EXTRASOLAR PLANETS & SUBSTELLAR OBJECTS
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    High Accuracy Radial velocity Planetary Search (HARPS)

    A program to detect extrasolar planets by the radial velocity method using the 3.6-meter telescope at the La Silla Observatory. When operational, the detection equipment will be capable of radial velocity measurements accurate to about 1 meter per second for a slowly rotating star.


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       • EXTRASOLAR PLANETS AND SUBSTELLAR OBJECTS





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