HR-e~NdZddlZddlZddlZddlZddlmZddlm Z m Z ddl m Z m Z ddlmZmZddlmZmZdd lmZmZdd lmZdd lmZdd lmZmZmZmZm Z m!Z!gd Z"dZ#ddddddZ$dZ%dddddddZ&dZ' d(dZ(d)dZ)d*dZ*dZ+d+dZ,dZ-d,dZ.e/e.je0r)e.xjej12dd z c_d+d!Z3e/e3je0r)e3xjej12dd z c_dddd"d#Z4d$Z5d%Z6d-d'Z7dS).aConvenience functions for working with FITS files. Convenience functions ===================== The functions in this module provide shortcuts for some of the most basic operations on FITS files, such as reading and updating the header. They are included directly in the 'astropy.io.fits' namespace so that they can be used like:: astropy.io.fits.getheader(...) These functions are primarily for convenience when working with FITS files in the command-line interpreter. If performing several operations on the same file, such as in a script, it is better to *not* use these functions, as each one must open and re-parse the file. In such cases it is better to use :func:`astropy.io.fits.open` and work directly with the :class:`astropy.io.fits.HDUList` object and underlying HDU objects. Several of the convenience functions, such as `getheader` and `getdata` support special arguments for selecting which HDU to use when working with a multi-extension FITS file. There are a few supported argument formats for selecting the HDU. See the documentation for `getdata` for an explanation of all the different formats. .. warning:: All arguments to convenience functions other than the filename that are *not* for selecting the HDU should be passed in as keyword arguments. This is to avoid ambiguity and conflicts with the HDU arguments. For example, to set NAXIS=1 on the Primary HDU: Wrong:: astropy.io.fits.setval('myimage.fits', 'NAXIS', 1) The above example will try to set the NAXIS value on the first extension HDU to blank. That is, the argument '1' is assumed to specify an HDU. Right:: astropy.io.fits.setval('myimage.fits', 'NAXIS', value=1) This will set the NAXIS keyword to 1 on the primary HDU (the default). To specify the first extension HDU use:: astropy.io.fits.setval('myimage.fits', 'NAXIS', value=1, ext=1) This complexity arises out of the attempt to simultaneously support multiple argument formats that were used in past versions of PyFITS. Unfortunately, it is not possible to support all formats without introducing some ambiguity. A future Astropy release may standardize around a single format and officially deprecate the other formats. N)AstropyUserWarning)FITSDiffHDUDiff) FILE_MODES_File)_BaseHDU _ValidHDU)HDUListfitsopen)ImageHDU PrimaryHDU) BinTableHDU)Header)_is_dask_array_is_intfileobj_closed fileobj_mode fileobj_name path_like) getheadergetdatagetvalsetvaldelvalwritetoappendupdateinfo tabledump tableload table_to_hdu printdiffct|\}}t||g|Ri|\}} ||}|j}||n#||wxYw|S)a, Get the header from an HDU of a FITS file. Parameters ---------- filename : path-like or file-like File to get header from. If an opened file object, its mode must be one of the following rb, rb+, or ab+). ext, extname, extver The rest of the arguments are for HDU specification. See the `getdata` documentation for explanations/examples. **kwargs Any additional keyword arguments to be passed to `astropy.io.fits.open`. Returns ------- header : `Header` object closed)_get_file_mode_getextheaderclose) filenameargskwargsmoder&hdulistextidxhdur)s ;lib/python3.11/site-packages/astropy/io/fits/convenience.pyrrcs*"(++LD&h>t>>>v>>OGV%fo V $$$$ V $$$$ Ms AA&)r)lowerupperviewct|\}}|d} |d} |d} t|dko | duo| duo| du } t||g|Ri|\} } | |}|j}|W| rt d|dt| dkrt d | d}|j}|t d |r|j}| | n#| | wxYwd|rtj d n|rtj d rN|j j dS|j j dddkrdSfd|j j D|j _ t|tr/t|t jr||}|r||fS|S)a Get the data from an HDU of a FITS file (and optionally the