The SNDICE calibrated light source (“LED-head”) is mounted on an altitude-azimuth (alt-az) motion, itself installed on the south-east platform fixed to the CFHT superior part of the dome in a overhanging position. The altitude and the azimuth motors are hold together by a right angle bracket. The azimuthal plate has been shimmed horizontally using a level. Both motors have an elementary step of 1°/400= 9”. The optical axis of the LED-head is materialized by a parallel beam, the “artificial planet” (AP), which angular aperture is 40”
We present the aberration field response of Ritchey-Chretien telescopes, with the aperture stop on t...
Accepted by Nuclear Inst. and Methods in Physics Research, A NIMAA calibration method for telescope ...
A 1-meter balloon-borne telescope has been constructed and flown to observe far-infrared radiation f...
The SNDICE calibrated light source (“LED-head”) is mounted on an altitude-azimuth (alt-az) motion, i...
The SNDICE calibrated light source (“LED-head”) is mounted on an altitude-azimuth (alt-az) motion, i...
International audienceWe present the first results of the SuperNova Direct Illumination Calibration ...
We present the first results of the SuperNova Direct Illumination Calibration Experiment (SNDICE), i...
The photometric calibration of the wide field imager MegaCam at the CFHTis the dominant systematic u...
Photometric calibration of wide field imagers is becoming a crucial issue in various cosmological me...
Theodolites are a common instrument in the testing, alignment, and building of various systems rangi...
version finalePhotometric calibration of wide field imagers is becoming a crucial issue in various c...
We present the very basic features—from the observer’s point of view—of the software pack allowing f...
Methods and instruments for the alignment of the optical sensors in the spacelabs Vega I. and II. ...
Sun and star trackers have been added to the latest version of the Geneva Observatory gondola. They ...
Accepted by Nuclear Inst. and Methods in Physics Research, A NIMAA calibration method for telescope ...
We present the aberration field response of Ritchey-Chretien telescopes, with the aperture stop on t...
Accepted by Nuclear Inst. and Methods in Physics Research, A NIMAA calibration method for telescope ...
A 1-meter balloon-borne telescope has been constructed and flown to observe far-infrared radiation f...
The SNDICE calibrated light source (“LED-head”) is mounted on an altitude-azimuth (alt-az) motion, i...
The SNDICE calibrated light source (“LED-head”) is mounted on an altitude-azimuth (alt-az) motion, i...
International audienceWe present the first results of the SuperNova Direct Illumination Calibration ...
We present the first results of the SuperNova Direct Illumination Calibration Experiment (SNDICE), i...
The photometric calibration of the wide field imager MegaCam at the CFHTis the dominant systematic u...
Photometric calibration of wide field imagers is becoming a crucial issue in various cosmological me...
Theodolites are a common instrument in the testing, alignment, and building of various systems rangi...
version finalePhotometric calibration of wide field imagers is becoming a crucial issue in various c...
We present the very basic features—from the observer’s point of view—of the software pack allowing f...
Methods and instruments for the alignment of the optical sensors in the spacelabs Vega I. and II. ...
Sun and star trackers have been added to the latest version of the Geneva Observatory gondola. They ...
Accepted by Nuclear Inst. and Methods in Physics Research, A NIMAA calibration method for telescope ...
We present the aberration field response of Ritchey-Chretien telescopes, with the aperture stop on t...
Accepted by Nuclear Inst. and Methods in Physics Research, A NIMAA calibration method for telescope ...
A 1-meter balloon-borne telescope has been constructed and flown to observe far-infrared radiation f...