bluuebunny/crossref_metadata_2025_split huggingface dataset:
STRATEGI PESANTREN NURUL JADID DALAM MEMBANGUN JIWA ENTERPREUNEUR PADA SANTRI
Authors: Febrianto Achmad , Muslimah Muniva 
Published: August 2022

Entrepreneur merupakan gabungan dari kreativitas, inovasi dan keberanian menghadapi resiko yang dilakukan dengan cara kerja keras untuk membentuk dan memelihara produk baru. Entrepreneur dapat menjadi suatu profesi atau dunia kerja yang dapat memberikan ketangguhan dalam menghadapi resiko dan keadaan yang tidak menentu. Dalam menghadapi tantangan zaman ini, Selain mengajarkan pendidikan agama dan umum, Pondok Pesantren Nurul Jadid Paiton Probolinggo beriktiar untuk menyiapkan santrinya menjadi santri yang siap pakai dimasyarakat setelah keluar dari Pondok Pesantren Nurul Jadid dengan membekali ilmu Entrepreneur. Penelitian ini bermaksud menjelaskan rencana pesantren Nurul Jadid Paiton Probolinggo dalam membangun jiwa entrepreneurship pada santri melalui pengembangan kewirausahaan dan pelatihan berwirausaha. Metode penelitian yang digunakan adalah kualitatif deskriptif berdasarkan records kongkrit dari fenomena yang ada di lapangan serta menggunakan pendekatan participation motion studies untuk menghasilkan infomasi, pengetahuan, keterampilan, memecahkan masalah pada objek penelitian. Dari analisis yang dilakukan, ditemukan bahwa tidak semua santri mempunyai jiwa entrepreneur. Maka yang dilakukan oleh pesantren dalam membangun santri yang mempunyai jiwa Entrepreneur dapat memberi stimulus kepada santri dengan adanya pendidikan kewirausahaan, ekstrakulikuler tentang kewirausahaan, pendampingan pembuatan produk, seminar dan motivasi dalam berwirausaha. Wujud adanya ikhtiar membangun jiwa santripreuneur Pondok Pesantren Nurul Jadid dapat mengimplementasikan secara nyata yaitu dalam mendirikan minimarket (ENJHEmart) santri dan masyarakat serta membuka lapak / gerai yang memproduksi hasil olahan laut dengan tempat lokasi yang strategis yaitu (Gerinthink food).Kata Kunci : Pesantren dan Entrepreneur
KINERJA KEUANGAN NPO PADA RANAH JARINGAN SOSIAL, KEPERCAYAAN, DAN MODAL SPRITUAL
Authors: Hartono Setyo Budi , Ristianawati Yuyun 
Published: August 2022

Masyarakat pondok pesantren moderen, modal sosial dan modal spiritual adalah hal yang dapat menyebabkan perubahan pada setiap sendi kehidupan. Pengaruh diantara keduanya dapat mengubah posisi pondok pesantren terutama dalam hal kinerja keuangannya. Dengan RBT sebagai dasar untuk menjadi sentral dalam mengelola jaringan sosial dan kepercayaan pada kinerja keuangan pondok pesantren moderen. Populasi pondok pesantren 80% ada di Jawa Tengah, sehingga pengambilan sampel sebanyak 40 pondok pesantren dapat mewakili aspek pengukuran dalam penelitian ini. Pengukuran dilakukan dengan menggunakan kuesioner dengan indikator yang terdapat dalam variabel jaringan sosial, kepercayaan, modal spiritual, dan kinerja keuangan. Pengolahan data dilakukan dengan menggunakan software WarpPLS 5.0 dengan tipe sampel yang kecil. Hasil dari penelitian ini adalah variabel jaringan sosial dan kepercayaan berpengaruh signifikan dan positif terhadap kinerja keuangan dengan nilai pengaruh sebesar 23% dan 33%. Sementara jika di moderasi dengan modal spiritual memiliki pengaruh pada hubungan variabel jaringan sosial dan kepercayaan terhadap kinerja keuangan sebesar 28% dan 21%. Dengan demikian modal spiritual akan memperkuat pada kedua hubungan tersebut.Kata Kunci : jaringan sosial, kepercayaan, modal spiritual, kinerja keuangan.
DETERMINAN GAYA KEPEMIMPINAN DAN KOMUNIKASI TERHADAP KINERJA PENGELOLA BUMDES DI MASA PANDEMI
Authors: Wijayantini Bayu , Safitri Raudatul 
Published: August 2022