header). Parameters ---------- filename : path-like or file-like File to get data from. If opened, mode must be one of the following rb, rb+, or ab+. ext The rest of the arguments are for HDU specification. They are flexible and are best illustrated by examples. No extra arguments implies the primary HDU:: getdata('in.fits') .. note:: Exclusive to ``getdata``: if ``ext`` is not specified and primary header contains no data, ``getdata`` attempts to retrieve data from first extension HDU. By HDU number:: getdata('in.fits', 0) # the primary HDU getdata('in.fits', 2) # the second extension HDU getdata('in.fits', ext=2) # the second extension HDU By name, i.e., ``EXTNAME`` value (if unique):: getdata('in.fits', 'sci') getdata('in.fits', extname='sci') # equivalent Note ``EXTNAME`` values are not case sensitive By combination of ``EXTNAME`` and EXTVER`` as separate arguments or as a tuple:: getdata('in.fits', 'sci', 2) # EXTNAME='SCI' & EXTVER=2 getdata('in.fits', extname='sci', extver=2) # equivalent getdata('in.fits', ('sci', 2)) # equivalent Ambiguous or conflicting specifications will raise an exception:: getdata('in.fits', ext=('sci',1), extname='err', extver=2) header : bool, optional If `True`, return the data and the header of the specified HDU as a tuple. lower, upper : bool, optional If ``lower`` or ``upper`` are `True`, the field names in the returned data object will be converted to lower or upper case, respectively. view : ndarray, optional When given, the data will be returned wrapped in the given ndarray subclass by calling:: data.view(view) **kwargs Any additional keyword arguments to be passed to `astropy.io.fits.open`. Returns ------- array : ndarray or `~numpy.recarray` or `~astropy.io.fits.Group` Type depends on the type of the extension being referenced. If the optional keyword ``header`` is set to `True`, this function will return a (``data``, ``header``) tuple. Raises ------ IndexError If no data is found in searched HDUs. extextnameextverrNzNo data in HDU #.rz2No data in Primary HDU and no extension HDU found.z2No data in either Primary or first extension HDUs.r%r3r4c&g|] }|Sr=).0ntranss r2 zgetdata..s!???EE!HH???)r'getlenr(data IndexErrorr)r*operator methodcallerdtypenamesdescr isinstancetype issubclassnpndarrayr5)r+r)r3r4r5r,r-r.r&r7r8r9 ext_givenr/r0r1rEhdrr@s @r2rrsA`"(++LD& **U  Cjj##G ZZ ! !F D QM3$;M7d?Mv~Ih>t>>>v>>OGV%fox < ? !=F!=!=!=>>>7||q   !UVVV!*C8D| !UVVV  *C V $$$$ V $$$$ E /%g.. /%g.. @ :  # F : A q !R ' ' F????dj.>??? $*T2:">">yy Sy s A1DD(cDd|vrd|d<t|g|Ri|}||S)a  Get a keyword's value from a header in a FITS file. Parameters ---------- filename : path-like or file-like Name of the FITS file, or file object (if opened, mode must be one of the following rb, rb+, or ab+). keyword : str Keyword name ext, extname, extver The rest of the arguments are for HDU specification. See `getdata` for explanations/examples. **kwargs Any additional keyword arguments to be passed to `astropy.io.fits.open`. *Note:* This function automatically specifies ``do_not_scale_image_data = True`` when opening the file so that values can be retrieved from the unmodified header. Returns ------- keyword value : str, int, or float do_not_scale_image_dataT)r)r+keywordr,r-rRs r2rr sA6!..,0() H .t . . .v . .C w<rBF)valuecommentbeforeafter savecommentc0d|vrd|d<t|} t|dg|Ri|\} } || | jvr|rd}| | j|||||| | dS#| | wxYw)as Set a keyword's value from a header in a FITS file. If the keyword already exists, it's value/comment will be updated. If it does not exist, a new card will be created and it will be placed before or after the specified location. If no ``before`` or ``after`` is specified, it will be appended at the