cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Ordinals are not as easy as one, two, three: The acquisition of cardinals and ordinals in Dutch
Creators: name: Meyer, Caitlin
name: Barbiers, Sjef
name: Weerman, Fred
Publisher: name: Taylor & Francis
Year: 2017
Subjects: subject: Cell Biology
subject: Neuroscience
subject: Ecology
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Science Policy
subject: Plant Biology

description: This study argues that the pattern and timing of ordinal acquisition differs substantially from that of cardinals and is influenced by different language-specific factors, such as (ir)regular ordinal morphology, superlative morphology, and the singular-plural distinction. We discuss data from a Give X task (Wynn 1992) administered to 77 Dutch monolinguals (2;11–6;04) that support a so-called knower-level acquisition pattern (e.g., Le Corre & Carey 2007) for Dutch cardinals but show a more complex picture for ordinals, which are acquired around the time a child masters the necessary counting principles and becomes a CP (cardinal principle) knower. Not only is the tiered pattern absent in regular low ordinals, we also see that it takes time for children to link drie ‘three’ to irregular derde ‘third.’ We take this as evidence that ordinals are acquired via rules, rather than being stored lexically one by one.
title: ADCO, Cartulaire de Cîteaux pour les possessions de Dijon et du Dijonnais (XVe siècle), Cart. 175 (11 H 479), 115 folios, f. 0165
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: Petot, Frédéric
name: CG21/F.PETOT/2017
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: cartulaire

description: Cartulaire de Cîteaux pour les possessions de Dijon et du Dijonnais (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 175 (11 H 479), 115 folios, f. 0165, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les possessions de Dijon et du Dijonnais (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 175 (11 H 479), 115 folios, f. 0165, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
Chirality-Controlled Enantiopure Crystal Growth of a Transition Metal Monosilicide by a Floating Zone Method
Creators: name: Kousaka, Yusuke
name: Iwasaki, Satoshi
name: Sayo, Taisei
name: Tanida, Hiroshi
name: Matsumura, Takeshi
name: Araki, Shingo
name: Akimitsu, Jun
name: Togawa, Yoshihiko
Publisher: name: arXiv
Year: 2022
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We performed a crystal growth to obtain chirality-controlled enantiopure crystals using a laser-diode-heated floating zone (LDFZ) method with a composition-gradient feed rod. It has been argued that the crystal handedness of $T$Si ($T$ : transition metal) is fixed depending on $T$ in the case of the ones grown by the conventional methods. We found that right-handed single crystals of CoSi and MnSi were grown from the composition gradient feed rods that consist of FeSi--CoSi and FeSi--MnSi, respectively. The obtained CoSi and MnSi crystals inherit the chirality from the seed part of FeSi, which grows in a right-handed structure, and thus have the chirality opposite to that for the crystals in the literature. The LDFZ method with the feed rods with various combinations of $T$Si compounds enables a flexible control of the chirality of $T$Si and will be useful for clarifying the interplay between the crystalline chirality and chirality-induced physical responses.
description: 10 pages, 3 figures
Supplementary document for Origin of frequency-sensitive super-collimation phenomenon from the geometry of band dispersion surface for two-dimensional photonic crystals - 5732096.pdf
Creators: name: Zhang, Meng
name: Huang, JunMing
name: Jiang, Xunya
Publisher: name: Optica Publishing Group
Year: 2022
Subjects: Uncategorized

description: Supplement 1
Supplementary Material for: Efficacy and Safety of Systemic Therapies for Advanced Hepatocellular Carcinoma: A Network Meta-Analysis of Phase III Trials
Creators: name: Cucchetti, A.
name: Piscaglia, F.
name: Pinna, A.D.
name: Djulbegovic, B.
name: Mazzotti, F.
name: Bolondi, L.
Publisher: name: Karger Publishers
Year: 2017
Subjects: Medicine

description: Aim/Background: After the introduction of sorafenib in the treatment of advanced hepatocellular carcinoma (HCC), different studies tried to evaluate whether other systemic therapies can improve survival. To provide a comprehensive indirect treatment comparison of efficacy and safety of novel drugs, a network meta-analysis (NMA) of phase III randomized controlled trials was performed. Methods: After pertinent literature search up to November 1, 2016, 6 studies were eligible for the analysis including 4,812 individual patients with advanced HCC: 2,454 received sorafenib, 577 received brivanib, 530 received sunitinib, 514 received linifanib, 358 received sorafenib + erlotinib and 379 received placebo. Frequentist NMA was used to compare treatments within a single analytical framework. Results: NMA showed that sorafenib alone, regardless of combination with erlotinib, and linifanib provide a significant survival advantage over placebo (p < 0.05) but without any significant difference between each other. Conversely, all regimens significantly ameliorate progression-free survival versus placebo (p < 0.05). The rank order of efficacy was: sorafenib ± erlotinib, linifanib, brivanib, sunitinib, and placebo. Sorafenib ± erlotinib was the regimen with the fewest number of adverse events that required discontinuation of treatment, whereas linifanib and brivanib resulted in the most adverse events. The risk-benefit summary identified one cluster of therapies with a similar balance between efficacy and safety which included sorafenib alone or in combination with erlotinib, having, at the same time, the highest efficacy and safety. Conclusions: Sorafenib remains the best systemic treatment for advanced HCC; linifanib also resulted in survival advantages over placebo but with a lower safety profile.
