P-A Colloquium: Early Results from the Dragonfly Telephoto Array
Speaker: Roberto Abraham, University of Toronto
Title: Early Results from the Dragonfly Telephoto Array
Refreshments at 3:30 pm in 1400 BPS.
Date: Thu, 29 Mar 2018, 4:10 pm – 5:10 pm
Location: 1415 BPS Bldg.
In this talk I will describe some early results from the Toronto/Yale/Harvard Dragonfly Telephoto Array (a.k.a. Dragonfly), a robotic imaging system optimized for the detection of extended ultra low surface brightness structures. Dragonfly is comprised of multiple (expensive!) commercial 400 mm f/2.8 telephoto lenses which have high-performance sub-wavelength nanostructure optical coatings designed to minimize scattered light and ghosting. This instrument is optimized to explore the night sky in a totally different parameter space from the Hubble or Keck telescopes, and in its chosen niche no conventional telescope can touch it: Dragonfly's wide-field low surface brightness imaging performance makes it capable of directly imaging low surface brightness structures (such as galactic streams, galaxy stellar halos and faint dwarf galaxies) about 10x fainter than is possible with conventional telescopes. In this talk I'll show some early results, mainly focusing on the properties of ultra-faint stellar halos, enormous stellar disks, and a new class of ghostlike galaxies that are as big as the Milky Way but have about 1/100 of its stellar mass. I will also report on our plans to upgrade the array order to enable a search for the Cosmic Web, a large-scale network of dark matter filaments that is believed to connect galaxies to each other, and which is thought to be the largest coherent structure in the Universe.