cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Evolution of the dust mass loss with luminosity along the giant branch of the globular cluster 47 Tuc
Creators: name: Ramdani, A.
name: Jorissen, A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The paper investigates the properties of the dust mass loss in stars populating the giant branch of the globular cluster 47 Tuc, by combining ISOCAM and DENIS data. Raster maps of 5 fields covering areas ranging from 4 x 4 to 15 x 15 arcmin2 at different distances from the center of the cluster have been obtained with ISOCAM at 11.5 mum (LW10 filter). The covered fields include most of the red variables known in this cluster. A detection threshold of about 0.2 mJy is achieved, allowing to detect giant stars at 11.5 mum all the way down to the horizontal branch. No dust-enshrouded asymptotic giant branch stars have been found in the observed fields, contrary to the situation encountered in LMC/SMC globular clusters with larger turnoff masses. The color index [12]-[2] (based on the ISO 11.5 mum flux and on the DENIS Ks magnitude) is used as a diagnostic of dust emission (and hence dust mass loss). Its evolution with luminosity along the giant branch reveals that dust mass loss is only present in V3 (the only cluster Mira variable observed in the present study) and in V18, a star presenting intermittent variability. This conclusion confirms the importance of stellar pulsations in the dust formation and ensuing mass loss.
description: 16 pages, accepted in Astronomy & Astrophysics
title: 03_0701
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/
The leading hadronic contribution to $(g-2)_μ$ from lattice QCD with $N_{\rm f}=2+1$ flavours of O($a$) improved Wilson quarks
Creators: name: Gérardin, Antoine
name: Cè, Marco
name: von Hippel, Georg
name: Hörz, Ben
name: Meyer, Harvey B.
name: Mohler, Daniel
name: Ottnad, Konstantin
name: Wilhelm, Jonas
name: Wittig, Hartmut
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The comparison of the theoretical and experimental determinations of the anomalous magnetic moment of the muon $(g-2)_μ$ constitutes one of the strongest tests of the Standard Model at low energies. In this article, we compute the leading hadronic contribution to $(g-2)_μ$ using lattice QCD simulations employing Wilson quarks. Gauge field ensembles at four different lattice spacings and several values of the pion mass down to its physical value are used. We apply the O($a$) improvement programme with two discretizations of the vector current to better constrain the approach to the continuum limit. The electromagnetic current correlators are computed in the time-momentum representation. In addition, we perform auxiliary calculations of the pion form factor at timelike momenta in order to better constrain the tail of the isovector correlator and to correct its dominant finite-size effect. For the numerically dominant light-quark contribution, we have rescaled the lepton mass by the pion decay constant computed on each lattice ensemble. We perform a combined chiral and continuum extrapolation to the physical point, and our final result is $ a_μ^{\rm hvp}=(720.0\pm12.4_{\rm stat}\,\pm9.9_{\rm syst})\cdot10^{-10}$. It contains the contributions of quark-disconnected diagrams, and the systematic error has been enlarged to account for the missing isospin-breaking effects.
description: 30 pages, 10 figures
title: Cambiando las Lineas de Nieve y las Lineas de Costa
Creators: name: Roop, Heidi A.
name: Mauger, Guillaume S.
name: Morgan, Harriet
name: Snover, Amy K.
name: Krosby, Meade
name: Zamanillo (Translator), I.C.
name: Lopez (Translator), E.
Publisher: name: The UW Climate Impacts Group
Year: 2021

description: This is a translation of a publication that came out last year (2020). Here is the full citation for the Spanish-language report:

Roop, H.A., G.S. Mauger, H. Morgan, A.K. Snover, and M. Krosby, 2020. “Cambiando las Líneas de Nieve y las Líneas de Costa. Informe especial del Grupo Intergubernamental de Expertos sobre el Cambio Climático sobre el Océano y la Criosfera y sus Implicaciones para el Estado de Washington.” Traducción por I.C. Zamanillo; E. Lopez, 2021. Documento informativo preparado para el Grupo de Impactos Climáticos de la Universidad de Washington, Seattle. https://doi.org/10.6069/w5jz-mm63

This is the link to the English language resource equivalent: https://cig.uw.edu/resources/special-reports/shifting-snowlines-shorelines/
Magnetic fields in cluster cores: Faraday rotation in A400 and A2634
Creators: name: Eilek, Jean A.
name: Owen, Frazer N.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present Faraday rotation data for radio sources in the centers of the Abell clusters A400 and A2634. These clusters contain large (> 100 kpc), tailed radio sources, each attached to the central cD galaxy. These clusters do not have strong cooling cores. Our data extend previous work on rotation measure in cluster centers to larger scales and non-cooling clusters. The rotation measure, and thus the magnetic field, is ordered on scales 10-20 kpc in both clusters. The geometry of the rotation measure appears to be determined by the distribution of the X-ray emitting gas, rather than by the radio tails themselves. We combine our data with previously published X-ray and radio data in order to analyze the magnetic fields in all 12 clusters whose central radio sources have been imaged in rotation measure. We find that the fields are dynamically significant in most clusters. We argue that the Faraday data measure fields in the intracluster medium, rather than in a skin of the radio source. Finally, we consider the nature and maintenance of the magnetic fields in these clusters, and conclude that either the cluster-wide field exists at similar levels, or that a weaker cluster-wide field is amplified by effects in the core.
description: Accepted for ApJ. 43 pages including 10 embedded figures. Higher resolution versions of the figures available at http://www.aoc.nrao.edu/~jeilek/pubs/Eilekpub.html
Improved generalized estimating equation analysis via xtqls for quasi–least squares in Stata
Creators: name: Shults, Justine
name: Ratcliffe, Sarah J.
name: Leonard, Mary
name: Shults, Justine
name: Ratcliffe, Sarah J.
name: Leonard, Mary
Publisher: name: Unknown
Year: 2007
Subjects: subject: Research Methods/ Statistical Methods
subject: xtqls
subject: correlated data
subject: clustered data
subject: longitudinal data
subject: generalized estimating equations
subject: quasi–least squares

