| 3 | | TODO |
| | 3 | === Inputs === |
| | 4 | During the skycalibration stage of stack photometry a new fiuts table is created which contains the |
| | 5 | parameters to be used for forced photometry. |
| | 6 | |
| | 7 | This table has one row for each source with the following columns |
| | 8 | {{{ |
| | 9 | #!rst |
| | 10 | |
| | 11 | ========================== =============================== ============================= |
| | 12 | **Column** **Value for Extended Source** **Value for Extended Source** |
| | 13 | ========================== =============================== ============================= |
| | 14 | ID IPP_IDET IPP_IDET |
| | 15 | X X_PSF X_EXT |
| | 16 | Y Y_PSF Y_EXT |
| | 17 | FLUX PSF_INST_FLUX/EXPTIME 10**(-0.4*EXT_INST_MAG) |
| | 18 | AP_RADIUS AP_MAG_RADIUS AP_MAG_RADIUS |
| | 19 | KRON_RADIUS MOMENTS_R1*2.5 MOMENTS_R1*2.5 |
| | 20 | PETRO_RADIUS PETRO_RADIUS PETRO_RADIUS |
| | 21 | FIT_GALAXY 0 1 |
| | 22 | PSF_STAR PM_SOURCE_MODE_PSFSTAR PM_SOURCE_MODE_PSFSTAR |
| | 23 | R_MAJOR 0 EXT_WIDTH_MAJ |
| | 24 | R_MINOR 0 EXT_WIDTH_MIN |
| | 25 | THETA 0 EXT_THETA |
| | 26 | MODEL_TYPE -1 model type for best fit |
| | 27 | INDEX 0 0.5 / EXT_PAR_07 |
| | 28 | ========================== =============================== ============================= |