cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Blaszakzercon : KEMAL & KOCAK 2009
Creators: name: Ujvári, Zs.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Mesostigmata
Zerconidae
Blaszakzercon

description: Blaszakzercon KEMAL & KOÇAK, 2009
 Allozercon BŁASZAK, 1984: 596.
 Allozercon: BŁASZAK et al., 1995: 254; LINDQUIST et MORAZA, 1998: 210; DÍAZ- AGUILAR et UJVÁRI, 2010: 26.
 Blaszakia: KOÇAK & KEMAL, 2008: 5. nom. nov. pro Allozercon BŁASZAK, 1984 non Allozercon VITZTHUM, 1926.
 Blaszakzercon: KEMAL & KOÇAK, 2009: 10. nom. nov. pro Blaszakia KOÇAK & KEMAL, 2008 non Blaszakia SKORACKI & SIKORA, 2008.
 Type species: Allozercon pulcher BŁASZAK, 1984: 596, by original designation.
 Diagnosis. Podonotal shield carapace-like. Peritrematal shields of female separated from dorsal shields by a triangular slit of membranous cuticle, their posterolateral tips expanded posteriorly. Peritrematal shields of male fused laterally to the ventrianal shield. Peritremes expanded to anterior half of coxae III, straight or slightly bent. Setae r1 and r3 shifted ventrally to peritrematal shields, both short, smooth (or finely barbed). Glands gv2 situated on small adgenital platelets. Ventrianal shield bearing 19 setae, setae Zv1 absent. Glands gv3 situated (antero) laterally to adanal setae. Setae z1 absent. Margin of opisthonotum with seven pairs of R-setae. Glands Po3 situated between setae J4 and Z3. Females characteristically possess strongly sclerotized, lobe-like structures covering the lateral pair of posterodorsal cavities. Epistome of Zercon - type (see UJVÁRI 2011).
description: Published as part of Ujvári, Zs., 2012, Review Of The American Genera Aspar Halašková, 1977 And Blaszakzercon Kemal & Koçak, 2009 (Acari, Mesostigmata, Zerconidae) With Description Of Three New Species, pp. 275-296 in Acta Zoologica Academiae Scientiarum Hungaricae 58 (3) on page 283, DOI: 10.5281/zenodo.5735834
Exactly Soluble Model for Nuclear Liquid-Gas Phase Transition
Creators: name: Bugaev, K. A.
name: Gorenstein, M. I.
name: Mishustin, I. N.
name: Greiner, W.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Nuclear Theory (nucl-th)
subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: Thermodynamical properties of nuclear matter undergoing multifragmentation are studied within a simplified version of the statistical model. An exact analytical solution has been found for the grand canonical ensemble. Excluded volume effects are taken into account in the thermodynamically self-consistent way. In thermodynamic limit the model exhibits a first order liquid-gas phase transition with specific mixed phase properties. An extension of the model including the Fisher's term is also studied. The possibility of the second order phase transition at or above the critical point is demonstrated. The fragment mass distributions in the different regions of the phase diagram are discussed.
description: 15 pages
Additional file 1 of Clinical characteristics of hypertrophic cranial pachymeningitis in granulomatosis with polyangiitis: a retrospective single-center study in China
Creators: name: Chen, Yiran
name: Gou, Lijuan
name: Wang, Li
name: Qian, Min
name: Wu, Qingjun
name: Zheng, Wenjie
name: Li, Mengtao
name: Zeng, Xiaofeng
name: Zhang, Fengchun
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Cell Biology
subject: Neuroscience
subject: Immunology
subject: FOS: Clinical medicine
subject: Science Policy
subject: Mental Health
subject: Hematology
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1: Table S1. Supplementary data on binary logistic regression analysis for GPA patients with HCP (method ‘forward conditional’). Table S2. Binary logistic regression analysis for GPA patients with HCP (method ‘enter’).
Diffusion of inertia-gravity waves by geostrophic turbulence
Creators: name: Kafiabad, Hossein
name: Savva, Miles A. C.
name: Vanneste, Jacques
Publisher: name: arXiv
Year: 2019
Subjects: subject: Atmospheric and Oceanic Physics (physics.ao-ph)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: The scattering of inertia-gravity waves by large-scale geostrophic turbulence in a rapidly rotating, strongly stratified fluid leads to the diffusion of wave energy on the constant-frequency cone in wavenumber space. We derive the corresponding diffusion equation and relate its diffusivity to the wave characteristics and the energy spectrum of the turbulent flow. We check the predictions of this equation against numerical simulations of the three-dimensional Boussinesq equations in initial-value and forced scenarios with horizontally isotropic wave and flow fields. In the forced case, wavenumber diffusion results in a $k^{-2}$ wave energy spectrum consistent with as-yet-unexplained features of observed atmospheric and oceanic spectra.
ISOCAM-CVF 5-12 mum Spectroscopy of Ultraluminous Infrared Galaxies
Creators: name: Tran, Q. D.
name: Lutz, D.
name: Genzel, R.
name: Rigopoulou, D.
name: Spoon, H. W. W.
name: Sturm, E.
name: Gerin, M.
name: Hines, D. C.
name: Moorwood, A. F. M.
name: Sanders, D. B.
name: Scoville, N.
name: Taniguchi, Y.
name: Ward, M.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present low resolution mid infrared spectra of 16 ultraluminous infrared galaxies (ULIRGs) obtained with the CVF spectroscopy mode of ISOCAM on board the Infrared Space Observatory ISO. Our sample completes previous ISO spectroscopy of ultra- and hyperluminous infrared galaxies towards higher luminosities. The combined samples cover an infrared luminosity range of \~10^{12 -13.1} Lo. For about half of the high luminosity ULIRGs studied here, strong aromatic emission bands suggest starburst dominance. Other spectra are dominated by a strong AGN-related continuum with weak superposed emission features of uncertain nature. An improved method to quantitatively characterize the relative contribution of star formation and AGN activity to the mid-infrared emission of ULIRGs is presented. As dominant source of the bolometric luminosity, starbursts prevail at the lower end and AGNs at the higher end of this range. The transition between mostly starburst and mostly AGN powered occurs at ~10^{12.4}$ to $10^{12.5} Lo, and individual luminous starbursts are found up to ~10^{12.65} Lo.
description: Accepted for publication in ApJ, 42 pages, 13 figures, 5 tables
SPLOT: a Snapshot survey for Polarised Light in Optical Transients
Creators: name: Higgins, A. B.
name: Wiersema, K.
name: Covino, S.
name: Starling, R. L. C.
name: Stevance, H. F.
name: Wyrzykowski, Ł.
name: Hodgkin, S. T.
name: Maund, J. R.
name: O'Brien, P. T.
name: Tanvir, N. R.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present SPLOT, a small scale pilot survey to test the potential of snapshot (single epoch) linear imaging polarimetry as a supplementary tool to traditional transient follow-up. Transients exist in a vast volume of observational parameter space and polarimetry has the potential to highlight sources of scientific interest and add value to near real-time transient survey streams. We observed a sample of $\sim 50$ randomly selected optical transients with the EFOSC2 and SofI instruments, on the 3.6m New Technology Telescope (NTT) to test the feasibility of the survey. Our sample contained a number of interesting individual sources: a variety of supernovae, X-ray binaries, a tidal disruption event, blazar outbursts, and, by design, numerous transients of unknown nature. We discuss the results, both for the individual sources and the survey in detail. We provide an overview on the success and limitations of SPLOT and also describe a novel calibration method for removing instrumental polarisation effects from Nasymth-mounted telescopes. We find that a SPLOT-like survey would be a benefit to the large scale future transient survey streams such as LSST. The polarimetric measurements have added scientific value to a significant number of the sources and, most importantly, has shown the potential to highlight unclassified transient sources of scientific interest for further study.
description: Accepted in MNRAS. 20 pages, 10 figures, 3 tables. Also contains a 10 page, two part appendix with unpolarised standard star measurements used for calibration (A) and individual source information and light curves (B). Corrected more typos
HUBUNGAN PEMBERDAYAAN IBU PEMANTAU JENTIK (BUMANTIK) DENGAN INDIKATOR KEBERHASILAN PEMBERANTASAN SARANG NYAMUK (PSN) DI KELURAHAN WONOKROMO SURABAYA
Creators: name: Efendi, Ferry
name: Rini, Arta Sapta
name: M.Has, Eka Misbahatul
Publisher: name: figshare
Year: 2019
Subjects: subject: 111799 Public Health and Health Services not elsewhere classified
subject: FOS: Health sciences

