cxprep/chandra.txt: complete registration
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@image
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url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-617L{1}X{2}Y{3}.png
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copyright: Public domain
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license_id: CC-PDDC
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-617.jpg
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astropix_ids: chandra|617
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credits> X-ray: NASA/CXC/University of Missouri-Kansas City/M.Brodwin et al; Optical: NASA/STScI; Infrared: JPL/CalTech
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---
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@scene
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place_uuid: d6341502-3902-4cd4-a280-42346d8226d0
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image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-617L{1}X{2}Y{3}.png
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outgoing_url: https://chandra.harvard.edu/photo/2016/idcs1426/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-617.jpg
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text> This multi-wavelength image shows the galaxy cluster called IDCS
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J1426.5+3508 (IDCS J1426 for short) in X-rays from the Chandra X-ray Observatory
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in blue, visible light from the Hubble Space Telescope in green, and infrared
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light from the Spitzer Space Telescope in red. This rare galaxy cluster, which
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is located 10 billion light years from Earth, weighs almost 500 trillion Suns.
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---
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@image
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url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-620L{1}X{2}Y{3}.png
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copyright: Public domain
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license_id: CC-PDDC
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-620.jpg
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astropix_ids: chandra|620
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credits> X-ray: NASA/CXC/Univ of Hertfordshire/M.Hardcastle et al., Radio: CSIRO/ATNF/ATCA
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---
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@scene
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place_uuid: c382d1ba-87c8-4a6d-a277-6f37235712fc
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image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-620L{1}X{2}Y{3}.png
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outgoing_url: https://chandra.harvard.edu/photo/2016/pictora/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-620.jpg
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text> The Star Wars franchise has featured the fictitious "Death Star," which
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can shoot powerful beams of radiation across space. The Universe, however,
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produces phenomena that often surpass what science fiction can conjure. The
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Pictor A galaxy is one such impressive object. This galaxy, located nearly 500
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million light years from Earth, contains a supermassive black hole at its
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center. A huge amount of gravitational energy is released as material swirls
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towards the event horizon, the point of no return for infalling material. This
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energy produces an enormous beam, or jet, of particles traveling at nearly the
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speed of light into intergalactic space.
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---
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@image
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url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-621L{1}X{2}Y{3}.png
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copyright: Public domain
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license_id: CC-PDDC
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-621.jpg
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astropix_ids: chandra|621
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credits> X-ray: NASA/CXC/ISAS/A.Simionescu et al, Optical: DSS
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---
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@scene
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place_uuid: 6cd4c6bd-08fe-4a86-98bc-ca776e5f1e57
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image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-621L{1}X{2}Y{3}.png
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outgoing_url: https://chandra.harvard.edu/photo/2016/b30727/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-621.jpg
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text> A jet from a very distant black hole being illuminated by the leftover
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glow from the Big Bang, known as the cosmic microwave background (CMB), has been
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found. Astronomers using NASA's Chandra X-ray Observatory discovered this
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faraway jet serendipitously when looking at another source in Chandra's field of
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view. Jets in the early Universe such as this one, known as B3 0727+409, give
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astronomers a way to probe the growth of black holes at a very early epoch in
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the cosmos.
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---
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@image
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url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-622aL{1}X{2}Y{3}.png
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copyright: Public domain
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license_id: CC-PDDC
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-622a.jpg
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astropix_ids: chandra|622a
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credits> X-ray: NASA/CXC/SAO/G.Ogrean et al.; Optical: NASA/STScI; Radio: NRAO/AUI/NSF
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---
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@scene
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place_uuid: 37878806-a1ae-4442-bb3a-af1b1f96926d
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image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-622aL{1}X{2}Y{3}.png
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outgoing_url: https://chandra.harvard.edu/photo/2016/frontier/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-622a.jpg
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text> Galaxy clusters are enormous collections of hundreds or even thousands of
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galaxies and vast reservoirs of hot gas embedded in massive clouds of dark
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matter, invisible material that does not emit or absorb light but can be
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detected through its gravitational effects. Located about 4.3 billion light
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years from Earth, MACS J0416 is a pair of colliding galaxy clusters that will
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eventually combine to form an even bigger cluster.
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---
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@image
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url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-622bL{1}X{2}Y{3}.png
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copyright: Public domain
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license_id: CC-PDDC
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-622b.jpg
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astropix_ids: chandra|622b
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credits> X-ray: NASA/CXC/SAO/van Weeren et al.; Optical: NASA/STScI; Radio: NRAO/AUI/NSF
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---
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@scene
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place_uuid: 8f4450e7-3dd1-4ba9-b2b8-12c89de6d936
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image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-622bL{1}X{2}Y{3}.png
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outgoing_url: https://chandra.harvard.edu/photo/2016/frontier/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-622b.jpg
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text> Galaxy clusters are enormous collections of hundreds or even thousands of
|
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galaxies and vast reservoirs of hot gas embedded in massive clouds of dark
|
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matter, invisible material that does not emit or absorb light but can be
|
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detected through its gravitational effects. MACS J0717, one of the most complex
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and distorted galaxy clusters known, is the site of a collision between four
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clusters. It is located about 5.4 billion light years away from Earth.
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---
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@image
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url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-624L{1}X{2}Y{3}.png
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copyright: Public domain
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license_id: CC-PDDC
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-624.jpg
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astropix_ids: chandra|624
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credits> X-ray (NASA/CXC/CfA/S.Chakraborti et al.)
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---
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@scene
|
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place_uuid: 620fa34f-ae3b-4001-b57f-bf76a38cda99
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image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-624L{1}X{2}Y{3}.png
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outgoing_url: https://chandra.harvard.edu/photo/2016/g19/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-624.jpg
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text> Scientists have used data from NASA's Chandra X-ray Observatory and the
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NSF's Jansky Very Large Array to determine the likely trigger for the most
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recent supernova in the Milky Way. Astronomers had previously identified
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G1.9+0.3 as the remnant of the most recent supernova in our Galaxy. It is
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estimated to have occurred about 110 years ago from the vantage point of Earth,
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in a dusty region of the Galaxy that blocked visible light from reaching Earth.
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---
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@image
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url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-626aL{1}X{2}Y{3}.png
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copyright: Public domain
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license_id: CC-PDDC
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-626a.jpg
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astropix_ids: chandra|626a
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credits> X-ray: NASA/CXC/Univ. of Alabama/A. Morandi et al; Optical: SDSS, NASA/STScI
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---
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@scene
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place_uuid: 0a2104ea-0141-4b63-beb3-a28e06ceaefd
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image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-626aL{1}X{2}Y{3}.png
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outgoing_url: https://chandra.harvard.edu/photo/2016/clusters/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-626a.jpg
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text> This galaxy cluster, Abell 1835, was part of a large survey of over 300
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clusters used to investigate dark energy, the mysterious energy that is
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currently driving the accelerating expansion of the Universe.
