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The predictive power of polygenic scores (PGSs) for lithium treatment response in bipolar disorder remains limited.
Aims
To enhance the prediction of lithium responsiveness by developing a multi-trait PGS (mt-PGS) combining genetic information from multiple phenotypes implicated in lithium response and/or bipolar disorder aetiology.
Method
We analysed data collected from bipolar disorder patients who had received lithium treatment for at least 6 months and participated in the International Consortium on Lithium Genetics study (N = 2367). The Alda scale was used to assess lithium responsiveness, and treatment outcome was defined as continuous total Alda score (0–10) and categorical outcome (favourable ≥7 versus unfavourable response). PGSs were calculated for 60 phenotypes grouped into 5 clinical–biological clusters: psychiatric and behavioural (#23 phenotypes), cardiometabolic (#17), autoimmune/inflammatory (#5), neurocognitive (#8) and renal function (#7). We applied cross-validated machine learning regression approaches in both outcomes within each cluster, with the selected features from each cluster subsequently combined to construct the final mt-PGS models. Model performance was assessed using explained variance (R2) for the continuous outcome, and both McFadden’s pseudo-R2 and standard classification model parameters for the categorical outcome.
Results
mt-PGS explained between 5.70% (continuous outcome) and 9.11% (categorical outcome) of the interindividual variability in lithium responsiveness. Classification accuracy (area under the curve) for the categorical outcome was 68.24% (95% CI: 64.98–71.66), with a Brier score of 0.257. Of the 5 clusters, the PGSs for psychiatric and behavioural phenotypes were most strongly associated with lithium responsiveness, accounting for 3.67–6.52% of its variability.
Conclusions
By integrating PGSs for multiple relevant phenotypes, predictive accuracy for lithium response improved substantially compared with single-trait methods. Future research incorporating larger, more diverse populations and combining genetic scores with clinical data holds promise for further enhancing prediction and advancing clinical implementation.
Psychotherapy is evolving in low- and middle-income countries, where expanding access must be balanced with cultural relevance. This paper examines how culturally grounded adaptations preserve theoretical fidelity while enhancing contextual responsiveness. Drawing on the 2025 World Federation for Psychotherapy Regional Meeting in Manila, three vignettes – from the Philippines, Uganda and Indonesia – illustrate how constructs such as kapwa, pakikiramdam, ubuntu and intergenerational obligation are integrated into evidence-based models. These adaptations demonstrate how core psychotherapeutic elements, particularly common factors such as alliance and empathy, are operationalised through local meaning systems while addressing structural conditions and trauma. Cultural grounding therefore extends, rather than fragments, psychotherapy’s theoretical foundations.
Emergency department (ED) urine culture stewardship may reduce low-value testing, but downstream effects on antibiotic use and postdischarge utilization remain uncertain.
Methods:
We evaluated an intervention in which an infectious diseases physician and microbiologist reviewed pyuric urinalysis-with-reflex encounters, assessed culture indications, and contacted clinicians to recommend cancellation when absent. Adult ED encounters from February–July 2025 to September 2025-February 2026 were included; August was washout. Outcomes were urinalysis with reflex within 24 hours, urine culture within 24 hours, antibiotic days of therapy (DOT) per 100 patient-days, length of stay (LOS), and 30-day ED revisit among ED discharges. We fit biweekly interrupted time series models.
Results:
Among 17,621 encounters, the intervention was associated with lower postintervention slopes for urinalysis with reflex within 24 hours (−0.5 percentage points per biweekly period; 95% CI, −0.9 to −0.1) and urine culture within 24 hours (−0.2 percentage points; 95% CI, −0.4 to −0.0). DOT showed no sustained change (postintervention slope change, 0.00; 95% CI, −0.23 to 0.24). LOS showed a lower postintervention slope (−0.05 d; 95% CI, −0.08 to −0.02). Thirty-day ED revisit showed a higher postintervention slope (0.8 percentage points; 95% CI, 0.3 to 1.3).
