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Delivering adequate healthcare in the setting of the ongoing pandemic is challenging. Due to 2019 coronavirus disease (COVID-19), the Tokyo Metropolitan government has been forced to expand their acute healthcare capacity corresponding to infectious diseases within a short period. Responding to this situation, health emergency and disaster experts of the Tokyo Disaster Medical Assistance Team took the initiative in creating a brief education course. We established the course for expanding infectious disease care capacity by a dedicated hands-on lecture for health professionals who are unfamiliar with infectious disease care in ordinary circumstances. Our lecture included the typical course of COVID-19, usage of personal protective equipment, environmental sterilization, medical-ward zoning, and safe caregiving. Hospitals that received customized lectures reported via a questionnaire that the lectures were well suited to their needs. Currently, the healthcare system in Tokyo has increased its capacity to meet the demand and has not been affected by COVID-19. Our experience shows that health emergency and disaster experts can assist hospitals in crisis by providing educational materials.
To analyse the Na content of bread by comparing the amount of salt and Na among the label, laboratory analysis and international guidelines.
Ten selected bakeries provided 3239 randomly selected samples of bread, which were weighed on-site. Triplicate samples were retrieved from each bakery (thirty samples) for analysis. Bread production was observed, and ingredient labels were queried to determine salt weights, which were used for comparison with the laboratory analysis. Flame photometry and the method for chlorides were utilised for analysing Na. Laboratory findings were compared to nine different international nutritional guidelines for Na consumption.
Florianopolis, south of Brazil.
Ninety independent bakeries locally producing Portuguese rolls were queried; rolls from ten conveniently selected bakeries were retrieved for further analysis.
The average weight of the rolls was 50·2 ± 5·3 g. The average amount of salt (g) per roll, by laboratory and label analyses, was 0·69 ± 0·0 and 0·62 ± 0·1 g, respectively. The mean level of Na (mg) reported on nutrient labels (478·2 ± 93·4/100 g) was significantly lower than by laboratory analysis (618·2 ± 73·8/100 g), P < 0·001. There was a difference for Na in rolls produced in the bakeries considering the unit weight of rolls (P ≤ 0·001) per 100 g (P = 0·026) and the mode of production. The consumption of two averaged units of rolls was equivalent to 51·7 % of the Brazilian guideline daily amount for Na for children and 31 % for adults.
The nutrient labels underreported Na values. This study strengthens the importance of monitoring Na of breads in Brazil.
The incidence of surgical site infection (SSI) is higher in spinal surgeries than in general orthopedic operations. In this study, we aimed to develop a scoring system with reduced health care costs for detecting spinal surgery patients at high risk for SSI.
Retrospective cohort study.
In total, 824 patients who underwent spinal surgery at 2 university hospitals from September 2005 to May 2011.
We reviewed the medical records of 824 patients, and we examined 19 risk factors to identify high-risk patients. After narrowing down the variables by univariate analysis, multiple logistic analysis was performed for factors with P values <.2, using SSI as a dependent variable. Only factors that showed P values <.05 were included in the final models, and each factor was scored based on the β coefficient values obtained. The clinical prediction rules were thereby prepared.
“Emergency operation,” “blood loss >400 mL,” “presence of diabetes,” “presence of skin disease,” and “total serum albumin value <3.2 g/dL” were detected by multivariable modeling and were incorporated into the risk scores. Applying these 5 independent predictive factors, we were able to predict the infection incidence after spinal surgery.
Our present study could aid physicians in making decisions regarding prevention strategies in patients undergoing spinal surgery. Stratification of risks employing this scoring system will facilitate the identification of patients most likely to benefit from complex, time-consuming and expensive infection prevention strategies, thereby possibly reducing healthcare costs.
We performed family psychoeducation for depression, and investigated the association between the education and expressed emotion of patients’ families and relapse of depression.
Of 103 patients diagnosed with major depressive disorder, and their primary family members, 53 patients and their primary family members gave consent. The patients were randomly allocated to an intervention or control group, consisting of 24 and 30 patients, respectively. The intervention group underwent 4 educational sessions and education in coping techniques. The relapse rate was compared between the intervention and control groups. In addition, the subjects were divided into high- and low-EE groups based on the EE judgment, and the effect of psychoeducation was compared in each group.