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---
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@image
|
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url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-626bL{1}X{2}Y{3}.png
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||||
copyright: Public domain
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||||
license_id: CC-PDDC
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-626b.jpg
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astropix_ids: chandra|626b
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credits> X-ray: NASA/CXC/Univ. of Alabama/A. Morandi et al; Optical: SDSS, NASA/STScI
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---
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@scene
|
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place_uuid: a5367509-e96b-4f4b-a368-1e915a20dea5
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image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-626bL{1}X{2}Y{3}.png
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outgoing_url: https://chandra.harvard.edu/photo/2016/clusters/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-626b.jpg
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text> This galaxy cluster, MS 1455.0+2232, was part of a large survey of over 300
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clusters used to investigate dark energy, the mysterious energy that is
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currently driving the accelerating expansion of the Universe.
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---
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@image
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url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-626cL{1}X{2}Y{3}.png
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||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-626c.jpg
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astropix_ids: chandra|626c
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credits> X-ray: NASA/CXC/Univ. of Alabama/A. Morandi et al; Optical: SDSS, NASA/STScI
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---
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@scene
|
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place_uuid: 13f7a422-fa14-4ca2-86ff-0e27a33c9309
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||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-626cL{1}X{2}Y{3}.png
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outgoing_url: https://chandra.harvard.edu/photo/2016/clusters/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-626c.jpg
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text> This galaxy cluster, RXJ 1347.5-1145, was part of a large survey of over 300
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clusters used to investigate dark energy, the mysterious energy that is
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currently driving the accelerating expansion of the Universe.
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---
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@image
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url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-626dL{1}X{2}Y{3}.png
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||||
copyright: Public domain
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||||
license_id: CC-PDDC
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-626d.jpg
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astropix_ids: chandra|626d
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credits> X-ray: NASA/CXC/Univ. of Alabama/A. Morandi et al; Optical: SDSS, NASA/STScI
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---
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@scene
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place_uuid: f26b1051-4951-471a-8d18-94cbedcbfae5
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image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-626dL{1}X{2}Y{3}.png
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outgoing_url: https://chandra.harvard.edu/photo/2016/clusters/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-626d.jpg
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text> This galaxy cluster, ZWCL 3146, was part of a large survey of over 300
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clusters used to investigate dark energy, the mysterious energy that is
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currently driving the accelerating expansion of the Universe.
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---
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@image
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url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-627L{1}X{2}Y{3}.png
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copyright: Public domain
|
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license_id: CC-PDDC
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-627.jpg
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astropix_ids: chandra|627
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credits> X-ray: NASA/CXC/GSFC/B.Williams et al; Optical: DSS
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---
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@scene
|
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place_uuid: b0ede79a-df48-4519-8bd2-76133e1969b1
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image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-627L{1}X{2}Y{3}.png
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outgoing_url: https://chandra.harvard.edu/photo/2016/tycho/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-627.jpg
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text> When the star that created this supernova remnant exploded in 1572, it was
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so bright that it was visible during the day. And though he wasn't the first or
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only person to observe this stellar spectacle, the Danish astronomer Tycho Brahe
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wrote a book about his extensive observations of the event, gaining the honor of
|
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it being named after him.
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---
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@image
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url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-630L{1}X{2}Y{3}.png
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copyright: Public domain
|
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license_id: CC-PDDC
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-630.jpg
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astropix_ids: chandra|630
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credits> X-ray: NASA/CXC/Univ. of Alberta/B.Tetarenko et al; Optical: NASA/STScI; Radio: NSF/AUI/NRAO/Curtin Univ./J. Miller-Jones
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---
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@scene
|
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place_uuid: 100876c2-24f6-45a9-9743-f5671b6be713
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image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-630L{1}X{2}Y{3}.png
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outgoing_url: https://chandra.harvard.edu/photo/2016/vla/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-630.jpg
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text> Astronomers have identified the true nature of an unusual source in the
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Milky Way galaxy, VLA J2130+12. This discovery implies that there could be a
|
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much larger number of black holes in the Galaxy that have previously been
|
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unaccounted for.
|
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|
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---
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@image
|
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url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-633L{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-633.jpg
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astropix_ids: chandra|633
|
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|
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credits> X-ray: NASA/CXC/ETH Zurich/L.Sartori et al, Optical: NASA/STScI
|
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|
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---
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@scene
|
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place_uuid: 889f11c6-7a92-46f3-91f1-3f8105775c93
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-633L{1}X{2}Y{3}.png
|
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outgoing_url: https://chandra.harvard.edu/photo/2016/ic2497/
|
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-633.jpg
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|
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text> Two cosmic structures show evidence for a remarkable change in behavior of
|
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a supermassive black hole in a distant galaxy. Using data from NASA’s Chandra
|
||||
X-ray Observatory and other telescopes, astronomers are piecing together clues
|
||||
from a cosmic “blob” and a gas bubble that could be a new way to probe the past
|
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activity of a giant black hole and its effect on its host galaxy. The Green
|
||||
Blob, a renowned cosmic structure also called “Hanny’s Voorwerp” (which means
|
||||
“Hanny’s object” in Dutch), is located about 680 million light years from Earth.
|
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This object was discovered in 2007 by Hanny van Arkel, at the time a school
|
||||
teacher, as part of the citizen science project called Galaxy Zoo.
|
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|
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---
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|
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@image
|
||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-634L{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-634.jpg
|
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astropix_ids: chandra|634
|
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|
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credits> X-ray: NASA/CXC/NCSU/K.Borkowski et al; Optical: DSS
|
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|
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---
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@scene
|
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place_uuid: a56c5956-2a3a-4370-a04f-7a559e17237a
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image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-634L{1}X{2}Y{3}.png
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outgoing_url: https://chandra.harvard.edu/photo/2016/g11/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-634.jpg
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|
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text> A new look at the debris from an exploded star in our galaxy has
|
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astronomers re-examining when the supernova actually happened. Recent
|
||||
observations of the supernova remnant called G11.2-0.3 with NASA's Chandra X-ray
|
||||
Observatory have stripped away its connection to an event recorded by the
|
||||
Chinese in 386 CE.
