Transformation equations between the standard and CCD Vilnius systems. III - The Loiano CCD system

Details Transformation equations between the standard and CCD Vilnius systems. III - The Loiano CCD system Transformation equations between the standard and CCD Vilnius systems. III - The Loiano CCD system

Sep 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997balta...6..445s&link_type=abstract

Baltic Astronomy, vol. 6, p. 445

Mathematics

1

Charge Coupled Devices, Astronomical Photometry, Stellar Magnitude, Stellar Color, Transformations (Mathematics), Ccd Cameras, Astronomical Observatories

Scientific paper

Transformation equations between magnitudes and color indices of the CCD and the standard Vilnius systems are calculated by the synthetic photometry method for the CCD camera of the 1.52-m telescope of the Loiano Observatory. The color equations take into account the temperature, luminosity, and interstellar reddening effects, and make possible transforming of the CCD color indices and magnitudes to the standard system with an accuracy of 0.01 mag.

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