bluuebunny/crossref_metadata_2025_split huggingface dataset:
Moses, money, and multiple-choice: The Moses illusion in a multiple-choice format with high incentives
Authors: Speckmann Felix , Unkelbach Christian 
Published: December 2020

AbstractWhen people answer the question “How many animals of each kind did Moses take on the Ark?”, they usually respond with “two,” although Moses does not appear in the biblical story of the Ark. We investigated this “Moses illusion” in a multiple-choice format and tested the influence of monetary incentives on the illusion’s strength. Thereby, we addressed the role of a cooperative communication context for the illusion’s emergence, as well as the role of participants’ motivation. In four experiments (total N = 914), we found that the Moses illusion persists in a multiple-choice format. As the multiple-choice format realizes a cooperative context in which the correct answer is always available, we exclude a cooperative context explanation for the illusion. Monetary incentives reduced the strength of the illusion. However, the reduction was numerically and statistically small. We thereby show that the illusion is not due to violations of cooperative communications, and not due to a lack of motivation. The multiple-choice approach will facilitate further research on the Moses illusion and the data provide additional evidence for the Moses illusion’s empirical robustness and constrain its theoretical explanations.
Nickel nanoparticle decorated reduced graphene oxide-WO3 nanocomposite - a promising candidate for gas sensing
Authors: Simon Ilka , Savitsky Alexandr , Mülhaupt Rolf , Pankov Vladimir , Janiak Christoph 
Published: December 2020

We report for the first time the doping of WO3 sensing elements with a non-noble metal carbon composite, namely a nickel metal nanoparticles-carbon composite (Ni@rGO). Previous work with WO3 had used either NiO (as part of the WO3 lattice) or carbon alone or Pd-surface decorated WO3 (Pd@WO3) or Pd or Pt@carbon@WO3. We demonstrate the gas response for pure WO3, rGO-doped WO3 and Ni@rGO doped WO3 sensing elements towards NO2 (10 ppm) and acetone (35,000 ppm) in air. The addition of 0.35 wt% Ni@rGO composite to WO3 enables the increase of the sensory response by more than 1.6 times for NO2 vapors as well as 4 times regarding acetone vapors (n-type response).
Principais modalidades fisioterapêuticas em idosos com pneumonia em um hospital privado de Goiânia
Authors: Ferreira de Oliveira Amanda , Francisca Ferreira Lima Leide , Francisca Ferreira Lima Leide , Nunes Correia Andressa , Araújo Martins Jackeline , Craveiro Ramos Gabrielly , Custódio Alcântara Erikson , Hugo Sousa Utida Victor 
Published: December 2020

Objetivo: Descrever e analisar as modalidades fisioterapêuticas descritas para idosos internados com pneumonia em um hospital privado. Métodos: Estudo de coorte retrospectivo e analítico, realizado com 164 pacientes diagnósticados com PMN no período de 1 ano, em um hospital privado de Goiânia, Goiás, Brasil. Os dados foram coletados através de análise de prontuários disponibilizados pelo hospital, e transcritos para uma planilha de excel. Para análise utilizou-se o teste de Kolmogorov-Smirnov para distribuição da amostra, e para correlação o teste de Sperman. Resultados: Foram encontradas 21 modalidades de fisioterapia realizadas em pacientes idosos com pneumonia, sendo as mais frequentes a terapia de expansão pulmonar (95,1%), terapia de higiene brônquica (50%) e posicionamento funcional no leito (74,2%). Sobre os desfechos clínicos, 82,3% dos pacientes receberam alta e 16,1% evoluíram para o óbito. Houve correlação significativa entre o óbito e o posicionamento funcional no leito, terapia de higiene brônquica e aspiração de TOT e VAS (p≤0,05). Conclusão: As modalidades terapia de expansão pulmonar, posicionamento funcional, terapia de higiene brônquica, bombeamento de extremidade, alongamentos, sedestação beira leito e orientações ao paciente e familiares são as mais realizadas em pacientes idosos com pneumonia.
Perfil epidemiológico das infecções por HIV e sífilis no município de Anápolis - Goiás entre os anos 2015 e 2019
Authors: Guilarde Torres Talita , Ferreira Dutra Ana Caroline , Cavalcante de Lima Gabriela Cavalcante , De Oliveira Silva Lorena , De Paula Sousa Marcos Vinicius , Vieira Queiroz Labre Luciana , Saori Takahashi Miranda Carina , Scaliante de Moura Rodrigo 
Published: December 2020

