Chelen Johnson
Detecting Brown Dwarfs in Interacting Cataclysmic Binaries: Using Spitzer Space Telescope infrared images to determine whether the companion of the remnant star EE Eri (a white dwarf) is in fact a very low-mass object (sometimes called 'failed star') known as a brown dwarf.
[from one of Ms. Piper's students, 4 years after NITARP:] I felt like I should tell you about my current trajectory because without you and our work with NITARP, I don't know where I'd be headed right now!
I really enjoyed meeting members of the other NITARP teams and comparing their experience to mine. Everyone’s experience was different, but there seemed to be an overwhelming consensus that NITARP was the most significant, educational, and enjoyable professional development experience they have ever had. I could not agree more.
Some of my students will be benefiting directly [from my AAS trip] as I currently have 7 students interested in being part of our research team for NITARP. My first day back from the conference I spent the class time sharing with them the exciting news regarding exoplanet research from Dr. Marcy's presentation on Monday as well as a discussion on YSOs and the likely direction that our project will take.
