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Accuracy and Results of Spectrophotometry with Objective Prism Plates

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Image Processing Techniques in Astronomy

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 54))

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Abstract

For its potential application to a large variety of astronomical investigations, objective prism is of fundamental importance among the astronomical techniques of data acquisition involving photographic plates. Reference may be made to the investigation on the interstellar extinction by Nandy (1964)1 on Nova Del 67 (Woszczyk et al., 1968), and to the calibration methods developed by Nandy and Smriglio (1970), Ardeberg and Virdefors (1972), and others.

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References

  • Ardeberg, A. and Virdefors, B.: 1972, Astron. and Astrophys. 20, 177.

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  • Cassatella, A. and Viotti, R.: 1972, Rapporto di Ricerca, Ossevatorio Astronomico di Roma, N.3.

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  • Cassatella, A. and Viotti, R.: 1974, Rapporto Interno, Laboratorio Astrofisica Spaziale, Prascati, N. 5.

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  • Nandy, K.: 1964, Publ. Roy. Obs. Edinburgh, 3, 142.

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© 1975 D. Reidel Publishing Company, Dordrecht-Holland

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Cassatella, A., Viotti, R. (1975). Accuracy and Results of Spectrophotometry with Objective Prism Plates. In: De Jager, C., Nieuwenhuijzen, H. (eds) Image Processing Techniques in Astronomy. Astrophysics and Space Science Library, vol 54. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-1881-4_46

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  • DOI: https://doi.org/10.1007/978-94-010-1881-4_46

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-1883-8

  • Online ISBN: 978-94-010-1881-4

  • eBook Packages: Springer Book Archive

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