ULTIMATE 10:30 - 11:10 [d06] Subaru and Roman Space Telescope
11:10 - 11:30	Break
11:30 - 12:15	Science Session 2 11:30 - 11:45 [o29] Discovery of a Faint Active Galactic Nucleus in an Ultraluminous IR Galaxy with Kpc-scale Fast Wind [Invited] Xiaoyang Chen 11:45 - 12:00 [o30] Optical follow-up observation for GW event with Subaru/HSC Takayuki Ohgami 12:00 - 12:15 [o31] The average MIR-FIR properties of protoclusters at z~4 [Invited] Mariko Kubo
12:15 - 13:00	Break
13:00 - 15:00	Science Session 3 13:00 - 13:15 [o32] Black hole mass and Eddington ratio distributions of the z=4 less-luminous quasars over the HSC Wide field [Invited] Wanqiu He 13:15 - 13:30 [o33] Cosmological constraints from galaxy-galaxy lensing and clustering with the Subaru HSC and SDSS BOSS data Hironao Miyatake 13:30 - 13:45 [o34] High-Dispersion Characterization of Exoplanets using REACH, IRD, and HDS on Subaru Hajime Kawahara 13:45 - 14:00 [o35] The rest-frame UV luminosity function of protocluster galaxies at z~4 revealed by HSC-SSP Kei Ito 14:00 - 14:15 [o36] Exploring the tail end of reionization with deep HSC surveys Daichi Kashino 14:15 - 14:30 [o37] Scientific Results from the Subaru Coronagraphic Extreme Adaptive Optics Project Thayne Currie 14:30 - 14:45 [o38] Mapping the large scale structure and environmental effects of the star formation galaxies at z~ 1.5 in the DEEP2-3 Field Ronaldo Laishram 14:45 - 15:00 [o39] The Lyman Continuum Escape Survey: Ionizing Radiation from Lyman Alpha Emitting Galaxies Kimihiko Nakajima
15:00 -	Closing Remark

List of Posters

[p01] Circumstellar brown dwarfs found by combined RV and astrometry analyses and their detectability with SCExAO/CHARIS

Masataka Aizawa

[p02] ULTIMATE-START : project status

Masayuki Akiyama

[p03] The UV Upturn: Helium-enhanced stellar populations in early-type galaxies [ 1 2 ]

Sadman Ali

[p04] Carbon-Enhanced Metal-Poor stars studied with LAMOST and Subaru

Wako Aoki

[p05] FOSSIL Phase I -- Rotation Periods of Jupiter Trojans and Hildas

Chan-Kao Chang

[p06] Current Status of Novel Gratings for Next Generation Astronomical Instruments VII [ 1 2 ]

Noboru Ebizuka

[p07] Prototyping TMT exoplanet imaging instrumentation at Subaru Telescope

Olivier Guyon

[p08] Current status of SMOKA

Aya Higuchi

[p09] Galaxy clusters in the AKARI North Ecliptic Pole field detected by Subaru Hyper Suprime-Cam

Ting-Chi Huang

[p10] On-sky performances of SWIMS on the Subaru Telescope

Masahiro Konishi

[p11] REACH: a new capability to realize very high-contrast and high spectral resolution observation for the Subaru Telescope by combining SCExAO and IRD

Takayuki Kotani

[p12]Characterization of sub-Neptune and rocky planets' atmosphere using high resolution NIR spectroscopy

Vigneshwaran Krishnamurthy

[p13] SCExAO/CHARIS High-Contrast Integral Field Spectroscopy and Polarimetry of Planet-Forming Disks [ gif ]

Kellen Lawson

[p14] Elemental abundances of 400 very metal-poor stars studied with LAMOST and Subaru

Haining Li

[p15] SCExAO: status of the instrument, testbed and system-level demonstrator for PSI

Julien Lozi

[p16] QSO-galaxy lensing study from HSC-SSP data

Wentao Luo

[p17] Revealing impacts of stellar mass and environment on galaxy quenching since z~1

Zhiying Mao

[p18] Scalable, spectrally dispersed and multi-baseline nulling interferometry with photonic-based technology: the GLINT instrument

Marc-Antoine Martinod

[p19] Subaru Laser Guide Star Upgrade: Current Status and Schedule toward the Open Use

Yosuke Minowa

[p20] Near-Infrared Photometry and Spectroscopy of Young Brown Dwarfs and Planetary-Mass Objects in Serpens

Yumiko Oasa

[p21] TXS 1206+549: a γ-ray detected narrow-line Seyfert 1 galaxy at z=1.34

Malte Schramm

[p22] SCExAO/MEC and CHARIS Discovery of a Low Mass, Jupiter-Separation Companion Using Stochastic Speckle Discrimination and High Contrast Spectroscopy

Sarah Steiger

[p23] Simple chi^2 analysis of orbiting stars around Sgr A* to constrain the dark mass distribution

Yohsuke Takamori

[p24] Dynamical properties of massive quiescent galaxies at z~4

Masayuki Tanaka

[p25] Hyper Suprime-Cam Legacy Archive [ 1 2 ]

Masayuki Tanaka

[p26] Optical Spectroscopy of Dual Quasar Candidates from the Subaru HSC-SSP program

Shenli Tang

[p27] An outline of measuring cosmic shear bispectrum extending the pseudo power spectrum method

Takanori Taniguchi

[p28] Proper motion measurements for stars with Subaru HSC and SDSS DR11

Akira Tokiwa

[p29] GALAXY CRUISE: Citizens Classify Galaxies in the HSC-SSP Big Data

Kumiko Usuda-Sato

[p30] imaging Protoplanetary Disks with SCExAO: Total Intensity

Taichi Uyama

[p31] FIRST, a Pupil-Remapping Fiber interferometer at the Subaru Telescope : Results and Future plans

Sebastien Vievard

[p32] two alpha-poor stars with r-process enhancement

Qianfan Xing

[p33] Tracing the Origin of Moving Groups : LAMOST-N1

Jingkun Zhao

Deadlines

Presentation	January 31, 2021 (JST) Closed
Participation	February 24, 2021 (JST) Closed

Deadlines

Presentation, accommodation in Cosmos-Kaikan, and financial support	December 15, 2018 (Japan standard time) Closed
Banquet participation	January 15, 2019 (Japan standard time) Closed

*We will inform you of your approved presentation style (oral/presentation) and the availability of the Cosmos-Kaikan and the financial support (for those who requested) within a few weeks after the registration is closed.

Last Update: March 10, 2021