CAOSP abstracts, Volume: 43, No.: 3, year: 2014

Abstract: The performance of a near infrared camera for photometry is investigated by observations of multiple samples of spatially close non-variable stars. Objects with a J-band magnitude less than 9.2 have been observed by the application of differential photometry. For the faint objects a statistical scatter of 7.9 mmag has been determined. Possible future applications include the examination of planets orbiting late type stars by an eclipse or a timing analysis.

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Last update: April 17, 2014