BEGIN:VCALENDAR VERSION:2.0 PRODID:-//AIP Calendar//www.aip.de// METHOD:PUBLISH BEGIN:VEVENT SUMMARY:Colloquium | Tobias Buck (Heidelberg) DTSTART:20261119T133000Z DTEND:20261119T143000Z DTSTAMP:20260619T183048Z UID:www.aip.de-2306 CATEGORIES:Scientific CATEGORIES:Generic Event CATEGORIES:Public CONTACT:Ewald Puchwein DESCRIPTION:Speaker: Tobias Buck (Heidelberg)\nTitle: TBD\n LOCATION:AIP\; Kirch building\, Conference room END:VEVENT BEGIN:VEVENT SUMMARY:Colloquium | Alessandro Morbidelli DTSTART:20260521T123000Z DTEND:20260521T133000Z DTSTAMP:20260619T183048Z UID:www.aip.de-2351 CATEGORIES:Scientific CATEGORIES:Scientific Talk CATEGORIES:Public CATEGORIES:Colloquium CONTACT:Julián Alvarado-Gómez DESCRIPTION:Speaker: Alessandro Morbidelli (Observatoire de la Cote d' \;Azur | Nice\, France)\nTitle: Formation and evolution of a protoplanetar y disk: combining observations\, simulations and cosmochemical constraints \nAbstract: Observations of protoplanetary disks with ALMA have revealed a large diversity of properties\, but also some common tendencies in terms of dust/gas density and radial extension ratios\, as well as the appearanc e of features like rings and gaps or cavities. It is too late to observe t he proto-solar disk\, but many of its properties can be inferred from the current distribution of planetesimals and using cosmochemical constraints on the chronology of planetesimal accretion and the isotopic heterogeneity of the disk. I will review the available data which can be used to recons truct the proto-solar disk. The view that emerges is that of a quite stand ard disk of about 90 au in gas radius and 45 au in dust radius\, forming p lanetesimals at two distinct epochs (one of which very early\, while the d isk was presumably still in Class-0 or Class-1 stage) and evolving towards a transition disk at the appearance of Jupiter and Saturn. Similarities a nd differences with the PDS70 disk will be discussed.\nNote: Host: Oliver Gressel\n LOCATION:AIP\; Kirch building\, Conference room END:VEVENT BEGIN:VEVENT SUMMARY:Colloquium | Serena Criscuoli (National Solar Observatory | Boulde r\, CO\, USA) DTSTART:20260618T123000Z DTEND:20260618T133000Z DTSTAMP:20260619T183048Z UID:www.aip.de-2352 CATEGORIES:Scientific CATEGORIES:Scientific Talk CATEGORIES:Public CATEGORIES:Colloquium CONTACT:Julián Alvarado-Gómez DESCRIPTION:Speaker: Serena Criscuoli (National Solar Observatory | Boulde r\, CO\, USA)\nTitle: Using Spatially Resolved Solar Observations to Impro ve Models of Solar and Stellar Variability\nAbstract: Models of solar and stellar variability are essential for a wide range of applications\, from understanding the influence of solar irradiance on Earth's atmosphere to c haracterizing exoplanet host stars and improving the detectability of exop lanets. Over the past decades\, irradiance variability models have achieve d considerable success in reproducing many observed signatures of magnetic activity. However\, important discrepancies remain\, highlighting limitat ions in our understanding of how different atmospheric structures contribu te to spectral variability.\nIn this seminar\, I will provide a brief over view of current solar and stellar variability models\, discussing both the ir achievements and their outstanding challenges. I will then focus on one puzzling problem: the variability of the hydrogen Balmer lines. These lin es\, especially Hα\, Hβ\, Hγ\, and Hδ\, are among the most widely used diagnostics of stellar magnetic activity\, yet recent observations have r evealed complex and sometimes unexpected behavior\, including weak or even anti-correlated variations with traditional chromospheric activity indica tors such as the Ca II lines.\nI will present recent efforts to understand the origin of this behavior through a combination of disk-integrated obse rvations\, spatially resolved measurements\, and semi-empirical atmospheri c modeling. I will discuss how modern high-resolution observations enable us to identify the physical origins of these discrepancies and refine exis ting models. Particular attention will be given to recent observations acq uired with the IAG spectrograph and results from the Visible Spectro-Polar imeter (ViSP) at the Daniel K. Inouye Solar Telescope\, which provide new insights into the relationship between magnetic activity and Balmer-line v ariability in the Sun and solar-like stars. Finally\, I will present preli minary results from an analysis of synoptic ChroTel Hα and Ca II K observ ations\, which suggest that chromospheric features\, often neglected in cu rrent solar and stellar irradiance models\, may play a role in shaping chr omospheric variability\nNote: Host: Meetu Verma\n LOCATION:AIP\; Kirch building\, Conference room END:VEVENT BEGIN:VEVENT SUMMARY:Colloquium | Antoine Strugarek (CEA Saclay | Paris\, France) DTSTART:20261015T123000Z DTEND:20261015T133000Z DTSTAMP:20260619T183048Z UID:www.aip.de-2353 CATEGORIES:Scientific CATEGORIES:Scientific Talk CATEGORIES:Public CATEGORIES:Colloquium CONTACT:Julián Alvarado-Gómez DESCRIPTION:Speaker: Antoine Strugarek (CEA Saclay | Paris\, France)\nTitl e: TBD\nAbstract: TBD\nNote: Hosts: Ilaria Civale and Katja Poppenhäger\n LOCATION:AIP\; Kirch building\, Conference room END:VEVENT BEGIN:VEVENT SUMMARY:Colloquium | Andrew Pontzen (Durham University) DTSTART:20261112T133000Z DTEND:20261112T143000Z DTSTAMP:20260619T183048Z UID:www.aip.de-2359 CATEGORIES:Scientific CATEGORIES:Scientific Talk CATEGORIES:Public CATEGORIES:Colloquium CONTACT:Ewald Puchwein DESCRIPTION:Speaker: Andrew Pontzen (Durham University)\nTitle: TBD\n LOCATION:AIP\; Kirch building\, Conference room END:VEVENT BEGIN:VEVENT SUMMARY:Colloquium | Boris Gaensicke (University of Warwick | Coventry\, U K) DTSTART:20260924T123000Z DTEND:20260924T133000Z DTSTAMP:20260619T183048Z UID:www.aip.de-2361 CATEGORIES:Scientific CATEGORIES:Scientific Talk CATEGORIES:Public CATEGORIES:Colloquium CONTACT:Julián Alvarado-Gómez DESCRIPTION:Speaker: Boris Gaensicke (University of Warwick | Coventry\, U K)\nTitle: TBD\nAbstract: TBD\nNote: Host: Axel Schwope\n LOCATION:AIP\; Kirch building\, Conference room END:VEVENT BEGIN:VEVENT SUMMARY:Colloquium | Tobias Buck (Heidelberg) DTSTART:20261119T133000Z DTEND:20261119T143000Z DTSTAMP:20260619T183048Z UID:www.aip.de-2365 CATEGORIES:Scientific CATEGORIES:Scientific Talk CATEGORIES:Public CATEGORIES:Colloquium CONTACT:Ewald Puchwein DESCRIPTION:Speaker: Tobias Buck (Heidelberg)\nTitle: TBD\n LOCATION:AIP\; Kirch building\, Conference room END:VEVENT BEGIN:VEVENT SUMMARY:Colloquium | Dominika Wylezalek (University of Heidelberg | German y) DTSTART:20261203T133000Z DTEND:20261203T143000Z DTSTAMP:20260619T183048Z UID:www.aip.de-2366 CATEGORIES:Scientific CATEGORIES:Scientific Talk CATEGORIES:Public CATEGORIES:Colloquium CONTACT:Julián Alvarado-Gómez DESCRIPTION:Speaker: Dominika Wylezalek (University of Heidelberg | German y)\nTitle: TBD\nAbstract: TBD\nNote: Hosts: Tanya Urrutia and Guilherme Co uto\n LOCATION:AIP\; Kirch building\, Conference room END:VEVENT BEGIN:VEVENT SUMMARY:Colloquium | Paul Groot (UCT/SAAO and Radboud University) DTSTART:20260625T123000Z DTEND:20260625T133000Z DTSTAMP:20260619T183048Z UID:www.aip.de-2369 CATEGORIES:Scientific CATEGORIES:Scientific Talk CATEGORIES:Public CATEGORIES:Colloquium CONTACT:Ivan Minchev