| Element |
Content |
Size |
 |
Chapter 1
Chapter 2 |
Why Build Stellar Interferometers?
Elementary Theory of Interferometry |
412 K |
 |
| Chapter 3 |
Beam Combination and Fringe Measurement |
407 K |
|
| Chapter 4 (a) |
Noise and Sensitivity in Interferometry |
380 K |
|
| Chapter 4 (b) |
Noise and Sensitivity in Interferometry (cont.) |
688 K |
|
| Chapter 5 |
Observing Through the Turbulent Atmosphere |
272 K |
|
| Chapter 6 (a) |
Design of Stellar Interferometers |
748 K |
|
| Chapter 6 (b) |
Design of Stellar Interferometers (cont.) |
2,900 K |
|
| Chapter 6 (c) |
Design of Stellar Interferometers (cont.) |
3,900 K |
|
| Chapter 6 (d) |
Design of Stellar Interferometers (cont.) |
3,200 K |
|
| Chapter 6 (e) |
Design of Stellar Interferometers (cont.) |
48 K |
|
| Chapter 7 |
Visibility Estimation and Calibration |
196 K |
|
| Chapter 8 |
Phase and Group Delay Estimation |
948 K |
|
| Chapter 9 |
Phase Referencing |
380 K |
|
| Chapter 10 (a) |
Wide-Angle Astronomy |
1,800 K |
|
| Chapter 10 (b) |
Wide-Angle Astronomy (cont.) |
248 K |
|
| Chapter 11 |
Ground-Based Narrow Angle Astronomy |
160 K |
|
| Chapter 12 |
Interferometry with Two Telescopes |
240 K |
|
| Chapter 13 (a) |
An Introduction to Closure Phase |
256 K |
|
| Chapter 13 (b) |
An Introduction to Closure Phase |
392 K |
|
| Chapter 14 |
Interferometer Design for Synthesis Imaging |
392 K |
|
| Chapter 15 |
Data Reduction for Synthesis Imaging |
468 K |
|
| Chapter 16 (a) |
Nulling Interferometry and Planet Detection |
520 K |
|
| Chapter 16 (b) |
Nulling Interferometry and Planet Detection (cont.) |
2,000 K |
|
| Chapter 16 (c) |
Nulling Interferometry and Planet Detection (cont.) |
99 K |
|
| Chapter 17 |
Binary Stars |
220 K |
|
| Chapter 18 |
Future Ground-Based Interferometry |
208 K |
|
| Appendices |
Notes on the History of Stellar Interferometry
Suggested Reading |
208 K |
|
| Page 317 |
this page is in Postscript format |
74 K |
|