description: Introduction : Mother larvae observer (Bumantik) empowerment is an effort empower communities to establish independency of the community in health, especially elimination of Dengue Hemorrhagic Fever (DHF). Although most of the household (RT) good enough in conducting of 3M Plus, but this activity has not been optimally. This study aims to clarify the relationship of empowerment Bumantik with indicators of mosquito breeding eradication (PSN) in the Wonokromo Village, Surabaya.Method: Design used in this study was cross sectional design. The population was all cadre Bumantik at RW 6 Wonokromo Village, Surabaya. Samples were collected by using the Total Sampling as many as 35 respondents. Data was collected using questionnaires and secondary data from the cadre Bumantik, and analyzed using a statistical test of correlation coefficient Cramer's V contingency with a significant level of p £0.01.Results: Results of analysis showed that no relation empowerment Bumantik with indicators larvae free rate (ABJ) (p = 0.588), an indicator of the Container Index (CI) (p = 0.512), 3M Plus activity indicators (p = 0.806).Conclusion: Bumantik empowerment is not related to indicators of ABJ, CI, and 3M Plus. This is caused by various factors affecting the success of the mosquito breeding eradication, so that local communities should also be considered.
Diamond Detectors for Direct Detection of Sub-GeV Dark Matter
Creators: name: Kurinsky, Noah
name: Yu, To Chin
name: Hochberg, Yonit
name: Cabrera, Blas
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: We propose to use high-purity lab-grown diamond for the detection of sub-GeV dark matter. Diamond targets can be sensitive to both nuclear and electron recoils from dark matter scattering in the MeV and above mass range, as well as to absorption processes of dark matter with masses between sub-eV to 10's of eV. Compared to other proposed semiconducting targets such as germanium and silicon, diamond detectors can probe lower dark matter masses via nuclear recoils due to the lightness of the carbon nucleus. The expected reach for electron recoils is comparable to that of germanium and silicon, with the advantage that dark counts are expected to be under better control. Via absorption processes, unconstrained QCD axion parameter space can be successfully probed in diamond for masses of order 10 eV, further demonstrating the power of our approach.
description: 17 pages, 8 figures, submitted to PRD
How IT allows E-Participation in Policy-Making Process
Creators: name: Mukherjee, Sourav
Publisher: name: figshare
Year: 2019
Subjects: subject: 160510 Public Policy
subject: FOS: Political science
subject: 160505 Economic Development Policy
subject: 160511 Research, Science and Technology Policy

