Whole Earth Telescope (WET)

 

WET Announcements

  • XCOV 25 , held in May 2006, was the first WET run sponsored by the Delaware Asteroseismic Research Center and Mt.Cuba Observatory. To view the results of this run, go to XCOV 25 Website. The paper is now accepted. Check out our publications list below.
  • The 2008 campaign on G29-38 is finished. Gemini obtained time-resolved spectroscopy, and ground based telescopes obtained extensive optical observations. To see the observations, go to 2008 G29-38. Contact Susan Thompson for the status of this campaign.
  • XCOV27 is starting in 2 weeks. The website has just been posted at XCOV27 page for details. We have lots of new features, including an XCOV27 Google Group. Please join the group and participate in the discussions during XCOV27:)
  • The November 2007 campaign on G38-29 is complete. We obtained over 225 hours of data. This campaign began as an investigation of G38-29 as a possible target for light curve fitting, and grew into nearly a full fledged WET run. Here in Delaware, we jokingly call it XCOV25.5. To see the observations, go to November 2007 G38-29 Website.
  • We are always looking for interesting targets. There is no formal application process. If you have an interesting target that you think needs WET, please send the info (the target name and a couple of paragraphs concerning the scientific goals) to Dr.Judi Provencal or anyone on the advisory board, or go to Target Proposal.
  • XCOV26 was held in April 2008. This data is still under analysis. To see the data, visit XCOV26

Recent WET Publications

The papers listed above can be obtained in electronic form from their respective links if your institution has the necessary journal subscriptions and copyright clearances.

See the Publications for more WET papers and for downloads.....


The Whole Earth Telescope (WET) is a collaborative effort between astronomers all over the world who are interested in studying the variability of astronomical objects. Objects that vary continuously require constant monitoring in order to unambiguously measure the intrinsic variations, which is impossible from a single site on Earth. The WET was one of the first worldwide collaborations of this type, and continues as an example of international cooperation in astronomy. This website contains information about the history, activities and publications of the WET collaboration.


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