2012
DOI: 10.1117/12.925600
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Operation, control, and data system for Antarctic Survey Telescope (AST3)

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Cited by 10 publications
(2 citation statements)
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“…1. Deprojection -Each image was re-sampled to the same geometry as the template image (earlier epoch image) so that images were photometrically aligned to facilitate subtraction per the SWarp software package (Shang et al 2012). 2.…”
Section: Appendix A: Reduction and Difference-imaging Technique (Mcdonald 2012)mentioning
confidence: 99%
“…1. Deprojection -Each image was re-sampled to the same geometry as the template image (earlier epoch image) so that images were photometrically aligned to facilitate subtraction per the SWarp software package (Shang et al 2012). 2.…”
Section: Appendix A: Reduction and Difference-imaging Technique (Mcdonald 2012)mentioning
confidence: 99%
“…2), were prepared for Dome A Shang et al, 2012) with the aim of conducting a survey for supernovae (SN) and transient sources. Furthermore, a 2.5 m optical/infrared telescope (KDUSTthe Kunlun Dark Universe Survey Telescope) has been proposed by the Chinese Center for Antarctic Astronomy (CCAA) for Dome A to in order to explore the dark universe (e.g., Yuan et al (2013); Zhu et al (2014)).…”
Section: Kunlun Station At Dome Amentioning
confidence: 99%