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def test_sky_frac(self): | |
frac = go.sky_frac(-90, 90, 0, 360) | |
self.assertTrue(frac > 0.99999999999) | |
frac = go.sky_frac(0, 90, 0, 360) | |
self.assertTrue(0.49 < frac < 0.51) | |
frac = go.sky_frac(0, 90, 0, 90) | |
self.assertTrue(0.124 < frac < 0.126) |
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import math | |
central_freq = 1400 #1374 | |
bw = 350 #288 | |
si = -1.4 | |
dist = 2.682277221706293 | |
lum_bol = 8e44 | |
z = 0.75 | |
f_high = 10e9 | |
f_low = 10e6 |
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import glob | |
import os | |
import subprocess | |
import sys | |
assert sys.version_info >= (3, 0), 'Please run with Python3' | |
def loc(f): | |
"""Returns full location path to file""" |
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def lb_to_radec(l, b): | |
""" | |
Convert galactic coordinates to RA, Dec | |
Formulas from 'An Introduction to Modern Astrophysics (2nd Edition)' by | |
Bradley W. Carroll, Dale A. Ostlie. | |
Args: | |
l (float): Galactic longitude [fractional degrees] | |
b (float): Galactic latitude [fractional degrees] |
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