cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The search for multiple populations in Magellanic Clouds clusters - V. Correlation between cluster age and abundance spreads
Creators: name: Martocchia, S.
name: Dalessandro, E.
name: Lardo, C.
name: Cabrera-Ziri, I.
name: Bastian, N.
name: Kozhurina-Platais, V.
name: Salaris, M.
name: Chantereau, W.
name: Geisler, D.
name: Hilker, M.
name: Kacharov, N.
name: Larsen, S.
name: Mackey, D.
name: Mucciarelli, A.
name: Niederhofer, F.
name: Platais, I.
name: Usher, C.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: In our HST photometric survey, we have been searching for multiple stellar populations (MPs) in Magellanic Clouds (MCs) massive star clusters which span a significant range of ages ($\sim 1.5-11$ Gyr). In the previous papers of the series, we have shown that the age of the cluster represents one of the key factors in shaping the origin of the chemical anomalies. Here we present the analysis of four additional clusters in the MCs, namely Lindsay 38, Lindsay 113, NGC 2121 and NGC 2155, for which we recently obtained new UV HST observations. These clusters are more massive than $\sim 10^4M_{\odot}$ and have ages between $\sim 2.5-6$ Gyr, i.e. located in a previously unexplored region of the cluster age/mass diagram. We found chemical anomalies, in the form of N spreads, in three out of four clusters in the sample, namely in NGC 2121, NGC 2155 and Lindsay 113. By combining data from our survey and HST photometry for 3 additional clusters in the Milky Way (namely 47 Tuc, M15 and NGC 2419), we show that the extent of the MPs in the form of N spread is a strong function of age, with older clusters having larger N spreads with respect to the younger ones. Hence, we confirm that cluster age plays a significant role in the onset of MPs.
description: Accepted for publication in MNRAS. 12 pages, 9 figures
Charge and sodium ordering in beta-Na_0.33V_2O_5
Creators: name: van Loosdrecht, P. H. M.
name: Presura, C. N.
name: Popinciuc, M.
name: van der Marel, D.
name: Maris, G.
name: Palstra, T. T. M.
name: van Bentum, P. J. M.
name: Yamada, H.
name: Yamauchi, T.
name: Ueda, Y.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Polarized Raman and optical spectra for the quasi one-dimensional metallic vanadate beta-Na0.33V2O3 are reported for various temperatures. The spectra are discussed in the light of the sodium and charge ordering transitions occurring in this material, and demonstrate the presence of strong electron phonon coupling.
description: To be published in J. Superconductivity: Incorporating Novel Magnetism (december 2002)
Hedychridium chloropygum subsp. spatium Lins. Linsenmaier 1959
Creators: name: Rosa, Paolo
name: Heim, René
name: Bernasconi, Marco Valerio
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Chrysididae
Hedychridium
Hedychridium chloropygum
Hedychridium chloropygum spatium linsenmaier, 1959a

description: Hedychridium chloropygum spatium Linsenmaier, 1959a
(Fig. 11A–11F)
Hedychridium (Hedychridium) chloropygum spatium Linsenmaier, 1959a: 59 (descr., roseum group), 187 (cat.), 198 (fig. 107); 1968: 36 (diagn., distr.); 1987: 142 (distr.).
Hedychridium chloropygum caputaureum Trautmann & Trautmann, 1919: Arens 2010: 406 (synonymised).
Type locality. Hungary, Rhodes, Sweden: “ Ungarn, Rhodos, Schweden. ♂ Type (Simontornya), ♀ Allotype (Rhodos) Coll. m., Paratypen Coll. m. und Museum Lund (Schweden)”.
Holotype, ♂: L. VII.15 Simontornya // 1924 Hung. occ. // ♂ Type Hedychridium chloropygum B. ssp. spatium Lins. Linsenmaier det. 1959 // 65 // NML _ ENT GBIF _ Chr0010961 (ex type-collection).
Allotype, ♀: Rodi Egeo Mai 1939 Dr. R. Meyer // ♀ Allotype Hedychridium chloropygum B. ssp. spatium Lins. Linsenmaier det. // NML _ ENT GBIF _ Chr0010962 (ex type-collection).
Paratype, 1 ex.: SH-Väster hejde Sigreips 11.8.31 CB Gaunitz // Hedychridium chloropygum B. ssp. spatium Lins. Linsenmaier det. 1959 // NML _ ENT GBIF _ Chr0010966.
Remarks. Arens (2010) synonymised Hedychridium chloropygum spatium with Hedychridium caputaureum Trautmann & Trautmann, 1919.
description: Published as part of Rosa, Paolo, Heim, René & Bernasconi, Marco Valerio, 2022, The Palaearctic types of Chrysididae (Insecta, Hymenoptera) deposited in the Linsenmaier collection. Part 2. Elampini: genus Hedychridium Abeille de Perrin, 1878, pp. 1-94 in Zootaxa 5090 (1) on pages 16-17, DOI: 10.11646/zootaxa.5090.1.1, http://zenodo.org/record/5836207
Additional file 2 of A diet-specific microbiota drives Salmonella Typhimurium to adapt its in vivo response to plant-derived substrates
Creators: name: Prax, Nicoletta
name: Wagner, Stefanie
name: Schardt, Jakob
name: Neuhaus, Klaus
name: Clavel, Thomas
name: Fuchs, Thilo M.
Publisher: name: figshare
Year: 2021
Subjects: subject: Plant Biology
subject: FOS: Biological sciences

