{"id":3248,"date":"2015-07-07T14:09:11","date_gmt":"2015-07-08T00:09:11","guid":{"rendered":"http:\/\/www.eaobservatory.org\/jcmt\/?page_id=3248"},"modified":"2015-07-07T14:32:30","modified_gmt":"2015-07-08T00:32:30","slug":"allocations-15b","status":"publish","type":"page","link":"https:\/\/www.eaobservatory.org\/jcmt\/proposals\/allocations\/allocations-15b\/","title":{"rendered":"Allocations 15B"},"content":{"rendered":"<table border=\"0\" cellspacing=\"0\">\n<tbody>\n<tr>\n<td align=\"CENTER\" height=\"16\">Project ID<\/td>\n<td align=\"LEFT\">P.I.<\/td>\n<td align=\"CENTER\">Award<\/td>\n<td align=\"CENTER\">Weather<\/td>\n<td align=\"CENTER\">Rx<\/td>\n<td align=\"LEFT\">Title of investigation<\/td>\n<td align=\"CENTER\">FoP<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"15\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\">hours<\/td>\n<td align=\"CENTER\">Band<\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"15\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"15\"><b>EAO<\/b><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"15\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi003<\/td>\n<td align=\"LEFT\">Tomoya Hirota<\/td>\n<td align=\"CENTER\">20<\/td>\n<td align=\"CENTER\">3<\/td>\n<td align=\"CENTER\">H<\/td>\n<td align=\"LEFT\">Survey of the vibrationally excited H2O lines in nearby massive YSO&#8230;<\/td>\n<td align=\"CENTER\">imc<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi004<\/td>\n<td align=\"LEFT\">Kazushi Sakamoto<\/td>\n<td align=\"CENTER\">2<\/td>\n<td align=\"CENTER\">1<\/td>\n<td align=\"CENTER\">H<\/td>\n<td align=\"LEFT\">Dense &amp; Warm Gas in a Starburst Merger<\/td>\n<td align=\"CENTER\">imc<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi006<\/td>\n<td align=\"LEFT\">Ian Smail<\/td>\n<td align=\"CENTER\">30<\/td>\n<td align=\"CENTER\">1,2<\/td>\n<td align=\"CENTER\">S<\/td>\n<td align=\"LEFT\">A SCUBA-2 survey of three z~1-1.5 clusters: catching cluster ellipt&#8230;<\/td>\n<td align=\"CENTER\">halp<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi007<\/td>\n<td align=\"LEFT\">Damian Rumble<\/td>\n<td align=\"CENTER\">2<\/td>\n<td align=\"CENTER\">4<\/td>\n<td align=\"CENTER\">H<\/td>\n<td align=\"LEFT\">Active star formation in W40 complex: how the most massive stars ar&#8230;<\/td>\n<td align=\"CENTER\">jgw<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"15\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi009<\/td>\n<td align=\"LEFT\">fei li<\/td>\n<td align=\"CENTER\">7<\/td>\n<td align=\"CENTER\">4<\/td>\n<td align=\"CENTER\">A<\/td>\n<td align=\"LEFT\">Dense gas tracers and their isotopes in nearby infrared bright gala&#8230;<\/td>\n<td align=\"CENTER\">imc<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi010<\/td>\n<td align=\"LEFT\">Michal Michalowski<\/td>\n<td align=\"CENTER\">3<\/td>\n<td align=\"CENTER\">2<\/td>\n<td align=\"CENTER\">S<\/td>\n<td align=\"LEFT\">A direct measurement of the dust destruction timescale in passive g&#8230;<\/td>\n<td align=\"CENTER\">halp<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi012<\/td>\n<td align=\"LEFT\">Hannah Calcutt<\/td>\n<td align=\"CENTER\">8<\/td>\n<td align=\"CENTER\">3<\/td>\n<td align=\"CENTER\">H<\/td>\n<td align=\"LEFT\">Characterising the emission of methyl formate in hot molecular cores<\/td>\n<td align=\"CENTER\">jgw<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi013<\/td>\n<td align=\"LEFT\">Gwanjeong Kim<\/td>\n<td align=\"CENTER\">6<\/td>\n<td align=\"CENTER\">3<\/td>\n<td align=\"CENTER\">H<\/td>\n<td align=\"LEFT\">Toward All Sky Survey of Outflow Activity in Very Low Luminosity Ob..