cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Do Tides Destabilize Trojan Exoplanets?
Creators: name: Dobrovolskis, Anthony R.
name: Lissauer, Jack J.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: One outstanding problem in extrasolar planet studies is why no co-orbital exoplanets have been found, despite numerous searches among the many known planetary systems, many of them in other mean-motion resonances. Here we examine the hypothesis that dissipation of energy by tides in Trojan planets is preventing their survival. The Appendix of this paper generalizes the conventional theory of tides to include tidal forces independent of dissipation, as well as the effects of one body on tides raised by another. The main text applies this theory to a model system consisting of a primary of stellar mass, a secondary of sub-stellar mass in a circular orbit about the primary, and a much lighter Trojan planet librating with small amplitude about an equilateral point of the system. Next, we linearize the equations of motion about the Trojan points, including the tidal forces, and solve for the motion of the Trojan. The results indicate that tides damp out the Trojan's motion perpendicular to the orbital plane of the primary and secondary, as well as its epicycles due to its eccentricity; but they pump up the amplitude of its tadpole librations exponentially. We then verify our analytic solutions by integrating the non-linearized equations of motion numerically for several sample cases. In each case, we find that the librations grow until the Trojan escapes its libration, which leads to a close encounter with either the primary or the secondary.
description: 37 pages, 9 figures (including 1 with color), 4 tables
Gallup Poll # 830
Creators: name: Gallup
Publisher: name: Roper Center for Public Opinion Research
Year: 2015

description: Richard Nixon job performance (1); Vietnam (1); cigarette smoking (2); Youth Conservation Corps (1); term limits (2); Richard Nixon vs. Edmund Muskie vs. George Wallace (1); Richard Nixon vs. Hubert Humphrey vs. George Wallace (1); Richard Nixon vs. Edward Kennedy vs. George Wallace (1); Communist China should/should not be admitted to U.N. (2).
Scaphoideini
Creators: name: Dietrich, Christopher H.
name: Nguyen, Huong T. T.
name: Pham, Hong Thai
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Cicadellidae

description: Tribe Scaphoideini
Mimotettix distiflangentus Dai, Zhang & Webb, 2010
Material examined. Holotype male, VIETNAM: Vinh Phuc, Tam Dao, 21.4561ºN 105.6501ºE, 983m, 10 July 2019, C.H.Dietrich, Hg vapor light in forest, VN19-7-1 (VNMN).
Notes. This species was previously recorded from southern China (Yunnan). It is here recorded from Vietnam for the first time.
description: Published as part of Dietrich, Christopher H., Nguyen, Huong T. T. & Pham, Hong Thai, 2020, New genera, new species and new records of leafhoppers (Hemiptera: Cicadellidae) from Vietnam, pp. 241-273 in Zootaxa 4877 (2) on page 255, DOI: 10.11646/zootaxa.4877.2.2, http://zenodo.org/record/4424088
Advection of Accelerated Electrons in Radio/X-ray Knots of AGN Jets
Creators: name: Rahman, Amal A.
name: Sahayanathan, S.
name: Subha, P. A
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The X-ray emission from the knots of the kilo-parsec scale jet of active galactic nuclei (AGN) suggests the high energy emission process is different from the radio/optical counterpart. Interpretation based on the Inverse Compton scattering of cosmic microwave photons has been ruled out through Fermi gamma-ray observations for low redshift sources. As an alternate explanation, synchrotron emission from a different electron population is suggested. We propose a model considering the advected electron distribution from the sites of particle acceleration in AGN knots. This advected electron distribution is significantly different from the accelerated electron distribution and satisfies the requirement of the second electron population. The synchrotron emission from the accelerated and the advected electron distribution can successfully reproduce the observed radio to X-ray fluxes of the knots of 3C 273. For the chosen combination of the model parameters, the spectrum due to inverse Compton scattering of cosmic microwave photons falls within the Fermi gamma-ray upper limits.
Estudo piloto para validação de um Protocolo de Rastreio Oftalmológico Infantil em Cuidados de Saúde Primários
Creators: name: Pinto, Fátima
name: Rodrigues, Sandra
name: Pessoa, Bernardete
name: Coelho, Pedro Pinto
Publisher: name: Portuguese Journal of Pediatrics
Year: 2014

description: Objectivo: Aferição de um protocolo de Rastreio Oftalmológico Infantil organizado e realizado numa consulta de Pediatria de ambulatório, com o intuito de serem referenciadas à consulta de Oftalmologia as crianças que dela realmente necessitam.

Material e Métodos: Análise comparativa com base num estudo prospectivo de uma população de 423 crianças observadas na consulta de Pediatria num Centro de Saúde urbano entre Abril de 2004 e Agosto de 2005. A amostra, de conveniência e consecutiva, foi constituída por crianças levadas à consulta programada de Vigilância Infantil da Pediatria de um Centro de Saúde urbano, sem qualquer queixa, aparentemente saudáveis e sem doença oftalmológica diagnosticada. Todas as crianças foram submetidas a rastreio oftalmológico, segundo um protocolo estruturado pela Pediatria e que incluiu exame ocular externo; reflexo vermelho pupilar; testes de cover e Hirschberg; movimentos oculares, reflexos pupilares fotomotores, acuidade visual e estereopsia. Deste grupo inicial foi seleccionado, de forma leatória simples, um subgrupo de 158 crianças para reavaliação pela especialidade de Oftalmologia de um Hospital Central Universitário que colaborou no estudo desconhecendo por completo os resultados da observação pediátrica.

