cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Genetic and environmental risk factors for chronic obstructive pulmonary disease
Creators: name: Matheson., Melanie Claire
Publisher: name: Monash University
Year: 2021

description: This thesis was scanned from the print manuscript for digital preservation and is copyright the author.
 Researchers can access this thesis by asking their local university, institution or public library to
 make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.
A 2D Model for Coronal Bright Points: Association with Spicules, UV bursts, Surges and EUV Coronal Jets
Creators: name: Nóbrega-Siverio, D.
name: Moreno-Insertis, F.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Coronal Bright Points (CBPs) are ubiquitous structures in the solar atmosphere composed of hot small-scale loops observed in EUV or X-Rays in the quiet Sun and coronal holes. They are key elements to understand the heating of the corona; nonetheless, basic questions regarding their heating mechanisms, the chromosphere underneath, or the effects of flux emergence in these structures remain open. We have used the Bifrost code to carry out a 2D experiment in which a coronal-hole magnetic nullpoint configuration evolves perturbed by realistic granulation. To compare with observations, synthetic SDO/AIA, Solar Orbiter EUI-HRI, and IRIS images have been computed. The experiment shows the self-consistent creation of a CBP through the action of the stochastic granular motions alone, mediated by magnetic reconnection in the corona. The reconnection is intermittent and oscillatory, and it leads to coronal and transition-region temperature loops that are identifiable in our EUV/UV observables. During the CBP lifetime, convergence and cancellation at the surface of its underlying opposite polarities takes place. The chromosphere below the CBP shows a number of peculiar features concerning its density and the spicules in it. The final stage of the CBP is eruptive: magnetic flux emergence at the granular scale disrupts the CBP topology, leading to different ejections, such as UV bursts, surges, and EUV coronal jets. Apart from explaining observed CBP features, our results pave the way for further studies combining simulations and coordinated observations in different atmospheric layers.
description: Accepted in ApJL. 9 pages, 5 figures, 2 movies
Kinematics of the H$α$ and H$β$ broad line region in an SDSS sample of type 1 AGNs
Creators: name: Rakić, Nemanja
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Here we investigate the kinematics of the part of the broad line region (BLR) in active galactic nuclei (AGNs) emitting H$β$ and H$α$ emission lines. We explore the widths and asymmetries of the broad H$β$ and H$α$ emission lines in a sample of high quality (i.e. high signal to noise ratio) spectra of type 1 AGN taken from the Data Release 16 of the Sloan Digital Sky Survey, in order to explore possible deviation from the gravitationally bound motion. To find only the broad component of H$β$ and H$α$ we use the FANTASY (Fully Automated pythoN Tool for AGN Spectra analYsis) code for the multi-component modeling of the AGN spectra and for careful extraction of the broad emission line parameters. We show that based on the broad line profiles widths and asymmetries, the BLR gas emitting H$β$ and H$α$ lines follows similar kinematics, and seems to be virialized in our sample of type 1 AGN.
description: 11 pages, 14 figures, accepted for publication in Monthly Notices of the Royal Astronomical Society
Additional file 1 of Free drug provision for tuberculosis increases patient follow-ups and successful treatment outcomes in the Indian private sector: a quasi experimental study using propensity score matching
Creators: name: Sodhi, Ridhima
name: Penkunas, Michael J.
name: Pal, Arnab
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Medicine
subject: Pharmacology
subject: Ecology
subject: FOS: Biological sciences
subject: Science Policy
classificationCode: 60506
subject: Virology
subject: Computational Biology

description: Supplementary Material 1
К ВОПРОСУ ОБ УГОЛОВНО-ПРАВОВОЙ ХАРАКТЕРИСТИКЕ РАЗБОЯ
Creators: name: ЛАТИФОВ ЭЛШАН ФИКРАТ-ОГЛЫ
Publisher: name: StudNet
Year: 2020
Subjects: РАЗБОЙ
ГРАБЕЖ
ПРЕСТУПЛЕНИЯ ПРОТИВ СОБСТВЕННОСТИ
ROBBERY
CRIMES AGAINST PROPERTY

description: В данной статье рассмотрено такое преступление, как разбой. На основе анализа законодательства, правовой позиции Верховного суда Российской Федерации, а также результатов теоретических исследований раскрыта правовая природа данного деяния, приведены его признаки. На основе подробного исследования состава данного преступления, разбой разграничен от иных общественно-опасных уголовно-правовых деяний. Статистика свидетельствует, что в Российской Федерации на протяжении многих лет наиболее распространенными являются преступления против собственности. В структуре зарегистрированных преступлений их доля неизменно превышает 50 %. Статистика также показывает, что в общем числе зарегистрированных преступлений заметным удельным весом обладает разбой.This article considers such a crime as robbery. Based on the analysis of the legislation, the legal position of the Supreme Court of the Russian Federation, as well as the results of theoretical studies, the legal nature of this act is revealed, its signs are given. Based on a detailed study of the composition of this crime, robbery is delimited from other socially dangerous criminal offenses. Statistics show that in the Russian Federation for many years the most common are crimes against property. In the structure of recorded crimes, their share invariably exceeds 50%. Statistics also show that robbery has a significant share in the total number of recorded crimes.
Role of Metal Nanoparticles on porosification of silicon by metal induced etching (MIE)
Creators: name: Saxena, Shailendra K.
name: Yogi, Priyanka
name: Yadav, Pooja
name: Mishra, Suryakant
name: Pandey, Haardik
name: Rai, Hari Mohan
name: Kumar, Vivek
name: Sagdeo, Pankaj R.
name: Kumar, Rajesh
Publisher: name: arXiv
Year: 2016
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Porosification of silicon (Si) by metal induced etching (MIE) process have been studies here to understand the etching mechanism. The etching mechanism has been discussed on the basis of electron transfer from Si to metal ion (Ag$^+$) and metal to H$_2$O$_2$. Role of silver nanoparticles (AgNPs) in the etching process has been investigated by studying the effect of AgNPs coverage on surface porosity. A quantitative analysis of SEM images, done using Image J, shows a direct correlation between AgNPs coverage and surface porosity after the porosification. Density of Si nanowires (NWs) also varies as a function of AgNPs fractional coverage which reasserts the fact that AgNPs governs the porosification process during MIE.
description: 8 pages, 5 figures
D1.5 Data Management Platform
Creators: name: Amram, Denise
name: Comandé, Giovanni
name: Noferi, Stefano
Publisher: name: Zenodo
Year: 2023
Subjects: Data
Data protocol
DMP