<\/td>\n<td align=\"CENTER\">halp<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"15\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi016<\/td>\n<td align=\"LEFT\">Lulu Fan<\/td>\n<td align=\"CENTER\">12<\/td>\n<td align=\"CENTER\">3<\/td>\n<td align=\"CENTER\">S<\/td>\n<td align=\"LEFT\">SCUBA-2 850 um observations of WISE-selected Hot,Dust-obscured Galaxie<\/td>\n<td align=\"CENTER\">halp<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi019<\/td>\n<td align=\"LEFT\">Hsi-Wei Yen<\/td>\n<td align=\"CENTER\">24<\/td>\n<td align=\"CENTER\">2<\/td>\n<td align=\"CENTER\">H<\/td>\n<td align=\"LEFT\">Signpost of Effective Magnetic Field: Probing Drift Velocity<\/td>\n<td align=\"CENTER\">pf<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi021<\/td>\n<td align=\"LEFT\">Chuan-Peng Zhang<\/td>\n<td align=\"CENTER\">16<\/td>\n<td align=\"CENTER\">2<\/td>\n<td align=\"CENTER\">H<\/td>\n<td align=\"LEFT\">H2D+ in Massive Infrared Quiet Cores<\/td>\n<td align=\"CENTER\">pf<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi025<\/td>\n<td align=\"LEFT\">Alastair Edge<\/td>\n<td align=\"CENTER\">4<\/td>\n<td align=\"CENTER\">1,3<\/td>\n<td align=\"CENTER\">S<\/td>\n<td align=\"LEFT\">Monitoring the extraordinarily inverted core of NGC5044<\/td>\n<td align=\"CENTER\">jgw<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"15\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi028<\/td>\n<td align=\"LEFT\">Eleni Kalfountzou<\/td>\n<td align=\"CENTER\">5<\/td>\n<td align=\"CENTER\">2<\/td>\n<td align=\"CENTER\">S<\/td>\n<td align=\"LEFT\">Submillimeter emission in binary QSOs<\/td>\n<td align=\"CENTER\">halp<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi036<\/td>\n<td align=\"LEFT\">Alexandra Tetarenko<\/td>\n<td align=\"CENTER\">12<\/td>\n<td align=\"CENTER\">1,2,3<\/td>\n<td align=\"CENTER\">S<\/td>\n<td align=\"LEFT\">Constraining the Jet Properties of Transient X-ray Binaries<\/td>\n<td align=\"CENTER\">jgw<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi038<\/td>\n<td align=\"LEFT\">Walter Gear<\/td>\n<td align=\"CENTER\">8<\/td>\n<td align=\"CENTER\">1<\/td>\n<td align=\"CENTER\">S<\/td>\n<td align=\"LEFT\">The highest redshift clusters as a laboratory of galaxy and star fo.<\/td>\n<td align=\"CENTER\">halp<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi041<\/td>\n<td align=\"LEFT\">A-Ran Lyo<\/td>\n<td align=\"CENTER\">30<\/td>\n<td align=\"CENTER\">3<\/td>\n<td align=\"CENTER\">S<\/td>\n<td align=\"LEFT\">SCUBA-2 survey of New Debris Disks from WISE<\/td>\n<td align=\"CENTER\">imc<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"15\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi042<\/td>\n<td align=\"LEFT\">Xue-Jian Jiang<\/td>\n<td align=\"CENTER\">27<\/td>\n<td align=\"CENTER\">4<\/td>\n<td align=\"CENTER\">H<\/td>\n<td align=\"LEFT\">CCH 4-3 mapping of massive star forming regions using HARP<\/td>\n<td align=\"CENTER\">jgw<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi046<\/td>\n<td align=\"LEFT\">Shih-Ping Lai<\/td>\n<td align=\"CENTER\">32<\/td>\n<td align=\"CENTER\">1<\/td>\n<td align=\"CENTER\">H<\/td>\n<td align=\"LEFT\">The evolutionary status of prestellar cores : observations of H2D+ ..