bluuebunny/crossref_metadata_2025_split huggingface dataset:
Pengaruh Karakter Individu Dan Kecerdasan Spiritual Terhadap Kinerja Pegawai Iakn Ambon Dengan Organizational Citizenship Behavior (Ocb) Sebagai Variabel Mediasi
Authors: Isfhanavia Dritin 
Published: January 2022

Latar Belakang : Kemajuan suatu organisasi dipengaruhi oleh manajemen Sumber Daya Manusia , yang memberikan pengaruh sebagai pendorong/motivator yang mampu memebri percepatan dalam mencapai tujuan organsiasi sesuai dengan target yang telah ditetapkan. Tujuan : Penelitian ini bertujuan untuk menguji dan menganalisis pengaruh kecerdasan karakter individu dan kecerdasan spiritual terhadap kinerja pegawai IAKN Ambon dengan Organizational Citizenship Behavior sebagai variabel mediasi. Metode : Populasi dalam penelitian ini adalah pegawai tetap/tenaga kependidikan yang berstatus ASN di IAKN Ambon Sampel yang digunakan dalam penelitian ini sebanyak 52 responden dengan menggunakan teknik Accidental sampling. Alat analisis yang digunakan dalam penelitian ini yaitu regresi linear berganda, analisi jalur, pengujian instrumen, koefisien determinasi, dan analisis parsial. Hasil : Hasil penelitian menyatakan bahwa variabel kecerdasan spiritual tidak berpengaruh terhadap kinerja pegawai. Variabel karakter individu berpengaruh positif dan signifikan terhadap kinerja pegawai. Kesimpulan : Variabel kecerdasan spiritual berpengaruh positif dan signifikan terhadap Organizational Citizenship Behavior (OCB). Variabel karakter individu dan kecerdasan spiritual berpengaruh positif dan signifikan terhadap Organizational Citizenship Behavior (OCB).
نص آرامي جديد من القرن السابع قبل الميلاد
Authors: طه أ.م.د. عدنان حميد 
Published: January 2022

تُبين دراسة هذا النص مكانة اللغة الارآمية في العهد الآشوري الحديث، وجاءت تُعضد الدراسات السابقة التي أثبتت أهمية اللغة الارامية في الحياة اليومية لبلاد الرافدين. يتكون النص من أحد عشر سطرا منقوشا على رقيم طيني مثلث الشكل قريب من شكل القلب، على الوجه سبعة أسطر وعلى القفا أربعة أسطر. ويوجد ثقبان عند الزاويتين العلويتين متصلان من الداخل، وعلى حافة الرقيم العليا توجد طبعة ختم منبسط. عُثر على الرقيم في قلعة آشور ، ورقمه في سجل المتحف العراقي 95344 وفي سجل المنقبين 67 آشور الموسم الثاني 1979. أما قياساته فهي 5x4.4 x 2.9 سم. يُمثل النص عقد قرض: كمية الفضة المقترضة، الفائدة، تأريخ الدفع ، وأسماء الشهود. لعب الآراميون دورا سياسيا مهما في تاريخ الشرق القديم منذ ظهورهم على مسرح التاريخ في ‏القرن الرابع عشر ق.م. في بلاد الشام والأجزاء الشمالية من وادي الرافدي([i]). وازداد دو‏رهم هذا ‏عندما أسسوا ممالك صغيرة كمملكة آرام صوبة ومملكة دمشق ومملكة بيت اديني([ii]). ‏رغم ذلك يعود أقدم النصوص الارامية المكتشفة حتى يومنا هذا إلى نهاية القرن العاشر ق.م([iii]). وقد ‏فرض تاريخ الآرامية الطويل وانتشارها الواسع، والذى امتد في القرن الخامس ق.م . من تخوم الهند شرقا حتى وادى النيل غربا ، تعددا للهجاتها التي يمكن توضيحها كالأتي([iv]): ‏1) الآرامية القديمة، وتمثلت بآرامية النقوش التي معظمها وجدت في الممالك الآرامية ومن فترة نهاية القرن العاشر ق.م. إلى ما يقارب نهاية القرن الثامن ق.م.
المرابطون وأثرهم الحضاري والفكري في بلاد الأندلس من (( 479هـ – 552هـ ))
Authors: نصيف م.م  خالدة عباس , بخيت أ. م.د  خليل جليل 
Published: January 2022

