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1. Enhancing Complex Thinking Through Active Learning: A Case Study in a Senior Management Course at a Business School

Author

González-Pérez, L. I., Enciso-González, J. A., Maraboto, J., Castillo-Martínez, I. M., Ramírez-Montoya, M. S., Huang, Ronghuai, Series Editor, Kinshuk, Series Editor, Jemni, Mohamed, Series Editor, Chen, Nian-Shing, Series Editor, Spector, J. Michael, Series Editor, Gonçalves, José Alexandre de Carvalho, editor, Lima, José Luís Sousa de Magalhães, editor, Coelho, João Paulo, editor, García-Peñalvo, Francisco José, editor, and García-Holgado, Alicia, editor

Published
2024
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2. Nuclear Techniques in Floating Artifacts in Peru, Latin America, and the World

Author

Mantari, J. L., Montoya, M., Saldarriaga, M., Huerta, J., Castro, J. L., Zúñiga, A., Ramos, J., Xiros, Nikolas I., Series Editor, Carral, Luis, editor, Vega, Adán, editor, Carreño, Jorge, editor, de Lara, José, editor, Lamas, María Isabel, editor, Cartelle, Juan José, editor, Tarrío, Javier, editor, Carballo, Rodrigo, editor, and Townsed, Patrick, editor

Published
2024
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3. MIRAC-5: A ground-based mid-IR instrumentwith the potential to detect ammonia in gas giants

Author

Bowens, R., Leisenring, J., Meyer, M. R., Montoya, M., Hoffmann, W., Morzinski, K., Hinz, P., Monnier, J. D., Bergin, E., Viges, E., Calissendorff, P., Forrest, W., McMurtry, C., Pipher, J., and Cabrera, M.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Earth and Planetary Astrophysics
Abstract

We present the fifth incarnation of the Mid-Infrared Array Camera (MIRAC-5) instrument which will use a new GeoSnap (3 - 13 microns) detector. Advances in adaptive optics (AO) systems and detectors are enabling ground-based mid-infrared systems capable of high spatial resolution and deep contrast. As one of the only 3 - 13 micron cameras used in tandem with AO, MIRAC-5 will be complementary to the James Webb Space Telescope (JWST) and capable of characterizing gas giant exoplanets and imaging forming protoplanets (helping to characterize their circumplanetary disks). We describe key features of the MIRAC-5 GeoSnap detector, a long-wave Mercury-Cadmium-Telluride (MCT) array produced by Teledyne Imaging Sensors (TIS), including its high quantum efficiency (> 65%), large well-depth, and low noise. We summarize MIRAC-5's important capabilities, including prospects for obtaining the first continuum mid-infrared measurements for several gas giants and the first 10.2-10.8 micron NH3 detection in the atmosphere of the warm companion GJ 504b (Teff ~550 K) within 8 hours of observing time. Finally, we describe plans for future upgrades to MIRAC-5 such as adding a coronagraph. MIRAC-5 will be commissioned on the MMT utilizing the new MAPS AO system in late 2022 with plans to move to Magellan with the MagAO system in the future., Comment: 8 pages, 4 figures, To appear in the SPIE Proceedings 'Astronomical Telescopes and Instrumentation' (2022)

Published
2022

5. The HOSTS survey: evidence for an extended dust disk and constraints on the presence of giant planets in the Habitable Zone of $\beta$ Leo

Author

Defrère, D., Hinz, P. M., Kennedy, G. M., Stone, J., Rigley, J., Ertel, S., Gaspar, A., Bailey, V. P., Hoffmann, W. F., Mennesson, B., Millan-Gabet, R., Danchi, W. C., Absil, O., Arbo, P., Beichman, C., Bonavita, M., Brusa, G., Bryden, G., Downey, E. C., Esposito, S., Grenz, P., Haniff, C., Hill, J. M., Leisenring, J. M., Males, J. R., McMahon, T. J., Montoya, M., Morzinski, K. M., Pinna, E., Puglisi, A., Rieke, G., Roberge, A., Rousseau, H., Serabyn, E., Spalding, E., Skemer, A. J., Stapelfeldt, K., Su, K., Vaz, A., Weinberger, A. J., and Wyatt, M. C.

Subjects
Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics
Abstract

The young (50-400 Myr) A3V star $\beta$ Leo is a primary target to study the formation history and evolution of extrasolar planetary systems as one of the few stars with known hot ($\sim$1600$^\circ$K), warm ($\sim$600$^\circ$K), and cold ($\sim$120$^\circ$K) dust belt components. In this paper, we present deep mid-infrared measurements of the warm dust brightness obtained with the Large Binocular Telescope Interferometer (LBTI) as part of its exozodiacal dust survey (HOSTS). The measured excess is 0.47\%$\pm$0.050\% within the central 1.5 au, rising to 0.81\%$\pm$0.026\% within 4.5 au, outside the habitable zone of $\beta$~Leo. This dust level is 50 $\pm$ 10 times greater than in the solar system's zodiacal cloud. Poynting-Robertson drag on the cold dust detected by Spitzer and Herschel under-predicts the dust present in the habitable zone of $\beta$~Leo, suggesting an additional delivery mechanism (e.g.,~comets) or an additional belt at $\sim$5.5 au. A model of these dust components is provided which implies the absence of planets more than a few Saturn masses between $\sim$5 au and the outer belt at $\sim$40 au. We also observationally constrain giant planets with the LBTI imaging channel at 3.8~$\mu$m wavelength. Assuming an age of 50 Myr, any planet in the system between approximately 5 au to 50 au must be less than a few Jupiter masses, consistent with our dust model. Taken together, these observations showcase the deep contrasts and detection capabilities attainable by the LBTI for both warm exozodiacal dust and giant exoplanets in or near the habitable zone of nearby stars., Comment: 11 pages, 9 figures, accepted for publication in Astronomical Journal

Published
2021
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11. The HOSTS Survey for Exozodiacal Dust: Preliminary results and future prospects

Author

Ertel, S., Kennedy, G. M., Defrère, D., Hinz, P., Shannon, A. B., Mennesson, B., Danchi, W. C., Gelino, C., Hill, J. M., Hoffmann, W. F., Rieke, G., Spalding, E., Stone, J. M., Vaz, A., Weinberger, A. J., Willems, P., Absil, O., Arbo, P., Bailey, V. P., Beichman, C., Bryden, G., Downey, E. C., Durney, O., Esposito, S., Gaspar, A., Grenz, P., Haniff, C. A., Leisenring, J. M., Marion, L., McMahon, T. J., Millan-Gabet, R., Montoya, M., Morzinski, K. M., Pinna, E., Power, J., Puglisi, A., Roberge, A., Serabyn, E., Skemer, A. J., Stapelfeldt, K., Su, K. Y. L., Vaitheeswaran, V., and Wyatt, M. C.

