From 356d18285947dd9a4a838ba38698c49ef1a8670e Mon Sep 17 00:00:00 2001 From: Peter Williams Date: Wed, 25 Sep 2024 12:58:27 -0400 Subject: [PATCH 1/2] cxprep/chandra.txt: prepare 2014 images for registration --- cxprep/chandra.txt | 384 +++++++++++++++++++++++++-------------------- 1 file changed, 215 insertions(+), 169 deletions(-) diff --git a/cxprep/chandra.txt b/cxprep/chandra.txt index 4f5ec07..f73649d 100644 --- a/cxprep/chandra.txt +++ b/cxprep/chandra.txt @@ -6,11 +6,8 @@ license_id: CC-PDDC thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-548.jpg astropix_ids: chandra|548 -credits> X-ray: NASA/CXC/SAO/F.Seward et ; This composite image contains data -from Chandra (purple) that provides evidence for the survival of a companion -star from the bl... +credits> X-ray: NASA/CXC/SAO/F.Seward et al; Optical: NOAO/CTIO/MCELS, DSS -wip: yes --- @scene @@ -19,9 +16,13 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-548L{1}X{2}Y{3}.pn outgoing_url: https://chandra.harvard.edu/photo/2014/deml241/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-548.jpg -text> Image File +text> When a massive star runs out fuel, it collapses and explodes as a +supernova. Although these explosions are extremely powerful, it is possible for +a companion star to endure the blast. A team of astronomers using NASA's Chandra +X-ray Observatory and other telescopes has found evidence for one of these +survivors. This hardy star is in a stellar explosion's debris field — also +called its supernova remnant — located in an HII region called DEM L241. -wip: yes --- @image @@ -31,10 +32,8 @@ license_id: CC-PDDC thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-559.jpg astropix_ids: chandra|559 -credits> redit: X-ray: NASA/CXC/Univ. of Alabama/W.P.Maksym et al & -NASA/CXC/GSFC/UMD/D.Donato, et al; Optical: CFHT. +credits> X-ray: NASA/CXC/Univ. of Alabama/W.P.Maksym et al & NASA/CXC/GSFC/UMD/D.Donato, et al; Optical: CFHT -wip: yes --- @scene @@ -43,9 +42,10 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-559L{1}X{2}Y{3}.pn outgoing_url: https://chandra.harvard.edu/photo/2014/a1795/more.html#img1a thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-559.jpg -text> Abell 1795 +text> A bright, long duration flare may be the first recorded event of a black +hole destroying a star in a dwarf galaxy. The dwarf galaxy is located in the +galaxy cluster Abell 1795, about 800 million light years from Earth. -wip: yes --- @image @@ -55,11 +55,8 @@ license_id: CC-PDDC thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-560.jpg astropix_ids: chandra|560 -credits> X-ray: NASA/CXC/Stanford/J.Hlava; Astronomers have used NASA's Chandra -X-ray Observatory and other telescopes to reveal one of the most powerful black -holes known... +credits> X-ray: NASA/CXC/Stanford/J.Hlavacek-Larrondo et al, Optical: NASA/ESA/STScI/M.Postman & CLASH team -wip: yes --- @scene @@ -68,9 +65,13 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-560L{1}X{2}Y{3}.pn outgoing_url: https://chandra.harvard.edu/photo/2014/rxj1532/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-560.jpg -text> Image File +text> Astronomers have used NASA's Chandra X-ray Observatory and a suite of +other telescopes to reveal one of the most powerful black holes known. The black +hole has created enormous structures in the hot gas surrounding it and prevented +trillions of stars from forming. The black hole is in a galaxy cluster named RX +J1532.9+3021 (RX J1532 for short), located about 3.9 billion light years from +Earth. -wip: yes --- @image @@ -80,11 +81,8 @@ license_id: CC-PDDC thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-561.jpg astropix_ids: chandra|561 -credits> X-ray: NASA/CXC/U.Birmingham/M.B; Centaurus A is a galaxy well known -for a gargantuan jet blasting away from a central supermassive black hole, which -is seen in t... +credits> X-ray: NASA/CXC/U.Birmingham/M.Burke et al. -wip: yes --- @scene @@ -93,9 +91,14 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-561L{1}X{2}Y{3}.pn outgoing_url: https://chandra.harvard.edu/photo/2014/cena/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-561.jpg -text> Centaurus A +text> This image of Centaurus A contains data from observations, equivalent to +over nine and a half days worth of time, taken between 1999 and 2012. In this +image, the lowest-energy X-rays Chandra detects are in red, while the +medium-energy X-rays are green, and the highest-energy ones are blue. As in all +of Chandra's images of Cen A, this one shows the spectacular jet of outflowing +material — seen pointing from the middle to the upper left — that is generated +by the giant black hole at the galaxy's center. -wip: yes --- @image @@ -105,11 +108,8 @@ license_id: CC-PDDC thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-562.jpg astropix_ids: chandra|562 -credits> X-ray: NASA/CXC/ISDC/L.Pavan et ; An extraordinary jet trailing behind -a runaway pulsar is seen in this composite image that contains X-ray data from -Chandra (pur... +credits> X-ray: NASA/CXC/ISDC/L.Pavan et al, Radio: CSIRO/ATNF/ATCA Optical: 2MASS/UMass/IPAC-Caltech/NASA/NSF -wip: yes --- @scene @@ -118,9 +118,13 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-562L{1}X{2}Y{3}.pn outgoing_url: https://chandra.harvard.edu/photo/2014/igrj11014/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-562.jpg -text> Image File +text> An extraordinary jet trailing behind a runaway pulsar is seen in this +composite image that contains data from NASA's Chandra X-ray Observatory +(purple), radio data from the Australia Compact Telescope Array (green), and +optical data from the 2MASS survey (red, green, and blue). The jet stretches for +37 light years, making it the longest ever seen from an object in the Milky Way +galaxy -wip: yes --- @image @@ -130,11 +134,8 @@ license_id: CC-PDDC thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-563.jpg astropix_ids: chandra|563 -credits> X-ray: NASA/CXC/Univ of Michigan; Multiple images of a distant quasar -known as RX J1131-1231 are visible in this combined view from Chandra (pink) and -Hubble (red... +credits> X-ray: NASA/CXC/Univ of Michigan/R.C.Reis et al; Optical: NASA/STScI -wip: yes --- @scene @@ -143,9 +144,11 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-563L{1}X{2}Y{3}.pn outgoing_url: https://chandra.harvard.edu/photo/2014/rxj1131/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-563.jpg -text> Image File +text> Multiple images of a distant quasar are visible in this combined view from +NASA's Chandra X-ray Observatory and the Hubble Space Telescope. The Chandra +data, along with data from ESA's XMM-Newton, were used to directly measure the +spin of the supermassive black hole powering this quasar. -wip: yes --- @image @@ -155,11 +158,8 @@ license_id: CC-PDDC thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-564.jpg astropix_ids: chandra|564,chandra|811c -credits> X-ray: NASA/CXC/UAH/M.Sun et al;; This image combines NASA/ESA Hubble -Space Telescope observations with data from the Chandra X-ray Observatory. As -well as the el... +credits> X-ray: NASA/CXC/UAH/M.Sun et al; Optical: NASA, ESA, & the Hubble Heritage Team (STScI/AURA) -wip: yes --- @scene @@ -168,9 +168,10 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-564L{1}X{2}Y{3}.pn outgoing_url: https://chandra.harvard.edu/photo/2014/eso137/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-564.jpg -text> ESO 137-001 +text> The spiral galaxy ESO 137-001 looks like a dandelion caught in a breeze in +this composite image from the Hubble Space Telescope and the Chandra X-ray +Observatory. -wip: yes --- @image @@ -185,7 +186,6 @@ Univ.), F. Menanteau (Rutgers Univ. & Univ. of Illinois, Urbana-Champaign), C. Sifon (Leiden Obs.), R. Mandelbum (Carnegie Mellon Univ.), L. Barrientos (Univ. Catolica de Chile), and K. Ng (Univ. of California, Davis) -wip: yes --- @scene @@ -194,9 +194,14 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-565L{1}X{2}Y{3}.pn outgoing_url: https://chandra.harvard.edu/photo/2014/elgordo/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-565.jpg -text> Image File +text> This is a composite image of X-rays from Chandra and optical data from +Hubble of the galaxy cluster ACT-CL J0102-4915, located about 7 billion light +years from Earth. This cluster has been nicknamed "El Gordo" (or, "the fat one" +in Spanish) because of its gigantic mass. Scientists first announced the +discovery of El Gordo with Chandra and ground-based optical telescopes in 2012. +They determined that El Gordo is the most massive, the hottest, and gives off +the most X-rays of any known galaxy cluster at its distance or beyond. -wip: yes --- @image @@ -206,11 +211,8 @@ license_id: CC-PDDC thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-566.jpg astropix_ids: chandra|566 -credits> X-ray: NASA/CXC/Morehead State U; Supernova remnants are created when a -massive star explodes and its remains are hurled into space. Astronomers have -found a supe... +credits> X-ray: NASA/CXC/Morehead State Univ/T.Pannuti et al.; Optical: DSS; Infrared: NASA/JPL-Caltech; Radio: NRAO/VLA/Argentinian Institute of Radioastronomy/G.Dubner -wip: yes --- @scene @@ -219,9 +221,11 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-566L{1}X{2}Y{3}.pn outgoing_url: https://chandra.harvard.edu/photo/2014/g352/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-566.jpg -text> Image File +text> The supernova remnant G352.7-0.1 (or, G352 for short) has swept up +material equivalent to about 45 times the mass of the Sun, as it expands. +Although this is not an exceptionally large amount, astronomers have found that +several other properties of the supernova remnant are unusual. -wip: yes --- @image @@ -231,11 +235,8 @@ license_id: CC-PDDC thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-568.jpg astropix_ids: chandra|568 -credits> X-ray: NASA/CXC/PSU/K.Getman, E.; Astronomers have studied two star -clusters to gain insight on how clusters of stars like our Sun form. This -composite image show... +credits> X-ray: NASA/CXC/PSU/K.Getman, E.Feigelson, M.Kuhn & the MYStIX team; Infrared:NASA/JPL-Caltech -wip: yes --- @scene @@ -244,9 +245,15 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-568L{1}X{2}Y{3}.pn outgoing_url: https://chandra.harvard.edu/photo/2014/flame/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-568.jpg -text> Flame Nebula +text> Stars are often born in clusters, in giant clouds of gas and dust. +Astronomers have studied two star clusters using NASA's Chandra X-ray +Observatory and infrared telescopes and the results show that the simplest ideas +for the birth of these clusters cannot work. This composite image shows one of +the clusters, NGC 2024, which is found in the center of the so-called Flame +Nebula about 1,400 light years from Earth. In this image, X-rays from Chandra +are seen as purple, while infrared data from NASA's Spitzer Space Telescope are +colored red, green, and blue. -wip: yes --- @image @@ -256,11 +263,8 @@ license_id: CC-PDDC thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-569.jpg astropix_ids: chandra|569 -credits> X-ray: NASA/CXC/Stanford Univ/N.; This four-panel of images represents -a sample