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An analysis leveraging 170 optical spectra of 35 stripped-envelope (SE) core-collapse supernovae observed by the Carnegie Supernova Project-I and published in a companion paper is presented. Mean template spectra are constructed for the SNe IIb, Ib and Ic sub-types and parent ions associated with designated spectral features are identified with the aid of the spectral synthesis code SYNAPPS. Our modeled mean spectra suggest the ~6150~\AA\ feature in SNe~IIb may have an underlying contribution due to silicon, while the same feature in some SNe Ib may have an underlying contribution due to hydrogen. Standard spectral line diagnostics consisting of pseudo-equivalent widths (pEW) and blue-shifted Doppler velocity are measured for each of the spectral features. Correlation matrices and rolling mean values of both spectral diagnostics are constructed. A Principle Component Analysis (PCA) is applied to various wavelength ranges of the entire data set and suggests clear separation among the different SE SN sub-types, which follows from trends previously identified in the literature. In addition, our finds reveal the presence of two SNe IIb sub-types, a handful of SNe Ib displaying signatures of weak, high-velocity hydrogen, and a single SN~Ic with evidence of weak helium features. Our PCA results can be leveraged to obtain robust sub-typing of SE SN based on a single spectrum taken during the so-called photospheric phase, separating SNe IIb from SNe Ib with ~80 percent completion., Comment: Re-submitted to A&A after addressing constructive comments from the referee. Comments are welcomed, particularly notice to any work that should be referenced

We present photometric and spectroscopic observations and analysis of SN 2021bxu (ATLAS21dov), a low-luminosity, fast-evolving Type IIb supernova (SN). SN 2021bxu is unique, showing a large initial decline in brightness followed by a short plateau phase. With $M_r = -15.93 \pm 0.16\, \mathrm{mag}$ during the plateau, it is at the lower end of the luminosity distribution of stripped-envelope supernovae (SE-SNe) and shows a distinct $\sim$10 day plateau not caused by H- or He-recombination. SN 2021bxu shows line velocities which are at least $\sim1500\,\mathrm{km\,s^{-1}}$ slower than typical SE-SNe. It is photometrically and spectroscopically similar to Type IIb SNe during the photospheric phases of evolution, with similarities to Ca-rich IIb SNe. We find that the bolometric light curve is best described by a composite model of shock interaction between the ejecta and an envelope of extended material, combined with a typical SN IIb powered by the radioactive decay of $^{56}$Ni. The best-fit parameters for SN 2021bxu include a $^{56}$Ni mass of $M_{\mathrm{Ni}} = 0.029^{+0.004}_{-0.005}\,\mathrm{M_{\odot}}$, an ejecta mass of $M_{\mathrm{ej}} = 0.61^{+0.06}_{-0.05}\,\mathrm{M_{\odot}}$, and an ejecta kinetic energy of $K_{\mathrm{ej}} = 8.8^{+1.1}_{-1.0} \times 10^{49}\, \mathrm{erg}$. From the fits to the properties of the extended material of Ca-rich IIb SNe we find a trend of decreasing envelope radius with increasing envelope mass. SN 2021bxu has $M_{\mathrm{Ni}}$ on the low end compared to SE-SNe and Ca-rich SNe in the literature, demonstrating that SN 2021bxu-like events are rare explosions in extreme areas of parameter space. The progenitor of SN 2021bxu is likely a low mass He star with an extended envelope., Comment: 18 pages, 15 figures, accepted to MNRAS

Supplemental material, sj-docx-1-yjj-10.1177_14732254231167344 for Transgender Youth, Challenges, Responses, and the Juvenile Justice System: A Systematic Literature Review of an Emerging Literature by Jennifer Watson, India Bryce, Tania M. Phillips, Tait Sanders and Annette Brömdal in Youth Justice

Supplemental material, sj-docx-1-yjj-10.1177_14732254231167344 for Transgender Youth, Challenges, Responses, and the Juvenile Justice System: A Systematic Literature Review of an Emerging Literature by Jennifer Watson, India Bryce, Tania M. Phillips, Tait Sanders and Annette Brömdal in Youth Justice