Subjects
Astrophysics - Earth and Planetary Astrophysics
Abstract

[abridged] The presence of large amounts of dust in the habitable zones of nearby stars is a significant obstacle for future exo-Earth imaging missions. We executed an N band nulling interferometric survey to determine the typical amount of such exozodiacal dust around a sample of nearby main sequence stars. The majority of our data have been analyzed and we present here an update of our ongoing work. We find seven new N band excesses in addition to the high confidence confirmation of three that were previously known. We find the first detections around Sun-like stars and around stars without previously known circumstellar dust. Our overall detection rate is 23%. The inferred occurrence rate is comparable for early type and Sun-like stars, but decreases from 71% [+11%/-20%] for stars with previously detected mid- to far-infrared excess to 11% [+9%/-4%] for stars without such excess, confirming earlier results at high confidence. For completed observations on individual stars, our sensitivity is five to ten times better than previous results. Assuming a lognormal luminosity function of the dust, we find upper limits on the median dust level around all stars without previously known mid to far infrared excess of 11.5 zodis at 95% confidence level. The corresponding upper limit for Sun-like stars is 16 zodis. An LBTI vetted target list of Sun-like stars for exo-Earth imaging would have a corresponding limit of 7.5 zodis. We provide important new insights into the occurrence rate and typical levels of habitable zone dust around main sequence stars. Exploiting the full range of capabilities of the LBTI provides a critical opportunity for the detailed characterization of a sample of exozodiacal dust disks to understand the origin, distribution, and properties of the dust., Comment: To appear in SPIE Astronomical Telescopes + Instrumentation 2018 proceedings. Some typos fixed, one reference added

Published
2018

12. The HOSTS survey - Exozodiacal dust measurements for 30 stars

Author

Ertel, S., Defrère, D., Hinz, P., Mennesson, B., Kennedy, G. M., Danchi, W. C., Gelino, C., Hill, J. M., Hoffmann, W. F., Rieke, G., Shannon, A., Spalding, E., Stone, Jordan M., Vaz, A., Weinberger, A. J., Willems, P., Absil, O., Arbo, P., Bailey, V. P., Beichman, C., Bryden, G., Downey, E. C., Durney, O., Esposito, S., Gaspar, A., Grenz, P., Haniff, C. A., Leisenring, J. M., Marion, L., McMahon, T. J., Millan-Gabet, R., Montoya, M., Morzinski, K. M., Pinna, E., Power, J., Puglisi, A., Roberge, A., Serabyn, E., Skemer, A. J., Stapelfeldt, K., Su, K. Y. L., Vaitheeswaran, V., and Wyatt, M. C.

Subjects
Astrophysics - Solar and Stellar Astrophysics
Abstract

The HOSTS (Hunt for Observable Signatures of Terrestrial Systems) survey searches for dust near the habitable zones (HZs) around nearby, bright main sequence stars. We use nulling interferometry in N band to suppress the bright stellar light and to probe for low levels of HZ dust around the 30 stars observed so far. Our overall detection rate is 18%, including four new detections, among which are the first three around Sun-like stars and the first two around stars without any previously known circumstellar dust. The inferred occurrence rates are comparable for early type and Sun-like stars, but decrease from 60 (+16/-21)% for stars with previously detected cold dust to 8 (+10/-3)% for stars without such excess, confirming earlier results at higher sensitivity. For completed observations on individual stars, our sensitivity is five to ten times better than previous results. Assuming a lognormal excess luminosity function, we put upper limits on the median HZ dust level of 13 zodis (95% confidence) for a sample of stars without cold dust and of 26 zodis when focussing on Sun-like stars without cold dust. However, our data suggest that a more complex luminosity function may be more appropriate. For stars without detectable LBTI excess, our upper limits are almost reduced by a factor of two, demonstrating the strength of LBTI target vetting for future exo-Earth imaging missions. Our statistics are so far limited and extending the survey is critical to inform the design of future exo-Earth imaging surveys., Comment: 26 pages, 7 figures, 5 tables, accepted for publication by AJ

Published
2018
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15. Psychometric Assessment of a Tool to Evaluate Motivation and Knowledge of an Energy-Related Topic MOOC

Author

Vázquez, J. A. Valdivia, Ramirez-Montoya, M. S., and González, J. R. Valenzuela

Abstract

Online education has increased over the last two decades in response to an increasing learning demand. Massive open online courses (MOOCs) seem to be an adequate tool to facilitate current educational dynamics. However, evaluating students' motivation and learning to predict their engagement when attending a MOOC represents a challenge. This study combines characteristics of data from MOOC environments (e.g., large sample size) with well-established psychometric methodology (validity and reliability estimations) to attain a reliable resource to evaluate MOOC participants. Four independent datasets from MOOCs on energy-related topics were used to psychometrically examine the new "Initial survey of interests, motivations, and knowledge regarding MOOCs" (EIIMC-MOOC). The results indicate that the EIIMC-MOOC is a valid, reliable and stable tool to evaluate initial motivation and prior knowledge of participants attending energy-related topics.

Published
2021
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17. P-Median Problem: A Real Case Application

Author

Bernábe-Loranca, M. B., González-Velázquez, R., Granillo-Martinez, Erika, Romero-Montoya, M., Barrera-Cámara, Ricardo A., Kacprzyk, Janusz, Series Editor, Pal, Nikhil R., Advisory Editor, Bello Perez, Rafael, Advisory Editor, Corchado, Emilio S., Advisory Editor, Hagras, Hani, Advisory Editor, Kóczy, László T., Advisory Editor, Kreinovich, Vladik, Advisory Editor, Lin, Chin-Teng, Advisory Editor, Lu, Jie, Advisory Editor, Melin, Patricia, Advisory Editor, Nedjah, Nadia, Advisory Editor, Nguyen, Ngoc Thanh, Advisory Editor, Wang, Jun, Advisory Editor, Abraham, Ajith, editor, Siarry, Patrick, editor, Ma, Kun, editor, and Kaklauskas, Arturas, editor

Published
2021
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21. Monte Carlo simulations and phantom validation of low-dose radiotherapy to the lungs using an interventional radiology C-arm fluoroscope

Author

Roa, D., Leon, S., Paucar, O., Gonzales, A., Schwarz, B., Olguin, E., Moskvin, V., Alva-Sanchez, M., Glassell, M., Correa, N., Moyses, H., Shankar, A., Hamrick, B., Sarria, G.R., Li, B., Tajima, T., Necas, A., Guzman, C., Challco, R., Montoya, M., Meza, Z., Zapata, M., Marquez, F., Neira, R., Vilca, W., Mendez, J., and Hernandez, J.

