cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Charge-to-heat transducers exploiting the Neganov-Trofimov-Luke effect for light detection in rare-event searches
Creators: name: Novati, V.
name: Bergé, L.
name: Dumoulin, L.
name: Giuliani, A.
name: Mancuso, M.
name: de Marcillac, P.
name: Marnieros, S.
name: Olivieri, E.
name: Poda, D. V.
name: Tenconi, M.
name: Zolotarova, A. S.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: In this work we present how to fabricate large-area (15 cm2), ultra-low threshold germanium bolometric photo-detectors and how to operate them to detect few (optical) photons. These detectors work at temperatures as low as few tens of mK and exploit the Neganov-Trofimov-Luke (NTL) effect. They are operated as charge-to-heat transducers: the heat signal is linearly increased by simply changing a voltage bias applied to special metal electrodes, fabricated onto the germanium absorber, and read by a (NTD-Ge) thermal sensor. We fabricated a batch of five prototypes and ran them in different facilities with dilution refrigerators. We carefully studied how impinging spurious infrared radiation impacts the detector performances, by shining infrared photons via optical-fiber-guided LED signals, in a controlled manner, into the bolometers. We hence demonstrated how the radiation-tightness of the test environment tremendously enhances the detector performances, allowing to set electrode voltage bias up to 90 volts without any leakage current and signal-to-noise gain as large as a factor 12 (for visible photons). As consequence, for the first time we could operate large-area NTD-Ge-sensor-equipped NTL bolometric photo-detectors capable to reach sub 10-eV baseline noise (RMS). Such detectors open new frontiers for rare-event search experiments based on low light yield Ge-NTD equipped scintillating bolometers, such the CUPID neutrinoless double-beta decay experiment.
Additional file 2: of Association between phenotype and deletion size in 22q11.2 microdeletion syndrome: systematic review and meta-analysis
Creators: name: M. Rozas
name: Benavides, Felipe
name: Leรณn, Luis
name: Repetto, Gabriela
Publisher: name: figshare
Year: 2019
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Science Policy
subject: Computational Biology

description: Raw data from individual studies. Table with the frequency of phenotypic outcomes cross tabulated with information on deletion size and segment of deletion. (PDF 52 kb)
Parity properties of an advection-dominated solar $α^2\Om$-dynamo
Creators: name: Bonanno, A.
name: Elstner, D.
name: Ruediger, G.
name: Belvedere, G.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have developed a high-precision code which solves the kinematic dynamo problem both for given rotation law and meridional flow in the case of a low eddy diffusivity of the order of $10^{11}$ cm$^2$/s known from the sunspot decay. All our models work with an \alf-effect which is positive (negative) in the northern (southern) hemisphere. It is concentrated in radial layers located either at the top or at the bottom of the convection zone. We have also considered an \alf-effect uniformly distributed in all the convection zone. In the present paper the main attention is focused on i) the parity of the solution, ii) the form of the butterfly diagram and iii) the phase relation of the resulting field components. If the helioseismologically derived internal solar rotation law is considered, a model without meridional flow of high magnetic Reynolds number (corresponding to low eddy diffusivity) fails in all the three issues in comparison with the observations. However, a meridional flow with equatorial drift at the bottom of the convection zone of few meters by second can indeed enforce the equatorward migration of the toroidal magnetic field belts similar to the observed butterfly diagram but, the solution has only a dipolar parity if the (positive) \alf-effect is located at the base of the convection zone rather than at the top. We can, therefore, confirm the main results of a similar study by Dikpati & Gilman (2001).
description: 9 pages, 16 figures, to appear on Astronomy and Astrophysics
Generalizations of the Ruzsa-Szemerédi and rainbow Turán problems for cliques
Creators: name: Gowers, W. T.
name: Janzer, Barnabás
Publisher: name: arXiv
Year: 2020
Subjects: subject: Combinatorics (math.CO)
subject: FOS: Mathematics

description: Considering a natural generalization of the Ruzsa-Szemerédi problem, we prove that for any fixed positive integers $r,s$ with $r
description: 19 pages, 1 figure. Minor changes in Subsection 5.1 compared to the first version
Additional file 1: of Association between phenotype and deletion size in 22q11.2 microdeletion syndrome: systematic review and meta-analysis
Creators: name: M. Rozas
name: Benavides, Felipe
name: Leรณn, Luis
name: Repetto, Gabriela
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: List of citations of the systematic review. Table with the information of individual studies that were identified by the systematic review, inclusion/exclusion status and justification. (PDF 455 kb)
ПРЕДПРИЯТИЕ И ЕГО ХОЗЯЙСТВЕННАЯ ДЕЯТЕЛЬНОСТЬ – КАК ОБЪЕКТ ПЛАНИРОВАНИЕ
Creators: name: Насруллаев Феруз Фурқатович Управляющий АКИБ "Ипотека банк"
Publisher: name: Zenodo
Year: 2024

description: В данной статье автором освещаются современная экономика и ее структурная структура, значение и роль планирования в развитии деятельности предприятия.