Pandemi Covid-19 sangat berpengaruh pada berbagai aspek kehidupan masyarakat. Namun atas segala keterpurukan itu ada beberapa usaha yang tetp bertahan dan diharapkan terus bekembang disaat krisis. Badan Usaha Milik Desa (BUMDes) dinilai menjadi salah satu elemen penting yang bisa memainkan peran membangkitkan dan menggairahkan perkonomian yang lesu di tengah pandemi. Penelitian ini bertujuan untuk mengetahui pengaruh gaya kepemimpinan dan komunikasi terhadap kinerja pengelola BUMDES di Desa Cangkring Kecamatan Jenggawah Kabupaten Jember, dimasa pandemi. Dari hasil Analisis dengan 32 responden yang menjadi sampel didapatkan hasil bahwa gaya kepemimpinan dan komunikasi berpengaruh terhadap terhadap kinerja pengelola BUMDES di Desa Cangkring Kecamatan Jenggawah Kabupaten Jember. Utamanya dalam masa pandemic covid -19 ini sangat memungkinkan terjadinya misskomunikasi dengan banyaknya informasi yang tersebar. Dengan adanya komunikasi yang baik diharapkan akan meminimalisir informasi hoax, sehingga kerjasama diantara pengelola Bumdes terjalin dengan baik, dan menjadi pendorong meningkatnya kinerja pengelola, guna memperkuat dan memajukan usaha BUMDes.Kata Kunci: Gaya Kepemimpinan; Komunikasi; dan Kinerja Karyawan, Pandemi Covid-19
SUMBER PENDANAAN, TEKNOLOGI INFORMASI, DAN KINERJA FINANSIAL PADA USAHA KECIL DAN MENENGAH PRA DAN SELAMA PANDEMI COVID-19
Authors: Hidayat Riskin , Sari Dian Anita 
Published: August 2022

This research test the mediating role of information technology on the influence of funding sources on the performance of SMEs before-during the COVID 19 pandemic. The sample of the study conducted is Coffee SMEs in Rembang Regency, which produces produces “Lelet Coffee”. In this study, all members of the population were sampled as 50 samples, but only 48 samples could be processed, because two samples were damage. The data analysis technique used path analysis with PLS. Test results show that funding sources had a significant positive impact on the performance of Lelet Coffee SMEs both pre-pandemic and during the Covid 19 pandemic. Similarly, when it is mediated through information technology, it can be seen that funding sources before and during the Covid 19 pandemic have a significant indirect impact on the performance of Coffee SMEs pre and during the covid-19 pandemic. In addition, the study shows that information technology has a significant positive impact on the performance of Coffee SMEs. This means that digital technology will play a very important role in driving the impact of funding sources on the financial performance of Rembang Regency's Coffee SMEs.Kata Kunci : funding sources, information technology, SME financial performance, covid-19 pandemic
Overview of the Remote Sensing Observations from PSP Solar Encounter 10 with Perihelion at 13.3 R
⊙
Authors: Howard Russell A. , Stenborg Guillermo , Vourlidas Angelos , Gallagher Brendan M. , Linton Mark G. , Hess Phillip , Rich Nathan B. , Liewer Paulett C. 
Published: August 2022

