cxprep/chandra.txt: complete registration

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@image
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-617L{1}X{2}Y{3}.png
copyright: Public domain
license_id: CC-PDDC
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-617.jpg
astropix_ids: chandra|617
credits> X-ray: NASA/CXC/University of Missouri-Kansas City/M.Brodwin et al; Optical: NASA/STScI; Infrared: JPL/CalTech
---
@scene
place_uuid: d6341502-3902-4cd4-a280-42346d8226d0
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-617L{1}X{2}Y{3}.png
outgoing_url: https://chandra.harvard.edu/photo/2016/idcs1426/
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-617.jpg
text> This multi-wavelength image shows the galaxy cluster called IDCS
J1426.5+3508 (IDCS J1426 for short) in X-rays from the Chandra X-ray Observatory
in blue, visible light from the Hubble Space Telescope in green, and infrared
light from the Spitzer Space Telescope in red. This rare galaxy cluster, which
is located 10 billion light years from Earth, weighs almost 500 trillion Suns.
---
@image
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-620L{1}X{2}Y{3}.png
copyright: Public domain
license_id: CC-PDDC
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-620.jpg
astropix_ids: chandra|620
credits> X-ray: NASA/CXC/Univ of Hertfordshire/M.Hardcastle et al., Radio: CSIRO/ATNF/ATCA
---
@scene
place_uuid: c382d1ba-87c8-4a6d-a277-6f37235712fc
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-620L{1}X{2}Y{3}.png
outgoing_url: https://chandra.harvard.edu/photo/2016/pictora/
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-620.jpg
text> The Star Wars franchise has featured the fictitious "Death Star," which
can shoot powerful beams of radiation across space. The Universe, however,
produces phenomena that often surpass what science fiction can conjure. The
Pictor A galaxy is one such impressive object. This galaxy, located nearly 500
million light years from Earth, contains a supermassive black hole at its
center. A huge amount of gravitational energy is released as material swirls
towards the event horizon, the point of no return for infalling material. This
energy produces an enormous beam, or jet, of particles traveling at nearly the
speed of light into intergalactic space.
---
@image
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-621L{1}X{2}Y{3}.png
copyright: Public domain
license_id: CC-PDDC
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-621.jpg
astropix_ids: chandra|621
credits> X-ray: NASA/CXC/ISAS/A.Simionescu et al, Optical: DSS
---
@scene
place_uuid: 6cd4c6bd-08fe-4a86-98bc-ca776e5f1e57
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-621L{1}X{2}Y{3}.png
outgoing_url: https://chandra.harvard.edu/photo/2016/b30727/
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-621.jpg
text> A jet from a very distant black hole being illuminated by the leftover
glow from the Big Bang, known as the cosmic microwave background (CMB), has been
found. Astronomers using NASA's Chandra X-ray Observatory discovered this
faraway jet serendipitously when looking at another source in Chandra's field of
view. Jets in the early Universe such as this one, known as B3 0727+409, give
astronomers a way to probe the growth of black holes at a very early epoch in
the cosmos.
---
@image
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-622aL{1}X{2}Y{3}.png
copyright: Public domain
license_id: CC-PDDC
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-622a.jpg
astropix_ids: chandra|622a
credits> X-ray: NASA/CXC/SAO/G.Ogrean et al.; Optical: NASA/STScI; Radio: NRAO/AUI/NSF
---
@scene
place_uuid: 37878806-a1ae-4442-bb3a-af1b1f96926d
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-622aL{1}X{2}Y{3}.png
outgoing_url: https://chandra.harvard.edu/photo/2016/frontier/
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-622a.jpg
text> Galaxy clusters are enormous collections of hundreds or even thousands of
galaxies and vast reservoirs of hot gas embedded in massive clouds of dark
matter, invisible material that does not emit or absorb light but can be
detected through its gravitational effects. Located about 4.3 billion light
years from Earth, MACS J0416 is a pair of colliding galaxy clusters that will
eventually combine to form an even bigger cluster.