Published
2022
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22. Crafting personalized learning paths with AI for lifelong learning: a systematic literature review.

Author

Bayly-Castaneda, K., Ramirez-Montoya, M.-S., and Morita-Alexander, A.

Subjects
LANGUAGE models, ARTIFICIAL intelligence, INDIVIDUALIZED instruction, SCIENCE databases, WEB databases
Abstract

The rapid evolution of knowledge requires constantly acquiring and updating skills, making lifelong learning crucial. Despite decades of artificial intelligence, recent advances promote new solutions to personalize learning in this context. The purpose of this article is to explore the current state of research on the development of artificial intelligence-mediated solutions for the design of personalized learning paths. To achieve this, a systematic literature review (SRL) of 78 articles published between 2019 and 2024 from the Scopus and Web or Science databases was conducted, answering seven questions grouped into three themes: characteristics of the published research, context of the research, and type of solution analyzed. This study identified that: (a) the greatest production of scientific research on the topic is developed in China, India and the United States, (b) the focus is mainly directed towards the educational context at the higher education level with areas of opportunity for application in the work context, and (c) the development of adaptive learning technologies predominates; however, there is a growing interest in the application of generative language models. This article contributes to the growing interest and literature related to personalized learning under artificial intelligence mediated solutions that will serve as a basis for academic institutions and organizations to design programs under this model. [ABSTRACT FROM AUTHOR]

Published
2024
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25. Simultaneous Water Vapor and Dry Air Optical Path Length Measurements and Compensation with the Large Binocular Telescope Interferometer

Author

Defrère, D., Hinz, P., Downey, E., Böhm, M., Danchi, W. C., Durney, O., Ertel, S., Hill, J. M., Hoffmann, W. F., Mennesson, B., Millan-Gabet, R., Montoya, M., Pott, J. -U., Skemer, A., Spalding, E., Stone, J., and Vaz, A.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

The Large Binocular Telescope Interferometer uses a near-infrared camera to measure the optical path length variations between the two AO-corrected apertures and provide high-angular resolution observations for all its science channels (1.5-13 $\mu$m). There is however a wavelength dependent component to the atmospheric turbulence, which can introduce optical path length errors when observing at a wavelength different from that of the fringe sensing camera. Water vapor in particular is highly dispersive and its effect must be taken into account for high-precision infrared interferometric observations as described previously for VLTI/MIDI or the Keck Interferometer Nuller. In this paper, we describe the new sensing approach that has been developed at the LBT to measure and monitor the optical path length fluctuations due to dry air and water vapor separately. After reviewing the current performance of the system for dry air seeing compensation, we present simultaneous H-, K-, and N-band observations that illustrate the feasibility of our feedforward approach to stabilize the path length fluctuations seen by the LBTI nuller., Comment: SPIE conference proceedings

Published
2016
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26. Nulling Data Reduction and On-Sky Performance of the Large Binocular Telescope Interferometer

Author

Defrère, D., Hinz, P. M., Mennesson, B., Hoffmann, W. F., Millan-Gabet, R., Skemer, A. J., Bailey, V., Danchi, W. C., Downey, E. C., Durney, O., Grenz, P., Hill, J. M., McMahon, T. J., Montoya, M., Spalding, E., Vaz, A., Absil, O., Arbo, P., Bailey, H., Brusa, G., Bryden, G., Esposito, S., Gaspar, A., Haniff, C. A., Kennedy, G. M., Leisenring, J. M., Marion, L., Nowak, M., Pinna, E., Powell, K., Puglisi, A., Rieke, G., Roberge, A., Serabyn, E., Sosa, R., Stapeldfeldt, K., Su, K., Weinberger, A. J., and Wyatt, M. C.

Subjects
Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

The Large Binocular Telescope Interferometer (LBTI) is a versatile instrument designed for high-angular resolution and high-contrast infrared imaging (1.5-13 microns). In this paper, we focus on the mid-infrared (8-13 microns) nulling mode and present its theory of operation, data reduction, and on-sky performance as of the end of the commissioning phase in March 2015. With an interferometric baseline of 14.4 meters, the LBTI nuller is specifically tuned to resolve the habitable zone of nearby main-sequence stars, where warm exozodiacal dust emission peaks. Measuring the exozodi luminosity function of nearby main-sequence stars is a key milestone to prepare for future exoEarth direct imaging instruments. Thanks to recent progress in wavefront control and phase stabilization, as well as in data reduction techniques, the LBTI demonstrated in February 2015 a calibrated null accuracy of 0.05% over a three-hour long observing sequence on the bright nearby A3V star beta Leo. This is equivalent to an exozodiacal disk density of 15 to 30 zodi for a Sun-like star located at 10pc, depending on the adopted disk model. This result sets a new record for high-contrast mid-infrared interferometric imaging and opens a new window on the study of planetary systems., Comment: 17 pages, 18 figures (resubmitted to ApJ with referee's comments)

Published
2016
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28. Exoplanet science with the LBTI: instrument status and plans

Author

Defrère, D., Hinz, P., Skemer, A., Bailey, V., Downey, E., Durney, O., Eisner, J., Hill, J. M., Hoffmann, W. F., Leisenring, J., McMahon, T., Montoya, M., Spalding, E., Stone, J., Vaz, A., Absil, O., Esposito, S., Kenworthy, M., Mennesson, B., Millan-Gabet, R., Nelson, M., Puglisi, A., Skrutskie, M. F., and Wilson, J.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Earth and Planetary Astrophysics
Abstract

The Large Binocular Telescope Interferometer (LBTI) is a strategic instrument of the LBT designed for high-sensitivity, high-contrast, and high-resolution infrared (1.5-13 $\mu$m) imaging of nearby planetary systems. To carry out a wide range of high-spatial resolution observations, it can combine the two AO-corrected 8.4-m apertures of the LBT in various ways including direct (non-interferometric) imaging, coronagraphy (APP and AGPM), Fizeau imaging, non-redundant aperture masking, and nulling interferometry. It also has broadband, narrowband, and spectrally dispersed capabilities. In this paper, we review the performance of these modes in terms of exoplanet science capabilities and describe recent instrumental milestones such as first-light Fizeau images (with the angular resolution of an equivalent 22.8-m telescope) and deep interferometric nulling observations., Comment: 12 pages, 6 figures, Proc. SPIE

