Fayl:Phot-22-06.jpg
Bu prevyuning hajmi: 406 × 599 piksel. Boshqa oʻlchamlari: 163 × 240 piksel | 325 × 480 piksel | 521 × 768 piksel | 1 085 × 1 600 piksel.
Asl fayl (1 085 × 1 600 piksel, fayl hajmi: 174 KB, MIME tipi: image/jpeg)
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| Taʼrif |
English: Composite image based on data acquired with the FORS1 multi-mode instrument in April and May 2006 for the European Supernova Collaboration. The observations were made in four different filters (B, V, R, and I) that were combined to make a colour image. The field of view covers 5.6 x 8.3 arcmin. North is up and East is to the left. The observations were done by Ferdinando Patat and the Paranal Science team (ESO), and the final processing was done by Olivia Blanchemain, Henri Boffin and Haennes Heyer (ESO).
ID: phot-22-06 Press Release: ESO 22/06 Long Caption Object: NGC 5917 Telescope: UT2/Kueyen Instrument: FORS1 Credit: ESO |
| Sanasi | April and May 2006 |
| Manba | http://www.eso.org/gallery/v/ESOPIA/Galaxies/phot-22-06.tif.html |
| Muallif | ESO: observations by Ferdinando Patat and the Paranal Science team (ESO), final processing by Olivia Blanchemain, Henri Boffin and Haennes Heyer (ESO). |
| Other versions | http://www.eso.org/gallery/d/3078-3/phot-22-06.tif 1347x1986 7864 kB TIFF |
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This media was created by the European Southern Observatory (ESO).
Their website states: "Unless specifically noted, the images, videos, and music distributed on the public ESO website, along with the texts of press releases, announcements, pictures of the week, blog posts and captions, are licensed under a Creative Commons Attribution 4.0 International License, and may on a non-exclusive basis be reproduced without fee provided the credit is clear and visible." To the uploader: You must provide a link (URL) to the original file and the authorship information if available. |
  This file is licensed under the Creative Commons Attribution 4.0 International license.
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| joriy | 20:27, 2009-yil 28-aprel | | 1 085 × 1 600 (174 KB) | Fabian RRRR | {{Information |Description={{en|1=Composite image based on data acquired with the FORS1 multi-mode instrument in April and May 2006 for the European Supernova Collaboration. The observations were made in four different filters (B, V, R, and I) that were c |
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