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Detection of Continuum Submillimeter Emission Associated with Candidate Protoplanets

  • Authors: Andrea Isella, Myriam Benisty, Richard Teague, Jaehan Bae, Miriam Keppler, Stefano Facchini, and Laura Pérez

2019 The Astrophysical Journal Letters 879 L25.

  • Provider: AAS Journals

Caption: Figure 6.

Left panel: image of the 855 μm continuum emission recorded toward PDS 70 and imaged with a robust parameter equal to 0.3, as in the central panel of Figure 1. Middle panel: image of the symmetric component of the continuum emission calculated as discussed in Appendix B. Right panel: image of the residuals obtained by subtracting the symmetric component of the emission (middle panel) from the observations (left panel). Dashed and solid contours correspond to ±3×  the rms noise level (rms = 19 μJy beam−1).

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