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authorAaron LI <aly@aaronly.me>2018-01-01 23:27:48 +0800
committerAaron LI <aly@aaronly.me>2018-01-01 23:27:48 +0800
commit55483e5408ce122cf43059f53409c19ca7adeeb9 (patch)
tree34b447daa09bf46362d91aabc3495cfd0cc038d7 /fg21sim/extragalactic/clusters/halo.py
parent3d8df30a95f3b74de20c5982445c6bb225b34e42 (diff)
downloadfg21sim-55483e5408ce122cf43059f53409c19ca7adeeb9.tar.bz2
Improve descriptions and minor cleanups
Diffstat (limited to 'fg21sim/extragalactic/clusters/halo.py')
-rw-r--r--fg21sim/extragalactic/clusters/halo.py4
1 files changed, 1 insertions, 3 deletions
diff --git a/fg21sim/extragalactic/clusters/halo.py b/fg21sim/extragalactic/clusters/halo.py
index 1da89b3..cd6b9bc 100644
--- a/fg21sim/extragalactic/clusters/halo.py
+++ b/fg21sim/extragalactic/clusters/halo.py
@@ -656,7 +656,7 @@ class RadioHalo:
omega = np.pi * self.angular_radius**2 # [arcsec^2]
if pixelsize and (omega < pixelsize**2):
omega = pixelsize ** 2 # [arcsec^2]
- logger.warning("Object size < 1 pixel; force to be 1 pixel!")
+ logger.warning("Halo size < 1 pixel; force to be 1 pixel!")
Tb = Fnu_to_Tb(flux, omega, frequencies) # [K]
return Tb
@@ -801,8 +801,6 @@ class RadioHalo:
So we assume that the main cluster grows linearly in time from
(M_main, z_merger) to (M_obs, z_obs).
- TODO: consider the full merging history.
-
Parameters
----------
t : float