The young massive SMC cluster NGC 330 seen by MUSE. III. Stellar parameters and rotational velocities - diagnostic plots

<p>This Zenodo repository hosts additional diagnostic plots for the article &quot;<em>The young massive SMC cluster NGC 330 seen by MUSE. III. Stellar parameters and rotational velocities</em>&quot; by Bodensteiner et al. 2023. It provides three diagnostic figures for each of the 282 stars in the sample described in the paper. Three example figures are given for one star (#654) in the Figures 2, 3, and 4 in the paper.</p> <p>Here, we provide a .zip archive with three additional figures for all other stars that are similar to the ones in the paper:</p> <ol> <li>the <strong>spectroscopic fit</strong> (&quot;<em>id###_spec.pdf</em>&quot;): Each panel, one for each of the six diagnostic spectral regions, shows the combined spectrum (black) and the best-fitting tlusty model (red). Grayed-out regions are only shown for comparison but were not included in the fit, which may vary from star to star.</li> <li>the <strong>photometric fit</strong> (&quot;<em>id###_phot.pdf</em>&quot;): The top panel shows a comparison between the observed HST&nbsp; fluxes (black crosses) and the flux (colored circles) computed from the best-fit model (gray line) by&nbsp; convolution with the HST filters (colored lines). The bottom panel gives residuals.</li> <li>the <strong>combined fit results</strong> (&quot;<em>correlationplot_comb_id###.pdf</em>&quot;): The diagonal gives the &chi;2-distribution as a function of each parameter and the panels below show 2-dimensional &chi;2 -maps. The red line marks the 95% confidence level.</li> </ol> <p>The star ids (###) correspond to the ones provided in Table 1 (also available at the CDS).</p>