cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5281/zenodo.2605357
title: Data for paper "Using synthetic semiochemicals to train canines to detect bark beetle-infested trees" in Ann For Sci

description: <strong>ESM_0</strong>      Photo. Entrainment of semiochemicals with Porapak <sup>® </sup>Q plug from cylinders used in stimuli delivery in dog training platform. (DOCX)

<strong>ESM_1</strong>      Fig. Educational scent platform. (PDF)<br>
<strong>ESM_2      </strong>Fig. Training platform stimuli layout and decline in response to no<br>
target scent. (PDF)<br>
<strong>ESM_3      </strong>Table. Evaluation of the dog detection performance as number of<br>
indications with decreasing amounts of scent molecules over time. (PDF)

<strong>ESM_4_V1</strong> Video. Educational scent platform in operation. (AVI)<br>
<strong>ESM_4_V2</strong> Video.<em> </em>Placement of cotton scent pad and the location of the scent by dog on a pine (a non-host tree of the beetle). (AVI)<br>
<strong>ESM_4_V3</strong> Video. The search, GPS tracking, and location of natural attacks.<em> </em>(AVI)<br>
<strong>ESM_4_V4</strong> Video. The search, location of two adjacent natural attacks, and rewarding. (AVI)

The dog detection allows timely removal by sanitation logging of first beetle-attacked trees before offspring emergence, preventing local beetle increases. Detection dogs rapidly learned responding to synthetic bark beetle pheromone components, with known chemical titres, allowing search training during winter in laboratory and field. Dogs trained on synthetics detected naturally attacked trees in summer at a distance of &gt;100 m.
description: This research was funded by two grants from "The Södra Foundation for Research, Development and Education", Växjö, Sweden to AJ. FS & GB was supported by the Linnaeus programme 'Insect Chemical Ecology, Ethology and Evolution' (IC-E3, #217-2006-1750) at SLU and later to FS ('Rapid olfactory detection of insect and fungal damage in forests', #2013-1583) both from "The Swedish Research Council Formas". FS was further supported by EXTEMIT-K project financed by OP RDE at Czech University of Life Sciences Prague (CZ.02.1.01/0.0/0.0/15-003/0000433).
DOI: 10.17632/fp7ky46yz3.1
title: Third molar development between ages 8 and 13 years

description: The model presented here has been fit to predict third molar development based on the mesiodistal length of the jaw space distal to the first permanent molar, while also controlling for age and jaw. Therefore, both upper and lower third molars are taken into account here. Sex was also a variable of interest in this investigation but, giving its lack of contribution for significantly predicting third molar development in our pilot tests, it was not kept in this final model. This model is the result of a study where 689 third molar regions were investigated on cone-beam computed tomography (CBCT) images of 179 Canadian children and adolescents aged 8.00 to 13.99 years.
DOI: 10.17632/fs473rtcky.1
title: Data for Manuscript Submitted to Journal of Geophysical Research - Solid Earth [Paper#2019JB017466R] Entitled " Magnetic Mineralogical Approach for Exploration of Gas Hydrates in the Bay of Bengal"

description: The data contains information on rockmagnetic, sedimentological, geochemical, geophysical, and mineralogical records of the sediment cores from Bay of Bengal. The data is uploaded for Manuscript Submitted to Journal of Geophysical Research - Solid Earth [Paper#2019JB017466R] Entitled " Magnetic Mineralogical Approach for Exploration of Gas Hydrates in the Bay of Bengal"
DOI: 10.17632/pdn62jgysj.1
title: Data for: 3361478

description: This is the software accompany the paper "Market Dynamics: On Directional Information Derived From (Time, Execution Price, Shares Traded) Transaction Sequences"
DOI: 10.17632/4w4ws2tsrp.2
title: Data For: Comparative Study of Radial Basis Function Neural Networks with Classification Methods for Urban Traffic Signal Control

