JCMT PI Projects Approved for Observation in Semester 20A











Updated: 2019/12/09











Project ID Principal Investigator Total Hrs WB FoP Title of Investigation (Color Code: Red = Target-of-Opportunity; Green = Time-specific; Italics = Daytime)
1 2 3 4 5
Hrs = hours approved; WB = weather band; FoP = "Friend" of the project (see below)
M20AP001 Yali Shao 17.4
17.4


XJJ & HALP The Star Formation and the Environments of 11 Radio-loud Quasars at z > 5
M20AP002 Wei-Ling Tseng 26

26

STM Gas composition of the long-period comet C/2017 K2 (PANSTARRS) beyond Jupiter’s orbit
M20AP004 Yusei Koyama 36.6 16.1 20.5


AJT Panoramic SCUBA-2 mapping of dusty starburst galaxies along the huge cosmic web at z=1.5
M20AP005 Chen Fatt Lim 8 8


XJJ & HALP Reddest galaxies in the Universe
M20AP006 Gary Fuller 28
28


MGR A direct test on the role of magnetic fields in filament fragmentation
M20AP008 Eun Jung Chung 17.7
13.1 4.6

STM Role of turbulence in the formation of hub-filaments structure in L1478
M20AP009 Alexandra Tetarenko 12
7 5

AJT Mapping Jet-ISM Interaction Zones near Black Hole X-ray Binaries with HARP
M20AP010 Jianfa Wang 48


48 STM HCN(3-2) and HCO+(3-2) survey and the dense gas excitation of nearby IR-bright galaxies
M20AP016 Matthew Smith 4
4


XJJ & HALP SCUBA2 Imaging of Low-Metallicity Galaxies
M20AP018 Chandreyee Sengupta 48



48 IM Determining Molecular Gas Content of Tidal Dwarf Galaxies.
M20AP019 Daniel Perley 15 15 (including up to 3h in B1)
MGR SCUBA-2 ToO Observations of Gamma-Ray Bursts
M20AP020 Hauyu Baobab Liu 1.8

1.8

STM Dust distribution and chemical segregation in the L1157 molecular outflow
M20AP021 Kate Pattle 44.4
44.4


SL Role of the magnetic field in the fragmentation of a star forming filament in the Orion B molecular cloud
M20AP022 Kate Pattle 25.32
25.3


HALP Magnetic fields in Bok globules
M20AP023 Junhao Liu 10
10


PT & MGR Does Magnetic Field Suppress Star Formation in Galactic Center Massive Clouds?
M20AP024 Junhao Liu 8.4
8.4


HALP Are supercritical filaments supported by magnetic fields?
M20AP025 Yuhui Zhao 10

10

STM Observing Comet C/2017 K2 (PANSTARRS) with Nāmakanui
M20AP026 Lulu Fan 2.3 2.3



PT & MGR SCUBA-2 identification of a Planck-selected 550 micron Peaker
M20AP027 Shaobo Zhang 9
9


HALP Fragmentation and dust growth in L1188
M20AP029 Jun Toshikawa 8.7 8.7


STM Localizing Dust Emission in a Protocluster at z∼4
M20AP032 Ray S. Furuya 8
8


AJT Tying the au-scale to the pc-scale magnetic field in massive star forming regions
M20AP035 Chen Wang 16.3

14 2.3
STM Molecular Gas toward GGMC1 and L 1570
M20AP036 Kotaro Kohno 7.2 7.2



AJT Characterizing gravitationally lensed HST-dark ALMA-sources via SCUBA-2 450 um imaging
M20AP039 Shih-Ping Lai 19.3 19.3



XJJ & HALP The evolutionary status of prestellar cores : observations of H2D+ at 372 GHz
M20AP040 Nicolas Peretto 10.5 10.5


PT & MGR Are magnetic fields regulating the dynamical evolution of IRDCs?
M20AP042 Wei Liu 12

12

HALP Isotope ratio 18^O/17^O toward molecular clouds in the Galactic disk
M20AP043 Jae-Woo Kim 17.5

17.5

MGR Constraining the variability of the most active Brightest Cluster Galaxies in the sub-mm
M20AP044 Xiaotong Feng 29.5

29.5

AJT Refining the far-infrared SED to determine the star formation rates of quasar host galaxies
M20AP045 Cheng Cheng 16 16


AJT SCUBA2 Imaging of the Spitzer IRAC Dark Field
M20AP047 Hong-Xin Zhang 60


60
HALP Molecular Gas in a Blue Compact Dwarf Galaxy Involved in Dwarf-Dwarf Merging
M20AP048 Junhao Liu 12

12

PT & MGR Dust polarization survey of massive dense cores in Cygnus-X
M20AP051 David Alexander 16.2

16.2

AJT A joint SCUBA-2/JWST survey of the environment of high-redshift QSOs
M20AP052 Sayantan Auddy 23 23


AJT Testing the "Core Field Structure" method against dust polarization observation of H-MM1
M20AP055 Giuliana Cosentino 11.441 11.4



STM Mapping Magnetic Field in Infrared Dark Clouds
M20AP057 Jingwen Wu 15

15

HALP Continuation of Searching for Cold, Inter-arm GMCs in M33 with ultra－deep SCUBA2 imaging
M20AP058 Chuan-Peng Zhang 5



5 STM To detect shock and PDR in the inner rims of a bubble shell
M20AP060 Dimitris Stamatellos 22



22 MGR Classification of Class 0/I sub-stellar objects











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 19B version of the project. Other project allocations may also be reduced if their fallback projects from earlier semesters obtain additional data during semester 19B.











Project ID Principal Investigator Total Hrs WB FoP Title of Investigation (Color Code: Red = Target-of-Opportunity; Green = Time-specific; Italics = Daytime)
1 2 3 4 5
M20AH04 Cowie (SCUBA-2) 96 40 56


MGR The Growth of Dusty Massive Galaxies and Obscured AGNs
M20AH??? Sandell (HARP) 30

30

PF The CO emission associated with the MWC 297 molecular cloud – blocked by a very cold optically thick cloud











"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








Per / PF Per – p.friberg @ eaobservatory.org








Izumi / IM Izumi – i.mizuno @ eaobservatory.org








Shaoliang /SL Shaoliang – s.li @ eaobservatory.org








Xue-Jian / XJJ Xue-Jian – x.jiang @ eaobservatory.org








Pablo / PT Pablo – p.torne @ eaobservatory.org








Harriet / HALP Harriet – h.parsons @ eaobservatory.org








Mark / MGR Mark – m.rawlings @ eaobservatory.org








Alex / AJT Alex – a.tetarenko @ eaobservatory.org








Steve / STM Steve – s.mairs @ eaobservatory.org