cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.1285/i24995835v2016n4p29
title: Dal computational thinking al systemic learning

description: Le tecnologie dell'informazione e della comunicazione (TIC) sono portatrici di un cambiamento trasformazionale della società. Per una società sostenibile è necessario, però, trasformare il modo di pensare oltre che quello di ordinare, conservare e interagire con l'informazione. I professionisti della computer science  (CS) hanno già un kit di strumenti concettuali finalizzati alla soluzione dei loro problemi. Questo kit, a volte, viene definito genericamente come "pensiero computazionale". Il pensiero computazionale, però, tende a vedere il mondo in termini di una serie di problemi (o di problemi-tipo) che hanno soluzioni computazionali o comunque possono essere ricondotti a modelli risolutivi noti. In questo lavoro, si cerca di argomentare a sostengo di una  idea di ponte necessario che unisca il pensiero computazionale alla pratica della sostenibilità. La sostenibilità, intesa in senso sistemico, è un approccio che consente di riconoscere la stretta interrelazione-interdipendenza tra tecnologia, comportamento umano e ambiente. Nelle pagine che seguono si cercherà di sviluppare, sia pure come abbozzo, una idea che fornisca una ontologia regionale pedagogica della relazione sostenibile tra comunità, ambiente e tecnologie ("mereologia" Putnam, Varzi Ferraris). In  particolare si indagheranno alcune questioni sollevate dal computational thinking (CT) nell'ambito dello sviluppo delle intelligenze.
description: The information and communication technologies (ICT) are the bearers of a transformational change in society. For a sustainable society is necessary, however, to transform the way we think as well as what to order, store and interact with information. The professionals of computer science (CS) already have a conceptual tool kit aimed at the solution of their problems. This kit, at times, is defined generically as "computational thinking". The computational thinking, however, tends to see the world in terms of a number of problems (or problems-type) that have computational solutions or however can be traced to known model solutions. In this paper, we try to argue in support of an idea of  necessary bridge that unites computational thinking to the practice of sustainability. Sustainability, understood in a systemic way, it's an approach that allows you to recognize the close inter-interdependence between technology, human behavior and the environment. In the following pages we will try to develop, even as a sketch, an idea that provides a pedagogical regional ontology of the sustainable relationship between the community, the environment and technology ("mereology" Putnam, Varzi Ferraris). In particular we will investigate some of the issues raised by the computational thinking (CT) in the development of intelligence.
DOI: 10.1285/i24995835v2016n4p3
title: Indice
DOI: 10.1285/i24995835v2016n4p7
title: La didattica inclusiva per studenti con disabilità sensoriali: fra multisensorialità, tecnologie e vicarianza

description: La presenza in classe di bambini sordi e ciechi sollecita un'importante riflessione circa le risorse e le modalità da attivare per rendere i contesti scolastici inclusivi. Information and Communication Technologies, accessibilità, autonomia, vicarianza, multimodalità e multisensorialità rappresentano i punti cardine di una didattica inclusiva per studenti con disabilità sensoriali.
description: The presence of deaf and blind children in class raises a significant reflection about the resources and methods to make inclusive the educational contexts. Information and Communication Technologies, accessibility, autonomy, vicariance, multimodality and multisensoriality, represent the key points of an inclusive education for students with sensorial disabilities.
DOI: 10.14457/cu.the.2007.1074
title: ภาระภาษีที่อยู่อาศัยที่มีผลต่อผู้มีรายได้น้อย เมื่อมีการประกาศใช้ร่างพระราชบัญญัติภาษีที่ดินและสิ่งปลูกสร้างใหม่ : กรณีศึกษาผู้มีรายได้น้อยในชุมชนวัดตึก จังหวัดสมุทรสาคร /
DOI: 10.14457/kmutt.res.2002.46
title: ผลของซัลเฟตต่อประสิทธิภาพการทำงานของถังปฏิกรณ์แบบไม่ใช้อากาศ /
DOI: 10.14457/kmutt.res.2002.47
title: ผลของชนิดตะกอนเริ่มต้นต่อการสร้างตะกอนเม็ด ในระบบยูเอเอสบีที่บำบัดน้ำเสียที่มีโปรตีนเป็นองค์ประกอบหลัง /
DOI: 10.14457/cu.the.2007.1067
title: การสังเคราะห์งานวิจัยด้านการจัดการเรียนการสอนแบบบูรณาการ : การวิเคราะห์อภิมานและการวิเคราะห์เนื้อหา /
DOI: 10.14457/kmutt.res.2003.77
title: ผลของชนิดตะกอนเริ่มต้นต่อการสร้างตะกอนเม็ด ของระบบบำบัดแบบยูเอเอสบีที่บำบัดน้ำเสียเลือดไก่เจือจาง /
DOI: 10.4225/08/58dd14c067929
title: Parkes observations for project P887 semester 2015APRS