The relapse rate during a 9-month period was 8.3% in the intervention group, being significantly lower than that (50%) in the control group. The relapse rate in the intervention group was slightly lower than that in the control group in the high-EE group, and significantly lower in the low-EE group. Regarding the influence of EE, in the control group, the relapse rate was 70% in the high-EE group, being significantly higher than that (40%) in the low-EE group. On multiple logistic regression analysis, psychoeducation (odds ratio: 25.53, 95% CI: 2.83-229.92) and the Hamilton score at the time of entry (odds ratio: 1.16, 95% CI: 1.045-1.298) were significantly associated with relapse.
It was suggested that the psychoeducation of families is very effective for the prevention of relapse in adult depressive patients.
There are no effective programs on return-to-work (RTW) despite an increase of stress related disorders. We developed an original rehabilitation program,’Ultra-short daily briefings care (USDBC)’. USDBC is based on a key concept of European Framework for Psychosocial Risk Management (PRIMA-EF; WHO, 2008) that provides the good practice guidelines at the workplace. We carried out USDBC at the worksite of Panasonic Healthcare Co., Ltd. to determine whether USDBC facilitates RTW.
To develop and establish the appropriate intervention that reduces depressive severity of sick-listed employees.
The aim of the study was to determine whether USDBC strengthen the sense of coherence (SOC; Antonovsky, 1985).
We compared two groups in a cross-sectional study design: 16 depressed RTW employees (USDBC group) vs. 121 healthy employees (control group) (Fig.1). USDBC group was received the instant face-to-face rehabilitation program in every workday (Fig.2). The primary outcome was the ability to cope with stress, measured by self-reported 13-items SOC scale for Japanese (Yamazaki, 1999).
In the USDBC group, significant changes were observed between baseline and measurement point in SOC score (40.3 vs. 54.4; 95% CI (20.6 to (7.5), whereas in the control group, no significant changes were observed (58.3 vs. 57.9; 95% CI (0.1 to 0.9) (Table.1).
The study suggests that USDBC strengthen the depressed employees’ SOC.
Participant now climt
Flow diagram showing the selection of USDBC group and control group
Intervention with USDBC
Depressive employees behave according to this flow in every workday.
Subjects’ characteristics and SOC.
USDBC group (n=l6)
39 (32 - 53)
Control group (n=121)
41 (21 - 59)
-0 1 to 0.9
In the USDBC goroup, significant change was found between baselne and tneasurment point. In the control group, no significant change was found.
Attention bias (AB) is a biased information processing towards threat among competing stimuli occurred in early stage of sensory input. Substantial evidence indicates that AB is involved in the development and maintenance of anxiety and depressive disorders. However, little is known about the relationships between AB and individual differences of endocrine and neuropsychological functions.
Thirty healthy participants without major physical illness or axis I/II mental disorders as evaluated with the Mini-International Neuropsychiatric Interview, were enrolled. Participants completed a dot-probe task, the Temperament and Character Inventory (TCI), the Beck Depression Inventory-II (BDI-II), the Interpersonal Sensitivity Measure, and the Trail Making Test (TMT). Salivary cortisol levels were measured at three time points per day for consecutive 2 days: immediately and 30 min after awaking in the morning and before sleep at night. Correlation analyses were performed between AB and psychological measures, cortisol levels, and attention measures.
As predicted, AB significantly correlated with BDI-II and Harm avoidance sub-dimension of the TCI. Above all, when those variables that were significantly correlated with AB were included in a step-wise multivariate regression analysis, higher cortisol level at night remained the most influential predictor for AB.
Our results suggest that AB is significantly influenced not only by anxious personality traits and depressive symptoms but also by individual differences of attention function and stress hormonal levels. Particularly, AB modification approach might have a beneficial effect on anxiety in individuals who have high cortisol levels.
There is increasing recognition that pain often coexists with depression. the current survey was undertaken to ascertain patients’ and clinicians’ perceptions of pain as a physical symptom associated with depression.
Web-based surveys were undertaken for patients with depression, and for physicians treating patients with depression (psychiatrists, psychosomatic physicians, general internists).
848 patients aged 20–59 years entered the main survey, of whom 663 returned the completed survey (78.2%). of the respondents, 424 (64.0%) experienced at least one painful symptom, with almost three-quarters (72.1%) reporting that the pain affected mental symptoms and 68.6% indicating that it prevented recovery from depression itself. Among 337 patients who discussed their painful symptoms with their physician, 52.5% initiated the discussion.
