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authorCoprDistGit <infra@openeuler.org>2023-05-15 05:39:41 +0000
committerCoprDistGit <infra@openeuler.org>2023-05-15 05:39:41 +0000
commit401e118b7213dce6c1f803b9ae709de4a6f7aa18 (patch)
treea9416c05ad0f6e19401266652ecc99d7527f4c87
parent88319be583144e2440e732876909549d3fc86e4b (diff)
automatic import of python-blimpy
-rw-r--r--.gitignore1
-rw-r--r--python-blimpy.spec456
-rw-r--r--sources1
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diff --git a/.gitignore b/.gitignore
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+/blimpy-2.1.4.tar.gz
diff --git a/python-blimpy.spec b/python-blimpy.spec
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index 0000000..d3f8975
--- /dev/null
+++ b/python-blimpy.spec
@@ -0,0 +1,456 @@
+%global _empty_manifest_terminate_build 0
+Name: python-blimpy
+Version: 2.1.4
+Release: 1
+Summary: Python utilities for Breakthrough Listen SETI observations
+License: BSD
+URL: https://github.com/ucberkeleyseti/blimpy
+Source0: https://mirrors.nju.edu.cn/pypi/web/packages/d2/0d/7ffc61a69a8582c810057c07445ed23d1617defe462ab9059981919bc2fc/blimpy-2.1.4.tar.gz
+BuildArch: noarch
+
+Requires: python3-astropy
+Requires: python3-numpy
+Requires: python3-six
+Requires: python3-setuptools
+Requires: python3-matplotlib
+Requires: python3-h5py
+Requires: python3-scipy
+Requires: python3-hdf5plugin
+Requires: python3-pandas
+Requires: python3-Pillow
+Requires: python3-psutil
+Requires: python3-pyparsing
+
+%description
+[![Build Status](https://github.com/UCBerkeleySETI/blimpy/workflows/Test%20Blimpy/badge.svg)](https://github.com/UCBerkeleySETI/blimpy/actions)
+[![Documentation Status](https://readthedocs.org/projects/blimpy/badge/?version=latest)](https://blimpy.readthedocs.io/en/latest/?badge=latest)
+[![codecov](https://codecov.io/gh/UCBerkeleySETI/blimpy/branch/master/graph/badge.svg)](https://codecov.io/gh/UCBerkeleySETI/blimpy)
+ [![JOSS status](http://joss.theoj.org/papers/e58ef21f0a924041bf9438fd75f8aed0/status.svg)](http://joss.theoj.org/papers/e58ef21f0a924041bf9438fd75f8aed0)
+
+## Breakthrough Listen I/O Methods for Python.
+
+### Filterbank + Raw file readers
+
+This repository contains Python 2/3 readers for interacting with [Sigproc filterbank](http://sigproc.sourceforge.net/sigproc.pdf) (.fil), HDF5 (.h5) and [guppi raw](https://baseband.readthedocs.io/en/stable/guppi/) (.raw) files,
+as used in the [Breakthrough Listen](https://seti.berkeley.edu) search for intelligent life.
+
+
+### Installation
+
+#### System Dependencies
+Sometimes the `pip` installation can fail if a system dependency is not installed. To fix this, make sure you have `curl` and install the required system dependencies with the command bellow:
+
+##### Debian/Ubuntu
+```
+curl https://raw.githubusercontent.com/UCBerkeleySETI/blimpy/master/dependencies.txt | xargs -n 1 sudo apt install --no-install-recommends -y
+```
+
+#### Manual Installation
+
+The latest release can be installed via pip directly from this repository:
+
+```
+python3 -m pip install -U git+https://github.com/UCBerkeleySETI/blimpy
+```
+
+Or, the latest version of the development code can be installed from the github [repo](https://github.com/UCBerkeleySETI/blimpy) and then run `python setup.py install` or `pip install .` (with sudo if required), or by using the following terminal command:
+
+```
+python3 -m pip install -U https://github.com/UCBerkeleySETI/blimpy/tarball/master
+```
+
+To install everything required to run the unit tests, run:
+
+```
+python3 -m pip install -e .[full]
+```
+
+You will need `numpy`, `h5py`, `astropy`, `scipy`, and `matplotlib` as dependencies. A `pip install` should pull in numpy, h5py, and astropy, but you may still need to install scipy and matplotlib separately.
