Near-infrared wavefront sensing for the VLT interferometer (2008)
Hippler, Stefan, Brandner, Wolfgang, Clénet, Yann, Hormuth, Felix, Gendron, Eric, Henning, Thomas, ...
The very large telescope (VLT) interferometer (VLTI) in its current operating state is equipped with high-order adaptive optics (MACAO) working in the visible spectrum. A low-order near-infrared...
Near-infrared wavefront sensing for the VLT interferometer (2008)
Hippler, Stefan, Brandner, Wolfgang, Clénet, Yann, Hormuth, Felix, Gendron, Eric, Henning, Thomas, ...
Near-infrared wavefront sensing for the VLT interferometer (2008)
Hippler, Stefan, Brandner, Wolfgang, Clénet, Yann, Hormuth, Felix, Gendron, Eric, Henning, Thomas, ...
The very large telescope (VLT) interferometer (VLTI) in its current operating state is equipped with high-order adaptive optics (MACAO) working in the visible spectrum. A low-order near-infrared...
Assemat, Francois, Gendron, Eric, Hammer, Francois
Integral field spectrographs are major instruments to study the mechanisms involved in the formation and the evolution of early galaxies. When combined with multi-object spectroscopy, those...
PSF reconstruction for NAOS-CONICA (2006)
Clénet, Yann, Kasper, Markus, Gendron, Eric, Fusco, Thierry, Rousset, Gérard, Gratadour, Damien, ...
Adaptive optics (AO) allows one to derive the point spread function (PSF) simultaneously to the science image, which is a major advantage in post-processing tasks such as astrometry/photometry or...
PSF reconstruction for NAOS-CONICA (2006)
Clénet, Yann, Kasper, Markus, Gendron, Eric, Fusco, Thierry, Rousset, Gérard, Gratadour, Damien, ...
Adaptive optics (AO) allows one to derive the point spread function (PSF) simultaneously to the science image, which is a major advantage in post-processing tasks such as astrometry/photometry or...
PSF reconstruction for NAOS-CONICA (2006)
Clénet, Yann, Kasper, Markus, Gendron, Eric, Fusco, Thierry, Rousset, Gérard, Gratadour, Damien, ...
Adaptive optics (AO) allows one to derive the point spread function (PSF) simultaneously to the science image, which is a major advantage in post-processing tasks such as astrometry/photometry or...
New algorithms for adaptive optics point-spread function reconstruction (2006)
Gendron, Eric, Clénet, Yann, Fusco, Thierry, Rousset, Gérard
Context. The knowledge of the point-spread function compensated by adaptive optics is of prime importance in several image restoration techniques such as deconvolution and astrometric/photometric...
New algorithms for adaptive optics point-spread function reconstruction (2006)
Gendron, Eric, Clénet, Yann, Fusco, Thierry, Rousset, Gérard
Context. The knowledge of the point-spread function compensated by adaptive optics is of prime importance in several image restoration techniques such as deconvolution and astrometric/photometric...
New algorithms for adaptive optics point-spread function reconstruction (2006)
Gendron, Eric, Clénet, Yann, Fusco, Thierry, Rousset, Gérard
Context. The knowledge of the point-spread function compensated by adaptive optics is of prime importance in several image restoration techniques such as deconvolution and astrometric/photometric...
PSF reconstruction for NAOS-CONICA (2006)
Clénet, Yann, Kasper, Markus, Gendron, Eric, Fusco, Thierry, Rousset, Gérard, Gratadour, Damien, ...
Adaptive optics (AO) allows one to derive the point spread function (PSF) simultaneously to the science image, which is a major advantage in post-processing tasks such as astrometry/photometry or...
New algorithms for adaptive optics point-spread function reconstruction (2006)
Gendron, Eric, Clénet, Yann, Fusco, Thierry, Rousset, Gérard
Context. The knowledge of the point-spread function compensated by adaptive optics is of prime importance in several image restoration techniques such as deconvolution and astrometric/photometric...
PSF reconstruction for NAOS-CONICA (2006)
Clénet, Yann, Kasper, Markus, Gendron, Eric, Fusco, Thierry, Rousset, Gérard, Gratadour, Damien, ...
Adaptive optics (AO) allows one to derive the point spread function (PSF) simultaneously to the science image, which is a major advantage in post-processing tasks such as astrometry/photometry or...
Overview of the coordinated ground-based observations of Titan during the Huygens mission (2006)
Witasse, Olivier, Lebreton, Jean-Pierre, Bird, Michael K., Dutta-Roy, Robindro, Folkner, William M., Preston, Robert A., ...
Coordinated ground-based observations of Titan were performed around or during the Huygens atmospheric probe mission at Titan on 14 January 2005, connecting the momentary in situ observations by the...
PSF reconstruction for NAOS-CONICA (2006)
Clénet, Yann, Kasper, Markus, Gendron, Eric, Fusco, Thierry, Rousset, Gérard, Gratadour, Damien, ...
