Decontaminating N95 and SN95 masks with ultraviolet germicidal irradiation does not impair mask efficacy and safety.

Inadequate supply of filtering facepiece respirators (FFRs) for healthcare workers during a pandemic such as the novel coronavirus outbreak (SARS-CoV-2) is a serious public health issue. The aim of this study was to synthesize existing data on the effectiveness of ultraviolet germicidal irradiation (UVGI) for N95 FFR decontamination. A systematic review (PROSPERO CRD42020176156) was conducted on UVGI in N95 FFRs using Embase, Medline, Global Health, Google Scholar, WHO feed, and MedRxiv. Two reviewers independently determined eligibility and extracted predefined variables. Original research reporting on function, decontamination, or mask fit following UVGI were included. Thirteen studies were identified, comprising 54 UVGI intervention arms and 58 N95 models. FFRs consistently maintained certification standards following UVGI. Aerosol penetration averaged 1.19% (0.70-2.48%) and 1.14% (0.57-2.63%) for control and UVGI arms, respectively. Airflow resistance for the control arms averaged 9.79 mm H2O (7.97-11.70 mm H2O) vs 9.85 mm H2O (8.33-11.44 mm H2O) for UVGI arms. UVGI protocols employing a cumulative dose >20,000 J/m2 resulted in a 2-log reduction in viral load. A >3-log reduction was observed in seven UVGI arms using >40,000 J/m2. Impact of UVGI on fit was evaluated in two studies (16,200; 32,400 J/m2) and no evidence of compromise was found. Our findings suggest that further work in this area (or translation to a clinical setting) should use a cumulative UV-C dose of 40,000 J/m2 or greater, and confirm appropriate mask fit following decontamination.

Cosmic-ray antinuclei as messengers of new physics: status and outlook for the new decade.

The precise measurement of cosmic-ray antinuclei serves as an important means for identifying the nature of dark matter and other new astrophysical phenomena, and could be used with other cosmic-ray species to understand cosmic-ray production and propagation in the Galaxy. For instance, low-energy antideuterons would provide a "smoking gun" signature of dark matter annihilation or decay, essentially free of astrophysical background. Studies in recent years have emphasized that models for cosmic-ray antideuterons must be considered together with the abundant cosmic antiprotons and any potential observation of antihelium. Therefore, a second dedicated Antideuteron Workshop was organized at UCLA in March 2019, bringing together a community of theorists and experimentalists to review the status of current observations of cosmic-ray antinuclei, the theoretical work towards understanding these signatures, and the potential of upcoming measurements to illuminate ongoing controversies. This review aims to synthesize this recent work and present implications for the upcoming decade of antinuclei observations and searches. This includes discussion of a possible dark matter signature in the AMS-02 antiproton spectrum, the most recent limits from BESS Polar-II on the cosmic antideuteron flux, and reports of candidate antihelium events by AMS-02; recent collider and cosmic-ray measurements relevant for antinuclei production models; the state of cosmic-ray transport models in light of AMS-02 and Voyager data; and the prospects for upcoming experiments, such as GAPS. This provides a roadmap for progress on cosmic antinuclei signatures of dark matter in the coming years.

Neither Basic Life Support knowledge nor self-efficacy are predictive of skills among dental students.

AIM: Basic life support (BLS) is considered a core competence for the graduating dentist. This study aimed to measure BLS knowledge, self-efficacy and skills of undergraduate dental students in Dublin. METHODS: This study consisted of a cross-sectional survey measuring BLS knowledge and self-efficacy, accompanied by a directly observed BLS skills assessment in a subsample of respondents. Data were collected in January 2014. Bivariate correlations between descriptive and outcome variables (knowledge, self-efficacy and skills) were tested using Pearson's chi-square. We included knowledge and self-efficacy as predictor variables, along with other variables showing association, into a binary logistic regression model with BLS skills as the outcome measure. RESULTS: One hundred and thirty-five students participated. Almost all (n = 133, 98.5%) participants had BLS training within the last 2 years. One hundred and four (77%) felt that they were capable of providing effective BLS (self-efficacy), whilst only 46 (34.1%) scored >80% of knowledge items correct. Amongst the skills (n = 85) subsample, 38.8% (n = 33) were found to pass the BLS skills assessment. Controlling for gender, age and skills assessor, the regression model did not identify a predictive relationship between knowledge or self-efficacy and BLS skills. CONCLUSIONS: Neither knowledge nor self-efficacy was predictive of BLS skills. Dental students had low levels of knowledge and skills in BLS. Despite this, their confidence in their ability to perform BLS was high and did not predict actual competence. There is a need for additional hands-on training, focusing on self-efficacy and BLS skills, particularly the use of AED.

