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VI/109
  Population Synthesis Models at very low metallicities (Schaerer, 2003)
Post annotation
  
1.VI/109/initialInitial parameters of the models (9 rows)
2.VI/109/type20Main output (file corresponding to output described in Schaerer & Vacca, 1998ApJ...497..618S) plus additional quantities (last four columns) (74289 rows)
3.VI/109/type21Output related to Wolf-Rayet stars (file corresponding to output described in Schaerer & Vacca, 1998ApJ...497..618S) (74289 rows)
4.VI/109/type22Nebular recombination lines - NEW V2.4 (74289 rows)
5.VI/109/type23Colors (filter bandpasses as in Starburst99 (Leitherer et al., 1999ApJS..123....3L) (74289 rows)
6.VI/109/type24UV spectral information (74289 rows)

 
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Column  Constraint Explain   (UCD)
  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
   (ALL)Z (char) Code for metallicity Z, indicates the model groups, see note (Note G1)   (phys.abund.Z)
  (1)WRmass solMass WR mass limit (phys.mass)
  (1)[M/H] [Sun] Input metallicity content of Kurucz model (phys.abund.Fe;meta.modelled)
  (1)Vturb km/s Input turbulent velocity of Kurucz model (phys.veloc;stat.param;meta.modelled)
  (1)L/H  Input convective parameter of Kurucz model (stat.param;meta.modelled)
  (1)WRMod (char) [YES NO] Include WR models (meta.code)
  (1)CoStarRad (char) [YES NO] use CoStar WR radii (meta.code)
  (1)CoStarMod (char) [YES NO] CoStar models (meta.code)
  (1)n_CoStarMod (char) [(M>20)] (M>20): (YES for masses≥20.000) (meta.note)
  (1)TLUSTYMod (char) [YES NO] use TLUSTY models (meta.code)

ALL cols
    
 (i)indexed column
  (1)Tracks (char) Tracks used (meta.note;instr.setup)
  (2+3+4+5+6)mup solMass Upper mass cut-off of IMF in M (Note G1)   (stat.param)
  (2+3+4+5+6)low solMass Lower mass cut-off of IMF in M (Note G1)   (stat.param)
  (2+3+4+5+6)sfh (char) Code for star formation history (G1) (cs1, cs3, cs4, is1, is3) (stat.param)
  (2+3+4+5+6)log(Age) [yr] Age (time.age)
  (2+5+6)Mbol mag Bolometric magnitude (phys.magAbs.bol)
  (2+4)log(Q0) [s-1] Lyman continuum photon flux (Q0=QH) (phot.flux.density;spect.continuum)
  (2+4)log(Q1) [s-1] He0 ionising photon flux (Q1=QHe) (phot.flux)
  (2+4)log(Q2) [s-1] He+ ionising photon flux (Q0=QHe+) (phot.flux)
  (2)NOstar  Number of O stars (meta.number)
  (2)WR/(WR+O)  Ratio of WR to WR+O stars (stat.param)
  (2)WR/O  Ratio of WR to O stars (stat.param)
  (2)WNL/(WR+O)  Ratio of WNL (late WN) to WR+O stars (stat.param)

ALL cols
    
 (i)indexed column
  (2)WNE/(WR+O)  Ratio of WNE (early WN) to WR+O stars (stat.param)
  (2)WC/(WR+O)  Ratio of WC to WR+O stars (stat.param)
  (2+3+4)EWHb 0.1nm Nebular Hβ equivalent width (Note G2)   (spect.line.eqWidth;em.line.Hbeta)
  (2+3+4)LHb 10-7W Nebular Hβ luminosity (Note G2)   (phys.luminosity;em.line.Hbeta)
  (2+4)EWHeI 0.1nm Nebular HeI 4471 equivalent width (CAUTION: Saturation effect !) (Note G2)   (spect.line.eqWidth)
  (2)LHeI  Relative Nebular HeI 4471 luminosity (in Hβ unit) (Note G2)   (phys.luminosity;em.line.Hbeta)
  (2)EWHeII 0.1nm Nebular HeII 4686 equivalent width (Note G2)   (spect.line.eqWidth)
  (2)LHeII  Nebular HeII 4686 luminosity (in Hβ unit) (Note G2)   (phys.luminosity;em.line.Hbeta)
  (2)EWWR 0.1nm WR bump (CIII/IV 4650 + HeII 4686) equivalent width (spect.line.eqWidth)
  (2)LWR  WR bump (CIII/IV 4650 + HeII 4686) luminosity (in Hβ unit) (Note G2)   (phys.luminosity;em.line.Hbeta)
  (2)EWCI 0.1nm CI V-WR equivalent width (spect.line.eqWidth)
  (2)LCI  CI V-WR luminosity (in Hβ unit) (Note G2)   (phys.luminosity;em.line.Hbeta)
  (2)Balmer mag Balmer jump, defined as -2.5*log(F(3640Å)/F(3650Å) (phot.mag)

