I present an overview of the molecular gas observations in high redshift galaxies. This field has seen tremendous progress in the past few years, with an increased number of detections of other molecules than CO. The molecular line observations are done towards different classes of massive starbursts, including submillimeter galaxies, quasars, and massive gas-rich disks. I will highlight results of detections of HCN, HCO+, and other small molecules, as well as the Spitzer detections of PAHs. Additionally, I will discuss about the excitation of CO and other species in the high-z galaxies and put this in the context of new telescopes such as ALMA
The discovery of a population of high-redshift dust-obscured submillimeter galaxies (SMGs) has revol...
12 pages, 2 figures. To appear in Nature, July, 2004Observations of the molecular gas phase in quasa...
We present ALMA CO (2-1) detections in 11 gas-rich cluster galaxies at z ∼ 1.6, constituting the lar...
I present an overview of the molecular gas observations in high redshift galaxies. This field has se...
International audienceI review some recent results about the molecular content of galaxies, obtained...
International audienceI review some recent results about the molecular content of galaxies, obtained...
International audienceI review some recent results about the molecular content of galaxies, obtained...
International audienceI review some recent results about the molecular content of galaxies, obtained...
We study the molecular gas properties of high-z galaxies observed in the ALMA Spectroscopic Survey (...
International audienceWe study the molecular gas properties of high-z galaxies observed in the ALMA ...
International audienceWe study the molecular gas properties of high-z galaxies observed in the ALMA ...
International audienceWe study the molecular gas properties of high-z galaxies observed in the ALMA ...
International audienceThe main achievements, current developments and prospects of molecular studies...
We present the average rest-frame spectrum of high-redshift dusty, star-forming galaxies from 250 to...
. We present results of an extensive search for molecular gas in 14 high redshift (z ? 2) radio gala...
The discovery of a population of high-redshift dust-obscured submillimeter galaxies (SMGs) has revol...
12 pages, 2 figures. To appear in Nature, July, 2004Observations of the molecular gas phase in quasa...
We present ALMA CO (2-1) detections in 11 gas-rich cluster galaxies at z ∼ 1.6, constituting the lar...
I present an overview of the molecular gas observations in high redshift galaxies. This field has se...
International audienceI review some recent results about the molecular content of galaxies, obtained...
International audienceI review some recent results about the molecular content of galaxies, obtained...
International audienceI review some recent results about the molecular content of galaxies, obtained...
International audienceI review some recent results about the molecular content of galaxies, obtained...
We study the molecular gas properties of high-z galaxies observed in the ALMA Spectroscopic Survey (...
International audienceWe study the molecular gas properties of high-z galaxies observed in the ALMA ...
International audienceWe study the molecular gas properties of high-z galaxies observed in the ALMA ...
International audienceWe study the molecular gas properties of high-z galaxies observed in the ALMA ...
International audienceThe main achievements, current developments and prospects of molecular studies...
We present the average rest-frame spectrum of high-redshift dusty, star-forming galaxies from 250 to...
. We present results of an extensive search for molecular gas in 14 high redshift (z ? 2) radio gala...
The discovery of a population of high-redshift dust-obscured submillimeter galaxies (SMGs) has revol...
12 pages, 2 figures. To appear in Nature, July, 2004Observations of the molecular gas phase in quasa...
We present ALMA CO (2-1) detections in 11 gas-rich cluster galaxies at z ∼ 1.6, constituting the lar...