|$M_{\rm ZAMS}$| ranges of PISN progenitors, for representative metallicities, obtained with the parsec-i, parsec-ii, and franec stellar evolution tracks. The ranges at metallicities in between the original ones from the stellar tracks are obtained via interpolation, as described in the text. All values are in solar units. Blanks indicate cases with no PISN, at |$Z\gt Z_{\rm max}$|. Masses |$\gt 300\:\mathrm{ M}_{\rm \odot }$| are fixed to |$300\:\mathrm{ M}_{\rm \odot }$|, that is, the highest |$M_{\rm up}$| considered in this work (see Appendix B for an additional variation with |$M_{\rm up}=600\:\mathrm{ M}_{\rm \odot }$|). The double intervals at |$Z=1\times 10^{-4}$| of parsec-ii are due to the non-monotonicity of the corresponding stellar track, which exits the PISN mass range and then re-enters again (see fig. 8 of Iorio et al. 2022).
 | 1 × 10−4 | 1 × 10−3 | 4 × 10−3 | 8 × 10−3 | 1 × 10−2 | 2 × 10−2 |
|---|---|---|---|---|---|---|
| parsec-i | ||||||
| 45–120 | 108–257 | 109–300 | 158–300 | 178–222 | – | – |
| 55–110 | 126–237 | 128–300 | 195–300 | – | – | – |
| 60–105 | 138–228 | 139–300 | 213–300 | – | – | – |
| parsec-ii | ||||||
| 45–120 | 107–229 | 112–239 | 92–221 | 111–294 | 133–300 | – |
| 55–110 | 117–150 | 130–227 | 109–202 | 138–270 | 166–300 | – |
| 153–211 | ||||||
| 60–105 | 125–145 | 140–221 | 118–193 | 151–258 | 182–300 | - |
| 158–203 | ||||||
franec | ||||||
| 45–120 | 111–262 | 113–272 | 136–300 | 183–300 | 220–300 | – |
| 55–110 | 131–242 | 134–251 | 173–300 | 233–300 | 282–300 | – |
| 60–105 | 141–232 | 145–240 | 192–300 | 259–300 | – | – |
| 1 × 10−4 | 1 × 10−3 | 4 × 10−3 | 8 × 10−3 | 1 × 10−2 | 2 × 10−2 |
|---|---|---|---|---|---|---|
| parsec-i | ||||||
| 45–120 | 108–257 | 109–300 | 158–300 | 178–222 | – | – |
| 55–110 | 126–237 | 128–300 | 195–300 | – | – | – |
| 60–105 | 138–228 | 139–300 | 213–300 | – | – | – |
| parsec-ii | ||||||
| 45–120 | 107–229 | 112–239 | 92–221 | 111–294 | 133–300 | – |
| 55–110 | 117–150 | 130–227 | 109–202 | 138–270 | 166–300 | – |
| 153–211 | ||||||
| 60–105 | 125–145 | 140–221 | 118–193 | 151–258 | 182–300 | - |
| 158–203 | ||||||
franec | ||||||
| 45–120 | 111–262 | 113–272 | 136–300 | 183–300 | 220–300 | – |
| 55–110 | 131–242 | 134–251 | 173–300 | 233–300 | 282–300 | – |
| 60–105 | 141–232 | 145–240 | 192–300 | 259–300 | – | – |
|$M_{\rm ZAMS}$| ranges of PISN progenitors, for representative metallicities, obtained with the parsec-i, parsec-ii, and franec stellar evolution tracks. The ranges at metallicities in between the original ones from the stellar tracks are obtained via interpolation, as described in the text. All values are in solar units. Blanks indicate cases with no PISN, at |$Z\gt Z_{\rm max}$|. Masses |$\gt 300\:\mathrm{ M}_{\rm \odot }$| are fixed to |$300\:\mathrm{ M}_{\rm \odot }$|, that is, the highest |$M_{\rm up}$| considered in this work (see Appendix B for an additional variation with |$M_{\rm up}=600\:\mathrm{ M}_{\rm \odot }$|). The double intervals at |$Z=1\times 10^{-4}$| of parsec-ii are due to the non-monotonicity of the corresponding stellar track, which exits the PISN mass range and then re-enters again (see fig. 8 of Iorio et al. 2022).
| 1 × 10−4 | 1 × 10−3 | 4 × 10−3 | 8 × 10−3 | 1 × 10−2 | 2 × 10−2 |
|---|---|---|---|---|---|---|
| parsec-i | ||||||
| 45–120 | 108–257 | 109–300 | 158–300 | 178–222 | – | – |
| 55–110 | 126–237 | 128–300 | 195–300 | – | – | – |
| 60–105 | 138–228 | 139–300 | 213–300 | – | – | – |
| parsec-ii | ||||||
| 45–120 | 107–229 | 112–239 | 92–221 | 111–294 | 133–300 | – |
| 55–110 | 117–150 | 130–227 | 109–202 | 138–270 | 166–300 | – |
| 153–211 | ||||||
| 60–105 | 125–145 | 140–221 | 118–193 | 151–258 | 182–300 | - |
| 158–203 | ||||||
franec | ||||||
| 45–120 | 111–262 | 113–272 | 136–300 | 183–300 | 220–300 | – |
| 55–110 | 131–242 | 134–251 | 173–300 | 233–300 | 282–300 | – |
| 60–105 | 141–232 | 145–240 | 192–300 | 259–300 | – | – |
| 1 × 10−4 | 1 × 10−3 | 4 × 10−3 | 8 × 10−3 | 1 × 10−2 | 2 × 10−2 |
|---|---|---|---|---|---|---|
| parsec-i | ||||||
| 45–120 | 108–257 | 109–300 | 158–300 | 178–222 | – | – |
| 55–110 | 126–237 | 128–300 | 195–300 | – | – | – |
| 60–105 | 138–228 | 139–300 | 213–300 | – | – | – |
| parsec-ii | ||||||
| 45–120 | 107–229 | 112–239 | 92–221 | 111–294 | 133–300 | – |
| 55–110 | 117–150 | 130–227 | 109–202 | 138–270 | 166–300 | – |
| 153–211 | ||||||
| 60–105 | 125–145 | 140–221 | 118–193 | 151–258 | 182–300 | - |
| 158–203 | ||||||
franec | ||||||
| 45–120 | 111–262 | 113–272 | 136–300 | 183–300 | 220–300 | – |
| 55–110 | 131–242 | 134–251 | 173–300 | 233–300 | 282–300 | – |
| 60–105 | 141–232 | 145–240 | 192–300 | 259–300 | – | – |
