cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The identification and characterisation of novel cytoplasmic ASC-1 complex protein interactions
Creators: name: Mordue, Ryan D.
Publisher: name: University of Leicester
Year: 2020
Subjects: Uncategorized

description: Cytoplasmic control of gene expression allows for a rapid reprogramming of specific cellular processes in response to stresses, such as exposure to agents that damage nucleic acids. These responses dictate cell fate in the absence of transcriptional regulation, by regulating the expression of proteins that permit a cell to promote cell survival pathways, or alternatively trigger cell death in situations where homeostasis cannot be restored. In general, cytoplasmic control of gene expression is achieved by the action of RNA-binding proteins, therefore, techniques that allow the analysis of the RNA-bound proteome, such as RNA-interactome capture (RIC), permit the identification of novel RNA-binding proteins (RBPs) that have a key regulatory role in these responses. Work within the Willis laboratory has previously identified Activating signal cointegrator 1 (ASC-1) complex subunit 3 (ASCC3) as a cytoplasmic protein that has increased affinity for RNA in response to UVB irradiation. ASCC3 is a member of the ASC-1 complex, which also includes ASCC2, TRIP4, and ASCC1.In this thesis, the ASC-1 complex members were investigated using immunoaffinity purification and size exclusion chromatography-based approaches. The data show that ASCC3 has increased binding to RNA in a range of cell lines following exposure to UVB and 4NQO, and that the response of ASCC3 and the ASC-1 complex to nucleic acid damage is conserved. FLAG-tagged versions of ASCC3 were generated, and when used as a bait in immunoaffinity purification reactions, the deubiquitinase OTUD4 was identified as a novel interactor of ASCC3. Further studies showed that OTUD4 was part of the cytoplasmic ASC-1 complex, although this interaction may occur with only a small proportion of total cytoplasmic OTUD4. While OTUD4 did not influence control of global protein synthesis rates or cell proliferation, it demonstrated increased binding to polyribosomes following treatment of cells with 4NQO, suggesting that it may function in the ribosome quality control pathway.
Testing General Relativity in the Solar System: present and future perspectives
Creators: name: De Marchi, Fabrizio
name: Cascioli, Gael
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences
subject: 83B05

description: The increasing precision of spacecraft radiometric tracking data experienced in the last number of years, coupled with the huge amount of data collected and the long baselines of the available datasets, has made the direct observation of Solar System dynamics possible, and in particular relativistic effects, through the measurement of some key parameters as the post-Newtonian parameters, the Nordtvedt parameter "eta" and the graviton mass. In this work we investigate the potentialities of the datasets provided by the most promising past, present and future interplanetary missions to draw a realistic picture of the knowledge that can be reached in the next 10-15 years. To this aim, we update the semi-analytical model originally developed for the BepiColombo mission, to take into account planet-planet relativistic interactions and eccentricity-induced effects and validate it against well-established numerical models to assess the precision of the retrieval of the parameters of interest. Before the analysis of the results we give a review of some of the hypotheses and constrained analysis schemes that have been proposed until now to overcome geometrical weaknessess and model degeneracies, proving that these strategies introduce model inconsistencies. Finally we apply our semi-analytical model to perform a covariance analysis on three samples of interplanetary missions: 1) those for which data are available now (e.g. Cassini, MESSENGER, MRO, Juno), 2) in the next years (BepiColombo) and 3) still to be launched as JUICE and VERITAS (this latter is waiting for the approval).
description: 18 pages, 5 figures
Additional file 1 of Effect of pyrene-induced changes in root activity on growth of Chinese cabbage (Brassica campestris L.), and the health risks caused by pyrene in Chinese cabbage at different growth stages
Creators: name: Yang, Xiaosong
name: Hu, Zhengyi
name: Liu, Yuexian
name: Xie, Xiaofan
name: Huang, Lijuan
name: Zhang, Ruili
name: Dong, Biya
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Biotechnology
subject: Ecology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Plant Biology

description: Additional file 1: Text S1. Determination of pyrene in soil and plants. Text S2. Determination of Root activity and malonaldehyde (MDA) levels. Text S3. Soil DNA extraction, PCR amplification and sequencing. Table S1. Measured concentration of pyrene after one week of aging (mg·kg-1). Table S2. Chao1 and Shannon–Weiner indices showing diversity of soil microbial communities without Chinese cabbage cultivation. Fig. S1. Effect of pyrene concentration on rate of inhibition of root elongation. Fig. S2. Composition of bacterial (a) and fungal (b) phyla in soils treated with different pyrene doses, at the seedling, rosette and heading stages. SS, seedling stage; RS, rosette stage; HS, heading stage. Fig. S3. Relative abundance (%) of detected bacteria at the genus level in soils treated with different doses of pyrene (Pyr) during the Chinese cabbage growth period. Fig. S4. Relative abundance (%) of detected fungi at the genus level in soils treated with different doses of pyrene (Pyr) during the Chinese cabbage growth period. Fig. S5. Dynamics of four pyrene-degrading bacterial genera (Mycobacterium, Bacillus, Rhodococcus and Pseudoxanthomonas) in soils treated with different concentrations of pyrene during the Chinese cabbage growth period.
Modeling the Void H I Column Density Spectrum
Creators: name: Manning, Curtis V.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The equivalent width distribution function (EWDF) of \hone absorbers specific to the void environment has been recently derived (Manning 2002), revealing a large line density of clouds (dN/dz ~500 per unit z for Log (N_HI)> 12.4). I show that the void absorbers cannot be diffuse (or so-called filamentary) clouds, expanding with the Hubble flow, as suggested by N-body/hydro simulations. Absorbers are here modeled as the baryonic remnants of sub-galactic perturbations that have expanded away from their dark halos in response to reionization at z ~ 6.5. A 1-D Lagrangian hydro/gravity code is used to follow the dynamic evolution and ionization structure of the baryonic clouds for a range of halo circular velocities. The simulation products at z=0 can be combined according to various models of the halo velocity distribution function to form a column density spectrum that can be compared with the observed. I find that such clouds may explain the observed EWDF if the halo velocity distribution function is as steep as that advanced by Klypin (1999), and the halo mass distribution is closer to isothermal than to NFW.
description: 21 pages, 15 figures. Paper in press; ApJ 591, n1
Podosphaeraster thalassae Cherbonnier 1970
Creators: name: Jangoux, Michel
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Echinodermata
Asteroidea
Valvatida
Podosphaerasteridae
Podosphaeraster
Podosphaeraster thalassae