Dippers from TESS Full-frame Images. II. Spectroscopic Characterization of Four Young Dippers
Creators: name: Kasagi, Yui
name: Kotani, Takayuki
name: Kawahara, Hajime
name: Tajiri, Tomoyuki
name: Muto, Takayuki
name: Aizawa, Masataka
name: Fujii, Michiko S.
name: Hattori, Kohei
name: Masuda, Kento
name: Momose, Munetake
name: Ohsawa, Ryou
name: Takita, Satoshi
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: Photometric monitoring by the Transiting Exoplanet Survey Satellite (TESS) has discovered not only periodic signals by transiting exoplanets but also episodic or quasi-periodic dimming around young stellar objects. The mechanisms of the dimming of these objects, so-called "dippers", are thought to be related to the property of the accretion or the structure of protoplanetary disks especially in regions close to the host star. Recently, we have created the catalog of dippers from the one year of TESS Full Frame Image (FFI) data. In this paper, we report spectral features of four newly found dippers in that catalog and show that they potentially shed light on the dimming mechanisms. We found that all of the targets exhibit the H alpha emission line, which is an indicator of an ongoing accretion. Based on its line profiles and/or their variability, we characterized the properties of the disks of each source, which can support the dimming mechanisms due to a dusty disk wind or an accretion warp. Also, we found an interesting dipper (TIC 317873721), "close-in binary dipper," showing the complex variability of the line profile and the large radial velocity variation. Since the dimming intervals are similar to the orbital period of the binary, we suggest that the dips are caused by dust in the warp of accretion from a circumbinary disk onto stars. Such a close-in ($
description: 15 pages, 10 figures, accepted for publication in ApJS
Asteroseismology of 3,642 Kepler Red Giants: Correcting the Scaling Relations based on Detailed Modeling
Creators: name: Li, Tanda
name: Li, Yaguang
name: Bi, Shaolan
name: Bedding, Timothy R.
name: Davies, Guy
name: Du, Minghao
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The paper presents a correction to the scaling relations for red-giant stars using model-based masses and radii. We measure radial-mode frequencies from Kepler observations for 3,642 solar-like oscillators on the red-giant branch and use them to characterise the stars with the grid-based modeling. We determine fundamental stellar parameters with good precision: the typical uncertainty is 4.5% for mass, 16% for age, 0.006 dex for surface gravity, and 1.7% for radius. We also achieve good accuracy for estimated masses and radii, based on comparing with those determined for eclipsing binaries. We find a systematic offset of ~15% in mass and ~7% in radius between the modeling solutions and the scaling relations. Further investigation indicates that these offsets are mainly caused by a systematic bias in the Delta nu scaling relation: the original scaling relation underestimates Delta nu value by ~4%, on average, and it is important to correct for the surface term in the calibration. We find no significant offset in the nu_max scaling relation, although a clear metallicity dependence is seen and we suggest including a metallicity term in the formulae. Lastly, we calibrate new scaling relations for red-giant stars based on observed global seismic parameters, spectroscopic effective temperatures and metallicities, and modeling-inferred masses and radii.
description: 20 Pages, accepted by ApJ
EUMillennialsTOUR
Creators: name: Laquidara, Giuseppe
name: Boém, Marika Mazzi
name: Et Alter
Publisher: name: figshare
Year: 2017
Subjects: subject: 150301 Business Information Management (incl. Records, Knowledge and Information Management, and Intelligence)
subject: FOS: Economics and business
subject: 150302 Business Information Systems
subject: 150399 Business and Management not elsewhere classified
subject: 159999 Commerce, Management, Tourism and Services not elsewhere classified
subject: 150402 Hospitality Management
subject: 150601 Impacts of Tourism
subject: 150307 Innovation and Technology Management
subject: 150602 Tourism Forecasting
subject: 150603 Tourism Management
subject: 150604 Tourism Marketing
subject: 150605 Tourism Resource Appraisal
subject: 150606 Tourist Behaviour and Visitor Experience

description: The EUMillennialsTOUR® is about the development of a transnational digital-tourism product, supported by high-technology features to increase tourism arrivals in the low-middle season.

 The value proposition is in delivering a system ready to capture millennials' wishes to travel, and to influence their behaviors (wishes, attitude to select destinations) towards special and unusual purpose and seasons along the year.

 To do this, we reversed analytics to detect tourism dynamics. For each region at different times, and basing on spatial and seasonal patterns sampled through sensors (ThePrimate®)and experts insights (AbC3®), we forced the classic destination management system (DMS) to match attractions with unusual factors and unrequited bookings purchased according to the most common seasonal trends. As a result, X23 with a group of key-partners has developed a system for seeking and booking touristic routes endowed with hyper-peculiarities, unmanaged by the common DMS in the touristic market.
 Hyper- and super- peculiarities results as a magic formula to allow touristic sites and point of interest to overcome the unproductive periods of low seasons. At the same time, it allows customers (i.e. schools that organize trips for their students) to identify infinite thematic routes by very granular factors similar to any special need.

 Four pilot-trips has been tested by 4 schools from Italy, Germany, Belgium and the UK. Two tour operators from STA Travel (UK) and CTS (Italy) modified the scheme produced by the algos on the map. The semantic-key set in the pilot trips refers to industrial heritage, a special typology in touristic destination commonly considered as peripheral in tourism industry.
3D hydrodynamical simulations of the impact of mechanical feedback on accretion in supersonic stellar-mass black holes
Creators: name: Bosch-Ramon, Valenti
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Isolated stellar-mass BH accrete gas, often at supersonic speeds, and can form outflows that can influence the accreted gas. The latter process, known as mechanical feedback, can significantly affect the accretion rate. We use hydrodynamical simulations to assess the impact of mechanical feedback on the accretion rate when the BH moves supersonically through a uniform medium. We carry out 3D hydrodynamical simulations of outflows fueled by accretion that interact with a uniform medium, probing scales similar to and larger than the accretor gravitational sphere of influence. In the simulations the accretor is at rest and the medium moves at supersonic speeds. The outflow power is assumed to be proportional to the accretion rate. The simulations are run for different outflow-medium motion angles and velocity ratios. The impact of different degrees of outflow collimation, accretor size, and resolution is also investigated. In general, the accretion rate is significantly affected by mechanical feedback. The effect is small for outflows perpendicular to the medium motion, and quickly grows for smaller angles. Moreover, the smaller the medium-to-outflow velocity ratio is, the more accretion decreases. On the other hand, the impact of outflow collimation seems moderate. The effect is enhanced when the accretor size is reduced. For a population of BH with random outflow orientations, the average accretion rate drops by (high-low resolution) ~0.2-0.4 and ~0.1-0.2 for medium-to-outflow velocity ratios of 1/20 and 1/100, respectively, when compared to the corresponding cases without outflow. Our results strongly indicate that, on the considered scales, mechanical feedback can easily reduce the energy available from supersonic accretion by a factor of several. This should be taken into account when studying the mechanical, thermal and non-thermal output of isolated BH.
description: 11 pages, 19 figures, astronomy and astrophysics, version after proofs
The Pulsating Helium-Atmosphere White Dwarfs I: New DBVs from the Sloan Digital Sky Survey
Creators: name: Vanderbosch, Zachary P.
name: Hermes, J. J.
name: Winget, Don E.
name: Montgomery, Michael H.
name: Bell, Keaton J.
name: Nitta, Atsuko
name: Kepler, S. O.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present a dedicated search for new pulsating helium-atmosphere (DBV) white dwarfs from the Sloan Digital Sky Survey using the McDonald 2.1m Otto Struve Telescope. In total we observed 55 DB and DBA white dwarfs with spectroscopic temperatures between 19,000 and 35,000K. We find 19 new DBVs and place upper limits on variability for the remaining 36 objects. In combination with previously known DBVs, we use these objects to provide an update to the empirical extent of the DB instability strip. With our sample of new DBVs, the red edge is better constrained, as we nearly double the number of DBVs known between 20,000 and 24,000K. We do not find any new DBVs hotter than PG 0112+104, the current hottest DBV at $T_{\mathrm{eff}}\,{\approx}$ 31,000K, but do find pulsations in four DBVs with temperatures between 27,000 and 30,000K, improving empirical constraints on the poorly defined blue edge. We investigate the ensemble pulsation properties of all currently known DBVs, finding that the weighted mean period and total pulsation power exhibit trends with effective temperature that are qualitatively similar to the pulsating hydrogen-atmosphere white dwarfs.
