Figure 22 from Probing for Exoplanets Hiding in Dusty Debris Disks: Disk Imaging, Characterization, and Exploration with HST/STIS Multi-roll Coronagraphy

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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 Journal 148 59.

Provider: AAS Journals

Caption: Figure 22.

Panels (A) and (B) from Buenzli et al. (2010). Panel (C): log₁₀ display from [−3] to [+2.13] dex counts s⁻¹ pixel⁻¹, FOV 400 × 250 STIS pixels (20 farcs 28 × 10 farcs 14). Panel (D): gradient-edge enhancement by high-pass spatial filtering (at the expense of flux conservation) emphasizes the inflection of the high(er) SB ridge where the edge of the skirt joins the ring ansae. Log₁₀ display from [−3.5] to [0] dex counts s⁻¹ pixel⁻¹. Panels (C) and (D): red circle r = 0 farcs 3 (6 STIS pixels = physical IWA angle limit of occulting WedgeA-0.6).

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