ELF>`@@UHH0EEEMYf~fnf~EMYE\EEE(YMXEE(YMXEE(YMXEE(YMXEEEEE,ЉEMX^UH}HuHUEHcHEHHHHHHEH]UH}HuHUEHcHEHHHHHHEH]UHH0H}EMHEHEYHEHHEHYXHEHHEHYXEEfnf~EfZEYEMYEEUHH}HuHEHH` PHEHEHH0 HHEHPHEHH0 HHEHPHEHH0 HEPHEHH( HHEHH0 Y^HE@ HEH^HE@(HEHH` HPHEHP0]UHHPH}HuHUHEHEHHEH@0HHEHEHfH~HEHUHEHHHE@HΉXfH~HEHE@ HEHP HEf(fHnHfH~HEfZUf~fnZEfZ]f~fnZEEf(^M\HEUHH`H}HuHUHMHEHHEH@0HHEHEHfH~HEHUHEHHHE@HΉ[fH~HEHUHEHHHE@HΉsfH~HEEf(YMHE@(YHEHE@ HEHP HEf(fHnH_fH~HEfZUf~fnZEfZ]f~fnZEEf(^M\HEUHHH8H0H(H DLH EH @E}us}umHHHHHhAAHǸHHHH8HHEH8HHEH(@EH0HHEH0HHEH0EH0EEf(YM^xH8H^pH8HHhHhH H@H`fEfEfEfEfEfEfEHE:HUHHHHHHEH@X<; HUHHHHHHEH@Y<HUHHHHHHEHHH`HHHHfH~HHHMEHΉfH~HHHMEHΉfH~HYpYHUHHHHHHEHH HUHHHHHHEH@ YHUHHHHHHEHP$HUHHHHHHEH@$YXHUHHHHHHEHP(HUHHHHHHEH@(YXZHfHnfH~fHnYxYfZf~fnZfZf~fnZf(^\EXEYMXEEXEYMXEYMXEEXEYMXEHEHEH;EEEEEEEEH@HHhAAHH@XHPPHX@`8h0p(fH*hf(YPXf(Y\f( fH*hf(Y@Hf(Y\f( YfH~fHnfH~HfH*hY8XYH\^H(YfH*h^HEHE0UHSHH}HuHxHpLhDdHhEHh@EHh@EHh@EHh@EHE@4E؃}u }u}tx}urHHHHHhAAHǸHHH}u}tx}trHHHHHhAAHǸHHHHEHff/v}uy}us}umHHHHHh"AAHǸHHH}u }LMDdHhHxHuHEH}WH}WHHdMf/HH]XH]HHHh4XfHnAAHǸHHHEf/HHeXH]HHHh<XfHnAAHǸHHH}t-H]H‹fHnùƿHEHE@YHE@YEHE@`EHEEHE@hYEf(YMEf(Y^f(EE^E^EEHEHE\~ fTf/HHHEHHHHEHhSf(fHnAAHǸHHHH]UH}}u]UHHpH}HuHUEHMHE@YHEf))@)@ f@0HEH` @tHEH@HUHHEHUHMHEHHHE@LfZEYuHHHHHhAAHǸHHHUHH}HuHUHE EHE@0EHE@8EEYMYEEYMYEE\EYE ^EHEHpHEHYEEYE]TotalMass?SmoothedGasMass?UnsmoothedGasMass?DarkMatterMass?StellarMass?BlackHoleMass?StarFormationRate/??@@@?@@@?3Ey?3Ey?3Ey?;f?;f?3Ey?3Ey?3Ey;f?;f??;f?;f3Ey?3Ey3Ey?;f?;f3Ey?3Ey3Ey;f?;f??;f?;f? @B>{>@B>{>=,?{>@B>{>@B>{>=,?{>=,?    neutrino/Default/neutrino.c[%04i] %s %s:%s():%i: Neutrino diagnostics only defined when using the delta-f method. [%04i] %s %s:%s():%i: Running without neutrino particles, but specified a neutrino model that requires them. [%04i] %s %s:%s():%i: Running with neutrino particles, but specified a neutrino model that is incompatible with particles. [%04i] %s %s:%s():%i: Running without neutrino particles, but specified neutrinos in the background cosmology and not using a neutrino model that does not use particles. [%04i] %s %s:%s():%i: There is no correlation between current and sampled neutrino momenta (r = %e, I = %e). Most likely, the neutrino seed is incorrect or the particle IDs have been scrambled. [%04i] %s %s:%s():%i: The neutrino particle weights are very large (r = %e, I = %e). Most likely, the particle velocities are incorrectly normalised. [%04i] %s %s: Neutrino delta-f diagnostic: I = %e [%04i] %s %s:%s():%i: The massive neutrino content of the simulation does not match the cosmology in the parameter file: cosmo.Omega_nu = %e particles Omega_nu = %e [%04i] %s %s:%s():%i: lightcone map function called on wrong particle type compute_neutrino_diagnosticsneutrino_check_cosmologylightcone_map_neutrino_mass_get_value;?r1?+= ,>>-??????-C6?@l?j?.\F F@int cc t#%#!##  c \Ac8-<-)2!-F82%]&C(J*,?-\?? $ 0( ! 3d5#d6#d<7< (  c  c   c " p # p $i 0^T`0a0bTcTd e$fT( d \ \$( C  Eu F G ?  \' Hp$0 K  M N Ot  \/ P$ l & n& o ? 6 \ p Q  d w r     t!B $m' t't'!t',t'7t * t(*t0*%t8*2t@*?tHsfh-!P0P0#X1`1 h2p2%x33#44)55#8c; t< t? B EcH  35c8 9 : ;  < (= 0> 8? @B HC PD XF `HhJcpQctS xVJW]XZ'b d1e;fg h Ficu@mB-m ' \,6 P \.P.PrC#)cD  \'* ()*c+c.E /E3 4 5 @/6c/7c/8 * \?  F\! 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