Burgarella, Denis, Buat, Veronique, Takeuchi, Tsutomu T., Wada, Takehiko, Pearson, Chris
Deep observations of the CDFS have been secured at 15um with AKARI/IRC infrared space telescope (ESA open time). From these observations, we define a sample of MIR-selected galaxies at 15um and we...
Ultraviolet and Infrared Diagnostics of Star Formation and Dust in NGC 7331 (2007)
Thilker, David A., Boissier, Samuel, Bianchi, Luciana, Calzetti, Daniela, Boselli, Alessandro, Dale, Daniel A., ...
We present images of NGC 7331 obtained with GALEX and Spitzer, tracing UV and IR signatures of star formation. NGC 7331's morphology at 8-850 μm is dominated by a central dust ring. This structure...
Rosa-Gonzalez, Daniel, Burgarella, Denis, Nandra, Kirpal, Kunth, Daniel, Terlevich, Elena, Terlevich, Roberto
We have combined multi-wavelength observations of a selected sample of starforming galaxies with galaxy evolution models in order to compare the results obtained for different SFR tracers and to...
Takeuchi, Tsutomu T., Buat, Veronique, Burgarella, Denis
Based on GALEX and IRAS/Spitzer datasets, we have found that both FUV and FIR luminosity functions (LFs) show a strong evolution from z=0 to z=1, but the FIR LF evolves much stronger than the FUV...
Ultraviolet and infrared diagnostics of star formation and dust in NGC 7331 (2007)
Thilker, David A., Boissier, Samuel, Bianchi, Luciana, Calzetti, Daniela, Boselli, Alessandro, Dale, Daniel A., ...
We present images of NGC 7331 obtained with GALEX and Spitzer, tracing
Takeuchi, Tsutomu T., Buat, Veronique, Burgarella, Denis
Based on GALEX and IRAS/Spitzer datasets, we have found that both FUV and FIR luminosity functions (LFs) show a strong evolution from z=0 to z=1, but the FIR LF evolves much stronger than the FUV...
Boissier, Samuel, De Paz, Armando Gil, Boselli, Alessandro, Madore, Barry F., Buat, Veronique, Cortese, Luca, ...
For a sample of 43 nearby, late-type galaxies, we have investigated the radial variation of both the current star formation rate and the dust-induced UV light attenuation. To do this we have...
Boissier, Samuel, De Paz, Armando Gil, Boselli, Alessandro, Madore, Barry F., Buat, Veronique, Cortese, Luca, ...
For a sample of 43 nearby, late-type galaxies, we have investigated the radial variation of both the current star formation rate and the dust-induced UV light attenuation. To do this we have...
Inoue, Akio K., Buat, Veronique, Burgarella, Denis, Panuzzo, Pasquale, Takeuchi, Tsutomu T., Iglesias-Paramo, Jorge
We discuss dust properties in the interstellar medium (ISM) of nearby normal galaxies, by comparing observations in the ultraviolet (UV) with simulations by a radiative transfer model. The observed...
Inoue, Akio K., Buat, Veronique, Burgarella, Denis, Panuzzo, Pasquale, Takeuchi, Tsutomu T., Iglesias-Paramo, Jorge
We discuss dust properties in the interstellar medium (ISM) of nearby normal galaxies, by comparing observations in the ultraviolet (UV) with simulations by a radiative transfer model. The observed...
Inoue, Akio K., Buat, Veronique, Burgarella, Denis, Panuzzo, Pasquale, Takeuchi, Tsutomu T., Iglesias-Paramo, Jorge
We discuss dust properties in the interstellar medium (ISM) of nearby normal galaxies, by comparing observations in the ultraviolet (UV) with simulations by a radiative transfer model. The observed...
Boissier, Samuel, De Paz, Armando Gil, Boselli, Alessandro, Madore, Barry F., Buat, Veronique, Cortese, Luca, ...
For a sample of 43 nearby, late-type galaxies, we have investigated the radial variation of both the current star formation rate and the dust-induced UV light attenuation. To do this we have...
Boissier, Samuel, De Paz, Armando Gil, Boselli, Alessandro, Madore, Barry F., Buat, Veronique, Cortese, Luca, ...
For a sample of 43 nearby, late-type galaxies, we have investigated the radial variation of both the current star formation rate and the dust-induced UV light attenuation. To do this we have...