description: Quasi–least squares (QLS) is an alternative method for estimating the correlation parameters within the framework of the generalized estimating equation (GEE) approach for analyzing correlated cross-sectional and longitudinal data. This article summarizes the development of QLS that occurred in several reports and describes its use with the user-written program xtqls in Stata. Also, it demonstrates the following advantages of QLS: (1) QLS allows some correlation structures that have not yet been implemented in the framework of GEE, (2) QLS can be applied as an alternative to GEE if the GEE estimate is infeasible, and (3) QLS uses the same estimating equation for estimation of Β as GEE; as a result, QLS can involve programs already available for GEE. In particular, xtqls calls the Stata program xtgee within an iterative approach that alternates between updating estimates of the correlation parameter and then using xtgee to solve the GEE for Β at the current estimate of α. The benefit of this approach is that after xtqls, all the usual postregression estimation commands are readily available to the user.
Hedychridium Abeille de Perrin 1878
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

description: Genus Hedychridium Abeille de Perrin, 1878
Hedychridium Abeille de Perrin, 1878: 3.
Type species: Hedychrum minutum Lepeletier, 1806
(= Chrysis ardens Coquebert, 1801), by subsequent designation of Ashmead 1902.
Hedychridium Abeille de Perrin, 1878 is the second largest genus within the family Chrysididae, after Chrysis Linnaeus, 1761, and the largest among the tribe Elampini, including more than 300 valid species. It is a heterogeneous genus of small to medium-sized cuckoo wasps (2.0–7.0 mm), distributed particularly in dry to arid areas of the Holarctic region. Semenov-Tian-Shanskij (1954) and Semenov-Tian-Shanskij & Nikol’skaya (1954) subdivided the genus Hedychridium into twelve genera, namely (besides Hedychridium s.str.): Actineuchrum Semenov-Tian-Shanskij,1954; Claudiola Semenov-Tian-Shanskij,1954; Colpopyga Semenov-Tian-Shanskij,1954; Cyrteuchridium Semenov-Tian-Shanskij, 1954; Cyrteuchrum Semenov-Tian-Shanskij, 1954; Euchridium Semenov-Tian-Shanskij, 1954; Euchrum Semenov-Tian-Shanskij, 1954; Homaleuchrum Semenov-Tian-Shanskij, 1954; Irenula Semenov-Tian-Shanskij & Nikol’skaya, 1954; Zarudnidium Semenov-Tian-Shanskij, 1954; Zarudnium Semenov-Tian-Shanskij, 1954. Currently, only Colpopyga Semenov-Tian-Shanskij, 1954 is considered as a valid genus (Rosa 2017), as recently confirmed by means of molecular analyses (Pauli et al. 2019). All other Semenov-Tian-Shanskij’s genera were synonymised with Hedychridium and treated as species groups by Linsenmaier (1968). The subgenus Prochridium Linsenmaier, 1968 was upgraded to genus rank by Kimsey & Bohart (1991), but we here follow Linsenmaier’s (1994, 1999) classification and consider it with subgeneric status only for practical reasons, as already did in Rosa et al. (2015).
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 7, DOI: 10.11646/zootaxa.5090.1.1, http://zenodo.org/record/5836207
Varunidae Milne-Edwards 1853
Creators: name: Wicksten, Mary K.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Varunidae

description: Key to species of family Varunidae   1. Carapace about as long as wide, frontal margin toothed, outer margin of chelipeds setose. Introduced into San Francisco Bay area.................................................................................. Eriocheir sinensis
– Carapace considerably more broad than long, frontal margin without teeth, outer margin of chelipeds not setose. Widespread, native.............................................................................................. 2
 2. Pereopods 2–5 setose. Front with deep median sinus. Chelae not spotted with red or purple....... Hemigrapsus oregonensis
 – Pereopods 2–5 not setose. Front somewhat sinuous. Chelae spotted with red or purple................ Hemigrapsus nudus
description: Published as part of Wicksten, Mary K., 2012, Decapod Crustacea of the Californian and Oregonian Zoogeographic Provinces 3371, pp. 1-307 in Zootaxa 3371 on page 264
Resource-Efficient Computing in Wearable Systems
Creators: name: Pedram, Mahdi
name: Rofouei, Mahsan
name: Fraternali, Francesco
name: Ashari, Zhila Esna
name: Ghasemzadeh, Hassan
Publisher: name: arXiv
Year: 2019
Subjects: subject: Machine Learning (cs.LG)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences

description: We propose two optimization techniques to minimize memory usage and computation while meeting system timing constraints for real-time classification in wearable systems. Our method derives a hierarchical classifier structure for Support Vector Machine (SVM) in order to reduce the amount of computations, based on the probability distribution of output classes occurrences. Also, we propose a memory optimization technique based on SVM parameters, which results in storing fewer support vectors and as a result requiring less memory. To demonstrate the efficiency of our proposed techniques, we performed an activity recognition experiment and were able to save up to 35% and 56% in memory storage when classifying 14 and 6 different activities, respectively. In addition, we demonstrated that there is a trade-off between accuracy of classification and memory savings, which can be controlled based on application requirements.
Eriocheir sinensis H. Milne-Edwards 1853
Creators: name: Wicksten, Mary K.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Varunidae
Eriocheir
Eriocheir sinensis

description: Eriocheir sinensis H. Milne-Edwards, 1853
(Fig. 61B)
 Eriocheir sinensis H. Milne-Edwards, 1853: 177; 1854: 146, pl. IX, fig. 1. — Ingle 1980:123, fig. 76, pl. 24b (extensive synonymy). — Cohen & Carlton 1995: 95; 1997: 1. — Debelius 1999: 96. — Clark 2006: 17 (Discussion of the correct date of publication of the original species description). — Gollasch 2006: 1, figs. 1–3. — Kuris et al. 2007: 641.
 Diagnosis (after Ingle 1980). Carapace slightly broader than long. Frontal region with pair prominently bifid, acute, submedian lobes, pair tuberculate dorsal carinae. Anterolateral margin of carapace with 3 well-developed teeth, posterolateral margin with single small tooth, lateral margins slightly convex, divergent distally. Chelipeds robust, dorsal surface tuberculate, outer face of chela with dense setae extending onto proximal part of dactylus, carpus with long spine. Pereopods 2–5 moderately stout, margins of carpus to dactylus setose. Female with chelipeds slightly smaller than those of male. Carapace length to 62 mm.
 Color in life. Dorsal surface of carapace grayish-green, pereopods lighter (Ingle 1980).
 Habitat and depth. Estuarine, ranging into freshwater at mouths of rivers, shallow.
 Range. Native range eastern Asia from Vladivostok to South China, especially China Sea. Introduced into Great Britain, almost all of the Baltic Sea and North Sea, northeastern Atlantic to Mediterranean Sea, Netherlands, Rhine and Seine River drainages in Europe (Ingle 1980, Noel 1992, Gollasch 2006); San Francisco Bay drainage. Sporadic reports from Volga River, Russia; Great Lakes region, U.S.A. Chesapeake Bay, Hudson River, Mississippi River Delta (Gollasch 2006). Type locality "coast of China.”
 Remarks. This crab is a nuisance, damaging riverbanks and levees by burrowing, competing with native species and serving as an intermediate host of the human liver fluke. Consult on-line databases of introduced marine species for the latest area in which this crab has been reported.
description: Published as part of Wicksten, Mary K., 2012, Decapod Crustacea of the Californian and Oregonian Zoogeographic Provinces 3371, pp. 1-307 in Zootaxa 3371 on pages 264-265
The KPNO/Deeprange Distant Cluster Survey: I. The Catalog & the Space Density of Intermediate Redshift Clusters
Creators: name: Postman, Marc
name: Lauer, Tod R.
name: Oegerle, William
name: Donahue, Megan
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have conducted an automated search for galaxy clusters within a contiguous 16 square degree I-band survey in the north Galactic hemisphere. A matched filter detection algorithm identifies 444 cluster candidates in the range 0.2 <= z <= 1.2. The full catalog is presented along with the results from a follow-up spectroscopic survey. The estimated redshift distribution of the cluster candidates is consistent with a constant comoving density over the range 0.2 <= z_est <= 0.8. A decline in the cluster space density by more than a factor of 3 over this redshift range is rejected at >99.9% confidence level. We find that the space density of Lambda_CL >= 40 clusters in our survey lies in the range (1.6 - 1.8) x 10^{-5} h_{75}^{3} Mpc^{-3}, ~1.5 times higher than the local distribution of comparably rich Abell RC >= 0 clusters. The Lambda_CL distribution is consistent with a power-law. The discrepancy between the space density of Abell clusters and the clusters in this survey declines quickly as Lambda_CL increases, suggesting that the difference at lower richness is due to significant incompleteness in the Abell catalog. A percolation analysis reveals that 10 - 20% of the spectroscopically confirmed distant clusters are linked into superclusters at overdensities between 10 < {δρ\over ρ} < 50, similar to what is seen in the local cluster distribution. This suggests that there has been little evolution of the cluster-cluster correlation length for z <= 0.5.
description: 35 pages, 14 figures. Accepted for publication in the Astrophysical Journal
Additional file 3 of Re-examination of two diatom reference genomes using long-read sequencing
Creators: name: Filloramo, Gina V.
name: Curtis, Bruce A.
name: Blanche, Emma
name: Archibald, John M.
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 3: Supplementary Table 2. Assembly statistics for various polishing iterations of the de novo long-read derived genomes for Thalassiosira pseudonana and Phaeodactylum tricornutum. Asterisks indicate the final working assembly for each species.
Hedychridium atratum Lins. Linsenmaier 1968
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 atratum

