[AstroPy] pywcs problem on Linux
OKUMURA, Akira
oxon at ceres.phys.s.u-tokyo.ac.jp
Wed May 6 10:07:27 EDT 2009
Hello Mike and Thomas,
I modified test.py to use the second or third argument, but still I
get a seg fault after calling wcs_pix2sky. And wcs.wcs.fix() always
cause a seg fault. I have uploaded my sample FITS and modified test.py.
http://www-utheal.phys.s.u-tokyo.ac.jp/~oxon/model_total_ICHII_bin00.fits
http://www-utheal.phys.s.u-tokyo.ac.jp/~oxon/test.py
Could you investigate it?
Regards,
OKUMURA, Akira oxon at ceres.phys.s.u-tokyo.ac.jp
Department of Physics, The University of Tokyo
7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033
TEL/FAX +81 3-5841-4173/4059
Skype : okumura.akira
On 2009/05/06, at 22:30, Michael Droettboom wrote:
> It looks as if your new traceback is related to an API change -- all
> of the transformation functions now require an "offset" argument,
> which should be 0 for C/Numpy indexing or 1 for Fortran/FITS indexing.
>
> If that change doesn't work for you, can you send me a FITS file and
> script to reproduce this off list? I'll see if I can reproduce what
> you're seeing here.
>
> Mike
>
>
>
> OKUMURA, Akira wrote:
>> Hello Nadia,
>>
>> Thank you for your reply. I didn't know that new version has been
>> released recently. I installed pywcs-1.4-4.3.tar.gz and tried
>> test.py in the package. But I got errors again.
>>
>> 1)
>> $ ./test.py .
>> = = =
>> =
>> =
>> =
>> =====================================================================
>> ./cmap.fits
>> zsh: segmentation fault ./test.py .
>>
>> the line wcs.wcs.fix() causes the seg fault.
>>
>> 2) comment out wcs.wcs.fix()
>> $ ./test.py .
>> = = =
>> =
>> =
>> =
>> =====================================================================
>> ./cmap.fits
>> Traceback (most recent call last):
>> File "./test.py", line 82, in <module>
>> run_directory(directory)
>> File "./test.py", line 74, in run_directory
>> test_file(filepath)
>> File "./test.py", line 38, in test_file
>> world = wcs.wcs_pix2sky(data3)
>> File "/usr/local/lib/python2.5/site-packages/pywcs/pywcs.py",
>> line 419, in wcs_pix2sky
>> *args, **kwargs)
>> File "/usr/local/lib/python2.5/site-packages/pywcs/pywcs.py",
>> line 378, in _array_converter
>> raise TypeError("Expected 2 or 3 arguments, %d given" %
>> len(args))
>> TypeError: Expected 2 or 3 arguments, 1 given
>>
>> I tried several FITS files but I got the same errors. Do you have
>> any idea?
>>
>> Regards,
>>
>> OKUMURA, Akira oxon at ceres.phys.s.u-tokyo.ac.jp
>> Department of Physics, The University of Tokyo
>> 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033
>> TEL/FAX +81 3-5841-4173/4059
>> Skype : okumura.akira
>>
>> On 2009/05/06, at 20:47, Nadezhda Dencheva wrote:
>>
>>
>>> Hi,
>>>
>>> You are running an older version of pywcs.
>>> I believe an upgrade to the latest release will fix this.
>>>
>>>
>>> Nadia Dencheva
>>>
>>> ---- Original message ----
>>>
>>>> Date: Wed, 6 May 2009 15:30:23 +0900
>>>> From: astropy-bounces at scipy.org (on behalf of "OKUMURA, Akira" <oxon at ceres.phys.s.u-tokyo.ac.jp
>>>>> )
>>>>>
>>>> Subject: [AstroPy] pywcs problem on Linux
>>>> To: astropy at scipy.org
>>>>
>>>> Hello all,
>>>>
>>>> I have installed pywcs in two environments.
>>>> (1) Scientific Linux 4.7 (64 bit)
>>>> + Python 2.5.4 (r254:67916, May 6 2009, 07:09:17)
>>>> + GCC 3.4.6 20060404 (Red Hat 3.4.6-10)] on linux2
>>>> + pyfits-1.3
>>>> + pywcs-1.3a1-4.3
>>>> (2) Red Hat Enterprise Linux 4 (32 bit).
>>>> + Python 2.5.1 (r251:54863, Aug 24 2007, 16:22:50)
>>>> + GCC 3.4.3 (TWW)] on linux2
>>>> + pywcs-1.3a1-4.3
>>>> + pyfits-2.1.1
>>>>
>>>> But I got following errors even though it runs properly on Mac OS X
>>>> 10.5.
