cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Closing the Light Gluino Window in Supersymmetric Grand Unified Models
Creators: name: Diaz, Marco Aurelio
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the light gluino scenario giving special attention to constraints from the masses of the light CP-even neutral Higgs $m_h$, the lightest chargino $m_{χ^{\pm}_1}$, and the second lightest neutralino $m_{χ^0_2}$, and from the $b\rightarrow sγ$ decay. We find that minimal $N=1$ supergravity, with a radiatively broken electroweak symmetry group and universality of scalar and gaugino masses at the unification scale, is incompatible with the existence of a light gluino.
description: 12 pages (plain tex), 1 figure not included, VAND-TH-94-7-R. An error is corrected. Modifications to the text and the figure are made
Additional file 1 of Aftershock analysis and forecasting for the crustal seismicity in Romania
Creators: name: Ghita, Cristian
name: Enescu, Bogdan
name: Marinus, Alexandru
name: Moldovan, Iren-Adelina
name: Ionescu, Constantin
name: Constantinescu, Eduard Gabriel
name: An, Like
Publisher: name: figshare
Year: 2025
Subjects: subject: Physical Sciences not elsewhere classified
subject: Neuroscience
subject: Biotechnology
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Mathematical Sciences not elsewhere classified
subject: Mental Health

description: Additional file 1.
Bulla amplustre Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Cephalaspidea
Bullidae
Bulla
Bulla amplustre

description: Bulla amplustre [spec. nov.]
B. testa subrotunda, spira elevata obtusa, fasciis incarnatis.
Gvalt. test. t. 13. f. FF.
List. conch. 4. s. 9. c. 10. t. 2. f. exterior.
Habitat in Asia.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 727, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Bulla hypnorum Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Cephalaspidea
Bullidae
Bulla
Bulla hypnorum

description: Bulla hypnorum [spec. nov.]
B. testa ovata pellucida sinistrorsa, spira prominente, apertura ovato-lanceolata.
Fn. svec. 1303.
Habitat in Europae Muscis humentibus.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on pages 727-728, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
title: Городской вандализм в цифровую эпоху: герои и злодеи
Creators: name: Симонова, Ирина
Publisher: name: Новгородский государственный университет имени Ярослава Мудрого (НовГУ)
Year: 2021

description: Вандализм, привычное явление для большинства современных городов, получил новое измерение благодаря возможностям демонстрации и последующего обсуждения вандальных актов в сети. Для молодежи это дает возможности как популяризировать свои «работы», так и становиться специфически организованным субъектом оценки вандальных действий. Нередко вандальные практики получают
широкую положительную оценку.
Dust scattering halo of 4U 1630-47 observed with Chandra and Swift: New constraints on the source distance
Creators: name: Kalemci, Emrah
name: Maccarone, Thomas J.
name: Tomsick, John A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We have observed the Galactic black hole transient 4U 1630-47 during the decay of its 2016 outburst with Chandra and Swift to investigate the properties of the dust scattering halo created by the source. The scattering halo shows a structure that includes a bright ring between 80" and 240" surrounding the source, and a continuous distribution beyond 250". An analysis of the $^{12}$CO $J=1-0$ map and spectrum in the line of sight to the source indicate that a molecular cloud with a radial velocity of -79 km s$^{-1}$ (denoted MC -79) is the main scattering body that creates the bright ring. We found additional clouds in the line of sight, calculated their kinematic distances and resolved the well known "near" and "far" distance ambiguity for most of the clouds. At the favored far distance estimate of MC -79, the modeling of the surface brightness profile results in a distance to 4U 1630-47 of 11.5 $\pm$ 0.3 kpc. If MC -79 is at the near distance, then 4U 1630-47 is at 4.7 $\pm$ 0.3 kpc. Future Chandra, Swift, and sub-mm radio observations not only can resolve this ambiguity, but also would provide information regarding properties of dust and distribution of all molecular clouds along the line of sight. Using the results of this study we also discuss the nature of this source and the reasons for the anomalously low soft state observation observed during the 2010 decay.
description: 12 pages, 12 figures, accepted for publication in Astrophysical Journal
The Accreting Object Database: Probing the Formation Mechanisms of Planets and (Sub-)Stellar Objects
Creators: name: Dacus, Beck
name: Plunkett, Cailin
name: Wang, Huichen
name: Follette, Kate
name: Ward-Duong, Kimberly
name: Robinson, Connor
name: Betti, Sarah
name: Peck, Anne
Publisher: name: Zenodo
Year: 2021