Ключевые слова. экономика, домашнее хозяйство, бизнес, предпринимательство.
Infrasonic, acoustic and seismic waves produced by the Axion Quark Nuggets
Creators: name: Budker, Dmitry
name: Flambaum, Victor V.
name: Zhitnitsky, Ariel
Publisher: name: arXiv
Year: 2020
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Atmospheric and Oceanic Physics (physics.ao-ph)
subject: Geophysics (physics.geo-ph)
subject: FOS: Physical sciences

description: We advocate an idea that the Axion Quark Nuggets (AQN) hitting the Earth can be detected by analysing the infrasound, acoustic and seismic waves which always accompany the AQN's passage in the atmosphere and underground. Our estimates for the infrasonic frequency $ν\simeq 5$ ~Hz and overpressure $δp\sim 0.3 ~$Pa for relatively large size dark matter (DM) nuggets suggest that sensitivity of presently available instruments is already sufficient to detect very intense (but very rare) events today with existing technology. A study of much more frequent but less intense events requires a new type of instruments. We propose a detection strategy for a systematic study to search for such relatively weak and frequent events by using Distributed Acoustic Sensing and briefly mention other possible detection methods.
description: Paper is restructured, title is changed. All technical results remain identically the same
NEWSERA (873125) Deliverable 6.1 - Events 1
Creators: name: Lazzarato, Lisa
name: Arias, Rosa
name: Agulló, Oriol
Publisher: name: Zenodo
Year: 2020
Subjects: science communication
citizen science
events
co-creation
co-design
network
european commission
open science
methodology
participation

description: This document presents the events attended and planned by the NEWSERA consortium to
 promote, disseminate and actively engage the project with different audiences during its first
 year of activity. NEWSERA will analyse and evaluate the complex and multidirectional science
 communication strategies, including digital and non-digital ones, addressed to
 quadruple helix stakeholders in citizen science projects across Europe as the new
 paradigm for science communication. The overall aim of NEWSERA is to demonstrate the virtues of citizen science as an
 inclusive, broad and powerful science communication mechanism that can allow to
 increase trust in science communication and, in turn, in science at large, while opening
 up science and innovation to society, raising awareness and educating in science, and
 reducing the chances of incurring in fake news by promoting critical thinking. This project has received funding from the European Union’s Horizon 2020 research
 and innovation programme under grant agreement No 873125
JHK Spectra of the z=2.39 Radio Galaxy 53W002
Creators: name: Motohara, K.
name: Yamada, T.
name: Iwamuro, F.
name: Hata, R.
name: Taguchi, T.
name: Harashima, T.
name: Maihara, T.
name: Iye, M.
name: Simpson, C.
name: Yoshida, M.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present low-resolution, near-IR JHK spectra of the weak z=2.39 radio galaxy 53W002, obtained with the OH-airglow Suppressor spectrograph (OHS) and Cooled Infrared Spectrograph and Camera for OHS (CISCO) on the Subaru Telescope. They cover rest-frame wavelengths of 3400-7200 A, and the emission lines of [O II]3727, Hb, [O III]4959, 5007, Ha, [N II]6548, 6583 and [S II]6716, 6731 were detected. Using the Ha/Hb line ratio, we find an extinction of E(B-V)=0.14. The emission-line ratios are reproduced by a cloud of electron density n_e=1x10^{3-4}(/cm3) with solar metallicity, ionized by an alpha=-0.7 power-law continuum with ionizing parameter U=1x10^-3. In addition to these emission lines, we make the first spectroscopic confirmation of the Balmer discontinuity in a high-z radio galaxy. Together with rest-frame UV photometry from the literature, we show that at least 1/3 of the present stellar mass was formed in the current starburst. The stellar mass was estimated to be (1-1.4)x10^11 M_sol by one-component model fitting, which is smaller than that of typical z~1 B2/6C radio galaxies. We suggest that 53W002 is currently assembling a large part of its stellar mass through merger events with the surrounding sub-galactic clumps, some of which can be identified with the Lya emitters detected in narrow-band imaging. After a few such events over the next few Gyr, 53W002 will evolve into a massive elliptical galaxy.
description: 10 pages, including 11 figures. Accepted for publication in PASJ(2001). Revised 5/15/2001
Mezira pauperula KORMILEV 1962
Creators: name: Heiss, E.
name: Moragues, G.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Aradidae
Mezira
Mezira pauperula

description: Mezira pauperula KORMILEV 1962
L i t e r a t u r e d a t a:describedfromBrazil.
M a t e r i a l e x a m i n e d:333 1♀ Guyane Française Camopi, lg. F. Geay 1900, coll. Mus. Paris and CEHI (ex. coll. Kormilev); 1♀ 2km SSO Sinnamary, Station de Paracou 5°16N, 52°56W 20m, 15.-16.VI.1995, Gusarov lg. (CEHI ex coll. Zool. Inst. St. Petersburg).
description: Published as part of Heiss, E. & Moragues, G., 2009, Flat Bugs of French Guyana - a preliminary faunal list (Heteroptera, Aradidae), pp. 1659-1675 in Linzer biologische Beiträge 41 (2) on page 1670, DOI: 10.5281/zenodo.5279382
Additional file 5: of Interventions to prevent iatrogenic anemia: a Laboratory Medicine Best Practices systematic review
Creators: name: Whitehead, Nedra
name: Williams, Laurina
name: Sreelatha Meleth
name: Kennedy, Sara
name: Nneka Ubaka-Blackmoore
name: Geaghan, Sharon
name: Nichols, James
name: Carroll, Patrick
name: McEvoy, Michael
name: Gayken, Julie
name: Ernst, Dennis
name: Litwin, Christine
name: Epner, Paul
name: Taylor, Jennifer
name: Graber, Mark
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: Computational Biology

