Processing of CCD images of star fields without the frame of a flat field by using new software in program shell of MIDAS/ROMAFOT

Results of CCD frames of star fields processing obtained by two ways, are analyzed. In the first case (a traditional method) the frame of flat field are used. In the second one the own large-scale flat field is obtained directly from the processable frames of image. That is we suggest to find the fr...

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Published in:Кинематика и физика небесных тел
Date:2005
Main Authors: Andruk, V.M., Vid'machenko, A.P., Ivashchenko, Yu.M.
Format: Article
Language:English
Published: Головна астрономічна обсерваторія НАН України 2005
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Online Access:https://nasplib.isofts.kiev.ua/handle/123456789/79719
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Journal Title:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Cite this:Processing of CCD images of star fields without the frame of a flat field by using new software in program shell of MIDAS/ROMAFOT / V.M. Andruk, A.P. Vid'machenko, Yu.M. Ivashchenko // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 544-550. — Бібліогр.: 2 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
id nasplib_isofts_kiev_ua-123456789-79719
record_format dspace
spelling Andruk, V.M.
Vid'machenko, A.P.
Ivashchenko, Yu.M.
2015-04-03T20:21:07Z
2015-04-03T20:21:07Z
2005
Processing of CCD images of star fields without the frame of a flat field by using new software in program shell of MIDAS/ROMAFOT / V.M. Andruk, A.P. Vid'machenko, Yu.M. Ivashchenko // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 544-550. — Бібліогр.: 2 назв. — англ.
0233-7665
https://nasplib.isofts.kiev.ua/handle/123456789/79719
Results of CCD frames of star fields processing obtained by two ways, are analyzed. In the first case (a traditional method) the frame of flat field are used. In the second one the own large-scale flat field is obtained directly from the processable frames of image. That is we suggest to find the frame of a flat field individually for each frame of the image. Photometric researches of regular errors are carried out for a wide interval of exposures (up to 100 times) for the same celestial objects in zones of overplanning of displaced frames (up to half of the frames size). Comparison of an instrumental photometric scale with a scale of photometric standards shows the absence of photometric field errors and brightness errors. Software procedure of cyclic processing of any quantity of CCD frames of star fields is realized in program shell of MIDAS/ROMAFOT.
Work is executed at partial financial support of the Scientific and Technological Center in Ukraine (grant NN43) and of the National Space Agency of Ukraine (contract “Astro”).
en
Головна астрономічна обсерваторія НАН України
Кинематика и физика небесных тел
MS6: New Trends, Research Directions, and Perspective Programs in the Field of Astronomy and Astrophysics
Processing of CCD images of star fields without the frame of a flat field by using new software in program shell of MIDAS/ROMAFOT
Article
published earlier
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
title Processing of CCD images of star fields without the frame of a flat field by using new software in program shell of MIDAS/ROMAFOT
spellingShingle Processing of CCD images of star fields without the frame of a flat field by using new software in program shell of MIDAS/ROMAFOT
Andruk, V.M.
Vid'machenko, A.P.
Ivashchenko, Yu.M.
MS6: New Trends, Research Directions, and Perspective Programs in the Field of Astronomy and Astrophysics
title_short Processing of CCD images of star fields without the frame of a flat field by using new software in program shell of MIDAS/ROMAFOT
title_full Processing of CCD images of star fields without the frame of a flat field by using new software in program shell of MIDAS/ROMAFOT
title_fullStr Processing of CCD images of star fields without the frame of a flat field by using new software in program shell of MIDAS/ROMAFOT
title_full_unstemmed Processing of CCD images of star fields without the frame of a flat field by using new software in program shell of MIDAS/ROMAFOT
title_sort processing of ccd images of star fields without the frame of a flat field by using new software in program shell of midas/romafot
author Andruk, V.M.
Vid'machenko, A.P.
Ivashchenko, Yu.M.
author_facet Andruk, V.M.
Vid'machenko, A.P.
Ivashchenko, Yu.M.
topic MS6: New Trends, Research Directions, and Perspective Programs in the Field of Astronomy and Astrophysics
topic_facet MS6: New Trends, Research Directions, and Perspective Programs in the Field of Astronomy and Astrophysics
publishDate 2005
language English
container_title Кинематика и физика небесных тел
publisher Головна астрономічна обсерваторія НАН України
format Article
description Results of CCD frames of star fields processing obtained by two ways, are analyzed. In the first case (a traditional method) the frame of flat field are used. In the second one the own large-scale flat field is obtained directly from the processable frames of image. That is we suggest to find the frame of a flat field individually for each frame of the image. Photometric researches of regular errors are carried out for a wide interval of exposures (up to 100 times) for the same celestial objects in zones of overplanning of displaced frames (up to half of the frames size). Comparison of an instrumental photometric scale with a scale of photometric standards shows the absence of photometric field errors and brightness errors. Software procedure of cyclic processing of any quantity of CCD frames of star fields is realized in program shell of MIDAS/ROMAFOT.
issn 0233-7665
url https://nasplib.isofts.kiev.ua/handle/123456789/79719
citation_txt Processing of CCD images of star fields without the frame of a flat field by using new software in program shell of MIDAS/ROMAFOT / V.M. Andruk, A.P. Vid'machenko, Yu.M. Ivashchenko // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 544-550. — Бібліогр.: 2 назв. — англ.
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