# # Galform code version information # iversion = [ 2, 6, 0,463] branchname = full_revision_name = stable compiled_by = j.c.helly@durham.ac.uk compiled_time = Thu Nov 6 14:00:20 UTC 2014 # # Maximum number of trees in any mass interval # ntreemax = 100 # # Actual output redshifts # zout_act = [ \ 6.140 ] # # Details of the filters used in the run: # # 1 = UA 1500A (1350-1650A) top-hat filter # A0-AB offset: -2.500 0 =Rest Frame # lambda_eff= 1.4900E+03 # 2 = UC COMBO-17 2800A (2600-3000A) top-hat filter # A0-AB offset: -1.546 0 =Rest Frame # lambda_eff= 2.7905E+03 # 3 = U RGO U # A0-AB offset: -0.903 0 =Rest Frame # lambda_eff= 3.5069E+03 # 4 = B RGO CCD B # A0-AB offset: 0.117 0 =Rest Frame # lambda_eff= 4.3691E+03 # 5 = V RGO CCD V # A0-AB offset: 0.008 0 =Rest Frame # lambda_eff= 5.4038E+03 # 6 = R RGO CCD R(Kron-Cousins) # A0-AB offset: -0.226 0 =Rest Frame # lambda_eff= 6.6557E+03 # 7 = I RGO CCD I(Kron-Cousins) # A0-AB offset: -0.430 0 =Rest Frame # lambda_eff= 8.1017E+03 # 8 = K UKIRT K filter # A0-AB offset: -1.870 0 =Rest Frame # lambda_eff= 2.1968E+04 # 9 = BJ Couch and Newell (80) BJ (photographic) fi # A0-AB offset: 0.089 0 =Rest Frame # lambda_eff= 4.4815E+03 # 10 = U RGO U # A0-AB offset: -0.903 1 =Observers Frame # lambda_eff= 3.5069E+03 # 11 = B RGO CCD B # A0-AB offset: 0.117 1 =Observers Frame # lambda_eff= 4.3691E+03 # 12 = V RGO CCD V # A0-AB offset: 0.008 1 =Observers Frame # lambda_eff= 5.4038E+03 # 13 = R RGO CCD R(Kron-Cousins) # A0-AB offset: -0.226 1 =Observers Frame # lambda_eff= 6.6557E+03 # 14 = I RGO CCD I(Kron-Cousins) # A0-AB offset: -0.430 1 =Observers Frame # lambda_eff= 8.1017E+03 # 15 = K UKIRT K filter # A0-AB offset: -1.870 1 =Observers Frame # lambda_eff= 2.1968E+04 # 16 = BJ Couch and Newell (80) BJ (photographic) fi # A0-AB offset: 0.089 1 =Observers Frame # lambda_eff= 4.4815E+03 # 17 = uS SDSS u standard (filter+CCD +1.3 air mass) # A0-AB offset: -0.910 0 =Rest Frame # lambda_eff= 3.5513E+03 # 18 = gS SDSS g standard (filter+CCD +1.3 air mass) # A0-AB offset: 0.100 0 =Rest Frame # lambda_eff= 4.6862E+03 # 19 = rS SDSS r standard (filter+CCD +1.3 air mass) # A0-AB offset: -0.138 0 =Rest Frame # lambda_eff= 6.1658E+03 # 20 = iS SDSS i standard (filter+CCD +1.3 air mass) # A0-AB offset: -0.355 0 =Rest Frame # lambda_eff= 7.4812E+03 # 21 = zS SDSS z standard (filter+CCD +1.3 air mass) # A0-AB offset: -0.512 0 =Rest Frame # lambda_eff= 8.9317E+03 # 22 = uS SDSS u standard (filter+CCD +1.3 air mass) # A0-AB offset: -0.910 1 =Observers Frame # lambda_eff= 3.5513E+03 # 23 = gS SDSS g standard (filter+CCD +1.3 air mass) # A0-AB