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Repository: kbarbary/sep
Branch: main
Commit: 93b3ac52e0f6
Files: 61
Total size: 935.7 KB
Directory structure:
gitextract_54cmwk4y/
├── .clang-format
├── .github/
│ └── workflows/
│ ├── build-wheels-upload-pypi.yml
│ └── python-package-tox.yml
├── .gitignore
├── .pre-commit-config.yaml
├── .readthedocs.yaml
├── AUTHORS.md
├── CHANGES.md
├── CMakeLists.txt
├── FindSEP.cmake
├── MANIFEST.in
├── Makefile
├── README.md
├── bench.py
├── codemeta.json
├── ctest/
│ ├── compare.py
│ └── test_image.c
├── data/
│ ├── README.md
│ ├── back.fits
│ ├── default.conv
│ ├── default.nnw
│ ├── default.param
│ ├── default.sex
│ ├── image.cat
│ ├── image.fits
│ └── rms.fits
├── docs/
│ ├── Makefile
│ ├── apertures.rst
│ ├── changelogs/
│ │ ├── changelog.rst
│ │ ├── changes_to_c_api.rst
│ │ ├── new_changes.rst
│ │ └── original_changes.md
│ ├── conf.py
│ ├── filter.rst
│ ├── index.rst
│ ├── reference.rst
│ ├── rtd-pip-requirements
│ └── tutorial.ipynb
├── licenses/
│ ├── BSD_LICENSE.txt
│ ├── LGPL_LICENSE.txt
│ └── MIT_LICENSE.txt
├── paper/
│ ├── paper.bib
│ └── paper.md
├── pyproject.toml
├── sep.pyx
├── setup.py
├── src/
│ ├── analyse.c
│ ├── aperture.c
│ ├── aperture.i
│ ├── background.c
│ ├── convolve.c
│ ├── deblend.c
│ ├── extract.c
│ ├── extract.h
│ ├── lutz.c
│ ├── overlap.h
│ ├── sep.h
│ ├── sepcore.h
│ └── util.c
├── test.py
└── tox.ini
================================================
FILE CONTENTS
================================================
================================================
FILE: .clang-format
================================================
# SPDX-License-Identifier: MIT
#
# Copyright (c) 2023 Intercreate, Inc.
# Author: J.P. Hutchins <jp@intercreate.io>
#
# Python(black)-inspired .clang-format for C repositories
#
# Includes Zephyr and Arm macro compatibility
---
BasedOnStyle: Google
AlignAfterOpenBracket: BlockIndent
AlignTrailingComments: false
AllowAllArgumentsOnNextLine: true
AllowAllParametersOfDeclarationOnNextLine: true
AllowShortBlocksOnASingleLine: Never
AllowShortCaseLabelsOnASingleLine: false
AllowShortEnumsOnASingleLine: false
AllowShortFunctionsOnASingleLine: Empty
AllowShortIfStatementsOnASingleLine: Never
AllowShortLoopsOnASingleLine: false
AttributeMacros:
- __aligned
- __deprecated
- __packed
- __printf_like
- __syscall
- __syscall_always_inline
- __subsystem
BinPackArguments: false
BinPackParameters: false
BraceWrapping:
AfterCaseLabel: false
AfterClass: false
AfterControlStatement: MultiLine
AfterEnum: false
AfterFunction: false
AfterNamespace: false
AfterObjCDeclaration: false
AfterStruct: false
AfterUnion: false
AfterExternBlock: false
BeforeCatch: false
BeforeElse: false
IndentBraces: false
SplitEmptyFunction: false
SplitEmptyRecord: false
SplitEmptyNamespace: false
BeforeLambdaBody: false
BeforeWhile: false
BitFieldColonSpacing: After
BreakBeforeBinaryOperators: NonAssignment
BreakBeforeBraces: Custom
BreakStringLiterals: true
ColumnLimit: 88
DerivePointerAlignment: false
ForEachMacros:
- 'FOR_EACH'
- 'FOR_EACH_FIXED_ARG'
- 'FOR_EACH_IDX'
- 'FOR_EACH_IDX_FIXED_ARG'
- 'FOR_EACH_NONEMPTY_TERM'
- 'RB_FOR_EACH'
- 'RB_FOR_EACH_CONTAINER'
- 'SYS_DLIST_FOR_EACH_CONTAINER'
- 'SYS_DLIST_FOR_EACH_CONTAINER_SAFE'
- 'SYS_DLIST_FOR_EACH_NODE'
- 'SYS_DLIST_FOR_EACH_NODE_SAFE'
- 'SYS_SFLIST_FOR_EACH_CONTAINER'
- 'SYS_SFLIST_FOR_EACH_CONTAINER_SAFE'
- 'SYS_SFLIST_FOR_EACH_NODE'
- 'SYS_SFLIST_FOR_EACH_NODE_SAFE'
- 'SYS_SLIST_FOR_EACH_CONTAINER'
- 'SYS_SLIST_FOR_EACH_CONTAINER_SAFE'
- 'SYS_SLIST_FOR_EACH_NODE'
- 'SYS_SLIST_FOR_EACH_NODE_SAFE'
- '_WAIT_Q_FOR_EACH'
- 'Z_FOR_EACH'
- 'Z_FOR_EACH_ENGINE'
- 'Z_FOR_EACH_EXEC'
- 'Z_FOR_EACH_FIXED_ARG'
- 'Z_FOR_EACH_FIXED_ARG_EXEC'
- 'Z_FOR_EACH_IDX'
- 'Z_FOR_EACH_IDX_EXEC'
- 'Z_FOR_EACH_IDX_FIXED_ARG'
- 'Z_FOR_EACH_IDX_FIXED_ARG_EXEC'
- 'Z_GENLIST_FOR_EACH_CONTAINER'
- 'Z_GENLIST_FOR_EACH_CONTAINER_SAFE'
- 'Z_GENLIST_FOR_EACH_NODE'
- 'Z_GENLIST_FOR_EACH_NODE_SAFE'
- 'STRUCT_SECTION_FOREACH'
- 'TYPE_SECTION_FOREACH'
IncludeBlocks: Preserve
IfMacros:
- 'CHECKIF'
IndentCaseBlocks: true
IndentCaseLabels: false
IndentWidth: 2
InsertBraces: true
MaxEmptyLinesToKeep: 2
PointerAlignment: Middle
SortIncludes: CaseSensitive
SpaceBeforeParens: ControlStatementsExceptControlMacros
UseTab: Never
WhitespaceSensitiveMacros:
- STRINGIFY
- Z_STRINGIFY
================================================
FILE: .github/workflows/build-wheels-upload-pypi.yml
================================================
# GitHub action for building the distribution and wheels of the sep package
# and uploading them to the PyPI package index.
name: build-wheels-upload-pypi
on: [push, workflow_dispatch]
# push:
# # Run this action on the trigger event when *any* tag is pushed
# tags:
# - '*'
jobs:
# This action is split into three jobs:
# - Building the source distribution
# - Building the wheels for the distribution
# - Uploading the artifacts to PyPI package
# The first and second job run in parallel.
# The uploading jos needs to have the other two finished without error.
# From now on, we run the tests before continuing with these jobs.
run_tests:
uses: ./.github/workflows/python-package-tox.yml
build_sdist:
needs: [run_tests]
# First the source distribution is done on ubuntu. This is not related
# to any operating system, so we could do it on the default os.
runs-on: ubuntu-24.04
steps:
- name: checkout
uses: actions/checkout@v4
with:
fetch-depth: 0
fetch-tags: true
- name: install_python
uses: actions/setup-python@v5
with:
python-version: '3.12'
# For the build, sep needs numpy and cython and we add twine and wheel
# for better testing and checking.
- name: Install dependencies
run: python -m pip install setuptools twine numpy wheel cython build
- name: Build sdist
run: python -m build --sdist
- name: Show files
run: ls -lh dist
shell: bash
- name: Check metadata
run: twine check dist/*
- name: Upload sdist
uses: actions/upload-artifact@v4
with:
name: dist
path: dist/*.tar.gz
build_wheels:
needs: [run_tests]
# Second the wheels are build for different OS and python versions. This is
# done with the help of the `cibuildwheel` package.
#
# The wheels are built for Windows, Linux and MacOS and the python versions
# 3.9 - 3.13.
#
# The three operating system could be done in parallel.
name: Build wheels on ${{ matrix.os }}
runs-on: ${{ matrix.os }}
env:
CIBW_ARCHS_MACOS: "x86_64 universal2 arm64"
strategy:
max-parallel: 4
matrix:
python-version: ["3.12"]
os: [windows-latest, macos-latest, ubuntu-24.04, ubuntu-24.04-arm]
steps:
- uses: actions/checkout@v4
- name: checkout
uses: actions/checkout@v4
with:
fetch-depth: 0
fetch-tags: true
- name: Setup Python ${{ matrix.python-version }}
uses: actions/setup-python@v5
with:
python-version: ${{ matrix.python-version }}
- name: Install cibuildwheel
run: python -m pip install cibuildwheel
- name: Build wheels
run: python -m cibuildwheel --output-dir wheelhouse
env:
CIBW_BUILD: "cp39-* cp310-* cp311-* cp312-* cp313-*"
CIBW_MANYLINUX_X86_64_IMAGE: manylinux2014
CIBW_MANYLINUX_I686_IMAGE: manylinux2014
CIBW_BUILD_VERBOSITY: 1
CIBW_SKIP: '*-musllinux_*'
CIBW_ARCHS_LINUX: "auto"
- name: Show files
run: ls -lh wheelhouse
shell: bash
- name: Upload wheels
uses: actions/upload-artifact@v4
with:
name: dist-${{ matrix.os }}
path: ./wheelhouse/*.whl
upload_to_pypi:
# Finally we collect all out data from the artifacts and put them back to
# dist directory for upload. The final step waits for the other jobs to be
# finished and starts only if the trigger event of the action was a push
# of a tag starting with <v> as version separation. All other jobs run
# without heading <v>
runs-on: [ubuntu-latest]
needs: [build_wheels, build_sdist]
environment:
name: pypi
url: https://pypi.org/p/sep
permissions:
id-token: write
# upload to PyPI on every tag starting with 'v'
if: github.event_name == 'push' && startsWith(github.event.ref, 'refs/tags/v')
steps:
- uses: actions/setup-python@v5
- uses: actions/download-artifact@v4
with:
pattern: dist*
merge-multiple: true
path: dist
- name: upload_to_pypi
uses: pypa/gh-action-pypi-publish@release/v1
# with:
# repository-url: https://test.pypi.org/legacy/
================================================
FILE: .github/workflows/python-package-tox.yml
================================================
# This workflow will install tox and use it to run tests.
# For more information see: https://help.github.com/actions/language-and-framework-guides/using-python-with-github-actions
name: CI
on: [push, workflow_call, workflow_dispatch, pull_request]
jobs:
build:
runs-on: ${{ matrix.os }}
strategy:
matrix:
python: ["3.9", "3.10", "3.11", "3.12", "3.13"]
os: [windows-latest, macos-latest, ubuntu-latest]
steps:
- uses: actions/checkout@v4
- name: Setup Python
uses: actions/setup-python@v5
with:
python-version: ${{ matrix.python }}
- name: Install Tox and any other packages
run: |
python -m pip install --upgrade pip
python -m pip install tox tox-gh-actions
- name: Run Tox
# Run tox using the version of Python in `PATH`, append platform
run: tox
env:
PLATFORM: ${{ matrix.os }}
================================================
FILE: .gitignore
================================================
# emacs
*~
# --------------------------------------------
# C
*.o
*.os
*.so
*.so.*
*.dylib
*.dylib.*
*.a
ctest/test_image
# generated by tests
data/sep.cat
data/sepback.fits
# scons
.sconsign.dblite
# tarball
sep-*.tar.gz
# -------------------------------------------
# Python
__pycache__
docs/_build
docs/api
build/
MANIFEST
*.egg-info
# pytest
.pytest_cache
.cache
# generated C file
sep.c
# PyCharm
.idea
.project
# Eclipse
.pydevproject
# Jupyter
.ipynb_checkpoints
# tox
.tox
# version
*_version.py
================================================
FILE: .pre-commit-config.yaml
================================================
exclude: "^data/"
repos:
- repo: https://github.com/pre-commit/pre-commit-hooks
rev: v5.0.0
hooks:
- id: trailing-whitespace
- id: end-of-file-fixer
- id: check-yaml
- id: check-added-large-files
- repo: https://github.com/pycqa/isort
rev: 5.13.2
hooks:
- id: isort
name: isort (python)
- repo: https://github.com/psf/black
rev: 24.10.0
hooks:
- id: black
args: [--preview]
- repo: https://github.com/numpy/numpydoc
rev: v1.8.0
hooks:
- id: numpydoc-validation
- repo: https://github.com/sphinx-contrib/sphinx-lint
rev: v1.0.0
hooks:
- id: sphinx-lint
args: [--enable=all, --disable=default-role, --max-line-length=75, -v]
files: ^docs\/|^.*\.(rst$|md$)
- repo: https://github.com/pre-commit/mirrors-clang-format
rev: v19.1.4
hooks:
- id: clang-format
types_or: [c++, c, cuda]
================================================
FILE: .readthedocs.yaml
================================================
# Read the Docs configuration file for Sphinx projects
# See https://docs.readthedocs.io/en/stable/config-file/v2.html for details
# Required
version: 2
# Set the OS, Python version and other tools you might need
build:
os: ubuntu-22.04
tools:
python: "3.12"
# You can also specify other tool versions:
# nodejs: "20"
# rust: "1.70"
# golang: "1.20"
# Build documentation in the "docs/" directory with Sphinx
sphinx:
configuration: docs/conf.py
# You can configure Sphinx to use a different builder, for instance use the dirhtml builder for simpler URLs
# builder: "dirhtml"
# Fail on all warnings to avoid broken references
# fail_on_warning: true
# Optionally build your docs in additional formats such as PDF and ePub
# formats:
# - pdf
# - epub
# Optional but recommended, declare the Python requirements required
# to build your documentation
# See https://docs.readthedocs.io/en/stable/guides/reproducible-builds.html
python:
install:
# - requirements: docs/requirements.txt
- method: pip
path: .
extra_requirements:
- docs
================================================
FILE: AUTHORS.md
================================================
* Emmanuel Bertin (bertin@iap.fr) : original SExtractor code
* Kyle Barbary (@kbarbary) : Conversion of SExtractor code to library
* Kyle Boone (@kboone) : Bugfix, matched filter
* Thomas Robitaille (@astrofrog) : Exact aperture overlap code
* Matt Craig (@mwcraig) : Windows & OS X support
* Curtis McCully (@cmccully): Parameter uncertainties
* Evert Rol (@evertrol): setup.py fixes
* Joe Lyman (@lyalpha): Make deblending limit settable
* Michael Wuertenberger (@mworion): PyPI wheels
* Ingvar Stepanyan (@rreverser): Build system, public API and thread safety fixes.
