Space Telescope Science Institute, April 27-29 1994
All links go to PostScript format files.
Posters
- An Automated classification system for faint galaxies.
- Roberto Abraham - Automated morphological classification of galaxies with the APS.
- Greg Aldering - Faint galaxies in WFPC2 Medium-Deep Survey images: how faint can morphological classification go?
- Stephano Casertano - IR morphology of z > 1 3C radio galaxies.
- Peter Eisenhardt - The contribution of low surface-brightness galaxies to faint galaxy counts.
- Henry Ferguson - Compact galaxies in the direction of the Virgo Cluster.
- Eduardo Hardy - Tidal triggering of star formation of the Butcher-Oemler effect.
- Mark Henriksen - Test of galaxy evolutionary models via angular sizes of galaxies.
- Myungshin Im - Morphological fits and redshift constraints for faint galaxies using WF/PC data.
- William Keel - The morphology of a damped Ly-Alpha absorber at z = 2.81
- Palle Möller &S. J. Warren - Automated morphological classification of galaxies with the APS.
- Stephen Odewahn - What determines the morphological fractions in clusters?
- Brad Whitmore - The Theta - z relation for galactic bulges and disks out to z = 0.6
- Rogier Windhorst - Quantitative measurements of galaxy sizes of radio-ellipticals.
- Esther Zirbel