cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
ВОЛОНТЕРСЬКА ДОПОМОГА ЗБРОЙНИМ СИЛАМ УКРАЇНИ ЯК ГРОМАДСЬКО- ПРАВОВИЙ ІНСТИТУТ УКРАЇНИ
Creators: name: Прохоренко, М. М.
name: Алієв, Р. В.
Publisher: name: Zenodo
Year: 2023
Subjects: волонтер, волонтерська допомога, правові інститути, громадськість, нормативно-правові акти, Збройні Сили України, особливий період.

description: У статті проаналізовано волонтерську допомогу Збройним Силам України та її роль у системі правових інститутів країни. Волонтерство, яке визначається як добровільна, соціально орієнтована та неприбуткова діяльність, є однією з ключових форм соціальної активності молоді та глибоко укорінене в національних традиціях. Відіграючи значну роль у медичній допомозі, цивільній обороні та соціальному захисті, волонтерська ініціатива забезпечує важливу підтримку у часи воєнних  конфліктів і соціальних криз.

У контексті правового регулювання волонтерської діяльності, стаття детально розглянула нормативну базу, що включає Конституцію України, національні закони та міжнародні договори, зокрема Закон України «Про волонтерську діяльність». Важливі зміни до законодавства були внесені з прийняттям Закону України «Про внесення змін до деяких законів України щодо волонтерської діяльності», який скасував деякі обмеження та спростив процедуру залучення волонтерів у військові зони та допомогу сім'ям загиблих та поранених волонтерів.

З’ясовано, що ефективна взаємодія між волонтерами та державними органами забезпечує не тільки невідкладну допомогу в умовах правового режиму надзвичайного стану, особливого періоду та кризових ситуаціях, але й сприяє довгостроковій стабілізації та соціальному розвитку. Волонтери забезпечують критичні ресурси, такі як медичні засоби, амуніцію та інші необхідності, що згуртовують громадськість і підвищують загальний моральний дух.

Обґрунтовано, що правова основа та гнучкість законодавчих рамок є критично важливими для забезпечення ефективності волонтерської діяльності, яка впливає на розвиток громадянського суспільства та посилення національної безпеки та оборони. Також доведено, що належне правове регулювання та інтеграція волонтерських зусиль в офіційні структури держави можуть значно підвищити якість і швидкість реагування на загрози національній безпеці України.

На підставі аналізу сформовані висновки про невід'ємну роль волонтерської допомоги в системі національної безпеки та оборони України, підкреслюючи необхідність подальшого розроблення та удосконалення правових механізмів залучення волонтерських ресурсів в стратегічні напрямки державного управління.
ASEAN identity in higher education through literary pedagogy perceived by teaching personnel at universities in Southern Tagalog Region, the Philippines
Creators: name: Ba?Ez, Richard Mendoza
Publisher: name: Silpakorn University Research Innovation and Creativity Administration Office
Year: 2022
Subjects: ASEAN identity
cultural modeling approach
higher education
literary curriculumpractices
literature pedagogy

description: Humanities, Arts and Social Sciences Studies, 22, 3, 561-567
Accelerating massive data processing in Python with Heat
Creators: name: Comito, Claudia
name: F. Hoppe
name: F. Osterfeld
name: A. Rüttgers
name: P. Knechtges
name: J.P. Gutiérrez Hermosillo Muriedas
name: M. Götz
name: B. Hagemeier
name: K. Krajsek
name: M. Tarnawa
name: H.-R. Klöckner
name: F. Jünemann
Publisher: name: Zenodo
Year: 2024

description: Processing massive scientific datasets is challenging. In astrophysics as in the vast majority of research communities, the standard approach involves breaking up and analyzing data in smaller chunks, an inefficient and very prone-to-errors process. The problem is exacerbated on GPUs, because of the smaller available memory. Popular solutions to distribute NumPy/SciPy computations are based on task parallelism, introducing significant runtime overhead, complicating implementation, and often limiting GPU support to one vendor. In this talk, I will present an alternative based on data parallelism. The open-source library Heat [https://github.com/helmholtz-analytics/heat] builds on PyTorch and the Message Passing Interface protocol to simplify porting of NumPy/SciPy-based code to multi-CPU, multi-GPU clusters. From a user perspective, Heat can be used seamlessly in the Python array ecosystem (numpy, scipy, xarray etc.).   Under the hood, massive memory-intensive operations are distributed transparently via MPI communication. I will not bore you with technical details, but rather show you practical situations in which your Python pipeline could benefit from using Heat as a backend for massive array manipulations, statistics, signal processing, machine learning, etc.
The Black Hole - Bulge Mass Relation in Megamaser Host Galaxies
Creators: name: Läsker, Ronald
name: Greene, Jenny E.
name: Seth, Anil
name: van de Ven, Glenn
name: Braatz, James A.
name: Henkel, Christian
name: Lo, K. Y.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present HST images for nine megamaser disk galaxies with the primary goal of studying photometric BH-galaxy scaling relations. The megamaser disks provide the highest-precision extragalactic BH mass measurements, while our high-resolution HST imaging affords us the opportunity to decompose the complex nuclei of their late-type hosts in detail. Based on the morphologies and shapes of the galaxy nuclei, we argue that most of these galaxies' central regions contain secularly evolving components (pseudo-bulges), and in many cases we photometrically identify co-existing "classical" bulge components as well. Using these decompositions, we draw the following conclusions: (1) The megamaser BH masses span two orders of magnitude ($10^6$ -- $10^8 M_\odot$) while the stellar mass of their spiral host galaxies are all $\sim 10^{11} M_\odot$ within a factor of three; (2) the BH masses at a given bulge mass or total stellar mass in the megamaser host spiral galaxies tend to be lower than expected, when compared to an extrapolation of the BH-bulge relation based on early-type galaxies; (3) the observed large intrinsic scatter of BH masses in the megamaser host galaxies raises the question of whether scaling relations exist in spiral galaxies.
description: 41 pages, 27 Figures, 7 Tables
Trees don't shout
Creators: name: De Kock, Pieter
Publisher: name: figshare
Year: 2023
Subjects: classificationCode: 330411
subject: Urban design

