cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.21227/hk13-dj64
title: Corona Virus (COVID-19) Tweets Dataset

description: Tweets Counter: 13,419,667This dataset includes CSV files which contain the tweet IDs. The tweets have been collected by the LSTM model deployed here at sentiment.live. The model monitors the real-time Twitter feed for corona virus-related tweets. As per the Twitter Developer Policy, it is not possible for me to provide information other than the Tweet IDs (this dataset has been completely re-designed on March 20, 2020, to comply with data sharing policies set by Twitter). Note: This dataset should be solely used for non-commercial research purpose (ignore every other LICENSE category given in this page).Schema of the CSV files: First column: tweet ID, Second column: Sentiment score for the particular tweet.Files details (time: GMT+5:45):corona_tweets_01.csv: 831,327 tweets (March 20, 2020 01:37 AM - March 20, 2020 10:28 AM)corona_tweets_02.csv: 870,924 tweets (March 20, 2020 10:31 AM - March 20, 2020 09:43 PM)corona_tweets_03.csv: 773,729 tweets (March 20, 2020 09:49 PM - March 21, 2020 09:25 AM)corona_tweets_04.csv: 1,233,340 tweets (March 21, 2020 09:27 AM - March 22, 2020 07:46 AM)corona_tweets_05.csv: 1,782,157 tweets (March 22, 2020 07:50 AM - March 23, 2020 09:08 AM)corona_tweets_06.csv: 1,771,295 tweets (March 23, 2020 09:11 AM - March 24, 2020 11:35 AM)corona_tweets_07.csv: 1,479,651 tweets (March 24, 2020 11:42 AM - March 25, 2020 11:43 AM)corona_tweets_08.csv: 1,272,592 tweets (March 25, 2020 11:47 AM - March 26, 2020 12:46 PM)corona_tweets_09.csv: 1,091,429 tweets (March 26, 2020 12:51 PM - March 27, 2020 11:53 AM)corona_tweets_10.csv: 1,172,013 tweets (March 27, 2020 11:56 AM - March 28, 2020 01:59 PM)corona_tweets_11.csv: 1,141,210 tweets (March 28, 2020 02:03 PM - March 29, 2020 04:01 PM)----- March 29, 2020 04:05 PM - March 30, 2020 12:30 PM -- Some folk(s) messed around with the server. Tweets for this period won't be available. However, I'll be continuing adding the new Tweet IDs. Some preventive measures have been taken. Sorry for the inconvenience. -----corona_tweets_12.csv: 793,417 tweets. (March 30, 2020 02:01 PM - March 31, 2020 10:16 AM)To make it easy for the NLP researchers to get access to the sentiment analysis of each collected tweet, the sentiment score out of TextBlob [1] has been appended as the second column. New databases will be added to this dataset every day. Bookmark this page for further updates. [1] https://textblob.readthedocs.io/en/dev/
DOI: 10.14457/tu.the.2008.692
title: การศึกษาสมบัติของเมมเบรนไคโตซานต่อกิ่งด้วยโพลิไวนิล แอลกอฮอล์เพื่อใช้สำหรับเซลล์เชื้อเพลิงแบบใช้เมทานอลโดยตรง
DOI: 10.14457/tu.the.2008.693
title: การนำแนวคิด balanced scorecard มาใช้เพื่อวัดผลการทำงานในองค์การ : ศึกษาเฉพาะกรณีธนาคารกรุงไทย จำกัด (มหาชน) สาขาท่าเตียน
DOI: 10.21227/29yp-n159
title: free dataset from news/message boards/blogs about CoronaVirus (4 month of data - 5.2M posts)

description: Free dataset from news/message boards/blogs about CoronaVirus (4 month of data - 5.2M posts). The time frame of the data is Dec/2019 - March/2020. The posts are in English mentioning at least one of the following: "Covid" OR CoronaVirus OR "Corona Virus".
DOI: 10.21227/kc4v-q323
title: free dataset from news/message boards/blogs about CoronaVirus (4 month of data - 5.2M posts)

