cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
AGN feedback and the origin and fate of the hot gas in early-type galaxies
Creators: name: Pellegrini, S.
name: Ciotti, L.
name: Negri, A.
name: Ostriker, J. P.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: A recent determination of the relationships between the X-ray luminosity of the ISM (Lx) and the stellar and total mass, for a sample of nearby early-type galaxies (ETGs), is used to investigate the origin of the hot gas, via a comparison with the results of hydrodynamical simulations of the ISM evolution for a large set of isolated ETGs. After the epoch of major galaxy formation (after z~2), the ISM is replenished by stellar mass losses and SN ejecta, at the rate predicted by stellar evolution, and is depleted by star formation; it is heated by the thermalization of stellar motions, SNe explosions and the mechanical (from winds) and radiative AGN feedback. The models agree well with the observed relations, even for the largely different Lx values at the same mass, thanks to the sensitivity of the gas flow to many galaxy properties; this holds for models including AGN feedback, and those without. Therefore, the mass input from the stellar population is able to account for a major part of the observed Lx; and AGN feedback, while very important to maintain massive ETGs in a time-averaged quasi-steady state, keeping low star formation and the black hole mass, does not dramatically alter the gas content originating in stellar recycled material. These conclusions are based on theoretical predictions for the stellar population contributions in mass and energy, and on a self-consistent modeling of AGN feedback.
description: 7 pages, 1 figure, accepted for publication in The Astrophysical Journal
The Radial Structure of the Cygnus Loop Supernova Remnant --- Possible evidence of a cavity explosion ---
Creators: name: Miyata, Emi
name: Tsunemi, Hiroshi
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We observed the North-East (NE) Limb toward the center region of the Cygnus Loop with the ASCA Observatory. We found a radial variation of electron temperature (kTe) and ionization timescale (log(τ)) whereas no variation could be found for the abundances of heavy elements. In this paper, we re-analyzed the same data set and new observations with the latest calibration files. Then we constructed the precise spatial variations of kTe, log(τ), and abundances of O, Ne, Mg, Si, and Fe over the field of view (FOV). We found a spatial variation not only in kTe and in log(τ) but also in most of heavy elements. As described in Miyata et al. (1994), values of kTe increase and those of log(τ) decrease toward the inner region. We found that the abundance of heavy elements increases toward the inner region. The radial profiles of O, Ne, and Fe show clear jump structures at a radius of 0.9 Rs, where Rs is the shock radius. Outside of 0.9 Rs, abundances of all elements are constant. On the contrary, inside of 0.9 Rs, abundances of these elements are 20--30 % larger than those obtained outside of 0.9 Rs. The radial profile of kTe also shows the jump structure at 0.9 Rs. This means that the hot and metal rich plasma fills the volume inside of 0.9 Rs. We concluded that this jump structure was the possible evidence for the pre-existing cavity produced by the precursor. If the ejecta fills inside of 0.9 Rs, the total mass of the ejecta was roughly 4\Msun. We then estimated the main-sequence mass to be roughly 15\Msun, which supports the massive star in origin of the Cygnus Loop supernova remnant and the existence of a pre-existing cavity.
description: 37 pages, 14 figures. Accepted for publication of ApJ
Additional file 2 of Diagnosis of pulmonary tuberculosis via identification of core genes and pathways utilizing blood transcriptional signatures: a multicohort analysis
Creators: name: Qiu, Qian
name: Peng, Anzhou
name: Zhao, Yanlin
name: Liu, Dongxin
name: Liu, Chunfa
name: Qiu, Shi
name: Xu, Jinhong
name: Cheng, Hongguang
name: Xiong, Wei
name: Chen, Yaokai
Publisher: name: figshare
Year: 2022
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 2: Table S2. Primers used in this study.
Resonant excitation of infra-red emission in GaN:(Mn,Mg)
Creators: name: Kysylychyn, Dmytro
name: Suffczyński, Jan
name: Woźniak, Tomasz
name: Szwacki, Nevill Gonzalez
name: Bonanni, Alberta
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: By combining experimental photoluminescence excitation spectroscopy and calculations based on density functional theory and many-body Green's functions, the most efficient excitation channels of infra-red (IR) emission from Mn-Mg$_{k}$ paramagnetic complexes stabilized in GaN:(Mn,Mg) are here identified. Moreover, a Tanabe-Sugano energy diagram for 3$d^{2}$Mn$ ^{5+}$ is reconstructed and Mn-Mg$_{3}$ are singled out as the predominant configurations responsible for the IR emission. The correlation of intensity of the individual emission lines as a function of temperature and excitation energy, allows assigning them to well defined and specific optical transitions.
description: 17 pages, 6 figures, 45 references
REGULAMENTO ENIC 2017 - UNINOVE.pdf
Creators: name: Cavalcante, Vinicius Holanda
Publisher: name: figshare
Year: 2018
Subjects: Education