description: 19 pages, 8 figures, 5 tables. Accepted to ApJ
title: ADCO, Cartulaire de Cîteaux pour les possessions de Chaugey et Maison-Dieu (Fin XVe siècle), Cart. 180 (11 H 755), 83 folios, f. 0152
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/2017
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 Cîteaux pour les possessions de Chaugey et Maison-Dieu (Fin XVe siècle), Archives départementales de la Côte-d'Or, Cart. 180 (11 H 755), 83 folios, f. 0152, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les possessions de Chaugey et Maison-Dieu (Fin XVe siècle), Archives départementales de la Côte-d'Or, Cart. 180 (11 H 755), 83 folios, f. 0152, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
The California-Kepler Survey. X. The Radius Gap as a Function of Stellar Mass, Metallicity, and Age
Creators: name: Petigura, Erik A.
name: Rogers, James G.
name: Isaacson, Howard
name: Owen, James E.
name: Kraus, Adam L.
name: Winn, Joshua N.
name: MacDougall, Mason G.
name: Howard, Andrew W.
name: Fulton, Benjamin
name: Kosiarek, Molly R.
name: Weiss, Lauren M.
name: Behmard, Aida
name: Blunt, Sarah
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: In 2017, the California-Kepler Survey (CKS) published its first data release (DR1) of high-resolution optical spectra of 1305 planet hosts. Refined CKS planet radii revealed that small planets are bifurcated into two distinct populations: super-Earths (smaller than 1.5 $R_E$) and sub-Neptunes (between 2.0 and 4.0 $R_E$), with few planets in between (the "Radius Gap.") Several theoretical models of the Radius Gap predict variation with stellar mass, but testing these predictions are challenging with CKS DR1 due to its limited $M_\star$ range of 0.8-1.4 $M_\odot$. Here, we present CKS DR2 with 411 additional spectra and derived properties focusing on stars of 0.5-0.8 $M_\odot$. We found the Radius Gap follows $R_p \propto P^m$ with $m = -0.10 \pm 0.03$, consistent with predictions of XUV- and core-powered mass-loss mechanisms. We found no evidence that $m$ varies with $M_\star$. We observed a correlation between the average sub-Neptune size and $M_\star$. Over 0.5 to 1.4 $M_\odot$, the average sub-Neptune grows from 2.1 to 2.6 $R_E$, following $R_p \propto M_\star^α$ with $α= 0.25 \pm 0.03$. In contrast, there is no detectable change for super-Earths. These $M_\star$-$R_p$ trends suggests that protoplanetary disks can efficiently produce cores up to a threshold mass of $M_c$, which grows linearly with stellar mass according to $M_c \approx 10 M_E~(M_\star / M_\odot)$. There is no significant correlation between sub-Neptune size and stellar metallicity (over $-$0.5 to $+$0.5 dex) suggesting a weak relationship between planet envelope opacity and stellar metallicity. Finally, there is no significant variation in sub-Neptune size with stellar age (over 1 to 10 Gyr), which suggests that the majority of envelope contraction concludes after $\sim$1 Gyr.
description: 30 pages, 16 figures, 4 tables; accepted for publication in The Astronomical Journal; machine readable versions of Tables 1 and 2 uploaded
title: The transcriptional basis of seasonal life-history transitions in the Siberian hamster
Creators: name: Stewart, Calum
Publisher: name: University of Glasgow
Year: 2024

description: Seasonal changes in physiology and behaviour are widespread in plants and animals. Changes in external photoperiod provide an initial predictive cue which animals used to drives changes in physiology. These long-term regulated changes in physiological stability are referred to as programmed rheostasis. Rheostasis controls changes in the set-point of homeostatically defended physiological variables. The aim of this thesis was to investigate the neuroendocrine mechanisms which regulate programmed regulation of energy rheostasis in the Siberian hamsters (Phodopus sungorus). Next-generation sequencing was used to examine the expression of transcripts within the hypothalamus during the photoperiod-induced involution and regrowth in body mass. Despite large changes in body mass and food intake, neuroendocrine markers showed limited changes in expression with only somatostatin (sst) showing large seasonal changes. Expression of many transcripts is upregulated exclusively when the set-point in body mass is decreasing. One such transcript Myocyte enhancer factor 2c (mef2c), is a transcription factor which may be involved in effecting transciption changes to control the set-point. Then, two separate studies using common manipulations of negative and positive energy balance were conducted to identify molecular markers associated with rheostatic and homeostatic regulation of energy balance. Short term food restriction was shown to increase neuropeptide-y (npy) expression. Conversely, Sst expression increased significantly in short photoperiod hamsters but remained stable despite food restriction. Next, by a manipulation of positive energy balance using a high-fat diet paradigm it was found that neither homeostatic, nor rheostatic programs in energy balance were impacted. Overall, the studies describe here provide evidence for two separate neuroendocrine systems that independently regulate short-term homeostatic, versus long-term rheostatic changes in energy balance.
