A retrospective comparative study of recombinant human thrombomodulin and gabexate mesilate in sepsis-induced disseminated intravascular coagulation patients

The novel biological agent recombinant human thrombomodulin (rhTM) has been used clinically in Japan to treat disseminated intravascular coagulation (DIC) since 2008. Previous studies have shown the efficacy of rhTM versus heparin therapy or non-rhTM therapy. We retrospectively evaluated and compared the efficacies of rhTM and gabexate mesilate (GM) in patients diagnosed with sepsis-induced DIC. From September 2010 to October 2012, patients with sepsis-induced DIC who were treated with rhTM (n = 13) or GM (n = 10) at Nagasaki Municipal Hospital were extracted. Patients receiving other anticoagulants in combination were excluded. Clinical information, laboratory data, Sequential Organ Failure Assessment (SOFA) scores, and DIC scores were obtained from the medical records. Mortality at days 7 and 30 after DIC diagnosis and changes in laboratory data and SOFA scores from days 1-7 were evaluated. The groups\u27 clinical characteristics did not differ, except for the relatively higher C-reactive protein (CRP) levels in the rhTM group (P = 0.0508). The survival rates of the rhTM and GM groups on days 7 and 30 were 92.3%, 69.2% and 80%, 70%, respectively, both group indicated similar mortality. However, on day 7, the platelet counts, SOFA scores, and CRP levels significantly improved in the rhTM group; the platelet counts and SOFA scores did not improve significantly in the GM group. The platelet counts of the rhTM group significantly improved compared to the GM group (P = 0.004). Recombinant human thrombomodulin might be more effective for sepsis-induced DIC than GM

DECIGO pathfinder

DECIGO pathfinder (DPF) is a milestone satellite mission for DECIGO (DECi-hertz Interferometer Gravitational wave Observatory) which is a future space gravitational wave antenna. DECIGO is expected to provide us fruitful insights into the universe, in particular about dark energy, a formation mechanism of supermassive black holes, and the inflation of the universe. Since DECIGO will be an extremely large mission which will formed by three drag-free spacecraft with 1000m separation, it is significant to gain the technical feasibility of DECIGO before its planned launch in 2024. Thus, we are planning to launch two milestone missions: DPF and pre-DECIGO. The conceptual design and current status of the first milestone mission, DPF, are reviewed in this article

The status of DECIGO

DECIGO (DECi-hertz Interferometer Gravitational wave Observatory) is the planned Japanese space gravitational wave antenna, aiming to detect gravitational waves from astrophysically and cosmologically significant sources mainly between 0.1 Hz and 10 Hz and thus to open a new window for gravitational wave astronomy and for the universe. DECIGO will consists of three drag-free spacecraft arranged in an equilateral triangle with 1000 km arm lengths whose relative displacements are measured by a differential Fabry-Perot interferometer, and four units of triangular Fabry-Perot interferometers are arranged on heliocentric orbit around the sun. DECIGO is vary ambitious mission, we plan to launch DECIGO in era of 2030s after precursor satellite mission, B-DECIGO. B-DECIGO is essentially smaller version of DECIGO: B-DECIGO consists of three spacecraft arranged in an triangle with 100 km arm lengths orbiting 2000 km above the surface of the earth. It is hoped that the launch date will be late 2020s for the present