Handbook of CCD Astronomy¶
Howell, S. B. (2006). Handbook of CCD Astronomy. Cambridge University Press.
Cited by¶
2 citations across 2 artifacts.
Each citation links to the sentence it supports in the citing article.
Primes¶
- Control Sample
- In astronomy and physics it is blank-sky exposures subtracted from imaging, off-source pointings, and beam-off detector runs that define what a signal run must rise above.
This sourceBias, dark, and blank-sky frames subtracted from astronomical imaging to define the signal above background.
- In astronomy and physics it is blank-sky exposures subtracted from imaging, off-source pointings, and beam-off detector runs that define what a signal run must rise above.
- Counterfactual Subtraction
- Signal processing and metrology: background-subtracted signal; dark-current subtraction in detectors; ambient-noise subtraction in acoustics; sky-subtracted astronomical spectra.
This sourceStandard data-reduction reference establishing bias/dark-current subtraction and sky/background subtraction as routine metrology practice — the observed frame minus a constructed background baseline.
- Signal processing and metrology: background-subtracted signal; dark-current subtraction in detectors; ambient-noise subtraction in acoustics; sky-subtracted astronomical spectra.
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Links previously used in the corpus¶
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Registry ID ref:03ef8e4766f0 · see in the full table