An in-depth numerical study of exact laws for compressible Hall magnetohydrodynamic turbulence
Creators: name: Ferrand, R.
name: Sahraoui, F.
name: Galtier, S.
name: Andrés, N.
name: Mininni, P.
name: Dmitruk, P.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: Various exact laws governing compressible magnetohydrodynamic (MHD) and Hall-MHD (CHMHD) turbulence have been derived in recent years. Other than their fundamental theoretical interest, these laws are generally used to estimate the energy dissipation rate from spacecraft observations in order to address diverse problems related, e.g., to heating of the solar wind (SW) and magnetospheric plasmas. Here we use various $1024^3$ direct numerical simulation (DNS) data of free-decay isothermal CHMHD turbulence obtained with the GHOST code (Geophysical High-Order Suite for Turbulence) to analyze two of the recently derived exact laws. The simulations reflect different intensities of the initial Mach number and the background magnetic field. The analysis demonstrates the equivalence of the two laws in the inertial range and relates the strength of the Hall effect to the amplitude of the cascade rate at sub-ion scales. When taken in their general form (i.e., not limited to the inertial range) some subtleties regarding the validity of the stationarity assumption or the absence of the forcing in the simulations are discussed. We show that the free-decay nature of the turbulence induces a shift from a large scale forcing towards the presence of a scale-dependent reservoir of energy fueling the cascade or dissipation. The reduced form of the exact laws (valid in the inertial range) ultimately holds even if the stationarity assumption is not fully verified.
description: 14 pages, 10 figures
Quantum mechanical simulations of the radical-radical chemistry on icy surfaces
Creators: name: Enrique-Romero, Joan
name: Rimola, Albert
name: Ceccarelli
name: Ugliengo, Piero
name: Balucani, Nadia
name: Skouteris, Dimitrios
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The formation of the interstellar complex organic molecules (iCOMs) is a hot topic in astrochemistry. One of the main paradigms trying to reproduce the observations postulates that iCOMs are formed on the ice mantles covering the interstellar dust grains as a result of radical--radical coupling reactions. We investigate iCOMs formation on the icy surfaces by means of computational quantum mechanical methods. In particular, we study the coupling and direct hydrogen abstraction reactions involving the CH$_3$ + X systems (X = NH$_2$, CH$_3$, HCO, CH$_3$O, CH$_2$OH) and HCO + Y (Y = HCO, CH$_3$O, CH$_2$OH), plus the CH$_2$OH + CH$_2$OH and CH$_3$O + CH$_3$O systems. We computed the activation energy barriers of these reactions as well as the binding energies of all the studied radicals, by means of density functional theory (DFT) calculations on two ice water models, made of 33 and 18 water molecules. Then, we estimated the efficiency of each reaction using the reaction activation, desorption and diffusion energies and derived kinetics with the Eyring equations. We find that radical--radical chemistry on surfaces is not as straightforward as usually assumed. In some cases, direct H abstraction reactions can compete with radical--radical couplings, while in others they may contain large activation energies. Specifically, we found that (i) ethane, methylamine and ethylene glycol are the only possible products of the relevant radical--radical reactions; (ii) glyoxal, methyl formate, glycolaldehyde, formamide, dimethyl ether and ethanol formation is likely in competition with the respective H-abstraction products, and (iii) acetaldehyde and dimethyl peroxide do not seem a likely grain surface products.
description: 46 pages, 15 figures. Accepted for publication in ApJs
Compact objects formation, retention, and growth through accretion onto gas-embedded white-dwarfs/neutron-stars in gas-enriched globular-clusters
Creators: name: Perets, Hagai B.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Observations of pulsars in globular clusters (GCs) give evidence that more >10-20% of neutron stars (NSs) ever formed in GCs were retained there. However, the velocity distribution of field pulsars peaks at 5-10 times the escape velocities of GCs. Consequently, only a small fraction of GC-NSs should have been retained, even accounting for low-velocity NSs formed through electron-capture supernovae. Thus, too few low-velocity NSs should have been retained in GCs, giving rise to the NS retention problem in GCs. Here we suggest a novel solution, in which the progenitors of most GC-NSs were ONe white-dwarfs (WDs) that accreted ambient intra-cluster gas and formed low-velocity NSs through accretion induced collapse (AIC). The existence of an early gas-enriched environment in GCs is supported by observations of GC multiple stellar populations. It is thought that 10s-100s of Myrs after the formation of the first generation of stars, and after ONe-WDs were already formed, GCs were replenished with gas which formed a second generation of stars. Accretion of such replenished gas onto the ONe-WDs catalyzed the AIC processes. The number of AIC-formed NSs is then sufficient to explain the large number of NSs retained in GCs. Similar processes might also drive CO-WDs to produce type-Ia SNe or to merge and form NSs, and similarly drive NSs to AIC and mergers producing BHs. Moreover, the wide variety of gas-catalyzed binary mergers and explosive transients suggest to occur in the gas-rich environments of AGN disk could similarly, and even more efficiently, occur in second-generation gas in GCs.
