{"id":3943,"date":"2015-12-11T11:57:00","date_gmt":"2015-12-11T21:57:00","guid":{"rendered":"http:\/\/www.eaobservatory.org\/jcmt\/?page_id=3943"},"modified":"2015-12-11T11:57:00","modified_gmt":"2015-12-11T21:57:00","slug":"allocations-16a","status":"publish","type":"page","link":"https:\/\/www.eaobservatory.org\/jcmt\/proposals\/allocations\/allocations-16a\/","title":{"rendered":"Allocations 16A"},"content":{"rendered":"\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n
TAC-approved observing programs for JCMT , semester 16A<\/span><\/b><\/td>\n<\/tr>\n
<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/tr>\n
Project ID<\/b><\/td>\nP.I.<\/b><\/td>\nAward<\/b><\/td>\nWeather<\/b><\/td>\nRx<\/b><\/td>\nTitle of investigation<\/b><\/td>\nFoP<\/b><\/td>\n<\/tr>\n
\u00a0<\/b><\/td>\n\u00a0<\/b><\/td>\nhours<\/b><\/td>\nBand<\/b><\/td>\n\u00a0<\/b><\/td>\n\u00a0<\/b><\/td>\n\u00a0<\/b><\/td>\n<\/tr>\n
<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/tr>\n
EAO<\/b><\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/tr>\n
<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/tr>\n
M16AP005<\/td>\nNial Tanvir<\/td>\n6<\/td>\n1,2,3<\/span><\/td>\nS<\/td>\nSCUBA-2 ToO Observations of Gamma-Ray Bursts<\/td>\nHarriet<\/span><\/td>\n<\/tr>\n
M16AP006<\/td>\nNgoc Phan-Bao<\/td>\n2<\/td>\n2<\/span><\/td>\nS<\/td>\nA search for debris disks around nearby young brown dwarfs<\/td>\nHarriet<\/span><\/td>\n<\/tr>\n
M16AP007<\/td>\nJiangShui Zhang<\/td>\n10<\/td>\n5<\/span><\/td>\nA<\/td>\nOxygen isotope ratio of 18O\/17O in Galactic molecular clouds<\/td>\nJan<\/span><\/td>\n<\/tr>\n
M16AP009<\/td>\nChuan-Peng Zhang<\/td>\n75<\/td>\n5<\/span><\/td>\nA<\/td>\nThe depletion of different species in dark and dense clumps<\/td>\nPer<\/span><\/td>\n<\/tr>\n
M16AP010<\/td>\nHsi-Wei Yen<\/td>\n12<\/td>\n2<\/span><\/td>\nH<\/td>\nProbing Drift Velocity: An Assessment of Importance of Magnetic Field<\/td>\nHarriet<\/span><\/td>\n<\/tr>\n
M16AP013<\/td>\nQiong Li<\/td>\n23.5<\/td>\n2<\/span><\/td>\nS<\/td>\nStudying the dust emission and environment of the quasar sample at 5.6<z<7.1<\/td>\nMark<\/span><\/td>\n<\/tr>\n
M16AP016<\/td>\nJia-Wei Wang<\/td>\n19.75<\/td>\n2<\/span><\/td>\nH<\/td>\nGas dynamic of filaments in hub-filament region in IC5146<\/td>\nMark<\/span><\/td>\n<\/tr>\n
M16AP018<\/td>\nAlexandra Tetarenko<\/td>\n12<\/td>\n1,2,3<\/span><\/td>\nS<\/td>\nConstraining the Jet Properties of Transient X-ray Binaries<\/td>\nHarriet<\/span><\/td>\n<\/tr>\n
M16AP019<\/td>\nYi-Jehng Kuan<\/td>\n35<\/td>\n3<\/span><\/td>\nS,H<\/td>\nCatching Comet 252P\/Linear<\/td>\nIain<\/span><\/td>\n<\/tr>\n
M16AP022<\/td>\nscott chapman<\/td>\n16<\/td>\n2<\/td>\nH<\/td>\nC+ in lensed SMGs from the Herschel-red survey<\/td>\nPer<\/span><\/td>\n<\/tr>\n
M16AP025<\/td>\nChang Won Lee<\/td>\n20<\/td>\n2<\/td>\nH<\/td>\nDense Core Formation in Filamentary clouds:Accretion toward Dense Cores from Filamentary clouds and Gravitational infall in the Cores<\/td>\nJan<\/span><\/td>\n<\/tr>\n
M16AP028<\/td>\nYu Gao<\/td>\n38.3<\/td>\n4<\/td>\nA<\/td>\nHCN(3-2) along the major axes of nearby IR-bright galaxies: the dense gas excitation and HCN(3-2) – SFR correlation<\/td>\nMark<\/span><\/td>\n<\/tr>\n
