cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The (im)perfect screenplay: a parody of craft and industry
Creators: name: Batty, Craig
Publisher: name: RMIT University
Year: 2024
Subjects: classificationCode: 360201
subject: Creative writing (incl. scriptwriting)

description: Research background This work sits within the emerging field of screenwriting practice as research and, specifically, the screenplay text as both creative writing and research artefact. Its content draws on the author's 12 years of researching screenwriting to offer a meta- narrative about how craft is deployed on the page for particular story effects. Responding to recent debates about the potential of screenwriting practice as research (Baker 2013, Baker et al 2015), the screenplay performs the research through its form and content. Research contribution A parody of an episode within the soap opera genre, the work draws attention to industry craft techniques/conventions by explicitly performing them. It uses both 'perfect' and 'imperfect' modes of operation, creating a collision of 'good' and 'bad' screenwriting. Examples include: starting scenes as late as possible and 'too early'; drawing attention to backstory but denying its exposition to take place; and, contrasting high drama with no drama at all. Research significance An invited contribution to this special issue, the work adds knowledge to the discipline of screenwriting through its embodiment of research in the form of a screenplay. Significance can be found in how the work composes screenwriting research as well as the author's own reflexivity, in which he reflects on his research career, to use it as the subject of critical inquiry. The author's fourth such work to appear in an academic journal, it is still one of only a handful of published 'academic screenplays' internationally. Works cited Baker, D 2013 'Scriptwriting as creative writing research: a preface', TEXT, special issue 19, at http://www.textjournal.com.au/speciss/issue19/Baker_preface.pdf (accessed 12 May 2015) (cont.)
Localization and delocalization properties in quasi-periodically driven one-dimensional disordered system
Creators: name: Yamada, Hiroaki S.
name: Ikeda, Kensuke S.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Localization and delocalization of quantum diffusion in time-continuous one-dimensional Anderson model perturbed by the quasi-periodic harmonic oscillations of $M$ colors is investigated systematically, which has been partly reported by the preliminary letter [PRE {\bf 103}, L040202(2021)]. We investigate in detail the localization-delocalization characteristics of the model with respect to three parameters: the disorder strength $W$, the perturbation strength $ε$ and the number of the colors $M$ which plays the similar role of spatial dimension. In particular, attentions are focused on the presence of localization-delocalization transition (LDT) and its critical properties. For $M\geq 3$ the LDT exists and a normal diffusion is recovered above a critical strength $ε$, and the characteristics of diffusion dynamics mimic the diffusion process predicted for the stochastically perturbed Anderson model even though $M$ is not large. These results are compared with the results of time-discrete quantum maps, i.e., Anderson map and the standard map. Further, the features of delocalized dynamics is discussed in comparison with a limit model which has no static disordered part.
description: 16 pages, 22 figures
Learning and Evaluating Graph Neural Network Explanations based on Counterfactual and Factual Reasoning
Creators: name: Tan, Juntao
name: Geng, Shijie
name: Fu, Zuohui
name: Ge, Yingqiang
name: Xu, Shuyuan
name: Li, Yunqi
name: Zhang, Yongfeng
Publisher: name: arXiv
Year: 2022
Subjects: subject: Information Retrieval (cs.IR)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: Structural data well exists in Web applications, such as social networks in social media, citation networks in academic websites, and threads data in online forums. Due to the complex topology, it is difficult to process and make use of the rich information within such data. Graph Neural Networks (GNNs) have shown great advantages on learning representations for structural data. However, the non-transparency of the deep learning models makes it non-trivial to explain and interpret the predictions made by GNNs. Meanwhile, it is also a big challenge to evaluate the GNN explanations, since in many cases, the ground-truth explanations are unavailable. In this paper, we take insights of Counterfactual and Factual (CF^2) reasoning from causal inference theory, to solve both the learning and evaluation problems in explainable GNNs. For generating explanations, we propose a model-agnostic framework by formulating an optimization problem based on both of the two casual perspectives. This distinguishes CF^2 from previous explainable GNNs that only consider one of them. Another contribution of the work is the evaluation of GNN explanations. For quantitatively evaluating the generated explanations without the requirement of ground-truth, we design metrics based on Counterfactual and Factual reasoning to evaluate the necessity and sufficiency of the explanations. Experiments show that no matter ground-truth explanations are available or not, CF^2 generates better explanations than previous state-of-the-art methods on real-world datasets. Moreover, the statistic analysis justifies the correlation between the performance on ground-truth evaluation and our proposed metrics. Source code is available at https://github.com/chrisjtan/gnn_cff.
description: Published at the Web Conference 2022 (WWW 2022)
Scolomus clypeatus Araujo & Santos 2018
Creators: name: Araujo, Rodrigo O.
name: Fernandes, Daniell R. R.
name: Pos, Davide Dal
name: Giovanni, Filippo Di
name: Moreira-Muñoz, Andrés
name: Pádua, Diego G.
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Ichneumonidae
Scolomus
Scolomus clypeatus

description: 14.3.1 Scolomus clypeatus Araujo & Santos, 2018 *
Distribution. Chile: Región de La Araucanía (Araujo et al. 2018).
description: Published as part of Araujo, Rodrigo O., Fernandes, Daniell R. R., Pos, Davide Dal, Giovanni, Filippo Di, Moreira-Muñoz, Andrés & Pádua, Diego G., 2025, Unveiling the secrets of South American Darwin wasps, part I: a comprehensive checklist of the Chilean Ichneumonidae (Hymenoptera: Ichneumonoidea), pp. 1-51 in Zootaxa 5631 (1) on page 31, DOI: 10.11646/zootaxa.5631.1.1, http://zenodo.org/record/15326657
Accuracy of Computer-Aided Detection of Occupational Lung Disease: Silicosis and Pulmonary Tuberculosis in Ex-Miners from the South African Gold Mines
Creators: name: Ehrlich, Rodney
name: Barker, Stephen
name: Te Water Naude, Jim
name: Rees, David
name: Kistnasamy, Barry
name: Naidoo, Julian
name: Yassi, Annalee
Publisher: name: Multidisciplinary Digital Publishing Institute
Year: 2024