end. When updating more than one keyword in a file, this convenience function is a much less efficient approach compared with opening the file for update, modifying the header, and closing the file. Parameters ---------- filename : path-like or file-like Name of the FITS file, or file object If opened, mode must be update (rb+). An opened file object or `~gzip.GzipFile` object will be closed upon return. keyword : str Keyword name value : str, int, float, optional Keyword value (default: `None`, meaning don't modify) comment : str, optional Keyword comment, (default: `None`, meaning don't modify) before : str, int, optional Name of the keyword, or index of the card before which the new card will be placed. The argument ``before`` takes precedence over ``after`` if both are specified (default: `None`). after : str, int, optional Name of the keyword, or index of the card after which the new card will be placed. (default: `None`). savecomment : bool, optional When `True`, preserve the current comment for an existing keyword. The argument ``savecomment`` takes precedence over ``comment`` if both specified. If ``comment`` is not specified then the current comment will automatically be preserved (default: `False`). ext, extname, extver The rest of the arguments are for HDU specification. See `getdata` for explanations/examples. **kwargs Any additional keyword arguments to be passed to `astropy.io.fits.open`. *Note:* This function automatically specifies ``do_not_scale_image_data = True`` when opening the file so that values can be retrieved from the unmodified header. rTTrNr%)rr(r)setr*) r+rUrVrWrXrYrZr,r-r&r/r0s r2rr-s@!..,0() H % %FhB4BBB6BBOGV% gfo, , , ,G""7E7FEJJJ V $$$$$ V $$$$s 7A==Bcd|vrd|d<t|}t|dg|Ri|\}} ||j|=||dS#||wxYw)a Delete all instances of keyword from a header in a FITS file. Parameters ---------- filename : path-like or file-like Name of the FITS file, or file object If opened, mode must be update (rb+). An opened file object or `~gzip.GzipFile` object will be closed upon return. keyword : str, int Keyword name or index ext, extname, extver The rest of the arguments are for HDU specification. See `getdata` for explanations/examples. **kwargs Any additional keyword arguments to be passed to `astropy.io.fits.open`. *Note:* This function automatically specifies ``do_not_scale_image_data = True`` when opening the file so that values can be retrieved from the unmodified header. rTTrr%N)rr(r)r*)r+rUr,r-r&r/r0s r2rrzs0!..,0() H % %FhB4BBB6BBOGV% FO "7 + V $$$$$ V $$$$s AA, exceptionct||}|jr&t|tst||}|||||dS)a Create a new FITS file using the supplied data/header. Parameters ---------- filename : path-like or file-like File to write to. If opened, must be opened in a writable binary mode such as 'wb' or 'ab+'. data : array or `~numpy.recarray` or `~astropy.io.fits.Group` data to write to the new file header : `Header` object, optional the header associated with ``data``. If `None`, a header of the appropriate type is created for the supplied data. This argument is optional. output_verify : str Output verification option. Must be one of ``"fix"``, ``"silentfix"``, ``"ignore"``, ``"warn"``, or ``"exception"``. May also be any combination of ``"fix"`` or ``"silentfix"`` with ``"+ignore"``, ``+warn``, or ``+exception" (e.g. ``"fix+warn"``). See :ref:`astropy:verify` for more info. overwrite : bool, optional If ``True``, overwrite the output file if it exists. Raises an ``OSError`` if ``False`` and the output file exists. Default is ``False``. checksum : bool, optional If `True`, adds both ``DATASUM`` and ``CHECKSUM`` cards to the headers of all HDU's written to the file. r)) overwrite output_verifychecksumN)_makehduis_imagerLrr)r+rEr)rbrarcr1s r2rrsoR 4 C |.JsJ77.f---KKI]XrBc  %ddlm}ddlm}m}d}|jrddlm}ddlm }ddl m }dd l m } |j|||f} | rd | D} t!d | |j|} | r| |\}}|} t#| t&jjrt&j| j}| jjD]\}\}}t'j| j|||kr|jr|jdjn|j}t=|t&jr-tAt&j!t&j!