bluuebunny/crossref_metadata_2025_split huggingface dataset:
Disorders of Sex Development: New Concepts of Diagnostics and Management in Children
Authors: Солнцева А.В. 
Published: March 2022

Нормальное половое развитие зависит от взаимодействия активирующих и подавляющих факторов в конкретном пространственно-временном паттерне. Нарушения формирования пола (НФП) включают в себя гетерогенную группу врожденных состояний, связанных с атипичным развитием внутренних и наружных половых органов. Они могут быть ассоциированы с изменениями в генах, программировании дифференцировки пола и гормонального статуса. НФП можно разделить на несколько групп, включая хромосомные, гонадные и анатомические аномалии. Генетические инструменты, такие как анализ микрочипов и методы секвенирования следующего поколения, позволили выявить новые генетические варианты среди детей с НФП. Ведение пациента с НФП должно быть индивидуализированным, особенно при решении вопросов, связанных с половым воспитанием, хирургической коррекцией, гормональным лечением и возможностью сохранения фертильности.
Normal sex development depends on the precise space-time sequence and coordination of mutually antagonistic activating and repressing factors. Disorders of sex development include a heterogenous group of congenital conditions associated with atypical development of internal and external genitalia. These conditions can be associated with variations in genes, developmental programming, and hormones. Disorders of sex development can be classified into several groups, including chromosomal, gonadal, and anatomic abnormalities. Genetic tools such as microarray analyses and next-generation sequencing techniques let to identify new genetic variants among children with disorders of sex development. Patient management needs to be individualized, especially in decisions related to sex education, surgical interventions, hormone treatment, and potential for fertility preservation.
Extracholecystostomic Endobiliary Correction of the Papilla Vatery Stricture: A Case Report
Authors: Орловский Ю.Н. , Салмин И.М. , Сазонов М.В. , Кутько А.П. , Пушков И.Е. , Глыздов А.П. 
Published: March 2022

В статье описывается клиническое наблюдение пациента с доброкачественной стриктурой большого дуоденального сосочка. Показаны трудности выбора лечебной тактики у данного пациента, а также продемонстрирована эффективность комбинированного малоинвазивного лечения с использованием антеградной чрезхолецистостомической эндобилиарной и ретроградной эндоскопической коррекции стриктуры большого дуоденального сосочка (методика Rendezvoux).Данная патология развивается наиболее часто при холангиолитиазе, рецидивирующих холангитах, хроническом панкреатите. Существуют различные варианты изолированных малоинвазивных вмешательств (эндоскопические, антеградные под УЗ- и рентген-контролем), а также комплексные, которые объединяют антеградные чреспеченочные и ретроградные эндоскопические.Комплексным вмешательствам на сегодняшний день отдается предпочтение при неэффективности изолированных манипуляций, а также при сложном холангиолитиазе, выраженной деформации двенадцатиперстной кишки, рубцовом процессе в зоне папиллы, хирургических вмешательствах с измененной анатомией панкреатодуоденобилиарной зоны. Эта методика хорошо себя зарекомендовала, ее эффективность достигает 85–100%, при этом частота осложнений составляет 3–10%, а летальность – менее 1%.
The article describes a case report of a patient with a benign stricture of the papilla Vatery. The difficulties in choosing the treatment tactics in this patient are shown, and the effectiveness of combined minimally invasive treatment with the use of antegrade transcholecystostomy endobiliary and retrograde endoscopic correction of the stricture of the papilla Vatery (Rendezvoux technique) is demonstrated.This pathology develops most often with cholangiolithiasis, recurrent cholangitis, chronic pancreatitis. There are various options for isolated low-invasive interventions (endoscopic, antegrade under ultrasound and X-ray control), as well as complex ones that combine antegrade transhepatic and retrograde endoscopic.Today, complex interventions are preferred in cases of ineffectiveness of isolated manipulations, as well as in complex cholangiolithiasis, pronounced deformity of the duodenum, cicatricial process in the papilla zone, surgical interventions with altered anatomy of the pancreatoduodenobiliary zone. This technique has proven itself well and its effectiveness reaches 85–100%, while the complication rate is 3–10%, and the mortality rate is less than 1%.
CONSTRUCTION OF WAQF ACCOUNTING BASED ON PSAK 112
Authors: Nawirah Nawirah , Fikri Mohamat Chazim 
Published: March 2022

