Dapsone hypersensitivity syndrome in an adolescent during treatment during of leprosy Síndrome de hipersensibilidade à dapsona em uma adolescente durante tratamento de hanseníase

A 12 y old girl was admitted 24 days after start a WHO multidrug therapy scheme for multibacillary leprosy (dapsone, clofazimine and rifampicin) with intense jaundice, generalized lymphadenopathy, hepatoesplenomegaly, oral erosions, conjunctivitis, morbiliform rash and edema of face, ankles and hands. The main laboratory data on admission included: hemoglobin, 8.4 g/dL; WBC, 15,710 cells/mm³; platelet count, 100,000 cells/mm³; INR = 1.49; increased serum levels of aspartate and alanine aminotransferases, gamma-glutamyl transpeptidase, alkaline phosphatase, direct and indirect bilirubin. Following, the clinical conditions had deteriorated, developing exfoliative dermatitis, shock, generalized edema, acute renal and hepatic failure, pancytopenia, intestinal bleeding, pneumonia, urinary tract infection and bacteremia, needing adrenergic drugs, replacement of fluids and blood product components, and antibiotics. Ten days after admission she started to improve, and was discharged to home at day 39th, after start new supervised treatment for leprosy with clofazimine and rifampicin, without adverse effects. This presentation fulfils the criteria for the diagnosis of dapsone hypersensitivity syndrome (fever, generalized lymphadenopathy, exfoliative rash, anemia and liver involvement with mixed hepatocellular and cholestatic features). Physicians, mainly in geographical areas with high prevalence rates of leprosy, should be aware to this severe, and probably not so rare, hypersensitivity reaction to dapsone.<br>Menina, 12 anos, foi admitida referindo o uso de esquema de poliquimioterapia preconizado pela OMS para tratamento de hanseníase forma multicibacilar (dapsona, rifampicina e clofazimina) há 24 dias, apresentando icterícia, linfadenomegalia generalizada, hepatoesplenomegalia, conjuntivite, úlceras orais, exantema morbiliforme e edema de face, mãos e tornozelo. Os principais achados laboratoriais à admissão incluíam: hemoglobina, 8,4 g/dl; leucograma, 15.710 céls/mm³; contagem de plaquetas, 100.000 céls/mm³; RNI = 1,49; aumento dos níveis séricos da alanino e aspartato aminotransferases, gama-glutamil transpeptidase, fosfatase alcalina e bilirrubinas. Em seqüência, ocorreu piora do quadro, desenvolvendo dermatite esfoliativa, choque, edema generalizado, insuficiências renal e hepática, pancitopenia, sangramento intestinal, pneumonia, infecção urinária e bacteremia, necessitando de drogas adrenérgicas, antibióticos, infusão de líquidos e hemoderivados. Iniciou melhora no 10º dia de internação, recebendo alta hospitalar no 39º dia, tendo iniciado novo tratamento supervisionado para hanseníase com rifampicina e clofazimina, sem efeitos adversos. O caso relatado preenche os critérios para o diagnóstico de síndrome de hipersensibilidade à dapsona (febre, dermatite esfoliativa, linfadenopatia, anemia e acometimento hepático com necrose hepatocítica e colestase). Os médicos, principalmente em regiões com alta prevalência de hanseníase, devem estar atentos para esta grave, e provavelmente não tão rara, reação de hipersensibilidade à dapsona

Multi-messenger Observations of a Binary Neutron Star Merger

International audienceOn 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of $\sim 1.7\,{\rm{s}}$ with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg(2) at a luminosity distance of ${40}_{-8}^{+8}$ Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 $\,{M}_{\odot }$. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at $\sim 40\,{\rm{Mpc}}$) less than 11 hours after the merger by the One-Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ∼10 days. Following early non-detections, X-ray and radio emission were discovered at the transient’s position $\sim 9$ and $\sim 16$ days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC 4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta