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[[FrontPage]] * Step 3 Catalog of 1052 LAE candidates, 4734 low-z emitter candidates, and 354 others selected in Step 2: &ref(Step3_LAE_all.dat); &ref(Step3_lowz_all.dat); &ref(Step3_others.dat); [#aacbedd3] - 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--112)flag for 12 IA bands[0:undetected, 1:detected] # (113)N_undetectedIA # (114--162)Step 1 related quantities: # --- (114+4i)flag of excess IA band for 12 IA-bands[-1:unjudged, 0:non-excess, others:excess][i=0--11] # --- (115+4i)IAc[ABmag][i=0--11] # --- (116+4i)IAc-IA[ABmag][i=0--11] # --- (117+4i)3sigma(IAc-IA)[ABmag][i=0--11] # ------ i= 0 (114,115,116,117)IA427 # ------ i= 1 (118,119,120,121)IA464 # ------ i= 2 (122,123,124,125)IA484 # ------ i= 3 (126,127,128,129)IA505 # ------ i= 4 (130,131,132,133)IA527 # ------ i= 5 (134,135,136,137)IA574 # ------ i= 6 (138,139,140,141)IA624 # ------ i= 7 (142,143,144,145)IA679 # ------ i= 8 (146,147,148,149)IA709 # ------ i= 9 (150,151,152,153)IA738 # ------ i=10 (154,155,156,157)IA767 # ------ i=11 (158,159,160,161)IA827 # --- (162)N_ex^temp # (163--195)Step 2 related quantities: # --- (163)Nsol # --- (164--179)quantities related to the primary z_ph solution: # ------ (164)P(z_ph1) # ------ (165)chi_nu^2(z_ph1) # ------ (166)z_ph1 # ------ (167--178)line ID for 12 IA bands(1:Lya, 2:CIV, 3:CIII], 4:MgII, 5:[OII], 6:[OIII]+Hb, 7:Ha+[NII], 99:others) # ------ (179)N_ex^cons # --- (180--195)quantities related to the secondary z_ph solution: # ------ (180)P(z_ph2)/P(z_ph1) # ------ (181)chi_nu^2(z_ph2) # ------ (182)z_ph2 # ------ (183--194)line ID for 12 IA bands(1:Lya, 2:CIV, 3:CIII], 4:MgII, 5:[OII], 6:[OIII]+Hb, 7:Ha+[NII], 99:others) # ------ (195)N_ex^cons # (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] ** Figures and data of the SED for 1052 LAE candidates: [#j65bebe3] - [[SEDs of all of the 1052 LAE candidates:http://cosmos.phys.sci.ehime-u.ac.jp/~kobayashi/files/SED_LAE_all.pdf]] -- [[2 component (stellar + AGN) SEDs of all of the 1052 LAE candidates:http://cosmos.phys.sci.ehime-u.ac.jp/~kobayashi/files/SED2comp.pdf]] - [[SED data of all the 1052 LAE candidates:http://cosmos.phys.sci.ehime-u.ac.jp/~kobayashi/files/SED_LAE.tar.gz]] - SEDs of the 35 AGN LAEs -- [[in ascending order of zph:http://cosmos.phys.sci.ehime-u.ac.jp/~kobayashi/files/SED_LAE_AGN_zph.pdf]] -- [[in descending order of best-fit stellar mass:http://cosmos.phys.sci.ehime-u.ac.jp/~kobayashi/files/SED_LAE_AGN_Mstar.pdf]] -- [[in descending order of best-fit rest-frame EW(Lya):http://cosmos.phys.sci.ehime-u.ac.jp/~kobayashi/files/SED_LAE_AGN_EW0.pdf]] - SEDs of the 735 star-forming LAEs -- [[in ascending order of zph:http://cosmos.phys.sci.ehime-u.ac.jp/~kobayashi/files/SED_LAE_nonAGN_zph.pdf]] -- [[in descending order of best-fit stellar mass:http://cosmos.phys.sci.ehime-u.ac.jp/~kobayashi/files/SED_LAE_nonAGN_Mstar.pdf]] -- [[in descending order of best-fit rest-frame EW(Lya):http://cosmos.phys.sci.ehime-u.ac.jp/~kobayashi/files/SED_LAE_nonAGN_EW0.pdf]] - SEDs of the 52 star-forming LAEs with EW0(Lya) >= 100 A -- [[in descending order of best-fit stellar mass:http://cosmos.phys.sci.ehime-u.ac.jp/~kobayashi/files/SED_LAE_nonAGN_sLAE_Mstar.pdf]] ** Figures and data of the SED for 4734 low-z emitter candidates: [#v6fcb6df] - [[SEDs of all of the 4734 low-z emitter candidates:http://cosmos.phys.sci.ehime-u.ac.jp/~kobayashi/files/SED_lowz_all.pdf]] -- [[in ascending order of zph:http://cosmos.phys.sci.ehime-u.ac.jp/~kobayashi/files/SED_lowz_all_zph.pdf]] -- [[in ascending order of χ_ν^2:http://cosmos.phys.sci.ehime-u.ac.jp/~kobayashi/files/SED_lowz_all_chinu2.pdf]] -- [[in descending order of best-fit stellar mass:http://cosmos.phys.sci.ehime-u.ac.jp/~kobayashi/files/SED_lowz_all_Mstar.pdf]] - [[SED data of all the 4734 low-z emitter candidates:http://cosmos.phys.sci.ehime-u.ac.jp/~kobayashi/files/SED_lowz.tar.gz]] ** Figures and data of the SED for 354 others selected in Step 2: [#zba783ef] - [[SEDs of all of the 354 others:http://cosmos.phys.sci.ehime-u.ac.jp/~kobayashi/files/SED_others.pdf]] - [[SED data of all of the 354 others:http://cosmos.phys.sci.ehime-u.ac.jp/~kobayashi/files/SED_others.tar.gz]]
