J/A+A/392/1 Spectrophotometry of simulated Stellar Populations (Schulz+, 2002)
Spectral & photometric evolution of Simple Stellar Populations at
various metallicities
Schulz J., Fritze-v.Alvensleben U., Moeller C.S.
<Astron. Astrophys. 392, 1 (2002)>
=2002A&A...392....1S 2002A&A...392....1S
ADC_Keywords: Clusters, globular ; Clusters, open ; Models, evolutionary ;
Spectrophotometry ; Colors
Keywords: globular clusters: general, open clusters and associations: general,
Galaxies: star clusters, Galaxies: evolution
Abstract:
A new set of evolutionary synthesis spectra are presented for Simple
Stellar Populations (SSPs) covering ranges in metallicity from
0.02≤Z/Z☉≤2.5 and ages from 4*106yr≤t≤16Gyr. They are
based on the most recent isochrones from the Padova group that extend
earlier models by the inclusion of the thermal pulsing AGB phase for
stars in the mass range 2M☉≤m≤7M☉ in accordance with the
fuel consumption theorem. We show that with respect to earlier models,
inclusion of the TP-AGB phase leads to significant changes in the
(V-I) and (V-K) colors of SSPs in the age range from 108 to
≳109yr. Using model atmosphere spectra from Lejeune et al. (1997,
Cat. J/A+AS/125/229, 1998, Cat. J/A+AS/130/65), we calculate the
spectral evolution of single burst populations of various
metallicities covering the wavelength range from 90Å through
160µm. Isochrone spectra are convolved with filter response
functions to describe the time evolution of luminosities and colors in
Johnson, Thuan & Gunn, Koo, HST, Washington and Stroemgren filters.
The models and their results are not only intended for use in the
interpretation of star clusters but also for combination with any kind
of dynamical galaxy formation and/or evolution model that contains a
star formation criterion. Moreover, the evolution of these single
burst single metallicity stellar populations is readily folded with
any kind of star formation -- and eventually chemical enrichment --
history to describe the evolutionary spectral synthesis of composite
stellar populations like galaxies of any type with continuous or
discontinuous star formation. For these latter purposes we also
present the time evolution of ejection rates for gas and metals for
two different Initial Mass Functions (IMFs) as well as cosmological
and evolutionary corrections for all the filters as a function of
redshift for 0≤z≤5 and two different cosmologies.
Description:
Spectra, colors and luminosities in various filter-systems as well as
cosmological and evolutionary corrections in 2 different cosmologies
(H0=75, Ω0=0.1, Λ0=0.9) (H0=65, {Omega0}=0.1,
{Lambda0}=0.0). The total mass in stars of all SPSs are 1.6*109
solar masses at the beginning of evolution. The time-step is
4*106years. The UBV filters are from Buser & Kurucz (1978A&A....70..555B 1978A&A....70..555B),
the RI filter from Bessell (1990PASP..102.1181B 1990PASP..102.1181B) and JHK from Bessel &
Brett (1988PASP..100.1134B 1988PASP..100.1134B).