* Gabe Brammer (@gbrammer): Fix memory addressing with large arrays.
* Peter Watson (@PJ-Watson): Add extraction from existing segmentation map.
================================================
FILE: CHANGES.md
================================================
v1.3.7 (8 November 2024)
========================
* Test against Python 3.13.
* Update the Makefile to support Semantic Versioning from git tags.
* Update the C libraries to allow for passing the version as a compiler
flag.
* Update `setup.py` to pass the SCM version to the Cython compiler.
* Include C tests in the Tox suite (for linux and macos only).
* Document any and all changes to the C API since forking.
* Restructure changelog documentation.
v1.3.6 (7 October 2024)
=======================
* Fix wrong int type in Windows
([#2](https://github.com/PJ-Watson/sep-pjw/issues/2), thanks to
@acenko for pointing this out).
* Update tests to run on multiple operating systems.
v1.3.5 (12 June 2024)
=====================
* Small fixes and updates to ensure compatibility with NumPy 2.0.
v1.3.4 (21 February 2024)
========================
* Include .clang-format as a pre-commit hook, to ensure consistent code
style (improved readability, easier maintenance).
* Fixed `make test` to account for the changes in
[v1.3.0](https://github.com/PJ-Watson/sep-pjw/releases/tag/v1.3.0).
* All header files include the correct definitions.
v1.3.3 (7 February 2024)
========================
* Add changelog to documentation.
* Add tests for re-running with seg map.
* Fix array boundary bugs when re-running with seg map.
* Fix bug with precision loss when calculating threshold.
* Improve error handling when object pixels exceed pix stack.
v1.3.2 (5 February 2024)
========================
* Move documentation to new location, fix package names and imports.
* Add wheels for Python 3.11/3.12.
* Fix C compilation errors on windows (VLAs).
* Publish updated version to PyPI under new name.
v1.3.1 (31 January 2024)
========================
* Formatting changes (follow [black](https://github.com/psf/black)
formatting style).
* Fix `bench.py` and `test.py`, removing deprecated functions.
* Move metadata into `pyproject.toml`.
* Add pre-commit hooks for code and docstring validation.
* Change to dynamic versioning (git tag/commit based).
v1.3.0 (1 December 2023)
========================
* The `segmentation_map` argument of `sep.extract()` will now accept
either an array or boolean. If an existing segmentation map is passed,
the object detection stage is skipped, and sources will be individually
analysed according to the provided map. This change is
backwards-compatible with respect to the Python module.
Please note that as no deblending is performed, the calculated
thresholds (and any dependent parameters) may not be the same as
originally derived.
* Use 64-bit integers throughout, to fix memory addressing with large
arrays
([#122](https://github.com/kbarbary/sep/issues/122 "Original issue"),
inspired by [Gabe Brammer's fork](https://github.com/gbrammer/sep)
with additional fixes).
================================================
FILE: CMakeLists.txt
================================================
cmake_minimum_required(VERSION 2.6)
project(sep C)
LIST(APPEND CMAKE_MODULE_PATH "${CMAKE_SOURCE_DIR}/cmake_modules/")
include(GNUInstallDirs)
set(SOURCES
${CMAKE_SOURCE_DIR}/src/analyse.c
${CMAKE_SOURCE_DIR}/src/convolve.c
${CMAKE_SOURCE_DIR}/src/deblend.c
${CMAKE_SOURCE_DIR}/src/extract.c
${CMAKE_SOURCE_DIR}/src/lutz.c
${CMAKE_SOURCE_DIR}/src/aperture.c
${CMAKE_SOURCE_DIR}/src/background.c
${CMAKE_SOURCE_DIR}/src/util.c
)
include_directories(${CMAKE_INCLUDE_PATH} ${CMAKE_SOURCE_DIR}/src ${CFITSIO_INCLUDE_DIR})
link_directories(${CMAKE_LIBRARY_PATH} ${CMAKE_SOURCE_DIR}/src)
add_library(sep SHARED ${SOURCES})
set_target_properties(sep PROPERTIES OUTPUT_NAME sep)
set_target_properties(sep PROPERTIES VERSION 0.6.0 SOVERSION 0)
set_target_properties(sep PROPERTIES C_VISIBILITY_PRESET hidden)
if (MSVC)
add_definitions(-D_USE_MATH_DEFINES)
else ()
add_compile_options(-Wcast-qual)
target_link_libraries(sep m)
endif()
install(TARGETS sep LIBRARY DESTINATION ${CMAKE_INSTALL_LIBDIR})
install(FILES ${CMAKE_SOURCE_DIR}/src/sep.h DESTINATION include)
================================================
FILE: FindSEP.cmake
================================================
# - Try to find SEP
# Once done this will define
#
# SEP_FOUND - system has SEP
# SEP_INCLUDE_DIR - the SEP include directory
# SEP_LIBRARIES - Link these to use SEP
# SEP_VERSION_STRING - Human readable version number of sep
# SEP_VERSION_MAJOR - Major version number of sep
# SEP_VERSION_MINOR - Minor version number of sep
# Copyright (c) 2017, Ilia Platone, <info@iliaplatone.com>
# Based on FindLibfacile by Carsten Niehaus, <cniehaus@gmx.de>
#
# Redistribution and use is allowed according to the terms of the BSD license.
# For details see the accompanying COPYING-CMAKE-SCRIPTS file.
if (SEP_LIBRARIES)
# in cache already
set(SEP_FOUND TRUE)
message(STATUS "Found SEP: ${SEP_LIBRARIES}")
else (SEP_LIBRARIES)
find_library(SEP_LIBRARIES NAMES sep
PATHS
${_obLinkDir}
${GNUWIN32_DIR}/lib
/usr/local/lib
)
if(SEP_LIBRARIES)
set(SEP_FOUND TRUE)
else (SEP_LIBRARIES)
set(SEP_FOUND FALSE)
endif(SEP_LIBRARIES)
if (SEP_FOUND)
if (NOT SEP_FIND_QUIETLY)
message(STATUS "Found SEP: ${SEP_LIBRARIES}")
endif (NOT SEP_FIND_QUIETLY)
else (SEP_FOUND)
if (SEP_FIND_REQUIRED)
message(FATAL_ERROR "SEP not found. Please install libsep-dev")
endif (SEP_FIND_REQUIRED)
endif (SEP_FOUND)
mark_as_advanced(SEP_LIBRARIES)
endif (SEP_LIBRARIES)
================================================
FILE: MANIFEST.in
================================================
include README.md
include CHANGES.md
include AUTHORS.md
include licenses/*
include pyproject.toml
include src/*.[c,h,i]
include sep.pyx
exclude sep.c
================================================
FILE: Makefile
================================================
OS ?= $(shell sh -c 'uname -s | tr "[A-Z]" "[a-z]"')
DESCRIBE := $(shell git describe --match "v*" --always --tags)
DESCRIBE_PARTS := $(subst -, ,$(DESCRIBE))
VERSION_TAG := $(word 1,$(DESCRIBE_PARTS))
COMMITS_SINCE_TAG := $(word 2,$(DESCRIBE_PARTS))
BUILD_ID := $(word 3,$(DESCRIBE_PARTS))
VERSION := $(subst v,,$(VERSION_TAG))
VERSION_PARTS := $(subst ., ,$(VERSION))
MAJOR := $(word 1,$(VERSION_PARTS))
MINOR := $(word 2,$(VERSION_PARTS))
MICRO := $(word 3,$(VERSION_PARTS))
NEXT_MICRO := $(shell echo $$(($(MICRO)+1)))
ifeq ($(strip $(COMMITS_SINCE_TAG)),)
CURRENT_VERSION_MICRO := $(MAJOR).$(MINOR).$(MICRO)
CURRENT_MICRO := $(MICRO)
else
CURRENT_VERSION_MICRO := $(MAJOR).$(MINOR).$(NEXT_MICRO)
CURRENT_MICRO := $(NEXT_MICRO)-dev$(COMMITS_SINCE_TAG)$(if $(BUILD_ID),-${BUILD_ID},)
endif
ifeq ($(OS), darwin)
SONAME = libsep.dylib
SONAME_MAJOR = libsep.$(MAJOR).dylib
SONAME_FULL = libsep.$(MAJOR).$(MINOR).$(CURRENT_MICRO).dylib
SONAME_FLAG = -install_name
LDPATHENV = DYLD_LIBRARY_PATH
else
ifeq ($(OS), linux)
SONAME = libsep.so
SONAME_MAJOR = libsep.so.$(MAJOR)
SONAME_FULL = libsep.so.$(MAJOR).$(MINOR).$(CURRENT_MICRO)
SONAME_FLAG = -soname
LDPATHENV = LD_LIBRARY_PATH
else
$(error OS not yet supported)
endif
endif
INSTALL ?= install
DESTDIR =
PREFIX ?= /usr/local
LIBDIR = $(PREFIX)/lib
INCLUDEDIR = $(PREFIX)/include
CC?=gcc
AR?=ar
CPPFLAGS ?=
LDFLAGS ?=
CPPFLAGS += -Isrc
CFLAGS += -Wall -Wextra -Wcast-qual -O3 -fvisibility=hidden # -Werror
CFLAGS += -DSEP_VERSION_STRING=\"$(MAJOR).$(MINOR).$(CURRENT_MICRO)\"
CFLAGS_LIB = $(CFLAGS) -fPIC
LDFLAGS_LIB = $(LDFLAGS) -shared -Wl,$(SONAME_FLAG),$(SONAME_MAJOR)
OBJS = src/analyse.o src/convolve.o src/deblend.o src/extract.o \
src/lutz.o src/aperture.o src/background.o src/util.o
default: all
src/analyse.o src/convolve.o src/deblend.o src/extract.o src/lutz.o: src/%.o: src/%.c src/extract.h src/sepcore.h src/sep.h
$(CC) $(CPPFLAGS) $(CFLAGS_LIB) -c src/$*.c -o $@
src/aperture.o: src/aperture.c src/aperture.i src/overlap.h src/sepcore.h src/sep.h
$(CC) $(CPPFLAGS) $(CFLAGS_LIB) -c src/aperture.c -o $@
src/background.o src/util.o: src/%.o: src/%.c src/sepcore.h src/sep.h
$(CC) $(CPPFLAGS) $(CFLAGS_LIB) -c src/$*.c -o $@
src/$(SONAME_FULL) src/$(SONAME_MAJOR) src/$(SONAME) &: $(OBJS)
$(CC) $(LDFLAGS_LIB) $^ -lm -o src/$(SONAME_FULL)
ln -sf $(SONAME_FULL) src/$(SONAME_MAJOR)
ln -sf $(SONAME_FULL) src/$(SONAME)
src/libsep.a: $(OBJS)
$(AR) rcs src/libsep.a $^
install: all
$(INSTALL) -d $(DESTDIR)$(INCLUDEDIR)
$(INSTALL) -m u=rw,g=r,o=r src/sep.h $(DESTDIR)$(INCLUDEDIR)
$(INSTALL) -d $(DESTDIR)$(LIBDIR)
$(INSTALL) -m u=rwx,g=rx,o=rx src/$(SONAME_FULL) $(DESTDIR)$(LIBDIR)
ln -sf $(SONAME_FULL) $(DESTDIR)$(LIBDIR)/$(SONAME_MAJOR)
ln -sf $(SONAME_FULL) $(DESTDIR)$(LIBDIR)/$(SONAME)
$(INSTALL) -m u=rw,g=r,o=r src/libsep.a $(DESTDIR)$(LIBDIR)
uninstall:
rm $(DESTDIR)$(INCLUDEDIR)/sep.h
rm $(DESTDIR)$(LIBDIR)/$(SONAME_FULL)
rm $(DESTDIR)$(LIBDIR)/$(SONAME_MAJOR)
rm $(DESTDIR)$(LIBDIR)/$(SONAME)
rm $(DESTDIR)$(LIBDIR)/libsep.a
test: ctest/test_image
$(LDPATHENV)=src ctest/test_image data/image.fits data/sep.cat
ctest/compare.py data/image.cat data/sep.cat
ctest/test_image: ctest/test_image.c src/$(SONAME)
$(CC) $(CPPFLAGS) $(CFLAGS) $(LDFLAGS) -Lsrc ctest/test_image.c -lm -lsep -o ctest/test_image
clean:
rm -f src/*.o src/*.a src/libsep.* ctest/test_image
all: src/$(SONAME_FULL) src/libsep.a
.PHONY: all test clean library install uninstall
================================================
FILE: README.md
================================================
SEP
===
Python and C library for Source Extraction and Photometry.
