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
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...
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...
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...
Submillimetre/TeraHertz Astronomy at Dome C with CEA filled bolometer array (2007)
Minier, Vincent, Durand, Gilles, Lagage, Pierre-Olivier, Talvard, Michel, Travouillon, Tony, Busso, Maurizio, ...
Submillimetre/TeraHertz (e.g. 200, 350, 450 microns) astronomy is the prime technique to unveil the birth and early evolution of a broad range of astrophysical objects. A major obstacle to carry out...
Submillimetre/TeraHertz Astronomy at Dome C with CEA filled bolometer array (2007)
Minier, Vincent, Durand, Gilles, Lagage, Pierre-Olivier, Talvard, Michel, Travouillon, Tony, Busso, Maurizio, ...
Submillimetre/TeraHertz (e.g. 200, 350, 450 microns) astronomy is the prime technique to unveil the birth and early evolution of a broad range of astrophysical objects. A major obstacle to carry out...
Submillimetre/TeraHertz Astronomy at Dome C with CEA filled bolometer array (2007)
Minier, Vincent, Durand, Gilles, Lagage, Pierre-Olivier, Talvard, Michel, Travouillon, Tony, Busso, Maurizio, ...
Submillimetre/TeraHertz (e.g. 200, 350, 450 microns) astronomy is the prime technique to unveil the birth and early evolution of a broad range of astrophysical objects. A major obstacle to carry out...
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...
Molecular and Ionic shocks in the Supernova Remnant 3C391 (2001)
Reach, William T., Rho, Jeonghee, Jarrett, T. H., Lagage, Pierre-Olivier
New observations of the supernova remnant 3C391 are in the H2 2.12 micron and [Fe II] 1.64 micron narrow-band filters at the Palomar 200-inch telescope, and in the 5-15 micron CVF on ISOCAM. Shocked...
Pierre-olivier Lagage, Gilles Durand, Charles Lyraud, Jan Willem Pel
In this paper, we present the status of VISIR, the mid-infrared instrument to be installed in 2001 at the Cassegrain focus of YEPUN, the telescope unit number 4 of the European Very Large Telescope...
Ellison, Donald C., Goret, Philippe, Baring, Matthew G., Grenier, Isabelle A., Lagage, Pierre-Olivier
We calculate particle spectra and continuum photon emission from the Cassiopeia A supernova remnant (SNR). The particle spectra, ion and electron, result from diffusive shock acceleration at the...