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Journal articles on the topic 'Modelo IMBA'

Author: Grafiati

Published: 4 June 2021

Last updated: 5 February 2022

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1

Aros, Francisco I., Anna C. Sippel, Alessandra Mastrobuono-Battisti, Abbas Askar, Paolo Bianchini, and Glenn van de Ven. "Dynamical modelling of globular clusters: challenges for the robust determination of IMBH candidates." Monthly Notices of the Royal Astronomical Society 499, no. 4 (2020): 4646–65. http://dx.doi.org/10.1093/mnras/staa2821.

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ABSTRACT The presence or absence of intermediate-mass black holes (IMBHs) at the centre of Milky Way globular clusters (GCs) is still an open question. This is due to either observational restrictions or limitations in the dynamical modelling method; in this work, we explore the latter. Using a sample of high-end Monte Carlo simulations of GCs, with and without a central IMBH, we study the limitations of spherically symmetric Jeans models assuming constant velocity anisotropy and mass-to-light ratio. This dynamical method is one of the most widely used modelling approaches to identify a centra

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Zocchi, Alice, Mark Gieles, and Vincent Hénault-Brunet. "On the uniqueness of kinematical signatures of intermediate-mass black holes in globular clusters." Proceedings of the International Astronomical Union 10, S312 (2014): 197–200. http://dx.doi.org/10.1017/s1743921315007802.

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AbstractFinding an intermediate-mass black hole (IMBH) in a globular cluster (GC), or proving its absence, is a crucial ingredient in our understanding of galaxy formation and evolution. The challenge is to identify a unique signature of an IMBH that cannot be accounted for by other processes. Observational claims of IMBH detection are often based on analyses of the kinematics of stars, such as a rise in the velocity dispersion profile towards the centre. In this contribution we discuss the degeneracy between this IMBH signal and pressure anisotropy in the GC. We show that that by considering

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Baumgardt, H., C. He, S. M. Sweet та ін. "No evidence for intermediate-mass black holes in the globular clusters ω Cen and NGC 6624". Monthly Notices of the Royal Astronomical Society 488, № 4 (2019): 5340–51. http://dx.doi.org/10.1093/mnras/stz2060.

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ABSTRACT We compare the results of a large grid of N-body simulations with the surface brightness and velocity dispersion profiles of the globular clusters ω Cen and NGC 6624. Our models include clusters with varying stellar-mass black hole retention fractions and varying masses of a central intermediate-mass black hole (IMBH). We find that an $\sim 45\, 000$ M⊙ IMBH, whose presence has been suggested based on the measured velocity dispersion profile of ω Cen, predicts the existence of about 20 fast-moving, m &gt; 0.5 M⊙, main-sequence stars with a (1D) velocity v &gt; 60 km s−1 in the

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Göttgens, Fabian, Sebastian Kamann, Holger Baumgardt, et al. "Central kinematics of the Galactic globular cluster M80." Monthly Notices of the Royal Astronomical Society 507, no. 4 (2021): 4788–803. http://dx.doi.org/10.1093/mnras/stab2449.

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ABSTRACT We use spectra observed with the integral-field spectrograph Multi Unit Spectroscopic Explorer (MUSE) to reveal the central kinematics of the Galactic globular cluster Messier 80 (M80, NGC 6093). Using observations obtained with the recently commissioned narrow-field mode of MUSE, we are able to analyse 932 stars in the central 7.5 arcsec by 7.5 arcsec of the cluster for which no useful spectra previously existed. Mean radial velocities of individual stars derived from the spectra are compared to predictions from axisymmetric Jeans models, resulting in radial profiles of the velocity

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Cao, Ding-feng, Bin Shi, Hong-hu Zhu, et al. "Feasibility Investigation of Improving the Modified Green–Ampt Model for Treatment of Horizontal Infiltration in Soil." Water 11, no. 4 (2019): 645. http://dx.doi.org/10.3390/w11040645.