description: Free dataset from news/message boards/blogs about CoronaVirus (4 month of data - 5.2M posts). The time frame of the data is Dec/2019 - March/2020. The posts are in English mentioning at least one of the following: "Covid" OR CoronaVirus OR "Corona Virus".
DOI: 10.14272/xfrikhrkyhjntp-uhfffaoysa-n.1
title: methyl 4-[1-hydroxy-2-(4-methoxycarbonylphenyl)-2-oxoethyl]benzoate
title: InChI=1S/C18H16O6/c1-23-17(21)13-7-3-11(4-8-13)15(19)16(20)12-5-9-14(10-6-12)18(22)24-2/h3-10,15,19H,1-2H3

description: This dataset contains experimental data from a sample (methyl 4-[1-hydroxy-2-(4-methoxycarbonylphenyl)-2-oxoethyl]benzoate, InChI=1S/C18H16O6/c1-23-17(21)13-7-3-11(4-8-13)15(19)16(20)12-5-9-14(10-6-12)18(22)24-2/h3-10,15,19H,1-2H3). The datasets from the following experiments are available: 1H nuclear magnetic resonance spectroscopy (1H NMR) 13C nuclear magnetic resonance spectroscopy (13C NMR) mass spectrometry (MS) infrared absorption spectroscopy (IR)
DOI: 10.14272/xfrikhrkyhjntp-uhfffaoysa-n/chmo0000470
title: mass spectrometry (MS) (methyl 4-[1-hydroxy-2-(4-methoxycarbonylphenyl)-2-oxoethyl]benzoate)
title: InChI=1S/C18H16O6/c1-23-17(21)13-7-3-11(4-8-13)15(19)16(20)12-5-9-14(10-6-12)18(22)24-2/h3-10,15,19H,1-2H3

description: dataset for mass spectrometry (MS) MS-FAB (m/z, 3-NBA): 329 [M + H]+, 311 [M – OH]+, 297 [C17H13O5]+; HRMS–FAB (m/z): [M + H]+ calcd for C18H17O6, 329.1025; found, 329.1026.
DOI: 10.14272/xfrikhrkyhjntp-uhfffaoysa-n/chmo0000593
title: 1H nuclear magnetic resonance spectroscopy (1H NMR) (methyl 4-[1-hydroxy-2-(4-methoxycarbonylphenyl)-2-oxoethyl]benzoate)
title: InChI=1S/C18H16O6/c1-23-17(21)13-7-3-11(4-8-13)15(19)16(20)12-5-9-14(10-6-12)18(22)24-2/h3-10,15,19H,1-2H3

description: dataset for 1H nuclear magnetic resonance spectroscopy (1H NMR) 1H NMR (300 MHz, CDCl3, ppm) δ = 8.08–8.01 (m, 2H, Car.H), 8.01–7.95 (m, 2H, Car.H), 7.95–7.88 (m, 2H, Car.H), 7.44–7.35 (m, 2H, Car.H), 6.01 (br s, 1H, CHOH), 4.55 (br s, 1H, CHOH), 3.91 (s, 3H, COOCH3), 3.87 (s, 3H, COOCH3).
DOI: 10.14272/xfrikhrkyhjntp-uhfffaoysa-n/chmo0000595
title: 13C nuclear magnetic resonance spectroscopy (13C NMR) (methyl 4-[1-hydroxy-2-(4-methoxycarbonylphenyl)-2-oxoethyl]benzoate)
title: InChI=1S/C18H16O6/c1-23-17(21)13-7-3-11(4-8-13)15(19)16(20)12-5-9-14(10-6-12)18(22)24-2/h3-10,15,19H,1-2H3

