diff --git a/cxprep/chandra.txt b/cxprep/chandra.txt index add0245..abcec62 100644 --- a/cxprep/chandra.txt +++ b/cxprep/chandra.txt @@ -1,612 +1,4 @@ -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-471L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-471.jpg -astropix_ids: chandra|471 - -credits> NASA/CXC/Wesleyan/R.Kilgard et al. - ---- - -@scene -place_uuid: 8d3ca8d9-de93-4e6d-bead-583c6ec457c4 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-471L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2011/m82/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-471.jpg - -text> A Chandra image of Messier 82, or M82, shows the result of star formation -on overdrive. M82 is located about 12 million light years from Earth and is the -nearest place to us where the conditions are similar to those when the Universe -was much younger with lots of stars forming. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-472L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-472.jpg - -credits> X-ray (NASA/CXC/Harvard/J.Neilsen et al); Optical (Palomar DSS2) - ---- - -@scene -place_uuid: a4f51693-38ce-43f1-b22d-28a2528c9dea -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-472L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2011/g1915/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-472.jpg - -text> This optical and infrared image from the Digitized Sky Survey shows the -crowded field around the binary system GRS 1915+105 (GRS 1915 for short) located -near the plane of our Galaxy. The top-left inset shows a close-up of the Chandra -image of GRS 1915 , and the bottom-right inset shows the remarkable "heartbeats" -seen in the X-ray light from this system. Using Chandra and the Rossi X-ray -Timing Explorer (RXTE), astronomers have discovered what drives these heartbeats -and given new insight into the ways that black holes can regulate their intake -and severely curtail their growth. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-473L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-473.jpg -astropix_ids: chandra|473 - -credits> X-ray (NASA/CXC/Virginia/A.Reines et al); Radio (NRAO/AUI/NSF); Optical -(NASA/STScI) - ---- - -@scene -place_uuid: 19a5406e-286e-4b0c-825f-55eb4a15ae09 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-473L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2011/he210/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-473.jpg - -text> The combined observations from multiple telescopes of Henize 2-10, a dwarf -starburst galaxy located about 30 million light years from Earth, has provided -astronomers with a detailed new look at how galaxy and black hole formation may -have occured in the early Universe. This image shows optical data from the -Hubble Space Telescope in red, green and blue, X-ray data from NASA's Chandra -X-ray Observatory in purple, and radio data from the National Radio Astronomy -Observatory's Very Large Array in yellow. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-474L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-474.jpg -astropix_ids: chandra|474 - -credits> X-ray: NASA/CXC/MIT/S.Rappaport et al, Optical: NASA/STScI - ---- - -@scene -place_uuid: d8ef9fdb-f785-41af-bb7b-bfe4cd3639ad -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-474L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2011/arp147/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-474.jpg - -text> This composite image of Arp 147, a pair of interacting galaxies located -about 430 million light years from Earth, shows X-rays from the NASA's Chandra -X-ray Observatory (pink) and optical data from the Hubble Space Telescope (red, -green, blue) produced by the Space Telescope Science Institute (STScI) in -Baltimore, MD. Arp 147 contains the remnant of a spiral galaxy that collided -with an elliptical galaxy. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-476L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-476.jpg -astropix_ids: chandra|476 - -credits> X-ray: NASA/CXC/UNAM/Ioffe/D.Page,P.Shternin et al; Optical: -NASA/STScI; Illustration: NASA/CXC/M.Weiss - ---- - -@scene -place_uuid: 8a8cc01c-8769-47ca-a7d5-e8a6f85cabc0 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-476L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2011/casa/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-476.jpg - -text> This composite image shows a beautiful X-ray and optical view of -Cassiopeia A (Cas A), a supernova remnant located in our Galaxy about 11,000 -light years away. These are the remains of a massive star that exploded about -330 years ago, as measured in Earth's time frame. X-rays from Chandra are shown -in red, green and blue along with optical data from Hubble in gold. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-477L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-477.jpg -astropix_ids: chandra|477 - -credits> X-ray: NASA/CXC/CfA/J.Wang et al.; Optical: Isaac Newton Group of -Telescopes, La Palma/Jacobus Kapteyn Telescope, Radio: NSF/NRAO/VLA - ---- - -@scene -place_uuid: 65571ab7-1b26-4ffe-bdbf-f8bfa6693790 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-477L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2011/n4151/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-477.jpg - -text> This composite image shows the central region of the spiral galaxy NGC -4151, dubbed the "Eye of Sauron" by astronomers for its similarity to the eye of -the malevolent character in "The Lord of the Rings". In the "pupil" of the eye, -X-rays (blue) from the Chandra X-ray Observatory are combined with optical data -(yellow) showing positively charged hydrogen ("H II") from observations with the -1-meter Jacobus Kapteyn Telescope on La Palma. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-478L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-478.jpg -astropix_ids: chandra|478 - -credits> X-ray: NASA/CXC/Rutgers/K.Eriksen et al.; Optical: DSS - ---- - -@scene -place_uuid: 551e84c1-9212-4af0-a725-4b6f10e148a0 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-478L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2011/tycho/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-478.jpg - -text> This image comes from a very deep Chandra observation of the Tycho -supernova remnant, produced by the explosion of a white dwarf star in our -Galaxy. Low-energy X-rays (red) in the image show expanding debris from the -supernova explosion and high energy X-rays (blue) show the blast wave, a shell -of extremely energetic electrons. These high-energy X-rays show a pattern of -X-ray "stripes" never previously seen in a supernova remnant. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-479L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-479.jpg -astropix_ids: chandra|479 - -credits> NASA/CXC/Warwick/A.Levan et al. - ---- - -@scene -place_uuid: 7dbfa8db-78b1-404f-af00-f97496360d75 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-479L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2011/grb110328/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-479.jpg - -text> The center of this image contains an extraordinary gamma-ray burst (GRB) -called GRB 110328A, observed with NASA's Chandra X-ray Observatory. This Chandra -observation confirms the association of GRB 110328A with the core of a distant -galaxy and shows that it was an exceptionally long lived and luminous event -compared to other GRBs. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-480L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-480.jpg -astropix_ids: chandra|480 - -credits> X-ray: NASA/U. of Sydney/G.Anderson et al; IR: NASA/JPL-Caltech - ---- - -@scene -place_uuid: 5dee1085-aae8-494a-b197-626f4fb90fc4 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-480L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2011/massive/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-480.jpg - -text> Like looking for Easter eggs in a lawn of long grass, the hunt for the -Milky Way's most massive stars takes persistence and sharp eyes. In their -stellar search through our Galactic backyard, astronomers have used powerful -telescopes sensitive to X-ray and infrared radiation to find evidence for a -substantial population of X-ray emitting massive stars. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-481L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-481.jpg -astropix_ids: chandra|481 - -credits> NASA/CXC/Chinese Academy of Sciences/F. Lu et al. - ---- - -@scene -place_uuid: 78fedc1b-453d-4e33-baeb-f0b307f0631b -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-481L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2011/tycho2/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-481.jpg - -text> This new image of Tycho's supernova remnant, dubbed Tycho for short, -contains striking new evidence for what triggered the original supernova -explosion, as seen from Earth in 1572. Tycho was formed by a Type Ia supernova, -a category of stellar explosion used in measuring astronomical distances because -of their reliable brightness. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-483L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-483.jpg -astropix_ids: chandra|483 - -credits> NASA/CXC/PSU/L.Townsley et al. - ---- - -@scene -place_uuid: cce0525c-4d04-4c45-bd77-b0252f9088c8 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-483L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2011/carina/more.html#img1c -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-483.jpg - -text> This Chandra image is 22 separate pointings of the telescope that have -been stitched together to look at the famous Carina Nebula like never before. In -this image, low, medium, and high-energy X-rays are colored red, green, and blue -respectively. Chandra detected over 14,000 stars in this region, revealed a -diffuse X-ray glow, and provided strong evidence that massive stars have already -self-destructed in this nearby supernova factory. The Carina Nebula is one of -the best places in the Milky Way to study how young and massive stars live and -die. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-484L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-484.jpg -astropix_ids: chandra|484 - -credits> X-ray: NASA/CXC/U.Hawaii/E.Treister et al; Infrared: NASA/STScI/UC -Santa Cruz/G.Illingworth et al; Optical: NASA/STScI/S.Beckwith et al - ---- - -@scene -place_uuid: 8461475c-4078-4e8b-865a-9c9ec39fd13c -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-484L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2011/cdfs/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-484.jpg - -text> This composite image from NASA's Chandra X-ray Observatory and Hubble -Space Telescope (HST) combines the deepest X-ray, optical and infrared views of -the sky. Astronomers obtained what is known as the Chandra Deep Field South -(CDFS) by pointing the telescope at the same patch of sky for over six weeks of -time. The composite image shows a small section of the CDFS, where the Chandra -sources are blue, the optical HST data are shown in green and blue, and the -infrared data from Hubble are in red and green. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-485L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-485.jpg -astropix_ids: chandra|485 - -credits> X-ray: NASA/CXC/ITA/INAF/J.Merten et al, Lensing: NASA/STScI; -NAOJ/Subaru; ESO/VLT, Optical: NASA/STScI/R.Dupke - ---- - -@scene -place_uuid: 601ecafb-1632-4f18-8c56-73b5e3709192 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-485L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2011/a2744/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-485.jpg - -text> One of the most complicated and dramatic collisions between galaxy -clusters ever seen is captured in this new composite image. This collision site, -known officially as Abell 2744, has been dubbed "Pandora's Cluster" because of -the wide variety of different structures seen. Data from NASA's Chandra X-ray -Observatory are colored red, showing gas with temperatures of millions of -degrees. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-486L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-486.jpg -astropix_ids: chandra|486 - -credits> X-ray: NASA/CXC/IUSS/A.De Luca et al; Optical: DSS - ---- - -@scene -place_uuid: 6f84278a-8539-42a1-92e6-55ec76258068 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-486L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2011/psrj0357/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-486.jpg - -text> A spinning neutron star is tied to a mysterious tail - or so it seems. -Astronomers using NASA's Chandra X-ray Observatory have found that this pulsar, -known as PSR J0357+3205 (or PSR J0357 for short), apparently has a long, X-ray -bright tail streaming away from it. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-487L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-487.jpg -astropix_ids: chandra|487 - -credits> X-ray: NASA/CXC/Univ. of Alabama/K.Wong et al, Optical: ESO/VLT - ---- - -@scene -place_uuid: 82a27eb0-9692-48ea-a5b2-0f40b32fe264 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-487L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2011/n3115/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-487.jpg - -text> The galaxy NGC 3115 is shown here in a composite image of data from NASA's -Chandra X-ray Observatory and the European Southern Observatory's Very Large -Telescope (VLT). Using the Chandra image, the flow of hot gas toward the -supermassive black hole in the center of this galaxy has been imaged. This is -the first time that clear evidence for such a flow has been observed in any -black hole. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-488L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-488.jpg -astropix_ids: chandra|488 - -credits> X-ray NASA/CXC/IfA/D.Sanders et al; Optical NASA/STScI/NRAO/A.Evans et -al - ---- - -@scene -place_uuid: b6bdc127-362a-497d-9ef6-32a6191b1018 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-488L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2011/vv340/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-488.jpg - -text> VV 340, also known as Arp 302, provides a textbook example of colliding -galaxies seen in the early stages of their interaction. The edge-on galaxy near -the top of the image is VV 340 North and the face-on galaxy at the bottom of the -image is VV 340 South. Millions of years later these two spirals will merge — -much like the Milky Way and Andromeda will likely do billions of years from now. -Data from NASA's Chandra X-ray Observatory (purple) are shown here along with -optical data from the Hubble Space Telescope (red, green, blue). VV 340 is -located about 450 million light years from Earth. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-489L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-489.jpg -astropix_ids: chandra|489 - -credits> X-ray: NASA/CXC/SAO/G.Fabbiano et al; Optical: NASA/STScI - ---- - -@scene -place_uuid: ec2b9585-5971-4906-9d62-0f18e1b3893f -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-489L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2011/n3393/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-489.jpg - -text> Evidence for a pair of supermassive black holes in a spiral galaxy has -been found in data from NASA's Chandra X-ray Observatory. This main image is a -composite of X-rays from Chandra (blue) and optical data from the Hubble Space -Telescope (gold) of the spiral galaxy NGC 3393. Meanwhile, the inset box shows -the central region of NGC 3993 as observed just by Chandra. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-491L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-491.jpg -astropix_ids: chandra|491 - -credits> X-ray: NASA/CXC/CfA/S.Wolk; IR: NASA/JPL/CfA/S.Wolk - ---- - -@scene -place_uuid: 392352c2-fa94-4dbe-9d4d-2724fdf74de3 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-491L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2011/ngc281/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-491.jpg - -text> High-mass stars are important because they are responsible for much of the -energy pumped into our galaxy over its lifetime. Unfortunately, these stars are -poorly understood because they are often found relatively far away and can be -obscured by gas and dust. The star cluster NGC 281 is an exception to this rule. -It is located about 9,200 light years from Earth and, remarkably, almost 1,000 -light years above the plane of the Galaxy, giving astronomers a nearly -unfettered view of the star formation within it. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-492L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-492.jpg -astropix_ids: chandra|492 - -credits> X-ray: NASA/CXC/U. Texas at Arlington/S.Park et al, ROSAT; Infrared: -2MASS/UMass/IPAC-Caltech/NASA/NSF - ---- - -@scene -place_uuid: 82c1feb7-d388-45a8-9840-1976d7ffcb42 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-492L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2011/g299/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-492.jpg - -text> G299.2-2.9 is an intriguing supernova remnant found about 16,000 light -years away in the Milky Way galaxy. Evidence points to G299.2-2.9 being the -remains of a Type Ia supernova, where a white dwarf has grown sufficiently -massive to cause a thermonuclear explosion. Because it is older than most -supernova remnants caused by these explosions, at an age of about 4500 years, -G299.2-2.9 provides astronomers with an excellent opportunity to study how these -objects evolve over time. It also provides a probe of the Type Ia supernova -explosion that produced this structure. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-494L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-494.jpg -astropix_ids: chandra|494 - -credits> X-ray: NASA/CXC/SAO & ESA; Infared: NASA/JPL-Caltech/B. Williams (NCSU) - ---- - -@scene -place_uuid: 5fc6778d-612b-4077-96ae-c303df6fdd68 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-494L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2011/rcw86/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-494.jpg - -text> This image combines data from four different space telescopes to create a -multi-wavelength view of all that remains of the oldest documented example of a -supernova, called RCW 86. The Chinese witnessed the event in 185 A.D., -documenting a mysterious "guest star" that remained in the sky for eight months. -X-ray images from NASA's Chandra X-ray Observatory and the European Space -Agency's XMM-Newton Observatory are combined to form the blue and green colors -in the image. The X-rays show the interstellar gas that has been heated to -millions of degrees by the passage of the shock wave from the supernova. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-495L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-495.jpg -astropix_ids: chandra|495 - -credits> X-ray: NASA/CXC/PSU/L.Townsley et al.; Infrared: NASA/JPL/PSU/L.Townsley et al. - ---- - -@scene -place_uuid: 19d149aa-0183-4d66-8ca1-8b0419050fe5 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-495L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2011/30dor/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-495.jpg - -text> The star-forming region, 30 Doradus, is one of the largest located close -to the Milky Way and is found in the neighboring galaxy Large Magellanic Cloud. -About 2,400 massive stars in the center of 30 Doradus, also known as the -Tarantula Nebula, are producing intense radiation and powerful winds as they -blow off material. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-497L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-497.jpg -astropix_ids: chandra|497 - -credits> X-ray: NASA/CXC/BU/E.Blanton; Optical: ESO/VLT - ---- - -@scene -place_uuid: 6fdede50-fa87-4191-8bcc-533713fa7206 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-497L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2011/a2052/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-497.jpg - -text> Like wine in a glass, vast clouds of hot gas are sloshing back and forth -in Abell 2052, a galaxy cluster located about 480 million light years from -Earth. X-ray data (blue) from NASA's Chandra X-ray Observatory shows the hot gas -in this dynamic system, and optical data (gold) from the Very Large Telescope -shows the galaxies. The hot, X-ray bright gas has an average temperature of -about 30 million degrees. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-498L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-498.jpg -astropix_ids: chandra|498 - -credits> X-ray: NASA/CXC/Univ.Potsdam/L.Oskinova et al & ESA/XMM-Newton; Optical: AURA/NOAO/CTIO/Univ.Potsdam/L.Oskinova et al - ---- - -@scene -place_uuid: 64314825-092c-4925-a492-233d5f65f533 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-498L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2011/sxp1062/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-498.jpg - -text> Data from NASA's Chandra X-ray Observatory and ESA's XMM-Newton have been -combined to discover a young pulsar in the remains of a supernova located in the -Small Magellanic Cloud, or SMC. This would be the first definite time a pulsar, -a spinning, ultra-dense star, has been found in a supernova remnant in the SMC, -a small satellite galaxy to the Milky Way. The pulsar, known as SXP 1062, is the -bright white source located on the right-hand side of the image in the middle of -the diffuse blue emission inside a red shell. - ---- - @image url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-499L{1}X{2}Y{3}.png copyright: Public domain diff --git a/imagesets/sky__visible.xml b/imagesets/sky__visible.xml index 2dc35ce..f1aab45 100644 --- a/imagesets/sky__visible.xml +++ b/imagesets/sky__visible.xml @@ -50612,7 +50612,7 @@ powers the dramatic activity seen by... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-471L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|471" - Xcxstatus="queue:chandra" + Xcxstatus="in:66c4a0db01d08292018533b5" > NASA/CXC/Wesleyan/R.Kilgard et a; M82 is a galaxy where stars are forming at rates that are tens or even hundreds of times higher than in a normal galaxy. In this... https://chandra.harvard.edu/photo/2011/m82/ @@ -50638,7 +50638,7 @@ powers the dramatic activity seen by... TileLevels="4" Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-472L{1}X{2}Y{3}.png" WidthFactor="1" - Xcxstatus="queue:chandra" + Xcxstatus="in:66c4a0dc01d08292018533b7" > X-ray (NASA/CXC/Harvard/J.Neilsen et al); Optical (Palomar DSS2) https://chandra.harvard.edu/photo/2011/g1915/ @@ -50665,7 +50665,7 @@ powers the dramatic activity seen by... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-473L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|473" - Xcxstatus="queue:chandra" + Xcxstatus="in:66c4a0dd01d08292018533b9" > X-ray (NASA/CXC/Virginia/A.Reine; Combined observations from Chandra (purple), the Very Large Array (yellow) along with Hubble (red, green, and blue) have provide... https://chandra.harvard.edu/photo/2011/he210/ @@ -50692,7 +50692,7 @@ powers the dramatic activity seen by... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-474L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|474" - Xcxstatus="queue:chandra" + Xcxstatus="in:66c4a0de01d08292018533bb" > X-ray: NASA/CXC/MIT/S.Rappaport et al, Optical: NASA/STScI https://chandra.harvard.edu/photo/2011/arp147/ @@ -50719,7 +50719,7 @@ powers the dramatic activity seen by... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-476L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|476" - Xcxstatus="queue:chandra" + Xcxstatus="in:66c4a0df01d08292018533bd" > X-ray: NASA/CXC/UNAM/Ioffe/D.Page,P.Shternin et al; Optical: NASA/STScI; Illustration: NASA/CXC/M.Weiss https://chandra.harvard.edu/photo/2011/casa/ @@ -50746,7 +50746,7 @@ powers the dramatic activity seen by... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-477L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|477" - Xcxstatus="queue:chandra" + Xcxstatus="in:66c4a0e001d08292018533bf" > X-ray: NASA/CXC/CfA/J.Wang et al.; Optical: Isaac Newton Group of Telescopes, La Palma/Jacobus Kapteyn Telescope, Radio: NSF/NRAO/VLA https://chandra.harvard.edu/photo/2011/n4151/ @@ -50773,7 +50773,7 @@ powers the dramatic activity seen by... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-478L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|478" - Xcxstatus="queue:chandra" + Xcxstatus="in:66c4a0e101d08292018533c1" > X-ray: NASA/CXC/Rutgers/K.Erikse; A long Chandra observation of Tycho has revealed a pattern of X-ray stripes never seen before in a supernova remnant. The @@ -50802,7 +50802,7 @@ s... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-479L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|479" - Xcxstatus="queue:chandra" + Xcxstatus="in:66c4a0e201d08292018533c3" > NASA/CXC/Warwick/A.Levan et al.; The center of this image contains an extraordinary gamma-ray burst (GRB 110328A) observed with Chandra. The burst was first seen... https://chandra.harvard.edu/photo/2011/grb110328/ @@ -50829,7 +50829,7 @@ s... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-480L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|480" - Xcxstatus="queue:chandra" + Xcxstatus="in:66c4a0e301d08292018533c5" > X-ray: NASA/U. of Sydney/G.Ander; Data from Chandra and Spitzer of a region near the Galactic plane have been combined to track down some of the Milky Way's @@ -50858,7 +50858,7 @@ h... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-481L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|481" - Xcxstatus="queue:chandra" + Xcxstatus="in:66c4a0e401d08292018533c7" > NASA/CXC/Chinese Academy of Scie; This Chandra image of the Tycho supernova remnant contains new evidence for what triggered the original supernova explosion. Ty... https://chandra.harvard.edu/photo/2011/tycho2/ @@ -50912,7 +50912,7 @@ h... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-483L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|483" - Xcxstatus="queue:chandra" + Xcxstatus="in:66c4a0e501d08292018533c9" > NASA/CXC/PSU/L.Townsley et al. https://chandra.harvard.edu/photo/2011/carina/more.html#img1c @@ -50939,7 +50939,7 @@ h... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-484L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|484" - Xcxstatus="queue:chandra" + Xcxstatus="in:66c4a0e601d08292018533cb" > X-ray: NASA/CXC/U.Hawaii/E.Treis; This composite image combines the deepest X-ray image ever taken with optical and infrared data from Hubble. Astronomers obtain... https://chandra.harvard.edu/photo/2011/cdfs/ @@ -50966,7 +50966,7 @@ h... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-485L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|485" - Xcxstatus="queue:chandra" + Xcxstatus="in:66c4a0e701d08292018533cd" > X-ray: NASA/CXC/ITA/INAF/J.Merte; This composite image features one of the most complicated and dramatic collisions between galaxy clusters ever seen. Known off... https://chandra.harvard.edu/photo/2011/a2744/ @@ -50993,7 +50993,7 @@ h... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-486L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|486" - Xcxstatus="queue:chandra" + Xcxstatus="in:66c4a0e801d08292018533cf" > X-ray: NASA/CXC/IUSS/A.De Luca e; Astronomers using Chandra have found evidence for a possible long, X- ray bright tail extending from the pulsar called PSR J0357... https://chandra.harvard.edu/photo/2011/psrj0357/ @@ -51020,7 +51020,7 @@ h... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-487L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|487" - Xcxstatus="queue:chandra" + Xcxstatus="in:66c4a0e901d08292018533d1" > X-ray: NASA/CXC/Univ. of Alabama; This composite image contains X-rays from Chandra (blue) and optical data from the VLT (gold) of the galaxy NGC 3115. Using the... https://chandra.harvard.edu/photo/2011/n3115/ @@ -51047,7 +51047,7 @@ h... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-488L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|488" - Xcxstatus="queue:chandra" + Xcxstatus="in:66c4a0ea01d08292018533d3" > X-ray NASA/CXC/IfA/D.Sanders et ; This composite image of VV 340 contains X-ray data from Chandra (purple) and optical data from Hubble (red, green, blue). The tw... @@ -51075,7 +51075,7 @@ and optical data from Hubble (red, green, blue). The tw... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-489L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|489" - Xcxstatus="queue:chandra" + Xcxstatus="in:66c4a0eb01d08292018533d5" > X-ray: NASA/CXC/SAO/G.Fabbiano e; Evidence for a pair of supermassive black holes in a spiral galaxy has been found in data from NASA's Chandra X-ray Observator... @@ -51103,7 +51103,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-491L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|491" - Xcxstatus="queue:chandra" + Xcxstatus="in:66c4a0ec01d08292018533d7" > X-ray: NASA/CXC/CfA/S.Wolk; IR: ; This composite image of NGC 281 contains X-ray data from Chandra (purple) with infrared observations from Spitzer (red, green, b... https://chandra.harvard.edu/photo/2011/ngc281/ @@ -51130,7 +51130,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-492L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|492" - Xcxstatus="queue:chandra" + Xcxstatus="in:66c4a0ed01d08292018533d9" > X-ray: NASA/CXC/U. Texas at Arlington/S.Park et al, ROSAT; Infrared: 2MASS/UMass/IPAC-Caltech/NASA/NSF https://chandra.harvard.edu/photo/2011/g299/ @@ -51157,7 +51157,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-494L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|494" - Xcxstatus="queue:chandra" + Xcxstatus="in:66c4a0ed01d08292018533db" > NASA/JPL-Caltech/B. Williams (NC; This image combines data from four different space telescopes to create a multi-wavelength view of all that remains of the oldes... https://chandra.harvard.edu/photo/2011/rcw86/ @@ -51184,7 +51184,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-495L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|495" - Xcxstatus="queue:chandra" + Xcxstatus="in:66c4a0ee01d08292018533dd" > X-ray: NASA/CXC/PSU/L.Townsley e; About 2,400 massive stars in the center of 30 Doradus are producing intense radiation and powerful winds as they blow off materi... https://chandra.harvard.edu/photo/2011/30dor/ @@ -51211,7 +51211,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-497L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|497" - Xcxstatus="queue:chandra" + Xcxstatus="in:66c4a0ef01d08292018533df" > X-ray: NASA/CXC/BU/E.Blanton; Optical: ESO/VLT https://chandra.harvard.edu/photo/2011/a2052/ @@ -51238,7 +51238,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-498L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|498" - Xcxstatus="queue:chandra" + Xcxstatus="in:66c4a0f001d08292018533e1" > X-ray & Optical: NASA/CXC/Univ.P; In this composite image, X-rays from Chandra and XMM-Newton (blue) have been combined with