M16AP029<\/td>\nGwanjeong Kim<\/td>\n10.8<\/td>\n2<\/td>\nH<\/td>\nToward All Sky Survey of Outflow Activity in Very Low Luminosity Objects<\/td>\nMark<\/span><\/td>\n<\/tr>\n
M16AP031<\/td>\nShanghuo Li<\/td>\n15<\/td>\n5<\/td>\nA<\/td>\nKinematic Structure Studies of Massive Star-forming Regions with HC3N<\/td>\nJan<\/span><\/td>\n<\/tr>\n
M16AP035<\/td>\nMichael Hogan<\/td>\n4<\/td>\n4<\/td>\nS<\/td>\n(Sub)mm Emission in Local LLAGN: A Direct View of Radiatively Inefficient Accretion?<\/td>\nMark<\/span><\/td>\n<\/tr>\n
M16AP036<\/td>\nXi Chen<\/td>\n17<\/td>\n3<\/td>\nA<\/td>\nA Search for High-frequency SiO Maser towards Water Fountain Nebulae<\/td>\nPer<\/span><\/td>\n<\/tr>\n
M16AP037<\/td>\nEun Jung Chung<\/td>\n18<\/td>\n4<\/td>\nH<\/td>\nOrigin of filament and dense core: kinematics in an intermediate-mass star-forming environment<\/td>\nJan<\/span><\/td>\n<\/tr>\n
M16AP039<\/td>\nShih-Ping Lai<\/td>\n14.5<\/td>\n1<\/td>\nH<\/td>\nThe evolutionary status of prestellar cores : observations of H2D+ at 372 GHz<\/td>\nPer<\/span><\/td>\n<\/tr>\n
M16AP040<\/td>\nChris Wilson<\/td>\n17<\/td>\n4<\/td>\nH<\/td>\nA CO survey of nearby southern galaxies<\/td>\nHarriet<\/span><\/td>\n<\/tr>\n
M16AP041<\/td>\nHelen Kirk<\/td>\n8<\/td>\n3<\/td>\nH<\/td>\nMapping Infall in a Massive Star-Forming Filament<\/td>\nMark<\/span><\/td>\n<\/tr>\n
M16AP042<\/td>\nJong Chul Lee<\/td>\n11<\/td>\n3<\/td>\nH<\/td>\nMolecular Gas Contents of Local Dust-Obscured Galaxies<\/td>\nMark<\/span><\/td>\n<\/tr>\n
M16AP046<\/td>\nDavid Eden<\/td>\n5<\/td>\n1<\/td>\nS<\/td>\nExtreme star formation in the Milky Way: A comparative study of the W49A and W51 star-forming regions<\/td>\nHarriet<\/span><\/td>\n<\/tr>\n
M16AP047<\/td>\nWalter Gear<\/td>\n4<\/td>\n1<\/td>\nS<\/td>\nThe highest redshift clusters as a laboratory of galaxy and star formation evolution<\/td>\nMark<\/span><\/td>\n<\/tr>\n
M16AP049<\/td>\nLei Qian<\/td>\n20<\/td>\n4<\/td>\nA<\/td>\nPilot study on the molecular gas of nearby galaxies hosting intermediate-mass black holes<\/td>\nPer<\/span><\/td>\n<\/tr>\n
M16AP051<\/td>\nChian-Chou Chen<\/td>\n10<\/td>\n2<\/td>\nS<\/td>\nDusty starbursts within and around HzRGs with SCUBA-2<\/td>\nJan<\/span><\/td>\n<\/tr>\n
M16AP052<\/td>\nHao Chen<\/td>\n27<\/td>\n3<\/td>\nH<\/td>\nHCN 4-3 Map in the Central Disk of M51<\/td>\nMark<\/span><\/td>\n<\/tr>\n
M16AP053<\/td>\nIan Smail<\/td>\n29.5<\/td>\n1,2<\/td>\nS<\/td>\nEnvironmental influences on the diversity of ULIRG populations in z~1-1.5 clusters<\/td>\nHarriet<\/span><\/td>\n<\/tr>\n
M16AP055<\/td>\nMichal Michalowski<\/td>\n21<\/td>\n2<\/td>\nS<\/td>\nStar-formation in the host galaxies and environments of the high-redshift quasars<\/td>\nMark<\/span><\/td>\n<\/tr>\n
M16AP057<\/td>\nQinghua Tan<\/td>\n10.6<\/td>\n3<\/td>\nH<\/td>\nCO J=4-3 emission of ultraluminous infrared galaxies and QSOs at z>~0.3<\/td>\nJan<\/span><\/td>\n<\/tr>\n
M16AP058<\/td>\nShunya Takekawa<\/td>\n76.5<\/td>\n3,4<\/td>\nH,A<\/td>\nTracing Kinematics and Physical Conditions of the Central 20 pc of our Galaxy<\/td>\nHarriet<\/span><\/td>\n<\/tr>\n
