bluuebunny/crossref_metadata_2025_split huggingface dataset:
“Panengen” Indigenous Knowledge as the Financial Behavior of Cikalong Community
Authors: Azizah Nurul , Nidar Sulaeman Rahman , Saefullah Kurniawan 
Published: August 2022

AbstractThis study aims to examine the panengen culture, an indigenous knowledge as the basis of the financial management of the Cikalong community. This study uses a qualitative method with a case study approach, which analyzes data based on in-depth interviews, non-participatory observations, and documentation about the panengen culture in the financial management of the Cikalong community. The results of this study show that the financial management process of the Cikalong community is based on the cultural concepts of panengen such as basajan, pamali, and neundeun miraweuy which shape their financial behavior.Keywords: Panengen culture, Financial Behavior, Financial Literacy AbstrakPenelitian ini bertujuan untuk mengkaji mengenai budaya panengen yang menjadi indigenous knowledge sebagai dasar pengetahuan dalam pengelolaan keuangan masyarakat Desa Cikalong. Metode yang digunakan dalam penelitian ini adalah metode kualitatif dengan pendekatan studi kasus, dimana data yang dianalisis berdasarkan data dari wawancara mendalam, observasi non partisipatoris, dan dokumentasi berkaitan dengan budaya panengen dalam pengelolaan keuangan masyarkat Desa Cikalong. Hasil dalam penelitian ini menunjukan proses pengelolaan keuangan masyarakat Desa Cikalong berlandaskan dari konsep-konsep budaya panengen yaitu basajan, pamali dan neundeun miraweuy yang membentuk financial behavior mereka.Kata Kunci: Budaya Panengen, Financial Behavior, Financial Literacy
The Religious Patterns of the Tablighi Jamaat in Indonesia
Authors: Saepuloh Aep , Koswara Nandang , Wildan Asep Dadan 
Published: August 2022

Abstract One of the promises of religion is happiness for its followers. The promise is translated according to their respective mindstreem. One of them is the Tablighi Jamaat. The Tablighi Jamaat claims to be a neutral community in terms of sects, mass organizations, and politics, but within the framework of ahl al-sunnah wa aljamâ'ah. They emphasize their religious activities in real terms through the practice of da'wah by prioritizing morality. This study aims to determine the religious pattern of the Tablighi Jamaat by studying the pattern of their life and da'wah. This study uses a qualitative approach with a descriptive method in describing the results of the study. The results of the research on the religious patterns of the Tablighi Jamaat mutually influence the dimensions of doctrine, teachings, rituals, appreciation and practice, so that the social interactions that are formed between the two are dialectically and associatively intertwined because they are influenced by motivational orientations and value orientations. In the application of the religious pattern, the Tablighi Jamaat adheres to the six doctrinal principles they profess. Keywords: Religion, Tablighi Jamaat, Religious Patterns.
Large Impact of the Mg ii h and k Incident Radiation Change on Results of Radiative Transfer Models and the Importance of Dynamics
Authors: Gunár Stanislav , Heinzel Petr , Koza Július , Schwartz Pavol 
Published: August 2022

Abstract
We demonstrate that changes in the incident radiation in Mg ii h and k lines have a significant impact on the results of radiative transfer modeling of prominence-like plasmas. To uncover the extent of this impact and allow easy comparison, here we study two cases, one representing the minimum of the solar activity and the other corresponding to the typical conditions during solar maxima. To represent well the properties of the prominence plasma, we use the 2D non-LTE (i.e., departures from local thermodynamic equilibrium) model of prominence fine structures in both the single-thread configuration and the multithread configuration incorporating prominence dynamics. We show that in the modeled environment of prominence fine structures, the change in the central, integrated, and peak intensities of the synthetic Mg ii h and k profiles can be as large as the change in the incident radiation itself. This means that the Mg ii h and k spectra of observed prominences can be affected by tens of percent because the illumination from the solar disk can change by such a degree over the solar cycle. That makes the knowledge and use of event-specific incident radiation data very important for the diagnostics of prominences and other chromospheric and coronal structures when using Mg ii h and k spectral observations. In addition, the observed Mg ii h and k spectra are strongly influenced by the line-of-sight dynamics, as the multithread configuration of the 2D model allows us to reveal. The effect of dynamics is, unsurprisingly, most pronounced in the line widths and integrated intensities.
Analytic Approach to the Late Stages of Giant Planet Formation
Authors: Adams Fred C. , Batygin Konstantin 
Published: August 2022