description: Regulamento para os pesquisadores e alunos de Iniciação Científica interessados em participar do; Encontro de Iniciação Científica e Seminário Nacional de Pesquisa da Universidade Nove de Julho - UNINOVE
Alexandrium pseudogonyaulax Yuki et Fukuyo
Creators: name: Hernández-Becerril, David U.
name: Pichardo-Velarde, Jorge G.
name: Alonso-Rodríguez, Rosalba
name: Maciel-Baltazar, Ebodio
name: Morquecho, Lourdes
name: Esqueda-Lara, Karina
name: Barón-Campis, Sofía A.
name: Quiroz-González, Nataly
Publisher: name: Zenodo
Year: 2023
Subjects: Biodiversity
Taxonomy
Chromista
Myzozoa
Dinophyceae
Gonyaulacales
Ostreopsidaceae
Alexandrium
Alexandrium pseudogonyaulax

description: 3.1.8 Alexandrium pseudogonyaulax (Biecheler) Horiguchi ex Yuki et Fukuyo (Figures 38–43)
References: Balech 1995, 73, pl. XVI, figs 1–18; Nguyen and Larsen 2004, 102, pl. 13, figs 1–3; Gu et al. 2013, 75, figs 4 A–D; Lassus et al. 2016, 53, pl. 9 A–D; Hernández-Becerril et al. 2021, 70, 71.
Solitary cells of medium to relatively large size, ovoid to pentagonal and slightly depressed longitudinally (Figure 38), epitheca slightly domed and shorter than hypotheca (Figures 38 and 39), which has an antapical concavity, cingulum wide and excavated (Figure 41), and sulcus wide and deep (Figures 38 and 39). First apical plate (1′) is not connected to Po (Figure 39) and has a pentagonal shape (Figures 39, 41, and 42) and a strong posterior indentation (notch). A large ventral pore appears between this plate and 4′ (Figures 39, 41–43), whereas 6″ is quadrangular. Po is elongate with a classical comma shape (Figure 40).
Measurements: 35–42 μm L, 40–45 μm W (Table 1).
Toxicity: this species produces goniodomins A and B (Krock et al. 2018).
Distribution: in the Gulf of Tehuantepec.
description: Published as part of Hernández-Becerril, David U., Pichardo-Velarde, Jorge G., Alonso-Rodríguez, Rosalba, Maciel-Baltazar, Ebodio, Morquecho, Lourdes, Esqueda-Lara, Karina, Barón-Campis, Sofía A. & Quiroz-González, Nataly, 2023, Diversity and distribution of species of the planktonic dinoflagellate genus Alexandrium (Dinophyta) from the tropical and subtropical Mexican Pacific Ocean, pp. 539-557 in Botanica Marina (Warsaw, Poland) (Warsaw, Poland) 66 (6) on pages 545-547, DOI: 10.1515/bot-2023-0037, http://zenodo.org/record/11000291
EGRET Spectral Index and the Low-Energy Peak Position in the Spectral Energy Distribution of EGRET-Detected Blazars
Creators: name: Lin, Y. C.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In current theoretical models of the blazar subclass of active galaxies, the broadband emission consists of two components: a low-frequency synchrotron component with a peak in the IR to X-ray band, and a high-frequency inverse Compton component with a peak in the gamma-ray band. In such models, the gamma-ray spectral index should be correlated with the location of the low-energy peak, with flatter gamma-ray spectra expected for blazars with synchrotron peaks at higher photon energies and vice versa. Using the EGRET-detected blazars as a sample, we examine this correlation and possible uncertainties in its construction.
description: 17 pages including 1 figure, accepted for publication in The Astrophysical Journal
МИКРОТОПОНИМЫ ТАШКЕНТА И ЛОНДОНА: СРАВНИТЕЛЬНО-КОГНИТИВНЫЙ АНАЛИЗ
Creators: name: Йулдошхонов Жавохирбек Дилшодбек угли Узбекский государственный университет мировых языков Кафедра теория перевода английского языка стажёр-учитель
Publisher: name: Zenodo
Year: 2025

description: В статье рассматриваются микротопонимы Ташкента и Лондона с позиций когнитивной лингвистики, выявляются особенности их семантики, концептуализации и роли в формировании локальной идентичности. Сравнительный анализ направлен на выявление универсальных и специфических черт в номинации малых географических объектов в культурно-языковом контексте двух мегаполисов. Микротопонимы интерпретируются как элементы языковой картины мира, отражающие когнитивные и этнокультурные особенности носителей языка.

