Konferans bildirisi Açık Erişim
Yilmaz, Ozgur; Selimoglu, Ozgur; Turk, Fethi
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<identifier identifierType="URL">https://aperta.ulakbim.gov.tr/record/91471</identifier>
<creators>
<creator>
<creatorName>Yilmaz, Ozgur</creatorName>
<givenName>Ozgur</givenName>
<familyName>Yilmaz</familyName>
<affiliation>Middle E Tech Univ, Tubitak Uzay Space Technol Res Inst, TR-06531 Ankara, Turkey</affiliation>
</creator>
<creator>
<creatorName>Selimoglu, Ozgur</creatorName>
<givenName>Ozgur</givenName>
<familyName>Selimoglu</familyName>
<affiliation>Middle E Tech Univ, Tubitak Uzay Space Technol Res Inst, TR-06531 Ankara, Turkey</affiliation>
</creator>
<creator>
<creatorName>Turk, Fethi</creatorName>
<givenName>Fethi</givenName>
<familyName>Turk</familyName>
<affiliation>Middle E Tech Univ, Tubitak Uzay Space Technol Res Inst, TR-06531 Ankara, Turkey</affiliation>
</creator>
</creators>
<titles>
<title>Development Of A Medium Size Swir Imaging Telescope: Integration, Calibration And Mtf Measurement</title>
</titles>
<publisher>Aperta</publisher>
<publicationYear>2013</publicationYear>
<dates>
<date dateType="Issued">2013-01-01</date>
</dates>
<resourceType resourceTypeGeneral="Text">Conference paper</resourceType>
<alternateIdentifiers>
<alternateIdentifier alternateIdentifierType="url">https://aperta.ulakbim.gov.tr/record/91471</alternateIdentifier>
</alternateIdentifiers>
<relatedIdentifiers>
<relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.1117/12.2024506</relatedIdentifier>
</relatedIdentifiers>
<rightsList>
<rights rightsURI="http://www.opendefinition.org/licenses/cc-by">Creative Commons Attribution</rights>
<rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
</rightsList>
<descriptions>
<description descriptionType="Abstract">Development of an imaging telescope having a large mirror generally requires a sound infrastructure including expensive devices such as collimators and interferometers. In this paper we investigate the development and characterization of a medium size telescope (140 mm aperture) using simple techniques. Alignment was done with a mechanical measurement device. Detector was placed using an image of a ruled outside building. Radiometric calibration was done with open-sky images. And finally MTF was measured using stellar images. We found that MTF of our telescope is greater than %15 all along the detector at 20 lp/mm, which is the Nyquist frequency of 25 mu m pixel size. This shows that alignment and focus adjustments work well enough in the telescope. These simple techniques can be used for the development and characterization of a medium-size and medium-resolution imaging telescopes.</description>
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