{"id":26,"date":"2025-11-12T13:08:21","date_gmt":"2025-11-12T11:08:21","guid":{"rendered":"https:\/\/teams.issibern.ch\/thermonuclearx-raybursts\/?page_id=26"},"modified":"2025-12-17T15:52:17","modified_gmt":"2025-12-17T13:52:17","slug":"first-meeting","status":"publish","type":"page","link":"https:\/\/teams.issibern.ch\/thermonuclearx-raybursts\/first-meeting\/","title":{"rendered":"First meeting"},"content":{"rendered":"<p>The first meeting of the team will be held at <a href=\"http:\/\/www.issibj.ac.cn\">ISSI-Beijing<\/a>; follow the link for contact and other details.<\/p>\n<p>Please review the <a href=\"http:\/\/www.issibj.ac.cn\/au\/AboutUs\/\">code of conduct<\/a> prior to the meeting<\/p>\n<p>Remote attendees will be able to view the talks and present via Zoom (https:\/\/us06web.zoom.us\/j\/81609492942?pwd=eQZT1E5c9ZDKkrgwRhr1WYJMp4jKiS.1, passwd: 714733).<\/p>\n<p>We plan two excursions during the meeting, the first on the morning of Wednesday 26th November, the second on the afternoon of Friday 28th November. More details will be provided at the meeting<\/p>\n<table style=\"border-collapse: collapse;width: 97.522986%\" border=\"1\">\n<tbody>\n<tr style=\"background-color: #d9d9d9\">\n<td style=\"width: 2.569583%\">Date<\/td>\n<td style=\"width: 8.655495%\">Time (CST)<\/td>\n<td style=\"width: 6.226181%\">Speaker<\/td>\n<td style=\"width: 38.48068%\">Event\/title<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 2.569583%\">Monday 24th Nov<\/td>\n<td style=\"width: 8.655495%\">09:00\u201309:20<\/td>\n<td style=\"width: 6.226181%\"><\/td>\n<td style=\"width: 38.48068%\">Registration<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">09:20\u201309:30<\/td>\n<td style=\"width: 6.226181%\">TBA<\/td>\n<td style=\"width: 38.48068%\">Welcome &amp; logistics<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">09:30\u201310:30<\/td>\n<td style=\"width: 6.226181%\">Li, Z<\/td>\n<td style=\"width: 38.48068%\">Team Progress on thermonuclear X-ray bursts<\/td>\n<\/tr>\n<tr style=\"background-color: #d9d9d9\">\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">10:30\u201311:00<\/td>\n<td style=\"width: 6.226181%\"><\/td>\n<td style=\"width: 38.48068%\">coffee break &amp; team photo<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">11:00\u201312:00<\/td>\n<td style=\"width: 6.226181%\">Galloway<\/td>\n<td style=\"width: 38.48068%\"><a href=\"https:\/\/next.issibern.ch\/f\/5519498\">State of the art of model &amp; observation comparisons<\/a><\/td>\n<\/tr>\n<tr style=\"background-color: #d9d9d9\">\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">12:00\u201314:00<\/td>\n<td style=\"width: 6.226181%\"><\/td>\n<td style=\"width: 38.48068%\">lunch at NSSC<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">14:00\u201315:00<\/td>\n<td style=\"width: 6.226181%\">Liu, H<\/td>\n<td style=\"width: 38.48068%\">Accreting neutron stars: Thermal evolution and Type I X-ray bursts<\/td>\n<\/tr>\n<tr style=\"background-color: #d9d9d9\">\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">15:00\u201315:30<\/td>\n<td style=\"width: 6.226181%\"><\/td>\n<td style=\"width: 38.48068%\">coffee break<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">16:15\u201317:30<\/td>\n<td style=\"width: 6.226181%\"><\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">Discussion (X-ray burst numerical modeling, including light curve simulation via KEPLER, MESA and HERES)<\/span><\/td>\n<\/tr>\n<tr style=\"background-color: #d9d9d9\">\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">17:30\u2013<\/td>\n<td style=\"width: 6.226181%\"><\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">dinner at NSSC<\/span><\/td>\n<\/tr>\n<tr>\n<td style=\"width: 2.569583%\">Tuesday 25th Nov<\/td>\n<td style=\"width: 8.655495%\">09:00\u201310:00<\/td>\n<td style=\"width: 6.226181%\">Aoyama<\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">Thermonuclear superburst of MAXI J1752-457 observed with NinjaSat and MAXI<\/span><\/td>\n<\/tr>\n<tr style=\"background-color: #d9d9d9\">\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">10:00\u201310:30<\/td>\n<td style=\"width: 6.226181%\"><\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">coffee break<\/span><\/td>\n<\/tr>\n<tr>\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">10:30\u201311:30<\/td>\n<td style=\"width: 6.226181%\">Dohi<\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">NinjaSat Observation of Clocked Bursters and Its Implication<\/span><\/td>\n<\/tr>\n<tr>\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">11:30\u201312:00<\/td>\n<td style=\"width: 6.226181%\">\u00a0Fu, T<\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">A comprehensive study of type I (thermonuclear) bursts in the new transient SRGA J144459.2\u2013604207<\/span><\/td>\n<\/tr>\n<tr style=\"background-color: #d9d9d9\">\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">12:00\u201314:00<\/td>\n<td