bluuebunny/crossref_metadata_2025_split huggingface dataset:
WGS characterization of MDR Enterobacterales with different ceftolozane/tazobactam susceptibility profiles during the SUPERIOR surveillance study in Spain
Authors: Hernández-García Marta , García-Fernández Sergio , García-Castillo María , Bou Germán , Cercenado Emilia , Delgado-Valverde Mercedes , Mulet Xavier , Pitart Cristina , Rodríguez-Lozano Jesús , Tormo Nuria , López-Mendoza Diego , Díaz-Regañón Jazmín , Cantón Rafael ,   SUPERIOR study group, Oliver Antonio , Mulet Xavier , Cercenado Emilia , Bou Germán , Fernández M Carmen , Pascual Álvaro , Delgado Mercedes , Gimeno Concepción , Tormo Nuria , Calvo Jorge , Rodríguez-Lozano Jesús , Alonso Ana Ávila , Vila Jordi , Marco Francesc , Pitart Cristina , García del Castillo María , Fernández Sergio García , Hernández-García Marta , Tato Marta , Cantón Rafael 
Published: September 2020

AbstractObjectivesTo analyse by WGS the ceftolozane/tazobactam (C/T) resistance mechanisms in Escherichia coli and Klebsiella spp. isolates recovered from complicated intra-abdominal and urinary tract infections in patients from Spanish ICUs (SUPERIOR surveillance study, 2016–17).MethodsThe clonal relatedness, the resistome and the virulome of 45 E. coli and 43 Klebsiella spp. isolates with different C/T susceptibility profiles were characterized.ResultsIn E. coli, two (C/T susceptible) carbapenemase producers (VIM-2-CC23, OXA-48-ST38) were detected. The most relevant clone was ST131-B2-O25:H4-H30 (17/45), particularly the CTX-M-15-ST131-H30-Rx sublineage (15/17). ST131 strains were mainly C/T susceptible (15/17) and showed an extensive virulome. In non-ST131 strains (28/45), CTX-M enzymes [CTX-M-14 (8/24); CTX-M-15 (6/24); CTX-M-1 (3/24); CTX-M-32 (2/24)] were found in different clones. C/T resistance was detected in non-clonal E. coli isolates (13%, 6/45) with ESBL (4/6) and non-ESBL (2/6) genotypes. Among Klebsiella spp., Klebsiella pneumoniae (42/43) and Klebsiella michiganensis (1/43) species were identified; 42% (18/43) were carbapenemase producers and 58% showed a C/T resistance phenotype (25/43). OXA-48-ST11 (12/18), OXA-48-ST392 (2/18), OXA-48-ST15 (2/18), NDM-1-ST101 (1/18) and OXA-48+VIM-2-ST15 (1/18) isolates were found, all C/T resistant. Correlation between carbapenemase detection and resistance to C/T was demonstrated (P &lt; 0.001). In non-carbapenemase-producing K. pneumoniae (25/43), C/T resistance (28%, 7/25) was detected in ESBL (3/7) and AmpC (2/7) producers. Overall, an extensive virulome was found and was correlated with carbapenemase carriage (P &lt; 0.001) and C/T resistance (P &lt; 0.05), particularly in OXA-48-ST11 strains (P &lt; 0.05).ConclusionsPrediction of antimicrobial susceptibility profiles using WGS is challenging. Carbapenemase-encoding genes are associated with C/T resistance in K. pneumoniae, but other resistance mechanisms might be additionally involved.
Modelling the effects of post-heading heat stress on biomass partitioning, and grain number and weight of wheat
Authors: Liu Bing , Liu Leilei , Asseng Senthold , Zhang Dongzheng , Ma Wei , Tang Liang , Cao Weixing , Zhu Yan 
Published: September 2020

