[{"data":1,"prerenderedAt":-1},["ShallowReactive",2],{"detail-sidebar-cat-1-en-105":3,"doc-seo-243699-105":53,"doc-detail-243699-en":126},{"code":4,"msg":5,"data":6},0,"success",[7,14,19,24,29,34,39,44,49],{"id":8,"doc_module":9,"doc_module_name":10,"category_name":11,"show_sort_weight":12,"slug":13},11,1,"Template","Presentations",90,"presentations",{"id":15,"doc_module":9,"doc_module_name":10,"category_name":16,"show_sort_weight":17,"slug":18},12,"Resumes",80,"resumes",{"id":20,"doc_module":9,"doc_module_name":10,"category_name":21,"show_sort_weight":22,"slug":23},14,"Invoices",70,"invoices",{"id":25,"doc_module":9,"doc_module_name":10,"category_name":26,"show_sort_weight":27,"slug":28},15,"Posters",60,"posters",{"id":30,"doc_module":9,"doc_module_name":10,"category_name":31,"show_sort_weight":32,"slug":33},16,"Social Media",50,"social-media",{"id":35,"doc_module":9,"doc_module_name":10,"category_name":36,"show_sort_weight":37,"slug":38},17,"Forms",40,"forms",{"id":40,"doc_module":9,"doc_module_name":10,"category_name":41,"show_sort_weight":42,"slug":43},18,"Letters",30,"letters",{"id":45,"doc_module":9,"doc_module_name":10,"category_name":46,"show_sort_weight":47,"slug":48},21,"Paper Templates",5,"papers-templates",{"id":50,"doc_module":9,"doc_module_name":10,"category_name":51,"show_sort_weight":4,"slug":52},158,"General","general-158",{"code":4,"msg":54,"data":55},"ok",{"site_id":56,"language":57,"slug":58,"title":59,"keywords":60,"description":61,"schema_data":62,"social_meta":119,"head_meta":121,"extra_data":123,"updated_unix":125},105,"en","10-years-to-lisa-agenda","10 Years to LISA - Agenda","","Program agenda spanning three days in Pacific Time (4/1/25–4/3/25) for a LISA-focused symposium. The schedule opens with coffee, check-in, welcome, and announcements, then runs thematic sessions covering gravitational-wave telescopes and observations through 2040, electromagnetic telescopes and observations, and population studies of LISA MBHBs using current and future observational strategies. Additional sessions address simulation-based learning, EM counterparts to GW signals, and related discussions, with talks available in in-person and virtual formats.",{"@graph":63,"@context":118},[64,80,101],{"@type":65,"itemListElement":66},"BreadcrumbList",[67,71,74,77],{"item":68,"name":69,"@type":70,"position":9},"https://docshare.wps.com","Home","ListItem",{"item":72,"name":10,"@type":70,"position":73},"https://docshare.wps.com/template/",2,{"item":75,"name":11,"@type":70,"position":76},"https://docshare.wps.com/template/presentations/",3,{"item":78,"name":59,"@type":70,"position":79},"https://docshare.wps.com/template/10-years-to-lisa-agenda/243699/",4,{"url":78,"name":59,"@type":81,"image":82,"author":87,"headline":59,"publisher":90,"fileFormat":93,"inLanguage":57,"description":61,"dateModified":94,"datePublished":95,"encodingFormat":93,"isAccessibleForFree":96,"interactionStatistic":97},"DigitalDocument",{"url":83,"@type":84,"width":85,"height":86},"https://docshare.wps.com/thumbnails/10-years-to-lisa-agenda/243699.png","ImageObject",442,249,{"name":88,"@type":89},"Mason","Person",{"url":68,"name":91,"@type":92},"DocShare","Organization","application/pdf","2026-10-18","2026-09-12",true,{"@type":98,"interactionType":99,"userInteractionCount":8},"InteractionCounter",{"@type":100},"ViewAction",{"@type":102,"mainEntity":103},"FAQPage",[104,110,114],{"name":105,"@type":106,"acceptedAnswer":107},"What time zone is used for the agenda schedule?","Question",{"text":108,"@type":109},"All