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Non-linearity and environmental dependence of the star forming galaxies Main Sequence
G. Erfanianfar, P. Popesso, A. Finoguenov +30
Using data from four deep fields (COSMOS, AEGIS, ECDFS, and CDFN), we study the correlation between the position of galaxies in the star formation rate (SFR) versus stellar mass pl…
The composite nature of Dust-Obscured Galaxies (DOGs) at z~2-3 in the COSMOS field: I. A Far-Infrared View
L. Riguccini, E. Le Floc'h, J. R. Mullaney +19
Dust-Obscured galaxies (DOGs) are bright 24 um-selected sources with extreme obscuration at optical wavelengths. They are typically characterized by a rising power-law continuum of…
GOODS-: identification of the individual galaxies responsible for the 80-290m cosmic infrared background
R. Leiton, D. Elbaz, K. Okumura +14
We propose a new method of pushing to its faintest detection limits using universal trends in the redshift evolution of the far infrared over 24m colours in the well-…
Physical properties of z>4 submillimeter galaxies in the COSMOS field
V. Smolcic, A. Karim, O. Miettinen +30
We study the physical properties of a sample of 6 SMGs in the COSMOS field, spectroscopically confirmed to lie at z>4. We use new GMRT 325 MHz and 3 GHz JVLA data to probe the rest…