description: This deliverable describes the Data Management Platform developed for the VALKYRIES project under T1.5. It includes three sections: the first one refers to a guided system to fill the data management plan, according to the instructions described in D1.3, D1.16 and D1.17 aiming to collect and curate data as open as possible and as close as necessary; the second one refers to guidelines for first responders and, more generally innovators, dealing with emergency scenarios in order to enable data sharing under the current EU Data Strategy as described in D3.3, D1.4, D1.19 and a section dedicated to the ethics and diversity management, already delivered in D1.6 and here updated as described in D1.19.
Analytic models of dust temperature in high-redshift galaxies
Creators: name: Hirashita, Hiroyuki
name: Chiang, I-Da
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We investigate physical reasons for high dust temperatures ($T_\mathrm{dust}\gtrsim 40$ K) observed in some high-redshift ($z>5$) galaxies using analytic models. We consider two models that can be treated analytically: the radiative transfer (RT) model, {where a broad distribution of values for $T_\mathrm{dust}$ is considered}, and the one-tempearture (one-$T$) model, which assumes {uniform $T_\mathrm{dust}$}. These two extremes {serve to bracket the most realistic scenario}. We adopt the Kennicutt--Schmidt (KS) law to relate stellar radiation field to gas surface density, and vary the dust-to-gas ratio. As a consequence, our model is capable of predicting the relation between the surface density of star formation rate ($Σ_\mathrm{SFR}$) or dust mass ($Σ_\mathrm{dust}$) and $T_\mathrm{dust}$. We show that the high $T_\mathrm{dust}$ observed at $z\gtrsim 5$ favour low dust-to-gas ratios ($\lesssim 10^{-3}$). An enhanced star formation compared with the KS law gives an alternative explanation for the high $T_\mathrm{dust}$. The dust temperatures are similar between the two (RT and one-$T$) models as long as we use ALMA Bands 6--8. We also examine the relation among $Σ_\mathrm{SFR}$, $Σ_\mathrm{dust}$ and $T_\mathrm{dust}$ without assuming the KS law, and confirm the consistency with the actual observational data at $z>5$. In the one-$T$ model, we also examine a clumpy dust distribution, which predicts lower $T_\mathrm{dust}$ because of the leakage of stellar radiation. This enhances the requirement of low dust abundance or high star formation efficiency to explain the observed high $T_\mathrm{dust}$.
description: 12 pages, 5 figures, Accepted for publication in MNRAS
Salacia jenkinsii Kurz 1875
Creators: name: Jadhav, Durga C.
name: Prabhugaonkar, Ashish V.
name: Nandikar, Mayur D.
Publisher: name: Zenodo
Year: 2016
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Celastrales
Celastraceae
Salacia
Salacia jenkinsii

description: 5. Salacia jenkinsii Kurz (1875: 203)
 Type:— INDIA, Assam, s.d., Jenkins s.n. [lectotype, CAL! (CAL0000007481, Fig. 5); isolectotype, CAL! (CAL0000007480), designated here].
 Kurz (1875) described Salacia jenkinsii from Assam based on the collection by A. E. Jenkins. Type collections mentioned in the protologue (Assam, Jenkins s.n.) are placed at CAL (CAL0000007480; CAL0000007481), which constitutes flowering twigs corresponding to the original description. The specimen CAL0000007481 is designated lectotype since it bears more flowers.
description: Published as part of Jadhav, Durga C., Prabhugaonkar, Ashish V. & Nandikar, Mayur D., 2016, Nomenclature notes on the genus Salacia L. (Celastraceae) in India, pp. 121-130 in Phytotaxa 265 (2) on pages 125-127, DOI: 10.11646/phytotaxa.265.2.3, http://zenodo.org/record/13662647
ИСТОРИЯ И РАЗВИТИЕ ПОНЯТИЯ ГОСУДАРСТВЕННОГО СУВЕРЕНИТЕТА
Creators: name: ЛОЙКО ЕВГЕНИЙ ЕВГЕНЬЕВИЧ
Publisher: name: StudNet
Year: 2020
Subjects: СУВЕРЕНИТЕТ
НЕЗАВИСИМОСТЬ
ГОСУДАРСТВО
ПРАВИТЕЛЬСТВО
НАРОД
SOVEREIGNTY
INDEPENDENCE
STATE
GOVERNMENT
PEOPLE

