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
Studies of the molecular interstellar medium that fuels star formation and supermassive black hole g...
International audienceWe study the molecular gas properties of high-z galaxies observed in the ALMA ...
Constraints on the molecular gas content of galaxies at high redshift are crucial to further our und...
I present an overview of the molecular gas observations in high redshift galaxies. This field has se...
We present here the sensitive HCN(1-0) observations made with the VLA of two submillimeter galaxies ...
We study the molecular gas properties of high-z galaxies observed in the ALMA Spectroscopic Survey (...
We study the molecular gas properties of high-z galaxies observed in the ALMA Spectroscopic Survey (...
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 audienceWe study the molecular gas properties of high-z galaxies observed in the ALMA ...
In the past decade, molecular gas observations have begun probing the high redshift universe in a sy...
International audienceWe study the molecular gas properties of high-z galaxies observed in the ALMA ...
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...
It becomes possible now to detect cold molecules at high redshift in the millimeter domain. Since th...
Studies of the molecular interstellar medium that fuels star formation and supermassive black hole g...
International audienceWe study the molecular gas properties of high-z galaxies observed in the ALMA ...
Constraints on the molecular gas content of galaxies at high redshift are crucial to further our und...
I present an overview of the molecular gas observations in high redshift galaxies. This field has se...
We present here the sensitive HCN(1-0) observations made with the VLA of two submillimeter galaxies ...
We study the molecular gas properties of high-z galaxies observed in the ALMA Spectroscopic Survey (...
We study the molecular gas properties of high-z galaxies observed in the ALMA Spectroscopic Survey (...
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 audienceWe study the molecular gas properties of high-z galaxies observed in the ALMA ...
In the past decade, molecular gas observations have begun probing the high redshift universe in a sy...
International audienceWe study the molecular gas properties of high-z galaxies observed in the ALMA ...
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...
It becomes possible now to detect cold molecules at high redshift in the millimeter domain. Since th...
Studies of the molecular interstellar medium that fuels star formation and supermassive black hole g...
International audienceWe study the molecular gas properties of high-z galaxies observed in the ALMA ...
Constraints on the molecular gas content of galaxies at high redshift are crucial to further our und...