description: This file contains the real-world vehicle arrivals to an isolated intersection. The first four columns represent vehicle arrivals to four lanes. The last four columns show adaptive green times for four lanes.
DOI: 10.17632/9rhscd27y4.1
title: UAV imagery and in-situ measurements for structure-from-motion snow depth mapping over the Laurichard rock glacier, France - surveyed in 2017

description: Unmanned aerial veichle (UAV) imagery and in-situ field measurements at the Combe de Laurichard, France (45.01ºN, 6.37ºE, 2500 m a.s.l.) were collected to explore uncertainties in mapping snow depth with structure-from-motion and multi-view stereo 3D reconstruction in an alpine area. Repeat UAV surveys were flown on each survey date to create multiple elevation models to determine the precision (i.e., repeatability) of SFM-MVS elevation models. This measure of uncertainty can be used to determine the precision of SFM-MVS snow depths using a model of error propagation. It also can illustrate how uncertainty in the SFM-MVS snow depths and elevation models vary spatially. The repeated snow-cover (snow-on) elevation models (6 in total) were acquired on June 1, 2017, and the snow-free (snow-off) elevation models (7 in total) on October 5, 2017. These elevation models were derived by performing SFM-MVS reconstruction using Agisoft PhotoScan. The UAV imagery was surveyed using a DJI Phantom 4, which flew in pre-programmed parallel flight paths with 75% side and top image overlap. The flying height of the UAV was approximately 60 m above ground level. Artificial targets were used for SFM camera calibration and georeferencing using the RGF93 / Lambert-93 projection and the NGF-IGN69 vertical datum (EPSG::5698). Validation data was collected by measuring topographic heights (i.e., check points) using a real-time-kinematic (RTK) global navigation satellite system (GNSS) survey with an accuracy &lt; 2 cm (at 1 σ). At each check point location, snow depths were measured using an avalanche probe to a maximum 3 m depth. This RTK-GNSS survey was also used for collecting ground control points (GCPs). The position of the base-station was corrected using the PUYA reference station, which is located approximately 19 km from the study area. Additionally, to compare the uncertainty of SFM-MVS snow depths in stable and active deforming terrain (i.e., rock glacier creep), a mask of the rock glacier area was mapped using the UAV derived imagery and elevation models.
DOI: 10.14455/nrct.img.2019.247
title: เพลงมโหรีกรุงศรีอยุธยา : การบันทึกแผ่นวีดิทัศน์พร้อมบทวิเคราะห์และโน้ตสากล (Ayutthaya’s   Series Song :   Recorded digital video disc (DVD) , Analytical Program Notes and Music Notaion.)
DOI: 10.14455/nrct.img.2019.249
title: รูปแบบการพัฒนาสมรรถนะด้านการจัดการเรียนการสอนของครูผู้สอนนักเรียนระดับปฐมวัยที่ใช้ภาษาไทยเป็นภาษาที่สองตามแนวคิดชุมชนแห่งการเรียนรู้ทางวิชาชีพครู
DOI: 10.14455/nrct.img.2019.250
title: การถ่ายทอดองค์ความรู้ทางการเกษตรเพื่อการพัฒนาด้านความมั่นคงในพื้นที่ชายแดนจังหวัดกาญจนบุรี
DOI: 10.14455/nrct.img.2019.253
title: การพัฒนาขั้นตอนวิธีในระบบตรวจจับการบุกรุกทางเครือข่ายด้วยเอดาบูทเอ็มวัน
DOI: 10.14455/nrct.img.2019.256
title: การพัฒนาผลิตภัณฑ์เพื่อเพิ่มขีดความสามารถในการแข่งขันของวิสาหกิจชุมชน ในจังหวัดมหาสารคาม
DOI: 10.14455/nrct.img.2019.259
title: แนวทางการส่งเสริม อนุรักษ์และพัฒนาซอบั้งชาวภูไท จังหวัดกาฬสินธุ์
DOI: 10.14455/nrct.img.2019.261
title: การออกแบบผลิตภัณฑ์จักสานไม้ไผ่โดยใช้ภูมิปัญญาท้องถิ่นวิสาหกิจชุมชนกลุ่มหัตถกรรมจักรสานพื้นบ้าน บ้านดงชะพลู ตำบลบางมะฝ่อ อำเภอโกรกพระ จังหวัดนครสวรรค์
DOI: 10.17632/cy8zywfhr3.1
title: Gender differences in the taste of food, the relationship with meals and eating habits.