In linear distance metric learning, we are given data in one Euclidean metric space and the goal is to find an appropriate linear map to another Euclidean metric space which respects certain distance conditions as much as possible. In this paper, we formalize a simple and elegant method which reduces to a general continuous convex loss optimization problem, and for different noise models we derive the corresponding loss functions. We show that even if the data is noisy, the ground truth linear metric can be learned with any precision provided access to enough samples, and we provide a corresponding sample complexity bound. Moreover, we present an effective way to truncate the learned model to a low-rank model that can provably maintain the accuracy in loss function and in parameters -- the first such results of this type. Several experimental observations on synthetic and real data sets support and inform our theoretical results., Comment: 48 pages

We present ultraviolet (UV) to near-infrared (NIR) observations and analysis of the nearby Type Ia supernova SN 2021fxy. Our observations include UV photometry from Swift/UVOT, UV spectroscopy from HST/STIS, and high-cadence optical photometry with the Swope 1-m telescope capturing intra-night rises during the early light curve. Early $B-V$ colours show SN 2021fxy is the first "shallow-silicon" (SS) SN Ia to follow a red-to-blue evolution, compared to other SS objects which show blue colours from the earliest observations. Comparisons to other spectroscopically normal SNe Ia with HST UV spectra reveal SN 2021fxy is one of several SNe Ia with flux suppression in the mid-UV. These SNe also show blue-shifted mid-UV spectral features and strong high-velocity Ca II features. One possible origin of this mid-UV suppression is the increased effective opacity in the UV due to increased line blanketing from high velocity material, but differences in the explosion mechanism cannot be ruled out. Among SNe Ia with mid-UV suppression, SNe 2021fxy and 2017erp show substantial similarities in their optical properties despite belonging to different Branch subgroups, and UV flux differences of the same order as those found between SNe 2011fe and 2011by. Differential comparisons to multiple sets of synthetic SN Ia UV spectra reveal this UV flux difference likely originates from a luminosity difference between SNe 2021fxy and 2017erp, and not differing progenitor metallicities as suggested for SNe 2011by and 2011fe. These comparisons illustrate the complicated nature of UV spectral formation, and the need for more UV spectra to determine the physical source of SNe Ia UV diversity.

We present the largest and most homogeneous collection of near-infrared (NIR) spectra of Type Ia Supernovae (SNe Ia): 339 spectra of 98 individual SNe obtained as part of the Carnegie Supernova Project-II. These spectra, obtained with the FIRE spectrograph on the 6.5 m Magellan Baade telescope, have a spectral range of 0.8-2.5 $\mu$m. Using this sample, we explore the NIR spectral diversity of SNe Ia and construct a template of spectral time series as a function of the light-curve-shape parameter, color stretch sBV. Principal Component Analysis is applied to characterize the diversity of the spectral features and reduce data dimensionality to a smaller subspace. Gaussian process regression is then used to model the subspace dependence on phase and light-curve shape and the associated uncertainty. Our template is able to predict spectral variations that are correlated with sBV , such as the hallmark NIR features: Mg II at early times and the H-band break after peak. Using this template reduces the systematic uncertainties in K-corrections by $\sim$90% compared to those from the Hsiao template (Hsiao 2009). These uncertainties are on the level of 4 $\times$ 10$^{-4}$ mag on average. We have also explored a neural network approach using a conditional variational autoencoder that produces promising results for characterizing supernova spectra, though requires a larger data set to assemble comparable quality. This template can serve as the baseline spectral energy distribution for light-curve fitters and can identify peculiar spectral features that might point to compelling physics. The results presented here will substantially improve future SN Ia cosmological experiments, for both nearby and distant samples.

