cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Anacronicta obscura
Creators: name: Irungbam, Jatishwor Singh
name: Fric, Zdenek Faltynek
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Noctuidae
Anacronicta
Anacronicta obscura

description: 4. Anacronicta obscura (Leech, 1900: p. 527) (Aplectoides)
(Figs. 12, 20)
Type locality. C & W China.
Material examined. Laos, 1♂, Phou Khoun, 13. December. 2017, native collector (in the collection of Keitaro Eda, Japan).
Diagnosis. Anacronicta obscura (Fig. 12) is very similar to the new species, A. albicans sp. nov. (Fig. 7) and A. infausta (Fig. 11) but differs in having more contrasting dark elements in the wing pattern and an area of ochre-yellowish coloration of the inner part of the hindwings. In the structure of male genitalia (Fig. 20), it differs by the shape of the valva and the position and size of the basal cornuti field of the vesica.
Distribution. India (Kashmir, Punjab, Kulu, Sultanpur), Pakistan, West China, North Vietnam. Thailand (Prov. Chaing Mai, Prow. Nan) (Kononenko & Pinratana 2013); Laos (Eda 2020).
description: Published as part of Irungbam, Jatishwor Singh & Fric, Zdenek Faltynek, 2025, Three new species of the genus Anacronicta Warren in Seitz, 1909 (Noctuidae: Pantheinae) from northeast India, pp. 171-185 in Zootaxa 5583 (1) on page 180, DOI: 10.11646/zootaxa.5583.1.10, http://zenodo.org/record/14797493
title: ADCO, Sixième cartulaire de Saint-Étienne de Dijon (1662), Cart. 30 (G 133), 441 folios, f. 460
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Sixième cartulaire de Saint-Étienne de Dijon (1662), Archives départementales de la Côte-d'Or, Cart. 30 (G 133), 441 folios, f. 460, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Sixième cartulaire de Saint-Étienne de Dijon (1662), Archives départementales de la Côte-d'Or, Cart. 30 (G 133), 441 folios, f. 460, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Field evaluation of new Kabuli chickpeas lines for the production of canned seeds
Creators: name: Casini, Paolo
Publisher: name: Advances in Horticultural Science
Year: 2018

description: There is an increased demand for canned chickpeas worldwide, which has also resulted in increased chickpea cultivation in Italy. The availability of Italian chickpea varieties, suitable for industrial transformation, is limited. The objective of the present study was to evaluate the field production of new Kabuli chickpea accessions and their suitability for industrial transformation. Thirteen accessions, provided by the International Centre for Agricultural Research of Turkey, together with ‘Blanco Sinaloa’, a commercial Mexican variety, were cultivated in Cesa, Tuscany, in 2016 and 2017. The average seed yield was 2.8 and 3.4 t ha-¹, respectively, in 2016 and 2017. Increased yield in 2017 was attributable to a more balanced rainfall pattern, compared to that in 2016 which induced increased vegetative growth. Based on production stability over the two-year trial, the varieties FLIP08-69C, FLIP-160C and FLIP05-157C turned out particularly suitable for cultivation. The climatic conditions in 2017 favored an increased presence of a Grade B seed classification [220-250 seeds per 100 g (caliber 8)] which is preferred by industry. Most varieties showed potential regarding seed dimension classification, however, of the varieties with a good production, FLIP05-157C was also characterized by seed gradation stability.
description: Advances in Horticultural Science, Vol 32 No 4 (2018)
Emergence of high-mass stars in complex fiber networks (EMERGE) IV. Environmental dependence of the fiber widths
Creators: name: Socci, A.
name: Hacar, A.
name: Bonanomi, F.
name: Tafalla, M.
name: Suri, S.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Despite their variety of scales throughout the interstellar medium, filaments in nearby low-mass clouds show a characteristic width of $\sim$ 0.1 pc from the analysis of {\it Herschel} observations. The origin of this characteristic width, however, has been a matter of intense discussions during the last decade. We explored a possible variation in this typical width with the EMERGE Early ALMA Survey, which includes seven star-forming regions in Orion (OMC-1/-2/-3/-4 South, LDN 1641N, NGC 2023, Flame Nebula). These targets, which exhibit different physical conditions, star formation histories, mass, and density regimes, were homogeneously surveyed at a resolution of $\sim$ 2000 au in N$_2$H$^+$ (1$-$0) with ALMA+IRAM-30m observations. We characterised the column density and temperature radial profiles of the 152 fibers identified in the survey using the automatic fitting routine FilChap. These Orion fibers show a departure from the isothermal condition with significant outward temperature gradients with $\nabla T_\mathrm{K} > 30$ K pc$^{-1}$. They also show a median full width at half maximum ($FWHM$) of $\sim 0.05$ pc, with a corresponding median aspect ratio of $\sim2$. More relevantly, we observe a systematic variation in these fiber $FWHM$ between different regions in our sample, and a direct inverse dependence of these $FWHM$ on their central column density, $N_0$, above $\gtrsim 10^{22}$ cm$^{-2}$. This dependency agrees with the expected $N_0-FWHM$ anti-correlation predicted in previous theoretical studies. Our homogeneous analysis returns the first observational evidence of an intrinsic and systematic variation in the fiber widths across different star-forming regions. While sharing comparable mass, length, and kinematic properties in all of our targets, fibers appear to adjust their $FWHM$ to their density and to the pressure in their host environment.
Diffusion Monte Carlo methods for Spin-Orbit-Coupled ultracold Bose gases
Creators: name: Sanchez-Baena, J.
name: Boronat, J.
name: Mazzanti, F.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: FOS: Physical sciences