description: Trees don’t shout, they don’t need to. This study explores two recurring strands of a central theme around how trees and the space formed by trees are relevant to urban design—the practical and the magical. Practical relevancy extends beyond environmental, health, social, and economic concerns to include sensitivity and careful consideration of type, size, mix, placement, and spacing of trees. Magical relevancy lies in the ‘sense of wonder’—a fine mist through which people invested in the evolution of our towns and cities are drawn, where light and shade filter both noise and quiet.
NASCENT-stars large program: origin of molecular complexity towards emerging high-mass protostars
Creators: name: Csengeri, Timea
name: Bouscasse
name: Arumguam
name: Lopez-Sepulcre
name: Le Gal
name: Baudry, Bontemps
name: Braine
name: Brouillet
name: Guilloteau
name: Herpin
name: Kessler
name: Valeille-Manet
name: Motte
name: Coutens
name: Vastel
name: Wyrowski
name: Menten
name: Beuther
name: Galvan-Madrid
name: Ortiz-Leon
name: Garrod
name: Bonfand
name: Ginsburg
name: Commercon
name: Cunningham
name: Dannhauer
name: Simon
name: Schneider
name: Gusdorf
Publisher: name: Zenodo
Year: 2024

description: During the star formation process, the interstellar medium gets enriched in a complex zoo of molecules. The extremely rich chemistry of the star forming gas holds the key to constrain the link between the chemistry of disks and their forming planetary systems. It is, however, unclear what are the key physical conditions that influence the emerging complex chemistry, and how the fundamental properties of the emerging star, or stellar clusters impact its evolution.
In this context, wide-band receivers open a new era by allowing us to perform quasi-instantaneously spectral surveys that are required for a more robust estimation of molecular abundances. The NASCENT-stars project (PI: Csengeri) is a large observing program started in 2023 at the IRAM NOEMA observatory with 228 hours allocated at the telescope making use of the newly commissioned high spectral resolution (250 kHz) and wide-band observing mode. Overall, we observe a 46.5 GHz non-continuous bandwidth to characterize the physico-chemical conditions of the most active star forming regions of the Cygnus-X molecular complex at the scale of 1400 au probing statistically significant samples individual protostellar envelopes. I would like to highlight the first results of NASCENT-stars and our efforts to develop artificial intelligence and machine learning methods facilitating the exploitation of these rich datasets. Results of this project should pave the way to the spectacular science cases enabled by the ALMA WSU.
Energy-momentum mapping of d-derived Au(111) states in a thin film
Creators: name: Sheverdyaeva, P. M.
name: Requist, R.
name: Moras, P.
name: Mahatha, S. K.
name: Papagno, M.
name: Ferrari, L.
name: Tosatti, E.
name: Carbone, C.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The quantum well states of a film can be used to sample the electronic structure of the parent bulk material and determine its band parameters. We highlight the benefits of two-dimensional film band mapping, with respect to complex bulk analysis, in an angle-resolved photoemission spectroscopy study of the 5d states of Au(111). Discrete 5d-derived quantum well states of various orbital characters form in Au(111) films and span the width of the corresponding bulk bands. For sufficiently thick films, the dispersion of these states samples the bulk band edges, as confirmed by first-principles calculations, thus providing the positions of the critical points of bulk Au in agreement with previously determined values. In turn, this analysis identifies several d-like surface states and resonances with large spin-splittings that originate from the strong spin-orbit coupling of the Au 5d atomic levels.
Soft skills development training program to enhance Cambodian university students' entrepreneurial capabilities
Creators: name: Sarom Tem, Ariyabhorn Kuroda
Publisher: name: Silpakorn University Research Innovation and Creativity Administration Office
Year: 2022
Subjects: Communication skills
critical thinking and problem-solving skills
entrepreneurial capabilities
leadership skills
training program

description: Humanities, Arts and Social Sciences Studies, 22, 3, 568-578
Amtliche Mitteilungen der Technischen Universität Dortmund Nr. 19/2016
Creators: name: (:Unkn) Unknown
Publisher: name: Technische Universität Dortmund
Year: 2016
Subjects: subject: 080

description: Zweite Ordnung zur Änderung der Fakultätsordnung für die Fakultät Raumplanung vom 20. Juni 2016
description: Ordnung zur Änderung der Satzung der Studierendenschaft der Technischen Universität Dortmund vom 27.04.2016
description: Dienstsiegelverlust
description: Amtliche Mitteilungen der Technischen Universität Dortmund;19, 2016
Orbital Dynamics of Exoplanetary Systems Kepler-62, HD 200964 and Kepler-11
Creators: name: Mia, Rajib
name: Kushvah, Badam Singh
Publisher: name: arXiv
Year: 2016
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences
subject: 70F15

