cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.21227/25z6-af08
title: Signing in the Wild dataset

description: Our Signing in the Wild dataset consists of various videos harvested from YouTube containing people signing in various sign languages and doing so in diverse settings, environments, under complex signer and camera motion, and even group signing. This dataset is intended to be used for sign language detection.For the negative set, we created two classes of videos, labelled‘speaking’ and ‘other’. Our motivation for the ‘speaking’ class isthat speech is often accompanied by hand gestures (gesticulation),which can be easily confused with signing. Signing can be discriminatedby its linguistic nature, i.e., its distinct phonological, morphologicaland categorical (discrete) structures, while gesticulationtends to be more spontaneous, idiosyncratic and analogue in nature.For the ‘other’ class, we looked for distractors to both ‘signing’and ‘speaking’, i.e., videos containing hand movements that arequite similar to signing/gesticulation and thus might confuse a classifier.Examples include: miming, hand exercises, various manualactivities like playing instruments, painting, writing, yoga and martialarts, sports like table tennis, etc. Also included are activitiessimilar to speech, like people laughing, clapping, nodding, listening to other speakers, etc.A total of 1120 videos are included in our dataset, each videocontributing the first 6.6 minutes, resulting in 2000 frames per videowhen sampled at 5Hz. We have 1.45 million video frames in total.Our videos are untrimmed, i.e., a video can contain multiple activities,background scenes, scene cuts, and other actions done by thesame or different actors. Thus the videos are unconstrained both spatiallyand also temporally. This is in line with recent trends in videoaction recognition [8], and unlike ASLR datasets where trimmedvideos are the norm. In particular, several videos in our dataset containall 3 classes (occasionally with temporal overlap), and sometimesthe same person alternating between signing and speaking.We performed manual groundtruthing at video frame level.Since action boundaries can be inherently fuzzy, we consider a shorttemporal context (10 frames) surrounding the frame to be labelledin order to decide on its class label. We also adopt certain spatialguidelines, e.g. mouth movements must be visible for action ‘speaking’,thus eliminating distant views and when the speaker turnshis/her back to the camera. Ambiguous cases are left unlabelled.We annotate video segments that do not contain signing or speaking as ‘other’, including opening/closing credits, title screens, scenetransitions, animations, background scenes, etc.If you find this dataset useful, please cite the following paper:  Mark Borg, Kenneth P. Camilleri, "Sign Language Detection "In The Wild" With Recurrent Neural Networks", ICASSP 2019.Any comments, suggestions, feedback are welcome: mborg2005 at gmail dot com
DOI: 10.14455/nrct.img.2019.136
title: การพัฒนาความเข้มแข็งของกลุ่มเกษตรกรเพื่อสร้างระบบการผลิตเกษตรเพื่ออาหารปลอดภัย
DOI: 10.14455/nrct.img.2019.142
title: รูปแบบการจัดการความรู้การเลี้ยงปลาในบ่อดินที่ประสบความสําเร็จในจังหวัดอ่างทอง (Successful model of knowledge on fish farming management in earthen ponds at Angthong province)
DOI: 10.5281/zenodo.2576272
title: Broccoli sprout beverage is safe for thyroid hormonal and autoimmune status: Results of a 12-week randomized trial.

description: The .csv file contains all the primary data for publication: <br>
Chartoumpekis DV, Ziros PG, Chen JG, Groopman JD, Kensler TW, Sykiotis GP.<br>
Broccoli sprout beverage is safe for thyroid hormonal and autoimmune status: Results of a 12-week randomized trial.<br>
Food Chem Toxicol. 2019 Feb 5;126:1-6.<br>
[Epub ahead of print] PubMed PMID: 30735751<br>
doi: 10.1016/j.fct.2019.02.004.

These data are used in all figures of the paper (Figure 1 and Figure 2).

The data are tabular. The headers are the following:

sample ID: It comprises 4 digits. The first 3 digits are the unique identifier of the subject in the trial, e.g., "613".<br>
The last digit indicates whether the sample was collected at the start of the trial "0", or at the end of the trial "1".<br>
E.g., "6130" is the sample collected from participant 613 at the beginning of the trial,<br>
and 6131 is the sample collected from the same participant at the end of the trial.

Autoimmunity: "0" means that both anti-TG and anti-TPO antibodies were within the reference range.<br>
"1" means that either anti-TG, or anti-TPO antibodies, or both, were above the reference range.

anti-TG (IU/ml): antibodies against thyroglobuline. The units are given in the parenthesis.

anti-TPO (IU/ml): antibodies against thyropreoxidase. The units are given in the parenthesis.

Treatment: "1"=placebo and "2"=broccoli sprouts extract beverage.

Gender: "F" for female and "M" for male. Data from males were not included in the analyses.

