[AstroPy] Proper Motions in astropy.coordinates
Russell Owen
rowen at uw.edu
Tue May 12 12:47:48 EDT 2015
It is not a hard computation, but I suggest working in spherical coordinates or using spherical trig for best results.
If you want a ready made solution, I wrote two that might be of interest:
- RO.Astro performs astronomical coordinate conversions, and handles proper motion, parallax and radial velocity. It is part of the RO package, which is pure python <https://pypi.python.org/pypi/RO>. pip install works.
- CoordConv is much faster (C++ with Python wrappers), but has many dependencies, including slalib, so it takes more work to install. <https://github.com/r-owen/coordConv>. I wrote this package for the Apache Point Observatory telescope control system.
Both packages also include a spherical trig solver and convenient conversion between spherical and cartesian coordinates.
-- Russell
On May 11, 2015, at 8:49 PM, gonghang.naoc <ghang.naoc at gmail.com> wrote:
> I have a similar question. Is there any other package about PM calculation?
> Thank you.
> Hang
>
> On Sun, May 10, 2015 at 5:24 PM, Josh Walawender <jmwalawender at gmail.com> wrote:
> Hi all,
>
> Is there a method do calculations of proper motions in astropy.coordinates? It looks to me as if the SkyCoord has obstime and equinox properties but how would I transform from a coordinate defined for a particular obstime and equinox to another obstime (e.g. for the same equinox)?
>
> I just did this calculation in a brute force way (multiplying the proper motion in mas/yr by number of years and adding that angle to the ra and dec independently), but it felt like there should be a better way.
>
> thanks!
> Josh
>
>
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