Files are following the naming-convention:
sa* = SSP with Salpeter IMF
sc* = SSP with Scalo IMF
The metallicities considered are:
Z1 = 0.0004 = 0.02Z☉
Z2 = 0.004 = 0.20Z☉
Z3 = 0.008 = 0.40Z☉
Z4 = 0.02 = 1.00Z☉
Z5 = 0.05 = 2.50Z☉
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
sajohn.dat 194 500 Luminosities and colors from the spectra in
Johnson filter-system, Salpeter IMF
scjohn.dat 194 500 Luminosities and colors from the spectra in
Johnson filter-system, Scalo IMF
samag.dat 156 500 Luminosities from the spectra in Koo,
Thuan & Gunn, Washington and Stroemgren
filter-systems, Salpeter IMF
scmag.dat 156 500 Luminosities from the spectra in Koo,
Thuan & Gunn, Washington and Stroemgren
filter-systems, Scalo IMF
sahst.dat 224 500 Luminosities from the spectra in HST
filter-system, Salpeter IMF
schst.dat 224 500 Luminosities from the spectra in HST
filter-system, Scalo IMF
saspect.dat 1226 6105 Spectra, with Salpeter IMF
scspect.dat 1226 6105 Spectra, with Scalo IMF
saplot1.dat 113 17505 Salpeter IMF isochrone intrinsic colors, part 1
scplot1.dat 113 17505 Scalo IMF isochrone intrinsic colors, part 1
saplot2.dat 112 17505 Salpeter IMF isochrone intrinsic colors, part 2
scplot2.dat 112 17505 Scalo IMF isochrone intrinsic colors, part 2
saplot3.dat 112 17505 Salpeter IMF isochrone intrinsic colors, part 3
scplot3.dat 112 17505 Scalo IMF isochrone intrinsic colors, part 3
saplot4.dat 152 17505 Salpeter IMF isochrone intrinsic colors, part 4
scplot4.dat 152 17505 Scalo IMF isochrone intrinsic colors, part 4
scecoeff.dat 385 650 Coefficients of e-correction in luminosity,
Scalo IMF
saecoeff.dat 385 650 Coefficients of e-correction in luminosity,
Salpeter IMF
sckcoeff.dat 385 650 Coefficients of k-correction in luminosity,
Scalo IMF
sakcoeff.dat 385 650 Coefficients of k-correction in luminosity,
Salpeter IMF
sckatt.dat 385 650 Coefficients of k-correction with attenuation
in luminosity, Scalo IMF
sakatt.dat 385 650 Coefficients of k-correction with attenuation
in luminosity, Salpeter IMF
--------------------------------------------------------------------------------
See also:
http://www.uni-sw.gwdg.de/~galev : The Goettingen Galaxy Evolution Group
VI/102 : Geneva stellar evolution tracks and isochrones (Lejeune+ 2001)
J/A+AS/125/229 : A standard stellar library (Lejeune+ 1997)
J/A+AS/130/65 : A standard stellar library. II. (Lejeune+ 1998)
J/A+AS/106/275 : Theoretical isochrones (Bertelli+ 1994)
J/A+AS/141/371 : Low-mass stars evolutionary tracks+isochrones (Girardi+, 2000)
J/A+AS/100/647 : Evolutionary Sequences II. (Bressan+ 1993)
J/A+AS/104/365 : Evolutionary sequences. III. (Fagotto+ 1994)
J/A+AS/105/29 : Evolutionary sequences IV. (Fagotto+ 1994)
J/A+AS/105/39 : Evolutionary sequences V. (Fagotto+ 1994)
J/A+AS/117/113 : Evolutionary stellar models. VI. Z=0.0001 (Girardi+, 1996)
Byte-by-byte Description of file: sajohn.dat scjohn.dat
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Bytes Format Units Label Explanations
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1- 6 F6.4 --- Z Metallicity (0.0004 0.004 0.008 0.02 0.05)
8- 13 I6 --- J Index
16- 26 E11.5 yr Age Age of system
29- 35 F7.3 mag Umag Johnson U magnitude
38- 44 F7.3 mag Bmag Johnson B magnitude
47- 53 F7.3 mag Vmag Johnson V magnitude
