ó šßÈ[c @`s:dZddlmZmZmZmZddlmZddlmZ ddl m Z m Z m Z mZmZeegƒddlZeƒZe dd gd gfe jd ed ed dƒe ddge jd ed ed dƒe dddge jd ed dd edidd6dd6ƒe dddddge jd ed ed d did!d6d"d6ƒe d#d$d%ge jd ed ed d&did'd6d(d6ƒe d)d*ge jejjejƒd ed ed d+ƒe d,d,gd‹ejdd ed ed d/ƒe d0d1gd2ejej d ed ed d3ƒe d4d5d6ge j!d ed ed d7did8d6d9d6ƒe d:d;d<d=d>ge j"d ed ed d?did@d6dAd6ƒe dBdCdDge j#d ed ed dEdidFd6dGd6ƒe dHge j$d ed dIdidJd6dKd6ƒe dLge j%d ed dMdidNd6dOd6ƒe dPdQdRge j&d ed edSdTdUgd dVƒe dWdXge j'e je j(jej)ej*ƒjej)ƒd ed ed dYdidZd6d[d6ƒe d\d]d^ge j+d ed ed d_did`d6dad6ƒe dbdcgdcgfdidcdd6dcde6d ed eƒe dfdgdhgdiej,ejdej-d ed ed djƒe dkdldmgdndoeje.ejdpej*dqej/dqd ed ed drƒe dsgd eƒe dtdugdugfdidudv6dudd6dude6d ed edSdwgƒe dxdygdygfdidydd6dyde6d ed eƒe dzgd ed eƒe d{gd ed eƒe d|d}gd}gfdid}dv6d}dd6d}de6d ed eƒe d~dgd~gfd ed e eƒe d€dgd€gfd‚e0d edid€de6d e edSdƒgƒe d„gd ed eƒe d…gd ed eƒe d†gd d‡d edidˆd6d‰d6ƒ[ [ [ddŠl1m2Z3edk r6ee3eƒƒ7ZndS(Œur This package defines the astrophysics-specific units. They are also available in the `astropy.units` namespace. i(tabsolute_importtdivisiontprint_functiontunicode_literalsi(tsii(tUnitBasetdef_unitt si_prefixestbinary_prefixestset_enabled_unitsNuAUuauuastronomical_unitt namespacetprefixestdocu>astronomical unit: approximately the mean Earth--Sun distance.upcuparsecu'parsec: approximately 3.26 light-years.usolRaduR_sunuRsunu Solar radiustformatu R_{\odot}ulatexuR⊙uunicodeu jupiterRaduR_jupuRjupu R_jupiteruRjupiteruJupiter radiusu R_{\rm J}uR♃uearthRaduR_earthuRearthu Earth radiusu R_{\oplus}uR⊕ulyru lightyearu Light yearubarni iäÿÿÿubarn: unit of area used in HEPucycleucyg@u3cycle: angular measurement, a full turn or rotationusolMassuM_sunuMsunu Solar massu M_{\odot}uM⊙u jupiterMassuM_jupuMjupu M_jupiteruMjupiteru Jupiter massu M_{\rm J}uM♃u earthMassuM_earthuMearthu Earth massu M_{\oplus}uM⊕uM_pu Proton massuM_{p}uMâ‚šuM_eu Electron massuM_{e}uMâ‚‘uuuDauDaltontexclude_prefixesuaudauUnified atomic mass unituRyurydberguDRydberg: Energy of a photon whose wavenumber is the Rydberg constantu R_{\infty}uR∞usolLumuL_sunuLsunuSolar luminanceu L_{\odot}uL⊙uphuphotonuogipuvounituJyuJanskyujanskygË®Ä@ˆ:uJansky: spectral flux densityuRuRayleighurayleighg _ BiiþÿÿÿiÿÿÿÿuRayleigh: photon fluxuSunuctucountufitsupupixupixeluchanubinuvoxuvoxelubitububyteuBiuduaduubeamuelectronuNumber of electronsue^{-}ueâ»(tgenerate_unit_summaryg`P¾ö°:(5t__doc__t __future__RRRRtRt constantst_sitcoreRRRRR tnumpyt_numpytglobalst_nstautTruetpctR_suntFalsetR_juptR_earthtctyrttotmtpitradtM_suntM_juptM_earthtm_ptm_etutRydthteVtstL_suntWtHztphtsrtbittutilsRt_generate_unit_summarytNone(((s6lib/python2.7/site-packages/astropy/units/astrophys.pyts²"(   *!  ()     6   . 6     %