Galaxy Spectral Evolution Library

GALAXEV

G. Bruzual and S. Charlot

UNIX Version (C) 1991-2011 - All Rights Reserved



1) Select metallicity for desired set of models and evolutionary tracks:
Model:
Files:
Tracks:
TP-AGB:
Comments:
Status:
Z:
BC03
bc2003
Padova 1994

-
-
BC03
bc2003
Padova 2000

-
-
CB07
cb2007
Padova 1994
Marigo 2007
Calibrated
Preliminary
CB09
cb2009
Padova 2008
Marigo 2007
Calibrated
Preliminary
CB09
cb2009
Padova 2008
Marigo 2008
Uncalibrated
Preliminary
CB10
cb2010
Padova 2008
Girardi 2010
-
Final


2) Select IMF: Stellar lower mass limit: Stellar upper mass limit:


or enter your own IMF as a multisegment power law: Segment 1: x: from mass: to mass:
Segment 2: x: from mass: to mass:
Segment 3: x: from mass: to mass:
Segment 4: x: from mass: to mass:
Segment 5: x: from mass: to mass:
Segment 6: x: from mass: to mass:


3) Select: