BCEFGHIJKLMNOP
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JCMT PI Programs approved for time in 23A
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PI queue
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Project IDPrincipal InvestigatorAllocated HoursFoPWeather BandTitle
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M23AP001Eun Jung Chung2.4JL2.4Does the energy balance of gravity, turbulence, and magnetic field determine the fragmentation types of filamentary molecular clouds?
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M23AP002Kate Pattle7.3HALP7.3Magnetic Fields in the UCHII Region G5.89-0.39
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M23AP004Tatsumi Ishikawa1.5HALP1.5Detailed Study of Dust Emission associated with W50/SS443
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M23AP006Ian Smail4.2HP4.2A JCMT+JWST survey through the massive cluster lens A1489
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M23AP007Nguyen Bich Ngoc8.7JL8.7Characterizing magnetic fields and probing dust physics using dust polarization from the head of the Snake filament (IFDC G11.11 -0.12)
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M23AP008Christian A. Flores Gonzalez33NO33.0Direct Measurements of Envelope Evolution in Protostars
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M23AP009Yi-Jehng Kuan30JL30.0Comet Chemistry: C/2022 E3 (ZTF) and 12P/Pons-Brooks
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M23AP010David Eden23.2IM23.2Optically Thin Tracers Towards MAJORS Sources
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M23AP011Tomomi Shimoikura26.5HALP19.07.5Revealing the velocity structure of a giant filament associated with the GGD 12-15 cluster-forming clump
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M23AP012Nguyen Bich Ngoc14.3HP14.3Understanding the low star-formation efficiency in Auriga-California molecular cloud: the role of magnetic fields
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M23AP017Liu Shuai2.2HP2.2Dust continuum observation towards a Hot dust obscured galaxy
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M23AP018Daniel Perley15HP3.05.05.02.0SCUBA-2 ToO Observations of Gamma-Ray Bursts
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M23AP019Jihye Hwang14JL14.0The role of magnetic field in a prestellar core, Barnard 68
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M23AP020Jinshi Sai33.6NO33.6Impact of Dense Core Properties on Disk Size
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M23AP022Juan Carlos Algaba13HALP13.0Unveiling the innermost physical conditions of blazar cores via multi frequency rotation measure variability with the JCMT and the KVN
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M23AP023Kim Ngan Nhat Nguyen14.7HP14.7Probing star formation rates in type-1 AGNs
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M23AP026Doris Arzoumanian18.8JL18.8Magnetic field observations towards dense star-forming clumps of RCW 120
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M23AP028Tianxian Luo14.1JL14.1Mapping the magnetic field morphology of the Crab Nebula at the submillimeter wavelength
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M23AP030Yoshiki Toba6HP6.0Tracing co-evolution of galaxy and SMBH for extremely luminous infrared galaxies discovered by eROSITA
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M23AP031Jonathan Marshall7.3JL2.12.82.4SCUBA-2 monitoring of Betelgeuse
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M23AP032Arup Kumar Maity14.8HALP14.8JCMT/SCUBA-2/POL-2 Polarization observations toward AFGL 5180 and AFGL 6366
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M23AP033Tian-wen Cao21.1HP21.1The Molecular Gas Content in Edge-on Low Surface Brightness Galaxies
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M23AP034Archana Soam1.8JL1.8Tracing the magnetic fields and grain alignment in Barnard 207 a.k.a. The Vulture head nebula
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M23AP037Sheng-Jun Lin26JL15.610.4Catching the 3-dimensional Magnetic Fields at Birth of a Dark Molecular Cloud
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M23AP038Kate Pattle17.8SL17.8Magnetic fields under stellar feedback in NGC 6357
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M23AP039Janik Karoly6.9HALP5.91.0Testing grain alignment of carbonaceous and silicate grains in the envelopes of AGB stars
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M23AP043Qilao Gu8.4HALP8.4Magnetic field of the W43-main cloud
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M23AP044Ekta Sharma8.5JL8.5Magnetic fields towards two massive clouds in different environments
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M23AP046Jia-Wei Wang13.3HALP8.05.3
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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M23AP047Kuiyun Huang18HALP6.06.06.0SCUBA-2 Follow-up of IceCube Neutrino events
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M23AP049Chian-Chou Chen9.8HP9.8Obscured star formation in and around X-ray selected protoclusters at z=1-1.5
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M23AP050Nicolas Peretto76.7HP26.650.1GASTON-SL: A spectral line follow up of the GASTON project
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M23AP052Stephen Eales8.5HP8.5Protoclusters in the Epoch of Reionisation - a Joint JCMT and LMT Project
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M23AP053Gary Fuller18JL18.0The Magnetic Field Structure in the Massive Clumps in the Filamentary Infrared Dark Cloud Fil24
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M23AP054Shang-Jing Lin8.6JL8.6Origins of the warped protostellar envelope around the Class 0 protostar Per-emb-8
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M23AP055Jorge Zavala12HP12.0Confirming and Characterizing Galaxy Proto-Clusters in the Early Universe
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M23AP056Kuiyun Huang33.3HP33.3Starforming galaxies as Neutrino counterparts
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M23AP058Dimitris Stamatellos36HALP36.0Classification of Class 0/I sub-stellar objects
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M23AP061Sandhyarani Panigrahy10.9JL10.9Revealing the imprints of cloud-cloud collision on the magnetic field morphology
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KeyFOP = Friend of Project
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Red = ToOHALP: Harriet Parsons 10
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Magenta = ResubmissionHP: Harold Peña12
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Green = Time SpecificJL: Junhao Liu12
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IM: Izumi Mizuno1Last updated: January 3rd 2023
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SL: Shaoliang Li1
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NO: Nagayoshi Ohashi 2
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