Table 1.
Summary of some intermediate- and high-resolution SSP models in the literature, compared to the present work.
| Reference | Code | Range (Å) | δλ (Å) | Rth | Z |
|---|---|---|---|---|---|
| LEB04 | PEGASE-HR | 4000 − 6800 | 0.55 | 9091 | 0.0002 − 0.05 |
| GON05 | Sed@ | 3000 − 7000 | 0.30 | 16 667 | 0.002 − 0.05 |
| PER09 | BASTI iso. | 2500 − 10 500 | 1.00 | 5000 | 0.0001 − 0.04 |
| M&S11 | Maraston | 1000 − 25 000 | 0.25 | 20 000 | 0.0001 − 0.04 |
| VAZ16 | MILES | 1680 − 500 000 | 0.90 | 5556 | 0.0001 − 0.04 |
| CON18 | FSPS | 3700 − 24 000 | 1.67 | 3000 | 0.00044 − 0.028 |
| CBC20 | GALAXEV | 3540 − 7410 | 0.90 | 3000 | 0.0002 − 0.030 |
| Ma20 | Fuel-consumption code | 3600 − 10 300 | 0.8–2.4 | 1800 | 0.00007 − 0.03 |
| XSL | 3500 − 24 000 | 0.12–0.8 | 10 000 | 0.0001 − 0.03 | |
| MI21 | PYPOPSTAR | 91–24 000 | 0.10 | 50 000 | 0.004 − 0.05 |
| This work | PYPOPSTAR | 2500–10 500 | 0.10 | 50 000 | 0.0001 − 0.05 |
Notes. References. LEB04: Le Borgne et al. (2004); GON05: González Delgado et al. (2005); PER09: Percival et al. (2009); M&S11: Maraston & Strömbäck (2011); VAZ16: Vazdekis et al. (2016); CON18: Conroy et al. (2018); CBC20: Coelho et al. (2020); Ma20: Maraston et al. (2020); MI21: Millán-Irigoyen et al. (2021); XSL: Verro et al. (2022).
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