Paper
14 September 2010 Improving photometry of the Pi of the Sky
Katarzyna Malek, Lech Mankiewicz, Rafal Opiela, Marcin Sokolowski, Aleksander Filip Zarnecki
Author Affiliations +
Proceedings Volume 7745, Photonics Applications in Astronomy, Communications, Industry, and High-Energy Physics Experiments 2010; 77450D (2010) https://doi.org/10.1117/12.872110
Event: Photonics Applications in Astronomy, Communications, Industry, and High-Energy Physics Experiments 2010, 2010, Wilga, Poland
Abstract
After brief introduction to the Pi of the Sky project standard photometry method used in the data reduction will be described. After data quality cuts uncertainty of the single measurement is of the order of 0.018-0.024 magnitudo for stars 7-10m. With new calibration algorithm taking into account the spectral type of reference stars stability of the photometry algorithm can be significantly improved. Preliminary results from the BGInd variable are presented showing than uncertainty of the order of 0.013 can be obtained.
© (2010) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Katarzyna Malek, Lech Mankiewicz, Rafal Opiela, Marcin Sokolowski, and Aleksander Filip Zarnecki "Improving photometry of the Pi of the Sky", Proc. SPIE 7745, Photonics Applications in Astronomy, Communications, Industry, and High-Energy Physics Experiments 2010, 77450D (14 September 2010); https://doi.org/10.1117/12.872110
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KEYWORDS
Stars

Photometry

Sensors

Databases

Cameras

Point spread functions

Algorithm development

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