optical data from the Cerro Tololo In... https://chandra.harvard.edu/photo/2011/sxp1062/ diff --git a/places/sky_ra00.yml b/places/sky_ra00.yml index b8c82e7..3866825 100644 --- a/places/sky_ra00.yml +++ b/places/sky_ra00.yml @@ -1679,8 +1679,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-454.jpg zoom_level: 3.49970317312 --- _uuid: 551e84c1-9212-4af0-a725-4b6f10e148a0 +astropix_id: chandra|478 classification: '' constellation: CAS +cxstatus: in:66c4a0e101d08292018533c2 data_set_type: Sky dec_deg: 64.1385494 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-478L{1}X{2}Y{3}.png @@ -1690,8 +1692,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-478.jpg zoom_level: 1.444427087872 --- _uuid: 78fedc1b-453d-4e33-baeb-f0b307f0631b +astropix_id: chandra|481 classification: '' constellation: CAS +cxstatus: in:66c4a0e501d08292018533c8 data_set_type: Sky dec_deg: 64.1385494 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-481L{1}X{2}Y{3}.png @@ -1701,8 +1705,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-481.jpg zoom_level: 1.14109739941888 --- _uuid: 601ecafb-1632-4f18-8c56-73b5e3709192 +astropix_id: chandra|485 classification: '' constellation: SCL +cxstatus: in:66c4a0e701d08292018533ce data_set_type: Sky dec_deg: -30.3998433 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-485L{1}X{2}Y{3}.png @@ -1712,8 +1718,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-485.jpg zoom_level: 0.509527588864 --- _uuid: 392352c2-fa94-4dbe-9d4d-2724fdf74de3 +astropix_id: chandra|491 classification: '' constellation: CAS +cxstatus: in:66c4a0ec01d08292018533d8 data_set_type: Sky dec_deg: 56.594963 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-491L{1}X{2}Y{3}.png diff --git a/places/sky_ra01.yml b/places/sky_ra01.yml index 2bedfc4..82e1084 100644 --- a/places/sky_ra01.yml +++ b/places/sky_ra01.yml @@ -1222,8 +1222,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-431.jpg zoom_level: 0.216174788608 --- _uuid: 64314825-092c-4925-a492-233d5f65f533 +astropix_id: chandra|498 classification: '' constellation: HYI +cxstatus: in:66c4a0f101d08292018533e2 data_set_type: Sky dec_deg: -73.5513431 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-498L{1}X{2}Y{3}.png diff --git a/places/sky_ra03.yml b/places/sky_ra03.yml index 9485d14..bcee267 100644 --- a/places/sky_ra03.yml +++ b/places/sky_ra03.yml @@ -1883,8 +1883,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-443.jpg zoom_level: 0.2320171008 --- _uuid: d8ef9fdb-f785-41af-bb7b-bfe4cd3639ad +astropix_id: chandra|474 classification: '' constellation: CET +cxstatus: in:66c4a0de01d08292018533bc data_set_type: Sky dec_deg: 1.3143841 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-474L{1}X{2}Y{3}.png @@ -1894,8 +1896,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-474.jpg zoom_level: 0.0680777465856 --- _uuid: 8461475c-4078-4e8b-865a-9c9ec39fd13c +astropix_id: chandra|484 classification: '' constellation: FOR +cxstatus: in:66c4a0e601d08292018533cc data_set_type: Sky dec_deg: -27.7828073 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-484L{1}X{2}Y{3}.png @@ -1905,8 +1909,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-484.jpg zoom_level: 0.166325247363728 --- _uuid: 6f84278a-8539-42a1-92e6-55ec76258068 +astropix_id: chandra|486 classification: '' constellation: PER +cxstatus: in:66c4a0e801d08292018533d0 data_set_type: Sky dec_deg: 32.0168478 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-486L{1}X{2}Y{3}.png diff --git a/places/sky_ra05.yml b/places/sky_ra05.yml index 5e48701..185a0c6 100644 --- a/places/sky_ra05.yml +++ b/places/sky_ra05.yml @@ -4686,8 +4686,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-482.jpg zoom_level: 0.234100297728 --- _uuid: 19d149aa-0183-4d66-8ca1-8b0419050fe5 +astropix_id: chandra|495 classification: '' constellation: DOR +cxstatus: in:66c4a0ef01d08292018533de data_set_type: Sky dec_deg: -69.0833858 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-495L{1}X{2}Y{3}.png diff --git a/places/sky_ra08.yml b/places/sky_ra08.yml index 6da45cb..a4e3266 100644 --- a/places/sky_ra08.yml +++ b/places/sky_ra08.yml @@ -538,8 +538,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-470.jpg zoom_level: 1.40640760004877 --- _uuid: 19a5406e-286e-4b0c-825f-55eb4a15ae09 +astropix_id: chandra|473 classification: '' constellation: PYX +cxstatus: in:66c4a0dd01d08292018533ba data_set_type: Sky dec_deg: -26.4094457 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-473L{1}X{2}Y{3}.png diff --git a/places/sky_ra09.yml b/places/sky_ra09.yml index 6b35d63..54412ba 100644 --- a/places/sky_ra09.yml +++ b/places/sky_ra09.yml @@ -715,8 +715,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-434.jpg zoom_level: 0.748183552 --- _uuid: 8d3ca8d9-de93-4e6d-bead-583c6ec457c4 +astropix_id: chandra|471 classification: '' constellation: UMA +cxstatus: in:66c4a0db01d08292018533b6 data_set_type: Sky dec_deg: 69.6810899 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-471L{1}X{2}Y{3}.png diff --git a/places/sky_ra10.yml b/places/sky_ra10.yml index 6b3427b..d06eb6d 100644 --- a/places/sky_ra10.yml +++ b/places/sky_ra10.yml @@ -1561,8 +1561,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-456.jpg