ABSTRAKTujuan penelitian ini adalah untuk menganalisis dan mengkontruksi laporan keuangan wakaf. Jenis penelitian ini merupakan penelitian kualilitatif menggunakan pendekatan deskriptif. Objek penelitian adalah Koperasi Masjid Sabilillah Kota Malang. Teknik Analisis digunakan dengan tujuan untuk mengetahui bagaimana perlakuan wakaf tunai yang diterima pengurus Koperasi Masjid Sabilillah Kota Malang, wakaf tunai akan ditinjau berdasarkan PSAK 112 dengan melihat perlakuan akuntansi wakaf. Tahapan selanjutnya kemudian melakukan kontruksi laporan keuangan sesuai dengan standart akuntansi wakaf yang telah disahkan oleh Ikatan Akuntan Indonesia. Penelitian ini memberikan hasil bahwa perlakuan akuntansi sesuai PSAK 112 secara umum menunjukkan baik serta transparan dalam hal penyampain informasi penerimaan wakaf tunai. Koperasi Masjid Sabilillah telah membuat Laporan keuangan yakni laporan laba rugi, laporan arus kas serta Laporan posisi keuangan. Terdapat beberapa laporan yang belum dibuat jika merujuk ke PSAK 112 yakni laporan aktivitas wakaf, laporan perubahan aset wakaf dan catatan atas laporan keuangan.Kata Kunci: Wakaf, Laporan Keuangan, PSAK 112 ABSTRACTThe purpose of this research is to examine and create waqf financial accounts. This study is a sort of qualitative research that takes a descriptive method. This study was carried out at the Sabilillah Mosque Cooperative in Malang City. The analysis technique was carried out to determine the treatment of cash waqf received by the management of the Sabilillah Mosque Cooperative Malang City. The cash waqf was reviewed based on the waqf accounting treatment referred to in PSAK 112, and the financial statements were constructed in accordance with the waqf accounting standards approved by the Indonesian Institute of Accountants. In general, the findings revealed that accounting treatment to PSAK 112 was good and straightforward in transmitting information on cash waqf receipts. The financial statements that have been made by the Sabilillah Mosque Cooperative as the management of the cooperative are the income statement, cash flow statement and balance sheet. There are several reports that have not been made when referring to PSAK 112, namely reports are waqf activity reports, reports on changes in waqf assets and notes to financial statements.Keywords: Waqf, Financial Reports, PSAK 112
IMPLEMENTASI METODE WEIGHTED PRODUCT UNTUK PEMILIHAN KARYAWAN TELADAN BERBASIS WEB PADA PT. DANA PURNA INVESTAMA
Authors: Arya Faturahman Dimas , Mufti Mufti 
Published: March 2022