description: Background: Computer-aided detection (CAD) of pulmonary tuberculosis (TB) and silicosis among ex-miners from the South African gold mines has the potential to ease the backlog of lung examinations in clinical screening and medical adjudication for miners’ compensation. This study aimed to determine whether CAD systems developed to date primarily for TB were able to identify TB (without distinction between prior and active disease) and silicosis (or “other abnormality”) in this population. Methods: A total of 501 chest X-rays (CXRs) from a screening programme were submitted to two commercial CAD systems for detection of “any abnormality”, TB (any) and silicosis. The outcomes were tested against the readings of occupational medicine specialists with experience in reading miners’ CXRs. Accuracy of CAD against the readers was calculated as the area under the curve (AUC) of the receiver operating characteristic (ROC) curve. Sensitivity and specificity were derived using a threshold requiring at least 90% sensitivity. Results: One system was able to detect silicosis and/or TB with high AUCs (>0.85) against both readers, and specificity > 70% in most of the comparisons. The other system was able to detect “any abnormality” and TB with high AUCs, but with specificity < 70%. Conclusion: CAD systems have the potential to come close to expert readers in the identification of TB and silicosis in this population. The findings underscore the need for CAD systems to be developed and validated in specific use-case settings.
Batesiana CHALUMEAU 1983
Creators: name: Skelley, Paul E.
name: Vaz-de-Mello, Fernando Z.
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Scarabaeidae
Batesiana

description: Batesiana Chalumeau, 1983
 Batesiana Chalumeau 1983: 143–144. Stebnicka 2009: 22.
 Type Species. Euparia tuberculata Bates, 1887 (by original designation).
 Diagnosis. Eupariini, body elongate-oval, robust. Head medially gibbous; ventral clypeal and prothoracic indentations form cavity to hold appendages and prothoracic legs when retracted. Pronotum strongly transverse; lateral margin short, straight, crenate; broadly explanate laterally, lacking fringe of setae; posterior margin lacking marginal line. Elytral humeral angle distinctly dentate, not prolonged anteriorly; intervals irregularly tuberculate laterally, some with minute orifices. Protibia with small teeth in apical quarter. Tarsomeres with dense ventral pads of setae in addition to those on margin. Apical meso- and metatibial spurs short, reduced.
 Distribution. Central America and northern South America.
 Remarks. Batesiana, Odontolytes Kozhantshikov, 1916, and Napoa Stebnicka, 1999 form a group of genera readily distinguished from all other New World Eupariini by the basal meso- and metatarsomeres being broadened and distinctly longer than the associated spurs. In addition, the ventral surfaces of these tarsomeres are usually covered with a dense pad of setae (other genera have a marginal fringe of setae only). Batesiana is distinguished from Odontolytes by the tuberculate elytra and from Napoa by the widely explanate lateral pronotal margin.
 The genus Odontolytes has 19 described species and several undescribed species that are morphologically diverse (Stebnicka 2009; P. Skelley, personal observation). Some of these species show intermediate character states among some members of Odontolytes, Batesiana, and Napoa. The genera Batesiana and Napoa have a few autapomorphies, most notably the tuberculate elytra that distinguish them from Odontolytes. The validity of these generic limits, along with the potential paraphyly of these genera, needs to be reviewed.However, generic level analysis of this complex is not the purpose of this paper.For now, we maintain the current generic limits.
description: Published as part of Skelley, Paul E. & Vaz-de-Mello, Fernando Z., 2022, A Second Species of Batesiana Chalumeau, 1983 (Coleoptera: Scarabaeidae: Aphodiinae: Eupariini), pp. 612-618 in The Coleopterists Bulletin 76 (4) on page 613, DOI: 10.1649/0010-065X-76.4.612, http://zenodo.org/record/13252933
Evaluation der Praxis der Strategischen Umweltprüfung in Deutschland und Entwicklung von Vorschlägen zur Optimierung des Vollzugs und des Rechtsrahmens
Creators: name: Führ, Martin
name: Schreider, Claudia
name: Meub, Lukas
Publisher: name: Umweltbundesamt
Year: 2023
Subjects: subject: Strategische Umweltprüfung
subject: UVP-Gesetz
subject: Gesetzesfolgenabschätzung
subject: Bauleitplanung
subject: Fachplanung
subject: Gesetz über die Umweltverträglichkeitsprüfung
subject: Nachhaltigkeit | Strategien | Internationales

