JCMT PI Projects Approved for Observation in Semester 20B |
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Updated: 2020/05/12 |
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Project ID |
Principal Investigator |
Total Hrs |
WB |
FoP |
Title of Investigation (Color Code: Red = Target-of-Opportunity; Green = Time-specific; Italics = Daytime) |
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1 |
2 |
3 |
4 |
5 |
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Hrs = hours approved; WB = weather band; FoP = "Friend" of the project (see below) |
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M20BP001 |
Jinjin Xie |
44.6 |
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30.6 |
14 |
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HALP |
Tracing the Assembly of Massive Clumps |
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M20BP004 |
Takayuki Muto |
7.1 |
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7.1 |
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AJT |
Exploring the Nature of Field Dippers |
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M20BP007 |
Hsi-Wei Yen |
20 |
20 |
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AJT |
Magnetic field structures in dense cores with embedded disks |
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M20BP009 |
Junhao Liu |
17.31 |
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17.31 |
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PT |
Does Magnetic Field Suppress Star Formation in Galactic Center Massive Clouds? |
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M20BP011 |
Eun Jung Chung |
19.8 |
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9 |
10.8 |
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XJJ |
Roles of gravity, B-field, and turbulence in the formation of hub-filaments structure in the IC5146 |
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M20BP015 |
Shih-Ping Lai |
14 |
14 |
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XJJ |
The evolutionary status of prestellar cores : observations of H2D+ at 372 GHz |
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M20BP016 |
David Eden |
17 |
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17 |
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HALP |
Dense Gas in High-Mass Star-Forming Regions |
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M20BP020 |
Yi-Jehng Kuan |
28 |
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28 (incl. 3 in B2, 5 in B3) |
XJJ |
Comet Chemistry: Target of Opportunity request |
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M20BP022 |
Kate Pattle |
24 |
13 |
11 |
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MGR |
Magnetic fields in the nearest starburst galaxies |
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M20BP023 |
Xue-Bing Wu |
20.7 |
20.7 |
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PT |
Dust Emission from Most Distant Luminous Quasars in the Reionization Epoch |
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M20BP025 |
Xue-Jian Jiang |
75 |
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75 |
XJJ |
Gas infall in massive filaments (synergy with SMA observations) |
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M20BP026 |
Daniel Perley |
15 |
15 (max. of 3 in Band 1) |
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MGR |
SCUBA-2 ToO Observations of Gamma-Ray Bursts |
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M20BP029 |
Junhao Liu |
19 |
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19 |
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STM |
Dust polarization survey of massive dense cores in Cygnus-X |
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M20BP032 |
Rajeshwari Dutta |
24 |
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24 |
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STM |
Investigating Molecular Gas Properties in Low-z Radio-loud Galaxy Mergers |
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M20BP033 |
Xiaotong Feng |
9 |
9 |
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AJT |
Refining the far-infrared SED to determine precise star formation rates and dust properties of Palomar-Green quasar hosts |
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M20BP035 |
Ram Kesh Yadav |
6.5 |
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6.5 |
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XJJ |
Understanding star formation in elephant trunk-like structures: a pilot study with SCUBA-2 |
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M20BP036 |
Joseph Cairns |
20.5 |
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20.5 |
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SL |
Cluster Cores at z > 4 |
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M20BP037 |
Rei Enokiya |
7 |
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7 |
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HALP |
High resolution observations of magnetic fields in the magnetically intertwined Double Helix Nebula in the Galactic Center |
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M20BP039 |
Rei Enokiya |
15 |
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15 |
IM |
Probing molecular gas associated with the Youngest Galactic Supernova Remnant G1.9+0.3 |
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M20BP040 |
Junhao Liu |
14 |
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14 |
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PT |
Are sub-virial clumps in IRDC G28.34 supported by magnetic fields? |
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M20BP042 |
Jack Birkin |
5.8 |
5.8 |
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STM |
A SCUBA-2 search for the reversal in the star-formation-density relation in distant clusters |
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M20BP043 |
Tie Liu |
14 |
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14 |
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STM |
Magnetic fields inside of a quiescent filament (Resubmission of M18BP041 and M19AP017) |
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M20BP044 |
Kate Pattle |
23.7 |
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23.7 |
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SL |
Role of the magnetic field in the fragmentation of a star forming filament in the Orion B molecular cloud |
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M20BP045 |
Xue-Jian Jiang |
41 |
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41 |
XJJ |
Constraining the Properties of Galactic Star-Forming Gas by Dense-Molecular-Gas Observations and Multiple-Line Analysis |
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M20BP046 |
Sheng-Jun Lin |
15 |
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15 |
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HALP |
Probing the magnetic field in the starless core L1512 |
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M20BP049 |
Tom Bakx |
20 |
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20 |
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STM |
Are the most intrinsically-bright Herschel galaxies tracing the cosmic web? |
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M20BP050 |
Sayantan Auddy |
12.25 |
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12.25 |
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AJT |