[](https://pypi.python.org/pypi/sep)
[](https://pypi.python.org/pypi/sep)
[](https://github.com/sep-developers/sep/actions)
[](https://sep.readthedocs.io/en/latest/?badge=latest)
[](http://dx.doi.org/10.21105/joss.00058)
*"... [it's] an SEP: Somebody Else's Problem."
"Oh, good. I can relax then."*
SEP, SEP-PJW, and Package Names
-------------------------------
`sep` was originally released by Kyle Barbary, at
[kbarbary/sep](https://github.com/kbarbary/sep) (``sep<=1.2.1``). For a
brief period, the package was maintained by Peter Watson, under the
`sep-pjw` package name, at
[PJ-Watson/sep-pjw](https://github.com/PJ-Watson/sep-pjw) and
[PyPI/sep-pjw](https://pypi.org/project/sep-pjw/)
(``1.3.0<=sep-pjw<=1.3.8``). Both of these repositories will be archived,
and future development will take place at
[sep-developers/sep](<https://github.com/sep-developers/sep>)
(``sep>=1.4.0``). Note that there may be some incompatibilities between
``sep==1.2.1`` and ``sep==1.4.0`` when using the C-API directly (to fix
an indexing bug arising with large arrays) - all changes are documented
[here](https://sep-pjw.readthedocs.io/en/latest/changelogs/changes_to_c_api.html).
About
-----
[Source Extractor](http://www.astromatic.net/software/sextractor)
(Bertin & Arnouts 1996) is a widely used
command-line program for segmentation and analysis of astronomical
images. It reads in FITS format files, performs a configurable series
of tasks, including background estimation, source detection,
deblending and a wide array of source measurements, and finally
outputs a FITS format catalog file.
While Source Extractor is highly useful, the fact that it can only be
used as an executable can limit its applicability or lead to awkward
workflows. There is often a desire to have programmatic access to
perform one or more of the above tasks on in-memory images as part of
a larger custom analysis.
**SEP makes the core algorithms of Source Extractor available as a
library of stand-alone functions and classes.** These operate directly
on in-memory arrays (no FITS files or configuration files). The code
is derived from the Source Extractor code base (written in C) and aims
to produce results compatible with Source Extractor whenever possible.
SEP consists of a C library with no dependencies outside the standard
library, and a Python module that wraps the C library in a Pythonic
API. The Python wrapper operates on NumPy arrays with NumPy as its
only dependency. See below for language-specfic build and usage
instructions.
Python
------
**Documentation:** http://sep.readthedocs.io
**Requirements:**
- Python 3.9+
- numpy 1.23+
**Install release version:**
SEP can be installed with [pip](https://pip.pypa.io):
```
python -m pip install sep
```
If you get an error about permissions, you are probably using your
system Python. In this case, we recommend using [pip's "user
install"](https://pip.pypa.io/en/latest/user_guide/#user-installs)
option to install sep into your user directory:
```
python -m pip install --user sep
```
Do **not** install sep or other third-party Python packages using
`sudo` unless you are fully aware of the risks.
**Install development version:**
Building the development version (from github) requires Cython.
Build and install in the usual place:
```
python -m pip install --editable .
```
**Run tests:** Tests require the [pytest](http://pytest.org) Python
package. To run the tests, execute `./test.py` in the top-level
directory. Some tests require a FITS reader (either fitsio or astropy)
and will be skipped if neither is present.
C Library
---------
_Note: The build process only works on Linux and OS X._
**CMake:** To build using CMake, enter these commands:
```
cd sep
mkdir -p build
cd build
cmake -DCMAKE_INSTALL_PREFIX=/usr ../
```
and follow next steps from the build folder
**Build:** To build the C library from source:
```
make
```
**Run tests:**
```
make test
```
**Install** The static library and header can be installed with
```
make install
make PREFIX=/path/to/prefix install
```
This will install the shared and static library in `/path/to/prefix/lib`
and header file in `/path/to/prefix/include`. The default prefix is
`/usr/local`.
**API:** The C library API is documented in the header file
[sep.h](src/sep.h).
**Rust bindings:** Low-level Rust wrapper for the C library can be found at https://crates.io/crates/sep-sys
Contributing
------------
- Report a bug or documentation issue: http://github.com/sep-developers/issues
- Ask (or answer) a question: https://github.com/sep-developers/sep/discussions/categories/q-a
Development of SEP takes place on GitHub at
[sep-developers/sep](http://github.com/sep-developers/sep). Contributions of bug fixes,
documentation improvements and minor feature additions are welcome via
GitHub pull requests. For major features, it is best to discuss the change first
via [GitHub Discussions](https://github.com/sep-developers/sep/discussions/).
Citation
--------
If you use SEP in a publication, please cite the following article in the Journal of Open Source Software:
[](http://dx.doi.org/10.21105/joss.00058)
Please also cite the original Source Extractor paper ([Bertin & Arnouts
1996](http://adsabs.harvard.edu/abs/1996A%26AS..117..393B)).
The DOI for the sep v1.0.0 code release is:
[](http://dx.doi.org/10.5281/zenodo.159035)
License
-------
The license for all parts of the code derived from Source Extractor is
LGPLv3. The license for code derived from photutils (`src/overlap.h`)
is BSD 3-clause. Finally, the license for the Python wrapper
(`sep.pyx`) is MIT. The license for the library as a whole is
therefore LGPLv3. The license for each file is explicitly stated at
the top of the file and the full text of each license can be found in
`licenses`.
FAQ
---
**Why isn't the C library part of Source Extractor?**
Source Extractor is *not* designed as a library with an
executable built on top of the library. In Source Extractor, background
estimation, object detection and photometry are deeply integrated into the
Source Extractor executable. Many changes to the code were necessary in
order to put the functionality in stand-alone C functions. It's too much
to ask of the Source Extractor developer to rewrite large parts of the
core of the Source Extractor program with little gain for the executable.
**What sort of changes?**
- Source Extractor reads in only a small portion of each image at a
time. This allows it to keep its memory footprint extremely low and
to operate on images that are much larger than the system's physical
memory. It also means that a FITS reader is deeply integrated into
the code. SEP operates on images in memory, so all the FITS I/O
machinery in Source Extractor is not used here.
- Error handling: When it encounters a problem, Source Extractor
immediately exits with an error message. This is fine for an
executable, but a library function doesn't have that luxury. Instead
it must ensure that allocated memory is freed and return an error
code.
- Options: Source Extractor has many options that affect its behavior. These
are stored in a global structure used throughout the executable. In SEP,
options for a particular function are passed as function parameters.
- Array types: Source Extractor can operate on FITS images containing various
types of data (float, double, int, etc). Internally, it does this by
converting all data to `float` immediately when reading from disk.
SEP does something similar, but in memory: SEP functions typically convert
input arrays to float on the fly within each function, then perform
all operations as floating point.
**Is SEP as fast as Source Extractor?**
It's fast. It should be similar to Source Extractor as a lot of the code
is identical. Source Extractor has the advantage of doing all the
operations (detection and analysis) simultaneously on each image
section, which may confer CPU cache advantages, but this hasn't been
tested at all. On the other hand, depending on your usage SEP might
let you avoid writing files to disk, which is likely to be a bigger
win.
**What happens when Source Extractor is updated in the future?**
SEP can be considered a fork of the Source Extractor code base: it's
development will not track that of Source Extractor in any automated
way. However, the algorithms implemented so far in SEP are stable in
Source Extractor: the SEP code was forked from v2.18.11, yet it is tested
against the results of v2.8.6. This indicates that the algorithms have
not changed in Source Extractor over the last few years.
**In the Python interface, why do I have to byte swap data when using
astropy.io.fits?**
This occurs because FITS files have big-endian [byte
order](http://en.wikipedia.org/wiki/Endianness), whereas most widely
used CPUs have little-endian byte order. In order for the CPU to
operate on the data, it must be byte swapped at *some point.* Some
FITS readers such as [fitsio](http://github.com/esheldon/fitsio) do
the byte swap immediately when reading the data from disk to memory,
returning numpy arrays in native (little-endian) byte order. However,
astropy.io.fits does not (for reasons having to do with memory
mapping). Most of the time you never notice this because when you do
any numpy operations on such arrays, numpy uses an intermediate buffer
to byte swap the array behind the scenes and returns the result as a
native byte order array. Internally, SEP is not using numpy
operations; it's just getting a pointer to the data in the array and
passing it to C code. As the C code does not include functionality to
do buffered byte swapping, the input array must already be in native
byte order.
It would be possible to add buffered byte swapping capability to the
SEP code, but it would increase the code complexity. A simpler
alternative would be to make a byte swapped copy of the entire input
array, whenever necessary. However, this would significantly increase
memory use, and would have to be done repeatedly in multiple SEP
functions: `Background`, `extract`, `sum_circle`, etc. Each would make
a copy of the entire data array. Given these considerations, it seemed
best to just explicitly tell the user to do the byte swap operation
themselves so they could just do it once, immediately after reading in
the data.
**I have more questions!**
Open a discussion on the [GitHub Discussions page](https://github.com/sep-developers/sep/discussions/categories/q-a)!
================================================
FILE: bench.py
================================================
#!/usr/bin/env python
"""Benchmarking SEP against equivalent photutils functions."""
from __future__ import print_function
import time
from pathlib import Path
import numpy as np
import sep
# try to import photutils for comparison timing
try:
import photutils
HAVE_PHOTUTILS = True
except ImportError:
HAVE_PHOTUTILS = False
# Try to import any FITS reader
try:
from fitsio import read as getdata
HAVE_FITS = True
NEED_BYTESWAP = False
except ImportError:
try:
from astropy.io.fits import getdata
HAVE_FITS = True
NEED_BYTESWAP = True
except ImportError:
HAVE_FITS = False
import argparse
parser = argparse.ArgumentParser(description="SEP Benchmark script.")
parser.add_argument(
"-c",
"--condensed",
default=False,
action="store_true",
help="Only run a condensed subset of the benchmarks.",
)
parser.add_argument(
"-t",
"--tiles",
default=4,
type=int,
help=(
"The maximum number of tiles for the image background benchmark, "
"i.e. the image size will be `(t*256)^2`."
),
)
parser.add_argument(
"-a",
"--apertures",
default=1000,
type=int,
help=(
"The number of apertures to use for benchmarking the aperture "
"photometry, by default 1000."
),
)
parser.add_argument(
"-r",
"--radii",
default=[3, 5, 10, 20],
type=float,
nargs="+",
help=(
"The radii of the apertures to test. Ignored if the `--condensed` "
"flag is passed, otherwise defaults to `3, 5, 10, 20`."
),
)
parser.add_argument(
"-n",
"--nloop",
default=50,
type=int,
help=("The number of loops to run for all tests, by default 50."),
)
args = parser.parse_args()
if HAVE_FITS:
rawdata = getdata(
Path(__file__).parent / "data" / "image.fits"
) # original is 256 x 256
if NEED_BYTESWAP:
rawdata = rawdata.astype(rawdata.dtype.newbyteorder("="))
else:
print("No FITS reader found, generating random data instead.")