|
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|
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---
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|
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@image
|
||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-635L{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-635.jpg
|
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astropix_ids: chandra|635
|
||||
|
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credits> X-ray: NASA/CXC/Université Paris/T.Wang et al; Infrared: ESO/UltraVISTA; Radio: ESO/NAOJ/NRAO/ALMA
|
||||
|
||||
---
|
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|
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@scene
|
||||
place_uuid: 16369967-82b7-4db1-b50e-34f6bf678cc3
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-635L{1}X{2}Y{3}.png
|
||||
outgoing_url: https://chandra.harvard.edu/photo/2016/clj1001/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-635.jpg
|
||||
|
||||
text> This image contains the most distant galaxy cluster, a discovery made
|
||||
using data from NASA's Chandra X-ray Observatory and several other telescopes.
|
||||
The galaxy cluster, known as CL J1001+0220, is located about 11.1 billion light
|
||||
years from Earth and may have been caught right after birth, a brief, but
|
||||
important stage of cluster evolution never seen before.
|
||||
|
||||
---
|
||||
|
||||
@image
|
||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-636L{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-636.jpg
|
||||
astropix_ids: chandra|636
|
||||
|
||||
credits> X-ray: NASA/CXC/University of Amsterdam/N.Rea et al; Optical: DSS
|
||||
|
||||
---
|
||||
|
||||
@scene
|
||||
place_uuid: 3681ac2d-0598-4412-8988-d960f77dbba5
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-636L{1}X{2}Y{3}.png
|
||||
outgoing_url: https://chandra.harvard.edu/photo/2016/rcw103/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-636.jpg
|
||||
|
||||
text> Astronomers have found evidence for what is likely one of the most extreme
|
||||
pulsars, or rotating neutron stars, ever detected. The source exhibits
|
||||
properties of a highly magnetized neutron star, or magnetar, yet its deduced
|
||||
spin period is thousands of times longer than any pulsar ever observed. For
|
||||
decades, astronomers have known there is a dense, compact source at the center
|
||||
of RCW 103, the remains of a supernova explosion located about 9,000 light years
|
||||
from Earth. This composite image shows RCW 103 and its central source, known
|
||||
officially as 1E 161348-5055 (1E 1613, for short), in three bands of X-ray light
|
||||
detected by Chandra.
|
||||
|
||||
---
|
||||
|
||||
@image
|
||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-638L{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-638.jpg
|
||||
astropix_ids: chandra|638
|
||||
|
||||
credits> X-ray: NASA/CXC/UNH/D.Lin et al; Optical: NASA/STScI
|
||||
|
||||
---
|
||||
|
||||
@scene
|
||||
place_uuid: f64e9432-00e7-4b3f-96cc-db45a23ace3e
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-638L{1}X{2}Y{3}.png
|
||||
outgoing_url: https://chandra.harvard.edu/photo/2016/xj1417/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-638.jpg
|
||||
|
||||
text> Astronomers have used NASA's Chandra X-ray Observatory and ESA's
|
||||
XMM-Newton X-ray observatory to discover an extremely luminous, variable X-ray
|
||||
source located outside the center of its parent galaxy. This peculiar object,
|
||||
referred to as XJ1417+52, could be a wandering black hole that came from a small
|
||||
galaxy falling into a larger one.
|
||||
|
||||
---
|
||||
|
||||
@image
|
||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-640aL{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-640a.jpg
|
||||
astropix_ids: chandra|640a
|
||||
|
||||
credits> X-ray: NASA/CXC/SAO/Sejong Univ./Hur et al; Optical: NASA/STScI
|
||||
|
||||
---
|
||||
|
||||
@scene
|
||||
place_uuid: 25c7f523-7113-403f-8a00-1b54ae795f3a
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-640aL{1}X{2}Y{3}.png
|
||||
outgoing_url: https://chandra.harvard.edu/photo/2016/archives/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-640a.jpg
|
||||
|
||||
text> A cluster of young stars — about one to two million years old — located
|
||||
about 20,000 light years from Earth. Data in visible light from the Hubble Space
|
||||
Telescope (green and blue) reveal thick clouds where the stars are forming.
|
||||
High-energy radiation in the form of X-rays, however, can penetrate this cosmic
|
||||
haze, and are detected by Chandra (purple).
|
||||
|
||||
---
|
||||
|
||||
@image
|
||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-640bL{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-640b.jpg
|
||||
astropix_ids: chandra|640b
|
||||
|
||||
credits> X-ray: NASA/CXC/Univ. of Bristol/M.Hardcastle et al; Optical: NASA/STScI
|
||||
|
||||
---
|
||||
|
||||
@scene
|
||||
place_uuid: c5bd942b-6a44-4034-ac71-223f3c6bc56f
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-640bL{1}X{2}Y{3}.png
|
||||
outgoing_url: https://chandra.harvard.edu/photo/2016/archives/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-640b.jpg
|
||||
|
||||
text> X-rays from the radio galaxy 3C31 (blue), located 240 million light years
|
||||
from Earth, allow astronomers to probe the density, temperature, and pressure of
|
||||
this galaxy, long known to be a powerful emitter of radio waves. The Chandra
|
||||
data also reveal a jet blasting away from one side of the central galaxy, which
|
||||
also is known as NGC 383. Here, the Chandra X-ray image has been combined with
|
||||
Hubble's visible light data (yellow).
|
||||
|
||||
---
|
||||
|
||||
@image
|
||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-640cL{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-640c.jpg
|
||||
astropix_ids: chandra|640c
|
||||
|
||||
credits> X-ray: NASA/CXC/George Washington Univ./N.Klingler et al; Optical: DSS; Radio: CSIRO/ATNF/ATCA
|
||||
|
||||
---
|
||||
|
||||
@scene
|
||||
place_uuid: 6fc184d6-03be-4444-8cc3-4b2b347b5607
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-640cL{1}X{2}Y{3}.png
|
||||
outgoing_url: https://chandra.harvard.edu/photo/2016/archives/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-640c.jpg
|
||||
|
||||
text> Pulsars were first discovered in 1967 and today astronomers know of over a
|
||||
thousand such objects. The pulsar, PSR J1509-5850, located about 12,000 light
|
||||
years from Earth and appearing as the bright white spot in the center of this
|
||||
image, has generated a long tail of X-ray emission trailing behind it, as seen
|
||||
in the lower part of the image. This pulsar has also generated an outflow of
|
||||
particles in approximately the opposite direction. In this image, X-rays
|
||||
detected by Chandra (blue) and radio emission (pink) have been overlaid on a
|
||||
visible light image from the Digitized Sky Survey of the field of view.
