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diff --git a/python-planet-tools.spec b/python-planet-tools.spec new file mode 100644 index 0000000..ea34a35 --- /dev/null +++ b/python-planet-tools.spec @@ -0,0 +1,259 @@ +%global _empty_manifest_terminate_build 0 +Name: python-Planet-tools +Version: 0.4.0 +Release: 1 +Summary: Package with useful functions for exoplanetary research +License: MIT License +URL: https://github.com/tundeakins/Planet_tools +Source0: https://mirrors.nju.edu.cn/pypi/web/packages/de/48/cef87894d1d689d89985e4778da339eca7894cf7897b2671efcd967dc983/Planet_tools-0.4.0.tar.gz +BuildArch: noarch + +Requires: python3-pytest + +%description +# Planet Tools +Useful functions to perform everyday conversions and calculation of quantities in exoplanetary science. It is a work in progress, so I am constantly adding and modifying them. + +<img src="https://github.com/tundeakins/Planet_tools/blob/master/Planet_tools/planet_tools.png" width="300"> + +[](https://github.com/tundeakins/Planet_tools/blob/master/LICENSE) +[](https://badge.fury.io/py/Planet-tools) + + +To install +```bash +pip install Planet-tools +``` +or + +```bash +git clone https://github.com/tundeakins/Planet_tools.git +cd Planet_tools +python setup.py install +``` + +The **convert_params** module contains the following functions: + + - **P_to_aR** - convert period to scaled semi-major axis. + - **aR_to_rho_star** - Compute transit derived stellar density from the planet period and scaled semi major axis + - **impact_parameter** - Convert inclination to impact parameter b + + - **inclination** - Convert impact parameter b to inclination in degrees. + - **convert_LD_coeffs** - Convert between different LD laws +The **calculate_params** module contains the follwing functions: + + - **RL_Rroche** - Calculate ratio of Laplace radius to Roche radius + - **R_hill** - Compute the hill radius of a planet + - **R_roche** - Compute roche radius of a planet as a function of the planet's radius + - **T_eq** - Calculate equilibrium temperature of planet in Kelvin + - **ingress_duration** - Calculate the duration of ingress/egress. + - **ldtk_ldc** - Estimate quadratic limb darkening coefficients for a given star + - **phase_fold** - Given the observation time and period, return the phase of each observation time + - **planet_prot** - Calculate period of rotation of a planet + - **sigma_CCF** - Calculate CCF width of non-rotating star in km/s based on resolution of spectrograph + - **transit_duration** - Calculate the transit duration + +The **estimate_effect** module contains the following functions: + + - **photo_granulation** - Estimate the amplitude and timescale of granulation noise in photometric observations as given by Gilliland 2011 + - **chaplin_exptime** - Compute the optimal exposure time to reduce stellar p-mode oscillation amplitude in the given star to 0.1m/s and 0.09m/s according to Chaplin et al. 2019. + - **rv_precision_degrade** - Calculate factor by which RV precision of a stellar spectral type degrades due to vsini. + +The **some_stats** module contains the following functions: + + - **bic** - Compute the bayesian information criteria + - **aic** - Calculate the Aikake information criterion. + - **rmse** - Calculate the root-mean-square of the inputed error array (residuals) + - **sse** - Calculate the sum of squared error of inputed error array (residuals) + - **mse** - Calculate the mean-square error of imputed error array + - **mae** - Calculate the mean-absolute error of imputed error array + - **rse** - Calculate the relative-square error from the observed and calculated values + - **rae** - Calculate the relative-absolute error from the observed and calculated values + - **r_squared** - Calculate the R2_score commonly + + + + + +%package -n python3-Planet-tools +Summary: Package with useful functions for exoplanetary research +Provides: python-Planet-tools +BuildRequires: python3-devel +BuildRequires: python3-setuptools +BuildRequires: python3-pip +%description -n python3-Planet-tools +# Planet Tools +Useful functions to perform everyday conversions and calculation of quantities in exoplanetary science. It is a work in progress, so I am constantly adding and modifying them. + +<img src="https://github.com/tundeakins/Planet_tools/blob/master/Planet_tools/planet_tools.png" width="300"> + +[](https://github.com/tundeakins/Planet_tools/blob/master/LICENSE) +[](https://badge.fury.io/py/Planet-tools) + + +To install +```bash +pip install Planet-tools +``` +or + +```bash +git clone https://github.com/tundeakins/Planet_tools.git +cd Planet_tools +python setup.py install +``` + +The **convert_params** module contains the following functions: + + - **P_to_aR** - convert period to scaled semi-major axis. + - **aR_to_rho_star** - Compute transit derived stellar density from the planet period and scaled semi major axis + - **impact_parameter** - Convert inclination to impact parameter b + + - **inclination** - Convert impact parameter b to inclination in degrees. + - **convert_LD_coeffs** - Convert between different LD laws +The **calculate_params** module contains the follwing functions: + + - **RL_Rroche** - Calculate ratio of Laplace radius to Roche radius + - **R_hill** - Compute the hill radius of a planet + - **R_roche** - Compute roche radius of a planet as a function of the planet's radius + - **T_eq** - Calculate equilibrium temperature of planet in Kelvin + - **ingress_duration** - Calculate the duration of ingress/egress. + - **ldtk_ldc** - Estimate quadratic limb darkening coefficients for a given star + - **phase_fold** - Given the observation time and period, return the phase of each observation time + - **planet_prot** - Calculate period of rotation of a planet + - **sigma_CCF** - Calculate CCF width of