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| author | Aaron LI <aaronly.me@outlook.com> | 2016-10-17 13:30:09 +0800 |
|---|---|---|
| committer | Aaron LI <aaronly.me@outlook.com> | 2016-10-17 13:30:09 +0800 |
| commit | 3a43ed26818eef66340bf35a2c678a96be3a2686 (patch) | |
| tree | 6a9eaf776313c223ffa12df5bd230ab48a6aff0a /fg21sim/galactic | |
| parent | a1ccf670ab733c75ff04ece33949a9dd8fb7e5f6 (diff) | |
| download | fg21sim-3a43ed26818eef66340bf35a2c678a96be3a2686.tar.bz2 | |
Fix the reStructuredText citation syntax
Diffstat (limited to 'fg21sim/galactic')
| -rw-r--r-- | fg21sim/galactic/freefree.py | 6 |
1 files changed, 3 insertions, 3 deletions
diff --git a/fg21sim/galactic/freefree.py b/fg21sim/galactic/freefree.py index fa6238a..352621b 100644 --- a/fg21sim/galactic/freefree.py +++ b/fg21sim/galactic/freefree.py @@ -24,9 +24,9 @@ class FreeFree: """ Simulate the diffuse Galactic free-free emission. - The [Dickinson2003] method is followed to derive the free-free template. - The H\alpha survey map [Finkbeiner2003] is first corrected for dust - absorption using the infrared 100-\mu{}m dust map [Schlegel1998], + The [Dickinson2003]_ method is followed to derive the free-free template. + The H\alpha survey map [Finkbeiner2003]_ is first corrected for dust + absorption using the infrared 100-\mu{}m dust map [Schlegel1998]_, and then converted to free-free emission map (brightness temperature). Parameters |