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n!(NAŚFSHDPx(Q6%%&FFRHP` a"(@sFSHDPx(v6%%K`BTLF[CWuKD46B7*JPQBwڱRFU`F"d)2^XB@=sl{nB7IBiZٞoOHDR!wiwiwiwi   6 #/2COHDR!wiwiwiwiA   4UhBkZ 5TREE GBTLF[CWTKD46B7*JPQBwڱRFU`F"d)2^XB@=sl{nB7IBiZٞOHDR!wiwiwiwi   xksZBTHDd(mxFRHPX B(y(wFSHDPx(6%%*BTLFjCWnKD46B7*JPQBwڱRFU`F"d82^XB@Lsl{nB7IBxZٞ#[D(OHDR!wiwiwiwi   w?@ABCDEFGHIJKLMNOPQRSTUVWXYZ[\]^_`abcdefghijklmnopqrstuvwxyz{|}~      !"#$%&'()*+,-./0123456789:;<=>?@ABCDEFGHIJKLMNOPQRSTUVWXYZ[\]^_`abcdefghijklmnopqrstuvwxyz{|}~      !"#$%&'()*+,-./0123456789:;<=>?@ABCDEFGHIJKLMNOPQRSTUVWXYZ[\]^_`abcdefghijklmnopqrstuvwxyz{|}~      !"#$%&'()*+,-./0123456789:;<=>?@ABCDEFGHIJKLMNOPQRSTUVWXYZ[\]^_`abcdefghijklmnopqrstuvwxyz{|}~/П`TREE BTLF[CWKD46B7*JPQBwڱRFU`F"d)2^XB@=sl{nB7IBiZٞsB@OHDR!wiwiwiwi @ ( 5$}TREE$FSSE :kFSSEMy[?FSSEƴFSSE b>rFSSE$ b@8FSSE'; MsFSSE1-} xYFSSEB; #&b1w"FRHP i(?%OqFSHD4Px(y7%%/"BTLF[CWKD46B7*JPQBwڱRFU`F"d)2^XB@=sl{nB7IBiZٞ(FSSE}ڈFSSE[_FSSE9 `{-FSSEZ$NK2FSSEZjKFSSE[x'֒FFSSE `#j3FSSERֶ FSSE`8FSSEF0j[BFSSEn!j]FSSEa"u FSSEB|8=VFSSE:t JFSSEwCAFSSEx EGFSSEjُLFSSEnQ[FSSEi(]6FHDBT+ DescriptionBinary tree describing splitting events. Particles that keep the original ID have a value of zero in a splitting event, whereasparticles given a new ID have a value of one.FHDB_ U_M exponent   U_L exponent   U_t exponent   U_I exponent   U_T exponent  h-scale exponent  a-scale exponent  "Expression for physical CGS units[ - ] Lossy compression filterNone Value stored as physical& Property can be converted to comovingBConversion factor to CGS (not including cosmological corrections) ?@4 4?GConversion factor to physical CGS (including cosmological corrections) ?@4 4?FHIB;7L$FHDBvLL DescriptionNumber of times this particle has been split. Note that both particles that take part in the splitting have their counter incremented.FHDBvXm U_M exponent   U_L exponent   U_t exponent   U_I exponent   U_T exponent  h-scale exponent  a-scale exponent  "Expression for physical CGS units[ - ] Lossy compression filterNone Value stored as physical& Property can be converted to comovingBConversion factor to CGS (not including cosmological corrections) ?@4 4?GConversion factor to physical CGS (including cosmological corrections) ?@4 4?FHIBvC?'FHDBu DescriptionID of the progenitor of this particle. If this particle is the result of one (or many) splitting events, this ID corresponds to the ID of the particle in the initial conditions that its lineage can be traced back to. If the particle was never split, this is the same as ParticleIDs.FHDB/+w U_M exponent   U_L exponent   U_t exponent   U_I exponent   U_T exponent  h-scale exponent  a-scale exponent  "Expression for physical CGS units[ - ] Lossy compression filterNone Value stored as physical& Property can be converted to comovingBConversion factor to CGS (not including cosmological corrections) ?@4 4?GConversion factor to physical CGS (including cosmological corrections) ?@4 4?FHIB L HFoFHDB0^R DescriptionFCo-moving gravitational Plummer-equivalent softenings of the particlesFHDB0{3! U_M exponent   U_L exponent  ? U_t exponent   U_I exponent   U_T exponent  h-scale exponent  a-scale exponent  ?"Expression for physical CGS units a U_L [ cm ]Lossy compression filterNone Value stored as physical& Property can be converted to comovingBConversion factor to CGS (not including cosmological corrections) ?@4 4?GConversion factor to physical CGS (including cosmological corrections) ?