cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 1: of Development of a measurement system for complex oral information transfer in medical consultations
Creators: name: J. Nordfalk
name: P. Gulbrandsen
name: J. Gerwing
name: M. Nylenna
name: J. Menichetti
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences

description: Coding System for Counting Complex Orally Provided Information and Patient Recall (PDF 649 kb)
A photometric and spectroscopic study of dwarf and giant galaxies in the Coma cluster - II. Spectroscopic observations
Creators: name: Mobasher, B.
name: Bridges, T. J.
name: Carter, D.
name: Poggianti, B.
name: Komiyama, Y.
name: Kashikawa, N.
name: Doi, M.
name: Iye, M.
name: Okamura, S.
name: Sekiguchi, M.
name: Shimasaku, K.
name: Yagi, M.
name: Yasuda, N.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: This is the second paper in a series studying the photometric and spectroscopic properties of galaxies of different luminosities in the Coma cluster. The sample selection, spectroscopic observations and completeness functions are presented here. To study the spectral properties of galaxies as a function of their local environment, two fields were selected for spectroscopic observations to cover both the core (Coma1) and outskirts (ie. south-west of the core and centered on NGC4839)- (Coma3) of the cluster. Medium resolution spectroscopy (6-9 Å) was carried out for a total of 490 galaxies in both fields (302 in Coma1 and 188 in Coma3), using the WYFFOS multi-fiber spectrograph on the William Herschel Telescope. The galaxies cover a range of $12 < R < 20$, corresponding to -23 < M_R < -15 (H0=65 km/sec/Mpc). The redshifts are measured with an accuracy of 100 km/sec. The spectral line strengths and equivalent widths are also measured for the same galaxies and analysed in Poggianti et al (2001- paper III). A total of 189 (Coma1) and 90 (Coma3) galaxies are identified as members of the Coma cluster. An analysis of the colors show that only two members of the Coma cluster in our sample have B-R > 2. The completeness functions for the spectroscopic sample is presented.
description: 27 pages, 11 Figures. Accepted for publication in Ap.J Suppl
Rottboellia cochinchinensis Clayton, Kew Bull.
Creators: name: Prunera-Olivé, Joan
name: Vorontsova, Maria S.
name: Williams, Emma V.
name: Mollel, Neduvoto P.
name: Hemp, Andreas
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Rottboellia
Rottboellia cochinchinensis

