First version of the CalSourceFlux3x3 product. The new fluxes were directly computed from the observations of many astronomical standards and the signal of the corresponding calibration block. Data was derived based on the central 3x3 spaxels.
Tables containing the fluxes of the calibration sources CS1 and CS2 at the key wavelengths of the calibration blocks: B3A_60, B2B_75, R1_150, R1_180.
HIPE> calTree = getCalTree(version=44) HIPE> csf3x3 = calTree.spectrometer.CalSourceFlux3x3 HIPE> kwId = csf3x3.keyWaveId # returns a String1d HIPE> kw = csf3x3.keyWave # returns a Double1d HIPE> cs1flux = csf3x3.cs1Flux # returns a Double3d HIPE> cs2flux = csf3x3.cs2Flux # returns a Double3d