تُعدُّ دولة المرابطين دولة لها تاريخها المؤثر في أحداث الدولة العربية، إذ نشأت في ظلٍّ ظروف قاسية وضعيفة مرت بها الدولة العربية، شحة للانقسام، وكثرة الإمارات المتحاربة والمتناصرة ، لقد برز دور المرابطين بنحوٍ واضح في أنها دولة استطاعت أن تجمع وتلم شمل تلك الأمارات تحت سلطة واحدة، وحكومة مركزية واحدة، أدى ذلك إلى أن تكون قوة قوية في وجه الصليبيين الذي كانت من ضمن مطامعهم بلاد الأندلس .
لقد كان أهم ما يميز حكم المرابطين الدور المميز الذي اداهُ الفقهاء ورجال الدين في إضفاء الشرعية لحكم حكام المرابطين. وقد برز في عصر المرابطين علماء وأدباء كُثر في مجالات شتى ، إذ أنهم كانوا يعتنون بالعلم والعلماء، وقد بلغ هذا الازدهار أوج عظمته في عهد يوسف بن تاشفين. كذلك اهتم المرابطين بالعمارة والفن، وإدخال التطعيم في عملية العمارة بالصدف والألوان التي هي سمة من سمات العمارة الأندلسية التي أخذت شهرة لا يضاهيها بلد من بلاد العرب .
مقاربة تاريخية وسياسية وحضارية في نتائج الاحتلالين الهكسوسي الكشي لمصر والعراق
Authors: الخفاجيّ أ.م.د. مزهر محسن 
Published: January 2022

يُعدُّ كلٌّ من الهكسوس والكشيين، من الأقوام الأجنبية التي غزت كلاً من بلاد وادي النيل وبلاد الرافدين ما بين القرن السابع عشر والسادس عشر قبل الميلاد، وإذا ما اقتنعنا باختلاف الباحثين في، أصلهم وطبيعة هجرتها، وتمددها الجغرافيّ، وغرابة تعاصرهما الزمانيّ، يبقى المتفق عليه أنَّ هذا الاحتلال قد ترك اثاراً في الأصعدة التاريخية السياسية والاجتماعية والحضارية.
هذا البحث محاولة لاقتفاء أثر هذين الاحتلالين في أهم حضارتين في الشرق الأدنى، وهو محاولة أولية لتأصيل فكرة المشترك المكانيّ والجغرافيّ والتاريخيّ والحضاريّ لهذه الاقوام، ونتائج هذا الاحتلال الحضارية والتاريخية على طبيعة المنجز الحضاريّ والتاريخيّ لكل من بلاد النيل وبلاد الرافدين .
Faktor yang Mempengaruhi Perilaku Konsumen Terhadap Keputusan Pembelian Buah di Pasar Induk Cibitung Bekasi
Authors: Prabowo Try 
Published: January 2022

This study aims to determine the faktors that influence the decision to buy fruit at the Pasar Induk Cibitung, Bekasi. Data was collected using questionnaires and documentation, with a total of 91 respondents. Comparison of r table (degree of freedom) with r arithmetic (Corrected Item Total Correlation) to see the effectiveness of the instrument with a significance level of 5% on multiple linear regression test. The results of this study are (1) the price faktor has a significant and important influence on fruit purchasing decisions, and the tcount is greater than the ttable value (11,769 > 1,663). (2) Product faktor has a big influence on the decision to buy fruit with tcount greater than ttable (0.989 > 1.663). (3) The shopping location faktor has a negative effect on fruit purchasing decisions with a value of tcount < ttable (-1.039 <1.663).
Abstrak
Penelitian ini bertujuan untuk mengetahui faktor - faktor yang mempengaruhi Keputusan Pembelian Buah di Pasar Induk Cibitung Bekasi. Pengumpulan data dilakukan dengan menggunakan kuesioner dan dokumentasi, dengan jumlah responden sebanyak 91 responden. Perbandingan r table (degree of freedom) dengan r hitung (Corrected Item Total Corelation) untuk melihat keefektifan instrument dengan tingkat signifikansi 5% pada uji regresi linier berganda. Hasil dari penelitian ini adalah (1) faktor harga memiliki pengaruh yang signifikan dan penting terhadap keputusan pembelian buah, dan nilai thitung lebih besar dari nilai ttable (11,769 > 1,663). (2) Faktor Produk berpengaruh besar terhadap keputusan membeli buah dengan nilai thitung lebih besar dari ttabel (0,989 > 1,663). (3) Faktor Lokasi belanja berpengaruh negative terhadap keputusan pembelian buah dengan nilai thitung < ttabel (-1,039 < 1,663).
Pengaruh Supervisi dan Peran Kepala Sekolah Terhadap Kinerja Mengajar Guru SD Negeri di Kecamatan Rumbai Pesisir
Authors: Prahara Teddy Okto , Mujtahid Iqbal Miftakhul , Rosita Tita 
Published: January 2022

