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:Institute of Astronomy Seminars
SUMMARY:The Nature of the Star Forming Main Sequence - Wil
 liam Baker
DTSTART;TZID=Europe/London:20221116T131500
DTEND;TZID=Europe/London:20221116T134000
UID:TALK192872AThttp://talks.cam.ac.uk
URL:http://talks.cam.ac.uk/talk/index/192872
DESCRIPTION:The Star-Forming Main Sequence describes how the s
 tellar mass and star formation rate of galaxies ar
 e observed to positively correlate. It is used fre
 quently for defining different galaxy populations 
 and predicting quantities. But is it a fundamental
  relationship? In this talk I will present results
  investigating the scaling relations that exist be
 tween star formation rate\, stellar mass and molec
 ular gas mass on both local (resolved) scales and 
 global (galaxy wide) scales for galaxies both in t
 he local universe and at high redshift. I use a co
 mbination of partial correlation coefficients and 
 random forest regression to uncover which scaling 
 relations are intrinsic\, and those that are inste
 ad indirect by-products of other more fundamental 
 relationships.
LOCATION:The Hoyle Lecture Theatre + Zoom 
CONTACT:Hannah Uebler
END:VEVENT
END:VCALENDAR