bluuebunny/crossref_metadata_2025_split huggingface dataset:
PENGARUH KOMPENSASI, MOTIVASI DAN LINGKUNGAN KERJA TERHADAP KINERJA KARYAWAN SANTANA BAKERY PURWODADI
Authors: Murtiningsih Tutik , Sudarmadi Sudarmadi 
Published: October 2023

The purpose of this study is to examine the effect of compensation, motivation and work environment on the performance of Santana Bakery Purwodadi employees. The population and sample in this study were all employees at Santana Bakery Purwodadi with 47 employees. Data collection techniques used in this study were through the dissemination of questionnaires. The data analysis methods used include the analysis of research instruments consisting of validity tests, reliability tests, classical assumption tests, and hypothesis tests. The results of this study show that partial compensation has a positive and significant effect on Employee Performance, motivation has a positive and significant effect on Employee Performance, the work environment has a positive and significant effect on Employee Performance. Simultaneously, the results of compensation, motivation and work environment have a positive and significant effect on the performance of Santana Bakery Purwodadi employees. The results of this study also show that the work environment variable is the most dominant variable in influencing the Performance of Santana Bakery Purwodadi Employees.
Acil Serviste Pulmoner Emboli Tanısı Alan Hastalarda Plazma Laktatının Prognostik Rolü
Authors: BİBEROĞLU Serap , KÜÇÜKBEZİRCİ Furkan 
Published: October 2023

Amaç: Pulmoner emboli (PE) en sık görülen üçüncü akut kardiyovasküler hastalıktır. Acil servisde 1 Ocak 2021 ile 1 Temmuz 2023 tarihleri arasında PE tanısı alan hastaların retrospektif analizi yapıldı. 2019 Avrupa Kardiyoloji Cemiyeti (ESC) algoritmasına venöz laktat eklenmesi risk sınıflandırmasını iyileştirebilmekle birlikte, çalışmamızda da yüksek laktat seviyesi ile ilişkili sağ ventrikül fonksiyon bozukluğu kombinasyonu ile acil serviste erken tedavi kararları ve mortalite tahminlerinde yol göstermede katkıda bulunması öngörülmektedir.
Gereç ve Yöntem: Retrospektif olarak, hastaların demografik verileri, vital bulguları, ek hastalıkların varlığı ve plazma laktat düzeyleri ile sonlanımları analiz edildi. 30 günlük mortaliteyi öngörmede ‘Pulmonary Embolism Severity Index’ (PESI), sağ kalp yetmezliği ve plazma laktat seviyeleri istatistiksel olarak analiz edildi.
Bulgular: Çalışmada PE tanısı alan 104 hastanın kategorik parametreleri; %52,9’u (n=55) kadın, %48,1’i (n=50) sigara kullanıyor ve %91,3’ünde (n=95) de ek hastalıkları var idi. %19,2’sinde (n=20) sağ ventrikül yetmezliği saptanmış olup, mortalitesi de %24,96 idi. Sağ ventrikül yetmezliği olan hastaların ortanca plazma laktat düzeyleri (2,25 mmol/L), sağ ventrikül yetmezliği gelişmeyenlere (1,7 mmol/L) kıyasla anlamlı yüksek idi (p=0,01). PESI sınıflamasına göre plazma laktat düzeylerinin karşılaştırılmasında Sınıf I (1,3 mmol/L) – II (1,9 mmol/L), Sınıf I (1,3 mmol/L) – IV ( 2,4 mmol/L), Sınıf I (1,3 mmol/L) – Sınıf V (1,9 mmol/L) ve Sınıf III (1,6 mmol/L) - IV (2,4 mmol/L) arasında istatistiksel olarak anlamlı fark mevcuttu (p
The Atacama Cosmology Telescope: Systematic Transient Search of 3 Day Maps
Authors: Li Yaqiong , Biermann Emily , Naess Sigurd , Aiola Simone , An Rui , Battaglia Nicholas , Bhandarkar Tanay , Calabrese Erminia , Choi Steve K. , Crowley Kevin T. , Devlin Mark , Duell Cody J. , Duff Shannon M. , Dunkley Jo , Dünner Rolando , Gallardo Patricio A. , Guan Yilun , Hervías-Caimapo Carlos , Hincks Adam D. , Hubmayr Johannes , Huffenberger Kevin M. , Hughes John P. , Kosowsky Arthur , Louis Thibaut , Mallaby-Kay Maya , McMahon Jeff , Nati Federico , Niemack Michael D. , Orlowski-Scherer John , Page Lyman , Salatino Maria , Sifón Cristóbal , Staggs Suzanne T. , Vargas Cristian , Vavagiakis Eve M. , Wang Yuhan , Wollack Edward J. 
Published: October 2023

Abstract
We conduct a systematic search for transients in 3 yr of data (2017–2019) from the Atacama Cosmology Telescope (ACT). ACT covers 40% of the sky at three bands spanning from 77–277 GHz. Analysis of 3 day mean-subtracted sky maps, which were match filtered for point sources, yielded 29 transient detections. Eight of these transients are due to known asteroids, and three others were previously published. Four of these events occur in areas with poor noise models and thus we cannot be confident they are real transients. We are left with 14 new transient events occurring at 11 unique locations. All of these events are associated with either rotationally variable stars or cool stars. Ten events have flat or falling spectra indicating radiation from synchrotron emission. One event has a rising spectrum indicating a different engine for the flare.
Varstrometry for Off-nucleus and Dual Subkiloparsec Active Galactic Nuclei (VODKA): Investigating the Nature of SDSS J0823+2418 at z = 1.81, A Likely Lensed Quasar
Authors: Gross Arran C. , Chen Yu-Ching , Foord Adi , Liu Xin , Shen Yue , Oguri Masamune , Goulding Andy , Hwang Hsiang-Chih , Zakamska Nadia L. , Ma 马 Yilun 逸伦 , Nolan Liam 
Published: October 2023

Abstract
Dual quasars at small physical separations are an important precursor phase of galaxy mergers, ultimately leading to the coalescence of the two supermassive black holes. Starting from a sample of dual and/or lensed quasar candidates discovered using astrometric jitter in Gaia data, we present a pilot case study of one of the most promising yet puzzling candidate dual quasars at cosmic noon (z ∼ 1.8). Using multiwavelength imaging and spectroscopy from X-ray to radio, we test whether the SDSS J0823+2418 system is two individual quasars in a bound pair at separation ∼0.″64, or instead a single quasar being gravitationally lensed by a foreground galaxy. We find consistent flux ratios (∼1.25−1.45) between the two sources in optical, near-IR (NIR), UV, and radio, and thus similar spectral energy distributions, suggesting a strong-lensing scenario. However, differences in the radio spectral index, as well as changing X-ray fluxes, hint at either a dual quasar with otherwise nearly identical properties or perhaps lensing-based time lag of ∼3 days paired with intrinsic variability. We find with lens mass modeling that the relative NIR positions and magnitudes of the two quasars and a marginally detected central galaxy are consistent with strong lensing. Archival Sloan Digital Sky Survey spectra likewise suggest a foreground absorber via Mg ii absorption lines. We conclude that SDSS J0823+2418 is likely a lensed quasar, and therefore that the VODKA sample contains a population of these lensed systems (perhaps as high as 50%) as well as dual quasars.
The Global Structure of Molecular Clouds. I. Trends with Mass and Star Formation Rate
Authors: Imara Nia , Forbes John C. 
Published: October 2023

Abstract
We introduce a model for the large-scale, global 3D structure of molecular clouds. Motivated by the morphological appearance of clouds in surface density maps, we model clouds as cylinders, with the aim of backing out information about the volume density distribution of gas and its relationship to star formation. We test our model by applying it to surface density maps for a sample of nearby clouds and find solutions that fit each of the observed radial surface density profiles remarkably well. Our most salient findings are that clouds with higher central volume densities are more compact and also have lower total mass. These same lower-mass clouds tend to have shorter gas depletion times, regardless of whether we consider their total mass or dense mass. Our analyses lead us to conclude that cylindrical clouds can be characterized by a universal structure that sets the timescale on which they form stars.
Relative Intrinsic Scatter in Hierarchical Type Ia Supernova Sibling Analyses: Application to SNe 2021hpr, 1997bq, and 2008fv in NGC 3147
Authors: Ward Sam M. , Thorp Stephen , Mandel Kaisey S. , Dhawan Suhail , Jones David O. , Taggart Kirsty , Foley Ryan J. , Narayan Gautham , Chambers Kenneth C. , Coulter David A. , Davis Kyle W. , de Boer Thomas , de Soto Kaylee , Earl Nicholas , Gagliano Alex , Gao Hua , Hjorth Jens , Huber Mark E. , Izzo Luca , Langeroodi Danial , Magnier Eugene A. , McGill Peter , Rest Armin , Rojas-Bravo César , Wojtak Radosław ,   Young Supernova Experiment
Published: October 2023

Abstract
We present Young Supernova Experiment grizy photometry of SN 2021hpr, the third Type Ia supernova sibling to explode in the Cepheid calibrator galaxy, NGC 3147. Siblings are useful for improving SN-host distance estimates and investigating their contributions toward the SN Ia intrinsic scatter (post-standardization residual scatter in distance estimates). We thus develop a principled Bayesian framework for analyzing SN Ia siblings. At its core is the cosmology-independent relative intrinsic scatter parameter, σ
Rel: the dispersion of siblings distance estimates relative to one another within a galaxy. It quantifies the contribution toward the total intrinsic scatter, σ
0, from within-galaxy variations about the siblings’ common properties. It also affects the combined distance uncertainty. We present analytic formulae for computing a σ
Rel posterior from individual siblings distances (estimated using any SN model). Applying a newly trained BayeSN model, we fit the light curves of each sibling in NGC 3147 individually, to yield consistent distance estimates. However, the wide σ
Rel posterior means σ
Rel ≈ σ
0 is not ruled out. We thus combine the distances by marginalizing over σ
Rel with an informative prior: σ
Rel ∼ U(0, σ
0). Simultaneously fitting the trio’s light curves improves constraints on distance and each sibling’s individual dust parameters, compared to individual fits. Higher correlation also tightens dust parameter constraints. Therefore, σ
Rel marginalization yields robust estimates of siblings distances for cosmology, as well as dust parameters for sibling–host correlation studies. Incorporating NGC 3147's Cepheid distance yields H
0 = 78.4 ± 6.5 km s−1 Mpc−1. Our work motivates analyses of homogeneous siblings samples, to constrain σ
Rel and its SN-model dependence.
Discovery of the Magellanic Stellar Stream Out to 100 kpc
Authors: Chandra Vedant , Naidu Rohan P. , Conroy Charlie , Bonaca Ana , Zaritsky Dennis , Cargile Phillip A. , Caldwell Nelson , Johnson Benjamin D. , Han Jiwon Jesse , Ting 丁 Yuan-Sen 源森 
Published: October 2023

Abstract
The Magellanic Stream (MS)—an enormous ribbon of gas spanning 140° of the southern sky trailing the Magellanic Clouds—has been exquisitely mapped in the five decades since its discovery. However, despite concerted efforts, no stellar counterpart to the MS has been conclusively identified. This stellar stream would reveal the distance and 6D kinematics of the MS, constraining its formation and the past orbital history of the Clouds. We have been conducting a spectroscopic survey of the most distant and luminous red giant stars in the Galactic outskirts. From this data set, we have discovered a prominent population of 13 stars matching the extreme angular momentum of the Clouds, spanning up to 100° along the MS at distances of 60–120 kpc. Furthermore, these kinematically selected stars lie along an [α/Fe]-deficient track in chemical space from −2.5 < [Fe/H] <− 0.5, consistent with their formation in the Clouds themselves. We identify these stars as high-confidence members of the Magellanic Stellar Stream. Half of these stars are metal-rich and closely follow the gaseous MS, whereas the other half are more scattered and metal-poor. We argue that the metal-rich stream is the recently formed tidal counterpart to the MS, and we speculate that the metal-poor population was thrown out of the SMC outskirts during an earlier interaction between the Clouds. The Magellanic Stellar Stream provides a strong set of constraints—distances, 6D kinematics, and birth locations—that will guide future simulations toward unveiling the detailed history of the Clouds.
FAST Discovery of a Fast Neutral Hydrogen Outflow
Authors: Su Renzhi , Gu Minfeng , Curran S. J. , Mahony Elizabeth K. , Tang Ningyu , Allison James R. , Li Di , Zhu Ming , Aditya J. N. H. S. , Yoon Hyein , Zheng Zheng , Wu Zhongzu 
Published: October 2023

Abstract
In this letter, we report the discovery of a fast neutral hydrogen outflow in SDSS J145239.38+062738.0, a merging radio galaxy containing an optical type I active galactic nucleus (AGN). This discovery was made through observations conducted by the Five-hundred-meter Aperture Spherical radio Telescope (FAST) using redshifted 21 cm absorption. The outflow exhibits a blueshifted velocity likely up to ∼−1000 km s−1 with respect to the systemic velocity of the host galaxy with an absorption strength of ∼−0.6 mJy beam−1 corresponding to an optical depth of 0.002 at v = −500 km s−1. The mass outflow rate ranges between 2.8 × 10−2 and 3.6 M
⊙ yr−1, implying an energy outflow rate ranging between 4.2 × 1039 and 9.7 × 1040 erg s−1, assuming 100 K < T
s < 1000 K. Plausible drivers of the outflow include the starbursts, AGN radiation, and radio jet, the last of which is considered the most likely culprit according to the kinematics. By analyzing the properties of the outflow, AGN, and jet, we find that if the H i outflow is driven by the AGN radiation, the AGN radiation does not seem powerful enough to provide negative feedback, whereas the radio jet shows the potential to provide negative feedback. Our observations contribute another example of a fast outflow detected in neutral hydrogen and demonstrate the capability of FAST in detecting such outflows.
SN 2022jli: A Type Ic Supernova with Periodic Modulation of Its Light Curve and an Unusually Long Rise
Authors: Moore T. , Smartt S. J. , Nicholl M. , Srivastav S. , Stevance H. F. , Jess D. B. , Grant S. D. T. , Fulton M. D. , Rhodes L. , Sim S. A. , Hirai R. , Podsiadlowski P. , Anderson J. P. , Ashall C. , Bate W. , Fender R. , Gutiérrez C. P. , Howell D. A. , Huber M. E. , Inserra C. , Leloudas G. , Monard L. A. G. , Müller-Bravo T. E. , Shappee B. J. , Smith K. W. , Terreran G. , Tonry J. , Tucker M. A. , Young D. R. , Aamer A. , Chen T.-W. , Ragosta F. , Galbany L. , Gromadzki M. , Harvey L. , Hoeflich P. , McCully C. , Newsome M. , Gonzalez E. P. , Pellegrino C. , Ramsden P. , Pérez-Torres M. , Ridley E. J. , Sheng X. , Weston J. 
Published: October 2023

Abstract
We present multiwavelength photometry and spectroscopy of SN 2022jli, an unprecedented Type Ic supernova discovered in the galaxy NGC 157 at a distance of ≈ 23 Mpc. The multiband light curves reveal many remarkable characteristics. Peaking at a magnitude of g = 15.11 ± 0.02, the high-cadence photometry reveals periodic undulations of 12.5 ± 0.2 days superimposed on the 200-day supernova decline. This periodicity is observed in the light curves from nine separate filter and instrument configurations with peak-to-peak amplitudes of ≃ 0.1 mag. This is the first time that repeated periodic oscillations, over many cycles, have been detected in a supernova light curve. SN 2022jli also displays an extreme early excess that fades over ≈25 days, followed by a rise to a peak luminosity of L
opt = 1042.1 erg s−1. Although the exact explosion epoch is not constrained by data, the time from explosion to maximum light is ≳ 59 days. The luminosity can be explained by a large ejecta mass (M
ej ≈ 12 ± 6 M
⊙) powered by 56Ni, but we find it difficult to quantitatively model the early excess with circumstellar interaction and cooling. Collision between the supernova ejecta and a binary companion is a possible source of this emission. We discuss the origin of the periodic variability in the light curve, including interaction of the SN ejecta with nested shells of circumstellar matter and neutron stars colliding with binary companions.
Quasiperiodic Peak Energy Oscillations in X-Ray Bursts from SGR J1935+2154
Authors: Roberts Oliver J. , Baring Matthew G. , Huppenkothen Daniela , Kouveliotou Chryssa , Göğüş Ersin , Kaneko Yuki , Lin Lin , van der Horst Alexander J. , Younes George 
Published: October 2023

Abstract
Magnetars are young neutron stars powered by the strongest magnetic fields in the Universe (1013–15 G). Their transient X-ray emission usually manifests as short (a few hundred milliseconds), bright, energetic (∼1040–41 erg) X-ray bursts. Since its discovery in 2014, SGR J1935+2154 has become one of the most prolific magnetars, exhibiting very active bursting episodes and other fascinating events, such as pulse timing antiglitches and fast radio bursts. Here we present evidence for possible 42 Hz (24 ms) quasiperiodic oscillations in the ν
F

ν
spectrum peak energy (E

p
) identified in a unique burst detected with the Fermi Gamma-ray Burst Monitor in 2022 January. While quasiperiodic oscillations have been previously reported in the intensity of magnetar burst light curves, quasiperiodic oscillations in E

p
have not. We also find an additional event from the same outburst that appears to exhibit a similar character in E

p
, albeit of lower statistical quality. For these two exceptional transients, such E

p
oscillations can be explained by magnetospheric density and pressure perturbations. For burst-emitting plasma consisting purely of e
+
e
− pairs, these acoustic modes propagate along a highly magnetized flux tube of length up to around L ∼ 130 neutron star radii, with L being lower if ions are present in the emission zone. Detailed time-resolved analyses of other magnetar bursts are encouraged to evaluate the rarity of these events and their underlying mechanisms.
A Pipeline for Modeling Rapidly Rotating Stars
Authors: Sackrider Jackson L. , Aufdenberg Jason P. 
Published: October 2023

Abstract
Recent stellar intensity interferometry observations of stars at 416 nm complement Michelson interferometry observations in the near-infrared where stellar surface intensity gradients (e.g., limb darkening) are weaker. Intensity gradients due to gravity darkening in rapidly rotating stars are also expected to show higher contrast at 416 nm relative to the near-infrared. We have created a software pipeline to model stellar photospheres of rapidly rotating stars to compare predictions at these wavelength regions. The pipeline can produce model images, visibility predictions, and synthetic spectra. Here we show examples for the Be star β CMi, which has not been interferometrically imaged. We see higher contrast from gravity darkening at 416 nm in model images for rapid rotators, but only for those stars that are not viewed equator-on.
Fille vs Garçon : entre Croyance et Conviction ?
Authors: Lippe Didier 
Published: October 2023

Que Maurice s’affirme et opère sa transformation physique en Madeleine, pour « retrouver sa véritable nature », n’est pas sans nous poser quelques questions, à son propos,… au nôtre. Quelle force extrême, ou quels mécanismes psychiques, (re)mettant en question tout un « être », une vie, amènent à cette conviction ou cette croyance intime et radicale ? Ils sont assurément à la mesure des enjeux vitaux qui sont là engagés, jusqu’à parfois engendrer « transition » et « réassignation sexuée ». « L’être de nature » et « l’être de culture » ne mobilisent pas les mêmes processus identificatoires de la construction psychique, sans pour autant s’exclure mutuellement, et l’on donnera une place importante à la notion « d’après-coup » dans ces questionnements.
À l’écoute des adolescents transgenres le premier entretien
Authors: Adrian Valérie 
Published: October 2023