Published
2015
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29. Co-phasing the Large Binocular Telescope: status and performance of LBTI/PHASECam

Author

Defrère, D., Hinz, P., Downey, E., Ashby, D., Bailey, V., Brusa, G., Christou, J., Danchi, W. C., Grenz, P., Hill, J. M., Hoffmann, W. F., Leisenring, J., Lozi, J., McMahon, T., Mennesson, B., Millan-Gabet, R., Montoya, M., Powell, K., Skemer, A., Vaitheeswaran, V., Vaz, A., and Veillet, C.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

The Large Binocular Telescope Interferometer is a NASA-funded nulling and imaging instrument designed to coherently combine the two 8.4-m primary mirrors of the LBT for high-sensitivity, high-contrast, and high-resolution infrared imaging (1.5-13 um). PHASECam is LBTI's near-infrared camera used to measure tip-tilt and phase variations between the two AO-corrected apertures and provide high-angular resolution observations. We report on the status of the system and describe its on-sky performance measured during the first semester of 2014. With a spatial resolution equivalent to that of a 22.8-meter telescope and the light-gathering power of single 11.8-meter mirror, the co-phased LBT can be considered to be a forerunner of the next-generation extremely large telescopes (ELT)., Comment: 8 pages, 5 figures, SPIE Conference proceedings

Published
2015
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30. First-light LBT nulling interferometric observations: warm exozodiacal dust resolved within a few AU of eta Corvi

Author

Defrère, D., Hinz, P. M., Skemer, A. J., Kennedy, G. M., Bailey, V. P., Hoffmann, W. F., Mennesson, B., Millan-Gabet, R., Danchi, W. C., Absil, O., Arbo, P., Beichman, C., Brusa, G., Bryden, G., Downey, E. C., Durney, O., Esposito, S., Gaspar, A., Grenz, P., Haniff, C., Hill, J. M., Lebreton, J., Leisenring, J. M., Males, J. R., Marion, L., McMahon, T. J., Montoya, M., Morzinski, K. M., Pinna, E., Puglisi, A., Rieke, G., Roberge, A., Serabyn, E., Sosa, R., Stapeldfeldt, K., Su, K., Vaitheeswaran, V., Vaz, A., Weinberger, A. J., and Wyatt, M. C.

Subjects
Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

We report on the first nulling interferometric observations with the Large Binocular Telescope Interferometer (LBTI), resolving the N' band (9.81 - 12.41 um) emission around the nearby main-sequence star eta Crv (F2V, 1-2 Gyr). The measured source null depth amounts to 4.40% +/- 0.35% over a field-of-view of 140 mas in radius (~2.6\,AU at the distance of eta Corvi) and shows no significant variation over 35{\deg} of sky rotation. This relatively low null is unexpected given the total disk to star flux ratio measured by Spitzer/IRS (~23% across the N' band), suggesting that a significant fraction of the dust lies within the central nulled response of the LBTI (79 mas or 1.4 AU). Modeling of the warm disk shows that it cannot resemble a scaled version of the Solar zodiacal cloud, unless it is almost perpendicular to the outer disk imaged by Herschel. It is more likely that the inner and outer disks are coplanar and the warm dust is located at a distance of 0.5-1.0 AU, significantly closer than previously predicted by models of the IRS spectrum (~3 AU). The predicted disk sizes can be reconciled if the warm disk is not centrosymmetric, or if the dust particles are dominated by very small grains. Both possibilities hint that a recent collision has produced much of the dust. Finally, we discuss the implications for the presence of dust at the distance where the insolation is the same as Earth's (2.3 AU)., Comment: 9 pages, 6 figures, accepted for publication in ApJ

Published
2015
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31. L'-band AGPM vector vortex coronagraph's first light on LBTI/LMIRCam

Author

Defrère, D., Absil, O., Hinz, P., Kuhn, J., Mawet, D., Mennesson, B., Skemer, A., Wallace, J. Kent, Bailey, V., Downey, E., Delacroix, C., Durney, O., Forsberg, P., Gomez, C., Habraken, S., Hoffmann, W. F., Karlsson, M., Kenworthy, M., Leisenring, J., Montoya, M., Pueyo, L., Skrutskie, M., and Surdej, J.

Subjects
Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

We present the first observations obtained with the L'-band AGPM vortex coronagraph recently installed on LBTI/LMIRCam. The AGPM (Annular Groove Phase Mask) is a vector vortex coronagraph made from diamond subwavelength gratings. It is designed to improve the sensitivity and dynamic range of high-resolution imaging at very small inner working angles, down to 0.09 arcseconds in the case of LBTI/LMIRCam in the L' band. During the first hours on sky, we observed the young A5V star HR\,8799 with the goal to demonstrate the AGPM performance and assess its relevance for the ongoing LBTI planet survey (LEECH). Preliminary analyses of the data reveal the four known planets clearly at high SNR and provide unprecedented sensitivity limits in the inner planetary system (down to the diffraction limit of 0.09 arcseconds)., Comment: 9 pages, 4 figures, SPIE proceedings

Published
2014
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32. Structural Optimization of a Reduced-Scale Model of a Wind Mill Tower for Wind Tunnel Testing

Author

Cid Montoya, M., Hernández, S., López, C., Álvarez, A., Romera, L., Jurado, J. Á., di Prisco, Marco, Series Editor, Chen, Sheng-Hong, Series Editor, Vayas, Ioannis, Series Editor, Kumar Shukla, Sanjay, Series Editor, Sharma, Anuj, Series Editor, Kumar, Nagesh, Series Editor, Wang, Chien Ming, Series Editor, Ricciardelli, Francesco, editor, and Avossa, Alberto Maria, editor

Published
2019
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33. On the Aerostructural Design of Long-Span Cable-Stayed Bridges: The Contribution of Parameter Variation Studies with Focus on the Deck Design

Author

Cid Montoya, M., Nieto, F., Hernández, S., Jurado, J. Á., di Prisco, Marco, Series Editor, Chen, Sheng-Hong, Series Editor, Vayas, Ioannis, Series Editor, Kumar Shukla, Sanjay, Series Editor, Sharma, Anuj, Series Editor, Kumar, Nagesh, Series Editor, Wang, Chien Ming, Series Editor, Ricciardelli, Francesco, editor, and Avossa, Alberto Maria, editor

Published
2019
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34. The Use of Gamification as a Teaching Methodology in a MOOC About the Strategic Energy Reform in México

