Results from the South Pole InfraRed EXplorer Telescope

• Main Authors: J. M. Rathborne, M. G. Burton
• Other Authors: The Pennsylvania State University CiteSeerX Archives
• Format: Text
• Language: English
• Published: 2003
• Subjects: Amundsen Scott South Pole Station; Amundsen-Scott; Amundsen-Scott South Pole Station; South Pole; South pole
• Online Access: http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.338.5127; http://arxiv.org/pdf/astro-ph/0310584v1.pdf

Abstract. The SPIREX telescope, located at the Amundsen–Scott South Pole Station, was a prototype system developed to exploit the excellent conditions for IR observing at the South Pole. Observations over two winter seasons achieved remarkably deep, high-resolution, wide-field images in the 3–5µm wavelength regime. Several star forming complexes were observed, including NGC 6334, Chamaeleon I, η Chamaeleontis, the Carina Nebula, 30 Doradus, RCW 57, RCW 38, as well as the Galactic Centre. Images were obtained of lines at 2.42µm H2, 3.29µm PAH and 4.05µm Br α, as well as 3.5µm L–band and 4.7µm M–band continuum emission. These data, combined with near–IR, mid–IR, and radio continuum maps, reveal the environments of these star forming sites, as well as any protostars lying within them. The SPIREX project, its observing and reduction methods, and some sample data are summarized here. 1.