Kualitas Pelayanan Kartu Tenaga Kerja Luar Negeri Elektronik di Pos Pelayanan Penempatan dan Perlindungan Tenaga Kerja Indonesia Cilacap

Skripsi ini berjudul “Kualitas Pelayanan Kartu Tenaga Kerja Elektronik di Pos Pelayanan Penempatan dan Perlindungan Tenaga Kerja Indonesia Cilacap“. Pelayanan publik oleh aparatur pemerintah dewasa ini masih banyak dijumpai kelemahan sehingga belum dapat memenuhi kualitas yang diharapkan masyarakat. Salah satunya pelayanan e-KTKLN di P4TKI Cilacap, masih ada berbagai keluhan yang datang dari masyarakat atau para TKI yang mengeluhkan kualitas di P4TKI ini. E-KTKLN ini merupakan suatu kartu tenaga kerja luar negeri yang berbentuk elektronik yang sangat diperlukan untuk para calon TKI yang akan bekerja di luar negeri. Tujuan penelitian ini adalah untuk mengetahui apakah kualitas pelayanan Kartu Tenaga Kerja Luar Negeri Elektronik di Pos Pelayanan Penempatan dan Perlindungan Tenaga Kerja Indonesia Cilacap sudah memuaskan.Penelitian ini menggunakan deskriptif kuantitatif dengan metode survey, lokasi penelitian di Pos Pelayanan Penempatan dan Perlindungan Tenaga Kerja Indonesia Cilacap.Sasaran penelitian ini adalah para calon TKI yang datang ke Pos Pelayanan Penempatan dan Perlindungan Tenaga Kerja Indonesia Cilacap untuk melakukan pembuatan e-KTKLN dengan jumlah responden sebanyak 312 orang. Teknik sampel yang digunakan adalah accidental sampling , sampel dapat terpilih karena berada pada waktu, situasi, dan tempat yang tepat. Pengumpulan data dilakukan dengan kuesioner dan dokumentasi. Metode analisis yang digunakan adalah Arithmetic Mean, Standar Deviasi dan Z-Score. Hasil penelitian ini menunjukan bahwa kualitas pelayanan Kartu Tenaga Kerja Luar Negeri Elektronik di Pos Pelayanan Penempatan dan Perlindungan Tenaga Kerja Indonesia Cilacap sudah baik dan memuaskan. Dari lima indikator yang digunakan untuk mengamati kualitas Kartu Tenaga Kerja Luar Negeri Elektronik di Pos Pelayanan Penempatan dan Perlindungan Tenaga Kerja Indonesia Cilacap menunjukan indikator (1) tangible/bukti fisik berada pada kategori baik, (2) reliability/keandalan berada pada kategori baik,(3)assurance/jaminan berada pada kategori baik,(4) empathy/kemudahan berada pada kategori baik dan (5) responsiveness/ketanggapan berada pada kategori baik. Berdasarkan hasil penelitian, dapat disimpulkan bahwa kelima indikator kualitas pelayanan e-KTKLN yang terdiri dari tangible, reliability, assurance,empathy, dan responsiveness sudah baik dan memuaskan. Walaupun sudah baik dan memuaskan tetapi masih perlu dijaga serta perlu adanya perbaikan dan peningkatan yang lebih agar pelayanan di Pos Pelayanan Penempatan dan Perlindungan Tenaga Kerja Indonesia Cilacap semakin baik dan semakin memuaskan serta menyenangkan untuk para pelanggannya

Erratum: Sequence data and association statistics from 12,940 type 2 diabetes cases and controls.

This corrects the article DOI: 10.1038/sdata.2017.179

Search for Gravitational Wave Bursts from Soft Gamma Repeaters

We present the results of a LIGO search for short-duration gravitational waves (GWs) associated with Soft Gamma Repeater (SGR) bursts. This is the first search sensitive to neutron star f-modes, usually considered the most efficient GW emitting modes. We find no evidence of GWs associated with any SGR burst in a sample consisting of the 27 Dec. 2004 giant flare from SGR 1806-20 and 190 lesser events from SGR 1806-20 and SGR 1900+14 which occurred during the first year of LIGO's fifth science run. GW strain upper limits and model-dependent GW emission energy upper limits are estimated for individual bursts using a variety of simulated waveforms. The unprecedented sensitivity of the detectors allows us to set the most stringent limits on transient GW amplitudes published to date. We find upper limit estimates on the model-dependent isotropic GW emission energies (at a nominal distance of 10 kpc) between 3x10^45 and 9x10^52 erg depending on waveform type, detector antenna factors and noise characteristics at the time of the burst. These upper limits are within the theoretically predicted range of some SGR models.Comment: 6 pages, 1 Postscript figur

Quantum state preparation and macroscopic entanglement in gravitational-wave detectors

