ABCEFGHIJKLMNOP
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JCMT PI Programs approved for time in 22B
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PI queue
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Project IDPrincipal InvestigatorAllocated HoursFoPWeather BandTitle
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M22BP005Jorge Zavala11.5HP11.5Confirming and Characterizing Galaxy Proto-Clusters in the Early Universe
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M22BP006Kate Pattle12.5HALP12.5Magnetic fields in the nearest starburst galaxies
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M22BP007Yanan Feng41.2HALP41.2Searching for molecular HCO+ towards S-type AGB Stars
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M22BP012Kate Pattle8HP8Magnetic fields under feedback in the massive star-forming region AFGL 961
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M22BP013Zhenzhen Miao7IM7Searching for AlF molecules toward the O-rich AGB stars
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M22BP014Yan Jiang2.1HP2.1Pilot study of the star formation activity in CHANG-ES galaxies via a high-J CO line
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M22BP015Ping Zhou15.9HALP15.9Origin of the high-excitation gas near the young supernova remnant G11.2-0.3
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M22BP017Jinshi Sai4HALP4Magnetic field, turbulence and velocity gradients in dense cores of single protostars hosting multiple outflows
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M22BP020Eswaraiah Chakali7.2JL7.25Study the importance of magnetic fields in massive star formation: a case study towards Cep A
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M22BP023Daniel Perley15HP3552SCUBA-2 ToO Observations of Gamma-Ray Bursts
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M22BP025Chian-Chou Chen23.5HP1211.5Testing the ubiquity of overdensity of dusty galaxies around z~3 quasar pairs
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M22BP027Hauyu Baobab Liu25HALP817Sub-virial molecular clouds in the outer Milky Way on core to parsec scales: Short-spacing for the SMA
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M22BP030Tomoharu Oka25.1IM25.1Unveiling Gamma-ray Heartbeat Powered by the Microquasar SS 433
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M22BP031Han-Tsung Lee5.6HP5.6SDC18, a shock-compressed filament or a gravitationally collapsing sheet
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M22BP033Yi-Jehng Kuan23JL815Comet Chemistry: Targets of Opportunity and 'K2' part 2
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M22BP034Eun Jung Chung19.1JL127.1Evolution of magnetic fields in filaments and cores
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M22BP035Eun Jung Chung1.8HP1.8Role of turbulence in the formation of hub-filaments structure in L1478
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M22BP036Ellis Owen9.3HP9.3
Mapping the magnetic fields of a molecular cloud complex near the high-energy TeV source HESS J1809-193 with POL-2
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M22BP037Archana Soam5JL5Tracing the magnetic fields and grain alignment in Barnard 207 a.k.a. The Vulture head nebula
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M22BP038
Kim Ngan Nhat Nguyen
7.2JL7.2Probing star formation rates in type-1 AGNs with powerful outflows and radio jets
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M22BP040Nicolas Peretto28.8HP28.8GASTON-SL: A spectral line follow up of the GASTON project
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M22BP041Sheng-Jun Lin3SL3BISTRO-3 Complementary Observations: Mapping the Extended Emission of Starless Cores with SCUBA-2
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M22BP042Dimitris Stamatellos31.5JL31.5Warm methanol in proto-brown dwarf jets
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M22BP043Dimitris Stamatellos34.8HP34.8Nitrogen chemistry in proto-brown dwarfs
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M22BP047Junhao Liu15.2JL15.2Dust polarization survey of massive dense cores in Cygnus-X
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M22BP049Jia-Wei Wang8.5HALP8.5Interplay between Filament, Magnetic fields, Gravity, and Velocity Gradients in Quiescent Hub-Filament System
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M22BP050Shaobo Zhang10SL10Dust growth in a colliding cloud L1188
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M22BP055VINEET RAWAT5JL5Understanding the role of magnetic field in the formation and stability of dense clumps in massive molecular clouds
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M22BP056Hsi-Wei Yen27.1JL11.215.9Magnetic field structures in dense cores with embedded disks
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M22BP057Hsi-Wei Yen39JL39JCMT survey of magnetic and turbulent energy in clumps and dense cores in Perseus
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M22BP061Xue-Jian Jiang14XJJ,JL68Monitoring the activity of distant comet C/2017 K2 near its perihelion
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M22BP065Kuiyun Huang18HALP666SCUBA-2 Follow-up of IceCube Neutrino events
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M22BP066Nagayoshi Ohashi17.5NO17.5Direct Measurements of Envelope Evolution in Protostars
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M22BP074Yeonsik Kim22.3HP22.3Characterizing dust emission for galaxies with 3.3um PAH emission
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M22BP075Xunchuan Liu31HP31Search for CO 2-1 in High Velocity Cloud G165
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M22BP078Ray S. Furuya15HALP15Does alpha dynamo really maintain galaxy-scale B field?
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University of Hawaiʻi queue
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Project IDPrincipal InvestigatorAllocated HoursFoPWeather BandTitle
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12345
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M22BH25ALennox Cowie105HPA. Developing a Sample of Faint Submm Sources and Determining their Properties
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M22BH10BMichael Connelley31HPB. Direct Measurements of Envelope Evolution in Protostars
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M22BH27CJonathan Williams40JLA. Resolving Protoplanetary Disk Kinematics to Interpret JWST Spectra
B. High Contrast Spectropolarimetric Imaging of Protoplanetary Disks
C. Connecting the Magnetic Field Geometry from Cores to Disks
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M22BH37AJason T. Hinkle24JLA. Rainbow Tide: Multi-Wavelength Follow-up of Tidal Disruption Events
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Key
FOP = Friend of Project
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Red = ToO
HALP: Harriet Parsons h.parsons @ eaobservatory.org
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Magenta = Resubmission
HP: Harold Peña, h.pena @ eaobservatory.org
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Green = Time SpecificJL: Junhao Lio j.liu @ eaobservatory.org
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IM: Izumi Mizuno, i.mizuno @ eaobservatory.org
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SL: Shaoliang Li, s.li @ eaobservatory.org
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XJJ: Xue-Jian Jiang, x.jiang @ eaobservatory.org
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NO: Nagayoshi Ohashi n.ohashi @ eaobservatory.org
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Last updated: June 27th 2022
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