<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Interactive Modeling |</title><link>https://mrkrmh.github.io/tags/interactive-modeling/</link><atom:link href="https://mrkrmh.github.io/tags/interactive-modeling/index.xml" rel="self" type="application/rss+xml"/><description>Interactive Modeling</description><generator>HugoBlox Kit (https://hugoblox.com)</generator><language>en-us</language><lastBuildDate>Mon, 20 Apr 2026 00:00:00 +0000</lastBuildDate><image><url>https://mrkrmh.github.io/media/icon_hu_da05098ef60dc2e7.png</url><title>Interactive Modeling</title><link>https://mrkrmh.github.io/tags/interactive-modeling/</link></image><item><title>Metallicity Calibrations in AGNs: N₂O₂ and N₂S₂ Diagnostics</title><link>https://mrkrmh.github.io/projects/xray-agn-diagnostics/</link><pubDate>Mon, 20 Apr 2026 00:00:00 +0000</pubDate><guid>https://mrkrmh.github.io/projects/xray-agn-diagnostics/</guid><description>&lt;p&gt;Standard strong-line diagnostics are often heavily biased by the intense radiation fields of AGNs. This ongoing project focuses on deriving new metallicity calibrations—specifically utilizing the N₂O₂ and N₂S₂ emission line ratios—that remain unaffected by structural nebular variations. By parameterizing models explicitly by intrinsic 2-10 keV X-ray luminosity, these tools lay the groundwork for analyzing high-resolution spectra from next-generation observatories.&lt;/p&gt;
&lt;h3 id="interactive-calibrations"&gt;Interactive Calibrations&lt;/h3&gt;
&lt;p&gt;&lt;strong&gt;N₂O₂ Simulator&lt;/strong&gt;
Demonstrating the robustness of the [N &lt;span style="font-variant: small-caps;"&gt;ii&lt;/span&gt;]/[O &lt;span style="font-variant: small-caps;"&gt;ii&lt;/span&gt;] ratio against X-ray luminosity variations compared to traditional diagnostics.&lt;/p&gt;
&lt;iframe src="https://mrkrmh.github.io/simulations/N2O2_Clean_Diagnostic.html" width="100%" height="550px" style="border:none; border-radius: 12px;"&gt;&lt;/iframe&gt;
&lt;p&gt;&lt;strong&gt;N₂S₂ Simulator&lt;/strong&gt;
Illustrating the volume-canceling properties of the [N &lt;span style="font-variant: small-caps;"&gt;ii&lt;/span&gt;]/[S &lt;span style="font-variant: small-caps;"&gt;ii&lt;/span&gt;] ratio and its independence from electron density fluctuations.&lt;/p&gt;
&lt;iframe src="https://mrkrmh.github.io/simulations/N2S2_Interactive_Pro.html" width="100%" height="550px" style="border:none; border-radius: 12px;"&gt;&lt;/iframe&gt;</description></item></channel></rss>