Objetivo: Tabular e analisar o perfil epidemiológico dos indivíduos infectados por sífilis e por HIV no município de Anápolis - Goiás, no período entre 2015 e 2019. Métodos: Trata-se de um estudo ecológico, descritivo, transversal, analítico, retrospectivo, quantitativo, cujos dados correspondem ao período entre os anos de 2015 e 2019. A coleta foi realizada por meio do Departamento de Informática do SUS e do Painel de Indicadores Epidemiológicos do Ministério da Saúde e as informações colhidas foram estatisticamente analisadas a partir do Microsoft Excel (Office 2007). Resultados: as taxas de incidência de HIV, tanto em Anápolis quanto em Goiás, permanecem acima da média nacional (17,8/100.000 habitantes) em todos os anos estudados, mas a taxa de crescimento tem tido decréscimo, desde 2015. Há maior prevalência de casos de HIV no sexo masculino. Em Anápolis, no ano de 2019, 86,90% das pessoas HIV positivo tinham acesso à Terapia Anti-Retroviral e, destas, 92% tinham carga viral indetectável. A média de gastos com internações foi de R$ 575,56 com os pacientes HIV positivos. Em relação a sífilis, também ocorreu um aumento considerável das taxas no estado de Goiás e no município de Anápolis. Em Anápolis, houve maior incidência em homens. Foram gastos uma média de R$ 1.657,79 com internações de pacientes sifilíticos. Conclusão: observa-se um crescimento no número de infecções por HIV e, principalmente, de sífilis, com predominância no sexo masculino. Além disso, nota-se uma subnotificação nos sistemas de saúde.
Where’s the Dust?: The Deepening Anomaly of Microwave Emission in NGC 4725 B
Authors: Murphy E. J. , Hensley B. S. , Linden S. T. , Draine B. T. , Dong D. , Momjian E. , Helou G. , Evans A. S. 
Published: December 2020

Abstract
We present new Atacama Large Millimeter Array (ALMA) observations toward NGC 4725 B, a discrete, compact, optically faint region within the star-forming disk of the nearby galaxy NGC 4725 that exhibits strong anomalous microwave emission (AME). These new ALMA data include continuum observations centered at 92, 133, 203, and 221 GHz accompanied by spectral observations of the 12CO (

) line. NGC 4725 B is detected in the continuum at all frequencies, although the detection at 203 GHz is marginal. While molecular gas is not detected at the exact location of NGC 4725 B, there is molecular gas in the immediate vicinity (i.e., ≲100 pc) along with associated diffuse 8 μm emission. When combined with existing Very Large Array continuum data at 1.5, 3, 5.5, 9, 14, 22, 33, and 44 GHz, the spectrum is best fit by a combination of AME, synchrotron, and free–free emission that is free–free absorbed below ∼6 GHz. Given the strength of the AME, there is surprisingly no indication of millimeter dust emission associated with NGC 4725 B on ≲6″ spatial scales at the sensitivity of the ALMA interferometric data. Based on the properties of the nearest molecular gas complex and the inferred star formation rate, NGC 4725 B is consistent with being an extremely young (∼3–5 Myr) massive (≲105
M
⊙) cluster that is undergoing active cluster feedback. However, the lack of millimeter thermal dust emission is difficult to reconcile with a spinning dust origin of the 30 GHz emission. On the other hand, modeling NGC 4725 B as a new class of background radio galaxy is also unsatisfactory.
Multiwavelength Radio Observations of Two Repeating Fast Radio Burst Sources: FRB 121102 and FRB 180916.J0158+65
Authors: Pearlman Aaron B. , Majid Walid A. , Prince Thomas A. , Nimmo Kenzie , Hessels Jason W. T. , Naudet Charles J. , Kocz Jonathon 
Published: December 2020