description: Searches for radio pulsations from Fermi sources have been astonishingly fruitful, both in discovering new pulsars and in probing the physics of high-energy emission.  We propose observations of members of two promising Fermi source classes: (1) candidate enshrouded millisecond pulsars (2) new "blind search" gamma-ray pulsars.  The former are fascinating systems in which the wind of an energetic recycled millisecond pulsar is disintegrating its companion; detecting pulsations turns them into laboratories for this process.  The latter are pulsars recently discovered in computational tour de force trawls of the Fermi data.  Radio pulsations greatly add to the information we can obtain; conversely, deep upper limits constrain emission models.
DOI: 10.14457/cu.the.2007.1066
title: การประมาณแบนด์วิดท์แบบปรับตัวได้ ของทีซีพีเพื่อควบคุมความคับคั่ง ในอินเทอร์เน็ตผ่านดาวเทียม /
DOI: 10.14457/cu.the.2007.1075
title: ความสัมพันธ์ระหว่างการจัดหน้าหนึ่งของหนังสือพิมพ์ และหนังสือพิมพ์ออนไลน์ และการรับรู้ลำดับความสำคัญของข่าว และการเลือกเปิดรับข่าว /
DOI: 10.4225/08/58dd1039ec3a0
title: Parkes observations for project P858 semester 2015APRS13

description: SUPERB is a large-scale survey for pulsars and extragalactic radio bursts. It will uses optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The pulsars discovered will enable studies of the interstellar medium, allow us to more accurately constrain the MSP luminosity function (which informs estimates of the SKA yield of MSPs), tests of theories of gravity and several will contribute to the precision timing projects of the PPTA. The FRBs discovered will have much more associated information than all previous detections. Firstly the discovery lag will be ~1 second, rather than months/years. The Parkes observations will be shadowed by the Molonglo telescope to allow, for the first time, localisation of FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors. The survey will discover ~20 MSPs, ~100 slower pulsars and ~10 FRBs.
DOI: 10.14457/cu.the.2007.1068
title: การจัดเรียงตัวของกลุ่มหุ่นยนต์แบบต่างชนิด /
DOI: 10.14457/kmutt.res.2004.60
title: ผลของชนิดตะกอนต่อการสร้างตะกอนเม็ดของระบบยูเอเอสบี ที่บำบัดน้ำเสียจากโรงงานผลไม้อบแห้ง /
DOI: 10.4225/08/58dd100f201b4
title: Parkes observations for project P858 semester 2015APRS10

description: SUPERB is a large-scale survey for pulsars and extragalactic radio bursts. It will uses optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The pulsars discovered will enable studies of the interstellar medium, allow us to more accurately constrain the MSP luminosity function (which informs estimates of the SKA yield of MSPs), tests of theories of gravity and several will contribute to the precision timing projects of the PPTA. The FRBs discovered will have much more associated information than all previous detections. Firstly the discovery lag will be ~1 second, rather than months/years. The Parkes observations will be shadowed by the Molonglo telescope to allow, for the first time, localisation of FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors. The survey will discover ~20 MSPs, ~100 slower pulsars and ~10 FRBs.
DOI: 10.4225/08/58dd104757bc0
title: Parkes observations for project P858 semester 2015APRS14