Perkembangan perusahaan sangat dipengaruhi oleh kinerja sumber daya manusia, sehingga setiap perusahaan akan berusaha mendapatkan karyawan yang berkualitas. PT. DPI(Dana Purna Investama), merupakan perusahaan yang bergerak dibidang pengelolaan fasilitas gedung serta menjalankan kegiatan usaha dibidang jasa pelatihan & keterampilan tenaga kerja. Penilaian dirasa perlu untuk meningkatkan kinerja dan semangat kerja karyawan dimana perusahaan dimungkinkan memberikan reward(penghargaan). Sebelumnya, belum ada sistem dapat mengambil keputusan untuk menentukan karyawan teladan dan pelaksanaannya yang masih dilakukan secara manual atau belum memiliki standar dalam penilaian, aturan dan perhitungan nilai. Oleh karna itu dalam penelitian ini dibuatlah sistem pemilihan karyawan teladan dengan menggunakan metode Weighted Product karena dapat mengevaluasi alternatif terhadap beberapa kriteria yang tidak saling bergantungan yang dibuat dengan bahasa pemrograman PHP berbasis web. Proses normalisasi pada metode ini yaitu dengan melakukan pemangkatan nilai atau rating alternatif kriteria dengan nilai bobot dari masing-masing kriteria yang kemudian dikalikan. Berdasarkan hasil uji coba yang dilakukan pada sistem pemilihan ini, aplikasi ini dapat membantu memberikan acuan dalam menentukan karyawan teladan berdasarkan kriteria-kriteria yang diberikan. Dengan adanya sistem penilaian karyawan teladan yang menggunakan metode Weighted Product ini dapat dipergunakan sebagai salah satu alat untuk pengambilan keputusan dalam memilih karyawan yang layak.
IMPLEMENTASI ALGORITME AES 128 UNTUK APLIKASI SERAH TERIMA DOKUMEN PROJECT PADA PT TELKOMSIGMA
Authors: Rusnadi Dahlia Damayanti , Juliasari Noni 
Published: March 2022

Telkomsigmamempunyai data yang penting untuk disimpan dalam komputer. Namun jika data disimpan tetapi tidak ada dengan pengamanan yang baik maka data tersebut mudah dicuri atau diubah oleh yang tidak berkepentingan dengan data tersebut. Proses serah terima pekerjaan secara manual rentan terhadap kerahasiaan dokumen karena proses serah terima secara manual biasanya mengirimkan dokumen dalam bentuk hardcopy. Oleh karena itu diperlukan suatu aplikasi yang dapat membantu proses serah terima pekerjaan tersebut. Dengan mengutamakan keamanan pada dokumen yang dikirim diperlukan metode pengamanan dengan systemkriptografi. Metode yang digunakan adalah Advanced Encryption Standard (AES) 128 dengan menggunakan kunci enkripsi dan dekripsi yang sama. Dengan adanya aplikasi ini diharapkan proses serah terima pekerjaan menjadi lebih mudah dan aman, sehingga dokumen yang diserahterimakan dapat tersampaikan dengan tepat.
Implementasi Fungsi Actuating dalam Meningkatkan Jumlah Jama’ah Majelis Subuhan al Busyro Bangil Pasuruan
Authors: Avisena Ahmad , Ulum Muhamad Bahrul 
Published: March 2022

Sebagai salah satu lembaga non-formal di masyarakat, Majelis Shubuhan Al-Busyro Bangil Pasuruan menjadi sarana yang potensial dalam menyampaikan dakwah dan membina masyarakat. Peningkatan jama’ah majelis tersebut meningkat dengan drastis dan pesat dalam wilayah perkotaan di mana para jama’ah mempunyai kesibukan yang padan dan tidak mempunyai banyak waktu untuk mempelajari ilmu agama. Tujuan penelitian ini yakni mengkaji tiga hal. 1) bagaimana impelentasi fungsi actuating dalam meningkatkan jumlah jama’ah di Majelis Subuhan Al-Busyro 2) bagaimana hasil dari impelentasi fungsi actuating dalam meningkatkan jumlah jama’ah di Majelis Subuhan Al-Busyro 3) faktor pendukung dan penghambat impelentasi fungsi actuating dalam meningkatkan jumlah jama’ah di Majelis Subuhan Al-Busyro. Peneliti memilih field research sebagai pendekatan dalam penelitian ini. Field reasearch digunakan sebagai metode untuk mengumpulkan data kualitatif. Sedangkan penelitian ini menggunakan jenis penelitian deskriptif kualitatif. Hasil dari penelitian ini adalah (1) Implementasi fungsi actuating menggunakan empat proses yaitu pemberian motivasi, bimbingan, menjalin hubungan yang harmonis antara pengurus dengan jama’ah serta komunikasi yang baik; (2) hasil dari implementasi fungsi actuating yaitu: bertambahnya jumlah jama’ah yang mengikuti majelis taklim dan juga Bertambahnya progam kerja yang ada; (3) faktor pendukung antara lain: adanya dukungan masyarakat, sumber daya manusia yang kompeten dan sarana prasarana yang cukup. Sedangkan faktor penghambatnya yaitu: kurangnya kedisiplinan jama’ah dan kesibukan para jama’ah.
THE BASIC PRINCIPLES OF THE IDEAL ISLAMIC SOCIETY (KHAIR UMMAH) IN MAINTAINING RELIGIOUS SOLIDARITY IN THE ISLAMIC WORLD.
Authors: Abdul Syukur  , Muhajir  , Eko Subroto  
Published: March 2022