description: Comparing the relationship between accretion rate and mass in the stellar and substellar regimes is an effective strategy to identify the point at which the formation pathway for brown dwarfs diverges between planet-like and star-like formation mechanisms. To this end, we have assembled a comprehensive database of published accretion diagnostics for over 500 observations of almost 400 unique objects with masses ranging from 0.005 to 2 solar masses (including 64 brown dwarfs and 4 giant planets). The studies compiled in our database reveal a scatter of 4 orders of magnitude in the accretion rate vs. mass relationship in the brown dwarf regime. To explore the extent to which third variables, such as age, multiplicity, and intrinsic accretion variability explain the observed scatter, systematic errors due to differences in methodology must be eliminated. Using a uniform evolutionary model, we re-estimated masses and radii for brown dwarfs in the database using published spectral types and age estimates. We then re-estimated the accretion rate for each object by applying a uniform set of scaling relations and Gaia DR2 parallaxes to reported line fluxes and equivalent widths. Ongoing analyses seek to bolster the statistical sample in the database by incorporating additional studies, thoroughly account for and minimize systematic sources of error, calibrate different accretion diagnostics, and robustly analyze third effects with variable distributions now corrected for methodological differences. This database represents the most thorough compilation of literature studies of low-mass accretors to date, and is a valuable tool for future exploration of how formation properties vary across the substellar regime.
A Consistency Test of Spectroscopic Gravities for Late-Type Stars
Creators: name: Prieto, Carlos Allende
name: Lopez, Ramon J. Garcia
name: Lambert, David L.
name: Gustafsson, Bengt
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Chemical analyses of late-type stars are usually carried out following the classical recipe: LTE line formation and homogeneous, plane-parallel, flux-constant, and LTE model atmospheres. We review different results in the literature that have suggested significant inconsistencies in the spectroscopic analyses, pointing out the difficulties in deriving independent estimates of the stellar fundamental parameters and hence,detecting systematic errors. The trigonometric parallaxes measured by the HIPPARCOS mission provide accurate appraisals of the stellar surface gravity for nearby stars, which are used here to check the gravities obtained from the photospheric iron ionization balance. We find an approximate agreement for stars in the metallicity range -1 <= [Fe/H] <= 0, but the comparison shows that the differences between the spectroscopic and trigonometric gravities decrease towards lower metallicities for more metal-deficient dwarfs (-2.5 <= [Fe/H] <= -1.0), which casts a shadow upon the abundance analyses for extreme metal-poor stars that make use of the ionization equilibrium to constrain the gravity. The comparison with the strong-line gravities derived by Edvardsson (1988) and Fuhrmann (1998a) confirms that this method provides systematically larger gravities than the ionization balance. The strong-line gravities get closer to the physical ones for the stars analyzed by Fuhrmann, but they are even further away than the iron ionization gravities for the stars of lower gravities in Edvardsson's sample. The confrontation of the deviations of the iron ionization gravities in metal-poor stars reported here with departures from the excitation balance found in the literature, show that they are likely to be induced by the same physical mechanism(s).
description: AAS LaTeX v4.0, 35 pages, 10 PostScript files; to appear in The Astrophysical Journal
Additional file 3: of Fatty acid oxidation is associated with proliferation and prognosis in breast and other cancers
Creators: name: Aiderus, Aziz
name: Black, Michael
name: Dunbier, Anita
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy

description: Figure S1. FAO signature expression is not associated with ovarian cancer overall survival from the KMplotter analysis. (PDF 180Â kb)
A New Culprit in the Second Parameter Problem in the Sculptor Dwarf Spheroidal Galaxy?
Creators: name: Hurley-Keller, D.
name: Mateo, M.
name: Grebel, E.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Color-magnitude diagrams from deep, wide-field CCD photometry of the Sculptor dwarf spheroidal galaxy reveal that the red horizonal branch (RHB) stars are strongly concentrated towards the center of the galaxy relative to the dominant old population in Sculptor, confirming an earlier claim of such a gradient (Da Costa et al. 1996). Since we find no radial gradients of the age or metallicity distribution within Sculptor, neither age nor metallicity can individually account for the internal `second parameter' problem observed within the galaxy. We have also identified an unusual `spur' of stars that extends from the main sequence turnoff region and located between the canonical blue straggler region and the subgiant branch. These stars are also more centrally concentrated than the oldest stars in Sculptor, although not as extremely as the RHB stars. Unable to convincingly interpret the spur either as an unusual young population or as a foreground population of stars, we conclude that binary stars offer the most reasonable explanation for the origin of the spur that is also consistent with other features in the CMD of Sculptor. We infer that 30-60% of all apparently single stars in the inner region of Sculptor may be binaries. We speculate that the possible radial gradient in the binary-star population may be related to the variation of the HB morphology in Sculptor.
description: 12 pages, 2 figures; Accepted for publication in ApJ Letters
Carta Abierta
Creators: name: García Castaño, Alberto
Publisher: name: HIDDEN arts
Year: 2024
Subjects: Artes Escénicas
Acreditación profesorado
UNESCO
Comité de Danza
Investigación Artística

