cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Unveiling the kinematics of a central region in the triple AGN host NGC 7733-7734 interacting group
Creators: name: Keshri, Saili
name: Barway, Sudhanshu
name: Das, Mousumi
name: Yadav, Jyoti
name: Combes, Francoise
Publisher: name: arXiv
Year: 2025
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a detailed study of the interacting triple active galactic nuclear system NGC 7733-34, focusing on stellar kinematics, ionised gas characteristics and star formation within the central region and stellar bars of both galaxies. We performed a comprehensive analysis using archival data from MUSE, HST/ACS, and DECaLS, complemented by observations from UVIT and IRSF. We identified a disc-like bulge in both NGC 7733 and NGC 7734 through 2-D decomposition. A central nuclear structure, with a semi-major axis of $\sim$1.113 kpc, was detected in NGC 7733 via photometric and kinematic analysis, confirmed by the strong anti-correlation between $V/σ$ and $h_{3}$, indicative of circular orbits in the centre. NGC 7734 lacks a distinct nuclear structure. The presence of disc-like bulge results in an anti-correlation between $V/σ$ and $h_{3}$ along with diffuse light. However, it does show higher central velocity dispersion, possibly attributed to an interaction with a smaller clump, which is likely a fourth galaxy within the system. Both galaxies demonstrate ongoing star formation, evidenced by $FUV$ and $Hα$ observations. NGC 7734 shows recent star formation along its bar, while NGC 7733 experiences bar quenching. The star formation rate (SFR) analysis of NGC 7734 reveals that the bar region's SFR dominates the galaxy's overall SFR. Conversely, in NGC 7733, the lack of star formation along the bar and the presence of a Seyfert 2 active galactic nuclei at the galaxy centre leave the possibility of a connection between both facts. However, it does not affect the galaxy's overall star formation. Our findings provide valuable insights into the stellar and gas kinematics, star formation processes, and active galactic nuclear feedback mechanisms in interacting galaxies hosting stellar bars.
description: 15 pages, 11 figures, accepted for publication in A&A
sj-docx-1-car-10.1177_19476035231194771 – Supplemental material for Il-1β Promotes Superficial Zone Cells Senescence in Articular Cartilage by Inhibiting Autophagy
Creators: name: Xu, Wei
name: Wang, Juan
name: Cui, Lin
name: Huang, Chen
name: Xia, Ning
name: Xie, Meiming
name: Liu, Da
name: Liao, Dongfa
Publisher: name: SAGE Journals
Year: 2023
Subjects: Orthopaedics
Sports Medicine
Surgery
Biological Sciences not elsewhere classified

description: Supplemental material, sj-docx-1-car-10.1177_19476035231194771 for Il-1β Promotes Superficial Zone Cells Senescence in Articular Cartilage by Inhibiting Autophagy by Wei Xu, Juan Wang, Lin Cui, Chen Huang, Ning Xia, Meiming Xie, Da Liu and Dongfa Liao in CARTILAGE
TeV afterglow emission from a structured GRB jet using the kinetic approach
Creators: name: Hope, John P.
name: van Eerten, Hendrik J.
name: Kundu, Sayan
name: Schady, Patricia
Publisher: name: arXiv
Year: 2025
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Recent years have seen a growing sample of TeV emission detections in gamma-ray burst afterglows, as well as an increasing role for structured jets in afterglow modelling. Using a kinetic approach, we show that the structure of an afterglow jet impacts its TeV emission, with jets where the energy falls off more sharply with angle showing a decrease in Inverse Compton (IC) peak flux relative to synchrotron peak flux. We use a modified version of the code katu, to which we have added adiabatic expansion and a fully self-consistent treatment of IC cooling both for the electron and photon populations. We compare our results to the semi-analytical code afterglowpy, finding a good agreement with our model except at early times off axis where the effects of baryon loading are important. We compare electron cooling in the cases where there is no IC cooling, Thomson cooling and an inclusion of Klein-Nishina effects, finding that the spectra can only be distinguished if the Compton potential is significantly increased. We obtain a similar cooling rate compared to semi-analytical solutions, with some small difference at the transition from IC to synchrotron dominated cooling. Finally, we use best-fit parameters determined by afterglowpy and re-scaled for our model to reproduce the light curves of GRB 170817A. For our choice of parameters, we find that GRB 170817 would not have been detected in the TeV domain if seen on-axis, even by the upcoming Cherenkov Telescope Array Observatory.
description: 20 pages, 13 figures. Fig.10b and associated analysis has been corrected due to an error in model comparison. Additionally, derivation of adiabatic timescale now assumes said timescale to be positive and has been updated accordingly. This is a pre-copyedited, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review
25 years of XMM-Newton observations of the Sgr A complex: 3D distribution and internal structure of the clouds
Creators: name: Stel, G.
name: Ponti, G.
name: Haardt, F.
name: Sormani, M. C.
Publisher: name: arXiv
Year: 2025
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Sgr A* is currently very faint. However, X-ray radiation reflected by the Sgr A complex, a group of nearby molecular clouds, suggests that it went through one or more periods of high activity some hundreds of years ago. We aim to determine whether previously proposed physical scenarios are consistent with the observed X-ray variability over the past 25 years, and to characterize the spatial distribution, shape, and internal structure of the clouds. We exploit the full set of XMM-Newton observations, extending the previously studied dataset on variability by at least 12 years. Starting from the recent IXPE result that places the so-called Bridge cloud 26 pc behind Sgr A*, we reconstruct the LOS position of the other clouds, assuming that they were illuminated by a single flare. Additionally, we derive the probability density function (PDF) of the molecular density. We also study the 3D geometry of the complex in case two flares illuminate the clouds. As of spring 2024, the lightfront is still illuminating the Sgr A complex, with the Bridge currently being the brightest cloud. The other clouds in the complex have faded significantly. In the single flare scenario, the Sgr A complex is located $\simeq$ 25 pc behind Sgr A*. In the past 25 years, the illuminated region spans 10-15 pc along the LOS. The derived PDF is roughly log-normal, consistent with previous Chandra results, with a possible high-density excess. Both a single and a multiple flares scenario can explain the observed X-ray variability. Previous concerns about the single flare scenario, raised by shorter monitoring, are now overcome in the 25 years of monitoring. If two flares illuminate the clouds, they must be separated by at least $\sim$ 30 years. We speculate that these clouds are closer to Sgr A* than the nuclear molecular ring at $\simeq$ 100-200 pc and possibly drifting from the ring to the inner region of the Galaxy.
description: 19 pages, 15 figures. Accepted for publication in A&A
sj-docx-1-jtt-10.1177_1357633X231187432 - Supplemental material for Effectiveness of mHealth-based psychosocial interventions for breast cancer patients and their caregivers: A systematic review and meta-analysis
Creators: name: Tan, Jia Yu Amelia
name: Ong, Germaine Yi Qing
name: Cheng, Ling Jie
name: Pikkarainen, Minna
name: He, Hong-Gu
Publisher: name: SAGE Journals
Year: 2023
Subjects: Health and Community Services
Public Health and Health Services not elsewhere classified