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Water infiltration in soil is a complex process that still requires appreciation of interactions among three phases (soil particles, water and air) to enable accurate estimation of water transport rates. To simulate this process, the Green–Ampt (GA) model and the Modified Green-Ampt (MGA) model introduced in the paper “A new method to estimate soil water infiltration based on a modified Green–Ampt model” have been widely used. The GA model is based on the hypothesis that the advance of the wetting front in soil under matric suction can be treated as a rectangular piston flow that is instantane

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YILMAZER, Tuba, Hilal TUZER, and Simay AKYÜZ. "Effect of Information-Motivation-Behavioral Skills Model-Based Intervention on Quality of Life of Ostomy Patients." Turkiye Klinikleri Journal of Nursing Sciences 12, no. 2 (2020): 182–89. http://dx.doi.org/10.5336/nurses.2019-72070.

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SEZGÜNSAY, Emine, Nazife ŞIVGIN, Süleyman Utku ÇELİK, and Mustafa DEVECİ. "Effect of Information-Motivation-Behavioral Skills Model-Based Intervention on Quality of Life of Ostomy Patients." Turkiye Klinikleri Journal of Nursing Sciences 12, no. 4 (2020): 643–44. http://dx.doi.org/10.5336/nurses.2020-77918.

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8

YILMAZER, Tuba, Hilal TUZER, and Simay AKYÜZ. "Effect of Information-Motivation-Behavioral Skills Model-Based Intervention on Quality of Life of Ostomy Patients." Turkiye Klinikleri Journal of Nursing Sciences 13, no. 1 (2021): 184–86. http://dx.doi.org/10.5336/nurses.2021-81703.

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9

Donnelley, Martin, Kaye S. Morgan, Regine Gradl, et al. "Live-pig-airway surface imaging and whole-pig CT at the Australian Synchrotron Imaging and Medical Beamline." Journal of Synchrotron Radiation 26, no. 1 (2019): 175–83. http://dx.doi.org/10.1107/s1600577518014133.

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The Australian Synchrotron Imaging and Medical Beamline (IMBL) was designed to be the world's widest synchrotron X-ray beam, partly to enable clinical imaging and therapeutic applications for humans, as well as for imaging large-animal models. Our group is currently interested in imaging the airways of newly developed cystic fibrosis (CF) animal models that display human-like lung disease, such as the CF pig. One key outcome measure for assessing the effectiveness of CF airway therapies is the ability of the lung to clear inhaled particulates by mucociliary transit (MCT). This study extends th

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10

Baumgardt, Holger, Antonio Sollima, and Michael Hilker. "On the presence of intermediate black holes in three globular clusters." Proceedings of the International Astronomical Union 14, S351 (2019): 400–403. http://dx.doi.org/10.1017/s1743921319007695.

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AbstractWe investigate whether the globular clusters 47 Tuc, ω Cen and NGC 6624 contain intermediate-mass black holes (IMBHs) by fitting a large grid of N-body simulations against their surface density and velocity dispersion profiles. In our simulations we vary the initial cluster size, the initial mass function and the initial density profile of the clusters as well as the mass fraction of a central intermediate-mass black hole. We find that the surface density and velocity dispersion profiles of all three clusters can be better reproduced by models that do not contain a central IMBH than by

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Egeten, Grifin Ryandi, Berlian Setiawaty, and Retno Budiarti. "Pendugaan Imbal Hasil Saham dengan Model Autoregressive Moving Average." Jambura Journal of Mathematics 3, no. 2 (2021): 140–54. http://dx.doi.org/10.34312/jjom.v3i2.10358.

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ABSTRAKSeorang investor pada umumnya berharap untuk membeli suatu saham dengan harga yang rendah dan menjual saham tersebut dengan harga yang lebih tinggi untuk memperoleh imbal hasil yang tinggi. Namun, kapan waktu yang tepat melakukannya menjadi tantangan tersendiri bagi para investor. Oleh sebab itu, dibutuhkan suatu model yang mampu menduga imbal hasil saham dengan baik, salah satunya adalah model autoregressive moving average (ARMA). Tujuan dari penelitian ini adalah untuk menerapkan model autoregressive (AR), model moving average (MA), atau model autoregressive moving average (ARMA) pada

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12

Sun, Xue, Lien-Fu Lai, Ping Chou, Liang-Rui Chen, and Chao-Chin Wu. "On GPU Implementation of the Island Model Genetic Algorithm for Solving the Unequal Area Facility Layout Problem." Applied Sciences 8, no. 9 (2018): 1604. http://dx.doi.org/10.3390/app8091604.

