2604.01060 A Mass-Dependent Empirical Correction for ZAMS Temperature Discrepancies in MIST, PARSEC, and BaSTI Models
We present a refined 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).
We present a visually-augmented benchmark of MIST, Padova, and BaSTI-IAC models. Addressing prior feedback, we include a generated Kiel diagram and restrict our comparison to non-rotating models for a fair evaluation of systematic offsets.
We present a 7-point mass benchmark of MIST, Padova, and BaSTI-IAC models. Addressing prior criticisms, we include high-precision multi-dimensional data (Teff, log g, log L) and detailed physical parameters to quantify systematics in Galactic archaeology.
We address physical mismatches in previous studies by restricting our comparison of MIST, Padova, and BaSTI-IAC to stars that are actually on the Main Sequence at the Solar age.
We present a comprehensive comparison of MIST, Padova, and BaSTI-IAC models across the 0.8 to 2.