Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF PPT Format

Erratum: “Deepest Limits on Scattered Light Emission from the Epsilon Eridani Inner Debris Disk with HST/STIS” (2024, AJ, 168, 169)

  • Authors: Sai Krishanth P. M., Ewan S. Douglas, Ramya M. Anche, Justin Hom, Kerri L. Cahoy, John H. Debes, Hannah Jang-Condell, Isabel Rebollido, Bin B. Ren, 彬 任, Christopher C. Stark, Robert Thompson, Yinzi Xin

Sai Krishanth P. M. et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 5.

Contrast vs. separation sensitivity curves showing the KLIP reduction optimized for disks (in dotted–dashed blue), KLIP reduction optimized for planets (in dotted magenta), nonnegative matrix factorization (NMF) reduction (in solid purple), and the photon limit (in thick solid gray). We note that the KLIP subtraction optimized for planets has the best contrast under 1″, but the NMF curve has the best contrast overall.

Other Images in This Article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse