Using THELI pipeline in order to reduce Abell 226 multi-band optical images
In this paper we review THELI (Erben & Schrimer, 2005), an image processing pipeline developed to reduce multipointing optical images taken by mosaic CCD cameras. This pipeline works on raw images by removing several instrumental contaminations, implementing photometric calibration and astro...
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| Published in: | Advances in Astronomy and Space Physics |
|---|---|
| Date: | 2013 |
| Main Authors: | , , , |
| Format: | Article |
| Language: | English |
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Головна астрономічна обсерваторія НАН України
2013
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| Online Access: | https://nasplib.isofts.kiev.ua/handle/123456789/119424 |
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| Journal Title: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Cite this: | Using THELI pipeline in order to reduce Abell 226 multi-band optical images / R. Joveini, S. Sotoudeh, A. Roozrokh, M. Taheri // Advances in Astronomy and Space Physics. — 2013. — Т. 3., вип. 1. — С. 38-41. — Бібліогр.: 7 назв. — англ. |
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Digital Library of Periodicals of National Academy of Sciences of Ukraine| _version_ | 1862641856554205184 |
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| author | Joveini, R. Sotoudeh, S. Roozrokh, A. Taheri, M. |
| author_facet | Joveini, R. Sotoudeh, S. Roozrokh, A. Taheri, M. |
| citation_txt | Using THELI pipeline in order to reduce Abell 226 multi-band optical images / R. Joveini, S. Sotoudeh, A. Roozrokh, M. Taheri // Advances in Astronomy and Space Physics. — 2013. — Т. 3., вип. 1. — С. 38-41. — Бібліогр.: 7 назв. — англ. |
| collection | DSpace DC |
| container_title | Advances in Astronomy and Space Physics |
| description | In this paper we review THELI (Erben & Schrimer, 2005), an image processing pipeline developed to reduce multipointing optical images taken by mosaic CCD cameras. This pipeline works on raw images by removing several instrumental contaminations, implementing photometric calibration and astrometric alignment, and constructing a
deep co-added mosaic image complemented by a weight map. We demonstrate the procedure of reducing NGC 3923 images from raw data to the final results. We also demonstrate the quality of our data reduction strategy using mag-count and mag-error in mag plots. Emphasis is mainly placed on photometric calibration which is of great interest to us due to our scientific case. Based on the cross-association of the extracted catalogue against a reference catalogue of stellar magnitudes, zero-point calibration is performed. Our data reduction strategy and the method employed for cross-correlating large catalogues is also presented.
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| first_indexed | 2025-12-01T05:10:42Z |
| format | Article |
| fulltext | |
| id | nasplib_isofts_kiev_ua-123456789-119424 |
| institution | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| issn | 2227-1481 |
| language | English |
| last_indexed | 2025-12-01T05:10:42Z |
| publishDate | 2013 |
| publisher | Головна астрономічна обсерваторія НАН України |
| record_format | dspace |
| spelling | Joveini, R. Sotoudeh, S. Roozrokh, A. Taheri, M. 2017-06-06T19:08:18Z 2017-06-06T19:08:18Z 2013 Using THELI pipeline in order to reduce Abell 226 multi-band optical images / R. Joveini, S. Sotoudeh, A. Roozrokh, M. Taheri // Advances in Astronomy and Space Physics. — 2013. — Т. 3., вип. 1. — С. 38-41. — Бібліогр.: 7 назв. — англ. 2227-1481 https://nasplib.isofts.kiev.ua/handle/123456789/119424 In this paper we review THELI (Erben & Schrimer, 2005), an image processing pipeline developed to reduce multipointing optical images taken by mosaic CCD cameras. This pipeline works on raw images by removing several instrumental contaminations, implementing photometric calibration and astrometric alignment, and constructing a
 deep co-added mosaic image complemented by a weight map. We demonstrate the procedure of reducing NGC 3923 images from raw data to the final results. We also demonstrate the quality of our data reduction strategy using mag-count and mag-error in mag plots. Emphasis is mainly placed on photometric calibration which is of great interest to us due to our scientific case. Based on the cross-association of the extracted catalogue against a reference catalogue of stellar magnitudes, zero-point calibration is performed. Our data reduction strategy and the method employed for cross-correlating large catalogues is also presented. The authors acknowledge IPM for providing computational facilities and also appreciate Reza Mansouri, Habib G. Khosroshahi and Alireza Molaeinezhad for useful discussions and guidance. en Головна астрономічна обсерваторія НАН України Advances in Astronomy and Space Physics Using THELI pipeline in order to reduce Abell 226 multi-band optical images Article published earlier |
| spellingShingle | Using THELI pipeline in order to reduce Abell 226 multi-band optical images Joveini, R. Sotoudeh, S. Roozrokh, A. Taheri, M. |
| title | Using THELI pipeline in order to reduce Abell 226 multi-band optical images |
| title_full | Using THELI pipeline in order to reduce Abell 226 multi-band optical images |
| title_fullStr | Using THELI pipeline in order to reduce Abell 226 multi-band optical images |
| title_full_unstemmed | Using THELI pipeline in order to reduce Abell 226 multi-band optical images |
| title_short | Using THELI pipeline in order to reduce Abell 226 multi-band optical images |
| title_sort | using theli pipeline in order to reduce abell 226 multi-band optical images |
| url | https://nasplib.isofts.kiev.ua/handle/123456789/119424 |
| work_keys_str_mv | AT joveinir usingthelipipelineinordertoreduceabell226multibandopticalimages AT sotoudehs usingthelipipelineinordertoreduceabell226multibandopticalimages AT roozrokha usingthelipipelineinordertoreduceabell226multibandopticalimages AT taherim usingthelipipelineinordertoreduceabell226multibandopticalimages |