cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Radôt est piégé
Creators: name: Langage, Langues Et Cultures D'Afrique
name: Simeone-Senelle, Marie-Claude
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2021
Subjects: subject: anthropological_linguistics
subject: Dahâlik
subject: dlk
subject: Annotation

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Scanner Data Price Indexes: Addressing Some Unresolved Issues
Creators: name: Melser, Daniel
Publisher: name: Taylor & Francis
Year: 2016
Subjects: subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics

description: Scanner data are increasingly being used in the calculation of price indexes such as the CPI. The preeminent approach is the RYGEKS method (Ivancic, Diewert and Fox 2011). This uses multilateral methods to construct price parities across a rolling year then links these to construct a nonrevisable index. While this approach performs well there remain some unresolved issues, in particular; the optimal window length and the linking method. In this note, these questions are addressed. A novel linking method is proposed along with the use of weighted GEKS as opposed to a fixed window. These approaches are illustrated empirically on a large scanner dataset and perform well.
X-ray observations of Blueberry galaxies
Creators: name: Adamcová, B.
name: Svoboda, J.
name: Kyritsis, E.
name: Kouroumpatzakis, K.
name: Zezas, A.
name: Boorman, P. G.
name: Borkar, A.
name: Bílek, M.
name: Clavel, M.
name: Petrucci, P. -O.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Compact star-forming galaxies were dominant galaxy types in the early Universe. Blueberry galaxies (BBs) represent their local analogues being very compact and having intensive star formation. Motivated by high X-ray emission recently found in other analogical dwarf galaxies, called Green Peas, we probe into the X-ray properties of BBs to determine if their X-ray emission is consistent with the empirical laws for star-forming galaxies. We performed the first X-ray observations of a small sample of BBs with the XMM-Newton satellite. Spectral analysis for detected sources and upper limits measured via Bayesian-based analysis for very low-count measurements were used to determine the X-ray properties of our galaxy sample. Clear detection was obtained only for 2 sources, with one source exhibiting an enhanced X-ray luminosity to the scaling relations. For the remaining 5 sources, only an upper limit was constrained, suggesting BBs to be rather underluminous as a whole. Our analysis shows that the large scatter cannot be easily explained by the stochasticity effects. While the bright source is above and inconsistent at almost the 99% confidence level, the upper limits of the two sources are below the expected distribution. These results indicate that the empirical relations between the star formation rate, metallicity, and X-ray luminosity might not hold for BBs with uniquely high specific star formation rates. One possible explanation could be that the BBs may not be old enough to have a significant X-ray binary population. The high luminosity of the only bright source can be then caused by an additional X-ray source, such as a hidden active galactic nucleus or more extreme ultraluminous X-ray sources.
description: 10 pages, 4 + 1 (appendix) figures, accepted for publication in Astronomy & Astrophysics on 9.8.2024
Archaeological Excavations at Little Paxton, Diddington, Cambridgeshire, 1992-3: First Interim Report; The Romano-British Period
Creators: name: Jones, Alex
name: Ferris, Iain M
Publisher: name: Archaeology Data Service
Year: 2002

description: Proceedings of the Cambridge Antiquarian Society, 82, 55-66
description: Interim summary of ongoing excavations concentrating on the RB cropmark complex. Pottery and tile were recovered along with environmental evidence.
Exploring the Clustering Effect of the Frailty Survival Model by Means of the Brier Score
Creators: name: Oirbeek, Robin Van
name: Lesaffre, Emmanuel
Publisher: name: Taylor & Francis
Year: 2016
Subjects: subject: Medicine
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Science Policy

description: In this article, the Brier score is used to investigate the importance of clustering for the frailty survival model. For this purpose, two versions of the Brier score are constructed, i.e., a “conditional Brier score” and a “marginal Brier score.” Both versions of the Brier score show how the clustering effects and the covariate effects affect the predictive ability of the frailty model separately. Using a Bayesian and a likelihood approach, point estimates and 95% credible/confidence intervals are computed. The estimation properties of both procedures are evaluated in an extensive simulation study for both versions of the Brier score. Further, a validation strategy is developed to calculate an internally validated point estimate and credible/confidence interval. The ensemble of the developments is applied to a dental dataset.
A Late Bronze Age enclosure at Lynton Way, Sawston, Cambridgeshire
Creators: name: Weston, Phil
name: Newton, Andrew A S
name: Nicholson, Kate
Publisher: name: Archaeology Data Service
Year: 2008

description: Proceedings of the Cambridge Antiquarian Society, 96, 7-20
description: Report on an archaeological excavation undertaken in 2005 on land at Lynton Way, Sawston, Cambridgeshire. The excavation revealed the southern part of a D-shaped enclosure, with an entrance located on its southeast side; the ditches extended beyond the limits of the excavation but the remainder of the enclosure and its associated field systems have been identified in an aerial photographic assessment. Along with further enclosures identified to the southwest, the excavated enclosure might have been part of a wide-reaching unified system of land apportionment. Close to its entrance, the enclosure ditch was cut by a large pit which might have had symbolic significance. In the northwest corner of the excavation, within the enclosure, two partial concentric circles of postholes and stakeholes were identified and interpreted as representing a roundhouse. Artefacts were sparse but the pottery and struck flint assemblages were consistent with the date of c. 1100 BC indicated by radiocarbon dating. Separately authored contributions include
The Chronicle Hills, Whittlesford, Cambridgeshire
Creators: name: Taylor, Christopher
name: Arbon, Ashley
Publisher: name: Archaeology Data Service
Year: 2008