56- 62 F7.3 mag Rmag Johnson R magnitude
65- 71 F7.3 mag Imag Johnson I magnitude
74- 80 F7.3 mag Jmag Johnson J magnitude
83- 89 F7.3 mag Hmag Johnson H magnitude
92- 98 F7.3 mag Kmag Johnson K magnitude
101-107 F7.3 mag Lmag Johnson L magnitude
109-114 F6.3 mag U-B Johnson U-B color index
117-122 F6.3 mag B-V Johnson B-V color index
125-130 F6.3 mag U-V Johnson U-V color index
133-138 F6.3 mag V-R Johnson V-R color index
141-146 F6.3 mag R-I Johnson R-I color index
149-154 F6.3 mag V-K Johnson V-K color index
157-162 F6.3 mag I-K Johnson I-K color index
165-170 F6.3 mag B-R Johnson B-R color index
173-178 F6.3 mag B-H Johnson B-H color index
181-186 F6.3 mag J-H Johnson J-H color index
189-194 F6.3 mag H-K Johnson H-K color index
--------------------------------------------------------------------------------
Byte-by-byte Description of file: samag.dat scmag.dat
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Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 6 F6.4 --- Z Metallicity (0.0004 0.004 0.008 0.02 0.05)
8- 13 I6 --- J Index
16- 26 E11.5 yr Age Age of system
29- 35 F7.3 mag ukmag Koo u magnitude
38- 44 F7.3 mag jkmag Koo j magnitude
47- 53 F7.3 mag fkmag Koo f magnitude
56- 62 F7.3 mag nkmag Koo n magnitude
65- 71 F7.3 mag gmag Thuan & Gunn g magnitude
74- 80 F7.3 mag rmag Thuan & Gunn r magnitude
82- 88 F7.3 mag Cmag Washington C magnitude
92- 98 F7.3 mag Mmag Washington M magnitude
102-108 F7.3 mag T1mag Washington T1 magnitude
112-118 F7.3 mag T2mag Washington T2 magnitude
120-126 F7.3 mag umag Stroemgren u magnitude
130-136 F7.3 mag vmag Stroemgren v magnitude
140-146 F7.3 mag bmag Stroemgren b magnitude
150-156 F7.3 mag ymag Stroemgren y magnitude
--------------------------------------------------------------------------------
Byte-by-byte Description of file: sahst.dat schst.dat
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Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 6 F6.4 --- Z Metallicity (0.0004 0.004 0.008 0.02 0.05)
8- 13 I6 --- J Index
16- 26 E11.5 yr Age Age of system
30- 37 F8.4 mag F160BW HST F160BW magnitude
41- 48 F8.4 mag F170W HST F170W magnitude
52- 59 F8.4 mag F185W HST F185W magnitude
63- 70 F8.4 mag F218W HST F218W magnitude
74- 81 F8.4 mag F255W HST F255W magnitude
85- 92 F8.4 mag F300W HST F300W = U(HDF) magnitude
96-103 F8.4 mag F336W HST F336W magnitude
107-114 F8.4 mag F380W HST F380W magnitude
118-125 F8.4 mag F439W HST F439W magnitude
129-136 F8.4 mag F450W HST F450W = B(HDF) magnitude
140-147 F8.4 mag F555W HST F555W = V(YSC) magnitude
151-158 F8.4 mag F569W HST F569W magnitude
162-169 F8.4 mag F606W HST F606W = V(HDF) magnitude
173-180 F8.4 mag F622W HST F622W magnitude
184-191 F8.4 mag F675W HST F675W magnitude
195-202 F8.4 mag F702W HST F702W magnitude
206-213 F8.4 mag F791W HST F791W magnitude
217-224 F8.4 mag F814W HST F814W = I(HDF) magnitude
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Byte-by-byte Description of file: saspect.dat scspect.dat
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Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 6 F6.4 --- Z Metallicity: 0.0004 0.004 0.008 0.02 0.05
10- 13 I4 --- J Index
16- 24 F9.1 0.1nm lambda Wavelength
29- 38 E10.5 10mW/m2/nm Flux1 Flux at a system age of 1.4000E+08yrs
