Miracle-dz/UniFAR-FTUs huggingface dataset:
The Influence Of Hotel Interior, Hotel Customer Process, And Hotel Design On Repurchase Intentions Mediated By Customer Satisfaction

The development of sharia hotels is considered as a support for tourism that is not only commercially oriented but always upholds the noble values of religion and customs of a nation. This study is a quantitative study that aims to test the influence of independent variables on dependent variables. The sample in this study was carried out by simple random sampling. The research data was obtained by spreading questionnaires to sharia hotel customers. The collected data were analyzed by path analysis assisted by the Smart PLS application. Smart PLS analysis in this study was carried out in 2 stages, namely outer model and inner model analysis. Inner model analysis for 1) testing the validity and reliability of the instrument and 2) conducting an r square test to determine the percentage of influence. The inner model analysis is carried out to test hypotheses. Based on the test results, it is known that all instruments are declared valid and flexible. Hotel Interior, Hotel Customer Process, and Hotel Design affect customer satisfaction by 94.0%, while Hotel Customer Process and Hotel Design affect customer satisfaction and customer satisfaction affects repurchase intention by 96.1%. The results of hypothesis testing show that the Hotel Customer Process, Hotel interior, and hotel design affect the company's satisfaction, and customer satisfaction can partially mediate the relationship between the hotel customer process, hotel interior, and hotel design to repurchase intention. Upcoming research is expected to add other variables because there are still many factors that affect consumer satisfaction and repurchase intentions of Islamic hotel customers. The reach for research on Islamic hotels can expand and expand widely.
BROADBAND STUDY WITH SUZAKU OF THE MAGNETAR CLASS

Broadband (0.8–70 keV) spectra of the persistent X-ray emission from nine magnetars were obtained with Suzaku, including three objects in apparent outburst. The soft X-ray component was detected from all of them, with a typical blackbody temperature of kT ∼ 0.5 keV, while the hard-tail component, dominating above ∼10 keV, was detected at ∼1 mCrab intensity from seven of them. Therefore, the spectrum composed of a soft emission and a hard-tail component may be considered to be a common property of magnetars, both in their active and quiescent states. Wide-band spectral analyses revealed that the hard-tail component has a 1–60 keV flux, Fh, comparable to or even higher than that carried by the 1–60 keV soft component, Fs. The hardness ratio (HR) of these objects, defined as ξ ≡ Fh/Fs, was found to be tightly anti-correlated with their characteristic age τc as ξ = (3.3 ± 0.3) × (τc/1 kyr)−0.67±0.04 with a correlation coefficient of −0.989, over the range from ξ ∼ 10 to ξ ∼ 0.1. Magnetars in outburst states were found to lie on the same correlation as relatively quiescent ones. This HR is also positively correlated with their surface magnetic fields with a correlation coefficient of 0.873. In addition, the hard-tail component becomes harder toward sources with older characteristic ages, with the photon index changing from ∼1.7 to ∼0.4.
Thyme Essential Oil Reduces Disease Severity and Induces Resistance against Alternaria linariae in Tomato Plants

Currently, the use of alternative tools for chemical control has become one of the most sustainable and eco-friendly options for crop protection against phytopathogens. Thus, the present study aimed to assess the effect of essential oils (EOs) on the control of tomato early blight (EB), a highly destructive disease of this crop. The antifungal activity and ability to induce resistance induction of the EOs of thyme (Thymus vulgaris), lemongrass (Cymbopogon citratus) and tea tree (Melaleuca alternifolia) were tested for control of A. linariae in tomato plants. In vitro, mycelial growth and conidial germination were strongly inhibited when thyme EO (TEO; 2000 ppm) and lemongrass (LGEO; 2000 ppm) were applied. The infected leaf area and final disease index were decreased by 47.78% and 39.00%, respectively, compared to the water treatment. Foliar spraying with TEO increased the activity of the defense-related enzymes peroxidase, polyphenol oxidase and β-1,3-glucanase. Furthermore, callose deposition and phenolic compound accumulation in tissues infected by A. linariae improved after TEO application. In conclusion, TEO stimulated the defense system of tomato plants infected by A. linariae, which was associated with a reduced severity of EB. These results indicate that TEO is a potential tool in tomato EB disease management.
The impact of cardiopulmonary exercise testing (CPET) and Charlson comorbidity index (CCI) in a large contemporary cohort of patients undergoing robot‐assisted radical cystectomy and intracorporeal urinary diversion (RARC‐ICUD)

