esbo_ds/ESBO-ETC
esbo_ds/ESBO-ETC
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This commit is contained in:
Lukas Klass 2020-07-21 13:45:40 +02:00
parent b618b9cbab
commit f21449d977
3 changed files with 46 additions and 42 deletions
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5
Jenkinsfile vendored
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@ -28,13 +28,16 @@ pipeline {
// clear out old files // clear out old files
sh 'rm -rf ${BUILD_DIR}' sh 'rm -rf ${BUILD_DIR}'
sh 'rm -f ${SPHINX_DIR}/sphinx-build.log' sh 'rm -f ${SPHINX_DIR}/sphinx-build.log'
sh 'ls ${WORKSPACE}' sh 'ls'
sh 'pyenv/bin/sphinx-build -b html docs/source docs/build/html'
/*
sh ''' sh '''
${WORKSPACE}/pyenv/bin/sphinx-build \ ${WORKSPACE}/pyenv/bin/sphinx-build \
-q -w ${SPHINX_DIR}/sphinx-build.log \ -q -w ${SPHINX_DIR}/sphinx-build.log \
-b html \ -b html \
-d ${SPHINX_DIR}/${BUILD_DIR}/doctrees ${SPHINX_DIR}/${SOURCE_DIR} ${SPHINX_DIR}/${BUILD_DIR} -d ${SPHINX_DIR}/${BUILD_DIR}/doctrees ${SPHINX_DIR}/${SOURCE_DIR} ${SPHINX_DIR}/${BUILD_DIR}
''' '''
*/
archiveArtifacts 'docs/build/html' archiveArtifacts 'docs/build/html'
} }
post { post {

79
esbo-etc_defaults.xml
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@ -1,62 +1,63 @@
<root> <root>
<common> <common>
<wl_min val="3" val_unit="um" comment="Shortest wavelength used for binning input spectra"/> <wl_min val="207.5" 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_max val="207.8" 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"/> <wl_delta val="0.15" val_unit="nm" comment="Wavelength increment used for binning input spectra"/>
<!-- <res val="1000" val_unit=""--> <res val="1.3127e6" val_unit=""
<!-- comment="Resolving power for common spectral binning. A linear binning wavelength integral is estimated as wl_min/R"/>--> 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"/> <d_aperture val="5" val_unit="m" comment="Diameter of the telescope aperture"/>
<psf val="Airy" osf="10" osf_unit="" comment="PSF of the optical system. Can be Airy or a file"/> <psf val="Airy" osf="10" osf_unit="" comment="PSF of the optical system. Can be Airy or a file"/>
<!-- <psf val="data/psf_2um.txt" osf="10" osf_unit="" comment="PSF of the optical system. Can be Airy or a file"/>--> <!-- <psf val="data/psf_2um.txt" osf="10" osf_unit="" comment="PSF of the optical system. Can be Airy or a file"/>-->
<!-- <jitter_sigma val="10" val_unit="arcsec" comment="Sigma of the telescope jitter"/>--> <!-- <jitter_sigma val="10" val_unit="arcsec" comment="Sigma of the telescope jitter"/>-->
<output path="output" format="fits" comment="Output directory to store output files"/> <output path="output" format="fits" comment="Output directory to store output files"/>
<exposure_time val="0.1, 1.2" val_unit="s" comment="The exposure time"/> <exposure_time val="2300" val_unit="s" comment="The exposure time"/>
<!-- <snr val="10, 10, 10" val_unit="" comment="Desired signal to noise ratio"/>--> <!-- <snr val="10, 10, 10" val_unit="" comment="Desired signal to noise ratio"/>-->
<!-- <snr val="data/snr.csv" comment="Desired signal to noise ratio"/>--> <!-- <snr val="data/snr.csv" comment="Desired signal to noise ratio"/>-->
<!-- <snr val="10" val_unit="" comment="Desired signal to noise ratio"/>--> <!-- <snr val="10" val_unit="" comment="Desired signal to noise ratio"/>-->
</common> </common>
<astroscene> <astroscene>
<target type="BlackBodyTarget" temp="5778" temp_unit="K" mag="10" mag_unit="mag" band="M" <target type="BlackBodyTarget" temp="26" temp_unit="K"/>
comment="Modeling the sun as mag 10 star. Size can be point or extended"/> <!-- <target type="FileTarget" file="data/target/science_case_point.csv"/>-->
<optical_component type="Atmosphere" transmittance="data/atmosphere/ESBO-DS_transmittance.txt" <!-- <target type="FileTarget" file="data/target/science_case.csv"/>-->
emission="data/atmosphere/ESBO-DS_emission.txt" comment="Including the atmosphere"/> <optical_component type="Atmosphere" transmittance="data/atmosphere/science_case_hcl.csv"/>
<optical_component type="CosmicBackground" temp="2.725" temp_unit="K"/>
<optical_component type="Atmosphere" transmittance="data/atmosphere/science_case.csv"
emission="data/atmosphere/science_case_emission.csv"/>
<!-- <optical_component type="StrayLight" emission="data/strayLight/emission.csv"--> <!-- <optical_component type="StrayLight" emission="data/strayLight/emission.csv"-->