description: Supplemental material, sj-docx-1-jtt-10.1177_1357633X231187432 for Effectiveness of mHealth-based psychosocial interventions for breast cancer patients and their caregivers: A systematic review and meta-analysis by Jia Yu Amelia Tan, Germaine Yi Qing Ong, Ling Jie Cheng, Minna Pikkarainen and Hong-Gu He in Journal of Telemedicine and Telecare
sj-docx-1-chi-10.1177_17423953231200678 - Supplemental material for Impact on diabetes outcomes and team skills of integrating dietetic services into interprofessional education and teamwork in primary care
Creators: name: Rowe, Gina C
name: McShane, Phyllis
name: Brennan Congdon, Heather
name: Pittman, Joan
name: Rios, Judith
Publisher: name: SAGE Journals
Year: 2023
Subjects: Nursing not elsewhere classified
Aged Health Care
Respiratory Diseases

description: Supplemental material, sj-docx-1-chi-10.1177_17423953231200678 for Impact on diabetes outcomes and team skills of integrating dietetic services into interprofessional education and teamwork in primary care by Gina C Rowe, Phyllis McShane, Heather Brennan Congdon, Joan Pittman and Judith Rios in Chronic Illness
Additional file 2 of The impact of evidence-based nursing leadership in healthcare settings: a mixed methods systematic review
Creators: name: Välimäki, Maritta
name: Hu, Shuang
name: Lantta, Tella
name: Hipp, Kirsi
name: Varpula, Jaakko
name: Chen, Jiarui
name: Liu, Gaoming
name: Tang, Yao
name: Chen, Wenjun
name: Li, Xianhong
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences

description: Supplementary Material 2
Additional file 1 of Upper gastrointestinal bleeding on veno-arterial extracorporeal membrane oxygenation support
Creators: name: de Roux, Quentin
name: Disli, Yekcan
name: Bougouin, Wulfran
name: Renaudier, Marie
name: Jendoubi, Ali
name: Merle, Jean-Claude
name: Delage, Mathilde
name: Picard, Lucile
name: Sayagh, Faiza
name: Cherait, Chamsedine
name: Folliguet, Thierry
name: Quesnel, Christophe
name: Becq, Aymeric
name: Mongardon, Nicolas
Publisher: name: figshare
Year: 2024
Subjects: subject: Biophysics
subject: Medicine
subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Biological Sciences not elsewhere classified
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences

description: Supplementary Material 1
sj-pdf-1-smo-10.1177_20503121231196703 – Supplemental material for Knowledge and attitude regarding the COVID-19 pandemic among undergraduate health science students of Nepal: An online survey
Creators: name: Anand, Ayush
name: Gupta, Ashwini
name: Singh, Sweta
name: Pyakurel, Sulav
name: Karkee, Rajendra
name: Pyakurel, Prajjwal
Publisher: name: SAGE Journals
Year: 2023
Subjects: subject: Health and Community Services
subject: Cardiology
subject: Dentistry not elsewhere classified
subject: Emergency Medicine
subject: Endocrinology
subject: Geriatrics and Gerontology
subject: Neurology and Neuromuscular Diseases
subject: FOS: Clinical medicine
subject: Nursing not elsewhere classified
subject: Nutrition and Dietetics not elsewhere classified
subject: Oncology and Carcinogenesis not elsewhere classified
subject: Orthopaedics
subject: Sports Medicine
subject: Otorhinolaryngology
subject: Aged Health Care
subject: Paediatrics
subject: Pharmacology and Pharmaceutical Sciences not elsewhere classified
subject: Psychology not elsewhere classified
subject: Psychiatry (incl. Psychotherapy)
subject: Public Health and Health Services not elsewhere classified
subject: Respiratory Diseases
subject: Sociological Methodology and Research Methods
subject: Surgery
subject: Veterinary Medicine

