Transformation equations between the standard and CCD Vilnius systems. IV. Two Mt. Graham CCD systems

Transformation equations between the standard and CCD Vilnius systems. IV. Two Mt. Graham CCD systems

Transformation equations between magnitudes and color indices of the CCD and the standard Vilnius systems are calculated by the synthetic photometry method for two CCD cameras being used on the 1.8-m telescope of the Vatican Observatory on Mt. Graham. The color equations take into account the temper...

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Veröffentlicht in:Baltic astronomy 1997, Vol.6 (3), p.457-470
Hauptverfasser: Straižys, V., Kazlauskas, A., Boyle, R. P., Smriglio, F.
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container_title Baltic astronomy
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creator Straižys, V.
Kazlauskas, A.
Boyle, R. P.
Smriglio, F.
description Transformation equations between magnitudes and color indices of the CCD and the standard Vilnius systems are calculated by the synthetic photometry method for two CCD cameras being used on the 1.8-m telescope of the Vatican Observatory on Mt. Graham. The color equations take into account the temperature, luminosity and interstellar reddening effects and make possible transforming the CCD color indices and magnitudes to the standard system with an accuracy of 0.01 mag. (Author)
doi_str_mv 10.1515/astro-1997-0309
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title Transformation equations between the standard and CCD Vilnius systems. IV. Two Mt. Graham CCD systems
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