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Contents
List of Tables
List of Figures
Overview
Introduction
Present Work
Future Possibilities
Observations: the raw material
The sample
Observations
Calibration
Preprocessing
Dark Subtraction
Bias Subtraction
Flat fielding
Cosmic Ray Removal
Sky Subtraction
Aligning multiple frames
Combining multiple frames
Standardization
Correction for Galactic Extinction
K-correction
Control Sample
Brightness distribution
Introduction
The radial profile
Introduction
Obtaining the fit
Procedure Adopted for the Sample
The different components
Ellipticals and bulges
Hubble's Law
King's Profiles
de Vaucouleurs' law
Petrosian's
function
The Jaffe Profile
Dehnen models
The disk
The point source
Decomposing the profile
Free Parameters
Input parameters
PSF
Model generation
Goodness of fit
Output
Procedure for minimization
Fitting Considerations
Consistency checks
2D distribution
:
Position Angle
Ellipticity
Summary
Scale lengths at different wavelengths
Results of profile fits
Goodness of fit
Disk parameters
Bulge parameters
Color gradients
Results for the samples
Color gradients and scale length ratios
Preference for scale lengths
Discussion
Extrapolated profiles
Conclusions
Radio galaxies with disks
Disky galaxies
Radio galaxies
1222-252
1053-282
1006-214
0952-224
1215-215
Control Sample
1251/190
1323/1477
1323/1673
1329/234
Morphological Signatures of disks
Discussion
Dusty galaxies
Introduction
Detection techniques
Color maps
Small scale features
Extrapolated profiles
Dust lane galaxies
0354-263
0420-263
1254-268
1257-253
1323-271
1344-241
Discussion and conclusions
Radio structure: using a different eye
Introduction
Optical-radio correlations
Disky galaxies
Blue centers
Optical luminosity
Morphological peculiarities and dust
Harmonic components
Induced star formation
Conclusions
Ages: how recent is the blue
Introduction
The existing picture
Synthetic spectra
Galaxy spectra
Modus operandi
Age of the most recent starburst
Conclusions
The emerging picture
The work goes on
Morphological processing
Dilation and erosion
Opening and closing
Gradient
Individual objects
0344-291
0349-278
0354-263
0420-263
0434-225
0446-206
0453-206
0520-289
0938-205
0950-239
0952-224
1006-214
1033-251
1048-238
1053-282
1056-272
1103-244
1126-246
1215-215
1222-252
1251-289
1254-268
1257-253
1303-215
1323-271
1329-257
1343-253
1344-241
1346-252
1354-251
References