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Table 2:

Astrometry of individual CCD frames of WFI mosaics.

Sky
Mean errors Frames No. UCAC2
path $\sigma(\Delta$$\alpha $cos$\delta)$ $\sigma(\Delta$$\delta)$ per year stars/frame
year mas mas    
2008 59 59 112 105
2009 58 56 112 79
2010 58 56 128 164
2011 61 59 160 153
2012 63 62 168 125
2013 63 62 168 107
2014 62 62 184 105
2015 58 57 168 132

Notes. Mean errors come from standard deviations of (O-C) residuals from individual (RA, Dec) solutions with the UCAC2 catalog. The six constants polynomial model was used to relate (x, y) measurements with (X, Y) tangent plane coordinates. The (x, y) centers were pre-corrected by the FDPs. See details in Sect. 4.2.


Source LaTeX | All tables | In the text

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