>>>> === Error on (1) ===
>>>>
>>>>>>> hdulist = pyfits.open("cmap.fits")
>>>>>>> wcs = pywcs.WCS(hdulist[0].header)
>>>>>>>
>>>> zsh: segmentation fault python
>>>>
>>>> === Error on (2) ===
>>>>
>>>>>>> hdulist = pyfits.open("cmap.fits")
>>>>>>> wcs = pywcs.WCS(hdulist[0].header)
>>>>>>>
>>>> Traceback (most recent call last):
>>>> File "<stdin>", line 1, in <module>
>>>> File "/u/gl/oxon/tmp/lib/python2.5/site-packages/pywcs/pywcs.py",
>>>> line 155, in __init__
>>>> self.footprint = self._calcFootprint(header)
>>>> File "/u/gl/oxon/tmp/lib/python2.5/site-packages/pywcs/pywcs.py",
>>>> line 181, in _calcFootprint
>>>> return self.all_pix2sky(corners)
>>>> File "/u/gl/oxon/tmp/lib/python2.5/site-packages/pywcs/pywcs.py",
>>>> line 307, in all_pix2sky
>>>> return self._array_converter(self._all_pix2sky, *args, **kwargs)
>>>> File "/u/gl/oxon/tmp/lib/python2.5/site-packages/pywcs/pywcs.py",
>>>> line 294, in _array_converter
>>>> return func(args[0], **kwargs)
>>>> SystemError: Python/getargs.c:1246: bad argument to internal
>>>> function
>>>>
>>>> Is there any tips on running pywcs with Linux ?
>>>>
>>>> The FITS is as follows.
>>>>
>>>>
>>>>>>> print hdulist[0].header
>>>>>>>
>>>> SIMPLE = T / File conforms to NOST standard
>>>> BITPIX = 32 / Bits per pixel
>>>> NAXIS = 2 / No data is associated with this
>>>> header
>>>> NAXIS1 = 160 / Length of data axis 1
>>>> NAXIS2 = 160 / Length of data axis 2
>>>> EXTEND = T / Extensions may be present
>>>> COMMENT FITS (Flexible Image Transport System) format is
>>>> defined in
>>>> 'Astronomy
>>>> COMMENT and Astrophysics', volume 376, page 359; bibcode:
>>>> 2001A&A...
>>>> 376..359H
>>>> CTYPE1 = 'GLON-AIT' / RA---%%%, %%% represents the
>>>> projection method
>>>> CRPIX1 = 80.5 / Reference pixel
>>>> CRVAL1 = 211. / RA at the reference pixel
>>>> CDELT1 = -0.25 / X-axis incr per pixel of physical
>>>> coord at posi
>>>> CUNIT1 = 'deg ' / Physical unit of X-axis
>>>> CTYPE2 = 'GLAT-AIT' / DEC---%%%, %%% represents the
>>>> projection method
>>>> CRPIX2 = 80.5 / Reference pixel
>>>> CRVAL2 = -17. / DEC at the reference pixel
>>>> CDELT2 = 0.25 / Y-axis incr per pixel of physical
>>>> coord at posi
>>>> CUNIT2 = 'deg ' / Physical unit of Y-axis
>>>> CROTA2 = 0. / Image rotation (deg)
>>>> DATE = '2009-04-01T15:34:22' / file creation date (YYYY-MM-
>>>> DDThh:mm:ss U
>>>> FILENAME= 'cmap.fits' /
>>>> TELESCOP= 'GLAST ' / name of telescope generating data
>>>> INSTRUME= 'LAT ' / name of instrument generating
>>>> data
>>>> DATE-OBS= '2009-03-11T21:33:18.000' / start date and time of the
>>>> observation (U
>>>> DATE-END= '2009-03-17T16:26:38.000' / end date and time of the
>>>> observation (UTC
>>>> NDSKEYS = 5
>>>> EQUINOX = 2000. / Equinox of RA & DEC specifications
>>>> OBSERVER= 'Peter Michelson' / GLAST/LAT PI
>>>> CREATOR = 'gtbin ' / Software and version creating file
>>>> HISTORY LatCountMapTemplate,v 1.3 2005/04/05
>>>> 21:06:39 peachey
>>>> HISTORY Exp
>>>> CHECKSUM= 'c8JZf8JXc8JXc8JX' / HDU checksum updated
>>>> 2009-04-01T06:34:22
>>>> DATASUM = '182648 ' / data unit checksum updated
>>>> 2009-04-01T06:34:22
>>>> DSTYP1 = 'TIME '
>>>> DSUNI1 = 's '
>>>> DSVAL1 = 'TABLE '
>>>> DSREF1 = ':GTI '
>>>> DSTYP2 = 'POS(RA,DEC)'
>>>> DSUNI2 = 'deg '
>>>> DSVAL2 = 'CIRCLE(86.81257852,-6.005536809,20)'
>>>> DSTYP3 = 'CTBCLASSLEVEL'
>>>> DSUNI3 = 'dimensionless'
>>>> DSVAL3 = '3: '
>>>> DSTYP4 = 'ENERGY '
>>>> DSUNI4 = 'MeV '
>>>> DSVAL4 = '200:20000'
>>>> DSTYP5 = 'ZENITH_ANGLE'
>>>> DSUNI5 = 'deg '
>>>> DSVAL5 = '0:100 '
>>>>
>>>>
>>>> Regards,
>>>>
>>>> OKUMURA, Akira oxon at ceres.phys.s.u-tokyo.ac.jp
>>>> Department of Physics, The University of Tokyo
>>>> 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033
>>>> TEL/FAX +81 3-5841-4173/4059
>>>> Skype : okumura.akira
>>>>
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>>
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>
> --
> Michael Droettboom
> Science Software Branch
> Operations and Engineering Division
> Space Telescope Science Institute
> Operated by AURA for NASA
>
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