cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
RETHINKING THE CRITICAL PARADIGM IN EDUCATION: A TURN TO AFFECTIVE PRAGMATISM
Creators: name: Raye, Shalin Lena
Publisher: name: Purdue University Graduate School
Year: 2023
Subjects: classificationCode: 390102
subject: Curriculum and pedagogy theory and development

description: ABSTRACT This dissertation is a philosophical inquiry into the pragmatics of emotion as an inherent dimension of the learning self (Ellsworth, 2005). This inquiry first establishes the socio-political context regarding emotional responses to critical forms of pedagogy currently rising across the United States. Secondly, this inquiry explores philosophical conceptualizations of emotions as pedagogical within the fields of public pedagogy, affect theory, and arts-based educational research, as well as the paradigmatic contexts underlying these philosophies. Finally, this inquiry “thinks-with” (Jackson & Mezzei, 2017) these conceptualizations by enacting an affective pragmatic inquiry, centering emotions and embodied experiences of learning through my own neurotypicality as pedagogical inquiry via an arts-based empirical component, consisting of my enrollment in a community pottery class over the course of 40 weeks. I advocate for the need to reconsider the current paradigm around critical forms of pedagogy toward a pragmatist paradigm that uses emotions and value systems of learners to facilitate ethical pedagogical response-abilities (Haraway, 2016) for what to do, pragmatically, with complicated knowledge about social problems that result in ideological and axiological impasses.
[Halle (Saale), Universitäts- und Landesbibliothek Sachsen-Anhalt, Morbio 5 (18)]
Creators: name: Imoldina
Publisher: name: Universitäts- und Landesbibliothek Sachsen-Anhalt
Year: 1351
Subjects: subject: Sonstige weltliche Aussteller
subject: Notarsurkunde
subject: Urkunde
subject: 090

description: Imoldina, Tochter des verstorbenen Baxianus Uerrus, aus Casalpusterlengo, nun wohnhaft in Guardamiglio im Bistum Piacenza, verkauft Mafretus Cagamostus, Sohn des verstorbenen Oto, aus Lodi, nun wohnhaft in Casalpusterlengo, Land, gelegen ebendort.
Additional file 3 of The effects of the Green-Mediterranean diet on cardiometabolic health are linked to gut microbiome modifications: a randomized controlled trial
Creators: name: Rinott, Ehud
name: Meir, Anat Yaskolka
name: Tsaban, Gal
name: Zelicha, Hila
name: Kaplan, Alon
name: Knights, Dan
name: Tuohy, Kieran
name: Scholz, Matthias Uwe
name: Koren, Omry
name: Stampfer, Meir J.
name: Wang, Dong D.
name: Shai, Iris
name: Youngster, Ilan
Publisher: name: figshare
Year: 2022
Subjects: subject: Ecology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified

description: Additional file 3: Table S2. Characteristics of the study population.
[Halle (Saale), Universitäts- und Landesbibliothek Sachsen-Anhalt, Morbio 5 (24)]
Creators: name: Uitalis De Consono
Publisher: name: Universitäts- und Landesbibliothek Sachsen-Anhalt
Year: 1352
Subjects: subject: Sonstige weltliche Aussteller
subject: Notarsurkunde
subject: Urkunde
subject: 090