description: Die Studie dient der wissenschaftlichen Evaluation der Praxis der Strategischen Umweltprüfung (SUP) in Deutschland. Maßstab der Evaluation sind die gesetzlichen Vorgaben des Gesetzes über die Umweltverträglichkeitsprüfung und weiterer Fachgesetze zur SUP. Neben der Untersuchung der positiven Wirksamkeit der SUP als gesetzliches Instrument der Umweltvorsorge wurden insbesondere auch Defizite ermittelt und Gestaltungsoptionen für einen effizienten und effektiven Vollzug aufgezeigt. Zur weiteren Optimierung der SUP-Praxis kommen administrativ-organisatorische Maßnahmen in Betracht, die im Bericht vorgestellt werden. Zudem werden punktuelle Änderungen auf gesetzlicher Ebene vorgeschlagen. Die Studie basiert auf der Untersuchung von 143 Fallstudien Strategischer Umweltprüfungen der Jahre 2005 bis 2018. Die Fallstudien aus den Bereichen Raumordnungsplanung, Bauleitplanung und Fachplanung repräsentieren einen breiten Querschnitt der SUP-Praxis in Deutschland. Quelle: umweltbundesamt.de
description: Die Studie dient der wissenschaftlichen Evaluation der Praxis der Strategischen Umweltprüfung (SUP) in Deutschland. Maßstab der Evaluation sind die gesetzlichen Vorgaben des Gesetzes über die ⁠Umweltverträglichkeitsprüfung⁠ und weiterer Fachgesetze zur SUP. Neben der Untersuchung der positiven Wirksamkeit der SUP als gesetzliches Instrument der Umweltvorsorge wurden insbesondere auch Defizite ermittelt und Gestaltungsoptionen für einen effizienten und effektiven Vollzug aufgezeigt. Zur weiteren Optimierung der SUP-Praxis kommen administrativ-organisatorische Maßnahmen in Betracht, die im Bericht vorgestellt werden. Zudem werden punktuelle Änderungen auf gesetzlicher Ebene vorgeschlagen.Die Studie basiert auf der Untersuchung von 143 Fallstudien Strategischer Umweltprüfungen der Jahre 2005 bis 2018. Die Fallstudien aus den Bereichen Raumordnungsplanung, ⁠Bauleitplanung⁠ und Fachplanung repräsentieren einen breiten Querschnitt der SUP-Praxis in Deutschland.
Precise magnetization measurements down to 500 mK using a miniature 3He cryostat and a closed-cycle 3He gas handling system installed in a SQUID magnetometer without continuous-cooling functionality
Creators: name: Shimamura, Kazutoshi
name: Wajima, Hiroki
name: Makino, Hayato
name: Abe, Satoshi
name: Haga, Yoshinori
name: Sato, Yoshiaki
name: Kawae, Tatsuya
name: Yoshida, Yasuo
Publisher: name: arXiv
Year: 2022
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We have conducted precise magnetization measurements down to 0.5 K with a miniature 3He cryostat and a closed-cycle 3He gas handling system for a commercial superconducting quantum interference device magnetometer [Magnetic Property Measurement System (Quantum Design)]. The gas handling system contains two sorption pumps filled with granular charcoals. We pressurize 3He gas up to ambient pressure for the liquification at 3 K and then pump the vaper for cooling. The lowest sample temperature is ~ 0.5 K and it can persist for 34 hours. We demonstrate the performance of the system by observing the Meissner effect of aluminum below the superconducting transition temperature ~ 1 K. We also measured the magnetization curve of the heavy fermion superconductor CeCoIn5 resulting in successful observation of the lower critical field at 0.5 K.
High-redshift cosmography: Application and comparison with different methods
Creators: name: Hu, J. P.
name: Wang, F. Y.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Cosmography is used in cosmological data processing in order to constrain the kinematics of the universe in a model-independent way. In this paper, we first investigate the effect of the ultraviolet (UV) and X-ray relation of a quasar on cosmological constraints. By fitting the quasar relation and cosmographic parameters simultaneously, we find that the 4$σ$ deviation from the cosmological constant cold dark matter ($Λ$CDM) model disappears. Next, utilizing the Pantheon sample and 31 long gamma-ray bursts (LGRBs), we make a comparison among the different cosmographic expansions ($z$-redshift, $y$-redshift, $E(y)$, $\log(1+z)$, $\log(1+z)+k_{ij}$, and Pad$\rm \acute{e}$ approximations) with the third-order and fourth-order expansions. The expansion order can significantly affect the results, especially for the $y$-redshift method. Through analysis from the same sample, the lower-order expansion is preferable, except the $y$-redshift and $E(y)$ methods. For the $y$-redshift and $E(y)$ methods, despite adopting the same parameterization of $y=z/(1+z)$, the performance of the latter is better than that of the former. Logarithmic polynomials, $\log(1+z)$ and $\log(1+z) + k_{ij}$, perform significantly better than $z$-redshift, $y$-redshift, and $E(y)$ methods, but worse than Pad$\rm \acute{e}$ approximations. Finally, we comprehensively analyze the results obtained from different samples. We find that the Pad$\rm \acute{e}_{(2,1)}$ method is suitable for both low and high redshift cases. The Pad$\rm \acute{e}_{(2,2)}$ method performs well in a high-redshift situation. For the $y$-redshift and $E(y)$ methods, the only constraint on the first two parameters ($q_{0}$ and $j_{0}$) is reliable.
description: 15 pages, 12 figures, accepted for publication in A&A
Scolomus maculatus Araujo & Santos 2018
Creators: name: Araujo, Rodrigo O.
name: Fernandes, Daniell R. R.
name: Pos, Davide Dal
name: Giovanni, Filippo Di
name: Moreira-Muñoz, Andrés
name: Pádua, Diego G.
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Ichneumonidae
Scolomus
Scolomus maculatus