Author

Mena, J., Rincón Flores, E. G., Ramírez-Velarde, R., Ramírez-Montoya, M. S., Kacprzyk, Janusz, Series Editor, Pal, Nikhil R., Advisory Editor, Bello Perez, Rafael, Advisory Editor, Corchado, Emilio S., Advisory Editor, Hagras, Hani, Advisory Editor, Kóczy, László T., Advisory Editor, Kreinovich, Vladik, Advisory Editor, Lin, Chin-Teng, Advisory Editor, Lu, Jie, Advisory Editor, Melin, Patricia, Advisory Editor, Nedjah, Nadia, Advisory Editor, Nguyen, Ngoc Thanh, Advisory Editor, Wang, Jun, Advisory Editor, Di Mascio, Tania, editor, Vittorini, Pierpaolo, editor, Gennari, Rosella, editor, De la Prieta, Fernando, editor, Rodríguez, Sara, editor, Temperini, Marco, editor, Azambuja Silveira, Ricardo, editor, Popescu, Elvira, editor, and Lancia, Loreto, editor

Published
2019
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42. Feasibility of Acquiring Radiotherapy Linac Commissioning Data with a Three-Dimensional Cubic Electronic Detector Array

Author

Paucar, O., primary, Meza, Z. M. Arqque, additional, Escobar, B. Perez, additional, Pancorbo, E. Paniagua, additional, Risco-Castillo, M., additional, Chalco, R. Challco, additional, Calcina, C. S. Guzman, additional, Galvez, A. Gonzales, additional, Montoya, M., additional, Ccoscco, A. E. Gonzales, additional, Hernandez, J., additional, and Roa, D.E., additional

Published
2023
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43. 12. Conclusions

Author

Gavier-Widén, D., primary, Bellini, S., additional, Chenais, E., additional, Ferreira, F., additional, Jori, F., additional, Le Potier, M.F., additional, Montoya, M., additional, Netherton, C.L., additional, Sánchez-Cordón, P.J., additional, Ståhl, K., additional, and Iacolina, L., additional

Published
2021
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47. Post-anaesthesia pulmonary complications after use of muscle relaxants (POPULAR): a multicentre, prospective observational study