Resultados: Compareceram à Consulta de Oftalmologia 101 crianças das 158 que concordaram participar no estudo. Na consulta de Pediatria houve suspeita de alteração oftalmológica em 22 crianças. Verificaram-se 13 casos de baixa acuidade visual/acuidade visual assimétrica, 2 de estrabismo, 9 de erro refractivo, 1 de megalocórnea e 1 de ptose palpebral. Na observação por Oftalmologia, detectaram-se 26 crianças com anomalia oftalmológica. Verificaram-se 4 casos de ambliopia, 5 de estrabismo (3 latente e 2 manifesto), 23 de erro refractivo e 1 de megalocórnea. Foi verificada concordância estatisticamente significativa entre os resultados obtidos pelas duas especialidades (teste Kappa, p <0.05).

Conclusões: Este estudo permite sustentar a validação do protocolo pediátrico proposto, como método de rastreio oftalmológico fácil, rápido, económico e eficaz a efectuar na Consulta de Vigilância Infantil.
description: Portuguese Journal of Pediatrics, vol. 38 n.º 3 (2007)
Detailed abundances of the wide pairs of stars with and without planets: the binary systems 16 Cyg and HD 219542
Creators: name: Ryabchikova, T.
name: Pakhomov, Yu.
name: Mashonkina, L.
name: Sitnova, T.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We present results of the comparative analysis of the two wide binary systems -- 16 Cyg, with a giant gas planet orbiting around 16 Cyg B, and HD 219542 without planet detected. Atmospheric parameters of the binary components and the Sun were determined using their high-resolution spectra and the SME tools for automatic spectral analysis. By applying the synthetic spectrum method, we derived abundances of 29 and 23 chemical elements in 16 Cyg and HD 219542, respectively. For 19 of these elements, our results are based on the non-local thermodynamic equilibrium (NLTE) line formation. For both 16 Cyg and HD 219542, we obtained a small abundance difference between the A and B components: +0.019$\pm$0.012 and -0.014$\pm$0.019, respectively, suggesting only a weak influence of the giant gas planet formation on chemical composition of the host star atmosphere. For HD 219542 A and B, trends of the relative-to-solar abundances with the dust condensation temperature are similar to the literature data for the solar analogues without detected planets. The components of 16 Cyg reveal very similar behaviour of [X/H] with the condensation temperature, however, it is different from that for HD 219542. This indicates a specific chemical composition of the cloud from which the 16 Cyg binary system formed.
description: 11 pages, 4 figures, 6 tables. Accepted in MNRAS
Virtual Reality for Emotion Elicitation -- A Review
Creators: name: Somarathna, Rukshani
name: Bednarz, Tomasz
name: Mohammadi, Gelareh
Publisher: name: arXiv
Year: 2021
Subjects: subject: Human-Computer Interaction (cs.HC)
subject: FOS: Computer and information sciences

description: Emotions are multifaceted phenomena that affect our behaviour, perception, and cognition. Increasing evidence indicates that induction mechanisms play a crucial role in triggering emotions by simulating the sensations required for an experimental design. Over the years, many reviews have evaluated a passive elicitation mechanism where the user is an observer, ignoring the importance of self-relevance in emotional experience. So, in response to the gap in the literature, this study intends to explore the possibility of using Virtual Reality (VR) as an active mechanism for emotion induction. Furthermore, for the success and quality of research settings, VR must select the appropriate material to effectively evoke emotions. Therefore, in the present review, we evaluated to what extent VR visual and audio-visual stimuli, games, and tasks, and 360-degree panoramas and videos can elicit emotions based on the current literature. Further, we present public datasets generated by VR and emotion-sensing interfaces that can be used in VR based research. The conclusions of this survey reveal that VR has a great potential to evoke emotions effectively and naturally by generating motivational and empathy mechanisms which makes it an ecologically valid paradigm to study emotions.
description: This work is submitted to IEEE for possible publication
Rastreio Oftalmológico Infantil nos Cuidados Primários*
Creators: name: Pinto, Fátima
name: Guerra, Isabel
name: Maia, Íris
name: Rodrigues, Sandra
Publisher: name: Portuguese Journal of Pediatrics
Year: 2014

description: Introdução: Aimportância da detecção de anomalias oculares em idade pediátrica reside na susceptibilidade deste grupo etário para desenvolver perda permanente e irreversível da visão central (ambliopia), que poderá ser evitada se precocemente identificada e tratada.

Objectivo: Avaliação da saúde visual das crianças que frequentam a consulta de Pediatria de um Centro de Saúde urbano.

Metodologia: Análise descritiva dos registos da aplicação de um protocolo de Rastreio Oftalmológico Infantil, previamente elaborado e validado, numa amostra de crianças observadas na consulta de Pediatria de um Centro de Saúde urbano. Foram critérios de exclusão a presença de sintomatologia oftalmológica, doença sistémica com manifestação ocular, seguimento numa consulta especializada de Oftalmologia e ausência de colaboração. Foram avaliados os parâmetros sexo, idade, exame ocular externo, transparência dos meios
ópticos, alinhamento ocular, acuidade visual de longe e de perto, visão estereoscópica e alteração oftalmológica com potencial ambliogénico.

Resultados: Das 704 crianças estudadas, com idades compreendidas entre 1 mês e 15 anos, suspeitou-se de patologia oftalmológica em 182 (25,9%): anomalia do exame ocular externo em 8; leucocória em 1; estrabismo em 39; diminuição da acuidade visual em 147; e má visão estereoscópica em 60. Em 78 (11,1%) casos suspeitou-se de doença potencialmente ambliogénica.

