{"id":12674,"date":"2022-10-05T16:25:24","date_gmt":"2022-10-06T02:25:24","guid":{"rendered":"https:\/\/www.eaobservatory.org\/jcmt\/?page_id=12674"},"modified":"2023-08-14T11:58:55","modified_gmt":"2023-08-14T21:58:55","slug":"users-meeting-2023","status":"publish","type":"page","link":"https:\/\/www.eaobservatory.org\/jcmt\/science\/users-meeting-2023\/","title":{"rendered":"Users Meeting 2023"},"content":{"rendered":"<div><span lang=\"EN-US\">The2023 JCMT science\/users meeting will be held <strong>from 30th May to 1st June<\/strong>\u00a0at University College London. There will be the opportunity to either attend the meeting in person or remotely. The meeting will have a programme of talks and posters about current JCMT science and instrumentation, and we will also discuss future submillimetre science projects and instrumentation. If there is enough demand, we will also arrange hands-on tuition sessions for JCMT software. If you would like to attend the meeting, please register at <a href=\"https:\/\/survey.alchemer.com\/s3\/7029255\/JCMT-Users-Meeting-2023\">https:\/\/survey.alchemer.com\/s3\/7029255\/JCMT-Users-Meeting-2023<\/a>.<\/span><\/div>\n<div>At the registration site, you can also submit a title and an abstract if you would like to give an oral presentation or a poster. The deadline for registering for the conference (there is no registration fee) is <span style=\"color: #ff0000\"><strong>March 31<sup>st<\/sup>.<\/strong><\/span><\/div>\n<p style=\"font-weight: 400\">We will make rooms available for teams that are carrying out current JCMT Large Programmes and for those who wish to discuss future Large Programmes. If you would like to use room for such discussions, please send your request to: <a href=\"mailto:JCMT_UM_2023@eaobservatory.org\">JCMT_UM_2023@eaobservatory.org<\/a>.<\/p>\n<div>You can find the latest agenda of the users meeting below. Please note that we will have parallel sessions in the Day3 (June 1st) afternoon.<\/div>\n<div><\/div>\n<div><span lang=\"EN-US\">If you have any questions about the meeting, please contact the chair of the Scientific Organising Committee Steve Eales (<\/span><span lang=\"EN-US\"><a href=\"mailto:steve.a.eales@gmail.com\" target=\"_blank\" rel=\"noopener\">steve.a.eales@gmail.com<\/a><\/span><span lang=\"EN-US\">), or send emails to <\/span><span lang=\"EN-US\"><a href=\"mailto:JCMT_UM_2023@eaobservatory.org\">JCMT_UM_2023@eaobservatory.org.<\/a><\/span><\/div>\n<p><img loading=\"lazy\" class=\"aligncenter wp-image-12953 size-large\" src=\"http:\/\/www.eaobservatory.org\/jcmt\/wp-content\/uploads\/sites\/2\/2023\/08\/JCMT-UM-2023-UK-1024x426.jpg\" alt=\"Image of participants at the JCMT Users Meeting 2023\" width=\"830\" height=\"345\" srcset=\"https:\/\/www.eaobservatory.org\/jcmt\/wp-content\/uploads\/sites\/2\/2023\/08\/JCMT-UM-2023-UK-1024x426.jpg 1024w, https:\/\/www.eaobservatory.org\/jcmt\/wp-content\/uploads\/sites\/2\/2023\/08\/JCMT-UM-2023-UK-300x125.jpg 300w, https:\/\/www.eaobservatory.org\/jcmt\/wp-content\/uploads\/sites\/2\/2023\/08\/JCMT-UM-2023-UK-768x320.jpg 768w, https:\/\/www.eaobservatory.org\/jcmt\/wp-content\/uploads\/sites\/2\/2023\/08\/JCMT-UM-2023-UK-1536x640.jpg 1536w, https:\/\/www.eaobservatory.org\/jcmt\/wp-content\/uploads\/sites\/2\/2023\/08\/JCMT-UM-2023-UK-2048x853.jpg 2048w, https:\/\/www.eaobservatory.org\/jcmt\/wp-content\/uploads\/sites\/2\/2023\/08\/JCMT-UM-2023-UK-150x62.jpg 150w\" sizes=\"(max-width: 830px) 100vw, 830px\" \/><\/p>\n<p>&nbsp;<\/p>\n<p><span style=\"font-size: 14pt\"><strong>The meeting venue: the Denys Holland Lecture Theatre in UCL\u2019s Bentham House <\/strong>(map is <a href=\"https:\/\/www.google.com\/maps\/d\/u\/0\/edit?mid=1mLvGAr0TrVuNJ9YUfRIxiCBMlG5qyxQ&amp;usp=sharing\">here)<\/a><\/span><\/p>\n<p><span style=\"font-size: 14pt\"><strong>Information on the nearby accommodation is <a href=\"http:\/\/www.eaobservatory.org\/jcmt\/wp-content\/uploads\/sites\/2\/2023\/05\/accommodation-list.pdf\">here<\/a><\/strong><\/span><\/p>\n<p><span style=\"font-size: 14pt\"><strong>Agenda-Day1<\/strong><\/span><\/p>\n<table style=\"border-collapse: collapse;width: 0%;height: 975px\">\n<tbody>\n<tr style=\"height: 24px\">\n<td style=\"width: 8.419441255262154%;height: 