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|Statement||edited by F. Macchetto, F. Pacini and M. Tarenghi.|
|Contributions||Macchetto, F., Pacini, F., Tarenghi, M., European Space Agency., European Southern Observatory.|
|LC Classifications||QB88 .E73 1979|
|The Physical Object|
|Pagination||xx, 407 :|
|Number of Pages||407|
|LC Control Number||82181255|
Download ESA/ESO Workshop on Astronomical Uses of the Space Telescope, Geneva, 12-14 February 1979
ESA/ESO Workshop on Astronomical Uses of the Space Telescope ( Geneva, Switzerland). ESA/ESO Workshop on Astronomical Uses of the Space Telescope, Geneva, February [Geneva?]: ESA/ESO,  (OCoLC) Material Type: Conference publication, Government publication, International government publication: Document Type: Book.
Macchetto, F., Pacini, F., Tarenghi, M., (eds.), Proceedings of the ESA/ESO Workshop on Astronomical Uses of the Space Telescope, Geneva, February Author: F. Macchetto. ESA/ESO Workshop on Astronomical Uses of the Space Telescope, Geneva ( February ) Proceedings edited by F Macchetto, F Pacini and M Tarenghi.
Google Scholar by: 1. Full text of "The Restoration of HST images and spectra: proceedings of a workshop held at the Space Telescope Science Institute, Baltimore, Maryland, August " See other formats.
The Organisation. de Zeeuw T., Pottasch S., Wilson R., Adriaan Blaauw, – importance of this can be seen in the fact that the journal at the time was more turbulent than it is at present. The telescope was installed in April in the T70 Swiss telescope building belonging to Geneva University (Figure 1).
This facility had not been used since the s and was completely. PDF | On Aug 1,Judith Kalman and others published A study of community as a space for reading and writing | Find, read and cite all the research you need on ResearchGateAuthor: Judy Kalman.
Figure 3: Left: The 1E ‘arc and core,’ a of the core (black dots) on scales of pc derived highly magnified z = star-forming Lyman-break from the SINFONI observations of the [O iii]l galaxy behind the galaxy cluster 1E, as seen emission line is compared to the rotation curve of the in the optical with the ACS camera.
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