The aim of this study was to investigate whether pre‐operative comorbidity status measured by the Charlson comorbidity index (CCI) or cardiopulmonary exercise testing (CPET) is associated with postoperative complications and length of stay (LOS) in patients undergoing robot‐assisted radical cystectomy and intracorporeal urinary diversion (RARC‐ICUD).
Potsdam Wolf-Rayet model atmosphere grids for WN stars

We present new grids of Potsdam Wolf-Rayet (PoWR) model atmospheres for Wolf-Rayet stars of the nitrogen sequence (WN stars). The models have been calculated with the latest version of the PoWR stellar atmosphere code for spherical stellar winds. The WN model atmospheres include the non-LTE solutions of the statistical equations for complex model atoms, as well as the radiative transfer equation in the co-moving frame. Iron-line blanketing is treated with the help of the superlevel approach, while wind inhomogeneities are taken into account via optically thin clumps. Three of our model grids are appropriate for Galactic metallicity. The hydrogen mass fraction of these grids is 50%, 20%, and 0%, thus also covering the hydrogen-rich late-type WR stars that have been discovered in recent years. Three grids are adequate for LMC WN stars and have hydrogen fractions of 40%, 20%, and 0%. Recently, additional grids with SMC metallicity and with 60%, 40%, 20%, and 0% hydrogen have been added. We provide contour plots of the equivalent widths of spectral lines that are usually used for classification and diagnostics.
Combined strong and weak lensing analysis of 28 clusters from the Sloan Giant Arcs Survey

We study the mass distribution of a sample of 28 galaxy clusters using strong and weak lensing observations. The clusters are selected via their strong lensing properties as part of the Sloan Giant Arcs Survey (SGAS) from the Sloan Digital Sky Survey (SDSS). Mass modelling of the strong lensing information from the giant arcs is combined with weak lensing measurements from deep Subaru/Suprime-cam images to primarily obtain robust constraints on the concentration parameter and the shape of the mass distribution. We find that the concentration cvir is a steep function of the mass, cvir∝M−0.59±0.12vir, with the value roughly consistent with the lensing-bias-corrected theoretical expectation for high-mass (∼1015 h−1 M⊙) clusters. However, the observationally inferred concentration parameters appear to be much higher at lower masses (∼1014 h−1 M⊙), possibly a consequence of the modification to the inner density profiles provided by baryon cooling. The steep mass–concentration relation is also supported from direct stacking analysis of the tangential shear profiles. In addition, we explore the 2D shape of the projected mass distribution by stacking weak lensing shear maps of individual clusters with prior information on the position angle from strong lens modelling, and find significant evidence for a large mean ellipticity with the best-fitting value of 〈e〉= 0.47 ± 0.06 for the mass distribution of the stacked sample. We find that the luminous cluster member galaxy distribution traces the overall mass distribution very well, although the distribution of fainter cluster galaxies appears to be more extended than the total mass.
Does Journal Indexation Matter? A Genre-Approach Move Analysis of Nursing English Research Article Abstracts

Background. A plethora of previous studies have discussed the importance of a genre-approach move analysis because the analysis results can provide a picture of the typical conventions of research article writing across disciplines. Purpose. Nursing as a professional discipline, however, has received scant attention, particularly in the abstract section in the journals with different indexation. To fill such an empirical void, this qualitative study probes the notion of whether journal indexation matters in manifesting the rhetorical moves in the nursing abstracts. Methods. Fifty abstracts from a Scopus-indexed Q1 journal and another 50 from three Sinta-indexed journals in Indonesia were analyzed manually. This study employed a descriptive comparative approach to analyze and present the data. Findings. The findings demonstrated conformity manifestations of method and results moves along with their linguistic realizations by using simple past tense in active or passive forms. The article abstracts from the Scopus-indexed nursing journal emphasized the novelty of the research more than their counterparts from the identification of gap of previous research and highlighting the significance of the study. Implications. This study suggests writers consider the contributing role of journal indexation type in projecting a higher standard of abstract writing in preparing their abstracts to increase the acceptance rate during an initial screening stage.
Formation of the Galactic bulge from a two‐component stellar disc: explaining cylindrical rotation and a vertical metallicity gradient