+To interact with compressed files, you'll need the `hdf5plugin` package too.
+
+Note that h5py generally needs to be installed in this way:
+
+```
+$ python3 -m pip install --no-binary=h5py h5py
+```
+
+### Command line utilities
+
+After installation, the following command will display the metadata (header) values and some information about the data matrix:
+
+`watutil -i`
+
+Other command line utilities available post-installation:
+* `bldice`, Extract a smaller frequency region from a Filterbank file (.fil or .h5 file).
+* `calcload`, Calculate the Waterfall max_load value needed to load the entire data array for a given Filterbank file.
+* `dsamp`, Down-sample (time-dimension only) from one Filterbank file to another.
+* `fil2h5`, Convert a .fil file into .h5 format.
+* `h52fil`, Convert an .h5 file into .fil format.
+* `matchfils`, Check if two .fil files are the same.
+* `peek`, Display a selected portion of values from the data matrix of a Filterbank file.
+* `rawhdr`, Display the header fields of a raw guppi file.
+* `rawutil`, Plot data in a guppi raw file.
+* `srcname`, Patch the header source_name field in a .h5 file.
+* `stax`, For a collection of .h5 or .fil files sharing the same frequency range, create a vertical stack of waterfall plots as a single PNG file.
+* `stix`, For a single very large Filterbank file, create a horizontal or vertical stack of waterfall plots as a single PNG file.
+* `watutil`, Information/read/write/plot utility for Filterbank files.
+
+Use the `-h` flag to any of the above command line utilities to display their available arguments.
+
+### Reading blimpy filterbank files in .fil or .h5 format
+
+The `blimpy.Waterfall` provides a Python API for interacting with filterbank data. It supports all BL filterbank data products; see this [example Jupyter notebook](https://github.com/UCBerkeleySETI/blimpy/blob/master/examples/voyager.ipynb) for an overview.
+
+From the python, ipython or jupiter notebook environments.
+
+```python
+from blimpy import Waterfall
+fb = Waterfall('/path/to/filterbank.fil')
+#fb = Waterfall('/path/to/filterbank.h5') #works the same way
+fb.info()
+data = fb.data
+```
+
+### Reading guppi raw files
+The [Guppi Raw format](https://github.com/UCBerkeleySETI/breakthrough/blob/master/doc/RAW-File-Format.md) can be read using the `GuppiRaw` class from `guppi.py`:
+
+```python
+from blimpy import GuppiRaw
+gr = GuppiRaw('/path/to/guppirawfile.raw')
+
+header, data = gr.read_next_data_block()
+```
+
+or
+
+```python
+from blimpy import GuppiRaw
+gr = GuppiRaw('/path/to/guppirawfile.raw')
+
+for header, data_x, data_y in gr.get_data():
+ # process data
+```
+
+Note: most users should start analysis with filterbank files, which are smaller in size and have been generated from the guppi raw files.
+
+### Using blimpy inside Docker
+The blimpy images are pushed to a public repository after each successful build on Travis.
+If you have Docker installed, you can run the following commands to pull our images, which have the environment and dependencies set up for you.
+
+`docker pull fx196/blimpy:py3_kern_stable`
+
+Here is a [more complete guide](./docker_guide.md) on using blimpy in Docker.
+
+### Further reading
+
+A detailed overview of the data formats used in Breakthrough Listen can be found in our [data format paper](https://ui.adsabs.harvard.edu/abs/2019arXiv190607391L/abstract). An archive of data files from the Breakthrough Listen program is provided at [seti.berkeley.edu/opendata](http://seti.berkeley.edu/opendata).
+
+### If you have any requests or questions, please lets us know!
+
+
+%package -n python3-blimpy
+Summary: Python utilities for Breakthrough Listen SETI observations
+Provides: python-blimpy
+BuildRequires: python3-devel
+BuildRequires: python3-setuptools
+BuildRequires: python3-pip
+%description -n python3-blimpy
+[![Build Status](https://github.com/UCBerkeleySETI/blimpy/workflows/Test%20Blimpy/badge.svg)](https://github.com/UCBerkeleySETI/blimpy/actions)
+[![Documentation Status](https://readthedocs.org/projects/blimpy/badge/?version=latest)](https://blimpy.readthedocs.io/en/latest/?badge=latest)
+[![codecov](https://codecov.io/gh/UCBerkeleySETI/blimpy/branch/master/graph/badge.svg)](https://codecov.io/gh/UCBerkeleySETI/blimpy)
+ [![JOSS status](http://joss.theoj.org/papers/e58ef21f0a924041bf9438fd75f8aed0/status.svg)](http://joss.theoj.org/papers/e58ef21f0a924041bf9438fd75f8aed0)
+
+## Breakthrough Listen I/O Methods for Python.