24px\">Time<\/td>\n<td style=\"width: 13.98775353999234%;height: 24px\">Chair<\/td>\n<td style=\"width: 77.5928052047455%;height: 24px\">Title and speaker<\/td>\n<\/tr>\n<tr style=\"height: 24px\">\n<td style=\"width: 8.419441255262154%;height: 24px\">10:30-11:00<\/td>\n<td style=\"width: 13.98775353999234%;height: 24px\"><\/td>\n<td style=\"width: 77.5928052047455%;height: 24px\">\n<div><span lang=\"EN-GB\">Introduction and status of JCMT; Paul T. P. Ho (EAO)<\/span><\/div>\n<\/td>\n<\/tr>\n<tr style=\"height: 24px\">\n<td style=\"width: 8.419441255262154%;height: 24px\">11:00-11:30<\/td>\n<td style=\"width: 13.98775353999234%;height: 24px\"><\/td>\n<td style=\"width: 77.5928052047455%;height: 24px\">\n<div><span lang=\"EN-GB\">Future of JCMT instrumentation; Dan Bintley (EAO)<\/span><\/div>\n<\/td>\n<\/tr>\n<tr style=\"height: 48px\">\n<td style=\"width: 8.419441255262154%;height: 48px\">11:30-11:50<\/td>\n<td style=\"width: 13.98775353999234%;height: 48px\"><\/td>\n<td style=\"width: 77.5928052047455%;height: 48px\">\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">Submillimeter Extragalactic Background Light;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Qi-Ning Hsu (ASIAA) &#8211; remote<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr style=\"height: 48px\">\n<td style=\"width: 8.419441255262154%;height: 48px\">11:50-12:10<\/td>\n<td style=\"width: 13.98775353999234%;height: 48px\"><\/td>\n<td style=\"width: 77.5928052047455%;height: 48px\">\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">JCMT-Venus\u2019 Atmosphere with the JCMT;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Dave Clements (UK) &#8211; remote<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr style=\"height: 48px\">\n<td style=\"width: 8.419441255262154%;height: 48px\">12:10-12:30<\/td>\n<td style=\"width: 13.98775353999234%;height: 48px\"><\/td>\n<td style=\"width: 77.5928052047455%;height: 48px\">\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">RAGERS \u2013 the Radio Galaxy Environment Reference Survey;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Thomas Greve (others) &#8211; remote<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr style=\"height: 48px\">\n<td style=\"width: 8.419441255262154%;height: 48px\">12:30-12:50<\/td>\n<td style=\"width: 13.98775353999234%;height: 48px\"><\/td>\n<td style=\"width: 77.5928052047455%;height: 48px\">\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">BISTRO: B-Fields in STar-Forming Region Observations;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Shih-Ping Lai (NTHU)<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 8.419441255262154%\">12:50-14:00<\/td>\n<td style=\"width: 13.98775353999234%\"><\/td>\n<td style=\"width: 77.5928052047455%\">\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">Lunch<\/span><\/span><\/p>\n<\/div>\n<\/td>\n<\/tr>\n<tr style=\"height: 48px\">\n<td style=\"width: 8.419441255262154%;height: 48px\">14:00-14:20<\/td>\n<td style=\"width: 13.98775353999234%;height: 48px\"><\/td>\n<td style=\"width: 77.5928052047455%;height: 48px\">\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">Latest Progress in STUDIES;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Wei-Hao Wang (ASIAA)<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr style=\"height: 48px\">\n<td style=\"width: 8.419441255262154%;height: 48px\">14:20-14:40<\/td>\n<td style=\"width: 13.98775353999234%;height: 48px\"><\/td>\n<td style=\"width: 77.5928052047455%;height: 48px\">\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">HASHTAG &amp; DOWSING: Understanding Nearby Galaxies with SCUBA-2;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Matt Smith (UK)<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr style=\"height: 48px\">\n<td style=\"width: 8.419441255262154%;height: 48px\">14:40-15:00<\/td>\n<td style=\"width: 13.98775353999234%;height: 48px\"><\/td>\n<td style=\"width: 77.5928052047455%;height: 48px\">\n<div>\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">Mapping the Decline with Redshift of Dusty Star-forming Galaxies Using JWST and SCUBA-2;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Amy Barger (USA)<\/span><\/div>\n<\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr style=\"height: 48px\">\n<td style=\"width: 8.419441255262154%;height: 48px\">15:00-15:20<\/td>\n<td style=\"width: 13.98775353999234%;height: 48px\"><\/td>\n<td style=\"width: 77.5928052047455%;height: 48px\">\n<div>\n<div>\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">MAJORS;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">David Eden (UK)<\/span><\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr style=\"height: 48px\">\n<td style=\"width: 8.419441255262154%;height: 48px\">15:20-15:40<\/td>\n<td style=\"width: 13.98775353999234%;height: 48px\"><\/td>\n<td style=\"width: 77.5928052047455%;height: 48px\">\n<div>\n<div>\n<div>\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">Bridging the gap between local and extragalactic star formation: dense gas tracers in large galactic filament;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Orsolya Feher (UK)<\/span><\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 8.419441255262154%\">15;40-16:10<\/td>\n<td style=\"width: 13.98775353999234%\"><\/td>\n<td style=\"width: 77.5928052047455%\">\n<div>\n<div>\n<div>\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">coffee break<\/span><\/span><\/p>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr style=\"height: 48px\">\n<td style=\"width: 8.419441255262154%;height: 48px\">16:10-16:30<\/td>\n<td style=\"width: 13.98775353999234%;height: 48px\"><\/td>\n<td style=\"width: 77.5928052047455%;height: 48px\">\n<div>\n<div>\n<div>\n<div>\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">The Nearby Evolved Stars Survey;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Peter Sciuna (ESO)<\/span><\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr style=\"height: 72px\">\n<td style=\"width: 8.419441255262154%;height: 72px\">16:30-16:50<\/td>\n<td style=\"width: 13.98775353999234%;height: 72px\"><\/td>\n<td style=\"width: 77.5928052047455%;height: 72px\">\n<div>\n<div>\n<div>\n<div>\n<div>\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">Early heterodyne results from NESS &#8211; The Nearby Evolved Stars Survey;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Sofia Wallstrom (Leuven)<\/span><\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr style=\"height: 48px\">\n<td style=\"width: 8.419441255262154%;height: 48px\">16:50-17:10<\/td>\n<td style=\"width: 13.98775353999234%;height: 48px\"><\/td>\n<td style=\"width: 77.5928052047455%;height: 48px\">\n<div>\n<div>\n<div>\n<div>\n<div>\n<div>\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">Role of magnetic field in cluster formation: A case study of G148.24+00.41 with JCMT SCUBA-2\/ POL-2;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Vineet Rawat (India)<\/span><\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr style=\"height: 72px\">\n<td style=\"width: 8.419441255262154%;height: 72px\">17:10-17:30<\/td>\n<td style=\"width: 13.98775353999234%;height: 72px\"><\/td>\n<td style=\"width: 77.5928052047455%;height: 72px\">\n<div>\n<div>\n<div>\n<div>\n<div>\n<div>\n<div>\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">The Hawaii SCUBA-2 cluster lensing survey;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Lennox Cowie (Univ. of Hawaii, USA)<\/span><\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 8.419441255262154%\">17:30-17:50<\/td>\n<td style=\"width: 13.98775353999234%\"><\/td>\n<td style=\"width: 77.5928052047455%\">\n<div>\n<div>\n<div>\n<div>\n<div>\n<div>\n<div>\n<div>\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">SPOTLESS: An efficient study of the densest regions in the Universe using near-infrared and submm observations;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Tom Bakx (Japan)<\/span><\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 8.419441255262154%\">17:50-18:10<\/td>\n<td style=\"width: 13.98775353999234%\"><\/td>\n<td style=\"width: 77.5928052047455%\">\n<div>\n<div>\n<div>\n<div>\n<div>\n<div>\n<div>\n<div>\n<div>\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">Dark Matter Halos and Star Formation Efficiencies of &#8220;Super-thin&#8221; Galaxies;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Tim Davis (UK)<\/span><\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<p>&nbsp;<\/p>\n<p><strong><span