AbstractGrain yield of wheat and its components are very sensitive to heat stress at the critical growth stages of anthesis and grain filling. We observed negative impacts of heat stress on biomass partitioning and grain growth in environment-controlled phytotron experiments over 4 years, and we quantified relationships between the stress and grain number and potential grain weight at anthesis and during grain filling using process-based heat stress routines. These relationships included reduced grain set under stress at anthesis and decreased potential grain weight under stress during early grain filling. Biomass partitioning to stems and spikes was modified under heat stress based on a source–sink relationship. The integration of our process-based stress routines into the original WheatGrow model significantly enhanced the predictions of the biomass dynamics of the stems and spikes, the grain yield, and the yield components under heat stress. Compared to the original model, the improved version decreased the simulation errors for grain yield, grain number, and grain weight by 73%, 48%, and 49%, respectively, in an evaluation using independent data under heat stress in the phytotron conditions. When tested with data obtained under field conditions, the improved model showed a good ability to reproduce the decreasing dynamics of grain yield and its components with increasing post-anthesis temperatures. Sensitivity analysis showed that the improved model was able to reproduce the responses to various observed heat-stress treatments. These improvements to the crop model will be of significant importance for assessing the effects on crop production of projected increases in heat-stress events under future climate scenarios.
A Note on the Curious Case of John Bale in Spain
Authors: Dominguez Freddy C 
Published: September 2020

Abstract
A slender folder at the Archivo Histórico Nacional in Madrid contains parts of a story about how John Bale’s Illustrium majoris Britanniae scriptorum … summarium (1548) ended up in sixteenth century Spain. Inquisition documents from 1583 reveal how the book got to Toledo from Lyon and how the Holy Office came to know about it. By briefly telling this story, this short note hopes to pique interest in the documents and to suggest ways in which the archives in which they reside can support further research on censorship and the early-modern book trade.
Intensive disc-reverberation mapping of Fairall 9: first year of Swift and LCO monitoring
Authors: Hernández Santisteban J V , Edelson R , Horne K , Gelbord J M , Barth A J , Cackett E M , Goad M R , Netzer H , Starkey D , Uttley P , Brandt W N , Korista K , Lohfink A M , Onken C A , Page K L , Siegel M , Vestergaard M , Bisogni S , Breeveld A A , Cenko S B , Dalla Bontà E , Evans P A , Ferland G , Gonzalez-Buitrago D H , Grupe D , Joner M D , Kriss G , LaPorte S J , Mathur S , Marshall F , Mehdipour M , Mudd D , Peterson B M , Schmidt T , Vaughan S , Valenti S 
Published: September 2020

ABSTRACT
We present results of time-series analysis of the first year of the Fairall 9 intensive disc-reverberation campaign. We used Swift and the Las Cumbres Observatory global telescope network to continuously monitor Fairall 9 from X-rays to near-infrared at a daily to subdaily cadence. The cross-correlation function between bands provides evidence for a lag spectrum consistent with the τ ∝ λ4/3 scaling expected for an optically thick, geometrically thin blackbody accretion disc. Decomposing the flux into constant and variable components, the variable component’s spectral energy distribution is slightly steeper than the standard accretion disc prediction. We find evidence at the Balmer edge in both the lag and flux spectra for an additional bound-free continuum contribution that may arise from reprocessing in the broad-line region. The inferred driving light curve suggests two distinct components, a rapidly variable (&lt;4 d) component arising from X-ray reprocessing, and a more slowly varying (&gt;100 d) component with an opposite lag to the reverberation signal.
The ULX source X-3 in NGC 4258: a search for its X-ray and optical properties
Authors: Akyuz A , Avdan S , Allak S , Aksaker N , Akkaya Oralhan I , Balman S 
Published: September 2020

ABSTRACT
We present the results of a search for the nature of ultraluminous X-ray source (ULX) X-3 in the nearby galaxy NGC 4258. We use archival data from XMM–Newton, Chandra, NuSTAR, and Hubble Space Telescope (HST) observations. Total X-ray data were analysed to find that the model parameters of the system are indicative of a stellar-mass black hole, ∼10 M⊙, as the central compact object. Furthermore, analyses of the optical data from HST reveal two optical candidates at 90 per cent confidence level within an error radius of 0.28 arcsec. Assuming the optical emission is dominated by the donor star, both of these candidates are found to have spectral types that lie between B3 and F1 with absolute magnitudes of MV ≈ −6.4. Moreover, the age and mass estimates for the candidates are found to be 10 and 18 Myr and 13 and 20 M⊙, respectively.
An outflow powers the optical rise of the nearby, fast-evolving tidal disruption event AT2019qiz
Authors: Nicholl M , Wevers T , Oates S R , Alexander K D , Leloudas G , Onori F , Jerkstrand A , Gomez S , Campana S , Arcavi I , Charalampopoulos P , Gromadzki M , Ihanec N , Jonker P G , Lawrence A , Mandel I , Schulze S , Short P , Burke J , McCully C , Hiramatsu D , Howell D A , Pellegrino C , Abbot H , Anderson J P , Berger E , Blanchard P K , Cannizzaro G , Chen T-W , Dennefeld M , Galbany L , González-Gaitán S , Hosseinzadeh G , Inserra C , Irani I , Kuin P , Müller-Bravo T , Pineda J , Ross N P , Roy R , Smartt S J , Smith K W , Tucker B , Wyrzykowski Ł , Young D R 
Published: September 2020

