tpstv¶
- erfa.tpstv(xi, eta, v0)[source]¶
In the tangent plane projection, given the star’s rectangular coordinates and the direction cosines of the tangent point, solve for the direction cosines of the star.
- Parameters:
- xidouble array
- etadouble array
- v0double array
- Returns:
- vdouble array
Notes
Wraps ERFA function
eraTpstv
. The ERFA documentation is:- - - - - - - - - e r a T p s t v - - - - - - - - - In the tangent plane projection, given the star's rectangular coordinates and the direction cosines of the tangent point, solve for the direction cosines of the star. Given: xi,eta double rectangular coordinates of star image (Note 2) v0 double[3] tangent point's direction cosines Returned: v double[3] star's direction cosines 1) The tangent plane projection is also called the "gnomonic projection" and the "central projection". 2) The eta axis points due north in the adopted coordinate system. If the direction cosines represent observed (RA,Dec), the tangent plane coordinates (xi,eta) are conventionally called the "standard coordinates". If the direction cosines are with respect to a right-handed triad, (xi,eta) are also right-handed. The units of (xi,eta) are, effectively, radians at the tangent point. 3) The method used is to complete the star vector in the (xi,eta) based triad and normalize it, then rotate the triad to put the tangent point at the pole with the x-axis aligned to zero longitude. Writing (a0,b0) for the celestial spherical coordinates of the tangent point, the sequence of rotations is (b-pi/2) around the x-axis followed by (-a-pi/2) around the z-axis. 4) If vector v0 is not of unit length, the returned vector v will be wrong. 5) If vector v0 points at a pole, the returned vector v will be based on the arbitrary assumption that the longitude coordinate of the tangent point is zero. 6) This function is a member of the following set: spherical vector solve for eraTpxes eraTpxev xi,eta eraTpsts > eraTpstv < star eraTpors eraTporv origin References: Calabretta M.R. & Greisen, E.W., 2002, "Representations of celestial coordinates in FITS", Astron.Astrophys. 395, 1077 Green, R.M., "Spherical Astronomy", Cambridge University Press, 1987, Chapter 13. This revision: 2018 January 2 Copyright (C) 2013-2023, NumFOCUS Foundation. Derived, with permission, from the SOFA library. See notes at end of file.