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We present estimates of line-of-sight distortion fields derived from the 95 and 150 GHz data taken by BICEP2, BICEP3, and the Keck Array up to the 2018 observing season, leading to cosmological constraints and a study of instrumental and astrophysical systematics. Cosmological constraints are derived from three of the distortion fields concerning gravitational lensing from large-scale structure, polarization rotation from magnetic fields or an axion-like field, and the screening effect of patchy reionization. We measure an amplitude of the lensing power spectrum ${A}_{L}^{\phi \phi }=0.95\pm 0.20$ . We constrain polarization rotation, expressed as the coupling constant of a Chern–Simons electromagnetic term g _a _γ ≤ 2.6 × 10 ^−2 / H _I , where H _I is the inflationary Hubble parameter, and an amplitude of primordial magnetic fields smoothed over 1 Mpc B _1Mpc ≤ 6.6 nG at 95 GHz. We constrain the rms of optical depth fluctuations in a simple “crinkly surface” model of patchy reionization, finding A ^τ < 0.19 (2 σ ) for the coherence scale of L _c = 100. We show that all of the distortion fields of the 95 and 150 GHz polarization maps are consistent with simulations including lensed ΛCDM, dust, and noise, with no evidence for instrumental systematics. In some cases, the EB and TB quadratic estimators presented here are more sensitive than our previous map-based null tests at identifying and rejecting spurious B -modes that might arise from instrumental effects. Finally, we verify that the standard deprojection filtering in the BICEP/Keck data processing is effective at removing temperature to polarization leakage.

We characterize Galactic dust filaments by correlating BICEP/Keck and Planck data with polarization templates based on neutral hydrogen (H i ) observations. Dust polarization is important for both our understanding of astrophysical processes in the interstellar medium (ISM) and the search for primordial gravitational waves in the cosmic microwave background (CMB). In the diffuse ISM, H i is strongly correlated with the dust and partly organized into filaments that are aligned with the local magnetic field. We analyze the deep BICEP/Keck data at 95, 150, and 220 GHz, over the low-column-density region of sky where BICEP/Keck has set the best limits on primordial gravitational waves. We separate the H i emission into distinct velocity components and detect dust polarization correlated with the local Galactic H i but not with the H i associated with Magellanic Stream i . We present a robust, multifrequency detection of polarized dust emission correlated with the filamentary H i morphology template down to 95 GHz. For assessing its utility for foreground cleaning, we report that the H i morphology template correlates in B modes at a ∼10%–65% level over the multipole range 20 < ℓ < 200 with the BICEP/Keck maps, which contain contributions from dust, CMB, and noise components. We measure the spectral index of the filamentary dust component spectral energy distribution to be β = 1.54 ± 0.13. We find no evidence for decorrelation in this region between the filaments and the rest of the dust field or from the inclusion of dust associated with the intermediate velocity H i . Finally, we explore the morphological parameter space in the H i -based filamentary model.

Praziquantel (PZQ) is currently the only approved drug for treating clonorchiasis, but its poor efficacy against Clonorchis sinensis larvae has highlighted the need to develop newer drugs. In this study, to address this challenge, we investigated the anti-parasitic efficacy of miltefosine (MLT), curcumin (CUR), and PZQ against C. sinensis metacercariae (CsMC), newly excysted juvenile worms (CsNEJs), and adults. Larvicidal effects of MLT and CUR surpassed those elicited by PZQ in vitro . These two drugs exerted their effect against both CsMC and CsNEJs in a dose- and time-dependent manner. To confirm the effect of these drugs in vivo , Syrian golden hamsters were orally infected with 100 CsMC and subsequently treated with MLT, CUR, or PZQ at 1 and 4 weeks post-infection (wpi). MLT and CUR reduced the worm recoveries at 1 and 4 wpi, indicating that these drugs were efficacious against both larvae and adult C. sinensis . PZQ was only efficacious against adult worms. Interestingly, both MLT and CUR showed lower levels of C. sinensis- specific IgG responses than the infection control group, implying that worm burden and bile IgG responses could be correlated. These results indicate that MLT and CUR are efficacious against both larval and adult stages of C. sinensis , thereby highlighting their potential for further development as alternative therapeutic options for clonorchiasis., Competing Interests: The authors declare no conflict of interest.