DESCRIPTION:Speaker: Paul Groot (UCT/SAAO and Radboud University)\nTitle: Ultra-compact binaries and gravitational-wave progenitors\nAbstract: TBD\n Note: Host: Alex Schwope\n LOCATION:AIP\; Kirch building\, Conference room END:VEVENT BEGIN:VEVENT SUMMARY:Colloquium | Eric F. Bell (University of Michigan) DTSTART:20260604T123000Z DTEND:20260604T133000Z DTSTAMP:20260619T183048Z UID:www.aip.de-2370 CATEGORIES:Scientific CATEGORIES:Scientific Talk CATEGORIES:Public CATEGORIES:Colloquium CONTACT:Ivan Minchev DESCRIPTION:Speaker: Eric F. Bell (University of Michigan)\nTitle: TBD\nNo te: Host: Roelof de Jong\n LOCATION:AIP\; Kirch building\, Conference room END:VEVENT BEGIN:VEVENT SUMMARY:Colloquium | Heino Falke (Radboud University Nijmegen | The Nether lands) DTSTART:20261126T133000Z DTEND:20261126T143000Z DTSTAMP:20260619T183048Z UID:www.aip.de-2373 CATEGORIES:Scientific CATEGORIES:Scientific Talk CATEGORIES:Public CATEGORIES:Colloquium CONTACT:Ewald Puchwein DESCRIPTION:Speaker: Heino Falke (Radboud University Nijmegen | The Nether lands)\nTitle: TBD\nAbstract: TBD\nNote: Host: Christoph Pfrommer\n LOCATION:AIP\; Kirch building\, Conference room END:VEVENT BEGIN:VEVENT SUMMARY:Thinkshop focused on the Magellanic Clouds DTSTART;VALUE=DATE:20270906 DTEND;VALUE=DATE:20270911 DTSTAMP:20260619T183048Z UID:www.aip.de-2388 CATEGORIES:Scientific CATEGORIES:Scientific Meeting CATEGORIES:Public DESCRIPTION: END:VEVENT BEGIN:VEVENT SUMMARY:Colloquium | Marta Volonteri (IAP\, Paris) DTSTART:20261105T133000Z DTEND:20261105T143000Z DTSTAMP:20260619T183048Z UID:www.aip.de-2406 CATEGORIES:Scientific CATEGORIES:Scientific Talk CATEGORIES:Public CATEGORIES:Colloquium CONTACT:Ewald Puchwein DESCRIPTION:Speaker: Marta Volonteri (IAP\, Paris)\nTitle: TBD\n LOCATION:AIP\; Kirch building\, Conference room END:VEVENT BEGIN:VEVENT SUMMARY:Jamboree (ISC) DTSTART:20261110T133000Z DTEND:20261110T143000Z DTSTAMP:20260619T183048Z UID:www.aip.de-2414 CATEGORIES:Internal Event CATEGORIES:Institute Event CATEGORIES:Public DESCRIPTION: LOCATION:Maria-Margaretha-Kirch building\, campus Babelsberg END:VEVENT BEGIN:VEVENT SUMMARY:Career Event DTSTART:20261006T123000Z DTEND:20261006T133000Z DTSTAMP:20260619T183048Z UID:www.aip.de-2415 CATEGORIES:Internal Event CATEGORIES:Institute Event CATEGORIES:Public DESCRIPTION: LOCATION:Conference room Maria-Margaretha-Kirch building\, campus Babelsbe rg END:VEVENT BEGIN:VEVENT SUMMARY:SOLER User Workshop DTSTART;VALUE=DATE:20260630 DTEND;VALUE=DATE:20260703 DTSTAMP:20260619T183048Z UID:www.aip.de-2429 CATEGORIES:Scientific CATEGORIES:Scientific Meeting CATEGORIES:Public CONTACT:Alexander Warmuth DESCRIPTION: END:VEVENT BEGIN:VEVENT SUMMARY:Day of Open Doors at Telegrafenberg - Great Refractor and Einstein Tower DTSTART;VALUE=DATE:20260926 DTEND;VALUE=DATE:20260927 DTSTAMP:20260619T183048Z UID:www.aip.de-2430 CATEGORIES:Public Event CATEGORIES:Outreach Event CATEGORIES:Public CONTACT:presse@aip.de DESCRIPTION: LOCATION:Science Park Albert-Einstein\, Telegrafenberg\, Potsdam END:VEVENT BEGIN:VEVENT SUMMARY:AIP Seminar | Junais (AIP) DTSTART:20260609T123000Z DTEND:20260609T133000Z DTSTAMP:20260619T183048Z UID:www.aip.de-2467 CATEGORIES:Scientific CATEGORIES:Scientific Talk CATEGORIES:Public CATEGORIES:AIP Seminar CONTACT:Marcel Pawlowski DESCRIPTION:Speaker: Junais (AIP)\nTitle: Low surface brightness galaxies in the era of deep large-sky surveys and artificial intelligence\nAbstract : Low surface-brightness (LSB) galaxies\, which are typically fainter than the night sky\, contribute to the majority of the total number density of galaxies in the universe. They are a crucial and powerful laboratory for testing our understanding of galaxy formation and evolution. However\, the extremely faint nature of these galaxies has long hindered in-depth studi es of them\, biasing our knowledge of galaxy physics towards only bright\, massive galaxies. With the advent of new\, powerful instruments capable o f carrying out deep\, large sky surveys (e.g.