description: We present two Diffusion Monte Carlo (DMC) algorithms for systems of ultracold quantum gases featuring synthetic spin-orbit interactions. The first one is a discrete spin generalization of the T- moves spin-orbit DMC, which provides an upper bound to the fixed-phase energy. The second is a spin-integrated DMC method which recovers the fixed-phase property by avoiding the definition of the effective Hamiltonian involved in the T-moves approach. The latter is a more accurate method but it is restricted to spin-independent two-body interactions. We report a comparison between both algorithms for different systems. As a check of the efficiency of both methods, we compare the DMC energies with results obtained with other numerical methods, finding agreement between both estimation
Bose-Einstein Correlations for Expanding Finite Systems
Creators: name: Csorgo, T.
name: Lorstad, B.
Publisher: name: arXiv
Year: 1995
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: There are two length-scales present simultaneously in all the principal directions for three-dimensionally expanding, finite systems. These are discussed in detail for the case of a longitudinally expanding system with a transverse flow and a transverse temperature profile. For systems with large geometrical sizes we find an $m_t$-scaling for the parameters of the Bose-Einstein correlation function, which may be valid in the whole transverse mass region for certain model parameters. In this limit, the Bose-Einstein correlations view only a small part of the source. The large geometrical sizes can be inferred from a simultaneous analysis of the invariant momentum distribution and the Bose-Einstein correlation function. A preliminary analysis of the NA44 data indicates that instead of a small fireball we are observing a big and expanding snowball in $S + Pb $ reactions at CERN SPS energies.
description: 5 pages, no figures, ReVTeX, uses espcrc1.sty, Quark Matter'95 conference, Nucl. Phys. A in press
Synthesis and in vitro evaluation of antiviral and cytostatic properties of novel 8-triazolyl acyclovir derivatives
Creators: name: Saftić, Dijana
name: Žinić, Biserka
name: Glavaš-Obrovac, Ljubica
name: Mirosława Studzińska
name: Paradowska, Edyta
name: Leśnikowski, Zbigniew J.
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: Pharmacology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: FOS: Biological sciences

description: As a part of the research aimed on identification of new nucleobase derivatives with improved biological properties, a series of novel 8-substituted acyclovir derivatives were synthesized. The 8-azidoguanosine 4 and novel 8-azidoacyclovir 9 were synthesized from commercially available guanosine 1 and acyclovir 6 which were transformed into 8-bromopurine derivatives 2 and 7 and hydrazine derivatives 3 and 8, respectively. 8-Triazolylguanosine 5 and 8-triazolylacyclovir analogs 10–12 were successfully synthesized via the Cu(I) catalyzed 1,3-dipolar cycloaddition reaction of azides 4 and 9 with propargyl alcohol, 4-pentyn-1-ol and 5-hexyn-1-ol. The novel 1,4-disubstituted 1,2,3-triazolyl compounds 5, 10–12 were evaluated for antiviral activity against selected DNA and RNA viruses and cytostatic activity against normal Madine Darby canine kidney (MDCK I) cells, and seven tumor cell lines (HeLa, CaCo-2, NCI-H358, Jurkat, K562, Raji and HuT78). While tested compounds exerted no antiviral activity at nontoxic concentrations, the 8-triazolyl acyclovir derivative 10, with the shortest alkyl substituent at the C-4 of triazole ring, was found to be the most active against the CaCo-2 cell line.
Spiralling whitefly and its management practices in the South Pacific. A review
Creators: name: Chand, Ravneel
name: Jokhan, Anjeela
name: Kelera, Railoa
Publisher: name: Advances in Horticultural Science
Year: 2018