Abstract
This paper constructs an analytic description for the late stages of giant planet formation. During this phase of evolution, the planet gains the majority of its final mass through gas accretion at a rapid rate. This work determines the density and velocity fields for material falling onto the central planet and its circumplanetary disk, and finds the corresponding column density of this infalling envelope. We derive a steady-state solution for the surface density of the disk as a function of its viscosity (including the limiting case where no disk accretion occurs). Planetary magnetic fields truncate the inner edge of the disk and determine the boundary conditions for mass accretion onto the planet from both direct infall and from the disk. The properties of the forming planet and its circumplanetary disk are determined, including the luminosity contributions from infall onto the planet and disk surfaces, and from disk viscosity. The radiative signature of the planet formation process is explored using a quasi-spherical treatment of the emergent spectral energy distributions. The analytic solutions developed herein show how the protoplanet properties (envelope density distribution, velocity field, column density, disk surface density, luminosity, and radiative signatures) vary with input parameters (instantaneous mass, orbital location, accretion rate, and planetary magnetic field strength).
The Star-forming Main Sequence of the Host Galaxies of Low-redshift Quasars
Authors: Zhuang 庄 Ming-Yang 明阳 , Ho Luis C. 
Published: August 2022

Abstract
We investigate the star-forming main sequence of the host galaxies of a large, well-defined sample of 453 redshift ∼0.3 quasars with previously available star formation rates by deriving stellar masses from modeling their broadband (grizy) spectral energy distribution. We perform two-dimensional, simultaneous, multi-filter decomposition of Pan-STARRS1 3π Steradian Survey images to disentangle the active galactic nucleus (AGN) from its host galaxy, by explicitly considering, for the first time, the wavelength variation of galaxy structures. We quantify the Sérsic profiles and sizes of the host galaxies from mock AGNs generated from both real and idealized galaxies. Detailed morphological classifications of the calibration galaxy sample using Hubble Space Telescope images enable us to estimate crude morphological types of the quasars. Although the majority (∼60%) of the quasars are hosted by bulge-dominated, early-type galaxies, a substantial fraction (∼40%) reside in disk-dominated, late-type galaxies, suggesting that at least in these systems major mergers have not played a significant role in regulating their AGN activity, in agreement with recent simulations and observations of nearby quasars. The vast majority (∼90%) of the quasars have star formation rates that place them on or above the galaxy star-forming main sequence, with more rapidly accreting AGNs displaced further above the main sequence. Quasar host galaxies generally follow the stellar mass–size relation defined by inactive galaxies, both for late-type and early-type systems, but roughly 1/3 of the population has smaller sizes at a given stellar mass, reminiscent of compact star-forming galaxies at higher redshift.
Combining Planck and SPT Cluster Catalogs: Cosmological Analysis and Impact on the Planck Scaling Relation Calibration
Authors: Salvati L. , Saro A. , Bocquet S. , Costanzi M. , Ansarinejad B. , Benson B. A. , Bleem L. E. , Calzadilla M. S. , Carlstrom J. E. , Chang C. L. , Chown R. , Crites A. T. , Haan T. de , Dobbs M. A. , Everett W. B. , Floyd B. , Grandis S. , George E. M. , Halverson N. W. , Holder G. P. , Holzapfel W. L. , Hrubes J. D. , Lee A. T. , Luong-Van D. , McDonald M. , McMahon J. J. , Meyer S. S. , Millea M. , Mocanu L. M. , Mohr J. J. , Natoli T. , Omori Y. , Padin S. , Pryke C. , Reichardt C. L. , Ruhl J. E. , Ruppin F. , Schaffer K. K. , Schrabback T. , Shirokoff E. , Staniszewski Z. , Stark A. A. , Vieira J. D. , Williamson R. 
Published: August 2022

