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The Dust Attenuation of Star-forming Galaxies at and Beyond: New Insights from ALMA Observations
Yoshinobu Fudamoto, Pascal A. Oesch, Eva Schinnerer +10
We present results on the dust attenuation of galaxies at redshift by studying the relationship between the UV spectral slope () and the infrared excess (IRX;…
Dust and Gas in Star Forming Galaxies at z~3 - Extending Galaxy Uniformity to 11.5 Billion Years
Georgios E. Magdis, D. Rigopoulou, E. Daddi +10
We present millimetre dust emission measurements of two Lyman Break Galaxies at z~3 and construct for the first time fully sampled infrared spectral energy distributions (SEDs), fr…
ALMA observations of cold molecular gas in AGN hosts at z~1.5 - Evidence of AGN feedback?
D. Kakkad, V. Mainieri, M. Brusa +10
Similarly to the cosmic star formation history, the black hole accretion rate density of the Universe peaked at 1<z<3. This cosmic epoch is hence best suited for investigating the…
"Super-deblended" Dust Emission in Galaxies: I. The GOODS-North Catalog and the Cosmic Star Formation Rate Density out to Redshift 6
Daizhong Liu, Emanuele Daddi, Mark Dickinson +10
We present a new technique to measure multi-wavelength "Super-deblended" photometry from highly confused images, which we apply to Herschel and ground-based far-infrared (FIR) and…
ALMA constraints on star-forming gas in a prototypical z=1.5 clumpy galaxy: the dearth of CO(5-4) emission from UV-bright clumps
A. Cibinel, E. Daddi, F. Bournaud +13
We present deep ALMA CO(5-4) observations of a main sequence, clumpy galaxy at z=1.5 in the HUDF. Thanks to the ~0.5" resolution of the ALMA data, we can link stellar population pr…
The unexpectedly large dust and gas content of quiescent galaxies at z>1.4
R. Gobat, E. Daddi, G. Magdis +13
Early type galaxies (ETG) contain most of the stars present in the local Universe and, above a stellar mass of ~5e10 Msun, vastly outnumber spiral galaxies like the Milky Way. Thes…