| ober 17, 2002) has been designed to obtain V-Johnson photometry. Due to technical limitations on the data processing electronics and the available telemetry, it is necessary to know, a priori, the objects to be monitored within the field of view (FOV) of the OMC. The OMC Input Catalogue, and subsequent updates, provides this information: astrometric and photometric reference stars for calibration and scientific targets for accurate photometric variability studies. | |
| Auth.: | DOMINGO A. |
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