---
@image
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-622bL{1}X{2}Y{3}.png
copyright: Public domain
license_id: CC-PDDC
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-622b.jpg
astropix_ids: chandra|622b
credits> X-ray: NASA/CXC/SAO/van Weeren et al.; Optical: NASA/STScI; Radio: NRAO/AUI/NSF
---
@scene
place_uuid: 8f4450e7-3dd1-4ba9-b2b8-12c89de6d936
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-622bL{1}X{2}Y{3}.png
outgoing_url: https://chandra.harvard.edu/photo/2016/frontier/
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-622b.jpg
text> Galaxy clusters are enormous collections of hundreds or even thousands of
galaxies and vast reservoirs of hot gas embedded in massive clouds of dark
matter, invisible material that does not emit or absorb light but can be
detected through its gravitational effects. MACS J0717, one of the most complex
and distorted galaxy clusters known, is the site of a collision between four
clusters. It is located about 5.4 billion light years away from Earth.
---
@image
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-624L{1}X{2}Y{3}.png
copyright: Public domain
license_id: CC-PDDC
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-624.jpg
astropix_ids: chandra|624
credits> X-ray (NASA/CXC/CfA/S.Chakraborti et al.)
---
@scene
place_uuid: 620fa34f-ae3b-4001-b57f-bf76a38cda99
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-624L{1}X{2}Y{3}.png
outgoing_url: https://chandra.harvard.edu/photo/2016/g19/
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-624.jpg
text> Scientists have used data from NASA's Chandra X-ray Observatory and the
NSF's Jansky Very Large Array to determine the likely trigger for the most
recent supernova in the Milky Way. Astronomers had previously identified
G1.9+0.3 as the remnant of the most recent supernova in our Galaxy. It is
estimated to have occurred about 110 years ago from the vantage point of Earth,
in a dusty region of the Galaxy that blocked visible light from reaching Earth.
---
@image
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-626aL{1}X{2}Y{3}.png
copyright: Public domain
license_id: CC-PDDC
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-626a.jpg
astropix_ids: chandra|626a
credits> X-ray: NASA/CXC/Univ. of Alabama/A. Morandi et al; Optical: SDSS, NASA/STScI
---
@scene
place_uuid: 0a2104ea-0141-4b63-beb3-a28e06ceaefd
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-626aL{1}X{2}Y{3}.png
outgoing_url: https://chandra.harvard.edu/photo/2016/clusters/
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-626a.jpg
text> This galaxy cluster, Abell 1835, was part of a large survey of over 300
clusters used to investigate dark energy, the mysterious energy that is
currently driving the accelerating expansion of the Universe.
---
@image
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-626bL{1}X{2}Y{3}.png
copyright: Public domain
license_id: CC-PDDC
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-626b.jpg
astropix_ids: chandra|626b
credits> X-ray: NASA/CXC/Univ. of Alabama/A. Morandi et al; Optical: SDSS, NASA/STScI
---
@scene
place_uuid: a5367509-e96b-4f4b-a368-1e915a20dea5
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-626bL{1}X{2}Y{3}.png
outgoing_url: https://chandra.harvard.edu/photo/2016/clusters/
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-626b.jpg
text> This galaxy cluster, MS 1455.0+2232, was part of a large survey of over 300
clusters used to investigate dark energy, the mysterious energy that is
currently driving the accelerating expansion of the Universe.
---
@image
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-626cL{1}X{2}Y{3}.png
copyright: Public domain
license_id: CC-PDDC
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-626c.jpg
astropix_ids: chandra|626c
credits> X-ray: NASA/CXC/Univ. of Alabama/A. Morandi et al; Optical: SDSS, NASA/STScI
---
@scene
place_uuid: 13f7a422-fa14-4ca2-86ff-0e27a33c9309
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-626cL{1}X{2}Y{3}.png
outgoing_url: https://chandra.harvard.edu/photo/2016/clusters/
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-626c.jpg
text> This galaxy cluster, RXJ 1347.5-1145, was part of a large survey of over 300
clusters used to investigate dark energy, the mysterious energy that is
currently driving the accelerating expansion of the Universe.