description: SUPERB is a large-scale survey for pulsars and extragalactic radio bursts. It will uses optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The pulsars discovered will enable studies of the interstellar medium, allow us to more accurately constrain the MSP luminosity function (which informs estimates of the SKA yield of MSPs), tests of theories of gravity and several will contribute to the precision timing projects of the PPTA. The FRBs discovered will have much more associated information than all previous detections. Firstly the discovery lag will be ~1 second, rather than months/years. The Parkes observations will be shadowed by the Molonglo telescope to allow, for the first time, localisation of FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors. The survey will discover ~20 MSPs, ~100 slower pulsars and ~10 FRBs.
DOI: 10.4225/08/58dd106418568
title: Parkes observations for project P858 semester 2015APRS16

description: SUPERB is a large-scale survey for pulsars and extragalactic radio bursts. It will uses optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The pulsars discovered will enable studies of the interstellar medium, allow us to more accurately constrain the MSP luminosity function (which informs estimates of the SKA yield of MSPs), tests of theories of gravity and several will contribute to the precision timing projects of the PPTA. The FRBs discovered will have much more associated information than all previous detections. Firstly the discovery lag will be ~1 second, rather than months/years. The Parkes observations will be shadowed by the Molonglo telescope to allow, for the first time, localisation of FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors. The survey will discover ~20 MSPs, ~100 slower pulsars and ~10 FRBs.
DOI: 10.4225/08/58dd14d896ea5
title: Parkes observations for project P858 semester 2015APRS_BPSR_42

description: SUPERB is a large-scale survey for pulsars and extragalactic radio bursts. It will uses optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The pulsars discovered will enable studies of the interstellar medium, allow us to more accurately constrain the MSP luminosity function (which informs estimates of the SKA yield of MSPs), tests of theories of gravity and several will contribute to the precision timing projects of the PPTA. The FRBs discovered will have much more associated information than all previous detections. Firstly the discovery lag will be ~1 second, rather than months/years. The Parkes observations will be shadowed by the Molonglo telescope to allow, for the first time, localisation of FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors. The survey will discover ~20 MSPs, ~100 slower pulsars and ~10 FRBs.
DOI: 10.4225/08/58dd0f9eacea4
title: Parkes observations for project P789 semester 2015APRS

description: Recently there has been great success at Parkes discovering millisecond pulsars (MSPs), a class that includes some of the most interesting and scientifically valuable pulsars known. In the last few years we have discovered more than 40 MSPs though the High Time Resolution Universe Survey (P630) and Fermi searches (P675/P814). Here we propose to carry out precision timing of these sources to fully exploit these discoveries. Additionally, continue to study the most significant of the discoveries from the Parkes Multibeam Pulsar Survey (P268). 
To maximise scientific impact we have combined the most important sources from various previous proposals into this project, reducing total observation time required and easing the burden on the scheduler.
This project also makes use of all beams of the 21-cm receiver to search for transient radio burst of extragalactic origin at the same time as performing timing observations.
DOI: 10.4225/08/58dd1077ddb24
title: Parkes observations for project P858 semester 2015APRS17

description: SUPERB is a large-scale survey for pulsars and extragalactic radio bursts. It will uses optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The pulsars discovered will enable studies of the interstellar medium, allow us to more accurately constrain the MSP luminosity function (which informs estimates of the SKA yield of MSPs), tests of theories of gravity and several will contribute to the precision timing projects of the PPTA. The FRBs discovered will have much more associated information than all previous detections. Firstly the discovery lag will be ~1 second, rather than months/years. The Parkes observations will be shadowed by the Molonglo telescope to allow, for the first time, localisation of FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors. The survey will discover ~20 MSPs, ~100 slower pulsars and ~10 FRBs.
DOI: 10.4225/08/58dd14cc84fc1
title: Parkes observations for project P858 semester 2015APRS_BPSR_43

