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BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20250131T110000
DTEND;TZID=Europe/Paris:20250131T120000
DTSTAMP:20260510T115108
CREATED:20250124T164739Z
LAST-MODIFIED:20250129T101537Z
UID:7720-1738321200-1738324800@cral.osu-lyon.fr
SUMMARY:CRAL@ENS internal seminar by Armand Leclerc
DESCRIPTION:New tools from wave topology for asteroseismology\nAsteroseismology studies waves in stars and uses them to infer what their internal structure is. Today\, hundreds of stars of every kind show oscillations which allowed us to deduce their mass\, radius\, rotation rate\, width of convective zone\, etc. Wave topology proposes a new light under which to look at the wave equation\, in order to obtain theoretical characterization of large-scale oscillation modes. This framework comes from quantum physics\, and complement the classical theories of stellar oscillations. I will present its concepts\, and show two new results obtained by it : a characterization of the fundamental mode n=0 at long horizontal wavelength\, and a correction term for low n modes at short horizontal wavelength. Both these predictions are confirmed in the case of the Sun\, opening perspectives for analytical low n modes seismology in other stars. \nWhere?\nENS-Monod – Amphi F
URL:https://cral.osu-lyon.fr/event/cralobs-internal-seminar-by-armand-leclerc/
LOCATION:ENS
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END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20250121T110000
DTEND;TZID=Europe/Paris:20250121T110000
DTSTAMP:20260510T115108
CREATED:20241218T110645Z
LAST-MODIFIED:20250113T171322Z
UID:7645-1737457200-1737457200@cral.osu-lyon.fr
SUMMARY:CRAL@Obs seminar by Nicolas Dobigeon (IRIT)
DESCRIPTION:Multiband image fusion under spectrally varying spatial blurs — Application to JWST data \nMultiband image fusion has been extensively studied in the literature of Earth observation. This task aims at recovering a multiband image of high spatial and high spectral resolutions from complementary measurements of lower spatial or spectral resolutions. While several methods developed in this context are able to fuse multiband images efficiently\, they are not suitable to handle astronomical images\, in particular in the context of observations made by the James Webb Space Telescope (JWST). Beyond the high dimensionality of the data\, one major challenge lies in the operators associated with spatial blurs that should be considered as spectrally varying. This crucial issue significantly increases the complexity of the forward models and makes the state-of-the-art fusion methods inoperative. The main contributions reported in this talk tackle both challenges: a new framework is proposed to fuse large-scale astronomical data efficiently while taking into account the specificities of astronomical imaging.
URL:https://cral.osu-lyon.fr/event/cralobs-seminar-by-nicolas-dobigeon-irit/
LOCATION:Observatoire
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END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20250120T140000
DTEND;TZID=Europe/Paris:20250120T170000
DTSTAMP:20260510T115108
CREATED:20250113T174832Z
LAST-MODIFIED:20250113T175025Z
UID:7681-1737381600-1737392400@cral.osu-lyon.fr
SUMMARY:CRAL@Obs PhD Defense by Théo Santos (CRAL\, LGL)
DESCRIPTION:Generative neural networks for parametrization in inverse methods: applications in astrophysics and geophysics \nIn physical science\, it is common to study the characteristics of an object that are not directly available but which certain effects within the physical system are observable. The observations can then be used to deduce the properties of the object of interest: the approach known as “inverse” focuses on such problems. An essential question is the parametrization: how to properly define the parameters that define the object to study? The choice is crucial\, as it determines the formulation of the inverse problem and therefore affects its difficulty to solve. \nIn recent years\, machine learning\, particularly generative neural networks\, has offered a promising opportunity for addressing parametrization. These generative networks can generate\, at will\, objects similar to training objects\, from only a few input parameters. A generative network can thus be trained on a set of possible objects and then used for parametrization. This approach presents several advantages: it is computationally efficient\, it attenuates the irregularities between the parameters defining the object and the observations\, it constrains the problem to a class of models similar to those in the training set\, and it requires few degrees of freedom. \nThis thesis is devoted to the methodological analysis of this parametrization. In particular\, I propose various tools to ensure the optimal training of a generator for this parametrization. I highlight the benefits\, limitations\, and specific considerations of this approach. To illustrate this methodological study\, I rely on a toy problem consisting of recovering a clear image of a ring from a blurred and noisy version. I use it to illustrate the various tools and issues related to parametrization\, which I apply within sampling and optimization inverse methods. Subsequently\, I apply this approach to a geophysical problem and an astrophysical one to demonstrate its relevance in these domains. In geophysics\, I apply this parametrization to a “downscaling” problem: the objective is to use a smooth image of the Earth’s mantle to derive a finer image containing small-scale details. To achieve this\, I train the generative network on models created through geodynamic simulations; the network acts as an approximation of the simulation\, more actionable for inverse problems. This application\, performed on synthetic data\, demonstrates the potential of this parametrization for future applications with real data. In astrophysics\, I apply this approach to the generation of point spread functions (PSF). In astrophysical imaging\, the PSF is an object\, characteristic of the optical system\, that defines how an image is blurred; estimating it accurately allows for efficient deblurring of an image. I thus parameterize the PSFs with a generative network\, making the generator as an useful tool in inverse problems involving the PSF. For this case\, the parametrization is performed on real PSF images\, enabling to explore specific issues related to using real data. \n— \nThe presentation will be done in French.
