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LSST Applications g00d0e8bbd7+edbf708997,g03191d30f7+6b31559d11,g118115db7c+ac820e85d2,g199a45376c+5137f08352,g1fd858c14a+90100aa1a7,g262e1987ae+64df5f6984,g29ae962dfc+1eb4aece83,g2cef7863aa+73c82f25e4,g3541666cd7+1e37cdad5c,g35bb328faa+edbf708997,g3fd5ace14f+fb4e2866cc,g47891489e3+19fcc35de2,g53246c7159+edbf708997,g5b326b94bb+d622351b67,g64539dfbff+dfe1dff262,g67b6fd64d1+19fcc35de2,g74acd417e5+cfdc02aca8,g786e29fd12+af89c03590,g7aefaa3e3d+dc1a598170,g87389fa792+a4172ec7da,g88cb488625+60ba2c3075,g89139ef638+19fcc35de2,g8d4809ba88+dfe1dff262,g8d7436a09f+db94b797be,g8ea07a8fe4+79658f16ab,g90f42f885a+6577634e1f,g9722cb1a7f+d8f85438e7,g98df359435+7fdd888faa,ga2180abaac+edbf708997,ga9e74d7ce9+128cc68277,gbf99507273+edbf708997,gca7fc764a6+19fcc35de2,gd7ef33dd92+19fcc35de2,gdab6d2f7ff+cfdc02aca8,gdbb4c4dda9+dfe1dff262,ge410e46f29+19fcc35de2,ge41e95a9f2+dfe1dff262,geaed405ab2+062dfc8cdc,w.2025.46
LSST Data Management Base Package
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Proper motion data for a reference star or fitted star. More...
#include <ProperMotion.h>
Public Member Functions | |
| ProperMotion (double ra, double dec, double raErr, double decErr, double raDecCov=0) | |
| ProperMotion (ProperMotion const &)=default | |
| ProperMotion (ProperMotion &&)=default | |
| ProperMotion & | operator= (ProperMotion const &)=default |
| ProperMotion & | operator= (ProperMotion &&)=default |
| ~ProperMotion ()=default | |
| Point | apply (const Point &star, double timeDeltaYears) const |
| Apply proper motion correction to the input star, returning a star with PM-corrected coordinates. | |
Friends | |
| std::ostream & | operator<< (std::ostream &stream, ProperMotion const &pm) |
Proper motion data for a reference star or fitted star.
Whether to just use these values or fit them is determined by the RefStar and FittedStar they belong to.
Units are radians/year Note: RA proper motion is pm_ra*cos(dec)
Definition at line 45 of file ProperMotion.h.
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Definition at line 47 of file ProperMotion.h.
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Apply proper motion correction to the input star, returning a star with PM-corrected coordinates.
NOTE: This method does not apply to the coordinate errors (Point does not include uncertainty).
| star | The star to correct for this proper motion. |
| timeDeltaYears | The difference in time from the correction epoch to correct for, in years. |
Definition at line 34 of file ProperMotion.cc.
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Definition at line 46 of file ProperMotion.cc.