description: e-governance is the product of information and communication technology (ICT) for providing government public services, information exchange, communication operations, incorporation of various systems and services to customers or to other businesses. This is nothing but governance in an electronic environment using electronic media and tools. Generally, the goals of the e-Governance are: · Serving the citizens through a better model · Leading towards transparency and accountability. · Enhance efficiency within government · Develop suitable connectivity between business and industry. Due to the growing use of computers, Internets, smartphones, changes our lifestyle and the way we undertake and execute any work, learn and respond. Around the world, governments are started to realize the benefits of the value of e-governance. If this is designed and implemented appropriately, the e-governance process can greatly benefit the people in terms of delivering high-quality government services, simplifying the government regulations, improving the citizen participation, creating an enabling trust in the government, and so on. For that reason, policymakers and other officials are looking to implement e-Government in countries around the world. Regarding e-empowerment, e-petitions and e-referenda are two possible ways for the collection of citizen opinions and remarks to control policy. The expansion of online populations of interest, in which certain policy concerns are debated and different proposals are devised all over again based on discussion forums, are also some instances of empowerment online. One of the most common ways to empower citizens are E-empowering. In this policy-making process, citizens are involved with encouraging active involvement and assisting bottom-up proposals to sway the political agenda. Since the bottom-up viewpoint, citizens are evolving as producers instead just users of the policy.
Limits on stable iron in Type$\,$Ia supernovae from NIR spectroscopy
Creators: name: Flörs, A.
name: Spyromilio, J.
name: Maguire, K.
name: Taubenberger, S.
name: Kerzendorf, W. E.
name: Dhawan, S.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We obtained optical and near-infrared spectra of Type$\,$Ia supernovae (SNe$\,$Ia) at epochs ranging from 224 to 496 days after the explosion. The spectra show emission lines from forbidden transitions of singly ionised iron and cobalt atoms. We used non-local thermodynamic equilibrium (NLTE) modelling of the first and second ionisation stages of iron, nickel, and cobalt to fit the spectra using a sampling algorithm allowing us to probe a broad parameter space. We derive velocity shifts, line widths, and abundance ratios for iron and cobalt. The measured line widths and velocity shifts of the singly ionised ions suggest a shared emitting region. Our data are fully compatible with radioactive $^{56}$Ni decay as the origin for cobalt and iron. We compare the measured abundance ratios of iron and cobalt to theoretical predictions of various SN$\,$Ia explosion models. These models include, in addition to $^{56}$Ni, different amounts of $^{57}$Ni and stable $^{54,56}$Fe. We can exclude models that produced only $^{54,56}$Fe or only $^{57}$Ni in addition to $^{56}$Ni. If we consider a model that has $^{56}$Ni, $^{57}$Ni, and $^{54,56}$Fe then our data imply that these ratios are $^{54,56}$Fe / $^{56}$Ni $=0.272\pm0.086$ and $^{57}$Ni / $^{56}$Ni $=0.032\pm0.011$.
description: 10 pages, 7 figures, Accepted for publication in A&A
Deviations from linear theory for fluctuations below the supercritical primary bifurcation to electroconvection
Creators: name: Scherer, Michael A.
name: Ahlers, Guenter
name: Hoerner, Frank
name: Rehberg, Ingo
Publisher: name: arXiv
Year: 2000
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We report measurements of thermally-induced mean-square director-angle fluctuations below primary supercritical bifurcations to electroconvection of the nematic liquid crystals I52 and "Merck Phase V". For epsilon_mf = V^2/V_c,mf^2 - 1 < -0.1 (V is the amplitude of the applied alternating voltage) we find proportional to epsilon_mf^(-gamma) with gamma given by linear theory (LT). Closer to the bifurcation there are deviations from LT with a smaller gamma and with V_c^2 > V_c,mf^2. For I52 measurements as a function of the conductivity sigma of above V_c^2 suggest a tricritical bifurcation at sigma_t = 4.0 x 10^(-9) Omega^(-1)m^(-1), and (V_c^2 - V_c,mf^2)/V_c^2 increases strongly as sigma_t is approached from above.
description: 4 pages, 5 figures, submitted to Phys. Rev. Lett
WGS of XDR in Beijing
Creators: name: 郭海萍(Guohaiping)
Publisher: name: CNGB
Year: 2025
Subjects: Raw sequence reads
Other
the genomic DNA of XDR strains
Medical

description: Samples were originated from XDR-TB patients with positive cultures in the Beijing Chest Hospital ,Beijing Changping District Tuberculosis Prevention and Control Institute and Beijing Institute of Tuberculosis Control and Prevention between 2014 and 2020.Minimum inhibitory concentrations(MIC) to multiple drugs were determined using 7H9 broth microdilution.WGS was used to determine the clustered strains and mutations conferring drug resistance
Machine learning-based vorticity evolution and superresolution of homogeneous isotropic turbulence using wavelet projection
Creators: name: Asaka, Tomoki
name: Yoshimatsu, Katsunori
name: Schneider, Kai
Publisher: name: arXiv
Year: 2024
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences
subject: 76F05, 76F65, 68T05, 68T07, 65T60

description: A wavelet-based machine learning method is proposed for predicting the time evolution of homogeneous isotropic turbulence where vortex tubes are preserved. Three-dimensional convolutional neural networks and long short-term memory are trained with a time series of direct numerical simulation (DNS) data of homogeneous isotropic turbulence at the Taylor microscale Reynolds number 92. The predicted results are assessed by using flow visualization of vorticity and statistics, e.g., probability density functions of vorticity and enstrophy spectra. It is found that the predicted results are in good agreement with DNS results. The small-scale flow topology considering the second and third invariant of the velocity gradient tensor likewise shows an approximate match. Furthermore, we apply the pre-trained neural networks to coarse-grained vorticity data using superresolution. It is shown that the superresolved flow field well agrees with the reference DNS field and thus small-scale information and vortex tubes are well regenerated.
description: 34 pages, 18 figures
A 6.7 GHz methanol maser survey of the central molecular zone
Creators: name: Rickert, Matthew
name: Yusef-Zadeh, F.
name: Ott, J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The Central Molecular Zone (CMZ) spans the inner ~450 pc (3 degrees) of our Galaxy. This region is defined by its enhanced molecular emission and contains 5% of the entire Galaxy's molecular gas mass. However, the number of detected star forming sites towards the CMZ may be low for the amount of molecular gas that is present, and improved surveys of star formation indicators can help clarify this. With the Karl G Jansky Very Large Array (VLA), we conducted a blind survey of 6.7 GHz methanol masers spanning the inner 3deg x 40arcmin (450 pc x 100 pc) of the Galaxy. We detected 43 methanol masers towards 28 locations, 16 of which are new detections. The velocities of most of these masers are consistent with being located within the CMZ. A majority of the detected methanol masers are distributed towards positive Galactic longitudes, similar to 2/3 of the molecular gas mass distributed at positive Galactic longitudes. The 6.7 GHz methanol maser is an excellent indicator of high mass (>8 solar mass) star formation, with new detections indicating sites of massive star formation in the CMZ.
description: 18 pages, 9 figures, 3 tables, MNRAS (in press)
Superconducting Material Diagnostics using a Scanning Near-Field Microwave Microscope
Creators: name: Anlage, Steven M.
name: Steinhauer, D. E.
name: Vlahacos, C. P.
name: Feenstra, B. J.
name: Thanawalla, A. S.
name: Hu, Wensheng
name: Dutta, Sudeep K.
name: Wellstood, F. C.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We have developed scanning near-field microwave microscopes which can image electrodynamic properties of superconducting materials on length scales down to about 2 $μ$m. The microscopes are capable of quantitative imaging of sheet resistance of thin films, and surface topography. We demonstrate the utility of the microscopes through images of the sheet resistance of a YBa2Cu3O7-d thin film wafer, images of bulk Nb surfaces, and spatially resolved measurements of Tc of a YBa2Cu3O7-d thin film. We also discuss some of the limitations of the microscope and conclude with a summary of its present capabilities.
description: 6 pages with 9 figures, Proceedings of the Applied Superconductivity Conference 1998
Co-existence of spin semi-metallic and Weyl semi-metallic behavior in FeRhCrGe
Creators: name: Venkateswara, Y.
name: Samatham, S. Shanmukharao
name: Babu, P. D.
name: Suresh, K. G.
name: Alam, Aftab
Publisher: name: arXiv
Year: 2019
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: In this letter, we report the discovery of a new class of spintronic materials, namely spin semi-metals (SSM), employing both theoretical and experimental tools. The band structure of this class of materials is such that one of the spin bands resembles that of a semi-metal, while the other is similar to that of an insulator/semiconductor. This report is the experimental verification of the first SSM, FeRhCrGe, a quaternary Heusler alloy with a magnetic moment 3 $μ_B$ and a Curie temperature of 550 K. The measurement below 300 K shows nearly temperature independent conductivity and a relatively moderate Hall effect. SSM behavior for FeRhCrGe is also confirmed by rigorous first principles calculations. Band structure calculations also reveal that the spin up (semi metallic) band has combined features of type II Weyl and nodal line semimetal. As such, this study opens up the possibility of a new class of material with combined spintronic and topological properties, which is important both from fundamental and applied point of view.
description: 7 figures, quaternary Heusler alloys, ferromagnetic materials, spintronics, spin semi-metals, Weyl semimetal, nodal line semimetal
BMMB-2017.pdf
Creators: name: Lee, Chung-Hao
name: Zhang, Will
name: Feaver, Kristen
name: Gorman, Robert C.
name: Gorman, Joseph H.
name: Sacks, Michael
Publisher: name: Health Research Alliance
Year: 2019
Subjects: subject: 110601 Biomechanics
subject: FOS: Health sciences