description: 14.3.2 Scolomus maculatus Araujo & Santos, 2018 *
Distribution. Chile: Región del Maule (Araujo et al. 2018, 2025); Región de Los Ríos (Araujo et al. 2018, 2025).
description: Published as part of Araujo, Rodrigo O., Fernandes, Daniell R. R., Pos, Davide Dal, Giovanni, Filippo Di, Moreira-Muñoz, Andrés & Pádua, Diego G., 2025, Unveiling the secrets of South American Darwin wasps, part I: a comprehensive checklist of the Chilean Ichneumonidae (Hymenoptera: Ichneumonoidea), pp. 1-51 in Zootaxa 5631 (1) on page 31, DOI: 10.11646/zootaxa.5631.1.1, http://zenodo.org/record/15326657
Maximal coin-walker entanglement in a ballistic quantum walk
Creators: name: Zhang, Rong
name: Yang, Ran
name: Guo, Jian
name: Sun, Chang-Wei
name: Duan, Jia-Chen
name: Zhou, Heng
name: Xie, Zhenda
name: Xu, Ping
name: Gong, Yan-Xiao
name: Zhu, Shi-Ning
Publisher: name: arXiv
Year: 2022
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We report the position-inhomogeneous quantum walk (IQW) can be utilized to produce the maximal high dimensional entanglement while maintaining the quadratic speedup spread of the wave-function. Our calculations show that the maximal coin-walker entanglement can be generated in any odd steps or asymptotically in even steps, and the nearly maximal entanglement can be obtained in even steps after $2$. We implement the IQW by a stable resource-saving time-bin optical network, in which a polarization Sagnac loop is employed to realize the precisely tunable phase shift. Our approach opens up an efficient way for high-dimensional entanglement engineering as well as promotes investigations on the role of coin-walker interactions in QW based applications.
description: 7 pages, 6 figures, 1 table
Prospects for Distinguishing Supernova Models Using a Future Neutrino Signal
Creators: name: Olsen, Jackson
name: Qian, Yong-Zhong
Publisher: name: arXiv
Year: 2022
Subjects: 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: The next Galactic core-collapse supernova (SN) should yield a large number of observed neutrinos. Using Bayesian techniques, we show that with an SN at a known distance up to 25 kpc, the neutrino events in a water Cherenkov detector similar to Super-Kamiokande (SK) could be used to distinguish between seven one-dimensional neutrino emission models assuming no flavor oscillations or the standard Mikheyev-Smirnov-Wolfenstein effect. Some of these models could still be differentiated with an SN at a known distance of 50 kpc. We also consider just the relative distributions of neutrino energy and arrival time predicted by the models and find that a detector like SK meets the requirement to distinguish between these distributions with an SN at an unknown distance up to $\sim 10$ kpc.
description: 12 pages, 2 figures
Noise 'n' Science
Creators: name: Henschke, Chris
Publisher: name: RMIT University
Year: 2024
Subjects: classificationCode: 360304
subject: Music performance
classificationCode: 360503
subject: Digital and electronic media art
classificationCode: 360599
subject: Screen and digital media not elsewhere classified

description: BACKGROUND Digital-based sonification methods have been used to turn particle physics data into sound and music, such as the LHC sound project at UCL. However, these projects have all translated the data into normalised musical tunings, giving an aesthetically pleasing output. My research sought to sonify the data in a less tuned form that allows for more raw expressive qualities to emerge. The sound is paired with video footage (of the Large Hadron Collider, for example) which I took as part of the research. The video is affected by the sound, and in a live context, this brings together the audio and video media in surprising and unexpected ways, creating unique forms of feedback that is both audiovisual and conceptual. CONTRIBUTION The 'Noise 'n' Science' ciné concert presented work I developed during my 'art@CMS' collaboration at the Compact Muon Solenoid, CERN, Switzerland. The work challenged the audiovisual boundaries of particle physics research at CERN. In collaboration with particle physicist Wolfgang Adam, particle collision data was turned into analogue CV signals that in turn controlled synthesizers live at the cine event. As this data and sound were generated, I improvised with the material, performing audiovisual expression of the LHC: a delicate balance between scientific order and nature, control and chaos SIGNIFICANCE This unique method of data sonification conceptually and energetically expresses the analogue and physical nature of the LHC detectors and particle collision events. In this sense, the data is more 'raw' or 'pure' than sonification projects that arbitrarily map data into aesthetically pleasing musical forms. Cinema Spoutnik is run by a former CERN scientist, who presents film and sound outside or on the border of traditional media, aiming to deepen the relationship between viewer and artists. The event was widely marketed around Geneva and drew an audience of 60 people including scientists, artists, film makers and the public.
Understanding the Associations among Social Vulnerabilities, Indigenous Peoples, and COVID-19 Cases within Canadian Health Regions
Creators: name: Huyser, Kimberly R.
name: Yellow Horse, Aggie J.
name: Collins, Katherine A.
name: Fischer, Jaimy
name: Jessome, Mary G.
name: Ronayne, Emma T.
name: Lin, Jonathan C.
name: Derkson, Jordan
name: Johnson-Jennings, Michelle
Publisher: name: Multidisciplinary Digital Publishing Institute
Year: 2024