description: The presence of mean-motion resonances (MMRs) in exoplanetary systems is a new exciting field of celestial mechanics which motivates us to consider this work to study the dynamical behaviour of exoplanetary systems by time evolution of the orbital elements of the planets. Mainly, we study the influence of planetary perturbations on semimajor axis and eccentricity. We identify $(r+1):r$ MMR terms in the expression of disturbing function and obtain the perturbations from the truncated disturbing function. Using the expansion of the disturbing function of three-body problem and an analytical approach, we solve the equations of motion. The solution which is obtained analytically is compared with that of obtained by numerical method to validate our analytical result. In this work, we consider three exoplanetary systems namely Kepler-62, HD 200964 and Kepler-11. We have plotted the evolution of the resonant angles and found that they librate around constant value. In view of this, our opinion is that two planets of each system Kepler-62, HD 200964 and Kepler-11 are in 2:1, 4:3 and 5:4 mean motion resonances, respectively. Keywords:astrometry - celestial mechanics - planetary systems.
description: E-mail:rajibmia.90@gmail.com, bskush@gmail.com
title: Arbre_4
Creators: name: Ségolène Delamare
name: Galinand, Cyrille
name: Université Paris1 Panthéon-Sorbonne
Publisher: name: Archeovision
Year: 2023
Subjects: subject: arborglyphe

description: arborglyphe
description: 1 fichier 3D (ply), 26 fichiers image (jpg)
The investigation of Chinese TFL learners' abilities to distinguish Thai initial consonant sounds
Creators: name: Orrathip Geerativudhipong, Songsri Soranasataporn
Publisher: name: Silpakorn University Research Innovation and Creativity Administration Office
Year: 2022
Subjects: Thai initial consonant sounds
Thai language
listening perception
Chinese TFL learners

description: Humanities, Arts and Social Sciences Studies, 22, 3, 579-588
Social media, body norms, and gendered bodies: The case study of conformity and plausible negotiation with the ideal body image
Creators: name: Porranee Singpliam
Publisher: name: Silpakorn University Research Innovation and Creativity Administration Office
Year: 2022
Subjects: Social media
body image
gender
embodiment

description: Humanities, Arts and Social Sciences Studies, 22, 3, 589-600
Discursive anarchism in J. M. Coetzee's Waiting for the Barbarians
Creators: name: Morakot Pan-Iam
Publisher: name: Silpakorn University Research Innovation and Creativity Administration Office
Year: 2022
Subjects: J. M. Coetzee
Waiting for the Barbarians
allegory
discursive anarchism

description: Humanities, Arts and Social Sciences Studies, 22, 3, 601-611
Genuine multipartite entanglement detection and lower bound of multipartite concurrence
Creators: name: Li, Ming
name: Fei, Shao-Ming
name: Li-Jost, Xianqing
name: Fan, Heng
Publisher: name: arXiv
Year: 2015
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The problems of genuine multipartite entanglement detection and classification are challenging. We show that a multipartite quantum state is genuine multipartite entangled if the multipartite concurrence is larger than certain quantities given by the number and the dimension of the subsystems. This result also provides a classification of various genuine multipartite entanglement. Then, we present a lower bound of the multipartite concurrence in terms of bipartite concurrences. While various operational approaches are available for providing lower bounds of bipartite concurrences, our results give an effective operational way to detect and classify the genuine multipartite entanglement. As applications, the genuine multipartite entanglement of tripartite systems is analyzed in detail.
description: 7 pages
The origin of chemical complexity: in the earth of young forming planetary system
Creators: name: De Simone, Marta
name: C. Codella
name: C. Ceccarelli
name: L. Podio
name: E. Bianchi
name: B.E. Svoboda
name: C.J. Chandler
name: M. Bouvier
name: S. Yamamoto
name: N. Sakai
name: A. Lopez-Sepulcre
name: P. Caselli
name: L. Testi
name: L. Loinard
name: B. Lefloch
name: J.E Pineda
name: N. Balucani
name: A. Rimola
name: J. Enrique-Romero
name: A. Miotello
name: L. Cacciapuoti
name: E. Macias
name: L. Tychoniec
Publisher: name: Zenodo
Year: 2024

description: Early planetary system formation reveals intricate chemistry with abundant prebiotic molecules in protostellar environments that serves as a crucial diagnostic tool for understanding underlying physical processes. Protostellar systems, at high angular resolution (below 100 au), exhibit complex interconnected physical processes, expanding beyond the traditional model of accreting central objects ejecting powerful jets to include compact disks, accretion streamers, shocks, and disk winds. The interplay between accretion and ejection mechanisms has a key role in the distribution of gas and dust in the disk, influencing the chemical content inherited by forming planets.
Relationship between the image of food and food satisfaction of international tourists: The moderating effect of tourist groups
Creators: name: Charoenchai Agmapisarn, Hyung-Min Choi
Publisher: name: Silpakorn University Research Innovation and Creativity Administration Office
Year: 2022
Subjects: Food image
food satisfaction
local food
European and non-European
moderating role

description: Humanities, Arts and Social Sciences Studies, 22, 3, 624-640
Advanced Waveguide Components and Technology for 2SB dual polarization receiver cartridges
Creators: name: Desmaris, Vincent
Publisher: name: Zenodo
Year: 2024