description: A few species of whiteflies are considered a serious insect pest of vegetation and ornamental plants across many countries. The Spiralling whiteflies, Aleurodicus dispersus Russell has been recorded on many different plant species across countries. These whiteflies feed exclusively on leaves and have the ability to spread plant diseases. A great deal of research has been done on whiteflies in relation to which control methods would be most effective in pest management. The management of Spiralling whitefly in the South Pacific is heavily reliant on biological control (using the parasitic wasps, predators, and entomopathogenic fungi). Other control methods include physical, botanical, and chemical to keep the whitefly population at lower levels. In this paper, an overview of Spiralling whiteflies and its management practices in the South Pacific will be reviewed.
description: Advances in Horticultural Science, Vol 33 No 1 (2019)
Can gap-edge illumination excite spirals in protoplanetary disks? Three-temperature radiation hydrodynamics and NIR image modelling
Creators: name: Muley, Dhruv
name: Fuksman, Julio David Melon
name: Klahr, Hubert
Publisher: name: arXiv
Year: 2024
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The advent of high-resolution, near-infrared instruments such as VLT/SPHERE and Gemini/GPI has helped uncover a wealth of substructure in planet-forming disks, including large, prominent spiral arms in MWC 758, SAO 206462, and V1247 Ori among others. In the classical theory of disk-planet interaction, these arms are consistent with Lindblad-resonance driving by multi-Jupiter-mass companions. Despite improving detection limits, evidence for such massive bodies in connection with spiral substructure has been inconclusive. In search of an alternative explanation, we use the PLUTO code to run 3D hydrodynamical simulations with two comparatively low planet masses (Saturn-mass, Jupiter-mass) and two thermodynamic prescriptions (three-temperature radiation hydrodynamics, and the more traditional $β$-cooling) in a low-mass disk. In the radiative cases, an $m = 2$ mode, potentially attributable to the interaction of stellar radiation with gap-edge asymmetries, creates an azimuthal pressure gradient, which in turn gives rise to prominent spiral arms in the upper layers of the disk. Monte Carlo radiative transfer (MCRT) post-processing with RADMC3D reveals that in near-infrared scattered light, these gap-edge spirals are significantly more prominent than the traditional Lindblad spirals for planets in the mass range tested. Our results demonstrate that even intermediate-mass protoplanets -- less detectable, but more ubiquitous, than super-Jupiters -- are capable of indirectly inducing large-scale spiral disk features, and underscore the importance of including radiation physics in efforts to reproduce observations.
description: 11 pages, 9 figures incl. Appendices. A&A accepted; further comments and questions welcome
Combination of alginate based edible coating-betel essential oil in extending the shelf life of rose apple cv. Dalhari (Syzygium samarangense)
Creators: name: Setiawan, Chandra
name: Utama, Nafi
name: Pradana, Bintang
Publisher: name: Advances in Horticultural Science
Year: 2018

description: Rose apple cv. Dalhari is a local fruit grown in Berbah District, Special Region of Yogyakarta. This fruit perishable easily loses its water content and is attacked by microbes. This research aimed to determine the best combination between alginate and betel essential oil to inhibit the growth of microbes and maintain quality of rose apple cv. Dalhari. Alginate and betel essential oil treatments were used at three concentration levels, alone and in combinations, respectively of 2%, 2.5%, 3% and 0%, 0.1%, 0.2%. The results showed that combination treatment of 2.5% alginate and 0.1% betel essential oil was the most effective to maintain the fruit quality. The sole addition of betel essential oil was not able to inhibit microbial growth. Furthermore, combination of alginate based edible coating and betel essential oil was able to maintain the quality of rose apple cv. Dalhari up to nine days.
description: Advances in Horticultural Science, Vol 33 No 1 (2019)
Biochemical characterization of artichoke (Cynara cardunculus var. scolymus L.) spring genotypes from Marche and Abruzzo regions (Central Italy)
Creators: name: Galieni, Angelica
name: Stagnari, Fabio
name: Pisante, Michele
name: Platani, Cristiano
name: Ficcadenti, Nadia
Publisher: name: Advances in Horticultural Science
Year: 2018

description: Ten artichoke genotypes from Marche and Abruzzo Regions [Ascolano (As), Castorano (Cs), Clone Monsampolo, Jesino (Je), Mazzaferrata (Mz), Montelupone A, Montelupone B, Urbisaglia1 (Ub_1), Urbisaglia2 and Violetto Tardivo di Pesaro] were characterized for their quality traits and peculiar end-use attitudes, in comparison with the reference Romanesco Clone C3 (Cl_C3). Total polyphenols content (TPC), total flavonoid content (TFC) and antiradical activity were assessed in the receptacle and external bracts of both main and first order capitula. Cl_C3 showed high TPC and TFC values in the receptacle of the main flower heads (7.4 mg gallic acid equivalents, GAE, g-1 dry weight, DW, and 3.6 mg rutin equivalents, RUE, g-1 DW, respectively), confirming its attitude for fresh consumption. Je and Ub_1 showed great and stable (among main and first order capitula) head quality, highlighting their potential for breeding programs to enhance the content of functional compounds. Conversely, Mz and As could be appreciable for processing or pharmaceutical applications, being characterized by great TPC (external bracts, first order capitula: 2.8 and 2.7 mg GAE g-1 DW, respectively) and TFC (external bracts, first order capitula: 2.1 and 2.7 mg GAE g-1 DW, respectively) values in the waste parts. High correlations between TPC and TFC with antiradical activity were also observed. Our results suggest the possibility to promote the utilization in genetic breeding programs of the autochthonous artichoke populations, according to their peculiar characteristics, including also their biochemical composition.
description: Advances in Horticultural Science, Vol 33 No 1 (2019)
Non-perturbative collective inertias for fission: a comparative study
Creators: name: Giuliani, Samuel A.
name: Robledo, Luis M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The non-perturbative method to compute Adiabatic Time Dependent Hartree Fock Bogoliubov (ATDHFB) collective inertias is extended to the Generator Coordinate Method (GCM) including the case of density dependent forces. The two inertias schemes are computed along the fission path of the $^{234}$U and compared with the perturbative results. We find that the non-perturbative schemes predict very similar collective inertias with a much richer structure than the one predicted by perturbative calculations. Moreover, the non-perturbative inertias show an extraordinary similitude with the exact GCM inertias computed numerically from the energy overlap. These results indicate that the non-perturbative inertias provide the right structure as a function of the collective variable and only a phenomenological factor is required to mock up the exact GCM inertia, bringing new soundness to the microscopic description of fission.
description: 8 pages, 2 figures
Influence of post-véraison water deficit on berries yield and quality of three table grape cultivars
Creators: name: Ashori, Marjan
name: Ghasemnezhad, Mahmood
name: Biglouei, Mohammad Hassan
Publisher: name: Advances in Horticultural Science
Year: 2018