description: Indigenous Peoples are at an increased risk for infectious disease, including COVID-19, due to the historically embedded deleterious social determinants of health. Furthermore, structural limitations in Canadian federal government data contribute to the lack of comparative rates of COVID-19 between Indigenous and non-Indigenous people. To make visible Indigenous Peoples’ experiences in the public health discourse in the midst of COVID-19, this paper aims to answer the following interrelated research questions: (1) What are the associations of key social determinants of health and COVID-19 cases among Canadian health regions? and (2) How do these relationships relate to Indigenous communities? As both proximal and distal social determinants of health conjointly contribute to COVID-19 impacts on Indigenous health, this study used a unique dataset assembled from multiple sources to examine the associations among key social determinants of health characteristics and health with a focus on Indigenous Peoples. We highlight key social vulnerabilities that stem from systemic racism and that place Indigenous populations at increased risk for COVID-19. Many Indigenous health issues are rooted in the historical impacts of colonization, and partially invisible due to systemic federal underfunding in Indigenous communities. The Canadian government must invest in collecting accurate, reliable, and disaggregated data on COVID-19 case counts for Indigenous Peoples, as well as in improving Indigenous community infrastructure and services.
Detecting and Monitoring Tidal Dissipation of Hot Jupiters in the Era of SiTian
Creators: name: Yang, Fan
name: Wang, Wei
name: Wei, Xing
name: Zhang, Hui
name: Zhou, Ji-Lin
name: Shan, Su-Su
name: Zheng, Jie
name: Zong, Wei-Kai
name: Yang, Ming
name: Bai, Yu
name: Wang, Song
name: Zheng, Jia-Chen
name: Xu, Yu-Ru
name: Li, Yu-Feng
name: Lu, You-Jun
name: Liu, Ji-Feng
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Transit Timing Variation (TTV) of hot Jupiters provides direct observational evidence of planet tidal dissipation. Detecting tidal dissipation through TTV needs high precision transit timings and long timing baselines. In this work, we predict and discuss the potential scientific contribution of SiTian Survey in detecting and analyzing exoplanet TTV. We develop a tidal dissipation detection pipeline for SiTian Survey that aims at time-domain astronomy with 72 1-meter optical telescopes. The pipeline includes the modules of light curve deblending, transit timing obtaining, and TTV modeling. SiTian is capable to detect more than 25,000 exoplanets among which we expect $\sim$50 sources showing evidence of tidal dissipation. We present detection and analysis of tidal dissipating targets, based on simulated SiTian light curves of XO-3b and WASP-161b. The transit light curve modeling gives consistent results within 1$σ$ to input values of simulated light curves. Also, the parameter uncertainties predicted by Monte-Carlo Markov Chain are consistent with the distribution obtained from simulating and modeling the light curve 1000 times. The timing precision of SiTian observations is $\sim$ 0.5 minutes with one transit visit. We show that differences between TTV origins, e.g., tidal dissipation, apsidal precession, multiple planets, would be significant, considering the timing precision and baseline. The detection rate of tidal dissipating hot Jupiters would answer a crucial question of whether the planet migrates at an early formation stage or random stages due to perturbations, e.g., planet scattering, secular interaction. SiTian identified targets would be constructive given that the sample would extend tenfold.
description: Accept for publication to RAA
L'insediamento musteriano di Grotta Reali. Rocchetta a Volturno, Molise, Italia
Creators: name: Perfetto, Carlo
Publisher: name: Sezione di Museologia Scientifica e Naturalistica
Year: 2013

description: Sezione di Museologia Scientifica e Naturalistica, Vol 8, N° 2 (2012): Naturalistica
Scolomus magellanicus Walkley 1962
Creators: name: Araujo, Rodrigo O.
name: Fernandes, Daniell R. R.
name: Pos, Davide Dal
name: Giovanni, Filippo Di
name: Moreira-Muñoz, Andrés
name: Pádua, Diego G.
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Ichneumonidae
Scolomus
Scolomus magellanicus

description: 14.3.3 Scolomus magellanicus Walkley, 1962 *
Distribution. Chile: Región de Ñuble (Lanfranco 1974a, b; Araujo et al. 2025); Región de La Araucanía (Lanfranco 1974b); Región de Los Lagos (Lanfranco 1974b; Araujo et al. 2025); Región de Magallanes y de la Antártica Chilena (Walkley 1962; Lanfranco 1974a; Araujo et al. 2025).
description: Published as part of Araujo, Rodrigo O., Fernandes, Daniell R. R., Pos, Davide Dal, Giovanni, Filippo Di, Moreira-Muñoz, Andrés & Pádua, Diego G., 2025, Unveiling the secrets of South American Darwin wasps, part I: a comprehensive checklist of the Chilean Ichneumonidae (Hymenoptera: Ichneumonoidea), pp. 1-51 in Zootaxa 5631 (1) on page 31, DOI: 10.11646/zootaxa.5631.1.1, http://zenodo.org/record/15326657
Optical Field Characterization using Off-axis Digital Holography
Creators: name: van der Heide, Sjoerd
name: van Esch, Bram
name: Hout, Menno van den
name: Bradley, Thomas
name: Velazquez-Benitez, Amado M.
name: Fontaine, Nicolas K.
name: Ryf, Roland
name: Chen, Haoshuo
name: Mazur, Mikael
name: Antonio-López, Jose Enrique
name: Alvarado-Zacarias, Juan Carlos
name: Amezcua-Correa, Rodrigo
name: Okonkwo, Chigo
Publisher: name: arXiv
Year: 2022
Subjects: subject: Optics (physics.optics)
subject: Image and Video Processing (eess.IV)
subject: FOS: Physical sciences
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: Angular resolved digital holography is presented as a technique for real-time characterization of the full optical field (amplitude and phase) of space-division multiplexing components and fibers, here a 6-mode photonic-lantern is characterized.
description: Demo zone paper to be presented at the 2022 Optical Fiber Communication Conference (OFC), March 7, 2022 from 2:00 PM to 4:15 PM PST
7° Convegno Nazionale di Archeozoologia
Creators: name: De Grossi Mazzorin, Jacopo
name: Thun Hohenstein, Ursula
Publisher: name: Sezione di Museologia Scientifica e Naturalistica
Year: 2013