description: The ALMA WSU strives for ``increase of the receiver IF bandwidth by at least a factor of two", as well an improvement of the beam squint performance of some existing cartridges in order to keep ALMA at the forefront of astrophysical facilities and to address three new fundamental science drivers: the origin of galaxies, the origins of chemical complexity and the origin of planets Aiming the two abovementioned challenges, an ESO study exploring advanced waveguide components and technologies for 2SB dual polarization receiver cartridges started in Dec 2023. The study focuses on the development of micro machined waveguide technology and its possible implementation in the form of form of low loss OMTs for band 7 and Band 9, which currently employs polarization splitting using grids. The developed technology employs photolithographically defined components exhibiting ultimate in linear dimension and superior surface accuracy enabling potentially large structure still with low loss. Additionally, the waveguide technology developed also enabled drop-in waveguide matched loads for the frequencies of B7 and B9 that will provide compact and reliable solution for use in respective 2SB mixers. At the workshop we will present the initial results and prospective of this collaborative study run between NOVA and GARD.
Opening Reproducible Research: a research project website and blog
Creators: name: Nüst, Daniel
name: Schutzeichel, Marc
name: Konkol, Markus
name: Koukouraki, Eftychia
Publisher: name: Zenodo
Year: 2018

description: All blog entries of the blog for the research project Opening Reproducible Research (o2r, see also Offene Reproduzierbare Forschung @ DFG GEPRIS), online at https://o2r.info. o2r was funded by the German Research Foundation (Deutsche Forschungsgemeinschaft, DFG) under project numbers PE 1632/10-1, KR 3930/3-1 and TR 864/6-1.
The Costa Rican National Open Science Outreach Initiative: what we learned and achieved in a decade
Creators: name: Ramirez-Vega, Alexa
name: Barrantes-Arrieta, Andrea
name: Marín-Campos, Andrea
name: Mora-Campos, Andrea
name: Seas-Carvajal, Carolina
name: Campos-Jara, Fabiola
name: Enríquez-Fallas, Jason
name: Polanco-Cortés, Jorge
name: Mena-Garita, Kattia
name: Garro-Acón, Meilyn
name: Segura-Jiménez, Steven
name: Franco-Poveda, Teresa
name: Sánchez Espinosa, Sharlin
Publisher: name: Zenodo
Year: 2023

description: The National Open Science Outreach Initiative of the Consejo Nacional de Rectores (CONARE, for its acronym in Spanish, it is in charge of coordinating the State University Higher Education System) in Costa Rica was created in 2012 as an open knowledge subcommittee for training, regulation and development of Open Science tools promoted through public funds in the country. The initiative also considers the participation of other governmental and private institutions throughout Latin America. The initiative includes the objective of measuring and improving the country's knowledge, focusing on open science. The work of the Open Knowledge Subcommittee is done through monthly meetings where common objectives are set on initiatives, policies, strategies and technological infrastructures to promote Open Science in public institutions in Costa Rica. An investigation of the international context is followed by an assessment of the state of the regional, national and local issues. Subsequently, experts and international organizations provide internal training for subcommittee members. Finally, implementation proposals are developed: visualization of need and importance, training and tools, guidelines and technical policies. Some results of the first ten years of implementation are: support for the digital portals of scientific journals of public universities; digitization of those journals and other university heritage; consolidation of scientific journals (e.g. diamond journals); improvement of infrastructure and technological tools of Open Science, and the creation in 2016 of the Kímuk National Repository, which includes documents (journal articles, thesis, reports, etc.) from different institutional repositories. Additionally, Open Science training and consulting at a national and international level. Current work includes the development of an Open Science Declaration for public universities in Costa Rica, official implementation of a national Index of Evaluation of Scientific Journals. Finally, future goals are the passing of a National Open Access Law, institutional data repositories and institutional strategies for the management of research data.
description: This poster was presented during the 4th Open Science Fair (25-27 September, Madrid, Spain)
Radio AGN in the local universe: unification, triggering and evolution
Creators: name: Tadhunter, Clive
Publisher: name: arXiv
Year: 2016
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Associated with one of the most important forms of active galactic nucleus (AGN) feedback, and showing a strong preference for giant elliptical host galaxies, radio AGN (L_1.4GHz > 10^24 W Hz^-1) are a key sub-class of the overall AGN population. Here I review our current state of understanding of the population of radio AGN at low and intermediate redshifts (z < 0.7), concentrating on their AGN and host galaxy properties, and covering three interlocking themes: the classification of radio AGN and its interpretation; the triggering and fuelling of the jet and AGN activity; and the evolution of the host galaxies. I show that much of the observed diversity in the AGN properties of radio AGN can be explained in terms of a combination of orientation/anisotropy, mass accretion rate, and variability effects. The detailed morphologies of the host galaxies are consistent with the triggering of strong-line radio galaxies (SLRG) in galaxy mergers. However, the star formation properties and cool ISM contents suggest that the triggering mergers are relatively minor in terms of their gas masses in most cases, and would not lead to major growth of the supermassive black holes and stellar bulges; therefore, apart from a minority (<20%) that show evidence for higher star formation rates and more massive cool ISM reservoirs, the SLRG represent late-time re-triggering of activity in mature giant elliptical galaxies. In contrast, the host and environmental properties of weak-line radio galaxies (WLRG) with Fanaroff-Riley class I (FRI) radio morphologies are consistent with more gradual fuelling of the activity via gas accretion at low rates onto the supermassive black holes.
description: Accepted for publication in Astronomy & Astrophysics Review, 67 pages, 17 figures
Widening our view of the hot Universe
Creators: name: Di Mascolo, Luca
Publisher: name: Zenodo
Year: 2024

