ESBO-ETC/tests/data/esbo-etc_defaults.xml
2020-09-09 16:59:40 +02:00

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XML

<root>
<common>
<wl_min val="0.4" val_unit="um" comment="Shortest wavelength used for binning input spectra"/>
<wl_max val="0.5" val_unit="um" comment="Shortest wavelength used for binning input spectra"/>
<wl_delta val="1" val_unit="nm" comment="Wavelength increment used for binning input spectra"/>
<!-- <res val="1000" val_unit=""-->
<!-- comment="Resolving power for common spectral binning. A linear binning wavelength integral is estimated as wl_min/R"/>-->
<d_aperture val="0.5" val_unit="m" comment="Diameter of the telescope aperture"/>
<psf val="Airy" osf="10" comment="PSF of the optical system. Can be Airy or a file"/>
<!-- <psf val="tests/data/ps2f.txt" comment="PSF of the optical system. Can be Airy or a file"/>-->
<jitter_sigma val="1" val_unit="arcsec" comment="Sigma of the telescope jitter"/>
<output path="output" format="fits" comment="Output directory to store output files"/>
<exposure_time val="0.1" val_unit="s" comment="The exposure time"/>
<!-- <output_path val="output" comment="Output directory to store output files"/>-->
</common>
<astroscene>
<target type="BlackBodyTarget" temp="5778" temp_unit="K" mag="10" mag_unit="mag" band="V"
comment="Modeling the sun as mag 10 star"/>
<optical_component type="Atmosphere" transmittance="tests/data/atmosphere/transmittance.csv"
emission="tests/data/atmosphere/emission.csv" comment="Including the atmosphere"/>
<optical_component type="StrayLight" emission="tests/data/strayLight/emission.csv"
comment="Including arbitrary noise sources"/>
</astroscene>
<common_optics>
<optical_component type="Mirror" reflectance="tests/data/mirror/reflectance.csv"
emissivity="tests/data/mirror/emissivity.csv" temp="70" temp_unit="K" comment="M1"
obstruction="0.1" obstructor_temp="70" obstructor_temp_unit="K"/>
<optical_component type="Mirror" reflectance="tests/data/mirror/reflectance.csv"
emissivity="tests/data/mirror/emissivity.csv" temp="70" temp_unit="K" comment="M2"/>
<optical_component type="Mirror" reflectance="tests/data/mirror/reflectance.csv"
emissivity="tests/data/mirror/emissivity.csv" temp="70" temp_unit="K" comment="M3"/>
<!-- <optical_component type="Filter" band="B"-->
<!-- emissivity="tests/data/filter/emissivity.csv" val="70" val_unit="K" comment="Filter wheel"/>-->
<optical_component type="Filter" start="400" start_unit="nm" end="480" end_unit="nm"
emissivity="tests/data/filter/emissivity.csv" temp="70" temp_unit="K" comment="Filter wheel"/>
</common_optics>
<instrument>
<optical_component type="Lens" transmittance="tests/data/lens/transmittance.csv"
emissivity="tests/data/lens/emissivity.csv" temp="70" temp_unit="K" comment="M4"/>
<sensor type="Imager">
<f_number val="13" val_unit="" comment="The working f/#"/>
<pixel_geometry val="1024, 1024" val_unit="pix" comment="Pixel geometry"/>
<center_offset val="0, 0" val_unit="pix" comment="Shift of the array center"/>
<pixel>
<quantum_efficiency val="tests/data/ccd/QE.csv" comment="Quantum efficiency of the detector pixel"/>
<pixel_size val="6.5" val_unit="um"/>
<dark_current val="20" val_unit="electron / (pix * s)" comment="Detector dark current"/>
<sigma_read_out val="10.0" val_unit="electron(1/2) / pix" comment="Detector readout noise in e-rms"/>
<well_capacity val="30000" val_unit="electron" comment="Well capacity of a pixel"/>
</pixel>
<photometric_aperture comment="The photometric aperture used to calculate signal and noise.">
<shape val="square" comment="Shape of the photometric aperture. Can be square / circle"/>
<contained_energy val="min" comment="Contained energy for calculating the SNR. Can be Peak, FWHM, Min or the percentage of encircled energy."/>
<!-- <aperture_size val="20" val_unit="pix" comment="Number of contained pixels."/>-->
</photometric_aperture>
</sensor>
</instrument>
</root>