---
@image
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-626dL{1}X{2}Y{3}.png
copyright: Public domain
license_id: CC-PDDC
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-626d.jpg
astropix_ids: chandra|626d
credits> X-ray: NASA/CXC/Univ. of Alabama/A. Morandi et al; Optical: SDSS, NASA/STScI
---
@scene
place_uuid: f26b1051-4951-471a-8d18-94cbedcbfae5
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-626dL{1}X{2}Y{3}.png
outgoing_url: https://chandra.harvard.edu/photo/2016/clusters/
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-626d.jpg
text> This galaxy cluster, ZWCL 3146, was part of a large survey of over 300
clusters used to investigate dark energy, the mysterious energy that is
currently driving the accelerating expansion of the Universe.
---
@image
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-627L{1}X{2}Y{3}.png
copyright: Public domain
license_id: CC-PDDC
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-627.jpg
astropix_ids: chandra|627
credits> X-ray: NASA/CXC/GSFC/B.Williams et al; Optical: DSS
---
@scene
place_uuid: b0ede79a-df48-4519-8bd2-76133e1969b1
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-627L{1}X{2}Y{3}.png
outgoing_url: https://chandra.harvard.edu/photo/2016/tycho/
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-627.jpg
text> When the star that created this supernova remnant exploded in 1572, it was
so bright that it was visible during the day. And though he wasn't the first or
only person to observe this stellar spectacle, the Danish astronomer Tycho Brahe
wrote a book about his extensive observations of the event, gaining the honor of
it being named after him.
---
@image
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-630L{1}X{2}Y{3}.png
copyright: Public domain
license_id: CC-PDDC
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-630.jpg
astropix_ids: chandra|630
credits> X-ray: NASA/CXC/Univ. of Alberta/B.Tetarenko et al; Optical: NASA/STScI; Radio: NSF/AUI/NRAO/Curtin Univ./J. Miller-Jones
---
@scene
place_uuid: 100876c2-24f6-45a9-9743-f5671b6be713
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-630L{1}X{2}Y{3}.png
outgoing_url: https://chandra.harvard.edu/photo/2016/vla/
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-630.jpg
text> Astronomers have identified the true nature of an unusual source in the
Milky Way galaxy, VLA J2130+12. This discovery implies that there could be a
much larger number of black holes in the Galaxy that have previously been
unaccounted for.
---
@image
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
astropix_ids: chandra|633
credits> X-ray: NASA/CXC/ETH Zurich/L.Sartori et al, Optical: NASA/STScI
---
@scene
place_uuid: 889f11c6-7a92-46f3-91f1-3f8105775c93
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-633L{1}X{2}Y{3}.png
outgoing_url: https://chandra.harvard.edu/photo/2016/ic2497/
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-633.jpg
text> Two cosmic structures show evidence for a remarkable change in behavior of
a supermassive black hole in a distant galaxy. Using data from NASAs 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
activity of a giant black hole and its effect on its host galaxy. The Green
Blob, a renowned cosmic structure also called “Hannys Voorwerp” (which means
“Hannys object” in Dutch), is located about 680 million light years from Earth.
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.
---
@image
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-634L{1}X{2}Y{3}.png
copyright: Public domain
license_id: CC-PDDC
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-634.jpg
astropix_ids: chandra|634
credits> X-ray: NASA/CXC/NCSU/K.Borkowski et al; Optical: DSS
---
@scene
place_uuid: a56c5956-2a3a-4370-a04f-7a559e17237a
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-634L{1}X{2}Y{3}.png
outgoing_url: https://chandra.harvard.edu/photo/2016/g11/
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-634.jpg
text> A new look at the debris from an exploded star in our galaxy has
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.
---
@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
astropix_ids: chandra|635
credits> X-ray: NASA/CXC/Université Paris/T.Wang et al; Infrared: ESO/UltraVISTA; Radio: ESO/NAOJ/NRAO/ALMA
---
@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

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@ -54259,7 +54259,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
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@ -54286,7 +54286,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
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<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>
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@ -54313,7 +54313,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
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@ -54475,7 +54475,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
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<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>
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@ -54583,7 +54583,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
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<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>
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@ -54610,7 +54610,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
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<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>
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<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>
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<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>
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<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>
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