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Galaxy Evolutionary Synthesis Models
help you understand your data on star clusters and galaxies from the early universe until today in terms of their relevant physical and chemical properties and their evolutionary state.
Emissionline Restframe wavelength Affects flux in filter ?
(angstroms) U B V R I J H K
Lalpha 1216.0
CII 1335.0
OIII 1663.0
CIII] 1909.0
NII 2141.0
CII] 2326.0
MgII 2798.0
[OII] 3727.0 x x
Hkappa 3750.0 x x
Hiota 3770.0 x x
Htheta 3797.0 x x
Heta 3835.0 x x
[Ne III] 3869.0 x x
Hzeta + HeI 3889.0 x x
Heps + [NeIII] 3970.0 x x
He I 4026.0 x x
[SII] 4068.6 x x
[SII] 4076.4 x x
Hdelta 4101.0 x x
Hgamma 4340.0 x
[OIII] 4363.0 x
HeI 4471.0 x
[ArIV] + HeI 4711.0 x
Hbeta 4861.0 x x
[OIII] 4958.9 x x
[OIII] 5006.8 x x
[NI] 5199.0 x x
[NII] 5755.0 x x
HeI 5876.0 x x
[OI] 6300.0 x x
[SIII] 6312.0 x x
[NII] 6548.1 x x
Halpha 6562.8 x x
[NII] 6583.5 x x
HeI 6678.0 x x
[SII] 6716.0 x x
[SII] 6730.0 x x
HeI 7065.0 x x x
[ArIII] 7135.8 x x x
[OII] 7320.0 x x x
[OII] 7330.7 x x x
[ArIII] 7751.1 x x
[SIII] 9068.6 x x
[SIII] 9530.9 x x
Pa-epsilon 9546.0 x x
Pa-delta 10049.0 x
[SII] 10286.7 x
[SII] 10320.5 x
[SII] 10336.4 x
Pa-gamma 10935.0 x x
Pa-beta 12818.0 x
Br- 15188.0 x
Br- 15256.0 x
Br- 15337.0 x
Br- 15435.0 x
Br- 15552.0 x
Br- 15696.0 x
Br- 15876.0 x
Br- 16105.0 x
Br- 16403.0 x
Br- 16802.0 x
Br- 17357.0 x
Br-epsilon 18169.0 x
Pa-alpha 18751.0
Br-delta 19440.0 x
Br-gamma 21649.0 x