Conclusions:
The intervention reduced urinary testing but did not reduce antibiotic DOT and was associated with increased 30-day ED revisit. Diagnostic stewardship in the ED may need to be paired with antimicrobial stewardship and prospective safety monitoring.
Research suggests that the gender gap in alcohol (Alc.) consumption may be narrowing, with increasing consumption by the female population. For women, the equivalent of 20-25 grams/day is considered harmful consumption. Many of the harmful effects of alcohol consumption occur more rapidly and more severely in women, yet the majority do not seek treatment
Objectives
To describe the prevalence of harmful use of alcohol in women admitted to hospital for other mental illness.
Methods
Retrospective observational study of six months duration. Data was collected from all patients admitted to the hospital during the period of study, with no specific exclusion criteria. Descriptive statistics were performed.
Results
During the study period, 312 patients were admitted to the hospital, 52.8% of whom were women, 21.8% of whom had a harmful use of Alc. The prevalence of harmful Alc. use in the different mental illnesses was: 22.2% in schizophrenia or other psychoses, 13.9% in bipolar affective disorder, 11.1% in depressive disorder, 13.9% in personality disorder, 19.4% in substance use disorder, 13.9% for other diagnoses and a prevalence of 5.56% for those of unknown diagnosis
Conclusions
In recent years, it has been shown that the overall prevalence of harmful alcohol use and alcohol use disorder has increased in women. They tend to seek care in settings where their alcohol problems may not be recognised. They have lower social support for treatment participation and greater barriers to accessing treatment, resulting in even higher rates of co-occurring medical and mental health problems. Prevention strategies and intervention programmes should be adapted to the specific needs of women, taking into account both individual risk factors and socio-cultural contexts
Stellar bars drive the galaxy secular evolution. While rotating around the galaxy centre with a given angular frequency, the bar pattern speed, they sweep material and modify the galaxy structure. In the LCDM model, bars are expected to slow down by exchanging angular momentum with the other omponents and/or through dynamical friction exerted by the dark matter halo. The only direct method to derive the bar pattern speed, the Tremaine-Weinberg method, revealed that real bars rotate fast, stressing a tension between the observations, conducted to date in the local universe, and the LCDM model. Measuring the bar pattern speed to bars up to z∼1-2 will reveal if the expected bar evolutionary path is actually taking place and/or to confirm if the dark matter is able to exert friction. Using high resolution N-body simulations we tested the applicability of the Tremaine-Weinberg method to deep spectroscopy of the NIRSpec@JWST for a sample of bars at z∼1-2. Our analysis can be used to prepare an observational proposal to get dedicated data.
We report 3 years of data from one meteorological and three smaller stations in University Valley, a high-elevation (1677 m) site in the Dry Valleys of Antarctica with extensive dry permafrost. Mean air temperature was -23.4°C. Summer air temperatures were virtually always < 0°C and were consistent with the altitude lapse rate and empirical relationships between summer temperature, distance from the coast and elevation. The measured frost point (-22.5°C) at the 42 cm deep ice table is equal to the surface frost point and above the atmospheric frost point (-29.6°C), providing direct evidence that surface conditions control ground ice depth. Observed peak surface soil temperatures reach 6°C for ice-cemented ground > 15 cm deep but stay < 0°C when it is shallower. We develop an energy balance model tuned to this rocky and dry environment. We find that differences in peak soil surface temperatures are primarily due to the higher thermal diffusivity of ice-cemented ground compared to dry soil. Sensitivity studies show that expected natural variability is insufficient for melt to form and significant excursions from current conditions are required. The site's ice table meets the criteria for a Special Region on Mars, with 30% of the year > -18°C and water activity > 0.6.
Studying phenotypic and genetic characteristics of age at onset (AAO) and polarity at onset (PAO) in bipolar disorder can provide new insights into disease pathology and facilitate the development of screening tools.