description: Evidence tables. (DOCX 24 kb)
Tuning of impurity-bound interlayer complexes in a van der Waals heterobilayer
Creators: name: Vialla, Fabien
name: Danovich, Mark
name: Ruiz-Tijerina, David A.
name: Massicotte, Mathieu
name: Schmidt, Peter
name: Taniguchi, Takashi
name: Watanabe, Kenji
name: Hunt, Ryan J.
name: Szyniszewski, Marcin
name: Drummond, Neil D.
name: Pedersen, Thomas G.
name: Fal'ko, Vladimir I.
name: Koppens, Frank H. L.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Due to their unique two-dimensional nature, charge carriers in semiconducting transition metal dichalcogenides (TMDs) exhibit strong unscreened Coulomb interactions and sensitivity to defects and impurities. The versatility of van der Waals layer stacking allows spatially separating electrons and holes between different TMD layers with staggered band structure, yielding interlayer few-body excitonic complexes whose nature is still debated. Here we combine quantum Monte Carlo calculations with spectrally and temporally resolved photoluminescence measurements on a top- and bottom-gated MoSe2/WSe2 heterostructure, and identify the emitters as impurity-bound interlayer excitonic complexes. Using independent electrostatic control of doping and out-of-plane electric field, we demonstrate control of the relative populations of neutral and charged complexes, their emission energies on a scale larger than their linewidth, and an increase of their lifetime into the microsecond regime. This work unveils new physics of confined carriers and is key to the development of novel optoelectronics applications.
$β$-Boundedness, Semipassivity, and the KMS-Condition
Creators: name: Kuckert, Bernd
Publisher: name: arXiv
Year: 2001
Subjects: subject: Mathematical Physics (math-ph)
subject: High Energy Physics - Theory (hep-th)
subject: Operator Algebras (math.OA)
subject: FOS: Physical sciences
subject: FOS: Mathematics
subject: 82B03, 82B10, 83A05, 46L60

description: The proof of a recent result by Guido and Longo establishing the equivalence of the KMS-condition with complete $β$-boundedness is shortcut and generalized in such a way that a covariant version of the theorem is obtained.
description: 7 pages, 'complete' inserted in statement of main theorem
Breast feeding practices among mothers attending measles immunisation for their infants at hingalol hospital".
Creators: name: Asia, Faisal Ahmed
Publisher: name: Zenodo
Year: 2025
Subjects: Breast feeding
practices among
mothers attending
measles immunisation for their infants at hingalol hospital

description: Abstract

Promotion, support and protection of optimal breastfeeding practices for infants aged 0–6 months at community and facility levels through promoting early initiation of breastfeeding within one hour of birth, exclusive breastfeeding in the first 6 months of life and continued breastfeeding up to 2+ years.  Establishment of a phased scaling-up of baby friendly health facilities to ensure that the health care system protects, promotes and supports optimal breastfeeding practices while providing women with the support.

Objectives: To asses breast feeding practices among mothers with babies aged less than or greater than 6 months attending immunization at hingalol hospital.

 

Methodology: This study was used quantitative descriptive cross-sectional study because; the cross-sectional study is in depth investigation of an individual, group. The cross sectional helps the researchers to study multiple entities in depth in order to gain insight into the larger case and to describe and explain rather than predict a phenomenon.

Results; The study was carried out hingalol hospital, to seek the BFP advantages of breast feeding both mothers and children and the objectives of the study have been met

Ø Maternal knowledge regarding advantages of breastfeeding was not adequate.

 Ø Undesirable cultural feeding practices such as giving other fluids and avoiding exclusive

 Ø Breastfeeding were still prevalent among mothers.

 Ø The mothers not get adequate awareness about breast feeding The main sources of information on breastfeeding for mothers were from their mothers

 Ø Majority of mothers practice breast feeding but the knowledge of breast feeding advantages and it‘s important not improved.

Recommendations;
Nannium kormilevi DOESBURG 1997
Creators: name: Heiss, E.
name: Moragues, G.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Aradidae
Nannium
Nannium kormilevi

