Alexander, D. M., Swinbank, A. M., Smail, I., McDermid, R., Nesvadba, N.
Leading models of galaxy formation require large-scale energetic outflows to regulate the growth of distant galaxies and their central black holes. However, current observational support for this...
Rodrigues, M., Hammer, F., Flores, H., Puech, M., Liang, Y. C., Fuentes-Carrera, I., ...
Intermediate mass galaxies (logM(Msun)>10) at z~0.6 are the likeliest progenitors of the present-day numerous population of spirals. There is growing evidence that they have evolved rapidly since the...
Bournaud, F., Daddi, E., Elmegreen, B. G., Elmegreen, D. M., Nesvadba, N., Vanzella, E., ...
We investigate the properties of a clump-cluster galaxy at redshift 1.57. The morphology of this galaxy is dominated by eight star-forming clumps in optical observations, and has photometric...
IMAGES-III: The evolution of the Near-Infrared Tully-Fisher relation over the last 6 Gyr (2008)
Puech, M., Flores, H., Hammer, F., Yang, Y., Neichel, B., Lehnert, M., ...
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 lines. We confirm...
Neichel, B., Hammer, F., Puech, M., Flores, H., Lehnert, M., Rawat, A., ...
We present a first combined analysis of the morphological and dynamical properties for the Intermediate MAss Galaxy Evolution Sequence (IMAGES) sample. It is a representative sample of 52 z~0.6...
Images I. Strong evolution of galaxy kinematics since z=1 (2008)
Yang, Y., Flores, H., Hammer, F., Neichel, B., Puech, M., Nesvadba, N., ...
IMAGES. I. Strong evolution of galaxy kinematics since z = 1 (2008)
Yang, Y., Flores, H., Hammer, F., Neichel, B., Puech, M., Nesvadba, N., ...
Nearly half the stellar mass of present-day spiral galaxies has formed since z = 1, and galaxy kinematics is an ideal tool to identify the underlying mechanisms responsible for the galaxy mass...
Rodrigues, M., Hammer, F., Flores, H., Puech, M., Liang, Y. C., Fuentes-Carrera, I., ...
Context: Intermediate mass galaxies (> 1010 M_o) at z ~ 0.6 are the likeliest progenitors of the present-day, numerous population of spirals. There is growing evidence that they have evolved rapidly...
IMAGES. III. The evolution of the near-infrared Tully-Fisher relation over the last 6 Gyr (2008)
Puech, M., Flores, H., Hammer, F., Yang, Y., Neichel, B., Lehnert, M., ...
Using the multi-integral field spectrograph GIRAFFE at VLT, we have derived the K-band Tully-Fisher relation (TFR) at z ÃÅ 0.6 for a representative sample of 65 galaxies with emission lines...
Neichel, B., Hammer, F., Puech, M., Flores, H., Lehnert, M., Rawat, A., ...
We present a first combined analysis of the morphological and dynamical properties for the intermediate-mass Galaxy Evolution Sequence (IMAGES) sample. It is a representative sample of 52...
Dynamical Properties of z ~ 2 Star-forming Galaxies and a Universal Star Formation Relation (2007)
Bouché, N., Cresci, G., Davies, R., Eisenhauer, F., Förster Schreiber, N. M., Genzel, R., ...
We present the first comparison of the dynamical properties of different samples of z ~ 1.4-3.4 star-forming galaxies from spatially resolved imaging spectroscopy from SINFONI/VLT integral field...
IMAGES I. Strong evolution of galaxy kinematics since z=1 (2007)
Yang, Y., Flores, H., Hammer, F., Neichel, B., Puech, M., Nesvadba, N., ...
(abbreviated) We present the first results of the ESO large program, ``IMAGES'' which aims at obtaining robust measurements of the kinematics of distant galaxies using the multi-IFU mode of GIRAFFE...
Dynamical Properties of z~2 Star Forming Galaxies and a Universal Star Formation Relation (2007)
Bouche, N., Cresci, G., Davies, R., Eisenhauer, F., Schreiber, N. M. Forster, Genzel, R., ...
We present the first comparison of the dynamical properties of different samples of z~1.4-3.4 star forming galaxies from spatially resolved imaging spectroscopy from SINFONI/VLT integral field...