of giant elliptical galaxies observed by Chandra and the Hershel Space -Observatory... +credits> X-ray: NASA/CXC/Stanford Univ/N.Werner et al. -wip: yes --- @scene @@ -269,9 +273,11 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-569L{1}X{2}Y{3}.pn outgoing_url: https://chandra.harvard.edu/photo/2014/coldgas/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-569.jpg -text> NGC 1399 +text> NASA's Chandra X-ray Observatory has shed new light on the mystery of why +giant elliptical galaxies (such as this one, NGC 1399) have few, if any, young +stars. This new evidence highlights the important role that supermassive black +holes play in the evolution of their host galaxies. -wip: yes --- @image @@ -282,7 +288,6 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-570.jpg credits> X-ray: NASA/CXC/Wesleyan Univ./R.Kilgard, et al; Optical: NASA/STScI -wip: yes --- @scene @@ -291,9 +296,15 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-570L{1}X{2}Y{3}.pn outgoing_url: https://chandra.harvard.edu/photo/2014/m51/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-570.jpg -text> Whirlpool Galaxy +text> Nearly a million seconds of observing time with NASA's Chandra X-ray +Observatory has revealed a spiral galaxy similar to the Milky Way glittering +with hundreds of X-ray points of light. The galaxy is officially named Messier +51 (M51) or NGC 5194, but often goes by its nickname of the "Whirlpool Galaxy." +Like the Milky Way, the Whirlpool is a spiral galaxy with spectacular arms of +stars and dust. M51 is located about 30 million light years from Earth, and its +face-on orientation to Earth gives us a perspective that we can never get of our +own spiral galactic home. This image combines X-ray and optical data. -wip: yes --- @image @@ -303,11 +314,8 @@ license_id: CC-PDDC thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-570a.jpg astropix_ids: chandra|570a -credits> X-ray: NASA/CXC/Wesleyan Univ./R; This image contains nearly a million -seconds worth of Chandra observing time (purple) along with optical data from -the Hubble Sp... +credits> X-ray: NASA/CXC/Wesleyan Univ./R.Kilgard, et al; Optical: NASA/STScI -wip: yes --- @scene @@ -316,9 +324,15 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-570aL{1}X{2}Y{3}.p outgoing_url: https://chandra.harvard.edu/photo/2014/m51/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-570a.jpg -text> Whirlpool Galaxy +text> Nearly a million seconds of observing time with NASA's Chandra X-ray +Observatory has revealed a spiral galaxy similar to the Milky Way glittering +with hundreds of X-ray points of light. The galaxy is officially named Messier +51 (M51) or NGC 5194, but often goes by its nickname of the "Whirlpool Galaxy." +Like the Milky Way, the Whirlpool is a spiral galaxy with spectacular arms of +stars and dust. M51 is located about 30 million light years from Earth, and its +face-on orientation to Earth gives us a perspective that we can never get of our +own spiral galactic home. This image shows X-ray data only. -wip: yes --- @image @@ -328,11 +342,8 @@ license_id: CC-PDDC thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-571.jpg astropix_ids: chandra|571 -credits> X-ray: NASA/CXC/SAO/E.Bulbul, e; A new study of the Perseus galaxy -cluster, shown in this image, and others using Chandra and XMM-Newton has -revealed a mysteriou... +credits> X-ray: NASA/CXC/SAO/E.Bulbul, et al. -wip: yes --- @scene @@ -341,9 +352,10 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-571L{1}X{2}Y{3}.pn outgoing_url: https://chandra.harvard.edu/photo/2014/perseus/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-571.jpg -text> Perseus A +text> A new study of the central region of the Perseus galaxy cluster, shown in +this image, using NASA's Chandra X-ray Observatory and 73 other clusters with +ESA's XMM-Newton has revealed a mysterious X-ray signal in the data. -wip: yes --- @image @@ -353,11 +365,8 @@ license_id: CC-PDDC thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-572.jpg astropix_ids: chandra|572 -credits> X-ray: NASA/CXC/Caltech/P.Ogle e; NGC 4258 is a spiral galaxy well -known to astronomers for having two so-called anomalous arms that glow in X-ray, -optical, and r... +credits> X-ray: NASA/CXC/Caltech/P.Ogle et al; Optical: NASA/STScI & R.Gendler; IR: NASA/JPL-Caltech; Radio: NSF/NRAO/VLA -wip: yes --- @scene @@ -366,9 +375,15 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-572L{1}X{2}Y{3}.pn outgoing_url: https://chandra.harvard.edu/photo/2014/m106/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-572.jpg -text> NGC 4258 (M106) +text> A galaxy about 23 million light years away is the site of impressive, +ongoing, fireworks. Rather than paper, powder, and fire, this galactic light +show involves a giant black hole, shock waves, and vast reservoirs of gas. This +galactic fireworks display is taking place in NGC 4258 (also known as M106), a +spiral galaxy like the Milky Way. This galaxy is famous, however, for something +that our Galaxy doesn't have — two extra spiral arms that glow in X-ray, +optical, and radio light. These features, or anomalous arms, are not aligned +with the plane of the galaxy, but instead intersect with it. -wip: yes --- @image @@ -378,11 +393,8 @@ license_id: CC-PDDC thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-576.jpg astropix_ids: chandra|576 -credits> NASA/CXC/SAO/R.Margutti et al; New Chandra data gives insight into the -explosion that produced SN 2014J, one of the closest supernovas discovered in -decades. ... +credits> NASA/CXC/SAO/R.Margutti et al -wip: yes --- @scene @@ -391,9 +403,14 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-576L{1}X{2}Y{3}.pn outgoing_url: https://chandra.harvard.edu/photo/2014/m82/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-576.jpg -text> M82 SN2014J +text> On January 21, 2014, astronomers witnessed a supernova soon after it +exploded in the Messier 82, or M82, galaxy. Telescopes across the globe and in +space turned their attention to study this newly exploded star, including +Chandra. Astronomers determined that this supernova, dubbed SN 2014J, belongs to +a class of explosions called "Type Ia" supernovas. These supernovas are used as +cosmic distance-markers and played a key role in the discovery of the Universe's +accelerated expansion, which has been attributed to the effects of dark energy. -wip: yes --- @image @@ -403,11 +420,8 @@ license_id: CC-PDDC thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-577.jpg astropix_ids: chandra|577 -credits> X-ray: NASA/CXC/IAFE/G.Dubner et; The destructive results of a powerful -supernova explosion are seen in a delicate tapestry of X-ray light in this new -image. The... +credits> X-ray: NASA/CXC/IAFE/G.Dubner et al & ESA/XMM-Newton -wip: yes --- @scene @@ -416,9 +430,13 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-577L{1}X{2}Y{3}.pn outgoing_url: https://chandra.harvard.edu/photo/2014/puppisa/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-577.jpg -text> Puppis A +text> The destructive results of a powerful supernova explosion reveal +themselves in a delicate tapestry of X-ray light, as seen in this image from +NASA's Chandra X-Ray Observatory and the European Space Agency's XMM-Newton. The +image shows the remains of a supernova that would have been witnessed on Earth +about 3,700 years ago. The remnant is called Puppis A, and is around 7,000 light +years away and about 100 light years across. -wip: yes --- @image @@ -430,7 +448,6 @@ astropix_ids: chandra|578 credits> NASA/CXC/GSFC/K.Hamaguchi, et al. -wip: yes --- @scene @@ -439,9 +456,11 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-578L{1}X{2}Y{3}.pn outgoing_url: https://chandra.harvard.edu/photo/2014/etacar/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-578.jpg -text> Eta Carinae +text> The Eta Carinae star system does not lack for superlatives. Not only does +it contain one of the biggest and brightest stars in our galaxy, weighing at +least 90 times the mass of the Sun, it is also extremely volatile and is +expected to have at least one supernova explosion in the future. -wip: yes --- @image @@ -451,11 +470,8 @@ license_id: CC-PDDC thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-580.jpg astropix_ids: chandra|580 -credits> X-ray: NASA/CXC/Univ. of Toulous; Ultraluminous X-ray Sources (ULXs) -are objects that produce more X-rays than most "normal" X-ray binary systems, in -which a star... +credits> X-ray: NASA/CXC/Univ. of Toulouse/M.Bachetti et al, Optical: NOAO/AURA/NSF -wip: yes --- @scene @@ -464,9 +480,12 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-580L{1}X{2}Y{3}.pn outgoing_url: https://chandra.harvard.edu/photo/2014/m82nu/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-580.jpg -text> M82X-2 +text> An Ultraluminous X-ray Source (ULX) that astronomers had thought was a +black hole is really the brightest pulsar ever recorded. ULXs are objects that +produce more X-rays than most "normal" X-ray binary systems, in which a star is +orbiting a neutron star or a stellar-mass black hole. Black holes in these X-ray +binary systems generally weigh about five to thirty times the mass of the sun. -wip: yes --- @image @@ -476,11 +495,8 @@ license_id: CC-PDDC thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-581a.jpg astropix_ids: chandra|581a -credits> X-ray: NASA/CXC/ESA-ESTEC/E.Wins; With the passing of Chandra's 15th -anniversary, the Chandra Data Archive, which houses all of the mission's data, -continues to g... +credits> X-ray: NASA/CXC/ESA-ESTEC/E.Winston et al, Near-IR: 2MASS/UMass/IPAC-Caltech/NASA/NSF, Infrared: NASA/JPL-Caltech -wip: yes --- @scene @@ -489,9 +505,15 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-581aL{1}X{2}Y{3}.p outgoing_url: https://chandra.harvard.edu/photo/2014/archives/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-581a.jpg -text> Image File +text> A young star cluster about 5,500 light years from Earth, RCW 38 provides +astronomers a chance to closely examine many young, rapidly evolving stars at +once. In this composite image, X-rays from Chandra are blue, while infrared data +from NASA's Spitzer Space Telescope are orange and additional infrared data from +the 2MASS survey appears white. There are many massive stars in RCW 38 that will +likely explode as supernovas. Astronomers studying RCW 38 are hoping to better +understand this environment as our Sun was likely born into a similar stellar +nursery. -wip: yes --- @image @@ -501,11 +523,8 @@ license_id: CC-PDDC thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-581c.jpg astropix_ids: chandra|581c -credits> X-ray: NASA/CXC/Univ. of Manitob; With the passing of Chandra's 15th -anniversary, the Chandra Data Archive, which houses all of the mission's data, -continues to g... +credits> X-ray: NASA/CXC/Univ. of Manitoba/H.Kumar et al, Optical: DSS, Infrared: NASA/JPL-Caltech, Radio: NSF/NRAO/VLA -wip: yes --- @scene @@ -514,9 +533,17 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-581cL{1}X{2}Y{3}.p outgoing_url: https://chandra.harvard.edu/photo/2014/archives/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-581c.jpg -text> Image File +text> The supernova remnant Kes 