esbo_ds/ESBO-ETC
esbo_ds/ESBO-ETC
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This commit is contained in:
Lukas Klass 2020-05-08 15:06:56 +02:00
parent da21b14d43
commit 0de92c26c7
1 changed files with 20 additions and 18 deletions
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38
tests/data/esbo-etc_defaults.xml
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@ -1,23 +1,19 @@
<root>
<common>
<wl_min val="400" val_unit="nm" comment="Shortest wavelength used for binning input spectra"/>
<wl_max val="500" val_unit="nm" comment="Shortest wavelength used for binning input spectra"/>
<wl_delta val="10" val_unit="nm" comment="Wavelength increment used for binning input spectra"/>
<wl_min val="3" val_unit="um" comment="Shortest wavelength used for binning input spectra"/>
<wl_max val="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="5" val_unit="m" comment="Diameter of the telescope aperture"/>
<jitter_rms val="0.1" val_unit="arcsec" comment="Sigma RMS of the telescope jitter"/>
<d_aperture val="0.5" val_unit="m" comment="Diameter of the telescope aperture"/>
<psf val="Airy" comment="PSF of the optical system. Can be Airy or a file"/>
<!-- <psf val="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 val="output" comment="Output directory to store output files"/>
</common>
<noise>
<EnableJitter val="False"/>
<EnableShotNoise val="True"/>
<EnableReadoutNoise val="True"/>
</noise>
<astroscene>
<target type="BlackBodyTarget" temp="5778" temp_unit="K" mag="10" band="V"
<target type="BlackBodyTarget" temp="5778" temp_unit="K" mag="10" mag_unit="mag" band="V" size="point"
comment="Modeling the sun as mag 10 star"/>
<optical_component type="Atmosphere" transmittance="data/atmosphere/transmittance.csv"
emission="data/atmosphere/emission.csv" comment="Including the atmosphere"/>
@ -42,15 +38,21 @@
<instrument>
<optical_component type="Lens" transmittance="data/lens/transmittance.csv"
emissivity="data/lens/emissivity.csv" temp="70" temp_unit="K" comment="M4"/>
<sensor type="CCD">
<f_number val="18.5" val_unit="" comment="The working f/#"/>
<pixel_geometry val="1024, 1024" val_unit="" comment="Pixel geometry"/>
<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="um" comment="Shift of the array center"/>
<pixel>
<quantum_efficiency val="data/ccd/qe.csv" comment="Quantum efficiency of the detector pixel"/>
<pixel_size val="15" val_unit="micron"/>
<dark_current val="20" val_unit="1/s" comment="Detector dark current"/>
<sigma_read_out val="10.0" val_unit="" comment="Detector readout noise in e-rms"/>
<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"/>
</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."/>
<!-- <contained_pixels val="20" val_unit="pix" comment="Number of contained pixels."/>-->
</photometric_aperture>
</sensor>
</instrument>
</root>