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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| Дата: | 2005 |
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| Автори: | , , |
| Формат: | Стаття |
| Мова: | English |
| Опубліковано: |
Головна астрономічна обсерваторія НАН України
2005
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| Назва видання: | Кинематика и физика небесных тел |
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| Онлайн доступ: | http://dspace.nbuv.gov.ua/handle/123456789/79719 |
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| Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Цитувати: | 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. |
Репозитарії
Digital Library of Periodicals of National Academy of Sciences of Ukraine| id |
irk-123456789-79719 |
|---|---|
| record_format |
dspace |
| spelling |
irk-123456789-797192015-04-04T03:02:10Z 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 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. 2005 Article 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 http://dspace.nbuv.gov.ua/handle/123456789/79719 en Кинематика и физика небесных тел Головна астрономічна обсерваторія НАН України |
| institution |
Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| collection |
DSpace DC |
| language |
English |
| topic |
MS6: New Trends, Research Directions, and Perspective Programs in the Field of Astronomy and Astrophysics MS6: New Trends, Research Directions, and Perspective Programs in the Field of Astronomy and Astrophysics |
| spellingShingle |
MS6: New Trends, Research Directions, and Perspective Programs in the Field of Astronomy and Astrophysics MS6: New Trends, Research Directions, and Perspective Programs in the Field of Astronomy and Astrophysics Andruk, V.M. Vid'machenko, A.P. Ivashchenko, Yu.M. Processing of CCD images of star fields without the frame of a flat field by using new software in program shell of MIDAS/ROMAFOT Кинематика и физика небесных тел |
| 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. |
| format |
Article |
| author |
Andruk, V.M. Vid'machenko, A.P. Ivashchenko, Yu.M. |
| author_facet |
Andruk, V.M. Vid'machenko, A.P. Ivashchenko, Yu.M. |
| author_sort |
Andruk, V.M. |
| 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 |
| 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 |
| publisher |
Головна астрономічна обсерваторія НАН України |
| publishDate |
2005 |
| topic_facet |
MS6: New Trends, Research Directions, and Perspective Programs in the Field of Astronomy and Astrophysics |
| url |
http://dspace.nbuv.gov.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. |
| series |
Кинематика и физика небесных тел |
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