Abstract
Every Muslim is obliged to invite others to the good and forbid them from bad deeds. In the Qur'an, Allah SWT mentions the characteristics of khairu ummah. Khairu ummah can be a glorious achievement for Muslims as illustrated in the verse of Allah above if the characteristics of khairu ummah are fulfilled. There are at least three characteristics that must be fulfilled, namely amar ma'ruf, nahi mungkar, and faith in Allah. This research uses a qualitative research approach based on its characteristics with the category of library research.
Snails across Scales: Local and Global Phase-mixing Structures as Probes of the Past and Future Milky Way
Authors: Gandhi Suroor S. , Johnston Kathryn V. , Hunt Jason A. S. , Price-Whelan Adrian M. , Laporte Chervin F. P. , Hogg David W. 
Published: March 2022

Abstract
Signatures of vertical disequilibrium have been observed across the Milky Way’s (MW’s) disk. These signatures manifest locally as unmixed phase spirals in z–v

z
space (“snails-in-phase”), and globally as nonzero mean z and v

z
, wrapping around the disk into physical spirals in the x–y plane (“snails-in-space”). We explore the connection between these local and global spirals through the example of a satellite perturbing a test-particle MW-like disk. We anticipate our results to broadly apply to any vertical perturbation. Using a z–v

z
asymmetry metric, we demonstrate that in test-particle simulations: (a) multiple local phase-spiral morphologies appear when stars are binned by azimuthal action J

ϕ
, excited by a single event (in our case, a satellite disk crossing); (b) these distinct phase spirals are traced back to distinct disk locations; and (c) they are excited at distinct times. Thus, local phase spirals offer a global view of the MW’s perturbation history from multiple perspectives. Using a toy model for a Sagittarius (Sgr)–like satellite crossing the disk, we show that the full interaction takes place on timescales comparable to orbital periods of disk stars within R ≲ 10 kpc. Hence such perturbations have widespread influence, which peaks in distinct regions of the disk at different times. This leads us to examine the ongoing MW–Sgr interaction. While Sgr has not yet crossed the disk (currently, z
Sgr ≈ −6 kpc, v

z,Sgr ≈ 210 km s−1), we demonstrate that the peak of the impact has already passed. Sgr’s pull over the past 150 Myr creates a global v

z
signature with amplitude ∝ M
Sgr, which might be detectable in future spectroscopic surveys.
Exploring the Milky Way Circumgalactic Medium in a Cosmological Context with a Semianalytic Model
Authors: Faerman Yakov , Pandya Viraj , Somerville Rachel S. , Sternberg Amiel 
Published: March 2022

