A telescope calibration method for type Ia supernovae photometry is proposed. It is based on the direct illumination of a telescope with a calibrated multi-LED light source. Its description includes traceability of the calibration process and check standard to maintain 0.2% accuracy over years period. Although opto-electronics read-out and control could be built from commercial off-the-shelf components, we report on developments relevant for large systems. Their requirements are tailored on a proposal for the SNLS experiment performed on the Megaprime instrument installed in CFHT for which our R&D is performed. Similar LED systems of larger size are working in high-energy physics optical calorimeters
Abstract. Dark Energy studies with type Ia supernovae set very tight constraints on the photometric ...
Ten years ago, type Ia supernovae used as distances indicators led to the discovery of the accelera...
Aims. We present the photometric calibration of the Supernova Legacy Survey (SNLS) fields. The SNLS ...
A telescope calibration method for type Ia supernovae photometry is proposed. It is based on the dir...
Accepted by Nuclear Inst. and Methods in Physics Research, A NIMAA calibration method for telescope ...
Dans les analyses récentes des relevés de SNe Ia pour caractériser l'énergie noire, les incertitudes...
International audienceWe present the first results of the SuperNova Direct Illumination Calibration ...
In recent SN Ia survey analyzes for dark energy characterization, statistical and systematic uncerta...
SNDICE primary goal was to provide a photometric calibration of the CFH telescope in order to supple...
The photometric calibration of the wide field imager MegaCam at the CFHTis the dominant systematic u...
This "habilitation thesis" consists in a series of three independent review papers, devoted to the r...
To Appear in "The Future of Photometric, Spectrophotometric and Polarimetric Standardization" Confer...
International audienceAims. We describe the design, operation, and first results of a photometric ca...
Aims. We describe the design, operation, and first results of a photometric calibration project, cal...
Il y a près d’une décennie, l'utilisation des supernovae de type Ia comme indicateurs de distan...
Abstract. Dark Energy studies with type Ia supernovae set very tight constraints on the photometric ...
Ten years ago, type Ia supernovae used as distances indicators led to the discovery of the accelera...
Aims. We present the photometric calibration of the Supernova Legacy Survey (SNLS) fields. The SNLS ...
A telescope calibration method for type Ia supernovae photometry is proposed. It is based on the dir...
Accepted by Nuclear Inst. and Methods in Physics Research, A NIMAA calibration method for telescope ...
Dans les analyses récentes des relevés de SNe Ia pour caractériser l'énergie noire, les incertitudes...
International audienceWe present the first results of the SuperNova Direct Illumination Calibration ...
In recent SN Ia survey analyzes for dark energy characterization, statistical and systematic uncerta...
SNDICE primary goal was to provide a photometric calibration of the CFH telescope in order to supple...
The photometric calibration of the wide field imager MegaCam at the CFHTis the dominant systematic u...
This "habilitation thesis" consists in a series of three independent review papers, devoted to the r...
To Appear in "The Future of Photometric, Spectrophotometric and Polarimetric Standardization" Confer...
International audienceAims. We describe the design, operation, and first results of a photometric ca...
Aims. We describe the design, operation, and first results of a photometric calibration project, cal...
Il y a près d’une décennie, l'utilisation des supernovae de type Ia comme indicateurs de distan...
Abstract. Dark Energy studies with type Ia supernovae set very tight constraints on the photometric ...
Ten years ago, type Ia supernovae used as distances indicators led to the discovery of the accelera...
Aims. We present the photometric calibration of the Supernova Legacy Survey (SNLS) fields. The SNLS ...