41- 50 E10.5 10mW/m2/nm Flux2 Flux at a system age of 2.8000E+08yrs
53- 62 E10.5 10mW/m2/nm Flux3 Flux at a system age of 4.2000E+08yrs
65- 74 E10.5 10mW/m2/nm Flux4 Flux at a system age of 5.6000E+08yrs
77- 86 E10.5 10mW/m2/nm Flux5 Flux at a system age of 7.0000E+08yrs
89- 98 E10.5 10mW/m2/nm Flux6 Flux at a system age of 8.4000E+08yrs
101- 110 E10.5 10mW/m2/nm Flux7 Flux at a system age of 9.8000E+08yrs
113- 122 E10.5 10mW/m2/nm Flux8 Flux at a system age of 1.1200E+09yrs
125- 134 E10.5 10mW/m2/nm Flux9 Flux at a system age of 1.2600E+09yrs
137- 146 E10.5 10mW/m2/nm Flux10 Flux at a system age of 1.4000E+09yrs
149- 158 E10.5 10mW/m2/nm Flux11 Flux at a system age of 1.5400E+09yrs
161- 170 E10.5 10mW/m2/nm Flux12 Flux at a system age of 1.6800E+09yrs
173- 182 E10.5 10mW/m2/nm Flux13 Flux at a system age of 1.8200E+09yrs
185- 194 E10.5 10mW/m2/nm Flux14 Flux at a system age of 1.9600E+09yrs
197- 206 E10.5 10mW/m2/nm Flux15 Flux at a system age of 2.1000E+09yrs
209- 218 E10.5 10mW/m2/nm Flux16 Flux at a system age of 2.2400E+09yrs
221- 230 E10.5 10mW/m2/nm Flux17 Flux at a system age of 2.3800E+09yrs
233- 242 E10.5 10mW/m2/nm Flux18 Flux at a system age of 2.5200E+09yrs
245- 254 E10.5 10mW/m2/nm Flux19 Flux at a system age of 2.6600E+09yrs
257- 266 E10.5 10mW/m2/nm Flux20 Flux at a system age of 2.8000E+09yrs
269- 278 E10.5 10mW/m2/nm Flux21 Flux at a system age of 2.9400E+09yrs
281- 290 E10.5 10mW/m2/nm Flux22 Flux at a system age of 3.0800E+09yrs
293- 302 E10.5 10mW/m2/nm Flux23 Flux at a system age of 3.2200E+09yrs
305- 314 E10.5 10mW/m2/nm Flux24 Flux at a system age of 3.3600E+09yrs
317- 326 E10.5 10mW/m2/nm Flux25 Flux at a system age of 3.5000E+09yrs
329- 338 E10.5 10mW/m2/nm Flux26 Flux at a system age of 3.6400E+09yrs
341- 350 E10.5 10mW/m2/nm Flux27 Flux at a system age of 3.7800E+09yrs
353- 362 E10.5 10mW/m2/nm Flux28 Flux at a system age of 3.9200E+09yrs
365- 374 E10.5 10mW/m2/nm Flux29 Flux at a system age of 4.0600E+09yrs
377- 386 E10.5 10mW/m2/nm Flux30 Flux at a system age of 4.2000E+09yrs
389- 398 E10.5 10mW/m2/nm Flux31 Flux at a system age of 4.3400E+09yrs
401- 410 E10.5 10mW/m2/nm Flux32 Flux at a system age of 4.4800E+09yrs
413- 422 E10.5 10mW/m2/nm Flux33 Flux at a system age of 4.6200E+09yrs
425- 434 E10.5 10mW/m2/nm Flux34 Flux at a system age of 4.7600E+09yrs
437- 446 E10.5 10mW/m2/nm Flux35 Flux at a system age of 4.9000E+09yrs
449- 458 E10.5 10mW/m2/nm Flux36 Flux at a system age of 5.0400E+09yrs
461- 470 E10.5 10mW/m2/nm Flux37 Flux at a system age of 5.1800E+09yrs
473- 482 E10.5 10mW/m2/nm Flux38 Flux at a system age of 5.3200E+09yrs
485- 494 E10.5 10mW/m2/nm Flux39 Flux at a system age of 5.4600E+09yrs
497- 506 E10.5 10mW/m2/nm Flux40 Flux at a system age of 5.6000E+09yrs
509- 518 E10.5 10mW/m2/nm Flux41 Flux at a system age of 5.7400E+09yrs
521- 530 E10.5 10mW/m2/nm Flux42 Flux at a system age of 5.8800E+09yrs
533- 542 E10.5 10mW/m2/nm Flux43 Flux at a system age of 6.0200E+09yrs
545- 554 E10.5 10mW/m2/nm Flux44 Flux at a system age of 6.1600E+09yrs
557- 566 E10.5 10mW/m2/nm Flux45 Flux at a system age of 6.3000E+09yrs
569- 578 E10.5 10mW/m2/nm Flux46 Flux at a system age of 6.4400E+09yrs
581- 590 E10.5 10mW/m2/nm Flux47 Flux at a system age of 6.5800E+09yrs
