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Image Inventory Using the Wavelet Transform
Published online by Cambridge University Press: 26 July 2016
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Today, large astronomical plates are digitised with fast scanners, leading to images with about 109 pixels. This amount of information permits astronomers to apply various computer vision techniques to get inventories of the objects on the plates.
- Type
- Part Five: Image Detection, Cataloguing and Classification
- Information
- Symposium - International Astronomical Union , Volume 161: Astronomy from Wide-Field Imaging , 1994 , pp. 213 - 217
- Copyright
- Copyright © Kluwer 1994
References
Bijaoui, A., Lago, G., Marchal, J and Ounnas, C., 1978. ‘Traitement des Images et Reconnaissance des Formes’, ed. INRIA, p. 848.Google Scholar
Coupinot, G., Hecquet, J., Aurière, M. and Futually, R., 1992. Astron. Astrophys., 259, 701.Google Scholar
Grossmann, A. and Morlet, J., 1985. ‘Mathematics and Physics, Lecture on recent results’, World Scientific Publ.
Google Scholar
Holdschneider, M., Kronland-Martinet, R., Morlet, J. and Tchamitchian, P., 1989. In ‘Wavelets’, ed. Combes, J.M. et al., Springer
Berlin, p. 286.CrossRefGoogle Scholar
Le Fèvre, O., Bijaoui, A., Mathez, G., Picat, J.P. and Lelièvre, G., 1986. Astron. Astrophys., 154, 92.Google Scholar
Slezak, E., Mars, G., Bijaoui, A., Balkowski, C. and Fontanelli, P., 1988b. Astron. Astrophys. Supp. Ser., 74, 83.Google Scholar
Stark, J.L. and Bijaoui, A., 1993. ‘Progress in Wavelet Analysis and Applications’, eds. Meyer, Y. and Roques, S., Editions Frontières Gif/Yvette, p. 447.Google Scholar
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