@4 4?FHIB0@T@PK{ FHDBgGConversion factor to physical CGS (including cosmological corrections) ?@4 4?FHDB U_M exponent   U_L exponent  @ U_t exponent   U_I exponent   U_T exponent  h-scale exponent  a-scale exponent  "Expression for physical CGS units a^-1 U_L^2 U_t^-2 [ cm^2 s^-2 ]Lossy compression filterNone Value stored as physical& Property can be converted to comovingBConversion factor to CGS (not including cosmological corrections) ?@4 4? Description>Co-moving gravitational potential at position of the particlesFHIBv\vX|FHDBw, DescriptionTime differential (over the previous step) of the velocity divergence field around the particles. Again, provided without cosmology as this includes a Hubble flow term. To get back to a peculiar velocity divergence time differential, x_pec = a^4 (x - a^{-2} n_D dH / dt)FHDBw9 U_M exponent   U_L exponent   U_t exponent   U_I exponent   U_T exponent  h-scale exponent  a-scale exponent  "Expression for physical CGS unitsU_t^-2 [ s^-2 ]Lossy compression filterNone Value stored as physical& Property can be converted to comovingBConversion factor to CGS (not including cosmological corrections) ?@4 4?GConversion factor to physical CGS (including cosmological corrections) ?@4 4?FHIBwd`:Q`FHDBs DescriptionLocal velocity divergence field around the particles. Provided without cosmology, as this includes the Hubble flow. To return to a peculiar velocity divergence, div . v_pec = a^2 (div . v - n_D H)FHDBs8 U_M exponent   U_L exponent   U_t exponent   U_I exponent   U_T exponent  h-scale exponent  a-scale exponent  "Expression for physical CGS unitsU_t^-1 [ s^-1 ]Lossy compression filterNone Value stored as physical& Property can be converted to comovingBConversion factor to CGS (not including cosmological corrections) ?@4 4?GConversion factor to physical CGS (including cosmological corrections) ?@4 4?FHIBslhPFHDBhB3v DescriptionMLaplacian (del squared) of the Internal Energy per unit mass of the particlesFHDBhB8 U_M exponent   U_L exponent   U_t exponent   U_I exponent   U_T exponent  h-scale exponent  a-scale exponent  "Expression for physical CGS unitsa^-4 U_t^-2 [ s^-2 ]Lossy compression filterNone Value stored as physical& Property can be converted to comovingBConversion factor to CGS (not including cosmological corrections) ?@4 4?GConversion factor to physical CGS (including cosmological corrections) ?@4 4?FHIBhBuq{tFHDB Mr Description3Diffusion coefficient (alpha_diff) of the particlesFHDB kE U_M exponent   U_L exponent   U_t exponent   U_I exponent   U_T exponent  h-scale exponent  a-scale exponent  "Expression for physical CGS units[ - ] Lossy compression filterNone Value stored as physical& Property can be converted to comovingBConversion factor to CGS (not including cosmological corrections) ?@4 4?GConversion factor to physical CGS (including cosmological corrections) ?@4 4?FHIB N}NyR#FHDB!N DescriptionTVisosity coefficient (alpha_visc) of the particles, multiplied by the balsara switchFHDB!Q U_M exponent   U_L exponent   U_t exponent   U_I exponent   U_T exponent  h-scale exponent  a-scale exponent  "Expression for physical CGS units[ - ] Lossy compression filterNone Value stored as physical& Property can be converted to comovingBConversion factor to CGS (not including cosmological corrections) ?@4 4?GConversion factor to physical CGS (including cosmological corrections) ?@4 4?FHIB!RFHDBpGConversion factor to physical CGS (including cosmological corrections) ?@4 4?FHDBZ' U_M exponent  ? U_L exponent   U_t exponent   U_I exponent   U_T exponent  h-scale exponent  a-scale exponent  "Expression for physical CGS units(a^-5 U_M U_L^-1 U_t^-2 [ g cm^-1 s^-2 ]Lossy compression filterNone Value stored as physical& Property can be converted to comovingBConversion factor to CGS (not including cosmological corrections) ?@4 4? Description$Co-moving pressures of the particlesFHIBY oFHDB Coordinates VelocitieseMassesSmoothingLengths"InternalEnergies$ ParticleIDs] Densities Entropies6 PressuresoViscosityParametersDiffusionParameters$LaplacianInternalEnergiesq'VelocityDivergences A#VelocityDivergenceTimeDifferentialsLE Potentialsmz Softenings׫ProgenitorParticleIDs SplitCounts SplitTrees FHDBKGConversion factor to physical CGS (including cosmological corrections) ?@4 4?FHDBCfQ U_M exponent  * U_L exponent  @ U_t exponent   U_I exponent   U_T exponent  h-scale exponent  a-scale exponent  "Expression for physical CGS units1U_M^-0.6667 U_L^4 U_t^-2 [ g^-0.6667 cm^4 s^-2 ]Lossy compression filterNone Value stored as physical& Property can be converted to comovingBConversion factor to CGS (not including cosmological corrections) ?@4 4? Description2Co-moving entropies per unit mass of the particlesFHIB9FHDB^ Description)Co-moving mass densities of the particlesFHDB7 U_M exponent  ? U_L exponent  @ U_t exponent   U_I exponent   U_T exponent  h-scale exponent  a-scale exponent  @"Expression for physical CGS unitsa^-3 U_M U_L^-3 [ g cm^-3 ]Lossy compression filterNone Value stored as physical& Property can be converted to comovingBConversion factor to CGS (not including cosmological corrections) ?@4 4?GConversion factor to physical CGS (including cosmological corrections) ?@4 4?FHIB&&gFHDB,Ł DescriptionUnique IDs of the particlesFHDB,Dk U_M exponent   U_L exponent   U_t exponent   U_I exponent   U_T exponent  h-scale exponent  a-scale exponent  "Expression for physical CGS units[ - ] Lossy compression filterNone Value stored as physical& Property can be converted to comovingBConversion factor to CGS (not including cosmological corrections) ?@4 4?GConversion factor to physical CGS (including cosmological corrections) ?@4 4?FHIB,\\Mh!FHDBR_GConversion factor to physical CGS (including cosmological corrections) ?@4 4?FHDBR_ U_M exponent   U_L exponent  @ U_t exponent   U_I exponent   U_T exponent  h-scale exponent  a-scale exponent  "Expression for physical CGS units a^-2 U_L^2 U_t^-2 [ cm^2 s^-2 ]Lossy compression filterNone Value stored as physical& Property can be converted to comovingBConversion factor to CGS (not including cosmological corrections) ?@4 4? Description9Co-moving thermal energies per unit mass of the particlesFHIBR_ߕFHDB[wVx DescriptionACo-moving smoothing lengths (FWHM of the kernel) of the particlesFHDB[+ U_M exponent   U_L exponent  ? U_t exponent   U_I exponent   U_T exponent  h-scale exponent  a-scale exponent  ?"Expression for physical CGS units a U_L [ cm ]Lossy compression filterNone Value stored as physical& Property can be converted to comovingBConversion factor to CGS (not including cosmological corrections) ?@4 4?GConversion factor to physical CGS (including cosmological corrections) ?@4 4?FHIB[ȸȴ~ FHDB#yi DescriptionMasses of the particlesFHDB#* U_M exponent  ? U_L exponent   U_t exponent   U_I exponent   U_T exponent  h-scale exponent  a-scale exponent  "Expression for physical CGS units U_M [ g ]Lossy compression filterNone Value stored as physical& Property can be converted to comovingBConversion factor to CGS (not including cosmological corrections) ?