rawdata = np.random.random((256, 256))
data = np.tile(rawdata, (4, 4))
print("test image shape:", data.shape)
print("test image dtype:", data.dtype)
t0 = time.time()
bkg = sep.Background(data) # estimate background
t1 = time.time()
print("measure background: {0:6.2f} ms".format((t1 - t0) * 1.0e3))
t0 = time.time()
bkg.subfrom(data) # subtract it
t1 = time.time()
print("subtract background: {0:6.2f} ms".format((t1 - t0) * 1.0e3))
t0 = time.time()
backarr = bkg.back(dtype=np.float64) # background
t1 = time.time()
print("background array: {0:6.2f} ms".format((t1 - t0) * 1.0e3))
t0 = time.time()
rmsarr = bkg.rms()
t1 = time.time()
print("rms array: {0:6.2f} ms".format((t1 - t0) * 1.0e3))
t0 = time.time()
objects = sep.extract(data, 1.5 * bkg.globalrms)
t1 = time.time()
print("extract: {0:6.2f} ms [{1:d} objects]".format((t1 - t0) * 1.0e3, len(objects)))
# --------------------------------------------------------------------------
# Background subtraction
print("")
if HAVE_PHOTUTILS:
print("sep version: ", sep.__version__)
print("photutils version:", photutils.__version__)
print(
"""
| test | sep | photutils | ratio |
|-------------------------|-----------------|-----------------|--------|"""
)
blankline = (
"| | | | |"
)
else:
print("sep version: ", sep.__version__)
print(
"""
| test | sep |
|-------------------------|-----------------|"""
)
blankline = "| | |"
for ntile in np.arange(1, args.tiles + 1, dtype=int):
data = np.tile(rawdata, (ntile, ntile))
line = "| {0:4d}^2 image background |".format(data.shape[0])
t0 = time.time()
for _ in range(0, args.nloop):
bkg = sep.Background(data)
t1 = time.time()
t_sep = (t1 - t0) * 1.0e3 / args.nloop
line += " {0:7.2f} ms |".format(t_sep)
if HAVE_PHOTUTILS:
t0 = time.time()
for _ in range(0, args.nloop):
from photutils import background
bkg = background.Background2D(data, (64, 64)) # estimate background
t1 = time.time()
t_pu = (t1 - t0) * 1.0e3 / args.nloop
line += " {0:7.2f} ms | {1:6.2f} |".format(t_pu, t_pu / t_sep)
print(line)
# ------------------------------------------------------------------------------
# Circular aperture photometry benchmarks
if not args.condensed:
print(blankline)
line = "| **aperture photometry** | |"
if HAVE_PHOTUTILS:
line += " | |"
print(line)
data = np.ones((2000, 2000), dtype=np.float32)
x = np.random.uniform(200.0, 1800.0, args.apertures)
y = np.random.uniform(200.0, 1800.0, args.apertures)
if args.condensed:
r_list = [5.0]
subpix_list = [(5, "subpixel", "subpix=5"), (0, "exact", "exact")]
else:
r_list = args.radii
subpix_list = [
(1, "center", "subpix=1"),
(5, "subpixel", "subpix=5"),
(0, "exact", "exact"),
]
for r in r_list:
for subpix, method, label in subpix_list:
line = "| circles r={0:2d} {1:8s} |".format(int(r), label)
t0 = time.time()
for _ in range(0, args.nloop):
flux, fluxerr, flag = sep.sum_circle(data, x, y, r, subpix=subpix)
t1 = time.time()
t_sep = (t1 - t0) * 1.0e6 / args.apertures / args.nloop
line += " {0:7.2f} us/aper |".format(t_sep)
if HAVE_PHOTUTILS:
from photutils import aperture
apertures = photutils.aperture.CircularAperture(np.column_stack((x, y)), r)
t0 = time.time()
for _ in range(0, args.nloop):
res = photutils.aperture.aperture_photometry(
data, apertures, method=method, subpixels=subpix
)
t1 = time.time()
t_pu = (t1 - t0) * 1.0e6 / args.apertures / args.nloop
line += " {0:7.2f} us/aper | {1:6.2f} |".format(t_pu, t_pu / t_sep)
print(line)
if not args.condensed:
print(blankline)
a = 1.0
b = 1.0
theta = np.pi / 4.0
for r in r_list:
for subpix, method, label in subpix_list:
line = "| ellipses r={0:2d} {1:8s} |".format(int(r), label)
t0 = time.time()
for _ in range(0, args.nloop):
flux, fluxerr, flag = sep.sum_ellipse(
data, x, y, a, b, theta, r, subpix=subpix
)
t1 = time.time()
t_sep = (t1 - t0) * 1.0e6 / args.apertures / args.nloop
line += " {0:7.2f} us/aper |".format(t_sep)
if HAVE_PHOTUTILS:
from photutils import aperture
apertures = photutils.aperture.EllipticalAperture(
np.column_stack((x, y)), a * r, b * r, theta
)
t0 = time.time()
for _ in range(0, args.nloop):
res = photutils.aperture.aperture_photometry(
data, apertures, method=method, subpixels=subpix
)
t1 = time.time()
t_pu = (t1 - t0) * 1.0e6 / args.apertures / args.nloop
line += " {0:7.2f} us/aper | {1:6.2f} |".format(t_pu, t_pu / t_sep)
print(line)
================================================
FILE: codemeta.json
================================================
{
"@context": "https://raw.githubusercontent.com/mbjones/codemeta/master/codemeta.jsonld",
"@type": "Code",
"author": [
{
"@id": "http://orcid.org/0000-0002-2532-3696",
"@type": "Person",
"email": "kylebarbary@gmail.com",
"name": "Kyle Barbary",
"affiliation": "University of California, Berkeley"
}
],
"identifier": "http://dx.doi.org/10.5281/zenodo.159035",
"codeRepository": "https://github.com/kbarbary/sep",
"datePublished": "2016-09-30",
"dateModified": "2016-09-30",
"dateCreated": "2016-09-30",
"description": "Python and C library for Source Extraction and Photometry",
"keywords": "astronomy, Python, image analysis",
"license": "LGPL v3.0",
"title": "SEP",
"version": "v1.0.0"
}
================================================
FILE: ctest/compare.py
================================================
#!/usr/bin/env python
"""Compare the output from SEP against SExtractor."""
from __future__ import print_function
import sys
def read_table(fname):
"""
Read in a whitespace-separated table.
Parameters
----------
fname : path-like
The filename of the table to be opened.
Returns
-------
List[List[int|float]]
A list of rows, each of which is a list of the values in that row.
"""
rows = []
for line in open(fname, "r"):
l = line.strip()
if len(l) == 0 or l[0] == "#":
continue
items = l.split()
typed_items = []
for it in items:
try:
typed_items.append(int(it))
except ValueError:
typed_items.append(float(it))
rows.append(typed_items)
return rows
def fracdiff(x, y):
"""
Return the fraction difference between two numbers.
Parameters
----------
x, y : float
The numbers to be compared.
Returns
-------
float
The fractional difference.
"""
return abs((y - x) / max(y, x))
if __name__ == "__main__":
fname1, fname2 = sys.argv[1:3]
ref = read_table(fname1)
sep = read_table(fname2)
# sort by y coordinate
ref.sort(key=lambda row: row[2])
sep.sort(key=lambda row: row[2])
assert len(ref) == len(sep)
for i in range(len(ref)):
assert abs(ref[i][1] - sep[i][1] - 1.0) < 1.0e-3 # x coordinate
assert abs(ref[i][2] - sep[i][2] - 1.0) < 1.0e-3 # y coordinate
assert fracdiff(ref[i][12], sep[i][3]) < 2.0e-4 # flux
print("compare passed")
================================================
FILE: ctest/test_image.c
================================================
#include <math.h>
#include <stdint.h>
#include <stdio.h>
#include <stdlib.h>
#include <string.h>
#include <sys/time.h>
#include "sep.h"
uint64_t gettime_ns() {
struct timeval tv;
gettimeofday(&tv, NULL);
return (uint64_t)tv.tv_sec * 1000000000ULL + tv.tv_usec * 1000ULL;
}
double * ones_dbl(int nx, int ny) {
int i, npix;
double *im, *imt;
im = (double *)malloc((npix = nx * ny) * sizeof(double));
imt = im;
for (i = 0; i < npix; i++, imt++) {
*imt = 1.0;
}
return im;
}
float * uniformf(float a, float b, int n)
/* an array of n random numbers from the uniform interval (a, b) */
{
int i;
float * result;
result = (float *)malloc(n * sizeof(float));
for (i = 0; i < n; i++) {
result[i] = a + (b - a) * rand() / ((double)RAND_MAX);
}
return result;
}
float * ones(int nx, int ny) {
int i, npix;
float *im, *imt;
im = (float *)malloc((npix = nx * ny) * sizeof(float));
imt = im;
for (i = 0; i < npix; i++, imt++) {
*imt = 1.0;
}
return im;
}
void addbox(float * im, int w, int h, float xc, float yc, float r, float val)
/* n = sersic index */
{
int xmin, xmax, ymin, ymax;
int x, y;
int rmax = (int)r;
xmin = (int)xc - rmax;
xmin = (xmin < 0) ? 0 : xmin;
xmax = (int)xc + rmax;
xmax = (xmax > w) ? w : xmax;
ymin = (int)yc - rmax;
ymin = (ymin < 0) ? 0 : ymin;
ymax = (int)yc + rmax;
ymax = (ymax > h) ? h : ymax;
for (y = ymin; y < ymax; y++) {
for (x = xmin; x < xmax; x++) {
im[x + w * y] += val;
}
}
}
void printbox(float * im, int w, int h, int xmin, int xmax, int ymin, int ymax)
/* print image values to the screen in a grid
Don't make box size too big!!
*/
{
int i, j;
for (j = ymin; j < ymax && j < h; j++) {
for (i = xmin; i < xmax && i < w; i++) {
printf("%6.2f ", im[w * j + i]);
}
printf("\n");
}
}
/* an extremely dumb reader for our specific test FITS file! */
int read_test_image(char * fname, float ** data, int64_t * nx, int64_t * ny) {
FILE * f;
char buf[80]; /* buffer to hold a line */
long pos;
size_t nbytes, nel, i, elsize, nread;
char * rawbytes = NULL;
short * rawdata;
char tmp;
int status = 0;
float bscale, bzero;
/* hard-code image size & element size */
*nx = 256;
*ny = 256;
elsize = 2;
nel = *nx * *ny;
bscale = 2.92273835509;
bzero = 3713.66692596;
f = fopen(fname, "r");
/* read first line and check if it is a FITS file */
nread = fread(buf, 1, 80, f);
if (nread != 80) {
status = 1;
goto exit;
}
if (strncmp(buf, "SIMPLE = T", 30) != 0) {
printf("not a FITS file");
status = 1;
goto exit;
}
/* read rows until we get to END keyword */
while (strncmp(buf, "END", 3) != 0) {
nread = fread(buf, 1, 80, f);
if (nread != 80) {
status = 1;
goto exit;
}
}
/* move to next 2880 byte boundary. */
pos = ftell(f) % 2880; /* position in "page" */
if (pos != 0) {
fseek(f, 2880 - pos, SEEK_CUR);
}
/* read raw data bytes */
nbytes = nel * elsize;
rawbytes = (char *)malloc(nbytes);
nread = fread(rawbytes, 1, nbytes, f);
if (nread != nbytes) {
status = 1;
goto exit;
}
/* swap bytes in raw data (FITS is big-endian) */
for (i = 0; i < nbytes; i += 2) {
tmp = rawbytes[i];
rawbytes[i] = rawbytes[i + 1];
rawbytes[i + 1] = tmp;
}
rawdata = (short *)rawbytes; /* buffer is now little-endian */
/* convert to float, applying bscale/bzero */
*data = (float *)malloc(nel * sizeof(float));
for (i = 0; i < nel; i++) {
(*data)[i] = bscale * rawdata[i] + bzero;
}
exit:
free(rawbytes);
return status;
}
float * tile_flt(
float * im, int nx, int ny, int ntilex, int ntiley, int * nxout, int * nyout
) {
int i, x, y;
int npixout;
float * imout;
*nxout = ntilex * nx;
*nyout = ntiley * ny;
npixout = *nxout * *nyout;
imout = (float *)malloc(npixout * sizeof(float));
for (i = 0; i < npixout; i++) {
x = (i % (*nxout)) % nx; /* corresponding x on small im */
y = (i / (*nxout)) % ny; /* corresponding y on small im */
imout[i] = im[y * nx + x];
}
return imout;
}
void print_time(char * s, uint64_t tdiff) {
printf("%-25s%6.1f ms\n", s, (double)tdiff / 1000000.);
}
int main(int argc, char ** argv) {
char *fname1, *fname2;
int i, status;
int64_t nx, ny;
double *flux, *fluxerr, *fluxt, *fluxerrt, *area, *areat;
short *flag, *flagt;
float *data, *imback;
uint64_t t0, t1;
sep_bkg * bkg = NULL;
float conv[] = {1, 2, 1, 2, 4, 2, 1, 2, 1};
sep_catalog * catalog = NULL;
FILE * catout;
status = 0;
flux = fluxerr = NULL;
flag = NULL;
/* Parse command-line arguments */
if (argc != 3) {
printf("Usage: test-image IMAGE_NAME CATALOG_NAME\n");
exit(1);
}
fname1 = argv[1];
fname2 = argv[2];
/* read in image */
status = read_test_image(fname1, &data, &nx, &ny);
if (status) {
goto exit;
}
/* test the version string */
printf("sep version: %s\n", sep_version_string);
/* background estimation */
t0 = gettime_ns();
sep_image im = {
data,
NULL,
NULL,
NULL,
SEP_TFLOAT,
0,
0,
0,
0,
0,
0,
nx,
ny,
0.0,
SEP_NOISE_NONE,
1.0,
0.0
};
status = sep_background(&im, 64, 64, 3, 3, 0.0, &bkg);
t1 = gettime_ns();
if (status) {
goto exit;
}
print_time("sep_background()", t1 - t0);
/* evaluate background */
imback = (float *)malloc((nx * ny) * sizeof(float));
t0 = gettime_ns();
status = sep_bkg_array(bkg, imback, SEP_TFLOAT);
t1 = gettime_ns();
if (status) {
goto exit;
}
print_time("sep_bkg_array()", t1 - t0);
/* subtract background */
t0 = gettime_ns();
status = sep_bkg_subarray(bkg, data, im.dtype);
t1 = gettime_ns();
if (status) {
goto exit;
}
print_time("sep_bkg_subarray()", t1 - t0);
/* extract sources
* Note that we set deblend_cont = 1.0 to turn off deblending.