Adaptive optics (AO) allows one to derive the point spread function (PSF) simultaneously to the science image, which is a major advantage in post-processing tasks such as astrometry/photometry or...
New algorithms for adaptive optics point-spread function reconstruction (2006)
Gendron, Eric, Clénet, Yann, Fusco, Thierry, Rousset, Gérard
Context. The knowledge of the point-spread function compensated by adaptive optics is of prime importance in several image restoration techniques such as deconvolution and astrometric/photometric...
Overview of the coordinated ground-based observations of Titan during the Huygens mission (2006)
Witasse, Olivier, Lebreton, Jean-Pierre, Bird, Michael K., Dutta-Roy, Robindro, Folkner, William M., Preston, Robert A., ...
Coordinated ground-based observations of Titan were performed around or during the Huygens atmospheric probe mission at Titan on 14 January 2005, connecting the momentary in situ observations by the...
Overview of the coordinated ground-based observations of Titan during the Huygens mission (2006)
Witasse, Olivier, Lebreton, Jean-Pierre, Bird, Michael K., Dutta-Roy, Robindro, Folkner, William M., Preston, Robert A., ...
Coordinated ground-based observations of Titan were performed around or during the Huygens atmospheric probe mission at Titan on 14 January 2005, connecting the momentary in situ observations by the...
Overview of the coordinated ground-based observations of Titan during the Huygens mission (2006)
Witasse, Olivier, Lebreton, Jean-Pierre, Bird, Michael K., Dutta-Roy, Robindro, Folkner, William M., Preston, Robert A., ...
Coordinated ground-based observations of Titan were performed around or during the Huygens atmospheric probe mission at Titan on 14 January 2005, connecting the momentary in situ observations by the...
Overview of the coordinated ground-based observations of Titan during the Huygens mission (2006)
Witasse, Olivier, Lebreton, Jean-Pierre, Bird, Michael K., Dutta-Roy, Robindro, Folkner, William M., Preston, Robert A., ...
Coordinated ground-based observations of Titan were performed around or during the Huygens atmospheric probe mission at Titan on 14 January 2005, connecting the momentary in situ observations by the...
A dual emission mechanism in Sgr A*/L' ? (2005)
Clénet, Yann, Rouan, Daniel, Gratadour, Damien, Marco, Olivier, Léna, Pierre, Ageorges, Nancy, ...
We have collected in 2004 adaptive optics corrected L' images of the Galactic Center region with NAOS-CONICA at VLT. A strong variability was observed as well as a correlation between the photocenter...
A dual emission mechanism in Sgr A*/L' ? (2005)
Clénet, Yann, Rouan, Daniel, Gratadour, Damien, Marco, Olivier, Léna, Pierre, Ageorges, Nancy, ...
We have collected in 2004 adaptive optics corrected L' images of the Galactic Center region with NAOS-CONICA at VLT. A strong variability was observed as well as a correlation between the photocenter...
A dual emission mechanism in Sgr A*/L' ? (2005)
Clénet, Yann, Rouan, Daniel, Gratadour, Damien, Marco, Olivier, Léna, Pierre, Ageorges, Nancy, ...
We have collected in 2004 adaptive optics corrected L' images of the Galactic Center region with NAOS-CONICA at VLT. A strong variability was observed as well as a correlation between the photocenter...
A dual emission mechanism in Sgr A*/L' ? (2005)
Clénet, Yann, Rouan, Daniel, Gratadour, Damien, Marco, Olivier, Léna, Pierre, Ageorges, Nancy, ...
We have collected in 2004 adaptive optics corrected L' images of the Galactic Center region with NAOS-CONICA at VLT. A strong variability was observed as well as a correlation between the photocenter...
A dual emission mechanism in Sgr A*/L' ? (2005)
Clénet, Yann, Rouan, Daniel, Gratadour, Damien, Marco, Olivier, Léna, Pierre, Ageorges, Nancy, ...
We have collected in 2004 adaptive optics corrected L' images of the Galactic Center region with NAOS-CONICA at VLT. A strong variability was observed as well as a correlation between the photocenter...
FALCON: a concept to extend adaptive optics corrections to cosmological fields (2004)
Hammer, Francois, Puech, Mathieu, Assémat, Francois, Gendron, Eric, Sayède, Frederic, Laporte, Philippe, ...
FALCON is an original concept for a next generation spectrograph at ESO VLT or at future ELTs. It is a spectrograph including multiple small integral field units (IFUs) which can be deployed within a...
FALCON: a concept to extend adaptive optics corrections to cosmological fields (2004)
Hammer, Francois, Puech, Mathieu, Assémat, Francois, Gendron, Eric, Sayède, Frederic, Laporte, Philippe, ...
FALCON is an original concept for a next generation spectrograph at ESO VLT or at future ELTs. It is a spectrograph including multiple small integral field units (IFUs) which can be deployed within a...
FALCON: a concept to extend adaptive optics corrections to cosmological fields (2004)
Hammer, Francois, Puech, Mathieu, Assemat, Francois, Gendron, Eric, Sayede, Frederic, Laporte, Philippe, ...