description: Revised following comments from the community. Submitted
A Study on Monte Carlo simulation of the radiation environment above GeV at the DAMPE orbit
Creators: name: Wang, S. X.
name: Zang, J. J.
name: Jiang, W.
name: Lei, S. J.
name: Luo, C. N.
name: Xu, Z. L.
name: Chang, J.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The Dark Matter Particle Explorer (DAMPE) has been undergoing a stable on-orbit operation for more than 6 years and acquired observation of over 11 billion events. And a better understanding of the overall radiation environment on the DAMPE orbit is crucial for both simulation data production and flight data analysis. In this work, we study the radiation environment at the low Earth orbit and develop a simulation software package using the framework of ATMNC3, in which state-of-the-art full 3D models of the Earth's atmospheric and magnetic-field configurations is integrated. We consider in our Monte Carlo procedure event-by-event propagation of the cosmic rays in the geomagnetic field and their interaction with the Earth's atmosphere, focusing on the particles above GeV that are able to trigger the DAMPE data acquisition system. We compare the simulation results with the cosmic-ray electrons and positrons (CREs) flux measurements made by DAMPE. The overall agreement on both the spectral and angular distribution of the CREs flux demonstrates that our simulation is well established. Our software package could be of more general usage for the simulation of the radiation environment at the low Earth orbit of various altitudes.
title: 01_0982
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
title: Ideology and the revolutionary process: two socialist case studies
Creators: name: Saab, Jade Miguel Bassem
Publisher: name: University of Glasgow
Year: 2024

description: Contemporary theories of revolution have been unable to convincingly integrate the role of ideology in understanding the process of revolutions. They have therefore been unsuccessful in overcoming, and reproduce, critical research gaps and problematics including a false structure/agency dichotomy and substituting macro-economic and class markers for causal analysis. This dissertation addresses these shortcomings by developing a theory of revolution which explains the process of revolutions through the ideologies of the groups and organisations which wage and resist them. This ideological analysis addresses current research gaps and provides a richer explanation of revolutions than competing theories. The dissertation first develops a theoretical framework for studying ideology at the level of groups and organisations by combining framing theory with Michael Freeden’s (1996) “conceptual approach”. The framework shows that ideology is a tangible force that enables and constrain practice. Furthermore, it informs the objectives, structures, tactics, and resources of groups and organisations.

A Marxist approach is utilised to illustrate the interaction of ideologies within a “field of power”. A four-stage process of revolution is derived from this field. The process highlights how revolutions emerge from social movements, and how participating groups and organisations change their ideologies as they simultaneously create and negotiate the stages. The ideological account of revolution is assessed against rational choice theories (RCT), resource mobilisation (RM), deprivation theories, and structural theories of revolution. This appraisal demonstrates that these theories are incomplete without an explicit account of ideology.

Ideological analysis is applied to the Bolshevik party and the Confederación Nacional del Trabajo (CNT, National Confederation of Labour) across specific phases of the Russian Revolution of 1917 and the Spanish Civil War and Revolution of 1936 respectively. The original insight developed in these case studies provides evidence that ideological analysis is better at explaining revolutionary processes than competing theoretical approaches.