Supernovae. 44Ti gamma-ray emission lines from SN1987A reveal an asymmetric explosion.

In core-collapse supernovae, titanium-44 ((44)Ti) is produced in the innermost ejecta, in the layer of material directly on top of the newly formed compact object. As such, it provides a direct probe of the supernova engine. Observations of supernova 1987A (SN1987A) have resolved the 67.87- and 78.32-kilo-electron volt emission lines from decay of (44)Ti produced in the supernova explosion. These lines are narrow and redshifted with a Doppler velocity of ~700 kilometers per second, direct evidence of large-scale asymmetry in the explosion.

Galaxy evolution. Black hole feedback in the luminous quasar PDS 456.

The evolution of galaxies is connected to the growth of supermassive black holes in their centers. During the quasar phase, a huge luminosity is released as matter falls onto the black hole, and radiation-driven winds can transfer most of this energy back to the host galaxy. Over five different epochs, we detected the signatures of a nearly spherical stream of highly ionized gas in the broadband x-ray spectra of the luminous quasar PDS 456. This persistent wind is expelled at relativistic speeds from the inner accretion disk, and its wide aperture suggests an effective coupling with the ambient gas. The outflow's kinetic power larger than 10(46) ergs per second is enough to provide the feedback required by models of black hole and host galaxy coevolution.

An ultraluminous X-ray source powered by an accreting neutron star.

The majority of ultraluminous X-ray sources are point sources that are spatially offset from the nuclei of nearby galaxies and whose X-ray luminosities exceed the theoretical maximum for spherical infall (the Eddington limit) onto stellar-mass black holes. Their X-ray luminosities in the 0.5-10 kiloelectronvolt energy band range from 10(39) to 10(41) ergs per second. Because higher masses imply less extreme ratios of the luminosity to the isotropic Eddington limit, theoretical models have focused on black hole rather than neutron star systems. The most challenging sources to explain are those at the luminous end of the range (more than 10(40) ergs per second), which require black hole masses of 50-100 times the solar value or significant departures from the standard thin disk accretion that powers bright Galactic X-ray binaries, or both. Here we report broadband X-ray observations of the nuclear region of the galaxy M82 that reveal pulsations with an average period of 1.37 seconds and a 2.5-day sinusoidal modulation. The pulsations result from the rotation of a magnetized neutron star, and the modulation arises from its binary orbit. The pulsed flux alone corresponds to an X-ray luminosity in the 3-30 kiloelectronvolt range of 4.9 × 10(39) ergs per second. The pulsating source is spatially coincident with a variable source that can reach an X-ray luminosity in the 0.3-10 kiloelectronvolt range of 1.8 × 10(40) ergs per second. This association implies a luminosity of about 100 times the Eddington limit for a 1.4-solar-mass object, or more than ten times brighter than any known accreting pulsar. This implies that neutron stars may not be rare in the ultraluminous X-ray population, and it challenges physical models for the accretion of matter onto magnetized compact objects.

Asymmetries in core-collapse supernovae from maps of radioactive 44Ti in Cassiopeia A.

Asymmetry is required by most numerical simulations of stellar core-collapse explosions, but the form it takes differs significantly among models. The spatial distribution of radioactive (44)Ti, synthesized in an exploding star near the boundary between material falling back onto the collapsing core and that ejected into the surrounding medium, directly probes the explosion asymmetries. Cassiopeia A is a young, nearby, core-collapse remnant from which (44)Ti emission has previously been detected but not imaged. Asymmetries in the explosion have been indirectly inferred from a high ratio of observed (44)Ti emission to estimated (56)Ni emission, from optical light echoes, and from jet-like features seen in the X-ray and optical ejecta. Here we report spatial maps and spectral properties of the (44)Ti in Cassiopeia A. This may explain the unexpected lack of correlation between the (44)Ti and iron X-ray emission, the latter being visible only in shock-heated material. The observed spatial distribution rules out symmetric explosions even with a high level of convective mixing, as well as highly asymmetric bipolar explosions resulting from a fast-rotating progenitor. Instead, these observations provide strong evidence for the development of low-mode convective instabilities in core-collapse supernovae.

A rapidly spinning supermassive black hole at the centre of NGC 1365.