ABSTRACT
At 66 Mpc, AT2019qiz is the closest optical tidal disruption event (TDE) to date, with a luminosity intermediate between the bulk of the population and the faint-and-fast event iPTF16fnl. Its proximity allowed a very early detection and triggering of multiwavelength and spectroscopic follow-up well before maximum light. The velocity dispersion of the host galaxy and fits to the TDE light curve indicate a black hole mass ≈106 M⊙, disrupting a star of ≈1 M⊙. By analysing our comprehensive UV, optical, and X-ray data, we show that the early optical emission is dominated by an outflow, with a luminosity evolution L ∝ t2, consistent with a photosphere expanding at constant velocity (≳2000 km s−1), and a line-forming region producing initially blueshifted H and He ii profiles with v = 3000–10 000 km s−1. The fastest optical ejecta approach the velocity inferred from radio detections (modelled in a forthcoming companion paper from K. D. Alexander et al.), thus the same outflow may be responsible for both the fast optical rise and the radio emission – the first time this connection has been observed in a TDE. The light-curve rise begins 29 ± 2 d before maximum light, peaking when the photosphere reaches the radius where optical photons can escape. The photosphere then undergoes a sudden transition, first cooling at constant radius then contracting at constant temperature. At the same time, the blueshifts disappear from the spectrum and Bowen fluorescence lines (N iii) become prominent, implying a source of far-UV photons, while the X-ray light curve peaks at ≈1041 erg s−1. Assuming that these X-rays are from prompt accretion, the size and mass of the outflow are consistent with the reprocessing layer needed to explain the large optical to X-ray ratio in this and other optical TDEs, possibly favouring accretion-powered over collision-powered outflow models.
Revisiting the local star-forming galaxies observed in the HETDEX Pilot Survey
Authors: Shinn Jong-Ho 
Published: September 2020

ABSTRACT
I have reanalysed the data obtained for local (z &lt; 0.15) star-forming galaxies during the pilot survey for the Hobby–Eberly Telescope Dark Energy Experiment (HETDEX) – called the HETDEX Pilot Survey (HPS) – which uses an integral-field-unit spectrograph and covers ∼3500−5800 Å at ∼5-Å resolution. I have newly determined the gas metallicities, $12 + \text{log (O/H)}$, following the Bayesian analysis scheme of the previous study, but dealing carefully with the uncertainty of strong-line calibration, performing reproducibility tests with mock data, and monitoring the convergence of the Markov chain Monte Carlo (MCMC) sampling. From the mock-data tests, I found that the nebular emission-line colour excess E(B − V) can be overestimated by as much as 2σ or more, although the metallicity can recover the input value to within 1σ. The new metallicity estimates on the HPS data are from well-converged MCMC samples (effective sample sizes &gt; 2000), and they are higher than the previous estimates by ∼2σ. Using the HPS data, I also showed that the MCMC sampling can have the statistical accuracy as poor as the one near the iteration start if done without convergence monitoring. The overestimation of E(B − V) indicates the overestimation of the star formation rates (SFRs) in the previous study, which can be as much as a factor of 5. This finding undermines the previous suggestion of a hitherto-unknown galaxy population based on the locations of galaxies in the mass–SFR plane. I found that the independent determination of E(B − V) using either H β-H γ or H α-H β line pair is ideal for the analysis of forthcoming HETDEX data, but it requires additional cost.
Free to Move
Authors: Somin Ilya 
Published: September 2020

