BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//talks.cam.ac.uk//v3//EN
BEGIN:VTIMEZONE
TZID:Europe/London
BEGIN:DAYLIGHT
TZOFFSETFROM:+0000
TZOFFSETTO:+0100
TZNAME:BST
DTSTART:19700329T010000
RRULE:FREQ=YEARLY;BYMONTH=3;BYDAY=-1SU
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0100
TZOFFSETTO:+0000
TZNAME:GMT
DTSTART:19701025T020000
RRULE:FREQ=YEARLY;BYMONTH=10;BYDAY=-1SU
END:STANDARD
END:VTIMEZONE
BEGIN:VEVENT
CATEGORIES:Galaxies Discussion Group
SUMMARY:The Extremes of Resolved Stellar Spectroscopy - Ev
 an Kirby (Notre Dame)
DTSTART;TZID=Europe/London:20240524T113000
DTEND;TZID=Europe/London:20240524T123000
UID:TALK212719AThttp://talks.cam.ac.uk
URL:http://talks.cam.ac.uk/talk/index/212719
DESCRIPTION:The study of local star clusters and galaxies with
  existing spectroscopic instruments and techniques
  has reached the point of diminishing returns.  Br
 eakthroughs require new instruments or innovation 
 in spectral analysis.  I will describe the measure
 ment of radial velocities and abundances of indivi
 dual stars at the threshold of spectral resolution
  and signal-to-noise ratio.  First\, I will addres
 s measurements from Keck/DEIMOS and KCWI.  I will 
 discuss the "backsplash" galaxy Andromeda XVIII (a
 t 1.33 Mpc!)\, neutron-capture abundances in Milky
  Way satellites\, and the "fundamental" stellar ma
 ss-stellar metallicity relation of low-mass field 
 galaxies.  New spectrograph innovations\, like the
  upgrade to DEIMOS and the Subaru Prime Focus Spec
 trograph\, will lead stellar spectroscopy into the
  future.\n
LOCATION:Ryle seminar room + online
CONTACT:Sandro Tacchella
END:VEVENT
END:VCALENDAR