Abstract
We provide the first combined cosmological analysis of the South Pole Telescope (SPT) and Planck cluster catalogs. The aim is to provide an independent calibration for Planck scaling relations, exploiting the cosmological constraining power of the SPT-SZ cluster catalog and its dedicated weak lensing (WL) and X-ray follow-up observations. We build a new version of the Planck cluster likelihood. In the νΛ CDM scenario, focusing on the mass slope and mass bias of Planck scaling relations, we find

α

SZ

=

1.49

−
0.10

+
0.07

and

1
−
b

SZ

=

0.69

−
0.14

+
0.07

, respectively. The results for the mass slope show a ∼4 σ departure from the self-similar evolution, α
SZ ∼ 1.8. This shift is mainly driven by the matter density value preferred by SPT data, Ω
m
= 0.30 ± 0.03, lower than the one obtained by Planck data alone,

Ω

m

=

0.37

−
0.06

+
0.02

. The mass bias constraints are consistent both with outcomes of hydrodynamical simulations and external WL calibrations, (1 − b) ∼ 0.8, and with results required by the Planck cosmic microwave background cosmology, (1 − b) ∼ 0.6. From this analysis, we obtain a new catalog of Planck cluster masses M
500. We estimate the ratio between the published Planck M
SZ masses and our derived masses M
500, as a “measured mass bias,”

1
−
b

M

. We analyze the mass, redshift, and detection noise dependence of

1
−
b

M

, finding an increasing trend toward high redshift and low mass. These results mimic the effect of departure from self-similarity in cluster evolution, showing different dependencies for the low-mass, high-mass, low-z, and high-z regimes.
Target and Velocity Dependence of Charge Exchange X-Ray Emission at Solar Wind Velocities
Authors: Zhang R. T. , Seely D. G. , Andrianarijaona V. M. , Jaeckel F. , Wulf D. , Morgan K. , McCammon D. , Havener C. C. 
Published: August 2022

Abstract
Laboratory measurements of X-ray emissions following charge exchange (CX) between highly charged ions and neutrals are important to assess their diagnostic utility for the nonequilibrium astrophysical plasma environments, where hot flows meet cold gases. With a high-resolution X-ray quantum microcalorimeter detector, we report the CX-induced X-ray spectra and line ratios in Ne8+ on He and Kr collisions at solar wind velocities of 392, 554, 678, and 876 km s−1, respectively. The experimentally determined line ratios quantify the differences in CX state selectivity and the following X-ray emission between He and Kr at different collision velocities. This suggests that target and velocity dependence should be considered for accurately modeling astrophysical CX plasmas.
Ionization Distributions in Outflows of Active Galaxies: Universal Trends and Prospect of Future XRISM Observations
Authors: Keshet Noa , Behar Ehud 
Published: August 2022

Abstract
The physics behind the ionization structure of outflows from black holes is yet to be fully understood. Using archival observations with the Chandra/HETG gratings over the past two decades, we measured an absorption measure distribution for a sample of outflows in nine active galactic nuclei (AGNs), namely the dependence of outflow column density, N
H, on the ionization parameter, ξ. The slope of

log

N
H versus

log
ξ

is found to be between 0.00 and 0.72. We find an anticorrelation between the log of total column density of the outflow and the log of AGN luminosity, and none with the black hole mass and accretion efficiency. A major improvement in the diagnostics of AGN outflows will potentially occur with the launch of the XRISM/Resolve spectrometer. We study the ability of Resolve to reveal the outflow ionization structure by constructing the absorption measure distribution from simulated Resolve spectra, utilizing its superior resolution and effective area. Resolve constrains the column density as well as HETG, but with much shorter observations.
Automated Filtering May Remove a Large Fraction of Records, But May Have Little Impact on Downstream Analyses
Authors: Zizka Alexander 
Published: August 2022