Conclusões: A necessidade de avaliar a função visual o mais precocemente possível apoia-se nos conceitos de plasticidade e do período crítico do seu desenvolvimento. Este estudo demonstra a utilidade da aplicação do Rastreio Oftalmológico Infantil generalizado a nível da consulta de vigilância infantil,contribuindo assim para a melhoria qualitativa da assistência pediátrica.
description: Portuguese Journal of Pediatrics, vol. 38 n.º 3 (2007)
title: Mose in der Tradition des jüdischen Rabbinertums und der christlichen Patristik
Creators: name: Koch, Andreas
Year: 2017

description: Die vorliegende Masterarbeit beschäftigt sich mit Mose in der jüdischen und christli-chen Tradition. Die leitende Forschungsfrage lautet: Ob und inwieweit hat eine gegen-seitige Beeinflussung und/oder Abgrenzung der jeweils jüdischen und christlichen Tra-ditionen stattgefunden. Das Forschungsprojekt wird an Ex 1,1-2,22, das die Geburt und die Jugendjahre des Mose erzählt, am Midrash Shemot Rabbah aus der rabbinischen Tradition und den Exodus Homilien I und II des Kirchenvaters Origenes durchgeführt. Die Arbeit gliedert sich in vier Teile. Der erste Teil legt Ex 1,1-2,22 auf Grundlage von einschlägigen Exoduskommentaren aus der jüdischen und christlichen Theologie in Hinblick auf die Person Mose aus. Im zweiten Teil erfolgt ein Vergleich mit den Deu-tung und Interpretationen des Midrash Shemot Rabbah, der eine ausführliche Textbear-beitung des jüdischen Midrash umfasst. Der dritte Teil geht auf die Exodus Homilien I und II des Kirchenvaters Origenes ein. Origenes gehört zweifelsohne zu den herausragendsten Kirchenväter der Antike. Ähn-lich wie im zweiten Teil wird dabei auf den Text der Homilien eingegangen. Im vierten Teil wird die leitende Forschungsfrage in Hinblick auf vorliegende Studien ausführli-cher untersucht. Vorausblickend kann gesagt werden, dass in Bezug auf eine mögliche gegenseitige Beeinflussung jüdischer und christlicher Traditionen, höchstwahrschein-lich auf christlicher Seite bejaht werden kann. Die christlich-patrisische Bibelhermeneu-tik wurde in Hinblick auf die Methodik nachweislich vom Rabbinismus geprägt. Auf jüdischer Seite gab es vermutlich, den Ausführungen von Stemberger folgend, eine be-wusste Abgrenzung vom aufstrebenden und gesellschaftlich dominierenden Christen-tum in der Zeit der Antike bis zum frühen Mittelalter. Ob, es z.B. regen Austausch zwi-schen Rabbinen und Origenes bzw. eine gegenseitige Beeinflussung beider Zugänge zu Person des Mose gegeben hat, wird von Wissenschaftlern unterschiedlich „beantwor-tet“. Einige Forscher gehen davon aus, dass es persönliche Kontakte und einen intensi-ven Austausch zwischen Rabbiner und Kirchenväter gab. Andere hingegen verneinen das. Aufgrund der Situation des Judentums in der Antike kann man eher davon ausge-hen, dass keine Anregungen aus patristischer Bibelhermeneutik übernommen wurden. Jedenfalls kann man das am Beispiel des Kirchenvater Origenes nachweisen. Der Schluss der Arbeit gibt einen Überblick über die angestellten Überlegungen.
Rue de Neuveville Freiburg
Creators: name: Rahn, Johann Rudolf
Publisher: name: [s.n.]
Year: 1871
Subjects: Freiburg im Üechtland

description: Dargestellt wird eine Ansicht (Ausschnitt) der Häuser an der Rue de la Neuveville in Freiburg im Üechtland
description: [Johann Rudolf Rahn]
description: Die Zeichnung ist eine Vorstudie zur Abbildung in: Johann Rudolf Rahn, Geschichte der bildenden Künste in der Schweiz, Zürich 1876, S. 425
Dynamical evolution of fermion-boson stars with realistic equations of state
Creators: name: Nyhan, Joseph E.
name: Kain, Ben
Publisher: name: arXiv
Year: 2022
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Fermion-boson stars are mixtures of the ordinary nuclear matter of a neutron star and bosonic dark matter. We dynamically evolve fermion-boson stars for the first time using a realistic equation of state for nuclear matter. We use our dynamical solutions to make a detailed study of the evolution of weakly and strongly perturbed static solutions. As examples of our findings, we identify a region of parameter space where weakly perturbed unstable static solutions migrate to a stable configuration and we determine the criteria under which strongly perturbed stable static solutions will always move to a stable configuration instead of collapsing to a black hole.
description: 12 pages, 6 figures. arXiv admin note: text overlap with arXiv:2201.02274
Gallup Poll # 1106G
Creators: name: Gallup
Publisher: name: Roper Center for Public Opinion Research
Year: 2006

description: Jimmy Carter job performance (1); Most important problem in U.S. (47); Political party better able to handle problem (1); Groups treated unfairly by Carter Administration (12); Blacks in today's society (2); Children going to school with black children (3); Black people living in neighborhood (2); 1980 Democratic Presidential Candidate (1); knowledge of certain people (8); 1980 Republican Presidential Candidate (1); Jimmy Carter vs. Gerald Ford (3); Edward Kennedy vs. Gerald Ford (3); Jimmy Carter vs. Ronald Reagan (3); Edward Kennedy vs. Ronald Reagan (3); Church Attendance (2); Party allegiance (4); Wage and Price controls (1).
Freyburg altes Spital im Ran
Creators: name: Rahn, Johann Rudolf
Publisher: name: [s.n.]
Year: 1871
Subjects: Freiburg im Üechtland