@4 4?GConversion factor to physical CGS (including cosmological corrections) ?@4 4?FHIB#FntFHDBzO DescriptioniPeculiar velocities of the stars. This is (a * dx/dt) where x is the co-moving positions of the particlesFHDBU ' U_M exponent   U_L exponent  ? U_t exponent   U_I exponent   U_T exponent  h-scale exponent  a-scale exponent  "Expression for physical CGS unitsU_L U_t^-1 [ cm s^-1 ]Lossy compression filterNone Value stored as physical& Property can be converted to comovingBConversion factor to CGS (not including cosmological corrections) ?@4 4?GConversion factor to physical CGS (including cosmological corrections) ?@4 4?FHIB44ZmdFHDBa6b~ Description$Co-moving positions of the particlesFHDBau U_M exponent   U_L exponent  ? U_t exponent   U_I exponent   U_T exponent  h-scale exponent  a-scale exponent  ?"Expression for physical CGS units a U_L [ cm ]Lossy compression filterNone Value stored as physical& Property can be converted to comovingBConversion factor to CGS (not including cosmological corrections) ?@4 4?GConversion factor to physical CGS (including cosmological corrections) ?@4 4?FHIBajjѐزFHDBc9,n/HeaderCode+PolicyPhysicalConstants HydroSchemeQ" SubgridScheme CosmologyC. Parameters8UnusedParameters8RecordingTriggersIUnits'JInternalCodeUnits%LCells#N PartType01 GasParticles /PartType0FHDB:\RRestarts:lustre_OST_checks0Restarts:lustre_OST_free0Restarts:lustre_OST_test0Restarts:delta_hours5Scheduler:tasks_per_cell0Scheduler:links_per_tasks25Scheduler:mpi_message_limit4FHDB:1 x$TimeIntegration:dt_RMS_use_gas_only0Statistics:scale_factor_first0.1Statistics:time_first0MetaData:run_nameUntitled SWIFT simulationRestarts:stop_steps100Restarts:max_run_time 3.40282e+38Restarts:resubmit_on_exit0Scheduler:nr_queues1%Scheduler:dependency_graph_frequency0 Scheduler:dependency_graph_cell0&Scheduler:task_level_output_frequency0"Scheduler:deadlock_waiting_time_s-1Statistics:energy_file_name statisticsStatistics:timestep_file_name timestepsSnapshots:output_list_on0Statistics:output_list_on0Restarts:enable1Restarts:save1Restarts:onexit0FHDB:HXsSnapshots:run_on_dump0Snapshots:compression0Snapshots:distributed0Snapshots:lustre_OST_checks0Snapshots:lustre_OST_free0Snapshots:lustre_OST_test0Snapshots:invoke_stf0Snapshots:invoke_fof0Snapshots:invoke_ps0Snapshots:use_delta_from_edge0 FOF:dump_catalogue_when_seeding0Snapshots:UnitMass_in_cgs1Snapshots:UnitLength_in_cgs1Snapshots:UnitVelocity_in_cgs1Snapshots:UnitCurrent_in_cgs1Snapshots:UnitTemp_in_cgs1&Scheduler:free_foreign_during_restart0&Scheduler:free_foreign_during_rebuild0$TimeIntegration:max_nr_rt_subcycles0"TimeIntegration:max_dt_RMS_factor0.25FHDB:z;Scheduler:cell_extra_sparts200Scheduler:cell_extra_gparts200Scheduler:cell_extra_bparts0Scheduler:cell_extra_sinks0%Scheduler:engine_max_parts_per_ghost1000&Scheduler:engine_max_sparts_per_ghost1000'Scheduler:engine_max_parts_per_cooling10000%Scheduler:engine_redist_alloc_margin1.2&Scheduler:engine_foreign_alloc_margin1.05+InitialConditions:smoothing_length_scaling1)InitialConditions:stars_smoothing_length-1/InitialConditions:black_holes_smoothing_length-1InitialConditions:shift  [0, 0, 0]Snapshots:scale_factor_first0.1Snapshots:subdir.Snapshots:subsample [0, 0, 0, 0, 0, 0, 0]Snapshots:subsample_fraction [0, 0, 0, 0, 0, 0, 0]FHDB: Ӷ#Scheduler:cell_sub_size_pair_stars 256000000#Scheduler:cell_sub_size_self_stars32000"Scheduler:cell_sub_size_pair_grav 