Probing for Exoplanets Hiding in Dusty Debris Disks: Disk Imaging, Characterization, and Exploration with HST/STIS Multi-roll Coronagraphy
Authors: Glenn Schneider, Carol A. Grady, Dean C. Hines, Christopher C. Stark, John H. Debes, Joe Carson, Marc J. Kuchner, Marshall D. Perrin, Alycia J. Weinberger, John P. Wisniewski, Murray D. Silverstone, Hannah Jang-Condell, Thomas Henning, Bruce E. Woodgate, Eugene Serabyn, Amaya Moro-Martin, Motohide Tamura, Phillip M. Hinz, and Timothy J. Rodigas
Schneider et al.
2014 The Astronomical Journal14859.
Provider: AAS Journals
Caption: Figure 20.
(A) ACS discovery image (Kalas et al. 2006, cf. Figure 1) with IWAeffectiver = 30 digital mask. (B) STIS five-roll combined PSFTSC image. Same image scale as panel (A). Improves IWAeffective by ×10 to IWAminimum = 03 (5.4 AU projected; small yellow circle). 400 × 400 STIS pixels, log10 display [−2.2] to [+1.5] {dex} counts s−1 pixel−1. (C) "Inner" disk undetectable with ACS observed with STIS, at two times the spatial scale with respect to panel (B) (same data); 200 × 20 pixels (1154 × 1154), log10 display [−1.5] to [+1.5] {dex} counts s−1 pixel−1. All images north up, east left.