MICROMEGAS chambers for hadronic calorimetry at a future linear collider (2009)
Adloff, C., Attie, D., Blaha, J., Cap, S., Chefdeville, M., Colas, P., ...
Prototypes of MICROMEGAS chambers, using bulk technology and analog readout, with 1x1cm2 readout segmentation have been built and tested. Measurements in Ar/iC4H10 (95/5) and Ar/CO2 (80/20) are...
Micromegas TPC studies at high magnetic fields using the charge dispersion signal (2008)
Dixit, M., Attie, D., Bellerive, A., Boudjemline, K., Colas, P., Giganon, P., ...
The International Linear Collider (ILC) Time Projection Chamber (TPC) transverse space-point resolution goal is 100 microns for all tracks including stiff 90 degree tracks with the full 2 meter...
Micromegas TPC studies at high magnetic fields using the charge dispersion signal (2008)
Dixit, M., Attie, D., Bellerive, A., Boudjemline, K., Colas, P., Giganon, P., ...
The International Linear Collider (ILC) Time Projection Chamber (TPC) transverse space-point resolution goal is 100 microns for all tracks including stiff 90 degree tracks with the full 2 meter...
Micromegas TPC studies at high magnetic fields using the charge dispersion signal (2008)
Dixit, M., Attie, D., Bellerive, A., Boudjemline, K., Colas, P., Giganon, P., ...
The International Linear Collider (ILC) Time Projection Chamber (TPC) transverse space-point resolution goal is 100 microns for all tracks including stiff 90 degree tracks with the full 2 meter...
Micromegas TPC studies at high magnetic fields using the charge dispersion signal (2007)
Dixit, Authors M., Attie, D., Bellerive, A., Boudjemline, K., Colas, P., Giganon, P., ...
The International Linear Collider (ILC) Time Projection Chamber (TPC) transverse space-point resolution goal is 100 microns for all tracks including stiff 90 degree tracks with the full 2 meter...
Calibration of the spectrometer aboard the INTEGRAL satellite (2007)
Schanne, S., Cordier, B., Gros, M., Attie, D., Von Ballmoos, P., Bouchet, L., ...
SPI, the Spectrometer on board the ESA INTEGRAL satellite, to be launched in October 2002, will study the gammaray sky in the 20 keV to 8 MeV energy band with a spectral resolution of 2 keV for...
Calibration of the spectrometer aboard the INTEGRAL satellite (2007)
Schanne, S., Cordier, B., Gros, M., Attie, D., Von Ballmoos, P., Bouchet, L., ...
SPI, the Spectrometer on board the ESA INTEGRAL satellite, to be launched in October 2002, will study the gammaray sky in the 20 keV to 8 MeV energy band with a spectral resolution of 2 keV for...
Calibration of the spectrometer aboard the INTEGRAL satellite (2007)
Schanne, S., Cordier, B., Gros, M., Attie, D., Von Ballmoos, P., Bouchet, L., ...
SPI, the Spectrometer on board the ESA INTEGRAL satellite, to be launched in October 2002, will study the gammaray sky in the 20 keV to 8 MeV energy band with a spectral resolution of 2 keV for...
Kiener, J., Gros, M., Tatischeff, V., Attie, D., Bailly, I., Bauchet, A., ...
Gamma-ray angular distributions for the resonances at Ep = 550 keV and 1747 keV of the radiative capture reaction 13-C(p,g)14-N have been measured, using intense proton beams on isotopically pure...
INTEGRAL detection of a strong outburst in 4U 1954+31 (2006)
Paltani, S., Attie, D., Domingo Garau, A., Larsson, S., Paul, J., Shtykovsky, P., ...
Search for 44Ti gamma-ray line emission from GRO J0852-4642 with INTEGRAL/SPI (2004)
Von Kienlin, A., Attie, D., Schanne, S., Cordier, B., Diehl, R., Iyudin, A. F., ...
The gamma-ray source GRO J0852-4642, discovered by COMPTEL, is a possible counterpart of the supernova remnant RX J0852-4622. Detection of radioactive decay from 44Ti nuclei would proof it to be the...
INTEGRAL broadband spectroscopy of Vela X-1 (2004)
Kretschmar, P., Staubert, R., Kreykenbohm, I., Chernyakova, M., Kienlin, A. V., Larsson, S., ...
The wind-accreting X-ray binary pulsar and cyclotron line source Vela X-1 has been observed extensively during INTEGRAL Core Program observations of the Vela region in June-July and November-December...
