Primary Header¶
The primary head will contain the following additional information:
$PrintPrimaryHeader fit/euc-she.xml she.psfLevel1CalibrationParameters
$SetSchemaPath she/euc-she-PsfLevel1CalibrationParameters.xsd
$PrintDataProductName
$PrintDataProductCustodian
$PrintSchemaFilename
1.1
$PrintDataProductElements
Creators:
SHE_PSFToolkit_GenerateInitialDefocusState
SHE_PSFToolkit_FitPDC
SHE_PSFToolkit_FitPDCInfocus
SHE_PSFToolkit_FitFieldZernikeModelState
Consumers:
SHE
PSF Level1 Calibration parameters, giving the current state of the telescope after fitting to defocused and infocus data at a particular roll angle.
Will include a set of Zernike amplitude/telescope optical layout parameters which describe wavefront propagation through the system, expected to consist of < 100 params (floats).
Detector state format TBD, will include parameters describing the brighter-fatter effect, chip-to-chip variation.
Will contain parameters describing the FOV-dependent mapping between the telescope model (optical layout) and zernike amplitudes, as a list of coefficients to a polynomial fit. TBD.
Will include catalogue of star identifier with \(\chi^2\) value per star, to satisfy R-SHE-PRD-F-100, as well as sub-pixel stellar position on the detector (2 floats), for the stellar images used in the calibration
CTI residual parameterisation TBD
The FITS output file will contain the following information:
HDU List
The primary head will contain the following additional information:
$PrintPrimaryHeader fit/euc-she.xml she.psfLevel1CalibrationParameters
These are parameters that describe mirror movements, based on a ray tracing model.
$PrintHDUTableContents fit/euc-she.xml she.psfLevel1CalibrationParameters SheTelescopeModeParams
The Zernike mode parameters describe the wavefront errors as a set of orthoganol functions that change in radial and azimuthal degree. A subset of all possible Zernike modes are used to describe the wavefront error. The coefficients are a combination of the modes that are related to different optical effects and polynomial functions that describe the variation across the field-of-view. A combination of defocused and infocus data helps to break the degeneracy between some of the different modes.
$PrintHDUTableContents fit/euc-she.xml she.psfLevel1CalibrationParameters SheZernikeModeParams
TBD. These are effects due to the detector electronics, such as the brighter-fatter effect.
$PrintHDUTableContents fit/euc-she.xml she.psfLevel1CalibrationParameters SheDetectorModelParams
A polynomial model describing the derived spectral throughput.
$PrintHDUTableContents fit/euc-she.xml she.psfLevel1CalibrationParameters ShePsfCalSpecThrough
The Fisher matrix parameters calculated from the maximum likelihood fit of the model to the stars in these field.
$PrintHDUTableContents fit/euc-she.xml she.psfLevel1CalibrationParameters ShePsfCalFisherMatrix
Details of the fit for each star used: how well the PSF models each individual star.
$PrintHDUTableContents fit/euc-she.xml she.psfLevel1CalibrationParameters ShePsfCalStarResiduals
The parameters used in the configuration of the SHE_PSF_Toolkit software.
$PrintHDUTableContents fit/euc-she.xml she.psfLevel1CalibrationParameters SheToolkitInputParams
The chi-squared and number of degrees of freedom of the fit.
$PrintHDUTableContents fit/euc-she.xml she.psfLevel1CalibrationParameters ShePsfDiagnostics