cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
57488: Thiepval Memorial
Creators: name: Project Team, First World War Poetry Digital Archive
Publisher: name: University of Oxford
Year: 2024
Subjects: classificationCode: 430304
subject: British history
classificationCode: 430308
subject: European history (excl. British, classical Greek and Roman)
classificationCode: 430316
subject: International history

description: The Thiepval Memorial commemorates almost 73,000 soldiers who died on the Somme battlefields between July 1915 and 20th March 1918 who have no known grave.
A tentative 114-minute orbital period challenges the ultra-compact nature of the X-ray binary 4U 1812-12
Creators: name: Padilla, M. Armas
name: Rodríguez-Gil, P.
name: Muñoz-Darias, T.
name: Torres, M. A. P.
name: Casares, J.
name: Degenaar, N.
name: Dhillon, V. S.
name: Heinke, C. O.
name: Littlefair, S. P.
name: Marsh, T. R.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present a detailed time-resolved photometric study of the ultra-compact X-ray binary candidate 4U 1812-12. The multicolor light curves obtained with HiPERCAM on the 10.4-m Gran Telescopio Canarias show an aprox 114 min modulation similar to a superhump. Under this interpretation, this period should lie very close to the orbital period of the system. Contrary to what its other observational properties suggest (namely, persistent dim luminosity, low optical-to-X-ray flux ratio and lack of hydrogen features in the optical spectrum), this implies that 4U1812-12 is most likely not an ultra-compact X-ray binary, which are usually defined as systems with orbital periods lower than 80 min. We discuss the nature of the system, showing that a scenario in which 4U 1812-12 is the progenitor of an ultra-compact X-ray binary may reconcile all the observables.
description: Accepted for publication in ApJ Letters
Speed of sound in QCD matter
Creators: name: He, Wei-bo
name: Shao, Guo-yun
name: Gao, Xue-yan
name: Yang, Xin-ran
name: Xie, Chong-long
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We systematically investigate the speed of sound in QCD matter under different conditions in the grand canonical ensemble within the Polyakov loop improved Nambu--Jona-Lasinio (PNJL) model. The numerical results indicate that the dependence of speed of sound on parameters like temperature and chemical potential can be indicative of QCD phase transition. Some new features of speed of sound are discovered, for instance, the hierarchy of sound velocity for $u(d)$ and $s$ quark at low temperature with the increasing chemical potential and the squared sound velocity approaching to almost zero in the critical region. We also formulate the relations between differently defined sound velocity using the fundamental thermodynamic relations. Some conclusions derived are useful for hydrodynamics simulation and calculation of transport coefficient of bulk viscosity.
description: 8 pages, 9 figures
Temperature-induced dephasing in high-order harmonic generation from solids
Creators: name: Du, Tao-Yuan
name: Ma, Chao
Publisher: name: arXiv
Year: 2022
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: High harmonic generation (HHG) in solid and gaseous targets has been proven to be a powerful avenue for the generation of attosecond pulses, whereas the influence of electron-phonon scattering on HHG is a critical outstanding problem. Here we first introduce a temperature dependent lattice vibration model by characterizing the spacing fluctuation. Our results reveal that (i) structural disorder induced by lattice vibration does not lead to generation of even-order harmonics; (ii) dephasing of HHG occurs as the lattice temperature is growing; (iii) an open-trajectory picture predicts the maximal photon energy in the temperature-dependent HHG spectra. Moreover, a formula assessing dephasing time with lattice temperature is proposed to identify the timescale of electron-phonon scattering. This work paves a way to study non-Born-Oppenheimer effect in solids driven by strong field.
Additional file 1 of To eat or not to eat oats: factors associated with oats consumption using the I-Change model
Creators: name: Van Kol, S.
name: van der Horst, H.C.
name: de Vries, H.
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Environmental Sciences not elsewhere classified
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy

description: Supplementary Material 1
On the stellar core physics of the 16 Cyg binary system: constraining the central hydrogen abundance using asteroseismology
Creators: name: Nsamba, Benard
name: Cunha, Margarida S.
name: Rocha, Catarina I. S. A.
name: Pereira, Cristiano J. G. N.
name: Monteiro, Mário J. P. F. G.
name: Campante, Tiago L.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The unprecedented quality of the asteroseismic data of solar-type stars made available by space missions such as NASA's Kepler telescope are making it possible to explore stellar interior structures. This offers possibilities of constraining stellar core properties (such as core sizes, abundances, and physics) paving the way for improving the precision of the inferred stellar ages. We employ 16 Cyg A and B as our benchmark stars for an asteroseismic study in which we present a novel approach aimed at selecting from a sample of acceptable stellar models returned from Forward Modelling techniques, down to the ones that better represent the core of each star. This is accomplished by comparing specific properties of the observed frequency ratios for each star to the ones derived from the acceptable stellar models. We demonstrate that in this way we are able to constrain further the hydrogen mass fraction in the core, establishing the stars' precise evolutionary states and ages. The ranges of the derived core hydrogen mass fractions are [0.01 - 0.06] and [0.12 - 0.19] for 16 Cyg A and B, respectively, and, considering that the stars are coeval, the age and metal mass fraction parameters span the region [6.4 - 7.4] Gyr and [0.023 - 0.026], respectively. In addition, our findings show that using a single helium-to-heavy element enrichment ratio, ($ΔY/ΔZ$), when forward modelling the 16 Cyg binary system, may result in a sample of acceptable models that do not simultaneously fit the observed frequency ratios, further highlighting that such an approach to the definition of the helium content of the star may not be adequate in studies of individual stars.
description: 13 pages, 8 figures, and 5 tables. Accepted for publication in MNRAS
pyspeckit: A spectroscopic analysis and plotting package
Creators: name: Ginsburg, Adam
name: Sokolov, Vlas
name: de Val-Borro, Miguel
name: Rosolowsky, Erik
name: Pineda, Jaime E.
name: Sipőcz, Brigitta M.
name: Henshaw, Jonathan D.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: pyspeckit is a toolkit and library for spectroscopic analysis in Python. We describe the pyspeckit package and highlight some of its capabilities, such as interactively fitting a model to data, akin to the historically widely-used splot function in IRAF. pyspeckit employs the Levenberg-Marquardt optimization method via the mpfit and lmfit implementations, and important assumptions regarding error estimation are described here. Wrappers to use pymc and emcee as optimizers are provided. A parallelized wrapper to fit lines in spectral cubes is included. As part of the astropy affiliated package ecosystem, pyspeckit is open source and open development and welcomes input and collaboration from the community.
description: Version 1.0 of pyspeckit is released alongside this paper; https://pyspeckit.readthedocs.io/en/latest/
Additional file 1 of Comparison of the ScreenFire and Xpert HPV assays for the detection of human papillomavirus and cervical precancer among women living with HIV in Malawi
Creators: name: Mungo, Chemtai
name: Guliam, Anagha
name: Chinula, Lameck
name: Inturrisi, Federica
name: Msowoya, Lizzie
name: Mkochi, Tawonga
name: Jawadu, Siniya
name: de Sanjosé, Silvia
name: Schiffman, Mark
name: Tang, Jennifer H.
name: Smith, Jennifer S.
Publisher: name: figshare
Year: 2024
Subjects: subject: Biotechnology
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology

description: Additional file 1.
sj-docx-9-mso-10.1177_20552173221103436 - Supplemental material for Continuous monitoring with wearables in multiple sclerosis reveals an association of cardiac autonomic dysfunction with disease severity
Creators: name: Hilty, Marc
name: Oldrati, Pietro
name: Barrios, Liliana
name: Müller, Tamara
name: Blumer, Claudia
name: Foege, Magdalena
name: consortium, PHRT
name: Holz, Christian
name: Lutterotti, Andreas
Publisher: name: SAGE Journals
Year: 2022
Subjects: subject: 110904 Neurology and Neuromuscular Diseases
subject: FOS: Clinical medicine
subject: Neuroscience

description: Supplemental material, sj-docx-9-mso-10.1177_20552173221103436 for Continuous monitoring with wearables in multiple sclerosis reveals an association of cardiac autonomic dysfunction with disease severity by Marc Hilty, Pietro Oldrati, Liliana Barrios, Tamara Müller, Claudia Blumer, Magdalena Foege, PHRT consortium, Christian Holz and Andreas Lutterotti in Multiple Sclerosis Journal – Experimental, Translational and Clinical
A Meta-Analysis of the Utility of Explainable Artificial Intelligence in Human-AI Decision-Making
Creators: name: Schemmer, Max
name: Hemmer, Patrick
name: Nitsche, Maximilian
name: Kühl, Niklas
name: Vössing, Michael
Publisher: name: arXiv
Year: 2022
Subjects: subject: Human-Computer Interaction (cs.HC)
subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences

description: Research in artificial intelligence (AI)-assisted decision-making is experiencing tremendous growth with a constantly rising number of studies evaluating the effect of AI with and without techniques from the field of explainable AI (XAI) on human decision-making performance. However, as tasks and experimental setups vary due to different objectives, some studies report improved user decision-making performance through XAI, while others report only negligible effects. Therefore, in this article, we present an initial synthesis of existing research on XAI studies using a statistical meta-analysis to derive implications across existing research. We observe a statistically positive impact of XAI on users' performance. Additionally, the first results indicate that human-AI decision-making tends to yield better task performance on text data. However, we find no effect of explanations on users' performance compared to sole AI predictions. Our initial synthesis gives rise to future research investigating the underlying causes and contributes to further developing algorithms that effectively benefit human decision-makers by providing meaningful explanations.
description: AAAI/ACM Conference on AI, Ethics, and Society (AIES'22)
55612: Destroyed German fortification by Riqueval Farm Bridge
Creators: name: Project Team, First World War Poetry Digital Archive
Publisher: name: University of Oxford
Year: 2024
Subjects: classificationCode: 430304
subject: British history
classificationCode: 430308
subject: European history (excl. British, classical Greek and Roman)
classificationCode: 430316
subject: International history

description: Exterior.
sj-docx-1-qix-10.1177_10778004221097060 – Supplemental material for Design Anthropological Filmmaking for Automated Futures
Creators: name: Pink, Sarah
Publisher: name: SAGE Journals
Year: 2022
Subjects: subject: 160807 Sociological Methodology and Research Methods
subject: FOS: Sociology

