2020-06-30 10:26:43 +02:00
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<root>
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<common>
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<wl_min val="157.773" val_unit="um" comment="Shortest wavelength used for binning input spectra"/>
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<wl_max val="157.775" 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="299792.458" val_unit=""
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comment="Resolving power for common spectral binning. A linear binning wavelength integral is estimated as (wl_min + wl_max)/(2*R)"/>
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<d_aperture val="2.527" val_unit="m" comment="Diameter of the telescope aperture"/>
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2020-10-26 18:01:39 +01:00
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<psf type="Airy" osf="10" osf_unit="" comment="PSF of the optical system. Can be Airy or a file"/>
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2020-06-30 10:26:43 +02:00
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<!-- <psf val="data/psf.txt" osf="10" osf_unit="" comment="PSF of the optical system. Can be Airy or a file"/>-->
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<!-- <jitter_sigma val="0.1" val_unit="arcsec" comment="Sigma of the telescope jitter"/>-->
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<output path="output" format="csv" comment="Output directory to store output files"/>
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<exposure_time val="1900" val_unit="s" comment="The exposure time"/>
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<!-- <snr val="10, 10, 10" val_unit="" comment="Desired signal to noise ratio"/>-->
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<!-- <snr val="data/snr.csv" comment="Desired signal to noise ratio"/>-->
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<!-- <snr val="10" val_unit="" comment="Desired signal to noise ratio"/>-->
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</common>
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<astroscene>
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<!-- <target type="LineTarget" brightness_temp="0.52" brightness_temp_unit="K"-->
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<!-- comment="Modeling the sun as mag 10 star. Size can be point or extended"/>-->
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2020-09-09 16:59:20 +02:00
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<target type="FileTarget" file="tests/data/target/line.csv"/>
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<optical_component type="Atmosphere" transmittance="tests/data/atmosphere/transmittance_great.csv"
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2020-06-30 10:26:43 +02:00
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comment="Including the atmosphere"/>
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<!-- <optical_component type="StrayLight" emission="data/atmosphere/ESBO-DS_emission.txt"-->
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<!-- comment="Including arbitrary noise sources"/>-->
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<optical_component type="CosmicBackground" temp="220" temp_unit="K" emissivity="0.14"
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comment="Thermal atmospheric emission"/>
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</astroscene>
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<common_optics>
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2020-09-09 16:59:20 +02:00
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<optical_component type="Mirror" reflectance="tests/data/mirror/reflectance_great.csv" emissivity="0.08" temp="230"
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2020-06-30 10:26:43 +02:00
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temp_unit="K" obstruction="0.0" comment="M1"/>
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<!-- <optical_component type="Mirror" reflectance="0.86"-->
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<!-- emissivity="0" temp="70" temp_unit="K" obstruction="0.0" comment="M1"/>-->
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<!-- <optical_component type="Mirror" reflectance="data/mirror/Reflectance_UV-enhanced-aluminium-mirror.txt"-->
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<!-- emissivity="0" temp="70" temp_unit="K" comment="M2"/>-->
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<!-- <optical_component type="Mirror" reflectance="data/mirror/Reflectance_UV-enhanced-aluminium-mirror.txt"-->
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<!-- emissivity="0" temp="70" temp_unit="K" comment="M3"/>-->
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<!-- <optical_component type="Filter" band="M"-->
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<!-- emissivity="data/filter/emissivity.csv" temp="70" temp_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="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="Mirror" reflectance="data/lens/Reflectance_UV-enhanced-aluminium-mirror.txt"-->
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<!-- emissivity="0" temp="70" temp_unit="K" comment="M4"/>-->
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<sensor type="Heterodyne">
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<aperture_efficiency val="0.55" val_unit="" comment="Aperture efficiency"/>
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<main_beam_efficiency val="0.67" val_unit="" comment="Main beam efficiency"/>
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<receiver_temp val="1050" val_unit="K" comment="Noise temperature of the receiver"/>
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<eta_fss val="0.97" val_unit="" comment="Forward scattering efficiency"/>
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<lambda_line val="157.774" val_unit="um" comment="Line wavelength"/>
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<kappa val="1" val_unit="" comment="Backend degradation factor"/>
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<!-- <n_on val="10" val_unit="" comment="Number of on-source observations"/>-->
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</sensor>
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</instrument>
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</root>
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