ALL cols
    
 (i)indexed column
  (2)log(QH2) [s-1] Ionising photon flux in Lyman-Werner band (QH2=QLW) (Note G3)   (phot.flux)
  (2)E(Q) eV Average energy per photon in Lyman-continuum (stat.param)
  (2)E(QHe+) eV (n) Average energy per photon with E>54eV (stat.param)
  (2+3+4+5+6)allQuantities (char) Display all output quantities for this model's parameters and age (meta.ref.url)
  (3)WNLType  Average WNL subtype (late WN) (src.spType)
  (3)WCType  Average WC subtype (src.spType)
  (3+4)EWHa 0.1nm Nebular Hα equivalent width (Note G2)   (spect.line.eqWidth;em.line.Halpha)
  (3)LHa  Nebular Hα luminosity (in Hβ unit) (Note G2)   (phys.luminosity;em.line.Halpha)
  (3)EWHe1640 0.1nm Stellar He1640 equivalent width (spect.line.eqWidth)
  (3)LHe  Stellar He1640 luminosity (in Hβ unit) (Note G2)   (phys.luminosity;em.line.Hbeta)
  (3)EWN4640 0.1nm Stellar N4640 equivalent width (spect.line.eqWidth)
  (3)LN  Stellar N4640 luminosity (in Hβ unit) (Note G2)   (phys.luminosity;em.line.Hbeta)
  (3)EWC4650 0.1nm Stellar C4650 equivalent width (spect.line.eqWidth;em.opt.B)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (3)LC4650  Stellar C4650 luminosity (in Hβ unit) (Note G2)   (phys.luminosity;em.line.Hbeta)
  (3)EWHe4686 0.1nm Stellar He4686 equivalent width (spect.line.eqWidth)
  (3)LHe4686  Stellar He4686 luminosity (in Hβ unit) (Note G2)   (phys.luminosity;em.line.Hbeta)
  (3)EWH4861 0.1nm Stellar H4861 equivalent width (spect.line.eqWidth)
  (3)LH4861  Stellar H4861 luminosity (in Hβ unit) (Note G2)   (phys.luminosity;em.line.Hbeta)
  (3)EWC5696 0.1nm Stellar C5696 equivalent width (spect.line.eqWidth;em.opt.V)
  (3)LC5696  Stellar C5996 luminosity (in Hβ unit) (Note G2)   (phys.luminosity;em.line.Hbeta)
  (3)EWC5808 0.1nm Stellar C5808 equivalent width (spect.line.eqWidth;em.opt.V)
  (3)LC5808  Stellar C5808 luminosity (in Hβ unit) (Note G2)   (phys.luminosity;em.line.Hbeta)
  (3)EWH6560 0.1nm Stellar H6560 equivalent width (spect.line.eqWidth)
  (3)LH6560  Stellar H6560 luminosity (in Hβ unit) (Note G2)   (phys.luminosity;em.line.Hbeta)
  (3)EWHe5412 0.1nm Stellar He5412 equivalent width (spect.line.eqWidth)
  (3)LHe5412  Stellar He5412 luminosity (in Hβ unit) (Note G2)   (phys.luminosity;em.line.Hbeta)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (4)EWHLya 0.1nm Lymanα equivalent width (Note G2)   (spect.line.eqWidth)
  (4)IHLy  Lymanα Intensity relative to Hβ (Note G2)   (phys.luminosity;em.line.Hbeta)
  (4)IHa  Hα intensity relative to Hβ (Note G2)   (phys.luminosity;em.line.Hbeta)
  (4)IHb   [1.00E+00] Hβ intensity relative to Hβ (Note G2)   (phys.luminosity;em.line.Hbeta)
  (4)IHeI  HeI 4471 intensity relative to Hβ (Note G2)   (phys.luminosity;em.line.Hbeta)