description: Государственный суверенитет это неотчуждаемое юридическое качество независимого государства, символизирующее его политико-правовую самостоятельность, высшую ответственность и ценность как первичного субъекта международного права, необходимое для исключительного верховенства государственной власти и предполагающее неподчинение власти другого государства, возникающее или исчезающее в силу добровольного изменения статуса независимого государства как цельного социального организма, обусловленное правовым равенством независимых государств и лежащее в основе современного международного права. В статье рассмотрены основные подходы и развитие понятия государственного суверенитета от XVI до XXI века. Изучены подходы различных политологов и теоретиков права, рассмотрены особенности государственного суверенитета в последнее время.State sovereignty is the inalienable legal quality of an independent state, symbolizing its political and legal independence, supreme responsibility and value as the primary subject of international law, necessary for the exclusive supremacy of state power and implying disobedience to the power of another state, arising or disappearing due to voluntary change in the status of an independent state as a whole social organism, due to the legal equality of independent states and underlying modern international law The article considers the main approaches and development of the concept of state sovereignty from the XVI to the XXI century. The approaches of various political scientists and legal theorists are studied, and the features of state sovereignty in recent times are considered
Additional file 1 of Suitability of visual cues for freezing of gait in patients with idiopathic Parkinson’s disease: a case–control pilot study
Creators: name: An, Eui Jin
name: Sim, Woo-Sob
name: Kim, Seung Min
name: Kim, Jun Yup
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Cell Biology
subject: Science Policy
classificationCode: 111714
subject: Mental Health

description: Additional File 1: A document file with additional tables.
Characterisation of mAb-defined MHC and non-MHC molecules expressed by thymic stromal cells and thymocytes
Creators: name: Masciantonio., Marilina
Publisher: name: Monash University
Year: 2021

description: This thesis was scanned from the print manuscript for digital preservation and is copyright the author.
 Researchers can access this thesis by asking their local university, institution or public library to
 make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.
Trigonometric Parallaxes and Proper Motions of 134 Southern Late M, L, and T Dwarfs from the Carnegie Astrometric Planet Search Program
Creators: name: Weinberger, A. J.
name: Boss, A. P.
name: Keiser, S. A.
name: Anglada-Escudé, G.
name: Thompson, I. B.
name: Burley, G.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We report trigonometric parallaxes for 134 low mass stars and brown dwarfs, of which 38 have no previously published measurement and 79 more have improved uncertainties. Our survey targeted nearby targets, so 119 are closer than 30 pc. Of the 38 stars with new parallaxes, 14 are within 20 pc and seven are likely brown dwarfs (spectral types later than L0). These parallaxes are useful for studies of kinematics, multiplicity, and spectrophotometric calibration. Two objects with new parallaxes are confirmed as young stars with membership in nearby young moving groups: LP 870-65 in AB Doradus and G 161-71 in Argus. We also report the first parallax for the planet-hosting star GJ 3470; this allows us to refine the density of its Neptune-mass planet. One T-dwarf, 2MASS J12590470-4336243, previously thought to lie within 4 pc, is found to be at 7.8 pc, and the M-type star 2MASS J01392170-3936088 joins the ranks of nearby stars as it is found to be within 10 pc. Five stars that are over-luminous and/or too red for their spectral types are identified and deserve further study as possible young stars.
description: Accepted to AJ; two long tables
ОСОБЕННОСТИ ПСИХОЛОГИЧЕСКОГО КОНСУЛЬТИРОВАНИЯ ОНЛАЙН
Creators: name: СЕЛЕЗНЕВА Е. П.
Publisher: name: StudNet
Year: 2020
Subjects: ОНЛАЙН КОНСУЛЬТИРОВАНИЕ
ДИСТАНЦИОННОЕ КОНСУЛЬТИРОВАНИЕ
ПСИХОЛОГИЧЕСКАЯ ПОМОЩЬ В ИНТЕРНЕТЕ
ОСОБЕННОСТИ ПСИХОЛОГИЧЕСКОГО КОНСУЛЬТИРОВАНИЯ
ONLINE COUNSELING
DISTANCE COUNSELING
PSYCHOLOGICAL HELP ONLINE
FEATURES OF PSYCHOLOGICAL COUNSELING

description: В статье выделены особенности психологического консультирования онлайн. Сделан вывод о том, что психологическое консультирование онлайн в современном мире имеет большие перспективы, так как позволяет решать психологические проблемы с минимальными затратами времени и сил. Также рассмотрено формирование и развитие дистанционного консультирование при помощи интернета. Рассмотрено развитие теории и практики профессионального психологического консультирования и немедицинской психотерапии онлайн.The article highlights the features of online psychological counseling. It is concluded that online psychological counseling in the modern world has great prospects, as it allows you to solve psychological problems with minimal time and effort. Also discussed is the formation and development of distance counseling via the Internet. The development of the theory and practice of professional psychological counseling and non-medical psychotherapy online is considered.
A New Cold Stream near the Southern Galactic Pole
Creators: name: Yang, Yong
name: Zhao, Jing-Kun
name: Xue, Xiang-Xiang
name: Ye, Xian-Hao
name: Zhao, Gang
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We report the discovery of a cold stream near the southern Galactic pole (dubbed as SGP-S) detected in $Gaia$ Early Data Release 3. The stream is at a heliocentric distance of $\sim$ 9.5 kpc and spans nearly 58$^\circ$ by 0.6$^\circ$ on sky. The colour-magnitude diagram of SGP-S indicates an old and metal-poor (age $\sim$ 12 Gyr, [M/H] $\sim$ -2.0 dex) stellar population. The stream's surface brightness reaches an exceedingly low level of $Σ_G \simeq$ 36.2 mag arcsec$^{-2}$. Neither extant globular clusters nor other known streams are associated with SGP-S.
Generating Functions on Covering Groups
Creators: name: Ginzburg, David
Publisher: name: arXiv
Year: 2016
Subjects: subject: Representation Theory (math.RT)
subject: FOS: Mathematics
subject: 11F70

