- Timestamp:
- Dec 21, 2019, 12:53:05 PM (7 years ago)
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trunk/doc/release.2015/ps1.calibration/calibration.tex
r41197 r41210 741 741 ID\_MEAS\_OBJECT\_HAS\_TYCHO & 0x40000000 & measurement comes from an object with tycho data \\ 742 742 \hline 743 \multicolumn{3}{l}{These DVO flags correspond to PSPS flags \ippdbtable{DetectionFlags3} (Paper VI, Table 18), but without the leading {\tt ID\_MEAS\_}.} \\ 744 \hline 743 745 \end{tabular} 744 746 \end{center} … … 777 779 ID\_SECF\_HAS\_DES & 0x00800000 & This photcode has DES photometry (not used for PV3) \\ 778 780 ID\_SECF\_OBJ\_EXT & 0x01000000 & Extended in this band \\ 781 \hline 782 \multicolumn{3}{l}{These DVO flags correspond to PSPS flags \ippdbtable{ObjectFilterFlags} (Paper VI, Table 13), but without the leading {\tt ID\_}.} \\ 779 783 \hline 780 784 \end{tabular} … … 823 827 ID\_OBJ\_BAD\_STACK & 0x40000000 & poor-quality object in the stack ($< 1$ good stack) \\ 824 828 \hline 829 \multicolumn{3}{l}{These DVO flags correspond to PSPS flags \ippdbtable{ObjectInfoFlags} (Paper VI, Table 11), but without the leading {\tt ID\_OBJ\_}.} \\ 830 \hline 825 831 \end{tabular} 826 832 \end{center} … … 850 856 ID\_IMAGE\_PHOTOM\_UBERCAL & 0x00000200 & externally-supplied photometry zero point from ubercal analysis \\ 851 857 ID\_IMAGE\_ASTROM\_GMM & 0x00000400 & image was fitted to positions corrected by the galaxy motion model \\ 858 \hline 859 \multicolumn{3}{l}{These DVO flags correspond to PSPS flags \ippdbtable{ImageFlags} (Paper VI, Table 14), but without the leading {\tt ID\_IMAGE\_}.} \\ 852 860 \hline 853 861 \end{tabular}
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