Ключевые слова: микротопонимы, когнитивная лингвистика, локальная идентичность, языковая картина мира, Ташкент, Лондон, концептуализация, метафора
title: ADCO, Grènetier de Cîteaux : comptes (1499-1503) (11 H 1173), f. 00386
Creators: name: de la Côte-d'Or, Archives départementales
name: CBMA/CG21/F.PETOT/2019
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: comptes
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Grènetier de Cîteaux : comptes (1499-1503), Archives départementales de la Côte-d'Or, (11 H 1173). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Grènetier de Cîteaux : comptes (1499-1503), Archives départementales de la Côte-d'Or, (11 H 1173), f. 00386, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
How to tell an accreting boson star from a black hole
Creators: name: Olivares, Hector
name: Younsi, Ziri
name: Fromm, Christian M.
name: De Laurentis, Mariafelicia
name: Porth, Oliver
name: Mizuno, Yosuke
name: Falcke, Heino
name: Kramer, Michael
name: Rezzolla, Luciano
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The capability of the Event Horizon Telescope (EHT) to image the nearest supermassive black hole candidates at horizon-scale resolutions offers a novel means to study gravity in its strongest regimes and to test different models for these objects. Here, we study the observational appearance at 230 GHz of a surfaceless black hole mimicker, namely a non-rotating boson star, in a scenario consistent with the properties of the accretion flow onto Sgr A*. To this end, we perform general relativistic magnetohydrodynamic simulations followed by general relativistic radiative transfer calculations in the boson star space-time. Synthetic reconstructed images considering realistic astronomical observing conditions show that, despite qualitative similarities, the differences in the appearance of a black hole -- either rotating or not -- and a boson star of the type considered here are large enough to be detectable. These differences arise from dynamical effects directly related to the absence of an event horizon, in particular, the accumulation of matter in the form of a small torus or a spheroidal cloud in the interior of the boson star, and the absence of an evacuated high-magnetization funnel in the polar regions. The mechanism behind these effects is general enough to apply to other horizonless and surfaceless black hole mimickers, strengthening confidence in the ability of the EHT to identify such objects via radio observations.
description: 16 pages, 12 figures. Published in MNRAS. Adding more information in the form of appendices, and a new simulation of a different boson star model. The conclusions do not change
Ecological Status of Kofiau MPA - 2016 Technical Report
Creators: name: Purwanto Purwanto
name: Awaludinnoer Awaludinnoer
name: J. Harris
name: R. Ardiwijaya
Publisher: name: figshare
Year: 2018
Subjects: subject: 50202 Conservation and Biodiversity
subject: FOS: Biological sciences
subject: Marine Biology

description: The Raja Ampat Islands encompass 4 million hectares of land and sea located in West Papua, Indonesia, right in the heart of the Coral Triangle. The Raja Ampat Islands are a part of the Bird’s Head Seascape, which has the greatest coral reef biodiversity on the planet and is a global priority for conservation. Kofiau MPA is the 5th largest MPA in the Raja Ampat MPA Network. It covers 170,000 hectares, including 17, 243 hectares (10%) in no-take zones. Under Indonesian law, MPAs allow for multiple uses which are regulated through management and zoning plans. The Kofiau MPA management and zoning plans were formalized in Oct 2011. Reef health monitoring data is used to support the development of management and zoning plans and, when repeated over time, can be used to assess the effectiveness of zoning and management plans and inform adaptive management. Therefore reef health monitoring was conducted annually from 2009 to 2012 and biannually in 2014 and 2016 in Kofiau MPA. In 2016, 24 sites were surveyed by an integrated team from Kofiau local community, Raja Ampat Conservation Implementation Unit (UPTD DKP Raja Ampat), students of Diponegoro University, University of Papua, Conservation International and The Nature Conservancy from 22-28 March.
Radiation mechanisms and geometry of Cygnus X-1 in the soft state
Creators: name: Gierlinski, M.
name: Zdziarski, A. A.
name: Poutanen, J.
name: Coppi, P. S.
name: Ebisawa, K.
name: Johnson, W. N.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present X-ray/gamma-ray spectra of Cyg X-1 observed during the transition from the hard to the soft state and in the soft state by ASCA, RXTE and OSSE in 1996 May and June. The spectra consist of a dominant soft component below ~2 keV and a power-law-like continuum extending to at least ~800 keV. We interpret them as emission from an optically-thick, cold accretion disc and from an optically-thin, non-thermal corona above the disc. A fraction f ~ 0.6 of total available power is dissipated in the corona. We model the soft component by multi-colour blackbody disc emission taking into account the torque-free inner-boundary condition. If the disc extends down to the minimum stable orbit, the ASCA/RXTE data yield the most probable black hole mass of about 10 solar masses and an accretion rate about 0.5 L_E/c^2, locating Cyg X-1 in the soft state in the upper part of the stable, gas-pressure dominated, accretion-disc solution branch. The spectrum of the corona is well modelled by repeated Compton scattering of seed photons from the disc off electrons with a hybrid, thermal/non-thermal distribution. The electron distribution can be characterized by a Maxwellian with an equilibrium temperature of kT ~ 30--50 keV and a Thomson optical depth of ~0.3 and a quasi-power-law tail. The compactness of the corona is between 2 and 7, and a presence of a significant population of electron-positron pairs is ruled out. We find strong signatures of Compton reflection from a cold and ionized medium, presumably an accretion disc, with an apparent reflector solid angle ~0.5--0.7. The reflected continuum is accompanied by a broad iron K-alpha line.
description: 18 pages, 12 figures, 2 landscape tables in a separate file. Accepted to MNRAS
Additional file 3 of Diagnosis of pulmonary tuberculosis via identification of core genes and pathways utilizing blood transcriptional signatures: a multicohort analysis
Creators: name: Qiu, Qian
name: Peng, Anzhou
name: Zhao, Yanlin
name: Liu, Dongxin
name: Liu, Chunfa
name: Qiu, Shi
name: Xu, Jinhong
name: Cheng, Hongguang
name: Xiong, Wei
name: Chen, Yaokai
Publisher: name: figshare
Year: 2022
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 3: Table S3. Significantly enriched GO terms and KEGG pathways of DEGs with P < 0.05 and gene counts ≥ 3.
Measurement of the $D^{*\pm}$ Cross Section using a Soft-Pion Analysis in Two-Photon Processes
Creators: name: Enomoto, R.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The differential cross section of $dσ(e^+e^-\to e^+e^-D^{*\pm}X)/dP_T$ was measured using a soft-pion analysis of $D^{*\pm}\to π_s^\pm D^0(\bar{D^0})$ at TRISTAN. The average $\sqrt{s}$ was 58.1 GeV and the integrated luminosity used in this analysis was 198 pb$^{-1}$, respectively.
description: 16 pages, Latex format, figures will be sent by 'figures' command
Digital quantum simulation of lattice gauge theories in three spatial dimensions
Creators: name: Bender, Julian
name: Zohar, Erez
name: Farace, Alessandro
name: Cirac, J. Ignacio
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: Quantum Gases (cond-mat.quant-gas)
subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In the present work, we propose a scheme for digital formulation of lattice gauge theories with dynamical fermions in 3+1 dimensions. All interactions are obtained as a stroboscopic sequence of two-body interactions with an auxiliary system. This enables quantum simulations of lattice gauge theories where the magnetic four-body interactions arising in two and more spatial dimensions are obtained without the use of perturbation theory, thus resulting in stronger interactions compared with analogue approaches. The simulation scheme is applicable to lattice gauge theories with either compact or finite gauge groups. The required bounds on the digitization errors in lattice gauge theories, due to the sequential nature of the stroboscopic time evolution, are provided. Furthermore, an implementation of a lattice gauge theory with a non-abelian gauge group, the dihedral group $D_{3}$, is proposed employing the aforementioned simulation scheme using ultracold atoms in optical lattices.
description: 38 pages, 5 figures
Tailoring polycarboxylate architecture to improve the rheological properties of cement paste
Creators: name: Wang, Xiumei
name: Yang, Yong
name: Shu, Xin
name: Wang, Yanwei
name: Ran, Qianping
name: Liu, Jiaping
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Biophysics
subject: Physical Sciences not elsewhere classified
subject: Medicine
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Hematology