+
+### Filterbank + Raw file readers
+
+This repository contains Python 2/3 readers for interacting with [Sigproc filterbank](http://sigproc.sourceforge.net/sigproc.pdf) (.fil), HDF5 (.h5) and [guppi raw](https://baseband.readthedocs.io/en/stable/guppi/) (.raw) files,
+as used in the [Breakthrough Listen](https://seti.berkeley.edu) search for intelligent life.
+
+
+### Installation
+
+#### System Dependencies
+Sometimes the `pip` installation can fail if a system dependency is not installed. To fix this, make sure you have `curl` and install the required system dependencies with the command bellow:
+
+##### Debian/Ubuntu
+```
+curl https://raw.githubusercontent.com/UCBerkeleySETI/blimpy/master/dependencies.txt | xargs -n 1 sudo apt install --no-install-recommends -y
+```
+
+#### Manual Installation
+
+The latest release can be installed via pip directly from this repository:
+
+```
+python3 -m pip install -U git+https://github.com/UCBerkeleySETI/blimpy
+```
+
+Or, the latest version of the development code can be installed from the github [repo](https://github.com/UCBerkeleySETI/blimpy) and then run `python setup.py install` or `pip install .` (with sudo if required), or by using the following terminal command:
+
+```
+python3 -m pip install -U https://github.com/UCBerkeleySETI/blimpy/tarball/master
+```
+
+To install everything required to run the unit tests, run:
+
+```
+python3 -m pip install -e .[full]
+```
+
+You will need `numpy`, `h5py`, `astropy`, `scipy`, and `matplotlib` as dependencies. A `pip install` should pull in numpy, h5py, and astropy, but you may still need to install scipy and matplotlib separately.
+To interact with compressed files, you'll need the `hdf5plugin` package too.
+
+Note that h5py generally needs to be installed in this way:
+
+```
+$ python3 -m pip install --no-binary=h5py h5py
+```
+
+### Command line utilities
+
+After installation, the following command will display the metadata (header) values and some information about the data matrix:
+
+`watutil -i`
+
+Other command line utilities available post-installation:
+* `bldice`, Extract a smaller frequency region from a Filterbank file (.fil or .h5 file).
+* `calcload`, Calculate the Waterfall max_load value needed to load the entire data array for a given Filterbank file.
+* `dsamp`, Down-sample (time-dimension only) from one Filterbank file to another.
+* `fil2h5`, Convert a .fil file into .h5 format.
+* `h52fil`, Convert an .h5 file into .fil format.
+* `matchfils`, Check if two .fil files are the same.
+* `peek`, Display a selected portion of values from the data matrix of a Filterbank file.
+* `rawhdr`, Display the header fields of a raw guppi file.
+* `rawutil`, Plot data in a guppi raw file.
+* `srcname`, Patch the header source_name field in a .h5 file.
+* `stax`, For a collection of .h5 or .fil files sharing the same frequency range, create a vertical stack of waterfall plots as a single PNG file.
+* `stix`, For a single very large Filterbank file, create a horizontal or vertical stack of waterfall plots as a single PNG file.
+* `watutil`, Information/read/write/plot utility for Filterbank files.
+
+Use the `-h` flag to any of the above command line utilities to display their available arguments.
+
+### Reading blimpy filterbank files in .fil or .h5 format
+
+The `blimpy.Waterfall` provides a Python API for interacting with filterbank data. It supports all BL filterbank data products; see this [example Jupyter notebook](https://github.com/UCBerkeleySETI/blimpy/blob/master/examples/voyager.ipynb) for an overview.
+
+From the python, ipython or jupiter notebook environments.