Abstract
The closest perihelion pass of Parker Solar Probe (PSP), so far, occurred between 2021 November 16 and 26 and reached ∼13.29 R
☉ from Sun center. This pass resulted in very unique observations of the solar corona by the Wide-field Instrument for Solar PRobe (WISPR). WISPR observed at least 10 coronal mass ejections (CMEs), some of which were so close that the structures appear distorted. All of the CMEs appeared to have a magnetic flux rope (MFR) structure, and most were oriented such that the view was along the axis orientation, revealing very complex interiors. Two CMEs had a small MFR develop in the interior, with a bright circular boundary surrounding a very dark interior. Trailing the larger CMEs were substantial outflows of small blobs and flux-rope-like structures within striated ribbons, lasting for many hours. When the heliospheric plasma sheet was inclined, as it was during the days around perihelion on 2021 November 21, the outflow was over a very wide latitude range. One CME was overtaken by a faster one, with a resultant compression of the rear of the leading CME and an unusual expansion in the trailing CME. The small Thomson surface creates brightness variations of structures as they pass through the field of view. In addition to this dynamic activity, a brightness band from excess dust along the orbit of asteroid/comet 3200 Phaethon is also seen for several days.
On the Nature of the Mass-gap Object in the GW190814 Event
Authors: Lopes Luiz L. , Menezes Debora P. 
Published: August 2022

Abstract
In this work, we conduct an extensive study of the conditions that allow the mass-gap object in the GW190814 event to be faced as a degenerate star instead of a black hole. We begin by revisiting some parameterizations of quantum hadrodynamics and then study under which conditions hyperons are present in such a massive star. Afterward, using a vector MIT-based model, we study whether self-bound quark stars, satisfying the Bodmer–Witten conjecture, fulfill all the observational constraints. Finally, we study hybrid stars within a Maxwell construction and check for what values of the bag, as well as the vector interaction, a quark core star with only nucleons, and with nucleons admixed with hyperons can reach at least 2.50 M
⊙. We conclude that, depending on the choice of parameters, none of the possibilities can be completely ruled out, i.e., the mass-gap object can be a hadronic (either nucleonic or hyperonic), a quark, or a hybrid star, although some cases are more probable than others.
Two-dimensional Configuration and Temporal Evolution of Spark Discharges in Pulsars
Authors: Basu Rahul , Melikidze George I. , Mitra Dipanjan 
Published: August 2022

Abstract
We report on our investigation of the evolution of a system of spark discharges in the inner acceleration region (IAR) above the pulsar polar cap. The surface of the polar cap is heated to temperatures of around 106 K and forms a partially screened gap (PSG), due to thermionic emission of positively charged ions from the stellar surface. The spark lags behind corotation speed during their lifetimes due to variable E × B drift. In a PSG, spark discharges arise in locations where the surface temperatures go below the critical level (T

i
) for ions to freely flow from the surface. The spark commences due to the large drop in potential developing along the magnetic field lines in these lower temperature regions and subsequently back-streaming particles heat the surface to T

i
. Regulation of the temperature requires the polar cap to be tightly filled with sparks and a continuous presence of sparks is required around its boundary since no heating is possible from the closed field line region. We estimate the time evolution of the spark system in the IAR, which shows a gradual shift in the spark formation along two distinct directions resembling clockwise and anticlockwise motions in two halves of the polar cap. Due to the differential shift of the spark pattern in the two halves, a central spark develops representing the core emission. The temporal evolution of the spark process was simulated for different orientations of a non-dipolar polar cap and reproduced the diverse observational features associated with subpulse drifting.
Investigation of the Broadband Emission of the Gamma-Ray Binary HESS J0632+057 Using an Intrabinary Shock Model
Authors: Kim Jinyoung , An Hongjun , Mori Kaya 
Published: August 2022