description: Additional file 2 Table S1. Significant influences of two diets on the microbiota composition.
Ring Formation in Magnetically Subcritical Clouds and Multiple Star Formation
Creators: name: Li, Zhi-Yun
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We study numerically the ambipolar diffusion-driven evolution of non-rotating, magnetically subcritical, disk-like molecular clouds, assuming axisymmetry. Previous similar studies have concentrated on the formation of single magnetically supercritical cores at the cloud center, which collapse to form isolated stars. We show that, for a cloud with many Jeans masses and a relatively flat mass distribution near the center, a magnetically supercritical ring is produced instead. The supercritical ring contains a mass well above the Jeans limit. It is expected to break up, through both gravitational and possibly magnetic interchange instabilities, into a number of supercritical dense cores, whose dynamic collapse may give rise to a burst of star formation. Non-axisymmetric calculations are needed to follow in detail the expected ring fragmentation into multiple cores and the subsequent core evolution. Implications of our results on multiple star formation in general and the northwestern cluster of protostars in the Serpens molecular cloud core in particular are discussed.
description: 25 pages, 4 figures, to appear in ApJ
Max-Min Rate of Cell-Free Massive MIMO Uplink with Optimal Uniform Quantization
Creators: name: Bashar, Manijeh
name: Cumanan, Kanapathippillai
name: Burr, Alister G.
name: Ngo, Hien Quoc
name: Debbah, Merouane
name: Xiao, Pei
Publisher: name: arXiv
Year: 2019
Subjects: subject: Information Theory (cs.IT)
subject: FOS: Computer and information sciences

description: Cell-free Massive multiple-input multiple-output (MIMO) is considered, where distributed access points (APs) multiply the received signal by the conjugate of the estimated channel, and send back a quantized version of this weighted signal to a central processing unit (CPU). For the first time, we present a performance comparison between the case of perfect fronthaul links, the case when the quantized version of the estimated channel and the quantized signal are available at the CPU, and the case when only the quantized weighted signal is available at the CPU. The Bussgang decomposition is used to model the effect of quantization. The max-min problem is studied, where the minimum rate is maximized with the power and fronthaul capacity constraints. To deal with the non-convex problem, the original problem is decomposed into two sub-problems (referred to as receiver filter design and power allocation). Geometric programming (GP) is exploited to solve the power allocation problem whereas a generalized eigenvalue problem is solved to design the receiver filter. An iterative scheme is developed and the optimality of the proposed algorithm is proved through uplink-downlink duality. A user assignment algorithm is proposed which significantly improves the performance. Numerical results demonstrate the superiority of the proposed schemes.
description: 9 figures
Neutron capture and 2.2 MeV emission in the atmosphere of the secondary of an X-ray binary
Creators: name: Jean, P.
name: Guessoum, N.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We consider the production of 2.22 MeV radiation resulting from the capture of neutrons in the atmosphere of the secondary in an X-ray binary system, where the neutrons are produced in the accretion disk around the compact primary star and radiated in all directions. We have considered several accretion disk models (ADAF, ADIOS, SLE, Uniform-Temperature) and a varity of parameters (accretion rate, mass of the compact object, mass, temperature and composition of the secondary star, distance between the two objects, etc.). The neutron rates are calculated by a network of nuclear reactions in the accretion disk, and this is handled by a reaction-rate formulation taking into account the structure equations given by each accretion model. The processes undergone by the neutrons in the atmosphere of the companion star are studied in great detail, including thermalization, elastic and inelastic scatterings, absorption, escape from the surface, decay, and capture by protons. The radiative transfer of the 2.22 MeV photons is treated separately, taking into consideration the composition and density of the star's atmosphere. The final flux of the 2.22 MeV radiation that can be detected from earth is calculated taking into account the distance to the source, the direction of observation with respect to the binary system frame, and the rotation of the source, as this can lead to an observable periodicity in the flux. We produce phasograms of the 2.22 MeV intensity as well as spectra of the line, where rotational Doppler shift effects can lead to changes in the spectra that are measurable by INTEGRAL's spectrometer (SPI).
description: 13 pages, 10 figures, A&A in press
Additional file 4 of Comparison of peri-implant submucosal microbiota in arches with zirconia or titanium implant-supported fixed complete dental prostheses: a study protocol for a randomized controlled trial
Creators: name: Jia, Pingyi
name: Yang, Jingwen
name: Yue, Zhaoguo
name: Liu, Jianzhang
name: Liu, Qi
name: Liu, Zhongning
name: Tang, Lin
name: Hou, Jianxia
Publisher: name: figshare
Year: 2020
Subjects: subject: Space Science
subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Cancer

