Submm-to-radio observations of molecular and atomic gas in massive high-redshift galaxies
by Jeffrey Wagg
at 1 p.m. on November, 13, 2008
in the IRAM library
The current generation of large single-dish submm/radio-wavelength telescopes and interferometers have opened up the study of gas and dust in galaxies and AGN out to the epoch of reionization at z>6. The IRAM facilities have been at the forefront of this revolution, and I will present our most recent results of an ongoing survey of dust continuum emission and molecular CO line emission in z~6 quasars using the CSO, the IRAM 30m, the PdBI and the GBT. I will also present our first attempts at using observations of redshifted CO line emission as a means of measuring redshifts for dust-obscured submm galaxies. Finally, I will discuss some of the applications of redshifted atomic lines such as neutral and ionized Carbon for studying star-formation in the first galaxies.
A 70m millimetric antenna in Plateau Suffa in Uzbekistan - The Suffa Project
by Dr. Igor Zinchenko, Mr. Vadim Gimmelman and Mr. Yuri Artemenko
at 9:30 a.m. on October, 29th, 2008
in the IRAM library in Granada