cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Validation and Improvement of the Pan-STARRS Photometric Calibration with the Stellar Color Regression Method
Creators: name: Xiao, Kai
name: Yuan, Haibo
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: As one of the best ground-based photometric dataset, Pan-STARRS1 (PS1) has been widely used as the reference to calibrate other surveys. In this work, we present an independent validation and re-calibration of the PS1 photometry using spectroscopic data from the LAMOST DR7 and photometric data from the corrected Gaia EDR3 with the Stellar Color Regression (SCR) method. Using per band typically a total of 1.5 million LAMOST-PS1-Gaia stars as standards, we show that the PS1 photometric calibration precisions in the $grizy$ filters are around $4\sim 5$ mmag when averaged over $20'$ regions. However, significant large- and small-scale spatial variation of magnitude offset, up to over 1 per cent, probably caused by the calibration errors in the PS1, are found for all the $grizy$ filters. The calibration errors in different filters are un-correlated, and are slightly larger for the $g$ and $y$ filters. We also detect moderate magnitude-dependent errors (0.005, 0.005, 0.005, 0.004, 0.003 mag per magnitude in the 14 -- 17 magnitude range for the $grizy$ filters, respectively) in the PS1 photometry by comparing with the Gaia EDR3 and other catalogs. The errors are likely caused by the systematic uncertainties in the PSF magnitudes. We provide two-dimensional maps to correct for such magnitude offsets in the LAMOST footprint at different spatial resolutions from $20'$ to $160'$. The results demonstrate the power of the SCR method in improving the calibration precision of wide-field surveys when combined with the LAMOST spectroscopy and Gaia photometry.
description: 12 pages, 15 figures, AJ accepted, see main results in Figures 7 and 14
Three neutralizing mAbs induced by MPXV A29L protein recognizing different epitopes act synergistically against orthopoxvirus
Creators: name: Li, Mengjun
name: Ren, Zuning
name: Wang, Yuelin
name: Jiang, Yushan
name: Yang, Minghui
name: Li, Delin
name: Chen, Jiayin
name: Liang, Zuxin
name: Lin, Yuhao
name: Zeng, Zhujun
name: Xu, Rui
name: Wang, Yiting
name: Zhu, Li
name: Xiao, Weiwei
name: Wu, Qinghua
name: Zhang, Bao
name: Wan, Chengsong
name: Yang, Yang
name: Wu, Bo
name: Peng, Jie
name: Zhao, Wei
name: Shen, Chenguang
Publisher: name: Taylor & Francis
Year: 2023
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Physiology
subject: Biotechnology
subject: Evolutionary Biology
subject: Science Policy
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Hematology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Virology
subject: Computational Biology

description: The worldwide outbreak of the monkeypox virus (MPXV) has become a “Public Health Emergency of International Concern” (PHEIC). Severe monkeypox virus infection can be fatal, however, effective therapeutic methods are yet to be developed. Mice were immunized with A35R protein and A29L protein of MPXV, and the binding and neutralizing activities of the immune sera against poxvirus-associated antigens and viruses were identified. A29L protein and A35R protein-specific monoclonal antibodies (mAbs) were generated and their antiviral activities of these mAbs were characterized in vitro and in vivo. Immunization with the MPXV A29L protein and A35R protein induced neutralizing antibodies against the orthopoxvirus in mice. None of the mAbs screened in this study against A35R could effectively neutralize the vaccinia virus (VACV), while three mAbs against A29L protein, 9F8, 3A1 and 2D1 were confirmed to have strong broad binding and neutralizing activities against orthopoxvirus, among which 9F8 showed the best neutralizing activity. 9F8, 3A1, and 2D1 recognized different epitopes on MPXV A29L protein, showing synergistic antiviral activity in vitro against the VACV Tian Tan and WR strains; the best activity was observed when the three antibodies were combined. In the vivo antiviral prophylactic and therapeutic experiments, 9F8 showed complete protective activity, whereas 3A1 and 2D1 showed partial protective activity. Similarly, the three antibodies showed synergistic antiviral protective activity against the two VACVs. In conclusion, three mAbs recognized different epitopes on MPXV A29L protein were developed and showed synergistic effects against orthopoxvirus.
MyGene2 automated match report: MYH11
Creators: name: Team, The MyGene2
Publisher: name: figshare
Year: 2017
Subjects: subject: 110311 Medical Genetics (excl. Cancer Genetics)
subject: FOS: Basic medicine

description: MyGene2.org is free, public, searchable & browsable website. Families with rare genetic conditions, clinicians, and researchers families who are interested in sharing health and genetic information can create MyGene2 profiles and use these to connect with other families, clinicians, and researchers who may have or be studying the same condition. If multiple MyGene2 profiles potentially match on a shared gene of interest, MyGene2 automatically generates a match report summarizing the information in these profiles. This automated match report is shared publicly to help facilitate further research and/or connections between the submitters of the MyGene2 profiles and other interested parties. This is an automated match report for MYH11.