*/
t0 = gettime_ns();
status = sep_extract(
&im,
1.5 * bkg->globalrms,
SEP_THRESH_ABS,
5,
conv,
3,
3,
SEP_FILTER_CONV,
32,
1.0,
1,
1.0,
&catalog
);
t1 = gettime_ns();
if (status) {
goto exit;
}
print_time("sep_extract()", t1 - t0);
/* aperture photometry */
im.noise = &(bkg->globalrms); /* set image noise level */
im.ndtype = SEP_TFLOAT;
fluxt = flux = (double *)malloc(catalog->nobj * sizeof(double));
fluxerrt = fluxerr = (double *)malloc(catalog->nobj * sizeof(double));
areat = area = (double *)malloc(catalog->nobj * sizeof(double));
flagt = flag = (short *)malloc(catalog->nobj * sizeof(short));
t0 = gettime_ns();
for (i = 0; i < catalog->nobj; i++, fluxt++, fluxerrt++, flagt++, areat++) {
sep_sum_circle(
&im, catalog->x[i], catalog->y[i], 5.0, 0, 5, 0, fluxt, fluxerrt, areat, flagt
);
}
t1 = gettime_ns();
printf(
"sep_sum_circle() [r= 5.0] %6.3f us/aperture\n",
(double)(t1 - t0) / 1000. / catalog->nobj
);
/* print results */
printf("writing to file: %s\n", fname2);
catout = fopen(fname2, "w+");
fprintf(catout, "# SEP catalog\n");
fprintf(catout, "# 1 NUMBER\n");
fprintf(catout, "# 2 X_IMAGE (0-indexed)\n");
fprintf(catout, "# 3 Y_IMAGE (0-indexed)\n");
fprintf(catout, "# 4 FLUX\n");
fprintf(catout, "# 5 FLUXERR\n");
for (i = 0; i < catalog->nobj; i++) {
fprintf(
catout,
"%3d %#11.7g %#11.7g %#11.7g %#11.7g\n",
i + 1,
catalog->x[i],
catalog->y[i],
flux[i],
fluxerr[i]
);
}
fclose(catout);
/* clean-up & exit */
exit:
sep_bkg_free(bkg);
free(data);
free(flux);
free(fluxerr);
free(flag);
if (status) {
printf("FAILED with status: %d\n", status);
char errtext[512];
sep_get_errdetail(errtext);
puts(errtext);
} else {
printf("test_image passed\n");
}
return status;
}
/***************************************************************************/
/* aperture photometry */
/*
int naper, j;
float *xcs, *ycs;
im = ones(nx, ny);
naper = 1000;
flux = fluxerr = 0.0;
flag = 0;
float rs[] = {3., 5., 10., 20.};
for (j=0; j<4; j++)
{
r = rs[j];
xcs = uniformf(2.*r, nx - 2.*r, naper);
ycs = uniformf(2.*r, ny - 2.*r, naper);
printf("sep_apercirc() [r=%4.1f] ", r);
t0 = gettime_ns();
for (i=0; i<naper; i++)
sep_apercirc(im, NULL, SEP_TFLOAT, nx, ny, 0.0, 0.0,
xcs[i], ycs[i], r, 5, &flux, &fluxerr, &flag);
t1 = gettime_ns();
printf("%6.3f us/aperture\n", (double)(t1 - t0) / 1000. / naper);
free(xcs);
free(ycs);
}
*/
================================================
FILE: data/README.md
================================================
Test Data
---------
The comparison catalog file `image.cat` is generated by running
```
sextractor image.fits -CATALOG_NAME image.cat
```
in this directory.
================================================
FILE: data/back.fits
================================================
SIMPLE = T / file does conform to FITS standard BITPIX = -32 / number of bits per data pixel NAXIS = 2 / number of data axes NAXIS1 = 256 / length of data axis 1 NAXIS2 = 256 / length of data axis 2 EXTEND = T / FITS dataset may contain extensions COMMENT FITS (Flexible Image Transport System) format is defined in 'AstronomyCOMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H CRPIX1 = -7.670000000000000E+02 / Reference pixel CRVAL1 = 1.000000000000E+00 / Coordinate at reference pixel CDELT1 = 1.000000000000E+00 / Coordinate increment per pixel CTYPE1 = ' ' / Units of coordinate CRPIX2 = -5.110000000000000E+02 / Reference pixel CRVAL2 = 1.000000000000E+00 / Coordinate at reference pixel CDELT2 = 1.000000000000E+00 / Coordinate increment per pixel CTYPE2 = ' ' / Units of coordinate BUNIT = ' ' / Units of data values BSCALE = 1.00000000 / Scaling factor: r = f*i + z BZERO = 0.00000000 / Zero offset: r = f*i + z DATAMAX = 9.852823437500E+04 / Maximum data value DATAMIN = 3.713666992188E+03 / Minimum data value ORIGIN = 'SExtractor' / Written by MIDAS DATE = '31/08/93' / Date of writting: DD/MM/YY FILENAME= 'NA36Rm50.bdf' / Original file name MIDASFTP= 'IMAGE ' / MIDAS File Type OBJECT = 'NA36Rc50 sum of 3 frames' / MIDAS desc.: IDENT(1) DATE-OBS= '26/10/92' / MIDAS desc.: O_TIME(1) MJD-OBS = 4.892162787000E+04 / MIDAS desc.: O_TIME(4) TM-START= 1.104800000000E+04 / MIDAS desc.: O_TIME(5) EXPTIME = 1.200000000000E+03 / MIDAS desc.: O_TIME(7) INSTRUME= 'EMMI ' / MIDAS desc.: INSTRUME(1) COMMENT IP_JIDNT 7 / IHAP: identifier system \COMMENT COMMENT IP_JSEQ 24887 / IHAP: sequence number \COMMENT COMMENT IP_AHGC 2857.489 / IHAP: high cut \COMMENT COMMENT IP_ALWC 2112.953 / IHAP: low cut \COMMENT COMMENT IP_ASCX 1. / IHAP: scaling in x \COMMENT COMMENT IP_ASCY 1. / IHAP: scaling in y \COMMENT COMMENT IP_FILE 'IHAP/FITS/EM9210260304099.FITS::USER ' / IHAP: Begin of keywor\COMMENT d COMMENT IP_FEND / IHAP: End of keyword file \COMMENT COMMENT EXPTIME 400.000 \COMMENT COMMENT IP_CBEND / IHAP: comment block end \COMMENT TELESCOP= 'ESONTTB ' / MIDAS desc.: TELESCOP(1) OBSERVER= 'LAPPARENT' / MIDAS desc.: OBSERVER(1) RA = 5.648170000000E+00 / MIDAS desc.: RA(1) DEC = -3.018297000000E+01 / MIDAS desc.: DEC(1) AIRMASS = 1.068349957466E+00 / MIDAS desc.: AIRMASS(1) ESO-LOG 00:00:00> DATE = '1992-10-26' / Mon Oct 26, 1992 ESO-LOG 03:04:08>-START EXPO EMMI RED / Start exp. on EMMI Red CC ESO-LOG 03:04:09> EXPO EMMI RED NO = 24887 / Exp. num. on EMMI Red CCD ESO-LOG 03:10:52>-STOP EXPO EMMI RED / Stop exp. on EMMI Red CCD HISTORY COMPUTE/IMAG imAR0051.bdf = #0001-bias50 \HISTORY COMPUTE/IMAG imAR0051.bdf = #0001 - 1.51001E-01 \HISTORY COMPUTE/IMAG NA36Rc501 = #0001 * 1.00000E+03 / fRc50 \HISTORY COMPUTE/IMAG NA36Rc50 = NA36Rc501 \HISTORY COMPUTE/IMAG NA36Rc50 = NA36Rc50 + NA36Rc503 \HISTORY COMPUTE/IMAG NA36Rc50 = NA36Rc50 + NA36Rc502 \HISTORY EXTRACT/IMAG intex = NA36Rc50[@0019,@0003:@1042,@1026] \HISTORY Renamed from intex.bdf to NA36Rc50.bdf \HISTORY SELE/TABL cursor MA36Rc50 2 0. 3 Y MA36Rc50 \HISTORY READ/TABL cursor interclean 0 6.85000E+03 3 Y \HISTORY interclean Renamed from interclean.bdf to MA36Rm\HISTORY 50.bdf READ/TABL cursor MA36Rm50 0 \HISTORY 6850 3 Y MA36Rm50 READ/TABL cursor MA\HISTORY 36Rm50 0 6850 3 Y MA36Rm50 READ/TABL \HISTORY cursor MA36Rm50 0 6850 3 Y MA36Rm50 RA = 5.648169994354E+00 / MIDAS desc.: O_POS(1) DEC = -3.018300056458E+01 / MIDAS desc.: O_POS(2) AIRMASS = 1.068349957466E+00 / MIDAS desc.: O_AIRM(1) HIERARCH ESO GEN ID = 'ARC-0001/1.2' HIERARCH ESO GEN PROJ ID = '000.00.000' HIERARCH ESO GEN EXPO NO = 24887 HIERARCH ESO GEN EXPO TYPE = 'SCI ' HIERARCH ESO GEN EXPO LST = 2.420000000000E+03 HIERARCH ESO TEL ID = 'ESONTTB ' HIERARCH ESO TEL LON = 7.073450000000E+01 HIERARCH ESO TEL LAT = -2.925840000000E+01 HIERARCH ESO TEL ALTITUDE = 2440 HIERARCH ESO TEL FOCU LEN = 3.848200000000E+01 HIERARCH ESO TEL FOCU SCALE = 1.489000000000E+00 HIERARCH ESO TEL TRAK RATEA = 4.200000000000E-03 HIERARCH ESO TEL TRAK RATED = 0.000000000000E+00 HIERARCH ESO ADA ID = 'ADAPTB ' HIERARCH ESO ADA MODE = 'STD ' HIERARCH ESO ADA ROT = 0.000000000000E+00 HIERARCH ESO ADA GUID-1 X = 1.294000000000E-02 HIERARCH ESO ADA GUID-1 Y = 1.717000000000E-01 HIERARCH ESO ADA GUID-2 X = 5.070000000000E-04 HIERARCH ESO ADA GUID-2 Y = 1.110000000000E-03 HIERARCH ESO INS ID = 'EMMI #1 ' HIERARCH ESO INS COMP ID = 'HP RTE-A V5' HIERARCH ESO INS MODE = 'RILD ' HIERARCH ESO INS OPTI-2 NO = 1 HIERARCH ESO INS OPTI-2 TYPE = 'MIRROR ' HIERARCH ESO INS OPTI-2 ID = 'RILD MIR' HIERARCH ESO INS OPTI-2 NAME = 'RILD ' HIERARCH ESO INS OPTI-3 NO = 1 HIERARCH ESO INS OPTI-3 TYPE = 'FREE ' HIERARCH ESO INS MIRR-3 NAME = 'UPPER RED' HIERARCH ESO INS MIRR-3 ST = 0 HIERARCH ESO INS OPTI-7 NO = 3 HIERARCH ESO INS OPTI-7 TYPE = 'FILTER ' HIERARCH ESO INS OPTI-7 ID = '#608 ' HIERARCH ESO INS OPTI-7 NAME = 'R ' HIERARCH ESO INS OPTI-9 NO = 9 HIERARCH ESO INS OPTI-9 TYPE = 'FREE ' HIERARCH ESO DET NAME = 'THX31156' HIERARCH ESO DET ID = 'ccd$18 ' HIERARCH ESO DET TYPE = 'CCD Four_Phase' HIERARCH ESO DET PIXSIZE = 1.900000000000E-05 HIERARCH ESO DET BITS = 16 HIERARCH ESO DET FRAM NAXIS1 = 1060 HIERARCH ESO DET FRAM CRVAL1 = 1 HIERARCH ESO DET FRAM CRPIX1 = 1 HIERARCH ESO DET FRAM CDELT1 = 1 HIERARCH ESO DET FRAM NAXIS2 = 1040 HIERARCH ESO DET FRAM CRVAL2 = 1 HIERARCH ESO DET FRAM CRPIX2 = 1 HIERARCH ESO DET FRAM CDELT2 = 1 HIERARCH ESO DET DKTIME = 4.000000000000E+02 HIERARCH ESO DET TEMP_VAR = 1.000000000000E-01 HIERARCH ESO DET TEMPMEAN = 1.376000000000E+02 HIERARCH ESO DET COMP ID = 'ccdr-V1.0' HIERARCH ESO DET PARM1 = 'CLOCK=tho1k' HIERARCH ESO DET PARM2 = 'HLO1 : 2.02 VLO1 : 1.01 VDD1 : 23.03' HIERARCH ESO DET PARM3 = 'HHI1 : 15.00 VHI1 : 12.01 VDR1 : 13.98' HIERARCH ESO DET PARM4 = 'HLO2 : 2.02 RLO1 : 1.01 VGS1 : 4.99' HIERARCH ESO DET PARM5 = 'HHI2 : 15.03 RHI1 : 10.07 ICCD1 : 0.00' HIERARCH ESO DET PARM6 = 'TL 1, 5 telem. data' HIERARCH ESO DET DATE = 1.989794555664E+03 HIERARCH ESO DET MODE = 'SLOW ' HIERARCH ESO DET GAIN = 1 HIERARCH ESO DET AD_VALUE = 2.100000000000E+00 HIERARCH ESO DET DIT = 4.000000000000E+02 HIERARCH ESO DET SHUT TMOPEN = 5.000000000000E-01 HIERARCH ESO DET SHUT TMCLOS = 5.000000000000E-01 HISTORY ESO-DESCRIPTORS START ................ HISTORY 'WIND_RAW' ,'R*4 ' , 1, 4,'5E14.7',' ',' ' HISTORY 1.9000000E+01 3.0000000E+00 1.0420000E+03 1.0260000E+03 HISTORY HISTORY 'STAT_RAW' ,'R*4 ' , 1, 13,'5E14.7',' ',' ' HISTORY 6.5800000E+02 3.2767000E+04 2.3813201E+03 5.6562799E+02 2.4699001E+10 HISTORY 3.8941301E+14 2.4969999E+09 2.3490701E+03 2.3460000E+03 2.0070000E+03 HISTORY 1.6000000E+01 6.5800000E+02 3.2767000E+04 HISTORY HISTORY 'WIND_OVER' ,'R*4 ' , 1, 4,'5E14.7',' ',' ' HISTORY 1.0000000E+01 1.0290000E+03 1.0550000E+03 1.0390000E+03 HISTORY HISTORY 'STAT_OVER' ,'R*4 ' , 1, 13,'5E14.7',' ',' ' HISTORY 2.1200000E+02 2.4400000E+02 2.2111700E+02 2.5815699E+00 1.0815500E+07 HISTORY 2.3924700E+09 2.5441800E+06 2.2058000E+02 2.2050000E+02 3.3000000E+01 HISTORY 1.0000000E+00 2.1200000E+02 2.4400000E+02 HISTORY HISTORY 'BIAS_FRAME' ,'C*1 ' , 1, 7,'7A1',' ',' ' HISTORY bias50 HISTORY HISTORY 'BIAS_OVER_DIFF' ,'R*4 ' , 1, 1,'5E14.7',' ',' ' HISTORY 1.5100101E-01 HISTORY HISTORY 'FLAT_WIND' ,'R*4 ' , 1, 4,'5E14.7',' ',' ' HISTORY 4.5000000E+02 3.8000000E+02 7.4000000E+02 6.2000000E+02 HISTORY HISTORY 'FLAT_BKG' ,'R*4 ' , 1, 1,'5E14.7',' ',' ' HISTORY 2.1311699E+03 HISTORY HISTORY 'SKIM_FRAC' ,'R*4 ' , 1, 1,'5E14.7',' ',' ' HISTORY 3.5154400E-04 HISTORY HISTORY 'AV_WIND_NAME' ,'C*1 ' , 1, 5,'5A1',' ',' ' HISTORY fRc50 HISTORY HISTORY 'FLAT_FRAME' ,'C*1 ' , 1, 5,'5A1',' ',' ' HISTORY fRc50 HISTORY HISTORY 'WIND_FIN' ,'R*4 ' , 1, 4,'5E14.7',' ',' ' HISTORY 1.9000000E+01 3.0000000E+00 1.0420000E+03 1.0260000E+03 HISTORY HISTORY 'STAT_FIN' ,'R*4 ' , 1, 13,'5E14.7',' ',' ' HISTORY 6.0423798E+02 3.2842602E+04 2.1606499E+03 5.5936798E+02 2.0734501E+10 HISTORY 3.5516501E+14 2.2656100E+09 2.1273799E+03 2.1162400E+03 2.0150000E+03 HISTORY 1.6000000E+01 6.0423798E+02 3.2842602E+04 HISTORY HISTORY 'WIND_SUM' ,'R*4 ' , 1, 4,'5E14.7',' ',' ' HISTORY 1.0000000E+00 1.0000000E+00 1.0240000E+03 1.0240000E+03 HISTORY HISTORY 'STAT_SUM' ,'R*4 ' , 1, 13,'5E14.7',' ',' ' HISTORY 3.7136699E+03 9.8528203E+04 6.9033799E+03 1.6677500E+03 6.1352398E+11 HISTORY 2.8897399E+16 7.2387098E+09 6.8047002E+03 6.7938701E+03 2.0480000E+03 HISTORY 4.6318802E+01 3.7136699E+03 9.8528203E+04 HISTORY HISTORY 'LHCUTS' ,'R*4 ' , 1, 4,'5E14.7',' ',' ' HISTORY 5.5000000E+03 9.0000000E+03 3.7136670E+03 9.8528234E+04 HISTORY HISTORY 'DISPLAY_DATA' ,'I*4 ' , 1, 9,'7I10',' ',' ' HISTORY 2 2 513 513 0 -1 -1 HISTORY -1 -1 HISTORY HISTORY 'BOX_MIN' ,'R*4 ' , 1, 6,'5E14.7',' ',' ' HISTORY 3.2100000E+02 2.1500000E+02 6.9644336E+03 6.3300000E+02 4.2300000E+02 HISTORY 6.8900532E+03 HISTORY HISTORY 'IJBORDER' ,'I*4 ' , 1, 4,'7I10',' ',' ' HISTORY 1 1 1024 1024 HISTORY HISTORY 'LHCUT' ,'R*4 ' , 1, 2,'5E14.7',' ',' ' HISTORY 3.6236699E+03 8.0148297E+04 HISTORY HISTORY 'ZEROMAGN' ,'R*4 ' , 1, 1,'5E14.7',' ',' ' HISTORY 2.4671000E+01 HISTORY HISTORY 'SEEING' ,'R*4 ' , 1, 2,'5E14.7',' ',' ' HISTORY 1.8308023E+00 9.6358800E-01 HISTORY HISTORY 'PAIRSPRT' ,'R*4 ' , 1, 1,'5E14.7',' ',' ' HISTORY 3.1899800E+00 HISTORY HISTORY 'MULTDTCT' ,'R*4 ' , 1, 1,'5E14.7',' ',' ' HISTORY 4.1900001E+00 HISTORY HISTORY 'PRFLCTRL' ,'I*4 ' , 1, 1,'7I10',' ',' ' HISTORY -5 HISTORY HISTORY 'OUPROFIL' ,'I*4 ' , 1, 1,'7I10',' ',' ' HISTORY 5 HISTORY HISTORY 'STMETRIC' ,'R*4 ' , 1, 2,'5E14.7',' ',' ' HISTORY 9.3000001E-01 5.5799999E+00 HISTORY HISTORY 'BRGHTLMT' ,'R*4 ' , 1, 1,'5E14.7',' ',' ' HISTORY 1.8387699E+01 HISTORY HISTORY 'NBSTARS' ,'I*4 ' , 1, 1,'7I10',' ',' ' HISTORY 17 HISTORY HISTORY 'PSFTAB' ,'I*4 ' , 1, 1,'7I10',' ',' ' HISTORY 1 HISTORY HISTORY 'THRESHOLD' ,'R*4 ' , 1, 5,'5E14.7',' ',' ' HISTORY 6.8047002E+03 1.1384800E+02 1.6730800E+00 2.0000000E+00 2.5446301E+01 HISTORY HISTORY 'N_SEARCH_ANA' ,'I*4 ' , 1, 2,'7I10',' ',' ' HISTORY 822 806 HISTORY HISTORY 'N_STAR_GAL_DEF' ,'I*4 ' , 1, 3,'7I10',' ',' ' HISTORY 46 744 16 HISTORY HISTORY 'HIST_BINS' ,'R*4 ' , 1, 5,'5E14.7',' ',' ' HISTORY 2.5600000E+02 2.8824686E+02 3.7136670E+03 7.7216609E+04 0.0000000E+00 HISTORY HISTORY 'HISTOGRAM' ,'I*4 ' , 1, 256,'7I10',' ',' ' HISTORY 1 0 0 0 0 0 0 HISTORY 0 0 0 10 64 23 12 HISTORY 3 3 4 4 3 1 2 HISTORY 0 0 1 1 0 1 0 HISTORY 0 0 0 3 0 1 0 HISTORY 0 1 0 1 0 1 0 HISTORY 0 0 1 1 0 1 0 HISTORY 1 0 0 0 0 0 0 HISTORY 0 0 1 1 0 0 0 HISTORY 0 0 0 0 0 0 0 HISTORY 0 0 0 0 0 0 0 HISTORY 0 0 0 0 0 0 0 HISTORY 0 1 0 0 0 0 0 HISTORY 0 0 0 0 0 0 0 HISTORY 0 0 0 0 0 1 0 HISTORY 0 0 0 0 0 0 0 HISTORY 0 1 0 1 0 0 1 HISTORY 0 0 0 0 0 0 0 HISTORY 0 0 0 0 0 0 0 HISTORY 0 1 0 0 0 0 0 HISTORY 1 0 0 0 0 0 0 HISTORY 0 0 0 0 0 1 0 HISTORY 0 0 0 0 0 1 0 HISTORY 0 0 0 0 1 0 0 HISTORY 0 1 0 0 0 0 0 HISTORY 0 0 0 0 1 0 0 HISTORY 0 1 0 0 0 0 0 HISTORY 0 0 0 0 0 0 0 HISTORY 0 0 0 0 0 0 0 HISTORY 0 0 0 0 0 0 1 HISTORY 0 0 0 0 0 0 0 HISTORY 0 0 0 0 0 0 0 HISTORY 0 0 0 0 0 0 0 HISTORY 0 0 0 0 0 0 0 HISTORY 0 0 0 0 0 0 0 HISTORY 0 0 1 0 0 0 0 HISTORY 0 0 1 0 HISTORY HISTORY 'STATISTIC' ,'R*4 ' , 1, 11,'5E14.7',' ',' ' HISTORY 3.7136670E+03 9.8528234E+04 6.9033760E+03 1.6677493E+03 6.1352378E+11 HISTORY 2.8897433E+16 7.2387144E+09 6.5048496E+03 3.8995779E+03 2.5600000E+02 HISTORY 3.7182184E+02 HISTORY HISTORY 'WINDOW_FROM' ,'I*4 ' , 1, 2,'7I10',' ',' ' HISTORY 1 1 HISTORY HISTORY 'WINDOW_TO' ,'I*4 ' , 1, 2,'7I10',' ',' ' HISTORY 1024 1024 HISTORY HISTORY 'NBMODIF' ,'I*4 ' , 1, 1,'7I10',' ',' ' HISTORY 1 HISTORY HISTORY 'STARS' ,'R*4 ' , 1, 51,'5E14.7',' ',' ' HISTORY 2.6300000E+02 8.8700000E+02 4.6759199E+04 7.5000000E+01 5.6300000E+02 HISTORY 1.5854400E+04 1.3000000E+01 3.1300000E+02 4.9727699E+04 3.3900000E+02 HISTORY 4.3300000E+02 9.6787102E+04 7.0100000E+02 1.6300000E+02 1.2378200E+04 HISTORY 8.5500000E+02 2.5500000E+02 3.5242898E+04 7.6100000E+02 3.3300000E+02 HISTORY 1.4904300E+04 1.0110000E+03 3.5700000E+02 2.5686801E+04 9.0700000E+02 HISTORY 4.0100000E+02 1.6969100E+04 8.4900000E+02 5.2500000E+02 1.4543700E+04 HISTORY 9.1700000E+02 5.4500000E+02 4.4644398E+04 7.7700000E+02 5.7700000E+02 HISTORY 3.6737199E+04 1.0010000E+03 6.9500000E+02 9.8214500E+04 8.2500000E+02 HISTORY 8.0100000E+02 2.0127900E+04 6.3100000E+02 6.3500000E+02 1.6520199E+04 HISTORY 5.8500000E+02 6.7500000E+02 1.5727300E+04 6.5900000E+02 6.6500000E+02 HISTORY 2.1833900E+04 HISTORY HISTORY 'DPROFILE' ,'R*4 ' , 1, 25,'5E14.7',' ',' ' HISTORY 3.2567519E-01 6.4562768E-01 6.5725815E-01 5.2960014E-01 4.1916752E-01 HISTORY 3.0000001E-01 2.8000000E-01 2.5999999E-01 2.3999999E-01 2.0000000E-01 HISTORY 1.8000001E-01 1.6000000E-01 1.4000000E-01 1.4000000E-01 1.4000000E-01 HISTORY 1.4000000E-01 1.4000000E-01 1.4000000E-01 1.4000000E-01 1.4000000E-01 HISTORY 1.4000000E-01 1.4000000E-01 1.4000000E-01 1.4000000E-01 1.4000000E-01 HISTORY HISTORY ESO-DESCRIPTORS END ................ 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gitextract_54cmwk4y/ ├── .clang-format ├── .github/ │ └── workflows/ │ ├── build-wheels-upload-pypi.yml │ └── python-package-tox.yml ├── .gitignore ├── .pre-commit-config.yaml ├── .readthedocs.yaml ├── AUTHORS.md ├── CHANGES.md ├── CMakeLists.txt ├── FindSEP.cmake ├── MANIFEST.in ├── Makefile ├── README.md ├── bench.py ├── codemeta.json ├── ctest/ │ ├── compare.py │ └── test_image.c ├── data/ │ ├── README.md │ ├── back.fits │ ├── default.conv │ ├── default.nnw │ ├── default.param │ ├── default.sex │ ├── image.cat │ ├── image.fits │ └── rms.fits ├── docs/ │ ├── Makefile │ ├── apertures.rst │ ├── changelogs/ │ │ ├── changelog.rst │ │ ├── changes_to_c_api.rst │ │ ├── new_changes.rst │ │ └── original_changes.md │ ├── conf.py │ ├── filter.rst │ ├── index.rst │ ├── reference.rst │ ├── rtd-pip-requirements │ └── tutorial.ipynb ├── licenses/ │ ├── BSD_LICENSE.txt │ ├── LGPL_LICENSE.txt │ └── MIT_LICENSE.txt ├── paper/ │ ├── paper.bib │ └── paper.md ├── pyproject.toml ├── sep.pyx ├── setup.py ├── src/ │ ├── analyse.c │ ├── aperture.c │ ├── aperture.i │ ├── background.c │ ├── convolve.c │ ├── deblend.c │ ├── extract.c │ ├── extract.h │ ├── lutz.c │ ├── overlap.h │ ├── sep.h │ ├── sepcore.h │ └── util.c ├── test.py └── tox.ini
SYMBOL INDEX (157 symbols across 16 files)
FILE: ctest/compare.py
function read_table (line 10) | def read_table(fname):
function fracdiff (line 40) | def fracdiff(x, y):
FILE: ctest/test_image.c
function gettime_ns (line 10) | uint64_t gettime_ns() {
function addbox (line 56) | void addbox(float * im, int w, int h, float xc, float yc, float r, float...