Dynamical properties of z 2 star-forming galaxies and a universal star formation relation (2007)
Bouché, N., Cresci, G., Davies, R., Eisenhauer, F., Förster Schreiber, N. M., Genzel, R., ...
The rapid formation a large rotating disk galaxy three billion years after the Big Bang (2006)
Genzel, R., Tacconi, L., Eisenhauer, F., Schreiber, N. M. Forster, Cimatti, A., Daddi, E., ...
[Abridged] Over the past two decades observations and theoretical simulations have established a global frame-work of galaxy formation and evolution in the young Universe. Galaxies formed as baryonic...
Schreiber, N. M. Forster, Genzel, R., Lehnert, M. D., Bouche, N., Verma, A., Erb, D. K., ...
We present 0.5" resolution near-IR integral field spectroscopy of the Ha line emission of 14 z~2 UV-selected BM/BX galaxies obtained with SINFONI at ESO/VLT. The mean Ha half-light radius r_1/2 is...
The rapid formation of a large rotating disk galaxy three billion years after the Big Bang (2006)
Genzel, R., Tacconi, L. J., Eisenhauer, F., Förster Schreiber, N., Cimatti, A., Daddi, E., ...
Submillimeter galaxies as tracers of mass assembly at large M (2005)
Genzel, R., Baker, A. J., Ivison, R. J., Bertoldi, F., Blain, A. W., Chapman, S. C., ...
Submillimeter galaxies as tracers of mass assembly at large M (2005)
Genzel, R., Baker, A. J., Ivison, R. J., Bertoldi, F., Blain, A. W., Chapman, S. C., ...
A Step Towards A Computing Grid For The LHC Experiments: ATLAS Data Challenge 1 (2004)
Sturrock, R, Bischof, R, Epp, B, Ghete, V M, Kuhn, D, Mello, A G, ...
The ATLAS Collaboration at CERN is preparing for the data taking and analysis at the LHC that will start in 2007. Therefore, a series of Data Challenges was started in 2002 whose goals are the...
A step towards a computing grid for the LHC experiments: ATLAS Data Challenge 1 (2004)
Sturrock, R., Bischof, R., Epp, B., Ghete, V.M., Kuhn, D., Mello, A.G., ...
SPIFFI observations of the starburst SMMJ14011+0252: Already old, fat, and rich by z = 2.565 (2004)
Tecza, M., Baker, A. J., Davies, R. I., Genzel, R., Lehnert, M. D., Eisenhauer, F., ...
Using the SPectrometer for Infrared Faint Field Imaging (SPIFFI) on the ESO VLT, we have obtained J, H, and K band integral field spectroscopy of the z = 2.565 luminous submillimeter galaxy...
Submillimeter Galaxies as Tracers of Mass Assembly at Large M (2004)
Genzel, R., Baker, A. J., Ivison, R. J., Bertoldi, F., Blain, A. W., Chapman, S. C., ...
Luminous submillimeter galaxies (SMGs) have been known for some time to produce a substantial fraction of the far-IR/submillimeter background. New observations show that these systems are not only...
SPIFFI observations of the starburst SMM J14011+0252: already old, fat, and rich by z = 2.565 (2004)
Tecza, M., Baker, A. J., Davies, R. I., Genzel, R., Lehnert, M. D., Eisenhauer, F., ...
A Step Towards A Computing Grid For The LHC Experiments: ATLAS Data Challenge 1
Sturrock,R., Bischof,R., Epp,B., Ghete,V. M., Kuhn,D., Mello,A. G., ...
The ATLAS Collaboration at CERN is preparing for the data taking and analysis at the LHC that will start in 2007. Therefore, a series of Data Challenges was started in 2002 whose goals are the...
A Step Towards A Computing Grid For The LHC Experiments: ATLAS Data Challenge 1
Sturrock, R., Bischof, R., Epp, B., Ghete, V. M., Kuhn, D., Mello, A. G., ...
The ATLAS Collaboration at CERN is preparing for the data taking and analysis at the LHC that will start in 2007. Therefore, a series of Data Challenges was started in 2002 whose goals are the...