File:GCLASS clusters (geminiann12001a).jpg
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GCLASS_clusters_(geminiann12001a).jpg (500 × 272 pixels, file size: 68 KB, MIME type: image/jpeg)
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[edit]DescriptionGCLASS clusters (geminiann12001a).jpg |
English: Left panel: The fraction of star-forming galaxies as a function of galaxy stellar mass for galaxies in different environments. Right panel: The fraction of star forming-galaxies as a function of environment for galaxies with different stellar masses. Both stellar mass and environment determine the likelihood of finding star-forming galaxies. |
Date | 25 January 2012, 21:34:00 (upload date) |
Source | GCLASS clusters |
Author | International Gemini Observatory/NOIRLab/NSF/AURA |
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[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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current | 18:43, 23 October 2023 | 500 × 272 (68 KB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/large/geminiann12001a.jpg via Commons:Spacemedia |
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Credit/Provider | International Gemini Observatory/NOIRLab/NSF/AURA |
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Short title |
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Image title |
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Date and time of data generation | 21:34, 25 January 2012 |
JPEG file comment | Left panel: The fraction of star-forming galaxies as a function of galaxy stellar mass for galaxies in different environments. Right panel: The fraction of star forming-galaxies as a function of environment for galaxies with different stellar masses. Both stellar mass and environment determine the likelihood of finding star-forming galaxies. |
Software used | Adobe Photoshop 21.2 (Windows) |
Date and time of digitizing | 09:45, 26 January 2012 |
File change date and time | 16:09, 31 July 2020 |
Date metadata was last modified | 16:09, 31 July 2020 |
Unique ID of original document | xmp.did:4A460FB70820681197A58242A1E93DA1 |
Keywords | Gemini Multi-Object Spectrograph (GMOS) |
Contact information |
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