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Changes between Version 15 and Version 16 of psphot_extended_source_fit


Ignore:
Timestamp:
Sep 6, 2013, 11:50:40 AM (13 years ago)
Author:
bills
Comment:

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  • psphot_extended_source_fit

    v15 v16  
    3232    I(r) = I(0) exp[ -k * R ** (1 / m) ]
    3333
    34 psphot extended source parameters meausred
     34psphot extended source parameters measured
    3535   EXT_INST_MAG
    3636   EXT_WIDTH_MAJ
     
    4040}}}
    4141
    42 Since all of the simulated galaxes in this sample have bulge inclination == 1 and disk inclination == 1,
     42Since all of the simulated galaxies in this sample have bulge inclination == 1 and disk inclination == 1,
    4343the major an minor axes should be equal and the angle will
    4444unmeasurable due to noise.
     
    7979[[Image(bulge_widths.jpg)]]
    8080
     81== Exponential Model ==
     82{{
     83Functional Form
    8184
     85    I(r) = I(0) exp[ -k * R ]
     86
     87psphot extended source parameters measured
     88   EXT_INST_MAG
     89   EXT_WIDTH_MAJ
     90   EXT_WIDTH_MIN
     91   EXT_THETA
     92}}}
     93
     94Since all of the simulated galaxies in this sample have bulge inclination == 1 and disk inclination == 1,
     95the major an minor axes should be equal and the angle will
     96unmeasurable due to noise.
     97
     98=== Exponential magnitudes ===
     99In general the magnitude fit with exponential model is slightly less than the expected value. However when the galaxy
     100sample is restricted to pure disks the magnitude differences are clustered around zero.
     101
     102[[Image(dmag_exp.jpg)]] [[Image(dmag_exp_disks.jpg]]