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X-WR-CALNAME:Erlangen Centre for Astroparticle Physics
X-ORIGINAL-URL:https://ecap.nat.fau.de
X-WR-CALDESC:Events for Erlangen Centre for Astroparticle Physics
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DTSTART:20230326T010000
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DTSTART;TZID=Europe/Berlin:20230112T130000
DTEND;TZID=Europe/Berlin:20230112T140000
DTSTAMP:20260417T080349
CREATED:20230105T153326Z
LAST-MODIFIED:20230105T153326Z
UID:4106-1673528400-1673532000@ecap.nat.fau.de
SUMMARY:ECAP Seminar: Norbert Werner
DESCRIPTION:Monitoring the High-Energy Sky with Small Satellites\nThanks to the recent remarkable progress in the development of nano/micro/small-satellites and new launchers on the market\, space is becoming increasingly more accessible. This provides new opportunities to diversify space astronomy which was hitherto dominated by relatively few large projects. I will describe the current plans for small missions\, including nano-satellite constellations\, to monitor the transient high-energy sky and thus also aid multi-messenger astronomy. I will summarise the results of the precursor missions GRBAlpha and VZLUSAT-2\, which are operating in orbit and detecting transients routinely as well as the development of a UV space telescope on a small-sat dedicated to follow-up observations of kilonovae.
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-2023-01-12-norbert-werner/
LOCATION:ECAP Laboratory\, 00.061\, Nikolaus-Fiebiger-Str. 2\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
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BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20230119T130000
DTEND;TZID=Europe/Berlin:20230119T140000
DTSTAMP:20260417T080349
CREATED:20230110T125510Z
LAST-MODIFIED:20230110T125510Z
UID:4110-1674133200-1674136800@ecap.nat.fau.de
SUMMARY:ECAP Seminar: Georg Hager\, Johannes Veh
DESCRIPTION:News from NHR@FAU – Fritz\, Alex and Woody\nThe last year has seen quite a few changes in systems and setups at NHR@FAU. Georg Hager\, Head of Training & Support\, will present details about the flagship systems “Fritz” (Top500 rank 151) and “Alex” (Top500 rank 174) and how to get access to them.\nJohannes Veh from the NHR@FAU Systems & Services division will get you up to speed on all these topics regarding Tier3 use of “Woody” so you can make the most out of the hardware.
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-2023-01-19-georg-hager-johannes-veh/
LOCATION:ECAP Laboratory\, 00.061\, Nikolaus-Fiebiger-Str. 2\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
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BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20230126T130000
DTEND;TZID=Europe/Berlin:20230126T140000
DTSTAMP:20260417T080349
CREATED:20230110T155940Z
LAST-MODIFIED:20230110T155940Z
UID:4113-1674738000-1674741600@ecap.nat.fau.de
SUMMARY:ECAP Seminar: Kathryn Kreckel
DESCRIPTION:Resolving the Baryon Cycle within Nearby Galaxies\nThe buildup of stellar mass through star formation is driven on small (<100pc) scales by physical processes and local conditions\, but regulated across larger (kpc) scales through the baryon cycle. This entails the transformation of gas into stars\, and eventual ejection and recycling of material to form the next generation of stars. The interstellar medium (ISM) provides crucial insights into these processes\, particularly our understanding of radiative and mechanical feedback from young massive stars. The PHANGS (Physics at High Angular resolution in Nearby GalaxieS) collaboration is building a library of uniform\, high-quality\, high-resolution observations of nearby galaxies at the critical “cloud scale” across star-forming galaxy disks by using observations from Hubble\, MUSE/VLT\, JWST\, and ALMA. This provides a characterization of the young star clusters\, the ionized HII regions\, the supernova remnants and the giant molecular clouds\, with which we can explore a comprehensive view of the star-formation process.\nI will present new results from my group\, which has focused on quantifying the impact of these stellar feedback processes on the ISM. I will show how we are leveraging our large statistical samples to establish an evolutionary sequence for HII regions\, linking ionized nebulae with their powering stellar sources. In charting the late-time and large-scale feedback\, I will show how morphological identification of bubbles in molecular and ionized gas\, and now with JWST in the dust\, provides quantitative constraints on different feedback mechanisms. Finally\, I will show how the Local Volume Mapper (LVM) project within SDSS-V will push us towards a 1-10pc view of these physical processes within our own Milky Way and Local Group (LMC/SMC) galaxies.
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-2023-01-26-kathryn-kreckel/
LOCATION:ECAP Laboratory\, 00.061\, Nikolaus-Fiebiger-Str. 2\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
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