| j|<t=|t&j"rt&j!| j|<t=|t&j#r d | j|<tIj%| &|| }|jD]M%d}%j'|vs%j'j(|vs| %j)j}|*tV%_,NntIj%| || }|jD]f%|%j)j-j'K|%j)j-jt\k}||%j)j-j'|}||%_/|%j)j0}|ddl m1}ddl2m3} |4d%_0|%j0dd#|$r,|j5}|d%j)dtm|dt $rud|4d}to%fd|j89dgDr|dz }n|dz }tuj;|txYbwxYwh|j8=di}|D][\}}|j|%d D]'} t}%| |9| d(|9d!d}!|!|!%_?\|j8D]\}"}#||"@s|"@|vrtuj;d"|"d#txX|"dkrd$}"t#|#tra|#D]]}$ |jBC|"|$f #t $r1tuj;d%|"d&t;|#d'txYZwxYw |#|jB|"<#t $r2tuj;d%|"d&t;|#d'txYwxYw|S)(a Convert an `~astropy.table.Table` object to a FITS `~astropy.io.fits.BinTableHDU`. Parameters ---------- table : astropy.table.Table The table to convert. character_as_bytes : bool Whether to return bytes for string columns when accessed from the HDU. By default this is `False` and (unicode) strings are returned, but for large tables this may use up a lot of memory. Returns ------- table_hdu : `~astropy.io.fits.BinTableHDU` The FITS binary table HDU. r)python_to_tdisp)REMOVE_KEYWORDSis_column_keywordNr) BaseColumn)Time)Quantity) time_to_fitsc&g|]}|jjSr=)rname)r>cols r2rAz table_to_hdu..s K K K3 K K KrBz(cannot write table with mixin column(s) r;)r)character_as_bytes)BIJK) logical_dtype)Unit)UnitScaleErrorfits)formatwarn)rz parse_strictz The column 'z>' could not be stored in FITS format because it has a scale '(zZ)' that is not recognized by the FITS standard. Either scale the data or change the units.z The unit 'z+' could not be saved in native FITS format c38K|]}d|vo djz|vVdS)SerializedColumnzname: N)ro)r>itemrps r2 ztable_to_hdu..PsM'$.N8ch3F$3NrBcommentszand hence will be lost to non-astropy fits readers. Within astropy, the unit can roundtrip using QTable, though one has to enable the unit before reading.zand cannot be recovered in reading. It can roundtrip within astropy by using QTable both to write and read back, though one has to enable the unit before reading.__coordinate_columns__) coord_type coord_unit time_ref_poszMeta-data keyword z@ will be ignored since it conflicts with a FITS reserved keywordrWz Attribute `z ` of type z* cannot be added to FITS Header - skipping)Dcolumnrgconnectrhrihas_mixin_columnsastropy.table.columnrj astropy.timerk astropy.unitsrlfitstimermcolumnsnot_isinstance ValueErrorrLas_arrayrOma MaskedArraydefault_fill_valuerIfieldsitemsall fill_valuesubdtyperMrNcomplexfloatingcomplexnaninexact characterr from_columnsfilledrzp_formatroastypeintnullrbooldispunitrwastropy.units.format.fitsrx to_stringscalestranymetarCwarningsr{rpopsetattrrr4listr)r)&tablerqrgrhrirRrjrkrlrmunsupported_colsunsupported_names time_colstarrayrcolnamecoldtype_coltype table_hdu int_formatsrlogical tdisp_formatrrwrxrwarning coord_metacol_namecol_infoattrtrposkeyrVrrps& @r2r"r"sj((''''';;;;;;;; C - 433333%%%%%%************!=77Xt8TUU   K K:J K K K N;LNN M,,T22  -%e,,JE3^^  F&"%+,,(  U55flCC&,l&9&?&?&A&A 4 4 "G]hvf'04Fw4OOPP 42:1BUH%a(-- gr'9::4181H1HF%g..44413F%g..66413F%g. , MMOOC>>88JSXf6BBBBBI"    $n438447:5zz444  ; ; ; *!1!1*** % z2 > >LGG RG  g'9:::::/ ;! ^ 8"==J(..00%%()/ 9 9D Cx||D$77 8 8 8 8 ^T22  $C j&&(( U  SYY[[ ) ) SYY[[O-K-K M/S///"     *  C eT " "   $++S$K8888!M:c::T%[[:::*  (-  %%    6#66e666&  s7M  B*O:9O:T::8U54U5: V8WWTc t|trtj|}t |\}}}|rt |||fd|i|dSt||} t| trt||} |s|s_t|fddi|} | | || _ | |dS#| |wxYwt|d} || _ | | | dS#| wxYw)a Append the header/data to FITS file if filename exists, create if not. If only ``data`` is supplied, a minimal header is created. Parameters ---------- filename : path-like or file-like File to write to. If opened, must be opened