description: There continues to be a critical need for developing data-informed computational modeling techniques that enable systematic evaluations of mitral valve (MV) function. This is important for a better understanding of MV organ-level biomechanical performance, in vivo functional tissue stresses, and the biosynthetic responses of MV interstitial cells (MVICs) in the normal, pathophysiological, and surgically repaired states. In the present study, we utilized extant ovine MV population-averaged 3D fiducial marker data to quantify the MV anterior leaflet (MVAL) deformations in various kinematic states. This approach allowed us to make the critical connection between the in vivo functional and the in vitro experimental configurations. Moreover, we incorporated the in vivo MVAL deformations and pre-strains into an enhanced inverse finite element modeling framework (Path 1) to estimate the resulting in vivo tissue prestresses …
Beyond Social Media Analogues
Creators: name: Dickinson, Gregory M.
Publisher: name: arXiv
Year: 2024
Subjects: subject: General Economics (econ.GN)
subject: FOS: Economics and business

description: The steady flow of social-media cases toward the Supreme Court shows a nation reworking its fundamental relationship with technology. The cases raise a host of questions ranging from difficult to impossible: how to nurture a vibrant public square when a few tech giants dominate the flow of information, how social media can be at the same time free from conformist groupthink and also protected against harmful disinformation campaigns, and how government and industry can cooperate on such problems without devolving toward censorship.
 To such profound questions, this Essay offers a comparatively modest contribution -- what not to do. Always the lawyer's instinct is toward analogy, considering what has come before and how it reveals what should come next. Almost invariably, that is the right choice. The law's cautious evolution protects society from disruptive change. But almost is not always, and, with social media, disruptive change is already upon us. Using social-media laws from Texas and Florida as a case study, this Essay shows how social-media's distinct features render it poorly suited to analysis by analogy and argues that courts should instead shift their attention toward crafting legal doctrines targeted to address social media's unique ills.
title: Negative concord in child African American English: Implications for Specific Language Impairment
Creators: name: Coles-White, D'Jaris
Publisher: name: University of Massachusetts Amherst
Year: 2004
Subjects: subject: negation
subject: AAE
subject: child language
subject: linguistic differences

description: In this study, African American English (AAE)-speaking children’s comprehension of 2 different types of double negative sentences was examined and contrasted with that of a comparison group of Standard American English (SAE)-speaking children. The first type of double negative, negative concord, involves 2 negative elements in a sentence that are interpreted together as single negation. The second type of double negative, called true double negation, involves 2 negatives that are interpreted as independent negatives. A cross-sectional cohort of 61 (35 AAE, 26 SAE) typically developing children ranging in age from 5;2 (years;months) to 7;11 participated. The children responded to story-based grammatical judgment tasks that required them to differentiate between negative concord and true double negation. Results revealed no statistically significant differences between AAE- and SAE-speaking children in the way they interpreted negative concord and true double negation. However, there were significantly more correct responses to negative concord sentences across combined groups. In particular, the older children (i.e., 7-year-olds) produced more correct responses to negative concord than did the younger group (i.e., 5-year-olds). Explanations for these findings are framed in terms of children’s knowledge about sentences with 2 negatives, the constraints affecting the interpretation of 2 negatives that include negative concord, and the clinical importance of negative concord for assessing specific language impairment in child AAE speakers
Jet stability and the generation of superluminal and stationary components
Creators: name: Agudo, I.
name: Gomez, J. L.
name: Marti, J. M.
name: Ibanez, J. M
name: Marscher, A. P.
name: Alberdi, A.
name: Aloy, M. A.
name: Hardee, P. E.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a numerical simulation of the response of an expanding relativistic jet to the ejection of a superluminal component. The simulation has been performed with a relativistic time-dependent hydrodynamical code from which simulated radio maps are computed by integrating the transfer equations for synchrotron radiation. The interaction of the superluminal component with the underlying jet results in the formation of multiple conical shocks behind the main perturbation. These trailing components can be easily distinguished because they appear to be released from the primary superluminal component, instead of being ejected from the core. Their oblique nature should also result in distinct polarization properties. Those appearing closer to the core show small apparent motions and a very slow secular decrease in brightness, and could be identified as stationary components. Those appearing farther downstream are weaker and can reach superluminal apparent motions. The existence of these trailing components indicates that not all observed components necessarily represent major perturbations at the jet inlet; rather, multiple emission components can be generated by a single disturbance in the jet. While the superluminal component associated with the primary perturbation exhibits a rather stable pattern speed, trailing components have velocities that increase with distance from the core but move at less than the jet speed. The trailing components exhibit motion and structure consistent with the triggering of pinch modes by the superluminal component.
description: Accepted by ApJ Letters. LaTeX, 19 pages, 4 PostScript figures
Leptocera atra
Creators: name: Papp, L.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Sphaeroceridae
Leptocera
Leptocera atra

