ICRS¶
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class
astropy.coordinates.ICRS(*args, **kwargs)[source] [edit on github]¶ Bases:
astropy.coordinates.BaseCoordinateFrameA coordinate or frame in the ICRS system.
If you’re looking for “J2000” coordinates, and aren’t sure if you want to use this or
FK5, you probably want to use ICRS. It’s more well-defined as a catalog coordinate and is an inertial system, and is very close (within tens of milliarcseconds) to J2000 equatorial.For more background on the ICRS and related coordinate transformations, see the references provided in the See Also section of the documentation.
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).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_representationframe_specific_representation_infonameAttributes Documentation
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default_representation¶
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frame_specific_representation_info¶
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name= 'icrs'¶
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