Jahnke, Knud, Elbaz, David, Pantin, Eric, Böhm, Asmus, Wisotzki, Lutz, Letawe, Geraldine, ...
(Abridged) The luminous z=0.286 quasar HE0450-2958 is interacting with a companion galaxy at 6.5 kpc distance and the whole system is a ULIRG. A so far undetected host galaxy triggered the hypothesis...
ADONIS high contrast infrared imaging of Sirius-B (2008)
Bonnet-Bidaud, Jean-Marc, Pantin, Eric
Sirius is the brightest star in the sky and a strong source of diffuse light for modern telescopes so that the immediate surroundings of the star are still poorly known. We study the close...
METIS - the Mid-infrared E-ELT Imager and Spectrograph (2008)
Brandl, Bernhard R., Lenzen, Rainer, Pantin, Eric, Glasse, Alistair, Blommaert, Joris, Venema, Lars, ...
METIS, the Mid-infrared ELT Imager and Spectrograph (formerly called MIDIR), is a proposed instrument for the European Extremely Large Telescope (E-ELT), currently undergoing a phase-A study. The...
Rahoui, Farid, Chaty, Sylvain, Lagage, Pierre-Olivier, Pantin, Eric
(abridged) Context: The INTEGRAL mission has led to the discovery of a new type of Supergiant X-ray Binaries (SGXBs) whose physical properties differ from those of previously known SGXBs. Two classes...
Rahoui, Farid, Chaty, Sylvain, Lagage, Pierre-Olivier, Pantin, Eric
Context: The INTEGRAL mission has led to the discovery of a new type of supergiant X-ray binaries (SGXBs), whose physical properties differ from those of previously known SGXBs. Those sources are in...
Rahoui, Farid, Chaty, Sylvain, Lagage, Pierre-Olivier, Pantin, Eric
(abridged) Context: The INTEGRAL mission has led to the discovery of a new type of Supergiant X-ray Binaries (SGXBs) whose physical properties differ from those of previously known SGXBs. Two classes...
Rahoui, Farid, Chaty, Sylvain, Lagage, Pierre-Olivier, Pantin, Eric
Context: The INTEGRAL mission has led to the discovery of a new type of supergiant X-ray binaries (SGXBs), whose physical properties differ from those of previously known SGXBs. Those sources are in...
Rahoui, Farid, Chaty, Sylvain, Lagage, Pierre-Olivier, Pantin, Eric
Context: The INTEGRAL mission has led to the discovery of a new type of supergiant X-ray binaries (SGXBs), whose physical properties differ from those of previously known SGXBs. Those sources are in...
METIS: the mid-infrared E-ELT imager and spectrograph (2008)
Brandl, Bernhard R., Lenzen, Rainer, Pantin, Eric, Glasse, Alistair, Blommaert, Joris, Venema, Lars, ...
METIS: the mid-infrared E-ELT imager and spectrograph (2008)
Brandl, Bernhard R., Lenzen, Rainer, Pantin, Eric, Glasse, Alistair, Blommaert, Joris, Venema, Lars, ...
METIS, the Mid-infrared ELT Imager and Spectrograph (formerly called MIDIR), is a proposed instrument for the European Extremely Large Telescope (E-ELT), currently undergoing a phase-A study. The...
Deconvolution by the Multiscale Maximum Entropy Method (2007)
. In 1994, to overcome the difficulties encountered by the Maximum Entropy Method (MEM) to restore images containing both high and low frequencies, Bontekoe et al. introduced the Pyramid Maximum...
Haas, Martin, Siebenmorgen, Ralf, Pantin, Eric, Horst, Hannes, Smette, Alain, Kaufl, Hans-Ulrich, ...
Half of the Seyfert-2 galaxies escaped detection of broad lines in their polarised spectra observed so far. Some authors have suspected that these non-HBLRs contain real Sy2 nuclei without intrinsic...
Dynamical modeling of the Deep Impact dust ejecta cloud (2007)
Bonev, Tanyu, Ageorges, Nancy, Bagnulo, Stefano, Barrera, Luis, B{ö}hnhardt, Hermann, Hainaut, Olivier, ...
The collision of Deep Impact with comet 9P/Tempel 1 generated a bright cloud of dust which dissipated during several days after the impact. The brightness variations of this cloud and the changes of...
A mid-infrared study of very low mass stars and brown dwarfs in Upper Scorpius (2006)
Bouy, Herve, Huelamo, Nuria, Martin, Eduardo L., Navascues, David Barrado Y, Sterzik, Michael, Pantin, Eric
We report the results of mid-IR observations with VISIR at the VLT of 10 ultracool dwarfs members of the nearby Upper Scorpius OB association in four filters ranging between 8.59 (PAH1) to 12.8...
An emission ring at 20 microns around the HAEBE star AB Aurigae: unveiling the disc structure (2004)
Pantin, Eric, Bouwman, Jeroen, Lagage, Pierre-Olivier
Isolated HAEBE stars are believed to represent an intermediate stage of objects between young stellar objects surrounded by massive, optically thick, gaseous and dusty disks and Vega like stars...
An emission ring at 20 microns around the HAEBE star AB Aurigae: unveiling the disc structure (2004)
Pantin, Eric, Bouwman, Jeroen, Lagage, Pierre-Olivier
Isolated HAEBE stars are believed to represent an intermediate stage of objects between young stellar objects surrounded by massive, optically thick, gaseous and dusty disks and Vega like stars...
An emission ring at 20 microns around the HAEBE star AB Aurigae: unveiling the disc structure (2004)
Pantin, Eric, Bouwman, Jeroen, Lagage, Pierre-Olivier
Isolated HAEBE stars are believed to represent an intermediate stage of objects between young stellar objects surrounded by massive, optically thick, gaseous and dusty disks and Vega like stars...
An emission ring at 20 microns around the HAEBE star AB Aurigae: unveiling the disc structure (2004)
Pantin, Eric, Bouwman, Jeroen, Lagage, Pierre-Olivier
Isolated HAEBE stars are believed to represent an intermediate stage of objects between young stellar objects surrounded by massive, optically thick, gaseous and dusty disks and Vega like stars...
An emission ring at 20 microns around the HAEBE star AB Aurigae: unveiling the disc structure (2004)
Pantin, Eric, Bouwman, Jeroen, Lagage, Pierre-Olivier
Isolated HAEBE stars are believed to represent an intermediate stage of objects between young stellar objects surrounded by massive, optically thick, gaseous and dusty disks and Vega like stars...
Determination of limits on disc masses around six pulsars at 15 and 90 microns (2001)
Koch-Miramond, Lydie, Haas, Martin, Pantin, Eric, Podsiadlowski, Philipp, Naylor, Tim, Sauvage, Marc
We have searched for evidence of emission at 15 microns with ISOCAM and at 90 microns with ISOPHOT from dust orbiting six nearby pulsars, both in binaries and in isolation, located at distances...