CCD Base Line Subtraction Algorithms

High statistics astronomical surveys require photometric accuracy on a few percent level. The accuracy of sensor calibration procedures should match this goal. The first step in calibration procedures is the base line subtraction. The accuracy and robustness of different base line subtraction techni...

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Veröffentlicht in:IEEE transactions on nuclear science 2010-08, Vol.57 (4), p.2200-2204
Hauptverfasser: Kotov, Ivan V, Kotov, Alexandra I, Frank, James, O'Connor, Paul, Perevoztchikov, Victor, Takacs, Peter
Format: Artikel
Sprache:eng
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Zusammenfassung:High statistics astronomical surveys require photometric accuracy on a few percent level. The accuracy of sensor calibration procedures should match this goal. The first step in calibration procedures is the base line subtraction. The accuracy and robustness of different base line subtraction techniques used for Charge Coupled Device (CCD) sensors are discussed.
ISSN:0018-9499
1558-1578
DOI:10.1109/TNS.2010.2049660