620 research outputs found

    Optical and near infrared photometry of Butcher-Oemler clusters

    Get PDF
    Rich clusters of galaxies at moderate redshifts (z approx. .3) have a larger proportion of optically blue galaxies than their low redshift counterparts. Spectroscopic examination of the blue galaxies by various authors has shown that the blue galaxies are generally Seyferts, show evidence for recent star formation, or are foreground objects. Unfortunately, spectroscopy is too time consuming to be used on large samples. Thus, we have looked for a way to separate Seyferts, starbursts, ellipticals and nonmembers using photometry alone. Five moderate redshift clusters, Abell numbers 777, 963, 1758, 1961 and 2218, have been observed in the V, R and K bands. We model the spectral energy distributions of various kinds of galaxies found in clusters and derive observed colors. We have modeled the spectral energy distributions (SED) of several kinds of galaxies and compute their colors as a function of redshift. We expect to see ellipticals, spirals, starbursts, post-starburst and Seyfert galaxies. The SED of elliptical and Sbc galaxies was observed by Rieke and Rieke. The SEDs for the starburst galaxies was created by adding a reddened 10(exp 8) year old burst to a spiral galaxy SED. The post-starburst (E+A) galaxy SEDs are composed of a slightly reddened 10(exp 9) year old burst and elliptical galaxy SED. SEDs for the Seyferts were created by adding a v(exp -1.1) power law, and a hot dust thermal spectrum to the Sbc. From the SEDs the colors of galaxies at various redshifts with assorted filters were computed. Lilly & Gunn (1985) have optical and infrared photometry for a sample of galaxies in CL0024+1654 observed spectroscopically by Dressler, Gunn and Schneider (1985). We have used this data to choose the most appropriate SEDs for our starburst and post-starburst models. The most likely explanation for the optically blue colors in most cluster galaxies is star formation. Very few galaxies lie in the Seyfert locus. Abel 1758 has more Seyfert candidates than the other clusters, we observed. It seems possible to roughly sort types of galaxies in clusters by color alone. The cluster population seems to vary considerably between clusters, but our K selected sample has few Seyferts in any cluster

    A multistage linear array assignment problem

    Get PDF
    The implementation of certain algorithms on parallel processing computing architectures can involve partitioning contiguous elements into a fixed number of groups, each of which is to be handled by a single processor. It is desired to find an assignment of elements to processors that minimizes the sum of the maximum workloads experienced at each stage. This problem can be viewed as a multi-objective network optimization problem. Polynomially-bounded algorithms are developed for the case of two stages, whereas the associated decision problem (for an arbitrary number of stages) is shown to be NP-complete. Heuristic procedures are therefore proposed and analyzed for the general problem. Computational experience with one of the exact problems, incorporating certain pruning rules, is presented with one of the exact problems. Empirical results also demonstrate that one of the heuristic procedures is especially effective in practice

    Characterization and synthesis of mono- and diphytanyl ethers of glycerol.

    Get PDF
    The methanolyzed lipids of the extreme halo- phile, Halobacterium cutirubrum, were separated into glycerol diether and glycerol monoether fractions. The diether was shown by synthesis to be 2,3-di-O-(3'R,7'R,ll 'R,15'-tetra- methylhexadecy1)-sn-glycerol. The monoether fraction was separated by thin-layer chromatography on boric acid-im- pregnated silicic acid into about equal amounts of a- and j3- isomers. The a-isomer was found to be identical with the synthetic 3-0-(3'R,7 'R,ll 'R,15 '-tetramethylhexadecy1)-sn- glycerol, and the j3-isomer was identical with the synthetic 2-0-(3 'R,7 'R,11 'R,15 '-tetramethylhexadecyl) glycerol

    Nonprofits and the Promotion of Civic Engagement: A Conceptual Framework for Understanding the “Civic Footprint” of Nonprofits within Local Communities

    Get PDF
    The literature suggests that nonprofit organizations provide civic benefits by promoting engagement within local communities. However, there exists minimal empirical evidence describing the ways in which nonprofits actually undertake this role. In order to address this omission, we conducted interviews with personnel of nonprofit organizations in one rural community in the United States. Our preliminary findings indicate that nonprofit organizations promote civic engagement through programs and activities that: 1) engage volunteers and donors; 2) bring community members together; 3) collaborate with organizations within and beyond the community; and 4) promote community education and awareness. Together, these findings help to develop a working model to understand the civic footprint of nonprofit organizations with methodological implications for future research that would seek to measure the extent to which nonprofits promote civic engagement

    Aligning Perspectives of Subjective Well-Being: Comparing Spouse and Colleague Perceptions of Social Worker Happiness

    Get PDF
    Social workers experience higher rates of burnout and attrition when compared to other health related occupational groups. Previous research on the well being of social workers has tended to focus on the social workers themselves. But the development of well-being is dynamic and is fostered through relationships and interactions with others. In the case of social workers, these relationships include workplace, professional, and personal life interactions. This research sought to better understand the level of congruence between a social worker’s perspective of well-being and perspectives held by significant people in their workplace and at home. Utilizing qualitative methods we interviewed colleagues and spouses (n=10) of social workers that were found to have high levels of work-related subjective well-being. The findings support previous conclusions on the positive subjective well-being (SWB) of practicing social workers, but also indicate a lack of a deeper understanding of the nuances that contribute to social worker SWB. These findings are particularly useful for social workers trying to enhance their SWB, and have direct applicability in education and professional development settings that seek to enhance social worker self-care