description: Gender differences in the taste of food, the relationship with meals and eating habits.
DOI: 10.17632/8484k6yh2p.1
title: The PCA-RR based method for uncertainty quantification

description: This research data relates to the article of "A statistical parsimony method for uncertainty quantification of FDTD computation based on the PCA and ridge regression" All the data has been uploaded.
DOI: 10.21227/pkyn-0434
title: Alcohol Detection in Drivers by Sensors and Computer Vision

description: The present dataset is based on implementing of 3 approaches  with respect to the acquisition of driver data. The same one that we propose to use a sensor of concentration of alcohol in the environment (physiological), a sensor that measure the temperature of the defined points on driver’s face (biological) and another one that allows to identify and recognize the thickness of the pupil (visual characteristics). As a first approach, a gas detection sensor is implemented. The same one that seeks to reveal the presence of ethanol. The selected sensor is the MQ-3, due to its sensitivity to different gases and its rapid integration into the systems. As a second approach, we seek to determine the facial thermal change of the person. Since it has been proven that the temperature increases in the face of an alcoholic person , due to that the arteries and blood vessels increase their activity. The MLX90621 temperature sensor must determine this variations. The third approach used is that of visual characteristics. Because a person who consumes alcohol the iris becomes darker, which means that its temperature compared to the sclerotic decreases. This is because the sclera is full of blood vessels that increase the temperature with alcohol consumption. We use a Raspberry Pi Camera to acquire images to the pupil and find the their radio.
DOI: 10.25919/5c9c5733b34b0
title: Parkes observations for project P456 semester 2018OCTS_36

description: The Parkes Pulsar Timing Array (PPTA) project has three primary goals: (a) detection of gravitational waves from astronomical sources, (b) establishment of a pulsar timescale, and (c) improvement of our understanding of Solar-system dynamics. The PPTA is the oldest of three international pulsar timing groups. We have the smallest telescope and the smallest group, but the best measurements and the best results. Our bound on the strength of the incoherent gravitational wave background is the only bound which significantly constrains theoretical models. We have maintained our leading position because: we have the southern sky; we have a small but well-focussed group; we have the best-calibrated receivers; and we have been able to observe with an almost regular cadence of 15 to 20 days at three different wavelengths. With this proposal we aim to maintain our pre-eminent position in the field.

Unlike most observing proposals, this is a continuing proposal for which the observations will continue to improve bounds on ultra-low-frequency gravitational waves until they are finally detected. Continued Parkes observations will remain valuable at least until the first stage of the SKA is able to improve on our sensitivity and observing cadence. Even after the gravitational wave background is detected we will want to continue observations in support of the nascent field of gravitational wave astronomy!
DOI: 10.5517/ccdc.csd.cc217b3r
title: CCDC 1883873: Experimental Crystal Structure Determination

description: Related Article: Gonzalo Campillo-Alvarado, Changan Li, Dale C. Swenson, Leonard R. MacGillivray|2019|Cryst.Growth Des.|19|2511|doi:10.1021/acs.cgd.9b00035
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: 10.5517/ccdc.csd.cc217b4s
title: CCDC 1883874: Experimental Crystal Structure Determination

description: Related Article: Gonzalo Campillo-Alvarado, Changan Li, Dale C. Swenson, Leonard R. MacGillivray|2019|Cryst.Growth Des.|19|2511|doi:10.1021/acs.cgd.9b00035
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: 10.5517/ccdc.csd.cc217b5t
title: CCDC 1883875: Experimental Crystal Structure Determination

