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The Palomar Distant Solar System Survey (PDSSS) was a wide-field survey aimed at finding distant trans-Neptunian objects that used the robotic 1.2 m Samuel Oschin Telescope at Palomar Observatory and the QUEST large-area CCD camera.The survey was specifically designed to identify putative members of a Sedna-like population with perihelia greater than 45 AU. The limiting magnitude of this study was 21.3 in the R-band, it was sensitive out to distances of 1000 AU, and 12,000 square degrees of sky were searched. This observing program was responsible for the discovery of 25 minor planets including trans-Neptunian objects and centaurs. (309239) 2007 RW10 and Gǃkúnǁʼhòmdímà ((229762) 2007 UK126) were among the objects discovered by this survey. It redetected Sedna but no other objects in Sedna-

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  • Palomar Distant Solar System Survey (en)
  • Palomar Distant Solar System Survey (pt)
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  • The Palomar Distant Solar System Survey (PDSSS) was a wide-field survey aimed at finding distant trans-Neptunian objects that used the robotic 1.2 m Samuel Oschin Telescope at Palomar Observatory and the QUEST large-area CCD camera.The survey was specifically designed to identify putative members of a Sedna-like population with perihelia greater than 45 AU. The limiting magnitude of this study was 21.3 in the R-band, it was sensitive out to distances of 1000 AU, and 12,000 square degrees of sky were searched. This observing program was responsible for the discovery of 25 minor planets including trans-Neptunian objects and centaurs. (309239) 2007 RW10 and Gǃkúnǁʼhòmdímà ((229762) 2007 UK126) were among the objects discovered by this survey. It redetected Sedna but no other objects in Sedna- (en)
  • O Palomar Distant Solar System Survey (PDSSS) foi um amplo campo de pesquisa que visava encontrar objetos transnetunianos distantes usando o telescópio robótico Samuel Oschin de 1,2 metro do Observatório Palomar e a QUEST large-area câmera CCD. O PDSSS foi projetado especificamente para identificar possíveis membros de uma população Sedna com periélios superiores a 45 UA. A limitação de magnitude deste estudo foi de 21,3 na banda R, era sensível para distâncias de 1,000 AU, e 12.000 graus quadrados do céu foram revistados. Este programa de observação foi o responsável pela descoberta de 25 corpos menores, incluindo objetos transnetunianos e centauros. (309239) 2007 RW10 e (229762) 2007 UK126 estavam entre os objetos descobertos pelo projeto. Ele foi capaz de detectar Sedna, mas não consegu (pt)
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  • March 2015 (en)
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  • when did it run? (en)
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  • The Palomar Distant Solar System Survey (PDSSS) was a wide-field survey aimed at finding distant trans-Neptunian objects that used the robotic 1.2 m Samuel Oschin Telescope at Palomar Observatory and the QUEST large-area CCD camera.The survey was specifically designed to identify putative members of a Sedna-like population with perihelia greater than 45 AU. The limiting magnitude of this study was 21.3 in the R-band, it was sensitive out to distances of 1000 AU, and 12,000 square degrees of sky were searched. This observing program was responsible for the discovery of 25 minor planets including trans-Neptunian objects and centaurs. (309239) 2007 RW10 and Gǃkúnǁʼhòmdímà ((229762) 2007 UK126) were among the objects discovered by this survey. It redetected Sedna but no other objects in Sedna-like orbits were identified. (en)
  • O Palomar Distant Solar System Survey (PDSSS) foi um amplo campo de pesquisa que visava encontrar objetos transnetunianos distantes usando o telescópio robótico Samuel Oschin de 1,2 metro do Observatório Palomar e a QUEST large-area câmera CCD. O PDSSS foi projetado especificamente para identificar possíveis membros de uma população Sedna com periélios superiores a 45 UA. A limitação de magnitude deste estudo foi de 21,3 na banda R, era sensível para distâncias de 1,000 AU, e 12.000 graus quadrados do céu foram revistados. Este programa de observação foi o responsável pela descoberta de 25 corpos menores, incluindo objetos transnetunianos e centauros. (309239) 2007 RW10 e (229762) 2007 UK126 estavam entre os objetos descobertos pelo projeto. Ele foi capaz de detectar Sedna, mas não consegui identificar outros objetos em órbitas como Sedna. (pt)
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