Chelen Johnson
The HIPS AGaiN (Hidden in Plain Sight AGaiN) team will be using archival surveys for stellar variability to detect variability in active galactic nuclei (AGN) in the background.
The "new" astronomy has become something we all knew was coming: handling huge chunks of data and learning how to mine this information from sets so large that it is simply mind boggling. The interesting thing is that many people are not aware of this, notably teachers in the trenches.
Having the opportunity to get new ideas from my peers and discuss projects, activities and strategies helps me to grow and keeps me from becoming stagnant in my teaching. Programs like this are like gold to me because the financial situation in the district in which I teach is such that there is no money available to send our faculty to national conferences.
Finally much of the [AAS 2009] invited talk by Eugene Churazov on Galaxy Clusters and Black Holes I found to be understandable because he used many equations from ideal gas laws that are familiar to high school teachers and their students. In talking with Dr. Churazov after his talk, he re-emphasized how far one could go on this topic with these familiar and seemingly simple equations.