\, Euclid\, LSST)\, combined with the era of modern artificial intelligence (AI) tools\, we are opening a new window into a comprehensive understanding of the LSB galaxies. In t his talk\, I will present our recent and ongoing work on LSB galaxies. Thi s includes the development of novel AI tools for the automatic identificat ion and characterisation of LSB and dwarf galaxies\, investigating the rol e of environment in their evolution\, morphology\, and gas content. Additi onally\, I will also present some follow-up observing campaigns we did on extreme cases like ultra-diffuse and giant LSB galaxies.\n LOCATION:AIP\; Schwarzschildhaus\, Lecture hall END:VEVENT BEGIN:VEVENT SUMMARY:AIP Summer Party (internal) DTSTART:20260701T130000Z DTEND:20260701T160000Z DTSTAMP:20260619T183048Z UID:www.aip.de-2468 CATEGORIES:Internal Event CATEGORIES:Institute Event CATEGORIES:Public DESCRIPTION: END:VEVENT BEGIN:VEVENT SUMMARY:Songs under the Starry Sky DTSTART:20260605T173000Z DTEND:20260605T200000Z DTSTAMP:20260619T183048Z UID:www.aip.de-2472 CATEGORIES:Public Event CATEGORIES:Outreach Event CATEGORIES:Public CONTACT:Axel Schwope DESCRIPTION:Beneficial concert in the Great Refractor on Telegrafenberg wi th Axel Schwope as solist. Adminission only after prior registration.\n LOCATION:Great Refractor\, Telegrafenberg\, 14473 Potsdam END:VEVENT BEGIN:VEVENT SUMMARY:4MOST All Hands Meeting DTSTART;VALUE=DATE:20260601 DTEND;VALUE=DATE:20260606 DTSTAMP:20260619T183048Z UID:www.aip.de-2490 CATEGORIES:Scientific CATEGORIES:Scientific Meeting CATEGORIES:Public DESCRIPTION: END:VEVENT BEGIN:VEVENT SUMMARY:Special Seminar | Nic Scott (Georgia State University (The CHARA A rray)) DTSTART:20260713T090000Z DTEND:20260713T100000Z DTSTAMP:20260619T183048Z UID:www.aip.de-2497 CATEGORIES:Scientific CATEGORIES:Scientific Talk CATEGORIES:Public CATEGORIES:Special Seminar CATEGORIES:other topic CONTACT:Kalaga Madhav DESCRIPTION:Speaker: Nic Scott (Georgia State University (The CHARA Array) )\nTitle: Recent technical and scientific highlights from the CHARA Array\ nAbstract: The Center for High Angular Resolution Astronomy (CHARA) Array is a six-element interferometer at Mount Wilson Observatory with baselines ranging from 34 to 331 m. The Array hosts a number of new or upgraded\, s ix-telescope beam combiners that span the spectrum from the visible R-band to the near-infrared K-band with a range in available spectral resolution . The most recent are the Silmaril beam combiner that is a three-telescope instrument for H- and K-bands that is designed for very high sensitivity on fainter targets and the CHARA Array Integrated Optics Testbed (CHARIOT) that is a platform for characterizing integrated optic combiners. A seven th\, mobile telescope is now on-site for use with fiber optics for H-band beam transport. The mobile telescope will extend the baseline range from 2 0 m to 579 m\, creating new opportunities for measurements of stars with l arge and small angular diameters. Observing time is available to the commu nity through a program funded by NSF. The observing programs are solicited and peer-reviewed by NSF's NOIRLab.