description: Supplemental material, sj-pdf-1-smo-10.1177_20503121231196703 for Knowledge and attitude regarding the COVID-19 pandemic among undergraduate health science students of Nepal: An online survey by Ayush Anand, Ashwini Gupta, Sweta Singh, Sulav Pyakurel, Rajendra Karkee and Prajjwal Pyakurel in SAGE Open Medicine
sj-docx-5-jet-10.1177_15266028231198206 – Supplemental material for Impact of Hospital Volume on Long-Term Outcomes After Endovascular Therapy for Peripheral Artery Disease
Creators: name: Setogawa, Nao
name: Ohbe, Hiroyuki
name: Matsui, Hiroki
name: Yasunaga, Hideo
Publisher: name: SAGE Journals
Year: 2023
Subjects: Cardiology
Medicine
Surgery

description: Supplemental material, sj-docx-5-jet-10.1177_15266028231198206 for Impact of Hospital Volume on Long-Term Outcomes After Endovascular Therapy for Peripheral Artery Disease by Nao Setogawa, Hiroyuki Ohbe, Hiroki Matsui and Hideo Yasunaga in Journal of Endovascular Therapy
Toylabs D4.1 - Collaboration Platform Design And Development
Creators: name: ToyLabs Consortium
Publisher: name: Zenodo
Year: 2017

description: Deliverable D4.1 titled as “Collaboration Platform Design and Development-v1” is used to document the architecture of the Toylabs Core Platform as well as to provide a plan for the integration of the Toylabs added-value components in the platform.

The deliverable has the nature of a “Demonstrator”, therefore the document at hand acts as an accompanying text to the developed software platform, the source code of which can be found in the project’s GitHub repository, located at https://github.com/singularlogic/ToyLabs

The architecture and (if needed) the integration plan presented in D4.1 will be updated throughout the project as the new components will be further developed and integrated at the end of each development circle, resulting to deliverables D4.2, D4.3 and D4.4 and to the release of the stable final version of the Collaboration Platform.
Constructivist Grounded Theory Analysis
Creators: name: Freitas, Francisco
Publisher: name: Zenodo
Year: 2022
Subjects: Qualitative Analysis
Grounded Theory Analysis
MAXQDA
CAQDAS
Constructivism
Data Analysis
Coding Data

description: A presentation comprising a description of Grounded Theory Analysis main features and how to transpose this theoretical framework to MAXQDA, a leading software package for qualitative and mixed methods data analysis. The focus is on the constructivist option proposed by Kathy Charmaz (1990, 2000, 2002, 2006), a very interesting framework to develop grounded theory analyses. The main concepts are presented to guide software usage accordingly. This methodological framework is used mostly on controlled amounts of textual data (e.g. interviews or focus groups).
Toylabs D4.2 - Integrated Platform Design And Development - V1
Creators: name: ToyLabs Consortium
Publisher: name: Zenodo
Year: 2018

description: Deliverable D4.2 titled as “Integrated Platform Design and Development-v1” is used to document the 1 st prototype version of the ToyLabs integrated platform.

The deliverable has the nature of a “Demonstrator”, therefore the document at hand acts as an accompanying text to the developed software, the source code of which can be found in the project’s GitHub repository, located at

https://github.com/singularlogic/ToyLabs

D4.2 will be updated throughout the project as the new components will be further developed and integrated, leading to a new version of the integrated platform at the end of each development circle, resulting to deliverables D4.3 and D4.4 and to the release of the stable final version of the Collaboration Platform.
Additional file 3 of Bacterial contamination of healthcare workers’ mobile phones in Africa: a systematic review and meta-analysis
Creators: name: Zenbaba, Demisu
name: Sahiledengle, Biniyam
name: Beressa, Girma
name: Desta, Fikreab
name: Teferu, Zinash
name: Nugusu, Fikadu
name: Atlaw, Daniel
name: Shiferaw, Zerihun
name: Gezahegn, Bereket
name: Mamo, Ayele
name: Desalegn, Tesfaye
name: Negash, Wogene
name: Negash, Getahun
name: Mama, Mohammedaman
name: Nigussie, Eshetu
name: Chattu, Vijay Kumar
Publisher: name: figshare
Year: 2024
Subjects: subject: Microbiology
subject: FOS: Biological sciences