description: La Convención para la Salvaguardia del Patrimonio Cultural Inmaterial, acogida por la UNESCO en 2003, reconoció las "artes del espectáculo" como manifestaciones protegidas por el Derecho Internacional. En este contexto, el IDC/UNESCO (Comité Internacional de Danza) se dedica a preservar el patrimonio cultural inmaterial de la danza, promoviendo su estudio, práctica y apreciación global. La organización aboga por la innovación y preservación de la danza como un elemento identitario y diverso que promueve la paz y amistad mundial. Asimismo, enfatiza la investigación y la creación artística, destacando la importancia de la formación y conservación de creaciones artísticas de calidad para contribuir al desarrollo sostenible y al bienestar social.
Transverse Polarization of Top Quarks Produced at a Photon-Photon Collider
Creators: name: Bernreuther, W.
name: Ma, J. P.
name: McKellar, B. H. J.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: At future $γγ$ colliders copious production of $t \bar{t}$ pairs is possible. This would allow a detailed investigation of the interactions involving the top quark. We propose some orrelations which are sensitive to $t \bar{t}$ final state interactions and we compute the QCD and standard model Higgs boson contributions to these correlations. QCD induced transverse polarization of top quarks is found to be sizeable and measurable at a high-energy $e^+e^-$ collider with an integrated luminosity of 10 $({\rm fb})^{-1}$ which is converted into a photon collider by backscattering of laser photons.
description: 8 pages. No fig. Preprint UM-P-94/25 and PITHA 94/17
Bulla pallida Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Cephalaspidea
Bullidae
Bulla
Bulla pallida

description: Bulla pallida [spec. nov.]
B. testa cylindrica, spira elevata acuta.
Habitat ..
T. livida, longitudinaliter griseo undulata.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 727, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Additional file 1 of Quantitative evaluation of parotid gland dysfunction in patients with hyposalivation using magnetic resonance imaging mapping technique
Creators: name: Lee, Chena
name: Lee, Ari
name: Choi, Yoon Joo
name: Han, Sang-Sun
name: Cho, Hee Woo
name: Jeon, Kug Jin
Publisher: name: figshare
Year: 2025
Subjects: subject: Biophysics
subject: Space Science
subject: Physical Sciences not elsewhere classified
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Physiology
subject: Chemical Sciences not elsewhere classified

description: Supplementary Material 1
Additional file 1: of CNS-border associated macrophages respond to acute ischemic stroke attracting granulocytes and promoting vascular leakage
Creators: name: Pedragosa, Jordi
name: Salas-Perdomo, Angélica
name: Gallizioli, Mattia
name: Cugota, Roger
name: Miró-Mur, Francesc
name: Briansó, Ferran
name: Justicia, Carles
name: Pérez-Asensio, Fernando
name: Marquez-Kisinousky, Leonardo
name: Urra, Xabier
name: Gieryng, Anna
name: Bozena Kaminska
name: Chamorro, Angel
name: Planas, Anna
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Pharmacology
subject: Evolutionary Biology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Computational Biology

description: Extended methods, additional tables and figures.ᅟ(DOCX 6178 kb)
title: Роль мифа в формировании сценариев и образов будущего России в контексте стратегических вызовов и глобальных угроз
Creators: name: Ставицкий, А.
Publisher: name: Новгородский государственный университет имени Ярослава Мудрого (НовГУ)
Year: 2021

description: Статья рассматривает и раскрывает роль мифа в современном цифровом обществе с учетом результатов исследований ведущих мифологов. Они показывают, что миф играет в жизни человека и общества огромную роль, поскольку наполняют жизнь человека смыслом. Исходя из этого, можно утверждать, что в цифровом обществе миф становится механизмом решения проблем, фактором политики и мощнейшим оружием в сфере управления сознанием. Одним из ключевых направлений использования мифа является сфера формирования сценариев и образов будущего в контексте стратегических вызовов и глобальных угроз, которые могут привести к гибели человечества и ставят человека перед необходимостью смены парадигмы цивилизационного развития.
Tidally Compressed Gas in Centers of Early Type and Ultraluminous Galaxies
Creators: name: Das, Mousumi
name: Jog, Chanda J.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In this paper we propose that the compressive tidal field in the centers of flat-core early type galaxies and ultraluminous galaxies compresses molecular clouds producing dense gas obseved in the centers of these galaxies. The effect of galactic tidal fields is usually considered disruptive in the literature. However, for some galaxies, the mass profile flattens towards the center and the resulting galactic tidal field is not disruptive but instead it is compressive within the flat-core region. We have used the virial theorem to determine the minimum density of a molecular cloud to be stable and gravitationally bound within the tidally compressive region of a galaxy. We have applied the mechanism to determine the mean molecular cloud densities in the centers of a sample of flat-core, early-type galaxies and ultraluminous galaxies.
description: 18 latex pages and uses aaspp4.sty, accepted for publication in Astrophysical Journal
The Reaction $πN \to ππN$ at Threshold
Creators: name: Bernard, V.
name: Kaiser, N.
name: Meißner, Ulf-G.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We consider the chiral expansion for the reaction $πN \to ππN$ in heavy baryon chiral perturbation theory. To order $M_π$ we derive novel low--energy theorems that compare favorably with recent determinations of the total cross sections for $π^+ p \to π^+ π^+ n$ and $π^- p \to π^0 π^0 n$.
description: 7 pp, LateX (uses epsf.sty), 3 figures appended as ps files (split off as ppnf1.ps,ppnf2.ps,ppnf3.ps), CRN 94/19
Bulla tornatilis Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Cephalaspidea
Bullidae
Bulla
Bulla tornatilis

description: Bulla tornatilis [spec. nov.]
B. testa ovata substriata, spira elevata acutiuscula, columella uniplicata.
Habitat ..
Testa rubicunda, fasciis albis.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 728, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
FACE RECOGNITION BASED ATTENDANCE
Creators: name: Sriwastav, Paridhi
Publisher: name: figshare
Year: 2021
Subjects: subject: 80104 Computer Vision
subject: FOS: Computer and information sciences
subject: 80106 Image Processing

description: Face recognition system plays a important role in almost every sector. Face recognition is one among the mostly used bio metrics. It can used for authentication, identification, and has got many more advantages. An automated system for human face recognition during a real time background for a university to mark the attendance of their employees. The task is difficult because the real time background subtraction during a picture remains a challenge. To detect real time human faces are used and an easy fast Principle Component Analysis has wont to recognize the faces detected with a high accuracy rate. The matched face is used to mark attendance of the employee. Our System maintains the attendance records of employees automatically. Manual taking of attendance in logbooks becomes a time taking task. So we designed an efficient system that comprises of face recognition to store the attendance records of employees. Our system enrolls the staffs and students face. The enrolling may be a one-time process and their face are going to be stored in the database. It is a one-time process and during enrolling of face we require a system. You can have your own employee id which is unique for each employee. The presence of each employee will be updated in a database. Attendance is marked after employee identification. This product gives much more solutions with accurate leads to user interactive manner rather than existing attendance and leave management system.
Designing and experimental verification of a photoacoustic flow sensor using computational fluid dynamics
Creators: name: Lassen, Mikael
name: Balslev-Harder, David
name: Brusch, Anders
name: Pelevic, Nikola
name: Persijn, Stefan
name: Petersen, Jan C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: A photoacoustic (PA) sensor for fast and real-time gas sensing is demonstrated. The PA sensor is a standalone system controlled by a Field-Programmable Gate Array (FPGA). The PA cell has been designed for flow noise immunity using computational fluid dynamics (CFD) analysis. The aim of the CFD analysis was to investigate and minimize the influence of the gas distribution and the flow noise on the PA signal. PA measurements were conducted at different flow rates by exciting molecular C-H stretch vibrational bands of hexane (C$_6$H$_{14}$) and decane (C$_{10}$H$_{22}$) molecules in clean air at 2950 cm$^{-1}$ (3.38 $μ$m) with a custom made mid-infrared interband cascade laser (ICL). We observe a (1$σ$, standard deviation) sensitivity of 0.4 $\pm0.1$ ppb (nmol/mol) for hexane in clean air at flow rates up to 1.7 L/min, corresponding to a normalized noise equivalent absorption (NNEA) coefficient of 2.5$\times 10^{-9}$ W cm$^{-1}$ Hz$^{-1/2}$, demonstrating high sensitivity and fast real-time gas analysis. An Allan deviation analysis for decane shows that the detection limit at optimum integration time is 0.25 ppbV (nmol/mol).
description: 6 pages, 5 figures
Additional file 2 of Clinical and genetic characterization of a large cohort of patients with Wilson’s disease in China
Creators: name: Zhang, Shijie
name: Yang, Wenming
name: Li, Xiang
name: Pei, Pei
name: Dong, Ting
name: Yang, Yue
name: Zhang, Jing
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Environmental Sciences not elsewhere classified
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Mental Health

description: Additional file 2: Table S2. Details of potential pathogenic variants of ATP7B identified in this study.
Centroids of Gamow-Teller transitions at finite temperature in fp-shell neutron-rich nuclei
Creators: name: Civitarese, O.
name: Ray, A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The temperature dependence of the energy centroids and strength distributions for Gamow-Teller (GT) $1^+$ excitations in several fp-shell nuclei is studied. The quasiparticle random phase approximations (QRPA) is extended to describe GT states at finite temperature. A shift to lower energies of the GT$^+$ strength is found, as compared to values obtained at zero temperature.
description: 12 pages, contains 3 tables. E-mail: akr@tifr.res.in, civitare@venus.fisica.unlp.edu.ar
Super Stores’ Impact on the Availability of Supplemental Nutrition Assistance Program-Approved Stores
Creators: name: Ollinger, Michael
name: Ver Ploeg, Michele
name: Dicken, Chris
name: Ollinger, Michael
name: Ver Ploeg, Michele
name: Dicken, Chris
Publisher: name: Unknown
Year: 2021
Subjects: subject: Community/Rural/Urban Development
subject: Consumer/Household Economics
subject: Demand and Price Analysis
subject: Food Security and Poverty
subject: Public Economics
subject: Research Methods/ Statistical Methods
subject: Supplemental Nutrition Assistance Program
subject: SNAP
subject: super stores
subject: grocery stores
subject: supermarkets
subject: Store Tracking and Redemption System
subject: STARS
subject: food and nutrition assistance
subject: store access
subject: store availability
subject: SNAP redemptions
subject: store exits
subject: store entry

