The Garching Core-Collapse Supernova Archive

Using the data in this archive is permitted for non-commercial purposes under the condition of citing this WWW page and the corresponding publication where one exists. If these data are used for a scientific publication, we appreciate a short notification. All efforts have been made to eliminate errors, but no warranty whatsoever is provided. Please inform us of any errors or inconsistencies that you may detect.

Some of the archives are password protected. Please get in touch if you need to use these data.

Contact address and responsibility:
Hans-Thomas Janka (thj (at) mpa-garching.mpg.de)

General archives, catalogs, and applications

Gravitational wave archive from 2D rotational core-collapse models

The following links provide information about the gravitational wave forms of stellar core collapse and a collection of the corresponding literature.

Gravitational waves from general relativistic stellar core collapse

Gravitational waves from Newtonian stellar core collapse

Literature catalog: Gravitational waves from stellar core collapse

3D plots of EOS quantities

The following Java applet can be used to study the behavior of different equation of states.

Java applet

Simulation data and supplementary material

Radial profiles at different postbounce times of the 2013 model series by Sukhbold & Woosley (2014) simulated with HotB (calibrated 1D simulations)
Simulations done by Thomas Ertl
Data
Comprehensive nucleosynthesis analysis for ejecta of compact binary mergers (2015)
O. Just, A. Bauswein, R. Ardevol Pulpillo, S. Goriely, H.-Th. Janka
MNRAS 448, 541 (2015), arXiv eprint 1406.2687
Tracer data
One- and two-dimensional simulation results for the pre-supernova progenitors of Woosley & Heger (2007)
Simulations done by Florian Hanke, data extraction done by Alexander Summa
Data
Trajectories for the exploding cases of the 2013 model series by Sukhbold & Woosley (2014) simulated with HotB (calibrated 1D simulations)
Simulations done by Thomas Ertl
Data
Neutrinos from the Formation, Cooling, and Black Hole Collapse of Neutron stars (2014)
Neutrino signals from models of the PhD Thesis of Lorenz Hüdepohl, TU München 2014
Neutrino data
Two- and three-dimensional simulations of an 11.2, a 27, and a 20 solar-mass progenitor (2013)
27 solar-mass case published in Hanke, F., Mueller, B., Wongwathanarat, A., Marek, A., Janka, H.-Th., 2013, ApJ, 770, 66, arXiv eprint 1303.6269
Neutrino data
Gravitational wave amplitudes
⇒ Movies
Neutrino emission properties obtained by applying observer projections (2014)
The observer projections are obtained from the neutrino data of a 3D simulation of a 27 solar-mass progenitor (see archive entry above) and are partly published in Tamborra et al., 2014, Phys. Rev. D 90, 045032, arXiv eprint 1406.0006.
Neutrino data (observer projections)
A New Multi-Dimensional General Relativistic Neutrino Hydrodynamics Code of Core-Collapse Supernovae. III. Gravitational Wave Signals from Supernova Explosion Models (2013)
Müller, B., Marek, A., & Janka, H.-Th.
ApJ 766, 43 (2013), arXiv eprint 1210.6984
Gravitational wave data
Long-time 3D core-collapse supernova models (2013)
Wongwathanarat, A., Müller, E., & Janka, H.-Th. (unpublished, to be submitted to A&A)
In the simulations, four different progenitor models (two 20 solar-mass RSGs from Woosley & Weaver (1995) and Limongi et al. (2000), a 15 solar-mass BSG from Woosley & Weaver (1988) and a 20 solar-mass BSG from Shigeyama et al. (1990)) are followed up to 30 hours after bounce. The Helmholtz EOS by Timmes & Swesty (2000) is used. The calculations make use of the Yin-Yang grid technique. 3D Newtonian self-gravity and an alpha reaction network consisting of 13(+1) species are included.
Data
New Two-dimensional Models of Supernova Explosions by the Neutrino-heating mechanism: Evidence for Different Instability Regimes in Collapsing Stellar Cores (2012)
Simulations done by Bernhard Müller
ApJ 761, 72 (2012), arXiv eprint 1205.7078
The hydro data are also used in the publication by Fernandez et al. (2014).
Hydro data
Tracer data
Spherically symmetric simulations of the accretion phase for a set of progenitors and EoS (2012)
Simulations done by Lorenz Hüdepohl
Partially published in Phys. Rev. D 85, 085031 (2012), arXiv eprint 1111.4483.
Data
Neutrino intensity for a 15 solar-mass star core collapse (2012)
Simulations done by Lorenz Hüdepohl
The simulation data are used in Phys. Rev. Lett. 108, 061101 (2012) (arXiv eprint 1109.3601) and in Phys. Rev. D 85, 113007 (2012) (arXiv eprint 1204.0971).
Data
Neutrino intensity for a set of progenitors (2012)
Simulations done by Lorenz Hüdepohl (unpublished)
In the one-dimensional simulations, progenitor models from Woosley, Heger & Weaver (2002) and the EOS by Lattimer & Swesty (1991) are used.
Neutrino data
Parametrized 3D models of neutrino-driven supernova explosions: Neutrino emission asymmetries and gravitational-wave signals (2012)
Müller, E., Janka, H.-Th., & Wongwathanarat, A.
A&A 537, A63 (2012), arXiv eprint 1106.6301
Neutrino data
Neutrino Signal of Electron-Capture Supernovae from Core Collapse to Cooling (2010)
Hüdepohl, L., Müller, B., Janka, H.-T., Marek, A., & Raffelt, G. G.
Physical Review Letters 104, 251101 (2010), arXiv eprint 0912.0260
PRL models
Additional data
Three-dimensional simulations of mixing instabilities in supernova explosions (2010)
Hammer, N. J., Janka, H.-Th., & Müller, E.
ApJ 714, 1371 (2010), arXiv eprint 0908.3474
Data
Equation-of-state dependent features in shock-oscillation modulated neutrino and gravitational-wave signals from supernovae (2009)
Marek, A., Janka, H.-Th., & Müller, E.
A&A 496, 475 (2009), arXiv eprint 0808.4136v2
Neutrino and gravitational wave data
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