description: thalassae Cherbonnier, 1970, Podosphaeraster
Podosphaeraster thalassae Cherbonnier, 1970: 203, figs 1-3. — Clark & Downey 1992: 226.
CURRENT STATUS. — Podosphaeraster thalassae Cherbonnier, 1970.
TYPE MATERIAL. — Spain • holotype and paratype; Thalassa expedition, off North-western Spanish coast; depth 500-520 m; MNHN-IE-2014-592.
description: Published as part of Jangoux, Michel, 2022, The type specimens of extant asteroids (Echinodermata) in the Muséum national d'Histoire naturelle of Paris, pp. 259-334 in Zoosystema 44 (11) on page 321, DOI: 10.5252/zoosystema2022v44a11, http://zenodo.org/record/6616817
ACCEPT - combining acalabrutinib with rituximab, cyclophosphamide, doxorubicin, vincristine and prednisolone (R-CHOP) for Diffuse Large B-cell Lymphoma (DLBCL): study protocol for a phase Ib/II open-label non-randomised clinical trial
Creators: name: Davies, Andrew
name: Kirit Ardeshna
name: Barrans, Sharon
name: Burton, Cathy
name: Caddy, Joshua
name: Chinnery, Fay
name: Collins, Graham
name: Day, Laura
name: Fernando, Diana
name: Johnson, Peter
name: McMillan, Andrew
name: Mercer, Katy
name: Radford, John
name: Rule, Simon
name: Griffiths, Gareth O.
Publisher: name: figshare
Year: 2020
Subjects: subject: 119999 Medical and Health Sciences not elsewhere classified
subject: FOS: Other medical sciences

description: Protocol, Informed consent forms and SPIRIT checklist for the ACCEPT trial.
Holographic drag force in 5d Kerr-AdS black hole
Creators: name: Aref'eva, Irina Ya.
name: Golubtsova, Anastasia A.
name: Gourgoulhon, Eric
Publisher: name: arXiv
Year: 2020
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We consider the 5d Kerr-AdS black hole as a gravity dual to rotating quark-gluon plasma. In the holographic prescription we calculate the drag force acting on a heavy quark. According to the holographic approach a heavy quark can be considered through the string in the gravity dual. We study the dynamics of the string for the Kerr-AdS backgrounds with one non-zero rotational parameter and two non-zero rotational parameters that are equal in magnitude. For the case of one non-zero rotational parameter we find good agreement with the prediction from the 4d case considered by arXiv:1012.3800).
description: 25 pp, refs. to 3 SageMath notebooks; v2: typos corrected, refs. added; v3: 38pp, overall corrections, a subsection on phase transition is added, 6 figs, to be published in JHEP
The Lyman-alpha Forest Power Spectrum from the Sloan Digital Sky Survey
Creators: name: McDonald, Patrick
name: Seljak, Uros
name: Burles, Scott
name: Schlegel, David J.
name: Weinberg, David H.
name: Shih, David
name: Schaye, Joop
name: Schneider, Donald P.
name: Brinkmann, J.
name: Brunner, Robert J.
name: Fukugita, Masataka
Publisher: name: arXiv
Year: 2004
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We measure the power spectrum, P_F(k,z), of the transmitted flux in the Ly-alpha forest using 3035 high redshift quasar spectra from the Sloan Digital Sky Survey. This sample is almost two orders of magnitude larger than any previously available data set, yielding statistical errors of ~0.6% and ~0.005 on, respectively, the overall amplitude and logarithmic slope of P_F(k,z). This unprecedented statistical power requires a correspondingly careful analysis of the data and of possible systematic contaminations in it. For this purpose we reanalyze the raw spectra to make use of information not preserved by the standard pipeline. We investigate the details of the noise in the data, resolution of the spectrograph, sky subtraction, quasar continuum, and metal absorption. We find that background sources such as metals contribute significantly to the total power and have to be subtracted properly. We also find clear evidence for SiIII correlations with the Ly-alpha forest and suggest a simple model to account for this contribution to the power. While it is likely that our newly developed analysis technique does not eliminate all systematic errors in the P_F(k,z) measurement below the level of the statistical errors, our tests indicate that any residual systematics in the analysis are unlikely to affect the inference of cosmological parameters from P_F(k,z). These results should provide an essential ingredient for all future attempts to constrain modeling of structure formation, cosmological parameters, and theories for the origin of primordial fluctuations.
description: 92 pages, 45 of them figures, submitted to ApJ, data available at http://feynman.princeton.edu/~pmcdonal/LyaF/sdss.html
An investigation of differentiation between Cornwall and Devon based on history, surnames, and Y-chromosomes
Creators: name: Lampert, Jodie E.
Publisher: name: University of Leicester
Year: 2020
Subjects: Uncategorized