Abstract
The spectra of fast radio bursts (FRBs) encode valuable information about the source’s local environment, underlying emission mechanism(s), and the intervening media along the line of sight. We present results from a long-term multiwavelength radio monitoring campaign of two repeating FRB sources, FRB 121102 and FRB 180916.J0158+65, with the NASA Deep Space Network (DSN) 70 m radio telescopes (DSS-63 and DSS-14). The observations of FRB 121102 were performed simultaneously at 2.3 and 8.4 GHz, and spanned a total of 27.3 hr between 2019 September 19 and 2020 February 11. We detected two radio bursts in the 2.3 GHz frequency band from FRB 121102, but no evidence of radio emission was found at 8.4 GHz during any of our observations. We observed FRB 180916.J0158+65 simultaneously at 2.3 and 8.4 GHz, and also separately in the 1.5 GHz frequency band, for a total of 101.8 hr between 2019 September 19 and 2020 May 14. Our observations of FRB 180916.J0158+65 spanned multiple activity cycles during which the source was known to be active and covered a wide range of activity phases. Several of our observations occurred during times when bursts were detected from the source between 400 and 800 MHz with the Canadian Hydrogen Intensity Mapping Experiment (CHIME) radio telescope. However, no radio bursts were detected from FRB 180916.J0158+65 at any of the frequencies used during our observations with the DSN radio telescopes. We find that FRB 180916.J0158+65's apparent activity is strongly frequency-dependent due to the narrowband nature of its radio bursts, which have less spectral occupancy at high radio frequencies (≳ 2 GHz). We also find that fewer or fainter bursts are emitted from the source at high radio frequencies. We discuss the implications of these results for possible progenitor models of repeating FRBs.
Combined ∼10 eV to ∼344 MeV Particle Spectra and Pressures in the Heliosheath along the Voyager 2 Trajectory
Authors: Dialynas Konstantinos , Galli Andre , Dayeh Maher A. , Cummings Alan C. , Decker Robert B. , Fuselier Stephen A. , Gkioulidou Matina , Roussos Elias , Krimigis Stamatios M. , Mitchell Donald G. , Richardson John D. , Opher Merav 
Published: December 2020

Abstract
We report a unique combination of ∼10 eV to ∼344 MeV in situ ion measurements from the Plasma Science (PLS), Low Energy Charged Particle (LECP), and Cosmic Ray Subsystem (CRS) experiments on the Voyager 2 (V2) spacecraft, and remotely sensed ∼110 eV to ∼55 keV energetic neutral atom (ENA) measurements from the Interstellar Boundary Explorer (IBEX) mission and Ion and Neutral Camera (INCA) on the Cassini mission. This combination is done over the time period from 2009 to the end of 2016, along the V2 trajectory, toward assessing the properties of the ion energy spectra inside the heliosheath. The combined energy spectra exhibit a series of softening and hardening breaks, providing important insights on the various ion acceleration processes inside the heliosheath. Ions in the <6 keV energy range dominate the total pressure distribution inside the heliosheath but the ion distributions at higher energies (>5.2 keV) provide a significant contribution to the total pressure. With the assumption that all ENAs (∼110 eV to 55 keV) are created by charge-exchange interactions inside the heliosheath, we estimate that the magnetic field upstream at the heliopause required to balance the pressure from the heliosheath in the direction of V2 is ∼0.67 nT. This number is consistent with the measured magnetic field at V2 from 2018 November, when the spacecraft entered interstellar space.
A Wide Planetary-mass Companion to a Young Low-mass Brown Dwarf in Ophiuchus
Authors: Fontanive Clémence , Allers Katelyn N. , Pantoja Blake , Biller Beth , Dubber Sophie , Zhang Zhoujian , Dupuy Trent , Liu Michael C. , Albert Loïc 
Published: December 2020

Abstract
We present the discovery of a planetary-mass companion to CFHTWIR-Oph 98, a low-mass brown dwarf member of the young Ophiuchus star-forming region, with a wide 200 au separation (1.″46). The companion was identified using Hubble Space Telescope images, and confirmed to share common proper motion with the primary using archival and new ground-based observations. Based on the very low probability of the components being unrelated Ophiuchus members, we conclude that Oph 98 AB forms a binary system. From our multiband photometry, we constrain the primary to be an M9–L1 dwarf, and the faint companion to have an L2–L6 spectral type. For a median age of 3 Myr for Ophiuchus, fits of evolutionary models to measured luminosities yield masses of 15.4 ± 0.8 M
Jup for Oph 98 A and 7.8 ± 0.8 M
Jup for Oph 98 B, with respective effective temperatures of 2320 ± 40 K and 1800 ± 40 K. For possible system ages of 1–7 Myr, masses could range from 9.6–18.4 M
Jup for the primary, and from 4.1–11.6 M
Jup for the secondary. The low component masses and very large separation make this binary the lowest binding energy system imaged to date, indicating that the outcome of low-mass star formation can result in such extreme, weakly bound systems. With such a young age, Oph 98 AB extends the growing population of young free-floating planetary-mass objects, offering a new benchmark to refine formation theories at the lowest masses.
The Optical Luminosity–Time Correlation for More than 100 Gamma-Ray Burst Afterglows
Authors: Dainotti M. G. , Livermore S. , Kann D. A. , Li L. , Oates S. , Yi S. , Zhang B. , Gendre B. , Cenko B. , Fraija N. 
Published: December 2020

