File:Arbitrarily scaled copies of the NIFS spectrum (geminiann08015b).tiff
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Arbitrarily_scaled_copies_of_the_NIFS_spectrum_(geminiann08015b).tiff (500 × 500 pixels, file size: 468 KB, MIME type: image/tiff)
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Arbitrarily scaled copies of the NIFS spectrum of the host galaxy of PG 1426+015 (black lines) with model fits (red lines) overlaid.
Summary
[edit]DescriptionArbitrarily scaled copies of the NIFS spectrum (geminiann08015b).tiff |
English: Arbitrarily scaled copies of the NIFS spectrum of the host galaxy of PG 1426+015 (black lines) with model fits (red lines) overlaid. The models of a M5 Ia supergiant (top spectrum) and a K5 III giant (bottom spectrum) have been broadened to match the width of the host-galaxy absorption features. The better fit with the supergiant spectrum is indicative of a young stellar population in the host galaxy. |
Date | 1 July 2008, 16:07:00 (upload date) |
Source | Arbitrarily scaled copies of the NIFS spectrum |
Author | International Gemini Observatory/NOIRLab/NSF/AURA |
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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. |
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 22:41, 23 October 2023 | ![]() | 500 × 500 (468 KB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/original/geminiann08015b.tif via Commons:Spacemedia |
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Image title | Arbitrarily scaled copies of the NIFS spectrum of the host galaxy of PG 1426+015 (black lines) with model fits (red lines) overlaid. The models of a M5 Ia supergiant (top spectrum) and a K5 III giant (bottom spectrum) have been broadened to match the width of the host-galaxy absorption features. The better fit with the supergiant spectrum is indicative of a young stellar population in the host galaxy. |
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Width | 500 px |
Height | 500 px |
Bits per component |
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Compression scheme | LZW |
Pixel composition | RGB |
Orientation | Normal |
Number of components | 3 |
Number of rows per strip | 128 |
Horizontal resolution | 150 dpi |
Vertical resolution | 150 dpi |
Data arrangement | chunky format |
Software used | GIMP 2.10.18 |
File change date and time | 13:58, 10 August 2020 |
Color space | sRGB |