LSST Applications
21.0.0-172-gfb10e10a+18fedfabac,22.0.0+297cba6710,22.0.0+80564b0ff1,22.0.0+8d77f4f51a,22.0.0+a28f4c53b1,22.0.0+dcf3732eb2,22.0.1-1-g7d6de66+2a20fdde0d,22.0.1-1-g8e32f31+297cba6710,22.0.1-1-geca5380+7fa3b7d9b6,22.0.1-12-g44dc1dc+2a20fdde0d,22.0.1-15-g6a90155+515f58c32b,22.0.1-16-g9282f48+790f5f2caa,22.0.1-2-g92698f7+dcf3732eb2,22.0.1-2-ga9b0f51+7fa3b7d9b6,22.0.1-2-gd1925c9+bf4f0e694f,22.0.1-24-g1ad7a390+a9625a72a8,22.0.1-25-g5bf6245+3ad8ecd50b,22.0.1-25-gb120d7b+8b5510f75f,22.0.1-27-g97737f7+2a20fdde0d,22.0.1-32-gf62ce7b1+aa4237961e,22.0.1-4-g0b3f228+2a20fdde0d,22.0.1-4-g243d05b+871c1b8305,22.0.1-4-g3a563be+32dcf1063f,22.0.1-4-g44f2e3d+9e4ab0f4fa,22.0.1-42-gca6935d93+ba5e5ca3eb,22.0.1-5-g15c806e+85460ae5f3,22.0.1-5-g58711c4+611d128589,22.0.1-5-g75bb458+99c117b92f,22.0.1-6-g1c63a23+7fa3b7d9b6,22.0.1-6-g50866e6+84ff5a128b,22.0.1-6-g8d3140d+720564cf76,22.0.1-6-gd805d02+cc5644f571,22.0.1-8-ge5750ce+85460ae5f3,master-g6e05de7fdc+babf819c66,master-g99da0e417a+8d77f4f51a,w.2021.48
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 (Point star, double timeDeltaYears) const |
Apply proper motion correction to the input star, returning a star with PM-corrected coordinates. More... | |
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 44 of file ProperMotion.cc.