description: Nannium kormilevi DOESBURG 1997
L i t e r a t u r e d a t a: described from Surinam.
M a t e r i a l e x a m i n e d 1♀ Amazon Nature Lodge, 30km SE Roura on Kaw Rd, N 04°.33.570’, W 52°.12.433’, 300m, 18-23.IV.2007, UV light trap, lg. J. Eger (CEHI).
 N o t e: This genus contains to date 5 Neotropical species (Brazil, Venezuela, Guatemala) and 1 Nearctic species (USA) and no key is available. However our specimen corresponds to the description of N. kormilevi.
D i s t r i b u t i o n: Surinam,FrenchGuyana.
description: Published as part of Heiss, E. & Moragues, G., 2009, Flat Bugs of French Guyana - a preliminary faunal list (Heteroptera, Aradidae), pp. 1659-1675 in Linzer biologische Beiträge 41 (2) on page 1670, DOI: 10.5281/zenodo.5279382
Gravitational waves from first-order phase transitions: Ultra-supercooled transitions and the fate of relativistic shocks
Creators: name: Jinno, Ryusuke
name: Seong, Hyeonseok
name: Takimoto, Masahiro
name: Um, Choong Min
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: We study the gravitational wave (GW) production in extremely strong first order phase transitions where the latent heat density dominates the plasma energy density, $α\gtrsim 1$. In such transitions, bubbles develop extremely thin and relativistic fluid configurations, resulting in strong shock waves after collisions. We first propose a strategy to understand the GW production in such a system by separating the problem into the propagation part and the collision part. Focusing on the former, we next develop an effective theory for the propagation of the relativistic fluid shells. Using this effective theory, we finally calculate the expected duration of the relativistic fluid configurations and discuss its implications to the GW production.
description: 34 pages, 14 figures
Interaction between Ionized and Molecular Gas in the Active Star-Forming Region W31
Creators: name: Kim, Kee-Tae
name: Koo, Bon-Chul
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have carried out 21 cm radio continuum, H76_αradio recombination line, and various (CO, ^13CO, CS, & C^34S) molecular line observations of the W31 complex. Our radio continuum data show that W31 is composed of two extended HII regions, G10.2-0.3 and G10.3-0.1, each of which comprises an ultracompact HII region, two or more compact components, and diffuse envelope. The W31 cloud appears as an incomplete shell on the whole and consists of southern spherical and northern flat components, which are associated with G10.2-0.3 and G10.3-0.1, respectively. We detect two large and massive CS-emitting regions in the northern and southern cloud components. The large amount of dense gas may suggest that the W31 cloud has ability to form rich stellar clusters and that star formation has only recently begun. The extended envelopes of both G10.2-0.3 and G10.3-0.1 are likely to be results of the champagne flows, based on the distributions of ionized and molecular gas and the velocity gradient of H76_αline emission. We find strong evidence of bipolar molecular outflows associated with the two ultracompact HII regions. In the vicinity of the ultracompact and compact HII regions in G10.3-0.1, the CO J=2-1/J=1-0 intensity ratio is high (1.4) and a small but prominent molecular gas hollow exists. These observations strongly indicate that the HII regions and their ionizing stars are interacting with the molecular cloud. Therefore, it is most likely that recently formed massive stars are actively disrupting their parental molecular cloud in the W31 complex.
description: 26 pages, including 10 figures, accepted for publication in ApJ
Thermodynamic cost, speed, fluctuations, and error reduction of biological copy machines
Creators: name: Song, Yonghyun
name: Hyeon, Changbong
Publisher: name: arXiv
Year: 2020
Subjects: subject: Biological Physics (physics.bio-ph)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: Due to large fluctuations in cellular environments, transfer of information in biological processes without regulation is inherently error-prone. The mechanistic details of error-reducing mechanisms in biological copying processes have been a subject of active research; however, how error reduction of a process is balanced with its thermodynamic cost and dynamical properties remain largely unexplored. Here, we study the error reducing strategies in light of the recently discovered thermodynamic uncertainty relation (TUR) that sets a physical bound to the cost-precision trade-off relevant in general dissipative processes. We found that the two representative copying processes, DNA replication by the exonuclease-deficient T7 DNA polymerase and mRNA translation by the \textit{E. coli} ribosome, reduce the error rates to biologically acceptable levels while also optimizing the processes close to the physical limit dictated by TUR.
description: 20 pages, 14 figures, 3 Tables
A New Measurement of the Primordial Abundance of Deuterium: Toward Convergence with the Baryon Density from the CMB?
Creators: name: Pettini, Max
name: Bowen, David V.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: From the analysis of the near-UV spectrum of the QSO 2206-199, obtained with a long series of exposures with STIS on the HST, we deduce a value (D/H) = (1.65 +/- 0.35) x 10(-5) (1 sigma error) for the abundance of deuterium in the z(abs) = 2.0762 damped Lyman alpha system (DLA) along this sight-line. The velocity structure of this absorber is very simple and its neutral hydrogen column density, N(H I), is accurately known; the error in D/H is mostly due to the limited signal-to-noise ratio of the spectrum. Since this is also one of the most metal-poor DLAs, with metal abundances of about 1/200 of solar, the correction due to astration of D is expected to be insignificant and the value we deduce should be essentially the primordial abundance of deuterium. When all (six) available measurements of D/H in high redshift QSO absorbers are considered, we find that the three DLAs---where N(H I) is measured most reliably---give consistently lower values than the three Lyman limit systems. We point out that the weighted mean of the DLA measurements, D/H = (2.2 +/- 0.2) x 10(-5), yields a baryon density Omega_B h^2 = 0.025 +/- 0.001 which is within 1 sigma of the value deduced from the analysis of the CMB angular power spectrum, and is still consistent with the present-day D/H and models of Galactic chemical evolution. Future observations of D I absorption in other DLAs are needed to establish whether our finding reflects a real advantage of DLAs over other classes of QSO absorbers for the measurement of D, or is just a statistical fluctuation.
description: 18 pages, LaTeX, 5 Postscript Figures. Revised version including latest CMB results. Accepted for publication in the Astrophysical Journal, scheduled for Vol. 560 (Oct 10, 2001 issue)
Neuroctenus longulus BERGROTH 1898
Creators: name: Heiss, E.
name: Moragues, G.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Aradidae
Neuroctenus
Neuroctenus longulus