description: Proceedings of the Cambridge Antiquarian Society, 96, 21-40
description: The extensive late prehistoric and Roman site at Whittlesford, first discovered in the early-nineteenth century, is re-examined and re-interpreted. The paper aims to publish the historiography of an archaeological site that has been misinterpreted in the past, to describe the results of a Local Heritage Initiative Project and to examine some of the problems with interpretation that have emerged.
Iron Age settlement and Romanisation on the Isle of Ely: the Hurst Lane Reservoir site
Creators: name: Evans, Christopher
name: Knight, Mark
name: Webley, Leo
Publisher: name: Archaeology Data Service
Year: 2008

description: Proceedings of the Cambridge Antiquarian Society, 96, 41-78
description: The rescue excavation of an extensive Middle/Later Iron Age settlement and its ensuing Romano-British occupation at Hurst Lane on the west side of Ely is reported, and the continuities between its two phases are explored. Having evidence of thirty-five roundhouses, this is one of the most dense Iron Age sites in the region. A development model of their associated compounds is outlined. One of these had marked affinities with the Wardy Hill Ringwork, which allows for discussion of the nature of concentric enclosure elaboration. Numerous `loose' human remains were recovered, including a modified skull found in `foundation deposit-like' circumstances associated with a major roundhouse. Review is made of the Iron Age and Romano-British settlements excavated on Ely during the 1990s. The island's cultural/`tribal' affiliations are considered, as is also the apparent poverty of its assemblages and the processes of its Romanisation. Separately authored contributions include
Prehistoric, Roman and Saxon activity on the Fen hinterland at Parnwell, Peterborough
Creators: name: Webley, Leo
Publisher: name: Archaeology Data Service
Year: 2008

description: Proceedings of the Cambridge Antiquarian Society, 96, 79-114
description: Report on an excavation and watching brief carried out in 2004--5 at Parnwell, Peterborough, providing an opportunity to investigate an extensive area of the clay hinterland adjacent to the gravel terraces surrounding Flag Fen. The earliest occupation took the form of a cluster of Early Neolithic pits. Subsequent activity in the Early Bronze Age was represented by a looser scatter of pits, which contained Collared and Biconical Urn pottery. A small area of Later Iron Age settlement was found at the southern edge of the site, with occupation probably continuing without a break into the Roman period, when a more substantial enclosed settlement was established. Features associated with the Romano-British settlement included a corn-drier, which had been used for roasting malt. The settlement lay within an extensive field system, which also contained a small cremation cemetery. Pollen evidence suggests that there was some regeneration of scrub or woodland following the abandonment of the settlement in the third century AD. Anglo-Saxon features consisted of fifty-seven pits with burnt fills scattered across the site, radiocarbon dated to the seventh to ninth century cal AD. These were probably associated with charcoal production, with no evidence of contemporary settlement in the immediate area. Cropmarks indicating ridge-and-furrow cultivation show that the site was cleared and put under arable use at some point in the medieval or early post-medieval periods. Separately authored contributions include
title: Qakkichchu Laaha (The Little Prince), chap.15
Creators: name: Treis, Yvonne
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2024
Subjects: subject: Kambaata
subject: ktb
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
description: Relation: Saint-Exupéry, Antoine de (1900-1944). Le Petit prince
Exposure of first-feeding cod larvae to dispersed crude oil results in similar transcriptional and metabolic responses as food deprivation
Creators: name: Hansen, Bjørn Henrik
name: Lie, Kai K.
name: Størseth, Trond R.
name: Nordtug, Trond
name: Altin, Dag
name: Olsvik, Pål A.
Publisher: name: Taylor & Francis
Year: 2016
Subjects: subject: Genetics
subject: FOS: Biological sciences
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: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Inorganic Chemistry

