7,507 research outputs found

    The Deep Diffuse Extragalactic Radio Sky at 1.75 GHz

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    We present a study of diffuse extragalactic radio emission at 1.751.75\,GHz from part of the ELAIS-S1 field using the Australia Telescope Compact Array. The resulting mosaic is 2.462.46\,deg2^2, with a roughly constant noise region of 0.610.61\,deg2^2 used for analysis. The image has a beam size of 150×60150 \times60\,arcsec and instrumental σn=(52±5)μ\langle\sigma_{\rm n}\rangle= (52\pm5)\, \muJy beam1^{-1}. Using point-source models from the ATLAS survey, we subtract the discrete emission in this field for S150μS \ge 150\, \muJy beam1^{-1}. Comparison of the source-subtracted probability distribution, or \pd, with the predicted distribution from unsubtracted discrete emission and noise, yields an excess of (76±23)μ(76 \pm 23) \, \muJy beam1^{-1}. Taking this as an upper limit on any extended emission we constrain several models of extended source counts, assuming Ωsource2\Omega_{\rm source} \le 2\,arcmin. The best-fitting models yield temperatures of the radio background from extended emission of Tb=(10±7)T_{\rm b}=(10\pm7) \,mK, giving an upper limit on the total temperature at 1.751.75\,GHz of (73±10)(73\pm10)\,mK. Further modelling shows that our data are inconsistent with the reported excess temperature of ARCADE2 to a source-count limit of 1μ1\, \muJy. Our new data close a loop-hole in the previous constraints, because of the possibility of extended emission being resolved out at higher resolution. Additionally, we look at a model of cluster halo emission and two WIMP dark matter annihilation source-count models, and discuss general constraints on any predicted counts from such sources. Finally, we report the derived integral count at 1.41.4\,GHz using the deepest discrete count plus our new extended-emission limits, providing numbers that can be used for planning future ultra-deep surveys.Comment: 18 pages, 15 figures, 7 tables, Accepted by MNRA

    A welcome to the “Creativity in Work-Applied Management” special issue, Journal of Work-Applied Management. ISSN 2205-2062

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    Welcome to the “Creativity in Work-Applied Management” special issue of the Journal of Work Applied Management. When we created the call for papers, we characterised creativity as both a process and an outcome within business and as essential for societal and economic growth (Shalley, 2013; Wall et al., 2017a). We thought such characterisation was likely to remain appropriate as technological development, globalisation and urbanisation trigger significant change in everyday life and employment, making it essential to recognise the skills and capabilities needed for continued participation and influence in the workplace, and that these will include “originality abilities” (Bakhshi et al., 2017). We also thought creativity could be considered through the use of creative problem-solving (Osborn, 1953), organisational aesthetics (Taylor and Hansen, 2005; Wall et al., 2017b), flow (Csikszentmihalyi, 1997), future skills (Ehlers and Kellermann, 2019) or development of the workforce through learning (Helyer, 2015). [...

    Automated clinical system for chromosome analysis

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    An automatic chromosome analysis system is provided wherein a suitably prepared slide with chromosome spreads thereon is placed on the stage of an automated microscope. The automated microscope stage is computer operated to move the slide to enable detection of chromosome spreads on the slide. The X and Y location of each chromosome spread that is detected is stored. The computer measures the chromosomes in a spread, classifies them by group or by type and also prepares a digital karyotype image. The computer system can also prepare a patient report summarizing the result of the analysis and listing suspected abnormalities

    Molecular gas temperature and density in spiral galaxies

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    We combine beam-matched CO-13, CO-12 J = 3 yields 2 and J = 2 yields 1 line data to infer the molecular gas excitation conditions in the central 500 to 1600 pc diameters of a small sample of infrared-bright external galaxies: NGC253, IC342, M 83, Maffei 2, and NGC6946. Additional observations of the J = 1 yields 0 lines of C-18O and CO-13 set limits on the opacity of the CO-13 J = 1 yields 0 line averaged over the central kiloparsec of these spiral galaxies

    A framework for realistic 3D tele-immersion

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    Meeting, socializing and conversing online with a group of people using teleconferencing systems is still quite differ- ent from the experience of meeting face to face. We are abruptly aware that we are online and that the people we are engaging with are not in close proximity. Analogous to how talking on the telephone does not replicate the experi- ence of talking in person. Several causes for these differences have been identified and we propose inspiring and innova- tive solutions to these hurdles in attempt to provide a more realistic, believable and engaging online conversational expe- rience. We present the distributed and scalable framework REVERIE that provides a balanced mix of these solutions. Applications build on top of the REVERIE framework will be able to provide interactive, immersive, photo-realistic ex- periences to a multitude of users that for them will feel much more similar to having face to face meetings than the expe- rience offered by conventional teleconferencing systems

    Label-free detection of hypoxia-induced extracellular vesicle secretion from MCF-7 cells

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    Nanoscale extracellular vesicles (EVs) including exosomes (50–150 nm membrane particles) have emerged as promising cancer biomarkers due to the carried genetic information about the parental cells. However the sensitive detection of these vesicles remains a challenge. Here we present a label-free electrochemical sensor to measure the EVs secretion levels of hypoxic and normoxic MCF-7 cells. The sensor design includes two consecutive steps; i) Au electrode surface functionalization for anti-CD81 Antibody and ii) EVs capture. The label-free detection of EVs was done via Differential Pulse Voltammetry (DPV) and Electrochemical Impedance Spectroscopy (EIS). The working linear range for the sensor was 102–109 EVs/ml with an LOD 77 EVs/mL and 379 EVs/ml for EIS and DPV based detection. A blood-abundant protein, RhD was used for the selectivity test. In order to assess the performance of the biosensor, the level of EVs secretion by the human breast cancer MCF-7 cell line was compared with enzyme-linked immunosorbent assays (ELISA) and Nanoparticle Tracking Analysis (NTA). Designed label-free electrochemical sensors utilized for quantification of EVs secretion enhancement due to CoCl2-induced hypoxia and 1.23 fold increase with respect to normoxic conditions was found

    Summary of Supersonic Jet and Rocket Noise

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    This paper summarizes a two-part special session, “Supersonic Jet and Rocket Noise,” which was held during the 174th Meeting of the Acoustical Society of America in New Orleans, Louisiana. The sessions were cosponsored by the Noise and Physical Acoustics Technical Committees and consisted of talks by government, academic, and industry researchers from institutions in the United States, Japan, France, and India. The sessions described analytical, computational, and experimental approaches to both fundamental and applied problems on model and full-scale jets and rocket exhaust plumes
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