Open Access
Table 4
Code outputs and computed models.
Code name | RT method | Bolometric flux | Spectrum or SED | Early times | Nebular times | Computed models | toy06 | toy01 DDC10 | DDC25 |
---|---|---|---|---|---|---|---|---|---|
ARTIS | MC | Calculated | ✓ | ✓ | ✓ | ✓ | ✕ | ✓ | ✕ |
CMFGEN | RTE-CMF | Calculated | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ |
CRAB | RH-1G | Calculated | ✕ | ✓ | ✕ | ✓ | ✕ | ✕ | ✕ |
KEPLER | FLD | Calculated | ✕ | ✓ | ✕ | ✓ | ✓ | ✓ | ✓ |
SEDONA | MC | Calculated | ✓ | ✓ | ✕ | ✓ | ✓ | ✓ | ✕ |
STELLA | RH-MG | Calculated | ✓ | ✓ | ✕ | ✓ | ✓ | ✓ | ✓ |
SUMO | MC | Calculated | ✓ | ✕ | ✓ | ✓ | ✓ | ✕ | ✕ |
SuperNu | MC | Calculated | ✓ | ✓ | ✕ | ✓ | ✓ | ✓ | ✓ |
TARDIS | MC | Input | ✓ | ✓ | ✕ | ✓ | ✓ | ✓ | ✓ |
URILIGHT | MC | Calculated | ✓ | ✓ | ✕ | ✓ | ✓ | ✓ | ✓ |
Notes. RT Method gives the numerical method used to solve the radiative-transfer equation (see Table 2).
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