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Facility layout problem (FLP) is one of the hottest research areas in industrial engineering. A good facility layout can achieve efficient production management, improve production efficiency, and create high economic values. Because FLP is an NP-hard problem, meaning it is impossible to find the optimal solution when problem becomes sufficiently large, various evolutionary algorithms (EAs) have been proposed to find a sub-optimal solution within a reasonable time interval. Recently, a genetic algorithm (GA) was proposed for unequal area FLP (UA-FLP), where the areas of facilities are not iden

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13

Shi, Yanlong, Michael Y. Grudić, and Philip F. Hopkins. "The mass budget for intermediate-mass black holes in dense star clusters." Monthly Notices of the Royal Astronomical Society 505, no. 2 (2021): 2753–63. http://dx.doi.org/10.1093/mnras/stab1470.

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ABSTRACT Intermediate-mass black holes (IMBHs) could form via runaway merging of massive stars in a young massive star cluster (YMC). We combine a suite of numerical simulations of YMC formation with a semi-analytic model for dynamical friction and merging of massive stars and evolution of a central quasi-star, to predict how final quasi-star and relic IMBH masses scale with cluster properties (and compare with observations). The simulations argue that inner YMC density profiles at formation are steep (approaching isothermal), producing some efficient merging even in clusters with relatively l

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14

Arca Sedda, Manuel, Pau Amaro Seoane, and Xian Chen. "Merging stellar and intermediate-mass black holes in dense clusters: implications for LIGO, LISA, and the next generation of gravitational wave detectors." Astronomy & Astrophysics 652 (August 2021): A54. http://dx.doi.org/10.1051/0004-6361/202037785.

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Context. The next generation of gravitational wave (GW) observatories would enable the detection of intermediate-mass black holes (IMBHs), an elusive type of BH expected to reside in the centres of massive clusters, dwarf galaxies, and possibly the accretion discs of active galactic nuclei. Intermediate-mass ratio inspirals (IMRIs), which are composed of an IMBH and a compact stellar object, constitute one promising source of GWs detectable by this new generation of instruments. Aims. We study the formation and evolution of IMRIs triggered by interactions between two stellar BHs and an IMBH in

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15

Lawin, Agnidé Emmanuel, Célestin Manirakiza, and Batablinlè Lamboni. "Trends and changes detection in rainfall, temperature and wind speed in Burundi." Journal of Water and Climate Change 10, no. 4 (2018): 852–70. http://dx.doi.org/10.2166/wcc.2018.155.

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Abstract This paper assessed the potential impacts of trends detected in rainfall, temperature and wind speed on hydro and wind power resources in Burundi. Two climatic stations located at two contrasting regions, namely Rwegura catchment and northern Imbo plain, were considered. Rainfall, temperature and wind speed observed data were considered for the period 1950–2014 and future projection data from seven Regional Climate Models (RCMs) for the period 2021–2050 were used. The interannual variability analysis was made using standardized variables. Trends and rupture were respectively detected

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Ng, Michael K., C. K. Sze, and S. P. Yung. "Wavelet algorithms for deblurring models." International Journal of Imaging Systems and Technology 14, no. 3 (2004): 113–21. http://dx.doi.org/10.1002/ima.20014.

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17

Kanungo, Tapas, Robert M. Haralick, and Ihsin Phillips. "Nonlinear global and local document degradation models." International Journal of Imaging Systems and Technology 5, no. 3 (1994): 220–30. http://dx.doi.org/10.1002/ima.1850050305.

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18

GERMANI, Yana Friedrich, Salette Amaral De FIGUEIREDO, Lauro Júlio CALLIARI, and Humberto Dias VIANNA. "O papel da antepraia na resposta costeira durante a elevação do nível do mar na Barreira Regressiva de Torres a Imbé, RS." Pesquisas em Geociências 47, no. 3 (2020): e098304. http://dx.doi.org/10.22456/1807-9806.109986.