Author

Abad Gurumeta, Alfredo, Abernethy, Caroline, Abigail, Patrick, Achaibar, Kira, Adam, Emily, Afshari, Arash, Agudelo Montoya, M. Elizabeth, Akgün, Fatma Nur, Aletti, Gabriele, Alkış, Neslihan, Allan, Katie, Allan, Ashley, Allaouchiche, Bernard, Allcock, Clare, Almasy, Emoke, Amey, Isobel, Amigoni, Maria, Andersen, Elin, Andersson, Peder, Anipchenko, Natalya, Antunes, Pedro, Armstrong, Earlene, Aslam, Tayyba Naz, Aslin, Bjorn, Assunção, José Pedro, Ausserer, Julia, Avvai, Mary, Awad, Nahla, Ayas Montero, Begoña, Ayuso, Mercedes, Azevedo, Patricia, Badarau, Victoria, Badescu, Roxana, Baiardo Redaelli, Martina, Baird, Colin, Baird, Yolanda, Baker, Tim, Balaji, Packianathaswamy, Bălan, Cristina, Balandin, Alina, Balescu-Arion, Carmen, Baliuliene, Vilda, Baltasar Isabel, Jorge, Baluch, Saif Nasr, Bandrabur, Daniela, Bankewitz, Carla, Barber, Katrina, Barbera, Francesco, Barcraft-Barnes, Helena, Barletti, Valentina, Barnett, Gill, Baron, Kirsty, Barros, Ana, Barsan, Victoria, Bartlett, Pauline, Batistaki, Chrysanthi, Baumgarten, Georg, Baytas, Volkan, Beauchamp, Nigel, Becerra Cayetano, Isabel A., Bell, Stephanie, Bellandi, Mattia, Belletti, Alessandro, Belmonte Cuenca, Julio, Benitez-Cano, Adela, Beretta, Luigi, Berger, Marc, Bergmann, Nicole, Bergmark, Kristina, Bermudez Lopez, Maria, Bernotaite, Monika, Beurskens, Charlotte, Bidd, Heena, Bifulco, Francesca, Bignami, Elena, Bilic, Aleksandar, Bilskiene, Diana, Bischoff, Petra, Bishop, Luke, Bjonness, Therese, Blaylock, Hether, Blethyn, Kate, Blincoe, Thomas, Blokhin, Ivan, Blunt, Nadia, Boer, Christa, Bois, Grégory, Bonicolini, Eleonora, Booth, Joanna, Borecka-Kedzierska, Miroslawa, Borstnar, Katarina, Borys, Michał, Boselli, Emmanuel, Bouvet, Lionel, Bouwman, Arthur, Bowen, Leonora, Bowrey, Sarah, Boxall, Leigh, Božić, Teodora, Bradley, Tom, Branco, Teresa, Brazzi, Luca, Brazzoni, Marcella, Brear, Tracy, Brogly, Nicolas, Brohi, Farooq, Broms, Jacob, Bubliauskas, Andrius, Bucolo, Gea Erika, Buerkle, Hartmut, Buggy, Donal, Buhre, Wolfgang, Bukauskas, Tomas, Butturini, Francesco, Byttner, Anders, Cabrera Díaz, Itahísa, Calderon, Adriana, Calhau, Ricardo, Callejo, Angel, Cammu, Guy, Campesato, Manuela, Can, Özlem S, Candeias, Margarida, Cantor, Andreea, Carise, Elsa, Carmona, Cristina, Carreteiro, Joana, Carrieri, Cosima, Carter, Anna, Casal, Manuela, Casanova, Irene, Cascella, Marco, Casero, Luis M., Casiraghi, Guiseppina Maria, Castelo-Branco, Laila, Castro Arranz, Carlos, Cernea, Daniela Denisa, Cervantes, Jesoporiol, Chandler, Ben, Charnock, Robert, Chatzimicali, Aikaterini, Chinery, Elane, Chishti, Ahmed, Chondhury, Priyakam, Christie, Emily, Christodoudiles, George, Ciardo, Stefano, Cimpeanu, Luminata, Cindea, Iulia, Cinnella, Gilda, Clark, Sebastian, Clayton, Matthew, Cocu, Simona, Collyer, Thomas, Colvin, Carie, Cope, Sean, Copeta, Filomena, Copotoiu, Sanda-Maria, Correia de Barros, Filinto, Corso, Ruggero Massimo, Cortegiani, Andrea, Costa, Gabriela, Cowton, Amanda, Cox, Nicolas, Craig, James, Cricca, Valentina, Cronin, John, Cunha, Mariana, Cuomo, Arturo, Curley, Katherine, Czuczwar, Mirosław, Dabrowska, Domenika, Damster, Sabrine, Danguy des Déserts, Marc, Daniliuc, Aura, Danninger, Thomas, Darwish, Imad, Dascalu, Corina, Davies, Kirsty, Davies, Simon, De Boer, Hans, De Flaviis, Adelisa, De Selincourt, Gabrielle, Deana, Cristian, Debaene, Bertrand, Debreceni, Gabor, Dedhia, Jatin, Delgado Garcia, Isabel, Della Rocca, Giorgio, Delroy-Buelles, Llana, Desai, Tejal, Dhillon, Parveen, Di Giacinto, Ida, Di Mauro, Piero, Diaz Gomez, Tamara V., Dimitrovski, Aleksandar, Dinic, Vesna, Dîrzu, Dan-Sebastian, Divander, Mona Britt, Dolinar, Janez, Domingues, Susana, Doolan, James, Downes, Charlotte, Dragoescu, Nicoleta Alice, Droc, Gabriela, Dum, Elisabeth, Dumitrescu, Alexandra, Duncan, Louise, Dzurňáková, Paul, Eberl, Susanne, Edwards, Jayne, Edwards, Mark, Ekelund, Kim, Ekengren, Patrik, Elghouty, Eyad, Ellerkmann, Richard, Ellis, Helen, Elme, Andreas, Ernst, Thomas, Errando, Carlos Luis, Estenes, Simao, Ewaldsson, Callis, Farid, Nahla, Featherstone, James, Febres, Daniela, Fedorov, Sergey, Feggeler, Johanna, Feijten, Prisca, Fellmann, Tobias, Fernandez Candil, Juan, Fernandez Castineira, Ana, Fernández Castineira, Juan, Fernando, Aruna, Ferrando, Carlos, Ferreira, Leonia, Ferreira, Patrick, Feyling, Anders, Filipescu, Daniela, Fleischer, Andreas, Floris, Leda, Foerster, Urs, Fox, Benjamin, Franke, Uwe, Frasca, Denis, Frey, Christian, Frost, Victoria, Fullin, Giorgio, Fumagalli, Jacopo, Furneval, Julie, Fusari, Maurizio, Gallacher, Stuart, Galushka, Svetlana, Gambale, Giorgio, Gambino, Irene, Garcia-Perez, Maria Luisa, Garg, Sanjeev, Garlak, Justyna, Gavranovic, Zeljka, Gavrilov, Roman, Gaynor, Lames, Gecaj Gashi, Agreta, Georghiou, Maria, Gerjevic, Bozena, Gferer, Gudrun, Giarratano, Antonino, Gibson, Andy, Gievski, Vanja, Giles, Julian, Gillberg, Lars, Gilowska, Katarzyna, Gilsanz Rodriguez, Fernando, Gioia, Antonio, Giovannoni, Cecilia, Girotra, Vandana, Gkinas, Dimitrios, Gkiokas, George, Godoroja, Daniela, Goebel, Ulrich, Goel, Vandana, Gonzalez, Matilde, Goranovic, Tatjana, Gornik-Wlaszczuk, Ewa, Gosavi, Smita, Gottfridsson, peter, Gottschalk, André, Granell, Manuel, Granstrom, Anna, Grassetto, Alberto, Greenwood, Anna, Grigoras, Ioana, Grintescu, Ioana, Gritsan, Alexey, Gritsan, Galina, Grynyuk, Andriy, Guadagnin, Giovanni Maria, Guarnieri, Marcello, Güçlü, Çiğdem, Guerrero