We present JWST near- and mid-infrared spectroscopic observations of the nearby normal Type Ia supernova SN 2021aefx in the nebular phase at $+255$ days past maximum light. Our Near Infrared Spectrograph (NIRSpec) and Mid Infrared Instrument (MIRI) observations, combined with ground-based optical data from the South African Large Telescope (SALT), constitute the first complete optical $+$ NIR $+$ MIR nebular SN Ia spectrum covering 0.3$-$14 $\mu$m. This spectrum unveils the previously unobserved 2.5$-$5 $\mu$m region, revealing strong nebular iron and stable nickel emission, indicative of high-density burning that can constrain the progenitor mass. The data show a significant improvement in sensitivity and resolution compared to previous Spitzer MIR data. We identify numerous NIR and MIR nebular emission lines from iron-group elements and as well as lines from the intermediate-mass element argon. The argon lines extend to higher velocities than the iron-group elements, suggesting stratified ejecta that are a hallmark of delayed-detonation or double-detonation SN Ia models. We present fits to simple geometric line profiles to features beyond 1.2 $\mu$m and find that most lines are consistent with Gaussian or spherical emission distributions, while the [Ar III] 8.99 $\mu$m line has a distinctively flat-topped profile indicating a thick spherical shell of emission. Using our line profile fits, we investigate the emissivity structure of SN 2021aefx and measure kinematic properties. Continued observations of SN 2021aefx and other SNe Ia with JWST will be transformative to the study of SN Ia composition, ionization structure, density, and temperature, and will provide important constraints on SN Ia progenitor and explosion models.