description: Dargestellt wird die Fassade eines Hauses an der Rue de la Neuveville in Freiburg im Üechtland
description: [Johann Rudolf Rahn]
Freiburg. Rue de la villeneuve N° 48
Creators: name: Rahn, Johann Rudolf
Publisher: name: [s.n.]
Year: 1873
Subjects: Freiburg im Üechtland

description: Dargestellt wird die Häuserzeile, mit dem Wohnhaus an der Hausnummmer 48 im Vordergrund, an der Rue de la Neuveville in Freiburg im Üechtland
description: [Johann Rudolf Rahn]
Probing the progenitor of high-$z$ short-duration GRB 201221D and its possible bulk acceleration in prompt emission
Creators: name: Yuan, Hao-Yu
name: Lü, Hou-Jun
name: Li, Ye
name: Zhang, Bin-Bin
name: Sun, Hui
name: Rice, Jared
name: Yang, Jun
name: Liang, En-Wei
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The growing observed evidence shows that the long- and short-duration gamma-ray bursts (GRBs) originate from massive star core-collapse and the merger of compact stars, respectively. GRB 201221D is a short-duration GRB lasting $\sim 0.1$ s without extended emission (EE) at high redshift $z=1.046$. By analyzing data observed with the Swift/BAT and Fermi/GBM, we find that a cutoff power-law model can adequately fit the spectrum with a soft $E_{\rm p}=113^{+9}_{-7}$ keV, and isotropic energy $E_{γ,iso} =1.36^{+0.17}_{-0.14}\times 10^{51}~\rm erg$. In order to reveal the possible physical origin of GRB 201221D, we adopted multi-wavelength criteria (e.g., Amati relation, $\varepsilon$-parameter, amplitude parameter, local event rate density, luminosity function, and properties of the host galaxy), and find that most of the observations of GRB 201221D favor a compact star merger origin. Moreover, we find that $\hatα$ is larger than $2+\hatβ$ in the prompt emission phase which suggests that the emission region is possibly undergoing acceleration during the prompt emission phase with a Poynting-flux-dominated jet.
description: 15 pages, 3 tables, 11 Figures. Accepted for published in RAA
Gallup/CNN/USA Today Poll: 2004 Presidential Election
Creators: name: CNN
name: USA Today
Publisher: name: Roper Center for Public Opinion Research
Year: 2006

description: How much thought given to upcoming election for president (1); do/do not know where people in neighborhood go to vote (1); ever voted in precinct/election district (1); how often vote (1); plans to vote in presidential election this November (2); John Kerry and John Edwards vs. George W. Bush and Dick Cheney (2); most important issue in vote for president (1); 2000 presidential election (1).
Sychentia vietnamensis Dietrich & Nguyen & Pham 2020, n. sp.
Creators: name: Dietrich, Christopher H.
name: Nguyen, Huong T. T.
name: Pham, Hong Thai
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Cicadellidae
Sychentia
Sychentia vietnamensis

description: Sychentia vietnamensis n. sp.
(Figures 6 A–F, 11Q)
Description. Length of male 7.0 mm. Coloration white, dorsum heavily marked with complex symmetrical pattern of pale brown spots and lines forming pair of prepical diamond-shaped transcommissural marks preapically and numerous false veins on forewings.
Leg chaetotaxy and forewing venation as described for S. hainanensis Wei & Zhang (2013).
Male pygofer dorsal margin deeply emarginate near midlength, distal part of lobe with darkly pigmented dorsal falcate portion contrasting with paler ventral area. Connective with subequal to length. Style apophysis sinuate with distal part curved mesad and slightly emarginate subapically. Aedeagus in lateral view with shaft ventral margin distinctly arcuate near base then straight through rest of length, parallel sided in lateral view. shaft in posterior view very slender and parallel sided with scattered indistinct lateral teeth, apex weakly expanded and poorly sclerotized.
Etymology. The species name refers to the country of origin.
Material examined. Holotype male, VIETNAM: Ninh Binh, Cuc Phuong NP, park rd. km 29, 20.3363ºN 105.6094ºE, 350m, 8 July 2019 C.H.Dietrich, Hg. vapor light, VN19-4-1 (VNMN).
Notes. This species is very similar to S. hainanensis, described from Hainan Island, China. Both species are known from single male specimens. Further collecting is needed to confirm that these two populations represent distinct species. The Vietnamese population is here treated as a distinct species based on the following morphological differences: size distinctly smaller (length of male 7.0 mm versus 7.7 mm in S. hainanensis); pygofer dorsal margin more deeply emarginate; connective slightly wider than long (distinctly longer than wide in S. hainanensis); aedeagus with posteroventral margin distinctly arched near base and nearly straight and parallel-sided for rest of length in lateral view (evenly curved and distinctly tapered in S. hainanensis).
description: Published as part of Dietrich, Christopher H., Nguyen, Huong T. T. & Pham, Hong Thai, 2020, New genera, new species and new records of leafhoppers (Hemiptera: Cicadellidae) from Vietnam, pp. 241-273 in Zootaxa 4877 (2) on page 258, DOI: 10.11646/zootaxa.4877.2.2, http://zenodo.org/record/4424088
Doubling of minute-long Quasi-Periodic Pulsations from super-flares on a low mass star
Creators: name: Doyle, J. Gerry
name: Irawati, Puji
name: Kolotkov, Dmitrii Y.
name: Ramsay, Gavin
name: Nhalil, Nived Vilangot
name: Dhillon, Vik S.
name: Marsh, Tom R.
name: Yadav, Ram Kesh
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Using the ULTRASPEC instrument mounted on the 2.4-m Thai National Telescope, we observed two large flares, each with a total energy close to 10^34 erg with sub-second cadence. A combination of a wavelet analysis, a Fourier transform plus an empirical mode decomposition, reveals quasi-period pulsations (QPP) which exhibit an apparent doubling of the oscillation period. Both events showed oscillations of a few minutes over a interval of several minutes, and despite the availability of sub-second cadence, there was no evidence of sub-minute oscillations. The doubling of the QPP periods and shorter lifetime of shorter-period QPP modes strongly favour resonant dynamics of magnetohydrodynamic waves in a coronal loop. We estimate loop lengths to be 0.2-0.7 R*, in agreement with a typical length of solar coronal loops. These observations presents rare and compelling evidence for the presence of compact plasma loops in a stellar corona.
Gallup/CNN/USA Today Poll # 2005-06: Democratic Party/Chairman of the Democratic National Committee
Creators: name: CNN
name: USA Today
Publisher: name: Roper Center for Public Opinion Research
Year: 2005

