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current and future ground- and space-based telescopes at radio through ultraviolet wavelengths, including major facilities such as the Square Kilometre Array (SKA), the Atacama Large Millimeter
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cryogenic germanium and silicon detectors equipped with sensors for the thermal energy of particle interaction. The next generation of the experiment, featuring upgraded detector technology, is currently
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Research (PCIGR ) in 2027. It is equipped with a mass filter, collision-reaction-cell, an extended collector array of 28 Faraday channels and increased mass dispersion. The day-to-day operations and
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facilitated by eminent experts across diverse fields. These workshops will encompass a wide array of topics, including research methodology, academic writing, and interdisciplinary collaboration. Through