Recent observational studies have revealed that the Galactic bulge has cylindrical rotation and a steeper vertical metallicity gradient. We adopt two representative models for the bulge formation and thereby investigate whether the two models can explain both the observed cylindrical rotation and vertical metallicity gradient in a self-consistent manner. One is the ‘pure disc scenario’ (PDS) in which the bulge is formed from a pure thin stellar disc through spontaneous bar instability. The other is the ‘two-component disc scenario’ (TCDS) in which the bulge is formed from a disc composed of thin and thick discs through bar instability. Our numerical simulations show that although the PDS can reproduce the cylindrical rotation, it shows a rather flatter vertical metallicity gradient that is inconsistent with observations. The derived flatter metallicity gradient is due to the vertical mixing of stars with different initial metallicities by the stellar bar. This result implies that the bulge cannot be simply formed from a pure thin stellar disc. On the other hand, the bulge formed from the two-component disc in the TCDS can explain both the observed cylindrical rotation and vertical metallicity gradient of the Galactic bulge reasonably well. In the TCDS, more metal-poor stars at higher |z| (vertical distance), which originate from the already dynamically hotter thick disc, cannot be strongly influenced by vertical mixing of the bar so that they can stay in situ for longer time-scales and thus keep the lower metallicity at higher |z|. Consequently, the vertical metallicity gradient of the bulge composed of initially thin and thick disc stars cannot be so flattened, even if the gradient of the thin disc can be flattened significantly by the bar in the TCDS. We therefore suggest that a significant fraction of the present Galactic bulge is composed of stars initially in the inner part of the thick disc and thus that these bulge stars and the thick disc have a common origin. We also suggest that the Galaxy might well have experienced some merger events that could dynamically heat up its inner regions until ∼10 Gyr ago.
Clinical Characteristics of Actinic Keratosis Associated with the Risk of Progression to Invasive Squamous Cell Carcinoma: A Systematic Review

Background: Actinic keratosis (AK) is one of the most common lesions on chronically sun-damaged skin that has the risk of progression to invasive squamous cell carcinoma (SCC). With the possibilities of using digital technologies for following-up skin lesions and their increased use in the past few decades, our objective was to update the review by Quaedvlieg et al., 2006, and to review prospective studies from 2005 onwards to identify the clinical characteristics of AK that later progressed to SCC. Methods: The PubMed, Scopus, and ScienceDirect databases were searched for relevant articles. The search had the following criteria: English language, human subjects and year from 2005 onwards. The study protocol was registered in the Prospero database with the record number CRD42020200429 and followed the PRISMA guidelines. The risk-of-bias assessment was performed using the QUIPS tool. Results: From the 5361 studies screened, 105 reports were evaluated for eligibility, and 2 articles with 621 patients were included. The main AK types associated with the development of SCC were found to be baseline AK, also known as a long-standing AK, and merging AK, also called an “AK patch”.
Utilization of WhatsApp in English for Islamic Education Learning as a Media of Communication between Lecturers and Students

WhatsApp is one of the most popular application used by students and lecturers. WhatsApp application gives convenience in interacting and communicating. This research aimed at determining the use of WhatsApp as a medium of communication between lecturers and students in supporting English learning activities at Islamic Education Study Program. The research method applied is quantitative research. The data source is 60 students from IAIN Palopo. This research used the Google form media in survey. The results show that most of the students felt that it was easier for them to communicate and support learning activities compared to other online media. Furthermore, more than 80% of students stated that the application of WhatsApp had a positive impact on their learning activities and supported the improvement of their communication with lecturers. So, WhatsApp is one of the media that has advantages including facilitating communication and supporting learning activities. The ease in using WhatsApp makes students feel helped by this application and becomes one of the important and preferred means of communication for students
Benchmark Performance of Digital QKD Platform Using Quantum Permutation Pad