description: Democratic party's approach to winning major elections (1); reason why Democrats lost 2004 presidential election (1); key to victory for Democratic party in future elections (1); would rather see Democratic party become more liberal/more moderate (1); how likely that Democrats will win 2008 presidential election (1); number of U.S. troops in Iraq (1); what approach should Democratic party take with George W. Bush and the Republicans over next four years (1); Democratic party should/should not only select someone as its next chair who is pro-choice (1); respondent's choice to be next chair of Democratic National Committee (3); what kind of job does respondent think Howard Dean would do if he were elected chair of Democratic National Committee (1).
Experimental study of the removal of excited state phosphorus atoms by H$_{2}$O and H$_{2}$: implications for the formation of PO in stellar winds
Creators: name: Douglas, Kevin M.
name: Gobrecht, David
name: Plane, John M. C.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The reactions of the low-lying metastable states of atomic phosphorus, P($^2$D) and P($^2$P), with H$_{2}$O and H$_{2}$ were studied by the pulsed laser photolysis at 248 nm of PCl$_{3}$ , combined with laser induced fluorescence detection of P($^2$D), P($^2$P) and PO. Rate coefficients between 291 and 740 K were measured, along with a yield for the production of PO from P($^2$D or $^2$P) + H$_{2}$O of (35$\pm$15)%. H$_{2}$ reacts with both excited P states relatively efficiently; physical (i.e. collisional) quenching, rather than chemical reaction to produced PH + H, is shown to be the more likely pathway. A comprehensive phosphorus chemistry network is then developed using a combination of electronic structure theory calculations and a Master Equation treatment of reactions taking place over complex potential energy surfaces. The resulting model shows that at the high temperatures within two stellar radii of a MIRA variable AGB star in oxygen-rich conditions, collisional excitation of ground-state P($^4$S) to P($^2$D), followed by reaction with H$_{2}$O, is a significant pathway for producing PO (in addition to the reaction between P($^4$S) and OH). The model also demonstrates that the PN fractional abundance in a steady (non-pulsating) outflow is under-predicted by about 2 orders of magnitude. However, under shocked conditions where sufficient thermal dissociation of N$_2$ occurs at temperatures above 4000 K, the resulting N atoms convert a substantial fraction of PO to PN.
description: 24 pages, 7 figures, accepted for publication in MNRAS
Pew Research Center Poll: February 1997, Media Survey
Creators: name: Pew Research Center
Publisher: name: Roper Center for Public Opinion Research
Year: 1998

description: Clinton job performance(1); Congressional job performance(1); status of American cities(1); Clinton in the news(1); TV programs and publications(10); news on TV(1); reading daily newspaper(1); balancing the federal budget(4); opinions about certain organizations(6); solving nation's problems(1); Republican leaders vs Democratic leaders(7); entertainment vs news shows(6); criticism from the press(1); monitoring personal and ethical behavior(2); criticism of proposals(2); people's privacy(2); accuracy of news organizations(1); news bias dealing with political and social issues(1); libel suits(1); press reports of crime suspects(1); Bob Dole's affair(1); investigative reporting(6); Richard Jewell(3); Jon Benet Ramsey(2); Dallas Cowboy players wrongfully accused of sexual assault(3); religious preference(2).
Pew Research Center Poll: April 1997, News Interest Index
Creators: name: Pew Research Center
Publisher: name: Roper Center for Public Opinion Research
Year: 1998

description: Clinton job performance(1); Congressional job performance(1); impression of Al Gore(1); stories in the news(8); federal government(1); immigrants(3); immigration laws(5); today's immigrants(1); immigrants impact on nation(11); Asian immigrants(6); Latin American immigrants(6); racial make up of neighborhood(1); interaction with non-English speaking immigrants(2); recent immigrants(2); people in the news(5); expansion of NATO(3); Congress(3); greatest threat to the United States(1); terrorism(6); nuclear attack(2); sending indecent materials to minors on the internet(2); policies and proposals(4); religious preference(2).
Stenometopiini
Creators: name: Dietrich, Christopher H.
name: Nguyen, Huong T. T.
name: Pham, Hong Thai
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Cicadellidae