Inoue, Akio K., Buat, Veronique, Burgarella, Denis, Panuzzo, Pasquale, Takeuchi, Tsutomu T., Iglesias-Paramo, Jorge
We discuss dust properties in the interstellar medium (ISM) of nearby normal galaxies, by comparing observations in the ultraviolet (UV) with simulations by a radiative transfer model. The observed...
Evolution of morphology in the Chandra Deep Field South (2005)
Lauger, Sébastien, Ilbert, Olivier, Buat, Véronique, Tresse, Laurence, Burgarella, Denis, Arnouts, Stéphane, ...
We studied the morphology of galaxies in the Chandra Deep Field South using ACS multi-wavelength data from the Great Observatories Origin Deep Survey and 524 spectroscopic redshifts from the VIMOS...
Burgarella, Denis, Buat, Veronique, Iglesias-Paramo, Jorge
We study two galaxy samples selected in ultraviolet (UV) and in far-infrared (FIR) for which the spectral energy distributions (SEDs) from the far UV (FUV) to the FIR are available. We compare the...
The evolution of the ultraviolet and infrared luminosity densities in the universe at 0 (2005)
Takeuchi, Tsutomu T., Buat, Veronique, Burgarella, Denis
The ratio between far-ultraviolet (FUV) and infrared (IR) luminosity densities from z=0 to z=1 is discussed by using the luminosity functions (LFs) of both wavelengths. The FUV LF (z=0-1) based on...
Burgarella, Denis, Kissler-Patig, Markus, Buat, Veronique
We studied the metal-poor globular cluster (GC) populations of a large variety of galaxies (47 galaxies spanning about 10mag in absolute brightness) and compared their mean [Fe/H] with the properties...
Burgarella, Denis, Buat, Veronique, Donas, Jose, Milliard, Bruno, Chapelon, Sandra
We used ultraviolet (200 nm) images of the local spiral galaxies M33, M51, M81, M100, M101 to compute morphological parameters of galactic disks at this wavelength : half-light radius $r_{hl}$,...
Burgarella, Denis, Kissler-Patig, Markus, Buat, Veronique
In this paper, we are exploring the properties of old, metal-poor globular clusters in galaxies. We investigate whether their properties are related to the properties of their host galaxies, and...
Evolution of morphology in the Chandra Deep Field South (2005)
Lauger, Sébastien, Ilbert, Olivier, Buat, Véronique, Tresse, Laurence, Burgarella, Denis, Arnouts, Stéphane, ...
We studied the morphology of galaxies in the Chandra Deep Field South using ACS multi-wavelength data from the Great Observatories Origin Deep Survey and 524 spectroscopic redshifts from the VIMOS...
Evolution of morphology in the Chandra Deep Field South (2005)
Lauger, Sébastien, Ilbert, Olivier, Buat, Véronique, Tresse, Laurence, Burgarella, Denis, Arnouts, Stéphane, ...
We studied the morphology of galaxies in the Chandra Deep Field South using ACS multi-wavelength data from the Great Observatories Origin Deep Survey and 524 spectroscopic redshifts from the VIMOS...
Evolution of morphology in the Chandra Deep Field South (2005)
Lauger, Sébastien, Ilbert, Olivier, Buat, Véronique, Tresse, Laurence, Burgarella, Denis, Arnouts, Stéphane, ...
We studied the morphology of galaxies in the Chandra Deep Field South using ACS multi-wavelength data from the Great Observatories Origin Deep Survey and 524 spectroscopic redshifts from the VIMOS...
The evolution of the ultraviolet and infrared luminosity densities in the universe at 0 (2005)
Takeuchi, Tsutomu T., Buat, Veronique, Burgarella, Denis
The ratio between far-ultraviolet (FUV) and infrared (IR) luminosity densities from z=0 to z=1 is discussed by using the luminosity functions (LFs) of both wavelengths. The FUV LF (z=0-1) based on...
Burgarella, Denis, Buat, Veronique, Iglesias-Paramo, Jorge
We study two galaxy samples selected in ultraviolet (UV) and in far-infrared (FIR) for which the spectral energy distributions (SEDs) from the far UV (FUV) to the FIR are available. We compare the...
Spectro-morphology of galaxies: A multi-wavelength (UV-R) classification method (2005)
Buat, Veronique, Burgarella, Denis, Lauger, Sébastien
We present a quantitative method to classify galaxies, based on multi-wavelength data and constructed from the properties of nearby galaxies. Our objective is to define an classification method that...
