Tg動物飼育システムSTAR及びSTAR/OKの紹介

Transgenic animal research is progressing in recent years. Severer cross-contamination prevention management is required for breeding transgenic animals in clean environment, like SPF animals. Moreover, contaminants and odors problems have posed the more serious influence to caretakers or researchers. In order that we might improve these problems, we got cooperation of Kumamoto University and developed the rack (STAR: System of Tonets Animal Rack)for transgenic animal research that have both the supply air-inlet and the exhaust air-outlet. If this system is used, the good experiment is possible that does not have a cross-contamination between cages and does not have diffusion contaminants and odors to an animal room. In this paper, we introduce also about the Okayama University specification (STAR/OK) as the application

The Effect of Surgical Repair for Pectum Excavatum on Cardiopulmonary Function

In five patients with corrective surgery for pectus Excavatum, the effectiveness of surgical repair were evaluated from the results of pulmonary function test as well as the finding on ECG according to follow-up study postoperativelly. Of five patient undergone the corrective surgery which sternoturnover with costalplasty employed in 4, and sternoplasty alone in I, all of them were male and the average age except 3 years of age was 14.8 years ranging from 10 to 21 years. There are no manifestation of clinical syndrome in all 5 cases. However, the fair mental growth demands psychologically the early corrective surgery in young chidren. By follow-up study after surgical correction for pectus excavatum during a period from 3 months to 3 years and 3 months, the finding on EKG of right ventricular overload revealed the improvement within 2 months after surgical correction in contrast the results of pulmonary function test disclosed no marked changes until 2 months following surgery. From the view of cosmetic efficacy of corrective surgery, sternoturnover with or without costalplasty are one of the adovocating operative procedures

Clinical Evaluation with Referrence to Operative Specificity on Tracheal and Bronchial Reconstruction

The clinical specificity were evaluated in those 11 cases who underwent tracheal recon - structive surgery and in those 25 cases who underwent bronchial reconstructive surgery respectively. Its prognosis after tracheal reconstruction at the level of intrathoracic region was extremely poor. The operative specificity with regard to tracheal surgery consist of being a poor genera- condition preoperativelly and of having an urgent demand of removal of tracheal stenotic lesion to alleviate respiratory distress . The prognosis after tracheal surgery was commonly poor and was similar to that after emergency operation as a general accep - tance for the reason of unfavorable general condtion . The present study was to define clinical problems in which the salvage after tracheal surgery was entirely difficult. The improvement of the prognosis following tracheal surgery should be found in maximum endeavor for prevention of postoperative complication related to operative death intimately. However, terminal tracheostomy employed for lesions of cervical trachea was one o

Real-world effectiveness and safety analysis of carfilzomib-lenalidomide-dexamethasone and carfilzomib-dexamethasone in relapsed/refractory multiple myeloma: a multicenter retrospective analysis

Background: Little is known about the real-world survival benefits and safety profiles of carfilzomib-lenalidomide-dexamethasone (KRd) and carfilzomib-dexamethasone (Kd). Methods: We performed a retrospective analysis to evaluate their efficacy and safety in 157 patients registered in the Kansai Myeloma Forum database. Results: A total of 107 patients received KRd. Before KRd, 99% of patients had received bortezomib (54% were refractory disease), and 82% had received lenalidomide (57% were refractory disease). The overall response rate (ORR) was 68.2%. The median progression-free survival (PFS) and overall survival (OS) were 8.8 and 29.3 months, respectively. Multivariate analysis showed that reduction of the carfilzomib dose and non-IgG M protein were significantly associated with lower PFS and reduction of the carfilzomib dose and refractoriness to prior bortezomib-based regimens were significantly associated with lower OS. A total of 50 patients received Kd. Before Kd, 96% of patients had received bortezomib (54% were refractory disease). The ORR was 62.0%. The median PFS and OS were 7.1 and 20.9 months, respectively. Based on the multivariate analysis, reduction of the carfilzomib dose and International Staging System Stage III (ISS III) were significantly associated with lower PFS. Grade III or higher adverse events were observed in 48% of KRd cases and 54% of Kd cases. Cardiovascular events, cytopenia, and infections were frequent, and 4 KRd patients died due to heart failure, arrhythmia, cerebral hemorrhage, and pneumonia. Conclusion: Our analysis showed that an adequate dose of carfilzomib is important for achieving the best survival benefits in a real-world setting. Adverse effects after KRd and Kd therapy should also be considered

The ASTRO-H X-ray Observatory

The joint JAXA/NASA ASTRO-H mission is the sixth in a series of highly successful X-ray missions initiated by the Institute of Space and Astronautical Science (ISAS). ASTRO-H will investigate the physics of the high-energy universe via a suite of four instruments, covering a very wide energy range, from 0.3 keV to 600 keV. These instruments include a high-resolution, high-throughput spectrometer sensitive over 0.3-2 keV with high spectral resolution of Delta E < 7 eV, enabled by a micro-calorimeter array located in the focal plane of thin-foil X-ray optics; hard X-ray imaging spectrometers covering 5-80 keV, located in the focal plane of multilayer-coated, focusing hard X-ray mirrors; a wide-field imaging spectrometer sensitive over 0.4-12 keV, with an X-ray CCD camera in the focal plane of a soft X-ray telescope; and a non-focusing Compton-camera type soft gamma-ray detector, sensitive in the 40-600 keV band. The simultaneous broad bandpass, coupled with high spectral resolution, will enable the pursuit of a wide variety of important science themes.Comment: 22 pages, 17 figures, Proceedings of the SPIE Astronomical Instrumentation "Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray

The Quiescent Intracluster Medium in the Core of the Perseus Cluster

Clusters of galaxies are the most massive gravitationally-bound objects in the Universe and are still forming. They are thus important probes of cosmological parameters and a host of astrophysical processes. Knowledge of the dynamics of the pervasive hot gas, which dominates in mass over stars in a cluster, is a crucial missing ingredient. It can enable new insights into mechanical energy injection by the central supermassive black hole and the use of hydrostatic equilibrium for the determination of cluster masses. X-rays from the core of the Perseus cluster are emitted by the 50 million K diffuse hot plasma filling its gravitational potential well. The Active Galactic Nucleus of the central galaxy NGC1275 is pumping jetted energy into the surrounding intracluster medium, creating buoyant bubbles filled with relativistic plasma. These likely induce motions in the intracluster medium and heat the inner gas preventing runaway radiative cooling; a process known as Active Galactic Nucleus Feedback. Here we report on Hitomi X-ray observations of the Perseus cluster core, which reveal a remarkably quiescent atmosphere where the gas has a line-of-sight velocity dispersion of 164+/-10 km/s in a region 30-60 kpc from the central nucleus. A gradient in the line-of-sight velocity of 150+/-70 km/s is found across the 60 kpc image of the cluster core. Turbulent pressure support in the gas is 4% or less of the thermodynamic pressure, with large scale shear at most doubling that estimate. We infer that total cluster masses determined from hydrostatic equilibrium in the central regions need little correction for turbulent pressure.Comment: 31 pages, 11 Figs, published in Nature July