HDF
F ` TREE H1 ( h 2 q g 8 x A 0 = 0 ` ٝ ! ( i X v X# Q 8 p HEAP x ,G . Consistent Trees_columns scale(0) id(1) desc_scale(2) desc_id(3) num_prog(4) pid(5) upid(6) desc_pid(7) phantom(8) sam_Mvir(9) Mvir(10) Rvir(11) rs(12) vrms(13) mmp?(14) scale_of_last_MM(15) vmax(16) x(17) y(18) z(19) vx(20) vy(21) vz(22) Jx(23) Jy(24) Jz(25) Spin(26) Breadth_first_ID(27) Depth_first_ID(28) Tree_root_ID(29) Orig_halo_ID(30) Snap_idx(31) Next_coprogenitor_depthfirst_ID(32) Last_progenitor_depthfirst_ID(33) Last_mainleaf_depthfirst_ID(34) Tidal_Force(35) Tidal_ID(36) Rs_Klypin(37) Mvir_all(38) M200b(39) M200c(40) M500c(41) M2500c(42) Xoff(43) Voff(44) Spin_Bullock(45) b_to_a(46) c_to_a(47) A[x](48) A[y](49) A[z](50) b_to_a(500c)(51) c_to_a(500c)(52) A[x](500c)(53) A[y](500c)(54) A[z](500c)(55) T/|U|(56) M_pe_Behroozi(57) M_pe_Diemer(58) Halfmass_Radius(59) rvmax(60) Macc(61) Mpeak(62) Vacc(63) Vpeak(64) Halfmass_Scale(65) Acc_Rate_Inst(66) Acc_Rate_100Myr(67) Acc_Rate_1*Tdyn(68) Acc_Rate_2*Tdyn(69) Acc_Rate_Mpeak(70) Acc_Log_Vmax_Inst(71) Acc_Log_Vmax_1*Tdyn(72) Mpeak_Scale(73) Acc_Scale(74) First_Acc_Scale(75) First_Acc_Mvir(76) First_Acc_Vmax(77) Vmax\@Mpeak(78) Tidal_Force_Tdyn(79) Log_(Vmax/Vmax_max(Tdyn;Tmpeak))(80) Time_to_future_merger(81) Future_merger_MMP_ID(82) Consistent Trees_metadata #scale(0) id(1) desc_scale(2) desc_id(3) num_prog(4) pid(5) upid(6) desc_pid(7) phantom(8) sam_Mvir(9) Mvir(10) Rvir(11) rs(12) vrms(13) mmp?(14) scale_of_last_MM(15) vmax(16) x(17) y(18) z(19) vx(20) vy(21) vz(22) Jx(23) Jy(24) Jz(25) Spin(26) Breadth_first_ID(27) Depth_first_ID(28) Tree_root_ID(29) Orig_halo_ID(30) Snap_idx(31) Next_coprogenitor_depthfirst_ID(32) Last_progenitor_depthfirst_ID(33) Last_mainleaf_depthfirst_ID(34) Tidal_Force(35) Tidal_ID(36) Rs_Klypin(37) Mvir_all(38) M200b(39) M200c(40) M500c(41) M2500c(42) Xoff(43) Voff(44) Spin_Bullock(45) b_to_a(46) c_to_a(47) A[x](48) A[y](49) A[z](50) b_to_a(500c)(51) c_to_a(500c)(52) A[x](500c)(53) A[y](500c)(54) A[z](500c)(55) T/|U|(56) M_pe_Behroozi(57) M_pe_Diemer(58) Halfmass_Radius(59) rvmax(60) Macc(61) Mpeak(62) Vacc(63) Vpeak(64) Halfmass_Scale(65) Acc_Rate_Inst(66) Acc_Rate_100Myr(67) Acc_Rate_1*Tdyn(68) Acc_Rate_2*Tdyn(69) Acc_Rate_Mpeak(70) Acc_Log_Vmax_Inst(71) Acc_Log_Vmax_1*Tdyn(72) Mpeak_Scale(73) Acc_Scale(74) First_Acc_Scale(75) First_Acc_Mvir(76) First_Acc_Vmax(77) Vmax\@Mpeak(78) Tidal_Force_Tdyn(79) Log_(Vmax/Vmax_max(Tdyn;Tmpeak))(80) Time_to_future_merger(81) Future_merger_MMP_ID(82)
#Omega_M = 0.308900; Omega_L = 0.691100; h0 = 0.677400
#Full box size = 2000.000000 Mpc/h
#Scale: Scale factor of halo.