Evolution of morphology in the Chandra Deep Field South (2005)
Lauger, Sébastien, Ilbert, Olivier, Buat, Véronique, Tresse, Laurence, Burgarella, Denis, Arnouts, Stéphane, ...
We studied the morphology of galaxies in the Chandra Deep Field South using ACS multi-wavelength data from the Great Observatories Origin Deep Survey and 524 spectroscopic redshifts from the VIMOS...
Burgarella, Denis, Buat, Veronique, Iglesias-Paramo, Jorge
We study two galaxy samples selected in ultraviolet (UV) and in far-infrared (FIR) for which the spectral energy distributions (SEDs) from the far UV (FUV) to the FIR are available. We compare the...
The evolution of the ultraviolet and infrared luminosity densities in the universe at 0 (2005)
Takeuchi, Tsutomu T., Buat, Veronique, Burgarella, Denis
The ratio between far-ultraviolet (FUV) and infrared (IR) luminosity densities from z=0 to z=1 is discussed by using the luminosity functions (LFs) of both wavelengths. The FUV LF (z=0-1) based on...
Evolution of morphology in the Chandra Deep Field South (2005)
Lauger, Sébastien, Ilbert, Olivier, Buat, Véronique, Tresse, Laurence, Burgarella, Denis, Arnouts, Stéphane, ...
We studied the morphology of galaxies in the Chandra Deep Field South using ACS multi-wavelength data from the Great Observatories Origin Deep Survey and 524 spectroscopic redshifts from the VIMOS...
Burgarella, Denis, Buat, Veronique, Iglesias-Paramo, Jorge
We study two galaxy samples selected in ultraviolet (UV) and in far-infrared (FIR) for which the spectral energy distributions (SEDs) from the far UV (FUV) to the FIR are available. We compare the...
The evolution of the ultraviolet and infrared luminosity densities in the universe at 0 (2005)
Takeuchi, Tsutomu T., Buat, Veronique, Burgarella, Denis
The ratio between far-ultraviolet (FUV) and infrared (IR) luminosity densities from z=0 to z=1 is discussed by using the luminosity functions (LFs) of both wavelengths. The FUV LF (z=0-1) based on...
Evolution of morphology in the Chandra Deep Field South (2005)
Lauger, Sébastien, Ilbert, Olivier, Buat, Véronique, Tresse, Laurence, Burgarella, Denis, Arnouts, Stéphane, ...
We studied the morphology of galaxies in the Chandra Deep Field South using ACS multi-wavelength data from the Great Observatories Origin Deep Survey and 524 spectroscopic redshifts from the VIMOS...
Evolution of morphology in the Chandra Deep Field South (2005)
Lauger, Sébastien, Ilbert, Olivier, Buat, Véronique, Tresse, Laurence, Burgarella, Denis, Arnouts, Stéphane, ...
We studied the morphology of galaxies in the Chandra Deep Field South using ACS multi-wavelength data from the Great Observatories Origin Deep Survey and 524 spectroscopic redshifts from the VIMOS...
Evolution of morphology in the Chandra Deep Field South (2005)
Lauger, Sébastien, Ilbert, Olivier, Buat, Véronique, Tresse, Laurence, Burgarella, Denis, Arnouts, Stéphane, ...
We studied the morphology of galaxies in the Chandra Deep Field South using ACS multi-wavelength data from the Great Observatories Origin Deep Survey and 524 spectroscopic redshifts from the VIMOS...
Evolution of morphology in the Chandra Deep Field South (2005)
Lauger, Sébastien, Ilbert, Olivier, Buat, Véronique, Tresse, Laurence, Burgarella, Denis, Arnouts, Stéphane, ...
We studied the morphology of galaxies in the Chandra Deep Field South using ACS multi-wavelength data from the Great Observatories Origin Deep Survey and 524 spectroscopic redshifts from the VIMOS...
UV emission and Star Formation in Stephan's Quintet (2004)
Xu, C. Kevin, Iglesias-Paramo, Jorge, Burgarella, Denis, Rich, R. Michael, Neff, Susan G., Lauger, Sebastien, ...
we present the first GALEX UV images of the well known interacting group of galaxies, Stephan's Quintet (SQ). We detect widespread UV emission throughout the group. However, there is no consistent...
Spectro-Morphology of Galaxies. (2004)
Lauger, Sébastien, Burgarella, Denis, Buat, Véronique
We present a quantitative method to classify galaxies, based on multi-wavelength data and elaborated from the properties of nearby galaxies. Our objective is to define an evolutionary method that can...