Public 360 4.1 SP8
Creators: Finansministeriets departement
Statens It
Publisher: name: Rigsarkivet
Year: 2025

description: Public 360 er et sags- og dokumenthåndteringssystem (ESDH-system), der har til formål at sikre en ensartet og systematisk dokumentation af sagsbehandlingen for at styrke samarbejde og videndeling.
Disk precession to explain the super-orbital modulation of LMC X-4: results from the Swift monitoring campaign
Creators: name: Ambrosi, Elena
name: d'Aì, Antonino
name: del Santo, Melania
name: Segreto, Alberto
name: Ferrigno, Carlo
name: Amato, Roberta
name: Cusumano, Giancarlo
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We studied the spectral changes of the high-mass X-ray binary system LMC X-4 to understand the origin and mechanisms beyond its super-orbital modulation (30.4 days). To this aim, we obtained a monitoring campaign with Swift/XRT (0.3-10 keV) and complemented these data with the years-long Swift/BAT survey data (15-60 keV). We found a self-consistent, physically motivated, description of the broadband X-ray spectrum using a Swift/XRT and a NuSTAR observation at the epoch of maximum flux. We decomposed the spectrum into the sum of a bulk+thermal Comptonization, a disk-reflection component and a soft contribution from a standard Shakura-Sunyaev accretion disk. We applied this model to 20 phase-selected Swift spectra along the super-orbital period. We found a phase-dependent flux ratio of the different components, whereas the absorption column does not significantly vary. The disk emission is decoupled with respect to the hard flux. We interpret this as a geometrical effect in which the inner parts of the disk are tilted with respect to the obscuring outer regions.
description: 14 pages, 15 figures, Accepted for publication in MNRAS
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 0902
Creators: name: de la Côte d'Or, Archives départementales
name: CG21/F.PETOT/2012
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 0902, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 0902, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Separation and Estimation of Periodic/Aperiodic State
Creators: name: Muramatsu, Hisayoshi
Publisher: name: arXiv
Year: 2022
Subjects: subject: Systems and Control (eess.SY)
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: Periodicity and aperiodicity can exist in a state simultaneously and typically become quasi-periodicity and quasi-aperiodicity in a dynamically changing state. The quasi-periodic and quasi-aperiodic states existing in the periodic/aperiodic state mostly correspond to different phenomena and require different controls. For separation control of these states, this paper defines the periodic/aperiodic, quasi-periodic, and quasi-aperiodic states to construct a periodic/aperiodic separation filter that separates the periodic/aperiodic state into the quasi-periodic and quasi-aperiodic states. Based on these definitions, the linearity of periodic-pass and aperiodic-pass functions and the orthogonality of quasi-periodic and quasi-aperiodic state functions are proved. Subsequently, the periodic/aperiodic separation filter composed of periodic-pass and aperiodic-pass filters that realize the periodic-pass and aperiodic-pass functions is designed and integrated with a Kalman filter for estimation of the quasi-periodic and quasi-aperiodic states.
Geochronology in the southern Midyan terrane: a review of constraints on the timing of magmatic pulses and tectonic evolution in a northwestern part of the Arabian Shield
Creators: name: Wiesław Kozdrój
name: Kennedy, Allen K.
name: Johnson, Peter R.
name: Małgorzata Ziółkowska-Kozdrój
name: Kadi, Khalid
Publisher: name: Taylor & Francis
Year: 2017
Subjects: subject: Medicine
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Developmental Biology
subject: Cancer

description: The southern Midyan terrane is a composite Tonian to Ediacaran tectonostratigraphic crustal block in the northern Arabian Shield that prior to Red Sea opening was contiguous with coeval rocks in the Eastern Desert of Egypt and Sinai. Ion microprobe (sensitive high-resolution ion microprobe [SHRIMP]) dating of 12 rock samples described here and the results of other dating programmes establish a clear timeframe for depositional, intrusive, and structural events in the region and provide a chronology of tectonism in this part of the Arabian-Nubian Shield. Deposition of Zaam and Bayda group volcanosedimentary rocks and emplacement of mafic-ultramafic complexes and TTG-type diorite, tonalite, and granodiorite denote formation of the Tonian (780–715 Ma) Zaam arc and fore-arc ophiolite above a possible west-dipping subduction system in the southern part of the Midyan terrane. Convergence with the Hijaz terrane farther south and obduction of ophiolite nappes resulted by ~700 Ma in development of the Yanbu suture. Ongoing or a new subduction system led to a ~705–660 Ma Cryogenian pulse of magmatism represented by I-type calc-alkaline diorite, granodiorite, and granite that have volcanic-arc and syn-collisional granite affinities. This was followed, after a brief end-Cryogenian hiatus, by a 635–~570 Ma period of Ediacaran magmatism marked by monzogranite, syenogranite, and minor gabbro and diorite. These rocks are reported to have within-plate to volcanic-arc and syncollision chemical characteristics but their precise tectonic setting is uncertain. Structurally, the intrusions are diapiric and were evidently emplaced in an extensional regime consistent with an overlap between intrusion and Najd faulting associated, at this time, with transpressional collision and northward extension through much of the ANS. Terminal magmatism in the southern Midyan terrane postdated cessation of Najd faulting at ~575 Ma and resulted in the emplacement of undeformed within-plate A-type alkali-feldspar granites and mafic (lamprophyre) and felsic dikes.