Abstract
We combine the Santa Cruz semianalytic model (SAM) for galaxy formation and evolution with the circumgalactic medium (CGM) model presented in Faerman et al. to explore the CGM properties of L
* galaxies. We use the SAM to generate a sample of galaxies with halo masses similar to the Milky Way (MW) halo, M
vir ≈ 1012
M
⊙, and find that the CGM mass and mean metallicity in the sample are correlated. We use the CGM masses and metallicities of the SAM galaxies as inputs for the FSM20 model and vary the amount of nonthermal support. The density profiles in our models can be approximated by power-law functions with slopes in the range of 0.75 < a

n
< 1.25, with higher nonthermal pressure resulting in flatter distributions. We explore how the gas pressure, dispersion measure, O VI–O VIII column densities, and cooling rates behave with the gas distribution and total mass. We show that for CGM masses below ∼3 × 1010
M
⊙ photoionization has a significant effect on the column densities of O VI and O VIII. The combination of different MW CGM observations favors models with similar fractions in thermal pressure, magnetic fields/cosmic rays, and turbulent support and with M
CGM ∼ (3–10) × 1010
M
⊙. The MW O VI column requires t
cool/t
dyn ∼ 4, independent of the gas distribution. The AGN jet-driven heating rates in the SAM are enough to offset the CGM cooling, although exact balance is not required in star-forming galaxies. We provide predictions for the column densities of additional metal ions—N V, Ne VIII, and Mg X.
Determining Star Formation Rates of Active Galactic Nucleus Host Galaxies Based on SED Fitting with Submillimeter Data
Authors: Kim Changseok , Woo Jong-Hak , Jadhav Yashashree , Chung Aeree , Baek Junhyun , Lee Jeong Ae , Shin Jaejin , Hwang Ho Seong , Luo Rongxin , Son Donghoon , Kim HyunGi , Woo Hyuk 
Published: March 2022

Abstract
We present the star formation rate (SFR) measurements based on the spectral energy distribution (SED) analysis with new submillimeter fluxes combined with archival multiwavelength data for a sample of 52 active galactic nucleus (AGN) host galaxies at z < 0.2. We carried out submillimeter observations using the SCUBA-2 camera at the James Clerk Maxwell Telescope and obtained flux or an upper limit at 450 and 850 μm for each target. By experimenting with the effect of the AGN dust component in the SED fit, we find that the dust luminosity can be overestimated if the AGN contribution is ignored. While the SFR based on the 4000 Å break shows a significant offset compared to the dust-luminosity-based SFR, the SFR obtained by the artificial neural network generally shows consistency, albeit with a large scatter. We find that SFR correlates with the AGN outflow strength manifested by the [O iii] λ5007 emission line, and that AGNs with higher Eddington ratios and stronger outflows are generally hosted by galaxies with a higher SFR, which is consistent with the correlation reported by Woo et al. This suggests no instantaneous quenching of star formation due to AGN feedback.
On the Use of CHIME to Detect Long-duration Radio Transients from Neutron Star Mergers
Authors: Shikauchi Minori , Cannon Kipp , Lin Haoxiang , Totani Tomonori , Shaw J. Richard 
Published: March 2022

Abstract
The short gamma-ray burst (SGRB) GRB 170817A was found to be related to a binary neutron star (BNS) merger. It is uncertain whether all SGRBs are caused by BNS mergers and also under what conditions a BNS merger can cause an SGRB. As BNS mergers can cause SGRBs, afterglow observations will also provide an alternative measurement of the BNS merger rate independent of gravitational-wave observations. In previous work by Feng et al., the feasibility of the detection of afterglows was considered using a variety of radio observatories and a simple flux threshold detection algorithm. Here, we consider a more sophisticated detection algorithm for SGRB afterglows and provide an estimate of the trials factors for a realistic search to obtain an updated estimate of the possibility of observing afterglows with the Canadian Hydrogen Intensity Mapping Experiment (CHIME). We estimate 893 and 312 afterglows per year can be detected using a 3σ confidence level threshold with two jet models, one with half-opening angle uniformly distributed in 6°–30° and the other uniformly distributed in 3°–8° with the median of 6°. We also find that 88% and 98%, respectively, of the detectable afterglows for each jet-opening distribution are off axis, which are candidates for orphan afterglows. Our result predicts fewer detectable sources per year than the earlier analysis but confirms the essential conclusion that using CHIME to search for afterglows will be effective in constraining the astrophysical merger rate.
AT 2019avd: A Tidal Disruption Event with a Two-phase Evolution
Authors: Chen 陈 Jin-Hong 劲鸿 , Dou 窦 Li-Ming 立明 , Shen 申 Rong-Feng 荣锋 
Published: March 2022