description: Additional file 4. Study prorocol
Generating Manhattan plots in Stata
Creators: name: Cook, Daniel E.
name: Ryckman, Kelli R.
name: Murray, Jeffrey C.
name: Cook, Daniel E.
name: Ryckman, Kelli R.
name: Murray, Jeffrey C.
Publisher: name: Unknown
Year: 2013
Subjects: subject: Research Methods/ Statistical Methods
subject: manhattan
subject: Manhattan plots
subject: genome-wide association studies
subject: single nucleotide polymorphisms

description: Genome-wide association studies hold the potential for discovering genetic causes for a wide range of diseases, traits, and behaviors. However, the incredible amount of data handling, advanced statistics, and visualization have made conducting these studies difficult for researchers. Here we provide a tool, manhattan, for helping investigators easily visualize genome-wide association studies data in Stata.
Hedychridium cupritibiale Lins. Linsenmaier 1987
Creators: name: Rosa, Paolo
name: Heim, René
name: Bernasconi, Marco Valerio
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Chrysididae
Hedychridium
Hedychridium cupritibiale

description: Hedychridium cupritibiale Linsenmaier, 1987
(Fig. 13A–13E)
Hedychridium (Hedychridium) cupritibiale Linsenmaier, 1987: 139 (descr., ardens group); 1997: 254 (diagn., allotype desig.), 255 (tab.), 288 (figs 27, 28).
Type locality. Spain: “Spanien, Granada, Sierra Chaparral 1100 m, ♀ Type leg. und Coll. Perraudin ”.
Holotype, ♀: Carro del Chupa [sic] 14.VI.1986 1100m coll. W. Perraudin Prov Granada coll. W. Perraudin // ♀ Type Hedychridium Ab. cupritibiale Lins. Linsenmaier det. 1987 // 415 // NML _ ENT GBIF _ Chr0009006 (ex type-collection)
Remarks. The holotype is described from Cerro del Chupa, a small locality in Sierra del Chaparral, in Granada Province, Spain. Linsenmaier’s (1997) designation of the allotype is invalid, since based on a male collected in 1988, not belonging to the original type series, bearing the following information: Granada Sierra D. Chaparral 1100m 16.6.88 leg. Linsenmaier // ♂ Paratype Hedychridium Ab. cupritibiale Lins. Linsenmaier 1991.
description: Published as part of Rosa, Paolo, Heim, René & Bernasconi, Marco Valerio, 2022, The Palaearctic types of Chrysididae (Insecta, Hymenoptera) deposited in the Linsenmaier collection. Part 2. Elampini: genus Hedychridium Abeille de Perrin, 1878, pp. 1-94 in Zootaxa 5090 (1) on pages 17-18, DOI: 10.11646/zootaxa.5090.1.1, http://zenodo.org/record/5836207
First spectroscopic evidence for carbon stars outside the Local Group: properties of a massive star cluster in NGC 7252
Creators: name: Mouhcine, M.
name: Lancon, A.
name: Leitherer, C.
name: Silva, S.
name: Groenewegen, M. A. T.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present near-IR spectroscopy of the massive intermediate age star cluster W3 in the merger remnant galaxy NGC 7252, obtained with the NTT telescope. This cluster has an age when the integrated near-IR properties of a stellar population are dominated by the cool and luminous AGB stars. We compare the data with instantaneous curst model predictions from new evolutionary synthesis models that include: (1) the computation of the evolution through the TP-AGB for low- and intermediate-massive stars, with the initial mass and metallicity dependent formation of carbon stars; (2) spectroscopic data from a new stellar library in which differences betwenn static giants, vriable O-rich TPAGB stars and carbon stars are accounted for. The comparison of the data to the models clearly shows that carbon stars are present: for the first time, carbon star spectral features are thus detected directly outside the Local Group (abriged)
description: Accepted for publication in A&A, 14 pages
Currents and correlations in Luttinger liquids and carbon nanotubes at finite temperature and size: a bosonization study
Creators: name: Caux, J. -S.
name: Lopez, A.
name: Suppa, D.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We consider problems of one dimensional interacting fermions confined to a finite size, multichannel geometry. Concentrating on Luttinger liquids and carbon nanotubes, we use nontrivial boundary conditions to represent the effect of external leads, and apply our framework to transport problems in a Josephson junction setup. We present an exact computation of all correlation functions, including finite-size and temperature effects, for two sets of solvable boundary conditions. In all cases, we compute physical quantities like the Josephson current and the pairing order parameter profile.
description: 30 pages, 2 EPS figures
Jointly Extracting and Compressing Documents with Summary State Representations
Creators: name: Mendes, Afonso
name: Narayan, Shashi
name: Miranda, Sebastião
name: Marinho, Zita
name: Martins, André F. T.
name: Cohen, Shay B.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Information Retrieval (cs.IR)
subject: Computation and Language (cs.CL)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: We present a new neural model for text summarization that first extracts sentences from a document and then compresses them. The proposed model offers a balance that sidesteps the difficulties in abstractive methods while generating more concise summaries than extractive methods. In addition, our model dynamically determines the length of the output summary based on the gold summaries it observes during training and does not require length constraints typical to extractive summarization. The model achieves state-of-the-art results on the CNN/DailyMail and Newsroom datasets, improving over current extractive and abstractive methods. Human evaluations demonstrate that our model generates concise and informative summaries. We also make available a new dataset of oracle compressive summaries derived automatically from the CNN/DailyMail reference summaries.
Hedychridium discordum Lins. Linsenmaier 1959
Creators: name: Rosa, Paolo
name: Heim, René
name: Bernasconi, Marco Valerio
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Chrysididae
Hedychridium
Hedychridium discordum