description: dataset for 13C nuclear magnetic resonance spectroscopy (13C NMR) 13C NMR (75 MHz, CDCl3, ppm) δ = 198.4 (Cq, 1C, CO), 166.5 (Cq, 1C, COOCH3), 165.9 (Cq, 1C, COOCH3), 143.1 (Cq, 1C, Car.), 136.7 (Cq, 1C, Car.), 134.9 (Cq, 1C, Car.), 130.7 (Cq, 1C, Car.), 130.6 (+, 2C, Car.H), 130.0 (+, 2C, Car.H), 129.1 (+, 2C, Car.H), 127.9 (+, 2C, Car.H), 76.3 (+, 1C, CHOH), 52.7 (+, 1C, COOCH3), 52.4 (+, 1C, COOCH3).
DOI: 10.14272/xfrikhrkyhjntp-uhfffaoysa-n/chmo0000630
title: infrared absorption spectroscopy (IR) (methyl 4-[1-hydroxy-2-(4-methoxycarbonylphenyl)-2-oxoethyl]benzoate)
title: InChI=1S/C18H16O6/c1-23-17(21)13-7-3-11(4-8-13)15(19)16(20)12-5-9-14(10-6-12)18(22)24-2/h3-10,15,19H,1-2H3

description: dataset for infrared absorption spectroscopy (IR) IR (ATR, ṽ) = 3462, 3432, 2955, 1720, 1679, 1609, 1572, 1438, 1415, 1405, 1387, 1310, 1276, 1247, 1186, 1108, 1095, 1018, 983, 963, 881, 863, 836, 815, 766, 721, 703, 687, 636, 615, 535, 513, 497, 483 cm–1.
DOI: 10.14272/pclyikbmkkhymd-uhfffaoysa-n.1
title: methyl 4-[2-(4-methoxycarbonylphenyl)-2-oxoacetyl]benzoate
title: InChI=1S/C18H14O6/c1-23-17(21)13-7-3-11(4-8-13)15(19)16(20)12-5-9-14(10-6-12)18(22)24-2/h3-10H,1-2H3

description: This dataset contains experimental data from a sample (methyl 4-[2-(4-methoxycarbonylphenyl)-2-oxoacetyl]benzoate, InChI=1S/C18H14O6/c1-23-17(21)13-7-3-11(4-8-13)15(19)16(20)12-5-9-14(10-6-12)18(22)24-2/h3-10H,1-2H3). The datasets from the following experiments are available: infrared absorption spectroscopy (IR) 1H nuclear magnetic resonance spectroscopy (1H NMR) 13C nuclear magnetic resonance spectroscopy (13C NMR) mass spectrometry (MS)
DOI: 10.14272/pclyikbmkkhymd-uhfffaoysa-n/chmo0000470
title: mass spectrometry (MS) (methyl 4-[2-(4-methoxycarbonylphenyl)-2-oxoacetyl]benzoate)
title: InChI=1S/C18H14O6/c1-23-17(21)13-7-3-11(4-8-13)15(19)16(20)12-5-9-14(10-6-12)18(22)24-2/h3-10H,1-2H3

description: dataset for mass spectrometry (MS) EI (m/z, 70 eV, 140 °C): 326 (5) [M]+, 295 (4) [M – OCH3]+, 163.1 (100) [C9H7O3]+; HRMS–EI (m/z): [M]+ calcd for C18H14O6, 326.0790; found, 326.0790.
DOI: 10.14272/pclyikbmkkhymd-uhfffaoysa-n/chmo0000593
title: 1H nuclear magnetic resonance spectroscopy (1H NMR) (methyl 4-[2-(4-methoxycarbonylphenyl)-2-oxoacetyl]benzoate)
title: InChI=1S/C18H14O6/c1-23-17(21)13-7-3-11(4-8-13)15(19)16(20)12-5-9-14(10-6-12)18(22)24-2/h3-10H,1-2H3