Reassessing the Evidence for Time Variability in the Atmosphere of the Exoplanet HAT-P-7 b
Creators: name: Lally, Maura
name: Vanderburg, Andrew
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We reassess the claimed detection of variability in the atmosphere of the hot Jupiter HAT-P-7 b, reported by Armstrong et al. (2016). Although astronomers expect hot Jupiters to have changing atmospheres, variability is challenging to detect. We looked for time variation in the phase curves of HAT-P-7 b in Kepler data using similar methods to Armstrong et al. (2016), and identified apparently significant variations similar to what they found. Numerous tests show the variations to be mostly robust to different analysis strategies. However, when we injected unchanging phase curve signals into the light curves of other stars and searched for variability, we often saw similar levels of variations as in the HAT-P-7 light curve. Fourier analysis of the HAT-P-7 light curve revealed background red noise from stellar supergranulation on timescales similar to the planet's orbital period. Tests of simulated light curves with the same level of noise as HAT-P-7's supergranulation show that this effect alone can cause the amplitude and phase offset variability we detect for HAT-P-7 b. Therefore, the apparent variations in HAT-P-7 b's atmosphere could instead be caused by non-planetary sources, most likely photometric variability due to supergranulation on the host star.
description: 27 pages, 18 figures, accepted for publication in the Astronomical Journal
Mass Transfer as an Explanation for the Lifetime-Travel Time Discrepancy in IT Librae
Creators: name: Wysocki, Peter
name: Gies, Douglas
name: Shepard, Katherine
name: Lester, Kathryn
name: Orosz, Jerome
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The eclipsing binary IT Librae is an unusual system of two B-type stars that is situated about 1 kpc above the galactic plane. The binary was probably ejected from its birthplace in the disk, but the implied time-of-flight to its current location exceeds the evolutionary lifetime of the primary star. Here we present a study of new high dispersion spectroscopy and an exquisite light curve from the Kepler K2 mission in order to determine the system properties and resolve the timescale discrepancy. We derive a revised spectroscopic orbit from radial velocity measurements and determine the component effective temperatures through comparison of reconstructed and model spectra ($T_1 = 23.8 \pm 1.8$ kK, $T_2 = 13.7 \pm 2.5$ kK). We use the Eclipsing Light Curve (ELC) code to model the K2 light curve, and from the inclination of the fit, we derive the component masses ($M_1 = 9.6 \pm 0.6 M_\odot$, $M_2 = 4.2 \pm 0.2 M_\odot$) and mean radii ($R_1 = 6.06 \pm 0.16 R_\odot$, $R_2 = 5.38 \pm 0.14 R_\odot$). The secondary star is overluminous for its mass and appears to fill its Roche lobe. This indicates that IT~Librae is a post-mass transfer system in which the current secondary was the mass donor star. The current primary star was rejuvenated by mass accretion, and its evolutionary age corresponds to the time since the mass transfer stage. Consequently, the true age of the binary is larger than the ejection time-of-flight, thus resolving the timescale discrepancy.
description: 21 pages, 12 figures
Pediatric cochlear implants and myringotomy tubes: a systematic review
Creators: name: Patel, Shubham
name: Robbins, Alexa
name: Tey, Ching Siong
name: Zhang, Chao
name: Peterson, Shenita
name: Govil, Nandini
Publisher: name: Taylor & Francis
Year: 2023
Subjects: subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Science Policy

description: To evaluate the intraoperative findings and post-operative complications associated with patients who have current or history of myringotomy tubes undergoing a cochlear implantation. Preferred Reporting Items for Systematic Reviews and Meta-Analyses (PRISMA) statement were followed. Studies from Pubmed, Cochrane, Embase, Web of Science, and Scopus were included. Studies were independently screened and analyzed by 2 reviewers. Publications assessing pediatric patients with current or history of myringotomy tubes at time of cochlear implantation were reviewed. Discrepancies were resolved by a team of 4 reviewers. 172 studies were screened, 15 met inclusion criteria, and 12 were incorporated into the study. All 12 of the studies were retrospective cohort studies. Meta-analysis showed no significant relationship between intraoperative findings at time of cochlear implantation (presence of effusion, granulation tissue, edematous middle ear tissue) and myringotomy tube insertion (p = 0.63). Additionally, there was no significant relationship between current or history of myringotomy tube and acute otitis media episode after CI (p = 0.25). There was no association noted between perioperative outcomes of pediatric cochlear implantation and myringotomy tube. This information will be helpful for surgeons planning to perform cochlear implantation in the pediatric population.
The cyclic behaviour in the N-S asymmetry of sunspots and solar plages for the period 1910 to 1937 using data from Ebro catalogues
Creators: name: de Paula, V.
name: Curto, J. J.
name: Oliver, R.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The heliophysics catalogues published by the Ebro Observatory during 1910--1937 have been converted into a digital format in order to provide the data for computational processing. This has allowed us to study in detail the North-South (N-S) asymmetry of solar activity in that period, focusing on two different structures located at two different layers of the solar atmosphere: sunspots (Photosphere) and solar plages (Chromosphere). The examination of the absolute and normalised N-S asymmetry indices in terms of their monthly sum of occurrences and areas has made possible to find out a cyclic behaviour in the solar activity, in which the preferred hemisphere changes systematically with a global period of 7.9 $\pm$ 0.2 yr. In order to verify and quantify accurately this periodicity and study its prevalence in time, we employed the RGO-USAF/NOAA sunspot data series during 1874--2016. Then, we examined each absolute asymmetry index time series through different techniques as the power spectrum analysis, the Complete Ensemble Empirical Mode Decomposition With Adaptive Noise algorithm, or the Morlet wavelet transform. The combined results reveal a cyclic behaviour at different time scales, consisting in two quite stable periodicities of 1.47 $\pm$ 0.02 yr and 3.83 $\pm$ 0.06 yr, which coexist with another three discontinuous components with more marked time-varying periods with means of 5.4 $\pm$ 0.2 yr, 9.0 $\pm$ 0.2 yr, and 12.7 $\pm$ 0.3 yr. Moreover, during 1910--1937, only two dominant signals with averaged periods of 4.10 $\pm$ 0.04 yr and 7.57 $\pm$ 0.03 yr can be clearly observed. Finally, in both signals, periods are slightly longer for plages in comparison with sunspots.
description: 18 pages, 8 figures, 14 tables
title: Mortality of Quebec chrysotile workers in relation to radiological findings while still employed
Creators: name: Liddell, FDK
Publisher: name: London School of Hygiene & Tropical Medicine
Year: 1978

description: Two cohorts of Quebec chrysotile miners and millers were selected in order to study how radiological changes in asbestos workers predict mortality. Cohort "A" comprised 988 men, with dust exposure, smoking history, respiratory symptoms and lung function recorded in 1967- 68, and six independent readings of an earlier chest radiograph; 130 men had died before 1976. Cohort "B" comprised all 4,559 men not in Cohort "A" who were born 1891 through 1920, with at least a month's employment and an x-ray; dust exposure, smoking history and a single x-ray reading were obtained. By the end of 1975, there had been 1,455 deaths in Cohort "B". A high Relative Risk (RR) of total mortality was related to each radiographic feature, cigarette smoking, excessive dust exposure, and, in Cohort "A", dyspnoea and poorer function. Death from pneumoaonioois was associated with small irregular parenchymal opacities, of profusion usually greater than 1/0, and with heavy dust exposure, but not with smoking. Almost all who died from chest cancer had smoked cigarettes (very high RR), have been heavily exposed to asbestos (high RR), or both. About half their x-rays showed pneumoconiotic change. There was insufficient evidence to determine whether chest cancer was a complication of asbestosis or an independent reaction to asbestos exposure. Five of the six mesothelioma cases had positive but varied radiographic appearances. The contribution of asbestos dust to some deaths attributed to heart disease was substantiated by high RRs for severe exposure, and for small parenchymal opac ities; smokers, and the breathless, also had high risks. Other neoplasms showed no consistent dust or x-ray patterns. RRs of deaths from some other causes were high for certain radiographic features. Not all these results can yet be explained. The main findings validated the UICC/Cincinnati classification convincingly. Studies to permit generalization are recommended.
Dissociative recombination and rotational transitions of D$_2^+$ in collisions with slow electrons
Creators: name: Epée, M. D. Epée
name: Motapon, O.
name: Pop, N.
name: Iacob, F.
name: Roueff, E.
name: Schneider, I. F.
name: Mezei, J. Zs
Publisher: name: arXiv
Year: 2022
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Rate coefficients for dissociative recombination and state-to-state rotational transitions of the D$_{2}^{+}$ ion induced by collisions with very low-energy electrons have been reported following our previous studies on HD$^{+}$ and H$_{2}^{+}$ [9,10]. The same molecular structure data sets, excitations ($N_{i}^{+} \rightarrow$ $N_{f}^{+}=N_{i}^{+}+2$ for $N_{i}^{+}=0$ to $10$) and de-excitations ($N_{i}^{+}$ $\rightarrow$ $N_{f}^{+}=N_{i}^{+}-2$, for $N_{i}^{+}=2$ to $10$) were used for collision energies ranging from $0.01$ meV to $0.3$ eV. Isotopic effects for dissociative recombination and rotational transitions of the vibrationally relaxed targets are presented.