description: Uitalis de Consono, Sohn des verstorbenen Asolinus, aus Consonno, gehörig zur plebs von Garlate, verkauft dem Januarius Farina, Sohn des Martinus Farina de Valdemaria, wohhaft in Tegnone, gehörig zur plebs von Missaglia, ein Stück Land, gelegen auf dem Gebiet von Consonno, um die jährlichen Abgaben an das Kloster von Civate entrichten zu könnnen.
GJ 1252b: A Hot Terrestrial Super-Earth With No Atmosphere
Creators: name: Crossfield, Ian J. M.
name: Malik, Matej
name: Hill, Michelle L.
name: Kane, Stephen R.
name: Foley, Bradford
name: Polanski, Alex S.
name: Coria, David
name: Brande, Jonathan
name: Zhang, Yanzhe
name: Wienke, Katherine
name: Kreidberg, Laura
name: Cowan, Nicolas B.
name: Dragomir, Diana
name: Gorjian, Varoujan
name: Mikal-Evans, Thomas
name: Benneke, Bjoern
name: Christiansen, Jessie L.
name: Deming, Drake
name: Morales, Farisa Y.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The increasing numbers of rocky, terrestrial exoplanets known to orbit nearby stars (especially M dwarfs) has drawn increased attention to the possibility of studying these planets' surface properties, and atmospheric compositions & escape histories. Here we report the detection of the secondary eclipse of the terrestrial exoplanet GJ1252b using the Spitzer Space Telescope's IRAC2 4.5 micron channel. We measure an eclipse depth of 149(+25/-32) ppm, corresponding to a day-side brightness temperature of 1410(+91/-125) K and consistent with the prediction for no atmosphere. Comparing our measurement to atmospheric models indicates that GJ1252b has a surface pressure of <10 bar, substantially less than Venus. Assuming energy-limited escape, even a 100 bar atmosphere would be lost in <1 Myr, far shorter than estimated age of 3.9+/-0.4 Gyr. The expected mass loss could be overcome by mantle outgassing, but only if the mantle's carbon content were >7% by mass - over two orders of magnitude greater than that found in Earth. We therefore conclude that GJ1252b has no significant atmosphere. Model spectra with granitoid or feldspathic surface composition, but with no atmosphere, are disfavored at >2 sigma. The eclipse occurs just +1.4(+2.8/-1.0) min after orbital phase 0.5, indicating e cos omega=+0.0025(+0.0049/-0.0018), consistent with a circular orbit. Tidal heating is therefore likely to be negligible to GJ1252b's global energy budget. Finally, we also analyze additional, unpublished TESS transit photometry of GJ1252b which improves the precision of the transit ephemeris by a factor of ten, provides a more precise planetary radius of 1.180+/-0.078 R_E, and rules out any transit timing variations with amplitudes <1 min.
description: ApJL in press. 16 pages, 12 figures, 10 eclipses, 1 bandpass. Models will be available at journal website
Updated orbital monitoring and dynamical masses for nearby M-dwarf binaries
Creators: name: Calissendorff, Per
name: Janson, Markus
name: Rodet, Laetitia
name: Köhler, Rainer
name: Bonnefoy, Mickaël
name: Brandner, Wolfgang
name: Brown-Sevilla, Samantha
name: Chauvin, Gaël
name: Delorme, Philippe
name: Desidera, Silvano
name: Durkan, Stephen
name: Fontanive, Clemence
name: Gratton, Raffaele
name: Hagelberg, Janis
name: Henning, Thomas
name: Hippler, Stefan
name: Lagrange, Anne-Marie
name: Langlois, Maud
name: Lazzoni, Cecilia
name: Maire, Anne-Lise
name: Messina, Sergio
name: Meyer, Michael
name: Möller-Nilsson, Ole
name: Rabus, Markus
name: Schlieder, Joshua
name: Vigan, Arthur
name: Wahhaj, Zahed
name: Wildi, Francois
name: Zurlo, Alice
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Young M-type binaries are particularly useful for precise isochronal dating by taking advantage of their extended pre-main sequence evolution. Orbital monitoring of these low-mass objects becomes essential in constraining their fundamental properties, as dynamical masses can be extracted from their Keplerian motion. Here, we present the combined efforts of the AstraLux Large Multiplicity Survey, together with a filler sub-programme from the SpHere INfrared Exoplanet (SHINE) project and previously unpublished data from the FastCam lucky imaging camera at the Nordical Optical Telescope (NOT) and the NaCo instrument at the Very Large Telescope (VLT). Building on previous work, we use archival and new astrometric data to constrain orbital parameters for 20 M-type binaries. We identify that eight of the binaries have strong Bayesian probabilities and belong to known young moving groups (YMGs). We provide a first attempt at constraining orbital parameters for 14 of the binaries in our sample, with the remaining six having previously fitted orbits for which we provide additional astrometric data and updated Gaia parallaxes. The substantial orbital information built up here for four of the binaries allows for direct comparison between individual dynamical masses and theoretical masses from stellar evolutionary model isochrones, with an additional three binary systems with tentative individual dynamical mass estimates likely to be improved in the near future. We attained an overall agreement between the dynamical masses and the theoretical masses from the isochrones based on the assumed YMG age of the respective binary pair. The two systems with the best orbital constrains for which we obtained individual dynamical masses, J0728 and J2317, display higher dynamical masses than predicted by evolutionary models.
description: Accepted for publication in A&A. 38 pages, 29 figures, 11 tables
Building family
Creators: name: Searles, Darcey
Publisher: name: No Publisher Supplied
Year: 2018

