Identifying Potential Classification Criteria for Calcium Pyrophosphate Deposition Disease: Item Generation and Item Reduction.

Classification criteria for calcium pyrophosphate deposition (CPPD) disease will facilitate clinical research on this common crystalline arthritis. Our objective was to report on the first 2 phases of a 4-phase process for developing CPPD classification criteria. CPPD classification criteria development is overseen by a 12-member steering committee. Item generation (phase I) included a scoping literature review of 5 literature databases and contributions from a 35-member combined expert committee and 2 patient research partners. Item reduction and refinement (phase II) involved a combined expert committee meeting, discussions among clinical, imaging, and laboratory advisory groups, and an item-rating exercise to assess the influence of individual items toward classification. The steering committee reviewed the modal rating score for each item (range -3 [strongly pushes away from CPPD] to +3 [strongly pushes toward CPPD]) to determine items to retain for future phases of criteria development. Item generation yielded 420 items (312 from the literature, 108 from experts/patients). The advisory groups eliminated items that they agreed were unlikely to distinguish between CPPD and other forms of arthritis, yielding 127 items for the item-rating exercise. Fifty-six items, most of which had a modal rating of +/- 2 or 3, were retained for future phases. As numerous imaging items were rated +3, the steering committee recommended focusing on imaging of the knee and wrist and 1 additional affected joint for calcification suggestive of CPP crystal deposition. A data- and expert-driven process is underway to develop CPPD classification criteria. Candidate items comprise clinical, imaging, and laboratory features

Expansion sequencing: Spatially precise in situ transcriptomics in intact biological systems.

Methods for highly multiplexed RNA imaging are limited in spatial resolution and thus in their ability to localize transcripts to nanoscale and subcellular compartments. We adapt expansion microscopy, which physically expands biological specimens, for long-read untargeted and targeted in situ RNA sequencing. We applied untargeted expansion sequencing (ExSeq) to the mouse brain, which yielded the readout of thousands of genes, including splice variants. Targeted ExSeq yielded nanoscale-resolution maps of RNAs throughout dendrites and spines in the neurons of the mouse hippocampus, revealing patterns across multiple cell types, layer-specific cell types across the mouse visual cortex, and the organization and position-dependent states of tumor and immune cells in a human metastatic breast cancer biopsy. Thus, ExSeq enables highly multiplexed mapping of RNAs from nanoscale to system scale

An\ue1lise comparativa da anatomia foliar de Melastomataceae em ambiente de vereda e cerrado sensu stricto

Este trabalho descreve a anatomia das lâminas foliares de três espécies de Melastomataceae, Lavoisiera bergii Cogn., Macairea radula (Bonpl.) DC. e Trembleya parviflora (D. Don) Cogn. que estão colonizando a zona alagável e aberta de fundo de vereda e de M. radula e T. parviflora que ocorrem no cerrado sensu stricto da Estação Ecológica de Águas Emendadas, Planaltina/DF. Os dados estruturais mostrados pelas três espécies indicam escleromorfia com características particulares a cada uma delas, como projeções nas células epidérmicas de L. bergii, diferentes tipos e localização de emergências formadas por esclereídes em L. bergii e M. radula, e evaginações na epiderme de T. parviflora. A caracterização anatômica das folhas de M. radula e T. parviflora não difere entre os ambientes. No entanto, as lâminas foliares dos indivíduos encontrados na vereda apresentaram plasticidade com valores significativamente (P< 0,05) maiores para espessura do mesofilo e do parênquima para massa foliar e massa foliar específica em relação aos indivíduos do cerrado sensu stricto. Esta relação é inversa para valores de área foliar específica. A capacidade de apresentar plasticidade estrutural, juntamente com a escleromorfia, pode ter sido relevante para o comportamento invasivo destas espécies na zona de fundo da vereda como destacado na discussão. Além deste ponto, o texto também apresenta uma breve discussão sobre outros aspectos relacionados à importância de estruturas anatômicas na taxonomia e ecologia destas espécies

Constraints on the structure and seasonal variations of Triton&apos;s atmosphere from the 5 October 2017 stellar occultation and previous observations

Context. A stellar occultation by Neptune&apos;s main satellite, Triton, was observed on 5 October 2017 from Europe, North Africa, and the USA. We derived 90 light curves from this event, 42 of which yielded a central flash detection. Aims. We aimed at constraining Triton&apos;s atmospheric structure and the seasonal variations of its atmospheric pressure since the Voyager 2 epoch (1989). We also derived the shape of the lower atmosphere from central flash analysis. Methods. We used Abel inversions and direct ray-tracing code to provide the density, pressure, and temperature profiles in the altitude range ∼8 km to ∼190 km, corresponding to pressure levels from 9 μbar down to a few nanobars. Results. (i) A pressure of 1.18 ± 0.03 μbar is found at a reference radius of 1400 km (47 km altitude). (ii) A new analysis of the Voyager 2 radio science occultation shows that this is consistent with an extrapolation of pressure down to the surface pressure obtained in 1989. (iii) A survey of occultations obtained between 1989 and 2017 suggests that an enhancement in surface pressure as reported during the 1990s might be real, but debatable, due to very few high S/N light curves and data accessible for reanalysis. The volatile transport model analysed supports a moderate increase in surface pressure, with a maximum value around 2005-2015 no higher than 23 μbar. The pressures observed in 1995-1997 and 2017 appear mutually inconsistent with the volatile transport model presented here. (iv) The central flash structure does not show evidence of an atmospheric distortion. We find an upper limit of 0.0011 for the apparent oblateness of the atmosphere near the 8 km altitude.