description: Tribe Stenometopiini
Stirellus neospeciosus Duan, Webb & Zhang 2016
Material examined. One female, VIETNAM: Ninh Binh, Cuc Phuong NP center 20.3522ºN 105.5983ºE, 370m, 8 July 2019, C.H.Dietrich, sweeping along rd., VN19-2-3; 1 male, same data except 5 July 2019, VN 19-2-1 (INHS).
Notes. This species is widespread in southern China. It is recorded here from Vietnam for the first time.
description: Published as part of Dietrich, Christopher H., Nguyen, Huong T. T. & Pham, Hong Thai, 2020, New genera, new species and new records of leafhoppers (Hemiptera: Cicadellidae) from Vietnam, pp. 241-273 in Zootaxa 4877 (2) on page 258, DOI: 10.11646/zootaxa.4877.2.2, http://zenodo.org/record/4424088
Pew Research Center Poll: May 1997, News Interest Index
Creators: name: Pew Research Center
Publisher: name: Roper Center for Public Opinion Research
Year: 1998

description: Presidential job performance(1); Congressional job performance(1); stories in the news(9); names of people in the news(12); federal budget deficit(1); federal budget sending(14); balancing the budget(4); Republican party goals(1); Democratic party goals(1); partial birth abortion(2); abortion(2); opinions of some organizations(10); juvenile offenders(1); personal financial situation(3); employee income(2); campaign fundraising abuses(1); Whitewater(3); concerns people may have(7); religious preference(2).
RR Lyrae-based Distances for 39 Nearby Dwarf Galaxies Calibrated to Gaia eDR3
Creators: name: Nagarajan, Pranav
name: Weisz, Daniel R.
name: El-Badry, Kareem
Publisher: name: arXiv
Year: 2021
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We provide uniform RR Lyrae-based distances to 39 dwarf galaxies in and around the Local Group. We determine distances based on a Bayesian hierarchical model that uses periods and magnitudes of published RR Lyrae in dwarf galaxies and is anchored to well-studied Milky Way (MW) RR Lyrae with spectroscopic metallicities and Gaia eDR3 parallaxes. Gaia eDR3 parallaxes for the anchor sample are a factor of 2, on average, more precise than DR2 parallaxes, and allow for a much better constrained period-luminosity-metallicity relation. While $\sim75$% of our distances are within 1-$σ$ of recent literature RR Lyrae distances, our distances are also $\sim2$-$3$ times more precise than literature distances, on average. On average, our distances are $\sim0.05$ mag closer than literature distances, as well as $\sim0.06$ mag closer than distances derived using a theoretical period-luminosity-metallicity relation. These discrepancies are largely due to our eDR3 parallax anchor. We show that the Hipparcos-anchored RR Lyrae distance scale of Carretta et al. (2000) over-predicts distances to MW RR Lyrae by $\sim0.05$ mag. The largest uncertainties in our distances are (i) the lack of direct metallicity measurements for RR Lyrae and (ii) the heterogeneity of published RR Lyrae photometry. We provide simple formulae to place new dwarf galaxies with RR Lyrae on a common distance scale with this work. We provide public code that can easily incorporate additional galaxies and data from future surveys, providing a versatile framework for cartography of the local Universe with RR Lyrae.
description: 34 pages, 15 figures, Published in ApJ
Pew Research Center Poll: : November 2006 Election Weekend Survey
Creators: name: Pew Research Center
Publisher: name: Roper Center for Public Opinion Research
Year: 2007

description: Thoughts about upcoming election (1); respondent certain to vote (1); interest in 2006 Congressional election (1); frequency of voting (2); know where people vote in respondent's neighborhood (1); interest in politics (1); 2006 Congressional election (10); most important issue for voting in the election (2); re-elected representative from Congress (2); more/less enthusiastic about this election (1); vote for Congress is a vote for/against George W. Bush (1); ways respondent has been contacted by political groups (4); confidence in respondent's vote being accurately counted (1); political campaigns (1); George W. Bush job performance (1); same-sex marriage (1); abortion (1); stem cell research (2); groups respondent belongs to (5); Iraq (3); economy (1); US winning/losing the war on terrorism (1); John Kerry's comments on US troops in Iraq (2); Donald Rumsfeld acting as Secretary of Defense until 2009 (2); send/receive email (1); attend religious services (1).
Hydrodynamic modelling of pulsation period decrease in the Mira-type variable T UMi
Creators: name: Fadeyev, Yuri A.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Pulsation period decrease during the initial stage of the thermal pulse in the helium-burning shell of the Mira-type variable T UMi is investigated with numerical methods of stellar evolution and radiation hydrodynamics. To this end, a grid of evolutionary tracks was calculated for stars with masses on the main sequence $1M_\odot\le M_\textrm{ZAMS}\le 2.2M_\odot$ and metallicity $Z=0.01$. Selected models of AGB evolutionary sequences were used for determination of the initial conditions and the time--dependent inner boundary conditions for the equations of hydrodynamics describing evolutionary changes in the radially pulsating star. The onset of period decrease during the initial stage of the thermal pulse is shown to nearly coincide with the peak helium-burning luminosity. The most rapid decrease of the period occurs during the first three decades. The pulsation period decreases due to both contraction of the star and mode switching from the fundamental mode to the first overtone. The time-scale of mode switching is of the order of a few dozen pulsation cycles. The present-day model of the Mira-type variable T UMi is the first-overtone pulsator with small-amplitude semi-regular oscillations. Theoretical estimates of the pulsation period at the onset of period decrease and the rate of period change three decades later are shown to agree with available observational data on T UMi for AGB stars with masses $ 1.04M_\odot\le M\le 1.48M_\odot$.
description: 6 pages, 10 figures, 1 table, accepted to MNRAS
Pew Research Center Poll: October 2012, Omnibus Week 2--2012 Presidential Election/Vice-Presidential Debate
Creators: name: Pew Research Center
Publisher: name: Roper Center for Public Opinion Research
Year: 2013

