VizieR

CfA VizieR . ADAC VizieR . Cambridge (UK) VizieR . IUCAA VizieR . INASAN VizieR .

VizieR

  
J/A+A/523/A64
  UV properties of starbursts (Raiter+, 2010)
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2010A&A...523A..64R
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1.J/A+A/523/A64/initial*List of available sets (Note) (128 rows)
2.J/A+A/523/A64/type20Main output (file corresponding to output described in Schaerer & Vacca, 1998ApJ...497..618S) plus additional quantities (last four columns) (112820 rows)
3.J/A+A/523/A64/type21Output related to Wolf-Rayet stars (file corresponding to output described in Schaerer & Vacca, 1998ApJ...497..618S) (112820 rows)
4.J/A+A/523/A64/type22Nebular recombination lines and Lyα absorption (112820 rows)
5.J/A+A/523/A64/type23Colors (filter bandpasses as in Starburst99, Leitherer et al., 1999ApJS..123....3L) (112820 rows)
6.J/A+A/523/A64/type24UV spectral information (112820 rows)
7.J/A+A/523/A64/type25Ionising flux, UV luminosities and slopes - NEW in v2.53 (112820 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 (Note G1)   (phys.abund.Z)
  (1)ttt (char) [ge0] Tracks (Note G1)   (meta.code)
   (ALL)IMF (char) IMF type (Note G1)   (meta.code)
  (1)mup  Upper mass cut-off of IMF in M☉ (Note G1)   (phys.mass)
  (1)low  Lower mass cut-off of IMF in M☉ (Note G1)   (phys.mass)
   (ALL)sfh (char) Code for star formation history (Note G1)   (meta.code)
  (1)model (char) Display all the data for this set of parameters (meta.ref.url)
  (2+3+4+5+6+7)mup solMass Upper mass cut-off of IMF in M☉ (Note G1)   (phys.mass)
  (2+3+4+5+6+7)low solMass Lower mass cut-off of IMF in M☉ (Note G1)   (phys.mass)
  (2+3+4+5+6+7)log(Age) [yr] Age (time.age)

ALL cols		    
 (i)indexed column
  (2+5+6+7)Mbol mag Bolometric magnitude (phys.magAbs.bol)
  (2+4+7)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)
  (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 WC/(WR+O) (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)

ALL cols		    
 (i)indexed column
  (2)LHeI  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)
  (2)log(QH2) [s-1] Ionising photon flux in Lyman-Werner band (QH2=QLW) (phot.flux)
  (2+4)E(Q) eV Average energy per photon in Lyman-continuum (stat.param)
  (2)E(QHe+) eV Average energy per photon with E>54eV (stat.param)
  (2+3+4+5+6+7)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)

ALL cols		    
 (i)indexed column
  (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)
  (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)

ALL cols		    
 (i)indexed column
  (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)
  (4)EWHLya 0.1nm Lymanα equivalent width (Note G2)   (spect.line.eqWidth)
  (4)IHLya  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)

ALL cols		    
 (i)indexed column
  (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)
  (4)LyaAbs 0.1nm Lyα absorption equivalent width (Note 1)   (spect.line.eqWidth)
  (4)ILyaAbs  Lyα absorption intensity relative to Hβ (Note 1)   (phys.absorption.gal;arith.ratio)
  (4)LyaAbsc 0.1nm Lyα absorption computed EXCLUDING nebular continuum equivalent width (Note 1)   (spect.line.eqWidth;spect.continuum;meta.modelled)
  (4)FcontLya 10+4W/m Continuum flux (stellar+nebular) at Lyα (in erg/s/Å units) (Note 1)   (phot.flux;em.UV)
  (4)LyaAbs2 0.1nm Lyα absorption equivalent width (Note 2)   (spect.line.eqWidth)

ALL cols		    
 (i)indexed column
  (4)ILyaAbs2  Lyα absorption intensity relative to Hβ (Note 2)   (phys.absorption.gal;arith.ratio)
  (4)LyaAbsc2 0.1nm Lyα absorption computed EXCLUDING nebular continuum equivalent width (Note 2)   (spect.line.eqWidth;spect.continuum;meta.modelled)
  (4)FcontLya2 10+4W/m Continuum flux (stellar+nebular) at Lyα (in erg/s/Å units) (Note 2)   (phot.flux;em.UV)
  (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)

ALL cols		    
 (i)indexed column
  (5)VMAG mag Absolute V magnitude (phys.magAbs;em.opt.V)
  (5)BMAG mag Absolute B magnitude (phys.magAbs;em.opt.B)
  (6+7)log(L15SB) [10-6W/nm]Average UV luminosity at 1500Å (over ±20Å band), in erg/s/Å (phys.luminosity;em.UV)
  (6+7)log(L1500) [10-6W/nm]Average UV luminosity at 1500Å (over ±150Å band), in erg/s/Å (phys.luminosity;em.UV)
  (6+7)log(L2800) [10-6W/nm]Average UV luminosity at 2800Å (over ±280Å band), in erg/s/Å (phys.luminosity;em.UV)
  (6+7)beta1550  UV slope 1300-1800Å using STELLAR + NEBULAR cont. emission (Note 1)   (spect.index)
  (6+7)beta2500  UV slope 2200-2800Å using STELLAR + NEBULAR cont. emission (Note 1)   (spect.index)
  (6+7)beta2000  UV slope 1800-2200Å using STELLAR + NEBULAR cont. emission (Note 1)   (spect.index)
  (6+7)beta1550*  UV slope 1300-1800Å using pure STELLAR emission (Note 1)   (spect.index)
  (6+7)beta2500*  UV slope 2200-2800Å using pure STELLAR emission (Note 1)   (spect.index)
  (6+7)beta2000*  UV slope 1800-2200Å using pure STELLAR emission (Note 1)   (spect.index)
  (6+7)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		    
 (i)indexed column
  (6)log(L1460) [10-6W/nm]Average UV luminosity at 1195Å (over ±85Å band) (phys.luminosity;em.UV)
  (6)beta1460  UV slope between 1195 (±85)Å and 1738 (±127)Å (spect.index)
  (6)betaGR  UV slope computed using Steidel G,R filter curves (cf. Shapley et al., 2003ApJ...588...65S) (Note 3)   (spect.index)
  (7)log(Q0/L1500) [10-6W/nm]Ionising photon flux per 1500Å luminosity (in erg/Å) (phys.luminosity)
  (7)log(Lybrk)  Lyman-break amplitude Lyb=912+/912- (Note 2)   (phot.flux;arith.ratio)
  (7)neb/1500  Contribution of the nebular continuum to the total continuum at 1500Å (Note 3)   (stat.param)
  (7)neb/2800  Contribution of the nebular continuum to the total continuum at 2800Å (Note 4)   (stat.param)

ALL cols		    
 (i)indexed column
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