description: Throughout the past decade, the superior capabilities of the Atacama Large Millimeter/Submillimeter Array (ALMA) have allowed astronomers to gain an unprecedented perspective on the Sunyaev-Zeldovich (SZ) effect -- a peculiar spectral signature imprinted in the ubiquitous cosmic microwave background by the warm/hot gas across the Universe. ALMA observations of the SZ effect over scales of a few arcseconds have started rivaling the more traditional X-ray measurements in terms of both resolution and sensitivity, conclusively establishing the central role of the SZ effect in the study of the thermal evolution of cosmic structures. However, the exploration of the SZ Universe with ALMA is still limited to only to a handful of pioneering studies targeting individual and/or somewhat extreme cases. In fact, the faint and diffuse nature of the SZ signal largely hampers its characterization due to major limitations inherent to radio-interferometric measurements -- namely, large-scale filtering, missing fluxes on smaller scales, and significant noise correlation in the image. Systematically extending our observational reach of the SZ effect will thus require a major advance that minimizes the impact of sparse sampling of the visibility plane while enhancing overall continuum sensitivity. In my talk, I will present detailed forecasts to discuss how the wideband sensitivity upgrade will be specifically suited for addressing such issues in the context of ALMA SZ observations.
Light-front representation of chiral dynamics with Delta isobar and large-N_c relations
Creators: name: Granados, C.
name: Weiss, C.
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Transverse densities describe the spatial distribution of electromagnetic current in the nucleon at fixed light-front time. At peripheral distances b = O(M_pi^{-1}) the densities are governed by chiral dynamics and can be calculated model-independently using chiral effective field theory (EFT). Recent work has shown that the EFT results can be represented in first-quantized form, as overlap integrals of chiral light-front wave functions describing the transition of the nucleon to soft-pion-nucleon intermediate states, resulting in a quantum-mechanical picture of the peripheral transverse densities. We now extend this representation to include intermediate states with Delta isobars and implement relations based on the large-N_c limit of QCD. We derive the wave function overlap formulas for the Delta contributions to the peripheral transverse densities by way of a three-dimensional reduction of relativistic chiral EFT expressions. Our procedure effectively maintains rotational invariance and avoids the ambiguities with higher-spin particles in the light-front time-ordered approach. We study the interplay of pi-N and pi-Delta intermediate states in the quantum-mechanical picture of the densities in a transversely polarized nucleon. We show that the correct N_c-scaling of the charge and magnetization densities emerges as the result of the particular combination of currents generated by intermediate states with degenerate N and Delta. The off-shell behavior of the chiral EFT is summarized in contact terms and can be studied easily. The methods developed here can be applied to other peripheral densities and to moments of the nucleon's generalized parton distributions.
description: 35 pages, 9 figures
Current IATV distribution in Europe
Creators: name: Polaina, Ester
Publisher: name: Zenodo
Year: 2020
Subjects: invasive species
sdm
species distribution model
biomod
Europe

description: Code accompanying the manuscript "Identifying hotspots of invasive alien terrestrial vertebrates in Europe to assist transboundary prevention and control", by Ester Polaina, Tomas Pärt and Mariano R. Recio, published in Scientific Reports.
Virtual historical sense of place in multimedia web tourism: a case of Bang Lamphu
Creators: name: ThirathepChonmaitree, Eakachat Joneurairatana
Publisher: name: Silpakorn University Research Innovation and Creativity Administration Office
Year: 2022
Subjects: Sense of place
experiential tourism
photography
storytelling

description: Humanities, Arts and Social Sciences Studies, 22, 3, 648-662
On-the-fly data reduction by streaming processing of visibilities
Creators: name: Dijkema, Tammo-Jan
name: Sarod Yatawatta
name: Stefan Wijnholds
name: André Gunst
Publisher: name: Zenodo
Year: 2024

description: Realising the scientific ambitions of ALMA's Wideband Sensitivity Upgrade (WSU) will require a significant increase in IF and correlator bandwidth. This will result in a larger output data rate of the correlator, putting increasing demands on storage capacity and I/O for the buffering of raw visibility data. To reduce the costs (in terms of energy consumption and hardware) of handling the raw visibility data, we started the Streaming Visibility Processing (SVP) development study in September 2023. The aim of this project is to demonstrate a prototype data processing pipeline that captures the visibility output stream from the ALMA correlator, performs a number of observation-dependent visibility processing steps and only stores the visibilities after reducing the visibility data volume. Possible examples of such data-volume reducing initial processing steps are Baseline-Dependent Averaging (BDA) and visibility data compression using the Dysco algorithm. Although these techniques are not lossless, they can be configured in such a way that the increase in the thermal noise level of the final images is less than 1\% while the data volume is reduced by an order of magnitude. A demonstration of this trade-off and its implications for ALMA science is part of the development study.
Reproductive rights of women in India with focus on tea plantation workers of Sonitpur District of Assam, India
Creators: name: Sarmah, Mridula
Publisher: name: Silpakorn University Research Innovation and Creativity Administration Office
Year: 2022
Subjects: Reproductive health
women
tea plantation
Assam