for update (rb+) unless it is a new file, then it must be opened for append (ab+). A file or `~gzip.GzipFile` object opened for update will be closed after return. data : array, :class:`~astropy.table.Table`, or `~astropy.io.fits.Group` The new data used for appending. header : `Header` object, optional The header associated with ``data``. If `None`, an appropriate header will be created for the data object supplied. checksum : bool, optional When `True` adds both ``DATASUM`` and ``CHECKSUM`` cards to the header of the HDU when written to the file. verify : bool, optional When `True`, the existing FITS file will be read in to verify it for correctness before appending. When `False`, content is simply appended to the end of the file. Setting ``verify`` to `False` can be much faster. **kwargs Additional arguments are passed to: - `~astropy.io.fits.writeto` if the file does not exist or is empty. In this case ``output_verify`` is the only possible argument. - `~astropy.io.fits.open` if ``verify`` is True or if ``filename`` is a file object. - Otherwise no additional arguments can be used. rcr.rr%r.N)rLrospath expanduser_stat_filename_or_fileobjrrdrr r r_output_checksumr*r_writeto) r+rEr)rcverifyr-ror&noexist_or_emptyr1fs r2rrslP(I&&07%%h//%>x%H%H"D&" $DDDVDDDDDtV$$ c: & & )4((C   ;;;F;;A ' (0$v&&&&&v&&&&hX...A '/$ Q  s&CC2D99Ecj|r.t|dtr|d}|dd}nd}|d|}t||}t |}t |dg|Ri|\}} |||<||dS#||wxYw)a Update the specified HDU with the input data/header. Parameters ---------- filename : path-like or file-like File to update. If opened, mode must be update (rb+). An opened file object or `~gzip.GzipFile` object will be closed upon return. data : array, `~astropy.table.Table`, or `~astropy.io.fits.Group` The new data used for updating. header : `Header` object, optional The header associated with ``data``. If `None`, an appropriate header will be created for the data object supplied. ext, extname, extver The rest of the arguments are flexible: the 3rd argument can be the header associated with the data. If the 3rd argument is not a `Header`, it (and other positional arguments) are assumed to be the HDU specification(s). Header and HDU specs can also be keyword arguments. For example:: update(file, dat, hdr, 'sci') # update the 'sci' extension update(file, dat, 3) # update the 3rd extension HDU update(file, dat, hdr, 3) # update the 3rd extension HDU update(file, dat, 'sci', 2) # update the 2nd extension HDU named 'sci' update(file, dat, 3, header=hdr) # update the 3rd extension HDU update(file, dat, header=hdr, ext=5) # update the 5th extension HDU **kwargs Any additional keyword arguments to be passed to `astropy.io.fits.open`. rrNr)rr%)rLrrrdrr(r*) r+rEr,r-r)new_hdur&r/_exts r2rrsL  47F++aABBxZZ& ) )FtV$$G H % %FHh@@@@@@MGT%  V $$$$$ V $$$$s =BB2c t|d\}}d|vrd|d<t|fd|i|} ||}|r|n#|r|wwxYw|S)a  Print the summary information on a FITS file. This includes the name, type, length of header, data shape and type for each HDU. Parameters ---------- filename : path-like or file-like FITS file to obtain info from. If opened, mode must be one of the following: rb, rb+, or ab+ (i.e. the file must be readable). output : file, bool, optional A file-like object to write the output to. If ``False``, does not output to a file and instead returns a list of tuples representing the HDU info. Writes to ``sys.stdout`` by default. **kwargs Any additional keyword arguments to be passed to `astropy.io.fits.open`. *Note:* This function sets ``ignore_missing_end=True`` by default. readonlydefaultignore_missing_endTr.)output)r'r rr*)r+rr-r.r&rrets r2rrs,"(J???LD&6))'+#$/////AffFf##   GGIII   GGIIII  Js AA4cfddD}|p|}t|tr|rt|\}}t|\}} t||g|Ri|\} } t||g|Ri|\} } n%#t$r| |wxYw | | }| | }t t||fi| || | dS#| || | wxYwt|tr|rtdt|tr1|s/t t||fidSt|tr|rtdt t||fidS)a` Compare two parts of a FITS file, including entire FITS files, FITS `HDUList` objects and FITS ``HDU`` objects. Parameters ---------- inputa : str, `HDUList` object, or ``HDU`` object The filename of a FITS file, `HDUList`, or ``HDU`` object to compare to ``inputb``. inputb : str, `HDUList` object, or ``HDU`` object The filename of a FITS file, `HDUList`, or ``HDU`` object to compare to ``inputa``. ext, extname, extver Additional positional arguments are for HDU specification if your inputs are string filenames (will not work if ``inputa`` and ``inputb`` are ``HDU`` objects or `HDUList` objects). They are flexible and are best illustrated by examples. In addition to using these arguments positionally you can directly call the keyword parameters ``ext``, ``extname``. By HDU number:: printdiff('inA.fits', 'inB.fits', 0) # the primary HDU printdiff('inA.fits', 'inB.fits', 2) # the second extension HDU printdiff('inA.fits', 'inB.fits', ext=2) # the second extension HDU By name, i.e., ``EXTNAME`` value (if unique). ``EXTNAME`` values are not case sensitive: printdiff('inA.fits', 'inB.fits', 'sci') printdiff('inA.fits', 'inB.fits', extname='sci') # equivalent By combination of ``EXTNAME`` and ``EXTVER`` as separate arguments or as a tuple:: printdiff('inA.fits', 'inB.fits', 'sci', 2) # EXTNAME='SCI' # & EXTVER=2 printdiff('inA.fits', 'inB.fits', extname='sci', extver=2) # equivalent printdiff('inA.fits', 'inB.fits', ('sci', 2)) # equivalent Ambiguous or conflicting specifications will raise an exception:: printdiff('inA.fits', 'inB.fits', ext=('sci', 1), extname='err', extver=2) **kwargs Any additional keyword arguments to be passed to `~astropy.io.fits.FITSDiff`. Notes ----- The primary use for the `printdiff` function is to allow quick print out of a FITS difference report and will write to ``sys.stdout``. To save the diff report to a file please use `~astropy.io.fits.FITSDiff` directly. cDi|]}|v||Sr=)r)r>rr-s r2 zprintdiff..}s1!$v VZZ__ rBr7r8r9r%z;Cannot use extension keywords when providing an HDU object.z=Extension specification with HDUList objects not implemented.N)rLrr'r( Exceptionr*printrreportr rr NotImplementedErrorr)inputainputbr,r- extensionhas_extensionsmodeaclosedamodebclosedbhdulistaextidxahdulistbextidxbhduahdubs ` r2r#r#@ssz(DI&YN&#(;>(;(//w'//w#FEFDFFFIFF'  ' J J J J J J Hgg    NN'N * * *   +G$DG$D '$////6688 9 9 9 NN'N * * * NN'N * * * * * NN'N * * * NN'N * * * * FI & &;>;VWWW FI & & ;~ ; gff////668899999 FG $ $;;! K    hvv00007799:::::s&A;;"B!=D .D:ct|d\}}t||} |sDtj|jj\} } | dzt|zdz}|||||||r| dSdS#|r| wwxYw)a Dump a table HDU to a file in ASCII format. The table may be dumped in three separate files, one containing column definitions, one containing header parameters, and one for table data. Parameters ---------- filename : path-like or file-like Input fits file. datafile : path-like or file-like, optional Output data file. The default is the root name of the input fits file appended with an underscore, followed by the extension number (ext), followed by the extension ``.txt``. cdfile : path-like or file-like, optional Output column definitions file. The default is `None`, no column definitions output is produced. hfile : path-like or file-like, optional Output header parameters file. The default is `None`, no header parameters output is produced. ext : int The number of the extension containing the table HDU to be dumped. overwrite : bool, optional If ``True``, overwrite the output file if it exists. Raises an ``OSError`` if ``False`` and the output file exists. Default is ``False``. Notes ----- The