Package coords
Package: AstroLib Coords
Purpose
This package aims to provide much of the IDL "astron"
functionality that pertains to coordinate manipulations in an OO
framework. Our target user is a typical astronomer who needs to analyze
data, work with catalogs, prepare observing proposals, and prepare for
observing runs.
The initial version will provide simple functionality for working
with positions in the same reference frame, without having to worry
about units.
Dependencies
numarray
pytpm -- a Python wrapper for the TPM library graciously contributed
by Jeff Percival
Example
>>> import coords as C
>>> print C.__version__
0.3
>>>
>>> ob=C.Position('12:34:45.34 -23:42:32.6')
>>> ob.hmsdms()
'12:34:45.340 -23:42:32.600'
>>> ob.dd()
(188.68891666666667, -23.709055555555555)
>>> ob.rad()
(3.2932428578545374, -0.41380108198269777)
>>>
>>> p1=C.Position("01:23:45.300 +65:43:31.240")
>>> p2=C.Position("01:23:45.62 +65:43:31.20")
>>> p1.angsep(p2)
0.000548 degrees
>>> delta=p1.angsep(p2)
>>> delta.arcsec()
1.973739377865491
>>> p1.within(p2,3.0,units='arcsec')
True
>>> epsilon=C.AngSep(5.0)
>>> epsilon
5.000000 arcsec
>>> delta > epsilon
False
>>>
>>> d=C.AstroDate('1997.3')
>>> d.year
1997.3
>>> d.jd
2450558.8250000002
>>> d.mjd
50558.325000000186
>>> d2=C.AstroDate('MJD50658.25')
>>> d2.year
1997.5735797399041
>>> d2 < d
False
>>>
>>> ob.j2000()
(188.68891666666667, -23.709055555555555)
>>> ob.b1950()
(188.03056480942405, -23.433637283819877)
>>> ob.galactic()
(298.01638938748795, 39.003358150874568)
>>> ob.ecliptic(timetag=C.AstroDate('J2000'))
(197.5848634558852, -18.293964120804738)
>>> p3=C.Position("01:23:45 -65:43:21.4",equinox='J2000')
>>> p4=C.Position("01:23:45 -65:43:21.4",equinox='B1950')
>>> p3.j2000()
(20.9375, -65.722611111111107)
>>> p4.j2000()
(21.356870704681981, -65.462921080444147)
>>> p3.angsep(p4)
0.312199 degrees
>>> p5=C.Position((0.0,0.0),system='galactic')
>>> p5.j2000()
(266.40499571858879, -28.936169261309555)
>>>
>>> polaris=C.Position("02:31:49.08 +89:15:50.8")
>>> polaris.dd()
(37.954500000000003, 89.264111111111106)
>>> polaris.hmsdms()
'02:31:49.080 +89:15:50.800'
>>> print polaris.details()
System: celestial
Equinox: j2000
>>>
>>> ob=C.Position((52.9860209, -27.7510006))
>>> ob.hmsdms()
'03:31:56.645 -27:45:03.602'
>>> ob.dd()
(52.9860209, -27.751000600000001)
>>>
>>>
>>> C.Position("12:34:45.4 -22:21:45.4").dd()
(188.68916666666667, -22.362611111111111)
TPM Citation
Investigators using this software for their research are requested
to explicitly acknowledge "use of the TPM software library, by
Jeffrey W. Percival" in any appropriate publications.
Version: '0.3 (2007-2-12)'
Author: Vicki Laidler
See Also: http://www.scipy.org/AstroLibCoordsHome
| Submodules |
-
astrodate: For more information about astronomical date specifications, consult a
reference source such as this page provided by
the US Naval Observatory.
-
pytpm
-
pytpm_wrapper: This routine wraps the pytpm.blackbox routine in order to apply
the longitude convention preferred in coords.
|
| Modules |
-
position: Position object to manage coordinate transformations
-
angsep: Angular separation between two Positions.
|