|
||||
|
||||
---
|
||||
|
||||
@image
|
||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-640dL{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-640d.jpg
|
||||
astropix_ids: chandra|640d
|
||||
|
||||
credits> X-ray: NASA/CXC/Univ. of Alabama/S.Dasadia et al, Radio: NSF/NRAO/VLA, Optical: SDSS
|
||||
|
||||
---
|
||||
|
||||
@scene
|
||||
place_uuid: 59856c0d-5b83-4108-83b2-28cc92d20a32
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-640dL{1}X{2}Y{3}.png
|
||||
outgoing_url: https://chandra.harvard.edu/photo/2016/archives/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-640d.jpg
|
||||
|
||||
text> Merging galaxy clusters can generate enormous shock waves, similar to cold
|
||||
fronts in weather on Earth. This system, known as Abell 665, has an extremely
|
||||
powerful shockwave, second only to the famous Bullet Cluster. Here, X-rays from
|
||||
Chandra (blue) show hot gas in the cluster. The bow wave shape of the shock is
|
||||
shown by the large white region near the center of the image. The Chandra image
|
||||
has been added to radio emission (purple) and visible light data from the Sloan
|
||||
Digital Sky Survey showing galaxies and stars (white).
|
||||
|
||||
---
|
||||
|
||||
@image
|
||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-640eL{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-640e.jpg
|
||||
astropix_ids: chandra|640e
|
||||
|
||||
credits> X-ray: NASA/CXC/SAO/R. van Weeren et al; Radio: LOFAR/ASTRON; Optical: NAOJ/Subaru
|
||||
|
||||
---
|
||||
|
||||
@scene
|
||||
place_uuid: 1e41d884-a562-43bc-a28b-a66c0cf7f4b1
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-640eL{1}X{2}Y{3}.png
|
||||
outgoing_url: https://chandra.harvard.edu/photo/2016/archives/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-640e.jpg
|
||||
|
||||
text> The phenomenon of pareidolia is when people see familiar shapes in images.
|
||||
This galaxy cluster has invoked the nickname of the "Toothbrush Cluster" because
|
||||
of its resemblance to the dental tool. In fact, the stem of the brush is due to
|
||||
radio waves (green) while the diffuse emission where the toothpaste would go is
|
||||
produced by X-rays observed by Chandra (purple). Visible light data from the
|
||||
Subaru telescope show galaxies and stars (white) and a map from gravitational
|
||||
lensing (blue) shows the concentration of the mass, which is mostly (about 80%)
|
||||
dark matter.
|
||||
|
||||
---
|
||||
|
||||
@image
|
||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-640fL{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-640f.jpg
|
||||
astropix_ids: chandra|640f
|
||||
|
||||
credits> X-ray: NASA/CXC/Morehead State Univ/T.Pannuti et al; Radio: Molonglo Obs. Synthesis Tel.; Infrared: NASA/JPL-Caltech
|
||||
|
||||
---
|
||||
|
||||
@scene
|
||||
place_uuid: cc961170-b5c6-4bf9-a254-d3d773c9ebc1
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-640fL{1}X{2}Y{3}.png
|
||||
outgoing_url: https://chandra.harvard.edu/photo/2016/archives/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-640f.jpg
|
||||
|
||||
text> Astronomers estimate that a supernova explosion should occur about every
|
||||
50 years on average in the Milky Way galaxy. The object known as CTB 37A is a
|
||||
supernova remnant located in our Galaxy about 20,000 light years from Earth.
|
||||
This image shows that the debris field glowing in X-rays (blue) and radio waves
|
||||
(pink) may be expanding into a cooler cloud of gas and dust seen in infrared
|
||||
light (orange).
|
||||
|
||||
---
|
||||
|
||||
@image
|
||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-641L{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-641.jpg
|
||||
astropix_ids: chandra|641
|
||||
|
||||
credits> NASA/CXC/UA/J.Irwin et al.
|
||||
|
||||
---
|
||||
|
||||
@scene
|
||||
place_uuid: e90c87d4-bd99-474a-b8ca-5b7a91a1e495
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-641L{1}X{2}Y{3}.png
|
||||
outgoing_url: https://chandra.harvard.edu/photo/2016/ngc5128/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-641.jpg
|
||||
|
||||
text> This image shows the location of a remarkable source that dramatically
|
||||
flares in X-rays unlike any ever seen. It was found in the elliptical galaxiy
|
||||
NGC 5128, also known as Centaurus A.
|
||||
|
||||
---
|
||||
|
||||
@image
|
||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-643L{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-643.jpg
|
||||
astropix_ids: chandra|643
|
||||
|
||||
credits> X-ray: NASA/CXC/SAO/M.McCollough et al, Radio: ASIAA/SAO/SMA
|
||||
|
||||
---
|
||||
|
||||
@scene
|
||||
place_uuid: ea92e6fa-ac51-4fa9-bece-be70008f8993
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-643L{1}X{2}Y{3}.png
|
||||
outgoing_url: https://chandra.harvard.edu/photo/2016/cygx3/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-643.jpg
|
||||
|
||||
text> A snapshot of the life cycle of stars has been captured where a stellar
|
||||
nursery is reflecting X-rays from a source powered by an object at the endpoint
|
||||
of its evolution. This discovery provides a new way to study how stars form.
|
||||
|
||||
---
|
||||
|
||||
@image
|
||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-645L{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-645.jpg
|
||||
astropix_ids: chandra|645
|
||||
|
||||
credits> X-ray: NASA/CXC/PSU/L.Townsley et al; Optical: UKIRT; Infrared: NASA/JPL-Caltech
|
||||
|
||||
---
|
||||
|
||||
@scene
|
||||
place_uuid: 2247db3d-b62e-43cc-8dc3-875c1e1d4d4f
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-645L{1}X{2}Y{3}.png
|
||||
outgoing_url: https://chandra.harvard.edu/photo/2016/ngc6357/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-645.jpg
|
||||
|
||||
text> Although there are no seasons in space, this cosmic vista invokes thoughts
|
||||
of a frosty winter landscape. It is, in fact, a region called NGC 6357 where
|
||||
radiation from hot, young stars is energizing the cooler gas in the cloud that
|
||||
surrounds them.