M16AP059<\/td>\nYuqing Lou<\/td>\n3.8<\/td>\n2,3,4<\/td>\nS,H,A<\/td>\nStudy of the forming region of an isolated pre-Brown dwarf or giant gas planet: The case of mini gas globule B71<\/td>\nIain<\/span><\/td>\n<\/tr>\n
M16AP060<\/td>\nIan Smail<\/td>\n4.2<\/td>\n3<\/td>\nS<\/td>\nUltraluminous starburst activity as the origin of the Inverse Compton X-ray emission in B3 J0727+409<\/td>\nJan<\/span><\/td>\n<\/tr>\n
M16AP061<\/td>\nKevin Lacaille<\/td>\n15<\/td>\n2<\/td>\nH<\/td>\nDetecting [NII] in lensed z~3 SMGs from the Planck Dusty-GEMS survey<\/td>\nHarriet<\/span><\/td>\n<\/tr>\n
M16AP062<\/td>\nJae-Woo Kim<\/td>\n11.5<\/td>\n2<\/td>\nS<\/td>\nSub-mm mapping of distant, massive galaxy clusters with SCUBA-2<\/td>\nMark<\/span><\/td>\n<\/tr>\n
M16AP064<\/td>\nSerena Viti<\/td>\n11.124<\/td>\n2,3<\/td>\nH,A<\/td>\nTriggered star formation in the gravitationally perturbed galaxy NGC 4449<\/td>\nJan<\/span><\/td>\n<\/tr>\n
M16AP067<\/td>\nHyunju Yoo<\/td>\n2<\/td>\n2<\/td>\nH<\/td>\nHCN (4\u00e2??3) Line Mapping of High-mass Infall Candidates<\/td>\nIain<\/span><\/td>\n<\/tr>\n
M16AP069<\/td>\nSasha Hinkley<\/td>\n4.465<\/td>\n3<\/td>\nS<\/td>\nSCUBA-2 Imaging of a Young Solar System Analogue<\/td>\nHarriet<\/span><\/td>\n<\/tr>\n
M16AP070<\/td>\nXin Zhou<\/td>\n35<\/td>\n5<\/td>\nA<\/td>\nShocked Molecular Filament in Supernova Remnant G127.1+0.5<\/td>\nHarriet<\/span><\/td>\n<\/tr>\n
M16AP071<\/td>\nHui Zhu<\/td>\n8<\/td>\n5<\/td>\nA<\/td>\nDoes the SNR G40.5-0.5 interact with a molecular cloud and have a contribution to the northern TeV emission of MGRO J1908+06?<\/td>\nJan<\/span><\/td>\n<\/tr>\n
M16AP074<\/td>\nXuefang Xu<\/td>\n12<\/td>\n3<\/td>\nH<\/td>\nThe Angular Momentum of Dense Clumps in Molecular Clouds<\/td>\nPer<\/span><\/td>\n<\/tr>\n
M16AP076<\/td>\nEmily Drabek-Maunder<\/td>\n23.6<\/td>\n4,5<\/td>\nA<\/td>\nMolecules from below the surface of icy outer moons<\/td>\nIain<\/span><\/td>\n<\/tr>\n
M16AP079<\/td>\nNingyu Tang<\/td>\n9.6<\/td>\n3<\/td>\nH<\/td>\nHCO+(4-3) observations toward CO Dark Molecular Gas with Extinction Av > 1.5 mag<\/td>\nJan<\/span><\/td>\n<\/tr>\n
M16AP081<\/td>\nYuji Urata<\/td>\n6<\/td>\n3<\/td>\nS<\/td>\nSystematic Rapid Search for Reverse Shock Emissions Associated with Gamma-Ray Bursts<\/td>\nIain<\/span><\/td>\n<\/tr>\n
M16AP082<\/td>\nXiaohu Li<\/td>\n24<\/td>\n5<\/td>\nA<\/td>\nSeeking molecular SiS in the S-type AGB star Chi Cyg<\/td>\nPer<\/span><\/td>\n<\/tr>\n
M16AP083<\/td>\nAlastair Edge<\/td>\n3<\/td>\n3<\/td>\nS<\/td>\nMonitoring the extraordinarily inverted core of NGC5044<\/td>\nHarriet<\/span><\/td>\n<\/tr>\n
M16AP084<\/td>\nHideo Sagawa<\/td>\n54<\/td>\n1,2,3,4<\/td>\nH,A<\/td>\nChlorine and Sulfur Chemistry of the Venus Dayside Atmosphere<\/td>\nIain<\/span><\/td>\n<\/tr>\n
M16AP087<\/td>\nJeeseon Song<\/td>\n7.2<\/td>\n2<\/td>\nS<\/td>\nGalaxy Population Study for High-redshift Hubble Space Telescope (HST) Massive Galaxy Cluster And Dusty High-redshift Galaxies at 450\/850micron<\/td>\nIain<\/span><\/td>\n<\/tr>\n
M16AP088<\/td>\nZhiyuan Ren<\/td>\n16<\/td>\n3,4<\/td>\nS,H<\/td>\nGas Flow in Dense Gas Filaments<\/td>\nJan<\/span><\/td>\n<\/tr>\n
<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/tr>\n