description: Additional file 3. Risk of bias assessment of included studies.
A theoretical framework for BL Her stars IV. New period-luminosity relations in the Rubin-LSST filters
Creators: name: Das, Susmita
name: Molnár, László
name: Szabó, Róbert
name: Singh, Harinder P.
name: Kanbur, Shashi M.
name: Bhardwaj, Anupam
name: Marconi, Marcella
name: Smolec, Radoslaw
Publisher: name: arXiv
Year: 2025
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present new theoretical light curves in the Rubin-LSST filters for a fine grid of BL Her models computed using MESA-RSP. We also derive new theoretical period-luminosity (PL) and period-Wesenheit (PW) relations in the Rubin-LSST filters with the goal to study the effect of convection parameters and metallicity on these relations. The grid of BL Her models was computed with the input stellar parameters: metallicity ($-2.0\; \mathrm{dex} \leq \mathrm{[Fe/H]} \leq 0.0\; \mathrm{dex}$), stellar mass ($0.5M_{\odot}-0.8M_{\odot}$), stellar luminosity ($50L_{\odot}-300L_{\odot}$), and effective temperature (across the full extent of the instability strip; in steps of 50K) and using four sets of convection parameters. Bolometric correction tables from MIST were used to transform the theoretical bolometric light curves of the BL Her models into the Rubin-LSST ugrizy filters. The PL relations of the BL Her models exhibit steeper slopes but smaller dispersion with increasing wavelengths in the Rubin-LSST filters. The PL and PW slopes for the complete set of BL Her models computed with radiative cooling (sets B and D) are statistically similar across the grizy filters. The BL Her models exhibit weak or negligible effect of metallicity on the PL relations for wavelengths longer than the g filter for both the cases of the complete set of models as well as the low-mass models. However, we find significant effect of metallicity on the PL relation in the u filter. Strong metallicity effects are observed in the PWZ relations involving the u filter and are found to have significant contribution from the high-metallicity BL Her models. Due to negligible metallicity effect for relations involving the Wesenheit indices $W(i,g-i)$, $W(z,i-z)$ and $W(y,g-y)$, we recommend these filter combinations for BL Her stars when observed with the Rubin-LSST to be used as reliable standard candles.
description: 19 pages, 7 figures, 13 tables. Accepted for publication in Astronomy & Astrophysics
MINCE III. Detailed chemical analysis of the UVES sample
Creators: name: Lucertini, F.
name: Sbordone, L.
name: Caffau, E.
name: Bonifacio, P.
name: Monaco, L.
name: Cescutti, G.
name: Lallement, R.
name: François, P.
name: Spitoni, E.
name: Hansen, C. J.
name: Korn, A. J.
name: Kučinskas, A.
name: Mucciarelli, A.
name: Magrini, L.
name: Lombardo, L.
name: Franchini, M.
name: de Melo, R. F.
Publisher: name: arXiv
Year: 2025
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Context. The MINCE (Measuring at Intermediate Metallicity Neutron-Capture Elements) project aims to provide high quality neutron-capture abundances measurements in several hundred stars at intermediate metallicity,-2.5 < [Fe/H] < -1.5. This project will shed light on the origin of the neutron-capture elements and the chemical enrichment of the Milky Way. Aims. The goal of this work is to chemically characterize the second sample of the MINCE project and compare the abundances with the galactic chemical evolution model at our disposal. Methods. We performed a standard abundance analysis based on 1D LTE model atmospheres on high-resolution and high-signal-to-noise-ratio UVES spectra. Results. We provide the kinematic classification (i.e., thin disk, thick disk, thin-to-thick disk, halo, Gaia Sausage Enceladus, Sequoia) of 99 stars and the atmospheric parameters for almost all stars. We derive the abundances for light elements (from Na to Zn) and neutron-capture elements (Rb, Sr, Y, Zr, Ba, La, Ce, Pr, Nd, Sm, Eu) in a subsample of 32 stars in the metallicity range -2.5 < Fe/H] < -1.00. In the subsample of 32 stars, we identify 8 active stars exhibiting (inverse) P-Cygni profile and one Li-rich star, CD 28-11039. We find a general agreement between the chemical abundances and the stochastic model computed for the chemical evolution of the Milky Way halo for the elements Mg, Ca, Si, Ti, Sc, Mn, Co, Ni, Zn, Rb, Sr, Y, Zr, Ba, La, and Eu . Conclusions. The MINCE project has already significantly increased the number of neutron-capture elements measurements in the intermediate metallicity range. The results from this sample are in perfect agreement with the previous MINCE sample. The good agreement between the chemical abundances and the chemical evolution model of the Galaxy supports the nucleosynthetic processes adopted to describe the origin of the n-capture elements.
description: 33 pages, 15 figures, 11 tables
Ludger Honnefelder (Hrsg.), Natur als Gegenstand der Wissenschaften
Creators: name: Mutschler, Hans-Dieter
Publisher: name: Theologie und Philosophie
Year: 1970

description: Theologie und Philosophie, Bd. 69 Nr. 1 (1994): Theologie und Philosophie, Band 69, Heft 1
Observing short-range correlations in nuclei through $ρ^0$ photo-production
Creators: name: Sharp, Phoebe
name: Schmidt, Axel
Publisher: name: arXiv
Year: 2025
Subjects: subject: Nuclear Theory (nucl-th)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: Short-range correlations (SRCs) are a universal feature of nuclear structure. A wide range of measurements, primarily using electron scattering, have revealed SRC properties, such as their abundance in different nuclei, as well as the strong preference for proton-neutron pairing over proton-proton or neutron-neutron pairing. Despite the inherent complexity of many-body systems, a number of the salient features of electron scattering measurements are described by a simple, factorized theory called Generalized Contact Formalism. A key element of this theory, the factorization of the interaction with a hard probe, has yet to be tested. An experiment conducted at Jefferson Lab in 2021 collected data from scattering a tagged photon beam, with an energy up to 10 GeV, from several nuclear targets, measuring final state particles in the large-acceptance GlueX spectrometer. In this paper, we propose a test of probe factorization by measuring cross section ratios sensitive to proton-proton pair prevalence and relative SRC abundances in $^4$He and $^{12}$C. We present GCF predictions of the observables and make projections of the expected precision the experiment can achieve.
description: 17 pages, 6 figures
Additional file 1 of The impact of evidence-based nursing leadership in healthcare settings: a mixed methods systematic review
Creators: name: Välimäki, Maritta
name: Hu, Shuang
name: Lantta, Tella
name: Hipp, Kirsi
name: Varpula, Jaakko
name: Chen, Jiarui
name: Liu, Gaoming
name: Tang, Yao
name: Chen, Wenjun
name: Li, Xianhong
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences

description: Supplementary Material 1
Additional file 1 of Test-reduced teaching for stimulation of intrinsic motivation (TRUST): a randomized controlled intervention study
Creators: name: Faure, Theresa
name: Weyers, Imke
name: Voltmer, Jan-Bennet
name: Westermann, Jürgen
name: Voltmer, Edgar
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Neuroscience
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Science Policy
subject: Mental Health

description: Supplementary Material 1
Toylabs D4.4 - Toylabs Integrated Platform Design, Development And Validation - Final Version
Creators: name: ToyLabs Consortium
Publisher: name: Zenodo
Year: 2018

description: Deliverable 4.4 titled as “Toylabs Integrated Platform Design, Development and Validation” refers to the final release of the Integrated ToyLabs platform, including all the features and characteristics covering the requirements identified during the project, as well as updates and fixes on the basis of the feedback gained from pilot’s execution and testing.