description: In this paper we prove Conjecture 1.2 in \cite{B-F}. This enables us to establish the meromorphic continuation of the standard partial $L$ function $L^S(s,π^{(n)})$. Here, $π^{(n)}$ is a genuine irreducible cuspidal representation of the group $GL_r^{(n)}({\bf A})$.
Warped Disk Galaxies. I. Linking U type Warps in Groups/Clusters to Jellyfish Galaxies
Creators: name: Zee, Woong-Bae G.
name: Yoon, Suk-Jin
name: Moon, Jun-Sung
name: An, Sung-Ho
name: Paudel, Sanjaya
name: Yun, Kiyun
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: arped disk galaxies are classified into two morphologies: S- and U-types. Conventional theories routinely attribute both types to galactic tidal interaction and/or gas accretion, but reproducing of U-types in simulations is extremely challenging. Here we investigate whether both types are governed by the same mechanisms using the most extensive sample of $\sim$8000 nearby (0.02\,$<$\,z\,$<$\,0.06) massive ($M_{*}/M_{\odot}$\,$>$\,$10^9$) edge-on disks from SDSS. We find that U-types show on average bluer optical colors and higher specific star formation rate (sSFR) than S-types, with more strongly warped U-types having higher sSFR. We also find that while the S-type warp properties correlate with the tidal force by the nearest neighbor regardless of the environment, there is no such correlation for U-types in groups/clusters, suggesting a non-tidal environmental could be at play for U-types, such as ram pressure stripping (RPS). Indeed, U-types are more common in groups/clusters than in fields and they have stellar mass, gas fraction, sSFR enhancement and phase-space distribution closely analogous to RPS-induced jellyfish galaxies in clusters. We furthermore show that the stellar disks of most RPS galaxies in the IllustirsTNG simulation are warped in U-shape and bent in opposite direction of stripped gas tails, satisfying theoretical expectations for stellar warps embeded in jellyfishes. We therefore suggest that despite the majority of U-types that live in fields being still less explained, RPS can be an alternative origin for those in groups/clusters.
description: 28 pages, 15 figures, accpeted for publication in ApJ
ФАКТОРЫ ПРОФЕССИОНАЛЬНОГО ВЫГОРАНИЯ ПСИХОЛОГОВ-КОНСУЛЬТАНТОВ
Creators: name: СЕЛЕЗНЕВА Е. П.
Publisher: name: StudNet
Year: 2020
Subjects: ВЫГОРАНИЕ
ПРОФЕССИОНАЛЬНОЕ ВЫГОРАНИЕ
ПСИХОЛОГ-КОНСУЛЬТАНТ
ФАКТОРЫ ВЫГОРАНИЯ
ЛИЧНОСТНЫЕ ФАКТОРЫ
СТАТУСНО-РОЛЕВЫЕ ФАКТОРЫ
КОРПОРАТИВНЫЕ (ПРОФЕССИОНАЛЬНО-ОРГАНИЗАЦИОННЫЕ) ФАКТОРЫ
BURNOUT
PROFESSIONAL BURNOUT
COUNSELING PSYCHOLOGIST
BURNOUT FACTORS
PERSONALITY FACTORS
ROLE-ROLE FACTORS
CORPORATE (PROFESSIONAL AND ORGANIZATIONAL) FACTORS

description: Понятие «синдром профессионального сгорания» означает конкретные изменения отношения специалиста к предмету профессиональной деятельности и к самому себе. В статье рассмотрены факторы профессионального выгорания психологов-консультантов, в частности, личностные, статусно-ролевые и корпоративные (профессионально-организационные). Сделан вывод о том, что корпоративные (профессионально-организационные) факторы являются основной причиной профессионального выгорания психологов-консультантов.The concept of "syndrome of professional combustion" means specific changes in the attitude of a specialist to the subject of professional activity and to himself. The article considers the factors of professional burnout of psychologists-consultants, in particular, personal, role-role and corporate (professional-organizational). It is concluded that corporate (professional and organizational) factors are the main reason for professional burnout of psychologists-consultants.
Tuning the work function in transition metal oxides and their heterostructures
Creators: name: Zhong, Zhicheng
name: Hansmann, Philipp
Publisher: name: arXiv
Year: 2016
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The development of novel functional materials in experimental labs combined with computer-based compound simulation brings the vision of materials design on a microscopic scale continuously closer to reality. For many applications interface and surface phenomena rather than bulk properties are key. One of the most fundamental qualities of a material-vacuum interface is the energy required to transfer an electron across this boundary, i.e. the work function. It is a crucial parameter for numerous applications, including organic electronics, field electron emitters, and thermionic energy converters. Being generally very resistant to degradation at high temperatures, transition metal oxides present a promising materials class for such devices. We have performed a systematic study for perovskite oxides that provides reference values and, equally important, reports on materials trends and the tunability of work functions. Our results identify and classify dependencies of the work function on several parameters including specific surface termination, surface reconstructions, oxygen vacancies, and heterostructuring.
Spatial segmentation methods
Creators: name: Raveendran, Nishanthi
Publisher: name: Macquarie University
Year: 2023
Subjects: Other education not elsewhere classified