Quantum permutation pad or QPP is a set of quantum permutation gates. QPP has been demonstrated for quantum secure encryption in both classical and quantum computing systems recently, even at a noisy 5-qubit IBMQ systems. In a classical computing system, QPP encryption is implemented as a permutation gate matrix multiplication with information state vectors. In a quantum computing system, QPP is compiled into a quantum encryption circuit in a native quantum computer and encryption is performed through QPP circuit. Leveraging its quantum mechanical characteristics, we report a digital QKD or D-QKD platform using QPP as a quantum mechanical algorithm implemented in classical systems to distribute quantum entropy, generated from physical quantum random number generators or QRNG, and quantum key over the internet. D-QKD interfaces have been developed to support the photonic QKD standard ETSI-014. This makes any systems with ETSI QKD standards compatible with D-QKD. D-QKD offers point-to-point quantum entropy and quantum key distributions as well as point-to-multi-points quantum key synchronizations with speeds 1000x faster than photonic QKD. This paper reports benchmark performance tests and randomness quality tests for pure quantum entropy generated by a QRNG and expanded entropy using the QPP protocol. The work has been funded by the PlanQK1 project and deployed within the OpenQKD2 testbed Berlin, operated by Deutsche Telekom.
GAS LOSS BY RAM PRESSURE STRIPPING AND INTERNAL FEEDBACK FROM LOW-MASS MILKY WAY SATELLITES

The evolution of dwarf satellites in the Milky Way (MW) is affected by a combination of ram pressure stripping (RPS), tidal stripping, and internal feedback from massive stars. We investigate gas loss processes in the smallest satellites of the MW using three-dimensional, high-resolution, idealized wind tunnel simulations, accounting for gas loss through both ram pressure stripping and expulsion by supernova feedback. Using initial conditions appropriate for a dwarf galaxy like Leo T, we investigate whether or not environmental gas stripping and internal feedback can quench these low-mass galaxies on the expected timescales, shorter than 2 Gyr. We find that supernova feedback contributes negligibly to the stripping rate for these low star formation rate galaxies. However, we also find that RPS is less efficient than expected in the stripping scenarios we consider. Our work suggests that although RPS can eventually completely strip these galaxies, other physics is likely at play to reconcile our computed stripping times with the rapid quenching timescales deduced from observations of low-mass MW dwarf galaxies. We discuss the roles additional physics may play in this scenario, including host-satellite tidal interactions, cored versus cuspy dark matter profiles, reionization, and satellite preprocessing. We conclude that a proper accounting of these physics together is necessary to understand the quenching of low-mass MW satellites.
MAPPING THE OUTER EDGE OF THE YOUNG STELLAR CLUSTER IN THE GALACTIC CENTER

We present new near-infrared spectroscopic observations of the outer edges of the young stellar cluster around the supermassive black hole at the Galactic center. The observations show a break in the surface density profile of young stars at ∼13″ (0.52 pc). These observations spectroscopically confirm previous suggestions of a break based on photometry. Using Gemini North's Near-Infrared Integral Field Spectrometer, we are able to detect and separate early- and late-type stars with a 75% completeness at K s = 15.5 ? > . We sample a region with radii between 7″ and 23″ (0.28–0.92 pc) from Sgr A* and present new spectral classifications of 144 stars brighter than K s = 15.5 ? > , where 140 stars are late-type ( > 1 ? > Gyr) and only four stars are early-type (young, 4–6 Myr). A broken power-law fit of the early-type surface density matches well with our data and previously published values. The projected surface density of late-type stars is also measured and found to be consistent with previous results. We find that the observed early-type surface-density profile is inconsistent with the theory of young stars originating from a tightly bound infalling cluster, as no significant trail of young stars is found at radii above 13″. We also note that either a simple disk instability criterion or a cloud–cloud collision could explain the location of the outer edge, though we lack information to make conclusive remarks on either alternative. If this break in surface density represents an edge to the young stellar cluster, it would set an important scale for the most recent episode of star formation at the Galactic center.
Star Formation in Quasar Host Galaxies at Redshift 6: Millimeter Surveys and New Insights from ALMA