Aims
To examine the genetic architecture of AAO and PAO and their association with bipolar disorder disease characteristics.
Method
Genome-wide association studies (GWASs) and polygenic score (PGS) analyses of AAO (n = 12 977) and PAO (n = 6773) were conducted in patients with bipolar disorder from 34 cohorts and a replication sample (n = 2237). The association of onset with disease characteristics was investigated in two of these cohorts.
Results
Earlier AAO was associated with a higher probability of psychotic symptoms, suicidality, lower educational attainment, not living together and fewer episodes. Depressive onset correlated with suicidality and manic onset correlated with delusions and manic episodes. Systematic differences in AAO between cohorts and continents of origin were observed. This was also reflected in single-nucleotide variant-based heritability estimates, with higher heritabilities for stricter onset definitions. Increased PGS for autism spectrum disorder (β = −0.34 years, s.e. = 0.08), major depression (β = −0.34 years, s.e. = 0.08), schizophrenia (β = −0.39 years, s.e. = 0.08), and educational attainment (β = −0.31 years, s.e. = 0.08) were associated with an earlier AAO. The AAO GWAS identified one significant locus, but this finding did not replicate. Neither GWAS nor PGS analyses yielded significant associations with PAO.
Conclusions
AAO and PAO are associated with indicators of bipolar disorder severity. Individuals with an earlier onset show an increased polygenic liability for a broad spectrum of psychiatric traits. Systematic differences in AAO across cohorts, continents and phenotype definitions introduce significant heterogeneity, affecting analyses.
Up to 45% of individuals who commit suicide contact their Primary Care physician (PCP) the month before. The objective is to study clinical characteristics of patients presenting death and/or suicidal ideation (SI) in Primary Care.
Methods:
195 patients attending their PCP were evaluated using systematic sampling in three Primary Care Centres. Patients completed the PHQ and a Life Changes Checklist. Demographic data, both psychiatric and medical conditions and treatments, visits to their PCP, and days out of work (last year) were also collected.
Results:
24 patients had death or suicidal ideation for the previous two weeks (12,4%; IC95% 8,3-18,8%). Most of them (87,5%) had a mental disease, major depressive disorder (62,5%) and general anxiety disorder (50%). Patients with SI had more somatic symptoms (p<0,001), a greater number and score of recent life changes (p<0,001) and days out of work (last year) ((p=0,028) than the rest of the sample.
Compared to patients with any psychiatric disorder, patients with SI had more depressive symptoms (p<0,001) and a higher score in life changes in the 6-12 month period (p=0,044).
14 (58,3%) patients with SI had no previous psychiatric diagnosis and only 8 (33%) were receiving treatment.
Conclusions:
In spite of a greater severity in depressive and other clinical characteristics of patients with SI most of them are not correctly detected and treated. Improving the rate of detection and treatment by the PCP of such patients would probably play a key role in the prevention of suicide.
Chronic insomnia (ChI) is a common condition in Primary Care (PC). Regardless that it's often related to psychiatric morbidity it appears to be a strong predictor of future depression and a disabling disorder by itself. The aim of this study was to measure and compare clinical and psychiatric characteristics of both patients with primary ChI and secondary ChI.
Methods:
A random sample of 225 subjects older than 18 years old, from 3 PC Centres of the area of Madrid (Spain) was interviewed using the Oviedo Sleep Questionnaire, a semi-structured interview for sleep disorders. The subjects completed the Patient Health Questionnaire. Data about medical conditions, drug treatments, days of work lost (last year) and use of health care services (last 3 months), were also collected. Psychiatric and clinical characteristics between groups (primary vs secondary ChI) were compared.
Results:
78 patients fulfilled criteria for ChI and 53 (67.9 %) of them were suffering from any psychiatric disorder (including subtreshold conditions). Patients with primary ChI compared to secondary insomnia patients had no significant differences in age, gender, use of health care resources and days of work lost. However, patients with secondary ChI compared to primary ChI had more somatic and depressive symptoms (U-Mann-Witney test; p=0.002 and p<0.001, respectively).