The deliverable includes for the integrated platform and for each added-value component included detailed step-by-step instructions on how the different functions operate, in a form of a basic tutorial.

Moreover, the deliverable provides technical information regarding the way that the different components have been integrated in the platform, as well as the time-plan followed by the development team for integrating all components in successive development circles.

In addition, D4.4 includes the software validation outcomes, as results of the testing process followed for the different components which constitute the Toylabs platform.

The deliverable is of type “Other”, acting as an accompanying text to the developed software, the source code of which can be found in the project’s GitHub repository, located at https://github.com/singularlogic/ToyLabs.
Demo of picoRing mouse: an ultra-low-powered wireless mouse ring with ring-to-wristband coil-based impedance sensing
Creators: name: Li, Yifan
name: Fukumoto, Masaaki
name: Kari, Mohamed
name: Yokota, Tomoyuki
name: Someya, Takao
name: Kawahara, Yoshihiro
name: Takahashi, Ryo
Publisher: name: arXiv
Year: 2025
Subjects: subject: Human-Computer Interaction (cs.HC)
subject: FOS: Computer and information sciences
subject: B.4.2

description: Wireless mouse rings offer subtle, reliable pointing interactions for wearable computing platforms, but the small battery below 27 mAh in the miniature rings restricts the ring's continuous lifespan to just 1-2 hours due to the power consumption of current low-powered wireless communication like BLE. However, the picoRing mouse addresses this by enabling continuous ring-based mouse interaction with ultra-low-powered ring-to-wristband wireless communication through a coil-based impedance sensing method called semi-passive inductive telemetry. This allows a wristband coil to capture a unique frequency response of a nearby ring coil via sensitive inductive coupling, converting the user's mouse input into the unique frequency response via an 820 uW mouse-driven modulation module. Thus, the continuous use of picoRing mouse can potentially last over 92 hours on a single charge of a 20 mAh battery while supporting subtle scrolling and pressing interactions.
Jürgen Schröder, Das Computermodell des Geistes in der analytischen Philosophie und in der kognitiven Psychologie des Sprachverstehens
Creators: name: Brüntrup, Godehard
Publisher: name: Theologie und Philosophie
Year: 1970

description: Theologie und Philosophie, Bd. 69 Nr. 1 (1994): Theologie und Philosophie, Band 69, Heft 1
Ludger Honnefelder (Hrsg.) / Werner Schüßler (Hrsg.), Transzendenz
Creators: name: Haeffner, Gerd
Publisher: name: Theologie und Philosophie
Year: 1970

description: Theologie und Philosophie, Bd. 69 Nr. 1 (1994): Theologie und Philosophie, Band 69, Heft 1
Distilling Large Language Models for Network Active Queue Management
Creators: name: Satish, Deol
name: Pokhrel, Shiva Raj
name: Kua, Jonathan
name: Walid, Anwar
Publisher: name: arXiv
Year: 2025
Subjects: subject: Networking and Internet Architecture (cs.NI)
subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences

description: The growing complexity of network traffic and demand for ultra-low latency communication require smarter packet traffic management. Existing Deep Learning-based queuing approaches struggle with dynamic network scenarios and demand high engineering effort. We propose AQM-LLM, distilling Large Language Models (LLMs) with few-shot learning, contextual understanding, and pattern recognition to improve Active Queue Management (AQM) [RFC 9330] with minimal manual effort. We consider a specific case where AQM is Low Latency, Low Loss, and Scalable Throughput (L4S) and our design of AQM-LLM builds on speculative decoding and reinforcement-based distilling of LLM by tackling congestion prevention in the L4S architecture using Explicit Congestion Notification (ECN) [RFC 9331] and periodic packet dropping. We develop a new open-source experimental platform by executing L4S-AQM on FreeBSD-14, providing interoperable modules to support LLM integration and facilitate IETF recognition through wider testing. Our extensive evaluations show L4S-LLM enhances queue management, prevents congestion, reduces latency, and boosts network performance, showcasing LLMs' adaptability and efficiency in uplifting AQM systems.
description: After a careful review, we identified some issues that need to be addressed. We temporarily withdraw the paper while we update our experimental results, ensuring that our demonstration and findings meet the highest standards of accuracy and clarity
Flaring Activities of Fast Rotating Stars have Solar-like Latitudinal Distribution
Creators: name: Yang, Huiqin
name: Cheng, Xin
name: Liu, Jifeng
name: Liu, Shuai
name: Zhao, Zhanhao
name: Zhou, Guiping
name: Hou, Yijun
name: Gao, Changliang
name: Niu, Zexi
Publisher: name: arXiv
Year: 2025
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The dynamo theory has always been one of the biggest mysteries in stellar physics. One key reason for its uncertainty is poor knowledge of the dynamo process on stars except the Sun. The most important observation feature of solar dynamo is that active regions only appear at low latitudes, which provides a crucial constraint to the dynamo theory, while Doppler imaging, the current technique to spatially resolve stellar hemisphere, is difficult to distinguish the equatorial region . Hence, the latitudinal distribution of active regions (LDAR) of stars is ambiguous and controversial, mainly due to the limit of the current technique for spatially resolving the stellar surface. Fast rotating stars, which are young and active, are thought to operate with a different dynamo process than the Sun. We study their LDAR and compare them with the Sun to reveal the underlying dynamo process. Flares are drastic and observational activity events, which occur in active regions. Here, we propose a new method to study how the apparent flaring activity varies with respect to the inclination to determine the LDAR of fast rotating stars.We find that the LDAR of fast rotating stars is consistent with that of the Sun, contrary to expectations. Our results provide a crucial constraint to stellar dynamo, indicating that the solar-like dynamo also applies to fast rotating stars, even spanning different stages of their evolution.
description: 12 pages,10 figures, accepted by A&A
On variability of DDO68-V1, a unique extremely metal-poor LBV
Creators: name: Pustilnik, S. A.
name: Perepelitsyna, Y. A.
Publisher: name: arXiv
Year: 2025
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: DDO68-V1 is a Luminous Blue Variable (LBV) star in the eXtremely Metal-Poor (XMP) galaxy DDO68. It resides in the HII region with 12+log(O/H)~7.1 dex, or Z ~ Zo/40. Since DDO68-V1 is the only known LBV with a so low initial metallicity, its in-deep study can give the hints for understanding the LBV evolutionary stage and the nature of their powerful and highly variable mass loss in the very low-metallicity regime. Our goal is to study the optical variability of DDO68-V1 during the last 36 years, with the emphasis on the period of the last 8 years, after the LBV giant eruption. We use our published results of monitoring in B, V, R bands of the total flux of HII region 'Knot 3', containing the LBV, along with photometry of the archive Hubble Space Telescope (HST) images, obtained in May 2010 and December 2017. This data allow us to disentangle the variable light of DDO68-V1 and that of the underlying HII region. From all available photometry of Knot 3, we derive the V-band lightcurve of DDO68-V1 since 1988, with a higher cadence during the years 2015-2023, when the lightcurve resembles that of S Doradus. The new data reveal the full range of DDO68-V1 absolute magnitudes M_V of [-5.9, --10.8] mag. The LBV variations after the fading of the 'giant eruption' show the unusually large amplitude of delta_V > 3.0-3.5mag on the time-scale of ~1-1.5 year. The apparent changes of the integrated B-V colour of Knot 3 are consistent with the expected colour variations of the LBV in course of the S Doradus 'normal eruptions'. These data, along with spectra of DDO68-V1, demonstrate the need for a higher-cadence photometry of DDO68-V1, in order to probe the possible periodicity in its lightcurve and binarity of the object.
description: Accepted (almost) to A&A Letters. 5 pages plus 6 pages of Appendices, 5 figures
Emergence of magnetic flux sheets in the quiet Sun. I. Statistical properties
Creators: name: Díaz-Castillo, S. M.
name: Fischer, C. E.
name: Moreno-Insertis, F.
name: Guglielmino, S. L.
name: Ishikawa, R.
name: Criscuoli, S.
Publisher: name: arXiv
Year: 2025
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Small-scale magnetic flux emergence in the quiet Sun is crucial for maintaining solar magnetic activity. On the smallest scales studied so far, namely within individual granules, two mechanisms have been identified: emergence in tiny magnetic loops and emergence in the form of magnetic flux sheets covering the granule. While there are abundant observations of tiny magnetic loops within granules, the evidence for the emergence of granule-covering magnetic sheets is much more limited. This work aims to statistically analyze magnetic flux sheets, quantify their frequency on the solar surface and their potential contribution to the solar magnetic budget in the photosphere, and investigate the plasma dynamics and granular-scale phenomena associated with their emergence. Using spectro-polarimetric datasets from the solar optical telescope aboard the Hinode satellite and the ground-based Swedish Solar telescope, we developed a two-step method to identify magnetic flux sheet emergence events, detecting magnetic flux patches based on the calculation of the transverse and longitudinal magnetic flux density and associating them with their host granules based on velocity field analysis. We identified 42 events of magnetic flux sheet emergence and characterized their magnetic properties and the associated plasma dynamics of their host granules. Our results align with numerical simulations, indicating a similar occurrence rate. We investigated the relationship between magnetic flux emergence and granular phenomena, finding that flux sheets often emerge in association with standard nascent granules, as well as exploding granules, or granules with granular lanes. In particular, we highlight the potential role of recycled magnetic flux from downflow regions in facilitating flux sheet emergence.
description: Accepted for publication A&A
Additional file 1 of Efficacy comparison between intramedullary nail fixation and plate fixation in distal tibia fractures: a meta-analysis of randomized controlled trials
Creators: name: Li, Xiaobin
name: Chen, Kaipeng
name: Xue, Haipeng
name: Cheng, Junwen
name: Yu, Xiaoping
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Science Policy

description: Supplementary Material 1
Experimenting with the Garsia-Milne Involution Principle
Creators: name: Ekhad, Shalosh B.
name: Zeilberger, Doron
Publisher: name: arXiv
Year: 2025
Subjects: subject: Combinatorics (math.CO)
subject: FOS: Mathematics

