72 research outputs found

    Revival of the magnetar PSR J1622-4950: observations with MeerKAT, Parkes, XMM-Newton, Swift, Chandra, and NuSTAR

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    New radio (MeerKAT and Parkes) and X-ray (XMM-Newton, Swift, Chandra, and NuSTAR) observations of PSR J1622-4950 indicate that the magnetar, in a quiescent state since at least early 2015, reactivated between 2017 March 19 and April 5. The radio flux density, while variable, is approximately 100x larger than during its dormant state. The X-ray flux one month after reactivation was at least 800x larger than during quiescence, and has been decaying exponentially on a 111+/-19 day timescale. This high-flux state, together with a radio-derived rotational ephemeris, enabled for the first time the detection of X-ray pulsations for this magnetar. At 5%, the 0.3-6 keV pulsed fraction is comparable to the smallest observed for magnetars. The overall pulsar geometry inferred from polarized radio emission appears to be broadly consistent with that determined 6-8 years earlier. However, rotating vector model fits suggest that we are now seeing radio emission from a different location in the magnetosphere than previously. This indicates a novel way in which radio emission from magnetars can differ from that of ordinary pulsars. The torque on the neutron star is varying rapidly and unsteadily, as is common for magnetars following outburst, having changed by a factor of 7 within six months of reactivation.Comment: Published in ApJ (2018 April 5); 13 pages, 4 figure

    Setting a baseline for global urban virome surveillance in sewage

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    The rapid development of megacities, and their growing connectedness across the world is becoming a distinct driver for emerging disease outbreaks. Early detection of unusual disease emergence and spread should therefore include such cities as part of risk-based surveillance. A catch-all metagenomic sequencing approach of urban sewage could potentially provide an unbiased insight into the dynamics of viral pathogens circulating in a community irrespective of access to care, a potential which already has been proven for the surveillance of poliovirus. Here, we present a detailed characterization of sewage viromes from a snapshot of 81 high density urban areas across the globe, including in-depth assessment of potential biases, as a proof of concept for catch-all viral pathogen surveillance. We show the ability to detect a wide range of viruses and geographical and seasonal differences for specific viral groups. Our findings offer a cross-sectional baseline for further research in viral surveillance from urban sewage samples and place previous studies in a global perspective

    Revival of the Magnetar PSR J1622-4950: Observations with MeerKAT, Parkes, XMM-Newton, Swift, Chandra, and NuSTAR

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    New radio (MeerKAT and Parkes) and X-ray (XMM-Newton, Swift, Chandra, and NuSTAR) observations of PSR J1622-4950 indicate that the magnetar, in a quiescent state since at least early 2015, reactivated between 2017 March 19 and April 5. The radio flux density, while variable, is approximately 100 larger than during its dormant state. The X-ray flux one month after reactivation was at least 800 larger than during quiescence, and has been decaying exponentially on a 111 19 day timescale. This high-flux state, together with a radio-derived rotational ephemeris, enabled for the first time the detection of X-ray pulsations for this magnetar. At 5%, the 0.3-6 keV pulsed fraction is comparable to the smallest observed for magnetars. The overall pulsar geometry inferred from polarized radio emission appears to be broadly consistent with that determined 6-8 years earlier. However, rotating vector model fits suggest that we are now seeing radio emission from a different location in the magnetosphere than previously. This indicates a novel way in which radio emission from magnetars can differ from that of ordinary pulsars. The torque on the neutron star is varying rapidly and unsteadily, as is common for magnetars following outburst, having changed by a factor of 7 within six months of reactivation

    The 1.28 GHz MeerKAT DEEP2 Image

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    We present the confusion-limited 1.28 GHz MeerKAT DEEP2 image covering one qb » ¢ 68 FWHM primarybeam area with θ = 7 6 FWHM resolution and s = m - n 0.55 0.01 Jy beam 1 rms noise. Its J2000 center position α = 04h 13m 26 4, δ = −80° 00′ 00″ was selected to minimize artifacts caused by bright sources. We introduce the new 64-element MeerKAT array and describe commissioning observations to measure the primary-beam attenuation pattern, estimate telescope pointing errors, and pinpoint (u, v) coordinate errors caused by offsets in frequency or time. We constructed a 1.4 GHz differential source count by combining a power-law count fit to the DEEP2 confusion P(D) distribution from 0.25 to 10 μJy with counts of individual DEEP2 sources between 10 μJy and 2.5 mJy. Most sources fainter than S ∼ 100 μJy are distant star-forming galaxies (SFGs) obeying the far-IR/ radio correlation, and sources stronger than 0.25 μJy account for ∼93% of the radio background produced by SFGs. For the first time, the DEEP2 source count has reached the depth needed to reveal the majority of the star formation history of the universe. A pure luminosity evolution of the 1.4 GHz local luminosity function consistent with the Madau & Dickinson model for the evolution of SFGs based on UV and infrared data underpredicts our 1.4 GHz source count in the range -5 log Jy 4 [ ( )] S

    Construction of behaviourally anchored rating scales (BARS) for the measurement of managerial performance

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    The original publication is available at http://www.sajip.co.zaBARS were initially developed as indices of behavioural change and to ensure greater comparability of ratings from different raters. In this study, BARS were developed for a major producer-wholesaler company in the liquor industry to serve as an independent criterion in the validation of the company's assessment center, to assess the impact of development activities on the skill levels of assessment centre participants and as a diagnostic tool in identifying performance deficiencies. A step-by-step account of the four stages in the development of BARS is presented, together with examples of actual scales for the final steps.Gedragsgeankerde skale (BARS) is oorspronklik ontwikkel as indekse van verandering, en om die vergelykbaarheid tussen beroordelings van verskillende beoordelaars te verhoog. In hierdie studie is BARS vir 'n groothandelaar in die drankbedryf ontwikkel ten einde te dien as 'n onafhanklike kriterium in die validering van hulle takseersentrum; om die invloed van ontwikkelingsaktiwiteite op die vaardigheidsvlakke van deelnemers aan die takseersentrum te meet; en as 'n diagnostiese hulpmiddel in die indentifisering van ontoereikende prestasie. 'n Stap-vir-stap beskrywing van die vier stadia in die ontwikkeling van BARS word gegee, met voorbeelde van werklike skale vir die finale stappe.Publisher's versio

    Validation of an assessment centre against BARS : an experience with performance related criteria

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    Original publication is available at http://www.sajip.co.zaThe objective of this study is to determine the validity of a middle management assessment centre. Behaviourally Anchored Rating Scales were developed specifically for this purpose. The results testify to the validity of this assessment centre and lend support to the argument that assessment centres do indeed predict performance criteria (viz a viz potential/advancement criteria). The validity coefficients for the various dimensions are indicated.Die doel van hierdie studie is om die geldigheid van 'n takseersentrum vir middelbestuur te bepaal. Vir die doel is gedragsgeankerde skale as kriterium spesiaal ontwikkel. Die resultate dui op die geldigheid van hierdie takseersentrum en verleen addisionele steun aan die argument dat takseersentrums wel prestasiekriteria (viz a viz potensiaal/bevorderingskriteria) voorspel. Die geldigheidskoeffisiente van die onderskeie bestuursdimensies word aangetoon.Publisher's versio
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