+
+```python
+from blimpy import Waterfall
+fb = Waterfall('/path/to/filterbank.fil')
+#fb = Waterfall('/path/to/filterbank.h5') #works the same way
+fb.info()
+data = fb.data
+```
+
+### Reading guppi raw files
+The [Guppi Raw format](https://github.com/UCBerkeleySETI/breakthrough/blob/master/doc/RAW-File-Format.md) can be read using the `GuppiRaw` class from `guppi.py`:
+
+```python
+from blimpy import GuppiRaw
+gr = GuppiRaw('/path/to/guppirawfile.raw')
+
+header, data = gr.read_next_data_block()
+```
+
+or
+
+```python
+from blimpy import GuppiRaw
+gr = GuppiRaw('/path/to/guppirawfile.raw')
+
+for header, data_x, data_y in gr.get_data():
+ # process data
+```
+
+Note: most users should start analysis with filterbank files, which are smaller in size and have been generated from the guppi raw files.
+
+### Using blimpy inside Docker
+The blimpy images are pushed to a public repository after each successful build on Travis.
+If you have Docker installed, you can run the following commands to pull our images, which have the environment and dependencies set up for you.
+
+`docker pull fx196/blimpy:py3_kern_stable`
+
+Here is a [more complete guide](./docker_guide.md) on using blimpy in Docker.
+
+### Further reading
+
+A detailed overview of the data formats used in Breakthrough Listen can be found in our [data format paper](https://ui.adsabs.harvard.edu/abs/2019arXiv190607391L/abstract). An archive of data files from the Breakthrough Listen program is provided at [seti.berkeley.edu/opendata](http://seti.berkeley.edu/opendata).
+
+### If you have any requests or questions, please lets us know!
+
+
+%package help
+Summary: Development documents and examples for blimpy
+Provides: python3-blimpy-doc
+%description help
+[![Build Status](https://github.com/UCBerkeleySETI/blimpy/workflows/Test%20Blimpy/badge.svg)](https://github.com/UCBerkeleySETI/blimpy/actions)
+[![Documentation Status](https://readthedocs.org/projects/blimpy/badge/?version=latest)](https://blimpy.readthedocs.io/en/latest/?badge=latest)
+[![codecov](https://codecov.io/gh/UCBerkeleySETI/blimpy/branch/master/graph/badge.svg)](https://codecov.io/gh/UCBerkeleySETI/blimpy)
+ [![JOSS status](http://joss.theoj.org/papers/e58ef21f0a924041bf9438fd75f8aed0/status.svg)](http://joss.theoj.org/papers/e58ef21f0a924041bf9438fd75f8aed0)
+
+## Breakthrough Listen I/O Methods for Python.
+
+### Filterbank + Raw file readers
+
+This repository contains Python 2/3 readers for interacting with [Sigproc filterbank](http://sigproc.sourceforge.net/sigproc.pdf) (.fil), HDF5 (.h5) and [guppi raw](https://baseband.readthedocs.io/en/stable/guppi/) (.raw) files,
+as used in the [Breakthrough Listen](https://seti.berkeley.edu) search for intelligent life.
+
+
+### Installation
+
+#### System Dependencies
+Sometimes the `pip` installation can fail if a system dependency is not installed. To fix this, make sure you have `curl` and install the required system dependencies with the command bellow:
+
+##### Debian/Ubuntu
+```
+curl https://raw.githubusercontent.com/UCBerkeleySETI/blimpy/master/dependencies.txt | xargs -n 1 sudo apt install --no-install-recommends -y
+```
+
+#### Manual Installation
+
+The latest release can be installed via pip directly from this repository:
+
+```
+python3 -m pip install -U git+https://github.com/UCBerkeleySETI/blimpy
+```
+
+Or, the latest version of the development code can be installed from the github [repo](https://github.com/UCBerkeleySETI/blimpy) and then run `python setup.py install` or `pip install .` (with sudo if required), or by using the following terminal command:
+
+```
+python3 -m pip install -U https://github.com/UCBerkeleySETI/blimpy/tarball/master
+```
+
+To install everything required to run the unit tests, run:
+
+```
+python3 -m pip install -e .[full]
+```
+
+You will need `numpy`, `h5py`, `astropy`, `scipy`, and `matplotlib` as dependencies. A `pip install` should pull in numpy, h5py, and astropy, but you may still need to install scipy and matplotlib separately.
