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LSST Applications g013ef56533+b8d55c8942,g083dd6704c+a047e97985,g199a45376c+0ba108daf9,g1fd858c14a+7a3b874d60,g210f2d0738+7416ca6900,g262e1987ae+1d557ba9a3,g29ae962dfc+519d34895e,g2cef7863aa+aef1011c0b,g30d7c61c20+36d16ea71a,g35bb328faa+8c5ae1fdc5,g3fd5ace14f+cb326ad149,g47891489e3+f459a6810c,g53246c7159+8c5ae1fdc5,g54cd7ddccb+890c8e1e5d,g5a60e81ecd+6240c63dbc,g64539dfbff+7416ca6900,g67b6fd64d1+f459a6810c,g6ebf1fc0d4+8c5ae1fdc5,g74acd417e5+0bae3c876a,g786e29fd12+668abc6043,g87389fa792+8856018cbb,g89139ef638+f459a6810c,g8d7436a09f+dee7680868,g8ea07a8fe4+81eaaadc04,g90f42f885a+34c0557caf,g97be763408+14b8164b5b,g98a1a72a9c+8389601a76,g98df359435+fff771c62d,gb8cb2b794d+6728931916,gbf99507273+8c5ae1fdc5,gc2a301910b+7416ca6900,gca7fc764a6+f459a6810c,gd7ef33dd92+f459a6810c,gdab6d2f7ff+0bae3c876a,ge410e46f29+f459a6810c,ge41e95a9f2+7416ca6900,geaed405ab2+e3b4b2a692,gf9a733ac38+8c5ae1fdc5,w.2025.43
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.