description: Super stores have become the store of choice for USDA’s Supplemental Nutrition Assistance Program (SNAP) beneficiaries over the past 30 years and now account for more than one-half of SNAP redemptions. However, by diverting SNAP beneficiaries away from supermarkets, grocery stores, and other food retailers, super stores could force some smaller stores to exit the market. These dynamics could mean reduced access for some SNAP beneficiaries while offering cost savings to many other SNAP beneficiaries. This study examines the impact of new super store entries on the survival of existing traditional stores and the cost savings accruing to SNAP beneficiaries. We find no evidence that super store entry has reduced the number of SNAP-approved stores. SNAP beneficiaries save about $6,390 in SNAP benefits per year, per super store. If extended across all super stores, the savings would be about $108.6 million in 2015—0.26 percent of SNAP benefits—based on estimates over 2005–15 and the number of super stores in 2015.
Bulla achatina Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Cephalaspidea
Bullidae
Bulla
Bulla achatina

description: Bulla achatina [spec. nov.]
B. testa ovata, apertura obovata apiceque sanguineis, columella laevi.
Column. aquat. t. 16. Buccinum exoticum.
List. conch. t. 579.
Bonan. recr. 3. t. 192.
Gvalt. test. t. 45. f. B.
Argenv. conch. t. 13. f. E.
Klein, ostr. t. 3. f. 60.
Habitat in O. Americano. Media inter Helices & Bullas.
* Columella dentata.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 728, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Additional file 1: of International pilot external quality assessment scheme for analysis and reporting of circulating tumour DNA
Creators: name: Keppens, Cleo
name: Dequeker, Elisabeth
name: Patton, Simon
name: Normanno, Nicola
name: Fenizia, Francesca
name: Butler, Rachel
name: Cheetham, Melanie
name: Fairley, Jennifer
name: Williams, Hannah
name: Hall, Jacqueline
name: Schuuring, Ed
name: Zandra Deans
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Molecular Biology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Science Policy

description: Example of individual feedback report. (PDF 136 kb)
Multiplicities for LHC Nuclear Collisions Using HERA Structure Functions
Creators: name: Eskola, K. J.
name: Kajantie, K.
name: Ruuskanen, P. V.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We compute in QCD perturbation theory the transverse energy carried by gluons, quarks and antiquarks with $p_T\ge p_0\approx 2$ GeV in Pb+Pb collisions at $\sqrt{s}=5500$ $A$GeV by using structure functions compatible with the small-$x$ increase observed at HERA. This gives a perturbative estimate for the energy and entropy density of the bulk system at times $τ\sim 0.1$ fm. The predicted initial gluon entropy density gives a lower limit of about 2200...3400 for the final charged multiplicity. Sources of further entropy increase are discussed.
description: HU-TFT-94-6, 7 pages, 3 PostScript figures included in the end of the tex-file
Tidal Disruption of Inclined or Eccentric Binaries by Massive Black Holes
Creators: name: Brown, Harriet
name: Kobayashi, Shiho
name: Rossi, Elena M.
name: Sari, Re'em
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Binary stars that are on close orbits around massive black holes (MBH) such as Sgr A* in the center of the Milky Way are liable to undergo tidal disruption and eject a hypervelocity star. We study the interaction between such a MBH and circular binaries for general binary orientations and penetration depths (i.e. binaries penetrate into the tidal radius around the BH). We show that for very deep penetrators, all binaries are disrupted when the binary rotation axis is roughly oriented toward the BH or it is in the opposite direction. The surviving chance becomes significant when the angle between the binary rotation axis and the BH direction is between π/4 and 3 π/4. The surviving chance is as high as $\sim$ 20$\%$ when the binary rotation axis is perpendicular to the BH direction. The angular dependence is opposite for very shallow penetrators where coplanar prograde orbits have the lowest surviving chance (or equivalently most vulnerable). We provide numerical fits to the disruption probability and energy gain at the the BH encounter as a function of the penetration depth. The latter can be simply rescaled in terms of binary masses, their initial separation and the binary-to-BH mass ratio to evaluate the ejection velocity of a binary members in various systems. We also investigate the disruption of coplanar, eccentric binaries by a MBH. It is shown that for highly eccentric binaries retrograde orbits have a significantly increased disruption probability and ejection velocities compared to the circular binaries.
Bulla fontinalis Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Cephalaspidea
Bullidae
Bulla
Bulla fontinalis