Abstract
Ballot box voting is often considered the essence of political freedom. But it has two major shortcomings: individual voters have only a tiny chance of making a difference, and they also have strong incentives to remain ignorant about the issues at stake. “Voting with your feet” is far superior on both counts. In Free to Move, Ilya Somin explains how expanding foot-voting opportunities can greatly enhance political freedom for millions of people around the world. That applies to foot voting in federal systems, foot voting in the private sector, and especially foot voting through international migration. These three types of foot voting are rarely considered together. But Somin explains how they have major common virtues, and can be mutually reinforcing. Free to Move addresses a variety of objections to expanded migration rights, including claims that the “self-determination” of natives requires giving them power to exclude migrants, and arguments that migration is likely to have harmful side effects, such as undermining political institutions, overburdening the welfare state, increasing crime and terrorism, and spreading undesirable cultural values. While these objections are usually directed at international migration, Somin shows how a consistent commitment to such theories would also justify severe restrictions on internal freedom of movement. That implication is yet another reason to be skeptical of such arguments. The book also shows how both domestic constitutional systems and international law can be structured to increase opportunities for foot voting while mitigating potential downsides of freedom of movement.
Teams Are Not All the Same
Authors: Tannenbaum Scott , Salas Eduardo 
Published: September 2020

Abstract
It would be great if all one needed to know were a few universal truths that apply to any team, but teamwork is not that simple. While teams can differ in countless ways, research shows that a few of the differences are particularly important. This chapter introduces five key ways that teams can differ and why these differences matter. It describes five continua and provides a matrix for assessing a team’s (a) reliance, (b) membership stability, (c) task consistency, (d) proximity, and (e) similarity. Understanding these differences allows you to apply the science of teamwork in a targeted, meaningful way. For example, teams with high reliance must continually coordinate with one another, so they are more influenced by collective efficacy than teams with lower reliance, which are more impacted by self-efficacy.
Communication
Authors: Tannenbaum Scott , Salas Eduardo 
Published: September 2020

Abstract
Communication breakdowns make a team vulnerable, but simply communicating “more” won’t necessarily make a team more effective. Communication quality is far more important than communication quantity. The basics of high-quality communication are to share useful information clearly, accurately, and on time to the right people. Beyond the basics, research has shown it is the sharing of unique information the drives team performance. Other hallmarks of effective communication are the use of closed-loop communication and effective boundary spanning with people outside the team. The chapter identifies the most common obstacles and challenges to effective communication, including biases such as “everybody knows” and highlights situations with the greatest risk of communication breakdowns. Advice is given for fostering better team communications and mitigating common risks.
Team Leaders
Authors: Tannenbaum Scott , Salas Eduardo 
Published: September 2020

Abstract
Leading a team can be challenging, but fundamentally, effective team leadership is about: a) ensuring that your team has all of the drivers it needs (i.e., the right capabilities, cooperation, coordination, communication, cognition, coaching and conditions); and b) enabling them to learn and adapt as needed. This chapter offers ten tangible tips specifically intended for people who are in a designated team leader role. The tips are derived from the science of teamwork.
Issues Faced by Faculty in an Industrial-Organizational Master’s Program
Authors: Sachau Daniel A. , Fritzsche Barbara A. 
Published: September 2020

Abstract
This chapter identifies challenges faculty face when teaching in a terminal industrial-organizational psychology master’s program. The authors discuss how faculty, particularly new/junior faculty, can deal with these issues to become productive in teaching, research, service, consulting, and shaping program culture. The authors offer suggestions for creating a successful program tailored to the needs of different types of students (recent graduates versus experienced students), strategies for maintaining an active research program, and ways to integrate consulting into a master’s program. This chapter includes a discussion of the challenges of offering both a master’s and doctoral program, managing administrators, and building a program culture.
A Field-Theoretic Model of Religious Strength
Authors: Vermurlen Brad 
Published: September 2020

Abstract
Chapter 4 develops a field-theoretic model of religious strength. It starts by revisiting the question of religious strength vis-à-vis the secularization thesis, and then it lays out the five leading theoretical frameworks currently on offer in the sociology of religion for making sense of religious vitality. Next, this chapter critically reviews each of these theories, drawing out the “nugget of truth” in each but finally showing how each is ill-suited, or at least incomplete, for explaining the New Calvinist movement sociologically. What each framework gets right is integrated into a new approach to religious strength based on Fligstein and McAdam’s strategic action field theory. After working through some “nuts and bolts” of this theory, the chapter concludes with a systematization of the theory/model, in which seventeen general social mechanisms are specified as causes that together produced the Reformed resurgence.
Demonstration of the Model, Part I
Authors: Vermurlen Brad 
Published: September 2020

