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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.aliyun.com/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 Jun 08 2023 Python_Bot <Python_Bot@openeuler.org> - 0.4.0-1
- Package Spec generated
|