description: Rottboellia cochinchinensis (Lour.) Clayton, Kew Bull. 35: 817 (1981).
 Distribution: Trop. & Subtrop. Old World to N. & NE. Australia
 Specimens: MOSHI Holili, Hemp, A. 1871 (NHT, UBT); Kikafu River, Hemp, A. 867 (UBT); Moshi, Haarer, A.E. 743 (K).
description: Published as part of Prunera-Olivé, Joan, Vorontsova, Maria S., Williams, Emma V., Mollel, Neduvoto P. & Hemp, Andreas, 2021, Checklist of Kilimanjaro grasses shows that both plot and herbarium methods are necessary to record diversity, pp. 201-244 in Phytotaxa 501 (2) on page 238, DOI: 10.11646/phytotaxa.501.2.1, http://zenodo.org/record/5424816
Testing Theoretical Models for the Higher-Order Moments of Dark Halo Distribution
Creators: name: Casas-Miranda, R.
name: Mo, H. J.
name: Boerner, G.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using high--resolution N--body simulations, we test two theoretical models, based either on spherical or on ellipsoidal collapse model, for the higher--order moments of the dark matter halo distribution in CDM models. We find that a theoretical model based on spherical collapse describes accurately the simulated counts--in--cells moments for haloes of several mass ranges. It appears that the model using ellipsoidal collapse instead of spherical collapse in defining dark haloes is unable to improve the models for the higher--order moments of halo distribution, for haloes much smaller than $M^*$ (the mass scale on which the fluctuation of the density field has a rms about 1). Both models are particularly accurate for the descendants of haloes selected at high redshift, and so are quite useful in interpreting the high--order moments of galaxies. As an application we use the theoretical model to predict the higher--order moments of the Lyman break galaxies observed at $z\approx 3$ and their descendants at lower redshifts.
description: 10 pages, 9 figures, MN2e LaTex class, Accepted for publication in MNRAS, Major changes
Generic quantized zero-bias conductance peaks in superconductor-semiconductor hybrid structures
Creators: name: Pan, Haining
name: Cole, William S.
name: Sau, Jay D.
name: Sarma, S. Das
Publisher: name: arXiv
Year: 2019
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We show theoretically that quantized zero-bias conductance peaks should be ubiquitous in superconductor-semiconductor hybrids by employing a zero-dimensional random matrix model with continuous tuning parameters. We demonstrate that a normal metal-superconductor (NS) junction conductance spectra can be generically obtained in this model replicating all features seen in recent experimental results. The theoretical quantized conductance peaks, which explicitly do not arise from spatially isolated Majorana zero modes, are easily found by preparing a contour plot of conductance over several independent tuning parameters, mimicking the effect of Zeeman splitting and voltages on gates near the junction. This suggests that, even stable apparently quantized conductance peaks need not correspond to isolated Majorana modes; rather, the $\textit{a priori}$ expectation should be that such quantized peaks generically occupy a significant fraction of the high-dimensional tuning parameter space that characterizes the NS tunneling experiments.
description: 6 pages, 4 figures
Excitation of Orbital Eccentricities by Repeated Resonance Crossings: Requirements
Creators: name: Chiang, E. I.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Divergent migration of planets within a viscous circumstellar disk can engender resonance crossings and dramatic excitation of orbital eccentricities. We provide quantitative criteria for the viability of this mechanism. For the orbits of two bodies to diverge, a ring of viscous material must be shepherded between them. As the ring diffuses in radius by virtue of its intrinsic viscosity, the two planets are wedged further apart. The ring mass must be smaller than the planetary masses so that the crossing of an individual resonance lasts longer than the resonant libration period. At the same time, the crossing cannot be of such long duration that the disk's direct influence on the bodies' eccentricities interferes with the resonant interaction between the two planets. This last criterion is robustly satisfied because resonant widths are typically tiny fractions of the orbital radius. We evaluate our criteria not only for giant planets within gaseous protoplanetary disks, but also for shepherd moons that bracket narrow planetary rings in the solar system. A shepherded ring of gas orbiting at a distance of 1 AU from a solar-type star and having a surface density of less than 500 g/cm^2, a dimensionless alpha viscosity of 0.1, and a height-to-radius aspect ratio of 0.05 can drive two Jovian-mass planets through the 2:1 and higher-order resonances so that their eccentricities amplify to values of several tenths. Because of the requirement that the disk mass in the vicinity of the planets be smaller than the planet masses, divergent resonance crossings may figure significantly into the orbital evolution of planets during the later stages of disk evolution, including the debris disk phase.
description: ApJ, in press, to appear in February 2003 issue
What have we learnt about the Sun from the measurement of the $^8$B neutrino flux?
Creators: name: Fiorentini, G.
name: Ricci, B.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: By combining the results of SNO and Super-Kamiokande one can derive - in the absence of sterile neutrinos - the total neutrino flux produced from $^8$B decay in the Sun. We use this information to check the accuracy of several input parameters of solar model calculations. Opacity and p-p fusion cross section are constrained by the $^8$B flux measurement to the level of few per cent. The central solar temperature is determined to the one-percent level. We also find an upper limit for the flux on Earth of sterile neutrinos. We discuss the role of nuclear physics uncertainties on these determinations.
description: 8 pages with 1 ps figure included. Revised version
IC 10: More evidence that it is a blue compact dwarf
Creators: name: Richer, M. G.
name: Bullejos, A.
name: Borissova, J.
name: McCall, Marshall L.
name: Lee, Henry
name: Kurtev, R.
name: Georgiev, L.
name: Kingsburgh, R. L.
name: Ross, R.
name: Rosado, M.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present optical spectroscopy of H {\sc ii} regions in the Local Group galaxy IC 10 and $UBVR$ photometry of foreground stars in three fields towards this galaxy. From these data, we find that the foreground reddening due to the Milky Way is $E(B-V)=0.77\pm 0.07 \mathrm{mag}$. We find that IC 10 contains considerable internal dust, which qualitatively explains the variety of reddening values found by studies of its different stellar populations. Based upon our foreground reddening, IC 10 has intrinsic photometric properties like those of a blue compact dwarf galaxy, and not those of a dwarf irregular. This result is consistent with much evidence that IC 10 is in the throes of a starburst that began at least $10 \mathrm{Myr}$ ago. We also report the discovery of a new WR star in the H {\sc ii} region HL111c.
Megalocoleus mellae
Creators: name: Linnavuori, Rauno E.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Miridae
Megalocoleus
Megalocoleus mellae

description: Megalocoleus mellae (Reuter, 1876)
 Material examined. Several specimens: GILAN: Darreh Dasht, 27.v.-20.vi.1995; Dasht-e-Veel, 10.-12.vi.2001; Deylaman, 16.-20.vii.1998; Rustam Abad – Salan Sar, 6.-8.vi.2001; Sang Rud, 30.vi.-1.vii.2003. ARDABIL: Khemes – Kolur, 27.-29.vi.2002. ZANJAN: Abbar, 12.-14.vi.2001; Mamalan, 12.-14.v.2002. TEHRAN: Azad Bar, 8.-10.vii.1995; Kandovan, 3.-4.vii.1995; Shahrestenak, 10.-12.vii.1995.
 Comments. In hilly meadows. Pontomediterranean. Recorded as M. molliculus (Fallén, 1829) in LINNAVUORI & MODARRES (1999: 226). The genus was revised by MATOCQ (2004).
description: Published as part of Linnavuori, Rauno E., 2007, Studies on the Miridae (Heteroptera) of Gilan and the adjacent provinces in northern Iran. II. List of species, pp. 17-56 in Acta Entomologica Musei Nationalis Pragae 47 on page 48, DOI: 10.5281/zenodo.5328235
Cosmological observations in scalar-tensor quintessence
Creators: name: Riazuelo, Alain
name: Uzan, Jean-Philippe
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The framework for considering the astronomical and cosmological observations in the context of scalar-tensor quintessence in which the quintessence field also accounts for a time dependence of the gravitational constant is developed. The constraints arising from nucleosynthesis, the variation of the constant, and the post-Newtonian measurements are taken into account. A simple model of supernovae is presented in order to extract the dependence of their light curves with the gravitational constant; this implies a correction when fitting the luminosity distance. The properties of perturbations as well as CMB anisotropies are also investigated.
description: 26 pages, 22 figures, to appear in PRD
Additional file 3: of Item response theory analysis and properties of decisional conflict scales: findings from two multi-site trials of men with localized prostate cancer
Creators: name: Pozzar, Rachel
name: Berry, Donna
name: Fangxin Hong
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Science Policy

