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authorAaron LI <aly@aaronly.me>2017-08-29 00:29:45 +0800
committerAaron LI <aly@aaronly.me>2017-08-29 00:29:45 +0800
commitc1c66c9f89b070645b70864b6b26db6fff41da01 (patch)
treed0d4414a3e11d96411bf62ed958a397434ba4a4b /fg21sim/utils
parent15ecc6b6df70efc905a4b360f6bd2e964aa13da8 (diff)
downloadfg21sim-c1c66c9f89b070645b70864b6b26db6fff41da01.tar.bz2
convert.py: do not use Numba JIT
Diffstat (limited to 'fg21sim/utils')
-rw-r--r--fg21sim/utils/convert.py22
1 files changed, 8 insertions, 14 deletions
diff --git a/fg21sim/utils/convert.py b/fg21sim/utils/convert.py
index d238339..9eb9061 100644
--- a/fg21sim/utils/convert.py
+++ b/fg21sim/utils/convert.py
@@ -5,9 +5,9 @@
Utilities for conversion among common astronomical quantities.
"""
-import numpy as np
import astropy.units as au
-import numba
+
+from .units import (UnitConversions as AUC, Constants as AC)
def Fnu_to_Tb(Fnu, omega, freq):
@@ -67,15 +67,12 @@ def Sb_to_Tb(Sb, freq):
return Fnu_to_Tb(Fnu, omega, freq)
-@numba.jit(nopython=True)
def Sb_to_Tb_fast(Sb, freq):
"""
Convert surface brightness to brightness temperature, using the
Rayleigh-Jeans law, in the Rayleigh-Jeans limit.
- This function does the calculations explicitly, and does NOT rely
- on the `astropy.units`, therefore it is much faster. However, the
- input parameters must be in right units.
+ Avoid using `astropy.units` to optimize the speed.
Tb = Sb * c^2 / (2 * k_B * nu^2)
@@ -100,22 +97,19 @@ def Sb_to_Tb_fast(Sb, freq):
Unit: [K]
"""
# NOTE: [rad] & [sr] are dimensionless
- arcsec2 = (np.deg2rad(1) / 3600) ** 2 # [sr]
- c = 29979245800.0 # speed of light, [cm/s]
- k_B = 1.3806488e-16 # Boltzmann constant, [erg/K]
- coef = 1e-35 # take care the unit conversions
- Tb = coef * (Sb * c*c) / (2 * k_B * freq*freq * arcsec2) # [K]
+ arcsec2 = AUC.arcsec2rad ** 2 # [sr]
+ Sb /= arcsec2 # [Jy/arcsec^2] -> [Jy/sr]
+ coef = 1e-35 # unit conversion coefficient
+ Tb = coef * (Sb * AC.c**2) / (2*AC.k_B * freq**2) # [K]
return Tb
-@numba.jit(nopython=True)
def Fnu_to_Tb_fast(Fnu, omega, freq):
"""
Convert flux density to brightness temperature, using the
Rayleigh-Jeans law, in the Rayleigh-Jeans limit.
- This function does NOT invoke the `astropy.units`, therefore it is
- much faster.
+ Avoid using `astropy.units` to optimize the speed.
Parameters
----------