+To interact with compressed files, you'll need the `hdf5plugin` package too.
+
+Note that h5py generally needs to be installed in this way:
+
+```
+$ python3 -m pip install --no-binary=h5py h5py
+```
+
+### Command line utilities
+
+After installation, the following command will display the metadata (header) values and some information about the data matrix:
+
+`watutil -i`
+
+Other command line utilities available post-installation:
+* `bldice`, Extract a smaller frequency region from a Filterbank file (.fil or .h5 file).
+* `calcload`, Calculate the Waterfall max_load value needed to load the entire data array for a given Filterbank file.
+* `dsamp`, Down-sample (time-dimension only) from one Filterbank file to another.
+* `fil2h5`, Convert a .fil file into .h5 format.
+* `h52fil`, Convert an .h5 file into .fil format.
+* `matchfils`, Check if two .fil files are the same.
+* `peek`, Display a selected portion of values from the data matrix of a Filterbank file.
+* `rawhdr`, Display the header fields of a raw guppi file.
+* `rawutil`, Plot data in a guppi raw file.
+* `srcname`, Patch the header source_name field in a .h5 file.
+* `stax`, For a collection of .h5 or .fil files sharing the same frequency range, create a vertical stack of waterfall plots as a single PNG file.
+* `stix`, For a single very large Filterbank file, create a horizontal or vertical stack of waterfall plots as a single PNG file.
+* `watutil`, Information/read/write/plot utility for Filterbank files.
+
+Use the `-h` flag to any of the above command line utilities to display their available arguments.
+
+### Reading blimpy filterbank files in .fil or .h5 format
+
+The `blimpy.Waterfall` provides a Python API for interacting with filterbank data. It supports all BL filterbank data products; see this [example Jupyter notebook](https://github.com/UCBerkeleySETI/blimpy/blob/master/examples/voyager.ipynb) for an overview.
+
+From the python, ipython or jupiter notebook environments.
+
+```python
+from blimpy import Waterfall
+fb = Waterfall('/path/to/filterbank.fil')
+#fb = Waterfall('/path/to/filterbank.h5') #works the same way
+fb.info()
+data = fb.data
+```
+
+### Reading guppi raw files
+The [Guppi Raw format](https://github.com/UCBerkeleySETI/breakthrough/blob/master/doc/RAW-File-Format.md) can be read using the `GuppiRaw` class from `guppi.py`:
+
+```python
+from blimpy import GuppiRaw
+gr = GuppiRaw('/path/to/guppirawfile.raw')
+
+header, data = gr.read_next_data_block()
+```
+
+or
+
+```python
+from blimpy import GuppiRaw
+gr = GuppiRaw('/path/to/guppirawfile.raw')
+
+for header, data_x, data_y in gr.get_data():
+ # process data
+```
+
+Note: most users should start analysis with filterbank files, which are smaller in size and have been generated from the guppi raw files.
+
+### Using blimpy inside Docker
+The blimpy images are pushed to a public repository after each successful build on Travis.
+If you have Docker installed, you can run the following commands to pull our images, which have the environment and dependencies set up for you.
+
+`docker pull fx196/blimpy:py3_kern_stable`
+
+Here is a [more complete guide](./docker_guide.md) on using blimpy in Docker.
+
+### Further reading
+
+A detailed overview of the data formats used in Breakthrough Listen can be found in our [data format paper](https://ui.adsabs.harvard.edu/abs/2019arXiv190607391L/abstract). An archive of data files from the Breakthrough Listen program is provided at [seti.berkeley.edu/opendata](http://seti.berkeley.edu/opendata).
+
+### If you have any requests or questions, please lets us know!
+
+
+%prep
+%autosetup -n blimpy-2.1.4
+
+%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-blimpy -f filelist.lst
+%dir %{python3_sitelib}/*
+
+%files help -f doclist.lst
+%{_docdir}/*
+
+%changelog
+* Mon May 15 2023 Python_Bot <Python_Bot@openeuler.org> - 2.1.4-1
+- Package Spec generated
diff --git a/sources b/sources
new file mode 100644
index 0000000..6cddee7
--- /dev/null
+++ b/sources
@@ -0,0 +1 @@
+f3aeb510fd6d319fa8283f09c06e76cc blimpy-2.1.4.tar.gz