bluuebunny/crossref_metadata_2025_split huggingface dataset:
DEVELOPMENT OF AN AGENT MODEL OF A QUEUING SYSTEM IN THE ANYLOGIC ENVIRONMENT ON THE EXAMPLE OF A GAS STATION
Authors: Белякова Анна Юрьевна , Бузина Татьяна Сергеевна 
Published: August 2022

В статье представлена агентная модель автозаправочной станции, разработанная в среде имитационного моделирования Anylogic, рассмотрены этапы ее разработки, проведен эксперимент работы модели.
The article presents an agent model of a gas station developed in the Anylogic simulation environment, the stages of its development are considered, an experiment of the model operation is carried out.
ARTIFICIAL INTELLIGENCE IN PUBLIC TRANSPORT
Authors: Большаков Илья Александрович , Микаева Светлана Анатольевна 
Published: August 2022

Авторами рассмотрены полезные свойства от использования искусственного интеллекта в общественном транспорте. Описаны возможности оптимизации и максимизации эффективности общественного транспорта, посредством анализа с помощью интеллектуальных данных, собранных умными камерами и системами видеонаблюдения.
The authors consider the useful properties of the use of artificial intelligence in public transport. The possibilities of optimizing and maximizing the efficiency of public transport are described by analyzing with the help of intelligent data collected by smart cameras and video surveillance systems.
Compact and Variable Radio Emission from an Active Galaxy with Supersoft X-Ray Emission
Authors: Yang Lei , Shu Xinwen , Zhang Fabao , Chandola Yogesh , Liu Daizhong , Liu Yi , Gu Minfeng , Giustini Margherita , Jiang Ning , Li Ya-Ping , Li Di , Elbaz David , Juneau Stephanie , Pannella Maurilio , Sun Luming , Tang Ningyu , Wang Tinggui , Zhou Hongyan 
Published: August 2022

Abstract
RX J1301.9+2747 is a unique active galaxy with a supersoft X-ray spectrum that lacks significant emission at energies above 2 keV. In addition, it is one of few galaxies displaying quasiperiodic X-ray eruptions that recur on a timescale of 13–20 ks. We present multiepoch radio observations of RX J1301.9+2747 using GMRT, Very Large Array (VLA), and Very Long Baseline Array (VLBA). The VLBA imaging at 1.6 GHz reveals a compact radio emission unresolved at a scale of <0.7 pc, with a brightness temperature of T
b > 5 × 107 K. The radio emission is variable by more than a factor of 2.5 over a few days, based on the data taken from VLA monitoring campaigns. The short-term radio variability suggests that the radio emitting region has a size as small as 8 × 10−4 pc, resulting in an even higher brightness temperature of T
b ∼ 1012 K. A similar limit on the source size can be obtained if the observed flux variability is not intrinsic and caused by the interstellar scintillation effect. The overall radio spectrum is steep with a time-averaged spectral index α = −0.78 ± 0.03 between 0.89 and 14 GHz. These observational properties rule out a thermal or star formation origin of the radio emission, and appear to be consistent with the scenario of episodic jet ejections driven by a magnetohydrodynamic process. Simultaneous radio and X-ray monitoring observations down to a cadence of hours are required to test whether the compact and variable radio emission is correlated with the quasiperiodic X-ray eruptions.
Chandra Observations of Six Peter Pan Disks: Diversity of X-Ray-driven Internal Photoevaporation Rates Does Not Explain Their Rare Longevity
Authors: Laos Emily , Wisniewski John P. , Kuchner Marc J. , Silverberg Steven M. , Günther Hans Moritz , Principe David A. , Bonine Brett , Kounkel Marina ,   The Disk Detective Collaboration
Published: August 2022

Abstract
We present Chandra X-ray observations of six previously identified Peter Pan objects, rare ∼40 Myr systems with evidence of primordial disk retention. We observe X-ray luminosities (0.8–3.0 keV) ranging from log L

