Centroid position measurements and subpixel sensitivity variations with the MAMA detector
Initial measurements of the position sensitivity of a visible-light multianode microchannel array detector show that centroid calculations for image spots are accurate to better than 0.04 pixels even with sources that are essentially delta functions at the photocathode.Subpixel sensitivity variation...
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Veröffentlicht in: | Applied Optics 1989-03, Vol.28 (6), p.1178-1192 |
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creator | Morgan, Jeffrey S. Slater, D. C. Timothy, John G. Jenkins, E. B. |
description | Initial measurements of the position sensitivity of a visible-light multianode microchannel array detector show that centroid calculations for image spots are accurate to better than 0.04 pixels even with sources that are essentially delta functions at the photocathode.Subpixel sensitivity variations of 10-15 percent are typically found for pixels in the array. Variations as large as 30 percent are possible in the worst conditions. These variations limit the photometric accuracy of the detector when very small scale features are observed. The photometric accuracy and the position sensitivity of the detector appear to be limited by cross-coupling effects within the anode array. Initial measurements with more recent designs of the detector show that most or all of this cross-coupling has been eliminated. |
doi_str_mv | 10.1364/AO.28.001178 |
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C.</creatorcontrib><creatorcontrib>Timothy, John G.</creatorcontrib><creatorcontrib>Jenkins, E. B.</creatorcontrib><title>Centroid position measurements and subpixel sensitivity variations with the MAMA detector</title><title>Applied Optics</title><addtitle>Appl Opt</addtitle><description>Initial measurements of the position sensitivity of a visible-light multianode microchannel array detector show that centroid calculations for image spots are accurate to better than 0.04 pixels even with sources that are essentially delta functions at the photocathode.Subpixel sensitivity variations of 10-15 percent are typically found for pixels in the array. Variations as large as 30 percent are possible in the worst conditions. These variations limit the photometric accuracy of the detector when very small scale features are observed. The photometric accuracy and the position sensitivity of the detector appear to be limited by cross-coupling effects within the anode array. Initial measurements with more recent designs of the detector show that most or all of this cross-coupling has been eliminated.</description><subject>Electronics And Electrical Engineering</subject><issn>0003-6935</issn><issn>1559-128X</issn><issn>1539-4522</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1989</creationdate><recordtype>article</recordtype><sourceid>CYI</sourceid><recordid>eNo90D1v2zAQBmCiaNC4SbeORcEtS-WSPFIiR8FI2gIJvDRDJoKijggLS3JIKh__PjKc9JYb7sGLw0vIV87WHGr5s92uhV4zxnmjP5AVV2AqqYT4SFaMMahqA-qUfM7532KErs0nciqYkroGvSJ3GxxLmmJP91OOJU4jHdDlOeGwHDJ1Y0_z3O3jM-5oxvFgHmN5oY8uRXfwmT7Fck_LPdKb9qalPRb0ZUrn5CS4XcYvb_uM3F5d_t38rq63v_5s2uvKSy5L5YLvODaNVwaYD8Ca4DpUQqpaeaeC6vsOfDBSB2yE4DUocMv7wUkNMgCckYtj7j5NDzPmYoeYPe52bsRpzraBZTRwscgfR-nTlHPCYPcpDi69WM7soUvbbq3Q9tjlwr-_Bc_dgP1__F7eAr4dweiys0uN2XKjDWPSABh4BRBgeJs</recordid><startdate>19890315</startdate><enddate>19890315</enddate><creator>Morgan, Jeffrey S.</creator><creator>Slater, D. 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C.</creatorcontrib><creatorcontrib>Timothy, John G.</creatorcontrib><creatorcontrib>Jenkins, E. B.</creatorcontrib><collection>NASA Scientific and Technical Information</collection><collection>NASA Technical Reports Server</collection><collection>PubMed</collection><collection>CrossRef</collection><collection>MEDLINE - Academic</collection><jtitle>Applied Optics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Morgan, Jeffrey S.</au><au>Slater, D. C.</au><au>Timothy, John G.</au><au>Jenkins, E. B.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Centroid position measurements and subpixel sensitivity variations with the MAMA detector</atitle><jtitle>Applied Optics</jtitle><addtitle>Appl Opt</addtitle><date>1989-03-15</date><risdate>1989</risdate><volume>28</volume><issue>6</issue><spage>1178</spage><epage>1192</epage><pages>1178-1192</pages><issn>0003-6935</issn><issn>1559-128X</issn><eissn>1539-4522</eissn><abstract>Initial measurements of the position sensitivity of a visible-light multianode microchannel array detector show that centroid calculations for image spots are accurate to better than 0.04 pixels even with sources that are essentially delta functions at the photocathode.Subpixel sensitivity variations of 10-15 percent are typically found for pixels in the array. Variations as large as 30 percent are possible in the worst conditions. These variations limit the photometric accuracy of the detector when very small scale features are observed. The photometric accuracy and the position sensitivity of the detector appear to be limited by cross-coupling effects within the anode array. Initial measurements with more recent designs of the detector show that most or all of this cross-coupling has been eliminated.</abstract><cop>Legacy CDMS</cop><pmid>20548638</pmid><doi>10.1364/AO.28.001178</doi><tpages>15</tpages></addata></record> |
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source | NASA Technical Reports Server; Alma/SFX Local Collection; Optica Publishing Group Journals |
subjects | Electronics And Electrical Engineering |
title | Centroid position measurements and subpixel sensitivity variations with the MAMA detector |
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