File:Deep Field in Canes Venatici- Chandra Resolves Cosmic X-Ray Glow and Finds Mysterious New Sources (2000-bg - bg xray).tiff
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![File:Deep Field in Canes Venatici- Chandra Resolves Cosmic X-Ray Glow and Finds Mysterious New Sources (2000-bg - bg xray).tiff](https://upload.wikimedia.org/wikipedia/commons/thumb/0/0a/Deep_Field_in_Canes_Venatici-_Chandra_Resolves_Cosmic_X-Ray_Glow_and_Finds_Mysterious_New_Sources_%282000-bg_-_bg_xray%29.tiff/lossy-page1-603px-Deep_Field_in_Canes_Venatici-_Chandra_Resolves_Cosmic_X-Ray_Glow_and_Finds_Mysterious_New_Sources_%282000-bg_-_bg_xray%29.tiff.jpg?20240613184131)
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Captions
Chandra Image of Deep Field in Canes Venatici. This Chandra X-ray Observatory image of a 27.7 hour observation of a region in the direction of the constellation Canes Venatici, close to the Big Dipper, shows about 3 dozen X-ray sources.
Summary
[edit]DescriptionDeep Field in Canes Venatici- Chandra Resolves Cosmic X-Ray Glow and Finds Mysterious New Sources (2000-bg - bg xray).tiff |
English: Chandra Image of Deep Field in Canes Venatici. This Chandra X-ray Observatory image of a 27.7 hour observation of a region in the direction of the constellation Canes Venatici, close to the Big Dipper, shows about 3 dozen X-ray sources. Some of the sources were too faint to be seen by optical telescopes such as the Hubble Space Telescope and the Keck 10 meter telescope in Hawaii. This new class of sources may represent some of the most distant objects ever detected. If this sample of the sky is typical, tens of millions of such sources must exist. |
Date | 13 January 2000 (upload date) |
Source | Deep Field in Canes Venatici: Chandra Resolves Cosmic X-Ray Glow and Finds Mysterious New Sources |
Author | NASA/GSFC (Mushotzky et al.) |
Other versions |
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Category InfoField | Cosmology/Deep Fields/X-ray Background |
Color Code InfoField | Intensity |
Constellation InfoField | Canes Venatici |
Coordinates (J2000) InfoField | RA |
Observation Date(s) InfoField | December 3, 1999 |
Observation ID(s) InfoField | 325 |
Observation Time InfoField | 28 hours |
Scale InfoField | Image is 2.3 arcmin across. |
Instruments InfoField | ACIS |
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This media is a product of the Chandra X-ray Observatory Credit and attribution belongs to the Chandra X-ray Center, NASA/SAO/Penn State University/MIT |
Licensing
[edit]Public domainPublic domainfalsefalse |
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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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current | 18:41, 13 June 2024 | ![]() | 2,400 × 2,386 (143 KB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://chandra.si.edu/photo/2000/bg/bg_xray.tif via Commons:Spacemedia |
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File usage on Commons
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- File:Deep Field in Canes Venatici- Chandra Resolves Cosmic X-Ray Glow and Finds Mysterious New Sources (2000-bg).mpeg
- File:Deep Field in Canes Venatici- Chandra Resolves Cosmic X-Ray Glow and Finds Mysterious New Sources (2000-bg).pdf
- File:Deep Field in Canes Venatici- Chandra Resolves Cosmic X-Ray Glow and Finds Mysterious New Sources (2000-bg - bg xray).jpg
- File:Deep Field in Canes Venatici- Chandra Resolves Cosmic X-Ray Glow and Finds Mysterious New Sources (2000-bg - xray optical background).jpg
- File:Deep Field in Canes Venatici- Chandra Resolves Cosmic X-Ray Glow and Finds Mysterious New Sources (2000-bg - xray optical background).tiff
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Image title | This Chandra X-ray Observatory image of a 27.7 hour observation of a region in the direction of the constellation Canes Venatici, close to the Big Dipper, shows about 3 dozen X-ray sources. Some of the sources are optically too faint to be seen by telescopes such as the Hubble Space Telescope and the Keck 10 meter telescope in Hawaii and so are only known through this Chandra observation. This new class of sources may represent some of the most distant objects ever detected. If this sample of the sky is typical, tens of millions of such sources must exist. |
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Author | Chandra X-ray Observatory Center |
Copyright holder | http://chandra.harvard.edu/photo/image_use.html |
Width | 2,400 px |
Height | 2,386 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 | 36 |
Horizontal resolution | 300 dpi |
Vertical resolution | 300 dpi |
Data arrangement | chunky format |
Software used | Adobe Photoshop CS3 Windows |
File change date and time | 13:00, 6 December 2007 |
Color space | sRGB |