description: Sezione di Museologia Scientifica e Naturalistica, Vol 8, N° 3 (2012): Naturalistica
Survey of Orion Disks with ALMA (SODA) I: Cloud-level demographics of 873 protoplanetary disks
Creators: name: van Terwisga, S. E.
name: Hacar, A.
name: van Dishoeck, E. F.
name: Oonk, R.
name: Zwart, S. Portegies
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: (Abridged) Surveys of protoplanetary disks in nearby star-forming regions (SFRs) have provided important information on their demographics, but due to their sample sizes, they cannot be used to study how disk properties vary with the environment. We conduct a survey of the unresolved millimeter continuum emission of 873 protoplanetary disks identified by Spitzer in the L1641 and L1647 regions of the Orion A cloud. This is the largest such survey yet, allowing us to identify even weak trends in the median disk mass as a function of position in the cloud and cluster membership. The sample detection rates and median masses are also compared to those of nearby (<300 pc) SFRs. The sample was observed with ALMA at 225 GHz, with a median rms of 0.08 mJy/beam (1.5 M$_{\oplus}$). The data were reduced and imaged using an innovative parallel data processing approach. We detect 58% (502/873) of the observed disks. This includes 20 disks with dust masses >100 M$_{\oplus}$, and two objects associated with extended dust emission. We infer a median disk dust mass in the full sample of $2.2^{+0.2}_{-0.2}$ M$_{\oplus}$. In L1641 and L1647 median dust masses are $2.1^{+0.2}_{-0.2}$ M$_{\oplus}$ and $2.6^{+0.4}_{-0.5}$ M$_{\oplus}$, respectively. The disk mass distribution of the full sample is similar to that of nearby low-mass SFRs at similar ages of 1-3 Myr. We find only weak trends in disk (dust) masses with galactic longitude and between the YSO clusters identified in the sample, with median masses varying by $\lesssim$ 50%. Age differences may explain these median disk mass variations. Apart from this, disk masses are essentially constant at scales of ~100 pc. This also suggests that the majority of disks, even in different SFRs, are formed with similar initial masses and evolve at similar rates, assuming no external irradiation, with disk mass loss rates of $\sim 10^{-8}$ M$_{\odot}$/yr.
description: Accepted in A&A. 19 pages, 13 figures, 5 tables in the main text; 5 pages, 1 table and 5 additional figures in appendices
Teknehub per i beni culturali. Un laboratorio della rete alta tecnologia Emilia Romagna a servizio delle imprese
Creators: name: Balzani, Marcello
Publisher: name: Sezione di Museologia Scientifica e Naturalistica
Year: 2013

description: Sezione di Museologia Scientifica e Naturalistica, Vol 8, N° 1 (2012): Naturalistica
Сфиральная эпигенетика: управление траекторией компании через фазовые состояния
Creators: name: Басаргин, Олег Сергеевич
Publisher: name: Zenodo
Year: 2025

description: В статье рассматривается расширенное понимание эпигенетики как уровня управления вложенными паттернами в бизнесе и организациях. Введена концепция фазового мышления на основе модели Сфирали, в которой кризис, выгорание и стратегическая стагнация трактуются как точки фазового перехода, а не сбоя. Предложен метод сфиральной диагностики, позволяющий видеть динамику и траекторию свития организационного поведения. Рассматриваются прикладные кейсы, в которых эпигенетический и фазовый подход дают результат — от индивидуальной трансформации лидеров до ритмики команд и структуры процессов. Работа ориентирована на стратегов, консультантов, бизнес-лидеров и исследователей нелинейных систем управления.
Spontaneous magnetic skyrmions in single-layer CrInX3(X=Te, Se)
Creators: name: Du, Wenhui
name: Dou, Kaiying
name: He, Zhonglin
name: Dai, Ying
name: Huang, Baibiao
name: Ma, Yandong
Publisher: name: arXiv
Year: 2022
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The realization of magnetic skyrmions in nanostructures holds great promise for both fundamental research and device applications. Despite recent progress, intrinsic magnetic skyrmions in two-dimensional lattice are still rarely explored. Here, using first-principles calculations and Monte-Carlo simulations, we report the identification of spontaneous magnetic skyrmions in single-layer CrInX3 (X = Te, Se). Due to the joint effect of broken inversion symmetry and strong spin-orbit coupling, inherent large Dzyaloshinskii-Moriya interaction occurs in both systems, endowing the intriguing Neel-type skyrmions in the absence of magnetic field. By further imposing moderate magnetic field, the skyrmion phase can be obtained and is stable within a wide temperature range. Particularly for single-layer CrInTe3, the size of skyrmions is sub-10 nm and the skyrmion phase can be maintained at an elevated temperature of 180 K. In addition, the phase diagrams of their topological spin textures under the variation of magnetic parameters of D, J, and K are mapped out. Our results greatly enrich the research of 2D skyrmionics physics.
Le ichnocenosi delle successioni sedimentarie Eocenico-Mioceniche affioranti tra il Lago Trasimeno e l'Alpe di Poti (Appennino Settentrionale)
Creators: name: Trecci, Tiziana
name: Monaco, Paolo
Publisher: name: Sezione di Museologia Scientifica e Naturalistica
Year: 2013