description: In order to investigate the effect of regulated deficient irrigation (RDI) on some quantitative and qualitative characteristics of the three commercial grapevine cultivars (i.e. Keshmeshi, Sahebi and Sharabi), an experiment was set in split plot arranged in an RCBD design with three replications. In this experiment, irrigation treatments including 100 (as control), 80%, 60% and 40% crop evapotranspiration (ETc) were implemented in a period between onset of berries color change (véraison) to harvest of fruits. At the end of experimental period, some traits such as berry weight, berry length, berry diameter and cluster weight as well as some fruit quality traits such as total soluble solids (TSS), titratable acidity (TA), flavonoids, anthocyanin, total phenol, and total antioxidant capacity were measured. The results of this experiment revealed that effect of RDI at different levels on yield, berry and cluster weight, berry length and diameter, TSS, TA, anthocyanin, phenol, and flavonoid was significant. Also, there was no significant difference between control and 80% ETc in terms of yield, berry diameter, TSS, and TA; and these treatment enhanced total phenol, anthocyanin and antioxidant activity in the three cultivars. In both years of experiment, RDI remarkably enhanced anthocyanin, flavonoids, antioxidant activity and phenolic concentration. Overall, the results indicated that 80% ETc might be sufficient to gain adequate yield in Keshmeshi, Sahebi and Sharabi without undermining the quality of fruit.
description: Advances in Horticultural Science, Vol 33 No 1 (2019)
title: Konstruktivistisches Prozessmodell Historischer Erkenntnisbildung
title: Constructivist modell of historiography
Creators: name: Ernst, Sebastian
name: Pröve, Ralf
name: Krieger, Jannis M.
Publisher: name: Universität Potsdam
Year: 2024
Subjects: subject: 370 Bildung und Erziehung
subject: 900 Geschichte und Geografie

description: Vergangenheit ist vergangen, Geschichte wird gemacht. An diesem Konstruktionsprozess sind nicht nur die historischen Akteur:innen und deren Quellen, sondern in besonderem Maße auch die Historiker:innen, die sich mit diesen auseinandersetzen, beteiligt. Sie sind es, die die Quellen erst zum Sprudeln bringen. Was dabei zutage tritt, ist somit in hohem Maße von den Forschenden selbst, von ihren Vorannahmen und Methoden aber auch von ihren sozialen, kulturellen und biografischen Prägungen abhängig. Das hier vorgestellte Prozessmodell versucht, diese als Einflussfaktoren zu fassen und sichtbar zu machen, um auf dieser Basis eine erweiterte wissenschaftliche (Selbst-)Reflexion zu ermöglichen.
description: The past is gone, history is made. In the process of making history, not only the historical actors and their sources are involved, but also historians who engage with them, to a significant extent. They are the ones who bring the sources to life. What emerges from this is therefore highly dependent on the researchers themselves, their assumptions and methods, but also on their social, cultural, and biographical backgrounds. The process model presented here attempts to capture these factors as influences and make them visible, in order to enable an extended scholarly (self-)reflection on this basis.
First Solar Orbiter observation of a dark halo in the solar atmosphere
Creators: name: Lezzi, Serena Maria
name: Long, David M.
name: Andretta, Vincenzo
name: Baker, Deborah
name: Dolliou, Antoine
name: Murabito, Mariarita
name: Parenti, Susanna
name: Prado, Natalia Zambrana
Publisher: name: arXiv
Year: 2024
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Solar active regions (ARs) are often surrounded by dark large areas of reduced emission compared to the quiet Sun, observed at various wavelengths corresponding to chromosphere, transition region (TR) and corona, and known as Dark Halos (DHs). DHs have been insufficiently studied, and the mechanisms behind their darker emission remain unclear. This study aims to investigate for the first time the fine structure of a DH observed by the EUV High Resolution Imager (HRI$_{EUV}$) onboard the ESA's Solar Orbiter (SO) mission and its appearance in the TR. We utilized the extensive 1-hour dataset from SO on 19 March 2022, which includes high-resolution observations of NOAA 12967 and part of the surrounding DH. We analyzed the dynamics of the HRI$_{EUV}$ DH fine structure and its appearance in the HRI$_{Lyα}$ image and the Spectral Imaging of the Coronal Environment (SPICE) Ly$β$, C III, N VI, O VI and Ne VIII lines, which sample the TR in the logT (K) $\sim$ 4.0 - 5.8 range. This analysis was complemented with a simultaneous B$_{LOS}$ magnetogram taken by the High Resolution Telescope (HRT). We report the presence of a peculiar fine structure which is not observed in the quiet Sun, characterized by combined bright EUV bundles and dark regions, arranged and interconnected in such a way that they cannot be clearly separated. They form a spatial continuum extending approximately radially from the AR core, suggesting a deep connection between the DH and the AR. Additionally, we find that the bright EUV bundles are observed in all the SPICE TR lines and the HRI$_{Lyα}$ band and present photospheric B$_{LOS}$ footprints in the HRT magnetogram. This spatial correlation indicates that the origin of the 174 Å DH may lie in the low atmosphere, i.e. photosphere/chromosphere.
description: 9 pages, 8 figures; accepted for A&A
Parameter estimation for fractional Poisson processes
Creators: name: Cahoy, Dexter
name: Uchaikin, Vladimir V.
name: Woyczynski, Wojbor A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Methodology (stat.ME)
subject: FOS: Computer and information sciences

