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+%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">
+
+[![license: MIT](https://img.shields.io/badge/license-MIT-blue.svg)](https://github.com/tundeakins/Planet_tools/blob/master/LICENSE)
+[![PyPI version](https://badge.fury.io/py/Planet-tools.svg)](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">
+
+[![license: MIT](https://img.shields.io/badge/license-MIT-blue.svg)](https://github.com/tundeakins/Planet_tools/blob/master/LICENSE)
+[![PyPI version](https://badge.fury.io/py/Planet-tools.svg)](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">
+
+[![license: MIT](https://img.shields.io/badge/license-MIT-blue.svg)](https://github.com/tundeakins/Planet_tools/blob/master/LICENSE)
+[![PyPI version](https://badge.fury.io/py/Planet-tools.svg)](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