description: Category characteristic curves for all subscales on the original DCS-12, aggregated DCS-12, and LL DCS-10. This figure displays the category characteristic curves for items on each subscale of the original DCS-12, aggregated DCS-12, and LL DCS-10. (DOCX 1243 kb)
Performance study of the Jalousie detector baseline design for the ESS thermal powder diffractometer HEIMDAL through GEANT4 simulations
Creators: name: Stefanescu, I.
name: Christensen, M.
name: Hall-Wilton, R.
name: Holm-Dahlin, S.
name: Iversen, K.
name: Klein, M.
name: Mannix, D.
name: Schefer, J.
name: Schmidt, C. J.
name: Schweika, W.
name: Stuhr, U.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: HEIMDAL is a thermal powder diffractometer designed to operate at the European Spallation Source, world's most intense neutron source. The detailed design of the instrument, which is expected to enter user operation in 2024/2025, assumes that the neutrons scattered by the powder under investigation will be collected with hundreds of large-area Multi-Wire Proportional Counters employing a $^{10}$B$_4$C-solid converter. The gas counters will consists of large active volumes and tapered trapezoidal shapes that allow for close packing into a cylindrical shell with high solid angle coverage. The whole detector will operate in an air environment within the shielding cave and provide signals with sensitivity for locating detection in three dimensions. This paper presents the results of a GEANT4 study of the baseline design for the HEIMDAL powder diffraction detector. The detector model was used to study key performance parameters such as detection efficiency and spatial resolution. The contribution of the detector to the resolving power of the instrument, one of the key figures-of-merit for powder diffractometers, was also investigated. Most of the simulation results reported in this work cannot be validated against a sufficiently similar physical reference until the first segment or module are constructed and tested with neutron beam. However, these results can help identify possible ways of optimising the detector design and provide the first glimpse into the expected performance of this technological approach.
Saccharum officinarum Linnaeus 1753
Creators: name: Prunera-Olivé, Joan
name: Vorontsova, Maria S.
name: Williams, Emma V.
name: Mollel, Neduvoto P.
name: Hemp, Andreas
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Saccharum
Saccharum officinarum

description: Saccharum officinarum L., Sp. Pl.: 54 (1753).
 Distribution: New Guinea.
 Specimens: none (see text).
description: Published as part of Prunera-Olivé, Joan, Vorontsova, Maria S., Williams, Emma V., Mollel, Neduvoto P. & Hemp, Andreas, 2021, Checklist of Kilimanjaro grasses shows that both plot and herbarium methods are necessary to record diversity, pp. 201-244 in Phytotaxa 501 (2) on page 238, DOI: 10.11646/phytotaxa.501.2.1, http://zenodo.org/record/5424816
Additional file 1: of Item response theory analysis and properties of decisional conflict scales: findings from two multi-site trials of men with localized prostate cancer
Creators: name: Pozzar, Rachel
name: Berry, Donna
name: Fangxin Hong
Publisher: name: figshare
Year: 2019
Subjects: Medicine
Molecular Biology
Developmental Biology

description: Decisional conflict defining characteristics and related factors. This table presents the defining characteristics of decisional conflict and its related factors as defined by NANDA International [10]. (DOCX 13 kb)
title: Das verdrängte Politikum. (Post-)Koloniale Migration nach Deutschland
Creators: name: Félix-Eyoum, Jean-Pierre
name: Wagner, Florian
Publisher: name: ZZF - Centre for Contemporary History: Zeitgeschichte online
Year: 2021

description: Im 20. Jahrhundert fanden es die Deutschen kaum verwunderlich, dass es wenig Zuwanderung aus den (ehemaligen) Kolonien gab. Aus Politik, Gesellschaft und Wissenschaft kam niemand auf die Idee, überhaupt die Frage nach (post-)kolonialer Einwanderung zu stellen. Die ausbleibende Verwunderung lässt sich durch die Selbstverständlichkeit erklären, mit der man annahm, Weiß-Sein sei eine Bedingung für Deutschsein und die deutsche Nation „kein Einwanderungsland” (Zitat Helmut Kohl, 1992). Beim Blick nach Frankreich und Großbritannien hätte man zwar ein Defizit bei der nachkolonialen Einwanderung nach Deutschland feststellen können (1974 gab es in Frankreich regulär über eine Million Menschen allein aus den ehemaligen afrikanischen Kolonien). Das Gegenteil war jedoch der Fall. Man bemühte in Deutschland den Vergleich mit Frankreich und Großbritannien lediglich, um zu behaupten, dass das deutsche Kolonialreich nur kurze Zeit existierte und zeitlich zu weit zurück lag, um einen dauernden Einfluss zu hinterlassen. Kohls Zitat, das deutsche Einwanderungsbehörden schon seit 1945 zum Leitmotiv ihrer Arbeit gemacht hatten, war weniger deskriptiv als präskriptiv gemeint. Bei der Zuwanderung nach Deutschland sollte es weder einen „Kolonialbonus“ für Auswanderungswillige aus den ehemaligen Überseegebieten geben, noch kam die deutsche Regierung auf die Idee, durch Bevorzugung von Migrant:innen oder „Gastarbeiter:innen“-Rekrutierung aus den ehemaligen Kolonien Wiedergutmachungspolitik zu betreiben, wie es zum Beispiel die englische Regierung mit der Einladung an die „Windrush-Generation“ aus karibischen Ländern zwischen 1948 und 1971 getan hatte.
Genuine multipartite correlations in Dicke Superradiance
Creators: name: Calegari, Susane
name: Lourenço, Antônio C.
name: Landi, Gabriel T.
name: Duzzioni, Eduardo I.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: A thorough understanding of the structure of correlations in multipartite systems is essential for the success of most quantum information processing applications. The problem, however, quickly becomes non-trivial as the size of the multipartition increases. With this motivation in mind, in this paper, we put forth a detailed study of genuine multipartite correlations (GMCs) in the Dicke model of superradiance. We compute all genuine $k$-partite correlations for Dicke states with arbitrary excitations and use these results to characterize the evolution of multipartite correlations during the superradiant dynamics. Non-trivial effects in the way correlations in Dicke states are distributed between the multiple parts are found, showing strong finite-size effects. We also employ the concept of weaving to classify how multipartite correlations scale with the number of particles in the system.
description: 7 pages, 8 figures
Additional file 1 of NUCB2/Nesfatin-1 drives breast cancer metastasis through the up-regulation of cholesterol synthesis via the mTORC1 pathway
Creators: name: Ning, Siyi
name: Liu, Caiying
name: Wang, Kangtao
name: Cai, Yubo
name: Ning, Zhicheng
name: Li, Ming
name: Zeng, Liang
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Cancer
subject: Plant Biology