Broad X-ray emission lines from neutral and partially ionized iron observed in active galaxies have been interpreted as fluorescence produced by the reflection of hard X-rays off the inner edge of an accretion disk. In this model, line broadening and distortion result from rapid rotation and relativistic effects near the black hole, the line shape being sensitive to its spin. Alternative models in which the distortions result from absorption by intervening structures provide an equally good description of the data, and there has been no general agreement on which is correct. Recent claims that the black hole (2 × 10(6) solar masses) at the centre of the galaxy NGC 1365 is rotating at close to its maximum possible speed rest on the assumption of relativistic reflection. Here we report X-ray observations of NGC 1365 that reveal the relativistic disk features through broadened Fe-line emission and an associated Compton scattering excess of 10-30 kiloelectronvolts. Using temporal and spectral analyses, we disentangle continuum changes due to time-variable absorption from reflection, which we find arises from a region within 2.5 gravitational radii of the rapidly spinning black hole. Absorption-dominated models that do not include relativistic disk reflection can be ruled out both statistically and on physical grounds.

Cigarette smoke induces demethylation of prometastatic oncogene synuclein-gamma in lung cancer cells by downregulation of DNMT3B.

The prometastatic oncogene synuclein-gamma (SNCG) is not expressed in normal lung tissues, but it is highly expressed in lung tumors. Here, we show that cigarette smoke extract (CSE) has strong inducing effects on SNCG gene expression in A549 lung cancer cells through demethylation of SNCG CpG island. CSE treatment also augments the invasive capacity of A549 cells in an SNCG-dependent manner. To elucidate the mechanisms underlying the demethylating effects of CSE, we examined expression levels of DNA methyltransferases (DNMTs), 1, 3A and 3B in CSE-treated cells. We show that the mRNA expression of DNMT3B is specifically downregulated by CSE with a kinetics concurrent to SNCG reexpression. Utilizing siRNA to knockdown DNMT3B expression, we show that inhibition of DNMT3B directly increases SNCG mRNA expression. We further show that exogenous overexpression of DNMT3B in an SNCG-positive lung cancer cell line H292 suppresses SNCG mRNA and protein expression and induces de novo methylation of SNCG CpG island, whereas overexpression of DNMT1 or DNMT3A has no effects. Taken together, these new findings demonstrate that tobacco exposure induces the abnormal expression of SNCG in lung cancer cells through downregulation of DNMT3B. This work sheds light on the molecular understanding of demethylation of this oncogene during cancer progression.

An exceptionally bright flare from SGR 1806-20 and the origins of short-duration gamma-ray bursts.

Soft-gamma-ray repeaters (SGRs) are galactic X-ray stars that emit numerous short-duration (about 0.1 s) bursts of hard X-rays during sporadic active periods. They are thought to be magnetars: strongly magnetized neutron stars with emissions powered by the dissipation of magnetic energy. Here we report the detection of a long (380 s) giant flare from SGR 1806-20, which was much more luminous than any previous transient event observed in our Galaxy. (In the first 0.2 s, the flare released as much energy as the Sun radiates in a quarter of a million years.) Its power can be explained by a catastrophic instability involving global crust failure and magnetic reconnection on a magnetar, with possible large-scale untwisting of magnetic field lines outside the star. From a great distance this event would appear to be a short-duration, hard-spectrum cosmic gamma-ray burst. At least a significant fraction of the mysterious short-duration gamma-ray bursts may therefore come from extragalactic magnetars.

Revisiting the accuracy hypothesis in families of young children with conduct problems.

Revisited the accuracy hypothesis in an examination of the relation between maternal depressive symptomatology and child conduct problems. All data were gathered as part of the pretreatment assessment in an outcome study of families with clinic-referred children with conduct problems (age 3 to 6). The mothers varied in their depressive symptomatology, from not at all symptomatic to severely symptomatic. Correlations indicated that with increasing depressive symptomatology, mothers (N = 97) displayed a higher rate of physical negative behaviors towards their child and reported more child conduct problems. Regression analyses revealed that at the lowest levels of maternal depressive symptomatology there was a discrepancy between mothers' reports of child behavior problems and child deviant behaviors observed during mother-child interaction. In contrast, at higher levels of depression, mothers' reports of child behavior were consistent with laboratory observations of their child's behavior. These findings provide evidence to support the accuracy hypothesis in reference to mothers who display a high degree of depressive symptomatology, but the results also call into question the validity of maternal report in families with children with conduct problems.

Analysis of genetic and epigenetic mechanisms of toxicity: potential roles of toxicogenomics and proteomics in toxicology.

The article highlighted in this issue is "An Aryl Hydrocarbon Receptor Independent Mechanism of JP-8 Jet Fuel Immunotoxicity in Ah-Responsive and Ah-Nonresponsive Mice" by Andrew C. Dudley, Margie M. Peden-Adams, Jackie EuDaly, Richard S. Pollenz, and Deborah E. Keil (pp. 251-259).