description: Related Article: Gonzalo Campillo-Alvarado, Changan Li, Dale C. Swenson, Leonard R. MacGillivray|2019|Cryst.Growth Des.|19|2511|doi:10.1021/acs.cgd.9b00035
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: 10.5517/ccdc.csd.cc217b6v
title: CCDC 1883876: Experimental Crystal Structure Determination

description: Related Article: Gonzalo Campillo-Alvarado, Changan Li, Dale C. Swenson, Leonard R. MacGillivray|2019|Cryst.Growth Des.|19|2511|doi:10.1021/acs.cgd.9b00035
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: 10.5517/ccdc.csd.cc217w8g
title: CCDC 1884405: Experimental Crystal Structure Determination

description: Related Article: Jin-Long Pan, Chang Liu, Chao Chen, Tuan-Qing Liu, Man Wang, Zhenliang Sun, Shu-Yu Zhang|2019|Org.Lett.|21|2823|doi:10.1021/acs.orglett.9b00812
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: 10.25919/5c9c58ecc489a
title: Parkes observations for project P455 semester 2018OCTS_08

description: This project is to continue timing and profile studies of the first double-pulsar system, a unique laboratory for gravitational physics. Recent results, including the first measurements of higher-order light-propagation effects and of the relativistic deformation of the orbit, highlight the importance of a long term observational campaign for this remarkable system. The main aims of this proposal are to provide the strongest tests to date for general relativity and to measure for the first time the moment-of-inertia of a neutron star. Additionally, we will determine the system geometry and map the pulsar beams via geodetic precession. Whenever possible, we will exploit the high sensitivity of the new UWL receiver.
DOI: 10.25919/5c9c59dee1ca5
title: Parkes observations for project P456 semester 2018OCTS_38

description: The Parkes Pulsar Timing Array (PPTA) project has three primary goals: (a) detection of gravitational waves from astronomical sources, (b) establishment of a pulsar timescale, and (c) improvement of our understanding of Solar-system dynamics. The PPTA is the oldest of three international pulsar timing groups. We have the smallest telescope and the smallest group, but the best measurements and the best results. Our bound on the strength of the incoherent gravitational wave background is the only bound which significantly constrains theoretical models. We have maintained our leading position because: we have the southern sky; we have a small but well-focussed group; we have the best-calibrated receivers; and we have been able to observe with an almost regular cadence of 15 to 20 days at three different wavelengths. With this proposal we aim to maintain our pre-eminent position in the field.

Unlike most observing proposals, this is a continuing proposal for which the observations will continue to improve bounds on ultra-low-frequency gravitational waves until they are finally detected. Continued Parkes observations will remain valuable at least until the first stage of the SKA is able to improve on our sensitivity and observing cadence. Even after the gravitational wave background is detected we will want to continue observations in support of the nascent field of gravitational wave astronomy!
DOI: 10.17632/ntx8swxs38.1
title: Data for: Holocene variations in North Atlantic export productivity as reflected in bathyal benthic foraminifera

description: Smart et al. Benthic foraminifera (&gt;63 µm) counts - ODP-162-980B (Holocene)
DOI: 10.25919/5c9c5b7ac133c
title: Parkes observations for project P456 semester 2018OCTS_37

description: The Parkes Pulsar Timing Array (PPTA) project has three primary goals: (a) detection of gravitational waves from astronomical sources, (b) establishment of a pulsar timescale, and (c) improvement of our understanding of Solar-system dynamics. The PPTA is the oldest of three international pulsar timing groups. We have the smallest telescope and the smallest group, but the best measurements and the best results. Our bound on the strength of the incoherent gravitational wave background is the only bound which significantly constrains theoretical models. We have maintained our leading position because: we have the southern sky; we have a small but well-focussed group; we have the best-calibrated receivers; and we have been able to observe with an almost regular cadence of 15 to 20 days at three different wavelengths. With this proposal we aim to maintain our pre-eminent position in the field.