description: Neuroctenus longulus BERGROTH 1898
L i t e r a t u r e d a t a: described from Cayenne.
M a t e r i a l e x a m i n e d 13 Régina, Montagne de Kaw PK35, 11.XII.2007 lg. Cerda (CGMM); 1♀ RN2 PK22, Montagne des Chevaux, 16.XI.2008, 13 22.XI.2008, piège vitre d’interception, lg. S. Brulé & P.H. Dalens (CGMM); 1♀ RN2 PK 65, Tibourou, 15.III.2008, piège vitre d’interception, lg. S. Brulé & P.H. Dalens (CGMM); 1♀ Régina, RN2 PK 125+3, 29.X.2007, 1♀ 5.XI.2007, 13 19.III.2008, 1♀ 2.VIII.2008, piège vitre d’interception, lg. J.L. Giuglaris (CGMM); 1♀ " Cayenne ", 1827 lg. Hille (CEHI ex Mus. Paris); 13 4♀♀ Montagne de Kaw, 200- 300m, 28.VI-12.VII.2007 lg. Puchner (CEHI).
D i s t r i b u t i o n:FrenchGuyana, Surinam.
 N o t e: The pygophore of the male is very similar to N. punctulatus BURMEISTER 1835 from Brazil. The key to Neotropical Neuroctenus given by KORMILEV (1963) is outdated due to several additional species which were described later and no genitalic structures were considered.
description: Published as part of Heiss, E. & Moragues, G., 2009, Flat Bugs of French Guyana - a preliminary faunal list (Heteroptera, Aradidae), pp. 1659-1675 in Linzer biologische Beiträge 41 (2) on page 1670, DOI: 10.5281/zenodo.5279382
TERRORISM EFFECTS ON SOCIETY AND INDIVIDUALS
Creators: name: Mohamoud, Hassan Zeid
Publisher: name: Zenodo
Year: 2025
Subjects: TERRORISM EFFECTS
SOCIETY AND INDIVIDUALS

description:                                                                  Abstract

The calculated use of violence creates a general climate of fear in a Population and thereby brings about a particular political objective known as terrorism has been practiced by political organizations with both rightist and nationalistic and religious groups, by revolutionaries, and even by state institutions such as armies, intelligence services, and police. Donations are rare and controversial.
Additional file 4: of Reproducible changes in the gut microbiome suggest a shift in microbial and host metabolism during spaceflight
Creators: name: Jiang, Peng
name: Green, Stefan
name: Chlipala, George
name: Turek, Fred
name: Vitaterna, Martha
Publisher: name: figshare
Year: 2019
Subjects: subject: Biophysics
subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Physiology
subject: Sociology
subject: FOS: Sociology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified

description: Figure S3. Comparison between inferred gene abundance of microbial pathways predicted with the PICRUSt default reference and iMGMC reference. (A) A Venn diagram showing the number of pathways uncovered with each of the reference catalogs. (B) Coefficients of pathway-wise correlations computed for each of the samples showing a high agreement in the predicted gene abundance of pathways uncovered by both reference catalogs. (C) Sample-wise correlations between the relative abundance predicted using the two reference catalogs were computed for each of the pathways, and a histogram is used here to show the distribution of correlation coefficients. CLR-transformed relative abundance was used to compute correlation coefficients. (D) A scatter plot showing the overall similarity (Pearsonâ s r = 0.61, P = 6.98 Ă 10-61) in the differential abundance effect sizes estimated by ALDEx2 using gene abundance predicted with either reference catalog. Each point denotes a pathway that commonly uncovered using both references, and points filled with colors indicate pathways found to be differentially abundant (FDR < 0.1, ALDEx2) when the abundance was predicted using either reference or both. The lower correlation coefficients in C and D compared to B was expected, as differences in the number of pathways uncovered with each reference influences the estimated total sequence abundance and thus the estimated relative abundance of each predicted pathway. (PDF 1300 kb)
NEWSERA (873125) Deliverable 6.3 - NEWSERA Visual Identity
Creators: name: Lazzarato, Lisa
name: Seoane, Nora Salas
name: Arias, Rosa
Publisher: name: Zenodo
Year: 2020
Subjects: communication plan
Visual Identity
NEWSERA
citizen science