The effect of DFMO induced uptake of [3H] putrescine on human glioma cells.

Polyamine synthesis inhibitors, such as a-difluoromethylornithine (DFMO), inhibit tumor cell growth in vitro and in vivo. However, upon cessation of treatment, tumor growth resumes. We hypothesized that incorporation of radioactive polyamines might kill the growth-arrested cells. This hypothesis was previously tested in rat 9L brain tumor cells in which DFMO increased both the uptake and the retention of [3H] putrescine. In these rat cells, DFMO-induced retention of high-specific-activity [3H] putrescine for 20 days resulted in several logs killing. In the present studies all of the 5 different human glioma cell lines tested with DFMO treatment also showed enhanced uptake of exogenous [3H] putrescine, reduced cell counts and enhanced killing of colony forming cells (CSF). Extending the time of DFMO treatment of cells that had taken up high-specific-activity (80 Ci/mmol) [3H] putrescine further increased the killing. A 10-day extension resulted in a 10,000-fold reduction in cumulative cell growth. A 5-day extension resulted in a 2-3 log decrease in numbers of surviving CFC. These data further support the hypothesis and suggest that DFMO-induced cell cycle arrest enhances cellular retention of [3H] putrescine, increasing the effective internal radiation dose enough to cause proliferative death. In a clinical setting, the short (approximately 1 microm) path-length of the tritium beta particle should limit effects to the tumor cells and spare adjacent normal cells. These results support the concept that treatment with the combination of polyamine inhibitors and radioactive polyamines might be a useful adjunct to current therapies for glioblastoma multiforme.

Formation and reactions of the heme-dioxygen intermediate in the first and second steps of nitric oxide synthesis as studied by stopped-flow spectroscopy under single-turnover conditions.

To better understand the mechanism of nitric oxide (NO) synthesis, we studied conversion of N-hydroxy-L-arginine (NOHA) or L-arginine (Arg) to citrulline and NO under single-turnover conditions using the oxygenase domain of neuronal nitric oxide synthase (nNOSoxy) and rapid scanning stopped-flow spectroscopy. When anaerobic nNOSoxy saturated with H(4)B and NOHA was provided with 0.5 or 1 electron per heme and then exposed to air at 25 degrees C, it formed 0.5 or 1 mol of citrulline/mol of heme, respectively, indicating that NOHA conversion had 1:1 stoichiometry with respect to electrons added. Identical experiments with Arg produced substoichiometric amounts of NOHA or citrulline even when up to 3 electrons were provided per heme. Transient spectral intermediates were investigated at 10 degrees C. For NOHA, four species were observed in the following sequence: starting ferrous nNOSoxy, a transient ferrous-dioxygen complex, a transient ferric-NO complex, and ferric nNOSoxy. For Arg, transient intermediates other than the ferrous-dioxygen species were not apparent during the reaction. Our results provide a kinetic framework for formation and reactions of the ferrous-dioxygen complex in each step of NO synthesis and establish that (1) the ferrous-dioxy enzyme reacts quantitatively with NOHA but not with Arg and (2) its reaction with NOHA forms 1 NO/heme, which immediately binds to form a ferric heme-NO complex.

Enhanced uptake of [3H] spermidine by 9L rat brain tumors after direct intratumoral infusion of inhibitors of enzymes of the polyamine biosynthetic pathway.

We have been exploring the feasibility of delivering ionizing radiation to brain tumor cells by using tritium labeled polyamines. Polyamines are taken up preferentially by dividing cells and form noncovalent bonds with DNA. Their uptake can be enhanced by drugs which deplete endogenous polyamines. To test this in vivo, 9L cells were implanted in the striatal region of the brain in male Fisher 344 rats. Osmotic pumps containing trace amounts of [3H] spermidine or [3H] putrescine with either difluoromethylornithine or combinations of 3 inhibitors of enzymes of the polyamine biosynthetic pathway were implanted subcutaneously and were connected to intratumoral cannulas. After 14-16 days the brains were removed and sliced in the coronal plane. The diameters of the tumors were measured and tumor tissue was dissected from each slice, weighed and lysed for scintillation counting. It was found that difluoromethylornithine enhanced the uptake of [3H] putrescine while a combination of inhibitors of enzymes of the polyamine biosynthetic pathway enhanced the uptake of [3H] putrescine and [3H] spermidine producing a localized region of radioactivity in the 9L tumor. It is estimated that if the [3H] polyamines were at higher specific activity (commercially available), instead of the trace dose given here, the [3H] polyamine uptake would be sufficient to kill 9L tumor cells within a 2 to 3 week period.