Abstract
We investigated a wealth of X-ray and gamma-ray spectral energy distribution (SED) and multiband light-curve (LC) data of the gamma-ray binary HESS J0632+057 using a phenomenological intrabinary shock (IBS) model. Our baseline model assumes that the IBS is formed by colliding winds from a putative pulsar and its Be companion and that particles accelerated in the IBS emit broadband radiation via synchrotron (SY) and inverse Compton upscattering (ICS) processes. Adopting the latest orbital solution and system geometry, we reproduced the global X-ray and TeV LC features, two broad bumps at ϕ ∼ 0.3 and ∼0.7, with the SY and ICS model components. We found that these TeV LC peaks originate from ICS emission caused by the enhanced seed photon density near periastron and superior conjunction or Doppler-beamed emission of bulk-accelerated particles in the IBS at inferior conjunction. While our IBS model successfully explained most of the observed SED and LC data, we found that phase-resolved SED data in the TeV band require an additional component associated with ICS emission from preshock particles (produced by the pulsar wind). This finding indicates a possibility of delineating the IBS emission components and determining the bulk Lorentz factors of the pulsar wind at certain orbital phases.
Mid-infrared and Maser Flux Variability Correlation in Massive Young Stellar Object G036.70+00.09
Authors: Uchiyama Mizuho , Ichikawa Kohei , Sugiyama Koichiro , Tanabe Yoshihiro , Yonekura Yoshinori 
Published: August 2022

Abstract
We present the discovery of the simultaneous flux variation of a massive young stellar object (MYSO) G036.70+00.09 (G036.70) both in the maser emission and mid-infrared (MIR; λ = 3–5 μm) bands. Using the ALLWISE and NEOWISE archival databases that cover a long time span of approximately 10 yr with a cadence of 6 months, we confirm that G036.70 indicates a stochastic year-long MIR variability with no signs of a WISE band color change of W1 (3.4 μm) −W2 (4.6 μm). Cross-matching the MIR data set with the high-cadence 6.7 GHz class II methanol maser flux using the Hitachi 32 m radio telescope that discovered its periodicity in the methanol maser of 53.0–53.2 days, we also determine the flux correlations between the two bands at two different timescales, year-long and day-long, both of which have never been reported in MYSOs, except when they are in the accretion burst phase. The results of our study support the scenario that a class II methanol maser is pumped up by infrared emission from accreting disks of MYSOs. We also discuss the possible origins of MIR and maser variability. To explain the two observed phenomena, a stochastic year-long MIR variability with no signs of significant color change and maser-MIR variability correlation or a change in mass accretion rate and line-of-sight extinction because of the nonaxisymmetric dust density distribution in a rotating accretion disk are possible origins. Observations through spectroscopic monitoring of accretion-related emission lines are essential for determining the origin of the observed variability in G036.70.
First Peek with JWST/NIRCam Wide-field Slitless Spectroscopy: Serendipitous Discovery of a Strong [O iii]/Hα Emitter at z = 6.11
Authors: Sun Fengwu , Egami Eiichi , Pirzkal Nor , Rieke Marcia , Boyer Martha , Correnti Matteo , Gennaro Mario , Girard Julien , Greene Thomas P. , Kelly Doug , Koekemoer Anton M. , Leisenring Jarron , Misselt Karl , Nikolov Nikolay , Roellig Thomas L. , Stansberry John , Williams Christina C. , Willmer Christopher N. A. ,   (Members of the JWST/NIRCam Commissioning Team)
Published: August 2022