Diez, Maria, Gunenc, Ferim, Günther, Ulf, Gupta, Pawan, Guttenthaler, Vera, Hack, Yvonne, Hafisayena, Ade, Hagau, Natalia, Haldar, Jagannath, Hales, Dawn, Hancı, Volkan, Hanna-Jumma, Sameer, Harazim, Hana, Harlet, Pierre, Harper, Daniel, Harris, Benjamin, Harvey, Orla, Hashimi, Medita, Hawkins, Lesley, Hayes, Conrad, Heaton, James, Heier, Tom, Helliwell, Laurence, Hemmes, Sabrine, Henderson, Kate, Hermanides, Jeroen, Hermanns, Henning, Herrera Hueso, Berta, Hestenes, Siv, Hettiarachchi, Roshane, Highgate, Judith, Hodgson, Keith, Hoelbling, Daniel, Holland, Jonathan, Horhota, Lucian, Hormis, Anil, Hribar, Renata, Hua, Alina, Humphreys, Sally, Humphries, Ryan, Humpliková, Simona, Hunt, Janez, Husnain, Ali, Hussein, Ahmed, Hyams, Benjamin, Iannuccelli, Fabrizio, Ilette, Katie, Ilyas, Carl, Inan, Turgay, India, Immaculada, Ionițăv, Victor, Irwin, Foo, Jain, Vipul, Janez, Benedikt, Jankovic, Radmilo, Jenkins, Sarah, Jenko, Matej, Jimenez, Raquel, Jiménez Gomez, Bárbara, Joachim, Sugganthi, Joelsson-Alm, Eva, John, John, Jonikaite, Lina, Jovic, Miomir, Jungwirth, Bettina, Junke, Etienne, Kabakov, Borys, Kadaoui, Salah-Din, Kanski, Andrzej, Karadag, Süheyla, Karbonskiene, Aurika, Karjagin, Juri, Kasnik, Darja, Katanolli, Fatos, Katsika, Eleni, Kaufmann, Kai, Keane, Helen, Kelly, Martin, Kent, Melanie, Keraitiene, Grazina, Khudhur, Ahmed, Khuenl-Brady, Karin, Kidd, Laurie, King, Siobhan, Kirchgäßner, Katharina, Klancir, Tino, Klucniks, Andris, Knotzer, Johann, Knowlden, Peter, Koers, Lena, Kompan, Janez, Koneti, Kiran K, Kooij, Fabian, Koolen, Eric, Koopman - van Gemert, Anna Wilhelmina Margaretha Maria, Kopp, Kristen, Korfiotis, Dimitrios, Korolkov, Oleg, Kosinová, Martina, Köstenberger, Markus, Kotzinger, Oskar, Kovačević, Marko, Kranke, Peter, Kranke, Eva, Kraus, Christiane, Kraus, Stephanie, Kubitzek, Christiane, Kucharski, Rafal, Kucukguclu, Semih, Kudrashou, Allaksandr, Kumar, Vinayak, Kummen, Live, Kunit, Cornelia, Kushakovsky, Vlad, Kuvaki, Bahar, Kuzmanovska, Biljana, Kyttari, Aikaterina, Landoni, Giovanni, Lau, Gary, Lazarev, Konstantin, Legett, Samantha, Legrottaglie, Anna Maria, Leonardi, Silvia, Leong, Maria, Lercher, Helene, Leuvrey, Matthieu, Leva, Brigitte, Levstek, Meta, Limb, James, Lindholm, Espen, Linton, Fiona, Liperi, Corradero, Lipski, Fabian, Lirk, Philipp, Lisi, Alberto, Lišková, Katarina, Lluch Oltra, Aitana, Loganathan, Vinothan, Lombardi, Stefania, Lopez, Eloisa, Lopez Rodríguez, Maria, Lorenzini, Laura, Lowicka, Malgorzata, Lugovoy, Alexander, Luippold, Madeleine, Lumb, Andrew, Macas, Andrius, Macgregor, Mark, Machado, Humberto, Maciariello, Maria, Madeira, Isabel, Maitan, Stefan, Majewski, Jacek, Maldini, Branka, Malewski, Georgia, Manfredini, Livia, Männer, Olja, Marchand, Bahareh, Marcu, Alexandra, Margalef, Jordi, Margarson, Michael, Marinheiro, Lucia, Markic, Ana, Markovic Bozic, Jasmina, Marrazzo, Francesco, Martin, Jane, Martin Ayuso, Maria, Martinez, Esteher, Martino, Enrico Antonio, Martinson, Victoria, Marusic-Gaser, Katarina, Mascarenhas, Catia, Mathis, Cindy, Matsota, Paraskevi, Mavrommati, Eleni, Mazul Sunko, Branka, McCourt, Killian, McGill, Neil, McKee, Raymond, Meço, Başak Ceyda, Meier, Sonja, Melbourne, Susan, Melbybråthen, Grethe, Meli, Andrea, Melia, Aiden, Melotti, Rita Maria, Menga, Maria Rosaria, Mercer, Pauline, Merotra, Susan, Mescolini, Silvia, Metterlein, Thomas, Michalov, Martin, Michlig, Sam, Midgley, Susan, Milić, Morena, Milojevic, Milan, Miñana, Amanda, Minto, Gary, Mirabella, Lucia, Mirea, Liliana, Mittelstädt, Ludger, Moeglen, Aude, Moise, Alida, Mokini, Zhirajr, Molin, Anna, Moltó, Luis, Monea, Maria Concetta, Montalto, Francesca, Montgomery, Jane, Montgomery, Claire, Montillo, Gerardo, Moore, Sally, Moore, Faye, Moreira, Zelia, Moreno, Tania, Moreno, Ricardo, Moret, Enrique, Moreton, Sarah, Morgan, Marianne, Moro Velasco, Concepción, Morri, Davide, Moull, Alice, Moura, Fernando, Mráz, Peter, Mrozek, Katarzyna, Mukhtar, Karim, Muniyappa, Sudeshkumar, Murray, Heather, Murthy, Burra VS, Mushambi, Mary, Nadolski, Maria, Nardelli, Pasquale, Nardin, Giordano, Navarro Pérez, Rosalía, Naveiro, Andrea, Negri, Manuela, Nesek Adam, Visnja, Neskovic, Vojislava, Neuwersch, Stefan, Neves, Miriam, Nguyen, Bavinh, Ní Eochagáin, Aisling, Nicholas, Caroline, Nightingale, Jeremy, Norrie, Kylie, Novak-Jankovic, Vesna, Novakova, Andrea, Novillo, Marta, Numan, Sandra, Oduro-Dominah, Louise, Oldner, Anders, Oliveira, Isabel, Ologoiu, Daniela, Oloktsidou, Irini, O'Reilly, Rosalind, Orlando, Alessandro, Ovezov, Alexey, Ozbilgin, Sule, Paal, Peter, Padin Barreiro, Lidia, Palugniok, Ryszard, Papaioannou, Alexandra, Papapostolou, Konstantinos, Paranthaman, Prabhakar, Pardey Bracho, Gilda, Parente, Suzana, Parfeni, Alexandru, Pasin, Laura, Passey, Samuel, Pastor, Ernesto, Patch, Sarah, Patil, Andan, Paunescu, Marilena-Alina, Pehboeck, Daniel, Pereira, Manuela, Pereira, Carla, Perez Caballero, Paula, Pérez García, Aníbal, Pérez Soto, Antonia, Perez Tejero, Gisela, Perez-Cerda, Francisco, Pesenti, Antonio, Petta, Rocco, Philippe, Simon, Pickering, David, Pico Veloso, Jandro, Pina, Pedro, Pinho-Oliveira, Vítor, Pinol, Santiago, Pinto, Rita, Pistidda, Laura, Pitterle, Manuela, Piwowarczyk, Paweł, Plotnikova, Olga, Pohl, Holger, Poldermann, Jorinde, Polkovicová, Lucia, Pompei, Livia, Popescu, Mihai, Popović, Radmila, Pota, Vincenzo, Potocnik, Miriam, Potręć, Beata, Potter, Alison, Pramod, Nalwaya, Prchalova, Martina, Preckel, Benedikt, Pugh, Richard, Pulletz, Mark, Radoeshki, Aleksandar, Rafi, Amir, Ragazzi, Riccardo, Raineri