primary use for the `tabledump` function is to allow editing in a standard text editor of the table data and parameters. The `tableload` function can be used to reassemble the table from the three ASCII files. rrrrz.txtN) r'r rrsplitext_fileroreprdumpr*) r+datafilecdfilehfiler7rar.r&rroottails r2r r sX"(J???LD&%%%A  7))!',77JD$czDII-6H # HfeY777   GGIIIII  6  GGIIII s A$B%%B> z c2tj|||dS)a Create a table from the input ASCII files. The input is from up to three separate files, one containing column definitions, one containing header parameters, and one containing column data. The header parameters file is not required. When the header parameters file is absent a minimal header is constructed. Parameters ---------- datafile : path-like or file-like Input data file containing the table data in ASCII format. cdfile : path-like or file-like Input column definition file containing the names, formats, display formats, physical units, multidimensional array dimensions, undefined values, scale factors, and offsets associated with the columns in the table. hfile : path-like or file-like, optional Input parameter definition file containing the header parameter definitions to be associated with the table. If `None`, a minimal header is constructed. Notes ----- The primary use for the `tableload` function is to allow the input of ASCII data that was edited in a standard text editor of the table data and parameters. The tabledump function can be used to create the initial ASCII files. T)replace)rload)rrrs r2r!r!s>  HfeT B B BBrBrchd||||d}t|dkrt|ds(t|tr1t|dkr|||t ||d}nt|dt r||t ||d}nd|d}n[t|dkr&|||t ||d}|d}n"t|dkrt d|vt|sgt|trCt|dkr0t|dt rt|dstd|$t|t std |t|std |||d}n6|||t ||r |r||f}n|df}n|r|t d t|fd |i|}||fS) z Open the input file, return the `HDUList` and the extension. This supports several different styles of extension selection. See the :func:`getdata()` documentation for the different possibilities. z0Redundant/conflicting extension arguments(s): {})r,r7r8r9rrNzToo many positional arguments.z_The ext keyword must be either an extension number (zero-indexed) or a (extname, extver) tuple.z&The extname argument must be a string.z'The extver argument must be an integer.z)extver alone cannot specify an extension.r.) rzrDrrLtuple TypeErrorrrr ) r+r.r7r8r9r,r-err_msgr/s r2r(r(sAGGcgHHG 4yyA~~ 47    3 6 6 3s88q=='"59K(((q'CC Q % % '"5(((1gGGq'CC Ta ?g1V5GG$$ $q'a TQ8999   sE " "CA 3q63''A  ;   :gs#;#;ABBB '&//BCCC {w6> g1V5G   E  F#CCA,CC EGOCDDDx55d5f55G C<rBc|t}tj||}|jttfvrt |t jr |jj t |t j rt||}nJt |t jst|rt||}ntd|S)Nr`zData must be a numpy array.)rr _from_data __class__r rLrOrPrIrrecarrayrrr KeyError)rEr)r1s r2rdrd^s ~  dF + +C }9--- tRZ ( ( :-1Z->-J bk * *.Kd6222CC bj ) ) :^D-A-A :4///CC899 9 JrBct|tjrtj|}t |}t |pd} |}n#t$rd}YnwxYw|oBtj | p"tj |dkp| o|dk}|||fS)Nr;r) rLrPathLikefspathrrtellAttributeErrorrexistsgetsize)r+r&rolocrs r2rrps(BK(('9X&& H % %F  ! ! 'RDmmoo  KbgnnT***Jrwt/D/D/I!( sax ) ))sA%% A43A4rc|}t|}t|}|8tj|}|"t d|||fS)z Allow file object to already be opened in any of the valid modes and and leave the file in the same state (opened or closed) as when the function was called. NzRFile mode of the input file object ({!r}) cannot be used to read/write FITS files.)rrrrCOSErrorrz)r+rr.r&fmodes r2r'r'sk D H % %F  " "E ~e$$ <))/  <rB)Nr^FF)F)NFT)N)NNNrF)r)8__doc__rGrrnumpyrOastropy.utils.exceptionsrdiffrrfilerrhdu.baser r hdu.hdulistr r hdu.imager r hdu.tablerr)rutilrrrrrr__all__rrrrrrr"rrrr#r rLr_tdump_file_formatrr!r(rdrr'r=rBr2rss55n 777777################))))))))********++++++++""""""   "@%)DtEEEEEPL    J%J%J%J%J%Z % % %L   ....bDDDDNIIIIX7%7%7%t""""Jj;j;j;Z9999x:i%%P 7??hOOOCCCCD:i%%P 7??hOOO(,T$HHHHHV$***$rB