| JCMT Projects Approved for Observation in Semester 19B | ||||||||||
| Updated: 2019/07/15 | ||||||||||
| 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) | ||||||||||
| M19BP001 | Peter Scicluna | 22 | 22 | Harriet | Testing radiative dust alignment using stellar winds | |||||
| M19BP003 | Peter Scicluna | 34.2 | 34.2 | Jan | The Nearby Evolved Stars Survey: Mapping evolved-star envelopes on arcminute scales | |||||
| M19BP006 | Zongnan Li | 59 | 19 | 40 | Jan | JCMT CO(3-2) mapping of the nuclear ring of M31 | ||||
| M19BP009 | Shaobo Zhang | 29 | 29 | Harriet | Fragmentation and dust growth in L1188 | |||||
| M19BP010 | Mattia Negrello | 20.2177 | 20.2177 | Alex | A systematic search for ultra-bright strongly lensed galaxies in the Planck all-sky survey | |||||
| M19BP011 | Qiong Li | 18.3 | 18.3 | Harriet | Completing a SCUBA-2 survey of most massive large-scale structures at z~2 | |||||
| M19BP014 | Qilao Gu | 17 | 17 | Jan | Verify Turbulence driven Ambipolar Diffusion (TAD) by line-width differences variations. | |||||
| M19BP015 | Minchul Kam | 8 | 8 (2 × 4h epochs) | Steve | Revealing the nature of blazar radio cores through multifrequency polarimetric observations with the JCMT, SMA, and KVN | |||||
| M19BP018 | Peter Scicluna | 35 | 35 | Alex | Are Carbon stars the only detached-shell sources? | |||||
| M19BP019 | Tie Liu | 9.1 | 9.1 | Jan | Tracing the pinched magnetic fields caused by accretion flows along filaments (resubmission of M19AP032) | |||||
| M19BP022 | Daniel Perley | 15 | 15 (including up to 3h in B1) | Mark | SCUBA-2 ToO Observations of Gamma-Ray Bursts | |||||
| M19BP025 | Alexandra Tetarenko | 18 | 18 | Alex | Constraining Jet Formation and Evolution with Transient X-ray Binaries | |||||
| M19BP028 | Ying-Tung Chen | 5 | 5 | Steve | Massive Dust Coma in Long Period Comet C/2017 K2 | |||||
| M19BP030 | Sayantan Auddy | 28 | 28 | Alex | Testing the "Core Field Structure" method against dust polarization observation of H-MM1 | |||||
| M19BP031 | Myungshin Im | 13 | 13 | Steve | Completing the SCUBA-2 observations of the JWST/GTO Time Domain Survey Field | |||||
| M19BP032 | Aaron Golden | 10 | 10 | Alex | 'Snow plows' through the local ISM - using nearby pulsars as probes of interstellar dust | |||||
| M19BP033 | Ke Wang | 43.8 | 15.1 | 28.7 | Jan | Global collapse during high-mass star formation: a mini survey | ||||
| M19BP034 | Rajeshwari Dutta | 35 | 35 | Per | Investigating Molecular Gas Properties in Low-z Radio-loud Galaxy Mergers | |||||
| M19BP037 | Junhao Liu | 4.6 | 4.6 | Mark | Dust polarization survey of massive dense cores in Cygnus-X | |||||
| M19BP038 | Jae-Woo Kim | 19 | 19 | Mark | Constraining the variability of the most active Brightest Cluster Galaxies in the sub-mm | |||||
| M19BP039 | Yi-Jehng Kuan | 26 | 26 | Steve | Comet Chemistry: Target of Opportunity request | |||||
| M19BP041 | Xiaotong Feng | 10 | 10 | Per | Study the star formation rates of AGN host galaxies by far-infrared SED | |||||
| M19BP042 | Jia-Wei Wang | 16 | 16 | Steve | How the magnetic field impact on the formation of hub-filament system G33.92+0.11 – 19A VERSION COMPLETED (CONTINGENCY TIME NO LONGER NEEDED) | |||||
| M19BP045 | Lulu Fan | 16.8 | 16.8 | Harriet | SCUBA-2 Observations of Herschel-selected ULIRGs at z>4 | |||||
| M19BP046 | Giuliana Cosentino | 11.441 | 11.441 | Steve | Mapping Magnetic Field in Infrared Dark Clouds | |||||
| M19BP047 | Guang-Xing Li | 10 | 10 | Jan | Mapping a cometary globule with a conical shape using CO isotopes | |||||
| M19BP048 | Michele Fumagalli | 30 | 30 | Harriet | A Systematic Search for Dusty Starbursts around z~3-4 Quasars | |||||
| M19BP049 | Li-Hwai Lin | 23.77 | 23.77 | Alex | Observing CO(2-1) in Red Star-forming Galaxies | |||||
| M19BP050 | Wei Liu | 150 | 150 | Jan | Isotope ratio 18^O/17^O toward molecular clouds in the Galactic disk | |||||
| M19BP051 | Patrick Koch | 6.4 | 6.4 | (N/A) | Mapping the B-Field towards a Filamentary Hub-System – 19A VERSION COMPLETED (CONTINGENCY TIME NO LONGER NEEDED) | |||||
| M19BP053 | Jim Geach | 7.5 | 7.5 | Alex | Measuring the total infrared luminosity of a galaxy driving a fast multi-phase outflow | |||||
| M19BP054 | Jingwen Wu | 7.6 | 7.6 | Harriet | Searching For Cold, Inter-arm GMCs in M33 with ultra-deep SCUBA2 imaging | |||||
| M19BP056 | Yu Sophia Dai | 2 | 2 | Alex | Constraining the far-IR properties with JCMT for the extremely rare, infra'red' dusty LBGs | |||||
| M19BP057 | Xunchuan Liu | 9 | 9 | Steve | Line maps with JCMT towards Shock Carbon Chain Chemistry region L1251-A | |||||
| M19BP058 | Nicolas Peretto | 32.85 | 32.85 | Per | Are magnetic fields regulating the dynamical evolution of IRDCs? | |||||
| M19BP059 | Yuan Lixia | 10.8 | 10.8 | Steve | Follow-up observation of the extended filamentary structure S242 | |||||
| M19BP060 | David Alexander | 10.4 | 10.4 | Alex | A joint SCUBA-2/JWST survey of the environment of high-redshift QSOs | |||||
| M19BP061 | Eswaraiah Chakali | 9.5 | 9.5 | Harriet | Unveiling the magnetic fields in a massive star/cluster forming clump Cepheus A East | |||||
| M19BP062 | Eswaraiah Chakali | 3.8 | 3.8 | Harriet | Are the magnetic fields guide filamentary flows to feed the massive star forming clump? | |||||
| 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 19A version of the project. | ||||||||||
| 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 | ||||||
| M19BH04A | Cowie (SCUBA-2) | 96 | 96 | Mark | The Growth of Dusty Massive Galaxies and Obscured AGNs | |||||
| M19BH16A1 | Reipurth (HARP) | 30 | 30 | Per | Destruction Of A Dense Globule (HARP) | |||||
| M19BH16A2 | Reipurth (SCUBA-2) | 12 | 12 | Per | Destruction Of A Dense Globule (SCUBA-2) | |||||
| "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 | |||||||||
| Jan / JGW | Jan - - - - j .wouterloot @ eaobservatory.org | |||||||||
| Jess / JTD | Jessica - - j.dempsey @ 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 | |||||||||