description: Leptocera atra (VANSCHUYTBROECK, 1951)
 Paracollinella atra VANSCHUYTBROECK, 1951: 7. Type locality: Zaire, Élisabethville (= Lubumbashi). The holotype male is deposited int the Collection of the IRSN.
 Leptocera (Leptocera) nigricorpus RICHARDS, 1980: 619 [unnecessary new name for Paracollinella atra VANSCHUYTBROECK, 1951, in Leptocera a secondary junior homonym of Limosina atra ADAMS, 1903, now Rachispoda atra (ADAMS, 1903)].
 For detailed synonymy see ROHÁČEK et al. 2001: 151.
Material studied: 2 female paratypes (one of them without head, HNHM): Congo belge, Eala-XI–1936, J. Ghesquière – P. Vanschuytbroeck det. 1951, Paracollinella atra Vansch. – [red] Paratype – cf. Bull. Inst. Sc. Nat. Belg. T. XXVII, n° 41, 1951, p. 7.
An easily identifiable species, which appears to be rare and restricted to the Congo Basin.
Hitherto only known from the type locality (Zaire).
description: Published as part of Papp, L., 2012, A Review Of The Afrotropical Species Of Leptocera Olivier (Diptera: Sphaeroceridae), pp. 225-258 in Acta Zoologica Academiae Scientiarum Hungaricae 58 (3) on pages 227-228, DOI: 10.5281/zenodo.5735888
Damage spreading and Lyapunov exponents in cellular automata
Creators: name: Bagnoli, F.
name: Rechtman, R.
name: Ruffo, S.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: Using the concept of the Boolean derivative we study damage spreading for one dimensional elementary cellular automata and define their maximal Lyapunov exponent. A random matrix approximation describes quite well the behavior of ``chaotic'' rules and predicts a directed percolation-type phase transition. After the introduction of a small noise elementary cellular automata reveal the same type of transition.
title: The effect of tuition fees on university graduation
Creators: name: Bachmeier, Marc
name: Marcus, Jan
Publisher: name: Hertie School
Year: 2025

description: This paper examines the impact of tuition fees on graduation rates among high-school leavers. We analyse the introduction of fees in several German states in 2006-07 (around EUR 1,000 annually), using administrative microdata on all university graduates and a difference-in-differences approach. The share of high-school leavers graduating fell by 1.8 percentage points, which is less than the 3.2-percentage point drop in enrolment, indicating many deterred students would not have graduated without fees. This underscores the importance of studying not only enrolment but also graduation rates, particularly in systems with high dropout rates and ``ghost students''–students enrolling primarily for non-educational benefits.
description: Berlin School of Economics Discussion Papers; 61
HUBUNGAN DUKUNGAN SOSIAL DENGAN KONSEP DIRI PADA ANAK JALANAN DI RUMAH SINGGAH SANGGAR ALANG-ALANG SURABAYA
Creators: name: Efendi, Ferry
name: Maharani, Reny
name: Retno Indarwati
Publisher: name: figshare
Year: 2019
Subjects: subject: 170106 Health, Clinical and Counselling Psychology
subject: FOS: Psychology
subject: 111712 Health Promotion
subject: FOS: Health sciences

description: Introduction: Self concept of street children was a conceptualization that worked by human into theirselves. Environment around street children could affect their self concept formation process. Human self concept developedby the time periode. Street children could have positive self concept if they got social support from their close environment.Methods: This study aimed to identified the relationship between social support with self concept of street children and analyzed relationship between both variables. This study used cross-sectoinal design. Samples were street children in SanggarAlang-alang, Surabaya. Sample size were 30 individuals, recruited using purposive sampling. Data were collected through questionnare and analyzed by means of Spearmen Rho statistical test with significance level of α<0,05.Result: Result of the research there was relationship between social support with self concept in street children with significance level p = 0.000 it means the relationship between two variable was reliable. The limitation in this research was too small sample to be used.Discussion: It could be conclude from this study that there was relationship between social support with self concept in street children. Further studies should involve more respondents and use standardized instrument to obtain better result.
Additional file 1 of A preliminary exploration on the mechanism of the carbapenem-resistance transformation of Serratia marcescens in vivo
Creators: name: Xu, Qian
name: Zheng, Beiwen
name: Li, Kaixuan
name: Shen, Ping
name: Xiao, Yonghong
Publisher: name: figshare
Year: 2024
Subjects: subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Biotechnology
subject: Evolutionary Biology
subject: Ecology
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences

description: Supplementary Material 1
A Change of Scenery: Transformative Insights from Retrospective VR Embodied Perspective-Taking of Conflict With a Close Other
Creators: name: Yong, Seraphina
name: Cui, Leo
name: Rosenberg, Evan Suma
name: Yarosh, Svetlana
Publisher: name: arXiv
Year: 2024
Subjects: subject: Human-Computer Interaction (cs.HC)
subject: FOS: Computer and information sciences

