format (written as headers in the above catalog):
# (1)ID (2,3)RA,DEC(J2000)[deg]
# (4--19)quantities from photo-z catalog:
# --- (4,5,6)median,1sigma lower,1sigma upper limits of photo-z measured using the galaxy templates[zPDF,zPDF_l68,zPDF_u68]
# --- (7)best fit template at zPDF[1--8:Ell-S0, 9--15:Sa-Sc, 16--19:Sd-Sdm from Polletta et al., >=20:starburst from BC03]
# --- (8)best-fit additional extinction E(B-V) at zPDF[mag]
# --- (9)extinction law[1:prevot, 2:Calzetti, 3,4:Calzetti+2175bump]
# --- (10)number of filters used in the fit
# --- (11)best-fit BC03 model (12)best-fit model age[yr] (13)best-fit model extinction E(B-V)[mag]
# --- (14,15,16)log10[Mstar/Msun] for median,1sigma lower,1sigma upper[mass_med,mass_inf,mass_sup]
# --- (17,18,19)log10[SFR/(Msun/yr)] for median,1sigma lower,1sigma upper[sfr_med,sfr_inf,sfr_sup]
# (20)auto-offset[mag](aperture correction from 3" diameter aperture magnitude to total magnitude, band independent)
# (21+2i,22+2i)mag, 1sigma error of mag corrected for Galactic extinction and offset[i=0--36]:
# --- i= 0 (21,22)CFHT u*
# --- i= 1 (23,24)Subaru B
# --- i= 2 (25,26)Subaru V
# --- i= 3 (27,28)Subaru g'
# --- i= 4 (29,30)Subaru r'
# --- i= 5 (31,32)Subaru i'
# --- i= 6 (33,34)CFHT i*
# --- i= 7 (35,36)Subaru z'
# --- i= 8 (37,38)UKIRT J
# --- i= 9 (39,40)CTIO/KPNO Ks
# --- i=10 (41,42)CFHT Ks
# --- i=11 (43,44)Subaru IA427
# --- i=12 (45,46)Subaru IA464
# --- i=13 (47,48)Subaru IA484
# --- i=14 (49,50)Subaru IA505
# --- i=15 (51,52)Subaru IA527
# --- i=16 (53,54)Subaru IA574
# --- i=17 (55,56)Subaru IA624
# --- i=18 (57,58)Subaru IA679
# --- i=19 (59,60)Subaru IA709
# --- i=20 (61,62)Subaru IA738
# --- i=21 (63,64)Subaru IA767
# --- i=22 (65,66)Subaru IA827
# --- i=23 (67,68)Subaru NB711
# --- i=24 (69,70)Subaru NB816
# --- i=25 (71,72)Spitzer IRAC ch1
# --- i=26 (73,74)Spitzer IRAC ch2
# --- i=27 (75,76)Spitzer IRAC ch3
# --- i=28 (77,78)Spitzer IRAC ch4
# --- i=29 (79,80)GALEX FUV
# --- i=30 (81,82)GALEX NUV
# --- i=31 (83,84)UltraVISTA Y
# --- i=32 (85,86)UltraVISTA J
# --- i=33 (87,88)UltraVISTA H
# --- i=34 (89,90)UltraVISTA Ks
# --- i=35 (91,92)CFHT H
# --- i=36 (93,94)Subaru z''
# (95--100)AGN-related flags:
# --- ( 95)flag for detection in all 4 IRAC bands[0:no, 1:yes]
# --- ( 96)flags for AGN from IRAC color[Donley+12 criteria][0:non-AGN, 1:AGN]
# --- ( 97)flags for AGN from Chandra[0:non-AGN, 1:AGN]
# --- ( 98)flags for AGN from XMM-Newton[0:non-AGN, 1:AGN]
# --- ( 99)flags for AGN from VLA[0:non-AGN, 1:AGN]
# --- (100)flags for AGN from one of them[0:non-AGN, 1:AGN]
# (101--149)Step 1 related quantities:
# --- (101+4i)flag of excess IA band for 12 IA-bands[0:non-excess, others:excess][i=0--11]
# --- (102+4i)IAc[ABmag][i=0--11]
# --- (103+4i)IAc-IA[ABmag][i=0--11]
# --- (104+4i)3sigma(IAc-IA)[ABmag][i=0--11]
# ------ i= 0 (101,102,103,104)IA427
# ------ i= 1 (105,106,107,108)IA464
# ------ i= 2 (109,110,111,112)IA484
# ------ i= 3 (113,114,115,116)IA505
# ------ i= 4 (117,118,119,120)IA527
# ------ i= 5 (121,122,123,124)IA574
# ------ i= 6 (125,126,127,128)IA624
# ------ i= 7 (129,130,131,132)IA679
# ------ i= 8 (133,134,135,136)IA709
# ------ i= 9 (137,138,139,140)IA738
# ------ i=10 (141,142,143,144)IA767
# ------ i=11 (145,146,147,148)IA827
# --- (149)N_ex^temp
# (150--195)Step 2 related quantities:
# --- (150)Nsol
# --- (151--166)quantities related to the primary z_ph solution:
# ------ (151)P(z_ph1)
# ------ (152)chi_nu^2(z_ph1)
# ------ (153)z_ph1
# ------ (154--165)line ID for 12 IA bands(1:Lya, 2:CIV, 3:CIII], 4:MgII, 5:[OII], 6:[OIII]+Hb, 7:Ha+[NII], 99:others)
# ------ (166)N_ex^cons
# --- (167--182)quantities related to the secondary z_ph solution:
# ------ (167)P(z_ph2)/P(z_ph1)
# ------ (168)chi_nu^2(z_ph2)
# ------ (169)z_ph2
# ------ (170--181)line ID for 12 IA bands(1:Lya, 2:CIV, 3:CIII], 4:MgII, 5:[OII], 6:[OIII]+Hb, 7:Ha+[NII], 99:others)
# ------ (182)N_ex^cons
# --- (183--194)flag for 12 IA bands[0:undetected, 1:detected]
# --- (195)N_undetectedIA
# (196--410+13*(N_ex^cons-1))Step 3 related quantities:
# --- (196,197)zph,4pi*d_L^2(zph)[cm^2]
# --- (198,199,200)chi2, reduced chi2, Nband used in the SED fitting
# --- (201+4i,202+4i,203+4i,204+4i)flag for the band used in the SED fitting[0:unused,1:used], mag, 1sigma fainter,brighter error of mag(i=0--36)
# ------ (201,202,203,204)CFHT u*
# ------ (205,206,207,208)Subaru B
# ------ (209,210,211,212)Subaru V
# ------ (213,214,215,216)Subaru g'
# ------ (217,218,219,220)Subaru r'
# ------ (221,222,223,224)Subaru i'
# ------ (225,226,227,228)CFHT i*
# ------ (229,230,231,232)Subaru z'
# ------ (233,234,235,236)UKIRT J
# ------ (237,238,239,240)CTIO/KPNO Ks
# ------ (241,242,243,244)CFHT Ks
# ------ (245,246,247,248)Subaru IA427
# ------ (249,250,251,252)Subaru IA464
# ------ (253,254,255,256)Subaru IA484
# ------ (257,258,259,260)Subaru IA505
# ------ (261,262,263,264)Subaru IA527
# ------ (265,266,267,268)Subaru IA574
# ------ (269,270,271,272)Subaru IA624
# ------ (273,274,275,276)Subaru IA679
# ------ (277,278,279,280)Subaru IA709
# ------ (281,282,283,284)Subaru IA738
# ------ (285,286,287,288)Subaru IA767
# ------ (289,290,291,292)Subaru IA827
# ------ (293,294,295,296)Subaru NB711
# ------ (297,298,299,300)Subaru NB816
# ------ (301,302,303,304)Spitzer IRAC ch1
# ------ (305,306,307,308)Spitzer IRAC ch2
# ------ (309,310,311,312)Spitzer IRAC ch3
# ------ (313,314,315,316)Spitzer IRAC ch4
# ------ (317,318,319,320)GALEX FUV
# ------ (321,322,323,324)GALEX NUV
# ------ (325,326,327,328)UltraVISTA Y
# ------ (329,330,331,332)UltraVISTA J
# ------ (333,334,335,336)UltraVISTA H
# ------ (337,338,339,340)UltraVISTA Ks
# ------ (341,342,343,344)CFHT H
# ------ (345,346,347,348)Subaru z''
# --- (349,350)ID and name of the best-fit SED template
# --- (351--355)best-fit value, ID and value of the 1sigma-lower,upper limit's SED template for normalization
# --- (356--360)best-fit value, ID and value of the 1sigma-lower,upper limit's SED template for age[Gyr]
# --- (361--365)best-fit value, ID and value of the 1sigma-lower,upper limit's SED template for e-folding time[Gyr]
# --- (366--370)best-fit value, ID and value of the 1sigma-lower,upper limit's SED template for stellar metallicity
# --- (371--375)best-fit value, ID and value of the 1sigma-lower,upper limit's SED template for Av[mag]
# --- (376--380)best-fit value, ID and value of the 1sigma-lower,upper limit's SED template for E(B-V)[mag]
# --- (381--385)best-fit value, ID and value of the 1sigma-lower,upper limit's SED template for Mstar[Msun]
# --- (386--390)best-fit value, ID and value of the 1sigma-lower,upper limit's SED template for SFR(SED)[Msun/yr]
# --- (391--395)best-fit value, ID and value of the 1sigma-lower,upper limit's SED template for SFR(UV)[Msun/yr]
# --- (396)N_ex^cons
# --- (397)N_ex
# --- (398--410+13i)quantities related to emission lines(i=0--N_ex^cons-1)
# ------ (398+13i)excess IA band
# ------ (399+13i)emission line identified in Step 2
# ------ (400+13i)IAc-IA[ABmag] evaluated using frequency-matched continuum in Step 1
# ------ (401--403+13i)IAc-IA[ABmag] evaluated using best-fit,1sigma-lower,1sigma-upper SED templates
# ------ (404--406+13i)best-fit,1sigma-lower,1sigma-upper line luminosity[erg/s]
# ------ (407--409+13i)best-fit,1sigma-lower,1sigma-upper rest-frame EW[A]
# ------ (410+13i)3sigma-lower limit for rest-frame EW[A]
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Step3_LAE_all.dat 
