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Star formation in the cluster CLG0218.3-0510 at z=1.62 and its large-scale environment: the infrared perspective
Joana S. Santos, Bruno Altieri, Masayuki Tanaka +7
The galaxy cluster CLG0218.3-0510 at z=1.62 is one of the most distant galaxy clusters known, with a rich muti-wavelength data set that confirms a mature galaxy population already…
The evolution of the dust temperatures of galaxies in the SFR plane up to
B. Magnelli, D. Lutz, A. Saintonge +38
[Abridged] We study the evolution of the dust temperatures of galaxies in the SFR-M* plane up to z~2 using observations from the Herschel Space Observatory. Starting from a sample…
Validation of the equilibrium model for galaxy evolution to z~3 through molecular gas and dust observations of lensed star-forming galaxies
Amelie Saintonge, Dieter Lutz, Reinhard Genzel +11
We combine IRAM Plateau de Bure Interferometer and Herschel PACS and SPIRE measurements to study the dust and gas contents of high-redshift star forming galaxies. We present new ob…
PHIBSS: molecular gas, extinction, star formation and kinematics in the z=1.5 star forming galaxy EGS13011166
R. Genzel, L. J. Tacconi, J. Kurk +23
We report matched resolution, imaging spectroscopy of the CO J=3-2 line (with the IRAM Plateau de Bure millimeter interferometer) and of the H-alpha line (with LUCI at the Large Bi…
Molecular gas mass functions of normal star forming galaxies since z~3
S. Berta, D. Lutz, R. Nordon +7
We use deep far-infrared data from the PEP/GOODS-Herschel surveys and rest frame ultraviolet photometry to study the evolution of the molecular gas mass function of normal star for…
Nuclear Activity is more prevalent in Star-Forming Galaxies
D. J. Rosario, P. Santini, D. Lutz +14
We explore the question of whether low and moderate luminosity Active Galactic Nuclei (AGNs) are preferentially found in galaxies that are undergoing a transition from active star…