non-rotating star in km/s based on resolution of spectrograph + - **transit_duration** - Calculate the transit duration + +The **estimate_effect** module contains the following functions: + + - **photo_granulation** - Estimate the amplitude and timescale of granulation noise in photometric observations as given by Gilliland 2011 + - **chaplin_exptime** - Compute the optimal exposure time to reduce stellar p-mode oscillation amplitude in the given star to 0.1m/s and 0.09m/s according to Chaplin et al. 2019. + - **rv_precision_degrade** - Calculate factor by which RV precision of a stellar spectral type degrades due to vsini. + +The **some_stats** module contains the following functions: + + - **bic** - Compute the bayesian information criteria + - **aic** - Calculate the Aikake information criterion. + - **rmse** - Calculate the root-mean-square of the inputed error array (residuals) + - **sse** - Calculate the sum of squared error of inputed error array (residuals) + - **mse** - Calculate the mean-square error of imputed error array + - **mae** - Calculate the mean-absolute error of imputed error array + - **rse** - Calculate the relative-square error from the observed and calculated values + - **rae** - Calculate the relative-absolute error from the observed and calculated values + - **r_squared** - Calculate the R2_score commonly + + + + + +%package help +Summary: Development documents and examples for Planet-tools +Provides: python3-Planet-tools-doc +%description help +# Planet Tools +Useful functions to perform everyday conversions and calculation of quantities in exoplanetary science. It is a work in progress, so I am constantly adding and modifying them. + +<img src="https://github.com/tundeakins/Planet_tools/blob/master/Planet_tools/planet_tools.png" width="300"> + +[](https://github.com/tundeakins/Planet_tools/blob/master/LICENSE) +[](https://badge.fury.io/py/Planet-tools) + + +To install +```bash +pip install Planet-tools +``` +or + +```bash +git clone https://github.com/tundeakins/Planet_tools.git +cd Planet_tools +python setup.py install +``` + +The **convert_params** module contains the following functions: + + - **P_to_aR** - convert period to scaled semi-major axis. + - **aR_to_rho_star** - Compute transit derived stellar density from the planet period and scaled semi major axis + - **impact_parameter** - Convert inclination to impact parameter b + + - **inclination** - Convert impact parameter b to inclination in degrees. + - **convert_LD_coeffs** - Convert between different LD laws +The **calculate_params** module contains the follwing functions: + + - **RL_Rroche** - Calculate ratio of Laplace radius to Roche radius + - **R_hill** - Compute the hill radius of a planet + - **R_roche** - Compute roche radius of a planet as a function of the planet's radius + - **T_eq** - Calculate equilibrium temperature of planet in Kelvin + - **ingress_duration** - Calculate the duration of ingress/egress. + - **ldtk_ldc** - Estimate quadratic limb darkening coefficients for a given star + - **phase_fold** - Given the observation time and period, return the phase of each observation time + - **planet_prot** - Calculate period of rotation of a planet + - **sigma_CCF** - Calculate CCF width of non-rotating star in km/s based on resolution of spectrograph + - **transit_duration** - Calculate the transit duration + +The **estimate_effect** module contains the following functions: + + - **photo_granulation** - Estimate the amplitude and timescale of granulation noise in photometric observations as given by Gilliland 2011 + - **chaplin_exptime** - Compute the optimal exposure time to reduce stellar p-mode oscillation amplitude in the given star to 0.1m/s and 0.09m/s according to Chaplin et al. 2019. + - **rv_precision_degrade** - Calculate factor by which RV precision of a stellar spectral type degrades due to vsini. + +The **some_stats** module contains the following functions: + + - **bic** - Compute the bayesian information criteria + - **aic** - Calculate the Aikake information criterion. + - **rmse** - Calculate the root-mean-square of the inputed error array (residuals) + - **sse** - Calculate the sum of squared error of inputed error array (residuals) + - **mse** - Calculate the mean-square error of imputed error array + - **mae** - Calculate the mean-absolute error of imputed error array + - **rse** - Calculate the relative-square error from the observed and calculated values + - **rae** - Calculate the relative-absolute error from the observed and calculated values + - **r_squared** - Calculate the R2_score commonly + + + + + +%prep +%autosetup -n Planet-tools-0.4.0 + +%build +%py3_build + +%install +%py3_install +install -d -m755 %{buildroot}/%{_pkgdocdir} +if [ -d doc ]; then cp -arf doc %{buildroot}/%{_pkgdocdir}; fi +if [ -d docs ]; then cp -arf docs %{buildroot}/%{_pkgdocdir}; fi +if [ -d example ]; then cp -arf example %{buildroot}/%{_pkgdocdir}; fi +if [ -d examples ]; then cp -arf examples %{buildroot}/%{_pkgdocdir}; fi +pushd %{buildroot} +if [ -d usr/lib ]; then + find usr/lib -type f -printf "/%h/%f\n" >> filelist.lst +fi +if [ -d usr/lib64 ]; then + find usr/lib64 -type f -printf "/%h/%f\n" >> filelist.lst +fi +if [ -d usr/bin ]; then + find usr/bin -type f -printf "/%h/%f\n" >> filelist.lst +fi +if [ -d usr/sbin ]; then + find usr/sbin -type f -printf "/%h/%f\n" >> filelist.lst +fi +touch doclist.lst +if [ -d usr/share/man ]; then + find usr/share/man -type f -printf "/%h/%f.gz\n" >> doclist.lst +fi +popd +mv %{buildroot}/filelist.lst . +mv %{buildroot}/doclist.lst . + +%files -n python3-Planet-tools -f filelist.lst +%dir %{python3_sitelib}/* + +%files help -f doclist.lst +%{_docdir}/* + +%changelog +* Thu May 18 2023 Python_Bot <Python_Bot@openeuler.org> - 0.4.0-1 +- Package Spec generated |