#ID: ID of halo (unique across entire simulation).
#Desc_Scale: Scale of descendant halo, if applicable.
#Descid: ID of descendant halo, if applicable.
#Num_prog: Number of progenitors.
#Pid: ID of least massive host halo (-1 if distinct halo).
#Upid: ID of most massive host halo (different from Pid when the halo is within two or more larger halos).
#Desc_pid: Pid of descendant halo (if applicable).
#Phantom: Nonzero for halos interpolated across timesteps.
#SAM_Mvir: Halo mass, smoothed across accretion history; always greater than sum of halo masses of contributing progenitors (Msun/h). Only for use with select semi-analytical models.
#Mvir: Halo mass (Msun/h).
#Rvir: Halo radius (kpc/h comoving).
#Rs: Scale radius (kpc/h comoving).
#Vrms: Velocity dispersion (km/s physical).
#mmp?: whether the halo is the most massive progenitor or not.
#scale_of_last_MM: scale factor of the last major merger (Mass ratio > 0.3).
#Vmax: Maxmimum circular velocity (km/s physical).
#X/Y/Z: Halo position (Mpc/h comoving).
#VX/VY/VZ: Halo velocity (km/s physical, peculiar).
#JX/JY/JZ: Halo angular momenta ((Msun/h) * (Mpc/h) * km/s (physical)).
#Spin: Halo spin parameter.
#Breadth_first_ID: breadth-first ordering of halos within a tree.
#Depth_first_ID: depth-first ordering of halos within a tree.
#Tree_root_ID: ID of the halo at the last timestep in the tree.
#Orig_halo_ID: Original halo ID from halo finder.
#Snap_idx: Index of snapshot (in original snapshot list) from which halo originated.
#Next_coprogenitor_depthfirst_ID: Depthfirst ID of next coprogenitor.
#Last_progenitor_depthfirst_ID: Depthfirst ID of last progenitor.
#Last_mainleaf_depthfirst_ID: Depthfirst ID of last progenitor on main progenitor branch.
#Tidal_Force: Strongest tidal force from any nearby halo, in dimensionless units (Rhalo / Rhill).
#Tidal_ID: ID of halo exerting strongest tidal force.
#Rs_Klypin: Scale radius determined using Vmax and Mvir (see Rockstar paper)
#Mvir_all: Mass enclosed within the specified overdensity, including unbound particles (Msun/h)
#M200b--M2500c: Mass enclosed within specified overdensities (Msun/h)
#Xoff: Offset of density peak from average particle position (kpc/h comoving)
#Voff: Offset of density peak from average particle velocity (km/s physical)
#Spin_Bullock: Bullock spin parameter (J/(sqrt(2)*MVR))
#b_to_a, c_to_a: Ratio of second and third largest shape ellipsoid axes (B and C) to largest shape ellipsoid axis (A) (dimensionless).
# Shapes are determined by the method in Allgood et al. (2006).
# (500c) indicates that only particles within R500c are considered.
#A[x],A[y],A[z]: Largest shape ellipsoid axis (kpc/h comoving)
#T/|U|: ratio of kinetic to potential energies
#M_pe_*: Pseudo-evolution corrected masses (very experimental)
#Halfmass_Radius rvmax: Radius within which 1/2 of Mvir is enclosed.
#Consistent Trees Version 1.01
#Macc,Vacc: Mass and Vmax at accretion.
#Mpeak,Vpeak: Peak mass and Vmax over mass accretion history.
#Halfmass_Scale: Scale factor at which the MMP reaches 0.5*Mpeak.