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A zona costeira é um sistema muito dinâmico, o qual busca atingir um estado de equilíbrio dinâmico. Nos últimos 5,5 ka, o nível médio do mar (NMM) apresentou comportamento praticamente estável, porém, devido às mudanças climáticas está em elevação. Objetivando analisar a influência das variações na morfologia do substrato entre setores costeiros adjacentes (Torres-Capão-Imbé), na resposta à elevação do NMM em médio e longo prazo, foram projetadas linhas de costa futuras para estes cenários. Além da morfologia, investigou-se a existência de diferenças significativas nessas projeções em função d

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19

Yan, Shuicheng, Xinwen Hou, Stan Z. Li, Hongjiang Zhang, and Qiansheng Cheng. "Face alignment using view-based direct appearance models." International Journal of Imaging Systems and Technology 13, no. 1 (2003): 106–12. http://dx.doi.org/10.1002/ima.10039.

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20

Vikram, T. N., and K. Chidananda Gowda. "Subspace models for document script and language identification." International Journal of Imaging Systems and Technology 20, no. 2 (2010): 140–48. http://dx.doi.org/10.1002/ima.20215.

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21

Cho, Myoung Won, and M. Y. Choi. "Brain networks: Graph theoretical analysis and development models." International Journal of Imaging Systems and Technology 20, no. 2 (2010): 108–16. http://dx.doi.org/10.1002/ima.20229.

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22

Hénault-Brunet, V., M. Gieles, J. Strader, M. Peuten, E. Balbinot, and K. E. K. Douglas. "On the black hole content and initial mass function of 47 Tuc." Monthly Notices of the Royal Astronomical Society 491, no. 1 (2019): 113–28. http://dx.doi.org/10.1093/mnras/stz2995.

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ABSTRACT The globular cluster (GC) 47 Tuc has recently been proposed to host an intermediate-mass black hole (IMBH) or a population of stellar mass black holes (BHs). To shed light on its dark content, we present an application of self-consistent multimass models with a varying mass function and content of stellar remnants, which we fit to various observational constraints. Our best-fitting model successfully matches the observables and correctly predicts the radial distribution of millisecond pulsars and their gravitational accelerations inferred from long-term timing observations. The data f

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23

Wirth, Henriette, and Kenji Bekki. "Formation of massive black holes in ultracompact dwarf galaxies: migration of primordial intermediate-mass black holes in N-body simulation." Monthly Notices of the Royal Astronomical Society 496, no. 1 (2020): 921–32. http://dx.doi.org/10.1093/mnras/staa1603.

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ABSTRACT Recent observational studies of ultracompact dwarf galaxies (UCDs) have discovered the massive black hole (MBH), with masses of more than ${10^6~\rm M_\odot }$, in their central regions. We here consider that these MBHs can be formed through the merging of intermediate-mass black hole (IMBH), with masses of (103–105) M⊙, within the stellar nuclei of dwarf galaxies, which are progenitors of UCDs. We numerically investigate this formation process for a wide range of model parameters using N-body simulations. This means that IMBH growth and feedback is neglected in this study. We find th

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Gimel'farb, G. L. "Intensity-based computer binocular stereo vision: Signal models and algorithms." International Journal of Imaging Systems and Technology 3, no. 3 (1991): 189–200. http://dx.doi.org/10.1002/ima.1850030304.

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Wang, Y. F., Jeng-Feng Lee, and Jih-Fang Wang. "Unification scheme for 3D surface reconstruction using physically based models." International Journal of Imaging Systems and Technology 3, no. 4 (1991): 279–99. http://dx.doi.org/10.1002/ima.1850030402.

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Zhang, Yu, and Norman I. Badler. "Face modeling and editing with statistical local feature control models." International Journal of Imaging Systems and Technology 17, no. 6 (2007): 341–58. http://dx.doi.org/10.1002/ima.20127.

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Häberle, Maximilian, Mattia Libralato, Andrea Bellini, et al. "Hunting for intermediate-mass black holes in globular clusters: an astrometric study of NGC 6441." Monthly Notices of the Royal Astronomical Society 503, no. 1 (2021): 1490–506. http://dx.doi.org/10.1093/mnras/stab474.

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ABSTRACT We present an astrometric study of the proper motions (PMs) in the core of the globular cluster NGC 6441. The core of this cluster has a high density and observations with current instrumentation are very challenging. We combine ground-based, high-angular-resolution NACO@VLT images with Hubble Space Telescope ACS/HRC data and measure PMs with a temporal baseline of 15 yr for about 1400 stars in the centremost 15 arcsec of the cluster. We reach a PM precision of ∼30 µas yr−1 for bright, well-measured stars. Our results for the velocity dispersion are in good agreement with other studie

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Lovis, C. "Sustainable Health Care Systems." Yearbook of Medical Informatics 16, no. 01 (2007): 19–21. http://dx.doi.org/10.1055/s-0038-1638524.

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SummaryTo summarize major current trends and research in the field of sustainable health care systems.Synopsis of the articles selected for the IMIA Yearbook 2007.Four excellent articles, four nations and four international peer-reviewed journals representing some important aspects of the research in this field have been selected for the IMIA Yearbook 2007. The first paper focuses on health care spending and use of information technologies in OECD countries; the second paper presents an original model and framework to describe and evaluate the risks and safety of e-health systems; the third pa

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Chan, Yung-Kuan, and Ching-Lin Wang. "An image compression method based on multiple models for the probabilities of patterns." International Journal of Imaging Systems and Technology 19, no. 4 (2009): 362–68. http://dx.doi.org/10.1002/ima.20214.

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Galih Gusti, Galih Gusti, and Henny Dewi Koeswanti. "EFEKTIVITAS PENGGUNAAN MODEL KOOPERATIF TIPE JIGSAW DAN STAD TERHADAP HASIL BELAJAR IPS SISWA KELAS V SD IMBAS GUGUS DIPONEGORO KABUPATEN BLORA." ELEMENTARY SCHOOL JOURNAL PGSD FIP UNIMED 7, no. 1 (2017): 110–18. http://dx.doi.org/10.24114/esjpgsd.v7i1.6408.

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Torres, F., F. A. Candelas, S. T. Puente, and F. G. Ortiz. "Graph models applied to specification, simulation, allocation, and scheduling of real-time computer vision applications." International Journal of Imaging Systems and Technology 11, no. 5 (2000): 287–91. http://dx.doi.org/10.1002/ima.1014.

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Rump, Alexis, Stefan Eder, Andreas Lamkowski, et al. "Development of New Biokinetic-Dosimetric Models for the Simulation of Iodine Blockade in the Case of Radioiodine Exposure in Man." Drug Research 69, no. 11 (2019): 583–97. http://dx.doi.org/10.1055/a-0960-5590.

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AbstractIn the case of nuclear incidents, radioiodine may be liberated. After incorporation it accumulates in the thyroid and by internal irradiation enhances the risk of cancer occurrence. By administering a large dose of non-radioactive iodine the uptake of radioiodine into the gland can be inhibited (“iodine blockade”). Biokinetic models using first order kinetics are not suited to simulate iodine blockade, as the uptake into the gland is mediated by a saturable active transport. Therefore, we integrated an uptake mechanism described by a Michaelis-Menten kinetic into a simple ICRP biokinet

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Lyman, J. D., L. Galbany, S. F. Sánchez, J. P. Anderson, H. Kuncarayakti, and J. L. Prieto. "Studying the environment of AT 2018cow with MUSE." Monthly Notices of the Royal Astronomical Society 495, no. 1 (2020): 992–99. http://dx.doi.org/10.1093/mnras/staa1243.

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ABSTRACT AT 2018cow was the nearest and best-studied example of a new breed of extragalactic, luminous, and rapidly evolving transient. Both the progenitor systems and explosion mechanisms of these rapid transients remain a mystery – the energetics, spectral signatures, and time-scales make them challenging to interpret in established classes of supernovae and tidal disruption events. The rich, multiwavelength data set of AT 2018cow has still left several interpretations viable to explain the nature of this event. In this paper, we analyze integral-field spectroscopic data of the host galaxy,

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Di Carlo, Ugo N., Michela Mapelli, Mario Pasquato, et al. "Intermediate-mass black holes from stellar mergers in young star clusters." Monthly Notices of the Royal Astronomical Society 507, no. 4 (2021): 5132–43. http://dx.doi.org/10.1093/mnras/stab2390.