description: The NEWSERA visual identity aims to provide an identifiable and unique look to the project, making it immediately recognizable in every dissemination and communication activities and materials. The power of visual communication is also well-known and fundamental to ensure a successful dissemination and communication plan.
 The project’s logo is the basis of the development of the visual identity, which encompasses a brand book containing guidelines for its implementation and template documents to be used in any project related activity. The NEWSERA website, designed according to the visual identity, is the primary source of information about the project. Its present version describes the project's most relevant information and will then expand, according to the project development, hosting more and more content. The website will also represent the NEWSERA project's legacy, making available results, contents, and materials long after the project end. This project has received funding from the European Union’s Horizon 2020 research and innovation programme under grant agreement No 873125
A Multi-Threaded Fast Convolver for Dynamically Parallel Image Filtering
Creators: name: Kepner, Jeremy
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: Distributed, Parallel, and Cluster Computing (cs.DC)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: 2D convolution is a staple of digital image processing. The advent of large format imagers makes it possible to literally ``pave'' with silicon the focal plane of an optical sensor, which results in very large images that can require a significant amount computation to process. Filtering of large images via 2D convolutions is often complicated by a variety of effects (e.g., non-uniformities found in wide field of view instruments). This paper describes a fast (FFT based) method for convolving images, which is also well suited to very large images. A parallel version of the method is implemented using a multi-threaded approach, which allows more efficient load balancing and a simpler software architecture. The method has been implemented within in a high level interpreted language (IDL), while also exploiting open standards vector libraries (VSIPL) and open standards parallel directives (OpenMP). The parallel approach and software architecture are generally applicable to a variety of algorithms and has the advantage of enabling users to obtain the convenience of an easy operating environment while also delivering high performance using a fully portable code.
description: 25 pages including color figures. Submitted to the Journal of Parallel and Distributed Computing
Eccentricity Evolution of Resonant Migrating Planets
Creators: name: Murray, N.
name: Paskowitz, M.
name: Holman, M.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We examine the eccentricity evolution of a system of two planets locked in a mean motion resonance, in which the outer planet loses energy and angular momentum. The sink of energy and angular momentum could be either a gas or planetesimal disk. We show that the eccentricity of both planetary bodies can grow to large values, particularly if the inner body does not directly exchange energy or angular momentum with the disk. We analytically calculate the eccentricity damping rate in the case of a single planet migrating through a planetesimal disk. We present the results of numerical integrations of two resonant planets showing rapid growth of eccentricity. We also present integrations in which a Jupiter-mass planet is forced to migrate inward through a system of 5-10 roughly Earth mass planets. The migrating planet can eject or accrete the smaller bodies; roughly 5% of the mass (averaged over all the integrations) accretes onto the central star. The results are discussed in the context of the currently known extrasolar planetary systems.
description: 35 pages, 7 figures
Ultracold collisions of Cs in excited hyperfine and Zeeman states
Creators: name: Frye, Matthew D.
name: Yang, B. C.
name: Hutson, Jeremy M.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: We investigate Cs+Cs scattering in excited Zeeman and hyperfine states. We calculate the real and imaginary parts of the s-wave scattering length; the imaginary part directly provides the rate coefficient for 2-body inelastic loss, while the real part allows us to identify regions of magnetic field where 3-body recombination will be slow. We identify field regions where Cs in its $(f,m_f)=(3,+2)$ and $(3,+1)$ states may be stable enough to allow Bose-Einstein condensation, and additional regions for these and the $(3,0)$ and $(3,-3)$ states where high-density clouds should be long-lived.
description: 7 pages, 3 figures
Experience of high resolution VLBI imaging using generalized maximum entropy method
Creators: name: Bajkova, Anisa T.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The generalized maximum entropy method (GMEM) is a special modification of the standard maximum entropy method (MEM) which seeks solutions in the space of complex functions. In this work a reduced version of the GMEM intended for reconstructing real images with positive and negative values is used. As compared with the standard MEM, intended for the reconstruction of only non-negative images, the GMEM allows us to obtain higher-quality images with a much lower level of nonlinear distortions caused by errors in the data. Here, we present the results of the GMEM imaging of 36 selected extragalactic radio sources with a resolution of 0.3-0.5 mas on astrometric and geodetic VLBI observations at 8.2 GHz, obtained with a global array in the period from 1994-1996. In VLBI mapping practice this is the first experience of imaging with such a high resolution using maximum entropy technique. A differential maximum entropy method intended for increasing the dynamic range of images is demonstrated on the radio source 0059+581. In the case of unreliable `closure' phases, completely `phaseless' methods of mapping are recommended. Maps of two sources 0615+820 and 0642+214 are obtained using one such method.
description: Latex, 11 pages with 4 Postscript figures (images of 36 extragalactic radio sources)
Phyllotingis lanceolata
Creators: name: Heiss, E.
name: Moragues, G.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Aradidae
Phyllotingis
Phyllotingis lanceolata

description: Phyllotingis lanceolata (FABRICIUS 1803)
L i t e r a t u r e d a t a: described from "America meridionalis"; 13 French Guyana, Cayenne, Alicoto III.1981 lg. León (HEISS 1993).
M a t e r i a l e x a m i n e d 13 Montagne de Kaw PK 36, 17.VII.2000, piège malaise, 1♀ 29.X.2003, à vue, lg. J.A. Cerda (CGMM); 13 2♀♀ Régina, RN 2 PK 125 + 3, 9.X.2007, 13 21.X.2007, 2♀♀ 19.III.2008, 1♀ 26.VII.2008, 1♀ 19.VII.2008, 13 6.XII.2008, all piège vitre d’interception, lg. J.L. Giuglaris (CGMM).
D i s t r i b u t i o n: Recorded from Surinam, French Guyana, Brazil and Peru.
description: Published as part of Heiss, E. & Moragues, G., 2009, Flat Bugs of French Guyana - a preliminary faunal list (Heteroptera, Aradidae), pp. 1659-1675 in Linzer biologische Beiträge 41 (2) on pages 1671-1672, DOI: 10.5281/zenodo.5279382
Model-independent constraints on the hydrogen-ionizing emissivity at z>6
Creators: name: Mason, Charlotte A.
name: Naidu, Rohan P.
name: Tacchella, Sandro
name: Leja, Joel
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Modelling reionization often requires significant assumptions about the properties of ionizing sources. Here, we infer the total output of hydrogen-ionizing photons (the ionizing emissivity, $\dot{N}_\textrm{ion}$) at $z=4-14$ from current reionization constraints, being maximally agnostic to the properties of ionizing sources. We use a Bayesian analysis to fit for a non-parametric form of $\dot{N}_\textrm{ion}$, allowing us to flexibly explore the entire prior volume. We infer a declining $\dot{N}_\textrm{ion}$ with redshift at $z>6$, which can be used as a benchmark for reionization models. Model-independent reionization constraints from the CMB optical depth and Ly$α$ and Ly$β$ forest dark pixel fraction produce $\dot{N}_\textrm{ion}$ evolution ($d\log_{10}\dot{N}_\textrm{ion}/dz|_{z=6\rightarrow8} = -0.31\pm0.35$ dex) consistent with the declining UV luminosity density of galaxies, assuming constant ionizing photon escape fraction and efficiency. Including measurements from Ly$α$ damping of galaxies and quasars produces a more rapid decline: $d\log_{10}\dot{N}_\textrm{ion}/dz|_{z=6\rightarrow8} =-0.44\pm0.22$ dex, steeper than the declining galaxy luminosity density (if extrapolated beyond $M_\mathrm{UV} \lesssim -13$), and constrains the mid-point of reionization to $z = 6.93\pm0.14$.
description: submitted to MNRAS
Phyllotingis Walker 1873
Creators: name: Heiss, E.
name: Moragues, G.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Aradidae
Phyllotingis

