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1 Introduction and Summary |
11 |
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1.1 Comparison of Distant and Nearby Galaxies |
12 |
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1.2 Limitations of Current Nearby Samples |
12 |
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1.3 Nearby Field Galaxy Survey Project Goals |
13 |
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1.4 Outline of this Thesis |
13 |
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1.4.1 UBR Surface Photometry |
13 |
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1.4.2 Nuclear and Integrated Spectrophotometry |
14 |
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1.4.3 [O II]: How Well Traceth the Tracer? |
14 |
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1.4.4 Quantifying Appearance |
15 |
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1.5 The Nearby Field Galaxy Survey and Beyond |
15 |
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1.5.1 Data in Hand |
15 |
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1.5.2 Observations in Progress |
16 |
1.5.3 Future Observations
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16
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2 Surface photometry of nearby field galaxies |
19 |
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2.1 Sample Selection |
20 |
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2.1.1 Merits and Limitations of the Sample |
22 |
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2.2 Observations, Reduction, and Calibration |
28 |
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2.2.1 Observations |
28 |
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2.2.2 Data Reduction |
28 |
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2.2.3 Calibration |
29 |
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2.2.4 Total Magnitudes: Extrapolation to Infinity |
30 |
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2.2.5 Evaluation of the Data Quality |
30 |
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2.3 Photometric Results |
31 |
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2.3.1 Data Presentation |
31 |
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ATLAS OF IMAGES AND RADIAL PROFILES |
33 |
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2.3.2 Properties of Our Sample |
50 |
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2.4 Summary |
54 |
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2.A Discussion of Individual Objects |
61 |
2.B Calibration of the Intensity Profiles
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62
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3 Spectrophotometry of nearby field galaxies |
65 |
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3.1 Observations and Data Reduction |
66 |
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3.1.1 Observations |
66 |
3.1.2 Data Reduction
|
72
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