| |
Perlman, E. S. |
| Volume |
Paper Title |
Page Number |
Authors |
| 227 |
The Emission Line Properties of DXRBS Blazars |
73 |
Landt, H.; Padovani, P.; Perlman, E. S.; Giommi, P. |
| 227 |
Surveys and the Blazar Parameter Space |
200 |
Perlman, E. S.; Padovani, P.; Landt, H.; Stocke, J. T.; Costamante, L.; Rector, T.; Giommi, P.; Schachter, J. F. |
| 255 |
Revealing the Energetics and Structure of AGN Jets |
233 |
Perlman, E. S.; Marshall, H. L.; Biretta, J. A. |
| 290 |
Results from a Complete Chandra Survey of Radio Jets |
359 |
Schwartz, D. A.; Marshall, H. L.; Miller, B. P.; Worrall, D. M.; Birkinshaw, M.; Lovell, J. E. J.; Jauncey, D. L.; Perlman, E. S.; Murphy, D. W.; Preston, R. A. |
| 424 |
How Much Light Has Been Produced since the Universe Was Born? Finally, a Way to Measure It. |
344 |
Georganopoulos, M.; Sambruna, R. M.; Kazanas, D.; Davis, D. S.; Cillis, A. N.; Cheung, C. C.; Perlman, E. S.; Blundell, K. M. |
| 427 |
A New Way to Measure How Much Light Has Been Produced Since the Universe was Born |
177 |
Georganopoulos, M.; Sambruna, R. M.; Kazanas, D.; Davis, D. S.; Cillis, A. N.; Cheung, C. C.; Perlman, E. S.; Blundell, K. M. |
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