description: Close relationships are irreplaceable social resources, yet prone to high-risk conflict. Building on findings from the fields of HCI, virtual reality, and behavioral therapy, we evaluate the unexplored potential of retrospective VR-embodied perspective-taking to fundamentally influence conflict resolution in close others. We develop a biographically-accurate Retrospective Embodied Perspective-Taking system (REPT) and conduct a mixed-methods evaluation of its influence on close others' reflection and communication, compared to video-based reflection methods currently used in therapy (treatment as usual, or TAU). Our key findings provide evidence that REPT was able to significantly improve communication skills and positive sentiment of both partners during conflict, over TAU. The qualitative data also indicated that REPT surpassed basic perspective-taking by exclusively stimulating users to embody and reflect on both their own and their partner's experiences at the same level. In light of these findings, we provide implications and an agenda for social embodiment in HCI design: conceptualizing the use of `embodied social cognition,' and envisioning socially-embodied experiences as an interactive context.
description: 18 pages, 5 figures, Proceedings of the 2024 CHI Conference on Human Factors in Computing Systems
Experimental nuclear astrophysics in Italy
Creators: name: Broggini, C.
name: Straniero, O.
name: Taiuti, M. G. F.
name: de Angelis, G.
name: Benzoni, G.
name: Bruno, G. E.
name: Bufalino, S.
name: Cardella, G.
name: Colonna, N.
name: Contalbrigo, M.
name: Cosentino, G.
name: Cristallo, S.
name: Curceanu, C.
name: De Filippo, E.
name: Depalo, R.
name: Di Leva, A.
name: Feliciello, A.
name: Gammino, S.
name: Galatà, A.
name: La Cognata, M.
name: Lea, R.
name: Leoni, S.
name: Lombardo, I.
name: Manzari, V.
name: Mascali, D.
name: Massimi, C.
name: Mengoni, A.
name: Mengoni, D.
name: Napoli, D. R.
name: Palmerini, S.
name: Piano, S.
name: Pirrone, S.
name: Pizzone, R. G.
name: Politi, G.
name: Prati, P.
name: Prete, G.
name: Russotto, P.
name: Tagliente, G.
name: Urciuoli, G. M.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Nuclear astrophysics, the union of nuclear physics and astronomy, went through an impressive expansion during the last twenty years. This could be achieved thanks to milestone improvements in astronomical observations, cross section measurements, powerful computer simulations and much refined stellar models. Italian groups are giving quite important contributions to every domain of nuclear astrophysics, sometimes being the leaders of worldwide unique experiments. In this paper we will discuss the astrophysical scenarios where nuclear astrophysics plays a key role and we will provide detailed descriptions of the present and future of the experiments on nuclear astrophysics which belong to the scientific programme of INFN (the National Institute for Nuclear Physics in Italy).
description: Added paragraphs 5.6 and 7.2. Paragraph 7.3 (former 7.2) revised. Accepted for publication in La Rivista del Nuovo Cimento
The inner nebula and central binary of the symbiotic star HM Sge
Creators: name: Eyres, S. P. S.
name: Bode, M. F.
name: Taylor, A. R.
name: Crocker, M. M.
name: Davis, R. J.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present contemporaneous HST WFPC2 and VLA observations of the symbiotic nova HM Sge. We identify a number of discreet features at spatial scales smaller than approximately 0.1 arcsec embedded in the extended nebula, with radio and optical emission well correlated in the inner 1 arcsec. For the first time we measure the positions of the binary components of a symbiotic star directly. We estimate the projected angular binary separation to be 40+/-9 milli-arcsec, with the binary axis at position angle 130+/-10 degrees. The latter is consistent with previous estimates made by indirect methods. The binary separation is consistent with a previous estimate of 50 au if the distance is 1250+/-280 pc. Temperature and density diagnostics show two distinct regions in the surrounding nebula, with a cool wedge to the south-west. An extinction map indicates the true interstellar extinction to be no more than E(B-V) = 0.35. This is consistent with a minimum distance of approximatelly 700 pc, but this would be reduced if there is a circumstellar contribution to the minimum in the extinction map. The extinction map also suggests a patchy dust distribution. We suggest that a southern concentration of dust and the south-west wedge are associated with the cool component wind. Alternatively, the southern dust concentration is the cause of the cool wedge, as it shields part of the nebula from the hot component radiation field.
description: 13 pages including 4 figures. To be published in ApJ vol. 551. Update to rescale Fig. 4
Additional file 1 of RACGAP1 promotes the progression and poor prognosis of lung adenocarcinoma through its effects on the cell cycle and tumor stemness
Creators: name: Liu, Yafeng
name: Han, Tao
name: Miao, Rui
name: Zhou, Jiawei
name: Guo, Jianqiang
name: Xu, Zhi
name: Xing, Yingru
name: Bai, Ying
name: Wu, Jing
name: Hu, Dong
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Cancer

description: Supplementary Material 1
The long delayed solution of the Bukhvostov Lipatov model
Creators: name: Saleur, H.
Publisher: name: arXiv
Year: 1998
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: In this paper I complete the solution of the Bukhvostov Lipatov model by computing the physical excitations and their factorized S matrix. I also explain the paradoxes which led in recent years to the suspicion that the model may not be integrable.
description: 9 pages
Dense gas is not enough: environmental variations in the star formation efficiency of dense molecular gas at 100pc scales in M51
Creators: name: Querejeta, M.
name: Schinnerer, E.
name: Schruba, A.
name: Murphy, E.
name: Meidt, S.
name: Usero, A.
name: Leroy, A. K.
name: Pety, J.
name: Bigiel, F.
name: Chevance, M.
name: Faesi, C. M.
name: Gallagher, M.
name: García-Burillo, S.
name: Glover, S. C. O.
name: Hygate, A. P. S.
name: Jiménez-Donaire, M. J.
name: Kruijssen, J. M. D.
name: Momjian, E.
name: Rosolowsky, E.
name: Utomo, D.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: It remains unclear what sets the efficiency with which molecular gas transforms into stars. Here we present a new VLA map of the spiral galaxy M51 in 33GHz radio continuum, an extinction-free tracer of star formation, at 3" scales (~100pc). We combined this map with interferometric PdBI/NOEMA observations of CO(1-0) and HCN(1-0) at matched resolution for three regions in M51 (central molecular ring, northern and southern spiral arm segments). While our measurements roughly fall on the well-known correlation between total infrared and HCN luminosity, bridging the gap between Galactic and extragalactic observations, we find systematic offsets from that relation for different dynamical environments probed in M51, e.g. the southern arm segment is more quiescent due to low star formation efficiency (SFE) of the dense gas, despite having a high dense gas fraction. Combining our results with measurements from the literature at 100pc scales, we find that the SFE of the dense gas and the dense gas fraction anti-correlate and correlate, respectively, with the local stellar mass surface density. This is consistent with previous kpc-scale studies. In addition, we find a significant anti-correlation between the SFE and velocity dispersion of the dense gas. Finally, we confirm that a correlation also holds between star formation rate surface density and the dense gas fraction, but it is not stronger than the correlation with dense gas surface density. Our results are hard to reconcile with models relying on a universal gas density threshold for star formation and suggest that turbulence and galactic dynamics play a major role in setting how efficiently dense gas converts into stars.
description: 23 pages, 9 figures, accepted for publication in A&A
Rachispoda basilewskyi Papp 2012, comb. n.
Creators: name: Papp, L.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Sphaeroceridae
Rachispoda
Rachispoda basilewskyi