description: This study elucidates the link between polycarboxylate (PC) architecture (random vs. block) and rheological properties of cement pastes at a low water-cement ratio (W/C = 0.22) through a systematic investigation on the rheological properties, adsorption properties, solution viscosity and polymer hydrodynamic radius. Adsorption data show that the adsorption amount of the block PC is larger than that of the random PC while the paste flow is the same even though the dosage of the former is smaller, possibly owing to the fact that the adsorbing carboxylic groups are concentrated at one end in the case of the block PC, and the absence of neutral side chains in the adsorbing block effectively reduces the free energy barrier of PC adsorption. Results on the polymer hydrodynamic radius from dynamic light scattering (DLS) illustrate that the hydrodynamic radius of the block PC is smaller than that of the random PC, and in consistence with the DLS results, the solution of the block PC is also found to have a lower viscosity at the same polymer weight concentration. It is worth-noting that the apparent viscosity of the cement paste has a close relation with the viscosity of PC remaining in solution. The dual effects of a larger adsorption amount and a smaller hydrodynamic radius of the block PC effectively reduce the viscosity of PC remaining in solution, and hence effective reduce the apparent viscosity of cement pastes. It is believed that this study allows for a better understanding of the influences of polycarboxylate architecture on rheological properties of cementitious materials.
Developments of Multi-wavelength Spectro-Polarimeter on the Domeless Solar Telescope at Hida Observatory
Creators: name: Anan, Tetsu
name: Huang, Yu Wei
name: Nakatani, Yoshikazu
name: Ichimoto, Kiyoshi
name: Ueno, Satoru
name: Kimura, Goichi
name: Ninomiya, Shota
name: Okada, Sanetaka
name: Kaneda, Naoki
Publisher: name: arXiv
Year: 2018
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: To obtain full Stokes spectra in multi-wavelength windows simultaneously, we developed a new spectro-polarimeter on the Domeless Solar Telescope at Hida Observatory. The new polarimeter consists of a 60 cm aperture vacuum telescope on an altazimuth mount, an image rotator, a high dispersion spectrograph, polarization modulator and analyzer composed of a continuously rotating waveplate with a retardation nearly constant around 127$^{circ}$ in 500 - 1100 nm and a polarizing beam splitter located closely behind the focus of the telescope, fast and large format CMOS cameras and an infrared camera. The slit spectrograph allows us to obtain spectra in as many wavelength windows as the number of cameras. We characterized the instrumental polarization of the entire system and established the polarization calibration procedure. The cross-talks among the Stokes Q,U and V are evaluated to be about 0.06% $sim$ 1.2% depending on the degree of the intrinsic polarizations. In a typical observing setup, a sensitivity of 0.03% can be achieved in 20 - 60 second for 500 nm - 1100 nm. The new polarimeter is expected to provide a powerful tool to diagnose the 3D magnetic field and other vector physical quantities in the solar atmosphere.
description: 22 pages, 12 figures, accepted for publication in PASJ (Hida topical issue)
Bird’s Head Seascape: Changes in Marine Protected Area Management Effectiveness
Creators: name: D.A. Andradi-Brown
name: G.N. Ahmadia
name: Awaludinnoer Awaludinnoer
name: J. Harris
name: A. Hasan
name: N. Hidayat
name: E. Ihsan
name: D. Matualage
name: R. Mabrasar
name: D. Pada
Publisher: name: figshare
Year: 2018
Subjects: subject: 50202 Conservation and Biodiversity
subject: FOS: Biological sciences
subject: Marine Biology

