Accepted Proposals for Semester S19A
The Call for Proposals for Semester S19A received 129 and 4 submitted proposals for the Normal and Intensive Programs, respectively, requesting a total of 354.9 nights. After screening by TAC, 62 (+ 12 ToO) nights were allocated to the following 46 proposals. In addition, 40 nights and 15 nights are assigned to HSC SSP Project and IRD SSP Project respectively, 4.5 nights are assigned to the Service Program observations, and 5.5 nights are assigned to the on-going Intensive Programs, S18B-011I(5 nights) and S18B-093I(0.5 night).
| ID | PI | Proposal Title | Inst | Nts | Abstract |
|---|---|---|---|---|---|
| S19A-006 | Yoshiaki Ono | Spectroscopy for Very Bright z ~ 7 Galaxies Found in 350 deg2 HSC Data | FOCAS | 1 | abstract |
| S19A-007 | Takuji Tsujimoto | Clocking r-process enrichment in the Sextans dwarf spheroidal galaxy | HDS | 3 | abstract |
| S19A-009 | Michitoshi Yoshida | Optical--infrared follow-up observations of gravitational wave sources | any of HSC/FOCAS/MOIRCS/IRCS/HDS | 4.5ToO | abstract |
| S19A-011 | Taichi Uyama | Follow-up observation of CI Tau with SCExAO+CHARIS | CHARIS+SCExAO+NGS | 0.5 | abstract |
| S19A-012 | Masaru Kajisawa | What drives the quenching of star formation in high-z massive galaxies II | DEIMOS(Keck) | 1 | abstract |
| S19A-013 | Mizuho Uchiyama | Follow-up infrared observations of methanol maser outburst MYSOs | IRCS+NGS-AO | 1 ToO | abstract |
| S19A-014 | Nobunari Kashikawa | What causes the patchy reionization? | HSC(Queue) | 1.5 | abstract |
| S19A-015 | Masafusa Onoue | Determination of the Black Hole Mass Function at z~6 | MOIRCS | 3 | abstract |
| S19A-017 | Yoshiaki Ono | Spectroscopy for High-z Very Blue UV Continuum Galaxies in HSC-SSP Fields | FOCAS | 1 | abstract |
| S19A-021 | Toru Misawa | Transverse Proximity Effects around BAL Quasars II | FOCAS | 1 | abstract |
| S19A-023 | Shogo Nishiyama | Exploring General Relativistic Effects and Environment of Galactic SMBH 3 | IRCS+LGS-AO | 3 | abstract |
| S19A-024 | Andy Goulding | Hyper Suprime-Cam Observations of the Chandra Deep Wide Field Survey | HSC(Queue) | 1.2 | abstract |
| S19A-026 | Masaomi Tanaka | Probing the Geometry of Superluminous Supernovae | FOCAS | 1 ToO | abstract |
| S19A-029 | Mitsuhiko Honda | Tracing time-dependent disk chemistry of periodic outbursting protostar EC53 | COMICS | 0.5 | abstract |
| S19A-031 | Nozomu Tominaga | Populations of Shock Breakouts: Variety of SN Progenitors and CSM Structure | HSC+GMOS(Gemini-N) | 2+2ToO | abstract |
| S19A-032 | Daichi Kashino | Structure of reionization: the origin for spatially variable IGM opacity II | HSC(Queue) | 1.5 | abstract |
| S19A-037 | Yuichi Harikane | Understanding Reionizing Source with Newly-Identified IRAC Excess Galaxy II | MOSFIRE(Keck) | 2 | abstract |
| S19A-042 | Yuhei Takagi | Calibration of stellar evolutionary models with high-resolution spectroscopy | IRCS+LGS-AO | 1 | abstract |
| S19A-043 | Koki Kakiichi | Understanding Ionizing Photons Escape From zβ 3 Lyman Emitting Galaxies | OSIRIS+LGS-AO(Keck) | 1.5 | abstract |
| S19A-049 | Russell Smith | The FOCAS-IFU Nearby Elliptical Lens Search: Low-z lenses to probe the IMF | FOCAS | 2 | abstract |
| S19A-051 | Masaomi Tanaka | Unveiling the Nature of Rapid Transients in the Local Universe | GMOS(Gemini-N) | 1.5 ToO | abstract |
| S19A-055 | Miho Ishigaki | Spectroscopy of Virgo I, a new Milky Way satellite discovered by HSC | FOCAS | 2 | abstract |
| S19A-056 | Masatoshi Imanishi | Growth of supermassive blackholes in gas-rich galaxy mergers | IRCS+LGS-AO | 1 | abstract |
| S19A-058 | Masato Onodera | Integral field spectroscopy of massive compact star-forming galaxies at z = 0.4 | FOCAS | 3 | abstract |
| S19A-060I | Sakurako Okamoto | * Subaru Near Field Cosmology Survey | HSC(Queue) | 2 | abstract |
| S19A-064 | Chan-Kao Chang | Rotation Period Survey of Jovian Trojans | HSC | 2 | abstract |
| S19A-066 | Stevanus Kristianto Nugroho | Searching for VO in the Day-side of Moderately Hot Jupiter | IRD+NGS-AO | 2 | abstract |
| S19A-069I | Norio Narita | * Subaru IRD TESS Intensive Follow-up Project | IRD+NGS-AO | 3 | abstract |
