Transfer-Step3-Catalogs のバックアップ(No.13)

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• Transfer-Step3-Catalogs は削除されています。
  • 1 (2015-08-31 (月) 22:09:43)
  • 2 (2015-10-02 (金) 03:16:27)
  • 3 (2015-10-05 (月) 23:03:09)
  • 4 (2015-10-06 (火) 10:13:41)
  • 5 (2015-10-15 (木) 14:15:03)
  • 6 (2015-10-15 (木) 15:25:58)
  • 7 (2015-10-16 (金) 16:33:58)
  • 8 (2015-10-23 (金) 17:49:00)
  • 9 (2015-10-23 (金) 17:50:10)
  • 10 (2015-10-26 (月) 12:07:53)
  • 11 (2015-11-10 (火) 12:36:04)
  • 12 (2015-11-10 (火) 19:37:35)
  • 13 (2022-08-09 (火) 08:03:25)
  • 14 (2022-08-11 (木) 23:51:17)

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Step 3 Catalog of 1052 LAE candidates, 4734 low-z emitter candidates, and 354 others selected in Step 2: Step3_LAE_all.dat Step3_lowz_all.dat Step3_others.dat †

• 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

• HD Film izle

# (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*

• HD Film izle

#  ------ (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]

• HD Film izle

#  --- (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: †

• SEDs of all of the 1052 LAE candidates
  • 2 component (stellar + AGN) SEDs of all of the 1052 LAE candidates
• SED data of all the 1052 LAE candidates
• SEDs of the 35 AGN LAEs
  • in ascending order of zph
  • in descending order of best-fit stellar mass
  • in descending order of best-fit rest-frame EW(Lya)
• SEDs of the 735 star-forming LAEs
  • in ascending order of zph
  • in descending order of best-fit stellar mass
  • in descending order of best-fit rest-frame EW(Lya)
• SEDs of the 52 star-forming LAEs with EW0(Lya) >= 100 A
  • in descending order of best-fit stellar mass
• HD Film izle

Figures and data of the SED for 4734 low-z emitter candidates: †

• SEDs of all of the 4734 low-z emitter candidates
  • in ascending order of zph
  • in ascending order of χ_ν^2
  • in descending order of best-fit stellar mass
• SED data of all the 4734 low-z emitter candidates

Figures and data of the SED for 354 others selected in Step 2: †

• SEDs of all of the 354 others
• SED data of all of the 354 others

     

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