description: In 1981, Adriano Garsia and Steve Milne found the first bijective proof of the celebrated Rogers-Ramanujan identities. To achieve this feat, they invented a versatile tool that they called the Involution Principle. In this note we revisit this useful principle from a very general perspective, independent of its application to specific combinatorial identities, and will explore its complexity.
description: In memory of Adriano Garsia (1928-2024) and in honor of Stephen C. Milne's 75th birthday
Tidal disruption events as the origin of the eROSITA and Fermi bubbles
Creators: name: Scheffler, Tassilo
name: Schulreich, Michael M.
name: Schurer, David P. P. R.
name: Breitschwerdt, Dieter
Publisher: name: arXiv
Year: 2025
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Context: The recently discovered spherical eROSITA bubbles arise up to a latitude of $\pm$80°-85°in the X-ray regime of the Milky Way halo. Similar to the $γ$-ray Fermi bubbles, they evolve around the Galactic center, making a common origin plausible. However, the driving mechanism and evolution of both bubbles are still under debate. Aims: We investigate whether hydrodynamic energy injections at the Galactic center, such as e.g. tidal disruption events (TDEs), could have inflated both bubbles. The supermassive black hole Sagittarius A* is expected to tidally disrupt a star every 10-100 kyr, potentially leading to an outflow from the central region that drives a shock propagating into the Galactic halo due to its vertically declining density distribution, ultimately forming a superbubble that extends out of the disk similar to the eROSITA and Fermi bubbles. Methods: We model TDEs in the Galaxy using three-dimensional hydrodynamical simulations, considering different Milky Way mass models and TDE rates. We then generate synthetic X-ray maps and compare them with observations. Results: Our simulation results of a $β$-model Milky Way halo show that superbubbles, blown for 16 Myr by regular energy injections at the Galactic center that occur every 100 kyr, can have a shape, shell stability, size, and evolution time similar to estimates for the eROSITA bubbles, and an overall structure reminiscent of the Fermi bubbles. The $γ$-rays in our model would stem from cosmic ray interactions at the contact discontinuity, where they were previously accelerated by first-order Fermi acceleration at in situ shocks. Conclusions: Regular TDEs in the past 10-20 Myr near the Galactic center could have driven an outflow resulting in both, the X-ray emission of the eROSITA bubbles and the $γ$-ray emission of the Fermi bubbles.
description: 13 pages, 7 figures, published in Astronomy & Astrophysics (A&A)
Additional file 4 of Ecological stress memory in wood architecture of two Neotropical hickory species from central-eastern Mexico
Creators: name: Rodríguez-Ramírez, Ernesto C.
name: Frei, Jonas
name: Ames-Martínez, Fressia N.
name: Guerra, Anthony
name: Andrés-Hernández, Agustina R.
Publisher: name: figshare
Year: 2024
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Ecology

description: Supplementary Material 4
sj-docx-1-pim-10.1177_14750902221112530 – Supplemental material for Aeration desulfurization of offshore oilfield produced water used for preparation of polymer solutions
Creators: name: Shi, Weiye
name: Fan, Zhenhua
name: Liu, Tongzhe
name: Zhang, Lei
Publisher: name: SAGE Journals
Year: 2022
Subjects: Engineering not elsewhere classified
Materials Engineering not elsewhere classified

description: Supplemental material, sj-docx-1-pim-10.1177_14750902221112530 for Aeration desulfurization of offshore oilfield produced water used for preparation of polymer solutions by Weiye Shi, Zhenhua Fan, Tongzhe Liu and Lei Zhang in Proceedings of the Institution of Mechanical Engineers, Part M: Journal of Engineering for the Maritime Environment
sj-pdf-1-wmr-10.1177_0734242X221105436 – Supplemental material for A simple and reliable method for separation of mineral oil/polychlorobiphenyl mixtures
Creators: name: Gherdaoui, Chems Eddine
name: Bouberka, Zohra
name: Delbarre, Jean-Philippe
name: Hutin, Olivier
name: Sansano, Roger
name: Leclercq, Laurent
name: Supiot, Philippe
name: Maschke, Ulrich
Publisher: name: SAGE Journals
Year: 2022
Subjects: subject: 111799 Public Health and Health Services not elsewhere classified
subject: FOS: Health sciences
subject: 99999 Engineering not elsewhere classified
subject: FOS: Other engineering and technologies

