Skip to content

Commit

Permalink
Merge pull request #42 from Athanaseus/release_100
Browse files Browse the repository at this point in the history
Release 100
  • Loading branch information
Athanaseus committed Oct 27, 2020
2 parents baa013b + 2ac8a80 commit 93c108b
Show file tree
Hide file tree
Showing 15 changed files with 744 additions and 426 deletions.
5 changes: 4 additions & 1 deletion .github/workflows/test_installation.yml
Original file line number Diff line number Diff line change
Expand Up @@ -37,4 +37,7 @@ jobs:
flake8 . --count --exit-zero --max-complexity=10 --max-line-length=127 --statistics
- name: Test with pytest
run: |
pytest
pytest -s -vvv
- name: Test command
run: |
aimfast -h
2 changes: 2 additions & 0 deletions .gitignore
Original file line number Diff line number Diff line change
Expand Up @@ -23,3 +23,5 @@ docs/_build/

# Compiled bytecode
aimfast/*.pyc
aimfast/__pycache__/
aimfast/tests/__pycache__/
26 changes: 0 additions & 26 deletions .travis.yml

This file was deleted.

7 changes: 0 additions & 7 deletions .travis/mypy.docker

This file was deleted.

7 changes: 0 additions & 7 deletions .travis/pep8.docker

This file was deleted.

18 changes: 0 additions & 18 deletions .travis/py3.docker

This file was deleted.

2 changes: 1 addition & 1 deletion README.rst
Original file line number Diff line number Diff line change
Expand Up @@ -15,7 +15,7 @@ Main website: https://aimfast.readthedocs.io
Introduction
==============

Image fidelity is a measure of the accuracy of the reconstructed sky brightness distribution. A related metric, dynamic range, is a measure of the degree to which imaging artifacts around strong sources are suppressed, which in turn implies a higher fidelity of the on-source reconstruction. Moreover, the choice of image reconstruction algorithm also affects the correctness of the on-source brightness distribution. For high dynamic ranges with wide bandwidths, algorithms that model the sky spectrum as well as the average intensity can yield more accurate reconstructions.
Image fidelity is a measure of the accuracy of the reconstructed sky brightness distribution. A related metric, dynamic range, is a measure of the degree to which imaging artifacts around strong sources are suppressed, which in turn implies a higher fidelity of the on-source reconstruction. Moreover, the choice of image reconstruction algorithm also affects the correctness of the on-source brightness distribution.

==============
Installation
Expand Down
Loading

0 comments on commit 93c108b

Please sign in to comment.