456 physicians completed the physician survey. When asked about the influence of pain associated with depression, 61.7% of physicians indicated that they ask their patients about pain during a consultation, and 79.9% considered that painful symptoms might disturb the patients’ daily life and 52.8% felt that they would delay recovery from depression.
The survey provides further evidence of the association between depression and pain, highlighting the fact that pain is prevalent in this patient population. Increased patient and physician awareness of pain in association with depression and improved doctor-patient communication, enabling patients to discuss painful symptoms with their physicians, and vice-versa, should lead to better overall management and treatment strategies.
There has been little research on the association of attention-deficit/hyperactivity disorder (ADHD) with co-occurring physical diseases. The aim of this study was to examine the association between possible ADHD and physical multimorbidity (i.e. = 2 physical diseases) among adults in the English general population.
Data were analyzed from 7274 individuals aged = 18 years that came from the Adult Psychiatric Morbidity Survey 2007. ADHD symptoms were assessed with the Adult Self-Report Scale (ASRS) Screener. Information was also obtained on 20 self-reported doctor/other health professional diagnosed physical health conditions present in the past 12 months. Multivariable logistic regression and mediation analyses were conducted to assess the associations.
There was a monotonic relation between the number of physical diseases and possible ADHD (ASRS score = 14). Compared to those with no diseases, individuals with = 5 diseases had over 3 times higher odds for possible ADHD (odds ratio [OR]: 3.30, 95% confidence interval [CI]: 2.48–4.37). This association was observed in all age groups. Stressful life events (% mediated 10.3–24.3%), disordered eating (6.8%), depression (12.8%), and anxiety (24.8%) were significant mediators in the association between possible ADHD and physical multimorbidity.
Adults that screen positive for ADHD are at an increased risk for multimorbidity and several factors are important in this association. As many adults with ADHD remain undiagnosed, the results of this study highlight the importance of detecting adult ADHD as it may confer an increased risk for poorer health outcomes, including physical multimorbidity.
Pear psyllids (Hemiptera: Psylloidea: Psyllidae: Cacopsylla spp.) belong to the most serious pests of pear (Pyrus spp.). They damage pear trees by excessive removal of phloem sap, by soiling the fruits with honeydew which, in turn, provides a substrate for sooty mould, and by transmission of Candidatus Phytoplasma spp., the causal agents of the pear decline disease. The morphological similarity, the presence of seasonal dimorphism that affects adult colour, size and wing morphology and uncritical use of species names, led to much confusion in the taxonomy of pear psyllids. As a result, pear psyllids have been frequently misidentified. Many of the entries attributed to Cacopsylla pyricola and other species in the GenBank are misidentifications which led to additional, unnecessary confusion. Here we analysed DNA barcodes of 11 pear psyllid species from eastern Asia, Europe and Iran using four mitochondrial gene fragments (COI 658 bp, COI 403 bp, COI-tRNAleu-COII 580 bp and 16S rDNA 452 bp). The efficiency of identification was notably high and considerable barcoding gaps were observed in all markers. Our results confirm the synonymies of the seasonal forms of Cacopsylla jukyungi ( = C. cinereosignata, winter form) and C. maculatili ( = C. qiuzili, summer form) previously suggested based on morphology. Some previous misidentifications (C. chinensis from China, Japan and Korea = misidentification of C. jukyungi; C. pyricola and C. pyrisuga from East Asia = misidentification of C. jukyungi and C. burckhardti, respectively; C. pyricola from Iran = misidentification of C. bidens, C. pyri and Cacopsylla sp.) are also corrected. There is no evidence for the presence of European pear psyllid species in East Asia.
Natural disasters affect long-term health by directly disrupting or destroying health-care systems and social support. We examined the associations between social support and subjective symptoms (SS) among disaster victims living in their homes approximately 1–2 years after the Great East Japan Earthquake and tsunami on March 11, 2011, which devastated the northeastern Japan seaboard and far inland, focusing on Ishinomaki, Miyagi Prefecture.
