Changes between Version 16 and Version 17 of fullforce_SAStest1
- Timestamp:
- Jan 31, 2014, 2:04:19 PM (12 years ago)
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fullforce_SAStest1
v16 v17 122 122 sersic model was the best. 123 123 124 SDSS did not measure a sersic model so we compare the SDSS model magnitude r with our sersicemagnitude.124 SDSS did not measure a sersic model so we compare the SDSS model magnitude r with our Sersic magnitude. 125 125 Here is a scatter plot comparing the two magnitudes and a histogram of the difference. 126 126 127 127 [[Image(dsermag_v_r.jpg)]] [[Image(dsermag.jpg)]] 128 128 129 As expected, the measured sersic index for these galaxies is concentrated at low values. Interestingly the peak is130 less than 1 ( exponential model).129 As expected, the measured Sersic index for these galaxies is concentrated at low values. Interestingly the peak is 130 less than 1 (where the Sersic model function is equivalent to an exponential model). 131 131 132 132 [[Image(sersic_index_exp.jpg)]] 133 133 134 134 135 ==== de Vaucouleurs Galaxies ==== 136 137 20030 of the 100513 objects matched to SDSS galaxies have devFrac_r = 1 indicating that the SDSS composite 138 model was equal to their deV model. 9196 of these had psphotStack extended model fits. The dev model was the best fit for 2046, 4661 sersic, and surprisingly for 2489 139 objects the exp model had the lowest chisq. 140 141 ===== devGalaxies dev model ===== 142 143 Here are plots of the difference between SDSS model fit major axis and magnitude and the psphot full force summary results 144 for the devGalaxies. 145 146 [[Image(ddevrad.jpg)]] [[Image(ddevmag.jpg)]] 147 148 And a scatter plot of the two differences. 149 150 [[Image(ddevmag_v_ddevrad.jpg)]] 151 152 And the magnitude difference versus SDSS magnitude. 153 154 [[Image(ddevmag_v_r.jpg)]] 155 156 157