description: Exposure of first-feeding cod larvae (Gadus morhua) to dispersed oil results in reduced feeding during an important transition period. First-feeding cod larvae were subjected to a 4-d treatment of food deprivation and sampled for microarray analyses. These microarray data were combined with data from cod larvae treated with mechanically and chemically dispersed oil in an attempt to understand to what extent starvation might explain some of the effects observed in first-feeding cod larvae during oil exposure. Transcriptional profiling of cod larvae suggested that the influence of oil exposure was almost as dramatic as being completely deprived of food. Protein and cellular degradation and loss of amino acids and glucose appear to be concomitant responses to both oil exposure and starvation. Fluorescence imaging of gut content indicated low uptake of food, and reduced growth (decrease in dry weight and in carbon and nitrogen content) was also noted in oil-exposed larvae, providing phenotypic anchoring of microarray data. The study displays the importance in combining use of high-throughput molecular tools with assessment of fitness-related endpoints in order to provide a greater understanding of toxicant-induced responses. This combined-approach investigation suggests that reduction of food uptake is an important process to be included when predicting effects of accidental oil spills. Finally, when comparing data from two oil treatments, exposure to chemically dispersed oil did not appear to result in greater toxicity than exposure to mechanically dispersed oil.
A new measurement of the Galactic $^{12}$C/$^{13}$C gradient from sensitive HCO$^+$ absorption observations
Creators: name: Luo, Gan
name: Colzi, Laura
name: Liu, Tie
name: Bisbas, Thomas G.
name: Li, Di
name: Sun, Yichen
name: Tang, Ningyu
Publisher: name: arXiv
Year: 2024
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a new constraint on the Galactic $^{12}$C/$^{13}$C gradient with sensitive HCO$^+$ absorption observations against strong continuum sources. The new measurements suffer less from beam dilution, optical depths, and chemical fractionation, allowing us to derive the isotopic ratios precisely. The measured $^{12}$C/$^{13}$C ratio in the Solar neighborhood (66$\pm$5) is consistent with those obtained from CH$^+$. Two measurements toward the Galactic Center are 42.2$\pm$1.7 and 37.5$\pm$6.5. Though the values are a factor of 2$\sim$3 higher than those derived from dense gas tracers (e.g., H$_2$CO, complex organic molecules) toward Sagittarius (Sgr) B2 regions, our results are consistent with the absorption measurements from c-C$_3$H$_2$ toward Sgr B2 ($\sim$40), and those from CH$^+$ toward Sgr A$^*$ and Sgr B2(N) ($>$30). We calculate a new Galactic $^{12}$C/$^{13}$C gradient of (6.4$\pm$1.9)$R_{\rm GC}$/kpc+(25.9$\pm$10.5), and find an increasing trend of $^{12}$C/$^{13}$C gradient obtained from high-density to low-density gas tracers, suggesting opacity effects and chemical fractionation may have a strong impact on the isotopic ratios observed at high-density regions.
description: 11 pages, 6 figures, accepted for publication in A&A
SWEET-Cat: A view on the planetary mass-radius relation
Creators: name: Sousa, S. G.
name: Adibekyan, V.
name: Delgado-Mena, E.
name: Santos, N. C.
name: Rojas-Ayala, B.
name: Barros, S. C.
name: Demangeon, O. D. S.
name: Hoyer, S.
name: Israelian, G.
name: Mortier, A.
name: Soares, B. M. T.
name: Tsantaki, M.
Publisher: name: arXiv
Year: 2024
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: SWEET-Cat (Stars With ExoplanETs Catalogue) was originally introduced in 2013, and since then, the number of confirmed exoplanets has increased significantly. A crucial step for a comprehensive understanding of these new worlds is the precise and homogeneous characterization of their host stars. We used a large number of high-resolution spectra to continue the addition of new stellar parameters for planet-host stars in SWEET-Cat following the new detection of exoplanets listed both at the Extrasolar Planets Encyclopedia and at the NASA exoplanet archive. We obtained high-resolution spectra for a significant number of these planet-host stars, either observed by our team or collected through public archives. For FGK stars, the spectroscopic stellar parameters were derived for the spectra following the same homogeneous process using ARES+MOOG as for the previous SWEET-Cat releases. The stellar properties are combined with the planet properties to study possible correlations that could shed more light into the star-planet connection studies. We increase the number of stars with homogeneous parameters by 232 ($\sim$ 25\% - from 959 to 1191). We then focus on the exoplanets with both mass and radius determined to review the mass-radius relation where we find consistent results with the ones previously reported in the literature. For the massive planets we also revisit the radius anomaly where we confirm a metallicity correlation for the radius anomaly already hinted in previous results.
description: 8 pages, 5 figures, Accepted for A&A
Drifts of the sub-stellar points of the TRAPPIST-1 planets
Creators: name: Alexandre, Revol
name: Bolmont, Émeline
name: Sastre, Mariana
name: Tobie, Gabriel
name: Libert, Anne-Sophie
name: Kervazo, Mathilde
name: Blanco-Cuaresma, Sergi
Publisher: name: arXiv
Year: 2024
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Accurate modeling of tidal interactions is crucial for interpreting recent JWST observations of the thermal emissions of TRAPPIST-1~b and c and for characterizing the surface conditions and potential habitability of the other planets in the system. Indeed, the rotation state of the planets, driven by tidal forces, significantly influences the heat redistribution regime. Due to their proximity to their host star and the estimated age of the system, the TRAPPIST-1 planets are commonly assumed to be in a synchronization state. In this work, we present the recent implementation of the co-planar tidal torque and forces equations within the formalism of Kaula in the N-body code Posidonius. This enables us to explore the hypothesis of synchronization using a tidal model well suited to rocky planets. We studied the rotational state of each planet by taking into account their multi-layer internal structure computed with the code Burnman. Simulations show that the TRAPPIST-1 planets are not perfectly synchronized but oscillate around the synchronization state. Planet-planet interactions lead to strong variations on the mean motion and tides fail to keep the spin synchronized with respect to the mean motion. As a result, the sub-stellar point of each planet experiences short oscillations and long-timescale drifts that lead the planets to achieve a synodic day with periods varying from $55$~years to $290$~years depending on the planet.
description: 7 pages, 6 figures
Humanística e Teologia, v. 5 n. 3 (1984)
Creators: name: Humanística E Teologia
Publisher: name: Humanística e Teologia
Year: 1984