x
∼ 27.7–29.1. We find that our Peter Pan sample exhibits X-ray properties similar to that of weak-lined T Tauri stars and do not exhibit evidence of stellar accretion induced X-ray suppression. Our observed Peter Pan X-ray luminosities are consistent with that measured for field dM stars of similar spectral type and age, implying their long primordial disk lifetimes are likely not a consequence of unusually faint X-ray host stars. Our derived X-ray photoevaporative mass-loss rates predict our systems have passed the point of rapid gas dispersal and call into question the impact of this internal mechanism for primordial disk dispersal around dM stars. Our qualitative assessment of the surrounding Peter Pan environments also does not predict unusually low levels of external photoevaporation relative to other respective moving group members. Overall, our results suggest Peter Pan disks may be a consequence of the low far-UV flux incident on the disk in low-mass dM stars given their relatively lower levels of accretion over the course of their pre-main-sequence evolution.
The GLASS-JWST Early Release Science Program. I. Survey Design and Release Plans
Authors: Treu T. , Roberts-Borsani G. , Bradac M. , Brammer G. , Fontana A. , Henry A. , Mason C. , Morishita T. , Pentericci L. , Wang X. , Acebron A. , Bagley M. , Bergamini P. , Belfiori D. , Bonchi A. , Boyett K. , Boutsia K. , Calabró A. , Caminha G. B. , Castellano M. , Dressler A. , Glazebrook K. , Grillo C. , Jacobs C. , Jones T. , Kelly P. L. , Leethochawalit N. , Malkan M. A. , Marchesini D. , Mascia S. , Mercurio A. , Merlin E. , Nanayakkara T. , Nonino M. , Paris D. , Poggianti B. , Rosati P. , Santini P. , Scarlata C. , Shipley H. V. , Strait V. , Trenti M. , Tubthong C. , Vanzella E. , Vulcani B. , Yang L. 
Published: August 2022

Abstract
The GLASS-JWST Early Release Science (hereafter GLASS-JWST-ERS) Program will obtain and make publicly available the deepest extragalactic data of the ERS campaign. It is primarily designed to address two key science questions, namely, “what sources ionized the universe and when?” and “how do baryons cycle through galaxies?”, while also enabling a broad variety of first look scientific investigations. In primary mode, it will obtain NIRISS and NIRSpec spectroscopy of galaxies lensed by the foreground Hubble Frontier Field cluster, Abell 2744. In parallel, it will use NIRCam to observe two fields that are offset from the cluster center, where lensing magnification is negligible, and which can thus be effectively considered blank fields. In order to prepare the community for access to this unprecedented data, we describe the scientific rationale, the survey design (including target selection and observational setups), and present pre-commissioning estimates of the expected sensitivity. In addition, we describe the planned public releases of high-level data products, for use by the wider astronomical community.
Powering Luminous Core Collapse Supernovae with Jets
Authors: Soker Noam 
Published: August 2022

Abstract
I examine recent fittings of luminous supernovae (LSNe) with extra energy sources of magnetar and helium burning and find that in about half of these LSNe the fitting parameters have some problems. In some LSNe the total energy of these two energy sources is larger than the kinetic energy of the ejecta that the fitting yields. In some other LSNe the total energy of the delayed neutrino explosion mechanism and these two extra sources combined is smaller than the kinetic energy that the fitting yields. These difficulties suggest that, like earlier claims that jets power superluminous supernovae (SLSNe), jets also power the less luminous LSNe. A magnetar might also supply energy. However, in most cases jets supply more energy than the magnetar, during the explosion and possibly at late times. I strengthen an earlier claim that jets launched at magnetar birth cannot be ignored. I explain the trend of maximum rise time for a given luminosity of hydrogen deficient core collapse supernovae, in particular LSNe and SLSNe, with a toy model of jets that are active for a long time after explosion.
Spectral Energy Distributions in Three Deep-drilling Fields of the Vera C. Rubin Observatory Legacy Survey of Space and Time: Source Classification and Galaxy Properties
Authors: Zou Fan , Brandt W. N. , Chen Chien-Ting , Leja Joel , Ni Qingling , Yan Wei , Yang Guang , Zhu Shifu , Luo Bin , Nyland Kristina , Vito Fabio , Xue Yongquan 
Published: August 2022

Abstract
W-CDF-S, ELAIS-S1, and XMM-LSS will be three Deep-Drilling Fields (DDFs) of the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST), but their extensive multiwavelength data have not been fully utilized as done in the COSMOS field, another LSST DDF. To prepare for future science, we fit source spectral energy distributions (SEDs) from X-ray to far-infrared in these three fields mainly to derive galaxy stellar masses and star formation rates. We use CIGALE v2022.0, a code that has been regularly developed and evaluated, for the SED fitting. Our catalog includes 0.8 million sources covering 4.9 deg2 in W-CDF-S, 0.8 million sources covering 3.4 deg2 in ELAIS-S1, and 1.2 million sources covering 4.9 deg2 in XMM-LSS. Besides fitting normal galaxies, we also select candidates that may host active galactic nuclei (AGNs) or are experiencing recent star formation variations and use models specifically designed for these sources to fit their SEDs; this increases the utility of our catalog for various projects in the future. We calibrate our measurements by comparison with those in well-studied smaller regions and briefly discuss the implications of our results. We also perform detailed tests of the completeness and purity of SED-selected AGNs. Our data can be retrieved from a public website.
Hubble Space Telescope Imaging Reveals That SN 2015bh Is Much Fainter than Its Progenitor
Authors: Jencson Jacob E. , Sand David J. , Andrews Jennifer E. , Smith Nathan , Strader Jay , Aghakhanloo Mojgan , Pearson Jeniveve , Valenti Stefano 
Published: August 2022

