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The Evolution of the Stellar Mass-Chemical Abundance Relation over Seven Billion Years

presentation
posted on 30.04.2020 by Caroline McCormick, Chun Ly
This talk was presented on 2020 April 18 at the 2019-20 NASA Arizona Space Grant Symposium. The event was virtually available via Zoom.

Submitted Abstract:
To understand how galaxies evolve, measurements that characterize the diffuse gas within galaxies are needed. One such measurement is the chemical content produced by stars. It is a fossilized record of cumulative star formation that is impacted by gas inflows and outflows. Driven by these insights, my NASA Space Grant project focused on constructing a stellar mass--chemical abundance relation for high-redshift galaxies. Contrary to previous work, my analyses derive chemical abundances using more robust measurements sensitive to the gas temperature. This makes it one of the first extragalactic studies to do so for the early universe. Specifically, we use the [OIII]4363 emission line and implement a spectral stacking approach to increase the detection signal for this weak emission line. With stacks for different stellar mass bins, our preliminary results illustrate that a correlation exists between stellar mass and chemical abundance for high-redshift galaxies.




For inquiries regarding the contents of this dataset, please contact the Corresponding Author listed in the README.txt file. Administrative inquiries (e.g., removal requests, trouble downloading, etc.) can be directed to data-management@arizona.edu

Funding

THE ARIZONA SPACE GRANT CONSORTIUM (AZSGC), IS A PHASE I NASA SPACE GRANT COLLEGE AND FELLOWSHIP CONSORTIUM WITH THE THREE STATE UNIVERSITIES: THE UNIVERSITY OF ARIZONA (UA), ARIZONA STATE UNIVERSITY (ASU), NORTHERN ARIZONA UNIVERSITY (NAU), AND EMBRY-RID

National Aeronautics and Space Administration

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