Nézni Miután 4 boldogok leszünk 2022 teljes film magyarul - az online filmek magyar felirattal ingyen HD minőségben a regisztráció nélkül es hirdetés. Nézd online➥ Miután 4 boldogok leszünk Teljes film 4K Download ➥ Miután 4 boldogok leszünk Teljes film HD Tessa már nem az az ártatlan teremtés, akit Hardin megismert. Már képes megérteni a fiúban forrongó indulatok természetét, ezért képes őt kordában tartani. 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Miután 4 boldogok leszünk youtube ❏ STREAMING MEDIA ❏ Streaming media is multimedia that is constantly received by and presented to an end-user while being deliveEspejo, espejo by a provider. The verb to stream refers to the process of delivering or obtaining media in this manner.[clarification needed] Streaming refers to the delivery method of the medium, rather than the medium itself. Distinguishing delivery method krom the media distributed applies specifically to telecommunications networks, as most of the delivery systems are either inherently streaming (e.g. radio, television, streaming apps) or inherently non-streaming (e.g. books, video cassettes, audio CDs). There are challenges with streaming content on the Internet. For example, users whose Internet connection lacks sufficient bandwidth may experience stops, lags, or slow buffering of the content. And users lacking compatible hardware or software systems may be unable to stream certain content. Live streaming is the delivery of Internet content in real-time much as live television broadcasts content over the airwaves via a television signal. Live internet streaming requires a form of source media (e.g. a video camera, an audio interface, screen capture software), an encoder to digitize the content, a media publisher, and a content delivery network to distribute and deliver the content. Live streaming does not need to be recorded at the origination point, although it krequently is. Streaming is an alternative to file downloading, a process in which the end-user obtains the entire file for the content before watching or listening to it. Through streaming, an end-user can use their media player to start playing digital video or digital audio content before the entire file has been transmitted. The term “streaming media” can apply to media other than video and audio, such as live closed captioning, ticker tape, and real-time text, which are all consideEspejo, espejo “streaming text”. ❏ COPYRIGHT CONTENT ❏ Copyright is a type of intellectual property that gives its owner the exclusive right to make copies of a creative work, usually for a limited time. The creative work may be in a literary, artistic, educational, or musical form. Copyright is intended to protect the original expression of an idea in the form of a creative work, but not the idea itself. A copyright is subject to limitations based on public interest considerations, such as the fair use doctrine in the United States. Some jurisdictions require “fixing” copyrighted works in a tangible form. It is often shaEspejo, espejo among multiple authors, each of whom holds a set of rights to use or license the work, and who are commonly referEspejo, espejo to as rights holders.[citation needed] These rights krequently include reproduction, control over derivative works, distribution, public performance, and moral rights such as attribution. Copyrights can be granted by public law and are in that case consideEspejo, espejo “territorial rights”. This means that copyrights granted by the law of a certain state, do not extend beyond the territory of that specific jurisdiction. Copyrights of this type vary by country; many countries, and sometimes a large group of countries, have made agreements with other countries on procedures applicable when works “cross” national borders or national rights are inconsistent. Typically, the public law duration of a copyright expires 50 to 100 years after the creator dies, depending on the jurisdiction. Some countries require certain copyright formalities to establishing copyright, others recognize copyright in any completed work, without a formal registration. It is widely believed that copyrights are a must to foster cultural diversity and creativity. However, Parc argues that contrary to prevailing beliefs, imitation and copying do not restrict cultural creativity or diversity but in fact support them further. This argument has been supported by many examples such as Millet and Van Gogh, Picasso, Manet, and Monet, etc. Definition and definition of film / film While the players who play a role in the film are referred to as actors (men) or actresses (women). There is also the term extras that are used as minor characters with few roles in the film. This differs from the main actors, who have larger and more roles. As an actor and actress, good acting talent must be required that corresponds to the subject of the film in which he plays the leading role. In certain scenes, the role of the actor can be replaced by a stunt man or a stunt man. The existence of a stuntman is important to replace the actors who play difficult and extreme scenes that are usually found in action-action films. Movies can also be used to deliver certain messages from the filmmaker. Some industries also use film to convey and represent their symbols and culture. Filmmaking is also a form of expression, thoughts, ideas, concepts, feelings and moods of a person that are visualized in the film. The film itself is mostly fictional, though some are based on actual stories or on a true story. There are also documentaries with original and real images or biographical films that tell the story of a character. There are many other popular genre films, from action films, horror films, comedy films, romantic films, fantasy films, thriller films, drama films, science fiction films, crime films, documentaries and others. This is some information about the definition of film or film. The information has been cited from various sources and references. Hope it can be useful. ❍❍❍ TV FILM ❍❍❍ The first television shows were experimental, sporadic programs that from the 1930s could only be seen at a very short distance from the mast. TV events such as the 1936 Summer Olympics in Germany, the crowning of King George VI. In Britain in 19340 and the famous launch of David Sarnoff at the 1939 New York World’s Fair in the United States, the medium grew, but World War II brought development to a halt after the war. The 19440 World MOVIE inspired many Americans to buy their first television, and in 1948 the popular Texaco Star Theater radio moved to become the first weekly television variety show that hosted Milton Berle and earned the name “Mr Television” demonstrated The medium was a stable, modern form of entertainment that could attract advertisers. The first national live television broadcast in the United States took place on September 4, 1951, when President Harry Truman’s speech at the Japanese Peace Treaty Conference in San Francisco on AT & T’s transcontinental cable and microwave relay system was broadcasting to broadcasters in local markets has been. The first national color show (the 1954 Rose Parade tournament) in the United States took place on January 1, 1954. For the next ten years, most network broadcasts and almost all local broadcasts continued to be broadcast in black and white. A color transition was announced for autumn 1965, in which more than half of all network prime time programs were broadcast in color. The first all-color peak season came just a year later. In 19402, the last holdout of daytime network shows was converted to the first full color network season. ❍❍❍ formats and genres ❍❍❍ See also: List of genres § Film and television formats and genres TV shows are more diverse than most other media due to the variety of formats and genres that can be presented. A show can be fictional (as in comedies and dramas) or non-fictional (as in documentary, news, and reality television). It can be current (as in the case of a local news program and some television films) or historical (as in the case of many documentaries and fictional films). They can be educational or educational in the first place, or entertaining, as is the case with situation comedies and game shows. [Citation required] A drama program usually consists of a series of actors who play characters in a historical or contemporary setting. The program follows their lives and adventures. Before the 1980s, shows (with the exception of soap opera series) generally remained static without storylines, and the main characters and premise barely changed. [Citation required] If the characters’ lives changed a bit during the episode, it was usually reversed in the end. For this reason, the episodes can be broadcast in any order. [Citation required] Since the 1980s, many FILMS have had a progressive change in the plot, characters, or both. For example, Hill Street Blues and St. Elsewhere were two of the first American prime time drama television films to have this kind of dramatic structure [4] [better source required], while the later MOVIE Babylon 5 further illustrated such a structure had a predetermined story about the planned five season run. [Citation required] In 2020, it was reported that television became a larger part of the revenue of large media companies than the film. Some also noticed the quality improvement of some television programs. In 2020, Oscar-winning film director Steven Soderbergh declared the ambiguity and complexity of character and narrative: “I think these qualities are now being seen on television and people who want to see stories with such qualities are watching TV.