description: Spatial statistics is one of the important topics in statistics. As a part of modelling a spatial distribution, spatial clustering is also an important component of spatial data analysis. Spatial data are often heterogeneous, indicating that there may not be a unique simple statistical model describing the data. However, if we cluster the data into homogeneous clusters or domains, it will be easier to apply the appropriate statistical model for each domain. The problem of finding homogeneous domains is known as segmentation, partitioning or clustering. It is commonly used in many areas including disease surveillance, spatial epidemiology, population genetics, landscape ecology, crime analysis and many other fields. For example, identifying the areas of risk and areas of safety is very important in spatial epidemiology. Generally, spatial clustering consists of two problems: identifying the number of homogeneous clusters and their boundaries. There is an extensive literature on a variety of different clustering problems and algorithms. In this thesis, we are particularly interested in developing new numerical algorithms for the spatial segmentation problem. We use binary data indicating the presence or absence of a particular plant species which are observed over a twodimensional lattice. To solve this segmentation problem, we propose to use the changepoint methodology, which is commonly used in time series analysis and many other research areas to identify abrupt points and their locations. In this thesis, we propose three new algorithms based on Sequential Importance Sampling (SIS), Markov Chain Monte Carlo (MCMC) and Cross-Entropy (CE) methods to spatial segmentation problem. The proposed algorithms are applied to both artificially generated and real data sets to illustrate their usefulness. Our results show that the proposed methodologies effectively identify homogeneous domains and their boundaries in spatial binary data.
Diamond OA in Europe: lessons learnt from the Diamas and Craft-OA projects
Creators: name: Mounier, Pierre
name: Bargheer, Margo
Publisher: name: Zenodo
Year: 2023

description: In September 2022 and January 2023, two EC funded projects started working on the development of resources to support Diamond OA in the European Research Area (ERA). While Diamas aims at providing non-technical resources to Diamond journals and publishers, such as guidelines, quality standards, training materials and toolkits, Craft-OA focuses on the technical side of publishing operations. The objective of Craft-OA is to upgrade publishing softwares used in the community, improve interoperability between platforms, and develop a “diamond discovery hub” that will support diamond journals’ visibility. Both project outputs will constitute the building blocks of a network of Capacity Centres that will form the European node of a global federation supporting Diamond OA worldwide. Our presentation will present the lessons learnt so far in the course of action of our projects. In particular: There is a wide variety of national, linguistic and disciplinary situations across the ERA regarding the organising and coordinating capacity of the Diamond OA community. There is no single quality standard for Diamond OA that can be applied uniformly across all specific national, linguistic and disciplinary communities. On the other hand, it is possible to identify a common core that can be adopted by all, forming the basis of what we call an “extensible” quality standard (EQSIP). Considering the variety of situations described above, it does not make sense to propose a centralised one-size-fits-all solution that would apply uniformly across the board. A distributed federated framework that selects, aggregates, and curates resources is much more adapted to the actual reality, while ensuring a core of common quality standards. There are specific challenges in engaging with a number of stakeholders who do not immediately identify themselves as “Diamond”, because they practise it without much reflection on what it entails. This is particularly true for many small learned societies who are de facto publishers of a single journal and are not aware of their particular status.
Salacia khasiana Purkayastha 1938
Creators: name: Jadhav, Durga C.
name: Prabhugaonkar, Ashish V.
name: Nandikar, Mayur D.
Publisher: name: Zenodo
Year: 2016
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Celastrales
Celastraceae
Salacia
Salacia khasiana

description: 6. Salacia khasiana Purkayastha (1938: 277)
 Type:— INDIA, Assam, Khasi Hills, 3–4,000 feet, Umteswar Forests, 07 July 1935, Shri Ram Sarma 12033 [lectotype, ASSAM! (sh. no. 5710, Fig. 6); isolectotype, ASSAM! (sh. no. 5711), designated here]; syntypes: ibid. 28 August 1936, Shri Ram Sarma 13541 ASSAM! (ASSAM 0000000046); ibid, 28 August 1936, Shri Ram Sarma 13542 CAL! (CAL0000007485).
 For his Salacia khasiana, Purkayastha neither gave type nor collector, only stated locality. Four specimens collected by Shri Ram Sarma as Salacia species, all from the Umteswar Forests, Assam, in 1935 and 1936 fit the protologue and placed at ASSAM and CAL.
 It has been found an annotation on Shri Ram Sarma 13541 (ASSAM 0000000046) as ‘lectotype’ signed by Rolla S. Rao, with no date or year mentioned, while on Shri Ram Sarma 12033 (sh. no. 5711) a label is pasted on the right lower part, in which the taxonomic note has been written by Rolla S. Rao on the 07 Dec.1967, but both are unpublished.
 Among these specimens Shri Ram Sarma 12033 (sh. no. 5710 and 5711) placed at ASSAM are best matches with the protologue, therefore, they are designated here as, respectively, lectotype and isolectotype while remaining collections are syntypes.
description: Published as part of Jadhav, Durga C., Prabhugaonkar, Ashish V. & Nandikar, Mayur D., 2016, Nomenclature notes on the genus Salacia L. (Celastraceae) in India, pp. 121-130 in Phytotaxa 265 (2) on pages 127-128, DOI: 10.11646/phytotaxa.265.2.3, http://zenodo.org/record/13662647
ОСОБЕННОСТИ АТРИБУТИВНОЙ ЛЕКСИКИ В ЭКСПРЕССИВНОЙ РЕЧИ ДЕТЕЙ СТАРШЕГО ДОШКОЛЬНОГО ВОЗРАСТА С ОБЩИМ НЕДОРАЗВИТИЕМ РЕЧИ
Creators: name: ИВАНОВА Н.В.
name: ИГНАТОВА Е.Д.
Publisher: name: StudNet
Year: 2020
Subjects: АТРИБУТИВНАЯ ЛЕКСИКА
СЛОВАРЬ
ДОШКОЛЬНЫЙ ВОЗРАСТ
ОБЩЕЕ НЕДОРАЗВИТИЕ РЕЧИ
ЭКСПРЕССИВНАЯ РЕЧЬ
ATTRIBUTIVE VOCABULARY
DICTIONARY
PRESCHOOL AGE
GENERAL SPEECH UNDERDEVELOPMENT
EXPRESSIVE SPEECH