description: Hedychridium atratum Linsenmaier, 1968
(Fig. 2A–2F)
Hedychridium (Hedychridium) atratum Linsenmaier, 1968: 129 (descr., monochroum group); 1987: 141 (allotype desig., descr., diagn.).
Holopyga (Chamaeholopyga) atrata: present paper.
Type locality. Turkey: “ Klein-Asien, Mut, V.67, leg. Schmidt, ♀ Type in Coll. m., ♀ Paratype in Coll. Schmidt ”.
Holotype, ♀: Mut Asia minor 27.–30.V.1967 leg. Jos. Schmidt // ♀ Type Hedychridium Ab. atratum Lins. Linsenmaier det. 1968 // 299 // NML _ ENT GBIF _ Chr0009747 (ex type-collection).
Remarks. The allotype designation by Linsenmaier (1987) is invalid because it was based on a specimen not included in the original description. Linsenmaier (1968) described this species in the Hedychridium monochroum group, nevertheless it belongs to Chamaeholopyga Linsenmaier, 1987. This species is strictly related to Chamaeholopyga rubrinigra Linsenmaier, 1987 from Israel. It can be separated from the latter by mesosomal punctation largely separated with polished intervals (vs. dense punctation, with contiguous punctures and without interspaces in C. rubrinigra). The genus Chamaeholopyga deserves the generic status, but this will be discussed in a forecoming paper focused on Chrysididae genera.
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 8, DOI: 10.11646/zootaxa.5090.1.1, http://zenodo.org/record/5836207
Trust
Creators: name: Micola Von Fürstenrecht, Marie Louise
Publisher: name: University of St Andrews
Year: 2021
Subjects: subject: PR6113.I3T8
subject: Gay couples--Fiction
subject: Non-monogamous relationships--Fiction
subject: Sexual dominance and submission--Fiction

description: This thesis is an excerpt of a full novel, which comprises chapters four to twenty. Chapters one to three are not included as they have been previously submitted as coursework. The synopsis below will only cover the content submitted within this thesis. Emma, a 26-year-old junior doctor in Cardiff has been suppressing her submissive identity out of shame. She’s been keeping people at arm’s length until she meets Inge on a night out, a 29-year-old dominant from The Netherlands, who seems to reveal very little about her past. They go on several dates and feel attracted to each other, but communication isn’t always easy. Inge hints at her interest in BDSM, while Emma is reluctant to admit her submissive desires. With some encouragement, Emma dips her toes into the kink community but then contact suddenly falters when Inge stops texting Emma back. A mutual friend urges them to talk and after clearing up a misunderstanding, Inge and Emma officially start dating. They engage in power play and start a D/s dynamic. Slowly Emma starts feeling safe and the relationship grows until she discovers that Inge might not be monogamous. While coming to grips with her jealousy, Emma begins to fear that she might lose it all.
Maximum likelihood and two-step estimation of an ordered-probit selection model
Creators: name: Chiburis, Richard
name: Lokshin, Michael
name: Chiburis, Richard
name: Lokshin, Michael
Publisher: name: Unknown
Year: 2007
Subjects: subject: Research Methods/ Statistical Methods
subject: oheckman
subject: selection bias
subject: ordered probit
subject: maximum likelihood

description: We discuss the estimation of a regression model with an ordered-probit selection rule. We have written a Stata command, oheckman, that computes two-step and full-information maximum-likelihood estimates of this model. Using Monte Carlo simulations, we compare the performances of these estimators under various conditions.
Additional file 2 of Re-examination of two diatom reference genomes using long-read sequencing
Creators: name: Filloramo, Gina V.
name: Curtis, Bruce A.
name: Blanche, Emma
name: Archibald, John M.
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 2: Supplementary Table 1. Detailed raw read data summary for unfiltered, Albacore “pass” and filtered Oxford Nanopore long-read sequencing datasets for Thalassiosira pseudonana and Phaeodactylum tricornutum. The filtered datasets for T. pseudonana and P. tricornutum included reads ≥30 kb and ≥ 20 kb, respectively.
Optimizing atmospheric turbulence predictions for optical links and astronomical observations
Creators: name: Medlej, Mary-Joe
name: Giordano, Christophe
name: Ziad, Aziz
name: Prunet, Simon
name: Rafalimanana, Alohotsy
name: Aristidi, Eric
Publisher: name: Proceedings of AO4ELT7 conference 2023 - Editors: Thierry Fusco and Benoit Neichel
Year: 2023
Subjects: ATMOSPHERIC TURBULENCE
ASTRONOMICAL COMMUNITY
FREE SPACE OPTICAL TELECOMMUNICATIONS
ELT
PREDICTIONS
NUMERICAL APPROACH
INSTRUMENTED DRONE
SITE LEARNING
STATISTICAL LEARNING ALGORITHMS

