Political Party Propaganda in DKI Jakarta Local Election 2017 in Online Media (Content Analysis Political Party Propaganda in DKI Jakarta Local Election 2017 in Kompas.com)

To reach its target, the political parties so as to package the message propagated. In the event the local elections DKI 2017, in an effort to get a seat regional head not inevitable then the propaganda is played by political parties. The purpose of this study was to determine the form of propaganda made by the political parties in local elections in 2017 DKI Media Online (Kompas.com). This research is a quantitative research using content analysis method with descriptive approach. To view the propaganda of this study are categorized kind of propaganda is hidden, open, vertical, horizontal and techniques of propaganda, name calling, glittering generalities, testimonials, transfer, plain folk, card stacking, bandwagon technique, reputable mouthpiece and using all forms of persuations. The recording unit of this study is an excerpt and image. After doing Coding, it was found that the most frequent Gerindra hidden propaganda that as many as 26 times, vertical propaganda as much as 26 times, and most frequently used techniques in their delivery Card Stacking in Kompas.com. Through the PPP Coding also found that the most frequently hidden propaganda that as many as 49 times, 49 times vertically, and the most frequently used technique Card Stacking ie as many as 23 times in Kompas.com. The use of propaganda techniques hidden impact to people who receive propaganda. By presenting a one-sided even using a falsehood, society becomes tercerdaskan in understanding the situation and take a decision. Mechanical testimony is unlikely to exist in a daily news excerpts. Can the emergence of this technique requires a propagandist flexibility in determining the content of the communication media with which to spread the message. With the limitation provisions of the news content, a propagandist would be difficult to use the techniques of propaganda in the news daily. Even if there is a statement from a figure reported by the authors, it will be difficult to identify the interested figure behind the deposit of the statemen

Non-commutative Geometry from Perturbative Quantum Gravity in de Sitter spacetime

We show that a non-commutative structure arises naturally from perturbative quantum gravity in a de Sitter background metric. Our work builds on recent advances in the construction of observables in highly symmetric background spacetimes [Brunetti et al., JHEP 08, 032 (2016); Fr\"ob and Lima, Class. Quant. Grav. 35, 095010 (2018)], where the dynamical coordinates that are needed in the relational approach were established for such backgrounds to all orders in perturbation theory. We show that these dynamical coordinates that describe events in the perturbed spacetime are naturally non-commuting, and determine their commutator to leading order in the Planck length. Our result generalizes the causal non-commutative structure that was found using the same approach in Minkowski space [Fr\"ob, Much and Papadopoulos, Phys. Rev. D 107, 064041 (2023)]

Pengaruh Sistem Manajemen Iso 9001:2008 Terhadap Pelayanan Kefarmasian Di Puskesmas Kabupaten Sleman

The vision of health development organized by the district health center is achieving district healthy. The need for improving the quality of health services in health centers contained in the WHO Annual Report 2008 under the title "Primary Health Care, Now More Than Ever". The efforts to improve the quality of services in health centers is ISO 9001:2008 certification at the International level. ISO 9001 certification is expected to improve the quality of pharmacy services at health centers. In order to ensure the implementation of quality management system certification ISO 9001:2008 in Sleman district health centers especially in pharmaceutical services, we need a special evaluation of pharmacy services at existing health centers and Sleman district that have not implemented ISO 9001:2008. The purpose of this study is to describe the influence of ISO 9001:2008 quality management system for pharmacy services at district Sleman health centers who have and have not implemented the ISO 9001:2008. The study design is a descriptive cross-sectional design. Data captured includes quantitative data from observations of pharmacy services at the health center and qualitative data from in-depth interviews. The study period October 23, 2012 until December 23, 2012. The results showed Score adherence to standard operating procedures at the clinic ISO and non-ISO is 1.25 and 1. Average preparation time for non-drug concoction and concoction at ISO puskemsas sequence was 383 seconds and 193 seconds. average preparation time mixing and non-mixing drugs in health centers in order are non ISO 446 seconds and 193 seconds. Average delivery time ISO medicine in health centers is 87 seconds, the average time on the drug delivery centers are non-ISO 60.75 seconds. Percentage suitability prescription drugs in health centers and ISO and non ISO is 100% and 99.98%. The percentage of drugs in health centers completeness label ISO and non ISO is 100% and 100%. The percentage of patients in the clinic knowledge of ISO and non-ISO is 84.97% and 72.47%.. The levels of patient satisfaction in ISO and non ISO clinic in category "Satisfied". The policy of Quality Management System ISO 9001:2008 that applied to the community health center in Sleman district does not affect the improvement of pharmaceutical services at the community health center. The observations indicate that the quality was not much different in the two types of community health center, it makes an ISO 9001:2008 should be reviewed. Key words: ISO 9001:2008, patient satisfaction, pharmaceutical services, public health center