description: dataset for 1H nuclear magnetic resonance spectroscopy (1H NMR) 1H NMR (400 MHz, CDCl3, ppm) δ = 8.23–8.13 (m, 4H, Car.H), 8.09–8.00 (m, 4H, Car.H), 3.96 (s, 6H, COOCH3).
DOI: 10.14272/pclyikbmkkhymd-uhfffaoysa-n/chmo0000595
title: 13C nuclear magnetic resonance spectroscopy (13C NMR) (methyl 4-[2-(4-methoxycarbonylphenyl)-2-oxoacetyl]benzoate)
title: InChI=1S/C18H14O6/c1-23-17(21)13-7-3-11(4-8-13)15(19)16(20)12-5-9-14(10-6-12)18(22)24-2/h3-10H,1-2H3

description: dataset for 13C nuclear magnetic resonance spectroscopy (13C NMR) 13C NMR (100 MHz, CDCl3, ppm) δ = 193.0 (Cq, 2C, CO), 166.0 (Cq, 2C, COOCH3), 135.9 (Cq, 2C, Car.), 135.7 (Cq, 2C, Car.), 130.3 (+, 4C, Car.H), 130.0 (+, 4C, Car.H), 52.8 (+, 2C, COOCH3).
DOI: 10.14272/pclyikbmkkhymd-uhfffaoysa-n/chmo0000630
title: infrared absorption spectroscopy (IR) (methyl 4-[2-(4-methoxycarbonylphenyl)-2-oxoacetyl]benzoate)
title: InChI=1S/C18H14O6/c1-23-17(21)13-7-3-11(4-8-13)15(19)16(20)12-5-9-14(10-6-12)18(22)24-2/h3-10H,1-2H3

description: dataset for infrared absorption spectroscopy (IR) IR (ATR, ṽ) = 3520, 2963, 1718, 1663, 1608, 1570, 1500, 1449, 1435, 1407, 1282, 1201, 1188, 1115, 1103, 1013, 980, 949, 890, 860, 820, 790, 782, 731, 713, 684, 674, 629, 584, 534, 473, 460, 449, 422 cm–1.
DOI: 10.14457/cu.res.2012.104
title: การศึกษาเปรียบเทียบไลเคนพลานัสในช่องปากระหว่างผู้ป่วยไทยและโครเอเทียน
DOI: 10.14457/cu.the.2010.2076
title: แบบจำลองเชิงคงทนในการกระจายสินค้าสำหรับอุตสาหกรรมน้ำตาลภายในประเทศ
DOI: 10.14457/cu.the.2010.2077
title: การวิเคราะห์เสถียรภาพความลาดของมวลหินเชิงความน่าจะเป็น กรณีศึกษาเหมืองหินปูนเขาวง จังหวัดสระบุรี
DOI: 10.25919/5e82e830aeb1d
title: Parkes observations for project P885 semester 2019OCTS_19

description: We propose to observe the magnetars 1E 1547.0-5408 and PSR J1622-4950 approximately weekly, to track their rotation, flux density, and polarisation, as we have been doing through this project. Also, as of late 2018, XTE J1810-197 is again a radio magnetar after 10 years dormant! Its chaotic rotation is better tracked in detail elsewhere, but weekly observations with the UWL receiver are already providing unique measurements of its radio spectrum and broad-band behaviour. Our observations provide an important window into remarkably dynamic magnetar magnetospheres, and characterise the conditions under which radio emission takes place therein, placing constraints on the emission mechanisms, which in at least some significant respects differ from those of ordinary pulsars.
DOI: 10.14457/cu.the.2010.2078
title: การวางแผนควบรวมสินค้าและจองตู้คอนเทนเนอร์สำหรับตัวแทนรับส่งสินค้าทางทะเล
DOI: 10.14457/cu.the.2010.2079
title: การปรับสูตรการผลิตพีวีซียืดหยุ่นโดยเติมคลอริเนเต็ดพาราฟินเป็นพลาสติไซเซอร์ทุติยภูมิสำหรับอุตสาหกรรมการผลิตรองเท้า
DOI: 10.5519/qd.0us9n74e
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (23 records)
DOI: 10.25919/5e82ea11d8eea
title: Parkes observations for project P1027 semester 2019OCTS_12

