JCMT PI Projects Approved for Observation in Semester 21B |
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Version 1.1 – Updated: 2021/07/01 |
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Project ID (Code order) |
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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M21BP002 |
Shaobo Zhang |
5.85 |
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5.85 |
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XJJ |
Dust growth in a colliding cloud L1188 |
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M21BP003 |
Ruining Zhao |
7.2 |
1.2 |
6 |
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STM |
SCUBA-2 Observation of Comet C/2021 A1 (Leonard) |
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M21BP004 |
Kate Pattle |
19 |
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19 |
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MGR, JL |
Magnetic fields in the NGC7023 reflection nebula |
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M21BP006 |
Ke Shi |
7.2 |
7.2 |
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MGR, JL |
Unveil dusty star-forming galaxies in a protocluster at z=3.13 |
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M21BP009 |
Charles L. H. Hull |
4 |
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4 |
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MGR, JL |
Multi-scale magnetic field observations in Cepheus Class 0 protostellar cores |
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M21BP010 |
Yi-Jehng Kuan |
10* |
10 night hours (see footnote *) |
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STM |
Ammoniated Salt Chemistry in the nucleus of comet 342P/SOHO and coma chemistry in C/2021 A1 (Leonard) |
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M21BP015 |
Yulong GAO |
2.4 |
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2.4 |
XJJ |
Probing the molecular gas in four merges of metal-poor gas-rich galaxies |
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M21BP017 |
Samar Safi-Harb |
14 |
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14 |
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HALP |
Using JCMT to settle the debate on Tycho's progenitor |
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M21BP018 |
Hao-Yuan Duan |
2 |
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2 |
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HALP |
Measuring the Turbulence Linewidths for Deriving the Magnetic Field Strength in Onsala 2 |
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M21BP020 |
Nicolas Peretto |
18 |
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18 |
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MGR, JL |
Mapping the magnetic field morphology of the NGC2024 filaments across the sub- to super-critical transition |
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M21BP021 |
Han-Tsung Lee |
6 |
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6 |
HALP |
SDC18, a shock-compressed filament or a gravitationally collapsing sheet |
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M21BP024 |
Kate Pattle |
13 |
13 |
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MGR, JL |
Magnetic fields in the nearest starburst galaxies |
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M21BP026 |
Sarah Sadavoy |
25.5 |
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25.5 |
HALP |
Mapping the Kinematics of L483 |
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M21BP027 |
Ya-Wen Tang |
7.6 |
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7.6 |
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STM |
A Comprehensive Study of Magnetic Fields and Fragmentation in Filaments |
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M21BP029 |
Jia-Wei Wang |
8 |
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8 |
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HALP |
Interplay between Filament, Magnetic fields, Gravity, and Velocity Gradients in Quiescent Hub-Filament System: Investigating the Initial Condition of HFS Formation |
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M21BP030 |
Ian Smail |
24 |
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24 |
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STM |
Using cold-dust-selected samples from SCUBA-2 to trace the growth of cluster galaxies out to z~2 |
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M21BP031 |
Qilao Gu |
16*** |
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16 |
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MGR, JL |
Does the Magnetic Field Suppress Star Formation in Galactic Center Massive Clouds? |
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M21BP032 |
Mariko Kubo |
10.3 |
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10.3 |
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SL |
SCUBA-2 follow up for an extremely bright IR source at z>3 |
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M21BP033 |
LuShiying |
12 |
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12 |
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STM |
Probing the Molecular Gas for 10 nearby star-forming S0 galaxies |
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M21BP034 |
Junfeng Wang |
6 |
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6 |
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STM |
Searching for Molecular Outflow in a Gaseous Merger with Restarted Radio Activities |
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M21BP036 |
Zhenzhen Miao |
15.8 |
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15.8 |
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XJJ |
Observation of molecular AlF towards S-type AGB stars |
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M21BP037 |
Yanan Feng |
15.9 |
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15.9 |
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XJJ |
Seeking "parent" molecules toward the S-type AGB star: BZ Cma |
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M21BP038 |
Yanan Feng |
15.3 |
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15.3 |
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XJJ |
Searching for characteristic molecules (C2H and SO) in two S-type AGB stars |
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M21BP041 |
Lingrui Lin |
0.5 |
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0.5 |
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HALP |
Exploring the low dust emissivity index of Galactic metal-poor molecular clouds |
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M21BP043 |
Sheng-Jun Lin |
3.7 |
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3.7 |
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SL |
BISTRO-3 Complementary Observations: Mapping the Extended Emission of Starless Cores with SCUBA-2 |
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M21BP044 |
Mike Chen |
78.9 |
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78.9 |
STM |
Probing Convergence Flows in B5 |
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M21BP045 |
Chang Won Lee |
16 |
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16 |
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HALP |
Testing grain alignment of carbonaceous and silicate grains in the envelopes of AGB stars |
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M21BP046 |
Eswaraiah Chakali |
12.568 |
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12.568 |
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XJJ |
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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M21BP049 |
Yan Duan |
11 |
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11 |
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STM |
HARP Observation of Taurus Gas and Star-Formation Feedback |
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M21BP050 |
Che-Yen Chu |
22** |
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22** |
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STM |
Studying sub-mm band spectral shape and time variability of radio magnetars |
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M21BP051 |
Qingzheng Yu |
21 |
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21 |
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XJJ |
Probing the cold gas evolution of MaNGA merging galaxies |
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M21BP052 |
Juan Tuo |
21 |
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21 |
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XJJ |