  (4)EWHeII1640 0.1nm HeII1640 equivalent width (Note G2)   (spect.line.eqWidth)
  (4)IHeII1640  HeII1640 intensity relative to Hβ (Note G2)   (phys.luminosity;em.line.Hbeta)
  (4)EWHeII4686 0.1nm HeII4686 equivalent width (Note G2)   (spect.line.eqWidth)
  (4)IHeII4686  HeII4686 intensity relative to Hβ (Note G2)   (phys.luminosity;em.line.Hbeta)
  (4)EWHeII3203 0.1nm HeII3203 equivalent width (Note G2)   (spect.line.eqWidth)
  (4)IHeII3203  HeII3203 intensity relative to Hβ (Note G2)   (phys.luminosity;em.line.Hbeta)
  (4)EWHeII4541 0.1nm HeII4541 equivalent width (Note G2)   (spect.line.eqWidth)
  (4)IHeII4541  HeII4541 intensity relative to Hβ (phys.luminosity;em.line.Hbeta)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (5)(130-V) mag (130-V) colour index (phot.color;em.UV;em.opt)
  (5)(210-V) mag (210-V) colour index (phot.color;em.UV;em.opt)
  (5)(U-B) mag (U-B) colour index (phot.color;em.opt.U;em.opt.B)
  (5)(B-V) mag (B-V) colour index (phot.color;em.opt.B;em.opt.V)
  (5)(V-R) mag (V-R) colour index (phot.color;em.opt.V;em.opt.R)
  (5)(V-I) mag (V-I) colour index (phot.color;em.opt.V;em.opt.I)
  (5)(V-J) mag (V-J) colour index (phot.color;em.opt.V;em.IR.J)
  (5)(V-H) mag (V-H) colour index (phot.color;em.opt.V;em.IR.H)
  (5)(V-K) mag (V-K) colour index (phot.color;em.opt.V;em.IR.K)
  (5)(V-L) mag (V-L) colour index (phot.color;em.opt.V;em.IR.3-4um)
  (5)VMAG mag Absolute V magnitude (phys.magAbs;em.opt.V)
  (5)BMAG mag Absolute B magnitude (phys.magAbs;em.opt.B)
  (6)log(L15SB) [10-6W/nm]Average UV luminosity at 1500Å (over ± 20Å band), in erg/s/Å (phys.luminosity;em.UV)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (6)log(L1500) [10-6W/nm]Average UV luminosity at 1500Å (over ±150Å band), in erg/s/Å (phys.luminosity;em.UV)
  (6)log(L2800) [10-6W/nm]Average UV luminosity at 2800Å (over ±280Å band), in erg/s/Å (phys.luminosity;em.UV)
  (6)beta1550  UV slope 1300-1800Å using STELLAR + NEBULAR cont. emission (Note 1)   (spect.index)
  (6)beta2500  UV slope 2200-2800Å using STELLAR + NEBULAR cont. emission (Note 1)   (spect.index)
  (6)beta2000  UV slope 1800-2200Å using STELLAR + NEBULAR cont. emission (Note 1)   (spect.index)
  (6)beta1550*  UV slope 1300-1800Å using pure STELLAR emission (Note 1)   (spect.index)
  (6)beta2500*  UV slope 2200-2800Å using pure STELLAR emission (Note 1)   (spect.index)
  (6)beta2000*  UV slope 1800-2200Å using pure STELLAR emission (Note 1)   (spect.index)
  (6)log(L900) [10-6W/nm]Average luminosity 912- in erg/s/Å (Note 2)   (phys.luminosity;em.UV)
  (6)log(Lybrk) [---] Lyman-break amplitude Lybrk=912+/912- (phot.flux;arith.ratio)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
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