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Changes between Version 16 and Version 17 of fullforce_SAStest1


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Timestamp:
Jan 31, 2014, 2:04:19 PM (12 years ago)
Author:
bills
Comment:

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  • fullforce_SAStest1

    v16 v17  
    122122sersic model was the best.
    123123
    124 SDSS did not measure a sersic model so we compare the SDSS model magnitude r with our sersice magnitude.
     124SDSS did not measure a sersic model so we compare the SDSS model magnitude r with our Sersic magnitude.
    125125Here is a scatter plot comparing the two magnitudes and a histogram of the difference.
    126126
    127127[[Image(dsermag_v_r.jpg)]] [[Image(dsermag.jpg)]]
    128128
    129 As expected, the measured sersic index for these galaxies is concentrated at low values. Interestingly the peak is
    130 less than 1 (exponential model).
     129As expected, the measured Sersic index for these galaxies is concentrated at low values. Interestingly the peak is
     130less than 1 (where the Sersic model function is equivalent to an exponential model).
    131131
    132132[[Image(sersic_index_exp.jpg)]]
    133133
    134134 
     135==== de Vaucouleurs Galaxies ====
     136
     13720030 of the 100513 objects matched to SDSS galaxies have devFrac_r = 1 indicating that the SDSS composite
     138model 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
     139objects the exp model had the lowest chisq.
     140
     141===== devGalaxies dev model =====
     142
     143Here are plots of the difference between SDSS model fit major axis and magnitude and the psphot full force summary results
     144for the devGalaxies.
     145
     146[[Image(ddevrad.jpg)]] [[Image(ddevmag.jpg)]]
     147
     148And a scatter plot of the two differences.
     149
     150[[Image(ddevmag_v_ddevrad.jpg)]]
     151
     152And the magnitude difference versus SDSS magnitude.
     153
     154[[Image(ddevmag_v_r.jpg)]]
     155
     156
     157