<\/td>\n<td align=\"CENTER\">pf<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi047<\/td>\n<td align=\"LEFT\">Ciska Kemper<\/td>\n<td align=\"CENTER\">40<\/td>\n<td align=\"CENTER\">2,3<\/td>\n<td align=\"CENTER\">S,H<\/td>\n<td align=\"LEFT\">The spatially resolved mass-loss history of nearby Asymptotic Giant..<\/td>\n<td align=\"CENTER\">jgw<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi048<\/td>\n<td align=\"LEFT\">Jae-Woo Kim<\/td>\n<td align=\"CENTER\">15<\/td>\n<td align=\"CENTER\">2<\/td>\n<td align=\"CENTER\">S<\/td>\n<td align=\"LEFT\">Sub-mm mapping for a supercluster at z~0.91 with SCUBA-2<\/td>\n<td align=\"CENTER\">halp<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"15\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi051<\/td>\n<td align=\"LEFT\">Nial Tanvir<\/td>\n<td align=\"CENTER\">12<\/td>\n<td align=\"CENTER\">1,2,3<\/td>\n<td align=\"CENTER\">S<\/td>\n<td align=\"LEFT\"><span style=\"color: #ff0000\">SCUBA-2 ToO Observations of Gamma-Ray Bursts<\/span><\/td>\n<td align=\"CENTER\">imc<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi052<\/td>\n<td align=\"LEFT\">Stephen Serjeant<\/td>\n<td align=\"CENTER\">40<\/td>\n<td align=\"CENTER\">1<\/td>\n<td align=\"CENTER\">S<\/td>\n<td align=\"LEFT\">The SCUBA-2 NEP Deep Survey: illuminating the galaxy main sequence<\/td>\n<td align=\"CENTER\">imc<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi053<\/td>\n<td align=\"LEFT\">Tadayuki Kodama<\/td>\n<td align=\"CENTER\">88<\/td>\n<td align=\"CENTER\">2<\/td>\n<td align=\"CENTER\">S<\/td>\n<td align=\"LEFT\">Deep submm imaging of dusty starbursts in proto-clusters at 2&lt;z&lt;6: .<\/td>\n<td align=\"CENTER\">halp<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi055<\/td>\n<td align=\"LEFT\">Ran Wang<\/td>\n<td align=\"CENTER\">24<\/td>\n<td align=\"CENTER\">2<\/td>\n<td align=\"CENTER\">S<\/td>\n<td align=\"LEFT\">Dust emission and environment of the most distant quasars<\/td>\n<td align=\"CENTER\">halp<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"15\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi057<\/td>\n<td align=\"LEFT\">Hong Wu<\/td>\n<td align=\"CENTER\">60<\/td>\n<td align=\"CENTER\">5<\/td>\n<td align=\"CENTER\">A<\/td>\n<td align=\"LEFT\">CO(2-1) Detection of HI-rich Low Surface Brightness Galaxies<\/td>\n<td align=\"CENTER\">jgw<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi058<\/td>\n<td align=\"LEFT\">Danielle Fenech<\/td>\n<td align=\"CENTER\">5<\/td>\n<td align=\"CENTER\">2,4,5<\/td>\n<td align=\"CENTER\">S<\/td>\n<td align=\"LEFT\">Constraining clumping in the winds of Wolf-Rayet stars<\/td>\n<td align=\"CENTER\">jgw<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi059<\/td>\n<td align=\"LEFT\">Mark Thompson<\/td>\n<td align=\"CENTER\">40<\/td>\n<td align=\"CENTER\">2,4<\/td>\n<td align=\"CENTER\">S,A<\/td>\n<td align=\"LEFT\">Determining the nature of SASSy sources<\/td>\n<td align=\"CENTER\">imc<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi060<\/td>\n<td align=\"LEFT\">Ting Xiao<\/td>\n<td align=\"CENTER\">30<\/td>\n<td align=\"CENTER\">4,5<\/td>\n<td align=\"CENTER\">A<\/td>\n<td align=\"LEFT\">Pilot CO Follow-up of the MaNGA Survey with JCMT<\/td>\n<td align=\"CENTER\">jtd<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"15\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi061<\/td>\n<td align=\"LEFT\">Tie Liu<\/td>\n<td align=\"CENTER\">35<\/td>\n<td align=\"CENTER\">4<\/td>\n<td align=\"CENTER\">S<\/td>\n<td align=\"LEFT\">Dust properties of Planck cold clumps<\/td>\n<td align=\"CENTER\">halp<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi063<\/td>\n<td align=\"LEFT\">Mark Thompson<\/td>\n<td align=\"CENTER\">12<\/td>\n<td align=\"CENTER\">3<\/td>\n<td align=\"CENTER\">H,A<\/td>\n<td align=\"LEFT\">Confirming the first known isolated proto-brown dwarf<\/td>\n<td align=\"CENTER\">jgw<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi064<\/td>\n<td align=\"LEFT\">Mark Thompson<\/td>\n<td align=\"CENTER\">10<\/td>\n<td align=\"CENTER\">1<\/td>\n<td align=\"CENTER\">S<\/td>\n<td align=\"LEFT\">SCUBA-2 photometry of extreme debris disks discovered in the Hersch&#8230;<\/td>\n<td align=\"CENTER\">jgw<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi067<\/td>\n<td align=\"LEFT\">qian jiao<\/td>\n<td align=\"CENTER\">40<\/td>\n<td align=\"CENTER\">5<\/td>\n<td align=\"CENTER\">S,A<\/td>\n<td align=\"LEFT\">JCMT follow-up observe of HIghMass galaxies<\/td>\n<td align=\"CENTER\">jtd<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"15\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi069<\/td>\n<td align=\"LEFT\">Chen Hao<\/td>\n<td align=\"CENTER\">15<\/td>\n<td align=\"CENTER\">3<\/td>\n<td align=\"CENTER\">H<\/td>\n<td align=\"LEFT\">HCN(4-3) emission in the disk of M51<\/td>\n<td align=\"CENTER\">jgw<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi070<\/td>\n<td align=\"LEFT\">Scott Chapman<\/td>\n<td align=\"CENTER\">20<\/td>\n<td align=\"CENTER\">1,2<\/td>\n<td align=\"CENTER\">H<\/td>\n<td align=\"LEFT\">[CII] in z~4.4 SMGs from the Herschel-red ALMA survey<\/td>\n<td align=\"CENTER\">halp<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi082<\/td>\n<td align=\"LEFT\">Stephen Eales<\/td>\n<td align=\"CENTER\">26<\/td>\n<td align=\"CENTER\">2<\/td>\n<td align=\"CENTER\">S<\/td>\n<td align=\"LEFT\">M31 &#8211; A Low Temperature Astrophysical Laboratory<\/td>\n<td align=\"CENTER\">halp<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi083<\/td>\n<td align=\"LEFT\">Gregory Herczeg<\/td>\n<td align=\"CENTER\">6<\/td>\n<td align=\"CENTER\">3<\/td>\n<td align=\"CENTER\">S<\/td>\n<td align=\"LEFT\">Accretion variability and the growth of protostars<\/td>\n<td align=\"CENTER\">imc<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"15\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi090<\/td>\n<td align=\"LEFT\">Chian-Chou Chen<\/td>\n<td align=\"CENTER\">26<\/td>\n<td align=\"CENTER\">3<\/td>\n<td align=\"CENTER\">S<\/td>\n<td align=\"LEFT\">Mapping starburst activity within and around HzRGs with SCUBA-2<\/td>\n<td align=\"CENTER\">halp<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi094<\/td>\n<td align=\"LEFT\">Yongjin Jeong<\/td>\n<td align=\"CENTER\">5<\/td>\n<td align=\"CENTER\">4<\/td>\n<td align=\"CENTER\">A<\/td>\n<td align=\"LEFT\">Molecular Gas Content of Infant AGNs<\/td>\n<td align=\"CENTER\">jgw<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi098<\/td>\n<td