#Acc_Rate_*: Halo mass (or log10 vmax) accretion rates in Msun/h/yr (or dex/yr).
# Inst: instantaneous; 100Myr: averaged over past 100Myr,
# X*Tdyn: averaged over past X*virial dynamical time.
# Mpeak: Growth Rate of Mpeak, averaged from current z to z+0.5
# Log_Vmax: Growth Rate of Log10(Vmax)
#Mpeak_Scale: Scale at which Mpeak was reached.
#Acc_Scale: Scale at which satellites were (last) accreted.
#First_Acc_Scale: Scale at which current and former satellites first passed through a larger halo.
#First_Acc_(Mvir|Vmax): Mvir and Vmax at First_Acc_Scale.
#Vmax@Mpeak: Halo Vmax at the scale at which Mpeak was reached.
#Tidal_Force_Tdyn: Dimensionless tidal force averaged over past dynamical time.
#Log_(Vmax/Vmax_max(Tdyn;TMpeak)): Log10 of Vmax_now over Vmax@(Tdyn ago) OR Vmax@Mpeak (if and only if Mpeak happened > 1Tdyn ago).
#Time_to_future_merger: Time (in Gyr) until the given halo merges into a larger halo. (-1 if no future merger happens)
#Future_merger_MMP_ID: most-massive progenitor of the halo into which the given halo merges. (-1 if the main progenitor of the future merger halo does not exist at the given scale factor.)
@ Consistent Trees_version 1.01 H
HDF5_version GCOL 1.10.1 2.10.0 H
h5py_version @ input_catalog_type Consistent Trees H input_filedatestamp ? @ 4 4 A P input_filename ' All100.hdf5/hlist_00000023_0.09549.list 8
TotNhalos @ ? @ 4 4 deflate 2 Cc P SNOD 80 JH x_ ( cv TREE
: x^5w\Mlj]ƽum}EEML
!(e3|eM%~sVsJ/;#Ÿ5o\Cn맽OZwy60.y8
|..)OΟѼu)>^0tx@1+*fs~+S1
#ŗ]/Q ~U[6̞,:_+0_'7}^c>_ 2t1L1Y!k\]Gp۴b=ulm";(zԸKHؖoFgH@XilO!Z$êҝ᭙q.
xCbO쇨6f$yܺԕ>d~nNg܉UCȭb 9Uu_'XϚ{*>(q 9MCy^I mƍ[qփqf[Z2˿N_)3VMQ!L5'm Ėl*yhܤU)}dzg#RU|t+LJ1_$A@mrGcj8_{$
)vLS~SzVk
6G͇F>\xu؋اns^&zyk|֛T`⯟&0OwJ}><9Jя)J7Ma>W
wU56 <#ǯ҂`3>Yx(u5
RGgX
_rpꡝtʟ
e,/H|r$HhOK<;;("/)E1\NRǫ;2gOc RMGRB"_I釒
`V2
^