URL:https://cral.osu-lyon.fr/event/cralobs-phd-defense-by-theo-santos-cral-lgl/
LOCATION:Observatoire
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END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20241220T110000
DTEND;TZID=Europe/Paris:20241220T120000
DTSTAMP:20260510T115108
CREATED:20241119T102559Z
LAST-MODIFIED:20241218T110443Z
UID:7569-1734692400-1734696000@cral.osu-lyon.fr
SUMMARY:CRAL@Obs seminar by Antoine Rocher (EPFL)
DESCRIPTION:Galaxy-halo connection in cosmology with wide spectroscopic surveys —\n \nSince the early 2000s\, wide spectroscopic surveys\, in particular multi-fibre experiments\, have provided significant insights into the three-dimensional distribution of galaxies and quasars in the Universe\, by constraining cosmological parameters through precise measurements of the baryon acoustic oscillation (BAO) scale and the non-linear growth rate of structure from redshift space distortions. Current and upcoming stage IV spectroscopic surveys\, such as the Dark Energy Spectroscopic Instrument (DESI) or the 4-metre Multi-Object Spectrograph Telescope (4MOST) aims to reach sub-percent precision on cosmological parameters over a broad redshift range of 0.1 < z < 3.5.\nIn this talk\, I will give an overview of the DESI survey and its scientific goals. In particular\, I will focus on the galaxy-halo connection\, i.e. how galaxies are connected to the underlying matter field. I will present results obtained using the early data release of DESI to constrain the connection between DESI galaxies (luminous red galaxies (LRGs) and Emission Line Galaxies (ELGs)) using the halo occupation distribution (HOD) framework\, an empirical approach to link galaxies and dark matter halos in N-body simulations.
URL:https://cral.osu-lyon.fr/event/cralobs-seminar-by-antoine-rocher-epfl/
LOCATION:Observatoire
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END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20241213T110000
DTEND;TZID=Europe/Paris:20241213T120000
DTSTAMP:20260510T115108
CREATED:20241127T165830Z
LAST-MODIFIED:20241127T165830Z
UID:7608-1734087600-1734091200@cral.osu-lyon.fr
SUMMARY:CRAL@ENS seminar by Ugo Lebreuilly (CEA Saclay)
DESCRIPTION:TBD
URL:https://cral.osu-lyon.fr/event/cralens-seminar-by-ugo-lebreuilly-cea-saclay/
LOCATION:ENS
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END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20241129T110000
DTEND;TZID=Europe/Paris:20241129T120000
DTSTAMP:20260510T115108
CREATED:20241119T101540Z
LAST-MODIFIED:20241119T131158Z
UID:7563-1732878000-1732881600@cral.osu-lyon.fr
SUMMARY:CRAL@Obs seminar by John Chisholm (UT Austin)
DESCRIPTION:JWST’s GLIMPSE: A view of the faintest galaxies in the first billion years of cosmic time —\n \nFaint high-redshift galaxies in the early universe constrain the properties of dark matter\, the early build-up of stellar mass\, and which sources reionized the early universe. The first two years of JWST observations have revealed a wealth of constraints on modestly bright galaxies in the first billion years of cosmic time\, but the faintest population has remained under-probed. JWST’s Glimpse is a Cycle 2 large program that pairs up to 39 hour integrations with the natural lensing of the massive foreground cluster Abell S1063. These observations probe a new regime of intrinsically faint galaxies (down to MUV of -10 or observed magnitudes of 34) in the early universe. With seven wide and two medium bands\, we find a new class of galaxy candidates within the first 200 Myr of cosmic time that must have formed extremely efficiently. We also constrain the number of very faint galaxies in Cosmic Dawn\, the star formation histories of early galaxies\, and explore how the faintest galaxies contributed to reionization. In this talk I will highlight our preliminary effort to reveal the population of the faintest early galaxies and their impact on the evolution of the universe.
URL:https://cral.osu-lyon.fr/event/cralobs-seminar-by-john-chisholm-ut-austin/
LOCATION:Observatoire
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END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20241109T080000
DTEND;TZID=Europe/Paris:20241111T170000
DTSTAMP:20260510T115108
CREATED:20241007T100815Z
LAST-MODIFIED:20241007T102345Z
UID:6132-1731139200-1731344400@cral.osu-lyon.fr
SUMMARY:Les Conférences\, Association française d'astronomie
DESCRIPTION:Plus de trente conférenciers qui font l’actualité astronomique et spatiale vous convient à un voyage extraordinaire jusqu’aux frontières de la connaissance. Il y est question de cosmologie\, d’espace\, de planétologie\, d’histoire des sciences\, de physique fondamentale\, de biologie… Connus pour leur aisance\, leur propension à nous faire vivre les découvertes\, leur aptitude à expliquer simplement des concepts difficiles… ou tout simplement leur passion\, les orateurs et oratrices des Rencontres sont des scientifiques\, des spécialistes. \n 
URL:https://cral.osu-lyon.fr/event/les-conferences-association-francaise-dastronomie/
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END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20241022T153000
DTEND;TZID=Europe/Paris:20241022T170000
DTSTAMP:20260510T115108
CREATED:20241014T074246Z
LAST-MODIFIED:20241014T074422Z
UID:6347-1729611000-1729616400@cral.osu-lyon.fr
SUMMARY:Séminaire de Laurent Mugnier (ONERA) à l'Observatoire
DESCRIPTION:Focal-plane wavefront sensing and applications : from Earth observation to astronomical imaging\, laser focusing and exoplanet detection
URL:https://cral.osu-lyon.fr/event/22-10-2024-330-pm-observatoire/
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