		 
objID            = cpt.extID
unique_psps_fo_id  = ipptopsps
ippObjID         = cpt.objID | cpt.catID << 32
nDetections      = sql sum of cps.NCODE (xnTotal)
batchID          = ipptopsps
---------------- = 
gStackID         = ipptopsps / gpc1 db
gnTotal          = cps.NWARP
gnIncPSFMag      = cps.nused_wrp
gnIncKronMag     = cps.nused_kron_wrp 
gnIncApMag       = cps.nused_ap_wrp
gnIncR5          = cpy.NMEAS 
gnIncR6          = cpy.NMEAS 
---------------- = 
gPSFMag          = cps.MAG_PSF_WRP
gPSFMagErr       = cps.MAG_PSF_WRP_ERR
gPSFMagStd       = cps.MAG_PSF_WRP_STD
gKronMag         = cps.MAG_KRON_WRP
gKronMagErr      = cps.MAG_KRON_WRP_ERR
gKronMagStd      = cps.MAG_KRON_WRP_STD
gApMag           = cps.MAG_AP_WRP
gApMagErr        = cps.MAG_AP_WRP_ERR
gApMagStd        = cps.MAG_AP_WRP_STD
---------------- = 
gFmeanflxR5      = cpy.FLUX_AP_R5
gFmeanflxR5Err   = cpy.FLUX_ERR_AP_R5
gFmeanflxR5Std   = cpy.FLUX_STD_AP_R5
gFmeanflxR5Fill  = cpy.FLUX_FIL_AP_R5
gFmeanflxR6      = cpy.FLUX_AP_R6
gFmeanflxR6Err   = cpy.FLUX_ERR_AP_R6
gFmeanflxR6Std   = cpy.FLUX_STD_AP_R6
gFmeanflxR6Fill  = cpy.FLUX_FIL_AP_R6
gFlags           = cps.FLAGS
---------------- = 
gLensObjSmearX11 = cpy.X11_SM_OBJ
gLensObjSmearX12 = cpy.X12_SM_OBJ
gLensObjSmearX22 = cpy.X22_SM_OBJ
gLensObjSmearE1  = cpy.E1_SM_OBJ
gLensObjSmearE2  = cpy.E2_SM_OBJ
gLensObjShearX11 = cpy.X11_SH_OBJ
gLensObjShearX12 = cpy.X12_SH_OBJ
gLensObjShearX22 = cpy.X22_SH_OBJ
gLensObjShearE1  = cpy.E1_SH_OBJ
gLensObjShearE2  = cpy.E2_SH_OBJ
gLensPSFSmearX11 = cpy.X11_SM_PSF
gLensPSFSmearX12 = cpy.X12_SM_PSF
gLensPSFSmearX22 = cpy.X22_SM_PSF
gLensPSFSmearE1  = cpy.E1_SM_PSF
gLensPSFSmearE2  = cpy.E2_SM_PSF
gLensPSFShearX11 = cpy.X11_SH_PSF
gLensPSFShearX12 = cpy.X12_SH_PSF
gLensPSFShearX22 = cpy.X22_SH_PSF
gLensPSFShearE1  = cpy.E1_SH_PSF
gLensPSFShearE2  = cpy.E2_SH_PSF
---------------- = 
gGamma           = cpy.GAMMA
gE1              = cpy.E1
gE2              = cpy.E2

[NOTES:

 * PSF Mag, Kron Mag, Ap Mag stats are all 
   calculated from values in the existing Measure table

   XXX : no! we need to record fluxes, not mags

 * R5 & R6 ap flux values & lensing parameters need
   a new table