|
||||
|
||||
---
|
||||
|
||||
@image
|
||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-646L{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-646.jpg
|
||||
astropix_ids: chandra|646
|
||||
|
||||
credits> X-ray: NASA/CXC/SAO/R. van Weeren et al; Optical: NAOJ/Subaru; Radio: NCRA/TIFR/GMRT
|
||||
|
||||
---
|
||||
|
||||
@scene
|
||||
place_uuid: 365181d7-3664-4428-bb2e-53dc58199ffc
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-646L{1}X{2}Y{3}.png
|
||||
outgoing_url: https://chandra.harvard.edu/photo/2017/a3411/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-646.jpg
|
||||
|
||||
text> Using data from NASA's Chandra X-ray Observatory and several other
|
||||
telescopes, astronomers have discovered a cosmic one-two punch unlike any ever
|
||||
seen in a pair of colliding galaxy clusters called Abell 3411 and Abell 3412.
|
||||
This result shows that an eruption from a supermassive black hole combined with
|
||||
a galaxy cluster merger can create a stupendous cosmic particle accelerator.
|
||||
|
||||
---
|
||||
|
||||
@image
|
||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-647L{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-647.jpg
|
||||
astropix_ids: chandra|647
|
||||
|
||||
credits> X-ray: NASA/CXC/Penn State/B.Luo et al.
|
||||
|
||||
---
|
||||
|
||||
@scene
|
||||
place_uuid: f08f9bc5-c492-4801-a019-4f99379e70ae
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-647L{1}X{2}Y{3}.png
|
||||
outgoing_url: https://chandra.harvard.edu/photo/2017/cdfs/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-647.jpg
|
||||
|
||||
text> The image is from the Chandra Deep Field-South, or CDF-S. The full CDF-S
|
||||
field covers an approximately circular region on the sky with an area about
|
||||
two-thirds that of the full Moon. However, the outer regions of the image, where
|
||||
the sensitivity to X-ray emission is lower, are not shown here.
|
||||
|
||||
---
|
||||
|
||||
@image
|
||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-648L{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-648.jpg
|
||||
astropix_ids: chandra|648
|
||||
|
||||
credits> X-ray: NASA/CXC/PSU/B.Posselt et al; Infrared: NASA/JPL-Caltech; Illustration: Nahks TrEhnl
|
||||
|
||||
---
|
||||
|
||||
@scene
|
||||
place_uuid: 7a90023f-aea0-4379-8339-27c4790c893e
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-648L{1}X{2}Y{3}.png
|
||||
outgoing_url: https://chandra.harvard.edu/photo/2017/geminga/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-648.jpg
|
||||
|
||||
text> This four-panel graphic shows the two pulsars observed by Chandra. Geminga
|
||||
is in the upper left and B0355+54 is in the upper right. In both of these
|
||||
images, Chandra's X-rays, colored blue and purple, are combined with infrared
|
||||
data from NASA's Spitzer Space Telescope that shows stars in the field of view.
|
||||
Below each data image, an artist's illustration depicts more details of what
|
||||
astronomers think the structure of each pulsar wind nebula looks like.
|
||||
|
||||
---
|
||||
|
||||
@image
|
||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-66L{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
|
|
|
@ -54178,7 +54178,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-617L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|617"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e160d1c7ef132a3905d"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/Univ of Missouri; Astronomers have made the most detailed study yet of an extremely massive young galaxy cluster using three of NASA's Great Obser...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2016/idcs1426/</CreditsUrl>
|
||||
|
@ -54205,7 +54205,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-620L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|620"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e170d1c7ef132a3905f"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/Univ of Hertford; The Pictor A galaxy has a supermassive black hole at its center, and material falling onto the black hole is driving an enormous...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2016/pictora/</CreditsUrl>
|
||||
|
@ -54232,7 +54232,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-621L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|621"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e180d1c7ef132a39061"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/ISAS/A.Simionesc; Jets in the early Universe give astronomers a way to probe the growth of black holes at a very early epoch in the cosmos. Using ...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2016/b30727/</CreditsUrl>
|
||||
|
@ -54259,7 +54259,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-622aL{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|622a"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e190d1c7ef132a39063"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/SAO/G.Ogrean et ; These two galaxy clusters are part of the "Frontier Fields" project, which uses some of the world's most powerful telescopes to ...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2016/frontier/</CreditsUrl>
|
||||
|
@ -54286,7 +54286,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-622bL{1}X{2}Y{3}.png"
|
||||
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|
||||
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|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e1a0d1c7ef132a39065"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/SAO/G.Ogrean et ; These two galaxy clusters are part of the "Frontier Fields" project, which uses some of the world's most powerful telescopes to ...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2016/frontier/</CreditsUrl>
|
||||
|
@ -54313,7 +54313,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-624L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|624"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e1b0d1c7ef132a39067"
|
||||
>
|
||||
<Credits>X-ray (NASA/CXC/CfA/S.Chakrabort; Scientists have found the likely trigger for the most recent supernova in the Milky Way, by studying the remnant called G1.9+0.3...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2016/g19/</CreditsUrl>
|
||||
|
@ -54340,7 +54340,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-626aL{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|626a"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e1c0d1c7ef132a39069"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/Univ. of Alabama; These four galaxy clusters were part of a large survey of over 300 clusters used to investigate dark energy, the mysterious ener...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2016/clusters/</CreditsUrl>
|
||||
|
@ -54367,7 +54367,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-626bL{1}X{2}Y{3}.png"
|
||||
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|
||||
Xastropix_ids="chandra|626b"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e1c0d1c7ef132a3906b"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/Univ. of Alabama; These four galaxy clusters were part of a large survey of over 300 clusters used to investigate dark energy, the mysterious ener...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2016/clusters/</CreditsUrl>
|
||||
|
@ -54394,7 +54394,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-626cL{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|626c"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e1d0d1c7ef132a3906d"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/Univ. of Alabama; These four galaxy clusters were part of a large survey of over 300 clusters used to investigate dark energy, the mysterious ener...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2016/clusters/</CreditsUrl>
