Características clínicas da fase aguda da infecção experimental de felinos pelo vírus da imunodeficiência felina

A infecção dos felinos pelo Vírus da Imunodeficiência Felina (FIV) resulta no desenvolvimento da síndrome de imunodeficiência dos felinos. Gengivite, perda de peso, linfadenomegalia generalizada, anemia, insuficiência renal crônica, complicações neurológicas, diarréia crônica e infecções bacterianas são encontradas frequentemente. A fase aguda da infecção pode ser assintomática, retardando o estabelecimento do diagnóstico e a implantação de medidas profiláticas para restringir o contágio e a transmissão do agente aos felinos suscetíveis. Com a finalidade de estudar as características clínicas da fase aguda da infecção, dez felinos jovens, sem definição racial, com oito meses de idade foram inoculados por via endovenosa com 1mL de sangue venoso de um gato portador do FIV subtipo B. A confirmação da infecção foi obtida através de teste sorológico em quatro e oito semanas pós-inoculação (p.i.) e por nested-PCR. Foram realizados hemogramas semanais, exame ultrassonográfico do abdômen quinzenais e exame oftalmológico mensal, durante doze semanas p.i. Discreta tendência a linfopenia na segunda semana p.i. e a neutropenia entre a quinta e sétima semana p.i., febre intermitente em alguns gatos, linfadenomegalia e hepato-esplenomegalia entre a quarta e a 12ª semana p.i. foram as alterações clínicas observadas. Apenas um gato apresentou uveíte unilateral direita. A fase aguda da infecção transcorreu com alterações clínicas inespecíficas. A linfadenomegalia e a hepato-esplenomegalia observadas no decorrer da infecção, refletindo hiperplasia linfóide, sugerem a necessidade de se realizar o teste sorológico para o FIV, em todos os gatos que se apresentarem com essas alterações, o que permitirá o diagnóstico precoce da infecção e a adoção de medidas profiláticas no sentido de minimizar a propagação da infecção

The James Webb Space Telescope Mission

Twenty-six years ago a small committee report, building on earlier studies, expounded a compelling and poetic vision for the future of astronomy, calling for an infrared-optimized space telescope with an aperture of at least 4 m. With the support of their governments in the US, Europe, and Canada, 20,000 people realized that vision as the 6.5 m James Webb Space Telescope. A generation of astronomers will celebrate their accomplishments for the life of the mission, potentially as long as 20 yr, and beyond. This report and the scientific discoveries that follow are extended thank-you notes to the 20,000 team members. The telescope is working perfectly, with much better image quality than expected. In this and accompanying papers, we give a brief history, describe the observatory, outline its objectives and current observing program, and discuss the inventions and people who made it possible. We cite detailed reports on the design and the measured performance on orbit. © 2023. The Author(s). Published by IOP Publishing Ltd on behalf of the Astronomical Society of the Pacific (ASP). All rights reserved.Open access articleThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at [email protected]

GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo during the Second Part of the Third Observing Run

The third Gravitational-Wave Transient Catalog (GWTC-3) describes signals detected with Advanced LIGO and Advanced Virgo up to the end of their third observing run. Updating the previous GWTC-2.1, we present candidate gravitational waves from compact binary coalescences during the second half of the third observing run (O3b) between 1 November 2019, 15∶00 Coordinated Universal Time (UTC) and 27 March 2020, 17∶00 UTC. There are 35 compact binary coalescence candidates identified by at least one of our search algorithms with a probability of astrophysical origin pastro>0.5. Of these, 18 were previously reported as low-latency public alerts, and 17 are reported here for the first time. Based upon estimates for the component masses, our O3b candidates with pastro>0.5 are consistent with gravitational-wave signals from binary black holes or neutron-star-black-hole binaries, and we identify none from binary neutron stars. However, from the gravitational-wave data alone, we are not able to measure matter effects that distinguish whether the binary components are neutron stars or black holes. The range of inferred component masses is similar to that found with previous catalogs, but the O3b candidates include the first confident observations of neutron-star-black-hole binaries. Including the 35 candidates from O3b in addition to those from GWTC-2.1, GWTC-3 contains 90 candidates found by our analysis with pastro>0.5 across the first three observing runs. These observations of compact binary coalescences present an unprecedented view of the properties of black holes and neutron stars. © 2023 authors. Published by the American Physical Society. Published by the American Physical Society under the terms of the "https://creativecommons.org/licenses/by/4.0/"Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI.Open access articleThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at [email protected]