align=\"LEFT\">Keping Qiu<\/td>\n<td align=\"CENTER\">16<\/td>\n<td align=\"CENTER\">3<\/td>\n<td align=\"CENTER\">H<\/td>\n<td align=\"LEFT\">Filaments, magnetic fields, and massive star formation<\/td>\n<td align=\"CENTER\">jtd<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi099<\/td>\n<td align=\"LEFT\">Emily Drabek-Maunder<\/td>\n<td align=\"CENTER\">28<\/td>\n<td align=\"CENTER\">4,5<\/td>\n<td align=\"CENTER\">A<\/td>\n<td align=\"LEFT\">Molecules from below the surface of icy outer moons<\/td>\n<td align=\"CENTER\">imc<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"15\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi104<\/td>\n<td align=\"LEFT\">Oscar Morata<\/td>\n<td align=\"CENTER\">24<\/td>\n<td align=\"CENTER\">4<\/td>\n<td align=\"CENTER\">S,H<\/td>\n<td align=\"LEFT\">Characterizing the properties of a sample of proto-brown dwarf cand..<\/td>\n<td align=\"CENTER\">imc<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi105<\/td>\n<td align=\"LEFT\">Ping Zhou<\/td>\n<td align=\"CENTER\">15<\/td>\n<td align=\"CENTER\">3<\/td>\n<td align=\"CENTER\">A<\/td>\n<td align=\"LEFT\">Spatially resolved study of CR-induced ionization in a molecular co&#8230;<\/td>\n<td align=\"CENTER\">jtd<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi109<\/td>\n<td align=\"LEFT\">Erik Rosolowsky<\/td>\n<td align=\"CENTER\">3<\/td>\n<td align=\"CENTER\">3<\/td>\n<td align=\"CENTER\">H<\/td>\n<td align=\"LEFT\">CO Excitation Across a Spiral Arm<\/td>\n<td align=\"CENTER\">jtd<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi111<\/td>\n<td align=\"LEFT\">Alastair Edge<\/td>\n<td align=\"CENTER\">33<\/td>\n<td align=\"CENTER\">4<\/td>\n<td align=\"CENTER\">S<\/td>\n<td align=\"LEFT\">Extending the SCUBA-2 Cluster Snapshot Survey to z&gt;0.5<\/td>\n<td align=\"CENTER\">imc<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"15\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi112<\/td>\n<td align=\"LEFT\">Yu Gao<\/td>\n<td align=\"CENTER\">45<\/td>\n<td align=\"CENTER\">4<\/td>\n<td align=\"CENTER\">A<\/td>\n<td align=\"LEFT\">HCN (3-2) mapping along the major axes of nearby IR-bright galaxies..<\/td>\n<td align=\"CENTER\">imc<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi113<\/td>\n<td align=\"LEFT\">Junhyun Baek<\/td>\n<td align=\"CENTER\">8<\/td>\n<td align=\"CENTER\">3<\/td>\n<td align=\"CENTER\">A<\/td>\n<td align=\"LEFT\">Probing Cold Gas Content of the Central Galaxies in Cool-Core and N..<\/td>\n<td align=\"CENTER\">jgw<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi114<\/td>\n<td align=\"LEFT\">Scott Chapman<\/td>\n<td align=\"CENTER\">8<\/td>\n<td align=\"CENTER\">2<\/td>\n<td align=\"CENTER\">S<\/td>\n<td align=\"LEFT\">Feedback in action: the CO-rich galaxy at the centre of the cool co..<\/td>\n<td align=\"CENTER\">imc<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi116<\/td>\n<td align=\"LEFT\">Yi-Jehng Kuan<\/td>\n<td align=\"CENTER\">33<\/td>\n<td align=\"CENTER\">2,3,4,5<\/td>\n<td align=\"CENTER\">S,H,A<\/td>\n<td align=\"LEFT\">Monitoring comet 67P<\/td>\n<td align=\"CENTER\">imc<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"15\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi119<\/td>\n<td align=\"LEFT\">Dimitris Stamatellos<\/td>\n<td align=\"CENTER\">12<\/td>\n<td align=\"CENTER\">2<\/td>\n<td