{"id":8459,"date":"2024-11-25T09:02:27","date_gmt":"2024-11-25T08:02:27","guid":{"rendered":"https:\/\/www.lapth.cnrs.fr\/event\/line-intensity-mapping-2025-lim25\/"},"modified":"2025-05-08T14:05:00","modified_gmt":"2025-05-08T12:05:00","slug":"line-intensity-mapping-2025-lim25","status":"publish","type":"tribe_events","link":"https:\/\/www.lapth.cnrs.fr\/en\/event\/line-intensity-mapping-2025-lim25\/","title":{"rendered":"LIM25 &#8211; Annecy"},"content":{"rendered":"<p>Line intensity mapping (LIM) is an emerging observational technique with the potential to greatly enhance our understanding of both cosmology and astrophysics. By probing the large-scale structure of the universe in three dimensions across a wide range of scales and cosmic epochs, LIM offers the ability to tackle many unresolved questions in cosmology, such as the physics of inflation, the properties of neutrinos, the nature of dark matter and dark energy, and the theory of gravity. In astrophysics, LIM observations at different wavelengths enable us to investigate various phases of the interstellar and intergalactic medium, providing valuable insights into the processes behind reionization and galaxy formation. Performing intensity mapping in different wavelengths would enable us to obtain robust detection of LIM signals and assure their cosmological\/astrophysical origin, and enhance the scientific return of individual observations. Despite its promise, LIM is still a relatively young field, which naturally comes with a range of instrumental, observational, and theoretical challenges that need to be addressed. The success of LIM as a reliable probe in both astrophysics and cosmology therefore depends heavily on the collaboration of experts across these areas.<br \/>\n\u00a0<br \/>\nLIM25 conference, the 9th edition of a series that began in 2016 (last two at Max-Planck Institute for Astrophysics, Germany (2023), and University of Illinois, NCSA, USA (2024)), seeks to bring together specialists from various disciplines central to LIM research. The event will focus on addressing current challenges, showcasing recent advances, discussing obstacles encountered during early experiments, and exploring prospects for large-scale surveys. By fostering these interactions, the conference will help to maximize LIM\u2019s potential as a powerful tool for both cosmology and astrophysics, while cultivating a vibrant, collaborative scientific community.<br \/>\n\u00a0<br \/>\nThe event will be held in person and we anticipate an audience of 70\u2013100 participants.<br \/>\n\u00a0<br \/>\n\ud83c\udf89 REGISTERATION AND ABSRACT SUBMISSION NOW OPEN! \ud83c\udf89 Please follow the links on the left or below.<br \/>\n\u00a0<br \/>\n\ud83d\udea8 SCAM ALERT: Please be aware of fraudulent emails, e.g., from olivia@cermix.org or michael@funds-indico.org or lodging@conferencecare.org, claiming to offer hotel bookings or registration confirmations. Our conference does NOT have an official hotel booking agent, and all registrations are handled exclusively through the Indico page. Do not share personal or payment details with unknown senders.