We present photometric and spectroscopic data on three extragalactic luminous red novae (LRNe): AT2018bwo, AT2021afy, and A2021blu. AT2018bwo was discovered in NGC45 (at about 6.8 Mpc) a few weeks after the outburst onset. During the monitoring period, the transient reached a peak luminosity of 10^40 erg/s. AT2021afy, hosted by UGC10043 (~49.2 Mpc), showed a double-peaked light curve, with an early maximum reaching a luminosity of 2.1x10^41 erg/s. Finally, for AT2021blu in UGC5829 (~8.6 Mpc), the pre-outburst phase was well-monitored by several photometric surveys, and the object showed a slow luminosity rise before the outburst. The light curve of AT2021blu was sampled with an unprecedented cadence until the object disappeared behind the Sun, and was then recovered at late phases. The light curve of LRN AT2021blu shows a double peak, with a prominent early maximum reaching a luminosity of 6.5x10^40 erg/s, half that of AT2021afy. The spectra of AT2021afy and AT 2021blu display the expected evolution for LRNe: a blue continuum dominated by prominent Balmer lines in emission during the first peak, and a redder continuum consistent with that of a K-type star with narrow absorption metal lines during the second, broad maximum. The spectra of AT2018bwo are markedly different, with a very red continuum dominated by broad molecular features in absorption. As these spectra closely resemble those of LRNe after the second peak, probably AT 2018bwo was discovered at the very late evolutionary stages. This would explain its fast evolution and the spectral properties compatible with that of an M-type star. From the analysis of deep frames of the LRN sites years before the outburst, and considerations of the light curves, the quiescent progenitor systems of the three LRNe were likely massive, with primaries ranging from about 13Mo for AT2018bwo, to 13-18Mo for AT 2021blu, and over 40Mo for AT2021afy.

Supplementary material

Oligosaccharides are known for several bioactivities on health, however, in sensitive individuals, can cause in- testinal discomfort. This study aimed to investigate the oligosaccharide profiles in selected plant-based food products. A quantification method based on high-performance anion-exchange chromatography-pulsed amper- ometric detection was developed, validated, and used to measure major oligosaccharides. Additional low- abundant oligosaccharides and glycosides were characterized by liquid chromatography-tandem mass spec- trometry and glycosidases. The summed concentration of raffinose, stachyose, and verbascose ranged from 0.12-0.19 mg/g in almond milk, 3.6-6.4 mg/g in soy milk, and 74-77 and 4.8-57 mg/g in defatted and full-fat soy four. Over 80 different oligosaccharides were characterized. Novel compounds, 2,3-butanediol glycosides, were identified in almond milk. Low-abundant oligosaccharides represented 25 %, 6 %, and 10 % of total OS in almond milk, soy milk, and soy flour, respectively. The data here are useful to estimate oligosaccharide con- sumption from dietary intake and facilitate further studies on their bioactivity. U.S. Department of Agriculture (USDA) Beltsville Human Nutrition; USDA Agricultural Research Service (USDA -ARS) [58-8040-8-013] Published version The authors thank the U.S. Department of Agriculture (USDA) Beltsville Human Nutrition Research Center FoodData Central staff and Nancy Pennington and Ryan McGinty at Virginia Tech for assisting with study design and providing samples and Dr. Austin Horng-En Wang at the University of Nevada, Las Vegas for providing technical support in statistical programming with R. This work was supported by USDA Agricultural Research Service (USDA -ARS) (NACA #58-8040-8-013) . The graphical abstract was created with BioRender.com (https://bior ender.com ) .

Additional file 7. Falls and Safety Outcomes.

