The following poster presentations will be provided at the 2019 JCMT Users Meeting in Taipei, Taiwan.<\/p>\n
Zamri Zainal Abidin<\/span>, University of Malaya<\/em> – Malaysia\/EAO Observer Consortium<\/a> All poster presenters are asked to give a brief 60 sec presentation of their poster in the poster flashes section on Wednesday November 6 (12:12 – 12:30). We ask that you please prepare one slide to accompany your poster flash presentation (this slide is to be uploaded onto the presentation computer by the end of the first coffee break on Nov 6; please see Mark Rawlings for assistance if needed). The poster flashes will run in alphabetical order (as displayed above).<\/p>\n Poster boards can accommodate posters of up to 90 cm in WIDTH and 180 cm in HEIGHT. Posters in either “portrait” or “landscape” format smaller than this dimension can be fitted on the board. An A0 size poster (84 cm by 120 cm), for example, can be displayed in portrait format.<\/p>\n Please provide observatory staff with a pdf of your poster ahead of time using the format:<\/p>\n <given name<\/span>>_<family name<\/span>>_JCMT2019UsersMeeting_poster_public<\/p>\n Please note that the LOC will not print posters for participants.<\/strong><\/p>\n Registration<\/a> | Local Logistics<\/a> | Program<\/a> | Posters<\/a> | Participants<\/a> | JCMT DR\/Tutorials | Remote connect<\/a> | SMA meeting<\/a>\u00a0| Splinter Meetings<\/a> | Code of Conduct<\/a><\/p>\n","protected":false},"excerpt":{"rendered":" The following poster presentations will be provided at the 2019 JCMT Users Meeting in Taipei, Taiwan. Zamri Zainal Abidin, University of Malaya – Malaysia\/EAO Observer Consortium Tao-Chung Ching, NAOC – Magnetic Fields in the DR21 Massive Star-forming Region from 10 to 0.03 pc Scales Pei-Ying Hsieh, ASIAA – The accretion\u2026 Continue reading<\/a><\/p>\n","protected":false},"author":5,"featured_media":0,"parent":8870,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":[],"_links":{"self":[{"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/pages\/10168"}],"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\/5"}],"replies":[{"embeddable":true,"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/comments?post=10168"}],"version-history":[{"count":24,"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/pages\/10168\/revisions"}],"predecessor-version":[{"id":10448,"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/pages\/10168\/revisions\/10448"}],"up":[{"embeddable":true,"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/pages\/8870"}],"wp:attachment":[{"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/media?parent=10168"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}
\nTao-Chung Ching<\/span>, NAOC<\/em> – Magnetic Fields in the DR21 Massive Star-forming Region from 10 to 0.03 pc Scales
\nPei-Ying Hsieh<\/span>, ASIAA<\/em> – The accretion process of cold molecular gas to the closest supermassive black hole SgrA*
\nYu-Hsuan Hwang<\/span>, ASIAA\/NTU<\/em> – A Submillimeter View of Quiescent Galaxies<\/a>
\nLapo Fanciullo,<\/span> ASIAA –<\/em> The role of POL-2 data in reconstructing dust properties from multi-wavelength polarimetry
\nNatsuko Izumi<\/span>, Ibaraki University<\/em> – CO observations of molecular clouds in the Extreme Outer Galaxy<\/a>
\nSihan Jiao<\/span>, NAOC<\/em> – Cloud structure from combining ground and space-based bolometric observations
\nDongjin Kim<\/span>, Max Planck Institute for Radioastronomy<\/em> – A search for molecular absorption in AGN
\nShanghuo\u00a0Li<\/span>, Shanghai Astronomical Observator<\/em>y – ALMA observations of NGC 6334S
\nHongjun Ma<\/span>, Purple Mountain Observatory\/EAO<\/em> – Identifying the foreground clouds in the CMZ<\/a>
\nKate Pattle<\/span>, National Tsing Hua University<\/em> – Dust grain alignment inferred using a Ricean noise model<\/a>
\nTravis Thieme<\/span>, NTHU<\/em> – Searching for Accretion Flows around Class 0 Protostars with ALMA<\/p>\n
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