Long-baseline laser-interferometer gravitational-wave detectors are operating at a factor of 10 (in amplitude) above the standard quantum limit (SQL) within a broad frequency band. Such a low classical noise budget has already allowed the creation of a controlled 2.7 kg macroscopic oscillator with an effective eigenfrequency of 150 Hz and an occupation number of 200. This result, along with the prospect for further improvements, heralds the new possibility of experimentally probing macroscopic quantum mechanics (MQM) - quantum mechanical behavior of objects in the realm of everyday experience - using gravitational-wave detectors. In this paper, we provide the mathematical foundation for the first step of a MQM experiment: the preparation of a macroscopic test mass into a nearly minimum-Heisenberg-limited Gaussian quantum state, which is possible if the interferometer's classical noise beats the SQL in a broad frequency band. Our formalism, based on Wiener filtering, allows a straightforward conversion from the classical noise budget of a laser interferometer, in terms of noise spectra, into the strategy for quantum state preparation, and the quality of the prepared state. Using this formalism, we consider how Gaussian entanglement can be built among two macroscopic test masses, and the performance of the planned Advanced LIGO interferometers in quantum-state preparation

First LIGO search for gravitational wave bursts from cosmic (super)strings

We report on a matched-filter search for gravitational wave bursts from cosmic string cusps using LIGO data from the fourth science run (S4) which took place in February and March 2005. No gravitational waves were detected in 14.9 days of data from times when all three LIGO detectors were operating. We interpret the result in terms of a frequentist upper limit on the rate of gravitational wave bursts and use the limits on the rate to constrain the parameter space (string tension, reconnection probability, and loop sizes) of cosmic string models.Comment: 11 pages, 3 figures. Replaced with version submitted to PR

Astrophysically Triggered Searches for Gravitational Waves: Status and Prospects

In gravitational-wave detection, special emphasis is put onto searches that focus on cosmic events detected by other types of astrophysical observatories. The astrophysical triggers, e.g. from gamma-ray and X-ray satellites, optical telescopes and neutrino observatories, provide a trigger time for analyzing gravitational wave data coincident with the event. In certain cases the expected frequency range, source energetics, directional and progenitor information is also available. Beyond allowing the recognition of gravitational waveforms with amplitudes closer to the noise floor of the detector, these triggered searches should also lead to rich science results even before the onset of Advanced LIGO. In this paper we provide a broad review of LIGO's astrophysically triggered searches and the sources they target

Stacked Search for Gravitational Waves from the 2006 SGR 1900+14 Storm

We present the results of a LIGO search for short-duration gravitational waves (GWs) associated with the 2006 March 29 SGR 1900+14 storm. A new search method is used, "stacking'' the GW data around the times of individual soft-gamma bursts in the storm to enhance sensitivity for models in which multiple bursts are accompanied by GW emission. We assume that variation in the time difference between burst electromagnetic emission and potential burst GW emission is small relative to the GW signal duration, and we time-align GW excess power time-frequency tilings containing individual burst triggers to their corresponding electromagnetic emissions. We use two GW emission models in our search: a fluence-weighted model and a flat (unweighted) model for the most electromagnetically energetic bursts. We find no evidence of GWs associated with either model. Model-dependent GW strain, isotropic GW emission energy E_GW, and \gamma = E_GW / E_EM upper limits are estimated using a variety of assumed waveforms. The stacking method allows us to set the most stringent model-dependent limits on transient GW strain published to date. We find E_GW upper limit estimates (at a nominal distance of 10 kpc) of between 2x10^45 erg and 6x10^50 erg depending on waveform type. These limits are an order of magnitude lower than upper limits published previously for this storm and overlap with the range of electromagnetic energies emitted in SGR giant flares.Comment: 7 pages, 3 figure

First joint search for gravitational-wave bursts in LIGO and GEO600 data

We present the results of the first joint search for gravitational-wave bursts by the LIGO and GEO600 detectors. We search for bursts with characteristic central frequencies in the band 768 to 2048 Hz in the data acquired between the 22nd of February and the 23rd of March, 2005 (fourth LSC Science Run - S4). We discuss the inclusion of the GEO600 data in the Waveburst-CorrPower pipeline that first searches for coincident excess power events without taking into account differences in the antenna responses or strain sensitivities of the various detectors. We compare the performance of this pipeline to that of the coherent Waveburst pipeline based on the maximum likelihood statistic. This likelihood statistic is derived from a coherent sum of the detector data streams that takes into account the antenna patterns and sensitivities of the different detectors in the network. We find that the coherentWaveburst pipeline is sensitive to signals of amplitude 30 - 50% smaller than the Waveburst-CorrPower pipeline. We perform a search for gravitational-wave bursts using both pipelines and find no detection candidates in the S4 data set when all four instruments were operating stably.Comment: 30 pages, 8 figure

Search for pair-produced long-lived neutral particles decaying to jets in the ATLAS hadronic calorimeter in ppcollisions at √s=8TeV

The ATLAS detector at the Large Hadron Collider at CERN is used to search for the decay of a scalar boson to a pair of long-lived particles, neutral under the Standard Model gauge group, in 20.3fb−1of data collected in proton–proton collisions at √s=8TeV. This search is sensitive to long-lived particles that decay to Standard Model particles producing jets at the outer edge of the ATLAS electromagnetic calorimeter or inside the hadronic calorimeter. No significant excess of events is observed. Limits are reported on the product of the scalar boson production cross section times branching ratio into long-lived neutral particles as a function of the proper lifetime of the particles. Limits are reported for boson masses from 100 GeVto 900 GeV, and a long-lived neutral particle mass from 10 GeVto 150 GeV