description: The prediction of the atmospheric and turbulence conditions are of great interest for the astronomical community
and free space optical telecommunications. With the advent of the next generation of extremely large telescopes
(ELT), the knowledge of atmospheric conditions several hours prior to observations has become essential. As
well, in the field of free space optical telecommunications, the propagation of optical signals in the atmosphere
is significantly influenced by weather conditions (clouds, fog, rain, etc.) and optical turbulence. A numerical
approach based on the Weather and Research Forecasting (WRF) model coupled with an optical turbulence
model for the predictions above the Calern site has been used. Results have shown good agreement between
predictions and observation. However, a difference persists in the first 500 m of the atmosphere. We present in
this paper two approaches to improve the predictions. The first one has been developed by Giordano et al. (2021)
using a site learning\' method. The second one consists of using data from an instrumented drone to improve
the initial conditions of the simulations. We will also present a new method for short-term prediction using two
statistical learning algorithms: ARIMA (Autoregressive Integrated Moving Average) and SARIMA (Seasonal
Autoregressive Integrated Moving Average).
Two postestimation commands for assessing confounding effects in epidemiological studies
Creators: name: Wang, Zhiqiang
name: Wang, Zhiqiang
Publisher: name: Unknown
Year: 2007
Subjects: subject: Research Methods/ Statistical Methods
subject: confall
subject: confgr
subject: chest
subject: epidemiological methods
subject: confounding
subject: all possible effects
subject: change in estimate

description: Confounding is a major issue in observational epidemiological studies. This paper describes two postestimation commands for assessing confounding effects. One command (confall) displays and plots all possible effect estimates against one of p-value, Akaike information criterion, or Bayesian information criterion. This computing-intensive procedure allows researchers to inspect the variability of the effect estimates from various possible models. Another command (chest) uses a stepwise approach to identify variables that have substantially changed the effect estimate. Both commands can be used after most common estimation commands in epidemiological studies, such as logistic regression, conditional logistic regression, Poisson regression, linear regression, and Cox proportional hazards models.
Characteristic X-ray Variability of TeV Blazars: Probing the Link between the Jet and the Central Engine
Creators: name: Kataoka, Jun
name: Takahashi, Tadayuki
name: Wagner, Stefan J.
name: Iyomoto, Naoko
name: Edwards, Philip G.
name: Hayashida, Kiyoshi
name: Inoue, Susumu
name: Madejski, Greg M.
name: Takahara, Fumio
name: Tanihata, Chiharu
name: Kawai, Nobuyuki
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have studied the rapid X-ray variability of three extragalactic TeV gamma-ray sources; Mrk 421, Mrk 501 and PKS 2155-304. Analyzing the X-ray light curves obtained from ASCA and/or RXTE observations between 1993 and 1998, we have investigated the variability in the time domain from 10^3 to 10^8 sec. For all three sources, both the power spectrum density (PSD) and the structure function (SF) show a roll-over with a time-scale of the order of 1 day or longer, which may be interpreted as the typical time-scale of successive flare events. Although the exact shape of turn-over is not well constrained and the low-frequency (long time-scale) behavior is still unclear, the high-frequency (short time-scale) behavior is clearly resolved. We found that, on time-scales shorter than 1 day, there is only small power in the variability, as indicated by a steep power spectrum density of f^{-2~-3}. This is very different from other types of mass-accreting black-hole systems for which the short time-scale variability is well characterized by a fractal, flickering-noise PSD (f^{-1~-2}). The steep PSD index and the characteristic time-scale of flares imply that the X-ray emitting site in the jet is of limited spatial extent; D > 10^{17} cm distant from the base of the jet, which corresponds to > 100 Schwarzschild radii for 10^{7-10} M_solar black-hole systems.
description: 46 pages, 8 figures, accepted for publication in the Astrophysical Journal
Preprocessing and Cutting Planes with Conflict Graphs
Creators: name: Brito, Samuel S.
name: Santos, Haroldo G.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Data Structures and Algorithms (cs.DS)
subject: Optimization and Control (math.OC)
subject: FOS: Computer and information sciences
subject: FOS: Mathematics
subject: G.1.6
subject: 90C10