description: Humanities, Arts and Social Sciences Studies, 22, 3, 663-672
GLOMICAVE FACTSHEET
Creators: name: Eurecat Communication Department
Publisher: name: Zenodo
Year: 2022
Subjects: Omics
Metabolomics
Genomics
Transcriptomics
Big Data
Artificial Intelligence

description: General facthseet of GLOMICAVE project
description: This project has received funding from the European Union's Horizon 2020 research and innovation programme under grant agreement No. 952908
Supplementary Material from Neural operator learning of heterogeneous mechanobiological insults contributing to aortic aneurysms
Creators: name: Goswami, Somdatta
name: Li, David S.
name: Rego, Bruno V.
name: Latorre, Marcos
name: Humphrey, Jay D.
name: Em Karniadakis, George
Publisher: name: The Royal Society
Year: 2022
Subjects: subject: Biological Engineering
subject: 110601 Biomechanics
subject: FOS: Health sciences
subject: 90399 Biomedical Engineering not elsewhere classified
subject: FOS: Medical engineering

description: Thoracic aortic aneurysm (TAA) is a localized dilatation of the aorta that can lead to life-threatening dissection or rupture. In vivo assessments of TAA progression are largely limited to measurements of aneurysm size and growth rate. There is promise, however, that computational modelling of the evolving biomechanics of the aorta could predict future geometry and properties from initiating mechanobiological insults. We present an integrated framework to train a deep operator network (DeepONet)-based surrogate model to identify TAA contributing factors using synthetic finite-element-based datasets. For training, we employ a constrained mixture model of aortic growth and remodelling to generate maps of local aortic dilatation and distensibility for multiple TAA risk factors. We evaluate the performance of the surrogate model for insult distributions varying from fusiform (analytically defined) to complex (randomly generated). We propose two frameworks, one trained on sparse information and one on full-field greyscale images, to gain insight into a preferred neural operator-based approach. We show that this continuous learning approach can predict the patient-specific insult profile associated with any given dilatation and distensibility map with high accuracy, particularly when based on full-field images. Our findings demonstrate the feasibility of applying DeepONet to support transfer learning of patient-specific inputs to predict TAA progression.
Autonomous Dome for Robotic Telescope
Creators: name: Kumar, Akash
name: Sengupta, Anand S.
name: Ganesh, Shashikiran
Publisher: name: arXiv
Year: 2016
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Physical Research Laboratory operates a 50cm robotic observatory at Mount Abu. This Automated Telescope for Variability Studies (ATVS) makes use of Remote Telescope System 2 (RTS2) for autonomous operations. The observatory uses a 3.5m dome from Sirius Observatories. We have developed electronics using Arduino electronic circuit boards with home grown logic and software to control the dome operations. We are in the process of completing the drivers to link our Arduino based dome controller with RTS2. This document is a short description of the various phases of the development and their integration to achieve the required objective.
description: Contributed paper in the Fourth Workshop on Robotic Autonomous Observatories, Malaga, Spain (September 28 - Oct 02, 2015)
The Integration of LNA Based Receivers for Millimetre and Sub-millimetre Wavelength Radio Astronomy
Creators: name: Franks, Elle
name: William McGenn
name: Brian Ellison
name: Gary Fuller
name: Danielle George
name: Hui Wang
name: Byron Alderman
name: Peter Huggard
Publisher: name: Zenodo
Year: 2024

description: With the recent developments of transistor technologies, Low Noise Amplifiers (LNAs) operating in the millimetre and sub-millimetre wave are now realisable with performance comparable to SIS junctions. This in turn allows for LNA based receiver instrumentation in these frequency ranges, such as the ESO ALMA Band 2 receiver (67-116GHz). The Millimetre-wave Technology group and the Technology Department at the STFC Rutherford Appleton Laboratory and the Advanced Radio Instrumentation Group at the University of Manchester have recently completed the sixteen-pixel, 70-116GHz Cryogenic Array Receiver for Users of the Sardinia Observatory (CARUSO) project. To achieve an appropriate spatial sampling of celestial sources the feedhorns of the receiver pixels were required to be tightly grouped together, limiting the available volume for the receiver components. This space limitation pushed the physical design of the individual components to the limits of what is achievable without further miniaturisation and integration of the receiver sub-components. Based on the success of the CARUSO receiver we have now embarked on TASER, a project funded by the ESO European ALMA Development Fund and the EU funded RADIOBLOCKS project. In this talk we will present the first steps toward highly integrated systems that will be able to provide a new generation of compact, highly sensitive, broad band receivers including, eventually, focal plane array systems for ALMA as well as other telescopes.
Deliverable 5.2: Digital Twins of components and  Living Labs development, preliminary  version
Creators: name: Jorge, Leao
name: Luís, Ibáñez
name: Genís, Carrillo
name: Mikel, Borrás
Publisher: name: Zenodo
Year: 2024

description: This deliverable highlights the successful integration of the BIM-GIS toolkit into the HYPERGRYD platform for DHC network piping and configuration planning, demonstrating its application in both SONNE and ENVI living labs.
Supplementary Material from Neural operator learning of heterogeneous mechanobiological insults contributing to aortic aneurysms
Creators: name: Goswami, Somdatta
name: Li, David S.
name: Rego, Bruno V.
name: Latorre, Marcos
name: Humphrey, Jay D.
name: Em Karniadakis, George
Publisher: name: The Royal Society
Year: 2022
Subjects: subject: Biological Engineering
subject: 110601 Biomechanics
subject: FOS: Health sciences
subject: 90399 Biomedical Engineering not elsewhere classified
subject: FOS: Medical engineering