description: Hedychridium discordum Linsenmaier, 1959a
(Fig. 14A–14E)
Hedychridium (Hedychridium) discordum Linsenmaier, 1959a: 45 (key), 50 (descr.), 187 (cat.); 1968: 26 (distr.); 1999: 60 (key), 62 (diagn.).
Type locality. Morocco: “Marocco, ♀ Type Coll. m. (Plateau de Oukaimeden 2500m, V.1953, leg. Teunissen)”.
Holotype, ♀: Maroc Plateau de Oukaimeden 2500m 29.V.1953 Teunissen // ♀ Type Hedychridium discordum Lins. Linsenmaier det. 1959 // 54 // NML _ ENT GBIF _ Chr0008632 (ex type-collection).
description: Published as part of Rosa, Paolo, Heim, René & Bernasconi, Marco Valerio, 2022, The Palaearctic types of Chrysididae (Insecta, Hymenoptera) deposited in the Linsenmaier collection. Part 2. Elampini: genus Hedychridium Abeille de Perrin, 1878, pp. 1-94 in Zootaxa 5090 (1) on page 18, DOI: 10.11646/zootaxa.5090.1.1, http://zenodo.org/record/5836207
Semiparametric fixed-effects estimator
Creators: name: Libois, Franccois
name: Verardi, Vincenzo
name: Libois, Franccois
name: Verardi, Vincenzo
Publisher: name: Unknown
Year: 2013
Subjects: subject: Research Methods/ Statistical Methods
subject: xtsemipar
subject: semiparametric estimations
subject: panel data
subject: fixed effects

description: In this article, we describe the Stata implementation of Baltagi and Li’s (2002, Annals of Economics and Finance 3: 103–116) series estimator of partially linear panel-data models with fixed effects. After a brief description of the estimator itself, we describe the new command xtsemipar. We then simulate data to show that this estimator performs better than a fixed-effects estimator if the relationship between two variables is unknown or quite complex.
Additional file 5 of A diet-specific microbiota drives Salmonella Typhimurium to adapt its in vivo response to plant-derived substrates
Creators: name: Prax, Nicoletta
name: Wagner, Stefanie
name: Schardt, Jakob
name: Neuhaus, Klaus
name: Clavel, Thomas
name: Fuchs, Thilo M.
Publisher: name: figshare
Year: 2021
Subjects: subject: Plant Biology
subject: FOS: Biological sciences

description: Additional file 5 Table S4. Significant influences of streptomycin on the microbiota composition.
t-analogues des operateurs d'ecrantage associes aux q-caracteres (t-analogs of screening operators related to q-characters)
Creators: name: Hernandez, David
Publisher: name: arXiv
Year: 2001
Subjects: subject: Quantum Algebra (math.QA)
subject: FOS: Mathematics

description: Frenkel and Reshetikhin introduced screening operators related to q-characters of finite dimensional representations of quantum affine algebras. We propose t-analogs of screening operators related to Nakajima's q,t-characters with the same properties of symmetry. Nakajima introduced non-commutative rings, so we propose bimodules. Our construction uses only combinatorial definition of q,t-characters, and therefore can be extended to the non-simply laced case.
description: 22 pages; in french, introduction in english
Additional file 3 of Comparison of peri-implant submucosal microbiota in arches with zirconia or titanium implant-supported fixed complete dental prostheses: a study protocol for a randomized controlled trial
Creators: name: Jia, Pingyi
name: Yang, Jingwen
name: Yue, Zhaoguo
name: Liu, Jianzhang
name: Liu, Qi
name: Liu, Zhongning
name: Tang, Lin
name: Hou, Jianxia
Publisher: name: figshare
Year: 2020
Subjects: subject: Space Science
subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Cancer

description: Additional file 3. Consent form
title: 01_1197
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/
A Hardware-Oriented and Memory-Efficient Method for CTC Decoding
Creators: name: Lu, Siyuan
name: Lu, Jinming
name: Lin, Jun
name: Wang, Zhongfeng
Publisher: name: arXiv
Year: 2019
Subjects: subject: Signal Processing (eess.SP)
subject: Machine Learning (cs.LG)
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: FOS: Computer and information sciences

