FK4¶
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class
astropy.coordinates.FK4(*args, **kwargs)[source] [edit on github]¶ Bases:
astropy.coordinates.BaseCoordinateFrameA coordinate or frame in the FK4 system.
Note that this is a barycentric version of FK4 - that is, the origin for this frame is the Solar System Barycenter, not the Earth geocenter.
Parameters: representation :
BaseRepresentationor NoneA representation object or None to have no data (or use the other keywords)
ra :
Angle, optional, must be keywordThe RA for this object (
decmust also be given andrepresentationmust be None).dec :
Angle, optional, must be keywordThe Declination for this object (
ramust also be given andrepresentationmust be None).distance :
Quantity, optional, must be keywordThe Distance for this object along the line-of-sight. (
representationmust be None).equinox : astropy.time.Time, optional, must be keyword
The equinox of this frame.
obstime : astropy.time.Time, optional, must be keyword
The time this frame was observed. If None, will be the same as
equinox.copy : bool, optional
If
True(default), make copies of the input coordinate arrays. Can only be passed in as a keyword argument.Attributes Summary
default_representationequinoxframe_attributesframe_specific_representation_infonameobstimeAttributes Documentation
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default_representation¶
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equinox= <Time object: scale='tai' format='byear_str' value=B1950.000>¶
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frame_attributes= OrderedDict([('equinox', <astropy.coordinates.baseframe.TimeFrameAttribute object>), ('obstime', <astropy.coordinates.baseframe.TimeFrameAttribute object>)])¶
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frame_specific_representation_info¶
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name= 'fk4'¶
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obstime= None¶
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