Unlike most observing proposals, this is a continuing proposal for which the observations will continue to improve bounds on ultra-low-frequency gravitational waves until they are finally detected. Continued Parkes observations will remain valuable at least until the first stage of the SKA is able to improve on our sensitivity and observing cadence. Even after the gravitational wave background is detected we will want to continue observations in support of the nascent field of gravitational wave astronomy!
DOI: 10.25912/5c9c5f3aa44f8
title: REACH Project: Hand hygiene data
DOI: 10.25919/5c9c5e4a45783
title: Parkes observations for project P996 semester 2018OCTS_23

description: We propose to measure the polarisation of ~200 pulsars (~100 this semester) using the Ultra-Wideband Low (UWL) receiver to investigate the structure of the Galactic disk magnetic field in and between distant spiral arms. Previous Parkes pulsar observations have revealed field reversals in nearby arm and interarm regions. We wish to exploit the greater sensitivity of the UWL receiver to extend this to more distant regions, thereby allowing us to distinguish more clearly between different models for the structure of the disk field. This work will have important implications for theories for the generation of Galactic magnetic fields and for other areas, e.g., cosmic-ray physics, which depend on a knowledge of the large-scale Galactic magnetic field for their interpretation.
DOI: 10.25919/5c9c5f04e9f50
title: Parkes observations for project P789 semester 2018OCTS_16

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, we 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.
DOI: 10.5517/ccdc.csd.cc1zfwdp
title: CCDC 1830593: Experimental Crystal Structure Determination

description: Related Article: Shivaiah Vaddypally, Warren Tomlinson, Owen T. O’Sullivan, Ran Ding, Megan M. Van Vliet, Bradford B. Wayland, Joseph P. Hooper, Michael J. Zdilla|2019|J.Am.Chem.Soc.|141|5699|doi:10.1021/jacs.8b10250
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: 10.5517/ccdc.csd.cc1zfwfq
title: CCDC 1830594: Experimental Crystal Structure Determination

description: Related Article: Shivaiah Vaddypally, Warren Tomlinson, Owen T. O’Sullivan, Ran Ding, Megan M. Van Vliet, Bradford B. Wayland, Joseph P. Hooper, Michael J. Zdilla|2019|J.Am.Chem.Soc.|141|5699|doi:10.1021/jacs.8b10250
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: 10.5281/zenodo.2613425
title: A narrative synthesis analysis of lifecourse domains within health service utilisation frameworks

description: This paper is a scoping review which identifies existing frameworks, other than Anderson's Behavioural model, that look at Health Service Utilisation (HSU). In addition it investigates if these frameworks incorporate the use of a life course approach to understand HSU.

The data included in this repository is:

1. PRISMA flowchart

2. PRISMA-ScR scoping review checklist

3. Spreadsheet which contains all 70 frameworks (Table 6)

4. References for the 70 Frameworks in Table6.
DOI: 10.5517/ccdc.csd.cc1zfwgr
title: CCDC 1830595: Experimental Crystal Structure Determination

description: Related Article: Shivaiah Vaddypally, Warren Tomlinson, Owen T. O’Sullivan, Ran Ding, Megan M. Van Vliet, Bradford B. Wayland, Joseph P. Hooper, Michael J. Zdilla|2019|J.Am.Chem.Soc.|141|5699|doi:10.1021/jacs.8b10250
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: 10.5517/ccdc.csd.cc1zjwr4
title: CCDC 1833487: Experimental Crystal Structure Determination

description: Related Article: Anders Reinholdt, Sean H. Majer, Rikke M. Gelardi, Samantha N. MacMillan, Anthony F. Hill, Ola F. Wendt, Kyle M. Lancaster, Jesper Bendix|2019|Inorg.Chem.|58|4812|doi:10.1021/acs.inorgchem.8b03222
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: 10.5517/ccdc.csd.cc21byfs
title: CCDC 1887355: Experimental Crystal Structure Determination

description: Related Article: Liping Zhu, Jiale Xiong, Junkai An, Nannan Chen, Jijun Xue, Xianxing Jiang|2019|Org.Biomol.Chem.|17|3797|doi:10.1039/C9OB00172G
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.