description: The Connectionist Temporal Classification (CTC) has achieved great success in sequence to sequence analysis tasks such as automatic speech recognition (ASR) and scene text recognition (STR). These applications can use the CTC objective function to train the recurrent neural networks (RNNs), and decode the outputs of RNNs during inference. While hardware architectures for RNNs have been studied, hardware-based CTCdecoders are desired for high-speed CTC-based inference systems. This paper, for the first time, provides a low-complexity and memory-efficient approach to build a CTC-decoder based on the beam search decoding. Firstly, we improve the beam search decoding algorithm to save the storage space. Secondly, we compress a dictionary (reduced from 26.02MB to 1.12MB) and use it as the language model. Meanwhile searching this dictionary is trivial. Finally, a fixed-point CTC-decoder for an English ASR and an STR task using the proposed method is implemented with C++ language. It is shown that the proposed method has little precision loss compared with its floating-point counterpart. Our experiments demonstrate the compression ratio of the storage required by the proposed beam search decoding algorithm are 29.49 (ASR) and 17.95 (STR).
description: 13 pages, 11 figures
The modelling of intermediate-age stellar populations: I- near-infrared properties
Creators: name: Mouhcine, M.
name: Lancon, A.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In this paper, we discuss how the integrated properties of intermediate-age single burst population, especially in the near-infrared, behave as a function of age and metallicity. Our models take into account all stellar evolutionary phases that affect the evolution of the integrated optical and near-infrared spectrum of such a population. Particular care was dedicated to the Asymptotic Giant Brach stars, which can be dominant at near-infrared wavelengths. First we present new synthetic model that takes into account the relevant physical processes that control the evolution through the thermally pulsing AGB. In the isochrone presented in this paper the lifetime and the nature of the AGB stars are established as consequences of the interplay between the physical processes that control the AGB star evolution. The contribution of these stars to the integrated light of the population is thus obtained in a consistent way. We optimize our models by using a new stellar library that explicitly takes into account the spectral features thar characterize only AGB stars in comparison to other cool and luminous stars (abriged)
description: Accepted for publication in A&A, 19 pages
Additional file 1 of Comparison of different dose accumulation strategies to estimate organ doses after stereotactic magnetic resonance-guided adaptive radiotherapy
Creators: name: Regnery, Sebastian
name: Leiner, Lukas
name: Buchele, Carolin
name: Hoegen, Philipp
name: Sandrini, Elisabetta
name: Held, Thomas
name: Deng, Maximilian
name: Eichkorn, Tanja
name: Rippke, Carolin
name: Renkamp, C. Katharina
name: König, Laila
name: Lang, Kristin
name: Adeberg, Sebastian
name: Debus, Jürgen
name: Klüter, Sebastian
name: Hörner-Rieber, Juliane
Publisher: name: figshare
Year: 2023
Subjects: subject: Biophysics
subject: Physical Sciences not elsewhere classified
subject: Medicine
subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biological Sciences not elsewhere classified
subject: Cancer

description: Supplementary Material 1
Laotia Saurin 1953
Creators: name: Páll-Gergely, Barna
name: Hunyadi, András
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Architaenioglossa
Alycaeidae
Laotia

description: Laotia Saurin, 1953
 Type species. Laotia pahiensis Saurin, 1953.
description: Published as part of Páll-Gergely, Barna & Hunyadi, András, 2021, A new species and a new subspecies of Laotia Saurin, 1953 (Gastropoda: Caenogastropoda: Alycaeidae) from Sơn La Province, Vietnam, pp. 118-123 in Raffles Bulletin of Zoology 69 on page 118, DOI: 10.26107/RBZ-2021-0010, http://zenodo.org/record/5351956
Exact Wilcoxon signed-rank and Wilcoxon Mann-Whitney ranksum
Creators: name: Harris, Tammy
name: Hardin, James W.
name: Harris, Tammy
name: Hardin, James W.
Publisher: name: Unknown
Year: 2013
Subjects: subject: Research Methods/ Statistical Methods
subject: ranksumex
subject: signrankex
subject: exact distributions
subject: nonparametric tests
subject: median
subject: Wilcoxon matched-pairs signed-rank test
subject: Wilcoxon ranksum test

description: We present new Stata commands for carrying out exact Wilcoxon one-sample and two-sample comparisons of the median. Nonparametric tests are often used in clinical trials, in which it is not uncommon to have small samples. In such situations, researchers are accustomed to making inferences by using exact statistics. The ranksum and signrank commands in Stata provide only asymptotic results, which assume normality. Because large-sample results are unacceptable in many clinical trials studies, these researchers must use other software packages. To address this, we have developed new commands for Stata that provide exact statistics in small samples. Additionally, when samples are large, we provide results based on the Student’s t distribution that outperform those based on the normal distribution.
Additional file 6 of A diet-specific microbiota drives Salmonella Typhimurium to adapt its in vivo response to plant-derived substrates
Creators: name: Prax, Nicoletta
name: Wagner, Stefanie
name: Schardt, Jakob
name: Neuhaus, Klaus
name: Clavel, Thomas
name: Fuchs, Thilo M.
Publisher: name: figshare
Year: 2021
Subjects: subject: Plant Biology
subject: FOS: Biological sciences

description: Additional file 6 Table S5. Significant influences of the S. Typhimurium infection on the microbiota composition.
Extending the flexible parametric survival model for competing risks
Creators: name: Hinchliffe, Sally R.
name: Lambert, Paul C.
name: Hinchliffe, Sally R.
name: Lambert, Paul C.
Publisher: name: Unknown
Year: 2013
Subjects: subject: Research Methods/ Statistical Methods
subject: stpm2cif
subject: survival analysis
subject: competing risks
subject: cumulative incidence
subject: cause-specific hazard