The INTEGRAL/SPI response and the Crab observations (2004)
Sizun, P., Shrader, C. R., Attie, D., Dubath, P., Schanne, S., Cordier, B., ...
The Crab region was observed several times by INTEGRAL for calibration purposes. This paper aims at underlining the systematic interactions between (i) observations of this reference source, (ii)...
Search for a light dark matter annihilation signal in the Sagittarius Dwarf Galaxy (2004)
Cordier, B., Attie, D., Casse, M., Paul, J., Schanne, S., Sizun, P., ...
The 511 keV emission from the Galactic Bulge observed by INTEGRAL/SPI could be the product of light (1-100 MeV) annihilating dark matter particles. In order to distinguish between annihilating light...
Transition to a hard state of 1RXP J130159.6-635806 (2004)
Chernyakova, M., Shtykovsky, P., Lutovinov, A., Revnivtsev, M., Courvoisier, T., Walter, R., ...
We report a detection of a transition to a hard state during the possible outburst of a ROSAT source 1RXP J130159.6-635806, located approximately 10 arc minutes from PSR 1259-63. Source was observed...
Kiener, J., Gros, M., Tatischeff, V., Attie, D., Bailly, I., Bauchet, A., ...
Gamma-ray angular distributions for the resonances at Ep = 550 keV and 1747 keV of the radiative capture reaction 13-C(p,g)14-N have been measured, using intense proton beams on isotopically pure...
First identification and modelling of SPI background lines (2003)
Weidenspointner, G., Kiener, J., Gros, M., Jean, P., Teegarden, BJ., Wunderer, C., ...
INTEGRAL/SPI ground calibration (2003)
Attie, D., Cordier, B., Gros, M., Laurent, P., Schanne, S., Tauzin, G., ...
Calibration of the spectrometer aboard the INTEGRAL satellite (2003)
Schanne, S., Cordier, B., Gros, M., Attie, D., Von Ballmoos, P., Bouchet, L., ...
First identification and modelling of SPI background lines (2003)
Weidenspointner, G., Kiener, J., Gros, M., Jean, P., Teegarden, BJ., Wunderer, C., ...
INTEGRAL/SPI ground calibration (2003)
Attie, D., Cordier, B., Gros, M., Laurent, P., Schanne, S., Tauzin, G., ...
Calibration of the spectrometer aboard the INTEGRAL satellite (2003)
Schanne, S., Cordier, B., Gros, M., Attie, D., Von Ballmoos, P., Bouchet, L., ...
First identification and modelling of SPI background lines (2003)
Weidenspointner, G., Kiener, J., Gros, M., Jean, P., Teegarden, BJ., Wunderer, C., ...
On Oct. 17, 2002, the ESA INTEGRAL observatory was launched into a highly elliptical orbit. SPI, a high resolution Ge spectrometer covering an energy range of 20-8000 keV, is one of its two main...
SPI instrumental background characteristics (2003)
Jean, P., Vedrenne, G., Roques, J.P., Schonfelder, V., Teegarden, B.J., Von Kienlin, A., ...
In its space environment the INTEGRAL observatory is subject to an intense irradiation by energetic cosmic-ray particles that leads, via nuclear interactions with the telescope and spacecraft...
First identification and modelling of SPI background lines (2003)
Weidenspointner, G., Kiener, J., Gros, M., Jean, P., Teegarden, BJ., Wunderer, C., ...
On Oct. 17, 2002, the ESA INTEGRAL observatory was launched into a highly elliptical orbit. SPI, a high resolution Ge spectrometer covering an energy range of 20-8000 keV, is one of its two main...
SPI instrumental background characteristics (2003)
Jean, P., Vedrenne, G., Roques, J.P., Schonfelder, V., Teegarden, B.J., Von Kienlin, A., ...
In its space environment the INTEGRAL observatory is subject to an intense irradiation by energetic cosmic-ray particles that leads, via nuclear interactions with the telescope and spacecraft...
First identification and modelling of SPI background lines (2003)
Weidenspointner, G., Kiener, J., Gros, M., Jean, P., Teegarden, BJ., Wunderer, C., ...
On Oct. 17, 2002, the ESA INTEGRAL observatory was launched into a highly elliptical orbit. SPI, a high resolution Ge spectrometer covering an energy range of 20-8000 keV, is one of its two main...
SPI instrumental background characteristics (2003)
Jean, P., Vedrenne, G., Roques, J.P., Schonfelder, V., Teegarden, B.J., Von Kienlin, A., ...
In its space environment the INTEGRAL observatory is subject to an intense irradiation by energetic cosmic-ray particles that leads, via nuclear interactions with the telescope and spacecraft...