Abstract
Chapter 5 presents Part I of a field-theoretic model of religious strength, focusing on the most powerful social mechanisms and ecological factors that precipitated the rise of the New Calvinist movement. The author describes three aspects of the American cultural backdrop along with three discursive opportunities, which together facilitated the onset of contention in the American Evangelical field. The chapter maps the correspondence between Evangelical leaders’ positions in the field and their corresponding religious dispositions. Additional precipitating factors are identified. The chapter ends by empirically establishing the “rules of the game,” which are the elements of the Bebbington Quadrilateral (i.e., crucicentrism, biblicism, activism, and conversionism), to which is added the more all-encompassing field rule of “the Gospel,” broadly defined. These rules are understood as endogenous to the social system such that the battle over American Evangelicalism is a battle with and over these rules.
The Solace
Authors: Glasgow Joshua 
Published: September 2020

Abstract
While navigating his own mother’s cancer diagnosis, the author explores how we might find solace in the fact that we will die. Traditionally, philosophical answers to this question center on two possibilities. First, some argue that death is not bad for the one who dies, because they won’t exist after once they are dead. Second, others argue that because immortality would be bad, death has considerable upside. Finding these two answers less than satisfying, the author explores a third option. This third source of solace starts with the idea that insofar as our lives are worth being grateful for, they must have a value. This book argues that because life is implicated in all of our good projects and relationships, its value radiates out to all of life’s parts, be they good or bad. And because passing away is one of the parts of life, it gets some of this radiant value. Finally, just as we are grateful for the value of our lives, so we can affirm this value in passing away. Gratitude is not the most fitting way of affirming the value in death, since passing away is also bad for those who die by depriving them of life’s good opportunities. A more fitting affirmation of the value that death borrows from life, when passing away also visits so much badness upon us, is to take some solace in the fact that our passing away has a portion of life’s positive value.
Introduction
Authors: Wilmarth Jr. Arthur E. 
Published: September 2020

Abstract
Universal banks arose in the U.S. during two periods in the past century—the 1920s and the late 1990s. On both occasions, universal banks in the U.S. and Europe promoted intense boom-and-bust cycles that led to global calamities—the Great Depression of the early 1930s and the Great Recession of 2007–09. Universal banks received extensive bailouts on both sides of the Atlantic during both crises. Three core features of universal banks cause them to generate destructive boom-and-bust cycles. First, pervasive conflicts of interest prevent them from acting as objective lenders or as impartial investment advisers. Second, bonus-driven cultures encourage their insiders to take speculative risks to produce short-term profits. Third, their ability to convert loans into asset-backed securities allows them to package risky loans into securities sold as purportedly “safe” investments to poorly informed investors. The Glass-Steagall Act of 1933 broke up universal banks and established structural buffers that prevented spillovers of risk between the banking system and other financial sectors. The U.S. avoided systemic financial crises after World War II until Glass-Steagall was undermined by regulators and ultimately repealed by Congress. Congress failed to adopt similar structural reforms after the Great Recession. As a result, universal banks continue to dominate our financial markets and pose unacceptable systemic dangers. We urgently need a new Glass-Steagall Act to break up universal banks again and restore a more stable and resilient financial system.
‘Inner Necessity’
Authors: Cooper John Michael 
Published: September 2020

Abstract
This chapter argues that Felix Mendelssohn’s Lobgesang represents a profound rethinking of the rhetorical and musical processes of the symphony as a genre. Rather than a unilinear array of symphonic movements whose telos is the coda of its finale, the chapter argues, the Lobgesang is a study in symphonic bitemporality—one in which a central, previously enacted parable-like narrative (Nos. 2–8) is framed by a symphonic introduction (No. 1) and a vocal-symphonic conclusion (Nos. 9–10) whose music and theological import derive from the memory of that central narrative. This view of the Lobgesang as a parable enfolded within a sermon is supported by evidence from the work’s compositional history, texts, and tonal structure.