description: Thoracic aortic aneurysm (TAA) is a localized dilatation of the aorta that can lead to life-threatening dissection or rupture. Assessments of TAA progression in vivo are largely limited to measurements of aneurysm size and growth rate. There is promise, however, that computational modelling of the evolving biomechanics of the aorta could predict future geometry and properties from initiating mechanobiological insults. We present an integrated framework to train a deep operator network (DeepONet)-based surrogate model to identify TAA contributing factors using synthetic finite-element-based datasets. For training, we employ a constrained mixture model of aortic growth and remodelling to generate maps of local aortic dilatation and distensibility for multiple TAA risk factors. We evaluate the performance of the surrogate model for insult distributions varying from fusiform (analytically defined) to complex (randomly generated). We propose two frameworks, one trained on sparse information and one on full-field greyscale images, to gain insight into a preferred neural operator-based approach. We show that this continuous learning approach can predict the patient-specific insult profile associated with any given dilatation and distensibility map with high accuracy, particularly when based on full-field images. Our findings demonstrate the feasibility of applying DeepONet to support transfer learning of patient-specific inputs to predict TAA progression.
Cold Fronts: Probes of Plasma Astrophysics in Galaxy Clusters
Creators: name: ZuHone, John
name: Roediger, Elke
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The most massive baryonic component of galaxy clusters is the "intracluster medium" (ICM), a diffuse, hot, weakly magnetized plasma that is most easily observed in the X-ray band. Despite being observed for decades, the macroscopic transport properties of the ICM are still not well-constrained. A path to determine macroscopic ICM properties opened up with the discovery of "cold fronts". These were observed as sharp discontinuities in surface brightness and temperature in the ICM, with the property that the brighter (and denser) side of the discontinuity is the colder one. The high spatial resolution of the Chandra X-ray Observatory revealed two puzzles about the cold fronts. First, they should be subject to Kelvin-Helmholtz instabilites, yet in many cases they appear relatively smooth and undisturbed. Second, the width of the interface between the two gas phases is typically narrower than the mean free path of the particles in the plasma, indicating negligible thermal conduction. From the time of their discovery, it was realized that these special characteristics of cold fronts may be used to probe the physical properties of the cluster plasma. In this review, we will discuss the recent simulations of cold front formation and evolution in galaxy clusters, with a focus on those which have attempted to use these features to constrain the physics of the ICM. In particular, we will focus on the effects of magnetic fields, viscosity, and thermal conductivity on the stability properties and long-term evolution of cold fronts. We conclude with a discussion on what important questions remain unanswered, and the future role of simulations and the next generation of X-ray observatories.
description: 44 pages, 27 figures, submitted to the Journal of Plasma Physics
COVID-19 pandemic: Security agencies and extrajudicial killings amid enforcement of government lockdown order in Nigeria
Creators: name: Ifejika, Solomon I.
Publisher: name: Silpakorn University Research Innovation and Creativity Administration Office
Year: 2022
Subjects: Coronavirus
state security
security agencies
human rights
extrajudicialkillings

description: Humanities, Arts and Social Sciences Studies, 22, 3, 686-699
Techniques for the identity connection of disguised characters in Thai classical literary work for imaginary creation: "The tale of Khun Chang Khun Phaen: Phlai Chumphon fights Thera Khwat"
Creators: name: Wanwisa Promjeen And Atithep Chaetnalao
Publisher: name: Silpakorn University Research Innovation and Creativity Administration Office
Year: 2022
Subjects: Collective identity
disguise
Thai classical literature
Thai visual arts
visual arts

description: Humanities, Arts and Social Sciences Studies, 22, 3, 700-716
Fermi Study of gamma-ray Millisecond Pulsars: the Spectral Shape and Pulsed 25--200 GeV Emission from J0614-3329
Creators: name: Xing, Yi
name: Wang, Zhongxiang
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We report our analysis of the Fermi Large Area Telescope data for 39 millisecond pulsars (MSPs) listed in the second $γ$-ray pulsar catalog. Spectra of the pulsars are obtained. We fit the spectra with a function of a power law with exponential cutoff, and find the best-fit parameters of photon index $Γ= 1.54^{+0.10}_{-0.11}$ and cutoff energy $E_{c} = 3.70^{+0.95}_{-0.70}$ GeV. This spectral shape, which includes the intrinsic differences in the spectra of the MSPs, can be used for finding candidate MSPs and unidentified types of sources detected by Fermi at high Galactic latitudes. In one of the MSPs PSR J0614-3329, we find significant pulsed emission upto 200 GeV. The result has thus added this MSP to the group of the Crab and Vela pulsars that have been detected with >50 GeV pulsed emission. Comparing the $γ$-ray spectrum of PSR J0614-3329 with those of the Crab and Vela pulsars, we discuss possible emission mechanisms for the very high-energy component.
description: 9 pages, 5 figures, submitted
A structural equation modeling of performance quality of local government organization accountants
Creators: name: Suthira Thipwiwatpotjana, Kanchana Khuma
Publisher: name: Silpakorn University Research Innovation and Creativity Administration Office
Year: 2022
Subjects: Accountants
organizational culture
job satisfaction
organizational engagement