description: В статье рассматриваются особенности атрибутивной лексики в экспрессивной речи детей старшего дошкольного возраста с общим недоразвитием речи. Актуальность темы определена тем, что трудности овладения атрибутивным словарем значительно минимизируют речевые контакты ребенка с окружающими. Без полноценного усвоения лексики невозможно овладеть речью как средством общения. Представлен теоретический анализ недостатков атрибутивного словаря у дошкольников с общим недоразвитием речи. Выдвигается исторический аспект изучения проблемы, рассмотрены точки зрения научных исследователей. Предлагаются основные направления работы и рекомендации с данной категорией детей.The article discusses the features of attributive vocabulary in the expressive speech of children of senior preschool age with a general underdevelopment of speech. The relevance of the topic is determined by the fact that the difficulties of mastering the attributive dictionary significantly minimize the child’s verbal contacts with others. Without the full mastery of vocabulary, it is impossible to master speech as a means of communication. A theoretical analysis of the deficiencies of the attributive dictionary among preschoolers with a general speech underdevelopment is presented. The historical aspect of studying the problem is advanced, the points of view of scientific researchers are considered. The main directions of work and recommendations with this category of children are offered.
MAXI J1957+032: a new accreting millisecond X-ray pulsar in an ultra-compact binary
Creators: name: Sanna, A.
name: Bult, P.
name: NG, M.
name: Ray, P. S.
name: Jaisawal, G. K.
name: Burderi, L.
name: Di Salvo, T.
name: Riggio, A.
name: Altamirano, D.
name: Strohmayer, T. E.
name: Manca, A.
name: Gendreau, K. C.
name: Chakrabarty, D.
name: Iwakiri, W.
name: Iaria, R.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: The detection of coherent X-ray pulsations at ~314 Hz (3.2 ms) classifies MAXI J1957+032 as a fast-rotating, accreting neutron star. We present the temporal and spectral analysis performed using NICER observations collected during the latest outburst of the source. Doppler modulation of the X-ray pulsation revealed the ultra-compact nature of the binary system characterised by an orbital period of ~1 hour and a projected semi-major axis of 14 lt-ms. The neutron star binary mass function suggests a minimum donor mass of 1.7e-2 Msun, assuming a neutron star mass of 1.4 Msun and a binary inclination angle lower than 60 degrees. This assumption is supported by the lack of eclipses or dips in the X-ray light curve of the source. We characterised the 0.5-10 keV energy spectrum of the source in outburst as the superposition of a relatively cold black-body-like thermal emission compatible with the emission from the neutron star surface and a Comptonisation component with photon index consistent with a typical hard state. We did not find evidence for iron K-alpha lines or reflection components.
description: 5 pages, 4 figures. Accepted for publication in MNRAS
Multi-Boson Correlation Sampling
Creators: name: Tamma, Vincenzo
name: Laibacher, Simon
Publisher: name: arXiv
Year: 2015
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We give a full description of the problem of Multi-Boson Correlation Sampling (MBCS) at the output of a random interferometer for single input photons in arbitrary multimode pure states. The MBCS prob- lem is the task of sampling at the interferometer output from the probability distribution associated with polarization- and time-resolved detections. We discuss the richness of the physics and the complexity of the MBCS problem for nonidentical input photons. We also compare the MBCS problem with the standard bo- son sampling problem, where the input photons are assumed to be identical and the system is "classically" averaging over the detection times and polarizations.
description: appears in Quantum Information Processing (2015)
Understanding the secular evolution of NGC 628 using UVIT
Creators: name: Ujjwal, K.
name: Kartha, Sreeja S.
name: Subramanian, Smitha
name: George, Koshy
name: Thomas, Robin
name: Mathew, Blesson
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Secular and environmental effects play a significant role in regulating the star formation rate and hence the evolution of the galaxies. Since UV flux is a direct tracer of the star formation in galaxies, the UltraViolet Imaging Telescope (UVIT) onboard ASTROSAT enables us to characterize the star forming regions in a galaxy with its remarkable spatial resolution. In this study, we focus on the secular evolution of NGC 628, a spiral galaxy in the local universe. We exploit the resolution of UVIT to resolve up to $\sim$ 63 pc in NGC 628 for identification and characterization of the star forming regions. We identify 300 star forming regions in the UVIT FUV image of NGC 628 using ProFound and the identified regions are characterized using Starburst99 models. The age and mass distribution of the star forming regions across the galaxy supports the inside-out growth of the disk. We find that there is no significant difference in the star formation properties between the two arms of NGC 628. We also quantify the azimuthal offset of the star forming regions of different ages. Since we do not find an age gradient, we suggest that the spiral density waves might not be the possible formation scenario of the spiral arms of NGC 628. The headlight cloud present in the disk of the galaxy is found to be having the highest star formation rate density ($0.23 M_{\odot} yr^{-1} kpc^{-2}$) compared to other star forming regions on spiral arms and the rest of the galaxy.
description: 11 pages, 11 Figures, Accepted in MNRAS
Additional file 1 of Prevalence and modifiable risk factors for dementia in persons with intellectual disabilities
Creators: name: Takenoshita, Shintaro
name: Terada, Seishi
name: Inoue, Tomokazu
name: Kurozumi, Taku
name: Yamada, Norihito
name: Kuwano, Ryozo
name: Suemitsu, Shigeru
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Neuroscience
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
classificationCode: 111714
subject: Mental Health

description: Additional file 1: Supplementary table 1. Demographic details of cognitive decline by age group.
A nuclear subcompartment involved in Plasmodium falciparum var gene regulation
Creators: name: Marty., Allison J.
Publisher: name: Monash University
Year: 2021