Conclussions:
There is an important group of patients among PC attendees suffering primary ChI. Patients suffering primary ChI are comparable to patients with psychiatric disorders and insomnia in terms of days of work lost and use of health care resources.
Previous data suggest that there is an important group of patients between primary care (PC) attendees suffering a psychiatric disorder that remain undetected. Our aim was to know data about this group of patients compared with patients without psychiatric pathology (PWP) and patients with already known psychiatric pathology (PKP).
Methods:
A random sample of 225 subjects older than 18 years old, from 3 PC Centres of the area of Madrid (Spain) completed the Patient Health Questionnaire (PHQ). Data about medical and psychiatric conditions, drug treatments, days of work lost (last year) and use of health care services (last 3 months), were also collected. Psychiatric and clinical characteristics between groups were compared.
Results:
50 (22,2%) patients were suffering a psychiatric condition according to PHQ but without recognition by their general practioner. This group of patients were younger than PWP and PKP (ANOVA; p=0,021 and p=0,013). They were suffering more depressive symptoms and somatic complaints than PWP (p<0,001 and p<0,001 respectively). In terms of days of work lost and use of health care services did not differ from PWP.
Conclusions:
The results suggest that other reasons rather than the symptomathology (depresive symptoms, somatic complaints) may be important in the proccess of detection of mental health problems in PC. Both days of work lost and the number of visits to general practioner appear to be two determinant factors.
Neurocognitive disorders are the only psychiatric disorders which underlying pathogeny can potentially be determined. This has important implications, for it makes possible the use of biomarkers in order to gain better diagnosis, and opens a door to more accurate treatments. Nonetheless, as biomarkers are not exclusive of a single disorder, the lengths of its utility are still unknown.
Objectives and aims
To understand the values and limitations of biomarkers in differential diagnosis of dementias.
Methods
We present three cases followed in the Neurology ward of our hospital, in which they were admitted for diagnosis and treatment of a subacute form of dementia. Medical history, core symptoms, screening tests for cognitive impairment, MRI, EEG and biomarkers in cerebrospinal fluid were used for diagnosis.
Results
Two cases had consistent clinical features and complementary explorations, and they were respectively diagnosed as Creutzfeldt-Jakob Disease and Lewy Body Dementia; however, the last case showed contradictory results between clinic and complementary explorations, particularly 14-3-3 protein, which was positive and led to the initial diagnosis as Creutzfeldt-Jakob Disease, which was proven wrong once necropsy was practiced.
Conclusions
Although complementary explorations, and biomarkers in particular, are of invaluable utility in the accurate diagnosis of multiple psychiatric diseases, they must always be considered within a context given by biography and clinical features, because, when failing to do so, they can lead to misdiagnosis and delay of correct treatment.
A comprehensive morphostratigraphic and chronological study of the complete set of Holocene tephras from Tafí and Santa María valleys (northwestern Argentina), including analyses of compositional characteristics, is presented. Five ash tephras are recognized: V0 (El Rincón), V1a (Carreras 1a ash), V1b (Carreras 1b ash), V2a (Carreras 2 ash), and V2b (El Paso 3 ash). Two of them (V1b and V2b) are described for the first time in the study area. The new 14C and accelerator mass spectrometry ages presented, along with the previously published information, allows for the establishment of a chronological framework. The V0 tephra was deposited in the Early Holocene (about 10,000 yr BP), V1a and V1b were deposited in the Middle Holocene (about 4200 and 3500 yr BP, respectively), and V2a and V2b were deposited in the Late Holocene (after about 800 yr BP). The mineralogical, textural, and geochemical characterizations of the five tephras suggest that their tephra provenance was mainly from the back-arc region. However, the determination of the exact source of each tephra requires more accurate high-resolution tephrochronological studies. At least five major eruptions affected the Tafí and Santa María valleys in the last 10,000 yr.
