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d g k sŸ t ‚ | j d t ƒ } | d
j d t | ƒ ƒ d d d d g k sä t ‚ t j j
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| j ƒ d j d t | ƒ d | ƒ d d d d d g k sMt ‚ | | g ƒ } | j ƒ } | d d d d d g k s‰t ‚ d S($ s1 Test printing with 'fake' multidimensional columni i
R i i i i2 s col0 [1,1] col1 [1,1] col2 [1,1]s ---------- ---------- ----------s 1 3 5s 10 30 50R
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g k sX t ‚ d S( s Include the unit header rowR: i R; i( R= s& col0 col1 ... col19 s& km2 ... kg s / m2s& ------------ ----------- ... ---------s& 0.000000e+00 1.000000 ... 19.0s& ... ... ... ...s& 1.960000e+03 1961.000000 ... 1979.0s& 1.980000e+03 1981.000000 ... 1999.0s Length = 100 rowsN( R- R) R R R ( R R R ( ( s> lib/python2.7/site-packages/astropy/table/tests/test_pprint.pyt test_format3® s
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test_clip1Ö s
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of 10
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k si t ‚ d | d _ t | d ƒ d k s’ t ‚ d
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| d _ t | d ƒ d k s´ t ‚ d | d _ t | d ƒ d k sÝ t ‚ d | d _ t | d ƒ d k st ‚ d | d _ t | d ƒ d k s/t ‚ d S( Ni i i i i RL RM RN R s a
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c C s¨ t d d d g d d d g g d d d
t ƒ} t t t g | d _ d t f d „ ƒ Y} | ƒ | d _ t | d ƒ d
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k s¤ t ‚ d S( Ng ð?g @g @i i i RL RM RN R R c B s e Z d „ Z RS( c S s t | d ƒ S( Ng @( R! ( R RW ( ( s> lib/python2.7/site-packages/astropy/table/tests/test_pprint.pyRZ å s ( R R RZ ( ( ( s> lib/python2.7/site-packages/astropy/table/tests/test_pprint.pyR ä s s a
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3.0 .. --
30.0 .. --( i i ( i i ( R
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but has to be converted to a python float.
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Test for #1346 and #4944. Make sure a bytestring (dtype=S) in Python 3
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$*c C s4 t j d d g ƒ } t | ƒ j d ƒ s0 t ‚ d S( sh Regression test for #2213, making sure a nameless column can be printed
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d d g k s{ t ‚ | j d t d
d ƒ } | d j d t | ƒ ƒ d d
d d g k sÆ t ‚ | j d t d
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