Abstract
Gamma-ray bursts (GRBs) are fascinating events due to their panchromatic nature. Their afterglow emission is observed from sub-TeV energies to radio wavelengths. We investigate GRBs that present an optical plateau, leveraging on the resemblance with the X-ray plateau shown in many GRB light curves (LCs). We comprehensively analyze all published GRBs with known redshifts and optical plateau observed mostly by the Neil Gehrels Swift Observatory (Swift). We fit 267 optical LCs and show the existence of the plateau in 102 cases, which is the largest compilation so far of optical plateaus. For 56 Swift GRBs with optical and X-ray plateaus, we compare the rest-frame end time at both wavelengths (

,

), and conclude that the plateau is achromatic between

and

. We also confirm the existence of the two-dimensional relations between

and the optical luminosity at the end of the plateau emission, which resembles the same luminosity–time correlation in X-rays (Dainotti et al. 2013). The existence of this optical correlation has been demonstrated for the largest sample of optical plateaus in the literature to date. The squared scatter in this optical correlation is smallest for the subset of the Gold GRBs with a decrease in the scatter equivalent to 52.4% when compared to the scatter of the entire GRB sample.
First Ultraviolet Outburst Detected from ASASSN-18eh Strengthens Its Interpretation as a Cataclysmic Variable
Authors: Verberne Sill , Modiano David , Wijnands Rudy ,   on behalf of the TUVO project
Published: December 2020

Abstract
As part of the Transient UV Objects project, we have discovered a new outburst (at the beginning of 2020 October) of the candidate cataclysmic variable (CV) ASASSN-18eh using the UV/Optical Telescope aboard the Neil Gehrels Swift Observatory. During the outburst its brightness increased by about 6 mag in UV compared to its brightness in the quiescent state. The properties of this outburst are consistent with it being a dwarf nova, strongly supporting the CV nature of ASASSN-18eh.
Evidence for Twice-ionized Praseodymium and Neodymium in the Upper Atmosphere of HD 99803 A
Authors: Monier Richard , Niemczura Ewa , Kılıçoğlu Tolgahan 
Published: December 2020

Abstract
Evidence is presented in this Note for the presence of twice ionized praseodymium and neodymium in the upper atmosphere of HD 99803 A, which turns out to be a newly discovered cool HgMn star in a binary system.
Detection of a Planet in 2M1938+4603 Revisited
Authors: Baran Andrzej S. , Silvotti Roberto 
Published: December 2020

Abstract
The Observed-minus-Calculated diagram shows a stability of a period being analyzed. In case of binary system, any nonlinear O − C variation indicates an orbital period variation that can be caused by e.g., mass loss or mass transfer between components (physical change), additional component(s) to the system (apparent change only). Baran et al. reported a sinusoidal variation of the O − C of 2M 1938+4603 and interpreted it as a circumbinary planet. We analyzed the newest and most reliable release of the Kepler data of 2M 1938+4603 and by using our newest approach we removed two main sources that could cause the variation not to be intrinsic to 2M 1938+4603. We removed significant signal not associated with binarity and folded eclipses to increase their cadences. Consequently, we lowered rms of the O − C diagram by a factor of six confirming the sinusoidal variation reported by Baran et al. and making it even more convincing now.
K2 Targets Observed in TESS Cycles 1–3
Authors: Dotson Jessie L. , Colón Knicole D. , Barentsen Geert , Hedges Christina , Barclay Thomas 
Published: December 2020

Abstract
Kepler, K2, and Transiting Exoplanet Survey Satellite (TESS) have demonstrated the power of high-precision uninterrupted photometry. Combining data sets from these two observatories can extend the baseline of high precision photometry on a target. In addition, for some investigations, the differing passbands of the two telescopes may provide additional information about the causes of the observed variability. In order to facilitate studies combining these unique data sets, we present a list of all the 55,641 targets observed by K2 which fell within the TESS field of view during its first three years of observations.
List of the Close Asteroid Pairs Strongly Perturbed by Three-body Resonances
Authors: Rosaev Alexey , Plavalova Eva , Galiazzo Mattia 
Published: December 2020

Abstract
The two and three body mean motion resonances with Jupiter and Mars (and possible with Earth) may have a significant effect on the dynamics of very young close asteroid pairs and families. The best known example is the influence 9:16 resonance with Mars to some members of Datura family. It is evident, that the evolution of this family can be properly reconstructed only when this fact has been taken into account. One of the results of resonance perturbation may be the temporary compensation of the Yarkovsky drift in the semimajor axis. Studying this relationship may greatly improve the age estimation of asteroid pairs and families. In this note we give a list of some close asteroid pairs in the vicinity of mean motion resonances.
Kalman Filtering for Tip-tilt Correction in Adaptive Optics
Authors: Sengupta Aditya Rohan , Jensen-Clem Rebecca 
Published: December 2020

