This archive is a catalogue of the maximum density evolution of 54 supernova core collapse models as described in detail in this paper: 1. Dimmelmeier, H., Ott, C.D., Marek, A., Janka, H.-T., and M\"uller, E., "General gravitational wave signals from the collapse of rotating stellar iron cores", Phys. Rev. Lett., 98, 251101, (2007); astro-ph/0702305. It contains the following files: signal_A1B0.05.dat signal_A2B0.05.dat signal_A3B0.05.dat signal_A1B0.07.dat signal_A2B0.07.dat signal_A3B0.07.dat signal_A1B0.10.dat signal_A2B0.10.dat signal_A3B0.10.dat signal_A1B0.15.dat signal_A2B0.15.dat signal_A3B0.15.dat signal_A1B0.25.dat signal_A2B0.25.dat signal_A3B0.25.dat signal_A1B0.35.dat signal_A2B0.35.dat signal_A3B0.35.dat signal_A1B0.50.dat signal_A2B0.50.dat signal_A3B0.50.dat signal_A1B0.70.dat signal_A2B0.70.dat signal_A3B0.70.dat signal_A1B0.90.dat signal_A2B0.90.dat signal_A3B0.90.dat signal_A1B1.10.dat signal_A2B1.10.dat signal_A3B1.10.dat signal_A1B1.30.dat signal_A2B1.30.dat signal_A3B1.30.dat signal_A1B1.60.dat signal_A2B1.60.dat signal_A3B1.60.dat signal_A1B1.80.dat signal_A2B1.80.dat signal_A3B1.80.dat signal_A1B2.00.dat signal_A2B2.00.dat signal_A3B2.00.dat signal_A1B2.50.dat signal_A2B2.50.dat signal_A3B2.50.dat signal_A1B3.00.dat signal_A2B3.00.dat signal_A3B3.00.dat signal_A1B3.50.dat signal_A2B3.50.dat signal_A3B3.50.dat signal_A1B4.00.dat signal_A2B4.00.dat signal_A3B4.00.dat The initial model is the presupernova stellar model s20 rotating at different rates with various profiles. Each collapse model is specified by two parameters, A and B: A1: A = 5.0 * 10^9 cm A2: A = 1.0 * 10^8 cm A3: A = 5.0 * 10^7 cm B0.05: beta_rot_ini = 0.05% B0.07: beta_rot_ini = 0.07% B0.10: beta_rot_ini = 0.10% B0.15: beta_rot_ini = 0.15% B0.25: beta_rot_ini = 0.25% B0.35: beta_rot_ini = 0.35% B0.50: beta_rot_ini = 0.50% B0.70: beta_rot_ini = 0.70% B0.90: beta_rot_ini = 0.90% B1.10: beta_rot_ini = 1.10% B1.30: beta_rot_ini = 1.30% B1.60: beta_rot_ini = 1.60% B1.80: beta_rot_ini = 1.80% B2.00: beta_rot_ini = 2.00% B2.50: beta_rot_ini = 2.50% B3.00: beta_rot_ini = 3.00% B3.50: beta_rot_ini = 3.50% B4.00: beta_rot_ini = 4.00% All signals have been obtained by using the quadrupole 'first momentum of momentum density formula', Column 1 is the coordinate time 't' in units of milliseconds. Column 2 is the dimensionless signal amplitude 'h^TT' at a distance of 10 kpc with optimal orientation of the source (i.e. measured in the equatorial plane). This waveform catalogue can be obtained freely from this URL: http://www.mpa-garching.mpg.de/rel_hydro/ ----------------------------------------------------------------- 22 December 2006, Harald Dimmelmeier (harrydee@mpa-garching.mpg.de).