style=\"width: 6.226181%\"><\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">lunch at NSSC<\/span><\/td>\n<\/tr>\n<tr>\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">14:00\u201315:00<\/td>\n<td style=\"width: 6.226181%\">Cavecchi<\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">The relation between accretion and burst recurrence time<\/span><\/td>\n<\/tr>\n<tr style=\"background-color: #d9d9d9\">\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">15:00\u201315:30<\/td>\n<td style=\"width: 6.226181%\"><\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">coffee break<\/span><\/td>\n<\/tr>\n<tr>\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">15:30\u201316:30<\/td>\n<td style=\"width: 6.226181%\">Speicher, J<\/td>\n<td style=\"width: 38.48068%\">Type I X-ray bursts as probes of the neutron star accretion flow<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">16:30\u201317:30<\/td>\n<td style=\"width: 6.226181%\"><\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">Discussion (How to understand mdot~trec relation especially for the case of SRGA J144459.2\u2014604207? constraints on the neutron star mass and radius: data &amp; method &amp; source list &amp; \u2026; How to define PRE bursts ?)<\/span><\/td>\n<\/tr>\n<tr style=\"background-color: #d9d9d9\">\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">18:00\u2013<\/td>\n<td style=\"width: 6.226181%\"><\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">ISSI-Beijing welcome dinner &amp; reception at the hotel (Park Plaza Beijing Science Park).<\/span><\/td>\n<\/tr>\n<tr>\n<td style=\"width: 2.569583%\">Wednesday 26th Nov<\/td>\n<td style=\"width: 8.655495%\">09:00\u201312:00<\/td>\n<td style=\"width: 6.226181%\"><\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">excursion to the Forbidden City (Z. Li will order the tickets, a passport number is required.)<\/span><\/td>\n<\/tr>\n<tr style=\"background-color: #d9d9d9\">\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">12:00\u201314:00<\/td>\n<td style=\"width: 6.226181%\"><\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">lunch (back at NSSC or we can find local food.)<\/span><\/td>\n<\/tr>\n<tr>\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">14:00\u201315:00<\/td>\n<td style=\"width: 6.226181%\">Ji, L<\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\"> Study of accretion flows using Type-I bursts<\/span><\/td>\n<\/tr>\n<tr style=\"background-color: #d9d9d9\">\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">15:00\u201315:30<\/td>\n<td style=\"width: 6.226181%\"><\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">\u00a0coffee break<\/span><\/td>\n<\/tr>\n<tr>\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">15:30\u201316:30<\/td>\n<td style=\"width: 6.226181%\">Lam, Y<\/td>\n<td style=\"width: 38.48068%\">\n<div dir=\"ltr\" data-setdir=\"false\">Key Role of Thermonuclear Reactions in Understanding the Type-I X-ray Bursts<\/div>\n<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">16:30\u201317:30<\/td>\n<td style=\"width: 6.226181%\"><\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\"> Discussion (X-ray burst data collection and analysis from NICER, MAXI, HXMT, NuSTAR, NinjaSat, especially intermediate-duration and super bursts)<\/span><\/td>\n<\/tr>\n<tr style=\"background-color: #d9d9d9\">\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">17:30\u2013<\/td>\n<td style=\"width: 6.226181%\"><\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">\u00a0dinner at NSSC<\/span><\/td>\n<\/tr>\n<tr>\n<td style=\"width: 2.569583%\">Thursday 27th Nov<\/td>\n<td style=\"width: 8.655495%\">09:00\u201310:00<\/td>\n<td style=\"width: 6.226181%\">Zhang, G<\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\"> An Investigation of Multi-peaked Type-I X-ray Bursts<\/span><\/td>\n<\/tr>\n<tr style=\"background-color: #d9d9d9\">\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">10:00\u201310:30<\/td>\n<td style=\"width: 6.226181%\"><\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">\u00a0coffee break<\/span><\/td>\n<\/tr>\n<tr>\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">10:30\u201311:00<\/td>\n<td style=\"width: 6.226181%\">Zhang, L<\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\"> A transition from mixed-fuel to pure-helium thermonuclear bursts in Terzan 5 X-3<\/span><\/td>\n<\/tr>\n<tr>\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">11:00\u201311:30<\/td>\n<td style=\"width: 6.226181%\">Peng, Z<\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">Quenching and recovery of persistent X-ray emission during a superburst in 4U 1820-30<\/span><\/td>\n<\/tr>\n<tr>\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">11:30-12:00<\/td>\n<td style=\"width: 6.226181%\">Cheng, H.Q.