description: Bulla fontinalis [spec. nov.]
B. testa ovata pellucida sinistrorsa, spira obsoleta, apertura ovato-oblonga.
Habitat in Lacuum plantis subaquaticis.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 727, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Slott-Agape Project
Creators: name: AGAPE Collaboration
name: Bozza, V.
name: Novati, S. Calchi
name: Capaccioli, M.
name: Capozziello, S.
name: Cardone, V.
name: Covone, G.
name: De Paolis, F.
name: de Ritis, R.
name: Ingrosso, G.
name: Iovane, G.
name: Lambiase, G.
name: Marino, A. A.
name: Marmo, G.
name: Musella, I.
name: Piedipalumbo, E.
name: Pezzuto, S.
name: Roncadelli, M.
name: Rubano, C.
name: Scarpetta, G.
name: Scudellaro, P.
name: Strafella, F.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: SLOTT-AGAPE (Systematic Lensing Observation at Toppo Telescope - Andromeda Gravitational Amplification Pixel Lensing Experiment) is a new collaboration project among international partners from England, France, Germany, Italy and Switzerland that intends to perform microlensing observation by using M31 as target. The MACHOs search is made thanks to the pixel lensing technique.
description: 4 pages, 2 figures, proceeding of XLIII Congresso della Societa' Astronomica Italiana, Napoli, 4-8 Maggio, 1999
Roughness as Classicality Indicator of a Quantum State
Creators: name: Lemos, Humberto C. F.
name: Almeida, Alexandre C. L.
name: Amaral, Barbara
name: Oliveira, Adélcio C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We define a new quantifier of classicality for a quantum state, the Roughness, which is given by the $\mathcal{L}^2 (\R^2)$ distance between Wigner and Husimi functions. We show that the Roughness is bounded and therefore it is a useful tool for comparison between different quantum states for single bosonic systems. The state classification via the Roughness is not binary, but rather it is continuous in the interval [0,1], being the state more classic as the Roughness approaches to zero, and more quantum when it is closer to the unity. The Roughness is maximum for Fock states when its number of photons is arbitrarily large, and also for squeezed states at the maximum compression limit. On the other hand, the Roughness reaches its minimum value for thermal states at infinite temperature and, more generally, for infinite entropy states. The Roughness of a coherent state is slightly below one half, so we may say that it is more a classical state than a quantum one. Another important result is that the Roughness performs well for discriminating both pure and mixed states. Since the Roughness measures the inherent quantumness of a state, we propose another function, the Dynamic Distance Measure (DDM), which is suitable for measure how much quantum is a dynamics. Using DDM, we studied the quartic oscillator, and we observed that there is a certain complementarity between dynamics and state, i.e. when dynamics becomes more quantum, the Roughness of the state decreases, while the Roughness grows as the dynamics becomes less quantum.
description: Pre-print version
Predictions for Proton Lifetime in Minimal Non-Supersymmetric SO(10) Models: An Update
Creators: name: Lee, D. G.
name: Mohapatra, R. N.
name: Parida, M. K.
name: Rani, M.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present our best estimates of the uncertainties due to heavy particle threshold corrections on the unification scale $M_U$, intermediate scale $M_I$ and coupling constant Alpha_U in the minimal non-supersymmetric SO(10) models. Using these , we update the predictions for proton life-time in these models.
description: UMD-PP-94-117 ( 20 pages;latex; no figures )
Heavy-Light Mesons in the Non-Relativistic Quark Model Using Laplace Transformation Method
Creators: name: Abu-Shady, M.
name: Khokha, E. M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: An analytic solution of the N-dimensional radial Schrödinger equation with the mixture of vector and scalar potentials via the Laplace transformation method (LTM) is studied. The present potential is extended to include the spin hyperfine, spin-orbit and tensor interactions. The energy eigenvalues and the corresponding eigenfunctions have been determined in the N-dimensional space. The present results are employed to study the different properties of the heavy-light mesons. The masses of the scalar, vector, pseudoscalar and pseudovector of B, Bs, D and Ds mesons have been calculated in the three dimensional space. The effect of the dimensional number space is studied on the masses of the heavy-light mesons. We find that the meson mass increases with increasing dimensional space. The decay constants of the pseudoscalar and vector mesons have been computed. In addition, the leptonic decay widths and branching ratio for the B+, D+ and Ds+ mesons have been studied. Therefore, the present method with the present potential gives good results which are in good agreement with experimental data and are improved in comparison with recently theoretical works.
description: 31 pages, 3 figures
Additional file 1: of Thyroid hormones and breast cancer association according to menopausal status and body mass index
Creators: name: Ortega-Olvera, Carolina
name: Ulloa-Aguirre, Alfredo
name: Ángeles-Llerenas, Angélica
name: Mainero-Ratchelous, Fernando Enrique
name: González-Acevedo, Claudia
name: Ma. Hernández-Blanco
name: Ziv, Elad
name: Avilés-Santa, Larissa
name: Pérez-Rodríguez, Edelmiro
name: Torres-Mejía, Gabriela
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Evolutionary Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer

description: Table S1. Associations between thyroid function tests and BC adjusted by anthropometric variables. CAMA Study1, Mexico 2004–2007. The table presents the multiple model stratified by menopausal status, adjusted by hip and waist measurements, WHR, and trajectory of the silhouettes. Table S2. Association between thyroid function tests and BC modified by anthropometric variables. CAMA Study1, Mexico 2004–2007. The table presents the multiple model stratified by menopausal status, and each of anthropometric variables (hip and waist measurements, WHR, and trajectory of the silhouettes). (DOCX 30 kb)
Gelingensfaktoren für die Integration von Schülerinnen und Schüler im Autismus-Spektrum. Von der Sonderschule zur Regelschule
Creators: name: Letonja, Lena
Publisher: name: Interkantonale Hochschule für Heilpädagogik
Year: 2024
Subjects: Sonderpädagogik
Masterarbeit
Autismus-Spektrum
Integration
Gelingensfaktoren
Sonderschule
Regelschule

description: Diese Masterarbeit untersucht die Gelingensfaktoren für eine schulische Integration von Schülerinnen und Schülern im Autismus-Spektrum, die von einer Sonderschule in das Regelschulsystem wechseln. Der Schwerpunkt liegt auf der Analyse unterstützender Massnahmen und Herausforderungen, die im Praxisfeld von Fachpersonen identifiziert wurden. Mithilfe einer qualitativen Inhaltsanalyse nach Mayring wurden sechs Interviews mit Lehrpersonen, Heilpädagoginnen und Schulleitungen ausgewertet. Die theoretischen Grundlagen umfassen allgemeine Theorien über das Autismus-Spektrum, Konzepte zur Separation, Integration und Inklusion im Bildungsbereich sowie den Prozess der Transition von der Sonderschule in die Regelschule. Zusätzlich werden in einem Literaturüberblick Gelingensfaktoren für die Integration auf individueller, interaktionaler und kontextueller Ebene dargestellt. Die empirischen Ergebnisse bestätigen diese theoretischen Gelingensfaktoren und verdeutlichen ihre Bedeutung in der Praxis. Auf der individuellen Ebene spielen eine sorgfältige Vorbereitung der Schülerinnen und Schüler und ein angepasster Lehrplan eine zentrale Rolle. Auf der interaktionalen Ebene wird die Bedeutung der Zusammenarbeit zwischen den beteiligten Personen sowie die Förderung von Peer-Beziehungen hervorgehoben. Die kontextuelle Ebene betont die Notwendigkeit einer integrativen Grundhaltung und einer klar strukturierten Lernumgebung. Aus den Ergebnissen werden konkrete Handlungsansätze abgeleitet, die den Integrationsprozess nachhaltig unterstützen können.
Young massive star clusters in nearby galaxies. II.Software tools, data reductions and cluster sizes
Creators: name: Larsen, S. S.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A detailed description is given of the data analysis leading to the discovery of young massive star clusters (YMCs) in a sample of 21 nearby galaxies. A new useful tool, ishape, for the derivation of intrinsic shape parameters of compact objects is presented, and some test results are shown. Completeness tests for the cluster samples are discussed, and ishape is used to estimate cluster sizes. Half-light radii of 0 - 20 pc are derived for clusters in 2 of the most cluster-rich galaxies, NGC 1313 and NGC 5236, which is within the range spanned by globular clusters in the Milky Way and by YMCs in the LMC and some starburst galaxies. Photometric data for all clusters, along with positions and estimated half-light radii, are tabulated.
description: Accepted for publication in A&A Suppl. Ser. 24 pages, 14 figures
The Equivalence Theorem for Chiral Lagrangians
Creators: name: Dobado, A.
name: Pelaez, J. R.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In this work we derive the version of the Equivalence Theorem that applies when the symmetry breaking sector of the Standard Model is described by a general chiral lagrangian. The demonstration is valid for renormalized fields for any value of the gauge parameter (in $R_ξ$ gauges) and any parametrization of the coset space. It is based in the absence of gauge anomalies which makes it possible to build an (anti)-BRS invariant chiral lagrangian in terms of the renormalized fields and therefore to use the corresponding Ward identities to obtain the theorem.
description: 18 pages, LaTeX, FT/UCM/2/94 (We have corrected some errata)
Additional file 1 of The response to individualized treatment after a standardized treatment protocol among neck pain sufferers: a secondary analysis of a randomized controlled trial
Creators: name: Galaasen Bakken, Anders
name: Eklund, Andreas
name: Oksanen, Anna
name: Axén, Iben
Publisher: name: figshare
Year: 2025
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Neuroscience
subject: Biotechnology
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: Science Policy
subject: Mental Health
subject: Infectious Diseases
subject: FOS: Health sciences