|
||||
|
@ -54421,7 +54421,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-626dL{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|626d"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e1e0d1c7ef132a3906f"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/Univ. of Alabama; These four galaxy clusters were part of a large survey of over 300 clusters used to investigate dark energy, the mysterious ener...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2016/clusters/</CreditsUrl>
|
||||
|
@ -54448,7 +54448,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-627L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|627"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e1f0d1c7ef132a39071"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/GSFC/B.Williams ; By combining observations from over 15 years with the Chandra X-ray Observatory and 30 years with the Very Large Array, scientis...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2016/tycho/</CreditsUrl>
|
||||
|
@ -54475,7 +54475,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-630L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|630"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e200d1c7ef132a39073"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/Univ. of Alberta; By combining data from Chandra and several other telescopes, astronomers have identified the true nature of an unusual source in...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2016/vla/</CreditsUrl>
|
||||
|
@ -54502,7 +54502,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-633L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|633"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e210d1c7ef132a39075"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/ETH Zurich/L.Sar; New data from Chandra and other telescopes of a cosmic 'blob' and a gas bubble could be a new way to probe the past activity of ...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2016/ic2497/</CreditsUrl>
|
||||
|
@ -54529,7 +54529,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-634L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|634"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e220d1c7ef132a39077"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/NCSU/K.Borkowski; New Chandra observations of the G11.2-0.3 supernova remnant in our Galaxy have stripped away its connection to an event recorded...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2016/g11/</CreditsUrl>
|
||||
|
@ -54556,7 +54556,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-635L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|635"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e220d1c7ef132a39079"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/Université Pari; The galaxy cluster CL J1001+0220 is the most distant galaxy cluster ever discovered and may have been caught right after birth, ...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2016/clj1001/</CreditsUrl>
|
||||
|
@ -54583,7 +54583,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-636L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|636"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e230d1c7ef132a3907b"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/University of Am; Using Chandra and other X-ray observatories, astronomers have found evidence for what is likely one of the most extreme pulsars,...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2016/rcw103/</CreditsUrl>
|
||||
|
@ -54610,7 +54610,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-638L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|638"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e240d1c7ef132a3907d"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/UNH/D.Lin et al;; Using Chandra and XMM-Newton, astronomers have discovered an extremely luminous, variable X-ray source located outside the core ...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2016/xj1417/</CreditsUrl>
|
||||
|
@ -54637,7 +54637,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-640aL{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|640a"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e250d1c7ef132a3907f"
|
||||
>
|
||||
<Credits>NASA/CXC/SAO; The Chandra Data Archive is a sophisticated digital system that ultimately contains all of the data obtained by the telescope, c...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2016/archives/</CreditsUrl>
|
||||
|
@ -54664,7 +54664,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-640bL{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|640b"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e260d1c7ef132a39081"
|
||||
>
|
||||
<Credits>NASA/CXC/SAO; The Chandra Data Archive is a sophisticated digital system that ultimately contains all of the data obtained by the telescope, c...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2016/archives/</CreditsUrl>
|
||||
|
@ -54691,7 +54691,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-640cL{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|640c"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e270d1c7ef132a39083"
|
||||
>
|
||||
<Credits>NASA/CXC/SAO; The Chandra Data Archive is a sophisticated digital system that ultimately contains all of the data obtained by the telescope, c...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2016/archives/</CreditsUrl>
|
||||
|
@ -54718,7 +54718,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-640dL{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|640d"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e280d1c7ef132a39085"
|
||||
>
|
||||
<Credits>NASA/CXC/SAO; The Chandra Data Archive is a sophisticated digital system that ultimately contains all of the data obtained by the telescope, c...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2016/archives/</CreditsUrl>
|
||||
|
@ -54745,7 +54745,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-640eL{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|640e"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e290d1c7ef132a39087"
|
||||
>
|
||||
<Credits>NASA/CXC/SAO; The Chandra Data Archive is a sophisticated digital system that ultimately contains all of the data obtained by the telescope, c...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2016/archives/</CreditsUrl>
|
||||
|
@ -54772,7 +54772,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-640fL{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|640f"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e290d1c7ef132a39089"
|
||||
>
|
||||
<Credits>NASA/CXC/SAO; The Chandra Data Archive is a sophisticated digital system that ultimately contains all of the data obtained by the telescope, c...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2016/archives/</CreditsUrl>
|
||||
|
@ -54799,7 +54799,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-641L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|641"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e2a0d1c7ef132a3908b"
|
||||
>
|
||||
<Credits>NASA/CXC/UA/J.Irwin et al.; Astronomers have found a pair of extraordinary objects that dramatically burst in X-rays. This discovery, obtained with NASA's C...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2016/ngc5128/</CreditsUrl>
|
||||
|