description: A «Ars Orandi» de Fr. Heitor Pinto e as raízes culturais da «Imagem da Vida Cristã»: no quarto centenário da sua morte...291-318 A Igreja templo vivo de Deus - a eucologia Comum da Dedicação...320-335 A conversão de Leonardo Coimbra: comentário à tese de Dr. Sant'Anna Dionísio...338-364 Subsídio para uma bibliografia sobre Leonardo Coimbra 1980-1984...365-370 Processos artificiais na transmissão da vida humana e a ética...371-374 Contexto linguístico do topónimo «Rondães» (Lamelas - S. Tirso)...375-378 A abertura das aulas no Instituto de Ciências Humanas e Teológicas...379-381
Exoplanet accretion monitoring spectroscopic survey (ENTROPY) I. Evidence for magnetospheric accretion in the young isolated planetary-mass object 2MASS J11151597+1937266
Creators: name: Viswanath, Gayathri
name: Ringqvist, Simon C.
name: Demars, Dorian
name: Janson, Markus
name: Bonnefoy, Mickaël
name: Aoyama, Yuhiko
name: Marleau, Gabriel-Dominique
name: Dougados, Catherine
name: Szulágyi, Judit
name: Thanathibodee, Thanawuth
Publisher: name: arXiv
Year: 2024
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Accretion among planets is a poorly understood phenomenon, due to lack of both observational and theoretical studies. Detection of emission lines from accreting gas giants facilitate detailed investigations into this process. This work presents a detailed analysis of Balmer lines from one of the few known young, planetary-mass objects with observed emission, the isolated L2 dwarf 2MASS J11151597+1937266 with a mass 7-21 Mj and age 5-45 Myr, located at 45+-2 pc. We obtained the first high-resolution (R~50,000) spectrum of the target with VLT/UVES, a spectrograph in the near-UV to visible wavelengths (3200-6800 AA). We report resolved H3-H6 and He I (5875.6 AA) emission in the spectrum. Based on the asymmetric line profiles of H3 and H4, 10% width of H3 (199+-1 km/s), tentative He I 6678 AA emission and indications of a disk from MIR excess, we confirm ongoing accretion at this object. Using the Gaia update of the parallax, we revise its temperature to 1816+-63 K and radius to 1.5+-0.1 Rj. Analysis of observed H I profiles using 1D planet-surface shock model implies a pre-shock gas velocity of v0=120(+80,-40) km/s and a pre-shock density of log(n0/cm^-3)=14(+0,-5). Pre-shock velocity points to a mass of 6(+8,-4) Mj for the target. Combining the H I line luminosities and planetary Lline-Lacc scaling relations, we derive a mass accretion rate of 1.4(+2.8,-0.9)x10^-8 Mj/yr.
description: Accepted for publication at A&A on 2024-09-11. 15 pages, 9 figures, 7 tables
Grafting of mesenchymal stem cell-seeded small intestinal submucosa to repair the deep partial-thickness burns
Creators: name: Guo, Xing
name: Xia, Bo
name: Lu, Xiao-Bo
name: Zhang, Zhong-Jie
name: Li, Zhong
name: Li, Wei-Ling
name: Xiong, Ai-Bing
name: Deng, Li
name: Tan, Mei-Yun
name: Huang, Yong-Can
Publisher: name: Taylor & Francis
Year: 2016
Subjects: subject: Biophysics
subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Molecular Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Developmental Biology

description: Purpose: Regenerative medicine provides many treatments for burn wounds, of which cell-seeded substitutes are encouraging for large and deep burns. To assess the feasibility of mesenchymal stem cell (MSC)-seeded small intestinal submucosa (SIS) to repair the deep partial-thickness burns, a rat study was performed. Materials & Methods: The burn model was created by contacting the dorsal surface directly with boiled water for 10 seconds. MSCs at passage 3 were seeded on the SIS before implantation. Three days after burn injury, the grafts were implanted onto the burn area. At 3, 7, 14 and 21 days post implantation, gross observation and histological assessments were performed. Results: SIS alone and MSC-seeded SIS were able to accelerate the burn wound closure by enhancing granulation tissue formation, increasing wound maturity, improving revascularization, and inducing the proliferation of neo-epidermal cells. Additionally, MSC-seeded SIS was much more effective than SIS alone for the repair of deep partial-thickness burns. Conclusion: Both SIS and MSC-seeded SIS were able to repair the large and deep burn wounds and the loaded MSCs possessed positive effects to accelerate the wound closure in a rat model.
A Hoard of Roman Bronze Bowls from Burwell, Cambridgeshire.
Creators: name: Gregory, Tony J
Publisher: name: Archaeology Data Service
Year: 2008

