IR-e :dZddlZddlmZddlmZmZmZddl m Z m Z m Z e Ze ddgejed d e d d gejdejzdejzdzzz ed d e ddgdejzejdzzejz ejz ed d e ddgdejzejdzzejz ejz ed d e ddgedgdgdfgd d!Z[ [ [[[edd"lmZeee z ZdSdS)#z This module defines magnitude zero points and related photometric quantities. The corresponding magnitudes are given in the description of each unit (the actual definitions are in `~astropy.units.function.logarithmic`). N)si) astrophyscgsr)UnitUnitBasedef_unitBolL_bolFzULuminosity corresponding to absolute bolometric magnitude zero (magnitude ``M_bol``).) namespaceprefixesdocbolf_bolg$@zVIrradiance corresponding to appparent bolometric magnitude zero (magnitude ``m_bol``).ABABfluxg1n;z5AB magnitude zero flux density (magnitude ``ABmag``).STSTfluxg|~+0/>z5ST magnitude zero flux density (magnitude ``STmag``).mgymaggynnanog& .>zMaggies - a linear flux unit that is the flux for a mag=0 object.To tie this onto a specific calibrated unit system, the zero_point_flux equivalency should be used.c4t|}t|fgS)a An equivalency for converting linear flux units ("maggys") defined relative to a standard source into a standardized system. Parameters ---------- flux0 : `~astropy.units.Quantity` The flux of a magnitude-0 object in the "maggy" system. )rr)flux0 flux_unit0s 9lib/python3.11/site-packages/astropy/units/photometric.pyzero_point_fluxr BseJ J   )generate_unit_summary)__doc__numpy_numpyastropy.constantsr_sirrcorerrr globals_nsL_bol0pipcergcmsHzAAr utilsr"_generate_unit_summaryr!rr7s3'''''' ********** gii GJ  !      GJ!fi-4),#61"<<=  !      8CG#cfbj0247"%? ?   8CG#cfbj0247"%? ?   Guvh% & 6     ! ! !"  Y  GFFFFF %%ggii000GGG r!