@ -54826,7 +54826,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-643L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|643"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e2b0d1c7ef132a3908d"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/SAO/M.McCollough; A snapshot of the life cycle of stars has been captured where a stellar nursery is reflecting X-rays from a source powered by an...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2016/cygx3/</CreditsUrl>
|
||||
|
@ -54853,7 +54853,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-645L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|645"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e2c0d1c7ef132a3908f"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/PSU/L.Townsley e; This composite image captures the star formation region called NGC 6357 located within the Milky Way galaxy. X-rays from Chandra...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2016/ngc6357/</CreditsUrl>
|
||||
|
@ -54880,7 +54880,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-646L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|646"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e2d0d1c7ef132a39091"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/SAO/R. van Weere; Astronomers have discovered what happens when the eruption from a supermassive black hole is swept up by the collision and merge...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2017/a3411/</CreditsUrl>
|
||||
|
@ -54907,7 +54907,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-647L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|647"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e2e0d1c7ef132a39093"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/Penn State/B.Luo; Made with over 7 million seconds of Chandra observing time, this image is part of the Chandra Deep Field-South (CDF-S) and is th...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2017/cdfs/</CreditsUrl>
|
||||
|
@ -54934,7 +54934,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-648L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|648"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:672d1e2f0d1c7ef132a39095"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/PSU/B.Posselt et; This four-panel graphic shows the two pulsars, Geminga (upper left) and B0355+54 (upper right), observed by Chandra. In both of ...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2017/geminga/</CreditsUrl>
|
||||
|
|
|
@ -1783,8 +1783,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-593e.jpg
|
|||
zoom_level: 0.449967128576
|
||||
---
|
||||
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|
||||
astropix_id: chandra|627
|
||||
classification: ''
|
||||
constellation: CAS
|
||||
cxstatus: in:672d1e1f0d1c7ef132a39072
|
||||
data_set_type: Sky
|
||||
dec_deg: 64.138614
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-627L{1}X{2}Y{3}.png
|
||||
|
|
|
@ -1287,8 +1287,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-593b.jpg
|
|||
zoom_level: 0.232704802816
|
||||
---
|
||||
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|
||||
astropix_id: chandra|640b
|
||||
classification: ''
|
||||
constellation: PSC
|
||||
cxstatus: in:672d1e260d1c7ef132a39082
|
||||
data_set_type: Sky
|
||||
dec_deg: 32.4124951
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-640bL{1}X{2}Y{3}.png
|
||||
|
|
|
@ -2000,8 +2000,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-601.jpg
|
|||
zoom_level: 1.36700780544
|
||||
---
|
||||
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|
||||
astropix_id: chandra|647
|
||||
classification: ''
|
||||
constellation: FOR
|
||||
cxstatus: in:672d1e2e0d1c7ef132a39094
|
||||
data_set_type: Sky
|
||||
dec_deg: -27.8097471
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-647L{1}X{2}Y{3}.png
|
||||
|
|
|
@ -760,8 +760,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-593a.jpg
|
|||
zoom_level: 0.245886353408
|
||||
---
|
||||
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|
||||
astropix_id: chandra|622a
|
||||
classification: ''
|
||||
constellation: ERI
|
||||
cxstatus: in:672d1e190d1c7ef132a39064
|
||||
data_set_type: Sky
|
||||
dec_deg: -24.074654
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-622aL{1}X{2}Y{3}.png
|
||||
|
|
|
@ -4790,8 +4790,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-612.jpg
|
|||
zoom_level: 113.4662598656
|
||||
---
|
||||
_uuid: c382d1ba-87c8-4a6d-a277-6f37235712fc
|
||||
astropix_id: chandra|620
|
||||
classification: ''
|
||||
constellation: PIC
|
||||
cxstatus: in:672d1e170d1c7ef132a39060
|
||||
data_set_type: Sky
|
||||
dec_deg: -45.7768467
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-620L{1}X{2}Y{3}.png
|
||||
|
|
|
@ -848,8 +848,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-613.jpg
|
|||
zoom_level: 5.47552690176
|
||||
---
|
||||
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|
||||
astropix_id: chandra|640e
|
||||
classification: ''
|
||||
constellation: AUR
|
||||
cxstatus: in:672d1e290d1c7ef132a39088
|
||||
data_set_type: Sky
|
||||
dec_deg: 42.2270032
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-640eL{1}X{2}Y{3}.png
|
||||
|
@ -859,8 +861,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-640e.jpg
|
|||
zoom_level: 1.557559361536
|
||||
---
|
||||
_uuid: 7a90023f-aea0-4379-8339-27c4790c893e
|
||||
astropix_id: chandra|648
|
||||
classification: ''
|
||||
constellation: GEM
|
||||
cxstatus: in:672d1e2f0d1c7ef132a39096
|
||||
data_set_type: Sky
|
||||
dec_deg: 17.7527598
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-648L{1}X{2}Y{3}.png
|
||||
|
|
|
@ -815,8 +815,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-610d.jpg
|
|||
zoom_level: 0.11340251136
|
||||
---
|
||||
_uuid: 6cd4c6bd-08fe-4a86-98bc-ca776e5f1e57
|
||||
astropix_id: chandra|621
|
||||
classification: ''
|
||||
constellation: LYN
|
||||
cxstatus: in:672d1e190d1c7ef132a39062
|
||||
data_set_type: Sky
|
||||
dec_deg: 40.831235
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-621L{1}X{2}Y{3}.png
|
||||
|
@ -826,8 +828,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-621.jpg
|
|||
zoom_level: 0.761291882496
|
||||
---
|
||||
_uuid: 8f4450e7-3dd1-4ba9-b2b8-12c89de6d936
|
||||
astropix_id: chandra|622b
|
||||
classification: ''
|
||||
constellation: AUR
|
||||
cxstatus: in:672d1e1a0d1c7ef132a39066
|
||||
data_set_type: Sky
|
||||
dec_deg: 37.7481384
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-622bL{1}X{2}Y{3}.png
|
||||
|
|
|
@ -616,8 +616,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-581a.jpg
|
|||
zoom_level: 2.00966684672
|
||||
---
|
||||
_uuid: 59856c0d-5b83-4108-83b2-28cc92d20a32
|
||||
astropix_id: chandra|640d
|
||||
classification: ''
|
||||
constellation: UMA
|
||||
cxstatus: in:672d1e280d1c7ef132a39086
|
||||
data_set_type: Sky
|
||||
dec_deg: 65.8653523
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-640dL{1}X{2}Y{3}.png
|
||||
|
@ -627,8 +629,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-640d.jpg
|
|||
zoom_level: 1.367419584512
|
||||
---
|
||||
_uuid: 365181d7-3664-4428-bb2e-53dc58199ffc
|
||||
astropix_id: chandra|646
|
||||
classification: ''
|
||||
constellation: HYA
|
||||
cxstatus: in:672d1e2d0d1c7ef132a39092
|
||||
data_set_type: Sky
|
||||
dec_deg: -17.5268228
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-646L{1}X{2}Y{3}.png
|
||||
|
|
|
@ -780,8 +780,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-580.jpg
|
|||
zoom_level: 0.697498697728
|
||||
---
|
||||
_uuid: 889f11c6-7a92-46f3-91f1-3f8105775c93
|
||||
astropix_id: chandra|633
|
||||
classification: ''
|
||||
constellation: LMI
|
||||
cxstatus: in:672d1e210d1c7ef132a39076
|
||||
data_set_type: Sky
|
||||
dec_deg: 34.7292506
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-633L{1}X{2}Y{3}.png
|
||||
|
|
|