Testing the "Core Field Structure" method against dust polarization observation of H-MM1 |
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M20BP051 |
Ray S. Furuya |
16 |
16 |
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AJT |
Does alpha dynamo really maintain galaxy-scale B field? |
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M20BP055 |
Yuji Urata |
9 |
9 |
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HALP |
SCUBA-2 Follow-up of IceCube Neutrino events |
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M20BP058 |
Hideo Sagawa |
42 |
42 (Daytime) |
STM |
Venus Observations Simultaneous/Contemporaneous with BepiColombo flyby |
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M20BP059 |
Chuan-Peng Zhang |
3 |
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3 |
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STM |
To detect shock and PDR in the inner rims of a bubble shell |
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M20BP060 |
Eun Jung Chung |
4.95 |
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4.95 |
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STM |
Magnetic fields of hub-filaments structure in L1478 |
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M20BP062 |
Qinghua Tan |
19 |
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11.4 |
7.6 |
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XJJ |
SCUBA-2 observations of ultraluminous infrared QSO hosts |
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M20BP063 |
Shinyoung Kim |
13 |
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13 |
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XJJ |
Dense Core Formation in Filamentary Clouds II |
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M20BP066 |
Xunchuan Liu |
19 |
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19 |
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AJT |
CO Outflow Survey in Low Luminosity Objects -- Candidates of Carbon Chain Molecules Production regions |
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M20BP069 |
Eswaraiah Chakali |
5 |
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5 |
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HALP |
Understanding the importance of magnetic fields in the ``collect and collapse model" of star formation - a case study towards S104 using SCUBA2-POL2 |
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M20BP070 |
Hyunjin Shim |
62.6 |
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53 |
9.6 |
IM |
Conditions of local extreme starbursts based on the [CII]/CO |
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M20BP072 |
Jae-Woo Kim |
14 |
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14 |
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AJT |
Constraining the variability of the most active Brightest Cluster Galaxies in the sub-mm |
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M20BP074 |
Jianfa Wang |
30.7 |
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30.7 |
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PT |
HCN(3-2) and HCO+(3-2) survey and the dense gas excitation of nearby IR-bright galaxies |
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M20BP077 |
Yuhui Zhao |
10 |
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10 |
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XJJ |
Observing Comet C/2017 K2 (PANSTARRS) with Nāmakanui |
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M20BP079 |
Hideo Sagawa |
16 |
16 |
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STM |
H2O2 Photochemistry in Mars Atmosphere |
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M20BP080 |
Jingwen Wu |
18 |
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18 |
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MGR |
Identifying the velocity field of possible stream flows of inter-arm GMCs in M31 |
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Note: A “Total Hrs” entry in magenta indicates a contingency amount, which may be subsequently reduced if some fraction of the time is used up by the 20A version of the project. Other project allocations may also be reduced if their fallback projects from earlier semesters obtain additional data during semester 20A. |
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Project ID |
Principal Investigator |
Total Hrs |
WB |
FoP |
Title of Investigation (Color Code: Red = Target-of-Opportunity; Green = Time-specific; Italics = Daytime) |
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1 |
2 |
3 |
4 |
5 |
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M20BH20A |
Len Cowie |
96 |
96 |
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MGR |
The growth of dusty massive galaxies and obscured AGNs |
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M20BH15A2 |
Jonathan Williams |
38 |
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38 |
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NO |
Early planet formation in embedded disks |
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M20BH11C |
Watson Varricatt |
22 |
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22 |
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MGR |
Understanding massive star formation through spectral line and continuum observations in the sub-mm |
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M20BH11B |
Watson Varricatt |
25 |
25 |
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MGR |
Mapping the magnetic fields in massive star forming regions |
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M20BH11C |
Watson Varricatt |
10 |
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10 |
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(MGR) |
Understanding massive star formation through spectral line and continuum observations in the sub-mm (additional time) |
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M20BH11B |
Watson Varricatt |
10 |
10 |
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(MGR) |
Mapping the magnetic fields in massive star forming regions (additional time) |
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"Friend of the Project" (FoP): Each project is assigned a "friend of the project" who is the first line of contact for assistance/advice/info |
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Per / PF |
Per – p.friberg @ eaobservatory.org |
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Izumi / IM |
Izumi – i.mizuno @ eaobservatory.org |
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Shaoliang /SL |
Shaoliang – s.li @ eaobservatory.org |
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Xue-Jian / XJJ |
Xue-Jian – x.jiang @ eaobservatory.org |
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Pablo / PT |
Pablo – p.torne @ eaobservatory.org |
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Harriet / HALP |
Harriet – h.parsons @ eaobservatory.org |
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Mark / MGR |
Mark – m.rawlings @ eaobservatory.org |
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Nagayoshi/ NO |
Nagayoshi – nohashi @ naoj.org |
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Alex / AJT |
Alex – a.tetarenko @ eaobservatory.org |
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Steve / STM |
Steve – s.mairs @ eaobservatory.org |
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