Abstract We have been carrying out a systematic survey of the star formation and ISM properties in the host galaxies of z∼6 quasars. Our 250 GHz observations, together with available data from the literature, yield a sample of 14 z∼6 quasars that are bright in millimeter dust continuum emission with estimated FIR luminosities of a few 1012 to 1013 L⊙. Most of these millimeter-detected z∼6 quasars have also been detected in molecular CO line emission, indicating molecular gas masses on order of 1010 M⊙. We have searched for [C II] 158 micron fine structure line emission toward four of the millimeter bright z∼6 quasars with ALMA and all of them have been detected. All these results suggest massive star formation at rates of about 600 to 2000 M⊙ yr−1 over the central few kpc region of these quasar host galaxies.
CHANDRA OBSERVATIONS OF THE NUCLEAR STAR CLUSTER AND ULTRALUMINOUS X-RAY SOURCES IN NGC 2139

We report Chandra observations of the Scd galaxy NGC 2139, which is known to host a recently formed (107.6 yr) nuclear star cluster. The star cluster is undetected in X-rays, with an upper bound on 0.5–7 keV luminosity of LX < 7.1 × 1037 erg s−1. This bound implies a bolometric accretion luminosity <0.3% of the Eddington luminosity for a black hole with the mass (∼3400 M☉) expected from extrapolation of the M − σ relation. The lack of X-ray emission indicates that a black hole, if present, is not undergoing significant accretion at the current time. While the central cluster is undetected, the data reveal a substantial population of bright X-ray point sources elsewhere in this galaxy, with eight qualifying as ultraluminous X-ray sources with LX > 1039 erg s−1. We use archival Hubble Space Telescope images to identify candidate optical counterparts for seven Chandra sources, which in most cases have optical luminosities and spatial profiles consistent with star clusters. Compared with other galaxies, the number of luminous X-ray sources in NGC 2139 is larger by a factor of ∼4–10 than expected based on its present star formation rate and stellar mass. This finding can be understood if NGC 2139 has concluded a burst of star formation in the recent past, and suggests that this galaxy could be important for testing the use of X-ray source populations as a chronometer of star formation history.
Outperforming Completely Randomized Designs

Split-plot designs have become increasingly popular in industrial experimentation because some of the factors under investigation are often hard-to-change. It is well-known that the resulting compound symmetric error structure not only affects estimation and inference procedures but also the efficiency of the experimental designs used. In this paper, we compute D-optimal first and second order split-plot designs and show that these designs, in many cases, outperform completely randomized designs in terms of D- and G-efficiency. This suggests that split-plot designs should be considered as an alternative to completely randomized designs even if running a completely randomized design is affordable.
Balance Competitivo en las Ligas Europeas de Baloncesto y la NBA

Las ligas deportivas dependen del equilibrio competitivo entre los equipos para ser atractivas para los espectadores, de ahi la aparicion del balance competitivo. Por ello, las distintas ligas deportivas han adquirido diferentes formatos que determinaran su competitividad. El objetivo de este articulo es comparar el balance competitivo de la NBA y las principales ligas europeas, teniendo en cuenta la NBA en su conjunto y cada una de sus conferencias de forma independiente. Las variables utilizadas para medir el balance competitivo han sido el indice Hirschman-Herfindal y las ratios C5 y C8. Los resultados muestran un mejor balance competitivo de la NBA en conjunto respecto a las ligas europeas, sin embargo estas diferencias desaparecen al analizar las conferencias de forma independiente. Se concluye que al tener en cuenta cada una de las conferencias de forma independiente, con una estructura mas similar a las ligas europeas, se presenta un balance competitivo parecido bajo los indicadores utilizados. Sin embargo, la NBA incluye limitaciones en la competicion que siguen favoreciendo la posibilidad de que sea mas atractiva para el espectador.