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<link>http://swift.gsfc.nasa.gov/</link>
<description>Swift</description>
<pubDate>Fri, 2 Mar 2012 11:29:00 -0500</pubDate>

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<title>NASA's Fermi, Swift See 'Shockingly Bright' Burst</title>
<link>http://www.nasa.gov/topics/universe/features/shocking-burst.html</link>
<description>A record-setting blast of gamma rays from a dying star in a distant galaxy has wowed astronomers around the world. The eruption, which is classified as a gamma-ray burst, or GRB, and designated GRB 130427A, produced the highest-energy light ever detected from such an event.</description>
<guid isPermaLink="false">id_72</guid>
<pubDate>03 May 2013</pubDate>
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<title>Dying Supergiant Stars Implicated in Hours-long Gamma-Ray Bursts</title>
<link>http://www.nasa.gov/mission_pages/swift/bursts/supergiant-stars.html</link>
<description>Three unusually long-lasting stellar explosions discovered by NASA's Swift satellite represent a previously unrecognized class of gamma-ray bursts (GRBs). Two international teams of astronomers studying these events conclude that they likely arose from the catastrophic death of supergiant stars hundreds of times larger than the sun.</description>
<guid isPermaLink="false">id_71</guid>
<pubDate>16 April 2013</pubDate>
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<title>NASA's Swift Sizes Up Comet ISON</title>
<link>http://www.nasa.gov/mission_pages/swift/bursts/ison.html</link>
<description>Astronomers from the University of Maryland at College Park (UMCP) and Lowell Observatory have used NASA's Swift satellite to check out comet C/2012 S1 (ISON), which may become one of the most dazzling in decades when it rounds the sun later this year.</description>
<guid isPermaLink="false">id_70</guid>
<pubDate>29 March 2013</pubDate>
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<title>NASA's Swift, Chandra Explore a Youthful 'Star Wreck'</title>
<link>http://www.nasa.gov/mission_pages/swift/bursts/star-wreck.html</link>
<description>While performing an extensive X-ray survey of our galaxy's central regions, NASA's Swift satellite has uncovered the previously unknown remains of a shattered star. Designated G306.3-0.9 after the coordinates of its sky position, the new object ranks among the youngest-known supernova remnants in our Milky Way galaxy.</description>
<guid isPermaLink="false">id_69</guid>
<pubDate>15 March 2013</pubDate>
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<title>Swift/UVOT CALDB Update</title>
<link>http://www.nasa.gov/mission_pages/swift/bursts/swift-images.html"</link>
<description><![CDATA[A new CALDB file describing the long term change in the sensitivity of the Swift/UVOT was released on January 18, 2013. The new file corrects the update on June 6, 2012, which erroneously produces no change in sensitivity instead of the actual gradual decline of 1.0% to 1.5% per year depending on filter. A more complete description of the file and its updates is available in <a href="http://swift.gsfc.nasa.gov/docs/heasarc/caldb/swift/docs/uvot/uvotcaldb_throughput_02b.pdf">this PDF</a>. General information about the use of Swift CALDB files is available at the <a href="http://heasarc.gsfc.nasa.gov/docs/heasarc/caldb/swift/">Swift Calibration</a> page.]]></description>
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<pubDate>25 February 2013</pubDate>
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<title>An Image Gallery Gift from NASA's Swift</title>
<link>http://www.nasa.gov/mission_pages/swift/bursts/swift-images.html</link>
<description>Of the three telescopes carried by NASA's Swift satellite, only one captures cosmic light at energies similar to those seen by the human eye. Although small by the standards of ground-based observatories, Swift's Ultraviolet/Optical Telescope (UVOT) plays a critical role in rapidly pinpointing the locations of gamma-ray bursts (GRBs), the brightest explosions in the cosmos</description>
<guid isPermaLink="false">id_67</guid>
<pubDate>28 December 2012</pubDate>
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<title>Swift Cycle 9 Results</title>
<link>http://heasarc.gsfc.nasa.gov/docs/swift/proposals/c9_acceptarg.html</link>
<description>Swift Cycle 9 Accepted Targets and Proposals Have Been Posted</description>
<guid isPermaLink="false">id_66</guid>
<pubDate>18 December 2012</pubDate>
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<title>Astronomers Catch Jet from Binge-Eating Black Hole</title>
<link>http://www.nasa.gov/topics/universe/features/andromeda-xray.html</link>
<description>Back in January, a new X-ray source flared and rapidly brightened in the Andromeda galaxy (M31), located 2.5 million light-years away. Classified as an ultraluminous X-ray source (ULX), the object is only the second ever seen in M31 and became the target of an intense observing campaign by orbiting X-ray telescopes - including NASA's Swift - and radio observatories on the ground. These efforts resulted in the first detection of radio-emitting jets from a stellar-mass black hole outside our own galaxy.</description>
<guid isPermaLink="false">id_65</guid>
<pubDate>12 December 2012</pubDate>
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<title>X-ray Satellites Monitor the Clashing Winds of a Colossal Binary</title>
<link>http://www.nasa.gov/mission_pages/swift/bursts/binary-clash.html</link>
<description>The hottest and most massive stars don't live long enough to disperse throughout the galaxy. Instead, they can be found near the clouds of gas and dust where they formed - and where they will explode as supernovae after a few million years. They huddle in tight clusters with other young stars or in looser groupings called OB associations, a name reflecting their impressive populations of rare O- and B-type stars.</description>
<guid isPermaLink="false">id_64</guid>
<pubDate>12 October 2012</pubDate>
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<title>Swift Cycle 9 GI Program</title>
<link>http://swift.gsfc.nasa.gov/</link>
<description>NASA received 158 proposals (slightly up from last year), requesting a total observing time of 13.2 Ms and $4.3M in funds for 866 targets. The Swift Cycle 9 Peer Review will be held in December to evaluate the merits of submitted proposals and choose those that are recommended for funding and observing time.</description>
<guid isPermaLink="false">id_64</guid>
<pubDate>05 October 2012</pubDate>
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<title>NASA's Swift Satellite Discovers a New Black Hole in our Galaxy</title>
<link>http://www.nasa.gov/mission_pages/swift/bursts/new-black-hole.html</link>
<description>NASA's Swift satellite recently detected a rising tide of high-energy X-rays from a source toward the center of our Milky Way galaxy. The outburst, produced by a rare X-ray nova, announced the presence of a previously unknown stellar-mass black hole.</description>
<guid isPermaLink="false">id_63</guid>
<pubDate>05 October 2012</pubDate>
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