description: Rachispoda basilewskyi (VANSCHUYTBROECK, 1962), comb. n.
 Paracollinella basilewskyi VANSCHUYTBROECK, 1962: 473.
 Leptocera basilewskyi: ROHÁČEK et al. 2001: 151.
Material studied: Holotype male (MRAC, double mounted on a long polyporus blicklet): 1) [yellowish] HOLOTYPUS m; 2) Coll. Mus. Congo, Tanganyika Terr.: Longido, Masai Distr., 1500 m. 17/ 20-IV–1957. 3) Mission Zoolog. I. R.S.A.C. en Afrique orientale (P. Basilewsky et N. Leleup); 4 [reddish] TYPE; 5) P. Vanschuytbroeck det., 195 “ Paracollinella m basilewskyi nsp.” [pencil hand-writing of P. V.]; 6) “ Rachispoda basilewskyi (Vanschuytbroeck, 1962) holotype L. Papp 2011”; 7) [reverse code label of MRAC] RMCA ENT 000016277. Some of its setae displaced or broken off, wings stuck together.
Paratype male (MRAC, abdomen and genitalia removed and kept in a plastic microvial with glycerol): 1) PARATYPUS m; 2)–3): same as on HT; 4) “ Paracollinella Basilewskyi n. sp. det. P. Vanschuytbroek [sic!] [handwriting with fine pen, P. V.]; 5) “ Rachispoda basilewskyi (Vanschuytbroeck, 1962) L. Papp 2011 ”. It is without head but otherwise well-preserved.
 This species is obviously a member of the R. fuscipennis group of Rachispoda. Foremost pair of dorsocentrals medially curved, scutellum with 8 larger and several short (mainly lateral marginal) setae. Facial plate bulging, bulbous prominent between antennae. Three strong pairs of interfrontal setae plus some short ones. I was able to detect 3 acrostichal macrochaetae. Discal cell with distinct posteroapical corner, paratype with minute vein stub there. Mid tibia with long ventral posteroapical bristle (similar to that of the Leptocera nigra species group). Ventral preapical seta of mid tibia much longer and thicker than ventral metatarsal seta. Hind tibia anterodorsally and posterodorsally with numerous long setae.
 A study of the male genitalia of the paratype confirmed that this species belongs to the Rachispoda fuscipennis species group.
Known only from the type locality (Tanzania).
description: Published as part of Papp, L., 2012, A Review Of The Afrotropical Species Of Leptocera Olivier (Diptera: Sphaeroceridae), pp. 225-258 in Acta Zoologica Academiae Scientiarum Hungaricae 58 (3) on pages 252-253, DOI: 10.5281/zenodo.5735888
How IT allows e-participation by Sourav Mukherjee_RG.docx
Creators: name: Mukherjee, Sourav
Publisher: name: figshare
Year: 2019
Subjects: subject: 160510 Public Policy
subject: FOS: Political science
subject: 160505 Economic Development Policy
subject: 160511 Research, Science and Technology Policy

description: e-governance is the product of information and communication technology (ICT) for providing government public services, information exchange, communication operations, incorporation of various systems and services to customers or to other businesses. This is nothing but governance in an electronic environment using electronic media and tools. Generally, the goals of the e-Governance are: · Serving the citizens through a better model · Leading towards transparency and accountability. · Enhance efficiency within government · Develop suitable connectivity between business and industry. Due to the growing use of computers, Internets, smartphones, changes our lifestyle and the way we undertake and execute any work, learn and respond. Around the world, governments are started to realize the benefits of the value of e-governance. If this is designed and implemented appropriately, the e-governance process can greatly benefit the people in terms of delivering high-quality government services, simplifying the government regulations, improving the citizen participation, creating an enabling trust in the government, and so on. For that reason, policymakers and other officials are looking to implement e-Government in countries around the world. Regarding e-empowerment, e-petitions and e-referenda are two possible ways for the collection of citizen opinions and remarks to control policy. The expansion of online populations of interest, in which certain policy concerns are debated and different proposals are devised all over again based on discussion forums, are also some instances of empowerment online. One of the most common ways to empower citizens are E-empowering. In this policy-making process, citizens are involved with encouraging active involvement and assisting bottom-up proposals to sway the political agenda. Since the bottom-up viewpoint, citizens are evolving as producers instead just users of the policy.