description: News stories followed closely (3); Barack Obama critical of Mitt Romney (1); Romney critical of Obama (1); vice-presidential debate (2); presidential debate (2); Obama handling Libya ambassador murder (1); knowledge about Libya situation (2).
Sonnenfleckenzeichnung Nr. 890.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 14.10.1890, erstellt von Alfred Wolfer
Creators: name: Eidgenössische Sternwarte in Zürich (ETH Zürich bzw. vor 1911 Polytechnikum)
Publisher: name: [s.n.]
Year: 1890

description: Bleistiftzeichnung, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich. Instrument: Kern-Merz-Refraktor.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Zugeordnete numerische Werte wurden in einer separat geführten, chronologischen Tabelle erfasst
description: ETH-Bibliothek
Inward and outward migration of massive planets: moving towards a stalling radius
Creators: name: Scardoni, C. E.
name: Clarke, C. J.
name: Rosotti, G. P.
name: Booth, R. A.
name: Alexander, R. D.
name: Ragusa, E.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Recent studies on the planet-dominated regime of Type II migration showed that, contrary to the conventional wisdom, massive planets can migrate outwards. Using `fixed-planet' simulations these studies found a correlation between the sign of the torques acting on the planet and the parameter $K'$ (which describes the depth of the gap carved by the planet in the disc). We perform `live-planet' simulations exploring a range of $K'$ and disc mass values to test and extend these results. The excitation of planet eccentricity in live-planet simulations breaks the direct dependence of migration rate (rate of change of semi-major axis) on the torques imposed, an effect that `fixed-planet' simulations cannot treat. By disentangling the contribution to the torque due to the semi-major axis evolution from that due to the eccentricity evolution, we recover the relation between the magnitude and sign of migration and $K'$ and argue that this relation may be better expressed in terms of the related gap depth parameter $K$. We present a toy model in which the sign of planetary migration changes at a limiting value of $K$, through which we explore planets' migration in viscously evolving discs. The existence of the torque reversal shapes the planetary system's architecture by accumulating planets either at the stalling radius or in a band around it (defined by the interplay between the planet migration and the disc evolution). In either case, planets pile up in the area $1-10$ au, disfavouring hot Jupiter formation through Type II migration in the planet-dominated regime.
description: 16 pages, 14 figures, accepted for publication in MNRAS
Pew Research Center Poll: October 2012, Omnibus Week 3--Internet/2012 Presidential Election
Creators: name: Pew Research Center
Publisher: name: Roper Center for Public Opinion Research
Year: 2013

description: Satisfaction with country (1); most important problems (3); Internet usage (1); sending emails (1); mobile internet access (1); social networking sites (2); news stories followed closely (4); election campaign description (5); presidential debate (2).
Cold Gas Reservoirs of Low- and High-mass Central Galaxies Differ in Response to Active Galactic Nucleus Feedback
Creators: name: Guo, Hong
name: Jones, Michael G.
name: Wang, Jing
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The growth of supermassive black holes, especially the associated state of active galactic nuclei (AGNs), is generally believed to be the key step in regulating star formation in massive galaxies. As the fuel of star formation, the cold gas reservoir is a direct probe of the effect of AGN feedback on their host galaxies. However, in observation, no clear connection has been found between AGN activity and the cold gas mass. In this paper, we find observational signals of significant depletion of the total neutral hydrogen gas reservoir in optically-selected type-2 AGN host central galaxies of stellar mass $10^{9}$--$10^{10}M_\odot$. The effect of AGN feedback on the cold gas reservoir is stronger for higher star formation rates and higher AGN luminosity. But it becomes much weaker above this mass range, consistent with previous findings focusing on massive galaxies. Our result suggests that low-mass and gas-rich AGN host central galaxies would first form dense cores before AGN feedback is triggered, removing their neutral hydrogen gas. More massive central galaxies may undergo a significantly different formation scenario by gradually building up dense cores with less effective and recurrent AGN feedback.
description: 9 pages, 4 figures. Match the accepted version in ApJL
Frischenberg i d Herrschaft Sax
Creators: name: Immler, Paul Peter
Publisher: name: [s.n.]
Year: 1865
Subjects: Sax, Sennwald

description: Dargestellt wird ein Grundriss der Burgruine Frischenberg in Sax bei Sennwald
description: PI [Monogramm]
description: Paul Peter Immler hat handschriftlich notiert "1/4000" und "Samml. A Nüscheler"
description: PI = Paul Peter Immler
Explainability's Gain is Optimality's Loss? -- How Explanations Bias Decision-making
Creators: name: Wan, Charles
name: Belo, Rodrigo
name: Zejnilović, Leid
Publisher: name: arXiv
Year: 2022
Subjects: subject: Human-Computer Interaction (cs.HC)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: Decisions in organizations are about evaluating alternatives and choosing the one that would best serve organizational goals. To the extent that the evaluation of alternatives could be formulated as a predictive task with appropriate metrics, machine learning algorithms are increasingly being used to improve the efficiency of the process. Explanations help to facilitate communication between the algorithm and the human decision-maker, making it easier for the latter to interpret and make decisions on the basis of predictions by the former. Feature-based explanations' semantics of causal models, however, induce leakage from the decision-maker's prior beliefs. Our findings from a field experiment demonstrate empirically how this leads to confirmation bias and disparate impact on the decision-maker's confidence in the predictions. Such differences can lead to sub-optimal and biased decision outcomes.
description: To appear in the Proceedings of the 2022 AAAI/ACM Conference on AI, Ethics, and Society (AIES '22)
Neutrino meets ultralight dark matter: $\boldsymbol{0νββ}$ decay and cosmology
Creators: name: Huang, Guo-yuan
name: Nath, Newton
Publisher: name: arXiv
Year: 2021
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We explore the neutrinoless double beta ($0νββ$) decay induced by an ultralight dark matter field coupled to neutrinos. The effect on $0νββ$ decay is significant if the coupling violates the lepton number, for which the $ΔL=2$ transition is directly driven by the dark matter field without further suppression of small neutrino masses. As the ultralight dark matter can be well described by a classical field, the effect features a periodic modulation pattern in decay events. However, we find that in the early Universe such coupling will be very likely to alter the standard cosmological results. In particular, the requirement of neutrino free-streaming before the matter-radiation equality severely constrains the parameter space, such that the future $0νββ$ decay experiments can hardly see any signal even with a meV sensitivity to the effective neutrino mass.
description: 10 pages, 5 figures, v2: matching the published version
title: Auswirkungen internationaler Sanktionen auf die iranische Energiepolitik
Creators: name: Saidpour, Nikol
Year: 2017