description: Sezione di Museologia Scientifica e Naturalistica, Vol 7 (2011)
Power distribution of oscillations in the atmosphere of a plage region: Joint observations with ALMA, IRIS and SDO
Creators: name: Narang, Nancy
name: Chandrashekhar, Kalugodu
name: Jafarzadeh, Shahin
name: Fleck, Bernhard
name: Szydlarski, Mikołaj
name: Wedemeyer, Sven
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present a statistical analysis of power distribution of oscillations in a plage region in active region NOAA AR12651, observed jointly with ALMA (Atacama Large Millimeter/Submillimeter Array), IRIS (Interface Region Imaging Spectrograph), and SDO (Solar Dynamics Observatory). We employ coordinated ALMA Band-6 (1.25 mm) brightness temperature maps, IRIS Slit-Jaw Images in 2796 Å passband, and observations in six passbands (1600 Å, 304 Å, 131 Å, 171 Å, 193 Å and 211 Å) of AIA (Atmospheric Imaging Assembly) onboard SDO. We perform Lomb-Scargle transforms to study the distribution of oscillation power over the observed region by means of dominant period maps and power maps. We study spatial association of oscillations through the atmosphere mapped by the different passbands, with focus on the correlation of power distribution of ALMA oscillations with others. We do not observe any significant association of ALMA oscillations with IRIS and AIA oscillations. While the global behavior of ALMA dominant oscillations shows similarity with that of transition region and coronal passbands of AIA, the ALMA dominant period maps and power maps do not show any correlation with those from the other passbands. The spatial distribution of dominant periods and power in different period intervals of ALMA oscillations is uncorrelated with any other passband. We speculate the non-association of ALMA oscillations with those of IRIS and AIA be due to significant variations in the height of formation of the millimeter continuum observed by ALMA. Additionally, the fact that ALMA directly maps the brightness temperature, in contrast to the intensity observations by IRIS and AIA, can result in the very different intrinsic nature of the ALMA oscillations compared to the IRIS and AIA oscillations.
description: Accepted for publication in A&A; abstract abridged to meet arXiv requirements
Three-dimensional imaging of convective cells in the photosphere of Betelgeuse
Creators: name: Ariste, A. López
name: Georgiev, S.
name: Mathias, Ph.
name: Lèbre, A.
name: Wavasseur, M.
name: Josselin, E.
name: Konstantinova-Antova, R.
name: Roudier, Th.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Understanding convection in red supergiants and the mechanisms that trigger the mass loss from these evolved stars are the general goals of most observations of Betelgeuse and its inner circumstellar environment. Linear spectropolarimetry of the atomic lines of the spectrum of Betelgeuse reveals information about the three-dimensional (3D) distribution of brightness in its atmosphere. We model the distribution of plasma and its velocities and use inversion algorithms to fit the observed linear polarization. We obtain the first 3D images of the photosphere of Betelgeuse. Within the limits of the used approximations, we recover vertical convective flows and measure the velocity of the rising plasma at different heights in the photosphere. In several cases, we find this velocity to be constant with height, indicating the presence of forces other than gravity acting on the plasma and counteracting it. In some cases, these forces are sufficient to maintain plasma rising at 60\,\kms to heights where this velocity is comparable to the escape velocity. Forces are present in the photosphere of Betelgeuse that allow plasma to reach velocities close to the escape velocity. These mechanisms may suffice to trigger mass loss and sustain the observed large stellar winds of these evolved stars.
description: 15 pages, 10 figures. In press with A&A
Scolomus valenzuelai Araujo, Padua & Silva-Santos 2025
Creators: name: Araujo, Rodrigo O.
name: Fernandes, Daniell R. R.
name: Pos, Davide Dal
name: Giovanni, Filippo Di
name: Moreira-Muñoz, Andrés
name: Pádua, Diego G.
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Ichneumonidae
Scolomus
Scolomus valenzuelai

description: 14.3.4 Scolomus valenzuelai Araujo, Pádua & Silva-Santos, 2025
Distribution. Chile: Región del Maule (Araujo et al. 2025).
description: Published as part of Araujo, Rodrigo O., Fernandes, Daniell R. R., Pos, Davide Dal, Giovanni, Filippo Di, Moreira-Muñoz, Andrés & Pádua, Diego G., 2025, Unveiling the secrets of South American Darwin wasps, part I: a comprehensive checklist of the Chilean Ichneumonidae (Hymenoptera: Ichneumonoidea), pp. 1-51 in Zootaxa 5631 (1) on page 31, DOI: 10.11646/zootaxa.5631.1.1, http://zenodo.org/record/15326657
Taphos 2011. 6th International Meeting on Taphonomy and Fossilization
Creators: name: H. Nebelsick, James
name: Friedrich, Jan-Peter
name: Dynowski, Janina
Publisher: name: Sezione di Museologia Scientifica e Naturalistica
Year: 2013