description: Competing risks are present when the patients within a dataset could experience one or more of several exclusive events and the occurrence of any one of these could impede the event of interest. One of the measures of interest for analyses of this type is the cumulative incidence function. stpm2cif is a postestimation command used to generate predictions of the cumulative incidence function after fitting a flexible parametric survival model using stpm2. There is also the option to generate confidence intervals, cause-specific hazards, and two other measures that will be discussed in further detail. The new command is illustrated through a simple example.
Nbody2: A Direct N-Body Integration Code
Creators: name: Aarseth, Sverre J.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We give a full description of the code NBODY2 for direct integration of the gravitational N-body problem. The method of solution is based on the neighbour scheme of Ahmad & Cohen (1973) which speeds up the force calculation already for quite modest particle numbers. Derivations of all the relevant mathematical expressions are given, together with a detailed discussion of the algorithms. The code may be used to study a wide variety of self-consistent problems based on a small softening of the interaction potential.
description: Latex (uses macros elsart.cls, harvard.sty. Accepted for publication in New Astronomy)
The First Candidate Colliding-Wind Binary in M33
Creators: name: Garofali, Kristen
name: Levesque, Emily M.
name: Massey, Philip
name: Williams, Benjamin F.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present the detection of the first candidate colliding-wind binary (CWB) in M33, located in the giant H II region NGC 604. The source was first identified in archival {\it Chandra} imaging as a relatively soft X-ray point source, with the likely primary star determined from precise astrometric alignment between archival {\it Hubble Space Telescope} and {\it Chandra} imaging. The candidate primary star in the CWB is classified for the first time in this work as a carbon-rich Wolf-Rayet star with a likely O star companion based on spectroscopy obtained from Gemini-North. We model the X-ray spectrum using {\it Chandra} and {\it XMM-Newton} observations, and find the CWB is well-fit as a $\sim$ 1 keV thermal plasma with a median unabsorbed luminosity in the 0.5--2.0 keV band of $L_{\rm X}$ $\sim$ 3 $\times$ 10$^{35}$ erg s$^{-1}$, making this source among the brightest of CWBs observed to date. We present a long term light curve for the candidate CWB from archival {\it Chandra} and {\it XMM-Newton} observations, and discuss the constraints placed on the binary by this light curve, as well as the X-ray luminosity at maximum. Finally, we compare this candidate CWB in M33 to other well-studied, bright CWBs in the Galaxy and Magellanic Clouds, such as $η$ Car.
description: 21 pages, 8 figures, 4 tables, Accepted for publication in ApJ
Additional file 2 of Comparison of peri-implant submucosal microbiota in arches with zirconia or titanium implant-supported fixed complete dental prostheses: a study protocol for a randomized controlled trial
Creators: name: Jia, Pingyi
name: Yang, Jingwen
name: Yue, Zhaoguo
name: Liu, Jianzhang
name: Liu, Qi
name: Liu, Zhongning
name: Tang, Lin
name: Hou, Jianxia
Publisher: name: figshare
Year: 2020
Subjects: subject: Space Science
subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Cancer

description: Additional file 2. Trials structured Study Protocol template
Additional file 7 of A diet-specific microbiota drives Salmonella Typhimurium to adapt its in vivo response to plant-derived substrates
Creators: name: Prax, Nicoletta
name: Wagner, Stefanie
name: Schardt, Jakob
name: Neuhaus, Klaus
name: Clavel, Thomas
name: Fuchs, Thilo M.
Publisher: name: figshare
Year: 2021
Subjects: subject: Plant Biology
subject: FOS: Biological sciences

description: Additional file 7 Table S6. Oligonucleotides used in this study.
Goodness-of-fit tests for categorical data
Creators: name: Bellocco, Rino
name: Algeri, Sara
name: Bellocco, Rino
name: Algeri, Sara
Publisher: name: Unknown
Year: 2013
Subjects: subject: Research Methods/ Statistical Methods
subject: saturated models
subject: categorical data
subject: deviance
subject: goodness-of-fit tests

description: A significant aspect of data modeling with categorical predictors is the definition of a saturated model. In fact, there are different ways of specifying it—the casewise, the contingency table, and the collapsing approaches—and they strictly depend on the unit of analysis considered. The analytical units of reference could be the subjects or, alternatively, groups of subjects that have the same covariate pattern. In the first case, the goal is to predict the probability of success (failure) for each individual; in the second case, the goal is to predict the proportion of successes (failures) in each group. The analytical unit adopted does not affect the estimation process; however, it does affect the definition of a saturated model. Consequently, measures and tests of goodness of fit can lead to different results and interpretations. Thus one must carefully consider which approach to choose. In this article, we focus on the deviance test for logistic regression models. However, the results and the conclusions are easily applicable to other linear models involving categorical regressors. We show how Stata 12.1 performs when implementing goodness of fit. In this situation, it is important to clarify which one of the three approaches is implemented as default. Furthermore, a prominent role is played by the shape of the dataset considered (individual format or events–trials format) in accordance with the analytical unit choice. In fact, the same procedure applied to different data structures leads to different approaches to a saturated model. Thus one must attend to practical and theoretical statistical issues to avoid inappropriate analyses.
Standardizing anthropometric measures in children and adolescents with functions for egen: Update
Creators: name: Vidmar, Suzanna I.
name: Cole, Tim J.
name: Pan, Huiqi
name: Vidmar, Suzanna I.
name: Cole, Tim J.
name: Pan, Huiqi
Publisher: name: Unknown
Year: 2013
Subjects: subject: Research Methods/ Statistical Methods
subject: zanthro()
subject: zbmicat()
subject: z scores
subject: LMS
subject: egen
subject: anthropometric standards