description: This dissertation employs the methods of Conversation Analysis to examine a collection of more than 30 hours of naturally-occurring video-recordings of families with young children. In building upon prior research regarding family communication and conversation analysis, this dissertation furthers our understanding of three communication practices that are recurrent in everyday family life: recruiting, updating, and monitoring object identification. First, I analyze the activity of recruiting, finding that wanna-format recruiting is more versatile than let’s-format recuiting. Let’s-format recruiting occurs only when the interactants are already engaged in an activity together, whereas wanna-format recruiting can occur then and when the interactants are not engaged together in an activity. Second, I examine how updating comes about in family interactions. I show how children produce updates in ways that are locally occasioned and how parents solicit updates from their children. If a child indicates some difficulty in responding to a solicited update, parents can work to scaffold subsequent update solicitations. Third, I examine how apposite object identification becomes relevant in family interactions. I examine parent and child monitoring of apposite object identification in reference to objects/items. Findings indicate that there is an ongoing monitoring of object identification in these family interactions, and that both parents and young children exploit this pervasive monitoring of apposite object identification to accomplish other actions. Overall, this dissertation has broader implications for our understanding of family communication, children’s interactional sophistication, and conversation analytic research. Future work could build on the findings presented in this dissertation in examining young children’s exploitation of ongoing courses of action, as well as work to provide practical implications for families with young children.
A Domain Generalization Approach for Out-Of-Distribution 12-lead ECG Classification with Convolutional Neural Networks
Creators: name: Ballas, Aristotelis
name: Diou, Christos
Publisher: name: arXiv
Year: 2022
Subjects: subject: Machine Learning (cs.LG)
subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences

description: Deep Learning systems have achieved great success in the past few years, even surpassing human intelligence in several cases. As of late, they have also established themselves in the biomedical and healthcare domains, where they have shown a lot of promise, but have not yet achieved widespread adoption. This is in part due to the fact that most methods fail to maintain their performance when they are called to make decisions on data that originate from a different distribution than the one they were trained on, namely Out-Of-Distribution (OOD) data. For example, in the case of biosignal classification, models often fail to generalize well on datasets from different hospitals, due to the distribution discrepancy amongst different sources of data. Our goal is to demonstrate the Domain Generalization problem present between distinct hospital databases and propose a method that classifies abnormalities on 12-lead Electrocardiograms (ECGs), by leveraging information extracted across the architecture of a Deep Neural Network, and capturing the underlying structure of the signal. To this end, we adopt a ResNet-18 as the backbone model and extract features from several intermediate convolutional layers of the network. To evaluate our method, we adopt publicly available ECG datasets from four sources and handle them as separate domains. To simulate the distributional shift present in real-world settings, we train our model on a subset of the domains and leave-out the remaining ones. We then evaluate our model both on the data present at training time (intra-distribution) and the held-out data (out-of-distribution), achieving promising results and surpassing the baseline of a vanilla Residual Network in most of the cases.
description: This paper has been accepted at: IEEE BigDataService2022 (http://big-dataservice.net/)
Exploratory Study of Deep Brain Stimulation in the Syngap1+/-Mouse Model of Autism Spectrum Disorder using Electrophysiology
Creators: name: Abdullah, Umm E Hani
Publisher: name: Purdue University Graduate School
Year: 2023
Subjects: Computational neuroscience (incl. mathematical neuroscience and theoretical neuroscience)
Neurology and neuromuscular diseases
Psychiatry (incl. psychotherapy)
Neural engineering