description: Additional file 1. Figure S1. (A) The schematic diagram depicts a pattern of secretory Nesfatin-1, 2, and 3 that NUCB2 splits to form. (B) The potential acetylated lysine residue of NUCB2 and the involved acetyltransferases were predicted by using the CUCKOO database. (C) The possibility of acetyltransferases involved in NUCB2 acetylation is predicted by the CUCKOO database. (D) Cell viability after being treated by C646 with different concentrations (0-80μM) for 24h was detected by CCK-8 reagent. Figure S2. Confirmation of NUCB2/Nesfatin-1 knockdown and scrambled stable cell lines in BT-549 and MDA-MB-231 determined by RT-qPCR (A), Western blot (B), and ELISA for detection of the Nesfatin-1 concentrations in the culture supernatant (C). 2×105 cell lines were seeded respectively in a six-well plate containing 2 mL medium nd cultured overnight. The supernatants were collected and detected the Nesfatin-1 concentration by ELISA. The unpaired T-test was used to verify the statistical significance. **P < 0.01, ***P < 0.001. Figure S3. (A) Cell activity after being treated with exogenous Nesfatin-1 with different concentrations (0, 10, 100, 1,000, and 10,000 pg/mL) measured by CCK-8 reagent. (B) Colony formation assay results in shNUCB2-BT-549 and shNUCB2-MDA-MB231 stable cell lines treated with 1000 pg/mL Nesfatin-1. The unpaired T-test was used to verify the statistical significance. *P < 0.05, **P < 0.01. Figure S4. (A) TCGA data showed SREBP2 mRNA expression in primary breast cancer tissues (n = 1097) and normal tissues (n = 114). (B) TCGA data showed HMGCR mRNA expression in primary breast cancer tissues (n = 1097) and normal tissues (n = 114). (C) Kaplan-Meier survival curve at univariate SREBP2 level based on TCGA data. (D) Kaplan-Meier survival curve at univariate HMGCR level based on TCGA data. The unpaired T-test was used to verify the statistical significance. *P < 0.05, **P < 0.01, ***P < 0.001.
Redshifts for a Sample of Radio-Selected Poor Clusters
Creators: name: Miller, Neal A.
name: Ledlow, Michael J.
name: Owen, Frazer N.
name: Hill, John M.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Multifiber optical spectroscopy has been performed on galaxies in the vicinity of strong, nearby radio galaxies. These radio galaxies were selected from the 3CR and B2 catalogs based on their exclusion from the Abell catalog, which is puzzling given the hypothesis that an external medium is required to confine the radio plasma of such galaxies. Velocities derived from the spectra were used to confirm the existence of groups and poor clusters in the fields of most of the radio galaxies. We find that all radio galaxies with classical FR I morphologies prove to reside in clusters, whereas the other radio galaxies often appear to be recent galaxy-galaxy mergers in regions of low galaxy density. These findings confirm the earlier result that the existence of extended X-ray emission combined with a statistical excess of neighboring galaxies can be used to identify poor clusters associated with radio galaxies.
description: 45 pages including tables and figures, to appear in the Astronomical Journal
Nanopsallus carduellus
Creators: name: Linnavuori, Rauno E.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Miridae
Nanopsallus
Nanopsallus carduellus

description: Nanopsallus carduellus (Horváth, 1888)
 Material examined. GILAN: Dasht-e-Veel, 1 specimen, 20.-25.ix.1998; Sang Rud, several specimens, 19.-28.viii.2002, 30.vi.-1.vii.2003. ARDABIL: Khalkhal, 2 specimens, 9.-11.viii.1998; Kivi, 5 specimens, 9.-11.viii.2002. TEHRAN: Evin, 1 specimen, 14.-18.vii.1995; Kordan, 1 specimen, 14.vii.2002.
 Comments. In mountain meadows. Recorded from Cirsium acarna. Pontomediterranean. New for Iran.
description: Published as part of Linnavuori, Rauno E., 2007, Studies on the Miridae (Heteroptera) of Gilan and the adjacent provinces in northern Iran. II. List of species, pp. 17-56 in Acta Entomologica Musei Nationalis Pragae 47 on page 48, DOI: 10.5281/zenodo.5328235
title: „Also, ich weiß nicht, ob ich da hin will“
title: Die Rekonstruktion geschlechtsspezifischer beruflicher (Karriere-)Orientierung und Sozialisation von Ärztinnen und Ärzten in Weiterbildung
titleType: Subtitle
Creators: name: Reimann, Swantje
name: Schacht, Robert
name: Sachse, Catherina
name: Alfermann, Dorothee
Publisher: name: Humboldt-Universität zu Berlin
Year: 2017
Subjects: subject: Sozialisation
subject: Geschlechtsspezifik
subject: Doing Gender
subject: Weiterbildung
subject: 303 Gesellschaftliche Prozesse