@ -1639,8 +1639,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-607.jpg
|
|||
zoom_level: 1.26286471168
|
||||
---
|
||||
_uuid: f26b1051-4951-471a-8d18-94cbedcbfae5
|
||||
astropix_id: chandra|626d
|
||||
classification: ''
|
||||
constellation: SEX
|
||||
cxstatus: in:672d1e1f0d1c7ef132a39070
|
||||
data_set_type: Sky
|
||||
dec_deg: 4.18634
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-626dL{1}X{2}Y{3}.png
|
||||
|
@ -1650,8 +1652,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-626d.jpg
|
|||
zoom_level: 0.192437764096
|
||||
---
|
||||
_uuid: 16369967-82b7-4db1-b50e-34f6bf678cc3
|
||||
astropix_id: chandra|635
|
||||
classification: ''
|
||||
constellation: SEX
|
||||
cxstatus: in:672d1e230d1c7ef132a3907a
|
||||
data_set_type: Sky
|
||||
dec_deg: 2.3361325
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-635L{1}X{2}Y{3}.png
|
||||
|
@ -1661,8 +1665,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-635.jpg
|
|||
zoom_level: 0.164778016768
|
||||
---
|
||||
_uuid: 25c7f523-7113-403f-8a00-1b54ae795f3a
|
||||
astropix_id: chandra|640a
|
||||
classification: ''
|
||||
constellation: CAR
|
||||
cxstatus: in:672d1e260d1c7ef132a39080
|
||||
data_set_type: Sky
|
||||
dec_deg: -57.76353613526
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-640aL{1}X{2}Y{3}.png
|
||||
|
|
|
@ -2472,8 +2472,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-593f.jpg
|
|||
zoom_level: 0.22027517952
|
||||
---
|
||||
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|
||||
astropix_id: chandra|626c
|
||||
classification: ''
|
||||
constellation: VIR
|
||||
cxstatus: in:672d1e1e0d1c7ef132a3906e
|
||||
data_set_type: Sky
|
||||
dec_deg: -11.7526049
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-626cL{1}X{2}Y{3}.png
|
||||
|
@ -2483,8 +2485,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-626c.jpg
|
|||
zoom_level: 0.167788003328
|
||||
---
|
||||
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|
||||
astropix_id: chandra|641
|
||||
classification: ''
|
||||
constellation: CEN
|
||||
cxstatus: in:672d1e2b0d1c7ef132a3908c
|
||||
data_set_type: Sky
|
||||
dec_deg: -43.0188596
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-641L{1}X{2}Y{3}.png
|
||||
|
|
|
@ -966,8 +966,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-610e.jpg
|
|||
zoom_level: 0.1142846029824
|
||||
---
|
||||
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|
||||
astropix_id: chandra|617
|
||||
classification: ''
|
||||
constellation: BOO
|
||||
cxstatus: in:672d1e170d1c7ef132a3905e
|
||||
data_set_type: Sky
|
||||
dec_deg: 35.1393564
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-617L{1}X{2}Y{3}.png
|
||||
|
@ -977,8 +979,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-617.jpg
|
|||
zoom_level: 0.1409575010304
|
||||
---
|
||||
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|
||||
astropix_id: chandra|626a
|
||||
classification: ''
|
||||
constellation: VIR
|
||||
cxstatus: in:672d1e1c0d1c7ef132a3906a
|
||||
data_set_type: Sky
|
||||
dec_deg: 2.8782473
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-626aL{1}X{2}Y{3}.png
|
||||
|
@ -988,8 +992,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-626a.jpg
|
|||
zoom_level: 0.231550173184
|
||||
---
|
||||
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|
||||
astropix_id: chandra|626b
|
||||
classification: ''
|
||||
constellation: BOO
|
||||
cxstatus: in:672d1e1d0d1c7ef132a3906c
|
||||
data_set_type: Sky
|
||||
dec_deg: 22.3441229
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-626bL{1}X{2}Y{3}.png
|
||||
|
@ -999,8 +1005,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-626b.jpg
|
|||
zoom_level: 0.201005203456
|
||||
---
|
||||
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|
||||
astropix_id: chandra|638
|
||||
classification: ''
|
||||
constellation: BOO
|
||||
cxstatus: in:672d1e250d1c7ef132a3907e
|
||||
data_set_type: Sky
|
||||
dec_deg: 52.4169249
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-638L{1}X{2}Y{3}.png
|
||||
|
|
|
@ -589,8 +589,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-606.jpg
|
|||
zoom_level: 0.365037254776471
|
||||
---
|
||||
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|
||||
astropix_id: chandra|640c
|
||||
classification: ''
|
||||
constellation: CIR
|
||||
cxstatus: in:672d1e270d1c7ef132a39084
|
||||
data_set_type: Sky
|
||||
dec_deg: -58.8050082
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-640cL{1}X{2}Y{3}.png
|
||||
|
|
|
@ -1392,8 +1392,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-581d.jpg
|
|||
zoom_level: 0.252133441536
|
||||
---
|
||||
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|
||||
astropix_id: chandra|636
|
||||
classification: ''
|
||||
constellation: NOR
|
||||
cxstatus: in:672d1e240d1c7ef132a3907c
|
||||
data_set_type: Sky
|
||||
dec_deg: -51.0404495
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-636L{1}X{2}Y{3}.png
|
||||
|
|
|
@ -2105,8 +2105,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-596.jpg
|
|||
zoom_level: 0.932067016704
|
||||
---
|
||||
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|
||||
astropix_id: chandra|624
|
||||
classification: ''
|
||||
constellation: SGR
|
||||
cxstatus: in:672d1e1b0d1c7ef132a39068
|
||||
data_set_type: Sky
|
||||
dec_deg: -27.1688425
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-624L{1}X{2}Y{3}.png
|
||||
|
@ -2116,8 +2118,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-624.jpg
|
|||
zoom_level: 0.311165108224
|
||||
---
|
||||
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|
||||
astropix_id: chandra|640f
|
||||
classification: ''
|
||||
constellation: SCO
|
||||
cxstatus: in:672d1e2a0d1c7ef132a3908a
|
||||
data_set_type: Sky
|
||||
dec_deg: -38.5334492
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-640fL{1}X{2}Y{3}.png
|
||||
|
@ -2127,8 +2131,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-640f.jpg
|
|||
zoom_level: 1.465168068608
|
||||
---
|
||||
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|
||||
astropix_id: chandra|645
|
||||
classification: ''
|
||||
constellation: SCO
|
||||
cxstatus: in:672d1e2c0d1c7ef132a39090
|
||||
data_set_type: Sky
|
||||
dec_deg: -34.3174881
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-645L{1}X{2}Y{3}.png
|
||||
|
|
|
@ -2154,8 +2154,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-615.jpg
|
|||
zoom_level: 0.2726928384
|
||||
---
|
||||
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|
||||
astropix_id: chandra|634
|
||||
classification: ''
|
||||
constellation: SGR
|
||||
cxstatus: in:672d1e220d1c7ef132a39078
|
||||
data_set_type: Sky
|
||||
dec_deg: -19.4242186
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-634L{1}X{2}Y{3}.png
|
||||
|
|
|
@ -1106,8 +1106,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-525.jpg
|
|||
zoom_level: 7.42803161088
|
||||
---
|
||||
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|
||||
astropix_id: chandra|643
|
||||
classification: ''
|
||||
constellation: CYG
|
||||
cxstatus: in:672d1e2b0d1c7ef132a3908e
|
||||
data_set_type: Sky
|
||||
dec_deg: 40.957851
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-643L{1}X{2}Y{3}.png
|
||||
|
|
|
@ -590,8 +590,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-176.jpg
|
|||
zoom_level: 0.0411975000064
|
||||
---
|
||||
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|
||||
astropix_id: chandra|630
|
||||
classification: ''
|
||||
constellation: PEG
|
||||
cxstatus: in:672d1e200d1c7ef132a39074
|
||||
data_set_type: Sky
|
||||
dec_deg: 12.162411
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-630L{1}X{2}Y{3}.png
|
||||
|
|
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