Adipogenesis, myogenesis and fibrogenesis are related processes that can contribute to meat quality. Therefore, extending the knowledge of these processes would facilitate the identification of molecular markers that predict intramuscular fat accretion. The main purpose of this work, based on previous results, was to further study the expression of key genes related to adipogenic, myogenic, fibrogenic processes and some cytokines in Longissimus thoracis (LT) and Masseter (MS) muscles of Pirenaica and Holstein young bulls. Longissimus thoracis and MS muscles from Pirenaica (n = 4) and Spanish Holstein (n = 4) were sampled for proximate analysis, determination of adipocyte size distribution and expression of key candidate genes. Fat percentage was lower in LT than in MS muscle in Pirenaica young bulls (P = 0.023) and was higher in LT muscle in Holstein than in Pirenaica young bulls (P = 0.007). Gene expression analysis revealed that the mRNA level of myogenic differentiation 1 (MYOD) was higher in LT than in MS muscles in both groups of animals (P < 0.001) and that myostatin (MSTN) expression was also higher in LT than in MS muscle in Holstein bulls (P = 0.001). On the other hand, MSTN and PPARG showed higher expression in LT and MS in Pirenaica young bulls (P = 0.026), while the expression of fatty acid-binding protein 4 (FABP4) was higher in Holstein young bulls, also in both muscles (P < 0.001). The results suggested that the development of intramuscular adipose depot was directly related to the expression of adipogenic genes, such as FABP4, but inversely related to the expression of the cytokine MSTN and the myogenic gene MYOD, genes which showed a muscle-specific expression.
This research communications addresses the hypothesis that a part of iso 17:0 and anteiso 17:0 in milk fat could come from endogenous extraruminal tissue synthesis. In order to confirm this a linear regression model was applied to calculate the proportions of iso 17:0 and anteiso 17:0 in milk fat that could come from elongation of their putative precursors iso 15:0 and anteiso 15:0, respectively. Sixteen dairy goats were allocated to two simultaneous experiments, in a crossover design with four animals per treatment and two experimental periods of 25 d. In both experiments, alfalfa hay was the sole forage and the forage to concentrate ratio (33 : 67) remained constant. Experimental diets differed on the concentrate composition, either rich in starch or neutral detergent fibre, and they were administered alone or in combination with 30 g/d of linseed oil. Iso 15:0, anteiso 15:0, iso 17:0 and anteiso 17:0, the most abundant branched-chain fatty acids in milk fat, were determined by gas chromatography using two different capillary columns. The regression model resolved that 49% of iso 17:0 and 60% of anteiso 17:0 in milk fat was formed extraruminally from iso 15:0 and anteiso 15:0 elongation.
We present surface photometry and stellar kinematics of NGC 4264, a lenticular galaxy in the region of the Virgo Cluster undergoing a tidal interaction with its neighbour, NGC 4261. We measured the bar radius and strength from SDSS imaging and the bar pattern speed from MUSE integral-field spectroscopy. We find that NGC 4264 hosts a strong and large bar, which is rotating fast. The accurate measurement of the bar rotation rate allows us to exclude that the formation of the bar was triggered by the ongoing interaction.