\nAbout Dr. Scott:\nNic Scott is the T elescope Systems Scientist at the Georgia State University Center for High Angular Resolution Astronomy (CHARA) Array. Nic directs all aspects of co ntrol and development of the telescopes\, enclosures\, and relay optics of the seven CHARA Array telescopes. Nic received dual PhD degrees from Geor gia State University and the Observatoire de Paris for his work on a novel fiber optics beam combiner at the Array. Prior to his current appointment at CHARA\, Nic was a Lead Research Scientist at the NASA Ames Research Ce nter where he developed speckle interferometry cameras for the WIYN\, Gemi ni-North\, and Gemini-South telescopes. Nic is currently leading the integ ration of the CHARA Array Integrated Optics Testbed (CHARIOT) experiment t o provide a flexible station in the beam combining laboratory to character ize novel integrated optics combiners.\nNote: Let me know if you want to m eet Nic. He will be at AIP until 14.05.\n LOCATION:AIP\; Kirch building\, Conference room END:VEVENT BEGIN:VEVENT SUMMARY:Virtual Babelsberg Starry Night DTSTART:20260521T180000Z DTEND:20260521T190000Z DTSTAMP:20260619T183048Z UID:www.aip.de-2498 CATEGORIES:Public Event CATEGORIES:Generic Event CATEGORIES:Public CONTACT:presse@aip.de DESCRIPTION:Talk (in German): Artemis II - To the Moon and back (Mirko Kru mpe)\n LOCATION:The talk is going to be available via the YouTube channel Urknall \, Weltall und das Leben. END:VEVENT BEGIN:VEVENT SUMMARY:Leibniz Academy Follow-up Workshop 2-10-25 DTSTART;VALUE=DATE:20260930 DTEND;VALUE=DATE:20261002 DTSTAMP:20260619T183048Z UID:www.aip.de-2500 CATEGORIES:Scientific CATEGORIES:Scientific Meeting CATEGORIES:Public CONTACT:Hakan Önel DESCRIPTION: LOCATION:Leibniz Institute for Astrophysics Potsdam (AIP)\, Research campu s Babelsberg\, Maria Margaretha Kirch Building END:VEVENT BEGIN:VEVENT SUMMARY:Virtual Babelsberg Starry Night DTSTART:20260618T180000Z DTEND:20260618T190000Z DTSTAMP:20260619T183048Z UID:www.aip.de-2502 CATEGORIES:Public Event CATEGORIES:Generic Event CATEGORIES:Public CONTACT:presse@aip.de DESCRIPTION:Talk (in German): Licht lesbar machen (Daniel Sablowski)\n LOCATION:The talk is going to be available via the YouTube channel Urknall \, Weltall und das Leben. END:VEVENT BEGIN:VEVENT SUMMARY:AIP Seminar | Kaffeerunde (AIP) DTSTART:20260707T123000Z DTEND:20260707T133000Z DTSTAMP:20260619T183048Z UID:www.aip.de-2503 CATEGORIES:Scientific CATEGORIES:Scientific Talk CATEGORIES:Public CATEGORIES:AIP Seminar CONTACT:Marcel Pawlowski DESCRIPTION:Speaker: Kaffeerunde (AIP)\nTitle: Kaffeerunde\n LOCATION:AIP\; Kirch building\, Conference room END:VEVENT BEGIN:VEVENT SUMMARY:AIP Seminar | Geraint Lewis (University of Sydney) DTSTART:20260616T123000Z DTEND:20260616T133000Z DTSTAMP:20260619T183048Z UID:www.aip.de-2504 CATEGORIES:Scientific CATEGORIES:Scientific Talk CATEGORIES:Public CATEGORIES:AIP Seminar CONTACT:Marcel Pawlowski DESCRIPTION:Speaker: Geraint Lewis (University of Sydney)\nTitle: Confront ing the Cosmological Principle: How secure are the foundations of the cosm os?\nAbstract: For nearly a century\, the cosmological principle has been the bedrock of our understanding of the universe. But what if this foundat ion is starting to crack? In this talk\, I describe how we have used quasa rs and radio galaxies to test the assumption that the cosmos is isotropic and homogeneous. We know that the Cosmic Microwave Background displays a s trong dipole\, attributed to our motion relative to the local Hubble flow\ , and if this motion truly defines our cosmic frame\, its imprint should a ppear elsewhere. Indeed\, we find a dipole in large-scale surveys of cosmo logical sources\, and whilst the direction agrees\, the amplitude does no t\, diverging sharply from expectations based on the CMB. I will explore p ossible explanations for these tensions and ask whether they signal new ph ysics or a fundamental shift in our cosmological worldview.