| Conditions | 1 |
| Total Lines | 10 |
| Lines | 0 |
| Ratio | 0 % |
| Changes | 2 | ||
| Bugs | 0 | Features | 0 |
| 1 | "Some utility methods" |
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| 49 | def galactic_to_galactocentric(l, b, distance, xyz_sun=[0, 8.5, 0]): |
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| 50 | slc = sin(l/180*pi) |
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| 51 | clc = cos(l/180*pi) |
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| 52 | sbc = sin(b/180*pi) |
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| 53 | cbc = cos(b/180*pi) |
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| 54 | rgalc = distance*cbc |
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| 55 | xc = xyz_sun[0] + rgalc*slc |
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| 56 | yc = xyz_sun[1] - rgalc*clc |
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| 57 | zc = xyz_sun[-1] + distance*sbc |
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| 58 | return np.array([xc, yc, zc]) |
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| 59 |