{"id":13270,"date":"2026-01-05T11:37:16","date_gmt":"2026-01-05T03:37:16","guid":{"rendered":"https:\/\/www.cag.ntnu.edu.tw\/?page_id=13270"},"modified":"2026-06-01T10:45:59","modified_gmt":"2026-06-01T02:45:59","slug":"seminars-latest-zh","status":"publish","type":"page","link":"https:\/\/www.cag.ntnu.edu.tw\/index.php\/seminars-latest-zh\/","title":{"rendered":"\u5c08\u984c\u6f14\u8b1b2026"},"content":{"rendered":"\t\t<div data-elementor-type=\"wp-page\" data-elementor-id=\"13270\" class=\"elementor elementor-13270\">\n\t\t\t\t\t\t<section class=\"elementor-section elementor-top-section elementor-element elementor-element-d3fc656 elementor-section-boxed elementor-section-height-default elementor-section-height-default\" data-id=\"d3fc656\" data-element_type=\"section\">\n\t\t\t\t\t\t<div class=\"elementor-container elementor-column-gap-default\">\n\t\t\t\t\t<div class=\"elementor-column elementor-col-100 elementor-top-column elementor-element elementor-element-3955487d\" data-id=\"3955487d\" data-element_type=\"column\">\n\t\t\t<div class=\"elementor-widget-wrap elementor-element-populated\">\n\t\t\t\t\t\t<div class=\"elementor-element elementor-element-2f4de2c0 elementor-widget elementor-widget-heading\" data-id=\"2f4de2c0\" data-element_type=\"widget\" data-widget_type=\"heading.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t\t\t<h2 class=\"elementor-heading-title elementor-size-default\">\u5c08\u984c\u6f14\u8b1b 2026<\/h2>\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t<div class=\"elementor-element elementor-element-324a0279 elementor-widget-divider--view-line elementor-widget elementor-widget-divider\" data-id=\"324a0279\" data-element_type=\"widget\" data-widget_type=\"divider.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t\t\t\t\t<div class=\"elementor-divider\">\n\t\t\t<span class=\"elementor-divider-separator\">\n\t\t\t\t\t\t<\/span>\n\t\t<\/div>\n\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/section>\n\t\t\t\t<section class=\"elementor-section elementor-top-section elementor-element elementor-element-5e596f38 elementor-section-boxed elementor-section-height-default elementor-section-height-default\" data-id=\"5e596f38\" data-element_type=\"section\">\n\t\t\t\t\t\t<div class=\"elementor-container elementor-column-gap-default\">\n\t\t\t\t\t<div class=\"elementor-column elementor-col-100 elementor-top-column elementor-element elementor-element-74191034\" data-id=\"74191034\" data-element_type=\"column\">\n\t\t\t<div class=\"elementor-widget-wrap elementor-element-populated\">\n\t\t\t\t\t\t<div class=\"elementor-element elementor-element-5fab2fa6 elementor-widget elementor-widget-text-editor\" data-id=\"5fab2fa6\" data-element_type=\"widget\" data-widget_type=\"text-editor.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t\t\t\t\t\t\t<p>\u9031\u56db\u4e2d\u5348\u5b9a\u671f\u8209\u8fa6<b>\u5c08\u984c\u6f14\u8b1b<\/b><\/p><p>\u5730\u9ede\uff1a\u6559\u5b78\u7814\u7a76\u5927\u6a13 S801-2\u8b1b\u5802<\/p><p>\u6642\u9593\uff1a12:20-13:20<\/p><ul><li><span style=\"font-size: 15px; color: var( --e-global-color-text );\">\u7269\u7406\u5b78\u7cfb\u8207\u5730\u7403\u79d1\u5b78\u7cfb\u5c08\u984c\u6f14\u8b1b\u6642\u9593\u5730\u9ede\u8acb\u898b\u7cfb\u7db2\u516c\u544a<\/span><\/li><li><b>\u5167\u90e8\u6f14\u8b1b<\/b>\u8207<b>\u5c08\u984c\u7814\u8b1b<\/b>\u9694\u9031\u8f2a\u6d41\u8fa6\u7406\uff0c\u7531\u4e2d\u5fc3\u6210\u54e1\u4e3b\u8b1b<\/li><\/ul>\t\t\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/section>\n\t\t\t\t<section class=\"elementor-section elementor-top-section elementor-element elementor-element-3d0e50dc elementor-section-boxed elementor-section-height-default elementor-section-height-default\" data-id=\"3d0e50dc\" data-element_type=\"section\">\n\t\t\t\t\t\t<div class=\"elementor-container elementor-column-gap-default\">\n\t\t\t\t\t<div class=\"elementor-column elementor-col-100 elementor-top-column elementor-element elementor-element-766e6752\" data-id=\"766e6752\" data-element_type=\"column\">\n\t\t\t<div class=\"elementor-widget-wrap elementor-element-populated\">\n\t\t\t\t\t\t<div class=\"elementor-element elementor-element-b06f459 elementor-widget elementor-widget-accordion\" data-id=\"b06f459\" data-element_type=\"widget\" data-widget_type=\"accordion.