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J/A+A/524/A45
  Overproduction factors of s-nuclei in massive stars (Pumo+, 2010)
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2010A&A...524A..45P
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1.J/A+A/524/A45/tablea4Overproduction factors for all the models with initial metallicity Z=0.02 (49 rows)
2.J/A+A/524/A45/tablea5Overproduction factors for all the M=20M☉ models with initial metallicity Z<0.02 (49 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)A   [69/209] Mass number (meta.id;meta.main)
   (ALL)El (char) Nuclide (chemical) symbol (meta.note)
  (1)M15T07  (n) Overproduction factors obtained by The, El Eid & Meyer (2007ApJ...655.1058T) for their Z=0.02, M=15M☉ stellar model (Note G1)   (stat.param)
  (1)M15f.001  Overproduction factors for our Z=0.02, M=15M☉ stellar model with overshooting parameter f=0.00001 (Note G1)   (stat.param)
  (1)M15f1  Overproduction factors for our Z=0.02, M=15M☉ stellar model with overshooting parameter f=0.01 (Note G1)   (stat.param)
  (1)M15f2  Overproduction factors for our Z=0.02, M=15M☉ stellar model with overshooting parameter f=0.02 (Note G1)   (stat.param)
  (1)M15f3.5  Overproduction factors for our Z=0.02, M=15M☉ stellar model with overshooting parameter f=0.035 (Note G1)   (stat.param)
  (1)M20T07  (n) Overproduction factors obtained by The, El Eid & Meyer (2007ApJ...655.1058T) for their Z=0.02, M=20M☉ stellar model (Note G1)   (stat.param)
  (1)M20f0001  Overproduction factors for our Z=0.02, M=20M☉ stellar model with overshooting parameter f=0.00001 (Note G1)   (stat.param)
  (1)M20f1  Overproduction factors for our Z=0.02, M=20M☉ stellar model with overshooting parameter f=0.01 (Note G1)   (stat.param)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1)M20f2  Overproduction factors for our Z=0.02, M=20M☉ stellar model with overshooting parameter f=0.02 (Note G1)   (stat.param)
  (1)M20f3.5  Overproduction factors for our Z=0.02, M=20M☉ stellar model with overshooting parameter f=0.035 (Note G1)   (stat.param)
  (1)M25T07  (n) Overproduction factors obtained by The, El Eid & Meyer (2007ApJ...655.1058T) for their Z=0.02, M=25M☉ stellar model (Note G1)   (stat.param)
  (1)M25f.001  Overproduction factors for our Z=0.02, M=25M☉ stellar model with overshooting parameter f=0.00001 (Note G1)   (stat.param)
  (1)M25f1  Overproduction factors for our Z=0.02, M=25M☉ stellar model with overshooting parameter f=0.01 (Note G1)   (stat.param)
  (2)M20Z.01f.001  Overproduction factors for our Z=0.0001, M=20M☉ stellar model with overshooting parameter f=0.00001 (Note G1)   (stat.param)
  (2)M20Z.01f1  Overproduction factors for our Z=0.0001, M=20M☉ stellar model with overshooting parameter f=0.01 (Note G1)   (stat.param)
  (2)M20Z.01f2  Overproduction factors for our Z=0.0001, M=20M☉ stellar model with overshooting parameter f=0.02 (Note G1)   (stat.param)
  (2)M20Z.01f3.5  Overproduction factors for our Z=0.0001, M=20M☉ stellar model with overshooting parameter f=0.035 (Note G1)   (stat.param)
  (2)M20Z.5f.001  Overproduction factors for our Z=0.005, M=20M☉ stellar model with overshooting parameter f=0.00001 (Note G1)   (stat.param)
  (2)M20Z.5f1  Overproduction factors for our Z=0.005, M=20M☉ stellar model with overshooting parameter f=0.01 (Note G1)   (stat.param)
  (2)M20Z.5f2  Overproduction factors for our Z=0.005, M=20M☉ stellar model with overshooting parameter f=0.02 (Note G1)   (stat.param)
  (2)M20Z.5f3.5  Overproduction factors for our Z=0.005, M=20M☉ stellar model with overshooting parameter f=0.035 (Note G1)   (stat.param)
  (2)M20Z1f.001  Overproduction factors for our Z=0.01, M=20M☉ stellar model with overshooting parameter f=0.00001 (Note G1)   (stat.param)
  (2)M20Z1f1  Overproduction factors for our Z=0.01, M=20M☉ stellar model with overshooting parameter f=0.01 (Note G1)   (stat.param)
  (2)M20Z1f2  Overproduction factors for our Z=0.01, M=20M☉ stellar model with overshooting parameter f=0.02 (Note G1)   (stat.param)
  (2)M20Z1f3.5  Overproduction factors for our Z=0.01, M=20M☉ stellar model with overshooting parameter f=0.035 (Note G1)   (stat.param)

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