Spectro-Morphology of Galaxies. (2004)
Lauger, Sébastien, Burgarella, Denis, Buat, Véronique
We present a quantitative method to classify galaxies, based on multi-wavelength data and elaborated from the properties of nearby galaxies. Our objective is to define an evolutionary method that can...
Spectro-Morphology of Galaxies (2004)
Lauger, Sebastien, Burgarella, Denis, Buat, Veronique
We present a quantitative method to classify galaxies, based on multi-wavelength data and elaborated from the properties of nearby galaxies. Our objective is to define an evolutionary method that can...
Spectro-Morphology of Galaxies. (2004)
Lauger, Sébastien, Burgarella, Denis, Buat, Véronique
We present a quantitative method to classify galaxies, based on multi-wavelength data and elaborated from the properties of nearby galaxies. Our objective is to define an evolutionary method that can...
Spectro-Morphology of Galaxies. (2004)
Lauger, Sébastien, Burgarella, Denis, Buat, Véronique
We present a quantitative method to classify galaxies, based on multi-wavelength data and elaborated from the properties of nearby galaxies. Our objective is to define an evolutionary method that can...
Spectro-Morphology of Galaxies. (2004)
Lauger, Sébastien, Burgarella, Denis, Buat, Véronique
We present a quantitative method to classify galaxies, based on multi-wavelength data and elaborated from the properties of nearby galaxies. Our objective is to define an evolutionary method that can...
Spectro-Morphology of Galaxies. (2004)
Lauger, Sébastien, Burgarella, Denis, Buat, Véronique
We present a quantitative method to classify galaxies, based on multi-wavelength data and elaborated from the properties of nearby galaxies. Our objective is to define an evolutionary method that can...
Burgarella, Denis, Buat, Veronique, Donas, Jose, Milliard, Bruno, Chapelon, Sandra
We used ultraviolet (200 nm) images of the local spiral galaxies M33, M51, M81, M100, M101 to compute morphological parameters of galactic disks at this wavelength : half-light radius $r_{hl}$,...
Burgarella, Denis, Kissler-Patig, Markus, Buat, Veronique
We studied the metal-poor globular cluster (GC) populations of a large variety of galaxies (47 galaxies spanning about 10mag in absolute brightness) and compared their mean [Fe/H] with the properties...
Burgarella, Denis, Kissler-Patig, Markus, Buat, Veronique
We studied the metal-poor globular cluster (GC) populations of a large variety of galaxies (47 galaxies spanning about 10mag in absolute brightness) and compared their mean [Fe/H] with the properties...
Burgarella, Denis, Buat, Veronique, Donas, Jose, Milliard, Bruno, Chapelon, Sandra
We used ultraviolet (200 nm) images of the local spiral galaxies M33, M51, M81, M100, M101 to compute morphological parameters of galactic disks at this wavelength : half-light radius $r_{hl}$,...
Burgarella, Denis, Kissler-Patig, Markus, Buat, Veronique
We studied the metal-poor globular cluster (GC) populations of a large variety of galaxies (47 galaxies spanning about 10mag in absolute brightness) and compared their mean [Fe/H] with the properties...
Burgarella, Denis, Buat, Veronique, Donas, Jose, Milliard, Bruno, Chapelon, Sandra
We used ultraviolet (200 nm) images of the local spiral galaxies M33, M51, M81, M100, M101 to compute morphological parameters of galactic disks at this wavelength : half-light radius $r_{hl}$,...
Burgarella, Denis, Kissler-Patig, Markus, Buat, Veronique
In this paper, we are exploring the properties of old, metal-poor globular clusters in galaxies. We investigate whether their properties are related to the properties of their host galaxies, and...
Burgarella, Denis, Kissler-Patig, Markus, Buat, Veronique
In this paper, we are exploring the properties of old, metal-poor globular clusters in galaxies. We investigate whether their properties are related to the properties of their host galaxies, and...
Burgarella, Denis, Kissler-Patig, Markus, Buat, Veronique
In this paper, we are exploring the properties of old, metal-poor globular clusters in galaxies. We investigate whether their properties are related to the properties of their host galaxies, and...
Buat, Veronique, Burgarella, Denis
We study the FIR and UV-visible properties of nearby star forming galaxies. This comparison is performed using the local luminosity functions at UV and FIR wavelengths and on individual starburst...