All meetings will be at the La Serena Club Resort Hotel, which is right across the street from the beach. Invited review talks are indicated by "**". The time indicated includes 15 minutes for discussion of invited talks, and 10 minute discussion for 25 minute talks.
| Sunday, May 17, 1998 | Welcoming Reception |
| 5:30-8:00PM | Registration in Centro Turistico Los Andes lobby |
| 6:00 - - - - | cocktail party at Centro Turistico Los Andes bar area |
| Monday, May 18, 1998 | Introduction. Observed emission line correlations. Jack Baldwin, Chair | |
| 8:30-9:30 | Registration, Club Resort Hotel outside meeting room | |
| 9:00 - 9:15 | Malcolm Smith, Director, CTIO | Welcoming address |
| 9:15-10:00 | Nick Suntzeff | Cosmological constants from supernovae |
| 10:00 - 10:55 ** | Pat Osmer | Basic line and continuum correlations |
| 10:55-11:25 | coffee | |
| 11:25-12:00 | Kirpal Nandra | X-Ray dependencies on luminosity in AGN |
| 12:00-12:35 | Michael Brotherton | The Effect of Intermediate Line Region on the Baldwin Effect |
| 12:35-2:30 | lunch | |
| 2:30-3:05 | Wei Zheng | The Baldwin Effect for HeII emission; can it be a reliable calibrator? |
| 3:05-3:30 | Brian Espey | Correlations in a large QSO Sample |
| 3:30-4:05 | coffee | |
| 4:05-4:40 | Joe Shields | Emission line properties of QSOs at z > 4 |
Optional no-host excursion: a fleet of taxis will arrive at the main hotel at 6:30 to take participants to the Coquimbo fish restaurant "La Picida"
| Tuesday, May 19, 1998 | Observed spectral energy distribution correlations, Pat Osmer chair | |
| 9:00-9:55 ** | Belinda Wilkes | Spectral Energy Distributions |
| 9:55-10:30 | Bev Wills | The PG X-Ray QSO sample: links between the UV-X-ray continuum and emission lines |
| 10:30-11:00 | coffee | |
| 11:00-11:35 | Joanna Kuraszkiewicz | Clues to Quasar structure from emission line/continuum correlations |
| 11:35-12:10 | Ari Laor | UV Properties of 1 Zw 1; the Ionizing Continuum in AGN |
| 12:10-2:00 | lunch | |
| 2:00-2:55 ** | Paul Green | Emission lines and the high energy continuum |
| 2:55-3:30 | Coffee | |
| 3:30-4:05 | Sergei Nayakshin | Magnetic flares and connection between Seyferts and quasars |
Optional no-host excursion: At 6:30PM participants can walk to La Mia Pizza, a nearby restaurant said to have the best food in La Serena.
| Wednesday May 20 1998 | Impact of the central engine, Malcolm Smith, chair | |
| 9:00-9:55 ** | Keith Horne | The structure of the emission line regions |
| 9:55-10:30 | Ari Laor | The masses of AGNs |
| 10:30-10:50 | coffee | |
| 11:25-12:00 | Joe Shields | The Intrinsic Baldwin Effect |
| 10.50-11:25 | Gary Ferland | Numerical simulations of photoionized clouds |
| 12:00-7:00 | Excursion to Cerro Tololo and Cerro Pachon | |
| Thursday, May 21, 1998 | unification, global structure, Joe Wampler, chair | |
| 9:00-9:55 ** | Kirk Korista | photoionization models of emission line correlations |
| 9:55-10:30 | Shai Kaspi | New method for BLR modeling |
| 10:30-11:05 | Tetsuo Yamamoto | Disk-Wind models for BAL QSOs |
| 11:05-11:35 | coffee | |
| 11:35-12:30 ** | Fred Hamann | early universe star/galaxy formation, BLR abundances |
| 12:30-1:05 | Amri Wandel | UV- X-ray spectral dependence of the BLR |
| 1:05-2:30 | lunch | |
| 2:30-3:25 ** | Peter Barthel | unification schemes and luminosity correlations |
| 3:25-3:50 | coffee | |
| 3:50-4:25 | Chris Willott | 7C quasars and orientation effects |
| 4:25-5:00 | Stefan Collier | The Hubble constant from accretion disk reverberations |
| 5:00-8:00 | free time | |
| 8:00-?? | Gala workshop banquet at Club Resort Hotel | |
| Friday, May 22, 1998 | Bringing it all together, Gary Ferland, chair | |
| 9-9:35 | Jack Baldwin | the Next Steps . . . |
| 9:35-10:30 ** | David Tytler | implications for cosmology |
| 10:30-11:00 | coffee | |
| 11:00-12:00 ** | Joe Wampler | roundtable, meeting summary |
| Monday-Friday | Posters (to remain up for the entire meeting) |
| Kentaro Aoki | Relations between FeII emission and the 1900A feature |
| Tinggui Wang | Continuum Anisotropy from line/continuum correlations |
| Bev Wills | The PG X-Ray QSO sample: links between the UV-X-ray continuum and emission lines |