Abstract
We report the serendipitous discovery of an [O iii] λ
λ4959/5007 and Hα line emitter in the Epoch of Reionization (EoR) with the James Webb Space Telescope (JWST) commissioning data taken in the NIRCam wide-field slitless spectroscopy (WFSS) mode. Located ∼55″ away from the flux calibrator P330-E, this galaxy exhibits bright [O iii] λ
λ4959/5007 and Hα lines detected at 3.7σ, 9.9σ, and 5.7σ, respectively, with a spectroscopic redshift of z = 6.112 ± 0.001. The total Hβ+[O iii] equivalent width is 664 ± 98 Å (454 ± 78 Å from the [O iii] λ5007 line). This provides direct spectroscopic evidence for the presence of strong rest-frame optical lines (Hβ+[O iii] and Hα) in EoR galaxies as inferred previously from the analyses of the Spitzer/IRAC spectral energy distributions (SEDs). Two spatial and velocity components are identified in this source, possibly indicating that this system is undergoing a major merger, which might have triggered the ongoing starburst with strong nebular emission lines over a timescale of ∼2 Myr, as our SED modeling suggests. The tentative detection of He ii
λ4686 line (1.9σ), if real, may indicate the existence of very young and metal-poor star-forming regions with a hard UV radiation field. Finally, this discovery demonstrates the power and readiness of the JWST/NIRCam WFSS mode, and marks the beginning of a new era for extragalactic astronomy, in which EoR galaxies can be routinely discovered via blind slitless spectroscopy through the detection of rest-frame optical emission lines.
On the Hydrosphere Stability of TESS Targets: Applications to 700 d, 256 b, and 203 b
Authors: Bonney Paul , Kennefick Julia 
Published: August 2022

Abstract
A main determinant of the habitability of exoplanets is the presence of stable liquid surface water. In an era of abundant possible targets, the potential to find a habitable world remains a driving force in prioritization. We present here a data-forward method to investigate the likelihood of a stable hydrosphere on the timescales of the formation of life, 1 Gyr, and beyond. As our primary application, we use this method to examine the potential hydrospheres of TESS objects of interest 700 d, 256 b (LHS 1140 b), and 203 b. We first present our selection criteria, which are based on an implementation of the Earth Similarity Index, as well as the results of an initial investigation into the desiccation of the targets, which reveals that TOI 203 b is almost certainly desiccated based on TESS observations. We then describe the characterization of the remaining targets and their host stars from 2MASS, Gaia, and TESS data and the derivation of sampled probability distributions for their parameters. Following this, we describe our process of simulating the desiccation of the targets’ hydrospheres using the Virtual Planet Simulator, VPlanet, with inputs directly linked to the previously derived probability distributions. We find that 50.86% of the likely cases for TOI 700 d are desiccated, and no modeled cases for TOI 256 b are without water. In addition, we calculate the remaining water inventory for the targets, the percentage of cases that are continuing to lose water, and the rate at which these cases are losing water.
NLRP3 Inflammasome Priming and Activation Are Regulated by a Phosphatidylinositol-Dependent Mechanism
Authors: Hamilton Claire , Olona Antoni , Leishman Stuart , MacDonald-Ramsahai Kelly , Cockcroft Shamshad , Larrouy-Maumus Gerald , Anand Paras K 
Published: August 2022

Abstract
Imbalance in lipid homeostasis is associated with discrepancies in immune signaling and is tightly linked to metabolic disorders. The diverse ways in which lipids impact immune signaling, however, remain ambiguous. The phospholipid phosphatidylinositol (PI), which is implicated in numerous immune disorders, is chiefly defined by its phosphorylation status. By contrast, the significance of the two fatty acid chains attached to the PI remains unknown. In this study, by using a mass spectrometry–based assay, we demonstrate a role for PI acyl group chains in regulating both the priming and activation steps of the NOD-like receptor family pyrin domain-containing 3 (NLRP3) inflammasome in mouse macrophages. In response to NLRP3 stimuli, cells deficient in ABC transporter ATP Binding Cassette Subfamily B Member 1 (ABCB1), which effluxes lipid derivatives, revealed defective inflammasome activation. Mechanistically, Abcb1 deficiency shifted the total PI configuration exhibiting a reduced ratio of short-chain to long-chain PI acyl lipids. Consequently, Abcb1 deficiency initiated the rapid degradation of Toll/IL-1R domain–containing adaptor protein, the TLR adaptor protein that binds PI (4,5)-bisphosphate, resulting in defective TLR-dependent signaling, and thus NLRP3 expression. Moreover, this accompanied increased NLRP3 phosphorylation at the Ser291 position and contributed to blunted inflammasome activation. Exogenously supplementing wild-type cells with linoleic acid (LA), but not arachidonic acid, reconfigured PI acyl chains. Accordingly, LA supplementation increased Toll/IL-1R domain–containing adaptor protein degradation, elevated NLRP3 phosphorylation, and abrogated inflammasome activation. Furthermore, NLRP3 Ser291 phosphorylation was dependent on PGE2-induced protein kinase A signaling because pharmacological inhibition of this pathway in LA-enriched cells dephosphorylated NLRP3. Altogether, our study reveals, to our knowledge, a novel metabolic-inflammatory circuit that contributes to calibrating immune responses.
Use of Aedes aegypti Oviposition Surveillance and a Geographic Information System for Planning Anti-Vectorial Measures
Authors: Abán Moreyra Daira N. , Castillo Paola M. , Escalada Andrés , Mangudo Carolina , Copa Griselda N. , Gleiser Raquel M. , Nasser Julio R. , Gil José F. 
Published: August 2022