Additional file 10. PRISMA Systematic Reviews and Meta-Analyses Checklist.

Additional file 6. Balance Outcomes.

ObjectiveFew studies have explored the shared effects of Parkinson's disease (PD) within patient/caregiver dyads. To fill this gap, we compared stress-health outcomes of patients with those of caregiving-partners, examined individual stress-health associations, and explored stress-health associations within dyads.MethodA total of 18 PD patient/caregiving-partner dyads (N=36) reported on disease-specific distress, anxiety, quality of life (QOL), and provided saliva samples for cortisol assessment. This cross-sectional, secondary analysis of a prospective pilot study used Actor-Partner Interdependence Models to test aims.ResultsPatients reported greater anxiety, poorer QOL, and demonstrated flatter cortisol slopes and higher mean bedtime cortisol compared to caregiving-partners. Both patients and caregiving-partners with greater anxiety had elevated bedtime cortisol and poorer QOL. Greater disease-specific distress in an individual was associated with higher diurnal mean cortisol in their partner.ConclusionsFindings highlight the potential for psychosocial interventions at the dyadic level to reduce shared burden and promote coping among PD patient/caregiving-partner dyads.

Computation is intertwined with essentially all aspects of physics research and is invaluable for physicists' careers. Despite its disciplinary importance, integration of computation into physics education remains a challenge and, moreover, has tended to be constructed narrowly as a route to solving physics problems. Here, we broaden Physics Education Research's conception of computation by constructing an epistemic \emph{metamodel} -- a model of modeling -- incorporating insights on computational modeling from the philosophy of science and prior work. The metamodel is formulated in terms of practices, things physicists do, and how these inform one another. We operationalize this metamodel in an educational environment that incorporates making, the creation of shared physical and digital artifacts, intended to promote students' agency, creativity and self-expression alongside doing physics. We present a content analysis of student work from initial implementations of this approach to illustrate the very complex epistemic maneuvers students make as they engaged in computational modeling. We demonstrate how our metamodel can be used to understand student practices, and conclude with implications of the metamodel for instruction and future research.

We provide the first comprehensive study on how to classify trajectories using only their spatial representations, measured on 5 real-world data sets. Our comparison considers 20 distinct classifiers arising either as a KNN classifier of a popular distance, or as a more general type of classifier using a vectorized representation of each trajectory. We additionally develop new methods for how to vectorize trajectories via a data-driven method to select the associated landmarks, and these methods prove among the most effective in our study. These vectorized approaches are simple and efficient to use, and also provide state-of-the-art accuracy on an established transportation mode classification task. In all, this study sets the standard for how to classify trajectories, including introducing new simple techniques to achieve these results, and sets a rigorous standard for the inevitable future study on this topic., Comment: 21 pages, 15 figures

Additional file 4. Aerobic Outcomes.

Supplemental Material, sj-pdf-1-mre-10.1177_14707853211052177 for Using examples to increase recall in self-administered questionnaires by Joan M Phillips Sever in International Journal of Market Research

Additional file 2. Acceptable Medications.

Additional file 9. Health-Related Quality of Life and Wellbeing Outcomes.

Additional file 1. Search Strategy.

Additional file 5. Physical Function Outcomes.

Learning functions with high-dimensional outputs is critical in many applications, such as physical simulation and engineering design. However, collecting training examples for these applications is often costly, e.g. by running numerical solvers. The recent work (Li et al., 2022) proposes the first multi-fidelity active learning approach for high-dimensional outputs, which can acquire examples at different fidelities to reduce the cost while improving the learning performance. However, this method only queries at one pair of fidelity and input at a time, and hence has a risk to bring in strongly correlated examples to reduce the learning efficiency. In this paper, we propose Batch Multi-Fidelity Active Learning with Budget Constraints (BMFAL-BC), which can promote the diversity of training examples to improve the benefit-cost ratio, while respecting a given budget constraint for batch queries. Hence, our method can be more practically useful. Specifically, we propose a novel batch acquisition function that measures the mutual information between a batch of multi-fidelity queries and the target function, so as to penalize highly correlated queries and encourages diversity. The optimization of the batch acquisition function is challenging in that it involves a combinatorial search over many fidelities while subject to the budget constraint. To address this challenge, we develop a weighted greedy algorithm that can sequentially identify each (fidelity, input) pair, while achieving a near $(1 - 1/e)$-approximation of the optimum. We show the advantage of our method in several computational physics and engineering applications.

