ó šßÈ[c@`sdZddlmZmZmZddlZddlmZddlm Z dej fd „ƒYZ d ej fd „ƒYZ d ejfd „ƒYZdS(s¿ sextractor.py: Classes to read SExtractor table format Built on daophot.py: :Copyright: Smithsonian Astrophysical Observatory (2011) :Author: Tom Aldcroft (aldcroft@head.cfa.harvard.edu) i(tabsolute_importtdivisiontprint_functionNi(tcorei(trangetSExtractorHeadercB`seZdZdZd„ZRS(s3Read the header from a file produced by SExtractor.s^\s*#\s*\S\D.*cC`s†i}tjdtjƒ}d}x”|D]Œ}|jdƒsG|}Pq(|j|ƒ}|r(t|jdƒƒ}|jdƒ}|jdƒ} |jdƒ} || | f|| [0-9]+)\s+ # number of the column in table (?P [-\w]+) # name of the column (?:\s+(?P \w .+) # column description, match any character until... (?:(?.+)\])?.* # match units in brackets t#t colnumbertcolnametcoldescrtcolunitiÿÿÿÿiis_{}is*No column names found in SExtractor headertnameN(NNN(tretcompiletVERBOSEtNonet startswithtsearchtinttgrouptsortedtlentsplittappendRtformattnamesRtInconsistentTableErrortcolstColumnt descriptiontunit(tselftlinestcolumnst re_name_deftdatalinetlinetmatchRRR R t colnumberst n_data_colstprevious_columntntct column_namet column_descrt column_unittcol((s:lib/python2.7/site-packages/astropy/io/ascii/sextractor.pytget_colssV           (t__name__t __module__t__doc__tcommentR/(((s:lib/python2.7/site-packages/astropy/io/ascii/sextractor.pyRstSExtractorDatacB`seZdZdZdZRS(it s\s*#(R0R1t start_linet delimiterR3(((s:lib/python2.7/site-packages/astropy/io/ascii/sextractor.pyR4est SExtractorcB`sGeZdZdZeZdZeZe Z e j Z d„Zd„ZRS(sªRead a SExtractor file. SExtractor is a package for faint-galaxy photometry. Bertin & Arnouts 1996, A&A Supp. 317, 393. http://www.astromatic.net/software/sextractor Example:: # 1 NUMBER # 2 ALPHA_J2000 # 3 DELTA_J2000 # 4 FLUX_RADIUS # 7 MAG_AUTO [mag] # 8 X2_IMAGE Variance along x [pixel**2] # 9 X_MAMA Barycenter position along MAMA x axis [m**(-6)] # 10 MU_MAX Peak surface brightness above background [mag * arcsec**(-2)] 1 32.23222 10.1211 0.8 1.2 1.4 18.1 1000.0 0.00304 -3.498 2 38.12321 -88.1321 2.2 2.4 3.1 17.0 1500.0 0.00908 1.401 Note the skipped numbers since flux_radius has 3 columns. The three FLUX_RADIUS columns will be named FLUX_RADIUS, FLUX_RADIUS_1, FLUX_RADIUS_2 Also note that a post-ID description (e.g. "Variance along x") is optional and that units may be specified at the end of a line in brackets. t sextractorsSExtractor format tablecC`s8tt|ƒj|ƒ}d|jkr4|jd=n|S(s Read input data (file-like object, filename, list of strings, or single string) into a Table and return the result. tcomments(tsuperR8treadtmeta(Rttabletout((s:lib/python2.7/site-packages/astropy/io/ascii/sextractor.pyR<‹s cC`s t‚dS(N(tNotImplementedError(RR>((s:lib/python2.7/site-packages/astropy/io/ascii/sextractor.pytwrite–s(R0R1R2t _format_nametFalset_io_registry_can_writet _descriptionRt header_classR4t data_classRtContinuationLinesInputtertinputter_classR<RA(((s:lib/python2.7/site-packages/astropy/io/ascii/sextractor.pyR8ks  (R2t __future__RRRR tRtextern.six.movesRt BaseHeaderRtBaseDataR4t BaseReaderR8(((s:lib/python2.7/site-packages/astropy/io/ascii/sextractor.pyts S