description: Proceedings of the Cambridge Antiquarian Society, 66, 63-80
description: [TL 585676]. Description, with technological details, of a hoard of eighteen bronzes found during field-levelling. There are eight bowls of Irchester type, three one-piece carinated cauldrons, a carinated bowl, a handled skillet, a hemispherical fluted bowl, two penannular rings and two fragmentary vessels. Excavations conducted on the site by D M Browne (81-91) threw no light on the circumstances of deposition.
Merging Galaxies in Isolated Environments II. Evolution of Star Formation and Accretion Activity during the Merging Process
Creators: name: Calderón-Castillo, Paula
name: Smith, Rory
Publisher: name: arXiv
Year: 2024
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: It is now well known that certain massive galaxies undergo enormous enhancements in their SFR when they undergo major mergers(100x). To analyse the SF enhancement and AGN fraction evolution during the merger process, we use a more timeline-like merger sequence. Also, to determine the relation between the SF enhancement in mergers and the morphology of the galaxies involved. Taking advantage of the Mstr and SFR of 600 nearby isolated mergers from our previous study, we calculate the distance of our galaxies from the SF MS, which we refer to as SFmode. We analyse how the SFmode varies during the merger process, for morphology and Mstr. We also analyse the AGN content of our mergers, using multiple diagnostics based on emission line ratios and WISE colours. We observe that, overall, merging galaxies show a SFmode that is governed by their morphology. Spirals typically show high SFmode values while highly-disturbed galaxies are generally even more enhanced (0.8dex and 1dex above the MS, resp). On the contrary, elliptical and lenticular galaxies show the lowest SF modes, as expected. However, even they show SF enhancement compared to their unperturbed counterparts (their median SFmode is within the 1-sigma scatter of the MS, and this can occur even before the galaxies have coalesced). We see a trend for SFmode to gradually increase with increasing merger stage. We do not find a clear dependency of the observed AGN fraction on merger stage for the majority of our classification methods. We find mergers can significantly enhance SF in galaxies of all morphologies. For early-type galaxies, this could suggest that some gas was present prior to the merger which may be triggered to form stars by the tidal interaction. As the SF enhancement continues throughout the merger process, this suggests that the enhancement may be a long-lived event, contrary to the short starbursts seen in some models.
description: A&A accepted. 16 pages, 13+5 figures
Anglo-Saxon Finds from Brooke, Norfolk, 1867-1869.
Creators: name: Kennett, David H
Publisher: name: Archaeology Data Service
Year: 2008

description: Proceedings of the Cambridge Antiquarian Society, 66, 93-118
description: ?near TM 294995. Forty objects in the British Museum are here published for the first time as a cemetery group. There were probably not more than twenty graves with objects, mostly inhumations, dating to the latter part of 6th century. Thirteen brooches and other bronzes, bead necklaces, spearheads, knives, shield bosses and two pots are illustrated. The presumed cemetery is discussed in the light of other mainly inhumation cemeteries in Norfolk, otherwise a predominantly cremation area.
Population of excited levels of Fe+, Ni+ and Cr+ in exocomets gaseous tails
Creators: name: Vrignaud, T.
name: Etangs, A. Lecavelier des
Publisher: name: arXiv
Year: 2024
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The star Beta Pic is widely known for harbouring a large population of exocomets, which create variable absorption signatures in the stellar spectrum as they transit the star. While the physical and chemical properties of these objects have long remained elusive, Vrignaud et al. (2024) recently introduced the exocomet curve of growth approach, enabling, for the first time, the estimate of exocometary column densities and excitation temperature using absorption measurements in many spectral lines. Using this new tool, we present a refined study of a Beta Pic exocomet observed on December 6, 1997 with the HST. We first show that the comet's signature in FeII lines is well explained by the transit of two gaseous components, with different covering factors and opacities. Then, we show that the studied comet is detected in the lines of other species, such as NiII and CrII. These species are shown to experience similar physical conditions than FeII (same radial velocity profile, same excitation temperature), hinting that they are well-mixed. Finally, using almost 100 FeII lines rising from energy levels between 0 and 33000 cm-1, we derive the complete excitation diagram of Fe+ in the comet. The transiting gas is found to be populated at an excitation temperature of 8190+-160 K, very close to the stellar effective temperature (8052 K). Using a model of radiative and collisional excitation, we show that the observed excitation diagram is compatible with a radiative regime, associated with a close transit distance (< 0.43 au) and a low electronic density (< 1e7 cm-3). In this regime, the excitation of Fe+ is controlled by the stellar flux, and do not depend on the local electronic temperature or density. These results allow us to derive the Ni+/Fe+ and Cr+/Fe+ ratios in the December 6, 1997 comet, at 8.5 +- 0.8 x 10-2 and 1.04 +- 0.15 x 10-2 respectively, close to solar abundances.
description: 12 pages, 14 figures. Appendices A-G. Accepted to A&A
Cognitive fusion and emotion differentiation: does getting entangled with our thoughts dysregulate the generation, experience and regulation of emotion?
Creators: name: Plonsker, Reut
name: Biran, Dana Gavish
name: Zvielli, Ariel
name: Bernstein, Amit
Publisher: name: Taylor & Francis
Year: 2016
Subjects: subject: Medicine
subject: Neuroscience
subject: Sociology
subject: FOS: Sociology
subject: Developmental Biology
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 60506 Virology
subject: FOS: Biological sciences