256000000"Scheduler:cell_sub_size_self_grav32000Scheduler:cell_split_size400Scheduler:grid_split_threshold400"Scheduler:cell_subdepth_diff_grav4'Scheduler:cell_recurse_size_self_hydro100'Scheduler:cell_recurse_size_pair_hydro100'Scheduler:cell_recurse_size_self_stars100'Scheduler:cell_recurse_size_pair_stars100-Scheduler:cell_recurse_size_self_black_holes100-Scheduler:cell_recurse_size_pair_black_holes100'Scheduler:cell_recurse_size_self_sinks100'Scheduler:cell_recurse_size_pair_sinks100Scheduler:cell_extra_parts0FHDB:\SPH:viscosity_alpha_max2SPH:viscosity_alpha_min0SPH:viscosity_length0.05SPH:diffusion_alpha0SPH:diffusion_beta1SPH:diffusion_alpha_max1SPH:diffusion_alpha_min0SPH:particle_splitting0SPH:convert_particles_at_h_max0&InitialConditions:metadata_group_nameICs_parametersNeutrino:use_delta_f0Neutrino:use_delta_f_mesh_only0Neutrino:use_model_none0Neutrino:generate_ics0Neutrino:neutrino_seed0Neutrino:use_linear_response0Scheduler:max_top_level_cells12Scheduler:cell_max_size8000000#Scheduler:cell_sub_size_pair_hydro 256000000#Scheduler:cell_sub_size_self_hydro32000FHDB: ܹRestarts:basenameswiftPhysicalConstants:G 6.6743e-08PhysicalConstants:mu_00.125664InitialConditions:replicate1,InitialConditions:cleanup_smoothing_lengths0$InitialConditions:cleanup_h_factors0+InitialConditions:cleanup_velocity_factors0&InitialConditions:generate_gas_in_ics0InitialConditions:remap_ids0SPH:h_tolerance0.0001 SPH:h_max 3.40282e+38SPH:h_min_ratio0SPH:max_ghost_iterations30SPH:use_mass_weighted_num_ngb0SPH:max_volume_change1.4SPH:initial_temperature0SPH:minimal_temperature0SPH:H_ionization_temperature10000SPH:H_mass_fraction0.752SPH:viscosity_alpha0.1FHDB:¢!#InternalUnitSystem:UnitMass_in_cgs1%InternalUnitSystem:UnitLength_in_cgs1'InternalUnitSystem:UnitVelocity_in_cgs1&InternalUnitSystem:UnitCurrent_in_cgs1#InternalUnitSystem:UnitTemp_in_cgs1TimeIntegration:time_begin0.TimeIntegration:time_end0.2TimeIntegration:dt_min1e-7TimeIntegration:dt_max1e-2Snapshots:basenamesodShockSnapshots:time_first0.Snapshots:delta_time0.2Statistics:delta_time1e-2SPH:resolution_eta1.2348SPH:CFL_condition0.1InitialConditions:file_name./sodShock.hdf5InitialConditions:periodic1Snapshots:select_output_on0Restarts:subdirrestartFHIB:=ݯ)FHDB0!T_CMB_0 [internal units] ?@4 4w_0 ?@4 4w_a ?@4 4w ?@4 4 Redshift ?@4 4 Scale-factor ?@4 4?"Critical density [internal units] ?@4 43Critical density at redshift zero [internal units] ?@4 4%Mean matter density [internal units] ?@4 4'Mean baryonic density [internal units] ?@4 4Virial overdensity (BN98) ?@4 4FHDB0Omega_b ?@4 4Omega_k ?@4 4 Omega_lambda ?@4 4 Omega_nu ?@4 4 Omega_nu_0 ?@4 4 Omega_ur ?@4 4 Omega_cdm ?@4 4Omega_g ?@4 4T_nu_0 [internal units] ?@4 4 T_nu_0 [eV] ?@4 4N_eff ?@4 4N_ur ?@4 4 N_nu  deg_nu_tot ?@4 4 T_CMB_0 [K] ?@4 4FHDB0| Cosmological run a_beg ?@4 4?a_end ?@4 4?time_beg [internal units] ?@4 4time_end [internal units] ?@4 4Universe age [internal units] ?@4 4Lookback time [internal units] ?@4 4h ?@4 4?H0 [internal units] ?@4 4H [internal units] ?@4 4Hubble time [internal units] ?@4 4Omega_m ?@4 4Omega_r ?@4 4FHIB0'FHDB&Eg)Alpha viscosity (min)  (Viscosity decay length [internal units]  L=Beta viscosity  @@Diffusion alpha  Diffusion alpha (max)  ?Diffusion alpha (min)  Diffusion beta  ?Thermal Conductivity Model#Simple treatment as in Price (2008)Viscosity Model,Simplified version of Cullen & Denhen (2011)FHDB&3}Volume log(max(delta h))  F>Volume max change time-step  33? Max ghost iterations Minimal temperature  .Minimal energy per unit mass [internal units]  Initial temperature  .Initial energy per unit mass [internal units]  Hydrogen mass fraction  @?