description: Sezione di Museologia Scientifica e Naturalistica, 2011: Volume Speciale
Characterizing elastic turbulence in the three-dimensional von Karman swirling flow using the Oldroyd-B model
Creators: name: van Buel, Reinier
name: Stark, Holger
Publisher: name: arXiv
Year: 2022
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: We present the full three-dimensional numerical investigation of the von Karman swirling flow between two parallel plates using the Oldroyd-B model and characterize the onset and development of elastic turbulence. We quantify the flow state with the secondary-flow strength, a measure of the average strength of the velocity fluctuations, and then define an order parameter as the time average of the secondary-flow strength. The order parameter displays a subcritical transition from the laminar to a bistable flow that switches between weakly chaotic flow and elastic turbulence. The transition to the bistable flow occurs at the critical Weissenberg number $\mathrm{Wi_c}=12$. Above $\mathrm{Wi_c}$, in the elastic turbulent state, we observe a strong increase in velocity fluctuations and flow resistance, which we define as the total work performed on the fluid. Upon starting simulations in the turbulent state and subsequently lowering $\mathrm{Wi}$ below its critical value, we observe hysteretic behavior in the order parameter and the flow resistance, which is a common feature of a subcritical transition. Hysteresis has also been found in experiments. Additionally, we find power-law scaling in the spatial and temporal power spectra of the velocity fluctuations, characteristic for elastic turbulence. The maximum values of the power-law exponents in our simulations are $α_t= 3.41$ for the temporal exponent and $α_s= 3.17$ for the spatial exponent, which are remarkably close to the values obtained in experiments.
Magnetization of Relativistic Current-Carrying Jets with Radial Velocity Shear
Creators: name: Król, Dominika Ł.
name: Stawarz, Łukasz
name: Begelman, Mitchell C.
name: Martí, José-María
name: Perucho, Manel
name: Petrenko, Bohdan A.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Astrophysical jets, launched from the immediate vicinity of accreting black holes, carry away large amounts of power in a form of bulk kinetic energy of jet particles and electromagnetic flux. Here we consider a simple analytical model for relativistic jets at larger distances from their launching sites, assuming a cylindrical axisymmetric geometry with a radial velocity shear, and purely toroidal magnetic field. We argue that, as long as the jet plasma is in magnetohydrostatic equilibrium, such outflows tend to be particle dominated, i.e. the ratio of the electromagnetic to particle energy flux, integrated over the jet cross-sectional area, is typically below unity, $σ< 1$. At the same time, for particular magnetic and radial velocity profiles, magnetic pressure may still dominate over particle pressure for certain ranges of the jet radius, i.e. the local jet plasma parameter $β_{pl} < 1$, and this may be relevant in the context of particle acceleration and production of high-energy emission in such systems. The jet magnetization parameter can be elevated up to the modest values $σ\lesssim \mathcal{O}(10)$ only in the case of extreme gradients or discontinuities in the gaseous pressure, and a significantly suppressed velocity shear. Such configurations, which consist of a narrow, unmagnetized jet spine surrounded by an extended, force-free layer, may require an additional poloidal field component to stabilize them against current-driven oscillations, but even this will not elevate substantially their $σ$ parameter.
description: The Astrophysical Journal, in press
backflow (CIRCULATION #0006)
Creators: name: Douglas, Mick
Publisher: name: RMIT University
Year: 2024
Subjects: classificationCode: 330399
subject: Design not elsewhere classified
classificationCode: 360603
subject: Performance art

description: BACKGROUND: The CIRCULATIONS series of new performance installations were developed for regional cluster events of 'Fluid States: Performances of Unknowing', the Performance Studies international globally distributed 2015 program. Employing salt as material and performative medium, CIRCULATIONS explores the dynamics of local specificities and global connectedness of cultural and ecological systems. Salt is a material in cyclical movement and transformation - through bodies of water, through the bodies of living organisms, through land; a material that elicits awareness of the porosity of entities and raises questions of equilibrium and change. CONTRIBUTION: 'Backflow' (CIRCULATION #6) provides a meditation on the Japanese symbolism of spiritual purification through salt, and the post 2011 tsunami consequences of seawater flooding agricultural lands in northern Japan, causing a shift from traditional rice-growing to rapeseed crops. Fluid States participants from around the world were invited to perform a shared action of depositing one kilo of their 'home' regional salts into the Museum of Art's storm-water drainage system, then 'backflowing' into the Aomori harbour. This work contributes a post-humanist example of a performative creative practice investigation into human-ecological relations. Our attention is directed to the range of human negotiations with natural systems and resources - commonly containing and capitalising - whilst circulations of salt continue to exceed control. SIGNIFICANCE: The work was selected for the international program 'Beyond Contamination', the Japanese cluster event of 'Fluid States'. The CIRCULATIONS series was selected for showing in 2015 in Bahamas, Rarotonga, Tohoku, Melbourne and Manila, and featured in Mick Douglas & Sam Trubridge, 'Concurrent Practices', Performance Research, vol 21: issue 2, 2016, pp96-107.
Mechanical, optical, and thermoelectric properties of semiconducting ZnIn2X4 (X= S, Se, Te) monolayers
Creators: name: Mohebpour, Mohammad Ali
name: Mortazavi, Bohayra
name: Rabczuk, Timon
name: Zhuang, Xiaoying
name: Shapeev, Alexander V.
name: Tagani, Meysam Bagheri
Publisher: name: arXiv
Year: 2022
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Mechanical stability of the ZnIn2X4 monolayers. The ZnIn2S4 and ZnIn2Se4 are semiconductors with direct band gaps of 3.94 and 2.77 eV, respectively whereas the ZnIn2Te4 shows an indirect band gap of 1.84 eV at the G0W0 level. The optical properties achieved from the solution of the Bethe-Salpeter equation predict the exciton binding energy of the ZnIn2S4, ZnIn2Se4, and ZnIn2Te4 monolayers to be 0.51, 0.41, and 0.34 eV, respectively, suggesting the high stability of the excitonic states against thermal dissociation. Using the iterative solutions of the Boltzmann transport equation accelerated by machine learning interatomic potentials, the room-temperature lattice thermal conductivity of the ZnIn2S4, ZnIn2Se4, and ZnIn2Te4 monolayers is predicted to be remarkably low as 5.8, 2.0, and 0.4 W/mK, respectively. Due to the low lattice thermal conductivity, high thermopower, and large figure of merit, we propose the ZnIn2Se4 and ZnIn2Te4 monolayers as promising candidates for thermoelectric energy conversion systems. This study provides an extensive vision concerning the intrinsic physical properties of the ZnIn2X4 nanosheets and highlights their characteristics for energy conversion and optoelectronics applications.
description: 11 pages, 6 figures