The Health and Life Revival Council of Ishinomaki District conducted door-to-door household surveys between April 2012 and January 2013. Replies to 12 questions regarding social support, specifically emotional, informational, and instrumental, were investigated. SS prevalence was calculated as the proportion of those having any of 8 predetermined symptoms including back pain, neck stiffness, sleep difficulty, dizziness, heart palpitations, poor appetite, or stomachache. Logistic regression analysis by sex was used to obtain crude and adjusted odds ratios for the association between SS prevalence and forms of social support.
From 4023 households, self-reported data on 2593 individuals from 1709 households were obtained. SS prevalence was 29.1%. Adjusted logistic regression analysis revealed that instrumental support with others and emotional support with personal and others were specific associated with SS in men and women, respectively.
Our findings suggest that providing social support depending on needs is potentially effective in preventing SS in disaster areas.
Recently huge amount of dust Mdust ≃ 106−7M⊙ in galaxies at z = 7–8 has been discovered by ALMA observations. The suggested timescale of the dust production was a few–several×108 yr, while the stellar mass was several × 109M⊙. This amount of dust cannot be easily explained only by a supply from supernovae if we consider the dust destruction by reverse shocks. We propose that these values can be consistently explained if we take into account the grain growth in the interstellar medium (ISM). This scenario successfully reproduces the evolution of the dust mass, as well as the SFR, and stellar mass simultaneously. We conclude that even at such an early epoch of the Universe, the dust grain growth in the ISM plays a significant role in galaxies.
The spectral energy distribution (SED) model should treat the evolution of a galaxy from its birth. Dust in galaxies affects the formation and evolution of galaxies in various ways. For example, dust grains scatter and absorb stellar emitted ultraviolet (UV) photons and re-emit the radiation at infrared (IR) wavelengths. In this work, we construct a galaxy SED model based on our dust evolution model (Asano et al. 2013a,b, 2014) with a rigorous treatment of the chemical evolution. To reduce the computational cost, we adopt mega-grain approximation (MGA; (MGA; Inoue, 2005). MGA regards a high density dusty region as a huge size (10 pc) dust grain for calculating dust scattering. In this approximation, we can solve the radiative transfer easily and provide SEDs and attenuation curves of galaxies. This model can be used to fit any galaxy in the wavelength range of 10 nm-3 mm.
Recently, spectroscopic detections of O[III] 88 μm and Ly-α emission lines from the z ≍ 9.1 galaxy MACS1149-JD1 have been presented, and with these, some interesting properties of this galaxy were uncovered. One such property is that MACS1149-JD1 exhibits a significant Balmer break at around rest-frame 4000 Å, which may indicate that the galaxy has experienced large variations in star formation rate prior to z ∼ 9, with a rather long period of low star formation activity. While some simulations predict large variations in star formation activity in high-redshift galaxies, it is unclear whether the simulations can reproduce the kind of variations seen in MACS1149-JD1. Here, we utilize synthetic spectra of simulated galaxies from two simulation suites in order to study to what extent these can accurately reproduce the spectral features (specifically the Balmer break) observed in MACS1149-JD1. We show that while the simulations used in this study produce galaxies with varying star formation histories, galaxies such as MACS1149-JD1 would be very rare in the simulations. In principle, future observations with the James Webb Space Telescope may tell us if MACS1149-JD1 represents something rare, or if such galaxies are more common than predicted by current simulations.
We have developed a new SED fitting tool specialized for frontier redshift galaxies. It is a common case for high-z galaxies that the available data are restricted to rich optical to near-infrared photometry and few far-infrared (FIR) data deep enough to detect the faint object (e.g., HST/WFC3 + Spitzer/IRAC + ALMA). In such situation, one cannot perform a complicated modeling of dust emission in FIR regime. We then adopt simple treatment for the dust emission using empirical LIRG templates. Instead, we adopt a sophisticated and physically motivated modeling for stellar and nebular emission parts in rest-frame UV-to-optical regime. Our new code fits not only broad band photometry but also spectral emission line flux. There is an option to fit observed SED with two templates with different physical properties. Our new code, PANHIT, is now in public, and was already applied to some high-z frontier galaxies.