description: We annually assessed nine Bird’s Head Seascape (BHS) marine protected areas (MPAs) using the World Bank MPA Score Card from 2012-2017. The score card provides a quantified summary of MPA management effectiveness, which allows status and trends in management to be tracked and compared through time. All nine BHS MPAs showed increases in management effectiveness. Mean management scores across the BHS MPA network increased from 60% in 2012 to 79% in 2017. The greatest gains were recorded for Kofiau, Kaimana, and Cenderawasih MPAs, with Kofiau MPA also having the greatest management effectiveness score in 2017 of all assessed MPAs. In general, our results suggest that MPA management effectiveness is improving in the BHS.
Cancer locusta Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Cancridae
Cancer
Cancer locusta

description: Cancer locusta [spec. nov.]
C. macrourus articularis, manibus adactylis, cauda attenuata spinis bifidis.
Roes. ins. 3. t. 62.
Klein. miss. 5. t. 6. f. A. B. C.
Habitat in Europae maritimis.
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 634, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Seyfert 1 mutation of the classical Seyfert 2 nucleus NGC 7582
Creators: name: Aretxaga, Itziar
name: Joguet, B.
name: Kunth, D.
name: Melnick, J.
name: Terlevich, R. J.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the transition towards a type 1 Seyfert experienced by the classical type 2 Seyfert nucleus in NGC 7582. The transition, found at most 20 days from its maximum peak, presents a unique opportunity to study these rare events in detail. At maximum the Ha line width is of about 12000 km/s. We examine three scenarios that could potentially explain the transition: capture of a star by a supermassive black hole, a reddening change in the surrounding torus, and the radiative onset of a type IIn supernova exploding in a compact nuclear/circumnuclear starburst.
description: Ap.J.Lett., in press. Also available at http://www.inaoep.mx/~itziar
XALQARO TURIZMNING MAZMUNI,  TURLARI VA TASHKILLASHTIRILISH BO'YICHA TASNIFLANISHI
Creators: name: Tashov, Mizrob
Publisher: name: Zenodo
Year: 2025

description: XX asrning so‘nggi o‘n yilligida xalqaro turizm eng yuqori texnologiyalar asosida rivojlanib borayotgan yaxlit bir infratuzilmaga aylandi.  Xalqaro turizmning mazmuni,  turlari va tashkillashtirilish bo‘yicha tasniflanishi haqida ilmiy mulohazalar yuritgan.
$K^0(\bar{K^0})$ Production in Two-Photon Processes at TRISTAN
Creators: name: Enomoto, R.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We have carried out an inclusive measurement of $K^0(\bar{K^0})$ production in two-photon processes at TRISTAN. The mean $\sqrt{s}$ was 58 GeV and the integrated luminosity was 199 pb$^{-1}$. High-statistics $K_s$ samples were obtained under such conditions as no-, anti-electron, and remnant-jet tags. The remnant-jet tag, in particular, allowed us, for the first time, to measure the cross sections separately for the resolved-photon and direct processes.
description: 20 pages, Latex format, 4 figures and KEK-mark included. Table 1 revised. To be published in Phys. Lett. B
Влияние сопроводительной иммунофармакотерапии на свободнорадикальные процессы и химиолучевую интоксикацию у больных раком шейки матки / С. В. Камышов, Д. А. Пулатов, О. Ю. Баленков, Н. Б. Юсупова // The scientific method, Warszawa, Poland. — 2018. — Т. 1, № 17. — С. 15–20.
Creators: name: Balenkov, Oleg
Publisher: name: figshare
Year: 2021

description: Influence of coherent immunopharmacotherapy on free radical processes and
chemoradiation intoxication in patients with uterine cervical cancer / S.
V. Kamyshov, D. A. Pulatov, O. Yu. Balenkov, N.B. Yusupova // // The
scientific method, Warszawa, Poland. — 2018. — V. 1, N 17. — P. 15–20.

Methods of extracorporeal immunopharmacotherapy made it possible to
significantly reduce the intensity of free radical processes in the blood serum
of patients with cervical cancer. At the same time, therapeutic measures to the
greatest extent reduced the indicators of the rapid flash and to the least -
the indicators of the light sum of the reaction of induced chemiluminescence.