<!-- comment="Including arbitrary noise sources"/>--> <!-- comment="Including arbitrary noise sources"/>-->
</astroscene> </astroscene>
<common_optics> <common_optics>
<optical_component type="Mirror" reflectance="data/mirror/Reflectance_UV-enhanced-aluminium-mirror.txt" <optical_component type="Mirror" reflectance="data/mirror/science_case.csv"
emissivity="1" temp="70" temp_unit="K" obstruction="0.04" comment="M1"/> emissivity="0.05" temp="-15" temp_unit="Celsius" obstruction="0.004"
<optical_component type="Mirror" reflectance="data/mirror/Reflectance_UV-enhanced-aluminium-mirror.txt" obstructor_temp="-20" obstructor_temp_unit="Celsius" obstructor_emissivity="0.05"
emissivity="1" temp="70" temp_unit="K" comment="M2"/> comment="M1"/>
<optical_component type="Mirror" reflectance="data/mirror/Reflectance_UV-enhanced-aluminium-mirror.txt" <optical_component type="Mirror" reflectance="data/mirror/science_case.csv"
emissivity="1" temp="70" temp_unit="K" comment="M3"/> emissivity="0.05" temp="-20" temp_unit="Celsius" comment="M2"/>
<!-- <optical_component type="Filter" band="M"--> <optical_component type="Mirror" reflectance="data/mirror/science_case.csv"
<!-- emissivity="data/filter/emissivity.csv" temp="70" temp_unit="K" comment="Filter wheel"/>--> emissivity="0.05" temp="-20" temp_unit="Celsius" comment="M3"/>
<!-- <optical_component type="Filter" start="400" start_unit="nm" end="480" end_unit="nm"--> <optical_component type="Mirror" reflectance="data/mirror/science_case.csv"
<!-- emissivity="data/filter/emissivity.csv" temp="70" temp_unit="K" comment="Filter wheel"/>--> emissivity="0.05" temp="-20" temp_unit="Celsius" comment="M4"/>
<optical_component type="Mirror" reflectance="data/mirror/science_case.csv"
emissivity="0.05" temp="-20" temp_unit="Celsius" comment="M5"/>
<optical_component type="Mirror" reflectance="data/mirror/science_case.csv"
emissivity="0.05" temp="4" temp_unit="K" comment="M6"/>
<optical_component type="Mirror" reflectance="data/mirror/science_case.csv"
emissivity="0.05" temp="4" temp_unit="K" comment="M7"/>
<optical_component type="Mirror" reflectance="data/mirror/science_case.csv"
emissivity="0.05" temp="4" temp_unit="K" comment="M8"/>
</common_optics> </common_optics>
<instrument> <instrument>
<optical_component type="Lens" transmittance="data/lens/Reflectance_UV-enhanced-aluminium-mirror.txt" <sensor type="Heterodyne">
emissivity="1" temp="70" temp_unit="K" comment="M4"/> <aperture_efficiency val="0.55" val_unit=""/>
<sensor type="Imager"> <main_beam_efficiency val="0.67" val_unit=""/>
<f_number val="13" val_unit="" comment="The working f/#"/> <receiver_temp val="1050" val_unit="K"/>
<pixel_geometry val="1024, 1024" val_unit="pix" comment="Pixel geometry"/> <eta_fss val="0.97" val_unit=""/>
<center_offset val="0.0, 0.0" val_unit="pix" comment="Shift of the array center"/> <lambda_line val="207.613" val_unit="um"/>
<pixel> <kappa val="1" val_unit=""/>
<quantum_efficiency val="data/ccd/PCO-Edge-42-QE.txt" comment="Quantum efficiency of the detector pixel"/> <!-- <n_on val="10" val_unit=""/>-->
<pixel_size val="6.5" val_unit="um"/>
<dark_current val="0.6" val_unit="electron / (pix * s)" comment="Detector dark current"/>
<sigma_read_out val="1.4" 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="80" comment="Contained energy for calculating the SNR. Can be Peak, FWHM, Min or the percentage of encircled energy."/>
<!-- <contained_pixels val="100" val_unit="pix" comment="Number of contained pixels."/>-->
</photometric_aperture>
</sensor> </sensor>
</instrument> </instrument>
</root> </root>

4
esbo_etc/classes/sensor/Heterodyne.py
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@ -314,8 +314,8 @@ class Heterodyne(ASensor):
else: else:
signal = SpectralQty(signal.wl, signal.qty.to(u.W / (u.m ** 2 * u.Hz * u.sr), signal = SpectralQty(signal.wl, signal.qty.to(u.W / (u.m ** 2 * u.Hz * u.sr),
equivalencies=u.spectral_density(signal.wl))) equivalencies=u.spectral_density(signal.wl)))
t_signal = signal * (u.sr * self.__main_beam_efficiency * self.__lambda_line ** 2 / ( t_signal = signal * (self.__main_beam_efficiency * signal.wl ** 2 / (
2 * k_B) * self.__eta_fss) 2 * k_B) * self.__eta_fss * u.sr)
t_signal = SpectralQty(t_signal.wl, t_signal.qty.decompose()) t_signal = SpectralQty(t_signal.wl, t_signal.qty.decompose())
logger.debug("Spectral signal temperature") logger.debug("Spectral signal temperature")
logger.debug(t_signal) logger.debug(t_signal)