Panchromatic modeling is one of the most powerful tools at our disposal to measure reliably the physical properties of galaxies across cosmic times. We present here an entirely new implementation in python of one such tool: CIGALE. Developed along three main design principles: simplicity, modularity, and efficiency, it has proven to be a versatile code that in addition to estimating the physical properties of galaxies (or regions within galaxies), can generate arbitrary sets of theoretical models or be used as a library to build other tools. Among its defining features, it is a truly panchromatic code ranging from the far-ultraviolet to the radio that takes into account numerous physical components (including active nuclei or synchrotron emission), that can fit non-photometric data, handle upper limits, determine photometric redshifts, and even build mock catalogs.
We present ALMA detection of the [O iii] 88 μm line and 850 μm dust continuum emission in a Y-dropout Lyman break galaxy, MACS0416_Y1. The [O iii] detection confirms the object with a spectroscopic redshift to be z = 8.3118±0.0003. The 850 μm continuum intensity (0.14 mJy) implies a large dust mass on the order of 4×106M⊙. The ultraviolet-to-far infrared spectral energy distribution modeling, where the [O iii] emissivity model is incorporated, suggests the presence of a young (τage ≍ 4 Myr), star-forming (SFR ≍ 60M⊙yr−1), and moderately metal-polluted (Z ≍ 0.2Z⊙) stellar component with a stellar mass of 3 × 108M⊙. An analytic dust mass evolution model with a single episode of star formation does not reproduce the metallicity and dust mass in ≍ 4 Myr, suggesting an underlying evolved stellar component as the origin of the dust mass.
Metallic glasses have attractive properties, but since the glassy state is inherently metastable, they are not normally considered for applications at elevated temperatures. Yet, studies have shown that multicomponent and pseudo high-entropy (PHE) compositions can confer useful heat resistance. The formation, thermal stability, and mechanical and chemical properties of multicomponent Fe-(Cr, Mo)- and Zr-based bulk metallic glasses (BMGs) are reviewed to assess their potential as heat-resistant structural materials. The composition Fe43Cr16Mo16C15B10 is castable and fully glassy with rod diameters up to 2.7 mm. Glassy coatings of this material with low porosity, good mechanical properties, and good corrosion resistance can be produced by high-velocity spray coating. The compositions Zr55–65Al7.5–10(TM1,TM2)27.5–35 (TM1 = Fe, Co, Ni, TM2 = Cu, Pd, Ag, Au) yield PHE BMGs, in which a stable cluster-like glassy phase without crystalline precipitates is formed by annealing at temperatures well above the first calorimetric transformation. It is suggested that proliferation of alloy components is an effective method to synthesize metastable metallic materials that retain high strength at elevated temperatures.
We report fourteen and twenty-eight protocluster candidates at z = 5.7 and 6.6 over 14 and 19 deg2 areas, respectively, selected from 2,230 Lyα emitters (LAEs) photometrically identified with Subaru/Hyper Suprime-Cam (HSC) deep images. Six out of the 42 protocluster candidates include at least 1 spectroscopically confirmed LAEs at redshifts up to z = 6.574. By the comparisons with the cosmological Lyα radiative transfer (RT) model reproducing LAEs with the reionization effects, we find that more than a half of these protocluster candidates might be progenitors of the present-day clusters with a mass of ≳ 1014M⊙. We also investigate the correlation between LAE overdensity and Lya rest-frame equivalent width (EW), because the cosmological Lyα RT model suggests that a slope of EW-overdensity relation is steepened towards the epoch of cosmic reionization (EoR), due to the existence of the ionized bubbles around galaxy overdensities easing the escape of Lyα emission from the partly neutral intergalactic medium. The available HSC data suggest that the slope of the EW-overdensity correlation does not evolve from the post-reionization epoch z = 5.7 to the EoR z = 6.6 beyond the moderately large statistical errors.
We present a 4.7σ detection of the [OIII] 88 μm line in a gravitationally-lensed Lyman break galaxy, RXC J2248-ID3, using the Atacama Large Millimeter/submillimeter Array (ALMA). We did not detect [CII] 158 μm and rest-frame 90 μm dust continuum emission, suggesting that the bulk of the interstellar medium (ISM) is ionized. Our two-component SED model combining the previous Hubble Space Telescope (HST) data and new photometry obtained from Very Large Telescope (VLT), Spitzer and ALMA suggests the presence of young (∼2 Myr) and mature (∼600 Myr) stellar components with the metallicity of Z = 0.2Z⊙. Our findings are in contrast with previous results claiming a very young, metal-poor stellar component.