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DTSTART;VALUE=DATE:20240930
DTEND;VALUE=DATE:20241005
DTSTAMP:20260423T170752
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SUMMARY:ERIS 2024 Tenth European Radio Interferometry School
DESCRIPTION:The tenth edition of the European Radio Interferometry School\, ERIS2024\, will be held in Granada\, Spain\, from Monday September 30th to Friday October 4th\, 2024. ERIS will provide a week of lectures and tutorials on how to achieve scientific results from radio interferometry. The school is co-organised by the Instituto de Astrofísica de Andalucía (IAA-CSIC) and JIVE – Joint Institute for VLBI ERIC. This school is sponsored by the OPTICON-RadioNET Pilot project and the Severo Ochoa training program of the IAA-CSIC. \nThe topics covered by the lectures/tutorials will include: \n\n   Calibration and imaging of continuum\, spectral line and polarization data\n   Low frequency (LOFAR domain)\, cm-wave (e-MERLIN domain)\, decimetre-wave (HI/OH domain)\, high frequency (ALMA/IRAM domain)\, and VLBI interferometry\n   Extracting the information from astronomical data and interpreting the results\n   Choosing the most suitable array and observing plan for your project.
URL:https://www.iaa.csic.es/evento/eris-2024-tenth-european-radio-interferometry-school/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Training
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DTSTART;TZID=Europe/Paris:20241003T123000
DTEND;TZID=Europe/Paris:20241003T133000
DTSTAMP:20260423T170752
CREATED:20240924T090032Z
LAST-MODIFIED:20250912T080235Z
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SUMMARY:SO Colloquium: The next generation of milliarcsecond surveys with SKA-VLBI
DESCRIPTION:Very Long Baseline Interferometry (VLBI)\, using both SKA-Low and SKA-Mid\, is poised to deliver groundbreaking observations with milliarcsecond resolution\, surpassing the capabilities of the standard SKA array. VLBI in conjunction with the SKA holds the promise of unlocking profound insights across various astrophysical topics and science working groups. \nVLBI with the SKA stands to revolutionise our understanding of galaxy evolution and the physics of jet accretion by studying Active Galactic Nuclei (AGN) at low luminosities. Moreover\, it is poised to make significant contributions to cosmology\, through constraining dark energy and dark matter via gravitational lenses and the study of nuclear water masers. The exploration of the stellar lifecycle\, including the temporal evolution of supernova remnants\, plus the rapid follow-up of transients (e.g.\, localising FRBs and tidal disruption events) adds another dimension to the diverse range of science that can be investigated by VLBI with the SKA. \nSKA-VLBI is set to offer unparalleled astrometric observations capable of measuring proper motions and parallaxes of galactic objects. This capability opens the door to mapping the structure of our Galaxy and testing gravity within binary systems. This overview highlights just a subset of the topics that will be addressed in this presentation\, where I will delve into the scientific achievements achievable through VLBI with the SKA and elucidate the operational aspects of SKA-VLBI. \nFecha: 03/10/2024 – 12:30Conferenciante: Dr. Jack RadcliffeFiliación: University of Pretoria\, South Africa
URL:https://www.iaa.csic.es/evento/so-coloquium-the-next-generation-of-milliarcsecond-surveys-with-ska-vlbi/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Colloquium
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