Abstract
We present Hubble Space Telescope (HST) imaging of the site of SN 2015bh in the nearby spiral galaxy NGC 2770 taken between 2017 and 2019, nearly four years after the peak of the explosion. In 2017–2018, the transient fades steadily in optical filters before declining more slowly to F814W = −7.1 mag in 2019, ≈4 mag below the level of its eruptive luminous blue variable (LBV) progenitor observed with HST in 2008–2009. The source fades at a constant color of F555W
−
F814W = 0.4 mag until 2018, similar to SN 2009ip and consistent with a spectrum dominated by interaction of the ejecta with circumstellar material (CSM). A deep optical spectrum obtained in 2021 lacks signatures of ongoing interaction (L
Hα
≲ 1038 erg s−1 for broadened emission ≲2000 km s−1), but indicates the presence of a nearby H ii region (≲300 pc). The color evolution of the fading source makes it unlikely that emission from a scattered-light echo or binary OB companion of the progenitor contributes significantly to the flattening of the late-time light curve. The remaining emission in 2019 may plausibly be attributed an evolved/inflated companion or an unresolved (≲3 pc), young stellar cluster. Importantly, the color evolution of SN 2015bh rules out scenarios in which the surviving progenitor is obscured by nascent dust and does not clearly indicate a transition to a hotter, optically faint state. The simplest explanation is that the massive progenitor did not survive. SN 2015bh likely represents a remarkable example of the terminal explosion of a massive star preceded by decades of end-stage eruptive variability.
A Robust Test of the Existence of Primordial Black Holes in Galactic Dark Matter Halos
Authors: Abramowicz Marek , Bejger Michał , Udalski Andrzej , Wielgus Maciek 
Published: August 2022

Abstract
If very low mass primordial black holes (PBH) within the asteroid/moon-mass range indeed reside in galactic dark matter halos, they must necessarily collide with galactic neutron stars (NSs). These collisions must, again necessarily, form light black holes (LBHs) with masses of typical NSs, M
LBH ≈ 1–2 M
⊙. LBHs may be behind events already detected by ground-based gravitational-wave detectors (GW170817, GW190425, and others such as a mixed stellar black hole–NS-mass event GW191219_163120), and most recently by microlensing (OGLE-BLG-2011-0462). Although the status of these observations as containing LBHs is not confirmed, there is no question that gravitational-wave detectors and microlensing are in principle and in practice capable of detecting LBHs. We have calculated the creation rate of LBHs resulting from these light primordial black hole (PBH) collisions with NSs. On this basis, we claim that if improved gravitational-wave detectors and microlensing statistics of the LBH events would indicate that the number of LBHs is significantly lower that what follows from the calculated creation rate, then this would be an unambiguous proof that there is no significant light PBH contribution to the galactic dark matter halos. Otherwise, if observed and calculated numbers of LBHs roughly agree, then the hypothesis of primordial black hole existence gets strong observational support, and in addition their collisions with NSs may be considered a natural creation channel for the LBHs, solving the problem of their origin, as it is known that they cannot be a product of standard stellar evolution.
Long-term Variability of Non-radial Pulsations in SXP 4.78
Authors: Schmidtke P. C. , Cowley A. P. , Udalski A. 
Published: August 2022

Abstract
OGLE I-band observations for [M2002] SMC 20671, the optical counterpart of SXP 4.78, were searched for periodicities with P > 0.5 days. Three sets of photometric signals were detected, which are attributed to non-radial pulsations of the Be star. All signals show considerable variability in power over the 16 seasons studied. The most likely periods of the NRPs are 0.5826, 0.6164, and 0.6424 days.
Wind/Waves Antenna Length Determined Using Quasi-Thermal Noise Spectroscopy
Authors: Martinović Mihailo M. , Klein Kristopher G. , Krishnan Hari G. 
Published: August 2022