description: Supplemental material, sj-pdf-1-wmr-10.1177_0734242X221105436 for A simple and reliable method for separation of mineral oil/polychlorobiphenyl mixtures by Chems Eddine Gherdaoui, Zohra Bouberka, Jean-Philippe Delbarre, Olivier Hutin, Roger Sansano, Laurent Leclercq, Philippe Supiot and Ulrich Maschke in Waste Management & Research
In-operando test of tunable Heusler alloys for thermomagnetic harvesting of low-grade waste heat
Creators: name: Cugini, F.
name: Gallo, L.
name: Garulli, G.
name: Olivieri, D.
name: Trevisi, G.
name: Fabbrici, S.
name: Albertini, F.
name: Solzi, M.
Publisher: name: arXiv
Year: 2025
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Thermomagnetic generation stands out as a promising technology for harvesting and converting low-grade waste heat below 100 °C. Despite the exponential growth in research on thermomagnetic materials and prototypes over the last decade, there remains, to unlock the full potential of this technology, a critical gap between fundamental research on materials and the design of advanced devices. In this study, we present the in-operando assessment of thermomagnetic performance of three representative Ni,Mn-based Heusler alloys optimized for harvesting low-grade waste heat below 373 K. These materials were tested under operational conditions using a specially designed laboratory-scale prototype of a thermomagnetic motor. The mechanical power output of the motor, operated with NiMnIn, NiMnSn and NiMnCuGa alloys, was correlated with the magnetic properties of the materials, highlighting the critical role of the magnetic transition temperature and saturation magnetization in determining the efficiency of thermomagnetic energy conversion. Austenitic Heusler alloys were confirmed to be promising thermomagnetic materials due to their highly tunable Curie temperature and significant magnetization changes in the 300-360 K temperature range. Among the tested materials, the Ni48Mn36In16 alloy demonstrated the highest thermomagnetic performance, surpassing the benchmark material Gd in the 320-340 K range. From an experimental perspective, the developed prototype of thermomagnetic motor serves as a flexible test-bench for evaluating and comparing the thermomagnetic performance of small amounts (less than 0.3 g) of new materials under variable conditions. Additionally, its modular design facilitates testing and optimization of its various components, thereby contributing to the advancement of thermomagnetic motor technology.
sj-docx-1-ggm-10.1177_23337214221115235 – Supplemental material for Effectiveness of Information Sessions About COVID-19 Vaccines in Healthcare Professionals Working in Geriatrics
Creators: name: Girard, Hélène
name: Bosshard, Wanda
name: Krief, Hélène
name: Büla, Christophe J.
Publisher: name: SAGE Journals
Year: 2022
Subjects: subject: 110308 Geriatrics and Gerontology
subject: FOS: Clinical medicine

description: Supplemental material, sj-docx-1-ggm-10.1177_23337214221115235 for Effectiveness of Information Sessions About COVID-19 Vaccines in Healthcare Professionals Working in Geriatrics by Hélène Girard, Wanda Bosshard, Hélène Krief and Christophe J. Büla in Gerontology and Geriatric Medicine
Matthias Kossler, Substantielles Wissen und subjektives Handeln: dargstellt in einem Vergleich von Hegel und Schopenhauer
Creators: name: Schöndorf, Harald
Publisher: name: Theologie und Philosophie
Year: 1970

description: Theologie und Philosophie, Bd. 69 Nr. 1 (1994): Theologie und Philosophie, Band 69, Heft 1
Light-induced reorientation transition in an antiferromagnetic semiconductor
Creators: name: Fichera, Bryan T.
name: Lv, Baiqing
name: Morey, Karna
name: Shen, Zongqi
name: Lee, Changmin
name: Donoway, Elizabeth
name: Liebman-Pelaez, Alex
name: Kogar, Anshul
name: Kurumaji, Takashi
name: Rodriguez-Vega, Martin
name: del Toro, Rodrigo Humberto Aguilera
name: Arruabarrena, Mikel
name: Ilyas, Batyr
name: Luo, Tianchuang
name: Muller, Peter
name: Leonardo, Aritz
name: Ayuela, Andres
name: Fiete, Gregory A.
name: Checkelsky, Joseph G.
name: Orenstein, Joseph
name: Gedik, Nuh
Publisher: name: arXiv
Year: 2025
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Due to the lack of a net magnetic moment, antiferromagnets possess a unique robustness to external magnetic fields and are thus predicted to play an important role in future magnetic technologies. However, this robustness also makes them quite difficult to control, and the development of novel methods to manipulate these systems with external stimuli is a fundamental goal of antiferromagnetic spintronics. In this work, we report evidence for a metastable reorientation of the order parameter in an antiferromagnetic semiconductor triggered by an ultrafast quench of the equilibrium order via photoexcitation above the band gap. The metastable state forms less than 10 ps after the excitation pulse, and persists for longer than 150 ps before decaying to the ground state via thermal fluctuations. Importantly, this transition cannot be induced thermodynamically, and requires the system to be driven out of equilibrium. Broadly speaking, this phenomenology is ultimately the result of large magnetoelastic coupling in combination with a relatively low symmetry of the magnetic ground state. Since neither of these properties are particularly uncommon in magnetic materials, the observations presented here imply a generic path toward novel device technology enabled by ultrafast dynamics in antiferromagnets.
description: 41 pages, 27 figures
Toylabs D7.2 - Data Management Handling Plan
Creators: name: ToyLabs Consortium
Publisher: name: Zenodo
Year: 2017

description: The TOYLABS Deliverable D7.2 (“Data Management Handling Plan”) presents the first version of the (open) data management plan (DMP) for the TOYLABS project as anticipated on Month 6 of the project. Such a data management plan investigates the appropriate methodologies, processes and open repositories for data management and dissemination to be adopted in the TOYLABS project.

The guiding principle of the TOYLABS project is openness as it aims at offering as much information as possible in a ‘FAIR’ manner (so as it is findable, accessible, interoperable and re-usable). Such information includes: the scientific publications prepared by the project consortium, the white papers published, the open source code generated, the public deliverables, the mock-up datasets used for supporting the development process etc. The list of research data expected to be released during the project consists of open methodologies (under creative commons licences), open source software components, and anonymous user statistics (from pilot operation). Such datasets are expected to be collected during the implementation and evaluation phases of the TOYLABS project and are therefore subject to change.

The publishing platforms, that can be accessed openly and are adopted by the TOYLABS project, are: the project website, Zenodo for long-term archiving (as proposed by EC), ResearchGate (for archiving and preservation of publications) and GitHub for open source code.

This deliverable is released as a living document that is expected to be updated whenever it is needed and to be respected by all partners.