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X-WR-CALNAME;VALUE=TEXT:ITC Seminar - Ryan Sanders (UCLA)
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SUMMARY:ITC Seminar - Ryan Sanders (UCLA)
DESCRIPTION:<blockquote type="cite">	"Galaxy metallicity measurements at high redshift: probing galaxy growth over the past 12 billion years"    <br><br><strong>Abstract:</strong>	<p>		The scaling of galaxy gas-phase metallicity with stellar mass and star-formation rate is a sensitive probe of the cycle of baryons and galaxy growth.  Characterizing the redshift evolution of these metallicity scaling relations provides a way to assess whether key processes governing galaxy growth (gas inflows, outflows, and star formation) proceed similarly throughout cosmic history.  Accurately determining metallicity at high redshifts (z&gt;1) is crucial to this approach, but the translation between strong emission-line ratios and metallicity is non-trivial.  I will discuss the issues surrounding metallicity measurements at high redshifts, and detail the progress that has been made in this area using direct-method metallicities based on electron temperature measurements at z~1-3.  I will present the mass-metallicity relation and fundamental metallicity relation (i.e., mass-SFR-metallicity) at z~2-3 based on both direct-method and strong-line ratio metallicities, and discuss the implications for baryon cycling.	</p></blockquote>
LOCATION:Phillips
STATUS:CONFIRMED
DTSTART:20200310T160000Z
DTEND:20200310T170000Z
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