style=\"font-size: 14pt\">Agenda- Day2<\/span><\/strong><\/p>\n<table style=\"border-collapse: collapse;width: 100%;height: 408px\">\n<tbody>\n<tr>\n<td style=\"width: 5.147340221967088%\">Time<\/td>\n<td style=\"width: 9.165709911978574%\">Chair<\/td>\n<td style=\"width: 85.68694986605435%\">\n<div>\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">Title and speaker<\/span><\/span><\/p>\n<\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr style=\"height: 48px\">\n<td style=\"width: 5.147340221967088%;height: 48px\">9:00-9:20<\/td>\n<td style=\"width: 9.165709911978574%;height: 48px\"><\/td>\n<td style=\"width: 85.68694986605435%;height: 48px\">\n<div>\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">Dense cores are rare in high-latitude Planck Galactic cold clumps;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Fengwe Xu (China) &#8211; remote<\/span><\/div>\n<\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr style=\"height: 48px\">\n<td style=\"width: 5.147340221967088%;height: 48px\">9:20-9:40<\/td>\n<td style=\"width: 9.165709911978574%;height: 48px\"><\/td>\n<td style=\"width: 85.68694986605435%;height: 48px\">\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\"><span lang=\"EN-GB\">SCUBA-2 Ultra Deep Imaging EAO Survey<\/span><\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">(STUDIES): Confusion-limited 450-micron Galaxy Number Counts and Machine Learning Identification;\u00a0<\/span><span lang=\"EN-GB\">Zhen-Kai Gao (ASIAA\/NCU) &#8211; remote<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr style=\"height: 48px\">\n<td style=\"width: 5.147340221967088%;height: 48px\">9:40-10:00<\/td>\n<td style=\"width: 9.165709911978574%;height: 48px\"><\/td>\n<td style=\"width: 85.68694986605435%;height: 48px\">\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">The Bistro Survey: two types of filaments in NGC 2264;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Jia-Wei Wang (ASIAA) &#8211; remote<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr style=\"height: 48px\">\n<td style=\"width: 5.147340221967088%;height: 48px\">10:00-10:20<\/td>\n<td style=\"width: 9.165709911978574%;height: 48px\"><\/td>\n<td style=\"width: 85.68694986605435%;height: 48px\">\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">Overview of results from the JINGLE survey;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Amelie Saintonge (UK)<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr style=\"height: 48px\">\n<td style=\"width: 5.147340221967088%;height: 48px\">10:20-10:40<\/td>\n<td style=\"width: 9.165709911978574%;height: 48px\"><\/td>\n<td style=\"width: 85.68694986605435%;height: 48px\">\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">Observing nearby galaxies with SCUBA-2 and POL-2;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Kate Pattle (UK)<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr style=\"height: 24px\">\n<td style=\"width: 5.147340221967088%;height: 24px\">10:40-11:10<\/td>\n<td style=\"width: 9.165709911978574%;height: 24px\"><\/td>\n<td style=\"width: 85.68694986605435%;height: 24px\">coffee break<\/td>\n<\/tr>\n<tr style=\"height: 48px\">\n<td style=\"width: 5.147340221967088%;height: 48px\">11:10-11:30<\/td>\n<td style=\"width: 9.165709911978574%;height: 48px\"><\/td>\n<td style=\"width: 85.68694986605435%;height: 48px\">\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">Revisiting the Nuclear Ring in our Neighborhood: a JCMT perspective of Andromeda;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Zongnan Li (China)<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr style=\"height: 24px\">\n<td style=\"width: 5.147340221967088%;height: 24px\">11:30-11:50<\/td>\n<td style=\"width: 9.165709911978574%;height: 24px\"><\/td>\n<td style=\"width: 85.68694986605435%;height: 24px\">\n<div><span lang=\"EN-GB\">Dust Polarization Astrophysics;\u00a0<\/span><\/div>\n<\/td>\n<\/tr>\n<tr style=\"height: 24px\">\n<td style=\"width: 5.147340221967088%;height: 24px\">11:50-12;10<\/td>\n<td style=\"width: 9.165709911978574%;height: 24px\"><\/td>\n<td style=\"width: 85.68694986605435%;height: 24px\">\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">Magnetic