Changes between Version 15 and Version 16 of psphot_extended_source_fit
- Timestamp:
- Sep 6, 2013, 11:50:40 AM (13 years ago)
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psphot_extended_source_fit
v15 v16 32 32 I(r) = I(0) exp[ -k * R ** (1 / m) ] 33 33 34 psphot extended source parameters mea usred34 psphot extended source parameters measured 35 35 EXT_INST_MAG 36 36 EXT_WIDTH_MAJ … … 40 40 }}} 41 41 42 Since all of the simulated galax es in this sample have bulge inclination == 1 and disk inclination == 1,42 Since all of the simulated galaxies in this sample have bulge inclination == 1 and disk inclination == 1, 43 43 the major an minor axes should be equal and the angle will 44 44 unmeasurable due to noise. … … 79 79 [[Image(bulge_widths.jpg)]] 80 80 81 == Exponential Model == 82 {{ 83 Functional Form 81 84 85 I(r) = I(0) exp[ -k * R ] 86 87 psphot extended source parameters measured 88 EXT_INST_MAG 89 EXT_WIDTH_MAJ 90 EXT_WIDTH_MIN 91 EXT_THETA 92 }}} 93 94 Since all of the simulated galaxies in this sample have bulge inclination == 1 and disk inclination == 1, 95 the major an minor axes should be equal and the angle will 96 unmeasurable due to noise. 97 98 === Exponential magnitudes === 99 In general the magnitude fit with exponential model is slightly less than the expected value. However when the galaxy 100 sample is restricted to pure disks the magnitude differences are clustered around zero. 101 102 [[Image(dmag_exp.jpg)]] [[Image(dmag_exp_disks.jpg]]
