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An analysis of the internal conditions of galaxies at z≈0 1 and the identifying features of galaxy sub types

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Figure

Figure 1. The remaining data plotted according to their R.A.and Dec positions which are in the previously mentioned red-shiftrange and which will be used for analysis.
Figure 3. Ratio of NFluxes, displaying the separation of each galaxy type; star-ii(6584)/Hα Fluxes against Oiii(5007)/Hβforming(Blue), Starburst(Green) and AGN (Magenta)
Table 1. Table showing the process taken to remove unwanted data from the catalogues. At each step in the process, the exactstatement used in addition to the one from the previous step to create a a new subset of the original data is quoted (using the subs
Figure 4. Intial classification of passive galaxies, defined as thoseHpossible passive galaxies under this condition, which constitutewith error on Hydrogen Hα Balmer line greater than Hydrogenα Balmer line itself
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