description: The paper proposes a formal estimation procedure for parameters of the fractional Poisson process (fPp). Such procedures are needed to make the fPp model usable in applied situations. The basic idea of fPp, motivated by experimental data with long memory is to make the standard Poisson model more flexible by permitting non-exponential, heavy-tailed distributions of interarrival times and different scaling properties. We establish the asymptotic normality of our estimators for the two parameters appearing in our fPp model. This fact permits construction of the corresponding confidence intervals. The properties of the estimators are then tested using simulated data.
X-Ray Binary Systems in the Small Magellanic Cloud
Creators: name: Kahabka, P.
name: Pietsch, W.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the result of a systematic search for spectrally hard and soft X-ray binary systems in the Small Magellanic Cloud (SMC). This search has been applied to ROSAT PSPC data (0.1-2.4 keV) collected during 9 pointed observations towards this galaxy covering a time span of 2 years from October 91 till October 93. Selection criteria have been defined in order to confine the sample of candidates. Finally 7 spectrally hard and 4 spectrally soft sources were selected from the list as candidates for binaries in the SMC. The sample is luminosity limited (>3.10**35 erg/s). SMC X-1 has been observed during a full binary orbit starting with a low-state covering an X-ray eclipse and emerging into a bright long-duration flare with two short-duration flares separated by 10 hours. The Be type transient SMC X-2 has been redetected with ROSAT. Variability has been found in the sources RX J0051.8-7231 and RX J0052.1-731 already discovered with Einstein. RX J0101.0-7206 has been discovered at the north-eastern boundary of the giant SMC HII region N66 during an X-ray outburst and half a year later during a quiescent phase. A variable source, RX J0049.1-7250, located north-east of the SMC supernova remnant N19 and which may either be an X-ray binary or an AGN turns out to be strongly absorbed. It may be located behind the SMC. If it is an X-ray binary then it radiates at the Eddington limit in the X-ray bright state. Another variable and hard X-ray source RX J0032.9-7348 has been discovered at the south-eastern border of the body of the SMC. A high mass X-ray binary nature is favored for this source. We searched for CAL87 like systems in the SMC catalog and found none. A new candidate supersoft source RX J0103.8-7254 has been detected. We cannot exclude that it is a foreground object.
description: 22 pages, Latex
title: Материаловедение. Текстильная промышленность
Creators: name: ELS IPR BOOKS
Publisher: name: Профобразование, Ай Пи Ар Медиа
Year: 2024

description: Издание состоит из практических занятий для закрепления знаний, полученных в рамках теоретического курса. Студенты научатся рассчитывать показатели свойств сырья, полуфабрикатов и тканей, а также технологические параметры текстильного оборудования. Практикум состоит из нескольких разделов, в каждом из которых представлены основные формулы для расчетов, приведены принципы и примеры решения типовых задач с учетом показателей работы оборудования. Подготовлен с учетом требований Федерального государственного образовательного стандарта среднего профессионального образования. Практикум предназначен для студентов, обучающихся по специальностям и профессиям укрупненных групп «Технологии легкой промышленности» и «Экономика и управление», изучающих дисциплину «Материаловедение».
DaFoEs: Mixing Datasets towards the generalization of vision-state deep-learning Force Estimation in Minimally Invasive Robotic Surgery
Creators: name: Reyzabal, Mikel De Iturrate
name: Chen, Mingcong
name: Huang, Wei
name: Ourselin, Sebastien
name: Liu, Hongbin
Publisher: name: arXiv
Year: 2024
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Artificial Intelligence (cs.AI)
subject: Robotics (cs.RO)
subject: FOS: Computer and information sciences