description: Syngap1+/ -haploinsufficiency is phenotypically characterized by autism spectrum disorder (ASD), intellectual disability (ID), and epilepsy. SynGAP(Synaptic Ras GTPase-activating protein) is a protein that regulates function in synapses. In addition, SynGAP protein is an integral component of the post-synaptic density and its role in signaling pathway converges with other autism risk genes and consequently autism risk proteins. A critical gap exists to understand how electrical stimulation as part of the Hebbian theory, can induce neuroplasticity. Previously, success in alleviating self-injurious behavior along with facilitating speech formation was demonstrated in adolescent patients undergoing deep brain stimulation (DBS) of the basolateral amygdala (BLA). Therefore, we sought to develop a chronic DBS model in Syngap1+/- haploinsufficient mice that can be used to assess the behavior and proteomic correlates due to DBS in BLA.
[Halle (Saale), Universitäts- und Landesbibliothek Sachsen-Anhalt, Morbio 5 (25)]
Creators: name: Anselmus Summo
Publisher: name: Universitäts- und Landesbibliothek Sachsen-Anhalt
Year: 1352
Subjects: subject: Sonstige weltliche Aussteller
subject: Notarsurkunde
subject: Urkunde
subject: 090

description: Anselmus Summo, [Sohn des verstorbenen Johannes de Summo, aus der Nachbarschaft St. Johannis novi sive St. Ellene in Cremona und] Vormund der Santina und der Bertolina, Töchter des verstorbenen Nicola de Camnibus, versichert vor dem Richter, dass er das Recht zum Erbantritt habe und ein Inventar der Güter anfertigen wolle.
Enhanced magnetoresistance in perpendicular magnetic tunneling junctions with MgAl2O4 barrier
Creators: name: Khanal, Pravin
name: Zhou, Bowei
name: Andrade, Magda
name: Mastrangelo, Christopher
name: Habiboglu, Ali
name: Enriquez, Arthur
name: Fox, Daulton
name: Warrilow, Kennedy
name: Wang, Wei-Gang
Publisher: name: arXiv
Year: 2022
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Perpendicular magnetic tunnel junction with MgAl2O4 barrier is investigated. It is found that reactive RF sputtering with O2 is essential to obtain strong perpendicular magnetic anisotropy and large tunneling magnetoresistance in MgAl2O4-based junctions. An interfacial perpendicular magnetic anisotropy energy density of 2.25 mJ/m2 is obtained for the samples annealed at 400C. An enhanced magnetoresistance of 60% has also been achieved. The Vhalf, bias voltage at which tunneling magnetoresistance drops to half of the zero-bias value, is found to be about 1V, which is substantially higher than that of MgO-based junctions.
Sonnenfleckenzeichnung Nr. 239.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 08.10.1996, 07:30, erstellt von Sergio Cortesi
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1996

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
How narrow is the M87* ring? II. A new geometric model
Creators: name: Lockhart, Will
name: Gralla, Samuel E.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The 2017 Event Horizon Telescope (EHT) observations of M87* detected a ring-shaped feature $\sim40μ$as in diameter, consistent with the event horizon scale of a black hole of the expected mass. The thickness of this ring, however, proved difficult to measure, despite being an important parameter for constraining the observational appearance. In the first paper of this series we asked whether the width of the ring was sensitive to the choice of likelihood function used to compare observed closure phases and closure amplitudes to model predictions. In this paper we investigate whether the ring width is robust to changes in the model itself. We construct a more realistic geometric model with two new features: an adjustable radial falloff in brightness, and a secondary "photon ring" component in addition to the primary annulus. This thin, secondary ring is predicted by gravitational lensing for any black hole with an optically thin accretion flow. Analyzing the data using the new model, we find that the primary annulus remains narrow (fractional width $\leq0.25$) even with the added model freedom. This provides further evidence in favor of a narrow ring for the true sky appearance of M87*, a surprising feature that, if confirmed, would demand theoretical explanation. Comparing the Bayesian evidence for models with and without a secondary ring, we find no evidence for the presence of a lensed photon ring in the 2017 observations. However, the techniques we introduce may prove useful for future observations with a larger and more sensitive array.
Linking phantom quintessences and tachyons
Creators: name: Forte, Mónica
Publisher: name: arXiv
Year: 2014
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We present a nonparametric form-invariance transformation through which we establish a link between phantom and tachyonic models in flat Friedmann-Robertson-Walker cosmologies.
description: 3 pages, no figures, accepted for publication in Phys. Rev. D
title: The role of shame and self-compassion in the relationship between weight-based stigma and health-related behaviours
Creators: name: Couturier, Laura
Publisher: name: Memorial University of Newfoundland
Year: 2023

