JCMT projects approved for observing in Semester 18B |
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Updated: 2018/05/10 |
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Project ID |
Principal Investigator |
Total Hrs |
WB |
FoP |
Title of Investigation (colour code: Target-of-Opportunity; Time-specific; daytime) |
1 |
2 |
3 |
4 |
5 |
Hrs=hours approved; WB=weather band; FoP="friend" of the project (see below) |
M18BP001 |
Harriet Parsons |
6.2 |
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6.2 |
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Harriet |
SCUBA-2 and HARP observations of L1340 |
M18BP002 |
Xing Lu |
32.0 |
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32.0 |
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Harriet |
Are supercritical filaments supported by magnetic fields? |
M18BP006 |
Yuki Yoshimura |
20.0 |
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20 |
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Jan |
The origin of molecular-cloud-scale chemical composition: prominent GMC-SNR association G23.3-0.4 |
M18BP009 |
Kate Pattle |
28.0 |
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28 |
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Harriet |
Investigating dust grain alignment in Ophiuchus L1689 |
M18BP010 |
Kotomi Taniguchi |
40.0 |
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40 |
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Harriet |
Establishment of Efficient Formation Mechanism of Cyanopolyynes in Hot Cores - A Clue to Origin of the Chemical Diversity - |
M18BP011 |
Sihan Jiao |
42.0 |
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32 |
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10 |
Harriet |
Compact Gas Clumps in M31 |
M18BP013 |
Hongjun An |
11.5 |
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11.5 |
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Mark |
Constraining the population of high-spin supermassive Black Holes in the Early Universe |
M18BP015 |
Tomomi Shimoikura |
51.0 |
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51 |
Steve |
A Study of Massive Clumps in The Early Stages of Cluster Formation |
M18BP019 |
Tie Liu |
1.8 |
1.8 |
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Harriet |
Magnetic field surrounding a massive clump near HII regions |
M18BP023 |
Tie Liu |
10.0 |
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10 |
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Steve |
Chemical and Dynamical Evolution of High Mass Young Stellar Objects---A joint proposal with KaVA large program |
M18BP025 |
Alexandra Tetarenko |
12.0 |
4 |
4 |
4 |
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Mark |
Constraining Jet Formation and Evolution with Transient X-ray Binaries |
M18BP026 |
Myungshin Im |
21.0 |
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21 |
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Steve |
SCUBA-2 observations of the JWST/GTO Time Domain Survey Field |
M18BP027 |
Alexandra Tetarenko |
6.5 |
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3.9 |
2.6 |
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Steve |
Mapping Jet-ISM Interactions Near the X-ray Binary SS 433 with HARP |
M18BP028 |
Qiong Li |
31.0 |
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31 |
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Harriet |
Completing a SCUBA-2 survey of most massive large-scale structures at z~2 |
M18BP030 |
Ilse De Looze |
20.0 |
20 |
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Steve |
Dust polarisation properties in Cassiopeia A |
M18BP031 |
Jason Kirk |
8.9 |
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8.9 |
Jan |
Probing turbulence dissipation in TMC1 |
M18BP032 |
Thavisha Dharmawardena |
9.8 |
7.6 |
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2.2 |
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Jan |
Multiple-shell formation in detached-shell AGB stars: the role of gas-grain decoupling |
M18BP035 |
Yi-Jehng Kuan |
35.0 |
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35 |
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Steve |
46P |
M18BP037 |
Yoshiaki Ono |
15.5 |
7.8 |
7.8 |
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Jan |
Deep Search for Sub-mm Galaxy Overdensities around the Highest-redshift Quasars |
M18BP038 |
Patrick Koch |
15.2 |
15.2 |
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Per |
Mapping the B-Field towards a Filamentary Hub-System |
M18BP039 |
Nicolas Peretto |
47.5 |
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47.5 |
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Per |
Are magnetic fields regulating the dynamical evolution of IRDCs on parsec scales? |
M18BP040 |
Daniel Perley |
15.0 |
3 |
5 |
5 |
2 |
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Mark |
SCUBA-2 ToO Observations of Gamma-Ray Bursts |
M18BP041 |
Archana Soam |
28.0 |
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28 |
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Steve |
Role of magnetic fields in dense core formation in filamentary clouds- II |
M18BP044 |
Chengpeng Zhang |
16.3 |
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16.3 |
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Jan |
Molecular gas in HI-bearing ultra-diffuse galaxies |
M18BP045 |
Ivan Oteo |
18.0 |
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18 |