align=\"CENTER\">S<\/td>\n<td align=\"LEFT\">The role of environment in brown dwarf formation<\/td>\n<td align=\"CENTER\">halp<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi122<\/td>\n<td align=\"LEFT\">Sebastian Oliver<\/td>\n<td align=\"CENTER\">50<\/td>\n<td align=\"CENTER\">2,3<\/td>\n<td align=\"CENTER\">S<\/td>\n<td align=\"LEFT\">An efficient survey of obscured star formation in the high redshift&#8230;<\/td>\n<td align=\"CENTER\">halp<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi123<\/td>\n<td align=\"LEFT\">Hideo Sagawa<\/td>\n<td align=\"CENTER\"><span style=\"color: #ff0000\">daytime<\/span><\/td>\n<td align=\"CENTER\">1,2,3<\/td>\n<td align=\"CENTER\">H,A<\/td>\n<td align=\"LEFT\">Spatial\/Temporal Variation in Venus&#8217; Nightside Atmospheric Dynamics&#8230;<\/td>\n<td align=\"CENTER\">imc<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi124<\/td>\n<td align=\"LEFT\">Samira Snaid<\/td>\n<td align=\"CENTER\">44<\/td>\n<td align=\"CENTER\">4,5<\/td>\n<td align=\"CENTER\">H,A<\/td>\n<td align=\"LEFT\">Mass loss rates and 12C\/13C ratio in evolved stars<\/td>\n<td align=\"CENTER\">jgw<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"15\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi126<\/td>\n<td align=\"LEFT\">Li Xiao<\/td>\n<td align=\"CENTER\">9<\/td>\n<td align=\"CENTER\">4<\/td>\n<td align=\"CENTER\">S,H<\/td>\n<td align=\"LEFT\">Dust and gas properties in the shocked molecular clumps of IC 443<\/td>\n<td align=\"CENTER\">jgw<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi128<\/td>\n<td align=\"LEFT\">Erik Rosolowsky<\/td>\n<td align=\"CENTER\">20<\/td>\n<td align=\"CENTER\">5<\/td>\n<td align=\"CENTER\">A<\/td>\n<td align=\"LEFT\">Understanding the Origins of Dense Star Forming Gas<\/td>\n<td align=\"CENTER\">halp<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi129<\/td>\n<td align=\"LEFT\">Angus Mok<\/td>\n<td align=\"CENTER\">19<\/td>\n<td align=\"CENTER\">4<\/td>\n<td align=\"CENTER\">A<\/td>\n<td align=\"LEFT\">Expanding the JCMT NGLS: Verifying CO(3-2) Detections and Determini..<\/td>\n<td align=\"CENTER\">jtd<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi133<\/td>\n<td align=\"LEFT\">Scott Chapman<\/td>\n<td align=\"CENTER\">10<\/td>\n<td align=\"CENTER\">2<\/td>\n<td align=\"CENTER\">S<\/td>\n<td align=\"LEFT\">. . . the Baryonic Structure Survey fields: the HS1549 protocluster field.<\/td>\n<td align=\"CENTER\">jgw<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"15\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi136<\/td>\n<td align=\"LEFT\">Juan Li<\/td>\n<td align=\"CENTER\">20<\/td>\n<td align=\"CENTER\">1<\/td>\n<td align=\"CENTER\">H<\/td>\n<td align=\"LEFT\">Cold, Quiescent Dense Gas in the Central Region of Orion B9<\/td>\n<td align=\"CENTER\">jgw<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi139<\/td>\n<td align=\"LEFT\">Thomas Greve<\/td>\n<td align=\"CENTER\">23<\/td>\n<td align=\"CENTER\">1,2<\/td>\n<td align=\"CENTER\">S<\/td>\n<td align=\"LEFT\">Tracing large-scale structure growth with SCUBA-2<\/td>\n<td align=\"CENTER\">halp<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bi140<\/td>\n<td align=\"LEFT\">Prof. Glenn White<\/td>\n<td align=\"CENTER\">10<\/td>\n<td align=\"CENTER\">5<\/td>\n<td align=\"CENTER\">H<\/td>\n<td align=\"LEFT\">The