function printbox (line 80) | void printbox(float * im, int w, int h, int xmin, int xmax, int ymin, in...
function read_test_image (line 97) | int read_test_image(char * fname, float ** data, int64_t * nx, int64_t *...
function print_time (line 194) | void print_time(char * s, uint64_t tdiff) {
function main (line 198) | int main(int argc, char ** argv) {
FILE: setup.py
function _new_version_scheme (line 13) | def _new_version_scheme(version: ScmVersion) -> str:
function _new_local_scheme (line 18) | def _new_local_scheme(version: ScmVersion) -> str:
FILE: src/analyse.c
function analysemthresh (line 39) | int analysemthresh(int objnb, objliststruct * objlist, int minarea, PIXT...
function preanalyse (line 100) | void preanalyse(int no, objliststruct * objlist) {
function analyse (line 168) | void analyse(int no, objliststruct * objlist, int robust, double gain) {
FILE: src/aperture.c
function sep_ellipse_axes (line 62) | int sep_ellipse_axes(
function sep_ellipse_coeffs (line 91) | void sep_ellipse_coeffs(
function boxextent (line 111) | static void boxextent(
function boxextent_ellipse (line 147) | static void boxextent_ellipse(
function oversamp_ann_circle (line 172) | static void oversamp_ann_circle(double r, double * r_in2, double * r_out...
function oversamp_ann_ellipse (line 180) | static void oversamp_ann_ellipse(double r, double b, double * r_in2, dou...
function sep_sum_circann_multi (line 348) | int sep_sum_circann_multi(
function inverse (line 578) | static double inverse(double xmax, const double * y, int64_t n, double y...
function sep_flux_radius (line 604) | int sep_flux_radius(
function sep_kron_radius (line 661) | int sep_kron_radius(
function sep_set_ellipse (line 781) | void sep_set_ellipse(
function sep_windowed (line 827) | int sep_windowed(
FILE: src/background.c
type backstruct (line 38) | typedef struct {
function sep_background (line 73) | int sep_background(
function backstat (line 277) | void backstat(
function backhisto (line 398) | void backhisto(
function backguess (line 466) | float backguess(backstruct * bkg, float * mean, float * sigma)
function filterback (line 540) | int filterback(sep_bkg * bkg, int64_t fw, int64_t fh, double fthresh)
function makebackspline (line 682) | int makebackspline(const sep_bkg * bkg, float * map, float * dmap) {
function sep_bkg_global (line 729) | float sep_bkg_global(const sep_bkg * bkg) {
function sep_bkg_globalrms (line 733) | float sep_bkg_globalrms(const sep_bkg * bkg) {
function sep_bkg_pix (line 740) | float sep_bkg_pix(const sep_bkg * bkg, int64_t x, int64_t y)
function bkg_line_flt_internal (line 790) | int bkg_line_flt_internal(
function sep_bkg_line_flt (line 915) | int sep_bkg_line_flt(const sep_bkg * bkg, int64_t y, float * line)
function sep_bkg_rmsline_flt (line 924) | int sep_bkg_rmsline_flt(const sep_bkg * bkg, int64_t y, float * line)
function sep_bkg_line (line 935) | int sep_bkg_line(const sep_bkg * bkg, int64_t y, void * line, int dtype) {
function sep_bkg_rmsline (line 966) | int sep_bkg_rmsline(const sep_bkg * bkg, int64_t y, void * line, int dty...
function sep_bkg_array (line 997) | int sep_bkg_array(const sep_bkg * bkg, void * arr, int dtype) {
function sep_bkg_rmsarray (line 1037) | int sep_bkg_rmsarray(const sep_bkg * bkg, void * arr, int dtype) {
function sep_bkg_subline (line 1077) | int sep_bkg_subline(const sep_bkg * bkg, int64_t y, void * line, int dty...
function sep_bkg_subarray (line 1105) | int sep_bkg_subarray(const sep_bkg * bkg, void * arr, int dtype) {
function sep_bkg_free (line 1138) | void sep_bkg_free(sep_bkg * bkg) {
FILE: src/convolve.c
function convolve (line 39) | int convolve(
function matched_filter (line 126) | int matched_filter(
FILE: src/deblend.c
function sep_set_sub_object_limit (line 41) | void sep_set_sub_object_limit(int val) {
function sep_get_sub_object_limit (line 45) | int sep_get_sub_object_limit() {
function deblend (line 63) | int deblend(
function allocdeblend (line 238) | int allocdeblend(int deblend_nthresh, int64_t w, int64_t h, deblendctx *...
function freedeblend (line 259) | void freedeblend(deblendctx * ctx) {
function gatherup (line 274) | int gatherup(objliststruct * objlistin, objliststruct * objlistout) {
function belong (line 399) | int belong(
FILE: src/extract.c
function sep_set_extract_pixstack (line 48) | void sep_set_extract_pixstack(size_t val) {
function sep_get_extract_pixstack (line 52) | size_t sep_get_extract_pixstack() {
function arraybuffer_init (line 99) | int arraybuffer_init(
function arraybuffer_readline (line 149) | void arraybuffer_readline(arraybuffer * buf) {
function arraybuffer_free (line 167) | void arraybuffer_free(arraybuffer * buf) {
function apply_mask_line (line 190) | void apply_mask_line(
function sep_extract (line 206) | int sep_extract(
function segsortit (line 877) | int segsortit(
function sortit (line 917) | int sortit(
function addobjdeep (line 996) | int addobjdeep(int objnb, objliststruct * objl1, objliststruct * objl2) {
function plistinit (line 1058) | void plistinit(int hasconv, int hasvar) {
function clean (line 1094) | void clean(objliststruct * objlist, double clean_param, int * survives) {
function PIXTYPE (line 1168) | PIXTYPE get_mean_thresh(infostruct * info, pliststruct * pixel) {
function free_catalog_fields (line 1188) | void free_catalog_fields(sep_catalog * catalog) {
function convert_to_catalog (line 1236) | int convert_to_catalog(
function sep_catalog_free (line 1389) | void sep_catalog_free(sep_catalog * catalog) {
FILE: src/extract.h
type pixstatus (line 42) | typedef enum {
type infostruct (line 50) | typedef struct structinfo {
type pliststruct (line 57) | typedef char pliststruct;
type pbliststruct (line 59) | typedef struct {
type arraybuffer (line 66) | typedef struct {
type objstruct (line 88) | typedef struct {
type objliststruct (line 129) | typedef struct {
type lutzbuffers (line 142) | typedef struct {
type deblendctx (line 166) | typedef struct {
FILE: src/lutz.c
function lutzalloc (line 42) | int lutzalloc(int64_t width, int64_t height, lutzbuffers * buffers) {
function lutzfree (line 77) | void lutzfree(lutzbuffers * buffers) {
function lutz (line 101) | int lutz(
function lutzsort (line 319) | void lutzsort(infostruct * info, objliststruct * objlist) {
function update (line 337) | void update(infostruct * infoptr1, infostruct * infoptr2, pliststruct * ...
FILE: src/overlap.h
function INLINE (line 19) | static INLINE double area_arc(double x1, double y1, double x2, double y2...
function INLINE (line 28) | static INLINE double area_triangle(
function INLINE (line 38) | static INLINE double circoverlap_core(
function circoverlap (line 102) | static double circoverlap(
type point (line 184) | typedef struct {
type intersections (line 189) | typedef struct {
function INLINE (line 193) | static INLINE void swap(double * a, double * b) {
function INLINE (line 200) | static INLINE void swap_point(point * a, point * b) {
function INLINE (line 208) | static INLINE void rotate(double * a, double * b, double * c) {
function in_triangle (line 217) | static int in_triangle(
function intersections (line 232) | static intersections circle_line(double x1, double y1, double x2, double...
function point (line 291) | static point circle_segment_single2(double x1, double y1, double x2, dou...
function intersections (line 317) | static inline intersections circle_segment(double x1, double y1, double ...
function triangle_unitcircle_overlap (line 351) | static double triangle_unitcircle_overlap(
function ellipoverlap (line 517) | static double ellipoverlap(
FILE: src/sep.h
type sep_image (line 71) | typedef struct {
type sep_bkg (line 96) | typedef struct {
type sep_catalog (line 114) | typedef struct {
FILE: src/sepcore.h
type LONG (line 41) | typedef int LONG;
type ULONG (line 42) | typedef unsigned int ULONG;
type BYTE (line 43) | typedef unsigned char BYTE;
type PIXTYPE (line 46) | typedef float PIXTYPE;
type PIXTYPE (line 51) | typedef PIXTYPE (*converter)(const void * ptr);
FILE: src/util.c
function PIXTYPE (line 37) | PIXTYPE convert_dbl(const void * ptr) {
function PIXTYPE (line 41) | PIXTYPE convert_flt(const void * ptr) {
function PIXTYPE (line 45) | PIXTYPE convert_int(const void * ptr) {
function PIXTYPE (line 49) | PIXTYPE convert_byt(const void * ptr) {
function get_converter (line 54) | int get_converter(int dtype, converter * f, int64_t * size) {
function convert_array_flt (line 78) | void convert_array_flt(const void * ptr, int64_t n, PIXTYPE * target) {
function convert_array_dbl (line 86) | void convert_array_dbl(const void * ptr, int64_t n, PIXTYPE * target) {
function convert_array_int (line 94) | void convert_array_int(const void * ptr, int64_t n, PIXTYPE * target) {
function convert_array_byt (line 102) | void convert_array_byt(const void * ptr, int64_t n, PIXTYPE * target) {
function get_array_converter (line 110) | int get_array_converter(int dtype, array_converter * f, int64_t * size) {
function write_array_dbl (line 137) | void write_array_dbl(const float * ptr, int64_t n, void * target) {
function write_array_int (line 145) | void write_array_int(const float * ptr, int64_t n, void * target) {
function get_array_writer (line 154) | int get_array_writer(int dtype, array_writer * f, int64_t * size) {
function subtract_array_dbl (line 173) | void subtract_array_dbl(const float * ptr, int64_t n, void * target) {
function subtract_array_flt (line 181) | void subtract_array_flt(const float * ptr, int64_t n, void * target) {
function subtract_array_int (line 189) | void subtract_array_int(const float * ptr, int64_t n, void * target) {
function get_array_subtractor (line 198) | int get_array_subtractor(int dtype, array_writer * f, int64_t * size) {
function sep_get_errmsg (line 224) | void sep_get_errmsg(int status, char * errtext)
function sep_get_errdetail (line 270) | void sep_get_errdetail(char * errtext) {
function put_errdetail (line 275) | void put_errdetail(const char * errtext) {
function fqcmp (line 282) | static int fqcmp(const void * p1, const void * p2)
function fqmedian (line 291) | float fqmedian(float * ra, int64_t n)
FILE: test.py
function assert_allclose_structured (line 70) | def assert_allclose_structured(x, y):
function matched_filter_snr (line 89) | def matched_filter_snr(data, noise, kernel):
function test_vs_sextractor (line 167) | def test_vs_sextractor():
function test_masked_background (line 312) | def test_masked_background():
function test_background_special (line 351) | def test_background_special():
function test_background_boxsize (line 369) | def test_background_boxsize():
function test_background_rms (line 380) | def test_background_rms():
function test_extract_with_noise_array (line 398) | def test_extract_with_noise_array():
function test_extract_with_noise_convolution (line 449) | def test_extract_with_noise_convolution():
function test_extract_matched_filter_at_edge (line 491) | def test_extract_matched_filter_at_edge():
function test_extract_with_mask (line 518) | def test_extract_with_mask():
function test_extract_with_maskthresh (line 542) | def test_extract_with_maskthresh():
function test_extract_segmentation_map (line 586) | def test_extract_segmentation_map():
function test_extract_seg_map_array (line 608) | def test_extract_seg_map_array():
function test_aperture_dtypes (line 702) | def test_aperture_dtypes():
function test_apertures_small_ellipse_exact (line 722) | def test_apertures_small_ellipse_exact():
function test_apertures_all (line 732) | def test_apertures_all():
function test_apertures_exact (line 756) | def test_apertures_exact():
function test_aperture_bkgann_overlapping (line 787) | def test_aperture_bkgann_overlapping():
function test_aperture_bkgann_ones (line 805) | def test_aperture_bkgann_ones():
function test_masked_segmentation_measurements (line 829) | def test_masked_segmentation_measurements():
function test_mask_ellipse (line 908) | def test_mask_ellipse():
function test_flux_radius (line 923) | def test_flux_radius():
function test_mask_ellipse_alt (line 937) | def test_mask_ellipse_alt():
function test_byte_order_exception (line 956) | def test_byte_order_exception():
function test_set_pixstack (line 972) | def test_set_pixstack():
function test_set_sub_object_limit (line 983) | def test_set_sub_object_limit():
function test_long_error_msg (line 994) | def test_long_error_msg():
Condensed preview — 61 files, each showing path, character count, and a content snippet. Download the .json file or copy for the full structured content (1,599K chars).