Observation of molecular HC3N towards the planetary nebula : Hb 5 |
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M21BP053 |
Ray S. Furuya |
14.4*** |
14.4 |
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HALP |
Does alpha dynamo really maintain galaxy-scale B field? |
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M21BP055 |
Myungshin Im |
20 |
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20 |
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MGR, JL |
SCUBA-2 Observations of the JWST/GTO NEP Time Domain Field: Going Deeper |
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M21BP058 |
Yong Zhang |
5.4 |
5.4 |
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SL |
Morphology of the extended dust envelope around Betelgeuse |
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M21BP059 |
Yuhui Zhao |
16.4 |
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16.4 |
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XJJ |
Production and kinematics of CO in distant comet C/2017 K2 |
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M21BP061 |
Ram Kesh Yadav |
3.7 |
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3.7 |
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STM |
Understanding star formation in elephant trunk-like structures: a pilot study with SCUBA-2 |
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M21BP063 |
Yi-Jehng Kuan |
30 |
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30 |
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STM |
Zero-Spacing Spectral Imaging of Orion KL |
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M21BP064 |
Yuji Urata |
18 |
18 |
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HALP |
SCUBA-2 Follow-up of IceCube Neutrino events |
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M21BP067 |
Hsi-Wei Yen |
15.5 |
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15.5 |
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MGR, JL |
Magnetic field structures in dense cores with embedded disks |
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M21BP073 |
Guodong Li |
6.7 |
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6.7 |
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XJJ |
Cold Dust Content of a Low-z Obscured Quasar W1904+4853 |
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M21BP074 |
Woojin Kwon |
26 |
5 |
21 |
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HALP |
Magnetic Field Morphologies and Strengths around Class 0 Young Stellar Objects |
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M21BP075 |
Gregory Sivakoff |
24 |
8 |
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16 |
STM |
Is SS Cyg, the Prototypical Cataclysmic Variable, a Bright Sub-mm Transient? |
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M21BP076 |
Jingwen Wu |
4.4 |
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4.4 |
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XJJ |
Cold Dust and Star Formation in low-z Hot DOGs |
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M21BP078 |
Graham Bell |
4*** |
4 |
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GSB |
Searching for a turn-up in the spectrum of magnetar XTE J1810-197 at 450µm |
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M21BP079 |
Laura Fissel |
7.75 |
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7.75 |
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STM |
Completing the Polarization Survey of Isolated Protostellar Cores in Perseus |
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M21BP080 |
Mengke Zhao |
11 |
11 |
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XJJ |
Magnetic field in the end-dominated collapsing filament structure S242 |
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M21BP082 |
Tom Bakx |
10.66 |
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10.66 |
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SL |
Dusty galaxies as signpost for distant proto-clusters at z~3-4 |
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M21BP083 |
Douglas Scott |
2.6 |
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2.6 |
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HALP |
Crab polarization as a CMB calibrator |
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M21BP084 |
Daniel Perley |
15 |
15 (max. of 3 in Band 1) |
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MGR, JL |
SCUBA-2 ToO Observations of Gamma-Ray Bursts |
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M21BP087 |
Chian-Chou Chen |
12 |
6 |
6 |
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SL |
Testing the ubiquity of overdensity of dusty galaxies around z~3 quasar pairs |
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M21BP090 |
Aaron Golden |
8.9 |
8.9 |
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SL |
'Snow plows' through the local ISM - using nearby pulsars as probes of interstellar dust via the detection of circumpulsar debris disks |
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M21BP091 |
Rei Enokiya |
1 |
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1 |
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XJJ |
Probing molecular gas associated with the Youngest Galactic Supernova Remnant G1.9+0.3 (continuation of 20B) |
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M21BP092 |
Tie Liu |
7.4*** |
7.4 |
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HALP |
Magnetic field of the W43-main cloud |
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* Proposal M21BP010: The night-time allocation is as listed above. However, the proposal was additionally awarded up to 82h of EO time for use in Bands 1-4. |
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** Proposal M21BP050: Time allocation is treated here as a ToO trigger, to allow (near-)simultaneous data acquisition with IRAM for two epochs, one month apart. JCMT time allocation contingent upon approval of corresponding IRAM time allocation. |
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*** A “Total Hrs” entry in magenta indicates a contingency amount of time. This may be subsequently reduced if some fraction of the time is used up by the 21A version of the project. Other project allocations may also be reduced if their fallback projects from earlier semesters obtain additional data during semester 21A. |
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Project ID (Rank Order) |
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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M21BH21A1 |
Len Cowie |
45 |
45 |
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MGR, JL |
Developing a sample of faint submm sources and determining their properties |
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M21BH20A |
Jonathan Williams |
20 |
20 |
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MGR, JL |
Magnetic field structure in dense cores with embedded disks – (For August targets) |
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M21BH03B |
Watson Varricatt |
25 |
25 |
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MGR, JL |
Mapping the magnetic fields in massive star forming regions |
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M21AH08B4 |
Benjamin Shappee |
24 |
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24 |
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MGR, JL |
Rainbow tide: multi-wavelength follow-up of tidal disruption events |
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M21AH20A |
Jonathan Williams |
30 |
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30 |
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MGR, JL |
Magnetic field structure in dense cores with embedded disks – (For targets observable later in the semester) |
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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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Harriet / HALP |
Harriet – h.parsons @ eaobservatory.org |
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Mark / MGR |
Mark – m.rawlings @ eaobservatory.org |
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Graham / GSB |
Graham – g.bell @ eaobservatory.org |
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Nagayoshi/ NO |
Nagayoshi – nohashi @ naoj.org |
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Junhao / JL |
Junhao Liu – j.liu @ eaobservatory.org |
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Steve / STM |
Steve – s.mairs @ eaobservatory.org |
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