offset: 0.100 1 =Observers Frame # lambda_eff= 4.6862E+03 # 24 = rS SDSS r standard (filter+CCD +1.3 air mass) # A0-AB offset: -0.138 1 =Observers Frame # lambda_eff= 6.1658E+03 # 25 = iS SDSS i standard (filter+CCD +1.3 air mass) # A0-AB offset: -0.355 1 =Observers Frame # lambda_eff= 7.4812E+03 # 26 = zS SDSS z standard (filter+CCD +1.3 air mass) # A0-AB offset: -0.512 1 =Observers Frame # lambda_eff= 8.9317E+03 # 27 = V RGO CCD V # A0-AB offset: 0.008 2 =Weighted Age # lambda_eff= 5.4038E+03 # 28 = V RGO CCD V # A0-AB offset: 0.008 3 =Weighted Metallicity # lambda_eff= 5.4038E+03 # 29 = BL Bolometric luminosity # A0-AB offset: 0.000 0 =Rest Frame # lambda_eff= -9.9900E+02 # 30 = LC Lyman continuum photons # A0-AB offset: 0.000 0 =Rest Frame # lambda_eff= -9.9900E+02 # 31 = SM Stellar mass # A0-AB offset: 0.000 0 =Rest Frame # lambda_eff= -9.9900E+02 # 32 = SM Stellar mass # A0-AB offset: 0.000 2 =Weighted Age # lambda_eff= -9.9900E+02 # 33 = B0 200-290 A top hat # A0-AB offset: -45.626 0 =Rest Frame # lambda_eff= 2.3944E+02 # 34 = B1 290-420 A top hat # A0-AB offset: -44.417 0 =Rest Frame # lambda_eff= 3.4700E+02 # 35 = B2 420-620 A top hat # A0-AB offset: -37.730 0 =Rest Frame # lambda_eff= 5.0707E+02 # 36 = B3 620-900 A top hat # A0-AB offset: -23.461 0 =Rest Frame # lambda_eff= 7.4268E+02 # 37 = B4 900-1200 A top hat # A0-AB offset: -11.286 0 =Rest Frame # lambda_eff= 1.0356E+03 # 38 = B5 1200-1600 A top hat # A0-AB offset: -2.973 0 =Rest Frame # lambda_eff= 1.3809E+03 # 39 = B6 1600-2100 A top hat # A0-AB offset: -2.005 0 =Rest Frame # lambda_eff= 1.8274E+03 # 40 = B7 2100-2800 A top hat # A0-AB offset: -1.814 0 =Rest Frame # lambda_eff= 2.4165E+03 # 41 = B8 2800-3800 A top hat # A0-AB offset: -1.203 0 =Rest Frame # lambda_eff= 3.2492E+03 # 42 = B9 3800-5700 A top hat # A0-AB offset: 0.072 0 =Rest Frame # lambda_eff= 4.6223E+03 # 43 = C0 5700-8600 A top hat # A0-AB offset: -0.260 0 =Rest Frame # lambda_eff= 6.9523E+03 # 44 = C1 8600-13000 A top hat # A0-AB offset: -0.654 0 =Rest Frame # lambda_eff= 1.0499E+04 # 45 = C2 13000-20000 A top hat # A0-AB offset: -1.299 0 =Rest Frame # lambda_eff= 1.6000E+04 # 46 = C3 20000-40000 A top hat # A0-AB offset: -2.208 0 =Rest Frame # lambda_eff= 2.7726E+04 # 47 = C4 40000-80000 A top hat # A0-AB offset: -3.535 0 =Rest Frame # lambda_eff= 5.5452E+04 # 48 = UB 1500A (1300-1700)A FUV top-hat filter # A0-AB offset: -2.539 0 =Rest Frame # lambda_eff= 1.4820E+03 # 49 = UD 2200A (1800-2600)A NUV top-hat filter # A0-AB offset: -1.897 0 =Rest Frame # lambda_eff= 2.1507E+03 # 50 = GF GALEX_FUV_filter # A0-AB offset: -2.397 0 =Rest