Abstract
Tidal disruption events (TDEs) can uncover the quiescent supermassive black holes (SMBHs) at the center of galaxies and also offer a promising method to study them. After the disruption of a star by an SMBH, the highly elliptical orbit of the debris stream will be gradually circularized due to the self-crossing, and then the circularized debris will form an accretion disk. The recent TDE candidate AT 2019avd has double peaks in its optical light curve, and the X-ray emerges near the second peak. The durations of the peaks are ∼400 and 600 days, respectively, and the separation between them is ∼700 days. We fit its spectral energy distribution and analyze its light curves in the optical/UV, mid-infrared, and X-ray bands. We find that this source can be interpreted as a two-phase scenario in which the first phase is dominated by the stream circularization, and the second phase is the delayed accretion. We use the succession of the self-crossing model and delayed accretion model to fit the first and second peaks, respectively. The fitting result implies that AT 2019avd can be interpreted by the partial disruption of a 0.9 M
⊙ star by a 7 × 106
M
⊙ SMBH, but this result is sensitive to the stellar model. Furthermore, we find that the large-amplitude (by factors up to ∼5) X-ray variability in AT 2019avd can be interpreted as the rigid-body precession of the misaligned disk due to the Lense–Thirring effect of a spinning SMBH, with a precession period of 10−25 days.
Mushroom-instability-driven Magnetic Reconnections in Collisionless Relativistic Jets
Authors: Kawashima Tomohisa , Ishiguro Seiji , Moritaka Toseo , Horiuchi Ritoku , Tomisaka Kohji 
Published: March 2022

Abstract
We study the kinetic plasma dynamics in collisionless relativistic jets with velocity shear, by carrying out particle-in-cell simulations in the transverse plane of a jet. It is discovered that intermittent magnetic reconnections (MRs) are driven by mushroom instability (MI), which is an important kinetic-scale plasma instability in the plasma shear flows with relativistic bulk speed. We refer to this sequence of kinetic plasma phenomena as “MI-driven MR.” The MI-driven MRs intermittently occur with moving the location of the reconnection points from the vicinity of the initial velocity-shear surface toward the center of the jet. As a consequence, the number density of high-energy electrons that are accelerated by MI-driven MRs increases with time in the region inside the initial velocity-shear surface with the accompanying generation and subsequent amplification of magnetic fields by MI. The maximum Lorentz factor of electrons increases with initial bulk Lorentz factor of the jet. A possible relation of MI-driven MR to the bright synchrotron emission in the jet spine of an active galactic nucleus jet is also discussed.
A 16 au Binary in the Class 0 Protostar L1157 MMS
Authors: Tobin John J. , Cox Erin G. , Looney Leslie W. 
Published: March 2022

Abstract
We present Very Large Array observations toward the Class 0 protostar L1157 MMS at 6.8 and 9 mm with a resolution of ∼0.″04 (14 au). We detect two sources within L1157 MMS and interpret these sources as a binary protostar with a separation of ∼16 au. The material directly surrounding the binary system within the inner 50 au radius of the system has an estimated mass of 0.11 M
☉, calculated from the observed dust emission. We interpret the observed binary system in the context of previous observations of its flattened envelope structure, low rates of envelope rotation from 5000 to 200 au scales, and an ordered, poloidal magnetic field aligned with the outflow. Thus, L1157 MMS is a prototype system for magnetically regulated collapse, and the presence of a compact binary within L1157 MMS demonstrates that multiple star formation can still occur within envelopes that likely have dynamically important magnetic fields.