description: Understanding genetic diversity among human populations can help uncover their histories. In 2015 the ‘People of the British Isles’ (PoBI) study of autosome-wide diversity revealed subtle but significantly different genetic clusters, including a clear distinction between the neighbouring counties of Cornwall and Devon; it proposed that Bodmin Moor and the River Tamar had formed a barrier between the two. This thesis uses a combination of historical, onomastic, and genetic approaches to investigate differentiation in this region in more detail.A survey of the historical literature examines whether Cornwall has been isolated from the rest of England and the Continent. Evidence from archaeology, historical documents, and place-names shows that both Roman and Anglo-Saxon influence on Cornwall was less than that on Devon, supporting the idea of Cornish distinctiveness at least over the last two millennia. However, the historical record also shows abundant evidence for Cornwall’s connectedness with the nearby nations of Ireland, Wales, and Brittany.Based on census and parish records, research was undertaken to analyse the specificity and persistence over time of surnames of the people of the Bodmin Moor region between 1702 and 1881. This showed a lack of regionally-specific names, and clear evidence of input from Devon and the rest of England.Analysis of the male-specific Y chromosome examined whether the autosomal Cornwall-Devon distinction seen in the PoBI study was also reflected in paternal lineages. Surname-ascertained samples were recruited from Bodmin Moor and supplemented with PoBI samples. DNAs were analysed with short tandem repeats and single nucleotide polymorphisms. Population genetic analysis supported Cornish distinctiveness, with Bodmin Moor more closely related to Devon. Differences are compatible with lower Anglo-Saxon influence on west Cornwall. Co-analysis with other datasets clusters Cornwall most closely with Wales and Ireland and supports affiliation with Brittany, while Bodmin Moor and Devon more closely resemble other English populations.
Complete population transfer in a degenerate 3-level atom
Creators: name: Rakhimov, Kh. Yu.
name: McGuire, J. H.
name: Shakov, Kh. Kh.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We find conditions required to achieve complete population transfer, via coherent population trapping, from an initial state to a designated final state at a designated time in a degenerate 3-level atom, where transitions are caused by an external interaction. Complete population transfer from an initially occupied state 1 to a designated state 2 occurs under two conditions. First, there is a constraint on the ratios of the transition matrix elements of the external interaction. Second, there is a constraint on the action integral over the interaction, or "area", corresponding to the phase shift induced by the external interaction. Both conditions may be expressed in terms of simple odd integers.
description: 22 pages, 4 figures
Additional file 2 of Distribution and factors associated with urogenital schistosomiasis in the Tiko Health District, a semi-urban setting, South West Region, Cameroon
Creators: name: Green, Adeline Enjema
name: Anchang-Kimbi, Judith Kuoh
name: Godlove Bunda Wepnje
name: Ndassi, Vicky Daonyle
name: Kimbi, Helen Kuokuo
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 2: The prevalence of Schistosoma haematobium infection in relation to distance to stream in the different communities in Tiko Health District
Non-LTE Model Atmospheres for Late-Type Stars I. A Collection of Atomic Data for Light Neutral and Singly-Ionized Atoms
Creators: name: Prieto, C. Allende
name: Lambert, D. L.
name: Hubeny, I.
name: Lanz, T.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: With the goal of producing a reliable set of model atoms and singly-ionized ions for use in building NLTE model atmospheres, we have combined measured energy levels, critically-compiled line transition probabilities, and resonance-averaged calculations of photoionization cross-sections. A majority of the elements from Li to Ca are considered, covering most of the important species in late-type atmospheres. These include elements which contribute free electrons and/or continuous opacity in the ultraviolet (e.g., Mg, and Si), as well as trace elements whose abundance determinations rely on ultraviolet lines (e.g., B from B I lines). The new data complement and, for the species in common, supersede a previous collection of model atoms originally designed for use in studies of early-type stars.
description: 6 pages, 4 figures, to appear in ApJS
Chemical properties of two dense cores in a Planck Galactic Cold Clump G168.72-15.48
Creators: name: Tang, Mengyao
name: Ge, J. X.
name: Qin, Sheng-Li
name: Liu, Tie
name: Wu, Yuefang
name: Kim, Kee-Tae
name: Liu, Sheng-Yuan
name: Zhang, Chao
name: He, J. H.
name: Ju, Bing-Gang
name: Fang, Xinhe
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: To deepen our understanding of the chemical properties of the Planck Galactic Cold Clump (PGCC) G168.72-15.48, we performed observations of nine molecular species, namely, \ce{c-C3H}, \ce{H2CO}, \ce{HC5N}, \ce{HC7N}, \ce{SO}, \ce{CCH}, \ce{N2H+}, \ce{CH3OH}, and \ce{CH3CCH}, toward two dense cores in PGCC G168.72-15.48 using the Tianma Radio Telescope and Purple Mountain Observatory Telescope. We detected \ce{c-C3H}, \ce{H2CO}, \ce{HC5N}, \ce{N2H+}, \ce{CCH}, and \ce{CH3OH} in both G168-H1 and G168-H2 cores, whereas \ce{HC7N} and \ce{CH3CCH} were detected only in G168-H1 and SO was detected only in G168-H2. Mapping observations reveal that the \ce{CCH}, \ce{N2H+}, \ce{CH3OH}, and \ce{CH3CCH} emissions are well coupled with the dust emission in G168-H1. Additionally, \ce{N2H+} exhibits an exceptionally weak emission in the denser and more evolved G168-H2 core, which may be attributed to the \ce{N2H+} depletion. We suggest that the \ce{N2H+} depletion in G168-H2 is dominated by \ce{N2} depletion, rather than the destruction by CO. The local thermodynamic equilibrium calculations indicate that the carbon-chain molecules of \ce{CCH}, \ce{HC5N}, \ce{HC7N}, and \ce{CH3CCH} are more abundant in the younger G168-H1 core. We found that starless core G168-H1 may have the properties of cold dark clouds based on its abundances of carbon-chain molecules. While, the prestellar core G168-H2 exhibits lower carbon-chain molecular abundances than the general cold dark clouds. With our gas-grain astrochemical model calculations, we attribute the observed chemical differences between G168-H1 and G168-H2 to their different gas densities and different evolutionary stages.
The s-process in metal-poor stars: Abundances for 22 neutron-capture elements in CS 31062-050
Creators: name: Johnson, Jennifer A.
name: Bolte, Michael
Publisher: name: arXiv
Year: 2004
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The CH star CS 31062-050 ([Fe/H]=-2.42) is one of the most useful stars yet discovered for evaluating the s-process in metal-poor stars. It is very abundant in heavy elements (e.g., [La/Fe]=2.2), and its relatively cool temperature and low gravity mean that there are many lines of interesting elements present in the spectrum. We measured the abundances of 22 elements with Z>29, including the rarely measured Lu and Pd. We derive an upper limit on the Th abundance as well. The abundances in CS 31062-050 show a similar pattern to many other metal-poor CH stars: high [Pb/Fe] and [Pb/La] ratios, low [Y/La] ratios and high [Eu/La] values compared to the solar system s-process. However, the Th limit, with additional assumptions, is not consistent with the idea that the excess Eu in CS 31062-050 is contributed by the r-process. In addition, the observed [Eu/Tb] cannot be explained by any ratio of solar-system s-process and r-process abundances. We therefore argue that the abundance pattern in CS 31062-050 is most likely the result of the s-process, and we discuss possible modifications that could explain the non-solar-system pattern observed.
description: to be published in ApJ
On the Purity of the ZZ Ceti Instability Strip: Discovery of More Pulsating DA White Dwarfs on the Basis of Optical Spectroscopy
Creators: name: Bergeron, P.
name: Fontaine, G.
name: Billeres, M.
name: Boudreault, S.
name: Green, E. M.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the discovery of two new ZZ Ceti pulsators, LP 133-144 and HE 1258+0123, selected on the basis of model atmosphere fits to optical spectroscopic data. The atmospheric parameters for LP 133-144, Teff = 11,800 +/- 200 K and log g = 7.87 +/- 0.05, and for HE 1258+0123, Teff = 11,410 +/- 200 K and log g = 8.04 +/- 0.05, place them within the empirical boundaries of the ZZ Ceti instability strip. This brings the number of known ZZ Ceti stars to a total of 36, a quarter of which have now been discovered using the spectroscopic approach for estimating their atmospheric parameters. This method has had a 100% success rate so far in predicting the variability of candidate ZZ Ceti stars. We have also analyzed additional spectra of known nonvariable white dwarfs in the vicinity of the ZZ Ceti instability strip. Our study further strengthens the idea that ZZ Ceti stars occupy a pure region in the log g-Teff plane, a region where no nonvariable stars are found. This result supports the thesis that ZZ Ceti pulsators represent a phase through which all DA stars must evolve.
description: 11 pages, 4 figures, accepted for publication in the Astrophysical Journal
COMPARATIVE EFFICACY AND SAFETY OF BIOLOGIC VERSUS NON-BIOLOGIC THERAPIES IN THE MANAGEMENT OF REACTIVE ARTHRITIS: A 52-WEEK COHORT STUDY
Creators: name: Abdujabborov, Jamshidbek
name: Omonov, Jamshid
name: Tursunboev, Ulugbek
name: Kushboeva, Shabnam
name: Abdurakhmanova, Sayyora
Publisher: name: Zenodo
Year: 2025