73, located about 28,000 light years away, +contains a so-called anomalous X-ray pulsar, or AXP, at its center. Astronomers +think that most AXPs are magnetars, which are neutron stars with ultra-high +magnetic fields. Surrounding the point-like AXP in the middle, Kes 73 has an +expanding shell of debris from the supernova explosion that occurred between +about 750 and 2100 years ago, as seen from Earth. The Chandra data (blue) reveal +clumpy structures along one side of the remnant, and appear to overlap with +infrared data (orange). The X-rays partially fill the shell seen in radio +emission (red) by the Very Large Array. Data from the Digitized Sky Survey +optical telescope (white) show stars in the field-of-view. -wip: yes --- @image @@ -526,11 +553,8 @@ license_id: CC-PDDC thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-581d.jpg astropix_ids: chandra|581d -credits> X-ray: NASA/CXC/SAO, Optical: NA; With the passing of Chandra's 15th -anniversary, the Chandra Data Archive, which houses all of the mission's data, -continues to g... +credits> X-ray: NASA/CXC/SAO, Optical: NASA/STScI, Radio: NSF/NRAO/VLA -wip: yes --- @scene @@ -539,9 +563,17 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-581dL{1}X{2}Y{3}.p outgoing_url: https://chandra.harvard.edu/photo/2014/archives/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-581d.jpg -text> Hercules A +text> Some galaxies have extremely bright cores, suggesting that they contain a +supermassive black hole that is pulling in matter at a prodigious rate. +Astronomers call these "active galaxies," and Hercules A is one of them. In +visible light (colored red, green and blue, with most objects appearing white), +Hercules A looks like a typical elliptical galaxy. In X-ray light, however, +Chandra detects a giant cloud of multimillion-degree gas (purple). This gas has +been heated by energy generated by the infall of matter into a black hole at the +center of Hercules A that is over 1,000 times as massive as the one in the +middle of the Milky Way. Radio data (blue) show jets of particles streaming away +from the black hole. The jets span a length of almost one million light years. -wip: yes --- @image @@ -551,11 +583,8 @@ license_id: CC-PDDC thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-581e.jpg astropix_ids: chandra|581e -credits> X-ray: NASA/CXC/SAO; Infared: NA; With the passing of Chandra's 15th -anniversary, the Chandra Data Archive, which houses all of the mission's data, -continues to g... +credits> X-ray: NASA/CXC/SAO; Infared: NASA/JPL-Caltech -wip: yes --- @scene @@ -564,9 +593,16 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-581eL{1}X{2}Y{3}.p outgoing_url: https://chandra.harvard.edu/photo/2014/archives/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-581e.jpg -text> PSR B1509-58 +text> Pareidolia is the psychological phenomenon where people see recognizable +shapes in clouds, rock formations, or otherwise unrelated objects or data. When +Chandra's image of PSR B1509-58, a spinning neutron star surrounded by a cloud +of energetic particles, was released in 2009, it quickly gained attention +because many saw a hand-like structure in the X-ray emission. In this new image +of the system, X-rays from Chandra in gold are seen along with infrared data +from NASA's Wide-field Infrared Survey Explorer (WISE) telescope in red, green, +and blue. Pareidolia may strike again in this image as some people report seeing +a shape of a face in WISE's infrared data. -wip: yes --- @image @@ -576,11 +612,8 @@ license_id: CC-PDDC thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-581f.jpg astropix_ids: chandra|581f -credits> X-ray: NASA/CXC/Universita di Bo; With the passing of Chandra's 15th -anniversary, the Chandra Data Archive, which houses all of the mission's data, -continues to g... +credits> X-ray: NASA/CXC/Universita di Bologna/S.Pellegrini et al, IR: NASA/JPL-Caltech; Optical: SDSS & NASA/STScI -wip: yes --- @scene @@ -589,9 +622,19 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-581fL{1}X{2}Y{3}.p outgoing_url: https://chandra.harvard.edu/photo/2014/archives/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-581f.jpg -text> Image File +text> NGC 4736 (also known as Messier 94) is a spiral galaxy that is unusual +because it has two ring structures. This galaxy is classified as containing a +"low ionization nuclear emission region," or LINER, in its center, which +produces radiation from specific elements such as oxygen and nitrogen. Chandra +observations (gold) of NGC 4736, seen in this composite image with infrared data +from Spitzer (red) and optical data from Hubble and the Sloan Digital Sky Survey +(blue), suggest that the X-ray emission comes from a recent burst of star +formation. Part of the evidence comes from the large number of point sources +near the center of the galaxy, showing that strong star formation has occurred. +In other galaxies, evidence points to supermassive black holes being responsible +for LINER properties. Chandra's result on NGC 4736 shows LINERs may represent +more than one physical phenomenon. -wip: yes --- @image @@ -601,11 +644,8 @@ license_id: CC-PDDC thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-582a.jpg astropix_ids: chandra|582a -credits> NASA/CXC/Stanford/I.Zhuravleva e; Chandra observations of the Perseus -and Virgo galaxy clusters have provided direct evidence that turbulence is -helping to preven... +credits> NASA/CXC/Stanford/I.Zhuravleva et al -wip: yes --- @scene @@ -614,9 +654,9 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-582aL{1}X{2}Y{3}.p outgoing_url: https://chandra.harvard.edu/photo/2014/perseusvirgo/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-582a.jpg -text> Image File +text> This Chandra image of the galaxy cluster known as Perseus has provided +direct evidence that turbulence is helping to prevent stars from forming. -wip: yes --- @image @@ -626,11 +666,8 @@ license_id: CC-PDDC thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-582b.jpg astropix_ids: chandra|582b -credits> NASA/CXC/Stanford/I.Zhuravleva e; Chandra observations of the Perseus -and Virgo galaxy clusters have provided direct evidence that turbulence is -helping to preven... +credits> NASA/CXC/Stanford/I.Zhuravleva et al -wip: yes --- @scene @@ -639,9 +676,9 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-582bL{1}X{2}Y{3}.p outgoing_url: https://chandra.harvard.edu/photo/2014/perseusvirgo/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-582b.jpg -text> Image File +text> This Chandra image of the galaxy cluster known as Virgo has provided +direct evidence that turbulence is helping to prevent stars from forming. -wip: yes --- @image @@ -651,11 +688,8 @@ license_id: CC-PDDC thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-583.jpg astropix_ids: chandra|583 -credits> NASA/CXC/Univ. of Wisconsin/Y.Ba; The supermassive black hole at the -center of the Milky Way may be producing tiny particles, called neutrinos, that -have virtuall... +credits> NASA/CXC/Univ. of Wisconsin/Y.Bai, et al. -wip: yes --- @scene @@ -664,9 +698,14 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-583L{1}X{2}Y{3}.pn outgoing_url: https://chandra.harvard.edu/photo/2014/sgra/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-583.jpg -text> Sgr A* +text> The supermassive black hole at the center of the Milky Way, seen in this +image from NASA's Chandra X-ray Observatory, may be producing mysterious +particles called neutrinos. Neutrinos are tiny particles that have virtually no +mass and carry no electric charge. Unlike light or charged particles, neutrinos +can emerge from deep within their sources and travel across the Universe without +being absorbed by intervening matter or, in the case of charged particles, +deflected by magnetic fields. -wip: yes --- @image @@ -676,11 +715,8 @@ license_id: CC-PDDC thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-584b.jpg astropix_ids: chandra|584b -credits> NASA/CXC/GSFC/T.Temim et al. ; A long observation with Chandra of the -supernova remnant MSH 11-62 reveals an irregular shell of hot gas, shown in red, -surround... +credits> NASA/CXC/GSFC/T.Temim et al. -wip: yes --- @scene @@ -689,9 +725,14 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-584bL{1}X{2}Y{3}.p outgoing_url: https://chandra.harvard.edu/photo/2014/msh11g327/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-584b.jpg -text> Image File +text> The supernova remnant G327.1-1.1, located about 29,000 light years from +Earth, is a spectacular debris field left behind when a massive star exploded. +The Chandra image of G327.1-1.1 shows the outward-moving, or forward, shock wave +(seen as the faint red color), and a bright pulsar wind nebula (blue). The +pulsar wind nebula appears to have been distorted by the combined action of the +reverse shock wave, which may have flattened it, and by the motion of the +pulsar, which created a comet, or lobster-like tail. -wip: yes --- @image @@ -701,11 +742,8 @@ license_id: CC-PDDC thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-585.jpg astropix_ids: chandra|585 -credits> X-ray: NASA/CXC/SAO/S.Mineo et a; X-ray data from Chandra have revealed -that NGC 2207 and IC 2163, currently in the process of colliding with one -another, have pr... +credits> X-ray: NASA/CXC/SAO/S.Mineo et al, Optical: NASA/STScI, Infrared: NASA/JPL-Caltech -wip: yes --- @scene @@ -714,9 +752,13 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-585L{1}X{2}Y{3}.pn outgoing_url: https://chandra.harvard.edu/photo/2014/ngc2207/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-585.jpg -text> NGC 2207 +text> When galaxies get together, there is the chance of a spectacular light +show as is the case with NGC 2207 and IC 2163. Located about 130 million light +years from Earth, in the constellation of Canis Major, this pair of spiral +galaxies has been caught in a grazing encounter. NGC 2207 and IC 2163 have +hosted three supernova explosions in the past 15 years and have produced one of +the most bountiful collections of super bright X-ray lights known. -wip: yes --- @image @@ -726,10 +768,8 @@ license_id: CC-PDDC thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-586.jpg astropix_ids: chandra|586 -credits> X-ray: NASA/CXC/INAF/P.Tozzi, et al; Optical: NAOJ/Subaru and ESO/VLT; -Infrared : ESA/Herschel +credits> X-ray: NASA/CXC/INAF/P.Tozzi, et al; Optical: NAOJ/Subaru and ESO/VLT; Infrared: ESA/Herschel -wip: yes --- @scene @@ -738,9 +778,15 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-586L{1}X{2}Y{3}.pn outgoing_url: https://chandra.harvard.edu/photo/2014/xdcp004/ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-586.jpg -text> Image File +text> A composite image shows the distant and massive galaxy cluster that is +officially known as XDCP J0044.0-2033. Researchers, however, have nicknamed it +"Gioiello", which is Italian for "jewel". They chose this name because an image +of the cluster contains many sparkling colors from the hot, X-ray emitting gas +and various star-forming galaxies within the cluster. Also, the research team +met to discuss the Chandra data for the first time at Villa il Gioiello, a 15th +century villa near the