[
{
"path": ".clang-format",
"chars": 2823,
"preview": "# SPDX-License-Identifier: MIT\n#\n# Copyright (c) 2023 Intercreate, Inc.\n# Author: J.P. Hutchins <jp@intercreate.io>\n#\n# "
},
{
"path": ".github/workflows/build-wheels-upload-pypi.yml",
"chars": 4409,
"preview": "# GitHub action for building the distribution and wheels of the sep package\n# and uploading them to the PyPI package ind"
},
{
"path": ".github/workflows/python-package-tox.yml",
"chars": 935,
"preview": "# This workflow will install tox and use it to run tests.\n# For more information see: https://help.github.com/actions/la"
},
{
"path": ".gitignore",
"chars": 520,
"preview": "# emacs\n*~\n\n# --------------------------------------------\n# C\n\n*.o\n*.os\n*.so\n*.so.*\n*.dylib\n*.dylib.*\n*.a\nctest/test_im"
},
{
"path": ".pre-commit-config.yaml",
"chars": 931,
"preview": "exclude: \"^data/\"\nrepos:\n- repo: https://github.com/pre-commit/pre-commit-hooks\n rev: v5.0.0\n hooks:\n - id:"
},
{
"path": ".readthedocs.yaml",
"chars": 1101,
"preview": "# Read the Docs configuration file for Sphinx projects\n# See https://docs.readthedocs.io/en/stable/config-file/v2.html f"
},
{
"path": "AUTHORS.md",
"chars": 716,
"preview": "* Emmanuel Bertin (bertin@iap.fr) : original SExtractor code\n* Kyle Barbary (@kbarbary) : Conversion of SExtractor code "
},
{
"path": "CHANGES.md",
"chars": 2847,
"preview": "v1.3.7 (8 November 2024)\n========================\n\n* Test against Python 3.13.\n* Update the Makefile to support Semantic"
},
{
"path": "CMakeLists.txt",
"chars": 1099,
"preview": "cmake_minimum_required(VERSION 2.6)\n\nproject(sep C)\n\nLIST(APPEND CMAKE_MODULE_PATH \"${CMAKE_SOURCE_DIR}/cmake_modules/\")"
},
{
"path": "FindSEP.cmake",
"chars": 1325,
"preview": "# - Try to find SEP\n# Once done this will define\n#\n# SEP_FOUND - system has SEP\n# SEP_INCLUDE_DIR - the SEP include di"
},
{
"path": "MANIFEST.in",
"chars": 151,
"preview": "include README.md\ninclude CHANGES.md\ninclude AUTHORS.md\ninclude licenses/*\ninclude pyproject.toml\n\ninclude src/*.[c,h,i]"
},
{
"path": "Makefile",
"chars": 3576,
"preview": "\nOS ?= $(shell sh -c 'uname -s | tr \"[A-Z]\" \"[a-z]\"')\n\nDESCRIBE := $(shell git describe --match \"v*\" --always "
},
{
"path": "README.md",
"chars": 11060,
"preview": "SEP\n===\n\nPython and C library for Source Extraction and Photometry.\n\n[![PyPI](https://img.shields.io/pypi/v/sep?label=Py"
},
{
"path": "bench.py",
"chars": 7339,
"preview": "#!/usr/bin/env python\n\n\"\"\"Benchmarking SEP against equivalent photutils functions.\"\"\"\n\nfrom __future__ import print_func"
},
{
"path": "codemeta.json",
"chars": 756,
"preview": "{\n \"@context\": \"https://raw.githubusercontent.com/mbjones/codemeta/master/codemeta.jsonld\",\n \"@type\": \"Code\",\n \"autho"
},
{
"path": "ctest/compare.py",
"chars": 1647,
"preview": "#!/usr/bin/env python\n\n\"\"\"Compare the output from SEP against SExtractor.\"\"\"\n\nfrom __future__ import print_function\n\nimp"
},
{
"path": "ctest/test_image.c",
"chars": 8683,
"preview": "#include <math.h>\n#include <stdint.h>\n#include <stdio.h>\n#include <stdlib.h>\n#include <string.h>\n#include <sys/time.h>\n\n"
},
{
"path": "data/README.md",
"chars": 160,
"preview": "Test Data\n---------\n\nThe comparison catalog file `image.cat` is generated by running\n\n```\nsextractor image.fits -CATALOG"
},
{
"path": "data/back.fits",
"chars": 177291,
"preview": "SIMPLE = T / file does conform to FITS standard BITPIX = -32 / number "
},
{
"path": "data/default.conv",
"chars": 88,
"preview": "CONV NORM\n# 3x3 ``all-ground'' convolution mask with FWHM = 2 pixels.\n1 2 1\n2 4 2\n1 2 1\n"
},
{
"path": "data/default.nnw",
"chars": 2187,
"preview": "NNW\n# Neural Network Weights for the SExtractor star/galaxy classifier (V1.3)\n# inputs:\t9 for profile parameters + 1 for"
},
{
"path": "data/default.param",
"chars": 201,
"preview": "NUMBER\nX_IMAGE\nY_IMAGE\nXWIN_IMAGE\nYWIN_IMAGE\nX2_IMAGE\nY2_IMAGE\nXY_IMAGE\nERRX2_IMAGE\nERRY2_IMAGE\nERRXY_IMAGE\nA_IMAGE\nFLUX"
},
{
"path": "data/default.sex",
"chars": 3840,
"preview": "# Default configuration file for SExtractor 2.5.0\n# EB 2006-07-14\n#\n \n#-------------------------------- Catalog --------"
},
{
"path": "data/image.cat",
"chars": 19888,
"preview": "# 1 NUMBER Running object number \n# 2 X_IMAGE Obj"
},
{
"path": "data/image.fits",
"chars": 159664,
"preview": "SIMPLE = T / file does conform to FITS standard BITPIX = 16 / number "
},
{
"path": "data/rms.fits",
"chars": 165441,
"preview": "SIMPLE = T / file does conform to FITS standard BITPIX = -32 / number "
},
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"path": "docs/Makefile",
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"preview": "# Makefile for Sphinx documentation\n#\n\n# You can set these variables from the command line.\nSPHINXOPTS =\nSPHINXBUILD "
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"path": "docs/apertures.rst",
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"preview": "Aperture photometry\n===================\n\nThere are four aperture functions available:\n\n================== ============="
},
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"path": "docs/changelogs/changelog.rst",
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"preview": ".. _changelog:\n\nChangelog\n=========\n\n\nUpgrading From kbarbary/sep\n---------------------------\n\n.. toctree::\n :maxdepth"
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"path": "docs/changelogs/changes_to_c_api.rst",
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"preview": "Changes to the C API\n====================\n\nThis page details cumulative changes to the C API between v1.2.1 and\nv1.4.0, "
},
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"path": "docs/changelogs/new_changes.rst",
"chars": 111,
"preview": "New Changelog\n=============\n\n**Full Changelog**\n\n.. include:: ../../CHANGES.md\n :parser: myst_parser.sphinx_\n"
},
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"path": "docs/changelogs/original_changes.md",
"chars": 5428,
"preview": "Original Changelog\n==================\n\nThis is the original changelog from [kbarbary/sep](https://github.com/kbarbary/se"
},
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"path": "docs/conf.py",
"chars": 9326,
"preview": "# -*- coding: utf-8 -*-\n#\n# seppy documentation build configuration file, created by\n# sphinx-quickstart on Mon Jul 7 1"
},
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"path": "docs/filter.rst",
"chars": 5381,
"preview": "Matched Filter (Convolution)\n============================\n\nFor source detection, SEP supports using a matched filter, wh"
},
{
"path": "docs/index.rst",
"chars": 4710,
"preview": "SEP\n===\n\n*Python library for Source Extraction and Photometry*\n\n\nAbout\n-----\n\n`Source Extractor <http://www.astromatic.n"
},
{
"path": "docs/reference.rst",
"chars": 1934,
"preview": "Reference/API\n=============\n\n\n**Background estimation & source detection**\n\n.. autosummary::\n :toctree: api\n\n sep.Ba"
},
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"path": "docs/rtd-pip-requirements",
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"preview": "numpy\nCython\nnbsphinx\nmatplotlib\nfitsio\nnumpydoc\njupyter\nsphinx-astropy[confv2]\n"
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"path": "docs/tutorial.ipynb",
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"preview": "{\n \"cells\": [\n {\n \"cell_type\": \"markdown\",\n \"metadata\": {},\n \"source\": [\n \"# Tutorial\\n\",\n \"\\n\",\n \"This "
},
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"path": "licenses/BSD_LICENSE.txt",
"chars": 1495,
"preview": "Copyright (c) 2011-14, photutils developers\nAll rights reserved.\n\nRedistribution and use in source and binary forms, wit"
},
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"path": "licenses/LGPL_LICENSE.txt",
"chars": 7651,
"preview": " GNU LESSER GENERAL PUBLIC LICENSE\n Version 3, 29 June 2007\n\n Copyright (C) 2007"
},
{
"path": "licenses/MIT_LICENSE.txt",
"chars": 1087,
"preview": "The MIT License (MIT)\n\nCopyright (c) 2014-2016: SEP developers\n\nPermission is hereby granted, free of charge, to any per"
},
{
"path": "paper/paper.bib",
"chars": 650,
"preview": "@ARTICLE{bertin96,\n author = {{Bertin}, E. and {Arnouts}, S.},\n title = \"{SExtractor: Software for source extraction"
},
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"path": "paper/paper.md",
"chars": 2886,
"preview": "---\ntitle: 'SEP: Source Extractor as a library'\ntags:\n - astronomy\nauthors:\n - name: Kyle Barbary\n orcid: 0000-0002-2"
},
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"path": "pyproject.toml",
"chars": 2218,
"preview": "[build-system]\nrequires = [\n \"setuptools>=61.0, <72.2.0\",\n \"wheel\",\n \"numpy>=2.0.0rc2\",\n \"Cython\",\n \"setu"
},
{
"path": "sep.pyx",
"chars": 80846,
"preview": "# This wrapper licensed under an MIT license.\n\n\"\"\"\nSource Extraction and Photometry\n\nThis module is a wrapper of the SEP"
},
{
"path": "setup.py",
"chars": 2002,
"preview": "\"\"\"Setup file to build the C library.\"\"\"\n\nimport os\nimport re\nimport sys\nfrom glob import glob\n\nfrom setuptools import E"
},
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"path": "src/analyse.c",
"chars": 8492,
"preview": "/*%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%\n *\n * This file is part of SEP\n *\n * Copy"
},
{
"path": "src/aperture.c",
"chars": 28985,
"preview": "/*%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%\n *\n * This file is part of SEP\n *\n * Copy"
},
{
"path": "src/aperture.i",
"chars": 5012,
"preview": "/*\n Adding (void *) pointers is a GNU C extension, not part of standard C.\n When compiling on Windows with"
},
{
"path": "src/background.c",
"chars": 29009,
"preview": "/*%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%\n *\n * This file is part of SEP\n *\n * Copy"
},
{
"path": "src/convolve.c",
"chars": 6628,
"preview": "/*%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%\n*\n* This file is part of SEP\n*\n* Copyrigh"
},
{
"path": "src/deblend.c",
"chars": 13159,
"preview": "/*%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%\n *\n * This file is part of SEP\n *\n * Copy"
},
{
"path": "src/extract.c",
"chars": 39757,
"preview": "/*%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%\n *\n * This file is part of SEP\n *\n * Copy"
},
{
"path": "src/extract.h",
"chars": 6453,
"preview": "/*%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%\n *\n * This file is part of SEP\n *\n * Copy"
},
{
"path": "src/lutz.c",
"chars": 10252,
"preview": "/*%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%\n *\n * This file is part of SEP\n *\n * Copy"
},
{
"path": "src/overlap.h",
"chars": 15310,
"preview": "/* Licensed under a 3-clause BSD style license.\n *\n * Functions for calculating exact overlap between shapes.\n *\n * Orig"
},
{
"path": "src/sep.h",
"chars": 16367,
"preview": "/*%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%\n *\n * This file is part of SEP\n *\n * Copy"
},
{
"path": "src/sepcore.h",
"chars": 4454,
"preview": "/*%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%\n *\n * This file is part of SEP\n *\n * Copy"
},
{
"path": "src/util.c",
"chars": 7615,
"preview": "/*%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%\n *\n * This file is part of SEP\n *\n * All "
},
{
"path": "test.py",
"chars": 30988,
"preview": "#!/usr/bin/env py.test\n\n\"\"\"Test the python functionality of SEP.\"\"\"\n\nfrom __future__ import division, print_function\n\nim"
},
{
"path": "tox.ini",
"chars": 349,
"preview": "[tox]\nminversion = 4.0\nenvlist = py-{linux,macos,windows}\nisolated_build = true\n\n[gh-actions:env]\nPLATFORM =\n ubuntu-"
}
]
About this extraction
This page contains the full source code of the kbarbary/sep GitHub repository, extracted and formatted as plain text for AI agents and large language models (LLMs). The extraction includes 61 files (935.7 KB), approximately 509.1k tokens, and a symbol index with 157 extracted functions, classes, methods, constants, and types. Use this with OpenClaw, Claude, ChatGPT, Cursor, Windsurf, or any other AI tool that accepts text input. You can copy the full output to your clipboard or download it as a .txt file.
Extracted by GitExtract — free GitHub repo to text converter for AI. Built by Nikandr Surkov.