description: Reactive Arthritis (ReA) is a form of seronegative spondyloarthritis often triggered by infections, primarily from the gastrointestinal or urogenital tracts. The disease is characterized by the sudden onset of asymmetric oligoarthritis, leading to significant pain, reduced mobility, and a decline in the quality of life (Sieper et al., 2002). While conventional therapies, including nonsteroidal anti-inflammatory drugs (NSAIDs) and disease-modifying antirheumatic drugs (DMARDs), are commonly used in the management of ReA, biologic therapies—especially tumor necrosis factor-alpha (TNF-α) inhibitors—have emerged as a promising alternative in treating refractory cases (Braun & Sieper, 2007). Despite the potential of biologic agents, their high cost and the risk of adverse effects require careful consideration, particularly in resource-limited settings (Coates et al., 2016).
Additional file 3 of Distribution and factors associated with urogenital schistosomiasis in the Tiko Health District, a semi-urban setting, South West Region, Cameroon
Creators: name: Green, Adeline Enjema
name: Anchang-Kimbi, Judith Kuoh
name: Godlove Bunda Wepnje
name: Ndassi, Vicky Daonyle
name: Kimbi, Helen Kuokuo
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 3: Reported access to improved water sources among the affected communities in Tiko Health District
Vacuum-field level shifts in a single trapped ion mediated by a single distant mirror
Creators: name: Wilson, M. A.
name: Bushev, P.
name: Eschner, J.
name: Schmidt-Kaler, F.
name: Becher, C.
name: Blatt, R.
name: Dorner, U.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: A distant mirror leads to a vacuum-induced level shift in a laser-excited atom. This effect has been measured with a single mirror 25 cm away from a single, trapped barium ion. This dispersive action is the counterpart to the mirror's dissipative effect, which has been shown earlier to effect a change in the ion's spontaneous decay [J. Eschner et al., Nature 413, 495-498 (2001)]. The experimental data are well described by 8-level optical Bloch equations which are amended to take into account the presence of the mirror according to the model in [U. Dorner and P. Zoller, Phys. Rev. A 66, 023816 (2002)]. Observed deviations from simple dispersive behavior are attributed to multi-level effects.
description: version accepted by PRL
Non-LTE Model Atmospheres for Late-Type Stars II. Restricted NLTE Calculations for a Solar-Like Atmosphere
Creators: name: Prieto, C. Allende
name: Hubeny, I.
name: Lambert, D. L.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We test our knowledge of the atomic opacity in the solar UV spectrum. Using the atomic data compiled in Paper I from modern, publicly available, databases, we perform calculations that are confronted with space-based observations of the Sun. At wavelengths longer than about 260 nm, LTE modeling can reproduce quite closely the observed fluxes; uncertainties in the atomic line data account fully for the differences between calculated and observed fluxes. At shorter wavelengths, departures from LTE appear to be important, as our LTE and restricted NLTE calculations differ. Analysis of visible-near infrared Na I and O I lines, two species that produce a negligible absorption in the UV, shows that observed departures from LTE for theses species can be reproduced very accurately with restricted (fixed atmospheric structure) NLTE calculations.
description: 13 pages, 11 figures, to appear in ApJ
Genetic diversity of Procambarus clarkii populations based on mitochondrial DNA and microsatellite markers in different areas of Guangxi, China
Creators: name: Yizhi Zhong
name: Zhangsheng Tang
name: Liming Huang
name: Dapeng Wang
name: Zhuanling Lu
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Plant Biology