description: Phyllotingis cf. triangula HEISS 1993
L i t e r a t u r e d a t a: described from Mato Grosso in Brazil, only the male holotype is known to date.
M a t e r i a l e x a m i n e d: 1♀ Régina, RN2 PK 125+3, 11.XI.2008, piège vitre d’interception, lg. J.L.Giuglaris (CEHI).
N o t e: Due to the pronotal structure, the size and the antennal segment II without pilosity, it seems possible that this specimen might represent the unknown female. Unless more material of both sexes is available for a comparative examination, the taxonomic assignment remains uncertain.
description: Published as part of Heiss, E. & Moragues, G., 2009, Flat Bugs of French Guyana - a preliminary faunal list (Heteroptera, Aradidae), pp. 1659-1675 in Linzer biologische Beiträge 41 (2) on page 1672, DOI: 10.5281/zenodo.5279382
Detection of Pulsed X-ray Emission from The Fastest Millisecond Pulsar PSR B1937+21 with ASCA
Creators: name: Takahashi, M.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have detected pulsed X-ray emission from the fastest millisecond pulsar known, PSR B1937+21 (P=1.558 msec), with ASCA. The pulsar is detected as a point source above $\sim 1.7$ keV, with no indication of nebulosity. The source flux in the 2--10 keV band is found to be $f = (3.7\pm 0.6) \times 10^{-13}$ erg s$^{-1}$ cm$^{-2}$, which implies an isotropic luminosity of $L_{\rm x} = 4 πD^2 f \sim (5.7\pm 1.0) \times 10^{32} ~(D/3.6 {\rm kpc})^2$ erg s$^{-1}$, where D is the distance, and an X-ray efficiency of $\sim 5 \times 10^{-4}$ relative to the spin-down power of the pulsar. The pulsation is found at the period predicted by the radio ephemeris with a very narrow primary peak, the width of which is about 1/16 phase ($\sim 100 μ$s), near the time resolution limit ($61 μ$s) of the observation. The instantaneous flux in the primary peak (1/16 phase interval) is found to be ($4.0\pm 0.8) \times 10^{-12}$ erg s$^{-1}$ cm$^{-2}$. Although there is an indication for the secondary peak, we consider its statistical significance too low to claim a definite detection. The narrow pulse profile and the detection in the 2--10 keV band imply that the X-ray emission is caused by the magnetospheric particle acceleration. Comparison of X-ray and radio arrival times of pulses indicates, within the timing errors, that the X-ray pulse is coincident with the radio interpulse.
description: 14 pages with 5 figures. Ap. J. in press
Power sums and Homfly skein theory
Creators: name: Morton, Hugh R.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Geometric Topology (math.GT)
subject: Quantum Algebra (math.QA)
subject: FOS: Mathematics
subject: 57M25, 20C08

description: The Murphy operators in the Hecke algebra H_n of type A are explicit commuting elements, whose symmetric functions are central in H_n. In [Skein theory and the Murphy operators, J. Knot Theory Ramif. 11 (2002), 475-492] I defined geometrically a homomorphism from the Homfly skein C of the annulus to the centre of each algebra H_n, and found an element P_m in C, independent of n, whose image, up to an explicit linear combination with the identity of H_n, is the m-th power sum of the Murphy operators. The aim of this paper is to give simple geometric representatives for the elements P_m, and to discuss their role in a similar construction for central elements of an extended family of algebras H_{n,p}.
description: Published by Geometry and Topology Monographs at http://www.maths.warwick.ac.uk/gt/GTMon4/paper15.abs.html
On weak convergence of locally periodic functions
Creators: name: Lukkassen, Dag
name: Wall, Peter
Publisher: name: arXiv
Year: 2002
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics

description: We prove a generalization of the fact that periodic functions converge weakly to the mean value as the oscillation increases. Some convergence questions connected to locally periodic nonlinear boundary value problems are also considered.
description: arxiv version is already official
Проблема оценки рисков использования возобнов-ляемых источников энергии
Creators: name: Людмила Вениаминовна Нефёдова
name: Юлия Юрьевна Рафикова
Publisher: name: Окружающая среда и энерговедение
Year: 2022
Subjects: возобновляемые источники энергии
гелиоэнергетика
ресурсные риски
риск-менеджмент
факторы риска
renewable energy sources
solar energy
resource risks
risk management
risk factors.

