activity
20042009
most citedVigorous star formation with low efficiency in massive disk galaxies at z=1.5

216 citations · 505 across the 4 of their papers we have counts for

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6 papers · 1 filter

astro-ph200826 cited

Obscured and powerful AGN and starburst activities at z~3.5

M. Polletta, A. Omont, S. Berta +9

We report the discovery of two sources at z=3.867 and z=3.427 that exhibit powerful starburst and AGN activities. They benefit from data from radio to X rays from the CFHTLS-D1/SWI…

astro-ph2008139 cited

IMAGES-III: The evolution of the Near-Infrared Tully-Fisher relation over the last 6 Gyr

M. Puech, H. Flores, F. Hammer +22

Using the multi-integral field spectrograph GIRAFFE at VLT, we have derived the K-band Tully-Fisher relation (TFR) at z~0.6 for a representative sample of 65 galaxies with emission…

astro-ph2007216 cited

Vigorous star formation with low efficiency in massive disk galaxies at z=1.5

E. Daddi, H. Dannerbauer, D. Elbaz +4

We present the first detection of molecular gas cooling CO emission lines from ordinary massive galaxies at z=1.5. Two sources were observed with the IRAM Plateau de Bure Interfero…

astro-ph2005

MAMBO 1.2 Millimeter observations of BzK-selected star-forming Galaxies at z~2

H. Dannerbauer, E. Daddi, M. Onodera +9

We present MAMBO 1.2 mm observations of five BzK-pre-selected vigorous starburst galaxies at z~2. Two of these were detected at more than 99.5% confidence levels, with 1.2 mm fluxe…

astro-ph2005

Follow-Up Near-infrared Spectroscopy of Ultraluminous Infrared Galaxies observed by ISO

H. Dannerbauer, D. Rigopoulou, D. Lutz +3

We present low resolution near-infrared spectroscopy of an unbiased sample of 24 ultraluminous infrared galaxies (ULIRGs), selected from samples previously observed spectroscopical…

astro-ph2004

The faint counterparts of MAMBO mm sources near the NTT Deep Field

H. Dannerbauer, M. D. Lehnert, D. Lutz +5

We discuss identifications for 18 sources from our MAMBO 1.2mm survey of the region surrounding the NTT Deep Field. We have obtained accurate positions from Very Large Array 1.4GHz…