Penelitian ini bertujuan untuk mengetahui pengaruh supervisi dan peran kepala sekolah terhadap kinerja mengajar guru SD Negeri di kecamatan Rumbai Pesisir Data dalam penelitian ini diperoleh dari kuesioner yang bersumber dari guru. Data dianalisis menggunakan regresi berganda. Hasil penelitian menunjukkan bahwa: 1) Terdapat pengaruh yang signifikan antara supervisi dan Peran kepala sekolah terhadap kinerja mengajar guru SD Negeri di kecamatan Rumbai Pesisir, dimana F<sub>hitung</sub> (61,101) &gt; F<sub>tabel </sub>(1,654). Berdasarkan koofisien determinasi (R Square) = 0.441 atau 44,1%. Besar pengaruh supervisi dan peran kepala sekolah terhadap kinerja mengajar guru SD Negeri di kecamatan Rumbai Pesisir sebesar 44,1% berada pada tingkat sedang. 2) Terdapat pengaruh yang signifikan antara peran supervisi terhadap kinerja mengajar guru SD Negeri di kecamatan Rumbai Pesisir, dimana F<sub>hitung</sub> (6,173) &gt; F<sub>tabel </sub>(1,654). Berdasarkan koofisien determinasi (R Square) = 0.440 atau 44%. Besar pengaruh supervisi dan peran kepala sekolah terhadap kinerja mengajar guru SD Negeri di kecamatan Rumbai Pesisir sebesar 44% berada pada tingkat sedang. 3) Terdapat pengaruh yang signifikan antara peran kepala sekolah terhadap kinerja mengajar guru SD Negeri di Kecamatan Rumbai Pesisir, dimana F<sub>hitung</sub> (5,417) &gt; F<sub>tabel </sub>(1,654). Berdasarkan koofisien determinasi (R Square) = 0.403 atau 40,3%. Besar pengaruh supervisi dan peran kepala sekolah terhadap kinerja mengajar guru SD Negeri di kecamatan Rumbai Pesisir sebesar 40,3% berada pada tingkat sedang. Kesimpulan dari penelitian ini bahwa supervisi dan peran kepala sekolah berpengaruh positif dan signifikan terhadap kinerja mengajar guru SD Negeri di kecamatan Rumbai Pesisir.
Analysis of Sales Growth of Chinese Car Brands in Russia in 2019-2020
Authors: Ivanchina A. A. 
Published: January 2022

The article provides an overview of the state of the Russian market for new passenger cars and also considers the dynamics of sales volumes in this market for the period from 2017 to August 2021. Special attention is paid to representatives of the Chinese brands Geely, Haval, Chery in Russia, which show positive dynamics in sales growth in the falling Russian market for new passenger cars. The article will be of interest to a representative of the automotive industry.The analysis showed that in a falling market, you can increase your share due to the right strategic decisions in the field of marketing. Since the companies do not disclose their plans to "conquer the world", we relied on open sources (official sites) and analyzed the already committed actions of representatives of Chinese brands, comparing them with the results achieved. The method of work is a systematic approach to the statistical analysis of the dynamics and structure of the Russian passenger car market.
Elemental Abundances of nearby M Dwarfs Based on High-resolution Near-infrared Spectra Obtained by the Subaru/IRD Survey: Proof of Concept
Authors: Ishikawa Hiroyuki Tako , Aoki Wako , Hirano Teruyuki , Kotani Takayuki , Kuzuhara Masayuki , Omiya Masashi , Hori Yasunori , Kokubo Eiichiro , Kudo Tomoyuki , Kurokawa Takashi , Kusakabe Nobuhiko , Narita Norio , Nishikawa Jun , Ogihara Masahiro , Ueda Akitoshi , Currie Thayne , Henning Thomas , Kasagi Yui , Kolecki Jared R. , Kwon Jungmi , Machida Masahiro N. , McElwain Michael W. , Nakagawa Takao , Vievard Sebastien , Wang Ji , Tamura Motohide , Sato Bun’ei 
Published: January 2022