description: In this article, we describe an extension to the egen functions zanthro() and zbmicat() (Vidmar et al., 2004, Stata Journal 4: 50–55). All functionality of the original version remains unchanged. In the 2004 version of zanthro(), z scores could be generated using the 2000 U.S. Centers for Disease Control and Prevention Growth Reference and the British 1990 Growth Reference. More recent growth references are now available. For measurement-for-age charts, age can now be adjusted for gestational age. The zbmicat() function previously categorized children according to body mass index (weight/height^2) as normal weight, overweight, or obese. “Normal weight” is now split into normal weight and three grades of thinness. Finally, this updated version uses cubic rather than linear interpolation to calculate the values of L, M, and S for the child‘s decimal age between successive ages (or length/height for weight-for-length/height charts).
Poly(oxymethylene) ethers: potential diesel fuels with low sooting tendencies
Creators: name: Zhu, Junqing
name: Chan, Fan Liang
name: Foust, Thomas D.
name: Lucas, Stephen
name: Montgomery, Matthew J.
name: Pfefferle, Lisa D.
name: Reardon, Kenneth F.
name: Windom, Bret C.
name: McEnally, Charles S.
Publisher: name: figshare
Year: 2021
Subjects: subject: 90201 Automotive Combustion and Fuel Engineering (incl. Alternative/Renewable Fuels)
subject: FOS: Environmental engineering

description: Work in Progress Poster presented at the 38th International Symposium on Combustion, Adelaide Australia, January 24 to 29 2021.
Diesel engines are a major contributor to total soot emissions because diesel fuels have high sooting tendencies. Poly(oxymethylene) ethers (POMEs) are biomass-derived sustainable diesel fuels reported to have low soot emissions from engines. The structures of the POMEs in these earlier studies are alternating oxygen and carbon atoms terminated with methyl groups on both ends. Unfortunately, methyl-POMEs suffer from high water solubility and low energy density. Replacing the methyl groups with larger alkyl groups can overcome these disadvantages. However, larger alkyl groups will lead to higher sooting tendencies. To optimize this trade-off, the sooting tendencies of methyl-POMEs and alkyl-POMEs need to be quantified. In this work, a series of methyl-POMEs and alkyl-POMEs were synthesized and their sooting tendencies were quantified.
The sooting tendencies were characterized by the Yield Sooting Index (YSI). This parameter is based on the maximum soot concentration measured in coflow diffusion flames whose fuel is CH4 doped with 1000 ppm of each test compound. The YSIs of the methyl-POMEs and alkyl-POMEs are at least one order of magnitude lower than a certification diesel fuel. The ratio of YSI to lower heating value (LHV) was calculated to evaluate the energy penalty of the oxygen atoms. The calculated YSI/LHV of the POMEs are lower than conventional diesel fuels and their components. These results demonstrate that all POMEs have soot emission benefits, and ongoing work is examining the trade-off between different POMEs.
Synthesis, molecular docking, binding free energy calculation and molecular dynamics simulation studies of benzothiazol-2-ylcarbamodithioates as Staphylococcus aureus MurD inhibitors
Creators: name: Srikanth Jupudi
name: Azam, Mohammed Afzal
name: Wadhwani, Ashish
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: A new series of benzothiazol-2-ylcarbamodithioate functional compounds 5a-f has been designed, synthesized and characterized by spectral data. These compounds were screened for their in vitro antibacterial activity against strains of Staphylococcus aureus (NCIM 5021, NCIM 5022 and methicillin-resistant isolate 43300), Bacillus subtilis (NCIM 2545), Escherichia coli (NCIM 2567), Klebsiella pneumoniae (NCIM 2706) and Psudomonas aeruginosa (NCIM 2036). Compounds 5a and 5d exhibited significant activity against all the tested bacterial strains. Specifically, compounds 5a and 5d showed potent activity against K. pneumoniae (NCIM 2706), while compound 5a also displayed potent activity against S. aureus (NCIM 5021). Compound 5d showed minimum IC50 value of 13.37 μM against S. aureus MurD enzyme. Further, the binding interactions of compounds 5a-f in the catalytic pocket have been investigated using the extra-precision molecular docking and binding free energy calculation by MM-GBSA approach. A 30 ns molecular dynamics simulation of 5d/modeled S. aureus MurD enzyme was performed to determine the stability of the predicted binding conformation.
Recruitment material DESIVE² Panel (in German)
Creators: name: Krems, Adeline
name: Bressel, Paulina
name: Dewitz, Leyla
name: Greifeneder, Elke
name: Henkel, Maria
name: Jacob, Armin
name: Peters, Isabella
name: Perrey, Lennart
name: Stiller, Juliane
name: Trkulja, Violeta
Publisher: name: Zenodo
Year: 2024

description: These recruitment materials for the DESIVE² panel include four postcard designs and two posters. The panel was recruited for studies on health information behavior and false information, with the goal to reach a broad audience. The materials were distributed across Germany in physical form.