fields in Cepheus A\/HW2-<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Eswaralah Chakall (India)<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr style=\"height: 24px\">\n<td style=\"width: 5.147340221967088%;height: 24px\">12:10-12:30<\/td>\n<td style=\"width: 9.165709911978574%;height: 24px\"><\/td>\n<td style=\"width: 85.68694986605435%;height: 24px\">\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">Calibrating submillimeter dust emissivities with the Nearby Evolved Stars Survey (NESS);<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Ciska Kemper (Spain)<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr style=\"height: 24px\">\n<td style=\"width: 5.147340221967088%;height: 24px\">12:30-14:00<\/td>\n<td style=\"width: 9.165709911978574%;height: 24px\"><\/td>\n<td style=\"width: 85.68694986605435%;height: 24px\">\u00a0Lunch<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 5.147340221967088%\">14:00-14:20<\/td>\n<td style=\"width: 9.165709911978574%\"><\/td>\n<td style=\"width: 85.68694986605435%\">\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">Preliminary Results from BISTRO3 &#8211; Star Formation across Evolutionary and Size Scales;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Janik Karoly (UK)<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 5.147340221967088%\">14:20-14:40<\/td>\n<td style=\"width: 9.165709911978574%\"><\/td>\n<td style=\"width: 85.68694986605435%\">\n<div>\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">JCMT-Venus: Monitoring HDO absorption in Venus&#8217; Atmosphere;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Wei Tang (UK)<\/span><\/div>\n<\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 5.147340221967088%\">14:40-15:00<\/td>\n<td style=\"width: 9.165709911978574%\"><\/td>\n<td style=\"width: 85.68694986605435%\">\n<div>\n<div>\n<div>\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">Understanding star formation in elephant trunk-like structures;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Ram Kesh Yadav<\/span><\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 5.147340221967088%\">15:00-15:20<\/td>\n<td style=\"width: 9.165709911978574%\"><\/td>\n<td style=\"width: 85.68694986605435%\">\n<div>\n<div>\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">A VLBI Test at 690 GHz;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Ming Tang Chen (ASIAA)<\/span><\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 5.147340221967088%\">15:20-15:40<\/td>\n<td style=\"width: 9.165709911978574%\"><\/td>\n<td style=\"width: 85.68694986605435%\">\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">SCUBA-2 uncovers excess of 850 micron\u00a0<\/span><\/span><span style=\"font-family: inherit;font-size: inherit\"><span style=\"font-family: inherit;font-size: inherit\">counts on Mpc scales around high-redshift quasars;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Fabrizo Arrigoni Battaia (Germany)<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 5.147340221967088%\">15:40-16:10<\/td>\n<td style=\"width: 9.165709911978574%\"><\/td>\n<td style=\"width: 85.68694986605435%\">\n<div><span lang=\"EN-GB\"><span lang=\"EN-GB\">coffee break<\/span><\/span><\/div>\n<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 5.147340221967088%\">16:10-16:30<\/td>\n<td style=\"width: 9.165709911978574%\"><\/td>\n<td style=\"width: 85.68694986605435%\">\n<div>\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">Magnetic fields towards NGC 7023 under stellar feedback;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Ekta Sharma (China)<\/span><\/div>\n<\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 5.147340221967088%\">16:30-16:50<\/td>\n<td style=\"width: 9.165709911978574%\"><\/td>\n<td style=\"width: 85.68694986605435%\">\n<div>\n<div>\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">Grain Alignment and Magnetic Field in Star-Forming Regions;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Ngoc Tram Le (Germany)<\/span><\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 5.147340221967088%\">16:50-17:10<\/td>\n<td style=\"width: 9.165709911978574%\"><\/td>\n<td style=\"width: 