File:Collage of Hubble and Spitzer Images of Galaxy Cluster MS1054.jpg
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DescriptionCollage of Hubble and Spitzer Images of Galaxy Cluster MS1054.jpg |
English: A Hubble Space Telescope snapshot of galaxy cluster MS1054 is featured in the center of this image, with individual galaxies spotted by the Spitzer Space Telescope are highlighted along the side in call-out images. Wisps of blue show infrared emission from star formation. |
Date | |
Source | http://www.spitzer.caltech.edu/images/2076-sig08-009-Collage-of-Hubble-and-Spitzer-Images-of-Galaxy-Cluster-MS1054 |
Author | J.Blakeslee (Washington State University); NASA/JPL-Caltech/A. Saintonge (University of Zurich) |
Image use policy: http://www.spitzer.caltech.edu/info/18-Image-Use-Policy
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Public domainPublic domainfalsefalse |
This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.) | ||
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 22:39, 13 June 2011 | 1,100 × 1,100 (933 KB) | Spitzersteph (talk | contribs) |
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Image title | A Hubble Space Telescope snapshot of galaxy cluster MS1054 is featured in the center of this image, with individual galaxies spotted by the Spitzer Space Telescope are highlighted along the side in call-out images. Wisps of blue show infrared emission from star formation. |
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Copyright holder | http://www.spitzer.caltech.edu/Media/mediaimages/copyright.shtml |
Width | 1,100 px |
Height | 1,100 px |
Compression scheme | LZW |
Pixel composition | RGB |
Orientation | Normal |
Number of components | 3 |
Horizontal resolution | 72 dpi |
Vertical resolution | 72 dpi |
Data arrangement | chunky format |
Software used | Adobe Photoshop CS3 Macintosh |
File change date and time | 14:37, 5 June 2009 |
Color space | Uncalibrated |
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6 August 2008
image/jpeg
b396889d876fd9ee481852f9544c5d1bbbc6b111
954,936 byte
1,100 pixel
1,100 pixel
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