Go to:

-Models E15x/E20x
-Models S11AxOy
-Models S15AxOy
-Models S20AxOy
-Models S40AxOy

Axisymmetric Core Collapse with Microphysics (Extended Model Set)
Relativistic Hydrodynamics
Waveform Catalog

Department of Astronomy and Steward Observatory

University of Arizona

These figures contain the time evolution of the maximum density and the signal amplitude for all 136 simulated models.

The vertical dotted lines mark the time of peak maximum density (time of bounce).

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• Models E15x/E20x:

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  Models E15A and E15B

  Models E20A and E20B

• Models S11AxOy:

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  Models S11A1O01 and S11A1O05	Models S11A1O07 and S11A1O09
  Models S11A1O13 and S11A2O05	Models S11A2O07 and S11A2O09
  Models S11A2O13 and S11A2O15	Models S11A3O05 and S11A3O07
  Models S11A3O09 and S11A3O12	Models S11A3O13 and S11A3O15

• Models S15AxOy:

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  Models S15A1O01 and S15A1O05	Models S15A1O07 and S15A1O09
  Models S15A1O13 and S15A2O05	Models S15A2O07 and S15A2O09
  Models S15A2O13 and S15A2O15	Models S15A3O05 and S15A3O07
  Models S15A3O09 and S15A3O12	Models S15A3O13 and S15A3O15

• Models S20AxOy:

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  Models S20A1O01 and S20A1O05	Models S20A1O07 and S20A1O09
  Models S20A1O13 and S20A2O05	Models S20A2O07 and S20A2O09
  Models S20A2O13 and S20A2O15	Models S20A3O05 and S20A3O07
  Models S20A3O09 and S20A3O12	Models S20A3O13 and S20A3O15

• Models S40AxOy:

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  Models S40A1O01 and S40A1O05	Models S40A1O07 and S40A1O09
  Models S40A1O13 and S40A2O05	Models S40A2O07 and S40A2O09
  Models S40A2O13 and S40A2O15	Models S40A3O05 and S40A3O07
  Models S40A3O09 and S40A3O12	Models S40A3O13 and S40A3O15