Challenges in Scientific Data Communication from Low-mass Interstellar Probes
Authors: David G. Messerschmitt, Philip Lubin, and Ian Morrison
2020 The Astrophysical Journal Supplement Series24936.
Provider: AAS Journals
Caption: Figure 18.
Figure 17 is repeated for λ = 1 μm. A floor in transmit power appears because interference becomes the dominant contributor to SBR for small dark count rate ﹩{{\rm{\Lambda }}}_{D}^{S}﹩ (see Figures 12 and 14).