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t\t\t\t\t<div class=\"elementor-accordion\">\n\t\t\t\t\t\t\t<div class=\"elementor-accordion-item\">\n\t\t\t\t\t<div id=\"elementor-tab-title-1851\" class=\"elementor-tab-title\" data-tab=\"1\" role=\"button\" aria-controls=\"elementor-tab-content-1851\" aria-expanded=\"false\">\n\t\t\t\t\t\t\t\t\t\t\t\t\t<span class=\"elementor-accordion-icon elementor-accordion-icon-left\" aria-hidden=\"true\">\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<span class=\"elementor-accordion-icon-closed\"><i class=\"fas fa-plus-circle\"><\/i><\/span>\n\t\t\t\t\t\t\t\t<span class=\"elementor-accordion-icon-opened\"><i class=\"fas fa-star\"><\/i><\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t<a class=\"elementor-accordion-title\" tabindex=\"0\">2026\/06\/04 Hau-Yu Liu (NSYSU): The Quest for Planet Formation: Insights from Protoplanetary Disks<\/a>\n\t\t\t\t\t<\/div>\n\t\t\t\t\t<div id=\"elementor-tab-content-1851\" class=\"elementor-tab-content elementor-clearfix\" data-tab=\"1\" role=\"region\" aria-labelledby=\"elementor-tab-title-1851\"><p>Are we alone? You often hear this question because the formation of a terrestrial planet had been, theoretically, considered difficult if not impossible. This was changed after the NASA Kepler and K2 missions found that rocky planets are ubiquitous. Afterwards, it has become popular to resolve the natal environment of rocky planets, the protoplanetary disks, and then investigate the planet-formation activities observationally\/theoretically. Without a surprise, most of those studies concluded that the protoplanetary disks we resolved are efficiently forming rocky planets, which, however, yield planets that are too wet and too carbonaceous to compare with our own Earth. Are we not alone? This is the issue I have been tackling. In this talk, I will provide an overview of this research field and outline our contribution\/destruction.<\/p><\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t\t\t<div class=\"elementor-accordion-item\">\n\t\t\t\t\t<div id=\"elementor-tab-title-1852\" class=\"elementor-tab-title\" data-tab=\"2\" role=\"button\" aria-controls=\"elementor-tab-content-1852\" aria-expanded=\"false\">\n\t\t\t\t\t\t\t\t\t\t\t\t\t<span class=\"elementor-accordion-icon elementor-accordion-icon-left\" aria-hidden=\"true\">\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<span class=\"elementor-accordion-icon-closed\"><i class=\"fas fa-plus-circle\"><\/i><\/span>\n\t\t\t\t\t\t\t\t<span class=\"elementor-accordion-icon-opened\"><i class=\"fas fa-star\"><\/i><\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t<a class=\"elementor-accordion-title\" tabindex=\"0\">2026\/03\/03 Cheryl Lau (NSTC research scholar) : Stellar feedback and how they shape the interstellar medium<\/a>\n\t\t\t\t\t<\/div>\n\t\t\t\t\t<div id=\"elementor-tab-content-1852\" class=\"elementor-tab-content elementor-clearfix\" data-tab=\"2\" role=\"region\" aria-labelledby=\"elementor-tab-title-1852\"><p>Feedback from massive stars is one of the greatest sources of energy and momentum in the interstellar medium (ISM). Ionizing radiation, stellar winds and supernovae collectively shape the molecular clouds, the birthplace of stars, as well as their host galaxies. They play a significant role in regulating the entire star formation process.<\/p><p>In this colloquium, I will provide an overview of how feedback interacts with the ISM, and how astrophysicists examine their impact using state-of-the-art computational simulations. Specifically, I will discuss why the highly-asymmetrical nature of supernova remnants may impose a problem to our current feedback models. I will demonstrate that supernovae could actually induce a higher\u00a0<span lang=\"EN-GB\">dynamical impact to its local ISM than what was previously expected.\u00a0<\/span><\/p><div><span lang=\"EN-GB\"> [CAG-ES joint colloquium] Venue: Room S101, 1F, Research Building\u00a0\u00a0(S101 \u6559\u5b78\u7814\u7a76\u5927\u6a13)<\/span><\/div><\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t\t\t<div class=\"elementor-accordion-item\">\n\t\t\t\t\t<div id=\"elementor-tab-title-1853\" class=\"elementor-tab-title\" data-tab=\"3\" role=\"button\" aria-controls=\"elementor-tab-content-1853\" aria-expanded=\"false\">\n\t\t\t\t\t\t\t\t\t\t\t\t\t<span class=\"elementor-accordion-icon elementor-accordion-icon-left\" aria-hidden=\"true\">\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<span class=\"elementor-accordion-icon-closed\"><i class=\"fas fa-plus-circle\"><\/i><\/span>\n\t\t\t\t\t\t\t\t<span class=\"elementor-accordion-icon-opened\"><i class=\"fas fa-star\"><\/i><\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t<a class=\"elementor-accordion-title\" tabindex=\"0\">2026\/04\/21 Prof. Sut-Leng Tam (Institute of Physics, NYCU): Using Gravitational Lensing to Study Dark Matter in our Universe<\/a>\n\t\t\t\t\t<\/div>\n\t\t\t\t\t<div id=\"elementor-tab-content-1853\" class=\"elementor-tab-content elementor-clearfix\" data-tab=\"3\" role=\"region\" aria-labelledby=\"elementor-tab-title-1853\"><p>In the standard cosmological model, the matter content of the Universe is dominated by dark matter\u2014an invisible component that governs the formation and evolution of cosmic structures. While dark matter cannot be observed directly, its gravitational influence can be detected through the deflection of light from background sources, a phenomenon known as gravitational lensing. In this\u00a0talk, I will introduce the gravitational lensing effect in galaxy clusters and explain how it serves as a powerful probe for detecting dark matter and constraining its physical properties. I will also present a new approach by using radial acceleration relation to constrain the dark matter self-interacting cross-section.\u00a0<\/p><p>[CAG-ES joint colloquium] Venue: Room S101, 1F, Research Building\u00a0\u00a0(S101 \u6559\u5b78\u7814\u7a76\u5927\u6a13)<\/p><\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t\t\t<div class=\"elementor-accordion-item\">\n\t\t\t\t\t<div id=\"elementor-tab-title-1854\" class=\"elementor-tab-title\" data-tab=\"4\" role=\"button\" aria-controls=\"elementor-tab-content-1854\" aria-expanded=\"false\">\n\t\t\t\t\t\t\t\t\t\t\t\t\t<span class=\"elementor-accordion-icon elementor-accordion-icon-left\" aria-hidden=\"true\">\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<span class=\"elementor-accordion-icon-closed\"><i class=\"fas fa-plus-circle\"><\/i><\/span>\n\t\t\t\t\t\t\t\t<span class=\"elementor-accordion-icon-opened\"><i class=\"fas fa-star\"><\/i><\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t<a class=\"elementor-accordion-title\" tabindex=\"0\">2026\/04\/23 Martin Spinrath (NTHU): Three Ideas for Quantum Sensors in Neutrino Physics<\/a>\n\t\t\t\t\t<\/div>\n\t\t\t\t\t<div id=\"elementor-tab-content-1854\" class=\"elementor-tab-content elementor-clearfix\" data-tab=\"4\" role=\"region\" aria-labelledby=\"elementor-tab-title-1854\"><p>In my talk, I want to discuss three ideas on how one could use quantum sensors for neutrino physics. I will discuss first how to use SQUIDs or similar devices to constrain neutrino charges. In the second half of my talk, I will discuss the detection prospects to use laser and atom interferometers to look for the Cosmic Neutrino Background. I will also briefly mention Dark Matter in that part.<\/p><\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t\t\t<div class=\"elementor-accordion-item\">\n\t\t\t\t\t<div id=\"elementor-tab-title-1855\" class=\"elementor-tab-title\" data-tab=\"5\" role=\"button\" aria-controls=\"elementor-tab-content-1855\" aria-expanded=\"false\">\n\t\t\t\t\t\t\t\t\t\t\t\t\t<span class=\"elementor-accordion-icon elementor-accordion-icon-left\" aria-hidden=\"true\">\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<span class=\"elementor-accordion-icon-closed\"><i class=\"fas fa-plus-circle\"><\/i><\/span>\n\t\t\t\t\t\t\t\t<span class=\"elementor-accordion-icon-opened\"><i class=\"fas fa-star\"><\/i><\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t<a class=\"elementor-accordion-title\" tabindex=\"0\">2026\/05\/07 Hsu-Wen Chiang (SUSTech): Is vector perturbation stable with non-minimal coupling?