The research project, to which this recuritment material belongs, is called "DESIVE² – Desinformationsverhalten verstehen / Understanding Disinformation Behavior“, funded by the Federal Ministry of Education and Research (BMBF) in Germany (Grant Agreement No.: 16KIS1529). Please mention when reusing this material: Recruitment material DESIVE² Panel (in German) by DESIVE² research group (2024) via [doi] under license CC BY 4.0.
Separation of instrumental and astrophysical foregrounds for mapping CMB anisotropies
Creators: name: Delabrouille, J.
name: Patanchon, G.
name: Audit, E.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We address the extended problem of component separation for CMB applications when a mixture of both astrophysical and instrumental components are present in the observations, and show how standard methods can be adapted to handle this more complex inversion problem.
description: 12 pages, 5 figures, submitted to MNRAS
Exploring structural features of EGFR–HER2 dual inhibitors as anti-cancer agents using G-QSAR approach
Creators: name: Shehnaz Fatima
name: Agarwal, Subhash Mohan
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Medicine
subject: Molecular Biology
subject: Biotechnology
subject: Ecology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified

description: Simultaneous inhibition of EGFR and HER2 by dual-targeting inhibitors is an established anti-cancer strategy. Therefore, a recent trend in drug discovery involves understanding the features of such dual inhibitors. In this study, three different G-QSAR models were developed corresponding to individual EGFR, HER2 and the dual-model for both receptors. The dual-model provided site-specific information wherein (i) increasing electronegative character and higher index of saturated carbon at R4 position; (ii) presence of chlorine atom at R2 position; (iii) decreasing alpha modified shape index at R1 and R3 positions; and (iv) less electronegativity at R2 position; were found important for enhancing the dual activity. Also, comparison of dual-model with the EGFR/HER2 individual models revealed that it incorporates the properties of both models and, thus, represents a combination of EGFR/HER2. Further, fragment analysis revealed that R2 and R4 are important for imparting high potency while specificity is decided by R1/R3 fragment. We also checked the predictive ability of the dual-model by determining applicability domain using William’s plot. Also, analysis of active molecules showed they show favorable substitutions that agree with the constructed dual-model. Thus, we have been successful in developing a single dual-response QSAR model to get an insight into various structural features influencing EGFR/HER2 activity.
A Nulling Wide Field Imager for Exoplanets Detection and General Astrophysics
Creators: name: Guyon, Olivier
name: Roddier, Francois
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a solution to obtain a high-resolution image of a wide field with the central source removed by destructive interference. The wide-field image is created by aperture synthesis with a rotating sparse array of telescopes in space. Nulling of the central source is achieved using a phase-mask coronagraph. The full (u,v) plane coverage delivered by the 60m, six 3-meter telescope array is particularly well-suited for the detection and characterization of exoplanets in the infrared (DARWIN and Terrestrial Planet Finder (TPF) missions) as well as for other generic science observations. Detection (S/N=10) of an Earth-like planet is achieved in less than 10 hours with a 1 micron bandwidth at 10 micron.
description: 18 pages, 16 figures. Accepted for publication in A&A
Bonferroni and Holm approximations for Šidák and Holland-Copenhaver q-values
Creators: name: Newson, Roger B.
name: Newson, Roger B.
Publisher: name: Unknown
Year: 2013
Subjects: subject: Research Methods/ Statistical Methods
subject: parmest
subject: qqvalue
subject: smileplot
subject: multproc
subject: multiple-test procedure
subject: familywise error rate
subject: Bonferroni
subject: Sidák
subject: Holm
subject: Holland
subject: Copenhaver

description: I describe the use of the Bonferroni and Holm formulas as approximations for Šidák and Holland–Copenhaver formulas when issues of precision are encountered, especially with q-values corresponding to very small p-values.
Test for Pairing Symmetry Based on Spin Fluctuations in Organic Superconductors $κ$-(BEDT-TTF)$_{2}$X
Creators: name: Li, Jian-Xin
Publisher: name: arXiv
Year: 2002
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We propose that the superconducting pairing symmetry of organic superconductors $κ$-(BEDT-TTF)$_{2}$X can be determined by measuring the position in momentum space of the incommensurate peaks of the spin susceptibility. We show that the positions of these peaks are uniquely determined by the symmetry of the superconducting state and the geometry of Fermi surface. Based on the effective Hubbard model on an anisotropic triangular lattice, we demonstrate the different incommensurate patters of spin responses for $d_{x^{2}-y^{2}}$- and $d_{xy}$-like pairing states. In addition, we predict the nonexistence of the spin resonance mode in this compound, which is an important feature in high-$T_{c}$ superconductors.
description: 4 pages, 5 figures