description: Supplemental material, sj-docx-1-qix-10.1177_10778004221097060 for Design Anthropological Filmmaking for Automated Futures by Sarah Pink in Qualitative Inquiry
Lensing cosmic drift
Creators: name: Covone, Giovanni
name: Sereno, Mauro
Publisher: name: arXiv
Year: 2022
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: As the Universe expands, the redshift of distant sources changes with time. Here we discuss gravitational lensing phenomena that are consequence of the redshift drift between lensed source, gravitational lens, and observer. When the source is located very close to the drifting caustics, a pair of images could occur (or disappear) because of the cosmological expansion. Furthermore, lensing systems act as signal converters of the redshift drift. The angular position, magnification, distortion, and time delay of already existing multiple images change. We estimate the expected frequency of these phenomena and the prospects to observe them in the era of deep and large surveys. The drift detection in image separation could be within reach of next generation surveys with $μ$arcsec angular resolution.
description: 6 pages, 2 figures. In press (MNRAS)
SeGraM: A Universal Hardware Accelerator for Genomic Sequence-to-Graph and Sequence-to-Sequence Mapping
Creators: name: Cali, Damla Senol
name: Kanellopoulos, Konstantinos
name: Lindegger, Joel
name: Bingöl, Zülal
name: Kalsi, Gurpreet S.
name: Zuo, Ziyi
name: Firtina, Can
name: Cavlak, Meryem Banu
name: Kim, Jeremie
name: Ghiasi, Nika Mansouri
name: Singh, Gagandeep
name: Gómez-Luna, Juan
name: Alserr, Nour Almadhoun
name: Alser, Mohammed
name: Subramoney, Sreenivas
name: Alkan, Can
name: Ghose, Saugata
name: Mutlu, Onur
Publisher: name: arXiv
Year: 2022
Subjects: subject: Hardware Architecture (cs.AR)
subject: Genomics (q-bio.GN)
subject: FOS: Computer and information sciences
subject: FOS: Biological sciences

description: A critical step of genome sequence analysis is the mapping of sequenced DNA fragments (i.e., reads) collected from an individual to a known linear reference genome sequence (i.e., sequence-to-sequence mapping). Recent works replace the linear reference sequence with a graph-based representation of the reference genome, which captures the genetic variations and diversity across many individuals in a population. Mapping reads to the graph-based reference genome (i.e., sequence-to-graph mapping) results in notable quality improvements in genome analysis. Unfortunately, while sequence-to-sequence mapping is well studied with many available tools and accelerators, sequence-to-graph mapping is a more difficult computational problem, with a much smaller number of practical software tools currently available. We analyze two state-of-the-art sequence-to-graph mapping tools and reveal four key issues. We find that there is a pressing need to have a specialized, high-performance, scalable, and low-cost algorithm/hardware co-design that alleviates bottlenecks in both the seeding and alignment steps of sequence-to-graph mapping. To this end, we propose SeGraM, a universal algorithm/hardware co-designed genomic mapping accelerator that can effectively and efficiently support both sequence-to-graph mapping and sequence-to-sequence mapping, for both short and long reads. To our knowledge, SeGraM is the first algorithm/hardware co-design for accelerating sequence-to-graph mapping. SeGraM consists of two main components: (1) MinSeed, the first minimizer-based seeding accelerator; and (2) BitAlign, the first bitvector-based sequence-to-graph alignment accelerator. We demonstrate that SeGraM provides significant improvements for multiple steps of the sequence-to-graph and sequence-to-sequence mapping pipelines.
description: To appear in ISCA'22
sj-docx-3-qix-10.1177_10778004221097060 – Supplemental material for Design Anthropological Filmmaking for Automated Futures
Creators: name: Pink, Sarah
Publisher: name: SAGE Journals
Year: 2022
Subjects: subject: 160807 Sociological Methodology and Research Methods
subject: FOS: Sociology

description: Supplemental material, sj-docx-3-qix-10.1177_10778004221097060 for Design Anthropological Filmmaking for Automated Futures by Sarah Pink in Qualitative Inquiry
Anti-glitches in accreting pulsars from superfluid vortex avalanches
Creators: name: Howitt, G.
name: Melatos, A.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Three sudden spin-down events, termed `anti-glitches', were recently discovered in the accreting pulsar NGC 300 ULX-1 by the \textit{Neutron Star Interior Composition Explorer} (NICER) mission. Unlike previous anti-glitches detected in decelerating magnetars, these are the first anti-glitches recorded in an accelerating pulsar. One standard theory is that pulsar spin-up glitches are caused by avalanches of collectively unpinning vortices that transfer angular momentum from the superfluid interior to the crust of a neutron star. Here we test whether vortex avalanches are also consistent with the anti-glitches in NGC 300 ULX-1, with the angular momentum transfer reversed. We perform $N$-body simulations of up to $5 \times 10^{3}$ pinned vortices in two dimensions in secularly accelerating and decelerating containers. Vortex avalanches routinely occur in both scenarios, propagating inwards and outwards respectively. The implications for observables, such as size and waiting time statistics, are considered briefly.
description: MNRAS accepted, 13 pages, 10 figures
Additional file 1 of Impact of access to coronary angiography and percutaneous coronary intervention on in-hospital and five-year mortality in patients with acute coronary syndrome: a propensity-matched cohort study in Thailand
Creators: name: Kumwichar, Ponlagrit
name: Thungthong, Jutatip
name: Liabsuetrakul, Tippawan
name: Tachimori, Hisateru
name: Hosozawa, Mariko
name: Saito, Eiko
name: Taniguchi, Yuta
name: Chongsuvivatwong, Virasakdi
name: Iso, Hiroyasu
Publisher: name: figshare
Year: 2024
Subjects: Medicine
Biological Sciences not elsewhere classified
Science Policy
Virology