FALCON is an original concept for a next generation spectrograph at ESO VLT or at future ELTs. It is a spectrograph including multiple small integral field units (IFUs) which can be deployed within a...
FALCON: a concept to extend adaptive optics corrections to cosmological fields (2004)
Hammer, Francois, Puech, Mathieu, Assémat, Francois, Gendron, Eric, Sayède, Frederic, Laporte, Philippe, ...
FALCON is an original concept for a next generation spectrograph at ESO VLT or at future ELTs. It is a spectrograph including multiple small integral field units (IFUs) which can be deployed within a...
FALCON: a concept to extend adaptive optics corrections to cosmological fields (2004)
Hammer, Francois, Puech, Mathieu, Assémat, Francois, Gendron, Eric, Sayède, Frederic, Laporte, Philippe, ...
FALCON is an original concept for a next generation spectrograph at ESO VLT or at future ELTs. It is a spectrograph including multiple small integral field units (IFUs) which can be deployed within a...
Rouan, Daniel, Lacombe, François, Gendron, Eric, Gratadour, Damien, Clénet, Yann, Lagrange, Anne-Marie, ...
We present K, L and M diffraction-limited images of NGC 1068 obtained with NAOS+CONICA at VLT/YEPUN over a 3.5" field around the central engine. Hot dust (Tcol = 550-650 K) is found in three...
VLT/NACO infrared adaptive optics images of small scale structures in OMC1 (2003)
Lacombe, François, Gendron, Eric, Rouan, Daniel, Clénet, Yann, Lemaire, Jean-Louis, Lagrange, Anne-Marie, ...
Near-infrared observations of line emission from excited H2 and in the continuum are reported in the direction of the Orion molecular cloud OMC1, using the European Southern Observatory Very...
Rouan, Daniel, Lacombe, François, Gendron, Eric, Gratadour, Damien, Clénet, Yann, Lagrange, Anne-Marie, ...
We present K, L and M diffraction-limited images of NGC 1068 obtained with NAOS+CONICA at VLT/YEPUN over a 3.5" field around the central engine. Hot dust (Tcol = 550-650 K) is found in three...
VLT/NACO infrared adaptive optics images of small scale structures in OMC1 (2003)
Lacombe, François, Gendron, Eric, Rouan, Daniel, Clénet, Yann, Lemaire, Jean-Louis, Lagrange, Anne-Marie, ...
Near-infrared observations of line emission from excited H2 and in the continuum are reported in the direction of the Orion molecular cloud OMC1, using the European Southern Observatory Very...
Rouan, Daniel, Lacombe, Francois, Gendron, Eric, Gratadour, Damien, Clenet, Yann, Lagrange, Anne-Marie, ...
We present K, L and M diffraction-limited images of NGC 1068 obtained with NAOS+CONICA at VLT/YEPUN over a 3.5" field around the central engine. Hot dust (Tcol = 550-650 K) is found in three...
Rouan, Daniel, Lacombe, François, Gendron, Eric, Gratadour, Damien, Clénet, Yann, Lagrange, Anne-Marie, ...
We present K, L and M diffraction-limited images of NGC 1068 obtained with NAOS+CONICA at VLT/YEPUN over a 3.5" field around the central engine. Hot dust (Tcol = 550-650 K) is found in three...
VLT/NACO infrared adaptive optics images of small scale structures in OMC1 (2003)
Lacombe, François, Gendron, Eric, Rouan, Daniel, Clénet, Yann, Lemaire, Jean-Louis, Lagrange, Anne-Marie, ...
Near-infrared observations of line emission from excited H2 and in the continuum are reported in the direction of the Orion molecular cloud OMC1, using the European Southern Observatory Very...
First diffraction limited images at VLT with NAOS and CONOCA (2003)
Lagrange, Anne M., Chauvin, Gael, Fusco, Thierry, Gendron, Eric, Rouan, Daniel, Hartung, Markus, ...
Polarization with adaptive optics at ESO Very Large Telescope (Yepun) (2003)
Ageorges, Nancy, Lenzen, Rainer, Hartung, Markus, Brandner, Wolfgang, Gendron, Eric, Moorwood, Alan F. M., ...
Rouan, Daniel, Lacombe, François, Gendron, Eric, Gratadour, Damien, Clénet, Yann, Lagrange, Anne-Marie, ...
We present K, L and M diffraction-limited images of NGC 1068 obtained with NAOS+CONICA at VLT/YEPUN over a 3.5" field around the central engine. Hot dust (Tcol = 550-650 K) is found in three...
VLT/NACO infrared adaptive optics images of small scale structures in OMC1 (2003)
Lacombe, François, Gendron, Eric, Rouan, Daniel, Clénet, Yann, Lemaire, Jean-Louis, Lagrange, Anne-Marie, ...
Near-infrared observations of line emission from excited H2 and in the continuum are reported in the direction of the Orion molecular cloud OMC1, using the European Southern Observatory Very...