D. Soderblom, J. Eisenhamer, S. Hulbert, C. Leitherer,
M. McGrath, L. Sherbert, and J. Skapik
May 07, 1996
Abstract
This is a report on an unusual phenomenon seen in a long series of ACCUM
observations of a star and of the wavelength calibration lamp. The phenomenon
is described, our initial hypotheses are explained and rejected, and further
investigations are presented. Our current best hypothesis is that the changes
seen in the lamp and star are independent of one another and are due to known
effects.
- Short-Term Variations in GHRS Response: An Investigation into an Apparent Anomaly
- Abstract