<\/a>\n\t\t\t\t\t<\/div>\n\t\t\t\t\t<div id=\"elementor-tab-content-1855\" class=\"elementor-tab-content elementor-clearfix\" data-tab=\"5\" role=\"region\" aria-labelledby=\"elementor-tab-title-1855\"><p>A scalar field non-minimally coupled to the spacetime curvature could become unstable in a wide class of black hole and cosmological spacetimes, leading to potentially observable effects. One naturally asks if a similar situation happens for the vector field counterpart. We will show that the instability is well-controlled in all Petrov type D spacetimes filled with comoving perfect fluid,\u00a0including common cases such as FLRW, $\\Lambda$LTB, Kerr-Newman-(A)dS. Explicitly, at the linear order in the eikonal limit, one cannot trigger tachyonic instability without ghost and\/or gradient instabilities.<\/p><\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t\t\t<div class=\"elementor-accordion-item\">\n\t\t\t\t\t<div id=\"elementor-tab-title-1856\" class=\"elementor-tab-title\" data-tab=\"6\" role=\"button\" aria-controls=\"elementor-tab-content-1856\" aria-expanded=\"false\">\n\t\t\t\t\t\t\t\t\t\t\t\t\t<span class=\"elementor-accordion-icon elementor-accordion-icon-left\" aria-hidden=\"true\">\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<span class=\"elementor-accordion-icon-closed\"><i class=\"fas fa-plus-circle\"><\/i><\/span>\n\t\t\t\t\t\t\t\t<span class=\"elementor-accordion-icon-opened\"><i class=\"fas fa-star\"><\/i><\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t<a class=\"elementor-accordion-title\" tabindex=\"0\">2026\/05\/15 [CAG special lecture] Prof. Sebastien Charnoz* (IPGP, Institut of the Physics of the Earth): Origin of the Moon<\/a>\n\t\t\t\t\t<\/div>\n\t\t\t\t\t<div id=\"elementor-tab-content-1856\" class=\"elementor-tab-content elementor-clearfix\" data-tab=\"6\" role=\"region\" aria-labelledby=\"elementor-tab-title-1856\"><p>How did our Moon form, and when? What evidence supports its origin? While it is often said that the Moon formed from a giant impact, many mysteries remain unsolved. Even today, no single explanation fully aligns with both astronomical and geophysical data. I will review what we currently know about the Moon\u2019s formation, explore the different possible scenarios and their challenges, and discuss the critical new data needed in the future to better constrain the origin of our Moon. I will focus on the question of its composition and show that many mysteries are still standing with potentially \u00a0important implications for the formation of terrestrial planets.<\/p><p><strong>*About the speaker:<\/strong>\u00a0Sebastien Charnoz is a professor of planetary science at Paris University and IPGP (Institut of the physics of the Earth). He is a theoretician, specialist of planet formation and satellite formation. He\u00a0was a member\u00a0of the Cassini-Huygens missions, in the camera team, and is\u00a0now a member\u00a0of the MMX space mission to Phobos, and HERA space\u00a0mission\u00a0to \u00a0binary asteroids Didymos.<\/p><p>[CAG special lecture] Venue: Room E301, College of Science Building, Gongguan Campus<\/p><\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t\t\t<div class=\"elementor-accordion-item\">\n\t\t\t\t\t<div id=\"elementor-tab-title-1857\" class=\"elementor-tab-title\" data-tab=\"7\" role=\"button\" aria-controls=\"elementor-tab-content-1857\" aria-expanded=\"false\">\n\t\t\t\t\t\t\t\t\t\t\t\t\t<span class=\"elementor-accordion-icon elementor-accordion-icon-left\" aria-hidden=\"true\">\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<span class=\"elementor-accordion-icon-closed\"><i class=\"fas fa-plus-circle\"><\/i><\/span>\n\t\t\t\t\t\t\t\t<span class=\"elementor-accordion-icon-opened\"><i class=\"fas fa-star\"><\/i><\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t<a class=\"elementor-accordion-title\" tabindex=\"0\">2026\/05\/21 Dr. Yu-Hsuan (Eltha) Teng (University of Maryland): The rise and fall of star formation: probing the evolution of nearby galaxies<\/a>\n\t\t\t\t\t<\/div>\n\t\t\t\t\t<div id=\"elementor-tab-content-1857\" class=\"elementor-tab-content elementor-clearfix\" data-tab=\"7\" role=\"region\" aria-labelledby=\"elementor-tab-title-1857\"><p>Star formation activities characterize the evolutionary stages of galaxies. As stars are born from the cold and dense molecular clouds, star formation is governed by the amount of molecular gas and how efficiently molecular gas is converted into stars (i.e., the star formation efficiency, SFE). However, the physical mechanisms that alter the level of star formation in galaxies are not well understood, due to a lack of precise knowledge in molecular gas mass and SFE variations across galaxies at different evolutionary stages.