LSST Applications 24.1.5,g02d81e74bb+fa3a7a026e,g180d380827+a53a32eff8,g2079a07aa2+86d27d4dc4,g2305ad1205+c0501b3732,g295015adf3+7d3e92f0ec,g2bbee38e9b+0e5473021a,g337abbeb29+0e5473021a,g33d1c0ed96+0e5473021a,g3a166c0a6a+0e5473021a,g3ddfee87b4+5dd1654d75,g48712c4677+3bf1020dcb,g487adcacf7+065c13d9cf,g50ff169b8f+96c6868917,g52b1c1532d+585e252eca,g591dd9f2cf+d7ac436cfb,g5a732f18d5+53520f316c,g64a986408d+fa3a7a026e,g858d7b2824+fa3a7a026e,g8a8a8dda67+585e252eca,g99cad8db69+a5a909b84f,g9ddcbc5298+9a081db1e4,ga1e77700b3+15fc3df1f7,ga8c6da7877+4cf350ccb2,gb0e22166c9+60f28cb32d,gba4ed39666+c2a2e4ac27,gbb8dafda3b+f991a0b59f,gc120e1dc64+9ccbfdb8be,gc28159a63d+0e5473021a,gcf0d15dbbd+5dd1654d75,gd96a1ce819+42fd0ee607,gdaeeff99f8+f9a426f77a,ge6526c86ff+0d71447b4b,ge79ae78c31+0e5473021a,gee10cc3b42+585e252eca,gff1a9f87cc+fa3a7a026e
LSST Data Management Base Package
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Classes | |
class | FgcmMakeLutConfig |
class | FgcmMakeLutConnections |
class | FgcmMakeLutParametersConfig |
class | FgcmMakeLutTask |
class | SensorCorrectionTerms |
Make a look-up-table (LUT) for FGCM calibration. This task computes a look-up-table for the range in expected atmosphere variation and variation in instrumental throughput (as tracked by the transmission_filter products). By pre-computing linearized integrals, the FGCM fit is orders of magnitude faster for stars with a broad range of colors and observing bands, yielding precision at the 1-2 mmag level. Computing a LUT requires running MODTRAN or with a pre-generated atmosphere table packaged with fgcm.