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University of Cambridge > Talks.cam > Institute of Astronomy Colloquia > Bridging Galaxy Evolution Across Cosmic Time With the CLASSY Survey
Bridging Galaxy Evolution Across Cosmic Time With the CLASSY SurveyAdd to your list(s) Download to your calendar using vCal
If you have a question about this talk, please contact Dominic Walton. Rest-frame far-ultraviolet (FUV) spectra are fundamental to our understanding of star-forming galaxies, providing a unique window on massive stellar populations, chemical evolution, feedback processes, and reionization. The launch of JWST and construction of the ELTs will soon usher in a new era, pushing the FUV spectroscopic frontier to z=15-20. The success of these future endeavors hinges on a comprehensive understanding of the massive star populations and interstellar medium (ISM) gas conditions that power the observed FUV spectral features. I will present the COS Legacy Archive Spectroscopic SurveY (CLASSY) Treasury as a powerful and promising solution. CLASSY is a large HST program creating the first high-quality, high-resolution FUV spectral catalog of star-forming galaxies at z=0, but which span similar properties as seen at high-z. The spectra contain a suite of emission and absorption lines that characterize the massive stellar populations that populate metal poor galaxies, the physical properties of large-scale outflows that regulate star formation, and the chemical abundance patterns of the gas and stars. CLASSY will improve the diagnostic power of the FUV lines for future JWST /ELT surveys, providing a long-lasting legacy to the astronomical community for decades to come. This talk is part of the Institute of Astronomy Colloquia series. This talk is included in these lists:
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