SORL1 Is Genetically Associated with Late-Onset Alzheimer’s Disease in Japanese, Koreans and Caucasians

To discover susceptibility genes of late-onset Alzheimer’s disease (LOAD), we conducted a 3-stage genome-wide association study (GWAS) using three populations: Japanese from the Japanese Genetic Consortium for Alzheimer Disease (JGSCAD), Koreans, and Caucasians from the Alzheimer Disease Genetic Consortium (ADGC). In Stage 1, we evaluated data for 5,877,918 genotyped and imputed SNPs in Japanese cases (n = 1,008) and controls (n = 1,016). Genome-wide significance was observed with 12 SNPs in the APOE region. Seven SNPs from other distinct regions with p-values ,261025 were genotyped in a second Japanese sample (885 cases, 985 controls), and evidence of association was confirmed for one SORL1 SNP (rs3781834, P=7.3361027 in the combined sample). Subsequent analysis combining results for several SORL1 SNPs in the Japanese, Korean (339 cases, 1,129 controls) and Caucasians (11,840 AD cases, 10,931 controls) revealed genome wide significance with rs11218343 (P=1.7761029) and rs3781834 (P=1.0461028). SNPs in previously established AD loci in Caucasians showed strong evidence of association in Japanese including rs3851179 near PICALM (P=1.7161025) and rs744373 near BIN1 (P = 1.3961024). The associated allele for each of these SNPs was the same as in Caucasians. These data demonstrate for the first time genome-wide significance of LOAD with SORL1 and confirm the role of other known loci for LOAD in Japanese. Our study highlights the importance of examining associations in multiple ethnic populations

Current status of space gravitational wave antenna DECIGO and B-DECIGO

Deci-hertz Interferometer Gravitational Wave Observatory (DECIGO) is the future Japanese space mission with a frequency band of 0.1 Hz to 10 Hz. DECIGO aims at the detection of primordial gravitational waves, which could be produced during the inflationary period right after the birth of the universe. There are many other scientific objectives of DECIGO, including the direct measurement of the acceleration of the expansion of the universe, and reliable and accurate predictions of the timing and locations of neutron star/black hole binary coalescences. DECIGO consists of four clusters of observatories placed in the heliocentric orbit. Each cluster consists of three spacecraft, which form three Fabry-Perot Michelson interferometers with an arm length of 1,000 km. Three clusters of DECIGO will be placed far from each other, and the fourth cluster will be placed in the same position as one of the three clusters to obtain the correlation signals for the detection of the primordial gravitational waves. We plan to launch B-DECIGO, which is a scientific pathfinder of DECIGO, before DECIGO in the 2030s to demonstrate the technologies required for DECIGO, as well as to obtain fruitful scientific results to further expand the multi-messenger astronomy.Comment: 10 pages, 3 figure

Current status of space gravitational wave antenna DECIGO and B-DECIGO

The Deci-hertz Interferometer Gravitational Wave Observatory (DECIGO) is a future Japanese space mission with a frequency band of 0.1 Hz to 10 Hz. DECIGO aims at the detection of primordial gravitational waves, which could have been produced during the inflationary period right after the birth of the Universe. There are many other scientific objectives of DECIGO, including the direct measurement of the acceleration of the expansion of the Universe, and reliable and accurate predictions of the timing and locations of neutron star/black hole binary coalescences. DECIGO consists of four clusters of observatories placed in heliocentric orbit. Each cluster consists of three spacecraft, which form three Fabry–Pérot Michelson interferometers with an arm length of 1000 km. Three DECIGO clusters will be placed far from each other, and the fourth will be placed in the same position as one of the other three to obtain correlation signals for the detection of primordial gravitational waves. We plan to launch B-DECIGO, which is a scientific pathfinder for DECIGO, before DECIGO in the 2030s to demonstrate the technologies required for DECIGO, as well as to obtain fruitful scientific results to further expand multi-messenger astronomy

Design of direct-drive mechanical arms

Robotics Institut

Control of a direct-drive arm

12 direct-drivc arm is a new mechanical ami in which the shafts of articulatcd joints arc directly co~iplcd to thc rotors of high pcrformance torque motors. Since the arm does not contain any gcars or transmission mechanisms between thc motors and their loads. the drive systems have no backlash, small friction and high mcchanical stiffncss, all of which are desirable for fast, accurate and vcrsatilc robots. At the Robotics Institute of Carncgic-Mellon University,we have built a first prototype direct-drive arm (referred to as CMU DDArm hcrcaftcr). This paper presents the characteristic analysis and the dcsign of the control system. First, we describe an outline of the developed CMU DDArm and compare its characteristics with convcntional indirect-drivc arms. Sccond, we discuss basic feedback control for singlc-link drive systcms in the frequency domain. Third, we apply a feedforward compcnsation to the control of multi-dcgrce-of-frcedom motion in ordcr to compensate for interactions among multiple links, and Coriolis, ccntrifugal and gravitational forces. Finally, the stcady-state characteristics are discussed with rcspect to servo stiffncss and positioning accuracy. The cxpcrimcnts show the exccllcnt pcrformance of the dircct-drive arm in terms of spccd and accuracy. Throughout the papcr comparison with indirect-drive methods is made to contrast thc advantage of the di rec t-d ri vc method. 1

Emotional Experiences of Skin Markings Among Patients Undergoing Radiotherapy and Related Factors: A Questionnaire-Based Cross-Sectional Study

Purpose: Patients undergoing radiotherapy often have their skin marked. Previous studies on skin markings examined the durability and physical effects of the markings, but no study has focused on patients' emotional experiences toward the markings. This study aimed to clarify how patients undergoing radiotherapy feel about skin markings, as well as factors that affect patients' emotional experiences. Patients and Methods: We conducted a cross-sectional study using a self-administered questionnaire and medical records. Participants were patients aged ≥20 years undergoing cancer radiotherapy at a designated cancer care hospital. The primary outcome was the level of uncomfortable emotions toward skin markings, and the secondary outcome was the level of favorable ratings on skin markings. To examine factors related to uncomfortable emotions, ordinal logistic regression analysis was performed. Results: Questionnaire forms were distributed to 153 patients, and responses were collected from 132 (86%). Among 108 patients included in the analysis, 56% (59/105, excluding 3 who did not answer this question) responded that they were uncomfortable with skin markings. The proportion of patients who favorably rated skin markings was 63% (59/93, excluding 15 who did not answer this question). No factors were significantly associated with the primary outcome. Conclusion: Many patients accepted skin markings with resignation, as they understood the necessity of the markings in their treatment. Medical staff should understand the emotional experiences of patients toward skin markings and take sufficient care to ensure that they are provided with explanations, including the impact of skin markings on their daily lives, as well as a sense of security that treatment is being performed in a precise manner