Abstract
The Wind/Waves instrument has been collecting in situ electric field measurements in the solar wind as well as Earth's magnetosphere and geotail since 1994. The Thermal Noise Receiver (TNR) sub-instrument uses a wire dipole made of very long and thin whip antennas, highly convenient for Quasi-Thermal Noise (QTN) measurements. The instrument team has determined that twice during the mission, in 2000 and 2002, one of the antenna arms broke, changing the antenna response to plasma fluctuations. In this note, we use the QTN spectroscopy method developed specially for the TNR to determine the antenna length after each of these breaks. By parametrically varying the value of the antenna length used in the QTN calculation, we find that initial 50 m long antenna arm was initially shortened to ∼25.5 m in 2000, and then to ∼20 m in 2002.
Acrocalymma chuxiongense sp. nov., a new species of Acrocalymmaceae (Pleosporales) on leaves of Quercus
Authors: Liu Yu-Wei , Zeng Xiang-Yu 
Published: August 2022

In Huafo Mountain, Mouding, Yunnan Province, China, we found black protrusions on the leaf surface of Quercus plants. The collection which we identified as Acrocalymma chuxiongense sp. nov., a new species of Acrocalymmaceae (Pleosporales) is characterised by dome-shaped ascomata, bitunicate asci with pedicel furcate and an ocular chamber and hyaline, obovoid to ellipsoid, 1-septate ascospores.
Morphologically, this species is typical with obovoid to ellipsoid, larger ascospores than other known species in Acrocalymma. Phylogenetic analysis also showed that it represents a distinct clade, distant to any other species of Acrocalymma. Therefore, we introduce it as Acrocalymma chuxiongense, a new species of Acrocalymmaceae. This study is adding to the current situation where there are very few species and lack of teleomorph characteristics.
De Didot (an III) à Laboulaye (1879) : l’avènement philosophique de Montesquieu
Authors: Volpilhac-Auger Catherine 
Published: August 2022

À la fin du XVIIIe siècle, l’édition des œuvres de Montesquieu relève encore de la polémique, avec l’édition de 1759 (remarques « anonymes » de Luzac) puis celle de Didot (1795), qui prétend s’appuyer sur Helvétius, ou de l’hagiographie, avec l’édition Plassan (1796-1797). Le XIXe siècle développe une pratique commercialement utile, mais aussi intellectuellement intéressante, qui consiste à juxtaposer les notes critiques extraites de divers commentateurs : l’œuvre devient ainsi matière à débat, en un temps (après la Restauration) où Montesquieu revient en grâce, tandis que se multiplient les éditions qui ne peuvent guère se différencier que par cet apparat critique hétéroclite. Les Œuvres complètes dues à Laboulaye (1875-1879) marquent une véritable rupture : se conjuguent la formation juridique et les positions politiques de ce partisan d’une monarchie constitutionnelle, mais surtout le désir d’entrer dans la pensée de Montesquieu plutôt que de la critiquer superficiellement, pour mieux y introduire le lecteur. C’est à ces conditions que l’œuvre ainsi éditée peut devenir proprement philosophique.
Un livre « utile en ce moment » : l’édition de Buffier comme pratique idéologique au XIXe siècle
Authors: Rouquayrol Louis 
Published: August 2022

Le Traité des premières vérités (1724) de Claude Buffier connaît, au XIXe siècle, deux éditions. L’une, d’inspiration catholique, insiste sur la continuité entre la philosophie du sens commun du jésuite et le principe d’autorité de Félicité de Lamennais. L’autre, qui émane de l’école cousinienne, insiste au contraire sur la dette de l’école écossaise du Common Sense à l’égard de l’œuvre de Buffier. L’une et l’autre cherchent à dissocier Buffier de la philosophie dont il se sentait peut-être le plus proche, mais qui préfigure à bien des égards tous les excès (sensualisme, matérialisme, athéisme) du XVIIIe siècle que catholiques et cousiniens combattent : celle de Locke. Par leurs défauts, ces deux éditions ne nous apprennent pas grand-chose sur le Traité des premières vérités, mais disent en revanche beaucoup des luttes idéologiques dont le XIXe siècle a été le théâtre.
Les éditions des philosophes écossais par Théodore Jouffroy. Mouvement historique et réforme philosophique
Authors: Clauzade Laurent 
Published: August 2022