description: 7 pages, 7 figures, 4 tables
Identification, mass and age of primary red clump stars from spectral features derived with the LAMOST DR7
Creators: name: He, Xu-Jiang
name: Luo, A-Li
name: Chen, Yu-Qin
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Although red clump (RC) stars are easy to identify due to their stability of luminosity and color, about 20-50% are actually red giant branch (RGB) stars in the same location on the HR diagram. In this paper, a sample of 210,504 spectra for 184 318 primary RC (PRC) stars from the LAMOST DR7 is identified, which has a purity of higher than 90 percent. The RC and the RGB stars are successfully distinguished through LAMOST spectra(R~1800 and SNR>10) by adopting the XGBoost ensemble learning algorithm, and the secondary RC stars are also removed. The SHapley Additive exPlanations (SHAP) value is used to explain the top features that the XGBoost model selected. The features are around Fe5270, MgH & MgIb, Fe4957, Fe4207, Cr5208, and CN, which can successfully distinguish RGB and RC stars. The XGBoost is also used to estimate the ages and masses of PRC stars by training their spectra with Kepler labeled asteroseismic parameters. The uncertainties of mass and age are 13 and 31 percent, respectively. Verifying the feature attribution model, we find the age-sensitive elements XGBoost gets are consistent with the literature. Distances of the PRC stars are derived by $K_{S}$ absolute magnitude calibrated by Gaia EDR3, which has an uncertainty of about 6 percent and shows the stars mainly locate at the Galactic disk. We also test the XGBoost with R$\sim$250, which is the resolution of the Chinese Space Station Telescope(CSST) under construction, it is still capable of finding sensitive features to distinguish RC and RGB.
description: 14 pages, 17 figures, accepted by MNRAS
title: ADCO, Cartulaire de l'abbaye de Saint-Seine (XIIIe siècle), Cart. 165 (10 H 6, ms. 139), 354 pages, f. 0162
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2009
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire de l'abbaye de Saint-Seine (XIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 165 (10 H 6, ms. 139), 354 pages, f. 0162, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de l'abbaye de Saint-Seine (XIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 165 (10 H 6, ms. 139), 354 pages, f. 0162, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Saint-Seine
description: Provenance: http://www.wikidata.org/entity/Q2820709
New approach for analysing dynamical processes on the surface of photospheric vortex tubes
Creators: name: Aljohani, Yasir
name: Fedun, Viktor
name: Ballai, Istvan
name: Silva, Suzana S. A.
name: Shelyag, Sergiy
name: Verth, Gary
Publisher: name: arXiv
Year: 2022
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: The majority of studies on multi-scale vortex motions employ a two-dimensional geometry by using a variety of observational and numerical data. This approach limits the understanding the nature of physical processes responsible for vortex dynamics. Here we develop a new methodology to extract essential information from the boundary surface of vortex tubes. 3D high-resolution magnetoconvection MURaM numerical data has been used to analyse photospheric intergranular velocity vortices. The Lagrangian Averaged Vorticity Deviation (LAVD) technique was applied to define the centers of vortex structures and their boundary surfaces based on the advection of fluid elements. These surfaces were mapped onto a constructed envelope grid that allows the study of the key plasma parameters as functions of space and time. Quantities that help in understanding the dynamics of the plasma, e.g. Lorentz force, pressure force, plasma-$β$ were also determined. Our results suggest that, while density and pressure have a rather global behaviour, the other physical quantities undergo local changes, with their magnitude and orientation changing in space and time. At the surface, the mixing in the horizontal direction is not efficient, leading to appearance of localized regions with higher/colder temperatures. In addition, the analysis of the MHD Poynting flux confirms that the majority of the energy is directed in the horizontal direction. Our findings also indicate that the pressure and magnetic forces that drive the dynamics of the plasma on vortex surfaces are unbalanced and therefore the vortices do not rotate as a rigid body.
Structural inheritance in the Central Pyrenees: the Variscan to Alpine tectonometamorphic evolution of the Axial Zone
Creators: name: Cochelin, Bryan
name: Lemirre, Baptiste
name: Denele, Yoann
name: Blanquat, Michel De Saint
name: Abdeltif Lahfid
name: Duchene, Stéphanie
Publisher: name: Geological Society of London
Year: 2017
Subjects: subject: Geology
subject: FOS: Earth and related environmental sciences

description: Raman spectroscopy of carbonaceous materials data and a figure illustrating peak-fitting of the Raman spectrum of carbonaceous material and Raman spectra from the various samples of the Pallaresa cross-section.
On the recurrence times of neutron star X-ray binary transients and the nature of the Galactic Centre quiescent X-ray binaries
Creators: name: Maccarone, Thomas J.
name: Degenaar, Nathalie
name: Tetarenko, Bailey E.
name: Heinke, Craig
name: Wijnands, Rudy
name: Sivakoff, Gregory R.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The presence of some X-ray sources in the Galactic Centre region which show variability, but do not show outbursts in over a decade of monitoring has been used to argue for the presence of a large population of stellar mass black holes in this region. A core element of the arguments that these objects are accreting black holes is the claim that neutron stars (NSs) in low mass X-ray binaries (LMXBs) do not have long transient recurrence times. We demonstrate in this paper that about half of the known transient LMXBs with clear signatures for NS primaries have recurrence times in excess of a decade for outbursts at the sensitivity of MAXI. We furthermore show that, in order to reconcile the expected total population of NS LMXBs with the observed one and with the millisecond radio pulsar (MSRP) population of the Galaxy, systems with recurrence times well in excess of a century for outbursts detectable by instruments like MAXI must be the dominant population of NS LMXBs, and that few of these systems have yet been discovered.
description: 7 pages, accepted to MNRAS, small correction made to abstract from originally posted version to remove an ambiguity
Transcriptome profiling of gene expression in phosphate-solubilizing bacterium Acinetobacter sp. strain m01 interacting with melon (Cucumis melo L.) seedling
Creators: name: Zhang, Jian
name: Wang, Pengcheng
name: Xiao, Qingqing
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: Biological Sciences not elsewhere classified
subject: Plant Biology
subject: Computational Biology

description: Phosphorus (P) is an important element for plant and bacteria growth. The response of bacteria to P transformation into adsorbed forms and their interaction with plants remain unclear. In this study, the mechanisms involved in P adsorption in plants and bacteria were analyzed by a RNA-seq technology. A phosphate-solubilizing bacterium (PSB) Acinetobacter sp. strain M01 was used in the transcriptome profiling of expressed genes and during interaction with melon (Cucumis melo L.). Results showed that the majority of genes related to cellular component and molecular function were up-regulated. The genes in the melon plant treated with M01 were down-regulated compared with those in the control. Genes for phenylalanine metabolism, amino acid, glycerolipid metabolism were identified in M01 DEGs related to transport and catabolism, carbohydrate metabolisms, and amino acid transport were marked in melon. This study provides an understanding of the gene interaction in PSB to fixed P and melon.
title: 19_F_VUILLERME-DUNAND_LaParisienne_FR_GAD
Creators: name: Vuillerme-Dunand, Victor-Napoléon
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2024
Subjects: subject: PuppetPlays
subject: Horizon 2020
subject: Plassard, Didier
subject: Guignol (personnage fictif)
subject: PuppetPlays
subject: Horizon 2020
subject: Plassard, Didier
subject: Guignol (personnage fictif)

description: Digitized by the ERC project PuppetPlays, receiving funding from the European Union's Horizon 2020 research and innovation programme under Grant Agreement ERC 835193.
description: MAM - Musée des Arts de la Marionnette (Musée Gadagne). B29 paquet 6/pochette 78.
Numérisé dans le cadre du projet ERC PuppetPlays, financé par le Programme de recherche et d'innovation Horizon 2020 de l'Union européenne (Grant Agreement 835193).
Configuration of magnetotail current sheet prior to magnetic reconnection onset
Creators: name: An, Xin
name: Artemyev, Anton
name: Angelopoulos, Vassilis
name: Runov, Andrei
name: Lu, San
name: Pritchett, Philip
Publisher: name: arXiv
Year: 2022
Subjects: subject: Space Physics (physics.space-ph)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: The magnetotail current sheet configuration determines magnetic reconnection properties that control the substorm onset, one of the most energetic phenomena in the Earth's magnetosphere. The quiet-time current sheet is often approximated as a two-dimensional (2D) magnetic field configuration balanced by isotropic plasma pressure gradients. However, reconnection onset is preceded by the current sheet thinning and the formation of a nearly one-dimensional (1D) magnetic field configuration. In this study, using particle-in-cell simulations, we investigate the force balance of such thin current sheets when they are driven by plasma inflow. We demonstrate that the magnetic field configuration transitions from 2D to 1D thanks to the formation of plasma pressure nongyrotropy and reveal its origin in the nongyrotropic terms of the ion distributions. We show that substorm onset may be controlled by the instability and dynamics of such nongyrotropic current sheets, having properties much different from the most commonly investigated 2D isotropic configuration.
description: 16 pages, 4 figures
Performance evaluation of baseline-dependent averaging based onfull-scale SKA1-LOW simulation
Creators: name: Deng, Qing-Wen
name: Wang, Feng
name: Deng, Hui
name: Mei, Ying
name: Li, Jing
name: Smirnov, Oleg
name: Guo, Shao-Guang
Publisher: name: arXiv
Year: 2022
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: The Square Kilometre Array (SKA) is the largest radio interferometer under construction in the world. Its immense amount of visibility data poses a considerable challenge to the subsequent processing by the science data processor (SDP). Baseline dependent averaging (BDA), which reduces the amount of visibility data based on the baseline distribution of the radio interferometer, has become a focus of SKA SDP development. This paper developed and implemented a full-featured BDA module based on Radio Astronomy Simulation, Calibration and Imaging Library (RASCIL). Simulated observations were then performed with RASCIL based on a full-scale SKA1-LOW configuration. The performance of the BDA was systematically investigated and evaluated based on the simulated data. The experimental results presented that the amount of visibility data is reduced by about 50\% to 85\% for different time intervals ($Δt_{max}$). In addition, different $Δt_{max}$ have a significant effect on the imaging quality. The smaller the $Δt_{max}$, the smaller the degradation of the imaging quality.
description: 11 pages, 10 figures, accepted by RAA
Моделирование физических процессов при выполнении лабораторных работ в курсе общей физики в техническом вузе
Creators: name: Кирк Яна Геннадьевна
Publisher: name: История и педагогика естествознания
Year: 2019
Subjects: методика
профессиональные компетенции
лабораторная работа по физике
физическая модель
моделирование реального физического процесса
погрешности измерений
учебный эксперимент.

description: В статье рассматриваются особенности методики проведения лабораторных работ в курсе общей физики в техническом вузе в условиях компетентностного подхода в образовании. Описываются различные виды учебных исследований, направленных на определение границ применимости физических моделей. На основе рассмотренных примеров учебных исследований обсуждается возможность и необходимость проектирования учебного эксперимента, главной целью которого является формирование у учащихся понятия физическая модель. Рассматриваются примеры постановки таких лабораторных работ и результаты их использования в учебном процессе.
Методические аспекты организации проектной мастерской по астрономии для младших школьников
Creators: name: Алексеевнина Альбина Камаловна
name: Буслова Надежда Сергеевна
Publisher: name: История и педагогика естествознания
Year: 2019
Subjects: обучение астрономии
обучение младших школьников
проектная мастерская
небесные объекты
познавательный интерес к астрономии.

description: В статье приведено описание состояния и перспективы школьного астрономического образования по стандартам второго поколения. Рассмотрены методы и приемы, способствующие повышению мотивации у учащихся к изучению вопросов астрономии. Одним из способов повышения интереса к астрономии является организация проектной мастерской по конструкторской деятельности. В рамках конструкторской деятельности учащиеся осваивают основные астрономические понятия, знакомятся с астрономической техникой и принципом ее действия, изучают параллельно историю вопроса. Подробно рассмотрены этапы занятий по созданию моделей астрономических приборов, космических аппаратов и пр.
Создание и развитие гуманитаризации, математизации, информационно-цифровых и психолого-педагогических технологий в магистерской образовательной системе
Creators: name: Мовсумзаде Эльдар Мирсамедович
name: Пахомов Сергей Иванович
Publisher: name: История и педагогика естествознания
Year: 2019
Subjects: гуманитаризация
информационные и цифровые технологии
математизация
моделирование
инженерное многопрофильное образование.

description: В статье рассмотрены проблемы формирования у студентов знаний, компетенций и ценностей, касающихся социогуманитарных смыслов их будущей деятельности. Показаны приоритеты современного технического образования, гарантирующие его высокое качество. Предложено создание в структуре технических высших учебных заведений подразделений специальной подготовки на выпускающих кафедрах, которые в дальнейшем могут быть преобразованы в кафедры инженерной педагогики. Представлены новые направления подготовки специалистов с возможностью многопрофильного получения образования, основными и важными из которых являются математические возможности базовых дисциплин, гуманитарные составляющие, информационные и цифровые технологии
Investigating transcriptional regulation of purine biosynthesis metabolic pathways with the Escherichia coli Whole-Cell Model
Creators: name: Zhang, Albert
name: Covert, Markus
Publisher: name: Stanford Digital Repository
Year: 2025
Subjects: Escherichia coli
Whole-Cell Model
Transcription factors
Gene regulation
Systems biology
Nucleotide metabolism

description: Escherichia coli is the most studied model bacterium with critical roles in advancing basic science and biotechnology. Decades of research have produced immense amounts of knowledge about E. coli, but this knowledge has yet to be unified into a quantitatively coherent scientific model with holistic, systems-level predictions and understanding. The E. coli Whole-Cell Modeling project aims to create the most detailed mechanistic, computational model of an entire E. coli cell to better understand, predict, and guide experimental discovery. The E. coli Whole-Cell Model (WCM) currently contains only 24 out of more than 300 transcription factors in E. coli. Furthermore, though detailed biochemical knowledge of transcription factor mechanisms and computational studies of transcription factor networks exist, a quantitative understanding of how many transcription factors function within their cellular context, e.g. metabolism, has yet to emerge. For these two purposes, this project aims to add more transcription factors to the E. coli WCM and evaluate their systems-level function. Gene regulation models are parameterized by analyzing gene expression within a large published microarray compendium across numerous environmental conditions and implemented in the WCM with more biochemically realistic assumptions than before. Surprisingly, this study found at least two categories of gene expression: genes that remain relatively constant and unregulated regardless of environment, and genes that roughly occupy only two values of expression in a switch-like manner. This study implements the switch-like gene regulation by the PurR transcription factor of most enzymes in the de novo purine biosynthesis pathway. In this and ongoing work, integrating this with a more kinetic model of metabolism could potentially help investigate how purine biosynthesis matches cellular demand through transcription at different growth rates, levels of purines in the media, and due to internal stochastic fluctuations. These findings offer a more nuanced, quantitative understanding of the role of certain transcription factors in E. coli. Furthermore, they improve the WCM, which aims to eventually become a “digital twin” of E. coli that guides experimental discovery and is useful for biotechnology.