description: This paper addresses the development of conflict graph-based algorithms and data structures into the COIN-OR Branch-and-Cut (CBC) solver, including: $(i)$ an efficient infrastructure for the construction and manipulation of conflict graphs; $(ii)$ a preprocessing routine based on a clique strengthening scheme that can both reduce the number of constraints and produce stronger formulations; $(iii)$ a clique cut separator capable of obtaining dual bounds at the root node LP relaxation that are $19.65\%$ stronger than those provided by the equivalent cut generator of a state-of-the-art commercial solver, $3.62$ times better than those attained by the clique cut separator of the GLPK solver and $4.22$ times stronger than the dual bounds obtained by the clique separation routine of the COIN-OR Cut Generation Library; and $(iv)$ an odd-cycle cut separator with a new lifting module to produce valid odd-wheel inequalities. The average gap closed by this new version of CBC was up to four times better than its previous version. Moreover, the number of mixed-integer programs solved by CBC in a time limit of three hours was increased by $23.53\%$.
description: Preprint submitted to Computers & Operations Research in September 14, 2019
A Dynamical Analysis of the 47 UMa Planetary System
Creators: name: Laughlin, Gregory
name: Chambers, John
name: Fischer, Debra
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The mass and period ratios of the two planets orbiting 47 UMa suggest a possible kinship to the Jupiter-Saturn pair in our solar system. We explore the current dynamical state of the 47 UMa system with numerical integrations, and compare the results with analytic secular theory. We find that the planets in the system are likely participating in a secular resonance in which the difference in the longitudes of pericenter librates around zero. Alternately, it is possible that the system is participating in the 7:3 mean motion resonance. We show that stability considerations restrict the mutual inclination between the two planets to 40 degrees or less, and that this result is relatively insensitive to the total mass of the two planets. We present hydrodynamical simulations which measure the torques exerted on the planets by a hypothesized external protoplanetary disk. We show that planetary migration in response to torques from the disk may have led to capture of the system into a 7:3 mean-motion resonance, although it is unclear how the eccentricities of the planets would have been damped after capture occured. We show that Earth-mass planets can survive for long periods in some regions of the habitable zone of the nominal co-planar system. A set of planetary accretion calculations, however, shows that it is unlikely that large terrestrial planets can form in the 47 UMa habitable zone.
description: Accepted by the Astrophysical Journal (Original submission November 2001)
Solvable models of Bose-Einstein condensates: a new algebraic Bethe ansatz scheme
Creators: name: Zhou, H. -Q.
name: Links, J.
name: Gould, M. D.
name: McKenzie, R. H.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: A new algebraic Bethe ansatz scheme is proposed to diagonalise classes of integrable models relevant to the description of Bose-Einstein condensates in dilute alkali gases. This is achieved by introducing the notion of Z-graded representations of the Yang-Baxter algebra.
description: 14 pages, latex, no figures
Ranatra gracilis Dallas 1850
Creators: name: Tran, A. D.
name: Zettel, H.
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Nepidae
Ranatra
Ranatra gracilis

description: Ranatra gracilis Dallas, 1850
 Ranatra gracilis Dallas, 1850: 10 (type locality: Bhutan). — Lansbury, 1972 (redescription). — D. Polhemus & J. Polhemus, 2013: 34 (diagnosis, records Laos and Vietnam).
[no material available]
 Diagnosis (based on description by Lansbury, 1972). Body length: males 28–29, females 29–30; ratio of siphon length: body length ca. 0.30–0.35; lorum lower clypeus and without nodule dorsally; ratio of eye width: interocular width ca. 0.8; posterior width of pronotum ca. 1.2× anterior width; hemelytra slightly surpassing posterior margin of abdominal tergum VI; posterior margin of metasternum emarginated, with very narrow or indistinct sublateral grooves; fore femur on flexor side with a median tooth and a median carina, without pre-apical tooth; hind femur, when folded back parallel to body not reaching posterior margin of abdominal sternum VI (in both sexes); paramere: ventral side before apical hook with large, truncate process separated by a distinct gap from apical hook, hook with pointed tip.
 Distribution. Bhutan, India (Assam), northern Thailand, Laos, northern Vietnam, Peninsular Malaysia (D. Polhemus & J. Polhemus, 2013).
description: Published as part of Tran, A. D. & Zettel, H., 2021, Taxonomic review of the Ranatra gracilis group sensu Lansbury, 1972 (Nepomorpha: Nepidae), with descriptions of four new species, pp. 45-70 in Raffles Bulletin of Zoology 69 on page 66, DOI: 10.26107/RBZ-2021-0005, http://zenodo.org/record/5351678
Infinitely many star products to play with
Creators: name: Gracia-Bondia, J. M.
name: Lizzi, F.
name: Marmo, G.
name: Vitale, P.
Publisher: name: arXiv
Year: 2001
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Mathematical Physics (math-ph)
subject: Operator Algebras (math.OA)
subject: Quantum Algebra (math.QA)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: While there has been growing interest for noncommutative spaces in recent times, most examples have been based on the simplest noncommutative algebra: [x_i,x_j]=i theta_{ij}. Here we present new classes of (non-formal) deformed products associated to linear Lie algebras of the kind [x_i,x_j]=ic_{ij}^k x_k. For all possible three-dimensional cases, we define a new star product and discuss its properties. To complete the analysis of these novel noncommutative spaces, we introduce noncompact spectral triples, and the concept of star triple, a specialization of the spectral triple to deformations of the algebra of functions on a noncompact manifold. We examine the generalization to the noncompact case of Connes' conditions for noncommutative spin geometries, and, in the framework of the new star products, we exhibit some candidates for a Dirac operator. On the technical level, properties of the Moyal multiplier algebra M(R_θ^{2n) are elucidated.
description: LaTeX, 36 pages. Minor corrections, references added
Representing and Using Knowledge with the Contextual Evaluation Model
Creators: name: Hansen, Victor E
Publisher: name: arXiv
Year: 2019
Subjects: subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences

description: This paper introduces the Contextual Evaluation Model (CEM), a novel method for knowledge representation and manipulation. The CEM differs from existing models in that it integrates facts, patterns and sequences into a single contextual framework. V5, an implementation of the model is presented and demonstrated with multiple annotated examples. The paper includes simulations demonstrating how the model reacts to pleasure/pain stimuli. The 'thought' is defined within the model and examples are given converting thoughts to language, converting language to thoughts and how 'meaning' arises from thoughts. A pattern learning algorithm is described. The algorithm is applied to multiple problems ranging from recognizing a voice to the autonomous learning of a simplified natural language.
Measurements of coal particle surface temperature – methodology and results
Creators: name: Katelbach-Woźniak, Anna
name: Klimanek, Adam
name: Korus, Agnieszka
name: Sławomir Sładek
name: Szlęk, Andrzej
Publisher: name: figshare
Year: 2019
Subjects: subject: 90405 Non-automotive Combustion and Fuel Engineering (incl. Alternative/Renewable Fuels)
subject: FOS: Environmental engineering

description: Abstract ISCP2019
Ranatra lansburyi Chen, Nieser & Ho 2004
Creators: name: Tran, A. D.
name: Zettel, H.
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Nepidae
Ranatra
Ranatra lansburyi

description: Ranatra lansburyi Chen, Nieser & Ho, 2004
 Ranatra lansburyi Chen, Nieser & Ho, 2004: 89 (type locality: Chiang Mai, Thailand). — D. Polhemus & J. Polhemus, 2012: 247 (record Myanmar).
 Material examined. THAILAND: 1 male, 1 female (NHMW, previously det. as R. parmata by N. Nieser), Chiang Mai Province, W Mae Rim, Mae Sa N.P., Mae Sa Falls, coll. H. Zettel, 30–31 October 1995.
 Diagnosis. Body length: males 27–31, females 31–34; ratio of siphon length: body length ca. 0.4; lorum lower clypeus and without nodule dorsally; ratio of eye width: interocular width ca. 0.8; posterior width of pronotum ca. 1.25× anterior width; pronotal length ca. 1.5× fore coxa length; hemelytra reaching posterior margin of abdominal tergum VI; posterior margin of metasternum roundly emarginated, with very narrow or indistinct sublateral grooves; fore femur on flexor side with a median tooth and a median carina, without preapical tooth; hind femur, when folded back parallel to body reaching anterior quarter of operculum (in males) or only slightly surpassing mid-length of abdominal sternum VI (in females); paramere: ventral side before apical hook with large, bi-lobed process, hook with truncate tip.
 Distribution. Myanmar, North Thailand (Chiang Mai), Southwestern China (Yunnan) (Chen et al., 2004; D. Polhemus & J. Polhemus, 2012).
description: Published as part of Tran, A. D. & Zettel, H., 2021, Taxonomic review of the Ranatra gracilis group sensu Lansbury, 1972 (Nepomorpha: Nepidae), with descriptions of four new species, pp. 45-70 in Raffles Bulletin of Zoology 69 on page 66, DOI: 10.26107/RBZ-2021-0005, http://zenodo.org/record/5351678
Opening the Treasure Chest in Carina
Creators: name: Mookerjea, B.
name: Sandell, G.
name: Guesten, R.
name: Riquelme, D.
name: Wiesemeyer, H.
name: Chambers, E.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We have mapped the G287.84-0.82 cometary globule (with the Treasure Chest cluster embedded in it) in the South Pillars region of Carina (i) in [CII], 63micron [OI], and CO(11-10) using upGREAT on SOFIA and (ii) in J=2-1 transitions of CO, 13CO, C18O and J=3-2 transitions of H2CO using the APEX telescope in Chile. We probe the morphology, kinematics, and physical conditions of the molecular gas and the photon dominated regions (PDRs) in G287.84-0.82. The [CII] and [OI] emission suggest that the overall structure of the pillar (with red-shifted photo evaporating tails) is consistent with the effect of FUV radiation and winds from eta-Car and O stars in Trumpler 16. The gas in the head of the pillar is strongly influenced by the embedded cluster, whose brightest member is an O9.5V star, CPD-59 2661. The emission of the [CII] and [OI] lines peak at a position close to the embedded star, while all other tracers peak at another position lying to the north-east consistent with gas being compressed by the expanding PDR created by the embedded cluster. The molecular gas inside the globule is probed with the J=2-1 transitions of CO and isotopologues as well as H2CO, and analyzed using a non-LTE model (escape-probability approach), while we use PDR models to derive the physical conditions of the PDR. We identify at least two PDR gas components; the diffuse part (~10^4 cm^-3) is traced by [CII], while the dense (n~ 2-8x10^5 cm^-3) part is traced by [CII], [OI], CO(11-10). Using the F=2-1 transition of [13CII] detected at 50 positions in the region, we derive optical depths (0.9-5), excitation temperatures of [CII] (80-255 K), and N(C+) of 0.3-1x10^19 cm^-2. The total mass of the globule is ~1000 Msun, about half of which is traced by [CII]. The dense PDR gas has a thermal pressure of 10^7-10^8 K cm^-3, which is similar to the values observed in other regions.
description: Accepted for publication in Astronomy and Astrophysics (abstract slightly abridged)
Ranatra schuhi D. Polhemus & J. Polhemus 2012
Creators: name: Tran, A. D.
name: Zettel, H.
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Nepidae
Ranatra
Ranatra schuhi

description: Ranatra schuhi D. Polhemus & J. Polhemus, 2012
 Ranatra schuhi D. Polhemus & J. Polhemus, 2012: 243–247 (type locality: Mandalay, Myanmar).
[no material available]
description: Published as part of Tran, A. D. & Zettel, H., 2021, Taxonomic review of the Ranatra gracilis group sensu Lansbury, 1972 (Nepomorpha: Nepidae), with descriptions of four new species, pp. 45-70 in Raffles Bulletin of Zoology 69 on page 66, DOI: 10.26107/RBZ-2021-0005, http://zenodo.org/record/5351678
Interaction of a heralded single photon with nitrogen-vacancy centers in a diamond
Creators: name: Gieysztor, Maria
name: Misiaszek, Marta
name: van der Veen, Joscelyn
name: Gawlik, Wojciech
name: Jelezko, Fedor
name: Kolenderski, Piotr
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: A simple, room-temperature, cavity- and vacuum-free interface for a photon-matter interaction is implemented. In the experiment, a heralded single photon generated by the process of spontaneous parametric down-conversion is absorbed by an ensemble of nitrogen-vacancy color centers. The broad absorption spectrum associated with the phonon sideband solves the mismatch problem of a narrow absorption bandwidth in a typical atomic medium and broadband spectrum of quantum light. The heralded single photon source is tunable in the spectral range 452-575 nm, which overlaps well with the absorption spectrum of nitrogen-vacancy centers.
description: 5 pages, 3 figures
Additional file 6 of Re-examination of two diatom reference genomes using long-read sequencing
Creators: name: Filloramo, Gina V.
name: Curtis, Bruce A.
name: Blanche, Emma
name: Archibald, John M.
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 6: Supplementary Table 5. Structural variation between the polished de novo Canu and Flye assemblies and the reference genomes for Phaeodactylum tricornutum and Thalassiosira pseudonana.
Statistical Properties of Galactic Starlight Polarization
Creators: name: Fosalba, Pablo
name: Lazarian, Alex
name: Prunet, Simon
name: Tauber, Jan A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a statistical analysis of Galactic interstellar polarization from the largest compilation available of starlight data. The data comprises ~ 9300 stars of which we have selected ~ 5500 for our analysis. We find a nearly linear growth of mean polarization degree with extinction. The amplitude of this correlation shows that interstellar grains are not fully aligned with the Galactic magnetic field, which can be interpreted as the effect of a large random component of the field. In agreement with earlier studies of more limited scope, we estimate the ratio of the uniform to the random plane-of-the-sky components of the magnetic field to be B_u/B_r = 0.8. Moreover, a clear correlation exists between polarization degree and polarization angle what provides evidence that the magnetic field geometry follows Galactic structures on large-scales. The angular power spectrum C_l of the starlight polarization degree for Galactic plane data (|b| < 10 deg) is consistent with a power-law, C_l ~ l^{-1.5} (where l ~ 180 deg/θis the multipole order), for all angular scales θ> 10 arcmin. An investigation of sparse and inhomogeneous sampling of the data shows that the starlight data analyzed traces an underlying polarized continuum that has the same power spectrum slope, C_l ~ l^{-1.5}. Our findings suggest that starlight data can be safely used for the modeling of Galactic polarized continuum emission at other wavelengths.
description: 31 pages, 11 figures. Minor corrections and some clarifications included. Matches version accepted for publication by the Astrophysical Journal
Hedychridium (Hedychridium) aheneum subsp. feritatum * 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 aheneum
Hedychridium (hedychridium) aheneum feritatum linsenmaier, 1959b

description: Hedychridium (Hedychridium) aheneum feritatum Linsenmaier, 1959b
(Fig. 1A–1E)
Hedychridium aheneum feritatum Linsenmaier, 1959b: 235 (descr.); 1969: 352 (cat., incrassatum group).
Hedychridium feritatum: Rosa 2020: 462 (elevated to species rank), 473 (figs 1, 3, 5).
Type locality. Palestine: “Palästina, ♂ Type und Paratype Coll. m., Paratypen Coll. Bytinski-Salz (verschiedene Fundorte [=different locations], VII.- VIII.)”.
Holotype, ♂: Ruhama Palestine 29.8.1949 leg. Bytinski-Salz // ♂ Type Hedychridium Ab. aheneum feritatum Lins. Linsenmaier det. 1959 // 183 // NML _ ENT GBIF _ Chr0010251 (ex type-collection).
Paratype, ♂: Palestine Kfor Ato [locality not found] 8.7. leg. Bytinski-Salz // ♂ Paratype Hedychridium Ab. aheneum feritatum Lins. Linsenmaier det. 1959 // NML _ ENT GBIF _ Chr0010243 (ex synoptic collection).
Remarks. In the type-collection, Linsenmaier labelled a female specimen as the allotype bearing the following labels: Israel Haifa 20.6.65 leg. Schlaefle // ♀ Allotype Hedychridium aheneum feritatum Lins. det. Linsenmaier 1965. This specimen was collected after the original description and does not belong to the type series. Hedychridium feritatum was upgraded to species rank by Rosa (2020).
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 7, DOI: 10.11646/zootaxa.5090.1.1, http://zenodo.org/record/5836207