new run happened

Author: actions-user

docs/_build/html/2303.12101.md

@@ -86,7 +86,7 @@ $\newcommand{\thebibliography}{\DeclareRobustCommand{\VAN}[3]{##3}\VANthebibliog
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-Fabian Scheuermann, et al. -- incl., <mark><mark>Kathryn Kreckel</mark></mark>, <mark><mark>Stephen Hannon</mark></mark>, <mark><mark>Janice C. Lee</mark></mark>, <mark><mark>Frank Bigiel</mark></mark>, <mark><mark>Eva Schinnerer</mark></mark>
+F. Scheuermann, et al.
 
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@@ -95,3 +95,24 @@ Fabian Scheuermann, et al. -- incl., <mark><mark>Kathryn Kreckel</mark></mark>,
 
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+<div id="div_fig1">
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+<img src="tmp_2303.12101/fig/nebulae_age_tracers_corner.png" alt="Fig6" width="100%"/>
+
+**Figure 6. -** Comparison between the proposed age tracers for the full \HII region catalogue. The nebulae are grouped by their host galaxy, sorted by stellar mass $M_{\star}$, with the median of the entire sample indicated by a black line. The 68 and 98 percentile ranges are shaded in grey. (*fig:age_tracers_corner*)
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+</div>
+<div id="div_fig2">
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+<img src="tmp_2303.12101/fig/overlap_rgb.png" alt="Fig1" width="100%"/>
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+**Figure 1. -** Examples for the overlap between the \HII regions and stellar associations in \galaxyname{NGC}{1365}. The cutouts show a three colour composite images, based on the 5 available _HST_ bands, overlaid with the $\HA$ line emission of MUSE in red. The boundaries of the \HII regions are shown in red and the stellar associations in blue. Flags that characterise the overlap between the two catalogues are showcased in this figure. (*fig:overlap*)
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+</div>
+<div id="div_fig3">
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+<img src="tmp_2303.12101/fig/catalogue_properties_2D_hist.png" alt="Fig2" width="100%"/>
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+**Figure 2. -** Distribution of masses and ages of the stellar associations in the matched catalogue (the \texttt{one-to-one} sample). The black lines mark the cuts that we apply to the sample to ensure a fully sampled IMF (more massive than $>\SI{e4}{\Msun}$) and to only include young clusters that should be associated with ionized gas (younger than $\leq\SI{8}{\mega\year}$). The mass cut leaves us with a sample of \num{1014} objects and the age cut with \num{3531}. Applying both cuts results in a sample of \num{756} objects. (*fig:catalogue_properties_2D_hist_v2*)
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+</div>

docs/_build/html/2303.12110.md

@@ -54,7 +54,7 @@ $\newcommand{\Magdis}{{\color{blue} M21}}$</div>
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-David Blánquez-Sesé, et al. -- incl., <mark>E. Schinnerer</mark>
+D. Blánquez-Sesé, et al. -- incl., <mark>E. Schinnerer</mark>
 
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