Project ID<\/b><\/td>\nP.I.<\/b><\/td>\nAward<\/b><\/td>\nWeather<\/b><\/td>\nRx<\/b><\/td>\nTitle of investigation<\/b><\/td>\nFoP<\/b><\/td>\n<\/tr>\n
\u00a0<\/b><\/td>\n\u00a0<\/b><\/td>\nhours<\/b><\/td>\nBand<\/b><\/td>\n\u00a0<\/b><\/td>\n\u00a0<\/b><\/td>\n\u00a0<\/b><\/td>\n<\/tr>\n
Univ. Hawaii<\/b><\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/tr>\n
m16ah01a<\/td>\nJonathan Williams<\/td>\n18<\/td>\n2,3<\/td>\nS<\/td>\nProtostellar Variability at Submillimeter Wavelengths<\/td>\nIain<\/td>\n<\/tr>\n
m16ah07b<\/td>\nLennox Cowie<\/td>\n56<\/td>\n2<\/td>\nS<\/td>\nA submillimeter survey of the GOODS\/CANDELS\/Chandra deep fields<\/td>\nMark<\/td>\n<\/tr>\n
m16ah08c<\/td>\nTucker Jones<\/td>\n16<\/td>\n2<\/td>\nS<\/td>\nThe interstellar gas content of galaxies at z=2<\/td>\nJan<\/td>\n<\/tr>\n
m16ah11b<\/td>\nDave Sanders<\/td>\n32<\/td>\n2,3<\/td>\nS<\/td>\nThe Morphology of Dust-obscured, Massive Starbursts<\/td>\nHarriet<\/td>\n<\/tr>\n
m16ah16a<\/td>\nLi-Yen Hsu<\/td>\n58<\/td>\n1,2<\/td>\nS<\/td>\nCharacterizing Faint Submillimeter Galaxies with Cluster Lensing<\/td>\nIain<\/td>\n<\/tr>\n
<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/tr>\n
<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/tr>\n
<\/td>\n<\/td>\n<\/td>\nFoPs<\/td>\n<\/td>\nHarriet Parsons h.parsons @ eaobservatory.org<\/td>\n<\/td>\n<\/tr>\n
<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\nJessica Dempsey j.dempsey @ eaobservatory.org<\/td>\n<\/td>\n<\/tr>\n
<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\nJan Wouterloot j.wouterloot @ eaobservatory.org<\/td>\n<\/td>\n<\/tr>\n
<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\nPer Friberg p.friberg @ eaobservatory.org<\/td>\n<\/td>\n<\/tr>\n
<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\nMark Rawlings m.rawlings @ eaobservatory.org<\/td>\n<\/td>\n<\/tr>\n
<\/td>\n<\/td>\n<\/td>\n<\/td>\n<\/td>\nIain Coulson i.coulson @ eaobservatory.org<\/td>\n<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n","protected":false},"excerpt":{"rendered":"

TAC-approved observing programs for JCMT , semester 16A Project ID P.I. Award Weather Rx Title of investigation FoP \u00a0 \u00a0 hours Band \u00a0 \u00a0 \u00a0 EAO M16AP005 Nial Tanvir 6 1,2,3 S SCUBA-2 ToO Observations of Gamma-Ray Bursts Harriet M16AP006 Ngoc Phan-Bao 2 2 S A search for debris disks\u2026 Continue reading<\/a><\/p>\n","protected":false},"author":7,"featured_media":0,"parent":3251,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":[],"_links":{"self":[{"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/pages\/3943"}],"collection":[{"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/users\/7"}],"replies":[{"embeddable":true,"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/comments?post=3943"}],"version-history":[{"count":1,"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/pages\/3943\/revisions"}],"predecessor-version":[{"id":3944,"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/pages\/3943\/revisions\/3944"}],"up":[{"embeddable":true,"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/pages\/3251"}],"wp:attachment":[{"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/media?parent=3943"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}