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SUMMARY:Submm and cm-Wavelength Emission Lines as Probes of Massive Galaxy
 \nFormation at High-Redshift - Jeff Wagg (ESO Chile)
DTSTART:20121113T163000Z
DTEND:20121113T173000Z
UID:TALK40730@talks.cam.ac.uk
CONTACT:David Titterington
DESCRIPTION:The past two decades have seen an enormous increase in the wea
 lth of observational data that reveal the nature of star-forming gas in th
 e interstellar medium of high-redshift galaxies.  New facilities operating
  in the submm through cm-wavelength regime have allowed us to study the mo
 lecular gas content of galaxies as far back as the first billion years aft
 er the big bang\, while ionised atomic gas emitting at mm-wavelengths has 
 been detected at even earlier cosmic times.  These observations provide im
 portant insight into galaxy formation processes and will ultimately help u
 s to understand how galaxies get their gas.  In this seminar\, I will pres
 ent some recent PdBI\, JVLA and ALMA observations of massive galaxies that
  existed during the first six billion years of the universe.\n
LOCATION:Martin Ryle Seminar Room\, Kavli Institute
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