<\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">Einstein Probe (EP): an X-ray mission for time-domain astronomy<\/span><\/td>\n<\/tr>\n<tr style=\"background-color: #d9d9d9\">\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">12:00\u201314:00<\/td>\n<td style=\"width: 6.226181%\"><\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">\u00a0lunch at NSSC<\/span><\/td>\n<\/tr>\n<tr>\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">14:00\u201315:00<\/td>\n<td style=\"width: 6.226181%\">Casten<\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">Hydrogen-Triggered X-ray Bursts: Linking Observations and Theory<\/span><\/td>\n<\/tr>\n<tr style=\"background-color: #d9d9d9\">\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">15:00\u201315:30<\/td>\n<td style=\"width: 6.226181%\"><\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">\u00a0coffee break<\/span><\/td>\n<\/tr>\n<tr>\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">15:30\u201316:30<\/td>\n<td style=\"width: 6.226181%\">Jaisawal, G<\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">NICER studies of thermonuclear X-ray bursts (remote)<\/span><\/td>\n<\/tr>\n<tr>\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">16:30\u201317:30<\/td>\n<td style=\"width: 6.226181%\"><\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\"> Discussion (multi-wavelength observations, EP, SVOM, FAST and others; burst-disk interactions, does persistent emission variation model always work?)<\/span><\/td>\n<\/tr>\n<tr style=\"background-color: #d9d9d9\">\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">17:30\u2013<\/td>\n<td style=\"width: 6.226181%\"><\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">\u00a0dinner at NSSC<\/span><\/td>\n<\/tr>\n<tr>\n<td style=\"width: 2.569583%\">Friday 28th Nov<\/td>\n<td style=\"width: 8.655495%\">09:00\u201310:00<\/td>\n<td style=\"width: 6.226181%\">Li, H<\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">Polar Mounds on Strangeon Stars: the Neutrino Emission from Ultraluminous X-ray Pulsars<\/span><\/td>\n<\/tr>\n<tr style=\"background-color: #d9d9d9\">\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">10:00\u201310:30<\/td>\n<td style=\"width: 6.226181%\"><\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">\u00a0coffee break<\/span><\/td>\n<\/tr>\n<tr>\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">10:30\u201311:30<\/td>\n<td style=\"width: 6.226181%\"><\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">Discussion (future missions, such as HUBS, eXTP; spectral lines\/edges detections; finalize the schedule\/date for the next ISSI-Bern meeting)<\/span><\/td>\n<\/tr>\n<tr style=\"background-color: #d9d9d9\">\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">11:30\u201312:00<\/td>\n<td style=\"width: 6.226181%\"><\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">lunch\u00a0<\/span><\/td>\n<\/tr>\n<tr>\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">12:30\u2013<\/td>\n<td style=\"width: 6.226181%\"><\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">take a bus on the front door of the hotel, and excursion to the Great Wall\u00a0<\/span><\/td>\n<\/tr>\n<tr style=\"background-color: #d9d9d9\">\n<td style=\"width: 2.569583%\"><\/td>\n<td style=\"width: 8.655495%\">18:00\u2013<\/td>\n<td style=\"width: 6.226181%\"><\/td>\n<td style=\"width: 38.48068%\"><span data-sheets-root=\"1\">dinner (we will find local food.)<\/span><\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n","protected":false},"excerpt":{"rendered":"<p>The first meeting of the team will be held at ISSI-Beijing; follow the link for contact and other details. Please review the code of conduct prior to the meeting Remote attendees will be able to view the talks and present via Zoom (https:\/\/us06web.zoom.us\/j\/81609492942?pwd=eQZT1E5c9ZDKkrgwRhr1WYJMp4jKiS.1, passwd: 714733). We plan two excursions during the meeting, the first on [&hellip;]<\/p>\n","protected":false},"author":170,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-26","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/teams.issibern.ch\/thermonuclearx-raybursts\/wp-json\/wp\/v2\/pages\/26","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/teams.issibern.ch\/thermonuclearx-raybursts\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/teams.issibern.ch\/thermonuclearx-raybursts\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/teams.issibern.ch\/thermonuclearx-raybursts\/wp-json\/wp\/v2\/users\/170"}],"replies":[{"embeddable":true,"href":"https:\/\/teams.issibern.ch\/thermonuclearx-raybursts\/wp-json\/wp\/v2\/comments?post=26"}],"version-history":[{"count":30,"href":"https:\/\/teams.issibern.ch\/thermonuclearx-raybursts\/wp-json\/wp\/v2\/pages\/26\/revisions"}],"predecessor-version":[{"id":64,"href":"https:\/\/teams.issibern.ch\/thermonuclearx-raybursts\/wp-json\/wp\/v2\/pages\/26\/revisions\/64"}],"wp:attachment":[{"href":"https:\/\/teams.issibern.ch\/thermonuclearx-raybursts\/wp-json\/wp\/v2\/media?parent=26"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}