description: Additional file 1.
On orthogonal bases in the Hilbert-Schmidt space of matrices
Creators: name: Siewert, Jens
Publisher: name: arXiv
Year: 2022
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Decomposition of (finite-dimensional) operators in terms of orthogonal bases of matrices has been a standard method in quantum physics for decades. In recent years, it has become increasingly popular because of various methodologies applied in quantum information, such as the graph state formalism and the theory of quantum error correcting codes, but also due to the intensified research on the Bloch representation of quantum states. In this contribution we collect various interesting facts and identities that hold for finite-dimensional orthogonal matrix bases.
description: 10 pages
Additional file 3 of Discovery of novel RNA viruses through analysis of fungi-associated next-generation sequencing data
Creators: name: Lu, Xiang
name: Dai, Ziyuan
name: Xue, Jiaxin
name: Li, Wang
name: Ni, Ping
name: Xu, Juan
name: Zhou, Chenglin
name: Zhang, Wen
Publisher: name: figshare
Year: 2024
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics

description: Supplementary Material 3.
Supplemental Material - Investigation of anticorrosion properties of epoxy GO nanocomposites spin coated Aluminum Alloy 7075
Creators: name: Gaur, Mulayam S
name: Raghav, Rajesh K
name: Sagar, Rohan
name: Tiwari, R.K.
Publisher: name: SAGE Journals
Year: 2022
Subjects: subject: 91299 Materials Engineering not elsewhere classified
subject: FOS: Materials engineering

description: Supplemental Material for Investigation of anticorrosion properties of epoxy GO nanocomposites spin coated Aluminum Alloy 7075 by Mulayam S Gaur, Rajesh K Raghav, Rohan Sagar and R.K. Tiwari in Polymers and Polymer Composites
Anisotropic-strain-enhanced hole mobility in GaN by lattice matching to ZnGeN$_2$ and MgSiN$_2$
Creators: name: Leveillee, Joshua
name: Ponce, Samuel
name: Adamski, Nicholas L.
name: Van de Walle, Chris G.
name: Giustino, Feliciano
Publisher: name: arXiv
Year: 2022
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The key obstacle toward realizing integrated gallium nitride (GaN) electronics is its low hole mobility. Here, we explore the possibility of improving the hole mobility of GaN via epitaxial matching to II-IV nitride materials that have recently become available, namely ZnGeN$_2$ and MgSiN$_2$. We perform state-of-the-art calculations of the hole mobility of GaN using the ab initio Boltzmann transport equation. We show that effective uniaxial compressive strain of GaN along the $[1\bar{1}00]$ by lattice matching to ZnGeN$_2$ and MgSiN$_2$ results in the inversion of the heavy hole band and split-off hole band, thereby lowering the effective hole mass in the compression direction. We find that lattice matching to ZnGeN$_2$ and MgSiN$_2$ induces an increase of the room-temperature hole mobility by 50% and 260% as compared to unstrained GaN, respectively. Examining the trends as a function of strain, we find that the variation in mobility is highly nonlinear; lattice matching to a hypothetical solid solution of Zn$_{0.75}$Ge$_{0.75}$Mg$_{0.25}$Si$_{0.25}$N$_2$ would already increase the hole mobility by 160%.
Gamma-ray observation towards the young massive star cluster NGC 6618 in the M17 region
Creators: name: Liu, Bing
name: Yang, Rui-zhi
name: Chen, Zhiwei
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Young massive clusters have been established as a new population of gamma-ray sources and potential cosmic ray (CR) accelerators. In this paper, we report the detection of gamma-ray emissions near the young star cluster NGC 6618, which is one of the youngest star clusters in our Galaxy. The detected gamma-ray emissions can be divided into two components. One component is point-like and reveals harder spectrum, while the other is extended and with softer spectrum. Such spectral features are significantly different from other young massive clusters and may be due to the propagation effects of CRs accelerated in NGC 6618.
description: 7 pages, 4 figures; accepted for publication in MNRAS
Additional file 3 of Advanced-stage breast cancer diagnosis and its determinants in Ethiopia: a systematic review and meta-analysis
Creators: name: Zewdie, Amare
name: Kassie, Tadele Derbew
name: Anagaw, Tadele Fentabel
name: Mazengia, Elyas Melaku
name: Gelaw, Sintayehu Shiferaw
name: Fenta, Eneyew Talie
name: Eshetu, Habitu Birhan
name: Kebede, Natnael
name: Bogale, Eyob Ketema
Publisher: name: figshare
Year: 2024
Subjects: Medicine
Biotechnology
Biological Sciences not elsewhere classified
Cancer
Science Policy