Abstract
Detailed chemical analyses of M dwarfs are scarce but necessary to constrain the formation environment and internal structure of planets being found around them. We present elemental abundances of 13 M dwarfs (2900 < T
eff < 3500 K) observed in the Subaru/IRD planet search project. They are mid- to late-M dwarfs whose abundance of individual elements has not been well studied. We use the high-resolution (∼70,000) near-infrared (970–1750 nm) spectra to measure the abundances of Na, Mg, Si, K, Ca, Ti, V, Cr, Mn, Fe, and Sr by the line-by-line analysis based on model atmospheres, with typical errors ranging from 0.2 dex for [Fe/H] to 0.3–0.4 dex for other [X/H]. We measure radial velocities from the spectra and combine them with Gaia astrometry to calculate the Galactocentric space velocities UVW. The resulting [Fe/H] values agree with previous estimates based on medium-resolution K-band spectroscopy, showing a wide distribution of metallicity (−0.6 < [Fe/H] < +0.4). The abundance ratios of individual elements [X/Fe] are generally aligned with the solar values in all targets. While the [X/Fe] distributions are comparable to those of nearby FGK stars, most of which belong to the thin-disk population, the most metal-poor object, GJ 699, could be a thick-disk star. The UVW velocities also support this. The results raise the prospect that near-infrared spectra of M dwarfs obtained in the planet search projects can be used to grasp the trend of elemental abundances and the Galactic stellar population of nearby M dwarfs.
Mapping the Diversity of Galaxy Spectra with Deep Unsupervised Machine Learning
Authors: Teimoorinia Hossen , Archinuk Finn , Woo Joanna , Shishehchi Sara , Bluck Asa F. L. 
Published: January 2022

Abstract
Modern spectroscopic surveys of galaxies such as MaNGA consist of millions of diverse spectra covering different regions of thousands of galaxies. We propose and implement a deep unsupervised machine-learning method to summarize the entire diversity of MaNGA spectra onto a 15 × 15 map (DESOM-1), where neighboring points on the map represent similar spectra. We demonstrate our method as an alternative to conventional full spectral fitting for deriving physical quantities and full probability distributions much more efficiently than traditional resource-intensive Bayesian methods. Since spectra are grouped by similarity, the distribution of spectra onto the map for a single galaxy, i.e., its “fingerprint,” reveals the presence of distinct stellar populations within the galaxy, indicating smoother or episodic star formation histories. We further map the diversity of galaxy fingerprints onto a second map (DESOM-2). Using galaxy images and independent measures of galaxy morphology, we confirm that galaxies with similar fingerprints have similar morphologies and inclination angles. Since morphological information was not used in the mapping algorithm, relating galaxy morphology to the star formation histories encoded in the fingerprints is one example of how the DESOM maps can be used to make scientific inferences.
Locating Red Supergiants in the Galaxy NGC 6822
Authors: Dimitrova Tzvetelina A. , Neugent Kathryn F. , Massey Philip , Levesque Emily M. 
Published: January 2022

Abstract
Using archival near-IR photometry, we identify 51 of the K-band brightest red supergiants (RSGs) in NGC 6822 and compare their physical properties with stellar evolutionary model predictions. We first use Gaia parallax and proper motion values to filter out foreground Galactic red dwarfs before constructing a J–K versus K color–magnitude diagram to eliminate lower-mass asymptotic giant branch star contaminants in NGC 6822. We then cross match our results to previously spectroscopically confirmed RSGs and other NGC 6822 content studies and discuss our overall completeness, concluding that radial velocity alone is an insufficient method of determining membership in NGC 6822. After transforming the J and K magnitudes to effective temperatures and luminosities, we compare these physical properties with predictions from both the Geneva single-star and Binary Population and Spectral Synthesis (BPASS) single and binary-star evolution tracks. We find that our derived temperatures and luminosities match the evolutionary model predictions well, however, the BPASS model, which includes the effects of binary evolution, provides the best overall fit. This revealed the presence of a group of cool RSGs in NGC 6822, suggesting a history of binary interaction. We hope this work will lead to further comparative RSG studies in other Local Group galaxies, opportunities for direct spectroscopic follow-up, and a better understanding of evolutionary model predictions.
Coronal Mass Ejections and Type II Radio Emission Variability during a Magnetic Cycle on the Solar-type Star ϵ Eridani
Authors: Ó Fionnagáin Dúalta , Kavanagh Robert D. , Vidotto Aline A. , Jeffers Sandra V. , Petit Pascal , Marsden Stephen , Morin Julien , Golden Aaron ,   (BCool Collaboration)
Published: January 2022