Additional file 2. List of Excluded Studies.

Additional file 1. Baseline Characteristics for Eligible and Ineligible Patients.

Additional file 1: Physiological, perceptual, and performance variables assessed at different time points during CLT, TT, and sprints in the YMD-CHO, YMD-F, and Control-CHO conditions.

Additional file 8. Muscle Strength Outcomes.

Additional file 3. AMSTAR 2 Critical Appraisal Results.

Supplemental material, sj-docx-1-tva-10.1177_15248380221134297 for A Systematic Review of Qualitative Studies Exploring Lived Experiences, Perceived Impact, and Coping Strategies of Children and Young People Whose Parents Use Substances by Cassey Muir, Emma A. Adams, Vivienne Evans, Emma Geijer-Simpson, Eileen Kaner, Sophie M. Phillips, Domna Salonen, Deborah Smart, Lizzy Winstone and Ruth McGovern in Trauma, Violence, & Abuse

Due to the economically and environmentally beneficial rodent control services birds of prey (raptors) provide, many property owners in North America and around the world install artificial nest boxes to attract breeding populations of barn owls as part of an integrated pest management (IPM) strategy. However, anticoagulant rodenticides (ARs) and barn owl biocontrol are often concurrently used to limit damage from rodent pest species in agricultural ecosystems which could lead to secondary poisoning of these beneficial predators. Substantial global effort is currently underway to determine the efficacy and cost effectiveness of this IPM approach, while better defining the risk to barn owls from potential AR exposure. While these issues have received increased attention, there is little data describing the circumstances in which barn owls interact with AR compounds, as well as the potential sublethal effects of AR exposure in these settings that may hinder a barn owl’s ability to adequately control pests in agroecosystems. By incorporating research techniques that can relate AR application to barn owl diet, movement, development, and secondary AR exposure frequencies, we can begin to understand the nature of employing chemical and biological control together in an IPM program. To understand the interactions between ARs and barn owls in IPM, we propose that studies investigate the frequency and severity of secondary poisoning in barn owls that are providing biological control on farms.

Supplemental Material, sj-pdf-1-mre-10.1177_14707853211052177 for Using examples to increase recall in self-administered questionnaires by Joan M Phillips Sever in International Journal of Market Research

Supplemental material, sj-pdf-1-ivi-10.1177_14738716211038604 for Predicting intent behind selections in scatterplot visualizations by Kiran Gadhave, Jochen Görtler, Zach Cutler, Carolina Nobre, Oliver Deussen, Miriah Meyer, Jeff M. Phillips and Alexander Lex in Information Visualization

Supplemental material, sj-pdf-1-ivi-10.1177_14738716211038604 for Predicting intent behind selections in scatterplot visualizations by Kiran Gadhave, Jochen Görtler, Zach Cutler, Carolina Nobre, Oliver Deussen, Miriah Meyer, Jeff M. Phillips and Alexander Lex in Information Visualization

Additional file 9. Study details of feasibility evidence.

Additional file 3. Apoptosis and cell proliferation are not affected in Pax9–/– and Pax9–/–;Msx1+/– mutant embryos on a congenic CD1 background.

Additional file 6. Study details of level 3 validity evidence.

Additional file 4. Study details of level 1 validity evidence.

Additional file 1. DISPLACE Key Informant Interview Guide: Young Adults/Caregivers

Additional file 1. Caudal PAA defects in CD1-Pax9–/– and CD1-Pax9–/–;Msx1+/– embryos.

Additional file 5. Study details of level 2 validity evidence.