<\/p><p>In this talk, I will present a series of work that tackle these challenges, using state-of-the-art telescopes including ALMA, JWST, and the Green Bank Telescope. We started by establishing an accurate, physics-grounded prescription for the CO-to-H2 conversion factor (\u03b1_CO) \u2014 a factor that has been causing major uncertainties in current molecular gas and SFE measurements. By re-evaluating molecular gas mass and SFE with our new prescription across ~150 galaxies ranging from starbursts to quiescent galaxies, we have revealed systematic differences in SFE which were obscured in previous studies due to limited \u03b1_CO knowledge. Our results show evidence that SFE variation is a dominant factor driving both the enhancement and regulation of star formation in galaxies. I will also talk about my ALMA and JWST programs in progress, which aim to uncover the exact molecular gas conditions and feedback processes that lead to galaxy quenching.\u00a0<\/p><\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t\t\t<div class=\"elementor-accordion-item\">\n\t\t\t\t\t<div id=\"elementor-tab-title-1858\" class=\"elementor-tab-title\" data-tab=\"8\" role=\"button\" aria-controls=\"elementor-tab-content-1858\" aria-expanded=\"false\">\n\t\t\t\t\t\t\t\t\t\t\t\t\t<span class=\"elementor-accordion-icon elementor-accordion-icon-left\" aria-hidden=\"true\">\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<span class=\"elementor-accordion-icon-closed\"><i class=\"fas fa-plus-circle\"><\/i><\/span>\n\t\t\t\t\t\t\t\t<span class=\"elementor-accordion-icon-opened\"><i class=\"fas fa-star\"><\/i><\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t<a class=\"elementor-accordion-title\" tabindex=\"0\">2026\/05\/26 [CAG-ES joint colloquium] Melaine Saillenfest (LTE, Paris Observatory): The MRT project: looking for Moons and Rings in Taiwan<\/a>\n\t\t\t\t\t<\/div>\n\t\t\t\t\t<div id=\"elementor-tab-content-1858\" class=\"elementor-tab-content elementor-clearfix\" data-tab=\"8\" role=\"region\" aria-labelledby=\"elementor-tab-title-1858\"><p>Discovering rings around exoplanets is among the next major milestones of extra-solar exploration. Yet, despite technical feasibility with existing instruments, no Saturn-like exoring has been confirmed to date. While part of the explanation is observational biases, the absence of detection also comes from our profound lack of knowledge about what are rings, how they form, and what are their lifetimes. With the MRT project (CAG, NTNU), we aim to answer these questions from the perspective of rings demographics in the Solar System. The existence of ring systems around small Solar System bodies gives us the opportunity of gathering many instances of rings, enabling statistical studies of their properties and natural evolution processes. To do so, the MRT project will run a network of telescopes dedicated to stellar occultations distributed across Taiwan\u2019s territory, while benefiting from theoretical advances brought by the companion French project WRAPS: \u201cWhere do Rings Appear in Planetary Systems?\u201d<\/p><p>[CAG-ES joint colloquium] Time:14:20 pm, Venue: Room S101, 1F, Research Building\u00a0\u00a0(S101 \u6559\u5b78\u7814\u7a76\u5927\u6a13)<\/p><\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t\t\t\t<\/div>\n\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/section>\n\t\t\t\t<\/div>\n\t\t","protected":false},"excerpt":{"rendered":"<p>\u5c08\u984c\u6f14\u8b1b 2026 \u9031\u56db\u4e2d\u5348\u5b9a\u671f\u8209\u8fa6\u5c08\u984c\u6f14\u8b1b \u5730\u9ede\uff1a\u6559\u5b78\u7814\u7a76\u5927\u6a13 S801-2\u8b1b\u5802 \u6642\u9593\uff1a12:20-13:2 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