Abstract
The FORS instruments for the VLT telescopes have been built by a joint consortium of the state observatory Heidelberg (P.I. I. Appenzeller) and the University observatories of Munich and Gottingen. A significant fraction of the joint consortiums guaranteed observing time was used for the FORS Deep Field (FDF) project. The main scientific objective of the FDF is to explore the physical properties of (proto)galaxies and their evolution as a function of cosmic age.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