85.68694986605435%\">\n<div>\n<div>\n<div>\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">Magnetic fields of the starless core L1512;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Sheng-Jun Lin (ASIAA)<\/span><\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 5.147340221967088%\">17:10-17:30<\/td>\n<td style=\"width: 9.165709911978574%\"><\/td>\n<td style=\"width: 85.68694986605435%\">\n<div>\n<div>\n<div>\n<div>\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">The SCUBA-2 Large eXtragalactic Survey: 850um map, catalogue and the bright-end number counts of the XMM-LSS field;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Tracy Garratt (UK)<\/span><\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<p><span style=\"font-size: 14pt\"><strong>Agenda- Day3 Morning<\/strong><\/span><\/p>\n<table style=\"border-collapse: collapse;width: 100%\">\n<tbody>\n<tr>\n<td style=\"width: 5.032529659395333%\">Time<\/td>\n<td style=\"width: 9.337925755836203%\">Chair<\/td>\n<td style=\"width: 85.62954458476847%\">Title and speaker<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 5.032529659395333%\">9:00-9:20<\/td>\n<td style=\"width: 9.337925755836203%\"><\/td>\n<td style=\"width: 85.62954458476847%\">\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">A multi-transition view of infall signatures in massive star forming regions;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Ke Wang (China) &#8211; remote<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 5.032529659395333%\">9:20-9:40<\/td>\n<td style=\"width: 9.337925755836203%\"><\/td>\n<td style=\"width: 85.62954458476847%\">\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">Dense gas and core formation in the nearby IRDCs as revealed in ALOHA survey;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Zhiyuan Ren (China) &#8211; remote<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 5.032529659395333%\">9:40-10:00<\/td>\n<td style=\"width: 9.337925755836203%\"><\/td>\n<td style=\"width: 85.62954458476847%\">\n<div><span lang=\"EN-GB\">JCMT as a mm\/submm VLBI Station; <\/span><\/div>\n<div><span lang=\"EN-GB\">Satoki Matsushita (ASIAA)<\/span><\/div>\n<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 5.032529659395333%\">10:00-10:20<\/td>\n<td style=\"width: 9.337925755836203%\"><\/td>\n<td style=\"width: 85.62954458476847%\">\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">Submm galaxy survey with JCMT SCUBA-2 in JWST NEP Time Domain Field to reveal the hidden hign-z star formation;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Minhee Hyun (Korea)<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 5.032529659395333%\">10:20-10:40<\/td>\n<td style=\"width: 9.337925755836203%\"><\/td>\n<td style=\"width: 85.62954458476847%\">\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">JCMT synergies: multi-wavelength polarization to study magnetic field structure and dust properties;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Lapo Fanciullo (NCHU)<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 5.032529659395333%\">10:40-11:10<\/td>\n<td style=\"width: 9.337925755836203%\"><\/td>\n<td style=\"width: 85.62954458476847%\">coffee break<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 5.032529659395333%\">11:10-11:30<\/td>\n<td style=\"width: 9.337925755836203%\"><\/td>\n<td style=\"width: 85.62954458476847%\">\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">how to write a proposal;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Kate Pattle<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 5.032529659395333%\">11:30-11:50<\/td>\n<td style=\"width: 9.337925755836203%\"><\/td>\n<td style=\"width: 85.62954458476847%\">\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">Potential Upgrade of JCMT Heterodyne Instruments;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Boon Kok Tan (UK)<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 5.032529659395333%\">11:50-12:20<\/td>\n<td style=\"width: 9.337925755836203%\"><\/td>\n<td style=\"width: 85.62954458476847%\">\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">an even bigger submm telescope &#8211; AtLAST;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Pamela Klaasen &#8211; remote<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 5.032529659395333%\">12:20-13:40<\/td>\n<td style=\"width: 9.337925755836203%\"><\/td>\n<td style=\"width: 85.62954458476847%\">\n<div><span lang=\"EN-GB\"><span lang=\"EN-GB\">Lunch<\/span><\/span><\/div>\n<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<p><span style=\"font-size: 14pt\"><strong>Agenda- Day3 afternoon Parallel Session I<\/strong><\/span><\/p>\n<table style=\"border-collapse: collapse;width: 100%\">\n<tbody>\n<tr>\n<td style=\"width: 5.089934940681211%\">13:40-14:10<\/td>\n<td style=\"width: 9.395331037122084%\"><\/td>\n<td style=\"width: 85.5147340221967%\">\n<div>\n<p><span lang=\"EN-GB\"><span lang=\"EN-GB\">STFC Astronomy Advisory Panel Roadmap: implications for submm astronomy;<\/span><\/span><\/p>\n<div><span lang=\"EN-GB\">Steve Serjeant (UK)<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 5.089934940681211%\">14:10-15:00<\/td>\n<td style=\"width: 9.395331037122084%\"><\/td>\n<td style=\"width: 85.5147340221967%\">\n<div><span lang=\"EN-GB\">Discussion of the future<\/span><\/div>\n<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<p><span style=\"font-size: 14pt\"><strong>Agenda-Day3 afternoon Parallel Session II<\/strong><\/span><\/p>\n<table style=\"border-collapse: collapse;width: 100%\">\n<tbody>\n<tr>\n<td style=\"width: 5.262150784538846%\">13:40-14:40<\/td>\n<td style=\"width: 9.452736318407965%\"><\/td>\n<td style=\"width: 85.2851128970532%\">ACSIS and SCUBA-2 pipelines: (talk\u00a0+ interactive tutorial)<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 5.262150784538846%\">14:40-15:10<\/td>\n<td style=\"width: 9.452736318407965%\"><\/td>\n<td style=\"width: 85.2851128970532%\">Calibration of ACSIS and SCUBA-2 data (talk)<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 5.262150784538846%\">15:10-15:25<\/td>\n<td style=\"width: 9.452736318407965%\"><\/td>\n<td style=\"width: 85.2851128970532%\">coffee break<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 5.262150784538846%\">15:25-16;25<\/td>\n<td style=\"width: 9.452736318407965%\"><\/td>\n<td style=\"width: 85.2851128970532%\">Project life cycle and the Observing Tool (talk\u00a0+ interactive tutorial)<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 5.262150784538846%\">16:25-17:25<\/td>\n<td style=\"width: 9.452736318407965%\"><\/td>\n<td style=\"width: 85.2851128970532%\">POL-2 DR (talk and tutorial)<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<p>Organising Committee:<br \/>\nMike Chen (Queen&#8217;s Univ.)<br \/>\nMing-Tang Chen (ASIAA)<br \/>\nDave Clements (Imperial College)<br \/>\nLennox Cowie (Univ. of Hawaii)<br \/>\nStephen A Eales (Cardiff Univ.): Chair<br \/>\nJongsoo Kim (KASI)<br \/>\nAmelie Saintonge (Univ. College Londo)<br \/>\nNagayoshi Ohashi (ASIAA\/EAO)<br \/>\nKate Pattle (Univ. College London)<br \/>\nMing Zhu (CAS)<\/p>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>The2023 JCMT science\/users meeting will be held from 30th May to 1st June\u00a0at University College London. There will be the opportunity to either attend the meeting in person or remotely. The meeting will have a programme of talks and posters about current JCMT science and instrumentation, and we will also\u2026 <a class=\"continue-reading-link\" href=\"https:\/\/www.eaobservatory.org\/jcmt\/science\/users-meeting-2023\/\">Continue reading<\/a><\/p>\n","protected":false},"author":83,"featured_media":0,"parent":69,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":[],"_links":{"self":[{"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/pages\/12674"}],"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\/83"}],"replies":[{"embeddable":true,"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/comments?post=12674"}],"version-history":[{"count":26,"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/pages\/12674\/revisions"}],"predecessor-version":[{"id":12954,"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/pages\/12674\/revisions\/12954"}],"up":[{"embeddable":true,"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/pages\/69"}],"wp:attachment":[{"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/media?parent=12674"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}