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 |