description: Обоснована актуальность разработки методологии риск-менеджмента для дальнейшего развития возобновляемой энергетики в России. Рас-смотрены этапы проведенных с 2015 г. исследований по проблеме оце-нок и управления рисками в возобновляемой энергетике. Описаны полу-ченные результаты: перечень факторов риска и методов управления ими по отраслям, выделение внутренних и внешних составляющих факторов риска, зависящих и не зависящих от девелоперов проектов на ВИЭ. Представлена разработанная методика оценки рисков в гелиоэнергетике на основе изменчивости статистических параметров инсоляции.
description: The importance of developing a risk management methodology for the de-velopment of the renewable energy sector in Russia is justified. The stages of researches on the problem of risk assessments and management in renewable energy in MSU since 2015 are considered. The results are described: a list of risk factors and methods of managing them by using different kinds of re-newable energy sources; internal and external components of risk factors that depend and not depend on the developers of RE projects are identified. The author's methodology for assessing resource risks level in the solar ener-gy industry based on the calculation of the variability of the statistical pa-rameters of insolation is presented
Phyllotingis eximia
Creators: name: Heiss, E.
name: Moragues, G.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Aradidae
Phyllotingis
Phyllotingis eximia

description: Phyllotingis eximia (HAGLUND 1868)
L i t e r a t u r e d a t a:describedfromBrazil.
M a t e r i a l e x a m i n e d: 1♀ Régina, RN2 PK125+3, 19.IX.2008, piège vitre d’ interception, lg. J.L. Giuglaris (CGMM).
D i s t r i b u t i o n: Brazil, Colombia. New for French Guyana. A key to the 5 species of this Neotropical genus is given by HEISS (1993).
description: Published as part of Heiss, E. & Moragues, G., 2009, Flat Bugs of French Guyana - a preliminary faunal list (Heteroptera, Aradidae), pp. 1659-1675 in Linzer biologische Beiträge 41 (2) on page 1671, DOI: 10.5281/zenodo.5279382
The structure of molecular clumps around high-mass young stellar objects
Creators: name: Fontani, F.
name: Cesaroni, R.
name: Caselli, P.
name: Olmi, L.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have used the IRAM 30-m and FCRAO 14-m telescopes to observe the molecular clumps associated with 12 ultracompact (UC) HII regions in the J=6-5, 8-7 and 13-12 rotational transitions of methyl-acetylene (CH3C2H). Under the assumption of LTE and optically thin emission, we have derived temperature estimates ranging from 30 to 56 K. We estimate that the clumps have diameters of 0.2-1.6 pc, H_2 densities of 10^5-10^6 {cm^{-3}}, and masses of 10^2-2 10^4 M_\odot. We compare these values with those obtained by other authors from different molecular tracers and find that the H_2 density and the temperature inside the clumps vary respectively like n_{H_2} ~ R^{-2.6} and T ~ R^{-0.5}, with R distance from the centre. We also find that the virial masses of the clumps are ~3 times less than those derived from the CH3C2H column densities: we show that a plausible explanation is that magnetic fields play an important role to stabilise the clumps, which are on the verge of gravitational collapse. Finally, we show that the CH3C2H line width increases for decreasing distance from the clump centre: this effect is consistent with infall in the inner regions of the clumps. We conclude that the clumps around UC HII regions are likely to be transient (~10^(5) yr) entities, remnants of isothermal spheres currently undergoing gravitational collapse: the high mass accretion rates (~10^{-2} M_\odot yr^{-1}) lead to massive star formation at the centre of such clumps.
description: 15 pages, 11 figures, A & A in press
Fluctuating exchange interactions enable quintet multiexciton formation in singlet fission
Creators: name: Collins, Miles I.
name: McCamey, Dane R.
name: Tayebjee, Murad J. Y.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: Several recent electron spin resonance studies have observed a quintet multiexciton state during the singlet fission process. Here we provide a general theoretical explanation for the generation of this state by invoking a time-varying exchange coupling between pairs of triplet excitons, and subsequently solving the relevant time-varying spin Hamiltonian for a range of transition times. We simulate experimental ESR spectra and draw qualitative conclusions about the adiabatic/diabatic transition between triplet pair spin states.
description: 7 pages, 8 figures, typos corrected
Additional file 4: of Interventions to prevent iatrogenic anemia: a Laboratory Medicine Best Practices systematic review
Creators: name: Whitehead, Nedra
name: Williams, Laurina
name: Sreelatha Meleth
name: Kennedy, Sara
name: Nneka Ubaka-Blackmoore
name: Geaghan, Sharon
name: Nichols, James
name: Carroll, Patrick
name: McEvoy, Michael
name: Gayken, Julie
name: Ernst, Dennis
name: Litwin, Christine
name: Epner, Paul
name: Taylor, Jennifer
name: Graber, Mark
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Science Policy
subject: 60506 Virology
subject: Computational Biology

description: Characteristics of included studies. (DOCX 40 kb)