agenda times are listed in Pacific Time.","Answer",{"name":111,"@type":106,"acceptedAnswer":112},"Which topics are covered in the Tuesday sessions?",{"text":113,"@type":109},"Tuesday includes a gravitational-wave telescopes and observations session covering progress to 2040, and an electromagnetic telescopes and observations session covering the same timeframe.",{"name":115,"@type":106,"acceptedAnswer":116},"How does the Wednesday program approach LISA MBHB science?",{"text":117,"@type":109},"Wednesday focuses on inferring the population of LISA MBHBs from current and future observations, then moves to what simulations have taught, and concludes with sessions on electromagnetic counterparts to gravitational-wave signals.","https://schema.org",{"og:url":78,"og:type":120,"og:title":59,"og:site_name":91,"og:description":61},"article",{"robots":122,"canonical":78},"index,follow",{"doc_id":124,"site_id":56},243699,1791745554,{"code":4,"msg":5,"data":127},{"doc_id":124,"user_id":128,"nickname":88,"user_avatar":129,"doc_module":9,"category_id":8,"category_name":11,"doc_title":59,"doc_description":61,"doc_content":130,"file_id":131,"file_url":132,"file_type":133,"file_size":134,"view_count":8,"is_deleted":4,"is_public":9,"is_downloadable":9,"audit_status":9,"page_count":135,"language":136,"language_code":57,"site_id":56,"html_lang":57,"table_of_contents":137,"faqs":138,"seo_title":139,"seo_description":61,"update_tm":140,"read_time":76},5909887256941,"https://ap-avatar.wpscdn.com/davatar_9964176cb1d06d4a9deccf72a44ae3dc","10 Years to LISA  \nAgenda for Tuesday (4/1/25)–in Pacific Time  \n\n| Time | Item | Talks (inp = in-person, vir = virtual) |\n| --- | --- | --- |\n| 8:00-8:45 AM | Coffee + Check-in |  |\n| 8:45-8:55 AM | Welcome by Shouleh Nikzad, Manager of JPL’s Science Division |  |\n| 8:55-9:30 AM | Announcements |  |\n| 9:30-10:20 AM | Session 1 :\u003Cbr>Gravitational-Wave Telescopes and Observations--From now to 2040\u003Cbr>(Chair: D.H. Shoemaker), part 1 | Overview of the LISA Mission-status etc. , O. Jennrich, vir, 9:30-10:00am\u003Cbr>Cosmology from terrestrial detectors, T. Baker, vir, 10:00-10:20am |\n| 10:20-10:45 AM | Coffee Break + Welcome from JPL Director Laurie Leshin (10:30 – 10:35) |  |\n| 10:45AM-12:25PM | Session 1 :\u003Cbr>Gravitational-Wave Telescopes and Observations--From now to 2040\u003Cbr>(Chair: D.H. Shoemaker), part 2 | NS/nuclear physics inaccessible to LISA ,\u003Cbr>A. Steiner, vir, 10:45-11:05am\u003Cbr>DarkMatter/exotica/surprises from terrestrial detectors, Sathyaprakash, vir, 11:05-11:25am\u003Cbr>Current ground based detectors and their likely evolution to 2040 , L.Thomas, vir, 11:25-11:45am\u003Cbr>ET/CE--what we hope to build, and what we could optimistically do by 2040 , J. Smith, inp. 11:45am-\u003Cbr>12:05\u003Cbr>PTAs – evolution of the network and its sensitivity, P. Meyers, inp , 12:05-12:25pm |\n| 12:25-1:35 PM | Lunch |  |\n| 1:35-3:05 PM | Session 2: EM Telescopes and Observations--From now to 2040 (Chair: D. Stern) | Overview, K. Burdge, inp , 1:35-2:05pm\u003Cbr>Searching for Massive Black Hole Binaries DESI, A. Palmese, vir , 2:05-2:25pm |\n\n\n|  |  | How Can the NASA/IPAC Extragalactic Database (NED) Support LISA?, D. Cook, inp , 2:25-2:45pm\u003Cbr>The value of Direct Acceleration Measurements, T. Donlon, vir, 2:45-3:05pm |\n| --- | --- | --- |\n| 3:05-3:20 PM | Coffee Break |  |\n| 3:20-4:50 PM | Optional Tour of JPL |  |\n\n10 Years to LISA  \nAgenda for Wed (4/2/25) -in Pacific Time  \n\n| Time | Item | Talks (inp = in-person, vir = virtual) |\n| --- | --- | --- |\n| 8:00-8:45 AM | Coffee + Check-in |  |\n| 8:45-9:00 AM | Announcements |  |\n| 9:00-11:00 AM | Session 3 : The Population of LISA MBHBs: Inference from Current & Future Observations (Chair: P. Natarajan\u003Cbr>(Acting Chair on 4/2 is Z. Haiman) | Insights and Predictions from GRMHD Simulations of Supermassive Black Hole Mergers: Shaping Future Observational Strategies, M.Campanelli, inp, 9:05-9:30am\u003Cbr>Multi-band Gravitational-wave Astronomy with Intermediate-Mass Black Holes in LISA, K. Jani, vir, 9:30-9:55am\u003Cbr>Where are the supermassive black holes measured by PTAs?, G. Sato-Polito , vir, 9:55-10:20am\u003Cbr>Black Hole Masses Inferred from Scaling Relations and Their Effect on LISA Predictions, J. Comerford , inp, 10:20-10:30am\u003Cbr>Using Observations of Tidal Disruption Events to Forecast the Rates and Host Environments of LISA MBHBs, S. Gezari, vir,10:30-10:40am\u003Cbr>The status of black hole binary waveform modeling and the requirements for LISA, S. McWilliams, vir, 10:40-10:50am\u003Cbr>Stars or gas? Constraining the hardening processes of massive black-hole binaries with LISA , A. Spadaro , inp, 10:50-11:00am |\n| 11:00-11:20 AM | Coffee Break |  |\n\n\n|  |  |  |\n| --- | --- | --- |\n| 11:20AM-12:15PM | Session 4: The Population of LISA MBHBs: What we have learned from simulations (Chair:\u003Cbr>Alberto Sesana, Univ. of Milano-Bicocca), part 1\u003Cbr>(on 4/2, Acting In-person Chair is T. Di Matteo & Remote Chair is A. Sesana) | Tracking on-the-fly massive black hole binary evolution and coalescence in galaxy simulations:\u003Cbr>RAMCOAL, K. Li (co-author M. Volonteri) , vir, 11:20-11:45am\u003Cbr>The BRAHMA simulations: Unveiling the first seeds of supermassive black holes using cosmological simulations of merging black hole populations, A. Bhomwick, inp, 11:45-12:00pm\u003Cbr>What we learned from the LISA MBH Catalogs Project, M. Habouzit, vir, 12:00-12:15pm |\n| 12:15-1:30 PM | Lunch |  |\n| 1:30-2:35 PM | Session 4: The Population of LISA MBHBs: What we have learned from simulations (Chair:\u003Cbr>Alberto Sesana, Univ. of Milano-Bicocca), part 2 | A","cbCaicgRUkGTOU7d","https://ap.wps.com/l/cbCaicgRUkGTOU7d","pdf",339706,8,"English","# Tuesday (4/1/25)\n## Session 1: Gravitational-Wave Telescopes and Observations--From now to 2040\n## Session 2: EM Telescopes and Observations--From now to 2040\n# Wednesday (4/2/25)\n## Session 3: The Population of LISA MBHBs: Inference from Current & Future Observations\n## Session 4: The Population of LISA MBHBs: What we have learned from simulations\n## Session 5: EM Counterparts to GW Signals from MBHBs\n# Thursday (4/3/25)\n## Session 6: Galactic Binaries","[{\"question\":\"What time zone is used for the agenda schedule?\",\"answer\":\"All agenda times are listed in Pacific Time.\"},{\"question\":\"Which topics are covered in the Tuesday sessions?\",\"answer\":\"Tuesday includes a gravitational-wave telescopes and observations session covering progress to 2040, and an electromagnetic telescopes and observations session covering the same timeframe.\"},{\"question\":\"How does the Wednesday program approach LISA MBHB science?\",\"answer\":\"Wednesday focuses on inferring the population of LISA MBHBs from current and future observations, then moves to what simulations have taught, and concludes with sessions on electromagnetic counterparts to gravitational-wave signals.\"}]","10 Years to LISA - Agenda | PDF",1789207231]