Abstract
Correcting the tip and tilt modes of optical aberrations can mitigate a large proportion of distortions in adaptive optics (AO) systems. We describe a method to greatly improve tip/tilt correction for the Keck telescopes, using a Kalman filter with a physics model conditioned by the expected tip/tilt power spectrum and vibration peaks. The model builds on similar implementations, such as that of the Gemini Planet Imager, by considering the effects of loop delays, the response of the control hardware, and systematics specific to Keck. We demonstrate improved correction in simulation, and discuss how this model could be tuned to a specific telescope and otherwise improved.
Estado y educación en Argentina
Authors: Canavese Mariana 
Published: December 2020

Dentro de la recepción de las propuestas del filósofo francés Michel Foucault en la historia argentina reciente, un conjunto de lecturas e intervenciones se produce en espacios vinculados con la educación y la pedagogía. En la Argentina de la década de 1990, las elaboraciones del filósofo constituyen una referencia significativa en la agenda educativa: operan respecto de la problemática del poder, la autoridad y el control en el aula, en análisis de las experiencias educativas y en relación con el pensamiento pedagógico en general. En este artículo se reconstruyen y analizan algunas lecturas y apropiaciones de la ‘caja de herramientas’ foucaultiana relacionadas con el área educativa y destinadas a pensar la reforma cristalizada con la sanción de la Ley Federal de Educación en 1993.
Identidade e Consumo na Meia-idade: Uma Perspectiva Teórica
Authors: Borges Juliana Vieira , Campos Alyce Cardoso , Cappelle Mônica Carvalho Alves , Rezende Daniel Carvalho de 
Published: December 2020

O período da meia-idade parece particularmente importante, uma vez que as mudanças na vida são evidenciadas, podendo ser marcado por um período de ‘crise’ onde prioridades são alteradas e existe um processo de reavaliação de fatores presentes no cotidiano. Grande parte destas mudanças estão relacionadas ao processo identitário do indivíduo, em que o consumo tem forte contribuição. Entretanto, durante um processo de ‘crise’, o consumo poderia representar um elemento de reconfiguração identitária? Para discutir a temática realizou-se um estudo teórico sobre meia-idade e a crise, o processo de consumo e extensão do self, e a identidade na meia-idade. Neste período, é possível identificar alterações significativas de papeis, ambiguidades, contradições e outras instabilidades de vida. A crise da meia-idade se configura diferenciadamente para homens e mulheres, e estão presentes conflitos em relação ao ego e aceitação em relação ao início do envelhecimento. A reconfiguração do self a partir do consumo se apresentou direcionada pelo consumo conspícuo, de estética, lazer e educação. A ressignificação da identidade e o processo de consumo inerente podem contribuir para que a passagem pela crise da meia-idade não seja um período estranho e de sofrimento, mas vivenciada como um momento de crescimento pessoal.
1o Censo Brasileiro dos Pesquisadores Acadêmicos de Marketing
Authors: Brei Vinícius Andrade , Mazzon José Afonso , Farias Salomão Alencar de , Matos Celso Augusto de 
Published: December 2020

Neste artigo analisamos os resultados do 1oCenso Brasileiro dos Pesquisadores Acadêmicos de Marketing, realizado pelo Comitê Científico de Marketing da ANPAD (2015-2017). A pesquisa teve os seguintes objetivos: 1) traçar um diagnóstico e divulgar quem são, onde estão e quais são os interesses/competências temáticos e metodológicos dos pesquisadores de marketing que atuam no Brasil; 2) identificar a criação/consolidação de projetos e de grupos/redes de pesquisa interinstitucionais; 3) auxiliar os órgãos de fomento, periódicos científicos, programas de pós-graduação, e organizadoras de congressos científicos, por meio da identificação dos temas e métodos de especialidade/interesse dos pesquisadores; e 4) fortalecer a comunidade científica brasileira de marketing, por meio da divulgação pública dos dados sobre os pesquisadores. Realizamos uma survey online respondida por 294 pesquisadores, de mais de 50 instituições de todo o Brasil. Os resultados mostram que temos uma comunidade científica jovem; com poucos vínculos institucionais acadêmicos; que apresenta baixa frequência de redes de pesquisa interorganizacionais (entre grupos de pesquisa/universidades) e de projetos de pesquisa financiados; grande concentração das pesquisas sobre consumo e comportamento do consumidor; foco metodológico em técnicas mais tradicionais e pouco inovadoras; e baixa inserção internacional.