description: Trotz annähernd gleicher Anzahl von Ärztinnen und Ärzten im Beruf bekleiden nur wenige Ärztinnen Führungspositionen. Historisch betrachtet ist die nominale Feminisierung des ärztlichen Berufs noch jung und das Krankenhaus kann auch heute noch als ein typischer Vertreter einer „gendered organization“ (Acker 1990) bezeichnet werden, deren Imperative einer idealen ärztlichen Tätigkeit und Führung mit männlichem Geschlecht assoziiert sind. Die normativen Leitbilder vermitteln sich implizit im Verlauf der Identifizierung mit der Arztrolle. Anhand von Gruppendiskussionen zeigen wir, mit welchen strukturellen und informellen Lehrplänen Ärztinnen und Ärzte in ihrer fachärztlichen Weiterbildung konfrontiert werden. Dabei sind Anforderungen an die Verausgabung für die Tätigkeit, Subjektivierungstendenzen, Führung und Macht sowie die Definition von Leistung zentrale und besonders eng mit Geschlecht assoziierte Sozialisationsinstitutionen. Auch wenn vordergründig geschlechtsspezifische Motivlagen für die Unterschiede verantwortlich gemacht werden, zeigen wir, dass es sich dabei um zustimmende Anpassungsleistungen an strukturelle Bedingungen ärztlicher Tätigkeit handelt.
description: „Well, I do not know if I want to“ The reconstruction of gender socialization of doctors in training Abstract: Despite approximately equal distribution of male and female physicians in occu- pations, only a few female doctors occupy leadership positions. Historically, the nominal feminization of the medical profession is still young and the hospital can still be regarded as a typical representative of a “gendered organization” (Acker 1990) which is identified among others by imperatives of an ideal medical practice and guidance associated with male gender. The normative models convey implicitly in the course of identification with the doctor role. Using focus groups, we show what structural and informal curricula physicians are confron- ted with in their training course. Requirements for the expenditure for the job, tendencies of subjectivation of employment, leadership and power and the definition of performance are central socialization institutions and strongly associated with gender. Although ostensibly gender typical motivations are made responsible, we show that these are favorable adjust- ments to structural conditions of medical practice.
Oncotylus (Oncotylus) viridiflavus subsp. longipes Wagner 1954
Creators: name: Linnavuori, Rauno E.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Miridae
Oncotylus
Oncotylus viridiflavus
Oncotylus (oncotylus) viridiflavus longipes wagner, 1954

description: Oncotylus (Oncotylus) viridiflavus longipes Wagner, 1954
 Material examined. Many specimens: GILAN: Astara, 8-9.vii.2003; Gyssom, 11.-18.vi.1995; Keshfi Lemir, 25 km S of Astara, 8.-9.vii.2003; Sang Rud, 30.vi.-1.vii.2003; Ziba Kenar, 7.-10.vi.1995, 29.vi.1996. ARDABIL: Khalkhal, 30.vii.1996; Majareh – Kolur, 21.vii.1996. ZANJAN: Zanjan, 13.-14.vii.2004.
 Comments. In hilly steppes. Known from Turkey. New for Iran.
 The nominotypical subspecies O. viridiflavus viridiflavus (Goeze, 1778) extends from Central and South Europe to Central Asia.
description: Published as part of Linnavuori, Rauno E., 2007, Studies on the Miridae (Heteroptera) of Gilan and the adjacent provinces in northern Iran. II. List of species, pp. 17-56 in Acta Entomologica Musei Nationalis Pragae 47 on page 49, DOI: 10.5281/zenodo.5328235
On Density-Critical Matroids
Creators: name: Campbell, Rutger
name: Grace, Kevin
name: Oxley, James
name: Whittle, Geoff
Publisher: name: arXiv
Year: 2019
Subjects: subject: Combinatorics (math.CO)
subject: FOS: Mathematics
subject: 05B35

description: For a matroid $M$ having $m$ rank-one flats, the density $d(M)$ is $\tfrac{m}{r(M)}$ unless $m = 0$, in which case $d(M)= 0$. A matroid is density-critical if all of its proper minors of non-zero rank have lower density. By a 1965 theorem of Edmonds, a matroid that is minor-minimal among simple matroids that cannot be covered by $k$ independent sets is density-critical. It is straightforward to show that $U_{1,k+1}$ is the only minor-minimal loopless matroid with no covering by $k$ independent sets. We prove that there are exactly ten minor-minimal simple obstructions to a matroid being able to be covered by two independent sets. These ten matroids are precisely the density-critical matroids $M$ such that $d(M) > 2$ but $d(N) \le 2$ for all proper minors $N$ of $M$. All density-critical matroids of density less than $2$ are series-parallel networks. For $k \ge 2$, although finding all density-critical matroids of density at most $k$ does not seem straightforward, we do solve this problem for $k=\tfrac{9}{4}$.
description: 16 pages
Additional file 2: of Item response theory analysis and properties of decisional conflict scales: findings from two multi-site trials of men with localized prostate cancer
Creators: name: Pozzar, Rachel
name: Berry, Donna
name: Fangxin Hong
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Science Policy

