The use of self-scanned silicon photodiode arrays for astronomical spectrophotometry

Details The use of self-scanned silicon photodiode arrays for astronomical spectrophotometry The use of self-scanned silicon photodiode arrays for astronomical spectrophotometry

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984nascp2350..182c&link_type=abstract

In NASA. Ames Research Center Proc. of the Workshop on Improvements to Photometry p 182-192 (SEE N85-17892 08-89)

Other

Arrays, Astronomical Photometry, Photodiodes, Errors, Precision, Scanning, Signal To Noise Ratios, Spectral Resolution, Spectrometers, Spectrophotometers

Scientific paper

The use of a Reticon self scanned silicon photodiode array for precision spectrophotometry is discussed. It is shown that internal errors are + or - 0.003 mag. Observations obtained with a photodiode array are compared with observations obtained with other types of detectors with agreement, from 3500 A to 10500 A, of 1%. The photometric properties of self scanned photodiode arrays are discussed. Potential pitfalls are given.

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