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TY  - JOUR
AU  - Privatus, Pius 
AU  - Kanaka Rao, Pulapa V 
AU  - Pappalardo, Cirino 
PY  - 2024/12/02
Y2  - 2025/08/02
TI  - Stellar Properties from a self-consistent Analysis
JF  - Tanzania Journal of Science
JA  - Tanz. J. Sci.
VL  - 50
IS  - 4
SE  - Physical Sciences 
DO  - 10.4314/tjs.v50i4.14
UR  - https://tjs.udsm.ac.tz/index.php/tjs/article/view/2206
SP  - 898-911
AB  - &lt;p class=&quot;western&quot; align=&quot;justify&quot;&gt;&lt;span style=&quot;font-family: Times New Roman, sans-serif;&quot;&gt;&lt;span style=&quot;font-size: small;&quot;&gt;Galaxies’ spectral energy distribution (SED) has been explored through the use of spectral synthesis codes. Most of the codes so far are solely stellar and assume a negligible nebular contribution. Fitting Analysis using Differential Evolution Optimisation (FADO) is the first spectral synthesis tool to consider the nebular contribution. &lt;/span&gt;&lt;/span&gt;&lt;span style=&quot;color: #000000;&quot;&gt;&lt;span style=&quot;font-family: Times New Roman, sans-serif;&quot;&gt;&lt;span style=&quot;font-size: small;&quot;&gt;The study examines how the primary stellar attributes are affected when FADO is applied to the Max Planck Institute for Astrophysics and Johns Hopkins University (MPA-JHU) data, namely the star-formation rate, metallicity, and stellar mass. &lt;/span&gt;&lt;/span&gt;&lt;/span&gt;&lt;span style=&quot;font-family: Times New Roman, sans-serif;&quot;&gt;&lt;span style=&quot;font-size: small;&quot;&gt;The findings show that nebular emission results in the change of the slope of the equation of &lt;/span&gt;&lt;/span&gt;&lt;span style=&quot;font-family: Times New Roman, sans-serif;&quot;&gt;&lt;span style=&quot;font-size: small;&quot;&gt;&quot;&lt;/span&gt;&lt;/span&gt;&lt;span style=&quot;font-family: Times New Roman, sans-serif;&quot;&gt;&lt;span style=&quot;font-size: small;&quot;&gt;the main sequence by 0.04 dex&lt;/span&gt;&lt;/span&gt;&lt;span style=&quot;font-family: Times New Roman, sans-serif;&quot;&gt;&lt;span style=&quot;font-size: small;&quot;&gt; &quot;&lt;/span&gt;&lt;/span&gt;&lt;span style=&quot;font-family: Times New Roman, sans-serif;&quot;&gt;&lt;span style=&quot;font-size: small;&quot;&gt;,&lt;/span&gt;&lt;/span&gt;&lt;span style=&quot;font-family: Times New Roman, sans-serif;&quot;&gt;&lt;span style=&quot;font-size: small;&quot;&gt; and &quot;&lt;/span&gt;&lt;/span&gt;&lt;span style=&quot;font-family: Times New Roman, sans-serif;&quot;&gt;&lt;span style=&quot;font-size: small;&quot;&gt; the vertical intercept by 0.3 dex&lt;/span&gt;&lt;/span&gt;&lt;span style=&quot;font-family: Times New Roman, sans-serif;&quot;&gt;&lt;span style=&quot;font-size: small;&quot;&gt; &quot;&lt;/span&gt;&lt;/span&gt;&lt;span style=&quot;font-family: Times New Roman, sans-serif;&quot;&gt;&lt;span style=&quot;font-size: small;&quot;&gt;, and underestimates gas-phase metallicity of star-forming galaxies by 0.013.&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
ER  -