593- 602 E10.5 10mW/m2/nm Flux48 Flux at a system age of 6.7200E+09yrs
605- 614 E10.5 10mW/m2/nm Flux49 Flux at a system age of 6.8600E+09yrs
617- 626 E10.5 10mW/m2/nm Flux50 Flux at a system age of 7.0000E+09yrs
629- 638 E10.5 10mW/m2/nm Flux51 Flux at a system age of 7.1400E+09yrs
641- 650 E10.5 10mW/m2/nm Flux52 Flux at a system age of 7.2800E+09yrs
653- 662 E10.5 10mW/m2/nm Flux53 Flux at a system age of 7.4200E+09yrs
665- 674 E10.5 10mW/m2/nm Flux54 Flux at a system age of 7.5600E+09yrs
677- 686 E10.5 10mW/m2/nm Flux55 Flux at a system age of 7.7000E+09yrs
689- 698 E10.5 10mW/m2/nm Flux56 Flux at a system age of 7.8400E+09yrs
701- 710 E10.5 10mW/m2/nm Flux57 Flux at a system age of 7.9800E+09yrs
713- 722 E10.5 10mW/m2/nm Flux58 Flux at a system age of 8.1200E+09yrs
725- 734 E10.5 10mW/m2/nm Flux59 Flux at a system age of 8.2600E+09yrs
737- 746 E10.5 10mW/m2/nm Flux60 Flux at a system age of 8.4000E+09yrs
749- 758 E10.5 10mW/m2/nm Flux61 Flux at a system age of 8.5400E+09yrs
761- 770 E10.5 10mW/m2/nm Flux62 Flux at a system age of 8.6800E+09yrs
773- 782 E10.5 10mW/m2/nm Flux63 Flux at a system age of 8.8200E+09yrs
785- 794 E10.5 10mW/m2/nm Flux64 Flux at a system age of 8.9600E+09yrs
797- 806 E10.5 10mW/m2/nm Flux65 Flux at a system age of 9.1000E+09yrs
809- 818 E10.5 10mW/m2/nm Flux66 Flux at a system age of 9.2400E+09yrs
821- 830 E10.5 10mW/m2/nm Flux67 Flux at a system age of 9.3800E+09yrs
833- 842 E10.5 10mW/m2/nm Flux68 Flux at a system age of 9.5200E+09yrs
845- 854 E10.5 10mW/m2/nm Flux69 Flux at a system age of 9.6600E+09yrs
857- 866 E10.5 10mW/m2/nm Flux70 Flux at a system age of 9.8000E+09yrs
869- 878 E10.5 10mW/m2/nm Flux71 Flux at a system age of 9.9400E+09yrs
881- 890 E10.5 10mW/m2/nm Flux72 Flux at a system age of 1.0080E+10yrs
893- 902 E10.5 10mW/m2/nm Flux73 Flux at a system age of 1.0220E+10yrs
905- 914 E10.5 10mW/m2/nm Flux74 Flux at a system age of 1.0360E+10yrs
917- 926 E10.5 10mW/m2/nm Flux75 Flux at a system age of 1.0500E+10yrs
929- 938 E10.5 10mW/m2/nm Flux76 Flux at a system age of 1.0640E+10yrs
941- 950 E10.5 10mW/m2/nm Flux77 Flux at a system age of 1.0780E+10yrs
953- 962 E10.5 10mW/m2/nm Flux78 Flux at a system age of 1.0920E+10yrs
965- 974 E10.5 10mW/m2/nm Flux79 Flux at a system age of 1.1060E+10yrs
977- 986 E10.5 10mW/m2/nm Flux80 Flux at a system age of 1.1200E+10yrs
989- 998 E10.5 10mW/m2/nm Flux81 Flux at a system age of 1.1340E+10yrs
1001-1010 E10.5 10mW/m2/nm Flux82 Flux at a system age of 1.1480E+10yrs
1013-1022 E10.5 10mW/m2/nm Flux83 Flux at a system age of 1.1620E+10yrs
1025-1034 E10.5 10mW/m2/nm Flux84 Flux at a system age of 1.1760E+10yrs
1037-1046 E10.5 10mW/m2/nm Flux85 Flux at a system age of 1.1900E+10yrs
1049-1058 E10.5 10mW/m2/nm Flux86 Flux at a system age of 1.2040E+10yrs
1061-1070 E10.5 10mW/m2/nm Flux87 Flux at a system age of 1.2180E+10yrs
1073-1082 E10.5 10mW/m2/nm Flux88 Flux at a system age of 1.2320E+10yrs
1085-1094 E10.5 10mW/m2/nm Flux89 Flux at a system age of 1.2460E+10yrs
1097-1106 E10.5 10mW/m2/nm Flux90 Flux at a system age of 1.2600E+10yrs
1109-1118 E10.5 10mW/m2/nm Flux91 Flux at a system age of 1.2740E+10yrs
1121-1130 E10.5 10mW/m2/nm Flux92 Flux at a system age of 1.2880E+10yrs
