File:Image of SBS 0335-052 (geminiann02009b).jpg
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Image_of_SBS_0335-052_(geminiann02009b).jpg (506 × 270 pixels, file size: 21 KB, MIME type: image/jpeg)
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Summary
[edit]DescriptionImage of SBS 0335-052 (geminiann02009b).jpg |
English: On the left is an image of SBS 0335-052 in the I band taken by HST in the optical domain. On the right is an image of the same galaxy obtained with OSCIR on the Gemini North Telescope in the mid-infrared (10.8 micron). All the mid-infrared flux comes from a dust embedded super stellar cluster that cannot be detected at optical wavelengths. |
Date | 9 October 2002 (upload date) |
Source | Image of SBS 0335-052 |
Author | International Gemini Observatory/NOIRLab/NSF/AURA |
Other versions |
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Licensing
[edit]This media was created by the National Optical-Infrared Astronomy Research Laboratory (NOIRLab).
Their website states: "Unless specifically noted, the images, videos, and music distributed on the public NOIRLab website, along with the texts of press releases, announcements, images of the week 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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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 21:35, 27 October 2023 | 506 × 270 (21 KB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/large/geminiann02009b.jpg via Commons:Spacemedia |
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Metadata
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Image title |
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Credit/Provider | International Gemini Observatory/NOIRLab/NSF/AURA |
Source | NSF's NOIRLab |
Short title |
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Usage terms |
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Date and time of data generation | 05:00, 9 October 2002 |
JPEG file comment | On the left is an image of SBS 0335-052 in the I band taken by HST in the optical domain. On the right is an image of the same galaxy obtained with OSCIR on the Gemini North Telescope in the mid-infrared (10.8 micron). All the mid-infrared flux comes from a dust embedded super stellar cluster that cannot be detected at optical wavelengths. |
Software used | GIMP 2.10.18 |
Unique ID of original document | xmp.did:e5145f01-133b-43ff-9235-028307bd1d27 |
Keywords | SBS 0335-052 |
Contact information |
950 North Cherry Ave. Tucson, AZ, 85719 USA |
IIM version | 4 |