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ABSTRACT Intermediate-mass black holes (IMBHs) in the mass range $10^2\!-\!10^5\, \mathrm{M_{\odot }}$ bridge the gap between stellar black holes (BHs) and supermassive BHs. Here, we investigate the possibility that IMBHs form in young star clusters via runaway collisions and BH mergers. We analyse 104 simulations of dense young star clusters, featuring up-to-date stellar wind models and prescriptions for core collapse and (pulsational) pair instability. In our simulations, only nine IMBHs out of 218 form via binary BH mergers, with a mass ∼100–140 M⊙. This channel is strongly suppressed by th

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Lala, Jonathan M., David R. Rounce, and Daene C. McKinney. "Modeling the glacial lake outburst flood process chain in the Nepal Himalaya: reassessing Imja Tsho's hazard." Hydrology and Earth System Sciences 22, no. 7 (2018): 3721–37. http://dx.doi.org/10.5194/hess-22-3721-2018.

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Abstract. The Himalayas of South Asia are home to many glaciers that are retreating due to climate change and causing the formation of large glacial lakes in their absence. These lakes are held in place by naturally deposited moraine dams that are potentially unstable. Specifically, an impulse wave generated by an avalanche or landslide entering the lake can destabilize the moraine dam, thereby causing a catastrophic failure of the moraine and a glacial lake outburst flood (GLOF). Imja-Lhotse Shar Glacier is amongst the glaciers experiencing the highest rate of mass loss in the Mount Everest r

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Dos Santos Martins, Valérie, Mickael Rodrigues, and Mamadou Diagne. "A multi-model approach to Saint-Venant equations: A stability study by LMIs." International Journal of Applied Mathematics and Computer Science 22, no. 3 (2012): 539–50. http://dx.doi.org/10.2478/v10006-012-0041-6.

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Abstract This paper deals with the stability study of the nonlinear Saint-Venant Partial Differential Equation (PDE). The proposed approach is based on the multi-model concept which takes into account some Linear Time Invariant (LTI) models defined around a set of operating points. This method allows describing the dynamics of this nonlinear system in an infinite dimensional space over a wide operating range. A stability analysis of the nonlinear Saint-Venant PDE is proposed both by using Linear Matrix Inequalities (LMIs) and an Internal Model Boundary Control (IMBC) structure. The method is a

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Christ, Olaf, and Ulrich G. Hofmann. "Video tracking of swimming rodents on a reflective water surface." Current Directions in Biomedical Engineering 1, no. 1 (2015): 232–35. http://dx.doi.org/10.1515/cdbme-2015-0058.

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AbstractAnimal models are an essential testbed for new devices on their path from the bench to the patient. Potential impairments by brain stimulation are often investigated in water mazes to study spatial memory and learning. Video camera based tracking systems exist to quantify rodent behaviour, but reflections of ambient lighting on the water surface and artefacts due to the waves caused by the swimming animal cause errors. This often requires tweaking of algorithms and parameters, or even potentially modifying the lab setup. In the following, we provide a simple solution to alleviate these

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Hosseinzadeh, Mostafa, Mohammad Reza Mehrnia, and Navid Mostoufi. "Experimental Study and Modeling of Fouling in Immersed Membrane Bioreactor Operating in Constant Pressure Filtration." Mathematical Problems in Engineering 2013 (2013): 1–7. http://dx.doi.org/10.1155/2013/456143.

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A new mathematical model is proposed based on filtration mechanisms for the prediction of fouling in airlift immersed membrane bioreactors (iMBRs). The cake formation on the membrane surface through constant pressure filtration process in the iMBR was explained by a proposed cake filtration mechanism which assumes that no particle enters the pores when forming the cake layer on the membrane surface. The cake porosity reduction due to diffusion of particles was described by an intermediate blocking mechanism. Experimental study of fouling was also performed in a lab-scale airlift flat-sheet iMB

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Sannasi Chakravarthy, S. R., and Harikumar Rajaguru. "Detection and classification of microcalcification from digital mammograms with firefly algorithm, extreme learning machine and non‐linear regression models: A comparison." International Journal of Imaging Systems and Technology 30, no. 1 (2019): 126–46. http://dx.doi.org/10.1002/ima.22364.

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Fiorentino, G., M. Bellazzini, M. Spera, et al. "Deep into the core of dense star clusters: an astrometric and photometric test case for ELT." Monthly Notices of the Royal Astronomical Society 494, no. 3 (2020): 4413–25. http://dx.doi.org/10.1093/mnras/staa869.