description: SUPERB is a large-scale survey for pulsars and extragalactic radio bursts. It will uses optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The pulsars discovered will enable studies of the interstellar medium, allow us to more accurately constrain the MSP luminosity function (which informs estimates of the SKA yield of MSPs), tests of theories of gravity and several will contribute to the precision timing projects of the PPTA. The FRBs discovered will have much more associated information than all previous detections. Firstly the discovery lag will be ~1 second, rather than months/years. The Parkes observations will be shadowed by the Molonglo telescope to allow, for the first time, localisation of FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors. The survey will discover ~20 MSPs, ~100 slower pulsars and ~10 FRBs.
DOI: 10.14457/kmutnb.the.1993.2
title: การประเมินผลการให้บริการแก่ชุมชนของกลุ่มอาชีวศึกษาจังหวัดเลย /
DOI: 10.14457/kmutnb.the.1993.3
title: สมรรถภาพทางวิชาชีพของช่างเทคนิค สาขาอิเล็กทรอนิกส์ ตามทัศนะของผู้บริหารสถานประกอบการอุตสาหกรรมอิเล็กทรอนิกส์ เพื่อการส่งออก /
DOI: 10.14457/kmutt.res.2002.48
title: ผลของชนิดตะกอนเริ่มต้นต่อการสร้างตะกอนเม็ด ในระบบยูเอเอสบีที่บำบัดน้ำเสียคาร์โบไฮเดรต /
DOI: 10.14457/kmutt.res.2008.101
title: ผลของชนิดถังปฏิกรณ์ต่อประสิทธิภาพการผลิตก๊าซชีวภาพ จากกากตะกอนโรงงานสกัดน้ำมันปาล์ม /
DOI: 10.4225/08/58dd110419a87
title: Parkes observations for project P858 semester 2015APRS_BPSR_53

description: SUPERB is a large-scale survey for pulsars and extragalactic radio bursts. It will uses optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The pulsars discovered will enable studies of the interstellar medium, allow us to more accurately constrain the MSP luminosity function (which informs estimates of the SKA yield of MSPs), tests of theories of gravity and several will contribute to the precision timing projects of the PPTA. The FRBs discovered will have much more associated information than all previous detections. Firstly the discovery lag will be ~1 second, rather than months/years. The Parkes observations will be shadowed by the Molonglo telescope to allow, for the first time, localisation of FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors. The survey will discover ~20 MSPs, ~100 slower pulsars and ~10 FRBs.
DOI: 10.4225/08/58dd111f47cda
title: Parkes observations for project P427 semester 2015APRS

description: Timing of the dozen pulsars discovered in six globular clusters by us in the framework of P303 and timed in the context of P427 has ensured high quality results, which have been reported in several papers, three more of which are in preparation.  We now propose to continue our timing project, performing a small number of visits to the six globular clusters, in order to measure higher order derivatives of the rotational and/or of the orbital parameters of the pulsars and to safely keep coherence in the timing solutions. With a very limited investment of additional telescope time, that will enable studying some poorly constrained aspects of the inner dynamics of the observed globular clusters, as well as providing the ephemeris for the best possible searches for gamma-ray and/or gravitational wave emission from the targeted pulsars.
DOI: 10.5061/dryad.g9k46/1
title: Supplementary results S1-S21

description: Supplementary results and figures S1-S21 for Evaluating the accuracy of biodiversity changes through geological times: from simulation to solution
DOI: 10.5061/dryad.g9k46/2
title: R function. Evaluating the accuracy of biodiversity changes through geological times

description: Based on a presence/absence matrix, the function allows the back-transformation of this discretized dataset into a reconstructed continuous-time dataset. The function generates plots of taxonomic richness and Foote’s taxonomic rates variation through time and a list of the 3 different (richness, origination p rate and extinction q rate) datasets and the associated 95 % confidence interval.
DOI: 10.5281/zenodo.439334
title: Data For "Using Transmission Kikuchi Diffraction To Characterise Alpha Variants In An Alpha+Beta Titanium Alloy"

description: This zipped folder contains data for "Using transmission Kikuchi diffraction to characterise alpha variants in an alpha+beta titanium alloy" published in Journal of Microscopy.