description: Subscales and associated items on the DCS-12 and LL DCS-10. This table provides an overview of the four subscales and associated items for the DCS-12 and LL DCS-10 as developed by Oâ Connor [1]. This information is included to assist the reader in interpreting the results of the current study; for full details regarding the DCS-12 and LL DCS-10, the reader is referred to the original content developed by Oâ Connor [1]. (DOCX 14 kb)
Interpreting the Cosmic Infrared Background: Constraints on the Evolution of the Dust Enshrouded Star Formation Rate
Creators: name: Chary, R.
name: Elbaz, D.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a detailed interpretation of the spectrum of the cosmic infrared background longwards of 5 microns and of galaxy counts from various surveys at mid-infrared, far-infrared and submillimeter wavelengths by evolving the mid-infrared local luminosity function with redshift. We find that all evolutionary models that fit the counts require a flattening at z~0.8 to avoid overproducing the CIRB. About 80% of the 140 micron CIRB is produced at 0 < z < 1.5 while only about 30% of the 850 micron background is produced within the same redshift range. The nature of the evolution is translated into a measure of the dust enshrouded star formation rate density as a function of redshift and compared with estimates from optical/near-infrared surveys. We find that the dust obscured star formation rate density appears to peak at z=0.8+/-0.1, much sooner than previously thought, with a value of 0.25+/-0.12 M_sun/yr and remains almost constant up to z~2. At least 70% of this star formation takes place in luminous infrared galaxies with L_IR > 10^11 L_sun. The long wavelength observations that constrain our evolutionary models do not strongly trace the evolution at z > 2 and a drop off in the dust enshrouded star formation rate is consistent with both the CIRB spectrum and the number counts. However, a comparison with the infrared luminosity function derived from extinction corrected optical/UV observations of the Lyman-break galaxy (LBG) population at z~3 suggests that the flat comoving star formation rate seen between redshifts 0.8 and 2, extends up to a redshift of z~4.
description: 44 pages, 16 figures (including 6 color), appearing in ApJ v556, 1 Aug 2001
Setaria appendiculata Stapf
Creators: name: Prunera-Olivé, Joan
name: Vorontsova, Maria S.
name: Williams, Emma V.
name: Mollel, Neduvoto P.
name: Hemp, Andreas
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Setaria
Setaria appendiculata

description: Setaria appendiculata (Hack.) Stapf in W.H.Harvey & auct. suc. (eds.), Fl. Cap. 7: 422 (1899).
 Distribution: Ethiopia to Tanzania, Angola to Cape Prov.
 Specimens: MOSHI Arusha Chini, Haarer, A.E. 1188 (K).
description: Published as part of Prunera-Olivé, Joan, Vorontsova, Maria S., Williams, Emma V., Mollel, Neduvoto P. & Hemp, Andreas, 2021, Checklist of Kilimanjaro grasses shows that both plot and herbarium methods are necessary to record diversity, pp. 201-244 in Phytotaxa 501 (2) on page 239, DOI: 10.11646/phytotaxa.501.2.1, http://zenodo.org/record/5424816
Stellar Collisions and the Interior Structure of Blue Stragglers
Creators: name: Lombardi, James C.
name: Warren, Jessica Sawyer
name: Rasio, Frederic A.
name: Sills, Alison
name: Warren, Aaron R.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Collisions of main sequence stars occur frequently in dense star clusters. In open and globular clusters, these collisions produce merger remnants that may be observed as blue stragglers. Detailed theoretical models of this process require lengthy hydrodynamic computations in three dimensions. However, a less computationally expensive approach, which we present here, is to approximate the merger process (including shock heating, hydrodynamic mixing, mass ejection, and angular momentum transfer) with simple algorithms based on conservation laws and a basic qualitative understanding of the hydrodynamics. These algorithms have been fine tuned through comparisons with the results of our previous hydrodynamic simulations. We find that the thermodynamic and chemical composition profiles of our simple models agree very well with those from recent SPH (smoothed particle hydrodynamics) calculations of stellar collisions, and the subsequent stellar evolution of our simple models also matches closely that of the more accurate hydrodynamic models. Our algorithms have been implemented in an easy to use software package, which we are making publicly available (see http://vassun.vassar.edu/~lombardi/mmas/). This software could be used in combination with realistic dynamical simulations of star clusters that must take into account stellar collisions.
description: This revised version has 37 pages, 13 figures, 4 tables; submitted to ApJ; for associated software package, see http://vassun.vassar.edu/~lombardi/mmas/ This revised version presents additional comparisons with SPH results and slightly improved merger recipes
Additional file 2 of NUCB2/Nesfatin-1 drives breast cancer metastasis through the up-regulation of cholesterol synthesis via the mTORC1 pathway
Creators: name: Ning, Siyi
name: Liu, Caiying
name: Wang, Kangtao
name: Cai, Yubo
name: Ning, Zhicheng
name: Li, Ming
name: Zeng, Liang
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Cancer
subject: Plant Biology

description: Additional file 2: Table S1. Primary antibodies and Second antibodies. Table S2. Primers for RT-qPCR. Table S3. IPA results of FDFT1, DHCR7, ACAT2, HMGCR, HMGCS15 genes.
Setaria homonyma Chiov., Nuovo Giorn. Bot. Ital.
Creators: name: Prunera-Olivé, Joan
name: Vorontsova, Maria S.
name: Williams, Emma V.
name: Mollel, Neduvoto P.
name: Hemp, Andreas
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Setaria
Setaria homonyma