Frame # lambda_eff= 1.5320E+03 # 51 = GN GALEX_NUV_filter # A0-AB offset: -1.841 0 =Rest Frame # lambda_eff= 2.2865E+03 # 52 = UB 1500A (1300-1700)A FUV top-hat filter # A0-AB offset: -2.539 1 =Observers Frame # lambda_eff= 1.4820E+03 # 53 = UD 2200A (1800-2600)A NUV top-hat filter # A0-AB offset: -1.897 1 =Observers Frame # lambda_eff= 2.1507E+03 # 54 = GF GALEX_FUV_filter # A0-AB offset: -2.397 1 =Observers Frame # lambda_eff= 1.5320E+03 # 55 = GN GALEX_NUV_filter # A0-AB offset: -1.841 1 =Observers Frame # lambda_eff= 2.2865E+03 # 56 = A2 UV flux 1500A # A0-AB offset: -2.443 0 =Rest Frame # lambda_eff= 1.4983E+03 # 57 = A2 UV flux 1500A # A0-AB offset: -2.443 1 =Observers Frame # lambda_eff= 1.4983E+03 nband = 57 bandname = [ \ UA 1500A (1350-1650A) top-hat filter, \ UC COMBO-17 2800A (2600-3000A) top-hat filter, \ U RGO U, \ B RGO CCD B, \ V RGO CCD V, \ R RGO CCD R(Kron-Cousins), \ I RGO CCD I(Kron-Cousins), \ K UKIRT K filter, \ BJ Couch and Newell (80) BJ (photographic) fi, \ U RGO U, \ B RGO CCD B, \ V RGO CCD V, \ R RGO CCD R(Kron-Cousins), \ I RGO CCD I(Kron-Cousins), \ K UKIRT K filter, \ BJ Couch and Newell (80) BJ (photographic) fi, \ uS SDSS u standard (filter+CCD +1.3 air mass), \ gS SDSS g standard (filter+CCD +1.3 air mass), \ rS SDSS r standard (filter+CCD +1.3 air mass), \ iS SDSS i standard (filter+CCD +1.3 air mass), \ zS SDSS z standard (filter+CCD +1.3 air mass), \ uS SDSS u standard (filter+CCD +1.3 air mass), \ gS SDSS g standard (filter+CCD +1.3 air mass), \ rS SDSS r standard (filter+CCD +1.3 air mass), \ iS SDSS i standard (filter+CCD +1.3 air mass), \ zS SDSS z standard (filter+CCD +1.3 air mass), \ V RGO CCD V, \ V RGO CCD V, \ BL Bolometric luminosity, \ LC Lyman continuum photons, \ SM Stellar mass, \ SM Stellar mass, \ B0 200-290 A top hat, \ B1 290-420 A top hat, \ B2 420-620 A top hat, \ B3 620-900 A top hat, \ B4 900-1200 A top hat, \ B5 1200-1600 A top hat, \ B6 1600-2100 A top hat, \ B7 2100-2800 A top hat, \ B8 2800-3800 A top hat, \ B9 3800-5700 A top hat, \ C0 5700-8600 A top hat, \ C1 8600-13000 A top hat, \ C2 13000-20000 A top hat, \ C3 20000-40000 A top hat, \ C4 40000-80000 A top hat, \ UB 1500A (1300-1700)A FUV top-hat filter, \ UD 2200A (1800-2600)A NUV top-hat filter, \ GF GALEX_FUV_filter, \ GN GALEX_NUV_filter, \ UB 1500A (1300-1700)A FUV top-hat filter, \ UD 2200A (1800-2600)A NUV top-hat filter, \ GF GALEX_FUV_filter, \ GN GALEX_NUV_filter, \ A2 UV flux 1500A, \ A2 UV flux 1500A ] bandid = [ UA, UC, U , B , V , R , I , K , BJ, U , B , V , R , I , K , BJ, uS, gS, rS, iS, zS, uS, gS, rS, iS, zS, V , V , BL, LC, SM, SM, B0, B1, B2, B3, B4, B5, B6, B7, B8, B9, C0, C1, C2, C3, C4, UB, UD, GF, GN, UB, UD, GF, GN, A2, A2] iselect = [ 0, 0, 0, 0, 0, 0, 0, 0, 0, 1, 1, 1, 1, 1, 1, 1, 0, 0, 0, 0, 0, 1, 1, 1, 1, 1, 2, 3, 0, 0, 0, 2, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 1, 1, 1, 1, 0, 1] a0_ab = [ -0.2500E+01, -0.1546E+01, -0.9031E+00, 0.1166E+00, 0.7930E-02, -0.2259E+00, -0.4300E+00, -0.1870E+01, 0.8878E-01, -0.9031E+00, 0.1166E+00, 0.7930E-02, -0.2259E+00, -0.4300E+00, -0.1870E+01, 0.8878E-01, -0.9105E+00, 0.1001E+00, -0.1376E+00, -0.3549E+00, -0.5117E+00, -0.9105E+00, 0.1001E+00, -0.1376E+00, -0.3549E+00, -0.5117E+00, 0.7930E-02, 0.7930E-02, 0.0000E+00, 0.0000E+00, 0.0000E+00, 0.0000E+00, -0.4563E+02, -0.4442E+02, -0.3773E+02, -0.2346E+02, -0.1129E+02, -0.2973E+01, -0.2005E+01, -0.1814E+01, -0.1203E+01, 0.7200E-01, -0.2599E+00, -0.6535E+00, -0.1299E+01, -0.2208E+01, -0.3535E+01, -0.2539E+01, -0.1897E+01, -0.2397E+01, -0.1841E+01, -0.2539E+01, -0.1897E+01, -0.2397E+01, -0.1841E+01, -0.2443E+01, -0.2443E+01] lambda_eff = [ 0.1490E+04, 0.2790E+04, 0.3507E+04, 0.4369E+04, 0.5404E+04, 0.6656E+04, 0.8102E+04, 0.2197E+05, 0.4482E+04, 0.3507E+04, 0.4369E+04, 0.5404E+04, 0.6656E+04, 0.8102E+04, 0.2197E+05, 0.4482E+04, 0.3551E+04, 0.4686E+04, 0.6166E+04, 0.7481E+04, 0.8932E+04, 0.3551E+04, 0.4686E+04, 0.6166E+04, 0.7481E+04, 0.8932E+04, 0.5404E+04, 0.5404E+04, -0.9990E+03, -0.9990E+03, -0.9990E+03, -0.9990E+03, 0.2394E+03, 0.3470E+03, 0.5071E+03, 0.7427E+03, 0.1036E+04, 0.1381E+04, 0.1827E+04, 0.2417E+04, 0.3249E+04, 0.4622E+04, 0.6952E+04, 0.1050E+05, 0.1600E+05, 0.2773E+05, 0.5545E+05, 0.1482E+04, 0.2151E+04, 0.1532E+04, 0.2287E+04, 0.1482E+04, 0.2151E+04, 0.1532E+04, 0.2287E+04, 0.1498E+04, 0.1498E+04] # # Emission lines calculated: # # Lyalpha lambda= 0.1216E+04 -0.8000E+02 0.1000E+03 0.8000E+02 0.1000E+03 # Halpha lambda= 0.6563E+04 -0.8000E+02 0.1000E+03 0.8000E+02 0.1000E+03 # Hbeta lambda= 0.4862E+04 -0.8000E+02 0.1000E+03 0.8000E+02 0.1000E+03 # OII3727 lambda= 0.3727E+04 -0.8000E+02 0.1000E+03 0.8000E+02 0.1000E+03 # emlines = T nline = 4 linename = [ Lyalpha, Halpha, Hbeta, OII3727] lambda_line = [ 0.1216E+04, 0.6563E+04, 0.4862E+04, 0.3727E+04] lam_off_ctm1 = [ -0.8000E+02, -0.8000E+02, -0.8000E+02, -0.8000E+02] lam_width_ctm1 = [ 0.1000E+03, 0.1000E+03, 0.1000E+03, 0.1000E+03] lam_off_ctm2 = [ 0.8000E+02, 0.8000E+02, 0.8000E+02, 0.8000E+02] lam_width_ctm2 = [ 0.1000E+03, 0.1000E+03, 0.1000E+03, 0.1000E+03] # # No molecular emission lines were calculated in this model # emlines = F nmolline = 0 # # Bazaar revision numbers of extensions # massfunc = 3 merging = 20