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Changes between Version 18 and Version 19 of psphot_extended_source_fit


Ignore:
Timestamp:
Sep 6, 2013, 12:09:08 PM (13 years ago)
Author:
bills
Comment:

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  • psphot_extended_source_fit

    v18 v19  
    3232    I(r) = I(0) exp[ -k * R ** (1 / m) ]
    3333
    34 psphot extended source parameters measured
     34psphot extended source parameters measured for PS_MODEL_SERSIC
    3535   EXT_INST_MAG
    3636   EXT_WIDTH_MAJ
     
    8585    I(r) = I(0) exp[ -k * R ]
    8686
    87 psphot extended source parameters measured
     87psphot extended source parameters measured for PS_MODEL_EXP
    8888   EXT_INST_MAG
    8989   EXT_WIDTH_MAJ
     
    108108[[Image(disk_widths_exp.jpg)]]
    109109
     110== de Vacouleur Model ==
     111The de Vacouleur model provides a good fit to elliptical galaxies. In our sample these are represented by the galaxies
     112with ht == -6 pure disks
     113
     114{{{
     115
     116    I(r) = I(0) exp[ -k * R ** (1 / 4) ]
     117
     118psphot extended source parameters measured for PS_MODE_DEV
     119   EXT_INST_MAG
     120   EXT_WIDTH_MAJ
     121   EXT_WIDTH_MIN
     122   EXT_THETA
     123}}
     124
     125It looks like there is something wrong with the DEV models
     126
     127[[Image(dmag_dev.jpg)]] [[Image(dmag_dev_bulges.jpg)]]