With the recent discovery of a dozen dusty star-forming galaxies and around 30 quasars at z > 5 that are hyper-luminous in the infrared (μ LIR > 1013 L⊙, where μ is a lensing magnification factor), the possibility has opened up for SPICA, the proposed ESA M5 mid-/far-infrared mission, to extend its spectroscopic studies toward the epoch of reionisation and beyond. In this paper, we examine the feasibility and scientific potential of such observations with SPICA’s far-infrared spectrometer SAFARI, which will probe a spectral range (35–230 μm) that will be unexplored by ALMA and JWST. Our simulations show that SAFARI is capable of delivering good-quality spectra for hyper-luminous infrared galaxies at z = 5 − 10, allowing us to sample spectral features in the rest-frame mid-infrared and to investigate a host of key scientific issues, such as the relative importance of star formation versus AGN, the hardness of the radiation field, the level of chemical enrichment, and the properties of the molecular gas. From a broader perspective, SAFARI offers the potential to open up a new frontier in the study of the early Universe, providing access to uniquely powerful spectral features for probing first-generation objects, such as the key cooling lines of low-metallicity or metal-free forming galaxies (fine-structure and H2 lines) and emission features of solid compounds freshly synthesised by Population III supernovae. Ultimately, SAFARI’s ability to explore the high-redshift Universe will be determined by the availability of sufficiently bright targets (whether intrinsically luminous or gravitationally lensed). With its launch expected around 2030, SPICA is ideally positioned to take full advantage of upcoming wide-field surveys such as LSST, SKA, Euclid, and WFIRST, which are likely to provide extraordinary targets for SAFARI.
The present study examined the association between high-quality diet (using the Mediterranean diet (MD) as an example) and well-being cross-sectionally and prospectively in Spanish children and adolescents. Participants included 533 children and 987 adolescents at baseline and 527 children and 798 adolescents at 2-year follow-up, included in the UP&DOWN study (follow-up in schoolchildren and adolescents with and without Down’s syndrome). The present study excluded participants with Down’s syndrome. Adherence to an MD was assessed using the KIDMED index. Well-being was measured using the Positive and Negative Affect Schedule and the KIDSCREEN-10 questionnaire. Associations between MD adherence and well-being were assessed using multi-level, mixed-effects linear regression. At baseline, MD adherence was positively related to health-related quality of life in secondary school girls and boys (β=0·41, se 0·10, P<0·001; β=0·46, se 0·10, P<0·001, respectively) and to positive affect in secondary school girls and boys (β=0·16, se 0·05, P=0·006; β=0·20, se 0·05, P<0·001, respectively) and in primary school boys (β=0·20, se 0·08, P=0·019). At 2-year follow-up, MD adherence was negatively related to negative affect in secondary school adolescent girls and boys (β=–0·15, se 0·07, P=0·047; β=–0·16, se 0·06, P=0·019, respectively), and MD adherence was associated with higher positive affect scores in secondary school girls (β=0·30, se 0·06, P<0·001) and in primary school boys (β=0·20, se 0·09, P=0·023). However, MD adherence at baseline did not predict well-being indicators at 2-year follow-up. In conclusion, higher MD adherence was found to behave as a protective factor for positive well-being in cross-sectional analysis.
The SPICA mid- and far-infrared telescope will address fundamental issues in our understanding of star formation and ISM physics in galaxies. A particular hallmark of SPICA is the outstanding sensitivity enabled by the cold telescope, optimised detectors, and wide instantaneous bandwidth throughout the mid- and far-infrared. The spectroscopic, imaging, and polarimetric observations that SPICA will be able to collect will help in clarifying the complex physical mechanisms which underlie the baryon cycle of galaxies. In particular, (i) the access to a large suite of atomic and ionic fine-structure lines for large samples of galaxies will shed light on the origin of the observed spread in star-formation rates within and between galaxies, (ii) observations of HD rotational lines (out to ~10 Mpc) and fine structure lines such as [C ii] 158 μm (out to ~100 Mpc) will clarify the main reservoirs of interstellar matter in galaxies, including phases where CO does not emit, (iii) far-infrared spectroscopy of dust and ice features will address uncertainties in the mass and composition of dust in galaxies, and the contributions of supernovae to the interstellar dust budget will be quantified by photometry and monitoring of supernova remnants in nearby galaxies, (iv) observations of far-infrared cooling lines such as [O i] 63 μm from star-forming molecular clouds in our Galaxy will evaluate the importance of shocks to dissipate turbulent energy. The paper concludes with requirements for the telescope and instruments, and recommendations for the observing strategy.