Santi, Maurizio, Rajamanickam, Tamiselvan, Rajput, Zahra, Ramachandran, Rajeskar, Ramasamy, Radhika, Ramessur, Suneil, Rao, Roshan, Rasmussen, Anders, Rato, André, Razaque, Usman, Real Navacerrada, M. Isabel, Reavley, Caroline, Reid, James, Reschreiter, Henrik, Rial, Erick, Ribas Carrasco, Patricia, Ribeiro, Sandy, Rich, Nathalie, Richardson, Lydia, Rimaitis, Kestutis, Rimaitis, Marius, Ringvold, Else-Marie, Ripke, Fabian, Ristescu, Irina, Ritchie, Keith, Ródenas, Frederic, Rodrigues, Patrícia, Rogers, Emma, Rogerson, David, Romagnoli, Stefano, Romero, Esther, Rondovic, Goran, Rose, Bernd Oliver, Roth, Winfried, Rotter, Marie-Therese, Rousseau, Guy, Rudjord, Anders, Rueffert, Henrik, Rundgren, Malin, Rupprecht, Korbinian, Rushton, Andrew, Russotto, Vincenzo, Rypulak, Elżbieta, Ryszka, Maciej, Sà, Jacinta, Sà Couto, Paula, Saby, Sandrine, Sagic, Jelena, Saleh, Omar, Sales, Gabriele, Sánchez Sánchez, Yván, Sanghera, Sumayer, Şanli Karip, Ceren, Santiveri Papiol, Francisco Javier, Santos, Sofia, Sarno, Stephen, Saul, Daniel, Saunders, David, Savic, Nenad, Scalco, Loïc, Scanlon, Deborah, Schaller, Stefan, Schax, Christoph, Scheffer, Gert Jan, Schening, Anna, Schiavone, Vincenzo, Schmidt-Ehrenberg, Florian, Schmidt-Mutter, Catherine, Schönberg, Christina, Schopflin, Christian, Schreiber, Jan-Uwe, Schultz, Marcus, Schurig, Marlen, Scott, Carmen, Sebestian, Siby, Sehgal, Selena, Sem, Victoria, Semenas, Egidijus, Serafini, Elena, Serchan, Pashalitsa, Shields, Martin, Shobha, Ramakrishnan, Shosholcheva, Mirjana, Siamansour, Tanja, Siddaiah, Narendra, Siddiqi, Khalid, Sinclair, Rhona, Singh, Permendra, Singh, Rajendra, Sinha, Aneeta, Sinha, Ashok, Skinner, Amanda, Smee, Elizabeth, Smekalova, Olga, Smith, Neil, Smith, Thomas, Smitz, Carine, Smole, Daniel, Sojčić, Nataša, Soler Pedrola, Maria, Somanath, Sameer, Sonksen, Julian, Sorella, Maria Christina, Sörmus, Alar, Soro, Marina, Soto, Carmen, Spada, Anna, Spadaro, Savino, Spaeth, Johannes, Sparr, Harald, Spielmann, Annika, Spindler-Vesel, Alenka, Stamelos, Matthaios, Stancombe L, Liucia, Stanculescu, Andreea, Standl, Thomas, Standley, Tom, Stanek, Ondrej, Stanisavljević, Snežana, Starczewska, Malgorzata, Stäuble, Christiane, Steen, Julie, Stefan, Oana Maria, Stell, Elizabeth, Stera, Caterina, Stevens, Markus, Stoerckel, Marlène, Stošić, Biljana, Stourac, Petr, Stroumpoulis, Konstantinos, Struck, Rafael, Suarez de la Rica, Alejandro, Sultanpori, Altaf, Sundara Rajan, Rajinikanth, Suying, Ong, Svensen, Christer, Swan, Louise, Syrogianni, Paulina, Sysiak, Justyna, Szederjesi, Janos, Taddei, Stefania, Tan Hao, Ern, Tanou, Virginia, Tarabová, Katarina, Tardaguila Sancho, Paula, Tarroso, Maria, Tartaglione, Marco, Taylor, Emma, Tbaily, Lee, Telford, Richard, Terenzoni, Massimo, Theodoraki, Kassiani, Thornley, Helen, Tiganiuc, Liviu, Toim, Hardo, Tomescu, Dana, Tommasino, Concezione, Toni, Jessica, Toninelli, Arturo, Toretti, Ilaria, Townley, Stephen, Trepenaitis, Darius, Trethowan, Brian, Tsaousi, Georgia, Tsiftsi, Aikaterini, Tudor, Adrada, Turan, Güldem, Turhan, Sanem Çakar, Unic-Stojanovic, Dragana, Unterbuchner, Christoph, Unzueta, Carmen, Uranjek, Jasna, Ursic, Tomaz, Vaida, Simona, Valldeperas Ferrer, Silvia, Valldeperas Hernandez, Maria Inmaculada, Valsamidis, Dimitri, Van Beek, Rienk, Van dasselaer, Nick, Van Der Beek, Tim, Van Duivenvoorde, Yoni, van Klei, Wilton A., Van Poorter, Frans, Van Zaane, Bas, Van Zundert, Tom, Van Zyl, Rebekka, Vargas Munoz, Ana Milena, Varsani, Nimu, Vasconcelos, Pedro, Vassilakis, Georgios, Vecchiatini, Tommaso, Vecera, Lubomir, Vercauteren, Marcel, Verdouw, Bas, Verheyen, Veerle, Verri, Marco, Vicari Sottosanti, Luigi Giancarlo, Vico, Manuel, Vidal Mitjans, Patricia, Vilardi, Anna, Vissicchio, Daniela, Vitale, Giovanni, Vitković, Bibiana, Vizcaychipi, Marcela Paola, Voicu, Alexandra, Voje, Minca, Volfová, Ivana, Volta, Carlo Alberto, Von Lutterotti, Theresa, von Tiesenhausen, Anna, Vrecic-Slabe, Simona, Vukcevic, Dejan, Vukovic, Rade, Vullo, P. Agostina, Wade, Andrew, Wallberg, Hanna, Wallden, Jakob, Wallner, Johann, Walther Sturesson, Louise, Watson, Davina, Weber, Stefan, Wegiel Leskiewiq, Anna, Weller, Debbie, Wensing, Carine, Werkmann, Markus, Westberg, Henrik, Wikström, Erik, Williams, Benedict, Wilson, Robin, Wirth, Steffen, Wittmann, Maria, Wood, Laura, Wright, Stella, Zachoval, Christian, Zambon, Massimo, Zampieri, Silvia, Zampone, Salvatore, Zangrillo, Alberto, Zani, Gianluca, Zavackiene, Asta, Zieglerder, Raphael, Zonneveldt, Harry, Zsisku, Lajos, Zucker, Tom-Philipp, Żukowski, Maciej, Zuleika, Mehrun, Zupanĕiĕ, Darja, Kirmeier, Eva, Eriksson, Lars I, Lewald, Heidrun, Jonsson Fagerlund, Malin, Hoeft, Andreas, Hollmann, Markus, Meistelman, Claude, Hunter, Jennifer M, Ulm, Kurt, and Blobner, Manfred

Published
2019
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50. Use of a Visual Programming Language to Gamify Statistics Instruction for Undergraduate Students: A Literature Review and the Path Forward

Author

Félix-Herrán, L.C., primary, Guerrero-Serrano, A., additional, Elizondo-Noriega, A., additional, Tiruvengadam, N., additional, Ceciliano-Meza, J. L., additional, Ruiz-Mendez, F., additional, Güemes-Castorena, D., additional, Meléndez-Alfaro, M., additional, Aldaco-Gastelum, A. N., additional, Castillo-Paz, A. A., additional, and Ramirez-Montoya, M. S., additional

Published
2023
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