description: Supplementary Material 3
The Factory and the Beehive. IV. A Comprehensive Study of the Rotation X-ray Activity Relation in Praesepe and the Hyades
Creators: name: Núñez, Alejandro
name: Agüeros, Marcel A.
name: Covey, Kevin R.
name: Douglas, Stephanie T.
name: Drake, Jeremy J.
name: Rampalli, Rayna
name: Bowsher, Emily C.
name: Cargile, Phillip A.
name: Kraus, Adam L.
name: Law, Nicholas M.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: X-ray observations of low-mass stars in open clusters are critical to understanding the dependence of magnetic activity on stellar properties and their evolution. Praesepe and the Hyades, two of the nearest, most-studied open clusters, are among the best available laboratories for examining the dependence of magnetic activity on rotation for stars with masses lower than $\approx 1\ M_{\odot}$. We present an updated study of the rotation X-ray activity relation in the two clusters. We updated membership catalogs that combine pre-Gaia catalogs with new catalogs based on Gaia Data Release 2. The resulting catalogs are the most inclusive ones for both clusters: 1739 Praesepe and 1315 Hyades stars. We collected X-ray detections for cluster members, for which we analyzed, re-analyzed, or collated data from ROSAT, the Chandra X-ray Observatory, the Neil Gehrels Swift Observatory, and XMM-Newton. We have detections for 326 Praesepe and 462 Hyades members, of which 273 and 164, respectively, have rotation periods, an increase of 6$\times$ relative to what was previously available. We find that at $\approx$700 Myr, only M dwarfs remain saturated in X-rays, with only tentative evidence for supersaturation. We also find a tight relation between the Rossby number and fractional X-ray luminosity $L_\mathrm{X}/L_\mathrm{bol}$ in unsaturated single members, suggesting a power-law index between $-3.2$ and $-3.9$. Lastly, we find no difference in the coronal parameters between binary and single members. These results provide essential insight into the relative efficiency of magnetic heating of the stars' atmospheres, thereby informing the development of robust age-rotation-activity relations.
description: 37 pages, 14 figures and 2 figure sets. Accepted for publication in the AAS Journals
Effects of Intercropping of Marigold and Yardlong Bean on Population of Cowpea Aphid, Aphis Craccivora Koch
Creators: name: Nathapong Matintarangson
Publisher: name: กองบริหารการวิจัย
Year: 2018
Subjects: Intercropping
Marigold
Yardlong Bean
Cowpea Aphid

description: Science & Technology Asia, 23, 2, 12-18
sj-pdf-1-jva-10.1177_11297298221086173 – Supplemental material for Functioning tailor-made 3D-printed vascular graft for hemodialysis
Creators: name: Li, Ming-Chia
name: Chang, Pu-Yuan
name: Luo, Huai-Rou
name: Chang, Ling-Yuan
name: Lin, Chuan-Yi
name: Yang, Chih-Yu
name: Lee, Oscar Kuang-Sheng
name: Wu Lee, Yan-Hwa
name: Tarng, Der-Cherng
Publisher: name: SAGE Journals
Year: 2022
Subjects: Cardiology

description: Supplemental material, sj-pdf-1-jva-10.1177_11297298221086173 for Functioning tailor-made 3D-printed vascular graft for hemodialysis by Ming-Chia Li, Pu-Yuan Chang, Huai-Rou Luo, Ling-Yuan Chang, Chuan-Yi Lin, Chih-Yu Yang, Oscar Kuang-Sheng Lee, Yan-Hwa Wu Lee and Der-Cherng Tarng in The Journal of Vascular Access
Additional file 2 of Arachidonic acid impairs natural killer cell functions by disrupting signaling pathways driven by activating receptors and reactive oxygen species
Creators: name: Hammoud, Mohamad K.
name: Meena, Celina
name: Dietze, Raimund
name: Hoffmann, Nathalie
name: Szymanski, Witold
name: Finkernagel, Florian
name: Nist, Andrea
name: Stiewe, Thorsten
name: Graumann, Johannes
name: von Strandmann, Elke Pogge
name: Müller, Rolf
Publisher: name: figshare
Year: 2024
Subjects: subject: Biophysics
subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer

description: Supplementary Material 2
Additional file 2 of Identification and validation of stable reference genes for RT-qPCR analyses of Kobresia littledalei seedlings
Creators: name: Sun, Haoyang
name: Li, Chunping
name: Li, Siyu
name: Ma, Jiaxin
name: Li, Shuo
name: Li, Xin
name: Gao, Cai
name: Yang, Rongchen
name: Ma, Nan
name: Yang, Jing
name: Yang, Peizhi
name: He, Xueqing
name: Hu, Tianming
Publisher: name: figshare
Year: 2024
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Plant Biology

description: Supplementary Material 2.
Towards a Comprehensive Solution for a Vision-based Digitized Neurological Examination
Creators: name: Hoang, Trung-Hieu
name: Zehni, Mona
name: Xu, Huaijin
name: Heintz, George
name: Zallek, Christopher
name: Do, Minh N.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Machine Learning (cs.LG)
subject: Neurons and Cognition (q-bio.NC)
subject: FOS: Computer and information sciences
subject: FOS: Biological sciences

description: The ability to use digitally recorded and quantified neurological exam information is important to help healthcare systems deliver better care, in-person and via telehealth, as they compensate for a growing shortage of neurologists. Current neurological digital biomarker pipelines, however, are narrowed down to a specific neurological exam component or applied for assessing specific conditions. In this paper, we propose an accessible vision-based exam and documentation solution called Digitized Neurological Examination (DNE) to expand exam biomarker recording options and clinical applications using a smartphone/tablet. Through our DNE software, healthcare providers in clinical settings and people at home are enabled to video capture an examination while performing instructed neurological tests, including finger tapping, finger to finger, forearm roll, and stand-up and walk. Our modular design of the DNE software supports integrations of additional tests. The DNE extracts from the recorded examinations the 2D/3D human-body pose and quantifies kinematic and spatio-temporal features. The features are clinically relevant and allow clinicians to document and observe the quantified movements and the changes of these metrics over time. A web server and a user interface for recordings viewing and feature visualizations are available. DNE was evaluated on a collected dataset of 21 subjects containing normal and simulated-impaired movements. The overall accuracy of DNE is demonstrated by classifying the recorded movements using various machine learning models. Our tests show an accuracy beyond 90% for upper-limb tests and 80% for the stand-up and walk tests.
Search for the tensor glueball
Creators: name: Klempt, E.
name: Sarantsev, A. V.
name: Denisenko, I.
name: Nikonov, K. V.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The tensor glueball is searched for in BESIII data on radiative $J/ψ$ decays into $π^0π^0$ and $K_sK_s$. The $ππ$ invariant mass distribution exhibits an enhancement that can be described by a pole at $(2210\pm 60) -i(180\pm 60)$\,MeV. We speculate if the tensor glueball could be distributed among high-mass tensor mesons.
description: 8 pages, 3 figures, 2 Tables
title: "Ritratto di fanciullo su busto moderno", Arte romana, inv. LXXVIe (ITA/EN)
title: Scheda catalogo digitale Borghese
titleType: AlternativeTitle
Creators: name: Clementi, Jessica
name: Galleria Borghese
Publisher: name: Galleria Borghese
Year: 2024