description: We propose to carry out Parkes follow-up observations of the new millisecond pulsar, J1431-6328, discovered by the Australian SKA Pathfinder (ASKAP) and Parkes Ultra-Wideband Low (UWL) receiver. The discovery demonstrated the power of identifying pulsar candidates in radio continuum images and then following up with high time resolution observations. The discovery itself is also interesting. PSR J1431-6328 has a spin period of 2.77 ms, and is likely to be in a binary system. Follow-up observations will enable us to measure the binary parameters, which will guide future multi-wavelength observations and might shed new lights on the binary evolution. The short spin period, relatively large flux density and sky location of PSR J1431-6328 also make it a promising candidate for pulsar timing arrays. The proposed observations will allow us to obtain a timing solution of this new pulsar, and are therefore essential for future timing observations.
DOI: 10.25919/5e82e729cb00a
title: Parkes observations for project P737 semester 2019OCTS_08

description: The aim of this proposal is to carry out tests of the new backend instruments which cannot be carried out during standard maintenance periods. The scheduled time is used to measure beam shapes, determine polarisation calibration solutions and commission the National Facility observing modes for the new wide-band receiver.
DOI: 10.25919/5e82e8c3cc6b6
title: Parkes observations for project P1027 semester 2019OCTS_11

description: We propose to carry out Parkes follow-up observations of the new millisecond pulsar, J1431-6328, discovered by the Australian SKA Pathfinder (ASKAP) and Parkes Ultra-Wideband Low (UWL) receiver. The discovery demonstrated the power of identifying pulsar candidates in radio continuum images and then following up with high time resolution observations. The discovery itself is also interesting. PSR J1431-6328 has a spin period of 2.77 ms, and is likely to be in a binary system. Follow-up observations will enable us to measure the binary parameters, which will guide future multi-wavelength observations and might shed new lights on the binary evolution. The short spin period, relatively large flux density and sky location of PSR J1431-6328 also make it a promising candidate for pulsar timing arrays. The proposed observations will allow us to obtain a timing solution of this new pulsar, and are therefore essential for future timing observations.
DOI: 10.5281/zenodo.3733998
title: GEO4962 input dataset for running CESM 2.1.0 case for the course

description: Contains the input dataset for running CESM 2.1.0 as part of the GEO4962 course at the University of Oslo.
DOI: 10.25919/5e82e7972c529
title: Parkes observations for project P885 semester 2019OCTS_18

description: We propose to observe the magnetars 1E 1547.0-5408 and PSR J1622-4950 approximately weekly, to track their rotation, flux density, and polarisation, as we have been doing through this project. Also, as of late 2018, XTE J1810-197 is again a radio magnetar after 10 years dormant! Its chaotic rotation is better tracked in detail elsewhere, but weekly observations with the UWL receiver are already providing unique measurements of its radio spectrum and broad-band behaviour. Our observations provide an important window into remarkably dynamic magnetar magnetospheres, and characterise the conditions under which radio emission takes place therein, placing constraints on the emission mechanisms, which in at least some significant respects differ from those of ordinary pulsars.
DOI: 10.5281/zenodo.3734020
title: Supporting R-code and data for "Why are population growth rate estimates of past and present hunter-gatherers so different?" (Tallavaara and Jørgensen, 2020)

description: This submission contains data and R-code that enable to reproduce the data manipulations and analyses in the paper “Why are population growth rate estimates of past and present hunter-gatherers so different?” by Miikka Tallavaara and Erlend Kirkeng Jørgensen (Philosophical transactions of the Royal Society B). Please, cite the paper and this Zenodo repository if you use the files included in this Zenodo record in your work. The submission includes a html-file titled “Why are population growth rate estimates of past and present hunter-gatherers so different? - Data analyses” (TJ2020.html) that contains R-code and instructions and comments for running the code (open this file in your browser). In addition, the submission includes Rdata-file (dataTJ2020.Rdata) containing all the data that are not created within the code and pure R-code (TJ2020.R).
DOI: 10.5281/zenodo.3734019
title: Supporting R-code and data for "Why are population growth rate estimates of past and present hunter-gatherers so different?" (Tallavaara and Jørgensen, 2020)