Additional file 2 of Remarkable metabolic reorganization and altered metabolic requirements in frog metamorphic climax
Creators: name: Zhu, Wei
name: Chang, Liming
name: Zhao, Tian
name: Wang, Bin
name: Jiang, Jianping
Publisher: name: figshare
Year: 2020
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Physiology
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: Developmental Biology
subject: Computational Biology

description: Additional file 2: Figure S1. Overview of the transcriptomes of control and T3-treated tadpoles. (A) Unigene length distribution. (B) Gene expression correlations between samples. (C–D) Volcano plots showing the DEGs of liver (C) and tail (D) metabolomes between control and T3-treated tadpoles. Figure S2. Liver size of control and T3-treated tadpoles. ***, p < 0.001. Figure S3. Scatter plots of PCAs based on liver (A) and tail (B) metabolomes of pro-metamorphic (stage 30–31) and T3-driven metamorphic tadpoles. Figure S4. Transcriptional variation of genes involved in primary bile acid biosynthesis and steroid metabolism in the liver. *, p < 0.05; **, p < 0.01; ***, p < 0.001. Figure S5. Transcriptional variation of genes with potential metabolic regulatory functions in the liver and tail. *, p < 0.05. Figure S6. Arachidonic acid metabolism highlighted by tail DEGs between control and T3-treated tadpoles. Figure S7. Variation of glutamine levels during metamorphic climax. Different letters denote significant differences between groups (p < 0.05), as shown by the Student–Newman–Keuls post hoc test after one-way ANOVA. *, p < 0.05. Figure S8. Transcriptional changes of genes involved in energy metabolism during metamorphic climax. (A) Transcriptional changes of genes involved in energy metabolism (TCA cycle and oxidative phosphorylation) in the liver. (B) Transcriptional changes of genes involved in TCA cycle in the tail. (C) Heatmap showing the transcriptional level of genes involved in oxidative phosphorylation in the tail. (D) Transcriptional changes of major energy consuming proteins in the tail. A positive logarithmic transformed fold change value means upregulation in T3-treated group, and vice versa; *, p < 0.05. PDH, pyruvate dehydrogenase; CS, citrate synthase; IDH, isocitrate dehydrogenase; 2-OGDH, 2-oxoglutarate dehydrogenase; SCL, succinyl-CoA ligase; SDH, succinate dehydrogenase; MDH, malate dehydrogenase; ND, NADH dehydrogenase; MCK, muscle creatine kinase; UCP, uncoupling protein.
Accreting on the edge: a luminosity-dependent cyclotron line in the Be/X-ray Binary 2S 1553-542 accompanied by accretion regimes transition
Creators: name: Malacaria, Christian
name: Bhargava, Yash
name: Coley, Joel B.
name: Ducci, Lorenzo
name: Pradhan, Pragati
name: Ballhausen, Ralf
name: Fuerst, Felix
name: Islam, Nazma
name: Jaisawal, Gaurava K.
name: Jenke, Peter
name: Kretschmar, Peter
name: Kreykenbohm, Ingo
name: Pottschmidt, Katja
name: Sokolova-Lapa, Ekaterina
name: Staubert, Rudiger
name: Wilms, Joern
name: Wilson-Hodge, Colleen A.
name: Wolff, Michael T.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Accreting X-ray pulsars (XRPs) undergo luminous X-ray outbursts during which the luminosity-dependent spectral and timing features of the neutron star's emission can be analyzed in detail, thus shedding light on the accretion regime at work. We took advantage of a monitoring campaign performed with NuSTAR, Swift/XRT, AstroSat and NICER, to follow the Be/X-ray Binary 2S 1553-542 along one of its rare outbursts and trace its spectral and timing evolution. We report the discovery of a luminosity-dependent cyclotron line energy for the first time in this source. The pulse profiles and pulsed fraction also show variability along the outburst, consistently with the interpretation that the source transitions from the sub-critical to the super-critical accretion regime, separated by a critical luminosity of L$_{crit}\approx4\times10^{37}$ erg/s.
description: Accepted on ApJ. 11 pages, 7 figures, 3 tables
title: The regulation of Green ICO in the UK and China
Creators: name: Cui, Sichang
Publisher: name: University of Glasgow
Year: 2024

description: This dissertation examines the intersection of Green Finance and Initial Coin Offerings (ICOs), with a particular emphasis on their regulatory landscapes in the UK and China. Amidst the global rise of sustainable financial practices, the innovative realm of FinTech has brought forth ICOs as a revolutionary fundraising mechanism. This research juxtaposes the trajectories of Green Finance and ICOs in two economically significant nations: the UK, known for its progressive financial regulations, and China, marked by its distinctive regulatory approach and vast market potential. Through a systematic comparative analysis, the study explores the advantages, challenges, and risks inherent in the amalgamation of Green Finance and ICOs. Subsequent chapters delve deep into the respective legal and regulatory frameworks of the UK and China, spotlighting areas of convergence, divergence, and potential cross-pollination. The research uncovers a spectrum of insights, from the intricacies of Greenwashing in the UK to China's unique "Yue Tan" regulatory perspective. Recommendations are proffered for both nations, reflecting a synthesis of shared learnings and country-specific nuances. The findings contribute to the burgeoning discourse on sustainable finance, offering policy implications, industry directives, and avenues for future research in an increasingly digitalized and ecoconscious global financial landscape.