description: Pubblicazione delle schede delle opere conservate nel museo ed estratte dal catalogo digitale di Galleria Borghese, nelle due versioni esistenti online, in italiano e inglese.

Collegamento al catalogo digitale:

ITA: https://www.collezionegalleriaborghese.it/

EN: https://www.collezionegalleriaborghese.it/en
Additional file 1 of Prevalence of depressive symptoms among children and adolescents in china: a systematic review and meta-analysis
Creators: name: Zhou, Jia
name: Liu, Yiang
name: Ma, Jingyao
name: Feng, Zizhao
name: Hu, Jie
name: Hu, Jia
name: Dong, Bin
Publisher: name: figshare
Year: 2024
Subjects: Biotechnology
Biological Sciences not elsewhere classified
Science Policy
Mental Health

description: Additional file 1.
Fertility Fortunes Exhibition Catalogue.pdf
Creators: name: Davis, Isabel
name: Burel, Anna
name: Gleizer, Anya
Publisher: name: figshare
Year: 2025
Subjects: classificationCode: 360602
subject: Fine arts
classificationCode: 441009
subject: Sociology of family and relationships
classificationCode: 441010
subject: Sociology of gender
classificationCode: 441011
subject: Sociology of health
classificationCode: 441014
subject: Sociology of religion

description: This exhibition catalogue accompanied the end of project gallery show for the (Mis)Conceptions project in January 2025. It offers a booklet version of the artist-designed cards which were co-produced through public engagement activities with diverse public festival goers and reproductive health professionals, throughout the time of the project. The catalogue was formatted by graphic designer Elisenda Losantos, using artwork by Anna Burel.
Structural and Natural Isotopic Abundance Analysis of Magnesium Gluconate Treated with Energy of Consciousness (The Trivedi Effect®)
Creators: name: Trivedi, Dahryn
Publisher: name: SMN - The ScienceMedia Network
Year: 2017
Subjects: Natural Sciences
Chemistry

description: The current research article was aimed to investigate the impact of The Trivedi Effect®- Energy of Consciousness Healing Treatment on the structural properties and isotopic abundance ratio (PM+1/PM and PM+2/PM) of magnesium gluconate using LC-MS and NMR spectroscopy. Magnesium gluconate was divided into two parts – one part was control, and another part was treated with The Trivedi Effect® remotely by eighteen renowned Biofield Energy Healers and defined as the Trivedi Effect® Treated sample. The liquid chromatogram of the control sample showed two peaks at Rt of 1.81 and 2.06 min, whereas the Trivedi Effect® Treated sample displayed these peaks at Rt of 1.79 and 2.03 min. The ESI-MS spectra of the control and the Trivedi Effect® Treated samples revealed the presence of the mass for magnesium gluconate ion in two forms at m/z 447 (adduct form with methanol) and 415 (protonated ion) in positive ionization mode. But, it showed the mass for the gluconate ion at m/z 195 in the negative ionization mode. The fragmentation pattern of magnesium gluconate in the treated sample was notably altered as compared to the control sample. The proton and carbon signals for CH, CH2 and CO groups in the proton and carbon NMR spectra were found almost similar for the control and the treated samples. The isotopic abundance ratio analysis revealed that the isotopic abundance ratio of PM+1/PM (2H/1H or 13C/12C or 17O/16O or 25Mg/24Mg) in two magnesium gluconate ion forms at m/z 447 and 415 in treated sample was significantly decreased by 59.82% and 55.44%, respectively compared with the control sample. The percentage change in the isotopic abundance ratio of PM+2/PM (18O/16O or 26Mg/24Mg) was remarkably decreased in the magnesium gluconate ion at m/z 447 in the treated sample by 78.26% compared with the control sample. Consequently, the isotopic abundance ratio of PM+1/PM (2H/1H or 13C/12C or 17O/16O) in gluconate ion in the treated sample was significantly increased by 37.35% with respect to the control sample. Thus, the Trivedi Effect® treated magnesium gluconate could be valuable for designing better pharmaceutical and/or nutraceutical formulations through its changed physicochemical and thermal properties, which might be providing better therapeutic response against various diseases such as diabetes mellitus, allergies, aging, inflammatory diseases, immunological disorders, and other chronic infections. The treated magnesium gluconate might be helpful to design the novel potent enzyme inhibitors by using its kinetic isotope effects.
Additional file 1 of Higher oxidative balance score was associated with decreased risk of erectile dysfunction: a population-based study
Creators: name: Xu, Zhixiao
name: Chu, Weiwei
name: Lei, Xiong
name: Chen, Chengshui
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Ecology
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy
subject: Computational Biology
subject: Cardiology