zoom_level: 0.0569144344576 --- _uuid: cce0525c-4d04-4c45-bd77-b0252f9088c8 +astropix_id: chandra|483 classification: '' constellation: CAR +cxstatus: in:66c4a0e501d08292018533ca data_set_type: Sky dec_deg: -59.7809334 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-483L{1}X{2}Y{3}.png @@ -1572,8 +1574,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-483.jpg zoom_level: 7.7107265536 --- _uuid: 82a27eb0-9692-48ea-a5b2-0f40b32fe264 +astropix_id: chandra|487 classification: '' constellation: SEX +cxstatus: in:66c4a0e901d08292018533d2 data_set_type: Sky dec_deg: -7.7205183 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-487L{1}X{2}Y{3}.png @@ -1583,8 +1587,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-487.jpg zoom_level: 0.567366664192 --- _uuid: ec2b9585-5971-4906-9d62-0f18e1b3893f +astropix_id: chandra|489 classification: '' constellation: HYA +cxstatus: in:66c4a0eb01d08292018533d6 data_set_type: Sky dec_deg: -25.1619389 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-489L{1}X{2}Y{3}.png diff --git a/places/sky_ra12.yml b/places/sky_ra12.yml index 2ddfd20..a777770 100644 --- a/places/sky_ra12.yml +++ b/places/sky_ra12.yml @@ -2815,8 +2815,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-467.jpg zoom_level: 0.390792511488 --- _uuid: 65571ab7-1b26-4ffe-bdbf-f8bfa6693790 +astropix_id: chandra|477 classification: '' constellation: CVN +cxstatus: in:66c4a0e001d08292018533c0 data_set_type: Sky dec_deg: 39.4049255 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-477L{1}X{2}Y{3}.png @@ -2826,8 +2828,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-477.jpg zoom_level: 0.232862498816 --- _uuid: 82c1feb7-d388-45a8-9840-1976d7ffcb42 +astropix_id: chandra|492 classification: '' constellation: MUS +cxstatus: in:66c4a0ed01d08292018533da data_set_type: Sky dec_deg: -65.479819 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-492L{1}X{2}Y{3}.png diff --git a/places/sky_ra14.yml b/places/sky_ra14.yml index 42568e6..6828c0b 100644 --- a/places/sky_ra14.yml +++ b/places/sky_ra14.yml @@ -875,8 +875,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-425.jpg zoom_level: 0.074936795136 --- _uuid: 5dee1085-aae8-494a-b197-626f4fb90fc4 +astropix_id: chandra|480 classification: '' constellation: CIR +cxstatus: in:66c4a0e401d08292018533c6 data_set_type: Sky dec_deg: -59.4327751 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-480L{1}X{2}Y{3}.png @@ -886,8 +888,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-480.jpg zoom_level: 2.47102783488 --- _uuid: b6bdc127-362a-497d-9ef6-32a6191b1018 +astropix_id: chandra|488 classification: '' constellation: BOO +cxstatus: in:66c4a0ea01d08292018533d4 data_set_type: Sky dec_deg: 24.6131728 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-488L{1}X{2}Y{3}.png @@ -897,8 +901,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-488.jpg zoom_level: 0.167625392128 --- _uuid: 5fc6778d-612b-4077-96ae-c303df6fdd68 +astropix_id: chandra|494 classification: '' constellation: CIR +cxstatus: in:66c4a0ee01d08292018533dc data_set_type: Sky dec_deg: -62.4631333802834 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-494L{1}X{2}Y{3}.png diff --git a/places/sky_ra15.yml b/places/sky_ra15.yml index 7dacda2..ebfe7c1 100644 --- a/places/sky_ra15.yml +++ b/places/sky_ra15.yml @@ -472,8 +472,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-468.jpg zoom_level: 0.894903451648 --- _uuid: 6fdede50-fa87-4191-8bcc-533713fa7206 +astropix_id: chandra|497 classification: '' constellation: SER1 +cxstatus: in:66c4a0f001d08292018533e0 data_set_type: Sky dec_deg: 7.0215835 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-497L{1}X{2}Y{3}.png diff --git a/places/sky_ra16.yml b/places/sky_ra16.yml index 34d5835..5262738 100644 --- a/places/sky_ra16.yml +++ b/places/sky_ra16.yml @@ -1340,8 +1340,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-458.jpg zoom_level: 1.19196168415418 --- _uuid: 7dbfa8db-78b1-404f-af00-f97496360d75 +astropix_id: chandra|479 classification: '' constellation: DRA +cxstatus: in:66c4a0e201d08292018533c4 data_set_type: Sky dec_deg: 57.583278 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-479L{1}X{2}Y{3}.png diff --git a/places/sky_ra19.yml b/places/sky_ra19.yml index c509390..ed03886 100644 --- a/places/sky_ra19.yml +++ b/places/sky_ra19.yml @@ -1409,8 +1409,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-455.jpg zoom_level: 0.9076298612736 --- _uuid: a4f51693-38ce-43f1-b22d-28a2528c9dea +astropix_id: null classification: '' constellation: AQL +cxstatus: in:66c4a0dc01d08292018533b8 data_set_type: Sky dec_deg: 11.300081423 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-472L{1}X{2}Y{3}.png diff --git a/places/sky_ra23.yml b/places/sky_ra23.yml index 8abbdd8..6765876 100644 --- a/places/sky_ra23.yml +++ b/places/sky_ra23.yml @@ -1074,8 +1074,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-463.jpg zoom_level: 1.03486538621673 --- _uuid: 8a8cc01c-8769-47ca-a7d5-e8a6f85cabc0 +astropix_id: chandra|476 classification: '' constellation: CAS +cxstatus: in:66c4a0df01d08292018533be data_set_type: Sky dec_deg: 58.814723 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-476L{1}X{2}Y{3}.png