1133-1142 E10.5 10mW/m2/nm Flux93 Flux at a system age of 1.3020E+10yrs
1145-1154 E10.5 10mW/m2/nm Flux94 Flux at a system age of 1.3160E+10yrs
1157-1166 E10.5 10mW/m2/nm Flux95 Flux at a system age of 1.3300E+10yrs
1169-1178 E10.5 10mW/m2/nm Flux96 Flux at a system age of 1.3440E+10yrs
1181-1190 E10.5 10mW/m2/nm Flux97 Flux at a system age of 1.3580E+10yrs
1193-1202 E10.5 10mW/m2/nm Flux98 Flux at a system age of 1.3720E+10yrs
1205-1214 E10.5 10mW/m2/nm Flux99 Flux at a system age of 1.3860E+10yrs
1217-1226 E10.5 10mW/m2/nm Flux100 Flux at a system age of 1.4000E+10yrs
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Byte-by-byte Description of file: saplot1.dat scplot1.dat
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Bytes Format Units Label Explanations
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1- 6 F6.4 --- Z Metallicity (1)
8- 20 E13.5 yr Age Actual age
21- 34 E14.5 solMass MassSys [1.00E+11] Total mass of system
35- 47 E13.5 solMass MassStar Total mass of stars in system
48- 60 E13.5 solMass MassGas Total mass of gas in system
61- 69 F9.5 --- Y Helium abundance, Y
70- 78 F9.5 --- Z0 [0.00000] Metallicity, Z (0 for SSPs)
79- 91 E13.3 solMass/yr SFR Star formation rate
92- 102 E11.3 --- --- [0.00000] ?
103-113 E11.3 --- ezj [0.00000] ejection rate (0 for SSPs)
--------------------------------------------------------------------------------
Note (1): Initial parameters:
TOTM=1.00E+11, TGAL=1.40E+10, Y0=0.280, Z0=0.000E+00, MMAX=45,
TSTEP=4.00E+06, JSTEP=4000, EBMV=0.02, X1=0.00, X2=0.00, X3=0.00,
MDOWN=0.000, M12=0.000, M23=0.000, MUP=0.000, FVM=0.000, F=0.00E+00,
YF=0.000, ZF=0.000, HH0=0.65, OMEGA0=0.10, LAMBD0=0.00, ZFORM=5.00,
ZRMAX=4.80, WITHOUT BURST, WITHOUT COSMOLOGY, J=3501
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Byte-by-byte Description of file: saplot2.dat scplot2.dat
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Bytes Format Units Label Explanations
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1- 6 F6.4 --- Z Metallicity (0.0004 0.004 0.008 0.02 0.05)
8- 20 E13.5 yr Age Actual age
21- 31 F11.4 mag mbol Bolometric magnitude
32- 40 F9.4 mag Umag Johnson U magnitude
41- 49 F9.4 mag Bmag Johnson B magnitude
50- 58 F9.4 mag Vmag Johnson V magnitude
59- 67 F9.4 mag Rmag Johnson R magnitude
68- 76 F9.4 mag Imag Johnson I magnitude
77- 85 F9.4 mag Jmag Johnson J magnitude
86- 94 F9.4 mag Hmag Johnson H magnitude
95-103 F9.4 mag Kmag Johnson K magnitude
104-112 F9.4 mag Lmag [0.0000] Johnson L magnitude
(not included in the isochrones)
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Byte-by-byte Description of file: saplot3.dat scplot3.dat
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Bytes Format Units Label Explanations
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1- 6 F6.4 --- Z Metallicity (0.0004 0.004 0.008 0.02 0.05)
8- 20 E13.5 yr Age Actual age
21- 31 F11.4 mag U-B Johnson color index U-B
32- 40 F9.4 mag B-V Johnson color index B-V
41- 49 F9.4 mag V-R Johnson color index V-R
50- 58 F9.4 mag R-I Johnson color index R-I
59- 67 F9.4 mag I-J Johnson color index I-J
68- 76 F9.4 mag J-H Johnson color index J-H
77- 85 F9.4 mag H-K Johnson color index H-K
86- 94 F9.4 mag L-J [0.0000] Johnson color index L-J (not included)
95-103 F9.4 mag U-V Johnson color index U-V