Gamma-Ray Spectra & Variability of the Crab Nebula Emission Observed by BATSE

We report ~ 600 days of BATSE earth-occultation observations of the total gamma-ray (30 keV to 1.7 MeV) emission from the Crab nebula, between 1991 May 24 (TJD 8400) and 1994 October 2 (TJD 9627). Lightcurves from 35-100, 100-200, 200-300, 300-400, 400-700, and 700-1000 keV, show that positive fluxes were detected by BATSE in each of these six energy bands at significances of approximately 31, 20, 9.2, 4.5, 2.6, and 1.3 sigma respectively per day. We also observed significant flux and spectral variations in the 35-300 keV energy region, with time scales of days to weeks. The spectra below 300 keV, averaged over typical CGRO viewing periods of 6-13 days, can be well described by a broken power law with average indices of ~ 2.1 and ~ 2.4 varying around a spectral break at ~ 100 keV. Above 300 keV, the long-term averaged spectra, averaged over three 400 d periods (TJD 8400-8800, 8800-9200, and 9200-9628, respectively) are well represented by the same power law with index of ~ 2.34 up to ~ 670 keV, plus a hard spectral component extending from ~ 670 keV to ~ 1.7 MeV, with a spectral index of ~ 1.75. The latter component could be related to a complex structure observed by COMPTEL in the 0.7-3 MeV range. Above 3 MeV, the extrapolation of the power-law continuum determined by the low-energy BATSE spectrum is consistent with fluxes measured by COMPTEL in the 3-25 MeV range, and by EGRET from 30-50 MeV. We interpret these results as synchrotron emission produced by the interaction of particles ejected from the pulsar with the field in different dynamical regions of the nebula system, as observed recently by HST, XMM-Newton, and Chandra.Comment: To be published in the November 20, 2003, Vol 598 issue of the Astrophysical Journa

INTEGRAL observations of the black hole candidate H 1743-322 in outburst

INTEGRAL made 3 observations in 2003 April of the black hole candidate H 1743-322 during the rising part, and close to the maximum, of an outburst. H 1743-322 was previously observed in outburst in 1977-1978. The source is located in a crowded region of the sky (l = 357 deg, b = -2 deg) and at least 18 sources are clearly detected in the field of view of the gamma-ray imager during a 277 ksec exposure. These are well known persistent X-ray binaries and 3 transient sources in outburst. The combined 5-200 keV JEM-X and SPI spectrum of H 1743-322 is well fit with an absorbed ((2.5 10E22 atom/cm2) soft (photon index 2.70 +/- 0.09) power-law model consistent with J 1743-322 being in a high/soft state.Comment: 5 pages. Figs. 2 and 3 are best viewed in color. To appear in INTEGRAL special edition of A&A