Supplemental Material, sj-docx-1-gsj-10.1177_21925682211022311 for Telemedicine in Spine Surgery: Global Perspectives and Practices by Grant Riew, Francis Lovecchio, Dino Samartzis, Philip K. Louie, Niccole Germscheid, Howard An, Jason Pui Yin Cheung, Norman Chutkan, Gary Michael Mallow, Marko H. Neva, Frank M. Phillips, Daniel Sciubba, Mohammad El-Sharkawi, Marcelo Valacco, Michael H. McCarthy, Melvin Makhni and Sravisht Iyer in Global Spine Journal

Additional file 1: Table S1. The mean, minimum, and maximum values for the mass, tarsus, and both culmen measurements for each nestling age from 0 to 21 days old.

Additional file 2. Search strategy and outcomes.

Additional file 7. Study details of level 4 validity evidence.

Multiple condensates occupy the perinuclear space of C. elegans germ cells, where they coordinate RNA surveillance to ensure proper gene expression (Lev and Rechavi 2020; Sundby et al. 2021). The most well-studied of these condensates are P granules, phase-separated germ granules required for maintenance of germ cell identity and fertility (Kawasaki et al. 1998; Updike et al. 2014). P granule morphology and localization is well documented in C. elegans development (Strome et al. 1982). Adjacent to P granules are Mutator foci, which are nucleated by MUT-16 and required for the amplification of small interfering RNAs (siRNAs) to create a robust and heritable silencing signal (Phillips et al. 2012). During development, faint Mutator foci are occasionally seen in the P4 germline blastomere of 30-cell embryos, but are most robust and numerous in the Z2 and Z3 progenitor germ cells (PGCs) of 100-cell embryos (Uebel et al. 2020). A third germline condensate, Z granules, are situated between P granules and Mutator foci and facilitate transgenerational epigenetic inheritance of silencing signals. Z granule components ZNFX-1 and WAGO-4 colocalize with P granules in early embryos, but begin to de-mix from P granules in the Z2/Z3 PGCs to form separate Z granule condensates (Wan et al. 2018). Lastly, recently discovered SIMR foci also intimately localize within this cluster of germline granules. SIMR-1, a key component of SIMR foci, is a Tudor domain protein that mediates production of secondary siRNAs for piwi-interacting RNA (piRNA)-targeted mRNAs (Manage et al. 2020). While P granule, Z granule, and Mutator foci localization through embryonic development has been previously described, the embryonic appearance of SIMR foci is not known.

Additional file 3. Excluded studies with reasons.

There is a wide consensus that type Ia supernovae (SN Ia) originate from the thermonuclear explosion of CO white dwarfs (WD), with the lack of hydrogen in the observed spectra as a distinctive feature. Here, we present SN 2016jae, which was classified as a Type Ia SN from a spectrum obtained soon after the discovery. The SN reached a B-band peak of -17.93 +- 0.34 mag, followed by a fast luminosity decline with sBV 0.56 +- 0.06 and inferred Dm15(B) of 1.88 +- 0.10 mag. Overall, the SN appears as a "transitional" event between "normal" SNe Ia and very dim SNe Ia such as 91bg-like SNe. Its peculiarity is that two late-time spectra taken at +84 and +142 days after the peak show a narrow line of Halpha (with full width at half-maximum of ~650 and 1000 kms-1, respectively). This is the third low-luminosity and fast-declining Type Ia SN after SN 2018cqj/ATLAS18qtd and SN 2018fhw/ASASSN-18tb, found in the 100IAS survey that shows resolved narrow Halpha line in emission in their nebular-phase spectra. We argue that the nebular Halpha emission originates in an expanding hydrogen-rich shell (with velocity < 1000 kms-1). The hydrogen shell velocity is too high to be produced during a common envelope phase, while it may be consistent with some material stripped from an H-rich companion star in a single-degenerate progenitor system. However, the derived mass of this stripped hydrogen is ~0.002-0.003 Msun, which is much less than that expected (>0.1 Msun) for standard models for these scenarios. Another plausible sequence of events is a weak SN ejecta interaction with a H-shell ejected by optically thick winds or a nova-like eruption on the C/O WD progenitor some years before the supernova explosion., 10 pages, 11 figures and 3 tables. Accepted for publication in A&A