dynamics of the massive star-forming regions in M17:<\/td>\n<td align=\"CENTER\">imc<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"15\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"15\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\"><b>U.Hawaii<\/b><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"15\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bh03b<\/td>\n<td align=\"LEFT\">Lennox Cowie<\/td>\n<td align=\"CENTER\">56<\/td>\n<td align=\"CENTER\">2<\/td>\n<td align=\"CENTER\">S<\/td>\n<td align=\"LEFT\">A submillimeter survey of the GOODS\/CANDELS\/Chandra deep \ufb01elds<\/td>\n<td align=\"CENTER\">imc<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bh12a<\/td>\n<td align=\"LEFT\">Li-Yen Hsu<\/td>\n<td align=\"CENTER\">84<\/td>\n<td align=\"CENTER\">1,2<\/td>\n<td align=\"CENTER\">S<\/td>\n<td align=\"LEFT\">Characterizing Faint Submillimeter Galaxies with Cluster Lensing<\/td>\n<td align=\"CENTER\">imc<\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\">m15bh24b<\/td>\n<td align=\"LEFT\">Dave Sanders<\/td>\n<td align=\"CENTER\">35<\/td>\n<td align=\"CENTER\">2<\/td>\n<td align=\"CENTER\">S<\/td>\n<td align=\"LEFT\">A Submillimeter-Bright z &gt; 2 Protocluster in the SHELA\/HETDEX Field<\/td>\n<td align=\"CENTER\">imc<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<p>&nbsp;<\/p>\n<table border=\"0\" cellspacing=\"0\">\n<tbody>\n<tr>\n<td align=\"CENTER\" height=\"15\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\">FoPs<\/td>\n<td align=\"CENTER\">halp<\/td>\n<td align=\"LEFT\">Harriet Parsons h.parsons @ eaobservatory.org<\/td>\n<td align=\"CENTER\"><\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\">jtd<\/td>\n<td align=\"LEFT\">Jessica Dempsey j.dempsey @ eaobservatory.org<\/td>\n<td align=\"CENTER\"><\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\">jgw<\/td>\n<td align=\"LEFT\">Jan Wouterloot j.wouterloot @ eaobservatory.org<\/td>\n<td align=\"CENTER\"><\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\">pf<\/td>\n<td align=\"LEFT\">Per Friberg p.friberg @ eaobservatory.org<\/td>\n<td align=\"CENTER\"><\/td>\n<\/tr>\n<tr>\n<td align=\"CENTER\" height=\"16\"><\/td>\n<td align=\"LEFT\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\"><\/td>\n<td align=\"CENTER\">imc<\/td>\n<td align=\"LEFT\">Iain Coulson i.coulson @ eaobservatory.org<\/td>\n<td align=\"CENTER\"><\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Project ID P.I. Award Weather Rx Title of investigation FoP hours Band EAO m15bi003 Tomoya Hirota 20 3 H Survey of the vibrationally excited H2O lines in nearby massive YSO&#8230; imc m15bi004 Kazushi Sakamoto 2 1 H Dense &amp; Warm Gas in a Starburst Merger imc m15bi006 Ian Smail 30\u2026 <a class=\"continue-reading-link\" href=\"https:\/\/www.eaobservatory.org\/jcmt\/proposals\/allocations\/allocations-15b\/\">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\/3248"}],"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=3248"}],"version-history":[{"count":2,"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/pages\/3248\/revisions"}],"predecessor-version":[{"id":3250,"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/pages\/3248\/revisions\/3250"}],"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=3248"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}