The zipped folder contains:<br>
- Phase map, where green regions are indexed as alpha Ti and red regions are indexed as beta Ti.<br>
- IPF orientation maps along the X, Y and Z directions (with both phases combined).<br>
- IPF colour keys for the alpha and beta phases.<br>
- FSD micrographs at lower and higher magnification (not resized: one pixel per acquisition data point).<br>
- TKD_Trial.ctf - text file describing orientations according to Bruker software conventions [1], as-exported from Bruker Esprit 2.1.<br>
- TKD_BOR_MTEXplotter.m, an MTEX  plotting tool which will plot orientations for this dataset (using MTEX version 4.3.2 installed on MATLAB 9.2 (R2017a)).

[1] T.B. Britton, J. Jiang, Y. Guo, A. Vilalta-Clemente, D. Wallis, L.N. Hansen, A. Winkelmann, A.J. Wilkinson, Tutorial: Crystal orientations and EBSD — Or which way is up?, Materials Characterization, Volume 117, July 2016, Pages 113-126, ISSN 1044-5803, http://dx.doi.org/10.1016/j.matchar.2016.04.008.<br>
(http://www.sciencedirect.com/science/article/pii/S1044580316300924)
DOI: 10.5517/ccdc.csd.cc1nr3tb
title: CCDC 1541562: Experimental Crystal Structure Determination

description: Related Article: Jan Grzegorz Malecki|2017|CSD Communication|||
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.14457/kmutnb.the.1993.4
title: ปัญหาและอุปสรรคด้านปัจจัยพื้นฐานของอุตสาหกรรมเสื้อผ้าสำเร็จรูปขนาดย่อมและขนาดกลาง /
DOI: 10.14457/kmutt.res.2004.61
title: ผลของจังหวะการฉีดเชื้อเพลิงต่อสมรรถนะและการปลดปล่อยมลพิษของเครื่องยนต์ดีเซล 6 สูบที่ใช้เชื้อเพลิงเอทิลเอสเทอร์ผสมดีเซล /
DOI: 10.14457/kmutt.res.2007.43
title: ผลของตะกอนจุลินทรีย์ ต่อประสิทธิภาพของระบบบำบัดน้ำเสียแบบเอสบีอาร์ ในการบำบัดน้ำเสียจากโรงงานชุบโลหะ /
DOI: 10.14457/kmutt.the.2007.484
title: ผลของชนิดถังปฏิกรณ์ต่อการย่อยสลายกากมันสำปะหลังแบบไร้อากาศ /
DOI: 10.3886/e100408v3
title: Geocoordinates of ATMs in Mexico

description: This data set contains the geocoordinates of all ATMs in Mexico. The data set is saved in .csv format for maximum compatibility, and has three columns:<br>1) Latitude<br>2) Longitude<br>3) Bank name<br><br>This material is based upon work supported by the National Science Foundation under Grant Number 1530800. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the National Science Foundation.<br><br><br>
DOI: 10.4225/08/58dd0fe48137b
title: Parkes observations for project P858 semester 2015APRS07

description: SUPERB is a large-scale survey for pulsars and extragalactic radio bursts. It will uses optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The pulsars discovered will enable studies of the interstellar medium, allow us to more accurately constrain the MSP luminosity function (which informs estimates of the SKA yield of MSPs), tests of theories of gravity and several will contribute to the precision timing projects of the PPTA. The FRBs discovered will have much more associated information than all previous detections. Firstly the discovery lag will be ~1 second, rather than months/years. The Parkes observations will be shadowed by the Molonglo telescope to allow, for the first time, localisation of FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors. The survey will discover ~20 MSPs, ~100 slower pulsars and ~10 FRBs.