Observatory of Arcetri, which was the last residence of +prominent Italian astronomer Galileo Galilei. -wip: yes --- @image From 6f8cb18c0d0f98cc4ec6ad6956c8258455b5e0a4 Mon Sep 17 00:00:00 2001 From: Peter Williams Date: Wed, 25 Sep 2024 13:00:48 -0400 Subject: [PATCH 2/2] cxprep/chandra.txt: complete registration --- cxprep/chandra.txt | 790 ------------------------------------- imagesets/sky__visible.xml | 60 +-- places/sky_ra00.yml | 2 + places/sky_ra01.yml | 2 + places/sky_ra03.yml | 6 + places/sky_ra05.yml | 4 + places/sky_ra06.yml | 2 + places/sky_ra08.yml | 4 + places/sky_ra09.yml | 4 + places/sky_ra10.yml | 2 + places/sky_ra11.yml | 4 + places/sky_ra12.yml | 6 + places/sky_ra13.yml | 8 + places/sky_ra15.yml | 6 + places/sky_ra16.yml | 4 + places/sky_ra17.yml | 4 + places/sky_ra18.yml | 2 + 17 files changed, 90 insertions(+), 820 deletions(-) diff --git a/cxprep/chandra.txt b/cxprep/chandra.txt index f73649d..79cbeb6 100644 --- a/cxprep/chandra.txt +++ b/cxprep/chandra.txt @@ -1,794 +1,4 @@ -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-548L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-548.jpg -astropix_ids: chandra|548 - -credits> X-ray: NASA/CXC/SAO/F.Seward et al; Optical: NOAO/CTIO/MCELS, DSS - ---- - -@scene -place_uuid: 0cbeed40-e266-4339-b3fb-579dcba27c8f -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-548L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/deml241/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-548.jpg - -text> When a massive star runs out fuel, it collapses and explodes as a -supernova. Although these explosions are extremely powerful, it is possible for -a companion star to endure the blast. A team of astronomers using NASA's Chandra -X-ray Observatory and other telescopes has found evidence for one of these -survivors. This hardy star is in a stellar explosion's debris field — also -called its supernova remnant — located in an HII region called DEM L241. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-559L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-559.jpg -astropix_ids: chandra|559 - -credits> X-ray: NASA/CXC/Univ. of Alabama/W.P.Maksym et al & NASA/CXC/GSFC/UMD/D.Donato, et al; Optical: CFHT - ---- - -@scene -place_uuid: 188e735c-ef2e-4bf9-ae46-00317d16ddcc -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-559L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/a1795/more.html#img1a -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-559.jpg - -text> A bright, long duration flare may be the first recorded event of a black -hole destroying a star in a dwarf galaxy. The dwarf galaxy is located in the -galaxy cluster Abell 1795, about 800 million light years from Earth. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-560L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-560.jpg -astropix_ids: chandra|560 - -credits> X-ray: NASA/CXC/Stanford/J.Hlavacek-Larrondo et al, Optical: NASA/ESA/STScI/M.Postman & CLASH team - ---- - -@scene -place_uuid: 79a8e6a1-daf7-4ef5-9260-0886c6c89cda -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-560L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/rxj1532/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-560.jpg - -text> Astronomers have used NASA's Chandra X-ray Observatory and a suite of -other telescopes to reveal one of the most powerful black holes known. The black -hole has created enormous structures in the hot gas surrounding it and prevented -trillions of stars from forming. The black hole is in a galaxy cluster named RX -J1532.9+3021 (RX J1532 for short), located about 3.9 billion light years from -Earth. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-561L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-561.jpg -astropix_ids: chandra|561 - -credits> X-ray: NASA/CXC/U.Birmingham/M.Burke et al. - ---- - -@scene -place_uuid: 3bdd1cb2-a304-4793-b3fd-586615783f31 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-561L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/cena/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-561.jpg - -text> This image of Centaurus A contains data from observations, equivalent to -over nine and a half days worth of time, taken between 1999 and 2012. In this -image, the lowest-energy X-rays Chandra detects are in red, while the -medium-energy X-rays are green, and the highest-energy ones are blue. As in all -of Chandra's images of Cen A, this one shows the spectacular jet of outflowing -material — seen pointing from the middle to the upper left — that is generated -by the giant black hole at the galaxy's center. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-562L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-562.jpg -astropix_ids: chandra|562 - -credits> X-ray: NASA/CXC/ISDC/L.Pavan et al, Radio: CSIRO/ATNF/ATCA Optical: 2MASS/UMass/IPAC-Caltech/NASA/NSF - ---- - -@scene -place_uuid: bca31a9f-87e8-40ae-89a8-48bfbc0f5257 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-562L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/igrj11014/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-562.jpg - -text> An extraordinary jet trailing behind a runaway pulsar is seen in this -composite image that contains data from NASA's Chandra X-ray Observatory -(purple), radio data from the Australia Compact Telescope Array (green), and -optical data from the 2MASS survey (red, green, and blue). The jet stretches for -37 light years, making it the longest ever seen from an object in the Milky Way -galaxy - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-563L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-563.jpg -astropix_ids: chandra|563 - -credits> X-ray: NASA/CXC/Univ of Michigan/R.C.Reis et al; Optical: NASA/STScI - ---- - -@scene -place_uuid: aa41bd34-f97f-4c34-bfd6-88fda21b15c9 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-563L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/rxj1131/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-563.jpg - -text> Multiple images of a distant quasar are visible in this combined view from -NASA's Chandra X-ray Observatory and the Hubble Space Telescope. The Chandra -data, along with data from ESA's XMM-Newton, were used to directly measure the -spin of the supermassive black hole powering this quasar. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-564L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-564.jpg -astropix_ids: chandra|564,chandra|811c - -credits> X-ray: NASA/CXC/UAH/M.Sun et al; Optical: NASA, ESA, & the Hubble Heritage Team (STScI/AURA) - ---- - -@scene -place_uuid: c7cef620-3bcf-4449-805c-3331078459bf -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-564L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/eso137/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-564.jpg - -text> The spiral galaxy ESO 137-001 looks like a dandelion caught in a breeze in -this composite image from the Hubble Space Telescope and the Chandra X-ray -Observatory. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-565L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-565.jpg -astropix_ids: chandra|565,chandra|809 - -credits> NASA, ESA, J. Jee (Univ. of California, Davis), J. Hughes (Rutgers -Univ.), F. Menanteau (Rutgers Univ. & Univ. of Illinois, Urbana-Champaign), C. -Sifon (Leiden Obs.), R. Mandelbum (Carnegie Mellon Univ.), L. Barrientos (Univ. -Catolica de Chile), and K. Ng (Univ. of California, Davis) - ---- - -@scene -place_uuid: 683d08a7-dc95-4ea3-aa5a-b0505fc09975 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-565L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/elgordo/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-565.jpg - -text> This is a composite image of X-rays from Chandra and optical data from -Hubble of the galaxy cluster ACT-CL J0102-4915, located about 7 billion light -years from Earth. This cluster has been nicknamed "El Gordo" (or, "the fat one" -in Spanish) because of its gigantic mass. Scientists first announced the -discovery of El Gordo with Chandra and ground-based optical telescopes in 2012. -They determined that El Gordo is the most massive, the hottest, and gives off -the most X-rays of any known galaxy cluster at its distance or beyond. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-566L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-566.jpg -astropix_ids: chandra|566 - -credits> X-ray: NASA/CXC/Morehead State Univ/T.Pannuti et al.; Optical: DSS; Infrared: NASA/JPL-Caltech; Radio: NRAO/VLA/Argentinian Institute of Radioastronomy/G.Dubner - ---- - -@scene -place_uuid: c9372e35-ff95-4567-a1be-38375af8527a -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-566L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/g352/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-566.jpg - -text> The supernova remnant G352.7-0.1 (or, G352 for short) has swept up -material equivalent to about 45 times the mass of the Sun, as it expands. -Although this is not an exceptionally large amount, astronomers have found that -several other properties of the supernova remnant are unusual. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-568L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-568.jpg -astropix_ids: chandra|568 - -credits> X-ray: NASA/CXC/PSU/K.Getman, E.Feigelson, M.Kuhn & the MYStIX team; Infrared:NASA/JPL-Caltech - ---- - -@scene -place_uuid: 1c542b75-9a62-41c9-93d6-162bc8809835 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-568L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/flame/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-568.jpg - -text> Stars are often born in clusters, in giant clouds of gas and dust. -Astronomers have studied two star clusters using NASA's Chandra X-ray -Observatory and infrared telescopes and the results show that the simplest ideas -for the birth of these clusters cannot work. This composite image shows one of -the clusters, NGC 2024, which is found in the center of the so-called Flame -Nebula about 1,400 light years from Earth. In this image, X-rays from Chandra -are seen as purple, while infrared data from NASA's Spitzer Space Telescope are -colored red, green, and blue. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-569L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-569.jpg -astropix_ids: chandra|569 - -credits> X-ray: NASA/CXC/Stanford Univ/N.Werner et al. - ---- - -@scene -place_uuid: ef17e870-3b56-44d9-aeee-96df03dd2474 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-569L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/coldgas/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-569.jpg - -text> NASA's Chandra X-ray Observatory has shed new light on the mystery of why -giant elliptical galaxies (such as this one, NGC 1399) have few, if any, young -stars. This new evidence highlights the important role that supermassive black -holes play in the evolution of their host galaxies. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-570L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-570.jpg - -credits> X-ray: NASA/CXC/Wesleyan Univ./R.Kilgard, et al; Optical: NASA/STScI - ---- - -@scene -place_uuid: e1302601-4d74-41f4-970c-7e36629a2a5d -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-570L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/m51/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-570.jpg - -text> Nearly a million seconds of observing time with NASA's Chandra X-ray -Observatory has revealed a spiral galaxy similar to the Milky Way glittering -with hundreds of X-ray points of light. The galaxy is officially named Messier -51 (M51) or NGC 5194, but often goes by its nickname of the "Whirlpool Galaxy." -Like the Milky Way, the Whirlpool is a spiral galaxy with spectacular arms of -stars and dust. M51 is located about 30 million light years from Earth, and its -face-on orientation to Earth gives us a perspective that we can never get of our -own spiral galactic home. This image combines X-ray and optical data. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-570aL{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-570a.jpg -astropix_ids: chandra|570a - -credits> X-ray: NASA/CXC/Wesleyan Univ./R.Kilgard, et al; Optical: NASA/STScI - ---- - -@scene -place_uuid: 9d6d0312-3140-4902-aa18-9d054e897748 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-570aL{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/m51/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-570a.jpg - -text> Nearly a million seconds of observing time with NASA's Chandra X-ray -Observatory has revealed a spiral galaxy similar to the Milky Way glittering -with hundreds of X-ray points of light. The galaxy is officially named Messier -51 (M51) or NGC 5194, but often goes by its nickname of the "Whirlpool Galaxy." -Like the Milky Way, the Whirlpool is a spiral galaxy with spectacular arms of -stars and dust. M51 is located about 30 million light years from Earth, and its -face-on orientation to Earth gives us a perspective that we can never get of our -own spiral galactic home. This image shows X-ray data only. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-571L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-571.jpg -astropix_ids: chandra|571 - -credits> X-ray: NASA/CXC/SAO/E.Bulbul, et al. - ---- - -@scene -place_uuid: 9fb71dc4-1c01-4f9e-ba7e-74176e2efb0f -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-571L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/perseus/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-571.jpg - -text> A new study of the central region of the Perseus galaxy cluster, shown in -this image, using NASA's Chandra X-ray Observatory and 73 other clusters with -ESA's XMM-Newton has revealed a mysterious X-ray signal in the data. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-572L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-572.jpg -astropix_ids: chandra|572 - -credits> X-ray: NASA/CXC/Caltech/P.Ogle et al; Optical: NASA/STScI & R.Gendler; IR: NASA/JPL-Caltech; Radio: NSF/NRAO/VLA - ---- - -@scene -place_uuid: c39a9afc-a717-4443-9263-6599ce721901 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-572L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/m106/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-572.jpg - -text> A galaxy about 23 million light years away is the site of impressive, -ongoing, fireworks. Rather than paper, powder, and fire, this galactic light -show involves a giant black hole, shock waves, and vast reservoirs of gas. This -galactic fireworks display is taking place in NGC 4258 (also known as M106), a -spiral galaxy like the Milky Way. This galaxy is famous, however, for something -that our Galaxy doesn't have — two extra spiral arms that glow in X-ray, -optical, and radio light. These features, or anomalous arms, are not aligned -with the plane of the galaxy, but instead intersect with it. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-576L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-576.jpg -astropix_ids: chandra|576 - -credits> NASA/CXC/SAO/R.Margutti et al - ---- - -@scene -place_uuid: 25f3c0bb-e7f3-4975-a579-0ed49bc8d276 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-576L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/m82/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-576.jpg - -text> On January 21, 2014, astronomers witnessed a supernova soon after it -exploded in the Messier 82, or M82, galaxy. Telescopes across the globe and in -space turned their attention to study this newly exploded star, including -Chandra. Astronomers determined that this supernova, dubbed SN 2014J, belongs to -a class of explosions called "Type Ia" supernovas. These supernovas are used as -cosmic distance-markers and played a key role in the discovery of the Universe's -accelerated expansion, which has been attributed to the effects of dark energy. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-577L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-577.jpg -astropix_ids: chandra|577 - -credits> X-ray: NASA/CXC/IAFE/G.Dubner et al & ESA/XMM-Newton - ---- - -@scene -place_uuid: ff6f866d-366b-40ae-b693-8c327d5c47ac -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-577L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/puppisa/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-577.jpg - -text> The destructive results of a powerful supernova explosion reveal -themselves in a delicate tapestry of X-ray light, as seen in this image from -NASA's Chandra X-Ray Observatory and the European Space Agency's XMM-Newton. The -image shows the remains of a supernova that would have been witnessed on Earth -about 3,700 years ago. The remnant is called Puppis A, and is around 7,000 light -years away and about 100 light years across. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-578L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-578.jpg -astropix_ids: chandra|578 - -credits> NASA/CXC/GSFC/K.Hamaguchi, et al. - ---- - -@scene -place_uuid: ae350083-505e-4ac8-9062-5e4e23c78992 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-578L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/etacar/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-578.jpg - -text> The Eta Carinae star system does not lack for superlatives. Not only does -it contain one of the biggest and brightest stars in our galaxy, weighing at -least 90 times the mass of the Sun, it is also extremely volatile and is -expected to have at least one supernova explosion in the future. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-580L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-580.jpg -astropix_ids: chandra|580 - -credits> X-ray: NASA/CXC/Univ. of Toulouse/M.Bachetti et al, Optical: NOAO/AURA/NSF - ---- - -@scene -place_uuid: 6089acba-2249-4429-929b-e23db1dda620 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-580L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/m82nu/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-580.jpg - -text> An Ultraluminous X-ray Source (ULX) that astronomers had thought was a -black hole is really the brightest pulsar ever recorded. ULXs are objects that -produce more X-rays than most "normal" X-ray binary systems, in which a star is -orbiting a neutron star or a stellar-mass black hole. Black holes in these X-ray -binary systems generally weigh about five to thirty times the mass of the sun. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-581aL{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-581a.jpg -astropix_ids: chandra|581a - -credits> X-ray: NASA/CXC/ESA-ESTEC/E.Winston et al, Near-IR: 2MASS/UMass/IPAC-Caltech/NASA/NSF, Infrared: NASA/JPL-Caltech - ---- - -@scene -place_uuid: d2bb7cfc-ca15-407a-9131-aa683f1d5594 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-581aL{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/archives/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-581a.jpg - -text> A young star cluster about 5,500 light years from Earth, RCW 38 provides -astronomers a chance to closely examine many young, rapidly evolving stars at -once. In this composite image, X-rays from Chandra are blue, while infrared data -from NASA's Spitzer Space Telescope are orange and additional infrared data from -the 2MASS survey appears white. There are many massive stars in RCW 38 that will -likely explode as supernovas. Astronomers studying RCW 38 are hoping to better -understand this environment as our Sun was likely born into a similar stellar -nursery. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-581cL{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-581c.jpg -astropix_ids: chandra|581c - -credits> X-ray: NASA/CXC/Univ. of Manitoba/H.Kumar et al, Optical: DSS, Infrared: NASA/JPL-Caltech, Radio: NSF/NRAO/VLA - ---- - -@scene -place_uuid: 5f4cc1e1-a723-4e1f-8061-ab51dbe65783 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-581cL{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/archives/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-581c.jpg - -text> The supernova remnant Kes 73, located about 28,000 light years away, -contains a so-called anomalous X-ray pulsar, or AXP, at its center. Astronomers -think that most AXPs are magnetars, which are neutron stars with ultra-high -magnetic fields. Surrounding the point-like AXP in the middle, Kes 73 has an -expanding shell of debris from the supernova explosion that occurred between -about 750 and 2100 years ago, as seen from Earth. The Chandra data (blue) reveal -clumpy structures along one side of the remnant, and appear to overlap with -infrared data (orange). The X-rays partially fill the shell seen in radio -emission (red) by the Very Large Array. Data from the Digitized Sky Survey -optical telescope (white) show stars in the field-of-view. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-581dL{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-581d.jpg -astropix_ids: chandra|581d - -credits> X-ray: NASA/CXC/SAO, Optical: NASA/STScI, Radio: NSF/NRAO/VLA - ---- - -@scene -place_uuid: 36b18326-a43b-4d4c-ba7c-8ebab6e54aea -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-581dL{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/archives/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-581d.jpg - -text> Some galaxies have extremely bright cores, suggesting that they contain a -supermassive black hole that is pulling in matter at a prodigious rate. -Astronomers call these "active galaxies," and Hercules A is one of them. In -visible light (colored red, green and blue, with most objects appearing white), -Hercules A looks like a typical elliptical galaxy. In X-ray light, however, -Chandra detects a giant cloud of multimillion-degree gas (purple). This gas has -been heated by energy generated by the infall of matter into a black hole at the -center of Hercules A that is over 1,000 times as massive as the one in the -middle of the Milky Way. Radio data (blue) show jets of particles streaming away -from the black hole. The jets span a length of almost one million light years. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-581eL{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-581e.jpg -astropix_ids: chandra|581e - -credits> X-ray: NASA/CXC/SAO; Infared: NASA/JPL-Caltech - ---- - -@scene -place_uuid: 4ff5fb2b-dcd5-4334-85f5-82af0e714d07 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-581eL{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/archives/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-581e.jpg - -text> Pareidolia is the psychological phenomenon where people see recognizable -shapes in clouds, rock formations, or otherwise unrelated objects or data. When -Chandra's image of PSR B1509-58, a spinning neutron star surrounded by a cloud -of energetic particles, was released in 2009, it quickly gained attention -because many saw a hand-like structure in the X-ray emission. In this new image -of the system, X-rays from Chandra in gold are seen along with infrared data -from NASA's Wide-field Infrared Survey Explorer (WISE) telescope in red, green, -and blue. Pareidolia may strike again in this image as some people report seeing -a shape of a face in WISE's infrared data. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-581fL{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-581f.jpg -astropix_ids: chandra|581f - -credits> X-ray: NASA/CXC/Universita di Bologna/S.Pellegrini et al, IR: NASA/JPL-Caltech; Optical: SDSS & NASA/STScI - ---- - -@scene -place_uuid: 06166636-3f0a-490c-8ff6-dfc1144a5672 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-581fL{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/archives/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-581f.jpg - -text> NGC 4736 (also known as Messier 94) is a spiral galaxy that is unusual -because it has two ring structures. This galaxy is classified as containing a -"low ionization nuclear emission region," or LINER, in its center, which -produces radiation from specific elements such as oxygen and nitrogen. Chandra -observations (gold) of NGC 4736, seen in this composite image with infrared data -from Spitzer (red) and optical data from Hubble and the Sloan Digital Sky Survey -(blue), suggest that the X-ray emission comes from a recent burst of star -formation. Part of the evidence comes from the large number of point sources -near the center of the galaxy, showing that strong star formation has occurred. -In other galaxies, evidence points to supermassive black holes being responsible -for LINER properties. Chandra's result on NGC 4736 shows LINERs may represent -more than one physical phenomenon. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-582aL{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-582a.jpg -astropix_ids: chandra|582a - -credits> NASA/CXC/Stanford/I.Zhuravleva et al - ---- - -@scene -place_uuid: 15900130-de3c-4ebb-85fd-2fa779432ccc -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-582aL{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/perseusvirgo/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-582a.jpg - -text> This Chandra image of the galaxy cluster known as Perseus has provided -direct evidence that turbulence is helping to prevent stars from forming. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-582bL{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-582b.jpg -astropix_ids: chandra|582b - -credits> NASA/CXC/Stanford/I.Zhuravleva et al - ---- - -@scene -place_uuid: 38db29ca-d277-4184-9554-893bf5bc25bd -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-582bL{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/perseusvirgo/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-582b.jpg - -text> This Chandra image of the galaxy cluster known as Virgo has provided -direct evidence that turbulence is helping to prevent stars from forming. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-583L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-583.jpg -astropix_ids: chandra|583 - -credits> NASA/CXC/Univ. of Wisconsin/Y.Bai, et al. - ---- - -@scene -place_uuid: 1fb67b23-7159-48db-bf28-bed745c5c62d -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-583L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/sgra/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-583.jpg - -text> The supermassive black hole at the center of the Milky Way, seen in this -image from NASA's Chandra X-ray Observatory, may be producing mysterious -particles called neutrinos. Neutrinos are tiny particles that have virtually no -mass and carry no electric charge. Unlike light or charged particles, neutrinos -can emerge from deep within their sources and travel across the Universe without -being absorbed by intervening matter or, in the case of charged particles, -deflected by magnetic fields. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-584bL{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-584b.jpg -astropix_ids: chandra|584b - -credits> NASA/CXC/GSFC/T.Temim et al. - ---- - -@scene -place_uuid: fc454d7c-ca82-49f8-9c4b-3ea919fd16c2 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-584bL{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/msh11g327/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-584b.jpg - -text> The supernova remnant G327.1-1.1, located about 29,000 light years from -Earth, is a spectacular debris field left behind when a massive star exploded. -The Chandra image of G327.1-1.1 shows the outward-moving, or forward, shock wave -(seen as the faint red color), and a bright pulsar wind nebula (blue). The -pulsar wind nebula appears to have been distorted by the combined action of the -reverse shock wave, which may have flattened it, and by the motion of the -pulsar, which created a comet, or lobster-like tail. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-585L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-585.jpg -astropix_ids: chandra|585 - -credits> X-ray: NASA/CXC/SAO/S.Mineo et al, Optical: NASA/STScI, Infrared: NASA/JPL-Caltech - ---- - -@scene -place_uuid: 01f54c3a-0259-4e65-8825-38cf84a01659 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-585L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/ngc2207/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-585.jpg - -text> When galaxies get together, there is the chance of a spectacular light -show as is the case with NGC 2207 and IC 2163. Located about 130 million light -years from Earth, in the constellation of Canis Major, this pair of spiral -galaxies has been caught in a grazing encounter. NGC 2207 and IC 2163 have -hosted three supernova explosions in the past 15 years and have produced one of -the most bountiful collections of super bright X-ray lights known. - ---- - -@image -url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-586L{1}X{2}Y{3}.png -copyright: Public domain -license_id: CC-PDDC -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-586.jpg -astropix_ids: chandra|586 - -credits> X-ray: NASA/CXC/INAF/P.Tozzi, et al; Optical: NAOJ/Subaru and ESO/VLT; Infrared: ESA/Herschel - ---- - -@scene -place_uuid: 33fe80e0-0c24-4703-b581-6a3b38b2a905 -image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-586L{1}X{2}Y{3}.png -outgoing_url: https://chandra.harvard.edu/photo/2014/xdcp004/ -thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-586.jpg - -text> A composite image shows the distant and massive galaxy cluster that is -officially known as XDCP J0044.0-2033. Researchers, however, have nicknamed it -"Gioiello", which is Italian for "jewel". They chose this name because an image -of the cluster contains many sparkling colors from the hot, X-ray emitting gas -and various star-forming galaxies within the cluster. Also, the research team -met to discuss the Chandra data for the first time at Villa il Gioiello, a 15th -century villa near the Observatory of Arcetri, which was the last residence of -prominent Italian astronomer Galileo Galilei. - ---- - @image url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-587aL{1}X{2}Y{3}.png copyright: Public domain diff --git a/imagesets/sky__visible.xml b/imagesets/sky__visible.xml index 75aaa86..aa88658 100644 --- a/imagesets/sky__visible.xml +++ b/imagesets/sky__visible.xml @@ -52261,7 +52261,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-548L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|548" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f44175955f03d76f65976a" > X-ray: NASA/CXC/SAO/F.Seward et ; This composite image contains data from Chandra (purple) that provides evidence for the survival of a companion star from the bl... https://chandra.harvard.edu/photo/2014/deml241/ @@ -52531,7 +52531,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-559L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|559" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f44176955f03d76f65976c" > redit: X-ray: NASA/CXC/Univ. of Alabama/W.P.Maksym et al & NASA/CXC/GSFC/UMD/D.Donato, et al; Optical: CFHT. https://chandra.harvard.edu/photo/2014/a1795/more.html#img1a @@ -52558,7 +52558,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-560L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|560" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f44177955f03d76f65976e" > X-ray: NASA/CXC/Stanford/J.Hlava; Astronomers have used NASA's Chandra X-ray Observatory and other telescopes to reveal one of the most powerful black holes known... https://chandra.harvard.edu/photo/2014/rxj1532/ @@ -52585,7 +52585,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-561L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|561" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f44177955f03d76f659770" > X-ray: NASA/CXC/U.Birmingham/M.B; Centaurus A is a galaxy well known for a gargantuan jet blasting away from a central supermassive black hole, which is seen in t... https://chandra.harvard.edu/photo/2014/cena/ @@ -52612,7 +52612,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-562L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|562" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f44178955f03d76f659772" > X-ray: NASA/CXC/ISDC/L.Pavan et ; An extraordinary jet trailing behind a runaway pulsar is seen in this composite image that contains X-ray data from Chandra (pur... https://chandra.harvard.edu/photo/2014/igrj11014/ @@ -52639,7 +52639,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-563L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|563" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f44179955f03d76f659774" > X-ray: NASA/CXC/Univ of Michigan; Multiple images of a distant quasar known as RX J1131-1231 are visible in this combined view from Chandra (pink) and Hubble (red... https://chandra.harvard.edu/photo/2014/rxj1131/ @@ -52666,7 +52666,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-564L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|564,chandra|811c" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f4417a955f03d76f659776" > X-ray: NASA/CXC/UAH/M.Sun et al;; This image combines NASA/ESA Hubble Space Telescope observations with data from the Chandra X-ray Observatory. As well as the el... https://chandra.harvard.edu/photo/2014/eso137/ @@ -52693,7 +52693,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-565L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|565,chandra|809" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f4417b955f03d76f659778" > NASA, ESA, J. Jee (Univ. of California, Davis), J. Hughes (Rutgers Univ.), F. Menanteau (Rutgers Univ. & Univ. of Illinois, Urbana-Champaign), C. Sifon (Leiden Obs.), R. Mandelbum (Carnegie Mellon Univ.), L. Barrientos (Univ. Catolica de Chile), and K. Ng (Univ. of California, Davis) https://chandra.harvard.edu/photo/2014/elgordo/ @@ -52720,7 +52720,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-566L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|566" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f4417c955f03d76f65977a" > X-ray: NASA/CXC/Morehead State U; Supernova remnants are created when a massive star explodes and its remains are hurled into space. Astronomers have found a supe... https://chandra.harvard.edu/photo/2014/g352/ @@ -52747,7 +52747,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-568L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|568" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f4417d955f03d76f65977c" > X-ray: NASA/CXC/PSU/K.Getman, E.; Astronomers have studied two star clusters to gain insight on how clusters of stars like our Sun form. This composite image show... https://chandra.harvard.edu/photo/2014/flame/ @@ -52774,7 +52774,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-569L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|569" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f4417e955f03d76f65977e" > X-ray: NASA/CXC/Stanford Univ/N.; This four-panel of images represents a sample of giant elliptical galaxies observed by Chandra and the Hershel Space Observatory... https://chandra.harvard.edu/photo/2014/coldgas/ @@ -52800,7 +52800,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... TileLevels="4" Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-570L{1}X{2}Y{3}.png" WidthFactor="1" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f4417e955f03d76f659780" > X-ray: NASA/CXC/Wesleyan Univ./R.Kilgard, et al; Optical: NASA/STScI https://chandra.harvard.edu/photo/2014/m51/ @@ -52827,7 +52827,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-570aL{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|570a" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f4417f955f03d76f659782" > X-ray: NASA/CXC/Wesleyan Univ./R; This image contains nearly a million seconds worth of Chandra observing time (purple) along with optical data from the Hubble Sp... https://chandra.harvard.edu/photo/2014/m51/ @@ -52854,7 +52854,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-571L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|571" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f44180955f03d76f659784" > X-ray: NASA/CXC/SAO/E.Bulbul, e; A new study of the Perseus galaxy cluster, shown in this image, and others using Chandra and XMM-Newton has revealed a mysteriou... https://chandra.harvard.edu/photo/2014/perseus/ @@ -52881,7 +52881,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-572L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|572" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f44181955f03d76f659786" > X-ray: NASA/CXC/Caltech/P.Ogle e; NGC 4258 is a spiral galaxy well known to astronomers for having two so-called anomalous arms that glow in X-ray, optical, and r... https://chandra.harvard.edu/photo/2014/m106/ @@ -52908,7 +52908,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-576L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|576" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f44182955f03d76f659788" > NASA/CXC/SAO/R.Margutti et al; New Chandra data gives insight into the explosion that produced SN 2014J, one of the closest supernovas discovered in decades. ... https://chandra.harvard.edu/photo/2014/m82/ @@ -52935,7 +52935,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-577L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|577" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f44183955f03d76f65978a" > X-ray: NASA/CXC/IAFE/G.Dubner et; The destructive results of a powerful supernova explosion are seen in a delicate tapestry of X-ray light in this new image. The... https://chandra.harvard.edu/photo/2014/puppisa/ @@ -52962,7 +52962,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-578L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|578" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f44184955f03d76f65978c" > NASA/CXC/GSFC/K.Hamaguchi, et al. https://chandra.harvard.edu/photo/2014/etacar/ @@ -52989,7 +52989,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-580L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|580" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f44185955f03d76f65978e" > X-ray: NASA/CXC/Univ. of Toulous; Ultraluminous X-ray Sources (ULXs) are objects that produce more X-rays than most "normal" X-ray binary systems, in which a star... https://chandra.harvard.edu/photo/2014/m82nu/ @@ -53016,7 +53016,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-581aL{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|581a" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f44186955f03d76f659790" > X-ray: NASA/CXC/ESA-ESTEC/E.Wins; With the passing of Chandra's 15th anniversary, the Chandra Data Archive, which houses all of the mission's data, continues to g... https://chandra.harvard.edu/photo/2014/archives/ @@ -53043,7 +53043,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-581cL{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|581c" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f44186955f03d76f659792" > X-ray: NASA/CXC/Univ. of Manitob; With the passing of Chandra's 15th anniversary, the Chandra Data Archive, which houses all of the mission's data, continues to g... https://chandra.harvard.edu/photo/2014/archives/ @@ -53070,7 +53070,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-581dL{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|581d" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f44187955f03d76f659794" > X-ray: NASA/CXC/SAO, Optical: NA; With the passing of Chandra's 15th anniversary, the Chandra Data Archive, which houses all of the mission's data, continues to g... https://chandra.harvard.edu/photo/2014/archives/ @@ -53097,7 +53097,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-581eL{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|581e" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f44188955f03d76f659796" > X-ray: NASA/CXC/SAO; Infared: NA; With the passing of Chandra's 15th anniversary, the Chandra Data Archive, which houses all of the mission's data, continues to g... https://chandra.harvard.edu/photo/2014/archives/ @@ -53124,7 +53124,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-581fL{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|581f" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f44189955f03d76f659798" > X-ray: NASA/CXC/Universita di Bo; With the passing of Chandra's 15th anniversary, the Chandra Data Archive, which houses all of the mission's data, continues to g... https://chandra.harvard.edu/photo/2014/archives/ @@ -53151,7 +53151,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-582aL{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|582a" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f4418a955f03d76f65979a" > NASA/CXC/Stanford/I.Zhuravleva e; Chandra observations of the Perseus and Virgo galaxy clusters have provided direct evidence that turbulence is helping to preven... https://chandra.harvard.edu/photo/2014/perseusvirgo/ @@ -53178,7 +53178,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-582bL{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|582b" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f4418b955f03d76f65979c" > NASA/CXC/Stanford/I.Zhuravleva e; Chandra observations of the Perseus and Virgo galaxy clusters have provided direct evidence that turbulence is helping to preven... https://chandra.harvard.edu/photo/2014/perseusvirgo/ @@ -53205,7 +53205,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-583L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|583" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f4418c955f03d76f65979e" > NASA/CXC/Univ. of Wisconsin/Y.Ba; The supermassive black hole at the center of the Milky Way may be producing tiny particles, called neutrinos, that have virtuall... https://chandra.harvard.edu/photo/2014/sgra/ @@ -53232,7 +53232,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-584bL{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|584b" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f4418d955f03d76f6597a0" > NASA/CXC/GSFC/T.Temim et al. ; A long observation with Chandra of the supernova remnant MSH 11-62 reveals an irregular shell of hot gas, shown in red, surround... @@ -53260,7 +53260,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-585L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|585" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f4418d955f03d76f6597a2" > X-ray: NASA/CXC/SAO/S.Mineo et a; X-ray data from Chandra have revealed that NGC 2207 and IC 2163, currently in the process of colliding with one another, have pr... https://chandra.harvard.edu/photo/2014/ngc2207/ @@ -53287,7 +53287,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator... Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-586L{1}X{2}Y{3}.png" WidthFactor="1" Xastropix_ids="chandra|586" - Xcxstatus="queue:chandra" + Xcxstatus="in:66f4418e955f03d76f6597a4" > X-ray: NASA/CXC/INAF/P.Tozzi, et al; Optical: NAOJ/Subaru and ESO/VLT; Infrared: ESA/Herschel https://chandra.harvard.edu/photo/2014/xdcp004/ diff --git a/places/sky_ra00.yml b/places/sky_ra00.yml index 0e82fac..fb649ee 100644 --- a/places/sky_ra00.yml +++ b/places/sky_ra00.yml @@ -1757,8 +1757,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-542.jpg zoom_level: 10.9227889012364 --- _uuid: 33fe80e0-0c24-4703-b581-6a3b38b2a905 +astropix_id: chandra|586 classification: '' constellation: CET +cxstatus: in:66f4418f955f03d76f6597a5 data_set_type: Sky dec_deg: -20.5674724 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-586L{1}X{2}Y{3}.png diff --git a/places/sky_ra01.yml b/places/sky_ra01.yml index aa8c753..3a8ca1c 100644 --- a/places/sky_ra01.yml +++ b/places/sky_ra01.yml @@ -1261,8 +1261,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-537.jpg zoom_level: 0.288164511744 --- _uuid: 683d08a7-dc95-4ea3-aa5a-b0505fc09975 +astropix_id: chandra|565 classification: '' constellation: PHE +cxstatus: in:66f4417b955f03d76f659779 data_set_type: Sky dec_deg: -49.2550899 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-565L{1}X{2}Y{3}.png diff --git a/places/sky_ra03.yml b/places/sky_ra03.yml index 764a8a6..3046ee2 100644 --- a/places/sky_ra03.yml +++ b/places/sky_ra03.yml @@ -1935,8 +1935,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-546.jpg zoom_level: 0.516740317184 --- _uuid: ef17e870-3b56-44d9-aeee-96df03dd2474 +astropix_id: chandra|569 classification: '' constellation: FOR +cxstatus: in:66f4417e955f03d76f65977f data_set_type: Sky dec_deg: -35.4499543 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-569L{1}X{2}Y{3}.png @@ -1946,8 +1948,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-569.jpg zoom_level: 0.491741134848 --- _uuid: 9fb71dc4-1c01-4f9e-ba7e-74176e2efb0f +astropix_id: chandra|571 classification: '' constellation: PER +cxstatus: in:66f44181955f03d76f659785 data_set_type: Sky dec_deg: 41.511793 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-571L{1}X{2}Y{3}.png @@ -1957,8 +1961,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-571.jpg zoom_level: 0.828658663424 --- _uuid: 15900130-de3c-4ebb-85fd-2fa779432ccc +astropix_id: chandra|582a classification: '' constellation: PER +cxstatus: in:66f4418a955f03d76f65979b data_set_type: Sky dec_deg: 41.5118326 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-582aL{1}X{2}Y{3}.png diff --git a/places/sky_ra05.yml b/places/sky_ra05.yml index 0b6355d..268f76d 100644 --- a/places/sky_ra05.yml +++ b/places/sky_ra05.yml @@ -4725,8 +4725,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-520.jpg zoom_level: 1.9205545984 --- _uuid: 0cbeed40-e266-4339-b3fb-579dcba27c8f +astropix_id: chandra|548 classification: '' constellation: DOR +cxstatus: in:66f44175955f03d76f65976b data_set_type: Sky dec_deg: -67.5637517 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-548L{1}X{2}Y{3}.png @@ -4736,8 +4738,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-548.jpg zoom_level: 1.78706251776 --- _uuid: 1c542b75-9a62-41c9-93d6-162bc8809835 +astropix_id: chandra|568 classification: '' constellation: ORI +cxstatus: in:66f4417d955f03d76f65977d data_set_type: Sky dec_deg: -1.8489455 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-568L{1}X{2}Y{3}.png diff --git a/places/sky_ra06.yml b/places/sky_ra06.yml index f660c15..7ffcccc 100644 --- a/places/sky_ra06.yml +++ b/places/sky_ra06.yml @@ -822,8 +822,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-462.jpg zoom_level: 4.54958546944 --- _uuid: 01f54c3a-0259-4e65-8825-38cf84a01659 +astropix_id: chandra|585 classification: '' constellation: CMA +cxstatus: in:66f4418e955f03d76f6597a3 data_set_type: Sky dec_deg: -21.3751199 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-585L{1}X{2}Y{3}.png diff --git a/places/sky_ra08.yml b/places/sky_ra08.yml index a425f97..d59bdc3 100644 --- a/places/sky_ra08.yml +++ b/places/sky_ra08.yml @@ -590,8 +590,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-540.jpg zoom_level: 0.0572051898368 --- _uuid: ff6f866d-366b-40ae-b693-8c327d5c47ac +astropix_id: chandra|577 classification: '' constellation: PUP +cxstatus: in:66f44183955f03d76f65978b data_set_type: Sky dec_deg: -43.0076723 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-577L{1}X{2}Y{3}.png @@ -601,8 +603,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-577.jpg zoom_level: 6.49738289152 --- _uuid: d2bb7cfc-ca15-407a-9131-aa683f1d5594 +astropix_id: chandra|581a classification: '' constellation: VEL +cxstatus: in:66f44186955f03d76f659791 data_set_type: Sky dec_deg: -47.5003611 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-581aL{1}X{2}Y{3}.png diff --git a/places/sky_ra09.yml b/places/sky_ra09.yml index 8110692..0be5752 100644 --- a/places/sky_ra09.yml +++ b/places/sky_ra09.yml @@ -754,8 +754,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-511.jpg zoom_level: 0.0669753344 --- _uuid: 25f3c0bb-e7f3-4975-a579-0ed49bc8d276 +astropix_id: chandra|576 classification: '' constellation: UMA +cxstatus: in:66f44182955f03d76f659789 data_set_type: Sky dec_deg: 69.6795082 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-576L{1}X{2}Y{3}.png @@ -765,8 +767,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-576.jpg zoom_level: 1.26825570304 --- _uuid: 6089acba-2249-4429-929b-e23db1dda620 +astropix_id: chandra|580 classification: '' constellation: UMA +cxstatus: in:66f44185955f03d76f65978f data_set_type: Sky dec_deg: 69.6712593 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-580L{1}X{2}Y{3}.png diff --git a/places/sky_ra10.yml b/places/sky_ra10.yml index a4960c9..3c32374 100644 --- a/places/sky_ra10.yml +++ b/places/sky_ra10.yml @@ -1613,8 +1613,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-513.jpg zoom_level: 0.07941029888 --- _uuid: ae350083-505e-4ac8-9062-5e4e23c78992 +astropix_id: chandra|578 classification: '' constellation: CAR +cxstatus: in:66f44184955f03d76f65978d data_set_type: Sky dec_deg: -59.6843723 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-578L{1}X{2}Y{3}.png diff --git a/places/sky_ra11.yml b/places/sky_ra11.yml index 593e454..881ce9a 100644 --- a/places/sky_ra11.yml +++ b/places/sky_ra11.yml @@ -1296,8 +1296,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-554e.jpg zoom_level: 2.09546477568 --- _uuid: bca31a9f-87e8-40ae-89a8-48bfbc0f5257 +astropix_id: chandra|562 classification: '' constellation: CAR +cxstatus: in:66f44179955f03d76f659773 data_set_type: Sky dec_deg: -60.9359673 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-562L{1}X{2}Y{3}.png @@ -1307,8 +1309,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-562.jpg zoom_level: 1.68405532672 --- _uuid: aa41bd34-f97f-4c34-bfd6-88fda21b15c9 +astropix_id: chandra|563 classification: '' constellation: CRT +cxstatus: in:66f4417a955f03d76f659775 data_set_type: Sky dec_deg: -12.5331568 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-563L{1}X{2}Y{3}.png diff --git a/places/sky_ra12.yml b/places/sky_ra12.yml index a03b6da..d849668 100644 --- a/places/sky_ra12.yml +++ b/places/sky_ra12.yml @@ -2880,8 +2880,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-550.jpg zoom_level: 0.241307877376 --- _uuid: c39a9afc-a717-4443-9263-6599ce721901 +astropix_id: chandra|572 classification: '' constellation: CVN +cxstatus: in:66f44182955f03d76f659787 data_set_type: Sky dec_deg: 47.3013126 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-572L{1}X{2}Y{3}.png @@ -2891,8 +2893,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-572.jpg zoom_level: 0.499527073792 --- _uuid: 06166636-3f0a-490c-8ff6-dfc1144a5672 +astropix_id: chandra|581f classification: '' constellation: CVN +cxstatus: in:66f44189955f03d76f659799 data_set_type: Sky dec_deg: 41.1252083 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-581fL{1}X{2}Y{3}.png @@ -2902,8 +2906,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-581f.jpg zoom_level: 1.107896107008 --- _uuid: 38db29ca-d277-4184-9554-893bf5bc25bd +astropix_id: chandra|582b classification: '' constellation: VIR +cxstatus: in:66f4418b955f03d76f65979d data_set_type: Sky dec_deg: 12.3913027 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-582bL{1}X{2}Y{3}.png diff --git a/places/sky_ra13.yml b/places/sky_ra13.yml index 60c0ecf..2ab8aa0 100644 --- a/places/sky_ra13.yml +++ b/places/sky_ra13.yml @@ -2394,8 +2394,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-535.jpg zoom_level: 1.5176962048 --- _uuid: 188e735c-ef2e-4bf9-ae46-00317d16ddcc +astropix_id: chandra|559 classification: '' constellation: BOO +cxstatus: in:66f44176955f03d76f65976d data_set_type: Sky dec_deg: 26.5958113 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-559L{1}X{2}Y{3}.png @@ -2405,8 +2407,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-559.jpg zoom_level: 0.515678486528 --- _uuid: 3bdd1cb2-a304-4793-b3fd-586615783f31 +astropix_id: chandra|561 classification: '' constellation: CEN +cxstatus: in:66f44178955f03d76f659771 data_set_type: Sky dec_deg: -43.0188596 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-561L{1}X{2}Y{3}.png @@ -2416,8 +2420,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-561.jpg zoom_level: 1.2713283584 --- _uuid: e1302601-4d74-41f4-970c-7e36629a2a5d +astropix_id: null classification: '' constellation: CVN +cxstatus: in:66f4417f955f03d76f659781 data_set_type: Sky dec_deg: 47.2134616 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-570L{1}X{2}Y{3}.png @@ -2427,8 +2433,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-570.jpg zoom_level: 0.728123441152 --- _uuid: 9d6d0312-3140-4902-aa18-9d054e897748 +astropix_id: chandra|570a classification: '' constellation: CVN +cxstatus: in:66f44180955f03d76f659783 data_set_type: Sky dec_deg: 47.2134616 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-570aL{1}X{2}Y{3}.png diff --git a/places/sky_ra15.yml b/places/sky_ra15.yml index 4d90200..efe30b3 100644 --- a/places/sky_ra15.yml +++ b/places/sky_ra15.yml @@ -511,8 +511,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-557.jpg zoom_level: 0.772295098368 --- _uuid: 79a8e6a1-daf7-4ef5-9260-0886c6c89cda +astropix_id: chandra|560 classification: '' constellation: CRB +cxstatus: in:66f44177955f03d76f65976f data_set_type: Sky dec_deg: 30.3498551 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-560L{1}X{2}Y{3}.png @@ -522,8 +524,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-560.jpg zoom_level: 0.1210088062976 --- _uuid: 4ff5fb2b-dcd5-4334-85f5-82af0e714d07 +astropix_id: chandra|581e classification: '' constellation: CIR +cxstatus: in:66f44189955f03d76f659797 data_set_type: Sky dec_deg: -59.1660759 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-581eL{1}X{2}Y{3}.png @@ -533,8 +537,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-581e.jpg zoom_level: 4.02085085184 --- _uuid: fc454d7c-ca82-49f8-9c4b-3ea919fd16c2 +astropix_id: chandra|584b classification: '' constellation: NOR +cxstatus: in:66f4418d955f03d76f6597a1 data_set_type: Sky dec_deg: -55.0936189 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-584bL{1}X{2}Y{3}.png diff --git a/places/sky_ra16.yml b/places/sky_ra16.yml index b85a79e..5cf3b41 100644 --- a/places/sky_ra16.yml +++ b/places/sky_ra16.yml @@ -1366,8 +1366,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-539.jpg zoom_level: 0.234902552576 --- _uuid: c7cef620-3bcf-4449-805c-3331078459bf +astropix_id: chandra|564 classification: '' constellation: TRA +cxstatus: in:66f4417a955f03d76f659777 data_set_type: Sky dec_deg: -60.7567317819 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-564L{1}X{2}Y{3}.png @@ -1377,8 +1379,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-564.jpg zoom_level: 0.122843136 --- _uuid: 36b18326-a43b-4d4c-ba7c-8ebab6e54aea +astropix_id: chandra|581d classification: '' constellation: HER +cxstatus: in:66f44188955f03d76f659795 data_set_type: Sky dec_deg: 4.9920737 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-581dL{1}X{2}Y{3}.png diff --git a/places/sky_ra17.yml b/places/sky_ra17.yml index 758eecd..0a7ea0e 100644 --- a/places/sky_ra17.yml +++ b/places/sky_ra17.yml @@ -2040,8 +2040,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-556.jpg zoom_level: 0.0926228004864 --- _uuid: c9372e35-ff95-4567-a1be-38375af8527a +astropix_id: chandra|566 classification: '' constellation: SCO +cxstatus: in:66f4417c955f03d76f65977b data_set_type: Sky dec_deg: -35.1080029 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-566L{1}X{2}Y{3}.png @@ -2051,8 +2053,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-566.jpg zoom_level: 1.09733707776 --- _uuid: 1fb67b23-7159-48db-bf28-bed745c5c62d +astropix_id: chandra|583 classification: '' constellation: SGR +cxstatus: in:66f4418c955f03d76f65979f data_set_type: Sky dec_deg: -29.0070133 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-583L{1}X{2}Y{3}.png diff --git a/places/sky_ra18.yml b/places/sky_ra18.yml index 955c17d..dd822b6 100644 --- a/places/sky_ra18.yml +++ b/places/sky_ra18.yml @@ -2102,8 +2102,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-551.jpg zoom_level: 0.0930775318528 --- _uuid: 5f4cc1e1-a723-4e1f-8061-ab51dbe65783 +astropix_id: chandra|581c classification: '' constellation: SCT +cxstatus: in:66f44187955f03d76f659793 data_set_type: Sky dec_deg: -4.9309987 foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-581cL{1}X{2}Y{3}.png