<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Projectsofts | Borja Perez-Diaz</title><link>https://borja-perez-diaz.github.io/me/projectsoft/</link><atom:link href="https://borja-perez-diaz.github.io/me/projectsoft/index.xml" rel="self" type="application/rss+xml"/><description>Projectsofts</description><generator>Hugo Blox Builder (https://hugoblox.com)</generator><language>en-us</language><lastBuildDate>Tue, 01 Sep 2020 00:00:00 +0000</lastBuildDate><image><url>https://borja-perez-diaz.github.io/me/media/icon_hu7729264130191091259.png</url><title>Projectsofts</title><link>https://borja-perez-diaz.github.io/me/projectsoft/</link></image><item><title>HII-CHI-Mistry</title><link>https://borja-perez-diaz.github.io/me/projectsoft/hcm/</link><pubDate>Tue, 01 Sep 2020 00:00:00 +0000</pubDate><guid>https://borja-perez-diaz.github.io/me/projectsoft/hcm/</guid><description>&lt;p>HII-CHI-Mistry is a collection of python subroutines aimed at the calculation of chemical abundances and physical properties using emission line fluxes from ionised gaseous nebulae.&lt;/p></description></item></channel></rss>