description: This submission contains data and R-code that enable to reproduce the data manipulations and analyses in the paper “Why are population growth rate estimates of past and present hunter-gatherers so different?” by Miikka Tallavaara and Erlend Kirkeng Jørgensen (Philosophical transactions of the Royal Society B). Please, cite the paper and this Zenodo repository if you use the files included in this Zenodo record in your work. The submission includes a html-file titled “Why are population growth rate estimates of past and present hunter-gatherers so different? - Data analyses” (TJ2020.html) that contains R-code and instructions and comments for running the code (open this file in your browser). In addition, the submission includes Rdata-file (dataTJ2020.Rdata) containing all the data that are not created within the code and pure R-code (TJ2020.R).
DOI: 10.14457/cu.the.2010.2080
title: การพัฒนารูปแบบการเรียนรู้ด้วยวิธีการค้นพบโดยใช้เทคโนโลยีสารสนเทศและการสื่อสารตาม แนวคิดการมีส่วนร่วมของชุมชนนักปฏิบัติและชุมชนแห่งการเรียนรู้เพื่อพัฒนาทักษะ การแก้ปัญหาของนักเรียนมัธยมศึกษาปีที่ 3 และการมีส่วนร่วมของชุมชน
DOI: 10.14457/cu.the.2010.2081
title: โครงสร้างและองค์ประกอบทางกายภาพของย่านพาณิชยกรรมเก่าตลาดพลู กรุงเทพมหานคร
DOI: 10.14457/cu.the.2010.2082
title: กลวิธีทางภาษากับการนำเสนออัตลักษณ์ของตนเองโดยกลุ่ม "เกย์ออนไลน์"
DOI: 10.5281/zenodo.3734008
title: Dataset From: Structuring of colloidal silica nanoparticle suspensions near water–silica interfaces probed by specular neutron reflectivity

description: The dataset for the publication "Structuring of colloidal silica nanoparticle suspensions near water–silica interfaces probed by specular neutron reflectivity". DOI: 10.1039/d0cp00465k. Files containing data have .dat extension and are in text format.
DOI: 10.5281/zenodo.3734007
title: Dataset From: Structuring of colloidal silica nanoparticle suspensions near water–silica interfaces probed by specular neutron reflectivity

description: The dataset for the publication "Structuring of colloidal silica nanoparticle suspensions near water–silica interfaces probed by specular neutron reflectivity". DOI: 10.1039/d0cp00465k. Files containing data have .dat extension and are in text format.
DOI: 10.25919/5e82ed392f953
title: Parkes observations for project P737 semester 2019OCTS_07

description: The aim of this proposal is to carry out tests of the new backend instruments which cannot be carried out during standard maintenance periods. The scheduled time is used to measure beam shapes, determine polarisation calibration solutions and commission the National Facility observing modes for the new wide-band receiver.
DOI: 10.5281/zenodo.3715314
title: A Verification Technique for Real-Time Information Flow Security

description: Evaluation artifacts accompanying the PhD thesis of Christopher Gerking, concerning the chapter on "A Verification Technique for Real-Time Information Flow Security".
DOI: 10.17186/1604987
title: Data Release and Project Closeout Procedure

description: A dataset containing procedures to: 1.) Make a dataset public 2.) Closeout out a project on the Data Hub
DOI: 10.5281/zenodo.3715313
title: A Verification Technique for Real-Time Information Flow Security

description: Evaluation artifacts accompanying the PhD thesis of Christopher Gerking, concerning the chapter on "A Verification Technique for Real-Time Information Flow Security".
DOI: 10.17042/1604996
title: Data Release and Project Closeout

description: A dataset containing procedures to: 1.) Make a dataset public 2.) Closeout a project on the Data Hub
DOI: 10.23722/1604997
title: Data Release and Project Closeout

