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