Le travail éditorial de Théodore Jouffroy s’est exclusivement attaché à présenter et à traduire les auteurs écossais : les Esquisses de philosophie morale de Dugald Stewart, et les Œuvres complètes de Thomas Reid. Cette étude essaie de déterminer le sens de ce travail, que Jouffroy ne concevait pas comme une contribution à l’histoire de la philosophie, mais plutôt comme une réflexion sur la nature et l’organisation des sciences philosophiques. La première partie de cette étude décrit le contexte historique complexe dans lequel ces éditions ont été élaborées. La seconde partie montre, à partir de la préface aux œuvres complètes de Reid, comment les rapports entre Jouffroy et l’éclectisme cousinien ont évolué.
Incidence of Anastomotic Pseudoaneurysm of Arteriovenous Fistula in Hemodialysis Patients Having Non-Cuffed Catheters as Vascular Access – Association or Causation?
Authors: Vyahalkar Sameer Vilas , Binnani Pooja G , Kulkarni Amar Vilas , Hoda Arif , Varyani Umesh Tulsidas , Nagarik Amit Prakash , Chaudhari Avinash E 
Published: August 2022

Background:
Anastomotic pseudoaneurysm affecting arteriovenous fistula created for hemodialysis is an unusual and catastrophic complication. There is lack of clinical data in literature about its incidence and management.

Aims and Objectives:
To study the incidence and understand the aetiology of anastomotic pseudoaneurysm of arteriovenous fistula (PA-AVF) occurring in first six months after surgery.

Materials and Methods:
Cohort study based on retrospective analysis of three-year data of case-series of PA-AVF occurring in first six months after AV fistula creation for hemodialysis.

Results:
Among the 283 AV fistula surgeries (215 distal forearm radio-cephalic AVF and 68 brachial artery or cubital region AVF), 7 patients (2.4%) developed PA-AVF within 1 to 8 weeks after AV fistula surgery. Over-extended dependence on non-cuffed hemodialysis (HD) catheter was a common factor among patients developing this complication. All the patients had a prolonged stay (34 to 75 days) of non-cuffed HD catheters before development of PA-AVF. Diagnosis of HD catheter-related blood stream infection (HD-CRBSI), which overlapped with development of PA-AVF, was proven in 4 patients, two of which also had surgical site infection. One patient had traumatic PA-AVF and in two patients the cause could not be established although features consistent with CRBSI were present. Excision of pseudoaneurysm and ligation of radial artery was done in all cases.

Conclusion:
Infection is the most common cause of anastomotic pseudoaneurysm of AV fistula. Our study points towards extended use of non-cuffed hemodialysis catehters as a risk factor for development of PA-AVF. Prevention and early aggressive management of CRBSI and surgical site infections along with a limited use of non-cuffed HD catheters for the minimum required duration is the key to reduce the incidence of this complication
Applicability of Ambulatory Cleft Lip Repair in North-western Nigeria
Authors: Taiwo Abdulrazaq Olanrewaju , Braimah Ramat Oyebunmi , Ibikunle Adebayo Aremu , Adigun Olufemi Ibrahim , Lawal Sikiru H. , Ile-Ogendengbe Bruno , Bala Mujtaba , Olayinka Adeyemi Micheal , Adeyemi Moshood Folorunsho , Farouk Mohammed A. 
Published: August 2022

Objective:
To report the applicability of ambulatory cleft lip repair (CLR) and to review the existing literature.

Materials and Methods:
This is a retrospective clinical case series study of ambulatory CLR in North-western Nigeria. The study was carried out in Usmanu Danfodiyo University Teaching Hospital (UDUTH), Sokoto, between January 2012 and December 2018. Relevant clinical data of the subjects obtained include sociodemographics, type of cleft, and complications. Protocol employed includes premedication with diazepam (0.5 mg/kg, IV) slowly, followed by administration of glycopyrrolate (0.005 mg/kg, IV) and diclofenac potassium (1 mg/kg, IV). Then, ketamine (0.1 mg/kg, IV) was infused slowly over a 5-min period to achieve procedural sedation (Ramsey sedation score of 3). The data were analyzed using (SPSS; Chicago, IL, USA) program, version 20. The results were presented in simple descriptive statistics.

Results:
The age ranged from 2 to 21 years with male preponderance (M: F = 4:1). All participants had unilateral clefts lip with or without alveolus. The left side was twice involved as the right. There were no perioperative complications nor mortality recorded and no patient required conversion to general anesthesia. All patients were successfully discharged home on the same day of the operation. No case of readmission was recorded and subsequent follow-up was uneventful.

Conclusions:
Parenteral use of ketamine and diazepam for outpatient pediatric cleft lip procedures is safe and of immense benefits in reducing the surgical cleft burden without compromising patients safety.