| S19A-073 | Mihoko Konishi | Statistical Investigation of Planet-disk Interaction in ALMA Ring Disks | VAMPIRES+SCExAO+CHARIS | 2 | abstract |
| S19A-074 | Masato Ishizuka | Probing Thermal Inversion in Hot-Jupiter's atmosphere with IRD | IRD+NGS-AO | 1 | abstract |
| S19A-077 | Takashi Tsukagoshi | Search for a Candidate Accretion Planet in the TW Hya Disk | VAMPIRES+SCExAO+NGS | 0.5 | abstract |
| S19A-079 | Tomoki Morokuma | Optical Follow-Up Observations for IceCube High-Energy Neutrino Sources | HSC&GMOS(Gemini-S) | 1ToO+1ToO | abstract |
| S19A-080 | Jun Toshikawa | Confirmation of Protoclusters at z~4 Found by the HSC-SSP | FOCAS | 2 | abstract |
| S19A-094 | Cristian Eduard Rusu | Mass distribution of quasars revealed through gravitational lensing | IRCS+LGS-AO | 1 | abstract |
| S19A-095 | Olivier Guyon | Characterizing Close Companions around young stars surrounded by dust | CHARIS+SCExAO+NGS | 1 | abstract |
| S19A-099 | Julien Lozi | Resolved spectro-polarimetric imaging of AGB shocks & mass-loss | CHARIS+SCExAO+NGS | 1 | abstract |
| S19A-101 | Hideki Umehata | Ultra-deep Ks-band imaging of ALMA Deep Field in SSA22 | MOIRCS | 1 | abstract |
| S19A-102 | Masafusa Onoue | The Nature of a Luminous Pop-III Galaxy Candidate at z=6.1 | MOSFIRE(Keck) | 1 | abstract |
| S19A-106 | Takayuki Kotani | Characterizing the kinematics and the atmospheres of HR8799 planets | IRD+NGS-AO | 1 | abstract |
| S19A-109 | Yutaka Komiyama | The Faint-End of Hα Luminosity Function of the Coma Cluster | FOCAS | 1 | abstract |
| S19A-115 | Yi Yang | Observations of protoplanetary disks' inner regions | VAMPIRES+SCExAO+NGS | 1.5 | abstract |
| S19A-116 | Yen-Ting Lin | Characterizing the Most Massive Distant Clusters from the HSC Survey | FOCAS | 2 | abstract |
| S19A-119 | Shuya Tan | Observing Europa's surface salts to characterize chemistry of the interior ocean | IRCS+NGS-AO | 1 | abstract |
| S19A-122 | Maria Hjorth | Towards a better understanding of the formation of warm and hot Jupiters | HDS | 1 | abstract |
| S19A-136 | Wanqiu He | Determine the z=4 QLF with faint quasars in the HSC-WIDE field | DEIMOS(Keck) | 2 | abstract |
| S19A-138 | Satoshi Kikuta | Probing Lyα nebulae across environments | HSC(Queue) | 0.3 | abstract |
We have time-exchange programs with Gemini and Keck. The instruments and nights written in italics are those of Gemini or Keck.
- These proposals have been accepted in the category of Intensive Program. S19A-069I will be assigned 3 nights per semester for the following 2 semesters. S19A-060I will be assigned 8 nights (=3+3+2) for the following 3 semesters.
NOTE
In order to compensate surplus telescope times, which resulted from cancellations due to instrument damage caused by hurricane, two backup proposals (see 1 below) were newly accepted and supplemental nights were added to already accepted two proposals (see 2 below).
*1
S19A-070, Wako Aoki et al.,
LAMOST/Subaru follow-up spectroscopy for extremely metal-poor stars
HDS, 0.5 night, abstract
S19A-121, Kento Masuda et al.,
Photometric Search for Compact Companions to Normal Stars
HDS, 1 night, abstract
*2
Additional 0.5 night for each of S19A-115, and S19A-073.
Service Programs Conducted in Semester S19A
The following proposals were conducted in S19A as Service Programs.
| ID | PI | Proposal Title | Inst | Achievement |
|---|---|---|---|---|
| S19A-146S | Wako Aoki | Double-lined spectroscopic binaries with very low metallicity | HDS | 30% |
| S19A-147S | Christian Eduard Rusu | The Substructure Mass Function From an Unusually Magnified Quasar Host | IRCS+LGS-AO | 100% |
| S19A-159S | Takashi Kojima | Deep FOCAS Spectroscopy for Remarkably Low-metallicity, Low-mass Galaxy | FOCAS | 95% |
| S19A-166S | Akira Arai | Spacial resolved imaging of ejecta of classical novae V339 Del and V1280 Sco | IRCS+NGS-AO | 50% |
| S19A-167S | Miho Ishigaki | Precision spectroscopy for the training set of PFS using Gaia Benchmark stars | HDS | 50% |
| S19A-170S | Haining Li | Studying binarity of Li-rich very metal-poor stars found with LAMOST/Subaru | HDS | 20% |
updated on February 14, 2021