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ABSTRACT We present a novel analysis of a young star cluster in the Large Magellanic cloud, R136-like, as seen by the Extremely Large Telescope (ELT). The main aim of this study is to quantify precision and accuracy of stellar proper motion measurements in crowded field when using an ELT working at its diffraction limit. This can serve as a reference study for future development of ELT scientific cases. In particular, we investigate our future ability to detect the dynamical signature of intermediate-mass black holes (IMBHs) with mass ∼104 M⊙ through detailed measurements of stellar proper mot

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Yustiardhi, Aulia Fitria, Mahdiah Aulia, and Reni Oktavia Permatasari. "Islamic Contracts for Home Financing: A Comparative Analysis." International Journal of Management and Applied Research 6, no. 4 (2019): 386–96. http://dx.doi.org/10.18646/2056.64.19-030.

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Home financing is widely needed by many people across different countries. Through the years, Islamic banks have developed several models for home financing to address the growing demand from customers. Two products that Islamic banks use extensively are Murabahah and Bay Bithaman Ajil (BBA) which in practice have similar characteristics to their conventional counterparts, which leads to criticism from Islamic scholars. Alternative Islamic home financing schemes that have been introduced to the market in recent years include Musharakah Mutanaqisah (MM), Ijarah Muntahiya Bit Tamlik (IMBT) and I

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Livingstone, Jayde, Jean-François Adam, Jeffrey C. Crosbie, et al. "Preclinical radiotherapy at the Australian Synchrotron's Imaging and Medical Beamline: instrumentation, dosimetry and a small-animal feasibility study." Journal of Synchrotron Radiation 24, no. 4 (2017): 854–65. http://dx.doi.org/10.1107/s1600577517006233.

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Therapeutic applications of synchrotron X-rays such as microbeam (MRT) and minibeam (MBRT) radiation therapy promise significant advantages over conventional clinical techniques for some diseases if successfully transferred to clinical practice. Preclinical studies show clear evidence that a number of normal tissues in animal models display a tolerance to much higher doses from MRT compared with conventional radiotherapy. However, a wide spread in the parameters studied makes it difficult to make any conclusions about the associated tumour control or normal tissue complication probabilities. T

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Koutkias, Vassilis, and Jacques Bouaud. "Contributions on Clinical Decision Support from the 2018 Literature." Yearbook of Medical Informatics 28, no. 01 (2019): 135–37. http://dx.doi.org/10.1055/s-0039-1677929.

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Objectives: To summarize recent research and select the best papers published in 2018 in the field of computerized clinical decision support for the Decision Support section of the International Medical Informatics Association (IMIA) yearbook. Methods: A literature review was performed by searching two bibliographic databases for papers referring to clinical decision support systems (CDSSs). The aim was to identify a list of candidate best papers from the retrieved bibliographic records, which were then peer-reviewed by external reviewers. A consensus meeting of the IMIA editorial team finally

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Rounce, D. R., D. J. Quincey, and D. C. McKinney. "Debris-covered energy balance model for Imja-Lhotse Shar Glacier in the Everest region of Nepal." Cryosphere Discussions 9, no. 3 (2015): 3503–40. http://dx.doi.org/10.5194/tcd-9-3503-2015.

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Abstract. Debris thickness plays an important role in regulating ablation rates on debris-covered glaciers as well as controlling the likely size and location of supraglacial lakes. Despite its importance, lack of knowledge about debris properties and associated energy fluxes prevents the robust inclusion of the effects of a debris layer into most glacier surface energy balance models. This study combines fieldwork with a debris-covered energy balance model to estimate debris temperatures and ablation rates on Imja-Lhotse Shar glacier located in the Everest region of Nepal. The debris properti

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Balbinotti, Marcos Alencar Abaide, Marcus Levi Lopes Barbosa, and Daniela Wiethaeuper. "Consistência interna e fatorial do Inventário Multifatorial de Coping para Adolescentes." Psico-USF 11, no. 2 (2006): 175–83. http://dx.doi.org/10.1590/s1413-82712006000200006.