description: Setaria homonyma (Steud.) Chiov., Nuovo Giorn. Bot. Ital., n.s., 26: 78 (1919).
 Distribution: Cameroon to Ethiopia and S. Africa, Indian Subcontinent to Myanmar
 Specimens: MOSHI Karanga River, Hemp, A. 3378 (NHT, UBT); Kibosho, Haarer, A.E. 746 (K); Kidia, Hemp, A. 283 (UBT); Kidia, Hemp, A. 578 (UBT); Lyamungu Coffe Research Station, Wallace, G.B. 1135 (K); Lyamungu Foothill, Hemp, A. 5729 (UBT); Machame route, Hemp, A. 5732 (UBT); Marangu, Volkens, G. 914 (K); Rau Forest Reserve, Hemp, A. 2816 (NHT, UBT); s. loc., Schlieben, H.J. 4709 (K).
description: Published as part of Prunera-Olivé, Joan, Vorontsova, Maria S., Williams, Emma V., Mollel, Neduvoto P. & Hemp, Andreas, 2021, Checklist of Kilimanjaro grasses shows that both plot and herbarium methods are necessary to record diversity, pp. 201-244 in Phytotaxa 501 (2) on page 239, DOI: 10.11646/phytotaxa.501.2.1, http://zenodo.org/record/5424816
Integration of adversarial autoencoders with residual dense convolutional networks for estimation of non-Gaussian hydraulic conductivities
Creators: name: Mo, Shaoxing
name: Zabaras, Nicholas
name: Shi, Xiaoqing
name: Wu, Jichun
Publisher: name: arXiv
Year: 2019
Subjects: subject: Computational Physics (physics.comp-ph)
subject: Machine Learning (cs.LG)
subject: Machine Learning (stat.ML)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: Inverse modeling for the estimation of non-Gaussian hydraulic conductivity fields in subsurface flow and solute transport models remains a challenging problem. This is mainly due to the non-Gaussian property, the non-linear physics, and the fact that many repeated evaluations of the forward model are often required. In this study, we develop a convolutional adversarial autoencoder (CAAE) to parameterize non-Gaussian conductivity fields with heterogeneous conductivity within each facies using a low-dimensional latent representation. In addition, a deep residual dense convolutional network (DRDCN) is proposed for surrogate modeling of forward models with high-dimensional and highly-complex mappings. The two networks are both based on a multilevel residual learning architecture called residual-in-residual dense block. The multilevel residual learning strategy and the dense connection structure ease the training of deep networks, enabling us to efficiently build deeper networks that have an essentially increased capacity for approximating mappings of very high-complexity. The CCAE and DRDCN networks are incorporated into an iterative ensemble smoother to formulate an inversion framework. The numerical experiments performed using 2-D and 3-D solute transport models illustrate the performance of the integrated method. The obtained results indicate that the CAAE is a robust parameterization method for non-Gaussian conductivity fields with different heterogeneity patterns. The DRDCN is able to obtain accurate approximations of the forward models with high-dimensional and highly-complex mappings using relatively limited training data. The CAAE and DRDCN methods together significantly reduce the computation time required to achieve accurate inversion results.
Exploring the Role of Jets in the Radio/X-ray Correlations of GX339-4
Creators: name: Markoff, S.
name: Nowak, M.
name: Corbel, S.
name: Fender, R.
name: Falcke, H.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The Galactic black hole candidate X-ray binary GX339-4 spends most of its time in the low/hard state, making it an ideal candidate for modeling the assumedly low accretion phase. The radio emission correlates very tightly with the X-rays over more than two orders of magnitude in X-ray flux density, suggesting that the jet plasma also plays a role at higher frequencies. We compare the predictions of our jet model, with and without acceleration, to thirteen broadband simultaneous or quasi-simultaneous spectra over this changing flux history. In addition, we consider a simple standard thin disk which transitions to an optically thin accretion flow, in order to account for the assumedly thermal optical data seen in some observations. A solution without acceleration cannot describe the data without unrealistic energy requirements. But because of the low disk luminosity, and possibly the assumed disk geometry, acceleration in the jet is limited only by synchrotron cooling and can extend easily into the X-rays. We present a model which can account for all the broadband spectra included here, by changing only two parameters in the jet model: the input power and the location of the first acceleration zone. However, the model is most sensitive to changes in the jet power, the varying of which can also account for the slope of the observed radio/X-ray correlation analytically. At the highest low/hard state luminosities, the synchrotron self-Compton emission from the jet could be detectable with missions such as {\em GLAST}, providing a way to test the extent of the synchrotron contribution. We conclude that jet synchrotron is a possible way to explain the broadband features and this correlation, and discuss ways of incorporating this component into the ``standard'' corona picture.
description: 16 pages, LaTeX, 6 EPS figures, A&A, in press
Deuterium toward the WD0621-376 sight line: Results from the Far Ultraviolet Spectroscopic Explorer (FUSE) Mission
Creators: name: Lehner, N.
name: Gry, C.
name: Sembach, K. R.
name: Hebrard, G.
name: Chayer, P.
name: Moos, H. W.
name: Howk, J. C.
name: Desert, J. -M.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Far Ultraviolet Spectroscopic Explorer observations are presented for WD0621-376, a DA white dwarf star in the local interstellar medium (LISM) at a distance of about 78 pc. The data have a signal-to-noise ratio of about 20-40 per 20 km/s resolution element and cover the wavelength range 905-1187 Å. LISM absorption is detected in the lines of D I, C II, C II*, C III, N I, N II, N III, O I, Ar I, and Fe II. This sight line is partially ionized, with an ionized nitrogen fraction of > 0.23. We determine the ratio $D/O = (3.9 \pm ^{1.3}_{1.0})\times 10^{-2}$ (2$σ$). Assuming a standard interstellar oxygen abundance, we derive ${\rm D/H} \approx 1. 3 \times 10^{-5}$. Using the value of N(H I) derived from EUVE data gives a similar D/H ratio. The D I/N I ratio is $(3.3 \pm ^{1.0}_{0.8})\times 10^{-1}$ (2$σ$).
description: accepted for publication in the ApJS
Additional file 3 of Comparative proteomic and transcriptomic analyses provide new insight into the formation of seed size in castor bean
Creators: name: Yu, Anmin
name: Li, Fei
name: Liu, Aizhong
Publisher: name: figshare
Year: 2020
Subjects: subject: Biochemistry
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology

description: Additional file 3: Figure S1. The COG functional category analysis of all proteins.
Shear and Mixing in Oscillatory Doubly Diffusive Convection
Creators: name: Paparella, Francesco
name: Spiegel, Edward A.
name: Talon, Suzanne
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: To investigate the mechanism of mixing in oscillatory doubly diffusive (ODD) convection, we truncate the horizontal modal expansion of the Boussinesq equations to obtain a simplified model of the process. In the astrophysically interesting case with low Prandtl number, large-scale shears are generated as in ordinary thermal convection. The interplay between the shear and the oscillatory convection produces intermittent overturning of the fluid with significant mixing. By contrast, in the parameter regime appropriate to sea water, large-scale flows are not generated by the convection. However, if such flows are imposed externally, intermittent overturning with enhanced mixing is observed.
description: 24 pages, 16 figures, Accepted for publication in Geophysical and Astrophysical Fluid Dynamics
Finite size effect on vector meson and baryon sectors in 2+1 flavor QCD at the physical point
Creators: name: Ishikawa, K. -I.
name: Ishizuka, N.
name: Kuramashi, Y.
name: Nakamura, Y.
name: Namekawa, Y.
name: Shintani, E.
name: Taniguchi, Y.
name: Ukita, N.
name: Yamazaki, T.
name: Yoshie, T.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We investigate the finite size effect on the vector meson and the baryon sectors using a subset of the "PACS10" configurations which are generated, keeping the space-time volumes over (10 fm$)^4$ in 2+1 flavor QCD at the physical point. Comparing the results on (5.5 fm$)^4$ and (10.9 fm$)^4$ lattices the ground states of octet baryons , which are stable on the lattice, show no finite size effect within less than 0.5% level of statistical errors. For those of vector mesons, which are unstable on the lattice, we observe that the effective masses are well below the experimental resonance levels both on (5.5 fm$)^4$ and (10.9 fm$)^4$ lattices. For the decuplet baryon sector we have found that the time dependence of the effective mass looks quite similar to that for the vector meson sector including the $Ω$ baryon channel. We discuss its origin due to a possible mixing with the nearby multihadron states. Since the $Ξ$ baryon mass can be determined with the smallest ambiguity among the vector meson and the baryon masses, we use it together with the pion and kaon masses as the physical inputs to determine the physical point.
description: 9 pages, 8 figures: published version
Setaria incrassata Hack.
Creators: name: Prunera-Olivé, Joan
name: Vorontsova, Maria S.
name: Williams, Emma V.
name: Mollel, Neduvoto P.
name: Hemp, Andreas
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Setaria
Setaria incrassata

description: Setaria incrassata (Hochst.) Hack. in H.G.A.Engler, Hochgebirgsfl. Afrika: 122 (1891).
 Distribution: Nigeria to Eritrea and S. Africa
 Specimens: MOSHI Engare Nairobi, Greenway, P.J. 6717 (K); Engare Nairobi, Greenway, P.J. 6844 (K).
description: Published as part of Prunera-Olivé, Joan, Vorontsova, Maria S., Williams, Emma V., Mollel, Neduvoto P. & Hemp, Andreas, 2021, Checklist of Kilimanjaro grasses shows that both plot and herbarium methods are necessary to record diversity, pp. 201-244 in Phytotaxa 501 (2) on page 239, DOI: 10.11646/phytotaxa.501.2.1, http://zenodo.org/record/5424816
Orthonotus rufifrons
Creators: name: Linnavuori, Rauno E.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Miridae
Orthonotus
Orthonotus rufifrons

description: Orthonotus rufifrons (Fallén, 1807)
 Material examined. Numerous specimens: GILAN: Darreh Dasht, 26.v.-20.vi.1995, 10.vii.1996; Dasht-e-Veel, 10.-12.v.2001; Deylaman, 16.-20.vii.1996; Deylaman – Barasar, 23.vii.1996; Fowman, 6.v.1995; Lounak, 30.v.- 24.vi.1995; Masuleh, 6.-26.vi.1995, 3.vii.1996; Rustam Abad – Salan Sar, 24.vii.1996, 6.-8.v.2001.
 Comments. In mountain forests, e.g. on Urtica. European, extending to Caucasus, Turkey, and Iran.
description: Published as part of Linnavuori, Rauno E., 2007, Studies on the Miridae (Heteroptera) of Gilan and the adjacent provinces in northern Iran. II. List of species, pp. 17-56 in Acta Entomologica Musei Nationalis Pragae 47 on page 49, DOI: 10.5281/zenodo.5328235