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Vector-borne pathogens induce hemoparasitism in cattle causing substantial economic losses in tropical and subtropical areas. Infectious cattle actively contribute to maintaining the transmission cycle, and the presence of these animals must be associated with husbandry management and environmental changes. In the present study, we conducted a cross-sectional study sampling 1,000 bovines to identify infectious cattle diagnosed by a direct technique and employed a dichotomic questionnaire for association analyses, hierarchical clustering, and Principal Component Analysis (PCA). Overall prevalence with infectious cattle was 34.99%, where 97% of the farms had at least one infectious animal per genera, and the prevalence in properties ranged between 16.39 and 53.85%. Of these animals, 26.20% tested positive for Anaplasma sp., 8.40% for Babesia spp., and 1.30% for Trypanosome spp. The main co-infection showed 5% Anaplasma sp. – Trypanosome spp., followed by 4% Babesia spp. – Trypanosome spp. These bovines showed association with the use of the Jersey breed (OR = 2.016 C.I:1.188–3.419), selling animals for replacement (OR = 1.417 CI:1.022–1.965), participation in livestock exhibitions (OR = 2.009 CI:1.262–3.199), premises with burials (OR = 2,064 CR: 1.414–3.011), use of palm kernel (OR = 1.935 C.I:1.198–3.124), and the use of ivermectin (OR = 1.548 CI: 1.085–2.210) as a susceptibility. The hierarchical clustering revealed clusters among properties with different hemoparasite prevalence, with notable co-infections observed. The subsequent PCA identified that significant risk factors contributed to hemoparasitism positivity. We conclude that infectious cattle in the endemic area showed an association with husbandry management that permits the success of vector and maintenance of the enzootic or epizootic cycle in the herds. [ABSTRACT FROM AUTHOR]

We have used an electron beam ion trap to measure electron-density-diagnostic line-intensity ratios for extreme ultraviolet lines from Fe xii, xiii, and xiv at wavelengths of ≈185–205 and 255–276 Å. These ratios can be used as density diagnostics for astrophysical spectra and are especially relevant to solar physics. We found that density diagnostics using the Fe xiii 196.53/202.04 and the Fe xiv 264.79/274.21 and 270.52A/274.21 line ratios are reliable using the atomic data calculated with the Flexible Atomic Code (FAC). On the other hand, we found a large discrepancy between the FAC theory and experiment for the commonly used Fe xii (186.85 + 186.88)/195.12 line ratio. These FAC theory calculations give results similar to the data tabulated in CHIANTI, which are commonly used to analyze solar observations. Our results suggest that the discrepancies seen between solar coronal density measurements using the Fe xii (186.85 + 186.88)/195.12 and Fe xiii 196.54/202.04 line ratios are likely due to issues with the atomic calculations for Fe xii. [ABSTRACT FROM AUTHOR]

Uncertainties in atomic models will introduce noticeable additional systematics in calculating the flux of weak dielectronic recombination (DR) satellite lines, affecting the detection and flux measurements of other weak spectral lines. One important example is the Ar xvii Heβ DR, which is expected to be present in emission from the hot intracluster medium of galaxy clusters and could impact measurements of the flux of the 3.5 keV line that has been suggested as a secondary emission from a dark matter interaction. We perform a set of experiments using the Lawrence Livermore National Laboratory’s electron beam ion trap (EBIT-I) and the X-ray Spectrometer quantum calorimeter (XRS/EBIT) to test the Ar xvii Heβ DR origin of the 3.5 keV line. We measured the X-ray emission following resonant DR onto helium-like and lithium-like Argon using EBIT-I’s Maxwellian simulator mode at a simulated electron temperature of Te = 1.74 keV. The measured flux of the Ar xvii Heβ DR lined is too weak to account for the flux in the 3.5 keV line, assuming reasonable plasma parameters. We, therefore, rule out Ar xvii Heβ DR as a significant contributor to the 3.5 keV line. A comprehensive comparison between the atomic theory and the EBIT experiment results is also provided. [ABSTRACT FROM AUTHOR]