title: ADCO, Cartulaire de Cîteaux pour les possessions de Chaugey et Maison-Dieu (Fin XVe siècle), Cart. 181 (11 H 754), 165 folios, f. 0108
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/2017
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire de Cîteaux pour les possessions de Chaugey et Maison-Dieu (Fin XVe siècle), Archives départementales de la Côte-d'Or, Cart. 181 (11 H 754), 165 folios, f. 0108, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les possessions de Chaugey et Maison-Dieu (Fin XVe siècle), Archives départementales de la Côte-d'Or, Cart. 181 (11 H 754), 165 folios, f. 0108, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: abbaye de Cîteaux
Spectral variation across Pulsar Profile due to Coherent Curvature Radiation
Creators: name: Basu, Rahul
name: Mitra, Dipanjan
name: Melikidze, George I.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The pulsar profile is characterised by two distinct emission components, the core and the cone. The standard model of a pulsar radio emission beam originating from dipolar magnetic fields, places the core at the centre surrounded by concentric layers of inner and outer conal components. The core emission is expected to have steeper spectra compared to the cones. We present a detailed analysis of the relative differences in spectra between the core and conal emission from a large sample of 53 pulsars over a wide frequency range between 100 MHz and 10 GHz. The core was seen to be much steeper than the cones particularly between 100 MHz and 1 GHz with a relative difference between the spectral index $Δα_{core/cone}\sim$ -1.0. In addition we also found the spectra of the outer conal components to be steeper than the inner cone with relative difference in the spectral index $Δα_{in/out}\sim$ +0.5. The flattening of the spectra from the magnetic axis towards the edge of the open field line region with increasing curvature of the field lines is a natural outcome of the coherent curvature radiation from charged soliton bunches, and explains the difference in spectra between the core and the cones. In addition due to the relativistic beaming effect, the radiation is only visible when it is directed towards the observer over a narrow angle $θ\leq 1/γ$, where $γ$ is the Lorentz factor of the outflowing plasma clouds. This restricts the emission particularly from outer cones, that are associated with field lines with larger curvature thereby making the spectra steeper than the inner cones.
description: 27 pages, 9 figures, Accepted for publication in ApJ
Predictors of receptive and expressive vocabulary development in children with Down syndrome
Creators: name: Deckers, Stijn R.J.M
name: Zaalen, Yvonne Van
name: Balkom, Hans Van
name: Verhoeven, Ludo
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Purpose: There is a lack of longitudinal data on predictors of vocabulary development in children with Down syndrome (DS). In typically developing children, many internal and external predictors of vocabulary development have been determined before. The purpose of the present study was to investigate the role of these variables in the receptive and expressive vocabulary development of children with DS. Method: The present study used a longitudinal design in young children with DS to study the vocabulary development over a period of 1.6 years and investigated the possible predictive role of child-related and environmental variables. Result: Receptive vocabulary development was best predicted by the adaptive level of functioning and early receptive vocabulary skills. Expressive vocabulary development was best predicted by the adaptive level of functioning, receptive vocabulary, maternal educational level, level of communicative intent of the child, attention skills and phonological/phonemic awareness. Conclusion: A wide range of internal and external predictors for vocabulary development of children with DS was found. Predictors resemble those predicting vocabulary development in peers with typical development between 1 and 6 years of age, as identified in other studies.
Theory of Electron Injection at Oblique Shock of Finite Thickness
Creators: name: Amano, Takanobu
name: Hoshino, Masahiro
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Plasma Physics (physics.plasm-ph)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: A theory of electron injection into diffusive shock acceleration (DSA) for the generation of cosmic-ray electrons at collisionless shocks is presented. We consider a recently proposed particle acceleration mechanism called stochastic shock drift acceleration (SSDA). We find that SSDA may be understood as a diffusive particle acceleration mechanism at an oblique shock of finite thickness. More specifically, it is described by a solution to the diffusion-convection equation for particles with the characteristic diffusion length comparable to the shock thickness. On the other hand, the same equation yields the standard DSA if the diffusion length is much longer than the thickness. Although SSDA predicts, in general, a spectral index steeper than DSA, it is much more efficient for low-energy electron acceleration and is favorable for injection. The injection threshold energy corresponds to the transition energy between the two different regimes. It is of the order of $0.1\text{-}1$ MeV in typical interstellar and interplanetary conditions if the dissipation scale of turbulence around the shock is determined by the ion inertial length. The electron injection is more efficient at high $M_\textrm{A} / \cos θ_{Bn}$ where $M_\textrm{A}$ and $θ_{Bn}$ are the Alfvén Mach number and the shock obliquity. The theory suggests that efficient acceleration of electrons to ultra-relativistic energies will be more easily realized at high-Mach-number young supernova remnant shocks, but not at weak or moderate shocks in the heliosphere unless the upstream magnetic field is nearly perpendicular to the shock normal.
description: 26 pages, 9 figures. Accepted for publication in ApJ