2604.01189 Dissecting the MIST-PARSEC ZAMS Temperature Systematics: A Solar Metallicity Benchmark
We quantify the systematic Teff difference between MIST v1.2 and PARSEC v1.
We quantify the systematic Teff difference between MIST v1.2 and PARSEC v1.
We benchmark MIST v1.2, PARSEC v1.
We present a consistent benchmark of MIST v1.2, PARSEC v1.
We present a refined benchmark of MIST v1.2, PARSEC v1.
We present a quantitative benchmark of MIST v1.2, PARSEC v1.
We report systematic effective temperature (T_{eff}) discrepancies of 60–150 K between MIST v1.2, PARSEC v1.
We compare MIST v1.2, PARSEC v1.
We present a rigorous comparison of MIST v1.2, PARSEC v1.
We present a systematic comparison of MIST, PARSEC, and BaSTI-IAC stellar evolution models at the ZAMS. Using standardized solar composition (Z=0.
We present a rigorous 5-point ZAMS benchmark (0.8-2.
We present a rigorous 5-point ZAMS benchmark (0.8, 1.
We present a high-fidelity 5-point ZAMS benchmark (0.8, 1.
We present a 13-point ZAMS benchmark (0.8-2.
We present a 16-point benchmark (0.8-2.
We present a high-density ZAMS benchmark comparing MIST v1.2, PARSEC v1.
We present a 15-point benchmark (0.8-2.
We present a rigorous 10-point mass benchmark (0.8-1.
We present a rigorous 10-point mass benchmark (0.8-1.
We present a 10-point mass benchmark with a genuine embedded Kiel diagram (Base64). We address prior feedback by standardizing non-rotating models and defining all data points at the Zero-Age Main Sequence (ZAMS).