Species occurrence records provide the basis for many analyses in biodiversity research. They often derive from georeferenced specimens deposited in natural history collections or visual observations, such as those obtained through various mobile applications. Given the rapid increase in availability of such data, the control of quality and accuracy constitutes a particular concern. Automated flagging has emerged as a feasible way to identify potentially problematic records and correct them when possible, or, if a correction is not feasible, remove them from downstream analyses (automated filtering). A large number of flagging criteria exist, implemented in various software tools - reaching from simple flags, such as identifying zero coordinates, to more complex flags based on external data. These flags are widely applied for data cleaning in large-scale biodiversity analyses, yet their effect is rarely quantified.
Here, I present the rationale behind the automated flags included in the CoordinateCleaner R package (https://docs.ropensci.org/CoordinateCleaner/). CoordinateCleaner implementents functions to identify recurrent errors in biodiversity data compiled from different sources, and provides a user-friedly way to apply those functions in a pipeline to any dataset that can be loaded into R. Furthermore, I illustrate how many records these flags remove when used as filters across 18 taxa of plants, animal, and fungi from tropical America (Zizka et al. 2020b), and show results on the effect of automated filtering on the accuracy of automated conservation assessments using cleaned species occurrence records from biological collections (Zizka et al. 2020a).
The results show that, on average, almost half of the records in most datasets are flagged as potentially problematic, with large variation across taxonomic groups. Only around 5% of records was identified as erroneous in the strict sense, but a much larger proportion (20%) as unfit for common downstream analyses. Interestingly, automated filtering had little effect on the accuracy of automated red listing despite the large amount of records removed. This discrepancy may be caused by an interaction of data quality with sampling bias and the overall under-sampling of species ranges. Automated record filtering can help in identifying problematic records, but requires customization of tests and thresholds to the taxonomic group and geographic area under focus. The results stress the importance of thorough recording and exploration of the meta-data associated with species records for biodiversity research.
COVID-19 mass testing and sequencing: Experiences from a laboratory in Western Kenya
Authors: Waitumbi John N. , Omuseni Esther , Nyataya Josphat , Masakhwe Clement , Sigei Faith , Lemtudo Allan , Awinda George , Muthanje Eric , Andika Brian , Githii Rachel , Liyai Rehema , Kimita Gathii , Mutai Beth 
Published: August 2022

Background: The Basic Science Laboratory (BSL) of the Kenya Medical Research Institute/Walter Reed Project in Kisumu, Kenya addressed mass testing challenges posed by the emergent coronavirus disease 2019 (COVID-19) in an environment of global supply shortages. Before COVID-19, the BSL had adequate resources for disease surveillance and was therefore designated as one of the testing centres for COVID-19.Intervention: By April 2020, the BSL had developed stringent safety procedures for receiving and mass testing potentially infectious nasal specimens. To accommodate increased demand, BSL personnel worked in units: nucleic acid extraction, polymerase chain reaction, and data and quality assurance checks. The BSL adopted procedures for tracking sample integrity and minimising cross-contamination.Lessons learnt: Between May 2020 and January 2022, the BSL tested 63 542 samples, of which 5375 (8.59%) were positive for COVID-19; 1034 genomes were generated by whole genome sequencing and deposited in the Global Initiative on Sharing All Influenza Data database to aid global tracking of viral lineages. At the height of the pandemic (August and November 2020, April and August 2021 and January 2022), the BSL was testing more than 500 samples daily, compared to 150 per month prior to COVID-19. An important lesson from the COVID-19 pandemic was the discovery of untapped resilience within BSL personnel that allowed adaptability when the situation demanded. Strict safety procedures and quality management that are often difficult to maintain became routine.Recommendations: A fundamental lesson to embrace is that there is no ‘one-size-fits-all’ approach and adaptability is the key to success.
The contribution of family physicians to African health systems
Authors: Mash Robert 
Published: August 2022