Abstract
We simulate possible stellar coronal mass ejection (CME) scenarios over the magnetic cycle of ϵ Eridani (18 Eridani; HD 22049). We use three separate epochs from 2008, 2011, and 2013, and estimate the radio emission frequencies associated with these events. These stellar eruptions have proven to be elusive, although a promising approach to detect and characterize these phenomena are low-frequency radio observations of potential type II bursts as CME-induced shocks propagate through the stellar corona. Stellar type II radio bursts are expected to emit below 450 MHz, similarly to their solar counterparts. We show that the length of time these events remain above the ionospheric cutoff is not necessarily dependent on the stellar magnetic cycle, but more on the eruption location relative to the stellar magnetic field. We find that these type II bursts would remain within the frequency range of LOFAR for a maximum of 20–30 minutes post-eruption for the polar CMEs (50 minutes for second harmonics). We find evidence of slower equatorial CMEs, which result in slightly longer observable windows for the 2008 and 2013 simulations. Stellar magnetic geometry and strength have a significant effect on the detectability of these events. We place the CMEs in the context of the stellar mass-loss rate (27–48× solar mass-loss rate), showing that they can amount to 3%–50% of the stellar wind mass-loss rate for ϵ Eridani. Continuous monitoring of likely stellar CME candidates with low-frequency radio telescopes will be required to detect these transient events.
Strong Perpendicular Velocity-space Diffusion in Proton Beams Observed by Parker Solar Probe
Authors: Verniero J. L. , Chandran B. D. G. , Larson D. E. , Paulson K. , Alterman B. L. , Badman S. , Bale S. D. , Bonnell J. W. , Bowen T. A. , de Wit T. Dudok , Kasper J. C. , Klein K. G. , Lichko E. , Livi R. , McManus M. D. , Rahmati A. , Verscharen D. , Walters J. , Whittlesey P. L. 
Published: January 2022

Abstract
The SWEAP instrument suite on Parker Solar Probe (PSP) has detected numerous proton beams associated with coherent, circularly polarized, ion-scale waves observed by PSP’s FIELDS instrument suite. Measurements during PSP Encounters 4−8 revealed pronounced complex shapes in the proton velocity distribution functions (VDFs), in which the tip of the beam undergoes strong perpendicular diffusion, resulting in VDF level contours that resemble a “hammerhead.” We refer to these proton beams, with their attendant “hammerhead” features, as the ion strahl. We present an example of these observations occurring simultaneously with a 7 hr ion-scale wave storm and show results from a preliminary attempt at quantifying the occurrence of ion-strahl broadening through three-component ion VDF fitting. We also provide a possible explanation of the ion perpendicular scattering based on quasilinear theory and the resonant scattering of beam ions by parallel-propagating, right circularly polarized, fast magnetosonic/whistler waves.
Hydrogenation of Accreting C Atoms and CO Molecules–Simulating Ketene and Acetaldehyde Formation Under Dark and Translucent Cloud Conditions
Authors: Fedoseev Gleb , Qasim Danna , Chuang Ko-Ju , Ioppolo Sergio , Lamberts Thanja , van Dishoeck Ewine F. , Linnartz Harold 
Published: January 2022

