Figure 3 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 3.

WedgeA-0.6 visit-level PSF subtractions—HD 181327. Top ((A)–(C)): visits 11, 12, and 14. Bottom ((D)–(F)): visits 15, 16, and 18. Top and bottom images use contemporaneously interleaved Visit 13 and 17 HD 180134 PSF templates, respectively (see Table 3 for details). 6 farcs 2 × 6 farcs 0 sub-array regions shown with a linear display from −1.0 (black) to +7.0 (white) counts s⁻¹ pixel⁻¹. The central red circle overlaid is r = 0 farcs 3 centered on the occulted position of the star.

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