Background: Africa is the last region to incorporate family physicians into its health systems. They are still a relatively new concept in many countries, small in numbers and deployed in a variety of ways. There is a need for more evidence on their contribution to African health systems to guide policymakers.Aim: The aim of this study was to review the special collection of short reports on the contribution of family physicians to African health systems, published in the African Primary Health Care and Family Medicine Journal in 2021.Method: Seventeen short reports from eight countries were qualitatively and thematically analysed in ATLAS.ti. Codes, which were derived inductively, were organised into categories according to the World Health Organization’s primary health care monitoring framework.Results: In the domain of health system determinants, family physicians made little contribution to governance, adjustment to population health needs or financing. They did, however, contribute substantially to the capacity of the health workforce, supply of equipment, functioning of the health information system and use of digital technologies. In the domain of service delivery, they strengthened the model of care and championed systems for improving the quality of care. This translated into improved availability and utilisation of services, core functions of primary care, quality of care and patient safety.Conclusion: Family physicians described their important contribution to service delivery in district hospitals and primary health care. This should lead to improvements in outcomes and impact for the health system. Their contribution to the concept of resilient facilities and health services needs further exploration.
Increasing unemployment rate amongst health professionals: Will there be jobs for newly graduated South African audiologists post-COVID-19?
Authors: Hlayisi Vera-Genevey 
Published: August 2022

Background: Before the coronavirus disease 2019 (COVID-19) pandemic in early 2020, the unemployment rate in South Africa was at its highest in history at 29.1%. During the COVID-19 pandemic to date, unemployment rose even higher to 35.3%. In this context, there has been an increase in the number of unemployed health professionals in South Africa.Objectives: This study aimed to determine the employment rates of newly graduated South African audiologists and identify the challenges in obtaining and maintaining employment for audiologists in South Africa.Methods: A descriptive online survey design was used. Participants were recruited online through professional association webpages using the snowball sampling technique. All qualified audiologists registered with the Health Professionals Council of South Africa were eligible to participate.Results: A total of 132 audiologists completed the survey. In the first-year postgraduation, 16% of the participants were unemployed, and this increased to 19% in the second-year postgraduation. In the majority (81%) of employed participants, almost a fifth (19%) were working within non-audiology/healthcare fields. The most common workplace challenges reported were remuneration (37%) followed by lack of resources (18%), workload (18%), work environment (10%), working hours (9%) and, lastly, interprofessional relationships (8%).Conclusion: Findings from this study are the first to document employment rates amongst South African audiologists. These findings have the potential to influence the critical discourse on hearing healthcare human resource planning, hearing healthcare labour capacity and potential for growth in the South African context post-COVID-19.
Incidence of diabetic ketoacidosis during Ramadan compared with non-fasting months in King Saud Medical City, Riyadh, Saudi Arabia
Authors: Alshahrani Mohsin , Alraddadi Ahmad 
Published: August 2022

Background:
Ramadan in Islam is the ninth month of the Muslim calendar and the holy month of fasting. In the fasting state, there is the danger of the blood glucose levels becoming too high when normal levels of medication are not taken. This can lead to diabetic ketoacidosis (DKA). The risk of diabetic emergencies, including DKA, is thought to be higher during Ramadan fasting due to metabolic changes and alterations in food habits. We aim to assess the incidence of DKA during Ramadan and perform a comparison pre and post month of Ramadan.

Methods:
This is a retrospective study that involves all adults who were admitted with DKA to King Saud Medical City in Riyadh, Saudi Arabia. We explored the relationship of admissions to Ramadan and compared it to the month before (Sha’aban) and the month after (Shawwal).

Results:
During the duration of the study, 51 patients with DKA were admitted to the hospital. Nineteen patients in Ramadan (37.3%), eight patients in Sha’aban (15.7%), and 24 patients in Shawwal (47%). This shows a significant increment in Ramadan compared to Sha’aban, and more increment in Shawwal (P = 0.019). The most common precipitating factor for diabetic ketoacidosis during Ramadan and Sha’aban is missing insulin dose, while infections are considered the main stimulating agent in Shawwal.

Conclusion:
There was an increase in the incidence of DKA episodes in Ramadan compared with the preceding month, but fewer DKA events compared to Shawwal, which might indicate that Ramadan fasting is a potential risk factor for DKA.