description: Precisely determining the contact force during safe interaction in Minimally Invasive Robotic Surgery (MIRS) is still an open research challenge. Inspired by post-operative qualitative analysis from surgical videos, the use of cross-modality data driven deep neural network models has been one of the newest approaches to predict sensorless force trends. However, these methods required for large and variable datasets which are not currently available. In this paper, we present a new vision-haptic dataset (DaFoEs) with variable soft environments for the training of deep neural models. In order to reduce the bias from a single dataset, we present a pipeline to generalize different vision and state data inputs for mixed dataset training, using a previously validated dataset with different setup. Finally, we present a variable encoder-decoder architecture to predict the forces done by the laparoscopic tool using single input or sequence of inputs. For input sequence, we use a recurrent decoder, named with the prefix R, and a new temporal sampling to represent the acceleration of the tool. During our training, we demonstrate that single dataset training tends to overfit to the training data domain, but has difficulties on translating the results across new domains. However, dataset mixing presents a good translation with a mean relative estimated force error of 5% and 12% for the recurrent and non-recurrent models respectively. Our method, also marginally increase the effectiveness of transformers for force estimation up to a maximum of ~15%, as the volume of available data is increase by 150%. In conclusion, we demonstrate that mixing experimental set ups for vision-state force estimation in MIRS is a possible approach towards the general solution of the problem.
La Gouvernance des Technologies Emergentes : Cas de la Fintech au Maroc
Creators: name: EL HAJOUJI, Amine
name: MESK, Hicham
Publisher: name: Zenodo
Year: 2024
Subjects: Fintech ; Regtech ; Sandbox ; Gouvernance ; Innovation Disruptive

description: L’industrie FINTECH à travers la panoplie des modèles économiques qu’elle développe est réellement disruptive pour l’ensemble de son écosystème et est capable de bouleverser l’hégémonie des acteurs traditionnels et de constituer un système financier alternatif qui fonctionne en parallèle et en collaboration avec le système financier classique.

En raison d'une rapide expansion de cette industrie, il est impératif pour les autorités de régulation de rester vigilants pour prévenir tout risque d'instabilité financière.

En effet, les autorités de régulation doivent assurer au maximum un équilibre entre d’une part l’encouragement des opportunités importantes qu’offrent les FINTECHS et ne pas freiner leur potentiel d’innovation et de l’autre part limiter les risques et contrôler leur activité pourvu de maintenir la stabilité financière, de protéger les consommateurs, et de garantir une équité vis-à-vis des acteurs traditionnels.

Le risque d'un dilemme réglementaire peut alors apparaître entre la réalisation d'un équilibre entre les règles prudentielles et la promotion de l'innovation fintech, tout en maintenant la stabilité financière et l’équité avec les acteurs traditionnels.

L’objectif de cet article est de passer en revue les différents modes de régulation possible de l’industrie FINTECH et de l’autre part faire un état des lieux de la situation au Maroc.
Charm Effects in the $\bar{MS}$ Bottom Quark Mass from $Υ$ Mesons
Creators: name: Hoang, A. H.
name: Manohar, A. V.
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the shift in the $Υ$ mass due to a non-zero charm quark mass. This shift affects the value of the $\bar{\rm MS}$ $b$-quark mass extracted from the $Υ$ system by about -20 MeV, due to an incomplete cancellation of terms that are non-analytic in the charm quark mass. The precise size of the shift depends on unknown higher order corrections, and might have a considerable uncertainty if they are large.
description: 7 pages, revtex, 2 postscript figures
Research Software Phases, Sustainability, and RSEs
Creators: name: Katz, Daniel S.
name: Clifford, Ben
name: Hunter Kesling, Kevin
name: Chard, Kyle
name: Babuji, Yadu
Publisher: name: Zenodo
Year: 2025

description: Abstract: Research software projects often are initially funded by a grant that supports development of the software. But when the grant ends, the projects have to shift to another model to support the required software maintenance, if the software is going to continue being used. This talk will look at the Parsl project and its effort to become sustainable, across a set of project phases. It will also look at the different kinds of RSE work that have taken place during the project. These activities, phases, and developer types appear to be useful concepts for planning or studying other research software projects, or research software as a whole. The talk will be partly aimed at finding others who want to collaborate on understanding how general these results are, and how much they can benefit other projects.
Shared identity and shared information in social media: development and validation of the identity bubble reinforcement scale
Creators: name: Kaakinen, Markus
name: Sirola, Anu
name: Savolainen, Iina
name: Oksanen, Atte
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Social media facilitates the formation of identity bubbles that reinforce shared identities, social homophily, and reliance on the information shared within the bubbles. Currently, researchers need more social psychological measures to assess how people perceive their relationships with online networks and information shared on social media. This article reports the development and Finnish and English validations of the identity bubble reinforcement scale (IBRS), consisting of subscales on social identification, homophily, and information bias. Studies 1 and 2 (N = 1200, N = 160; age 15–25 years) validated the 6-item measure (IBRS-6) in Finland and Study 3 replicated the results with both 6-item and 9-item (IBRS-9) measures in the United States (N = 501, age 18–25 years). Across all 3 studies and 2 countries, the IBRS showed good construct validity and correlated positively with social media use and group-behavior measures. The IBRS is an applicable measure for social media group behavior, and its subscales can also be used separately.
Documentation of Some Lunar and Solar Events at Casa Grande, AZ. (and other items)
Creators: name: Evans, John H.
name: Hillman, Harry
Year: 1979
Subjects: subject: Pioneer through Classic periods
valueUri: https://core.tdar.org/browse/temporal-keyword/5421/pioneer-through-classic-periods
subject: Hohokam
valueUri: https://core.tdar.org/browse/culture-keyword/21/hohokam
subject: Great House / Big House
valueUri: https://core.tdar.org/browse/site-type/317/great-house-big-house
subject: Architectural Documentation
valueUri: https://core.tdar.org/browse/investigation-type/16/architectural-documentation
subject: Archaeological Overview
valueUri: https://core.tdar.org/browse/investigation-type/1/archaeological-overview

