We present a census of the molecular gas properties of galaxies in the most distant known X-ray cluster, CLJ1001, at z = 2.51, using deep observations of CO(1-0) with the Karl G. Jansky Very Large Array. In total, 14 cluster members with M * > 1010.5 M ☉ are detected, including all of the massive star-forming members within the virial radius, providing the largest galaxy sample in a single cluster at z > 2 with CO(1-0) measurements. We find a large variety in the gas content of these cluster galaxies, which is correlated with their relative positions (or accretion states), with those closer to the cluster core being increasingly gas-poor. Moreover, despite their low gas content, the galaxies in the cluster center exhibit an elevated s...
International audienceWe investigate how the galaxy reservoirs of molecular gas fuelling star format...
We present an extremely deep CO(1-0) observation of a confirmed z = 1.62 galaxy cluster. We detect t...
International audienceWe investigate how the galaxy reservoirs of molecular gas fuelling star format...
We present a census of the molecular gas properties of galaxies in the most distant known X-ray clus...
We present a census of the molecular gas properties of galaxies in the most distant known X-ray clus...
We present a census of the molecular gas properties of galaxies in the most distant known X-ray clus...
We present a census of the molecular gas properties of galaxies in the most distant known X-ray clus...
International audienceContext. Probing both star formation history and evolution of distant cluster ...
International audienceContext. Probing both star formation history and evolution of distant cluster ...
International audienceContext. Probing both star formation history and evolution of distant cluster ...
International audienceContext. Probing both star formation history and evolution of distant cluster ...
This paper is the second of a series that tackles the properties of molecular gas in galaxies residi...
This paper is the second of a series that tackles the properties of molecular gas in galaxies residi...
International audienceWe investigate how the galaxy reservoirs of molecular gas fuelling star format...
International audienceWe investigate how the galaxy reservoirs of molecular gas fuelling star format...
International audienceWe investigate how the galaxy reservoirs of molecular gas fuelling star format...
We present an extremely deep CO(1-0) observation of a confirmed z = 1.62 galaxy cluster. We detect t...
International audienceWe investigate how the galaxy reservoirs of molecular gas fuelling star format...
We present a census of the molecular gas properties of galaxies in the most distant known X-ray clus...
We present a census of the molecular gas properties of galaxies in the most distant known X-ray clus...
We present a census of the molecular gas properties of galaxies in the most distant known X-ray clus...
We present a census of the molecular gas properties of galaxies in the most distant known X-ray clus...
International audienceContext. Probing both star formation history and evolution of distant cluster ...
International audienceContext. Probing both star formation history and evolution of distant cluster ...
International audienceContext. Probing both star formation history and evolution of distant cluster ...
International audienceContext. Probing both star formation history and evolution of distant cluster ...
This paper is the second of a series that tackles the properties of molecular gas in galaxies residi...
This paper is the second of a series that tackles the properties of molecular gas in galaxies residi...
International audienceWe investigate how the galaxy reservoirs of molecular gas fuelling star format...
International audienceWe investigate how the galaxy reservoirs of molecular gas fuelling star format...
International audienceWe investigate how the galaxy reservoirs of molecular gas fuelling star format...
We present an extremely deep CO(1-0) observation of a confirmed z = 1.62 galaxy cluster. We detect t...
International audienceWe investigate how the galaxy reservoirs of molecular gas fuelling star format...