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Jan |
Do the most luminous dusty starbursts in the early Universe trace extreme protoclusters? |
M18BP046 |
Jia-Wei Wang |
16.0 |
16 |
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Steve |
How the magnetic field impact on the formation of hub-filament system G33.92+0.11 |
M18BP047 |
Junhao Liu |
10.0 |
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10 |
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Mark |
Dust polarization survey of massive dense cores in Cygnus-X |
M18BP048 |
Yuri Nishimura |
14.5 |
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14.5 |
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Harriet |
Molecular-cloud-scale mapping observation toward W3(OH) in the 0.8 mm band II |
M18BP050 |
Xue-Bing Wu |
22.0 |
22 |
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Jan |
Dust emission from luminous quasars at the reionization era |
M18BP051 |
Patrick Koch |
12.0 |
12 |
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Jan |
Linking the magnetic field structures and the gas dynamics in the Class 0 protostar B335 |
M18BP053 |
Giuliana Cosentino |
11.5 |
11.469 |
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Steve |
Mapping Magnetic Field in Infrared Dark Clouds |
M18BP055 |
Huei-Ru Vivien Chen |
19.0 |
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19 |
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Steve |
Mapping Magnetic Fields in the Filamentary Cloud NGC 7538 |
M18BP056 |
Ryan Cheale |
11.0 |
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11 |
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Mark |
SCUBA-2 Cluster Snapshot Survey - confirming a sample of lensed submillimeter galaxies |
M18BP058 |
Yinghe Zhao |
0.4 |
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0.4 |
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Mark |
SCUBA-2 Observations of a Possible Hyper-luminous Galaxy of LIR ~ 5E14 Lsun at Redshift~ 2.1 |
M18BP060 |
Patrick Koch |
8.3 |
8.3 |
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Harriet |
Dust Polarization Mapping toward Infrared Dark Clouds |
M18BP061 |
Jianfa Wang |
49.8 |
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49.8 |
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Harriet |
HCN(3-2) and HCO+(3-2) survey and the dense gas excitation of nearby IR-bright galaxies |
M18BP062 |
Yujin Yang |
10.0 |
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10 |
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Harriet |
Unveiling Dust Emission Associated with Extended Quasar Nebulae |
M18BP063 |
Ryan Chown |
28.6 |
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28.6 |
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Harriet |
Observing red star-forming galaxies from xCOLD GASS with SCUBA-2 |
M18BP064 |
Hideo Sagawa |
63.0 |
6 |
39 |
10 |
4 |
4 |
Jan |
Correlations among Spatial/Temporal Variations of Venus Atmospheric Photochemistry and Dynamics |
M18BP067 |
Sang-Sung Lee |
6.0 |
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6 |
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Per |
Detection of linear polarization of radio-loud AGNs at 450 and 850 microns |
M18BP069 |
Chenlin Zhou |
3.0 |
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3 |
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Jan |
Warm gas observation in bubble N131 |
M18BP070 |
Jong-Hak Woo |
19.5 |
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19.5 |
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Jan |
Delayed AGN feedback?- constraining star formation rate of the AGNs (PI: Jong-Hak Woo) |
M18BP071 |
Scott Chapman |
7.9 |
7.9 |
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Mark |
The SED and environment of the exceptional Q2345 QSO |
M18BP072 |
Tao-Chung Ching |
6.2 |
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6.2 |
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Steve |
Probing the Origin of Different Star Formation Modes and Cloud Conditions Through Mapping CO 3-2 in Taurus |
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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 18A version of the project |
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Project ID |
Principal Investigator |
Total Hrs |
WB |
FoP |
Title of Investigation (colour code: Target-of-Opportunity; Time-specific; daytime) |
1 |
2 |
3 |
4 |
5 |
M18BH02A |
Lennox Cowie (SCUBA-2) |
96 |
40 |
56 |
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Mark |
The Growth of Dusty Massive Galaxies and Obscured AGNs |
M18BH13A |
Bo Reipurth (HARP, SCUBA-2) |
52 |
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Per |
Destruction of Two Dense Globules by Outflow Activity |
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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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PF |
Per - - - - p.friberg @ eaobservatory.org |
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JGW |
Jan - - - - j .wouterloot @ eaobservatory.org |
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JTD |
Jessica - - j.dempsey @ eaobservatory.org |
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HALP |
Harriet - - h.parsons @ eaobservatory.org |
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MGR |
Mark - - - m.rawlings @ eaobservatory.org |
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STM |
Steve - - - - s.mairs @ eaobservatory.org |