description: This thesis was scanned from the print manuscript for digital preservation and is copyright the author.
 Researchers can access this thesis by asking their local university, institution or public library to
 make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.
СИСТЕМА МОНИТОРИНГА УСПЕВАЕМОСТИ ШКОЛЬНИКОВ ПРИ ИНТЕРАКТИВНОМ ОБУЧЕНИИ С ИСПОЛЬЗОВАНИЕМ ГАПТИЧЕСКИХ ПЕРЧАТОК
Creators: name: АНТОНОВ ВЛАДИМИР ОЛЕГОВИЧ
name: АПУРИН АРТЁМ АЛЕКСАНДРОВИЧ
name: НЕЧВОЛОДА ВАЛЕРИЙ ЭДУАРДОВИЧ
name: БЫЧИХИН ИВАН ПЕТРОВИЧ
Publisher: name: StudNet
Year: 2020
Subjects: ИНТЕРАКТИВНОЕ ОБУЧЕНИЕ
СИСТЕМА ОЦЕНИВАНИЯ
ВИРТУАЛЬНАЯ РЕАЛЬНОСТЬ
ГАПТИЧЕСКИЕ ПЕРЧАТКИ
INTERACTIVE LEARNING
GRADING SYSTEM
VIRTUAL REALITY
HAPTIC GLOVES

description: В статье решается проблема мониторинга успеваемости школьников средних и старших классов при интерактивном обучении. Для повышения эффективности обучения предлагается программно-аппаратный комплекс альтернативного обучения с использованием гаптических перчаток и VR-технологий. Применение предлагаемых интерактивных технологий позволит решить следующие проблемы: низкая заинтересованность учеников в образовательном процессе, наличие стресса, восприятие оценки как травмирующего фактора и боязнь неудач в соответствии с этим.The article solves the problem of monitoring the performance of middle and high school students with interactive learning. To increase the effectiveness of training, a hardware-software complex of alternative training using haptic gloves and VR technologies is proposed. The application of the proposed interactive technologies will solve the following problems: low interest of students in the educational process, the presence of stress, the perception of assessment as a traumatic factor and the fear of failure in accordance with this.
Simultaneous Trapping of Two Optical Pulses in an Atomic Ensemble as Stationary Light Pulses
Creators: name: Kim, U-Shin
name: Kim, Yoon-Ho
Publisher: name: arXiv
Year: 2022
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The stationary light pulse (SLP) refers to a zero-group-velocity optical pulse in an atomic ensemble prepared by two counter-propagating driving fields. Despite the uniqueness of an optical pulse trapped within an atomic medium without a cavity, observations of SLP so far have been limited to trapping a single optical pulse due to the stringent SLP phase-matching condition, and this has severely hindered the development of SLP-based applications. In this paper, we first show theoretically that the SLP process in fact supports two phase-matching conditions and we then utilize the result to experimentally demonstrate simultaneous SLP trapping of two optical pulses for the duration from 0.8 $μ$s to 2.0 $μ$s. The characteristic dissipation time, obtained by the release efficiency measurement from the SLP trapping state, is 1.22 $μ$s, which corresponds to an effective Q-factor of $2.9\times 10^9$. Our work is expected to bring forth interesting SLP-based applications, such as, efficient photon-photon interaction, spatially multi-mode coherent quantum memory, creation of exotic photonic gas states, etc.
Fine Structure of Cyclotron Resonance in a Two-Dimensional Electron System
Creators: name: Muravev, V. M.
name: Andreev, I. V.
name: Gubarev, S. I.
name: Belyanin, V. N.
name: Kukushkin, I. V.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: It is established that cyclotron resonance (CR) in a high-quality GaAs/AlGaAs two-dimensional electron system (2DES) originates as a \textit{pure} resonance, that does not hybridize with dimensional magnetoplasma excitations. The magnetoplasma resonances form a fine structure of the CR. The observed fine structure of the CR results from the interplay between coherent radiative and incoherent collisional mechanisms of 2D plasma relaxation. We show that the range of 2DES filling factors from which the phenomenon arises is intimately connected to the fundamental fine-structure constant.
Solar and stellar activity cycles -- no synchronization with exoplanets
Creators: name: Obridko, V. N.
name: Katsova, M. M.
name: Sokoloff, D. D.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Cyclic activity on the Sun and stars is primarily explained by generation of the magnetic field by a dynamo mechanism, which converts the energy of the poloidal field into the energy of the toroidal component due to differential rotation. There is, however, an alternative point of view, which explains the field generation by gravitational influence of the planetary system and, first of all, Jupiter. This hypothesis can be verified by comparing the characteristics of exoplanets with the activity variations on their associated stars. We have performed such a comparison and have drawn a negative conclusion. No relationship between the gravitational influence of the exoplanets and cycle of the host star could be found in any of the cases considered. Moreover, there are reasons to believe that a strong gravitational influence may completely eliminate cyclic variation in stellar activity.
description: 5 pages, 2 tables. Accepted to MNRAS (April 2022)
Additional file 2 of Prevalence and modifiable risk factors for dementia in persons with intellectual disabilities
Creators: name: Takenoshita, Shintaro
name: Terada, Seishi
name: Inoue, Tomokazu
name: Kurozumi, Taku
name: Yamada, Norihito
name: Kuwano, Ryozo
name: Suemitsu, Shigeru
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Neuroscience
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
classificationCode: 111714
subject: Mental Health

