Abstract
We summarize the Sloan Digital Sky Survey data acquisition and processing steps, and describe runQA, a pipeline designed for automated data quality assessment. In particular, we show how the position of the stellar locus in color-color diagrams can be used to estimate the accuracy of photometric zeropoint calibration to better than 0.01 mag in 0.03 deg 2 patches. Using this method, we estimate that typical photometric zeropoint calibration errors for SDSS imaging data are not larger than ∼ 0.01 mag in the g, r, and i bands, 0.02 mag in the z band, and 0.03 mag in the u band (root-mean-scatter for zeropoint offsets).
Original language | English (US) |
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Pages (from-to) | 583-589 |
Number of pages | 7 |
Journal | Astronomische Nachrichten |
Volume | 325 |
Issue number | 6-8 |
DOIs | |
State | Published - 2004 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science
Keywords
- Methods: data analysis
- Stars: fundamental parameters
- Stars: statistics
- Surveys
- Techniques: photometric