\n LOCATION:AIP\; Kirch building\, Conference room END:VEVENT BEGIN:VEVENT SUMMARY:AIP Seminar | Dr. habil. Anne K. Krüger DTSTART:20260527T123000Z DTEND:20260527T133000Z DTSTAMP:20260619T183048Z UID:www.aip.de-2505 CATEGORIES:Scientific CATEGORIES:Scientific Talk CATEGORIES:Public CATEGORIES:AIP Seminar CONTACT:Meetu Verma DESCRIPTION:Speaker: Dr. habil. Anne K. Krüger (Forschungsgruppenleitung "Reorganisation von Wissenspraktiken"\, Weizenbaum-Institut e.V.)\nTitle: Generative AI in science - How does it change scientific practice?\n LOCATION:AIP\; Kirch building\, Conference room END:VEVENT BEGIN:VEVENT SUMMARY:EPIC Technology Meeting DTSTART;VALUE=DATE:20260608 DTEND;VALUE=DATE:20260610 DTSTAMP:20260619T183048Z UID:www.aip.de-2506 CATEGORIES:Scientific CATEGORIES:Scientific Meeting CATEGORIES:Public DESCRIPTION:EPIC Technology Meeting on Photonics for Space and New Space a t AIP\n LOCATION:Kirch building\, conference room\, AIP campus Babelsberg END:VEVENT BEGIN:VEVENT SUMMARY:AIP Seminar | Oliver Gressel (AIP) DTSTART:20260623T123000Z DTEND:20260623T133000Z DTSTAMP:20260619T183048Z UID:www.aip.de-2518 CATEGORIES:Scientific CATEGORIES:Scientific Talk CATEGORIES:Public CATEGORIES:AIP Seminar CONTACT:Rainer Arlt DESCRIPTION:Speaker: Oliver Gressel (AIP)\nTitle: Magnetic phenomena in pr otoplanetary discs\nAbstract: Advances in global magnetohydrodynamic (MHD) simulations along with radiative-chemical modelling have greatly promoted our understanding of protoplanetary discs. With few exceptions\, magnetic fields are playing a pivotal role. The evolutionary processes are general ly found to depend sensitively on the overall amplitude of the large-scale magnetic flux. This mandates to follow the magnetic flux evolution in tan dem with the non-ideal plasma effects. In the context of planet-formation theories\, our models can serve as the backdrop for population synthesis – governing the growth as well as orbital migration of the evolving plan ets\, and discerning in-situ from ex-situ formation pathways.\n LOCATION:AIP\; Kirch building\, Conference room END:VEVENT BEGIN:VEVENT SUMMARY:AIP Seminar | Jake Mitchell (AIP) DTSTART:20260929T123000Z DTEND:20260929T133000Z DTSTAMP:20260619T183048Z UID:www.aip.de-2519 CATEGORIES:Scientific CATEGORIES:Scientific Talk CATEGORIES:Public CATEGORIES:AIP Seminar CONTACT:Rainer Arlt DESCRIPTION:Speaker: Jake Mitchell (AIP)\nTitle: tba.\n LOCATION:AIP\; Kirch building\, Conference room END:VEVENT BEGIN:VEVENT SUMMARY:AIP Seminar | Kaffeerunde (AIP) DTSTART:20260901T123000Z DTEND:20260901T133000Z DTSTAMP:20260619T183048Z UID:www.aip.de-2520 CATEGORIES:Scientific CATEGORIES:Scientific Talk CATEGORIES:Public CATEGORIES:AIP Seminar CONTACT:Rainer Arlt DESCRIPTION:Speaker: Kaffeerunde (AIP)\nTitle: -\n LOCATION:AIP\; Kirch building\, Conference room END:VEVENT BEGIN:VEVENT SUMMARY:AIP Seminar | Kaffeerunde (AIP) DTSTART:20261103T133000Z DTEND:20261103T143000Z DTSTAMP:20260619T183048Z UID:www.aip.de-2521 CATEGORIES:Scientific CATEGORIES:Scientific Talk CATEGORIES:Public CATEGORIES:AIP Seminar CONTACT:Rainer Arlt DESCRIPTION:Speaker: Kaffeerunde (AIP)\nTitle: -\n LOCATION:AIP\; Kirch building\, Conference room END:VEVENT BEGIN:VEVENT SUMMARY:AIP Seminar | Kaffeerunde (AIP) DTSTART:20261208T133000Z DTEND:20261208T143000Z DTSTAMP:20260619T183048Z UID:www.aip.de-2522 CATEGORIES:Scientific CATEGORIES:Scientific Talk CATEGORIES:Public CATEGORIES:AIP Seminar CONTACT:Rainer Arlt DESCRIPTION:Speaker: Kaffeerunde (AIP)\nTitle: -\n LOCATION:AIP\; Kirch building\, Conference room END:VEVENT END:VCALENDAR