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Submillimeter Extragalactic Background Light;<\/span><\/span><\/p>\nQi-Ning Hsu (ASIAA) – remote<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n\n| 11:50-12:10<\/td>\n | <\/td>\n | \n\n JCMT-Venus\u2019 Atmosphere with the JCMT;<\/span><\/span><\/p>\nDave Clements (UK) – remote<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n\n| 12:10-12:30<\/td>\n | <\/td>\n | \n\n RAGERS \u2013 the Radio Galaxy Environment Reference Survey;<\/span><\/span><\/p>\nThomas Greve (others) – remote<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n\n| 12:30-12:50<\/td>\n | <\/td>\n | \n\n BISTRO: B-Fields in STar-Forming Region Observations;<\/span><\/span><\/p>\nShih-Ping Lai (NTHU)<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n\n| 12:50-14:00<\/td>\n | <\/td>\n | \n\n Lunch<\/span><\/span><\/p>\n<\/div>\n<\/td>\n<\/tr>\n\n| 14:00-14:20<\/td>\n | <\/td>\n | \n\n Latest Progress in STUDIES;<\/span><\/span><\/p>\nWei-Hao Wang (ASIAA)<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n\n| 14:20-14:40<\/td>\n | <\/td>\n | \n\n HASHTAG & DOWSING: Understanding Nearby Galaxies with SCUBA-2;<\/span><\/span><\/p>\nMatt Smith (UK)<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n\n| 14:40-15:00<\/td>\n | <\/td>\n | \n\n \n Mapping the Decline with Redshift of Dusty Star-forming Galaxies Using JWST and SCUBA-2;<\/span><\/span><\/p>\nAmy Barger (USA)<\/span><\/div>\n<\/div>\n<\/div>\n<\/td>\n<\/tr>\n\n| 15:00-15:20<\/td>\n | <\/td>\n | \n\n \n \n MAJORS;<\/span><\/span><\/p>\nDavid Eden (UK)<\/span><\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/td>\n<\/tr>\n\n| 15:20-15:40<\/td>\n | <\/td>\n | \n\n \n \n \n Bridging the gap between local and extragalactic star formation: dense gas tracers in large galactic filament;<\/span><\/span><\/p>\nOrsolya Feher (UK)<\/span><\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/td>\n<\/tr>\n\n| 15;40-16:10<\/td>\n | <\/td>\n | \n\n \n \n \n coffee break<\/span><\/span><\/p>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/td>\n<\/tr>\n\n| 16:10-16:30<\/td>\n | <\/td>\n | \n\n \n \n \n \n The Nearby Evolved Stars Survey;<\/span><\/span><\/p>\nPeter Sciuna (ESO)<\/span><\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/td>\n<\/tr>\n\n| 16:30-16:50<\/td>\n | <\/td>\n | \n\n \n \n \n \n \n Early heterodyne results from NESS – The Nearby Evolved Stars Survey;<\/span><\/span><\/p>\nSofia Wallstrom (Leuven)<\/span><\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/td>\n<\/tr>\n\n| 16:50-17:10<\/td>\n | <\/td>\n | \n\n \n \n \n \n \n \n Role of magnetic field in cluster formation: A case study of G148.24+00.41 with JCMT SCUBA-2\/ POL-2;<\/span><\/span><\/p>\nVineet Rawat (India)<\/span><\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/td>\n<\/tr>\n\n| 17:10-17:30<\/td>\n | <\/td>\n | \n\n \n \n \n \n \n \n \n The Hawaii SCUBA-2 cluster lensing survey;<\/span><\/span><\/p>\nLennox 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\n| 17:30-17:50<\/td>\n | <\/td>\n | \n\n \n \n \n \n \n \n \n \n SPOTLESS: An efficient study of the densest regions in the Universe using near-infrared and submm observations;<\/span><\/span><\/p>\nTom 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\n| 17:50-18:10<\/td>\n | <\/td>\n | \n\n \n \n \n \n \n \n \n \n \n Dark Matter Halos and Star Formation Efficiencies of “Super-thin” Galaxies;<\/span><\/span><\/p>\nTim 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>\n Agenda- Day2<\/span><\/strong><\/p>\n\n\n\n| Time<\/td>\n | Chair<\/td>\n | \n\n \n Title and speaker<\/span><\/span><\/p>\n<\/div>\n<\/div>\n<\/td>\n<\/tr>\n\n| 9:00-9:20<\/td>\n | <\/td>\n | \n\n \n Dense cores are rare in high-latitude Planck Galactic cold clumps;<\/span><\/span><\/p>\nFengwe Xu (China) – remote<\/span><\/div>\n<\/div>\n<\/div>\n<\/td>\n<\/tr>\n\n| 9:20-9:40<\/td>\n | <\/td>\n | \n\n SCUBA-2 Ultra Deep Imaging EAO Survey<\/span><\/span><\/span><\/p>\n(STUDIES): Confusion-limited 450-micron Galaxy Number Counts and Machine Learning Identification;\u00a0<\/span>Zhen-Kai Gao (ASIAA\/NCU) – remote<\/span><\/div>\n<\/div>\n<\/td>\n<\/tr>\n\n| 9:40-10:00<\/td>\n | <\/td>\n | \n | | | | | | | | | | | | | | | | | | | |