ABSTRACT.
Arboviruses transmitted by Aedes aegypti pose a threat to global public health. Because there are no vaccines or drugs available, the prevention of these diseases in Argentina is based on integrated vector control. In this work, the spatiotemporal dynamics of the vector distribution was analyzed by monitoring oviposition. This information allowed the planning of anti-vector interventions and the evaluation of their effect on the relative abundance of mosquito populations in San Ramón de la Nueva Orán. Observed data were compared with the eggs expected via a statistical model based on meteorological variables. The oviposition substrate preference of mosquito females was also evaluated, and the possible relationship between the relative abundance of the vector and sociodemographic and environmental variables (normalized difference vegetation index and normalized difference water index) was explored. A total of 4,193 eggs of Ae. aegypti were collected, and spatial clusters were detected for all months for which the presence of the mosquito was reported. The observed number of eggs was significantly less than the expected-corrected egg abundance. A significant correlation of oviposition activity was found with three sociodemographic variables, whereas no significant correlation was found with mean or median values of the environmental variables studied. This monitoring strategy made it possible to address the interventions and evaluate them, proposing them as good complementary tools for the control of Ae. aegypti in northern Argentina.
Case Report: Bloodstream Infection with Toxigenic Corynebacterium diphtheriae and Gram-Negative Sepsis in a Child with Burns
Authors: Jamir Imola , Ketan Priyadarshi , Anguraj Symphonia , Jahan Lulu , Parameswaran Narayanan , Divakarjose Rajeswari Rethinaswamy , Sastry Apurba Sankar 
Published: August 2022

ABSTRACT.
Corynebacterium (C.) diphtheriae is the agent for a contagious infection, diphtheria. It may manifest as pharyngitis with pseudomembrane formation and cervical lymphadenopathy, cutaneous infection, or as an asymptomatic carrier. Corynebacterium (C.) diphtheriae is not an invasive organism and it remains in the superficial layers of skin lesions and respiratory mucosa. Systemic complications, such as bacteremia, are rare. We report a case of toxigenic C. diphtheriae detected from blood culture of a 1-year-old male patient with burns, who succumbed to the infection after 8 days of stay in the hospital. Patient did not have specific clinical features suggestive of diphtheria. Initial identification of C. diphtheriae was done based on culture, Albert stain findings, biochemical tests and subsequently toxigenicity testing was done by polymerase chain reaction. Although diphtheria vaccination in infancy is universally recommended since the creation of the Expanded Program on Immunization in the 1970s, there have been reports of toxigenic strains of C. diphtheriae in a considerable number of cases. Rapid and accurate identification of C. diphtheriae infection is crucial to prevent mortality. Continued surveillance for diphtheria is needed to reduce transmission and mortality rates.