description: Supplementary Material 1
Dust coagulation during the early stages of star formation: molecular cloud collapse and first hydrostatic core evolution
Creators: name: Bate, Matthew R.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Planet formation in protoplanetary discs requires dust grains to coagulate from the sub-micron sizes that are found in the interstellar medium into much larger objects. For the first time, we study the growth of dust grains during the earliest phases of star formation using three-dimensional hydrodynamical simulations. We begin with a typical interstellar dust grain size distribution and study dust growth during the collapse of a molecular cloud core and the evolution of the first hydrostatic core, prior to the formation of the stellar core. We examine how the dust size distribution evolves both spatially and temporarily. We find that the envelope maintains its initial population of small dust grains with little growth during these phases, except that in the inner few hundreds of au the smallest grains are depleted. However, once the first hydrostatic core forms rapid dust growth to sizes in excess of $100~μ$m occurs within the core (before stellar core formation). Progressively larger grains are produced at smaller distances from the centre of the core. In rapidly-rotating molecular cloud cores, the `first hydrostatic core' that forms is better described as a pre-stellar disc that may be gravitationally unstable. In such cases, grain growth is more rapid in the spiral density waves leading to the larger grains being preferentially found in the spiral waves even though there is no migration of grains relative to the gas. Thus, the grain size distribution can vary substantially in the first core/pre-stellar disc even at these very early times.
description: Accepted for publication in MNRAS. 17 pages, 14 figures. 5 animations available at: http://www.astro.ex.ac.uk/people/mbate/Research/DustGrowth.html
On the origin of core radio emissions from black hole sources in the realm of relativistic shocked accretion flow
Creators: name: Das, Santabrata
name: Nandi, Anuj
name: Stalin, C. S.
name: Rakshit, Suvendu
name: Dihingia, Indu Kalpa
name: Singh, Swapnil
name: Aktar, Ramiz
name: Mitra, Samik
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We study the relativistic, inviscid, advective accretion flow around the black holes and investigate a key feature of the accretion flow, namely the shock waves. We observe that the shock-induced accretion solutions are prevalent and such solutions are commonly obtained for a wide range of the flow parameters, such as energy (${\cal E}$) and angular momentum ($λ$), around the black holes of spin value $0\le a_{\rm k} < 1$. When the shock is dissipative in nature, a part of the accretion energy is released through the upper and lower surfaces of the disc at the location of the shock transition. We find that the maximum accretion energies that can be extracted at the dissipative shock ($Δ{\cal E}^{\rm max}$) are $\sim 1\%$ and $\sim 4.4\%$ for Schwarzschild black holes ($a_{\rm k}\rightarrow 0$) and Kerr black holes ($a_{\rm k}\rightarrow 1$), respectively. Using $Δ{\cal E}^{\rm max}$, we compute the loss of kinetic power (equivalently shock luminosity, $L_{\rm shock}$) that is enabled to comply with the energy budget for generating jets/outflows from the jet base ($i.e.$, post-shock flow). We compare $L_{\rm shock}$ with the observed core radio luminosity ($L_R$) of black hole sources for a wide mass range spanning $10$ orders of magnitude with sub-Eddington accretion rate and perceive that the present formalism seems to be potentially viable to account $L_R$ of $16$ Galactic black hole X-ray binaries (BH-XRBs) and $2176$ active galactic nuclei (AGNs). We further aim to address the core radio luminosity of intermediate-mass black hole (IMBH) sources and indicate that the present model formalism perhaps adequate to explain core radio emission of IMBH sources in the sub-Eddington accretion limit.
description: 15 pages, 4 figures, and 3 tables; accepted for publication in MNRAS
Consciousness Energy Healing Treatment Based Herbomineral Formulation: A Safe and Effective Approach for Skin Health
Creators: name: Trivedi, Dahryn
Publisher: name: SMN - The ScienceMedia Network
Year: 2017
Subjects: Natural Sciences
Chemistry