<br \/>\n\u00a0<br \/>\nConfirmed Invited Speakers:<br \/>\nTzu-Ching Chang (Jet Propulsion Laboratory, USA),Opportunities in Optical\/New Infrared Line Intensity Mapping<br \/>\nKieran Cleary (Caltech, USA), LIM with CO and COMAP<br \/>\nKirit Karkare (Boston University), Current and Future Technologies for Line Intensity Mapping<br \/>\nGuilaine Lagache (Laboratoire d\u2019Astrophysique de Marseille, France), Status of  Intensity Mapping in the Era of CONCERTO<br \/>\nSteven Murray (Scuola Normale Superiore di Pisa), Data Analysis Challenges in Line Intensity Mapping: a HERA perspective<br \/>\nRachel Somerville (CCA &#8211; Flatiron Institute, USA), LIM and Galaxy Formation<br \/>\nMatteo Viel (SISSA &#8211; Scuola Internazionale Studi Superiori Avanzati, Italy), Line Intensity Mapping and Cosmology<br \/>\nSaleem Zaroubi (University of Groningen, Netherlands),The Epoch of Reionization with 21 cm Intensity Mapping, an Overview of the Current Status<br \/>\n\u00a0<br \/>\nScientific Organizing Commity:\u00a0<br \/>\nReza Ansari (Universit\u00e9 Paris-Saclay &amp; CEA-Irfu, France)<br \/>\nJose Bernal (Instituto de F\u00edsica de Cantabria, Spain)<br \/>\nYi-Kuan Chiang (Academia Sinica Institute of Astronomy and Astrophysics, Taiwan)<br \/>\nDongwoo Chung (Cornell University, USA)<br \/>\nHoward Hui (California Institute of Technology, USA)<br \/>\nGarrett K. Keating (Harvard-Smithsonian Center for Astrophysics, USA)<br \/>\nAzadeh Moradinezhad (Laboratoire Annecy-le-Vieux de Physique Th\u00e9orique, France)<br \/>\nMarta Spinelli (Observatoire de la C\u00f4te d&#8217;Azur, France)<br \/>\nJoaquin Vieira (University of Illinois | NCSA, USA)<br \/>\nJessica Avva Zebrowski (University of Chicago, USA)<br \/>\nLocal Organizing Commity:\u00a0<br \/>\nAzadeh Moradinezhad (Laboratoire Annecy-le-Vieux de Physique Th\u00e9orique, France)<br \/>\nPasquale Serpico (Laboratoire Annecy-le-Vieux de Physique Th\u00e9orique, France)<br \/>\nReza Ansari (Universit\u00e9 Paris-Saclay &amp; CEA-Irfu, France)<br \/>\nMarta Spinelli (Observatoire de la C\u00f4te d&#8217;Azur, France)<br \/>\nAdminstrative Support:\u00a0<br \/>\nV\u00e9ronique Journey<br \/>\nVirginie Malaval<br \/>\nDominique Turc<br \/>\nFinancial Sponsors: CNRS-INSU, USMB, LAPTh, enigmass+, CPTGA\u00a0<br \/>\n\u00a0<br \/>\nhttps:\/\/indico.in2p3.fr\/event\/33647\/<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Line intensity mapping (LIM) is an emerging observational technique with the potential to greatly enhance our understanding of both cosmology and astrophysics. By probing the large-scale structure of the universe [&hellip;]<\/p>\n","protected":false},"author":8,"featured_media":0,"template":"","meta":{"_acf_changed":false,"_tribe_events_status":"","_tribe_events_status_reason":"","footnotes":""},"tags":[],"tribe_events_cat":[],"class_list":["post-8459","tribe_events","type-tribe_events","status-publish","hentry"],"acf":[],"_links":{"self":[{"href":"https:\/\/www.lapth.cnrs.fr\/en\/wp-json\/wp\/v2\/tribe_events\/8459","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.lapth.cnrs.fr\/en\/wp-json\/wp\/v2\/tribe_events"}],"about":[{"href":"https:\/\/www.lapth.cnrs.fr\/en\/wp-json\/wp\/v2\/types\/tribe_events"}],"author":[{"embeddable":true,"href":"https:\/\/www.lapth.cnrs.fr\/en\/wp-json\/wp\/v2\/users\/8"}],"version-history":[{"count":4,"href":"https:\/\/www.lapth.cnrs.fr\/en\/wp-json\/wp\/v2\/tribe_events\/8459\/revisions"}],"predecessor-version":[{"id":11027,"href":"https:\/\/www.lapth.cnrs.fr\/en\/wp-json\/wp\/v2\/tribe_events\/8459\/revisions\/11027"}],"wp:attachment":[{"href":"https:\/\/www.lapth.cnrs.fr\/en\/wp-json\/wp\/v2\/media?parent=8459"}],"wp:term":[{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.lapth.cnrs.fr\/en\/wp-json\/wp\/v2\/tags?post=8459"},{"taxonomy":"tribe_events_cat","embeddable":true,"href":"https:\/\/www.lapth.cnrs.fr\/en\/wp-json\/wp\/v2\/tribe_events_cat?post=8459"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}