Методы экстракорпоральной иммунофармакотерапии
позволяли в значительной остепени снизить интенсивность свободнорадикальных
процессов в сыворотке крови больных раком шейки матки. При этом лечебные
мероприятия в наибольшей степени снижали показатели быстрой вспышки и в
наименьшей – показатели светосуммы реакции индуцированной хемилюминесценции.
Improved graphene blisters by ultrahigh pressure sealing
Creators: name: Manzanares-Negro, Y.
name: Ares, P.
name: Jaafar, M.
name: López-Polín, G.
name: Gómez-Navarro, C.
name: Gómez-Herrero, J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Graphene is a very attractive material for nanomechanical devices and membrane applications. Graphene blisters based on silicon oxide micro-cavities are a simple but relevant example of nanoactuators. A drawback of this experimental set up is that gas leakage through the graphene-SiO2 interface contributes significantly to the total leak rate. Here we study the diffusion of air from pressurized graphene drumheads on SiO2 micro-cavities and propose a straightforward method to improve the already strong adhesion between graphene and the underlying SiO2 substrate, resulting in reduced leak rates. This is carried out by applying controlled and localized ultrahigh pressure (> 10 GPa) with an Atomic Force Microscopy diamond tip. With this procedure, we are able to significantly approach the graphene layer to the SiO2 surface around the drumheads, thus enhancing the interaction between them allowing us to better seal the graphene-SiO2 interface, which is reflected in up to ~ 4 times lower leakage rates. Our work opens an easy way to improve the performance of graphene as a gas membrane on a technological relevant substrate such as SiO2.
description: pages 19, 4 figures + supplementary information
title: 02_0523
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
Squeezed vacuum used to accelerate the search for a weak classical signal
Creators: name: Malnou, M.
name: Palken, D. A.
name: Brubaker, B. M.
name: Vale, Leila R.
name: Hilton, Gene C.
name: Lehnert, K. W.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Many experiments that interrogate fundamental theories require detectors whose sensitivities are limited by the laws of quantum mechanics. In cavity-based searches for axionic dark matter, vacuum fluctuations in the two quadratures of the cavity electromagnetic field limit the sensitivity to an axion-induced field. In an apparatus designed to partially mimic existing axion detectors, we demonstrate experimentally that such quantum limits can be overcome through the use of squeezed states. By preparing a microwave cavity in a squeezed state and measuring just the squeezed quadrature, we enhance the spectral scan rate by a factor of $2.12 \pm 0.08$. This enhancement is in excellent quantitative agreement with a theoretical model accounting for both imperfect squeezing and measurement.
description: 17 pages, 9 figures
Adaptive Bayesian Radio Tomography
Creators: name: Lee, Donghoon
name: Berberidis, Dimitris
name: Giannakis, Georgios B.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Signal Processing (eess.SP)
subject: Applications (stat.AP)
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: FOS: Computer and information sciences

description: Radio tomographic imaging (RTI) is an emerging technology to locate physical objects in a geographical area covered by wireless networks. From the attenuation measurements collected at spatially distributed sensors, radio tomography capitalizes on spatial loss fields (SLFs) measuring the absorption of radio frequency waves at each location along the propagation path. These SLFs can be utilized for interference management in wireless communication networks, environmental monitoring, and survivor localization after natural disaster such as earthquakes. Key to success of RTI is to model accurately the shadowing effects as the bi-dimensional integral of the SLF scaled by a weight function, which is estimated using regularized regression. However, the existing approaches are less effective when the propagation environment is heterogeneous. To cope with this, the present work introduces a piecewise homogeneous SLF governed by a hidden Markov random field (MRF) model. Efficient and tractable SLF estimators are developed by leveraging Markov chain Monte Carlo (MCMC) techniques. Furthermore, an uncertainty sampling method is developed to adaptively collect informative measurements in estimating the SLF. Numerical tests using synthetic and real datasets demonstrate capabilities of the proposed algorithm for radio tomography and channel-gain estimation.
Bounds on tail probabilities for quadratic forms in dependent sub-gaussian random variables
Creators: name: Zajkowski, Krzysztof
Publisher: name: arXiv
Year: 2018
Subjects: subject: Probability (math.PR)
subject: FOS: Mathematics
subject: 60E15

description: We show bounds on tail probabilities for quadratic forms in sub-gaussian non-necessarily independent random variables. Our main tool will be estimates of the Luxemburg norms of such forms. This will allow us to formulate the above-mentioned bounds. As an example we give estimates of the excess loss in fixed design linear regression in dependent observations.
description: 11 pages
Cancer salinus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Cancridae
Cancer
Cancer salinus