BATSE Observations of the Piccinotti Sample of AGN

BATSE Earth occultation data have been used to search for emission in the 20-100 keV band from all sources in the Piccinotti sample, which represents to date the only complete 2-10 keV survey of the extragalactic sky down to a limiting flux of 3.1 x 10^(-11) erg cm^(-2)$ s^(-1). Nearly four years of observations have been analyzed to reach a 5sigma sensitivity level of about 7.8x 10^(-11) erg cm^(-2) s^(-1) in the band considered. Of the 36 sources in the sample, 14 have been detected above 5sigma confidence level while marginal detection (3<sigma<5) can be claimed for 13 sources; for 9 objects 2sigma upper limits are reported. Comparison of BATSE results with data at higher energies is used to estimate the robustness of our data analysis: while the detection level of each source is reliable, the flux measurement maybe overestimated in some sources by as much as 35%, probably due to incomplete data cleaning. Comparison of BATSE fluxes with X-ray fluxes, obtained in the 2-10 keV range and averaged over years, indicates that a canonical power law of photon index 1.7 gives a good description of the broad band spectra of bright AGNs and that spectral breaks preferentially occur above 100 keV.Comment: 18 pages, 1 figure. Accepted for publication on Apj

COMPTEL images locations of gamma‐ray bursts

The γ‐ray telescope COMPTEL onboard GRO has so far located 6 gamma‐ray bursts which occurred in its ∼1 sr field of view. The positions of the sources were derived by the maximum‐entropy method. Systematic and statistical uncertainties for the four strongest bursts are approximately 1° to 2° and can be reduced in future analysis

The Burst and Transient Source Experiment Earth Occultation Technique

An Earth orbiting detector sensitive to gamma ray photons will see step-like occultation features in its counting rate when a gamma ray point source crosses the Earth's limb. This is due to the change in atmospheric attenuation of the gamma rays along the line of sight. In an uncollimated detector, these occultation features can be used to locate and monitor astrophysical sources provided their signals can be individually separated from the detector background. We show that the Earth occultation technique applied to the Burst and Transient Source Experiment (BATSE) on the Compton Gamma Ray Observatory (CGRO) is a viable and flexible all-sky monitor in the low energy gamma ray and hard X-ray energy range (20 keV - 1 MeV). The method is an alternative to more sophisticated photon imaging devices for astronomy, and can serve well as a cost-effective science capability for monitoring the high energy sky. Here we describe the Earth occultation technique for locating new sources and for measuring source intensity and spectra without the use of complex background models. Examples of transform imaging, step searches, spectra, and light curves are presented. Systematic uncertainties due to source confusion, detector response, and contamination from rapid background fluctuations are discussed and analyzed for their effect on intensity measurements. A sky location-dependent average systematic error is derived as a function of galactic coordinates. The sensitivity of the technique is derived as a function of incident photon energy and also as a function of angle between the source and the normal to the detector entrance window. Occultations of the Crab Nebula by the Moon are used to calibrate Earth occultation flux measurements independent of possible atmospheric scattering effects.Comment: 39 pages, 24 figures. Accepted for publication in the Astrophysical Journal Supplement

Energetics and atomic mechanisms of dislocation nucleation in strained epitaxial layers

We study numerically the energetics and atomic mechanisms of misfit dislocation nucleation and stress relaxation in a two-dimensional atomistic model of strained epitaxial layers on a substrate with lattice misfit. Relaxation processes from coherent to incoherent states for different transition paths are studied using interatomic potentials of Lennard-Jones type and a systematic saddle point and transition path search method. The method is based on a combination of repulsive potential minimization and the Nudged Elastic Band method. For a final state with a single misfit dislocation, the minimum energy path and the corresponding activation barrier are obtained for different misfits and interatomic potentials. We find that the energy barrier decreases strongly with misfit. In contrast to continuous elastic theory, a strong tensile-compressive asymmetry is observed. This asymmetry can be understood as manifestation of asymmetry between repulsive and attractive branches of pair potential and it is found to depend sensitively on the form of the potential.Comment: 11 pages, 9 figures, to appear in Phys. Rev.