Être à l’écoute des adolescents transgenres présuppose de connaître l’évolution générationnelle du concept de transsexualisme au concept de transidentité. Dans le contexte actuel de révolution numérique, les adolescents accèdent aux « savoirs trans » et le nombre de « coming out » transgenres à l’adolescence fait événement. La demande des adolescents rencontre l’offre protocolaire de soins. Les modalités de ce « coming out » mobilisent la parentalité sur un mode nouveau. Quel rôle y joue la narrativité ? Quels fantasmes y sont associés ? Entre auto-assignation et fantasme d’auto-engendrement, la mise en jeu du fantasme d’androgynie est questionnée.
Complexe fraternel et dissymétrie. Emmy von N…
Authors: Orasanu Brindusa 
Published: October 2023

Dans la théorie et la clinique psychanalytiques, la figure fraternelle et le transfert fraternel semblent être rarement abordés, et lorsqu’ils sont remarqués, ils semblent être considérés plutôt comme des défenses contre les transferts parentaux. L’hypothèse de l’auteure est que la transmission de cet évitement le long de l’histoire de la psychanalyse a sa source dans le fait que Freud a découvert la règle de l’association libre pendant qu’il traitait Emmy von N…, patiente qui venait avec un fantasme fraternel d’allure traumatique. Ainsi, le germe même de la dissymétrie de l’association libre dans la méthode psychanalytique pourrait être imprégné d’un tel fantasme fraternel, ensemble avec l’évitement, chez l’analyste, d’une régression vers le traitement « préhistorique » par l’intermédiaire de la suggestion.
La problématique narcissique : la vision d’André Green
Authors: Hebbrecht Marc 
Published: October 2023

Selon Green, la problématique du patient narcissique pourrait être décrit en ces termes : il craint de nouer une relation de dépendance, car pour lui entretenir des contacts est traumatisant en raison de l’imprévisibilité et l’altérité de l’objet qui peut occasionner une douleur psychique insupportable. La solution narcissique est donc de renoncer à avoir une relation avec un objet externe et concentrer tout son amour sur le Moi : soit on opte pour l’autosatisfaction orgueilleuse qui rejette l’autre (le narcissisme de vie), soit on opte pour la tranquillité et le zéro (le narcissisme de mort). Grâce à son œuvre, on comprend mieux ce qu’est le désespoir, la dépression chronique, les sentiments de vide et la désertification psychique. Le narcissisme négatif mène fréquemment à une désillusion grave pour le patient et pour l’analyste. Les hypothèses de Green sont illustrées par une vignette clinique de l’auteur.
La dépression : perte de l’objet, perte du fantasme et sortie
Authors: Rizet Clément 
Published: October 2023

Dans cet article, il s’agit de reprendre ce qu’il en est d’une définition de la dépression au sens psychanalytique : à la fois arrêt critique dans un état pathologique, position psychique et relance du travail psychique. À partir de la notion de désespoir chez Kierkegaard, de l’ambiguë dépressivité, entre mélancolie et hystérie, d’Emma Bovary et de la question du travail de deuil chez Freud, sera évoquée la question de l’anesthésie conservatoire de l’objet dans l’état déprimé d’après Fédida. Une courte vignette clinique et une plus longue illustreront la perte du fantasme et le dégagement du marasme dépressif chez une patiente endeuillée de longue date par une perte traumatique.
Contribución al conocimiento de los híbridos naturales de los géneros Aeonium y Greenovia (crassulaceae) en La Gomera, Islas Canarias
Authors: Arango Octavio 
Published: October 2023

Como parte del estudio fitocorológico y eco-biológico realizado en La Gomera con las nueve especies, dos subespecies y dos variedades que componen los géneros Aeonium y Greenovia, fueron descubiertos siete híbridos nuevos, que se suman a los 10 híbridos anteriormente descritos por otros autores en la isla. Se aportan las descripciones botánicas completas en cinco de los nuevos híbridos descubiertos, y en los dos restantes, puesto que solo conocemos la parte vegetativa, se dan a conocer algunos datos corológicos, morfológicos y taxonómicos, y se ilustran fotográficamente las plantas. Se hace el diagnóstico diferencial de los nuevos híbridos con otros nototaxones descritos anteriormente en la isla, especialmente con los que compartían alguno de los parentales. Los tipos nomenclaturales fueron depositados en los herbarios canarios LPA y TFC.