description: This document includes 4 versions of a report about lunar and solar events at the Great House at Casa Grande Ruins National Monument. These include: a presentation paper, a published version, a version prepared for Arizona Highway Magazine and a Science News summary. There is also a constellation chart to check Canopus alignment. The report outlines basic history and construction of the Great House that facilitates astronomical events. The report references computer data, cutting edge at the time, but sadly outdated today.
Numerical Simulation of a Two-Dimensional Blume-Capel Ferromagnet in an Oscillating Magnetic Field with a Constant Bias
Creators: name: Mendes, Celeste
name: Buendia, Gloria M.
name: Rikvold, Per Arne
Publisher: name: arXiv
Year: 2024
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We perform a numerical study of the kinetic Blume-Capel (BC) model to find if it exhibits the metamagnetic anomalies previously observed in the kinetic Ising model for supercritical periods. We employ a heat-bath Monte Carlo (MC) algorithm on a square lattice in which spins can take values of $\pm 1, 0$, with a non-zero crystal field, subjected to a sinusoidal oscillating field in conjunction with a constant bias. In the ordered region, we find an equivalent hysteretic response of the order parameters with its respective conjugate fields between the kinetic and the equilibrium model. In the disordered region (supercritical periods), we observed two peaks, symmetrical with respect to zero bias, in the susceptibility and scaled variance curves, consistent with the numerical and experimental findings on the kinetic Ising model. This behavior does not have a counterpart in the equilibrium model. Furthermore, we find that the peaks occur at higher values of the bias field and become progressively smaller as the density of zeros, or the amplitude of the oscillating field, increases. Using nucleation theory, we demonstrate that these fluctuations, as in the Ising model, are not a critical phenomenon, but that they are associated with a crossover between a single-droplet (SD) and a multi-droplet (MD) magnetization switching mechanism. For strong (weak) bias, the SD (MD) mechanism dominates. We also found that the zeros concentrate on the droplets' surfaces, which may cause a reduced interface tension in comparison with the Ising model . Our results suggest that metamagnetic anomalies are not particular to the kinetic Ising model, but rather are a general characteristic of spin kinetic models, and provide further evidence that the equivalence between dynamical phase transitions and equilibrium ones is only valid near the critical point.
description: 34 pages, 11 figures
A Picture of D-branes at Strong Coupling II. Spinning Partons
Creators: name: Gustafsson, H.
name: Lindstrom, U.
Publisher: name: arXiv
Year: 1998
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study the Born-Infeld D-brane action in the limit when the string coupling goes to infinity. The resulting actions is presented in an arbitrary background and shown to describe a foliation of the world-volume by strings. Using a recently developed ``degenerate'' supergravity the parton picture is shown to be applicable also to supersymmetric D-branes.
description: 14 pages, Latex
Likelihood inference for dynamic linear models with Markov switching parameters: on the efficiency of the Kim filter
Creators: name: Kim, Young Min
name: Kang, Kyu Ho
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Biophysics
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer
subject: Inorganic Chemistry