+Hydrogen ionization transition temperature  @F/ Maximal time-bin difference between neighbours Alpha viscosity  =Alpha viscosity (max)  @FHDB&@r}Adiabatic index  UU?Pressure floornoneEquation of state Ideal gas Dimension Neighbour number definition unweightedSchemeSPHENIX (Borrow+ 2020) MHD Scheme No MHD schemeKernel functionCubic spline (M4)Kernel target N_ngb  @Kernel delta N_ngb  L9 Kernel eta   ? Kernel gamma  ٳ?Smoothing length tolerance  8*Maximal smoothing length [internal units]  CFL parameter  = MHD FlavourNo MHDFHIB&, ,,lpFHDB]#Oastronomical_unit ?@4 4`16Bparsec ?@4 4 CiC light_year ?@4 4Gt.BC solar_radius ?@4 420B earth_radius ?@4 4A solar_mass ?@4 4ƞsPF earth_mass ?@4 41l0LEsolar_luminosity ?@4 4KㄗFT_CMB_0 ?@4 4@primordial_He_fraction ?@4 4X9v?reduced_hubble ?@4 4wM< caseb_recomb ?@4 4nb]KR=FHDB]#12 newton_G ?@4 4Eq>speed_light_c ?@4 4B planck_h ?@4 4lQYg: planck_hbar ?@4 47{PT: boltzmann_k ?@4 4O<avogadro_number ?@4 4WʅDthomson_cross_section ?@4 43F:stefan_boltzmann ?@4 4GLХ ?electron_charge ?@4 4S )ڤ<electron_volt ?@4 4@/|=electron_mass ?@4 4o R:vacuum_permeability ?@4 4s<? proton_mass ?@4 4"6-;year ?@4 4S~AFHIB]#bbk@FHDBG1rastronomical_unit ?@4 4`16Bparsec ?@4 4 CiC light_year ?@4 4Gt.BC solar_radius ?@4 420B earth_radius ?@4 4A solar_mass ?@4 4ƞsPF earth_mass ?@4 41l0LEsolar_luminosity ?@4 4KㄗFT_CMB_0 ?@4 4@primordial_He_fraction ?@4 4X9v?reduced_hubble ?@4 4wM< caseb_recomb ?@4 4nb]KR=FHDBGwMk newton_G ?@4 4Eq>speed_light_c ?@4 4B planck_h ?@4 4lQYg: planck_hbar ?@4 47{PT: boltzmann_k ?@4 4O<avogadro_number ?@4 4WʅDthomson_cross_section ?@4 43F:stefan_boltzmann ?@4 4GLХ ?electron_charge ?@4 4S )ڤ<electron_volt ?@4 4@/|=electron_mass ?@4 4o R:vacuum_permeability ?@4 4s<? proton_mass ?@4 4"6-;year ?@4 4S~AFHIBG/FHDBq&Em feedback  black holes  fof search  time-step limiter  time-step sync  csds  line of sight  sink  rt  power spectra  moving mesh  moving mesh hydro  no_io FHDBq@W~ steal  keep  block  cpu tight  mpi  numa affinity  hydro  self gravity  external gravity  cosmological integration  drift everything  reconstruct multi-poles  temperature  cooling  stars  structure finding  star formation FHIBq$ ŠFHDB)Go! MPI libraryNon-MPI version of SWIFT RandomSeed FHDBpCodeSWIFT Code Version2026.01Compiler Name LLVM/ClangCompiler Version19.0.0 Git Branch(HEAD detached at 9972efde1) Git Revisionv2026.01-192-g9972efde Git Date2026-02-19 18:00:25 +0100Configuration optionsa'--with-hydro-dimension=1 --with-parmetis --enable-debugging-checks --disable-vec --enable-debug'CFLAGS'-g -O0 -debug inline-debug-info -O3 -ansi-alias -fma -ftz -fomit-frame-pointer -march=core-avx2 -mavx2 -no-vec -Qunused-arguments -pthread -Wall -Wextra -Wno-unused-parameter -Wshadow -Werror -Wstrict-prototypes'HDF5 library version1.14.4Thread barrierspthread Allocators!Compiler version (probably glibc)FFTW library version3.x (details not available)GSL library version2.8FHIB-)#SFHDB} CanHaveTypes  ZoomIn  OutputType FullVolumeFHDB~8( NumPart_Total_HighWord  TotalNumberOfParticles@ NumParticles_InCells@ NumParticles_OutsideCells@ MassTable ?@4 4InitialMassTable ?@4 4@zT? Flag_Entropy_ICs  NumFilesPerSnapshot  ThisFile  SelectOutputDefault Virtual FHDB>4BoxSize ?@4 4@@@Time ?@4 4 Dimension  Redshift ?@4 4 Scale-factor ?@4 4?CodeSWIFTRunNameUntitled SWIFT simulationSystemga003.pri.cosma.localShift ?@4 4 NumPartTypes TimeBase_dloga ?@4 4 TimeBase_dt ?@4 49< SnapshotDate20:51:44 2026-02-19 GMT NumPart_ThisFile@ NumPart_Total FHIB:9:5:1ċ