    Differentiable Modelling of Percussive Audio with Transient and Spectral Synthesis

    Get PDF
    Differentiable digital signal processing (DDSP) techniques, including methods for audio synthesis, have gained attention in recent years and lend themselves to interpretability in the parameter space. However, current differentiable synthesis methods have not explicitly sought to model the transient portion of signals, which is important for percussive sounds. In this work, we present a unified synthesis framework aiming to address transient generation and percussive synthesis within a DDSP framework. To this end, we propose a model for percussive synthesis that builds on sinusoidal modeling synthesis and incorporates a modulated temporal convolutional network for transient generation. We use a modified sinusoidal peak picking algorithm to generate time-varying non-harmonic sinusoids and pair it with differentiable noise and transient encoders that are jointly trained to reconstruct drumset sounds. We compute a set of reconstruction metrics using a large dataset of acoustic and electronic percussion samples that show that our method leads to improved onset signal reconstruction for membranophone percussion instruments

    Effect of Increased Nitrogen Application Rates and Environment on Protein, Oil, Fatty Acids, and Minerals in Sesame (Sesamum indicum) Seed Grown under Mississippi Delta Conditions

    Get PDF
    Information on the effect of nitrogen fertilizer rates and environment on sesame seed composition and nutrition is scarce. The objective of this research was to investigate the effects of nitrogen fertilizer application rates on sesame seed yield, protein, oil, fatty acids, and mineral nutrition. A two-year (2014, 2015) field experiment was conducted. Nitrogen fertilizer (urea ammonium nitrate) solution (UAN, 32% N) was applied by side dressing to four sesame varieties (S-34, S-35, S-38, S-39) at rates of 44.7, 67.2, 89.6 and 112.0 kg\ub7ha-1. Rate of 44.7 kg\ub7ha-1 was used as control since this rate is traditionally recommended in the region. Increasing nitrogen application rates resulted in higher protein and oleic acid contents in two varieties in 2014, and in all varieties in 2015. Increased protein and oleic acid were accompanied by lower total oil and linoleic acid. Increased nitrogen application also resulted in higher seed N, S, B, Cu, Fe, and Zn in 2014 in S-34 and S-35, but either a decline or no clear change was observed in seed levels of these nutrients in S-38 and S-39. In 2015, increased nitrogen application resulted in significantly higher seed N in all varieties, and higher S, B, Cu, Fe, and Zn in some varieties. A significant positive correlation was observed between nitrogen application rate and yield, and with seed levels of protein, oleic, acid, N, B, Cu, Fe, and Zn. A significant negative correlation was observed between nitrogen application rate and seed oil and linoleic acid. Thus, increased nitrogen fertilizer application resulted in higher seed protein, oleic acid, and some mineral nutrients, but lower oil and linoleic acid. However, this effect depended on variety and environmental conditions. Because higher protein and oleic acid are desirable traits for sesame seed nutritional value and oil stability, regional breeders should select sesame varieties for efficient fertilizer response

    Dust and gas in luminous infrared galaxies - results from SCUBA observations

    Full text link
    We present new data taken at 850 μ\mum with SCUBA at the JCMT for a sample of 19 luminous infrared galaxies. Fourteen galaxies were detected. We have used these data, together with fluxes at 25, 60 and 100 μ\mum from IRAS, to model the dust emission. We find that the emission from most galaxies can be described by an optically thin, single temperature dust model with an exponent of the dust extinction coefficient (kλλβk_\lambda \propto \lambda^{-\beta}) of β1.52\beta \simeq 1.5 - 2. A lower β1\beta\simeq 1 is required to model the dust emission from two of the galaxies, Arp 220 and NGC 4418. We discuss various possibilities for this difference and conclude that the most likely is a high dust opacity. In addition, we compare the molecular gas mass derived from the dust emission, MdustM_{dust}, with the molecular gas mass derived from the CO emission, MCOM_{CO}, and find that MCOM_{CO} is on average a factor 3 higher than MdustM_{dust}.Comment: 10 pages, 6 figures, latex, with MN-macros, accepted by MNRAS - revised version (changed flux values for some galaxies

    A Chromosome-Length Reference Genome for the Endangered Pacific Pocket Mouse Reveals Recent Inbreeding in a Historically Large Population

    Get PDF
    High-quality reference genomes are fundamental tools for understanding population history, and can provide estimates of genetic and demographic parameters relevant to the conservation of biodiversity. The federally endangered Pacific pocket mouse (PPM), which persists in three small, isolated populations in southern California, is a promising model for studying how demographic history shapes genetic diversity, and how diversity in turn may influence extinction risk. To facilitate these studies in PPM, we combined PacBio HiFi long reads with Omni-C and Hi-C data to generate a de novo genome assembly, and annotated the genome using RNAseq. The assembly comprised 28 chromosome-length scaffolds (N50 = 72.6 MB) and the complete mitochondrial genome, and included a long heterochromatic region on chromosome 18 not represented in the previously available short-read assembly. Heterozygosity was highly variable across the genome of the reference individual, with 18% of windows falling in runs of homozygosity (ROH) >1 MB, and nearly 9% in tracts spanning >5 MB. Yet outside of ROH, heterozygosity was relatively high (0.0027), and historical Ne estimates were large. These patterns of genetic variation suggest recent inbreeding in a formerly large population. Currently the most contiguous assembly for a heteromyid rodent, this reference genome provides insight into the past and recent demographic history of the population, and will be a critical tool for management and future studies of outbreeding depression, inbreeding depression, and genetic load
    corecore