description: Der Iran gilt als eines der Ölreichsten Länder der Welt. Die Wirtschaft und das BIP des Landes sind zum Großteil von dem Energieexport und den daraus erhaltenen Einnahmen abhängig. Trotz dieser Anhängigkeit wurde seit der Erschließung der ersten Ölfelder keine einheitliche Energiepolitik seitens der Regierungen erarbeitet. Die Energiepolitik ist die Summe aller Pläne, Aktionen und Policies welche die Handlungen einer Regierung bezüglich der Produktion, Distribution und Verbrauch von Energie bestimmen. Dazu zählen auch die Nachhaltigkeit und alle internationalen Verträge und Investitionen im Energiesektor. Daher ist die Energiepolitik eines Landes von großer Bedeutung. Durch die Zuspitzung des iranischen Atomkonflikts mit dem Westen und die immer schwerwiegendere Sanktionierung des Wirtschafts- und Energiesektors wurde es für den Iran immer schwieriger sein Öl zu exportieren. Dieser Umstand machte deutlich, dass die Entwicklung einer Energiepolitik mehr denn je von Nöten war. Im Zuge dieser Masterarbeit soll die Energiepolitik des Irans zwischen den Jahren 2006-2017-also mit dem Erlass der ersten nuklearen Sanktionen bis zwei Jahre nach dem Joint comprehensive plan of action (JCPOA)- und Auswirkungen der internationalen Sanktionen auf die Energiepolitik untersucht werden. Besonderes Augenmerk liegt hierbei auf die Energiediplomatie des Irans.
Not perfect, but it can be used to measure relational aggression: Psychometric properties of the Indonesian version of the Relational Aggression Scale
Creators: name: Muttaqin, Darmawan
name: Wibaningrum, Gayatri
name: Dermawan, Kevin
name: Ryan, Timothy
name: Tanuwijaya, Shannen Vania
Publisher: name: Psychology Hub
Year: 2024

description: Relational aggression is one form of violence that can occur in interpersonal relationships. Relational aggression has various construct variations and measurement tools. Recently, a new measurement tool for relational aggression called the Relational Aggression Scale (RAS) has been developed, which can be used to measure the construct of relational aggression directly, indirectly, proactively, and reactively. This study aims to evaluate the psychometric properties of the RAS in an Indonesian sample. Participants in the study were 712 individuals aged 18-25 years (M = 20.987, SD = 1.552) residing in Surabaya. The evaluation of the psychometric properties of the Indonesian version of the RAS included content validity, item accuracy, factor structure, and convergent validity. The study found that not all items of the Indonesian version of the RAS have satisfactory item quality based on Aiken V calculation and infit and outfit estimates of the Rasch model. However, the Indonesian version of the RAS has a satisfactory factor structure and convergent validity. Although the Indonesian version of the RAS is not perfect in terms of item quality, the Indonesian version of the RAS can be used to measure relational aggression in the Indonesian sample.
description: Psychology Hub, Vol. 41 No. 1 (2024)
Roper Fortune # 17: War/Politics/Government/The Election/Parties
Creators: name: Fortune Magazine
Publisher: name: Roper Center for Public Opinion Research
Year: 1999

description: Keep US out of war: Republican v.s. Democratic Party (1); things next administration should/should not do (10); most important problem for next administration (2); foreign trade (1); re-elect Roosevelt (3); 1928 presidential election (1); 1932 presidential election (1); 1936 presidential election (1); changing political parties (1); Republican nomination for president (3); government and business (1).
Balbillini
Creators: name: Dietrich, Christopher H.
name: Nguyen, Huong T. T.
name: Pham, Hong Thai
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Cicadellidae

description: Tribe Balbillini
Stenotortor subhimalaya Viraktamath & Wesley, 1988
(Figure 11S)
Material examined. VIETNAM: Vinh Phuc, Tam Dao summit trail, 21.4622ºN 105.6473ºE, 970m 11 July 2019, C.H.Dietrich, sweeping forest understory, incl. bamboo, VN19-6-1 (INHS).
Notes. This species was previously recorded from India. It is here recorded from Vietnam for the first time.
description: Published as part of Dietrich, Christopher H., Nguyen, Huong T. T. & Pham, Hong Thai, 2020, New genera, new species and new records of leafhoppers (Hemiptera: Cicadellidae) from Vietnam, pp. 241-273 in Zootaxa 4877 (2) on page 260, DOI: 10.11646/zootaxa.4877.2.2, http://zenodo.org/record/4424088