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Coping é um construto multidimensional relativo às formas como as pessoas lidam com situações estressantes. Diversas pesquisas assinalam a importância dessas "respostas de enfrentamento". Este estudo visa verificar os índices de consistência interna e fatorial confirmatórios do Inventário Multifatorial de Coping para Adolescentes (IMCA-43). Assim, a coleta de dados foi realizada mediante aplicações coletivas, em sala de aula, em uma amostra de 285 estudantes do ensino fundamental e médio, de ambos os sexos e com idades variando de 13 a 18 anos. Os resultados dos índices alfa de Cronbach (0,71

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Xu, Fei, Yuri Bazilevs, and Ming-Chen Hsu. "Immersogeometric analysis of compressible flows with application to aerodynamic simulation of rotorcraft." Mathematical Models and Methods in Applied Sciences 29, no. 05 (2019): 905–38. http://dx.doi.org/10.1142/s0218202519410033.

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We present an immersogeometric analysis (IMGA) approach for the simulation of compressible flows around complex geometries. In this method, compressible flow simulations are performed directly on various boundary representations (B-reps) of mechanical designs, circumventing the labor-intensive and time-consuming cleanup of complex geometric models. A new formulation for the weak imposition of essential boundary conditions in the context of non-body-fitted meshes is proposed. The formulation employs the non-symmetric Nitsche method, which yields good performance especially when the penalty para

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Nickovic, Slobodan, Bojan Cvetkovic, Fabio Madonna, et al. "Cloud ice caused by atmospheric mineral dust – Part 1: Parameterization of ice nuclei concentration in the NMME-DREAM model." Atmospheric Chemistry and Physics 16, no. 17 (2016): 11367–78. http://dx.doi.org/10.5194/acp-16-11367-2016.

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Abstract. Dust aerosols are very efficient ice nuclei, important for heterogeneous cloud glaciation even in regions distant from desert sources. A new generation of ice nucleation parameterizations, including dust as an ice nucleation agent, opens the way towards a more accurate treatment of cold cloud formation in atmospheric models. Using such parameterizations, we have developed a regional dust-atmospheric modelling system capable of predicting, in real time, dust-induced ice nucleation. We executed the model with the added ice nucleation component over the Mediterranean region, exposed to

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Chanamé, Julio, Justice Bruursema, Rupali Chandar, Jay Anderson, Roeland van der Marel, and Holland Ford. "HST's hunt for intermediate-mass black holes in star clusters." Proceedings of the International Astronomical Union 5, S266 (2009): 231–37. http://dx.doi.org/10.1017/s1743921309991098.

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AbstractEstablishing or ruling out, either through solid mass measurements or upper limits, the presence of intermediate-mass black holes (IMBHs; with masses of 102 − 105 M⊙) at the centers of star clusters would profoundly impact our understanding of problems ranging from the formation and long-term dynamical evolution of stellar systems, to the nature of the seeds and the growth mechanisms of supermassive black holes. While there are sound theoretical arguments both for and against their presence in today's clusters, observational studies have so far not yielded truly conclusive IMBH detecti

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Rounce, D. R., D. J. Quincey, and D. C. McKinney. "Debris-covered glacier energy balance model for Imja–Lhotse Shar Glacier in the Everest region of Nepal." Cryosphere 9, no. 6 (2015): 2295–310. http://dx.doi.org/10.5194/tc-9-2295-2015.

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Abstract. Debris thickness plays an important role in regulating ablation rates on debris-covered glaciers as well as controlling the likely size and location of supraglacial lakes. Despite its importance, lack of knowledge about debris properties and associated energy fluxes prevents the robust inclusion of the effects of a debris layer into most glacier surface energy balance models. This study combines fieldwork with a debris-covered glacier energy balance model to estimate debris temperatures and ablation rates on Imja–Lhotse Shar Glacier located in the Everest region of Nepal. The debris

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Koutkias, V., and J. Bouaud. "Contributions from the 2016 Literature on Clinical Decision Support." Yearbook of Medical Informatics 26, no. 01 (2017): 133–38. http://dx.doi.org/10.15265/iy-2017-031.

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Summary Objectives: To summarize recent research and select the best papers published in 2016 in the field of computerized clinical decision support for the Decision Support section of the IMIA yearbook. Methods: A literature review was performed by searching two bibliographic databases for papers related to clinical decision support systems (CDSSs). The aim was to identify a list of candidate best papers from the retrieved papers that were then peer-reviewed by external reviewers. A consensus meeting of the IMIA editorial team finally selected the best papers on the basis of all reviews and s

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