description: Humanities, Arts and Social Sciences Studies, 22, 3, 717-724
Development of Thai culture ontology-based metadata: Heet Sib Song (Twelve Months Festival)
Creators: name: Wirapong Chansanam And Kulthida Tuamsuk
Publisher: name: Silpakorn University Research Innovation and Creativity Administration Office
Year: 2022
Subjects: Ontology
metadata
Thai culture
Heet Sib Song
semantic integration

description: Humanities, Arts and Social Sciences Studies, 22, 3, 725-737
The three processes for de-duplication of organisations, data sources, and results of the OpenAIRE Graph
Creators: name: De Bonis, Michele
name: Baglioni, Miriam
name: Artini, Michele
name: Atzori, Claudio
name: Bardi, Alessia
Publisher: name: Zenodo
Year: 2023

description: The OpenAIRE Graph is one of the largest open scholarly record collections worldwide, key in fostering Open Science and establishing its practices in the daily research activities. It is a massive collection of metadata and links between scientific products such as articles, datasets, software, and other research products, entities like organisations, funders, funding streams, projects, communities, and data sources. To build the graph, OpenAIRE collects metadata records from more than 2K scholarly communication sources from all over the world, including Open Access institutional repositories, data archives, journals. Metadata records about the same scholarly work can be collected from different sources. Each metadata record can possibly carry different information because, for example, some sources are not aware of links to projects, keywords or other details. Another common case is when OpenAIRE collects one metadata record from a repository about a pre-print and another record from a journal about the published article. OpenAIRE detects that the two are two manifestations of the same scholarly work and merges them together. This poster describes the de-duplication approaches applied by OpenAIRE for three different types of entities: organisations, data sources, research results (i.e. publications, datasets, software and other types of research products). The poster will highlight how the deduplication process is completely automated for research results and specialised for different types of results. In the cases of organisations and data sources, instead, the process includes a step of manual curation. In particular for the organisations, the curation of the duplicates is performed by authorised people, who are experts of the research landscape of their country or discipline via a dedicated web tool. For the case of the data sources, instead, the curation is performed by the OpenAIRE technical team, who supervises the results of an automatic process and ensures the correct matching among data sources from DRIS, FAIRSharing, re3data, OpenDOAR, and the EOSC service catalogue.
description: This poster was presented during the 4th Open Science Fair (25-27 September, Madrid, Spain)
Trade-off Relations of Bell Violations among Pairwise Qubit Systems
Creators: name: Qin, Hui-Hui
name: Fei, Shao-Ming
name: Li-Jost, Xianqing
Publisher: name: arXiv
Year: 2015
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We investigate the nonlocality distributions among multiqubit systems based on the maximal violations of the Clauser-Horne-Shimony-Holt (CHSH) inequality of reduced pairwise qubit systems. We present a trade-off relation satisfied by these maximal violations, which gives rise to restrictions on the distribution of nonlocality among the subqubit systems. For a three-qubit system, it is impossible that all pairs of qubits violate the CHSH inequality, and once a pair of qubits violates the CHSH inequality maximally, the other two pairs of qubits must both obey the CHSH inequality. Detailed examples are given to illustrate the trade-off relations, and the trade-off relations are generalized to arbitrary multiqubit systems.
description: 9 pages
Reaction Rates and Kinetic Isotope Effects of H$_2$ + OH $\rightarrow$ H$_2$O + H
Creators: name: Meisner, Jan
name: Kästner, Johannes
Publisher: name: arXiv
Year: 2016
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We calculated reaction rate constants including atom tunneling of the reaction of dihydrogen with the hydroxy radical down to a temperature of 50 K. Instanton theory and canonical variational theory with microcanonical optimized multidimensional tunneling (CVT/$μ$OMT) were applied using a fitted potential energy surface [J. Chem. Phys. 138, 154301 (2013)]. All possible protium/deuterium isotopologues were considered. Atom tunneling increases at about 250 K (200 K for deuterium transfer). Even at 50 K the rate constants of all isotopologues remain in the interval $ 4 \cdot 10^{-20}$ to $4 \cdot 10^{-17}$ cm$^3$ s$^{-1}$ , demonstrating that even deuterated versions of the title reaction are possibly relevant to astrochemical processes in molecular clouds. The transferred hydrogen atom dominates the kinetic isotope effect at all temperatures.
description: title page, 16 pages, followed by 6 pages of SI
Amtliche Mitteilungen der Technischen Universität Dortmund Nr. 17/2016
Creators: name: (:Unkn) Unknown
Publisher: name: Technische Universität Dortmund
Year: 2016
Subjects: subject: 080

description: Erste Ordnung zur Änderung der Fakultätsordnung für die Fakultät Raumplanung vom 31.05.2016
description: Amtliche Mitteilungen der Technischen Universität Dortmund;17, 2016
China's foreign policy trends towards Russia, late 20th - early 21st century (economic aspects)
Creators: name: Md. Sayedur Rahman AndShakila -Tul-Kubra
Publisher: name: Silpakorn University Research Innovation and Creativity Administration Office
Year: 2022
Subjects: China
Russia
economic relation
foreign policy
bilateral trade
international relations

description: Humanities, Arts and Social Sciences Studies, 22, 3, 738-754