description: Supplementary Material 1
MOESM8 of Chimeric Plasmodium falciparum parasites expressing Plasmodium vivax circumsporozoite protein fail to produce salivary gland sporozoites
Creators: name: Catherin Marin-Mogollon
name: Pul, Fiona
name: Miyazaki, Shinya
name: Imai, Takashi
name: Ramesar, Jai
name: Salman, Ahmed
name: Winkel, Beatrice
name: Othman, Ahmad
name: Kroeze, Hans
name: Chevalley-Maurel, Severine
name: Reyes-Sandoval, Arturo
name: Roestenberg, Meta
name: Franke-Fayard, Blandine
name: Janse, Chris
name: Khan, Shahid
Publisher: name: figshare
Year: 2018
Subjects: subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Physiology
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Marine Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 8. Chimeric rodent parasite lines pb-pvcsp(vk210) and pb-pvcsp(vk247) are able to produce salivary gland sporozoites that are infectious to mice. A. Upper panel, left: Light microscope pictures of wild type P. berghei (WT) and pb-pvcsp oocyst at days 7, 10 and 14 after feeding of An. stephensi mosquitoes. Black arrows indicate oocyst with sporozoite formation and white arrows indicate degenerated, vacuolated oocyst without sporozoite formation (scale bar, 10 µm). Upper panel, right, Percentage of degenerated oocyst in An. stephensi mosquitoes (n = 5) at day 14 after feeding (***P =
Optical single photon detection in micron-scaled NbN bridges
Creators: name: Korneeva, Y.
name: Vodolazov, D. Yu.
name: Semenov, A. V.
name: Florya, I.
name: Simonov, N.
name: Baeva, E.
name: Korneev, A. A.
name: Goltsman, G. N.
name: Klapwijk, T. M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We demonstrate experimentally that single photon detection can be achieved in micron-wide NbN bridges, with widths ranging from 0.53 $μ$m to 5.15 $μ$m and for photon-wavelengths from 408 nm to 1550 nm. The microbridges are biased with a dc current close to the experimental critical current, which is estimated to be about 50 % of the theoretically expected depairing current. These results offer an alternative to the standard superconducting single-photon detectors (SSPDs), based on nanometer scale nanowires implemented in a long meandering structure. The results are consistent with improved theoretical modelling based on the theory of non-equilibrium superconductivity including the vortex-assisted mechanism of initial dissipation.
description: 13 pages, 12 figures
Bulla auris judae Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Cephalaspidea
Bullidae
Bulla
Bulla auris judae

description: Bulla auris judae [spec. nov.]
B. testa oblonga, spira laevi, columella tridentata. M. L. U.
Habitat ..
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 728, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Sgr A$^*$ envelope explosion and the young stars in the centre of the Milky Way
Creators: name: Nayakshin, Sergei
name: Zubovas, Kastytis
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Sgr A$^*$ is the super massive black hole residing in the centre of the Milky Way. There is plenty of observational evidence that a massive gas cloud fell into the central parsec of the Milky Way $\sim 6$ million years ago, triggering formation of a disc of young stars and activating Sgr A$^*$. In addition to the disc, there is an unexplained population of young stars on randomly oriented orbits. Here we hypothesize that these young stars were formed by fragmentation of a massive quasi-spherical gas shell driven out from Sgr A$^*$ potential well by an energetic outflow. To account for the properties of the observed stars, the shell must be more massive than $10^5$ Solar masses, be launched from inside $\sim 0.01$~pc, and the feedback outflow has to be highly super-Eddington albeit for a brief period of time, producing kinetic energy of at least $10^{55}$~erg. The young stars in the central parsec of the Galaxy may be a unique example of stars formed from atomic rather than molecular hydrogen, and forged by extreme pressure of black hole outflows.
description: Accepted (w. minor revisions) to MNRAS Letters
Flattened Galactic Haloes and Baryonic Dark Matter
Creators: name: Samurovic, Srdjan
name: Cirkovic, Milan M.
name: Milosevic-Zdjelar, Vesna
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We discuss the tight interconnection between microlensing optical depths, flattening of dark haloes and low-to-intermediate redshift baryonic census. By analysing plots of the microlensing optical depth as a function of galactic coordinates for different values of axis ratio $q$ of the galactic MACHO halo, we have shown that observations are best described by a flattened halo with $q \simeq 0.6$. There is no dynamical obstacle for such a choice of global halo shape. Both extremely flattened $q \simeq 0.2$ and spherical $q \simeq 1$ haloes have several difficulties, although not of equal severity. Consequences of such flattening for the cosmological density fraction contained in MACHOs are considered and comparison with mass in low and intermediate-redshift Ly$α$ forest and other plausible reservoirs of gas is discussed in context of a unified description of the evolution of baryonic content of the universe.
description: 14 pages, 15 figures, TeX, uses mn.tex and psfig.tex, MNRAS accepted