| dbo:abstract |
Texas Supernova Search (TSS) is one of many ongoing projects to identify and record supernova events. The project is led by Robert Quimby and to date has found 35 supernovae, 29 of which they were the first to report on. In addition they have discovered twelve (extragalactic) novae (in M31 and M33, including a probable LBV) and six dwarf novae. The project's most notable successes are SN 2005ap and SN 2006gy, the two most powerful supernovae yet recorded. SN 2005ap was an extremely energetic type II supernova. It is reported to be the brightest supernova yet recorded, twice as bright as the previous record holder, SN 2006gy.Although SN 2005ap was twice as bright at its peak than SN 2006gy it was not as energetic overall as the former brightened and dimmed in a typical period of a few days whereas the latter remained very bright for many months. SN2005ap was about 300 times brighter than normal for a type II supernova. It has been speculated that this supernova involved the formation of a quark star. Time magazine listed the discovery of SN 2006gy as third in its Top 10 Scientific Discoveries for 2007. (en) Texas Supernova Search (TSS) – projekt poszukiwania gwiazd supernowych. Korzysta z automatycznego teleskopu optycznego ROTSE-IIIb, jednego z czterech zbudowanych przez ROTSE collaboration, w celu poszukiwania optycznych poświat błysków promieniowania gamma oraz 9,2-metrowego Hobby-Eberly Telescope (HET). (pl) 德州超新星搜尋(Texas Supernova Search)是許多正在進行，以尋找和記錄超新星事件的專案計畫之一。這個專案由主持，迄今已發現35顆超新星，且其中29顆是他們第一個發現的。此外，他們還發現12顆在M31和M33的新星 (包括可疑的LBV)，和6顆矮新星[1]。 這個專案最顯著的成就是發現SN 2005ap和SN 2006gy，這2顆是迄今所發現最明亮的超新星。SN 2005ap是能量最高的II型超新星，並且是所有報告中最明亮的超新星，比原先的紀錄保持者SN 2006gy還要亮2倍[2]。雖然SN 2005ap在它的峰值比SN 2006gy 亮2倍，但它的總能量沒有後者充沛。SN 2005ap如同一般的超新星只增亮了幾天就開始轉趨暗淡，而SN 2006gy的增光則維持了好幾個月。SN 2005ap的亮度是一般的II型超新星的300倍，因此推測這顆超新星的前身可能是顆夸克星 [3] （页面存档备份，存于互联网档案馆）。 時代雜誌將SN 2006gy的發現選為2007年十大科學發現的第三名[4] （页面存档备份，存于互联网档案馆）。 (zh) |
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http://www.nbcnews.com/id/21259692 http://www.journals.uchicago.edu/cgi-bin/resolve%3Fid=doi:10.1086/522862&erFrom=7094954502098682650Guest http://mcdonaldobservatory.org/news/releases/2007/1010.html https://web.archive.org/web/20080706134118/http:/grad40.as.utexas.edu/~quimby/tss/index.html https://www.newscientist.com/channel/astronomy/dn12778-enigmatic-supernova-smashes-brightness-record.html |
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| rdfs:comment |
Texas Supernova Search (TSS) – projekt poszukiwania gwiazd supernowych. Korzysta z automatycznego teleskopu optycznego ROTSE-IIIb, jednego z czterech zbudowanych przez ROTSE collaboration, w celu poszukiwania optycznych poświat błysków promieniowania gamma oraz 9,2-metrowego Hobby-Eberly Telescope (HET). (pl) 德州超新星搜尋(Texas Supernova Search)是許多正在進行，以尋找和記錄超新星事件的專案計畫之一。這個專案由主持，迄今已發現35顆超新星，且其中29顆是他們第一個發現的。此外，他們還發現12顆在M31和M33的新星 (包括可疑的LBV)，和6顆矮新星[1]。 這個專案最顯著的成就是發現SN 2005ap和SN 2006gy，這2顆是迄今所發現最明亮的超新星。SN 2005ap是能量最高的II型超新星，並且是所有報告中最明亮的超新星，比原先的紀錄保持者SN 2006gy還要亮2倍[2]。雖然SN 2005ap在它的峰值比SN 2006gy 亮2倍，但它的總能量沒有後者充沛。SN 2005ap如同一般的超新星只增亮了幾天就開始轉趨暗淡，而SN 2006gy的增光則維持了好幾個月。SN 2005ap的亮度是一般的II型超新星的300倍，因此推測這顆超新星的前身可能是顆夸克星 [3] （页面存档备份，存于互联网档案馆）。 時代雜誌將SN 2006gy的發現選為2007年十大科學發現的第三名[4] （页面存档备份，存于互联网档案馆）。 (zh) Texas Supernova Search (TSS) is one of many ongoing projects to identify and record supernova events. The project is led by Robert Quimby and to date has found 35 supernovae, 29 of which they were the first to report on. In addition they have discovered twelve (extragalactic) novae (in M31 and M33, including a probable LBV) and six dwarf novae. Time magazine listed the discovery of SN 2006gy as third in its Top 10 Scientific Discoveries for 2007. (en) |
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Texas Supernova Search (pl) Texas Supernova Search (en) 德州超新星搜尋 (zh) |
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