Quantifying Galaxy Morphology at High Redshift
Space Telescope Science Institute, April 27-29 1994

Posters

1. An Automated classification system for faint galaxies.
   Roberto Abraham
2. Automated morphological classification of galaxies with the APS.
   Greg Aldering
3. Faint galaxies in WFPC2 Medium-Deep Survey images: how faint can morphological classification go?
   Stephano Casertano
4. IR morphology of 3C radio galaxies.
   Peter Eisenhardt
5. The contribution of low surface-brightness galaxies to faint galaxy counts.
   Henry Ferguson
6. Compact galaxies in the direction of the Virgo Cluster.
   Eduardo Hardy
7. Tidal triggering of star formation of the Butcher-Oemler effect.
   Mark Henriksen
8. Test of galaxy evolutionary models via angular sizes of galaxies.
   Myungshin Im
9. Morphological fits and redshift constraints for faint galaxies using WF/PC data.
   William Keel
10. The morphology of a damped Ly absorber at
    Palle Möller &S. J. Warren
11. Automated morphological classification of galaxies with the APS.
    Stephen Odewahn
12. What determines the morphological fractions in clusters?
    Brad Whitmore
13. The - relation for galactic bulges and disks out to
    Rogier Windhorst
14. Quantitative measurements of galaxy sizes of radio-ellipticals.
    Esther Zirbel