description: The Kim filter (KF) approximation is widely used for the likelihood calculation of dynamic linear models with Markov regime-switching parameters. However, despite its popularity, its approximation error has not yet been examined rigorously. Therefore, this study investigates the reliability of the KF approximation for maximum likelihood (ML) and Bayesian estimations. To measure the approximation error, we compare the outcomes of the KF method with those of the auxiliary particle filter (APF). The APF is a numerical method that requires a longer computing time, but its numerical error can be sufficiently minimized by increasing simulation size. According to our extensive simulation and empirical studies, the likelihood values obtained from the KF approximation are practically identical to those of the APF. Furthermore, we show that the KF method is reliable, particularly when regimes are persistent and sample size is small. From the Bayesian perspective, we show that the KF method improves the efficiency of posterior simulation. This study contributes to the literature by providing evidence to justify the use of the KF method in both ML and Bayesian estimations.
Compact Anisotropic Models in General Relativity by Gravitational Decoupling
Creators: name: Morales, E.
name: Tello-Ortiz, Francisco
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Durgapal's fifth isotropic solution describing spherically symmetric and static matter distribution is extended to an anisotropic scenario. To do so we employ the gravitational decoupling through the minimal geometric deformation scheme. This approach allows to split Einstein's field equations in two simply set of equations, one corresponding to the isotropic sector and other to the anisotropic sector described by an extra gravitational source. The isotropic sector is solved by the Dugarpal's model and the anisotropic sector is solved once a suitable election on the minimal geometric deformation is imposes. The obtained model is representing some strange stars candidates and fulfill all the requirements in order to be a well behaved physical solution to the Einstein's field equations.
Smart Drug-Delivery Systems for Cancer Nanotherapy
Creators: name: Sanchez-Moreno, Paola
name: Ortega-Vinuesa, Juan Luis
name: Peula-Garcia, Jose Manuel
name: Marchal, Juan Antonio
name: Boulaiz, Houria
Publisher: name: arXiv
Year: 2024
Subjects: subject: Tissues and Organs (q-bio.TO)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Applied Physics (physics.app-ph)
subject: Biological Physics (physics.bio-ph)
subject: FOS: Biological sciences
subject: FOS: Physical sciences

description: Despite all the advances achieved in the field of tumor-biology research, in most cases conventional therapies including chemotherapy are still the leading choices. The main disadvantage of these treatments, in addition to the low solubility of many antitumor drugs, is their lack of specificity, which explains the frequent occurrence of serious side effects due to nonspecific drug uptake by healthy cells. Progress in nanotechnology and its application in medicine have provided new opportunities and different smart systems. Such systems can improve the intracellular delivery of the drugs due to their multifunctionality and targeting potential. The purpose of this manuscript is to review and analyze the recent progress made in nanotherapy applied to cancer treatment. First, we provide a global overview of cancer and different smart nanoparticles currently used in oncology. Then, we analyze in detail the development of drug-delivery strategies in cancer therapy, focusing mainly on the intravenously administered smart nanoparticles with protein corona to avoid immune-system clearance. Finally, we discuss the challenges, clinical trials, and future directions of the nanoparticle-based therapy in cancer.
description: Preprint version, 25 pages, 7 figures, 3 tables. Authors thank to Bentham Science the posibility of deposit the ACCEPTED VERSION of the peer-reviewed article after 12 months of publication on journal web site on arXiv repository. The published manuscript is available at EurekaSelect via https://www.eurekaselect.com/openurl/content.php?genre=article&doi=10.2174/1389450117666160527142544
Mapping radial abundance gradients with Gaia-ESO open clusters: Evidence of recent gas accretion in the Milky Way disk
Creators: name: Palla, Marco
name: Magrini, Laura
name: Spitoni, Emanuele
name: Matteucci, Francesca
name: Vázquez, Carlos Viscasillas
name: Franchini, Mariagrazia
name: Molero, Marta
name: Randich, Sofia
Publisher: name: arXiv
Year: 2024
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Context. Recent evidences from spectroscopic surveys point towards the presence of a metal-poor, young stellar population in the chemical thin disk. In this context, the investigation of the spatial distribution and time evolution of precise, unbiased abundances is fundamental to disentangle the scenarios of evolution of the Galaxy. Aims. We study the evolution of abundance gradients in the Milky Way by taking advantage of a large sample of open clusters, which are among the best tracers for this purpose. In particular, we use data from the last release of the Gaia-ESO survey. Methods. We perform careful selection of open cluster stars excluding those that may be affected by biases in spectral analysis. The cleaned open clusters sample is compared with detailed chemical evolution models for the Milky Way, using well tested stellar yields and prescription for radial migration. Different scenarios of Galaxy evolution are tested to explain the data, i.e. the two-infall and the three-infall frameworks, suggesting that the chemical thin disk is formed by one or two subsequent gas accretion episodes, respectively. Results. With the performed selection in cluster stars, we still find a metallicity decrease between intermediate age (1
description: 15 pages + appendices, 10 Figures, 3 Tables. Accepted for publication in A&A
Investigating the Surrogate Modeling Capabilities of Continuous Time Echo State Networks
Creators: name: Bhatnagar, Saakaar
Publisher: name: arXiv
Year: 2023
Subjects: subject: Computational Engineering, Finance, and Science (cs.CE)
subject: FOS: Computer and information sciences

description: Continuous Time Echo State Networks (CTESNs) are a promising yet under-explored surrogate modeling technique for dynamical systems, particularly those governed by stiff Ordinary Differential Equations (ODEs). A key determinant of the generalization accuracy of a CTESN surrogate is the method of projecting the reservoir state to the output. This paper shows that of the two common projection methods (linear and nonlinear), the surrogates developed via the nonlinear projection consistently outperform those developed via the linear method. CTESN surrogates are developed for several challenging benchmark cases governed by stiff ODEs, and for each case, the performance of the linear and nonlinear projections is compared. The results of this paper demonstrate the applicability of CTESNs to a variety of problems while serving as a reference for important algorithmic and hyper-parameter choices for CTESNs