description: Oxidative stress causes serious skin damage that is characterized by ageing, wrinkling, roughness, laxity and pigmentation. In the present work, the impact of Biofield Energy (The Trivedi Effect®-Consciousness Energy Healing) Treatment on the herbomineral test formulation and cell medium (DMEM) was evaluated for skin health parameters. The test formulation was consisted of minerals (zinc chloride, sodium selenate, and sodium molybdate), L-ascorbic acid, herbal (Centella asiatica) extract, and tetrahydrocurcumin (THC). The test formulation and DMEM media were divided into two parts. One part received the Biofield Energy Treatment by Jagdish Singh and was termed as the Biofield Treated (BT) sample, while other was denoted as the untreated (UT) samples. MTT assay showed that test formulation was found safe and nontoxic with greater than 75% cell viability against various tested concentrations. Cell proliferation data using BrdU method showed an improved cell proliferation by 149.13% and 118.80% at 8.75 µg/mL in the UT-DMEM + BT-Test formulation and BT-DMEM + UT-Test formulation groups, respectively compared with the untreated group. The collagen level was significantly increased by 28.14% and 44.45% at 1.25 and 0.625 µg/mL, respectively in the UT-DMEM + BT-Test formulation compared with the untreated group. The elastin level was increased by 10.38%, 14.66%, and 48.24% at 2.5, 1.25, and 0.625 µg/mL, respectively in the BT-DMEM + UT-Test formulation group, compared with the untreated group. Moreover, melanin synthesis was significantly inhibited by 5.93%, 1.43%, and 1.43% in the UT-DMEM + BT-Test formulation, BT-DMEM + UT-Test formulation, and BT-DMEM + BT-Test formulation groups, respectively at 0.0625 µg/mL compared with the untreated group. However, melanin synthesis was decreased by 11.71% and 15.75% at 0.125 µg/mL in the UT-DMEM + BT-Test formulation and BT-DMEM + UT-Test formulation groups, respectively. Anti-wrinkling effects exhibited improved cell viability by 17.19% and 28.68% at 2.5 µg/mL in the UT-DMEM + BT-Test formulation and BT-DMEM + BT-Test formulation groups, respectively in HFF-1 cells compared with the untreated group. Wound healing activity using scratch assay showed a significantly improved healing rate upto 5% in the HFF-1 and HaCaT cells lines in the Biofield Energy Healing based test formulation. Overall, the data suggests that The Trivedi Effect® treated test formulation and DMEM has the capacity to improve the skin health and suggests its use in psoriasis, seborrheic dermatitis, skin cancer, rashes from bacterial or fungal infections, and many more skin diseases.
Regarding Flows Under the Free Energy Principle: A Comment on "How Particular is the Physics of the Free Energy Principle?" by Aguilera, Millidge, Tschantz, and Buckley
Creators: name: Sakthivadivel, Dalton A R
Publisher: name: arXiv
Year: 2022
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Adaptation and Self-Organizing Systems (nlin.AO)
subject: History and Philosophy of Physics (physics.hist-ph)
subject: FOS: Physical sciences

description: In a recent technical critique of the free energy principle (FEP) due to Aguilera-Millidge-Tschantz-Buckley, it is argued that there are a number of instances where the FEP$\unicode{x2014}$as conventionally written, in terms of densities over states$\unicode{x2014}$is uninformative about the dynamics of many physical systems, and by extension, many 'things.' In this informal comment on their critique, I highlight two points of interest where their derivations are largely correct, but where their arguments are not fatal to the FEP. I go on to conjecture that a path-based formulation of the FEP has key features which restore its explanatory power in broad physical regimes. Correspondingly, this piece takes the position that the application of a state-based formulation of the FEP is inappropriate for certain simple systems, but, that the FEP can be expected to hold regardless.
description: Five pages. Invited comment
57491: Thiepval Memorial
Creators: name: Project Team, First World War Poetry Digital Archive
Publisher: name: University of Oxford
Year: 2024
Subjects: classificationCode: 430304
subject: British history
classificationCode: 430308
subject: European history (excl. British, classical Greek and Roman)
classificationCode: 430316
subject: International history

description: The Thiepval Memorial commemorates almost 73,000 soldiers who died on the Somme battlefields between July 1915 and 20th March 1918 who have no known grave.
Additional file 3 of Prevalence of depressive symptoms among children and adolescents in china: a systematic review and meta-analysis
Creators: name: Zhou, Jia
name: Liu, Yiang
name: Ma, Jingyao
name: Feng, Zizhao
name: Hu, Jie
name: Hu, Jia
name: Dong, Bin
Publisher: name: figshare
Year: 2024
Subjects: Biotechnology
Biological Sciences not elsewhere classified
Science Policy
Mental Health

description: Additional file 3.
The Great Planetary Heist: Theft and capture in star-forming regions
Creators: name: Daffern-Powell, Emma C.
name: Parker, Richard J.
name: Quanz, Sascha P.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Gravitational interactions in star-forming regions are capable of disrupting and destroying planetary systems, as well as creating new ones. In particular, a planet can be stolen, where it is directly exchanged between passing stars during an interaction; or captured, where a planet is first ejected from its birth system and is free-floating for a period of time, before being captured by a passing star. We perform sets of direct N-body simulations of young, substructured star-forming regions, and follow their evolution for 10 Myr in order to determine how many planets are stolen and captured, and their respective orbital properties. We show that in high density star-forming regions, stolen and captured planets have distinct properties. The semimajor axis distribution of captured planets is significantly skewed to wider orbits compared to the semimajor axis distribution of stolen planets and planets that are still orbiting their parent star (preserved planets). However, the eccentricity and inclination distributions of captured and stolen planets are similar, but in turn very different to the inclination and eccentricity distributions of preserved planets. In low-density star-forming regions these differences are not as distinct but could still, in principle, be used to determine whether observed exoplanets have likely formed in situ or have been stolen or captured. We find that the initial degree of spatial and kinematic substructure in a star-forming region is as important a factor as the stellar density in determining whether a planetary system will be altered, disrupted, captured or stolen.
description: 15 pages, 10 figures, 1 appendix, accepted for publication in MNRAS
Additional file 1 of The Hippo pathway terminal effector TAZ/WWTR1 mediates oxaliplatin sensitivity in p53 proficient colon cancer cells
Creators: name: Slaninová, Věra
name: Heron-Milhavet, Lisa
name: Robin, Mathilde
name: Jeanson, Laura
name: Aissanou, Adam
name: Kantar, Diala
name: Tosi, Diego
name: Bréhélin, Laurent
name: Gongora, Céline
name: Djiane, Alexandre
Publisher: name: figshare
Year: 2024
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Hematology
subject: Plant Biology
subject: Computational Biology

description: Supplementary Material 1.