description: We tested whether cognitive fusion impairs emotion differentiation and thereby mediates relations between cognitive fusion and depression and panic symptoms among 55 adults (Mage = 26.8 (3.9), 50.9% women). Using visual stimuli, we elicited multiple emotion states and measured (a) emotional intensity – the subjective emotion intensity of elicited emotions (i.e. Specific Emotion Intensity – SEI), as well as (b) emotional differentiation – the degree of co-activation of multiple negative emotions when a specific emotion was elicited (i.e. Multiple Emotion Co-Activation – MECA). First, as hypothesised, we found that cognitive fusion predicted lower levels of emotion differentiation (MECA). In contrast, as hypothesised, these effects were significantly greater than the (null) effects of cognitive fusion on emotion intensity (SEI). Second, as predicted, MECA, but not SEI, predicted depression and panic symptoms. Finally, we found that MECA mediated the effects of cognitive fusion on depression and panic symptoms. The present findings contribute novel, preliminary empirical insight into associations between cognitive fusion, impaired emotion differentiation and mental ill-health.
LC–MS profiling of glucosinolates in the seeds of Brassica elongata Ehrh., and of the two stenoendemic B. botteri Vis and B. cazzae Ginzb. & Teyber
Creators: name: Montaut, Sabine
name: Blažević, Ivica
name: Ruščić, Mirko
name: Rollin, Patrick
Publisher: name: Taylor & Francis
Year: 2016
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
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: Ecology
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Plant Biology

description: The glucosinolates (GLs) present in seed extracts of Brassica elongata Ehrh., B. botteri Vis and B. cazzae Ginzb. & Teyber from Croatia were identified by LC–MS. 4-Hydroxyindol-3-ylmethyl GL (3) was the major GL in the seeds of B. elongata, along with the four minor GLs 2-(R)-hydroxy-3-butenyl- (1), 3-butenyl- (2), 4-pentenyl- (4) and indol-3-ylmethyl (5). The seeds of B. botteri (Vis island) and B. cazzae (Sušac island) contained 2 as the major GL as well as 1, 3, 5 and 4-methoxyindol-3-ylmethyl GL (6). However, the GLs in B. botteri (Palagruža island) differed from other varieties having 2-propenyl GL (7) as the major GL in the seeds, and the four minor GLs 2, 3, 5 and 6. This first report of the GL content in the seeds of B. elongata, B. botteri and B. cazzae indicates that the unique GL profiles could be specific to the geographical origin of the plant.
title: Qakkichchu Laaha (The Little Prince), chap.9
Creators: name: Treis, Yvonne
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2024
Subjects: subject: Kambaata
subject: ktb
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
description: Relation: Saint-Exupéry, Antoine de (1900-1944). Le Petit prince
Anglo-Saxon and medieval boundaries and burials at the former Oblic Engineering site, Church Street, Litlington
Creators: name: Woolhouse, Thomas
Publisher: name: Archaeology Data Service
Year: 2008

description: Proceedings of the Cambridge Antiquarian Society, 96, 115-126
description: An excavation carried out on land adjacent to Litlington parish church found boundary ditches dating from the sixth to the tenth centuries AD and eleventh to thirteenth centuries AD. three undated inhumation burials are thought to be broadly contemporary with the earliest ditches, which may have demarcated the eastern limit of a burial ground connected to an earlier church. Separately authored contributions include
Mid-Saxon burials at Barnwell Road, Cambridge
Creators: name: Newton, Andrew A S
Publisher: name: Archaeology Data Service
Year: 2008