description: Background: Weight-based stigma (WS) has been associated with a number of maladaptive health-related behaviours. Given that perceived negative evaluations from others are theorized contributors to heightened shame, and that shame has been linked with poor health-related behaviours, shame may explain the association between WS and health-related behaviours. Self-compassion, suggested to be an antidote to shame, may act as a protective factor against the impact of WS. The current study examined how WS relates to health-related behaviours in a young adult sample, whether heightened shame mediates the relationships between WS and health-related behaviours, and whether self-compassion moderates these relationships. Method: Participants (299 undergraduate students aged 18-25) completed online self-report measures of WS, health-related behaviours (i.e., disordered eating, physical activity, and substance use), shame, and self-compassion. Correlation coefficients between variables were generated and a mediation analysis was used to examine whether shame mediated the relationships between WS and health-related behaviours. A moderated mediation model was used to determine whether self-compassion moderated this mediation. Results: After controlling for body mass index (BMI), WS was associated with increased disordered eating and increased physical activity, with small to medium effect sizes, but was not significantly correlated with substance use. The association between WS and disordered eating was partially mediated by shame. Self-compassion did not moderate this mediation. Shame did not mediate the relationship between WS and physical activity. Conclusions: WS is a significant predictor of disordered eating and physical activity in young adults after controlling for BMI, with the relationship between WS and disordered eating partially explained by increased shame. Implications for clinical settings and anti-WS awareness programs are discussed.
Sonnenfleckenzeichnung Nr. 266.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 20.11.1996, 13:30, erstellt von Sergio Cortesi
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1996

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Automated Self-Admitted Technical Debt Tracking at Commit-Level: A Language-independent Approach
Creators: name: Sheikhaei, Mohammad Sadegh
name: Tian, Yuan
Publisher: name: figshare
Year: 2023
Subjects: Automated software engineering

description: This package contains the replication materials for our SATD tracking approach, which we presented in our paper titled "Automated Self-Admitted Technical Debt Tracking at Commit-Level: A Language-Independent Approach" at the TechDebt 2023 conference. To obtain the necessary meta information about commits, we rely on vcsSHARK. The two agz files provide the meta information of Ant and Tomcat projects extracted by vcsSHARK. From this meta information, we first extract raw self-admitted technical debts (SATDs), which may contain some false positives due to SATD updates that appeare as SATD deletions and creations. To address this, we then merge the raw SATDs that refer to the same SATD, thereby removing false positives.
Additional file 4 of The effects of the Green-Mediterranean diet on cardiometabolic health are linked to gut microbiome modifications: a randomized controlled trial
Creators: name: Rinott, Ehud
name: Meir, Anat Yaskolka
name: Tsaban, Gal
name: Zelicha, Hila
name: Kaplan, Alon
name: Knights, Dan
name: Tuohy, Kieran
name: Scholz, Matthias Uwe
name: Koren, Omry
name: Stampfer, Meir J.
name: Wang, Dong D.
name: Shai, Iris
name: Youngster, Ilan
Publisher: name: figshare
Year: 2022
Subjects: subject: Ecology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified

description: Additional file 4: Figure S1. Flow Diagram of the DIRECT-PLUS trial.
Sonnenfleckenzeichnung Nr. 158.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 13.07.1996, 07:15, erstellt von Sergio Cortesi
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1996

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 4.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)