Characterization of the stage in natural killer cell development in 14.5-day mouse fetal liver using adult bone marrow stroma.

Nonstimulated fetal liver (FL) from 14.5-day gestation mice had no natural killer (NK) cell activity and <3% expressed NK1.1. Even after short-term (3-4 day) culture of FL with the late-acting cytokines, interleukin (IL)-15 or IL-2, little or no NK activity was detected. However, longer-term (13 day) culture with IL-2 plus stroma derived from bone marrow (BM) of adult mice, resulted in extensive proliferation and differentiation to mature NK cells. Cell numbers began to increase after 4 days, and by day 13, they had increased 40-fold and 69% of the cells were NK1.1+ with high NK activity and 5%-10% were NK1.1- B220+. With stroma, but no IL-2, equivalent proliferation occurred, but differentiated cells were predominantly NK1.1- B220+, not NK cells. Culture for 13 days without stroma, but with either IL-2, IL-15, FLTK3-ligand (L) or stroma-conditioned medium, resulted in less than fivefold expansion, and minimal NK activity. Culture with combinations of FLTK3-L or ckit-L plus IL-15 or IL-2 increased both cell number and NK activity, but the increase in cell number was less than that seen with stroma plus IL-2. By limiting dilution assay on stroma plus IL-2, the precursor frequency was 1/(2660+/-292) whole FL cells and the absolute number, but not the frequency, increased during culture on stroma without IL-2. The NK cell progenitors were found in sorted NK1.1- and Sca-1+ c-kit+ lineage- subpopulations at a frequency of 1/(156+/-52.5). Together, these data suggest that the NK lineage cells in FL are primarily in early stages of development. They are highly proliferative, respond to early acting cytokines and express stem cell markers.

Bone marrow as a potential source of hepatic oval cells.

Bone marrow stem cells develop into hematopoietic and mesenchymal lineages but have not been known to participate in production of hepatocytes, biliary cells, or oval cells during liver regeneration. Cross-sex or cross-strain bone marrow and whole liver transplantation were used to trace the origin of the repopulating liver cells. Transplanted rats were treated with 2-acetylaminofluorene, to block hepatocyte proliferation, and then hepatic injury, to induce oval cell proliferation. Markers for Y chromosome, dipeptidyl peptidase IV enzyme, and L21-6 antigen were used to identify liver cells of bone marrow origin. From these cells, a proportion of the regenerated hepatic cells were shown to be donor-derived. Thus, a stem cell associated with the bone marrow has epithelial cell lineage capability.

Expression of murine CD34 by fetal liver NK cell progenitors.

Although 14.5-day murine fetal liver (FL) has few, if any, mature natural killer (NK) cells, culture of FL with recombinant human IL-2 (rhIL-2) and stroma from irradiated NK longterm bone marrow cultures (NK-LTBMC) allows proliferation and differentiation of NK cell progenitors. Using this system, NK cell progenitors were found in both CD34+ and CD34- sorted subpopulations of FL. The CD34 antigen was expressed by 14+/-1.3% of whole FL cells, while mature NK cells cultured from NK cell precursors in FL did not express the CD34 antigen. Anti-TER-119 mAb reacted with 84%+/-10.3% of the FL cells, and NK cell progenitors were enriched in the TER-119- subpopulation. After coculture with rhIL-2 and stroma, neither TER-119- nor TER-119+ cells expressed antigens associated with T cells (CD3, CD4, and CD8) or myeloid cells (Gr-1 and Mac-1). Only the TER-119 subpopulation generated NK1.1+ (77%) and B220+ (87%) cells. Within the TER-119 subpopulation, both CD34+ and CD34- cells generated cytolytic and NK1.1+ cells after culture. By a limiting dilution assay (LDA) of the Lin (i.e., negative for NK1.1, CD3, CD4, CD8, B220, Gr-1, and TER-119) CD34 positive or negative subpopulations, the calculated mean frequency of NK cell progenitors was about 1/100 for the CD34+Lin- subpopulation and about 1/(200-300) for the CD34-Lin- subpopulation. In kinetic studies, we found that NK1.1 antigen expression continued to increase with time in culture for both the CD34+Lin- and CD34-Lin- fractions. In contrast, the percentage of CD34+ cells decreased rapidly and produced CD34- cells, and the CD34- population remained CD34-. These data suggest that both CD34+ and CD34- subpopulations of FL can differentiate into NK cells when cocultured for 13 days with irradiated NK-LTBMC stroma and rhIL-2, and that CD34+ progenitors differentiate to CD34- precursors, which in turn differentiate to CD34- mature NK cells.