description: Proceedings of the Cambridge Antiquarian Society, 96, 127-134
description: Report on an excavation and watching brief carried out in 2005 at land to the rear of 1--23 Barnwell Road, Cambridge, following an evaluation carried out at the site earlier in the year. The excavation identified two graves, which between them contained three burials, as well as a pit and a linear feature. Three further burials were identified during the watching brief phase of the project. A copper-alloy buckle similar to others found elsewhere in sixth-, seventh- and eighth-century contexts found with one of the burials has dated one individual to the Anglo--Saxon period. By association, the other burials on the site have been tentatively dated to the same period.
Triple trouble with PSR J1618-3921: Mass measurements and orbital dynamics of an eccentric millisecond pulsar
Creators: name: Grunthal, K.
name: Krishnan, V. Venkatraman
name: Freire, P. C. C.
name: Kramer, M.
name: Bailes, M.
name: Buchner, S.
name: Burgay, M.
name: Cameron, A. D.
name: Chen, C. -H. R.
name: Cognard, I.
name: Guillemot, L.
name: Lower, M. E.
name: Possenti, A.
name: Theureau, G.
Publisher: name: arXiv
Year: 2024
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: PSR J1618-3921 is one of five known millisecond pulsars (MSPs) in eccentric orbits (eMPSs) located in the Galactic plane, whose formation is poorly understood. Earlier studies of these objects revealed significant discrepancies between observation and predictions from standard binary evolution scenarios of pulsar-Helium white dwarf binaries. We conducted observations with the L-band receiver of the MeerKAT radio telescope and the UWL receiver of the Parkes Murriyang radio telescope between 2019 and 2021. These data were added to archival observations. We perform an analysis of this joint 23-year-dataset. We use the recent observations to give a brief account of the emission properties of J1618-3921, including a Rotating Vector model fit of the linear polarisation position angle of the pulsar. The long timing baseline allowed for a highly significant measurement of the rate of advance of periastron of $\dotω$. We can only report a low significance detection of the orthometric Shapiro delay parameters $h_3$ and $ς$, leading to mass estimates of the total and individual binary masses. We detect an unexpected change in the orbital period of, which is an order of magnitude larger and carries an opposite sign to what is expected from Galactic acceleration and the Shklovskii effect. We also detect a significant second derivative of the spin frequency. Furthermore, we report an unexpected, abrupt change of the mean pulse profile in June 2021 with unknown origin. We propose that the anomalous $\dot{P_b}$ and $\ddot{f}$ indicate an additional varying acceleration due to a nearby mass, i.e., the J1618-3921 binary system is likely part of a hierarchical triple. This finding suggests that at least some eMSPs might have formed in triple star systems. Although the uncertainties are large, the binary companion mass is consistent with the $P_b$ - $M_{WD}$ relation.
description: 17 pages, 11 figures, 3 tables
Automated detection of exploding granules with SDO/HMI data
Creators: name: Ballot, J.
name: Roudier, T.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Exploding granules on the solar surface play a major role in the dynamics of the outer part of the convection zone, especially in the diffusion of the magnetic field. We aim to develop an automated procedure able to investigate the location and evolution of exploding granules over the solar surface and to get rid of visual detection. We used sequences of observations of intensity and Doppler velocity, as well as magnetograms, provided by the Helioseismic and Magnetic Imager aboard the Solar Dynamics Observatory. The automated detection of the exploding granules was performed by applying criteria on either three or two parameters: the granule area, the amplitude of the velocity field divergence, and, at the disc centre, the radial Doppler velocity. Our analyses show that granule area and divergence amplitudes are sufficient to detect the largest exploding granules; thus, we can automatically detect them, not only at the disc centre, but across the whole solar surface. Using a 24-hour-long observation sequence, we have demonstrated the important contribution of the most dynamic exploding granules in the diffusion of the magnetic field in the quiet Sun. Indeed, we have shown that the most intense exploding granules are sufficient to build a large part of the photospheric network. We have also applied our procedure on Hinode observations to locate the exploding granules relative to trees of fragmenting granules (TFGs). We conclude that, during a first phase of about 300 minutes after the birth of a TFG, exploding granules are preferentially located on its edge. Finally, we also show that the distribution of exploding granules is homogeneous (at the level of our measurement errors) over the solar surface without a significant dependency on latitude.
description: 9 pages, 9 figures, accepted for publication in Astronomy and Astrophysics (languaged-edited version)
Early Saxon and medieval remains adjacent to the round moat, Fowlmere
Creators: name: Spoerry, Paul
name: Hinman, Mark
Publisher: name: Archaeology Data Service
Year: 2008

description: Proceedings of the Cambridge Antiquarian Society, 96, 135-142
description: An Early Saxon building containing an assemblage of pottery was found next to a horse burial. These, together with the remnants of other buildings and a network of ditches, suggest the possibility of early settlement of the area of Fowlmere. Separately authored contributions include
The East Fields of Cambridge
Creators: name: Hesse, Mary
Publisher: name: Archaeology Data Service
Year: 2008

description: Proceedings of the Cambridge Antiquarian Society, 96, 143-160
description: Using documentary sources, the study completes as far as possible the mapping of the fourteenth-century East Field of Cambridge. Although this Field is now almost entirely built upon, striking correspondences emerge between the patterns of the medieval furlongs and the modern streets. The reconstruction of the fourteenth-century field pattern shows strip-cultivation extending as far as the waterlogged fenland at its eastern boundary. There is, however, evidence to suggest that arable cultivation in the late-eleventh century occupied only about half the fourteenth-century area, with a wide arc of common, pasture and moorland within the eastern and southern boundaries. The possible pre-conquest origins of the open-field system are also discussed.
Comparative thermal unfolding study of psychrophilic and mesophilic subtilisin-like serine proteases by molecular dynamics simulations
Creators: name: Du, Xing
name: Sang, Peng
name: Xia, Yuan-Ling
name: Li, Yi
name: Liang, Jing
name: Shi-Meng Ai
name: Xing-Lai Ji
name: Fu, Yun-Xin
name: Liu, Shu-Qun
Publisher: name: Taylor & Francis
Year: 2016
Subjects: subject: Biophysics
subject: Biochemistry
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Cell Biology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: Computational Biology