description: The red swamp crayfish (Procambarus clarkii) is a famous invasive species. However, it has become one of the most important freshwater aquaculture resources in China. Herein, we focus on five artificial cultured populations of P. clarkii in Guangxi, southern China to investigate the genetic diversity based on mitochondrial DNA and microsatellites. The results revealed that the genetic diversity of P. clarkii populations in southern Guangxi (NN and DT) was lower than in central (LZ and LB) and northern (RS) Guangxi. A total of 17 haplotypes were captured from 100 individuals and haplotype 2 mainly existed, and the number of haplotype in NN and DT was less than other populations. The AMOVA showed that genetic variation was determined by within populations. The observed mismatch distribution of overall populations fit the expected distributions, indicating that no obvious demographic expansion, but unimodal was observed in RS, LZ and LB. Fst among most of groups exhibited moderate differentiation. Nevertheless, the gene flow demonstrated there had extensive gene exchanges between different populations, particularly between LZ and LB. UPGMA tree revealed that NN and DT belonged to the same clade, whereas the remaining populations were in the other clade. According to the genetic diversity, there is a need to improve the germplasm resources of P. clarkii in southern Guangxi.
Cosmological constant and vacuum energy
Creators: name: Volovik, G. E.
Publisher: name: arXiv
Year: 2004
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The general thermodynamic analysis of the quantum vacuum, which is based on our knowledge of the vacua in condensed-matter systems, is consistent with the Einstein earlier view on the cosmological constant. In the equilibrium Universes the value of the cosmological constant is regulated by matter. In the empty Universe, the vacuum energy is exactly zero, lambda=0. The huge contribution of the zero point motion of the quantum fields to the vacuum energy is exactly cancelled by the higher-energy degrees of freedom of the quantum vacuum. In the equilibrium Universes homogeneously filled by matter, the vacuum is disturbed, and density of the vacuum energy becomes proportional to the energy density of matter. This consideration applies to any equilibrium vacuum irrespective of whether the vacuum is false or true, and is valid both in the Einstein general theory of relativity and within the special theory of relativity, i.e. in the world without gravity.
description: 23 pages, accepted for special topic issue of Annalen der Physik related to Einstein's contributions to physics, references and figure added
Locality Preserving Loss: Neighbors that Live together, Align together
Creators: name: Ganesan, Ashwinkumar
name: Ferraro, Francis
name: Oates, Tim
Publisher: name: arXiv
Year: 2020
Subjects: subject: Machine Learning (cs.LG)
subject: Computation and Language (cs.CL)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences
subject: I.2.7

description: We present a locality preserving loss (LPL) that improves the alignment between vector space embeddings while separating uncorrelated representations. Given two pretrained embedding manifolds, LPL optimizes a model to project an embedding and maintain its local neighborhood while aligning one manifold to another. This reduces the overall size of the dataset required to align the two in tasks such as cross-lingual word alignment. We show that the LPL-based alignment between input vector spaces acts as a regularizer, leading to better and consistent accuracy than the baseline, especially when the size of the training set is small. We demonstrate the effectiveness of LPL optimized alignment on semantic text similarity (STS), natural language inference (SNLI), multi-genre language inference (MNLI) and cross-lingual word alignment(CLA) showing consistent improvements, finding up to 16% improvement over our baseline in lower resource settings.
Leioastra triangularis Mah 2018
Creators: name: Jangoux, Michel
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Echinodermata
Asteroidea
Valvatida
Goniasteridae
Leioastra
Leioastra triangularis

description: triangularis Mah, 2018 Leioastra
Leioastra triangularis Mah, 2018: 46.
CURRENT STATUS. — Leioastra triangularis Mah, 2018.
TYPE MATERIAL. — Madagascar • holotype; 26°9’S, 45°40’E, depth 549 m; MNHN-IE-2007-3946.
description: Published as part of Jangoux, Michel, 2022, The type specimens of extant asteroids (Echinodermata) in the Muséum national d'Histoire naturelle of Paris, pp. 259-334 in Zoosystema 44 (11) on page 321, DOI: 10.5252/zoosystema2022v44a11, http://zenodo.org/record/6616817
Exact Seiberg-Witten Map and Induced Gravity from Noncommutativity
Creators: name: Yang, Hyun Seok
Publisher: name: arXiv
Year: 2004
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We find a closed form for Seiberg-Witten (SW) map between ordinary and noncommutative (NC) Dirac-Born-Infeld actions. We show that NC Maxwell action after the exact SW map can be regarded as ordinary Maxwell action coupling to a metric deformed by gauge fields. We also show that reversed procedure by inverse SW map leads to a similar interpretation in terms of induced NC geometry. This implies that noncommutativity in field theory can be interpreted as field dependent fluctuations of spacetime geometry, which genuinely realizes an interesting idea recently observed by Rivelles.
description: 12 pages, Latex; version to appear in Mod. Phys. Lett. A
Chaeridiona feae Gestro. Uhmann 1958
Creators: name: Staines, C. L.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Chrysomelidae
Chaeridiona
Chaeridiona feae

description: Chaeridiona feae Gestro
Figure 3
 Choeridiona feae Gestro 1890: 239 [Syntypes: Palon, L. Fea/ Co-type (white disk with green border)/ Chaeridiona feae Gestro cotyp. (BMNH, Genoa)]. Weise 1911a: 49, 1911b: 73 (catalog); Maulik 1919: 88 (India species); Uhmann 1943: 245 (morphology); Gaedike & Döbler 1971: 372 (type specimens).
 Chaeridiona feae Gestro. Uhmann 1958: 251 (catalog); Würmli 1976: 403 (revision).
 Body oblong; shining black with metallic purplish sheen; antennae, legs, and venter brownish-black. Head: coarsely punctate; produced anteriorly; with longitudinal carina in middle. Antenna: antennomere I thickest, rounded; II smaller; III longer than II; remainder subequal in length; apical 4 darker, slightly thicker than preceding; I–VII slightly rugose. Pronotum: subcylindrical; subquadrate; parallel-sided; convex; lateral margin slightly bisinuate, margined; anterior angle notched with minute tooth; surface coarsely rugose-punctate, deeply excavated on disc; pronotal width 0.9 mm; pronotal length 0.9–1.0 mm. Scutellum: depressed; smooth; impunctate; parallel-sided; rounded at apex. Elytron: combined much wider than base of pronotum; dilated posteriorly; lateral margin parallel, margined, serrate; with four weak costae- 1 st and 4 th entire, extending nearly to apex; 2 nd interrupted behind middle, less raised at base than apex; 3 rd interrupted in middle (where there is a depression) and near apex; depression present on interspace 6 near middle; interspace 7 slightly raised in middle; suture raised; elytral width 1.6–1.9 mm; elytral length 2.9–3.0 mm. Venter: smooth; shining; impunctate. Total length: 4.1–4.6 mm.
 Comparative notes. This species is one of the two totally dark Chaeridiona. It can be distinguished from C. picea by the rounded exterior apical angle of the elytra and by having elytral costae 1 and 4 entire.
 Food plants. Unknown.
 Distribution. Myanmar: Pegu; Palon; Tharrawaddy.
 Specimens examined. No locality (USNM, 2). Myanmar: no further data (BMNH, 3); Palon (BMNH, 1); Palon, Pegu (BMNH, 3), IX.1887, L. Fea (USNM, 3), VIII–IX.1887, L. Fea (NHMB, 1); Tharrawaddy (BMNH, 3). Total: 16.
description: Published as part of Staines, C. L., 2007, A review of the genus Chaeridiona Baly, 1869 (Coleoptera: Chrysomelidae: Cassidinae), pp. 19-29 in Zootaxa 1521 (1) on page 23, DOI: 10.11646/zootaxa.1521.1.3, http://zenodo.org/record/5087559
WMAP constraint on the P-term inflationary model
Creators: name: Wang, Bin
name: Lin, Chi-Yong
name: Abdalla, Elcio
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: In light of WMAP results, we examine the observational constraint on the P-term inflation. With the tunable parameter $f$, P-term inflation contains richer physics than D-term and F-term inflationary models. We find the logarithmic derivative spectral index with $n>1$ on large scales and $n<1$ on small scales in agreement to observation. We obtained a reasonable range for the choice of the gauge coupling constant $g$ in order to meet the requirements of WMAP observation and the expected number of the e-foldings. Although tuning $f$ and $g$ we can have larger values for the logarithmic derivative of the spectral index, it is not possible to satisfy all observational requirements for both, the spectral index and its logarithmic derivative at the same time.
description: 6 pages, double column, 13 figures included. Version appearing in the Physical Review D
Additional file 1 of A benchmark for RNA-seq deconvolution analysis under dynamic testing environments
Creators: name: Haijing Jin
name: Liu, Zhandong
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology

description: Additional file 1: Figures S1–S18, the outline of simulation frameworks, evaluation results based on three benchmarking frameworks, variance analysis based on real and simulated data.
MOESM1 of Variability among autumn migration patterns of Mongolian Common Shelducks (Tadorna tadorna)
Creators: name: Wang, Xin
name: Cao, Lei
name: Batbayar, Nyambayar
name: Fox, Anthony
Publisher: name: figshare
Year: 2018
Subjects: subject: Molecular Biology
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified

description: Additional file 1: Fig. S1. Comparison of land use patterns at each site of Common Shelduck (Tadorna tadorna) individuals, based on MODIS land cover dataset (MCD12Q1) in 2010 and 2016.
Population control of 2s-2p transitions in hydrogen
Creators: name: Shakov, Kh. Kh.
name: McGuire, J. H.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We consider the time evolution of the occupation probabilities for the 2s-2p transition in a hydrogen atom interacting with an external field, V(t). A two-state model and a dipole approximation are used. In the case of degenerate energy levels an analytical solution of the time-dependent Shroedinger equation for the probability amplitudes exists. The form of the solution allows one to choose the ratio of the field amplitude to its frequency that leads to temporal trapping of electrons in specific states. The analytic solution is valid when the separation of the energy levels is small compared to the energy of the interacting radiation.
description: 6 pages, 3 figures
Characterization and formation of on-disk spicules in the Ca II K and Mg II k spectral lines
Creators: name: Bose, Souvik
name: Henriques, Vasco M. J.
name: Joshi, Jayant
name: van der Voort, Luc Rouppe
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We characterize, for the first time, type-II spicules in Ca II K 3934Å using the CHROMIS instrument at the Swedish 1-m Solar Telescope. We find that their line formation is dominated by opacity shifts with the K$_{3}$ minimum best representing the velocity of the spicules. The K$_{2}$ features are either suppressed by the Doppler-shifted K$_{3}$ or enhanced via an increased contribution from the lower layers, leading to strongly enhanced but un-shifted K$_{2}$ peaks, with widening towards the line-core as consistent with upper-layer opacity removal via Doppler-shift. We identify spicule spectra in concurrent IRIS Mg II k 2796Å observations with very similar properties. Using our interpretation of spicule chromospheric line-formation, we produce synthetic profiles that match observations.
description: 10 pages, 8 figures, accepted for publication in Astronomy and Astrophysics Letters
Additional file 1 of ADHD Prescription Medications and Their Effect on Athletic Performance: A Systematic Review and Meta-analysis
Creators: name: Berezanskaya, Jenny
name: Cade, William
name: Best, Thomas M.
name: Paultre, Kristopher
name: Kienstra, Carolyn
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Pharmacology
subject: Sociology
subject: FOS: Sociology
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 1. Boolean terms utilized for database searches.
Additional file 2 of A benchmark for RNA-seq deconvolution analysis under dynamic testing environments
Creators: name: Haijing Jin
name: Liu, Zhandong
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology

description: Additional file 2: Tables S1–S4, organized description of the benchmarking framework, tested factors, tested methods, and measurement scales.
Interaction induced non-reciprocal three-level quantum transport
Creators: name: Li, Sai
name: Chen, Tao
name: Liu, Jia
name: Xue, Zheng-Yuan
Publisher: name: arXiv
Year: 2020
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Besides its fundamental importance, non-reciprocity has also found many potential applications in quantum technology. Recently, many quantum systems have been proposed to realize non-reciprocity, but stable non-reciprocal process is still experimentally difficult in general, due to the needed cyclical interactions in artificial systems or operational difficulties in solid state materials. Here, we propose a new kind of interaction induced non-reciprocal operation, based on the conventional STIRAP setup, which removes the experimental difficulty of requiring cyclical interaction, and thus it is directly implementable in various quantum systems. Furthermore, we also illustrate our proposal on a chain of three coupled superconducting transmons, which can lead to a non-reciprocal circulator with high fidelity without a ring coupling configuration as in the previous schemes or implementations. Therefore, our protocol provides a promising way to explore fundamental non-reciprocal quantum physics as well as realize non-reciprocal quantum device.
description: 6 pages, 3 figures
Additional file 3 of A benchmark for RNA-seq deconvolution analysis under dynamic testing environments
Creators: name: Haijing Jin
name: Liu, Zhandong
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology

description: Additional file 3: Data description with the GEO accession number.
An Interpretation of the $hν_{peak}$ - $E_{iso}$ Correlation for GRB
Creators: name: Eichler, David
name: Levinson, Amir
Publisher: name: arXiv
Year: 2004
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The $hν_{peak}/100 KeV \sim [E_{iso}/10^{52} \rm{erg}]^{1/2}$ correlation reported recently by Amati et al. (2002) and Lamb et al. (2003) for long GRB's can be interpreted as a viewing angle effect if the emitting region of the fireball is ring-shaped.
description: 12 pages. 5 figures
Chaetaster troscheli Muller & Troschel 1842
Creators: name: Jangoux, Michel
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Echinodermata
Asteroidea
Forcipulatida
Asteriidae
Chaetaster
Chaetaster troscheli

description: * troscheli Müller & Troschel, 1842, Chaetaster
Chaetaster troscheli Müller & Troschel, 1842: 28.
CURRENT STATUS. — Nomen dubium.
REMARK
The species is of uncertain identity (Clark 1993: 189).
description: Published as part of Jangoux, Michel, 2022, The type specimens of extant asteroids (Echinodermata) in the Muséum national d'Histoire naturelle of Paris, pp. 259-334 in Zoosystema 44 (11) on page 321, DOI: 10.5252/zoosystema2022v44a11, http://zenodo.org/record/6616817
High rank torus actions on contact manifolds
Creators: name: Occhetta, Gianluca
name: Romano, Eleonora A.
name: Conde, Luis E. Solá
name: Wiśniewski, Jarosław A.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Algebraic Geometry (math.AG)
subject: FOS: Mathematics
subject: Primary 14L30, Secondary 14M17, 14M25

description: We prove LeBrun--Salamon conjecture in the following situation: if $X$ is a contact Fano manifold of dimension $2n+1$ whose group of automorphisms is reductive of rank $\geq \max(2,(n-3)/2)$ then $X$ is the adjoint variety of a simple group. The rank assumption is fulfilled not only by the three series of classical linear groups but also by almost all the exceptional ones.
description: Minor changes committed
Neochauliodes wuminganus Yang & Yang 1986
Creators: name: Liu, Xingyue
name: Hayashi, Fumio
name: Yang, Ding
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Megaloptera
Corydalidae
Neochauliodes
Neochauliodes wuminganus

description: Neochauliodes wuminganus Yang &Yang
(Fig. 42)
 Neochauliodes wuminganus Yang & Yang, 1986. Entomotaxon. 8: 91. Type locality: Guangxi (Wuming).
 Distribution. China (Guangxi).
description: Published as part of Liu, Xingyue, Hayashi, Fumio & Yang, Ding, 2007, Revision of the Neochauliodes sinensis species-group (Megaloptera: Corydalidae: Chauliodinae), pp. 29-54 in Zootaxa 1511 (1) on page 49, DOI: 10.11646/zootaxa.1511.1.3, http://zenodo.org/record/5087291
title: Peuplement juif de la circonscription de Taliouine
title: Peuplement juif de la circonscription de Taliouine
Creators: name: :Unkn
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2023
Subjects: subject: Minorités
subject: Juifs

description: Cartographie
description: BESM-carto_1952-54-p455_54-06
description: 455
description: 54
description: Bulletin économique et social du Maroc
description: Source: Maison méditerranéenne des sciences de l'homme, Cité numérique de la Méditerranée (Cinumed), Bibliothèque nationale du Royaume du Maroc (BNRM)
description: Source: Bulletin économique et social du Maroc
description: Source: Bulletin économique et social du Maroc (BESM) > BESM (Cartographie)
description: Relation: https://cinumed.mmsh.univ-aix.fr/idurl/1/81884
description: Coverage: Maroc
description: Coverage: Taliouine
description: Coverage: XXe siècle
description: Temporal: XXe siècle
description: Bibliographic citation: « Peuplement juif de la circonscription de Taliouine », In Bulletin économique et social du Maroc (BESM), n° 54, 1952
description: Provenance: Maison méditerranéenne des sciences de l'homme, Cité numérique de la Méditerranée (Cinumed), Bibliothèque nationale du Royaume du Maroc (BNRM)
description: Provenance: https://cinumed.mmsh.univ-aix.fr/
Bose-Einstein condensation at constant temperature
Creators: name: Erhard, M.
name: Schmaljohann, H.
name: Kronjäger, J.
name: Bongs, K.
name: Sengstock, K.
Publisher: name: arXiv
Year: 2004
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: We present a novel experimental approach to Bose-Einstein condensation by increasing the particle number of the system at almost constant temperature. In particular the emergence of a new condensate is observed in multi-component F=1 spinor condensates of 87-Rb. Furthermore we develop a simple rate-equation model for multi-component BEC thermodynamics at finite temperature which well reproduces the measured effects.
description: 4 pages, 3 figures, RevTeX