description: Additional file 2: Supplementary table 2. Demographic details in each corporation by age group.
Detailed Evolutionary Models for Twins in Sight of New Spectral Data: AN Cam, RS Ari, and V455 Aur
Creators: name: Yücel, Gökhan
name: Bakış, Volkan
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present the evolutionary scenarios for three eclipsing twin ($q(M_2/M_1)\sim$1) binary systems using their combined spectroscopic and photometric data. Using accurate \textit{TESS} photometric data, RV measurements, and spectroscopic data enabled us to calculate fundamental parameters, such as mass and radius, better than 2 percent. The temperature of each component and metallicity of the systems have been obtained via high-resolution spectra. According to our spectral analysis, the metallicity values of AN Cam, RS Ari, and V455 Aur are \text{[M/H]}=\,0.00$\pm$0.12, 0.05$\pm$0.08, and -0.07$\pm$0.07, respectively. Using the derived metallicity for each system, initial orbital parameters and detailed evolutionary status of these three systems are calculated with high precision by using \textsc{mesa}. According to our analysis, both components of AN Cam have passed the terminal age main-sequence, the primary component of RS Ari is in the giant phase while the secondary component has passed the terminal age main-sequence, finally, both components of V455 Aur are still on the main-sequence. The current ages of the three systems AN Cam, RS Ari, and V455 Aur are 3.0, 3.3, and 1.4 Gyrs, respectively, and they will approximately start to transfer mass between components in 400, 250, and 2700 Myrs, respectively.
description: Accepted by MNRAS. 15 pages, 17 figures, 6 tables
АКТУАЛЬНОСТЬ ПРИМЕНЕНИЯ БИОРЕЗОНАНСНОЙ ДИАГНОСТИКИ ХРОНИЧЕСКОГО БРОНХИТА И ПРОГНОЗИРОВАНИИ ЕГО ИСХОДА
Creators: name: ГОРБУНОВ А.А
name: КАСАЕВА Г.Р.
Publisher: name: StudNet
Year: 2020
Subjects: ТОРСИОННЫЕ ПОЛЯ
БИОРЕЗОНАНСНАЯ ДИАГНОСТИКА
БРОНХИТ
ХРОНИЧЕСКИЙ БРОНХИТ
ДИАГНОСТИКА
ПРОГНОЗИРОВАНИЕ
БИОПОЛЕ ЧЕЛОВЕКА
TORSION FIELDS
BIORESONANCE DIAGNOSTICS
BRONCHITIS
CHRONIC BRONCHITIS
DIAGNOSTICS
PREDICTION
HUMAN BIOFIELD

description: В статье рассматривается потенциально новый метод в диагностике и прогнозировании исхода хронического бронхита для более успешной диагностики данного заболевания при помощи торсионных полей. Был изучен и применен новый класс природных явлений, перенос информации о веществе через торсионные излучения и воздействие этого поля на физические и биологические процессы. Диагностическое и лечебное действие торсионных полей заключается в низком уровне энергоемкости и большом уровне информационной емкости с благоприятным воздействием на организм человека. Именно эти явления являются основой нового метода в диагностике и прогнозировании исхода хронического бронхита.The article considers a potentially new method for diagnosing and predicting the outcome of chronic bronchitis for more successful diagnosis of this disease using torsion fields. A new class of natural phenomena was studied and applied, the transfer of information about a substance through torsion radiation and the effect of this field on physical and biological processes. The diagnostic and therapeutic effect of torsion fields is a low level of energy intensity and a large level of information capacity with a favorable effect on the human body. These phenomena are the basis of a new method for diagnosing and predicting the outcome of chronic bronchitis.
Recursive Recovery of Sparse Signal Sequences from Compressive Measurements: A Review
Creators: name: Vaswani, Namrata
name: Zhan, Jinchun
Publisher: name: arXiv
Year: 2016
Subjects: subject: Information Theory (cs.IT)
subject: FOS: Computer and information sciences

description: In this article, we review the literature on design and analysis of recursive algorithms for reconstructing a time sequence of sparse signals from compressive measurements. The signals are assumed to be sparse in some transform domain or in some dictionary. Their sparsity patterns can change with time, although, in many practical applications, the changes are gradual. An important class of applications where this problem occurs is dynamic projection imaging, e.g., dynamic magnetic resonance imaging (MRI) for real-time medical applications such as interventional radiology, or dynamic computed tomography.
description: To appear in IEEE Trans. Signal Processing
Salacia malabarica Gamble 1916
Creators: name: Jadhav, Durga C.
name: Prabhugaonkar, Ashish V.
name: Nandikar, Mayur D.
Publisher: name: Zenodo
Year: 2016
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Celastrales
Celastraceae
Salacia
Salacia malabarica

description: 7. Salacia malabarica Gamble (1916: 133)
 Type:— INDIA, Kerala, Kollam district, Tranvancore Hills, November 1887, T. F. Bourdillon 18 [lectotype, MH! (MH00001913, Fig. 7), designated here]; syntypes: INDIA, Karnataka, South Canara, s.d., Beddome ? s.n. [MH! (MH00001912)]; Travancore, 25 November 1893, T. F. Bourdillon s.n. [K (K000669995, image!)].
 Salacia malabarica was described by Gamble based on the R. A. Beddome and T. F. Bourdillon collections. In the protologue no specific type has been given and therefore a typification is required. Two collections by Bourdillon deposited at MH and K, other one is presumably from Beddome deposited at MH. One of the Bourdillon collections at MH (MH 00001913) from Travancore hills agrees with protologue and is designated here as lectotype. Although remaining two collections by T. F. Bourdillon (K 000669995) from Travancore at K and Beddome? (MH 00001912) from south Canara at MH are kept as syntypes. Later collection is without collector details, but it is annotated by Gamble and locality is the same as in protologue, therefore, kept as an original material.
description: Published as part of Jadhav, Durga C., Prabhugaonkar, Ashish V. & Nandikar, Mayur D., 2016, Nomenclature notes on the genus Salacia L. (Celastraceae) in India, pp. 121-130 in Phytotaxa 265 (2) on pages 128-129, DOI: 10.11646/phytotaxa.265.2.3, http://zenodo.org/record/13662647