description: A dataset containing procedures to: 1.) Make a dataset public 2.) Closeout a project on the Data Hub
DOI: 10.5281/zenodo.3734039
title: The [CII] 158 μm line emission in high-redshift galaxies: Data Set

description: This data set contains all data tables associated to the publication: "The [CII] 158 μm line emission in high-redshift galaxies"; A&A Lagache, Cousin, Chatzikos 2018. Please cite it if you use those data.
description: {"references": ["Lagache, Cousin, Chatzikos 2018"]}
DOI: 10.5281/zenodo.3734040
title: The [CII] 158 μm line emission in high-redshift galaxies: Data Set

description: This data set contains all data tables associated to the puplication: "The [CII] 158 μm line emission in high-redshift galaxies"; Lagache, Cousin, Chatzikos 2018. Please cite it if you use those data.
description: {"references": ["Lagache, Cousin, Chatzikos 2018"]}
DOI: 10.5281/zenodo.3733766
title: Summarizing the state of the terrestrial biosphere in few dimensions

description: This repository contains the data and a docker container to reproduce the analysis in Kraemer, G., Camps-Valls, G., Reichstein, M., & Mahecha, M. D. (2020). Summarizing the state of the terrestrial biosphere in few dimensions. <em>Biogeosciences</em>, <em>17</em>(9), 2397–2424. https://doi.org/10.5194/bg-17-2397-2020 If you use this data and/or code, please cite the paper. This dataset is a subset of the DataCube v1.0.0 (https://www.earthsystemdatacube.net) plus a the FAPAR_tip dataset from DataCube v1.0.2 The code to reproduce the analysis can also be found in http://doi.org/10.5281/zenodo.3733783 and https://github.com/gdkrmr/summarizing_the_state_of_the_biosphere To run the docker container, import the container, extract the data, run the command below, and open your web browser to access the jupyter server. Modify the command below as necessary, for details please consult the documentation for docker and jupyter: PORT=8333<br> IP=0.0.0.0<br> docker run -it \<br> -v /path/to/data/low-res/:/home/science/summarizing_biosphere/data \<br> -v /path/to/results_and_temporary_files/:/home/science/summarizing_biosphere/results \<br> -p $PORT:$PORT \<br> summarizing_biosphere \<br> /home/science/.julia/conda/3/bin/jupyter \<br> notebook \<br> --port=$PORT \<br> --ip=$IP \<br> --no-browser
description: {"references": ["Kraemer, G., Camps-Valls, G., Reichstein, M., & Mahecha, M. D. (2020). Summarizing the state of the terrestrial biosphere in few dimensions. Biogeosciences, 17(9), 2397\u20132424. https://doi.org/10.5194/bg-17-2397-2020"]}
DOI: 10.21227/6hg6-pg82
title: 1450 fundus images with 899 glaucoma data and 551 normal data.

description: This set contains 1450 fundus images with 899 glaucoma data and 551 normal data.All text about patient information and the date that the associated images were collected are replaced by 0, which is black.
DOI: 10.21227/8qwd-zr67
title: Fallout of the Mover Eccentricity on the PM Eddy Current Loss of Quasi-Halbach T-LSMs

description: The paper is aimed at an investigation of the effectsof the mover eccentricity on the PM eddy current loss oftubular-linear synchronous machines (T-LSMs) equipped withquasi-Halbach magnetized PMs. The study is initiated by ananalytical prediction of the no-load spatial repartition of the fluxdensity taking into account the non-coaxiality of the mover andstator, and its validation by a 3D finite element analysis (FEA).Then a special attention is paid to an analytical formulationof the PM eddy current loss in presence of eccentricity. Thisis achieved considering the case of the radially-magnetizedPMs and the axially-magnetized ones. The developed modelenables the investigation of the eddy current loss versus themover eccentricity and the armature magnetic reaction harmoniccontent range. The obtained results are validated by 3D FEA.This latter is extended to the PM eddy current loss densitymapping and loops considering a given range of the armaturemagnetic reaction harmonic content.