MSST - the multi-site spectroscopic telescope - represents an idea for a virtual instrument based on a network of 2m - 4m class telescopes.

An international team intends to use it to study non-radial pulsations in the subdwarf B star PG1605+072 (aka V338 Ser). This involves making observations over 2 weeks for nearly 24 hours a day in order to measure brightness, temperature, and radial velocity variations on the stellar surface.

These pages contain information that is primarily operational. With the exception of the press releases, they are not intended for public readers.

Enquiries about the project should be addressed to msst-core-team@astro.uni-tuebingen.de or directly to one of:

Prof Ulrich Heber,	Universität Erlangen-Nürnberg,	Germany
Dr Simon Jeffery,	Armagh Observatory,	United Kingdom
Dr Simon O'Toole,	University of Sydney,	Australia
Dr Stefan Dreizler,	Universität Tübingen,	Germany

Any data presented on this and subsequent pages are not public domain. You may not use any kind of information extracted from these page for your own purposes. The data are the result of a quick-look analysis and may contain errors. They are meant only to inform observers and other collaborators of how the data look and what results may come out of them.