description: Molecular dynamics (MD) simulations of a subtilisin-like serine protease VPR from the psychrophilic marine bacterium Vibrio sp. PA-44 and its mesophilic homologue, proteinase K (PRK), have been performed for 20 ns at four different temperatures (300, 373, 473, and 573 K). The comparative analyses of MD trajectories reveal that at almost all temperatures, VPR exhibits greater structural fluctuations/deviations, more unstable regular secondary structural elements, and higher global flexibility than PRK. Although these two proteases follow similar unfolding pathways at high temperatures, VPR initiates unfolding at a lower temperature and unfolds faster at the same high temperatures than PRK. These observations collectively indicate that VPR is less stable and more heat-labile than PRK. Analyses of the structural/geometrical properties reveal that, when compared to PRK, VPR has larger radius of gyration (Rg), less intramolecular contacts and hydrogen bonds (HBs), more protein-solvent HBs, and smaller burial of nonpolar area and larger exposure of polar area. These suggest that the increased flexibility of VPR would be most likely caused by its reduced intramolecular interactions and more favourable protein-solvent interactions arising from the larger exposure of the polar area, whereas the enhanced stability of PRK could be ascribed to its increased intramolecular interactions arising from the better optimized hydrophobicity. The factors responsible for the significant differences in local flexibility between these two proteases were also analyzed and ascertained. This study provides insights into molecular basis of thermostability of homologous serine proteases adapted to different temperatures.
title: The German Communist Struggle 1918-1923
Creators: name: Thulin, Steven Ross
Publisher: name: Old Dominion University
publisherIdentifier: https://ror.org/04zjtrb98
publisherIdentifierScheme: ROR
Year: 1977

description: This paper examines the formation and development of the German Communist movement during the first critical years of the Weimar Republic. Concentrating on leadership as the decisive factor, it traces the origins of German Communism from indigenous revolutionary Marxists in the Spartakan hierarchy and discusses the division of the KPD between conflicting Luxemburg and Liebknecht traditions. A leadership crisis characterized the KPD after the deaths of its prominent veteran leaders, leading to competition with Bolshevik presti.ge and a growing disadvantage for individual German party chiefs. Paul Levi in particular led the KPD to its highest point in 1921 within the Luxemburg tradition but fell victim to rampant German internationalism. Moscow shortly ruined the KPD with cynical offensive tactics. Lenin and Radek moved toward the Luxemburg tradition in 1921, but they were unable to rebuild the KPD to its former strength. Consequently, despite impressive worker support in the national crisis of 1923, the KPD failed to organize and execute a victorious Communist insurrection.
Unveiling Hidden Vulnerabilities in Quantum Systems by Expanding Attack Vectors through Heisenberg's Uncertainty Principle
Creators: name: Rosas-Bustos, Jose R.
name: Thé, Jesse Van Griensven
name: Fraser, Roydon Andrew
Publisher: name: arXiv
Year: 2024
Subjects: subject: Quantum Physics (quant-ph)
subject: Emerging Technologies (cs.ET)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: This study uncovers novel vulnerabilities within Quantum Key Distribution (QKD) protocols that extend beyond traditional implementation flaws, such as loopholes. These newly identified vulnerabilities arise from the complex interaction between Bell Inequalities (BIs) and Hidden Variable Theories (HVTs), further exacerbated by the Heisenberg Uncertainty Principle (HUP). Through a combination of theoretical analysis, simulations, and quantum experiments, we reveal critical security weaknesses that challenge the core assumptions of today's quantum cryptography. While these vulnerabilities differ from known loopholes, when considered alongside them and traditional cyberattacks, they present a significant threat to the robustness of QKD and quantum integrity systems. These results provide a new perspective to rethink current quantum security frameworks to ensure the robustness of future quantum cryptographic and quantum integrity protocols.
The tight correlation of PAH and CO emission from z~0-4
Creators: name: Shivaei, Irene
name: Boogaard, Leindert
Publisher: name: arXiv
Year: 2024
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Aim: The cold molecular gas mass is one of the crucial, yet challenging parameters in galaxy evolution studies. Here, we introduce a new calibration for estimating molecular gas masses using mid-infrared (MIR) photometry. This topic is timely, as JWST now allows us to detect the MIR emission of typical main-sequence galaxies across a wide range of masses and star formation rates with modest time investments. This Letter highlights the strong synergy between ALMA and JWST for studies of dust and gas at cosmic noon. Methods: We combine a sample of 14 main sequence galaxies at z=1-3 with robust CO detections and multi-band MIR photometry, along with a literature sample at z=0-4 with CO and PAH spectroscopy, to study the relationship between PAH, CO(1-0), and total IR luminosities. PAH luminosities are derived from modeling rest-frame UV to sub-mm data. The new z=1-3 sample extends previous high-z studies to about an order-of-magnitude lower PAH and CO luminosities, into the regime of local starbursts for the first time. Results: The PAH-to-CO luminosity ratio remains constant across a wide range of luminosities, for various galaxy types, and throughout the explored redshift range. In contrast, the PAH-to-IR and CO-to-IR luminosity ratios deviate from a constant value at high L(IR). The intrinsic scatter in the L(PAH)-L'(CO) relation is 0.21 dex, with a median of 1.40, and a power-law slope of $1.07 \pm 0.04$. Both the PAH-IR and CO-IR relations are sub-linear. Given the tight and uniform PAH-CO relation over ~3 orders of magnitude, we provide a recipe to estimate the cold molecular gas mass of galaxies from PAH luminosities, with a PAH-to-molecular gas conversion factor of $α_{\rm PAH7.7} = (3.08 \pm 1.08)(4.3/α_{\rm CO})\,M_{\odot}/L_{\odot}$. This method opens a new window to explore the gas content of galaxies beyond the local Universe using multi-wavelength JWST/MIRI imaging.
description: 7 pages, 3 figures, 2 tables. Accepted for publication in A&A Letters