description: Cancer salinus [spec. nov.]
C. macrourus articularis, manibus adactylis, pedibus patentibus, cauda subulata.
Matii diar. britann. 1756.
Habitat in Angliae Salinis Limingtonianis. D. Schlosserus.
Corpus pediculo majus, oblongum. Oculi distantes, laterales, pedunculati. Antennae setaceae, corpore breviores. Cauda filiformi-subulata, exserta, longitudine corporis. Pedes utrinque 10 patentes & quasi pinnatim digesti.
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 634, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
On the Kinematic Reconstruction of Deep Inelastic Scattering at HERA: the $Σ$ Method
Creators: name: Bassler, Ursula
name: Bernardi, Gregorio
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We review and compare the reconstruction methods of the inclusive deep inelastic scattering variables used at HERA. We introduce a new prescription, the $Σ$ method, which allows to measure the structure function of the proton $F_2(x,Q^2)$ in a large kinematic domain, and in particular in the low x-low$Q^2$ region, with small systematic errors and small radiative corrections. A detailed comparison between the $Σ$ method and the other methods is shown. Extensions of the $Σ$ method are presented. The effect of QED radiation on the kinematic reconstruction and on the structure function measurement is discussed.
description: 18 pages, latex, 5 uuencoded figures
Comportamiento de la caries dental en la Comunidad Los Magallanes, San Diego estado Carabobo. Venezuela
Creators: name: Maylen Mendez
Publisher: name: figshare
Year: 2018
Subjects: subject: 110599 Dentistry not elsewhere classified
subject: FOS: Clinical medicine

description: Comportamiento de la caries en una comunidad de Venezuela
Affine equivalence and saddle connection graphs of half-translation surfaces
Creators: name: Pan, Huiping
Publisher: name: arXiv
Year: 2018
Subjects: subject: Geometric Topology (math.GT)
subject: Complex Variables (math.CV)
subject: FOS: Mathematics
subject: 30F60, 30F30, 54H15

description: To every half-translation surface, we associate a saddle connection graph, which is a subgraph of the arc graph. We prove that every isomorphism between two saddle connection graphs is induced by an affine homeomorphism between the underlying half-translation surfaces. We also investigate the automorphism group of the saddle connection graph, and the corresponding quotient graph.
description: 39 pages, 10 figures. Minor changes. Final version
Public Health Sector Readiness to Provide Malaria Case Management in Uganda
Creators: name: Muhwezi Stephen, Marian Warsame, Dr.Abdisalan Noor
Publisher: name: Zenodo
Year: 2024

description: Background: Malaria continues to be a global health burden, low and middle-income countries particularly in the World Health Organization Africa Region account for the highest disease burden in the Public Health Sector.  Readiness to provide appropriate care and management of malaria is pivotal in malaria control and elimination however there are research gaps in understanding the degree of readiness for Public Health Sector in Uganda. The purpose of this study was to measure the readiness of the public health facilities in Uganda to provide management for malaria. 

Methods: The study is a retrospective study based on health facility data available on the national health management information system; secondary data collected that is available in Ministry of health district reports; end-user verification surveys (EUV) done between 2016-2019 in collaboration with the United States President’s Malaria Initiative and Service Availability and Readiness Assessment (SARA) Uganda survey done in 2014 in collaboration with the World Health Organization. Analysis was done by region in Uganda. The indicators analysed were on treatment and availability of malaria commodities.

Results: The hospital and HC IV distribution across the regions in Uganda indicates northern region has 35 facilities compared to 51 and above facilities in other regions. The key health workers (nurses, doctors and clinical officers) approved positions filled in the different regions shows eastern region has the lowest at 68% and highest at 112% of the positions in the central region. In average, malaria treatments and diagnostics were available in 60% and 83%, respectively, in all regions. Stock out of commodities for case management (Rapid Diagnostic Tests and medicines) were the highest in 2016 and 2017.  Western region has the highest malaria testing rate (90.3%).

Conclusions. The survey found that Uganda's Public Health Service is not yet at 100 percent readiness, which is the benchmark level. However, the government should put emphasis on test and treat policies and evaluating health services on a regular basis. Furthermore, more efforts are needed on reducing stock outs of malaria case management commodities, notably RDTs, which are critical for giving fast and accurate test results.
Orthogonality of super-Jack polynomials and a Hilbert space interpretation of deformed Calogero-Moser-Sutherland operators
Creators: name: Atai, Farrokh
name: Hallnäs, Martin
name: Langmann, Edwin
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Algebra (math.QA)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences

description: We prove orthogonality and compute explicitly the (quadratic) norms for super-Jack polynomials $SP_λ((z_1,\ldots,z_n),(w_1,\ldots,w_m);θ)$ with respect to a natural positive semi-definite, but degenerate, Hermitian product $\langle\cdot,\cdot\rangle_{n,m}^\prime$. In case $m=0$ (or $n=0$), our product reduces to Macdonald's well-known inner product $\langle\cdot,\cdot\rangle_n^\prime$, and we recover his corresponding orthogonality results for the Jack polynomials $P_λ((z_1,\ldots,z_n);θ)$. From our main results, we readily infer that the kernel of $\langle\cdot,\cdot\rangle_{n,m}^\prime$ is spanned by the super-Jack polynomials indexed by a partition $λ$ not containing the $m\times n$ rectangle $(m^n)$. As an application, we provide a Hilbert space interpretation of the deformed trigonometric Calogero-Moser-Sutherland operators of type $A(n-1,m-1)$.
description: 19 pages, 1 figure
An Interplay of Topology and Quantized Geometric Phase for two Different Symmetry-Class Hamiltonians
Creators: name: S, Rahul
name: R, Ranjith Kumar
name: Kartik, Y R
name: Banerjee, Amitava
name: Sarkar, Sujit
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Study of symmetry, topology and geometric phase can reveal many new and interesting results on the topological states of matter. Here we present a completely new and interesting result of symmetry, topology and quantization of geometric phase along with the physical explanation for two different symmetry classes. We present a detailed study of the auxiliary space for two different symmetry classes of Hamiltonians. We show explicitly that the origin of the auxiliary space inside the curve is only a necessary condition but it is not a sufficient condition for the topological state. One of the most interesting results is that same symmetry-class Hamiltonians show different behaviour in topology and quantized geometric phase.
description: Comments are welcome
On Planetary Companions to the MACHO-98-BLG-35 Microlens Star
Creators: name: Rhie, S. H.
name: Bennett, D. P.
name: Becker, A. C.
name: Peterson, B. A.
name: Fragile, P. C.
name: Johnson, B. R.
name: Quinn, J. L.
name: Crouch, A.
name: Gray, J.
name: King, L.
name: Messenger, B.
name: Thomson, S.
name: Bond, I. A.
name: Abe, F.
name: Carter, B. S.
name: Dodd, R. J.
name: Hearnshaw, J. B.
name: Honda, M.
name: Jugaku, J.
name: Kabe, S.
name: Kilmartin, P. M.
name: Koribalski, B. S.
name: Masuda, K.
name: Matsubara, Y.
name: Muraki, Y.
name: Nakamura, T.
name: Nankivell, G. R.
name: Noda, S.
name: Rattenbury, N. J.
name: Reid, M.
name: Rumsey, N. J.
name: Saito, To.
name: Sato, H.
name: Sato, S.
name: Sekiguchi, M.
name: Sullivan, D. J.
name: Sumi, T.
name: Watase, Y.
name: Yanagisawa, T.
name: Yock, P. C. M.
name: Yoshizawa, M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present observations of microlensing event MACHO-98-BLG-35 which reached a peak magnification factor of almost 80. These observations by the Microlensing Planet Search (MPS) and the MOA Collaborations place strong constraints on the possible planetary system of the lens star and show intriguing evidence for a low mass planet with a mass fraction $4\times 10^{-5} \leq ε\leq 2\times 10^{-4}$. A giant planet with $ε= 10^{-3}$ is excluded from 95% of the region between 0.4 and 2.5 $R_E$ from the lens star, where $R_E$ is the Einstein ring radius of the lens. This exclusion region is more extensive than the generic "lensing zone" which is $0.6 - 1.6 R_E$. For smaller mass planets, we can exclude 57% of the "lensing zone" for $ε= 10^{-4}$ and 14% of the lensing zone for $ε= 10^{-5}$. The mass fraction $ε= 10^{-5}$ corresponds to an Earth mass planet for a lensing star of mass $\sim 0.3 \msun$. A number of similar events will provide statistically significant constraints on the prevalence of Earth mass planets. In order to put our limits in more familiar terms, we have compared our results to those expected for a Solar System clone averaging over possible lens system distances and orientations. We find that such a system is ruled out at the 90% confidence level. A copy of the Solar System with Jupiter replaced by a second Saturn mass planet can be ruled out at 70% confidence. Our low mass planetary signal (few Earth masses to Neptune mass) is significant at the $4.5σ$ confidence level. If this planetary interpretation is correct, the MACHO-98-BLG-35 lens system constitutes the first detection of a low mass planet orbiting an ordinary star without gas giant planets.
description: ApJ, April 1, 2000; 27 pages including 8 color postscript figures
New Tagging Method of B Flavor of Neutral B Meson in CP Violation Measurement in Asymmetric B-Factory Experiment
Creators: name: Enomoto, R.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: In CP violation measurements in asymmetric B-factory experiments, a determination of the B flavor of the neutral B mesons is necessary. A new method to this purpose using only three vectors of charged particles has been developed. This method (weighted charge method) does not require either lepton identification or charged-kaon identification. The tagging efficiency, probability for incorrect tagging, and effective tagging efficiency of this method are 43.1, 18.3, and 17.3\%, respectively.
description: 6 pages, Latex format (article), 3 figures, published in J. of Phys. Soc. Jpn. Vol. 63 (1994) 3542
Neue europäische Geschichte(n) wagen
Creators: name: Unger, Corinna R.
Publisher: name: Comparativ
Year: 2021

description: Besprechung der Reihe Making Europe: Technology and Transformations, 1850–2000. Hrsg. von Johan Schot und Philip Scranton, 6 Bände, Basingstoke: Palgrave Macmillan, 2013–2019.
description: Comparativ, Vol. 31 No. 01 (2021): Re-Education Revisited: Conflicting Agendas and Cross-Cultural Agency in the Early Cold War