ǩ#E%̀_¬r8ٕעeVO$NBzʒF(.>_VV-eގ^1z] c_pd2RUhqh4: 1-5cl4˪EJب2Vaz%[\_m/\As+te"0cצiQ.2)Wݜ:͖txs]}92j)q m9hko!eCVGEb'3w[%wyXI/&s娱u
@t"},I)j(
FLwbw!~,Wx]Nj7z
Mͥ=]я ' ޞD>j:bhۄfa F wʿFK]ɈnDլ7Mp 5ZG\Q;朩N [vh7t*jK~ƪjȹ~o]O4B]*P
PIȗsw \]h^jJdW+fɻ!,q':D~\]dJP>\C@zh.ݠOR7˱W99ua7/7ԙ<;rABxذf>`y]Lfab0W~xu3y˺8v
?zKa@vm2zg<:)r4j} oL߶st9[p~ǼA;9d64 FϫcW W|P 6iq#F0?Q@f>1/nUb;Vc1- .6?{
IѪ_Q>kQ^zUN~FO{_ 0"xQ:;rciOmbi-;t
Kl,6xg
b=r;jBǻх&G_o7as壗_72nF5n2)>Zƞ*`vN]|Z@tr>iyAqtrd$ی՝դ#FD:&K3^Vsjz"!O</gm2HDF# Hٶ4j)8+&bs>q'52 %D4}ٕB'RDP#Ĉ/KOo SA&3tA$TRMȓb$ݕԝnyƛ-4*` Ŷl_@
"Qz
2&/>K`Efz^@F̱-}*ai(GO5>Kgt71{H ? @ 4 4 deflate ZI Cc P TREE
Q x^5y4trw "o+,Z<7|OX0)je6m$l}oo|=w)4JѺ(>TIɉe[D0pt1'[)ͽ:[n
r^f%AQ >qzKԑADX3/$P-)a ſ؟ɂ
.ec qp8z=r!#TzW<}KŦpvS onG gNAeëlo}0{M\h\
mSBt-=
Q1@C<ָ7CGhS<3LE}YcԢu<t~
p(
CDP7C)\*lMDPӶ2,0C$M
)-s_gduI5?M!wq\01Er
ES7ֻjꪨ,V|b+6@vKt+Q~%|>'z=Óݽ
'77͇ZkJ2U5y3d}Cɻ>Zl9 C^=]yf.ІK^\krpSg96|c0XX΄}$
nuv5^1`>)JwyZ8sokWdu@pYsHz-cn="'X4y?n7YJ>,3Rq
MY"pc7l
z[G Oſ`waણRWjFwn:r*IB]Y`?Sʥ>r*gĭ *+0L|ތO:a|#δj{
hh0w^{PXZ9.}ĕJD_|lRVt@;:,-.2CުMMTc0Unw
_w'j"ohFYوXtA>Aٗ)pOiBKvorMó38֠Aa^t7v0VGE
DȬM!byR&~Vk
z+d&zݵ6~ccԀEYW'Q6
w^rBȦtߢE;,b֕PlX1(bY] }hwzDm>hY%$3S 'XF[P<`FR#gx݊GNG0.NS4,,"xp03dǻ,@W5.{7+cܦ
x]v^~_C
|qR-0[|-VGpЏYȤzy}:pc%uE;BȽhh1F-#k1Ф\o/(L7B#7(m>_f]|j_/ٯtXƯp/9
[;X![Kj{
LypU#6Z@禼 )d,('"[S44]NhRtͧ]- p7![O$|sB닸hh%.oîi/qX`0g/|s`nͧQ3}M}
\1Tn
XՆ
a}sD_Jzp@ŤЂ+YA6)('PULE(@%af(m
V1KƤ&4P}S]v`V|˚/mi2n#KjnK Ie{J$]b#V` vǫ=Nu
w*uCJ.JHUe NFz:$W16*_&͆<S4LR1@uwI2;ɇkYguHAc;-tޗ,+PRz"lͻڞc4K{ocIm ީ"9½HsTry[:)8]FW_{܉HSowZj-P#R[_C&&y4B(|ɑ >}'F;$˖
;>`hJf)!/2ͥj/SУd{oNډh[ ["'#ZnN1sAGL=_:&|g
K2г:<0lep2-@3Rn eF=i)|*8>CǯlhքVI,@ʋY,H-)Pߩ0S B:e}EnsɎbXvd&uWai#"#gkPj , 2n#B REGddJ
ClX@6 ,צspm ZE۠EA '?)(S潻2!(
H,Y()|qW+sY LÄ&S4`S:
{63g6j:RM6Y41PmNRGPGq9wA0yw+y#PBެ;.meC p-,
'1eNF`E`Ib>N5M?{Wy}K
%m/\ya䧘4Ɇ
+k*H+9zX2Xe-Re,OX^qlpӲ6P+F
4^;({m$ȲU+fi"SEH.ñ?ߍ!_qP>vPF,OTDsB@!aPі+_R~/|tPO/=,5paz9ձcԂKH9u#b!;XEa]I#A<_E]W8tn {db#NXHya9>G;dZ&+Pr
n{JUZvN