{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2026,3,5]],"date-time":"2026-03-05T22:27:17Z","timestamp":1772749637187,"version":"3.50.1"},"reference-count":17,"publisher":"MDPI AG","issue":"3","license":[{"start":{"date-parts":[[2010,3,3]],"date-time":"2010-03-03T00:00:00Z","timestamp":1267574400000},"content-version":"vor","delay-in-days":0,"URL":"https:\/\/creativecommons.org\/licenses\/by\/3.0\/"}],"content-domain":{"domain":[],"crossmark-restriction":false},"short-container-title":["Sensors"],"abstract":"<jats:p>In this paper we show how the techniques of image deconvolution can increase the ability of image sensors as, for example, CCD imagers, to detect faint stars or faint orbital objects (small satellites and space debris). In the case of faint stars, we show that this benefit is equivalent to double the quantum efficiency of the used image sensor or to increase the effective telescope aperture by more than 30% without decreasing the astrometric precision or introducing artificial bias. In the case of orbital objects, the deconvolution technique can double the signal-to-noise ratio of the image, which helps to discover and control dangerous objects as space debris or lost satellites. The benefits obtained using CCD detectors can be extrapolated to any kind of image sensors.<\/jats:p>","DOI":"10.3390\/s100301743","type":"journal-article","created":{"date-parts":[[2010,3,3]],"date-time":"2010-03-03T11:01:12Z","timestamp":1267614072000},"page":"1743-1752","update-policy":"https:\/\/doi.org\/10.3390\/mdpi_crossmark_policy","source":"Crossref","is-referenced-by-count":12,"title":["Improving the Ability of Image Sensors to Detect Faint Stars and Moving Objects Using Image Deconvolution Techniques"],"prefix":"10.3390","volume":"10","author":[{"given":"Octavi","family":"Fors","sequence":"first","affiliation":[{"name":"Departament d'Astronomia i Meteorologia and Institut de Ci\u00e8ncies del Cosmos (ICC), Universitat de Barcelona (UB\/IEEC), Av. Diagonal 647, 08028 Barcelona, Spain"},{"name":"Observatori Fabra, Barcelona, Spain"}]},{"given":"Jorge","family":"N\u00fa\u00f1ez","sequence":"additional","affiliation":[{"name":"Departament d'Astronomia i Meteorologia and Institut de Ci\u00e8ncies del Cosmos (ICC), Universitat de Barcelona (UB\/IEEC), Av. Diagonal 647, 08028 Barcelona, Spain"},{"name":"Observatori Fabra, Barcelona, Spain"}]},{"given":"Xavier","family":"Otazu","sequence":"additional","affiliation":[{"name":"Computer Vision Center, Computer Science Department, Universitat Aut\u00f2noma de Barcelona, Campus UAB, Cerdanyola del Vall\u00e8s, 08193 Barcelona, Spain"}]},{"given":"Albert","family":"Prades","sequence":"additional","affiliation":[{"name":"Departament d\u2019Enginyeria del Terreny, Cartogr\u00e0fica i Geof\u00edsica, Universitat Polit\u00e8cnica de Catalunya, Barcelona, Spain"}]},{"given":"Robert  D.","family":"Cardinal","sequence":"additional","affiliation":[{"name":"NEOSSat Mission, Department of Geoscience, University of Calgary, Calgary, Canada"}]}],"member":"1968","published-online":{"date-parts":[[2010,3,3]]},"reference":[{"key":"ref_1","unstructured":"White, R.L., and Allen, R.J. (1990). The Restoration of HST Images and Spectra, STScI."},{"key":"ref_2","unstructured":"Hanisch, R.J., and White, R.L. 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