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