104-112 F9.4 mag V-K Johnson color index V-K
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Byte-by-byte Description of file: saplot4.dat scplot4.dat
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Bytes Format Units Label Explanations
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1- 6 F6.4 --- Z Metallicity (0.0004 0.004 0.008 0.02 0.05)
10- 20 E11.5 yr Age Actual age
23- 33 E11.5 solLum Lbol bolometric luminosity
35- 45 E11.5 solLum LUmag luminosity in U
47- 57 E11.5 solLum LBmag luminosity in B
59- 69 E11.5 solLum LVmag luminosity in V
71- 81 E11.5 solLum LRmag luminosity in R
83- 93 E11.5 solLum LImag luminosity in I
95-105 E11.5 solLum LJmag luminosity in J
107-117 E11.5 solLum LHmag luminosity in H
119-129 E11.5 solLum LKmag luminosity in k
131-141 E11.5 solLum LLmag [0.0000] luminosity in L (not included)
144-152 E9.3 solLum LLya [0.0000] Lyman-continuum-photons
(not calculated)
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Byte-by-byte Description of file: s[ac]ecoeff.dat s[ac]kcoeff.dat s[ac]katt.dat
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Bytes Format Units Label Explanations
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1- 6 F6.4 --- Z Metallicity (0.0004 0.004 0.008 0.02 0.05)
8- 9 I2 --- H0 Hubble constant value (65 or 75)
11- 18 F8.2 --- z Redshift
19- 30 F12.4 --- cu e- or k-correction for Johnson U
31- 42 F12.4 --- cb e- or k-correction for Johnson B
43- 54 F12.4 --- cv e- or k-correction for Johnson V
55- 66 F12.4 --- cr e- or k-correction for Johnson R
67- 78 F12.4 --- ci e- or k-correction for Johnson I
79- 90 F12.4 --- cj e- or k-correction for Johnson J
91-102 F12.4 --- ch e- or k-correction for Johnson H
103-114 F12.4 --- ck e- or k-correction for Johnson K
115-126 F12.4 --- cku e- or k-correction for Koo u
127-138 F12.4 --- ckb e- or k-correction for Koo j
139-150 F12.4 --- ckv e- or k-correction for Koo f
151-162 F12.4 --- ckr e- or k-correction for Koo n
163-174 F12.4 --- cgi e- or k-correction for Thuan & gunn g
175-186 F12.4 --- cgj e- or k-correction for Thuan & gunn r
188-198 F11.4 --- cF160BW e- or k-correction HST F160BW
199-209 F11.4 --- cF170W e- or k-correction HST F170W
210-220 F11.4 --- cF185W e- or k-correction HST F185W
221-231 F11.4 --- cF218W e- or k-correction HST F218W
232-242 F11.4 --- cF255W e- or k-correction HST F255W
243-253 F11.4 --- cF300W e- or k-correction HST F300W ⟺ U(HDF)
254-264 F11.4 --- cF336W e or k-correction HST F336W
265-275 F11.4 --- cF380W e- or k-correction HST F380W
276-286 F11.4 --- cF439W e- or k-correction HST F439W
287-297 F11.4 --- cF450W e- or k-correction HST F450W ⟺ B(HDF)
298-308 F11.4 --- cF555W ? e- or k-correction HST F555W ⟺ V(YSC)
309-319 F11.4 --- cF569W ? e- or k-correction HST F569W
320-330 F11.4 --- cF606W ? e- or k-correction HST F606W ⟺ V(HDF)
331-341 F11.4 --- cF622W ? e- or k-correction HST F622W
342-352 F11.4 --- cF675W ? e- or k-correction HST F675W
353-363 F11.4 --- cF702W ? e- or k-correction HST F702W
364-374 F11.4 --- cF791W ? e- or k-correction HST F791W
375-385 F11.4 --- cF814W ? e- or k-correction HST F814W ⟺ I(HDF)
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Acknowledgements: Jochen Schulz
(End) Patricia Bauer [CDS] 14-May-2002