Quantum Information Scrambling in Molecules
Creators: name: Zhang, Chenghao
name: Wolynes, Peter G.
name: Gruebele, Martin
Publisher: name: arXiv
Year: 2022
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Out-of-time-order correlators (OTOCs) can be used to probe how quickly a quantum system scrambles information when the initial conditions of the dynamics are changed. In sufficiently large quantum systems, one can extract from the OTOC the quantum analog of the Lyapunov coefficient that describes the time scale on which a classical chaotic system becomes scrambled. OTOCs have been applied only to a very limited number of toy models, such as the SYK model connected with black hole information scrambling, but they could find much wider applicability for information scrambling in quantum systems that allow comparison with experiments. The vibrations of polyatomic molecules are known to undergo a transition from regular dynamics at low energy to facile energy flow at sufficiently high energy. Molecules therefore represent ideal quantum systems to study scrambling in many-body systems of moderate size (here 6 to 36 degrees of freedom). By computing quantum OTOCs and their classical counterparts we quantify how information becomes 'scrambled' quantum mechanically in molecular systems. Between early 'ballistic' dynamics, and late 'saturation' of the OTOC when the full density of states is explored, there is indeed a regime where a quantum Lyapunov coefficient can be defined for all molecules in this study. Comparison with experimental rate data shows that slow scrambling as measured by the OTOC can reach the time scale of molecular reaction dynamics. Even for the smallest molecules we discuss, the Maldacena bound remains satisfied by regularized OTOCs, but not by unregularized OTOCs, highlighting that the former are more useful for discussing information scrambling in this type of moderate-size quantum system.
Seeing the advantage: visually grounding word embeddings to better capture human semantic knowledge
Creators: name: Merkx, Danny
name: Frank, Stefan L.
name: Ernestus, Mirjam
Publisher: name: arXiv
Year: 2022
Subjects: subject: Computation and Language (cs.CL)
subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: Distributional semantic models capture word-level meaning that is useful in many natural language processing tasks and have even been shown to capture cognitive aspects of word meaning. The majority of these models are purely text based, even though the human sensory experience is much richer. In this paper we create visually grounded word embeddings by combining English text and images and compare them to popular text-based methods, to see if visual information allows our model to better capture cognitive aspects of word meaning. Our analysis shows that visually grounded embedding similarities are more predictive of the human reaction times in a large priming experiment than the purely text-based embeddings. The visually grounded embeddings also correlate well with human word similarity ratings. Importantly, in both experiments we show that the grounded embeddings account for a unique portion of explained variance, even when we include text-based embeddings trained on huge corpora. This shows that visual grounding allows our model to capture information that cannot be extracted using text as the only source of information.
Nature vs. Nurture: Investigating the Effects of Measurement Uncertainties in the Assessment of Potential Trends Between Planetary and Stellar Properties
Creators: name: Safsten, Emily D.
name: Dawson, Rebekah I.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Correlations between planetary and stellar properties, particularly age, can provide insight on planetary formation and evolution processes. However, the underlying source of such trends can be unclear, and measurement uncertainties and small sample sizes can leave doubt as to whether an observed trend truly exists. We use a Bayesian framework to examine how uncertainties in measured parameters influence the odds ratios of competing hypotheses for the source of an observed trend. We analyze three reported trends from the literature. In each application, while uncertainties do affect the numerical value of the odds ratios, our conclusions remain the same whether or not uncertainties are taken into account: hot Jupiter eccentricities are circularized over time, obliquities of hot Jupiter hosts are driven by stellar temperature, and there is not enough evidence to favor a trend of 2:1 orbital resonances with age over a chance relation. Updated samples for the 2:1 resonances and obliquities cases do not change the original conclusions. Simulated 2:1 resonance data show that sample size may be more important than measurement precision for drawing a firm conclusion. However, if 2:1 resonances get disrupted on a wide range of timescales, an age trend will be inherently difficult to confirm over a chance relation, even with a large sample. For some applications, full incorporation of measurement uncertainties may be too computationally expensive, making it preferable to use the framework without uncertainties and perform additional tests to examine the effects of highly uncertain measurements.
description: Accepted for publication in AJ