<?xml version="1.0" encoding="utf-8" ?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom" xmlns:r="https://r-universe.dev"><channel><title>chesterdeocaris.r-universe.dev</title><link>https://chesterdeocaris.r-universe.dev</link><description>Recent package updates in chesterdeocaris</description><generator>R-universe</generator><image><url>https://github.com/chesterdeocaris.png</url><title>R packages by chesterdeocaris</title><link>https://chesterdeocaris.r-universe.dev</link></image><lastBuildDate>Wed, 10 Jan 2024 02:39:46 GMT</lastBuildDate><item><title>[chesterdeocaris] PUPMCR 0.2.0</title><author>ccdeocaris@pup.edu.ph (Chester Deocaris)</author><description>Image-based color matching using the &quot;Mycological Colour
Chart&quot; by Rayner (1970, ISBN:9780851980263) and its associated
fungal pigments. This package will assist mycologists in
identifying color during morphological analysis.</description><link>https://github.com/r-universe/chesterdeocaris/actions/runs/25782033956</link><pubDate>Wed, 10 Jan 2024 02:39:46 GMT</pubDate><r:package>PUPMCR</r:package><r:version>0.2.0</r:version><r:status>success</r:status><r:repository>https://chesterdeocaris.r-universe.dev</r:repository><r:upstream>https://github.com/cran/PUPMCR</r:upstream></item><item><title>[chesterdeocaris] PUPAK 0.1.1</title><author>ccdeocaris@pup.edu.ph (Chester Deocaris)</author><description>Contains model fitting functions for linear and non-linear
adsorption kinetic and diffusion models. Adsorption kinetics is
used for characterizing the rate of solute adsorption and the
time necessary for the adsorption process. Adsorption kinetics
offers vital information on adsorption rate, adsorbent
performance in response time, and mass transfer processes. In
addition, diffusion models are included in the package as
solute diffusion affects the adsorption kinetic experiments.
This package consists of 20 adsorption and diffusion models,
including Pseudo First Order (PFO), Pseudo Second Order (PSO),
Elovich, and Weber-Morris model (commonly called the
intraparticle model) stated by Plazinski et al. (2009)
&lt;doi:10.1016/j.cis.2009.07.009&gt;. This package also contains a
summary function where the statistical errors of each model are
ranked for a more straightforward determination of the best fit
model.</description><link>https://github.com/r-universe/chesterdeocaris/actions/runs/25910577868</link><pubDate>Fri, 01 Jul 2022 14:20:06 GMT</pubDate><r:package>PUPAK</r:package><r:version>0.1.1</r:version><r:status>success</r:status><r:repository>https://chesterdeocaris.r-universe.dev</r:repository><r:upstream>https://github.com/cran/PUPAK</r:upstream></item><item><title>[chesterdeocaris] PUPMSI 0.1.0</title><author>ccdeocaris@pup.edu.ph (Chester Deocaris)</author><description>Contains sixteen moisture sorption isotherm models, which
evaluate the fitness of adsorption and desorption curves for
further understanding of the relationship between moisture
content and water activity. Fitness evaluation is conducted
through parameter estimation and error analysis. Moreover,
graphical representation, hysteresis area estimation, and
isotherm classification through the equation of Blahovec &amp;
Yanniotis (2009) &lt;doi:10.1016/j.jfoodeng.2008.08.007&gt; which is
based on the classification system introduced by Brunauer et.
al. (1940) &lt;doi:10.1021/ja01864a025&gt; are also included for the
visualization of models and hysteresis.</description><link>https://github.com/r-universe/chesterdeocaris/actions/runs/25788718850</link><pubDate>Tue, 31 May 2022 09:50:04 GMT</pubDate><r:package>PUPMSI</r:package><r:version>0.1.0</r:version><r:status>success</r:status><r:repository>https://chesterdeocaris.r-universe.dev</r:repository><r:upstream>https://github.com/cran/PUPMSI</r:upstream></item><item><title>[chesterdeocaris] extraterrestrial 0.1.0</title><author>ccdeocaris@pup.edu.ph (Chester C. Deocaris)</author><description>Finding life outside the planet Earth several is the
ultimate goal of an astrobiologist. Using known astronomical
measurements and assumptions the probability of
extraterrestrial life existence could be estimated. Equations
such as the Drake equation (1961) as stated in the paper of
Molina (2019) &lt;arXiv:1912.01783&gt;, Seager (2013)
&lt;https://www.space.com/22648-drake-equation-alien-life-seager.html&gt;
and Foucher et al, (2017) &lt;doi:10.3390/life7040040&gt; are
included in the 'extraterrestrial' package.</description><link>https://github.com/r-universe/chesterdeocaris/actions/runs/25714958407</link><pubDate>Sat, 28 Mar 2020 10:30:02 GMT</pubDate><r:package>extraterrestrial</r:package><r:version>0.1.0</r:version><r:status>success</r:status><r:repository>https://chesterdeocaris.r-universe.dev</r:repository><r:upstream>https://github.com/cran/extraterrestrial</r:upstream></item></channel></rss>