Abstract
Simple and complex organic molecules (COMs) are observed along different phases of star and planet formation and have been successfully identified in prestellar environments such as dark and translucent clouds. Yet the picture of organic molecule formation at those earliest stages of star formation is not complete and an important reason is the lack of specific laboratory experiments that simulate carbon atom addition reactions on icy surfaces of interstellar grains. Here we present experiments in which CO molecules as well as C and H atoms are codeposited with H2O molecules on a 10 K surface mimicking the ongoing formation of an “H2O-rich” ice mantle. To simulate the effect of impacting C atoms and resulting surface reactions with ice components, a specialized C-atom beam source is used, implemented on SURFRESIDE3, an ultra-high vacuum cryogenic setup. Formation of ketene (CH2CO) in the solid state is observed in situ by means of reflection absorption IR spectroscopy. C18O and D isotope labeled experiments are performed to further validate the formation of ketene. Data analysis supports that CH2CO is formed through C-atom addition to a CO molecule, followed by successive hydrogenation transferring the formed :CCO into ketene. Efficient formation of ketene is in line with the absence of an activation barrier in C+CO reaction reported in the literature. We also discuss and provide experimental evidence for the formation of acetaldehyde (CH3CHO) and possible formation of ethanol (CH3CH2OH), two COM derivatives of CH2CO hydrogenation. The underlying reaction network is presented and the astrochemical implications of the derived pathways are discussed.
Prospects of Fast Flavor Neutrino Conversion in Rotating Core-collapse Supernovae
Authors: Harada Akira , Nagakura Hiroki 
Published: January 2022

Abstract
There is mounting evidence that neutrinos undergo fast flavor conversion (FFC) in core-collapse supernova (CCSN). In this paper, we investigate the roles of stellar rotation on the occurrence of FFC by carrying out axisymmetric CCSN simulations with full Boltzmann neutrino transport. Our result suggests that electron neutrino lepton number (ELN) angular crossings, which are the necessary and sufficient condition to trigger FFC, preferably occur in the equatorial region for rotating CCSNe. By scrutinizing the neutrino–matter interaction and neutrino radiation field, we find some pieces of evidence that the stellar rotation facilitates the occurrence of FFC. The low-electron-fraction region in the post-shock layer expands by centrifugal force, enhancing the disparity of neutrino absorption between electron-type neutrinos (ν
e) and their anti-particles (

ν

¯

e

). This has a significant impact on the angular distribution of neutrinos in momentum space, in which ν
e tends to be more isotropic than

ν

¯

e

;

consequently, ELN crossings emerge. The ELN crossing found in this study is clearly associated with rotation, which motivates further investigation on how the subsequent FFC influences explosion dynamics, nucleosynthesis, and neutrino signals in rotating CCSNe.
The Spectroscopic Binaries from the LAMOST Medium-resolution Survey. I. Searching for Double-lined Spectroscopic Binaries with a Convolutional Neural Network
Authors: Zhang Bo , Jing Ying-Jie , Yang Fan , Wan Jun-Chen , Ji Xin , Fu Jian-Ning , Liu Chao , Zhang Xiao-Bin , Luo Feng , Tian Hao , Zhou Yu-Tao , Wang Jia-Xin , Guo Yan-Jun , Zong Weikai , Xiong Jian-Ping , Li Jiao 
Published: January 2022

Abstract
We developed a convolutional neural network model to distinguish the double-lined spectroscopic binaries (SB2s) from others based on single-exposure medium-resolution spectra (R ∼ 7500). The training set consists of a large set of mock spectra of single stars and binaries synthesized based on the MIST stellar evolutionary model and ATLAS9 atmospheric model. Our model reaches a novel theoretic false-positive rate by adding a proper penalty on the negative sample (e.g., 0.12% and 0.16% for the blue/red arm when the penalty parameter Λ = 16). Tests show that the performance is as expected and favors FGK-type main-sequence (MS) binaries with high mass ratio (q ≥ 0.7) and large radial velocity separation (Δv ≥ 50 km s−1). Although the real false-positive rate cannot be estimated reliably, validating on eclipsing binaries identified from Kepler light curves indicates that our model predicts low binary probabilities at eclipsing phases (0, 0.5, and 1.0) as expected. The color–magnitude diagram also helps illustrate its feasibility and capability of identifying FGK MS binaries from spectra. We conclude that this model is reasonably reliable and can provide an automatic approach to identify SB2s with period ≲10 days. This work yields a catalog of binary probabilities for over 5 million spectra of 1 million sources from the LAMOST medium-resolution survey (MRS) and a catalog of 2198 SB2 candidates whose physical properties will be analyzed in a follow-up paper. Data products are made publicly available online, as well as our Github website.