Age: In years.

<br>
For any questions, contact: gerasimos.sykiotis@chuv.ch
DOI: 10.5281/zenodo.2576273
title: Broccoli sprout beverage is safe for thyroid hormonal and autoimmune status: Results of a 12-week randomized trial.

description: The .csv file contains all the primary data for publication: <br>
Chartoumpekis DV, Ziros PG, Chen JG, Groopman JD, Kensler TW, Sykiotis GP.<br>
Broccoli sprout beverage is safe for thyroid hormonal and autoimmune status: Results of a 12-week randomized trial.<br>
Food Chem Toxicol. 2019 Feb 5;126:1-6.<br>
[Epub ahead of print] PubMed PMID: 30735751<br>
doi: 10.1016/j.fct.2019.02.004.

These data are used in all figures of the paper (Figure 1 and Figure 2).

The data are tabular. The headers are the following:

sample ID: It comprises 4 digits. The first 3 digits are the unique identifier of the subject in the trial, e.g., "613".<br>
The last digit indicates whether the sample was collected at the start of the trial "0", or at the end of the trial "1".<br>
E.g., "6130" is the sample collected from participant 613 at the beginning of the trial,<br>
and 6131 is the sample collected from the same participant at the end of the trial.

Autoimmunity: "0" means that both anti-TG and anti-TPO antibodies were within the reference range.<br>
"1" means that either anti-TG, or anti-TPO antibodies, or both, were above the reference range.

anti-TG (IU/ml): antibodies against thyroglobuline. The units are given in the parenthesis.

anti-TPO (IU/ml): antibodies against thyropreoxidase. The units are given in the parenthesis.

Treatment: "1"=placebo and "2"=broccoli sprouts extract beverage.

Gender: "F" for female and "M" for male. Data from males were not included in the analyses.

Age: In years.

<br>
For any questions, contact: gerasimos.sykiotis@chuv.ch
DOI: 10.25919/5c733914630cc
title: Parkes observations for project PX500 semester 2018OCTS_63

description: This proposal relates to time purchased by the Chinese Academy of Sciences for Parkes follow-up confirmation and timing of FAST discoveries.  As the observing time has been purchased this proposal (and the related PX501) does not require TAC grading.  The primary reason for submitting a proposal is to ensure an outreach statement and that the proposal is entered into OPAL for the data archive to access. The Chinese team have two time requests. The time scheduled for the first, relating to this proposal, will be allocated in blocks of 24 hours and the data will become available in the data archive with an 18 month embargo period.  The second type of time will be scheduled in shorter blocks and the data archived with a 10 year embargo.
DOI: 10.18716/nmrshiftdb2/40248436/nmredata_cdcl3
title: NMR dataset for (9S)-6'-Methoxycinchonan-9-ol
DOI: 10.6073/pasta/16c683fb2b62f08a14d64aac1834570d
title: 2-meter elevation contours, Saddle grid, Niwot Ridge LTER, Colorado

description: Coverage of 2-meter contours at Saddle grid. 1:500 scale. This dataset is part of the Saddle grid geographic information system (GIS). Additional information concerning the Niwot Ridge LTER hierarchical GIS can be found in Walker et al. (1993).
DOI: 10.6073/pasta/389166bc6493a5d165a1e1c2b89a85e5
title: 3.23-meter elevation lattice grid, Martinelli Snowfield, Niwot Ridge LTER, Colorado

description: Martinelli snow field lattice.  This dataset is part of the Martinelli grid geographic information system (GIS). Additional information concerning the Niwot Ridge LTER hierarchical GIS can be found in Walker et al. (1993).
DOI: 10.6073/pasta/4cb59b8f6263622df9c1cfff619b90e2
title: 25-meter elevation lattice grid, Niwot Ridge LTER Project Area, Colorado

description: 25-meter lattice made from the Niwot Ridge LTER TIN model (ltertin). This dataset was made to support hierarchical GIS databases at the Niwot Ridge LTER. Additional information concerning the Niwot Ridge LTER hierarchical GIS can be found in Walker et al. (1993).
DOI: 10.6073/pasta/bafdd674a3b708449afaa20ea9027dc6
title: 0.5-meter elevation lattice grid, Saddle grid, Niwot Ridge LTER, Colorado

description: This is a 0.5m lattice/DEM derived using the TOPOGRID command. 1:500 scale.  This dataset is part of the Saddle grid geographic information system (GIS). Additional information concerning the Niwot Ridge LTER hierarchical GIS can be found in Walker et al. (1993).
DOI: 10.6073/pasta/5d1b1097b1208f05eb7d9874f86918d8
title: 5-meter elevation contours, Martinelli Snowfield, Niwot Ridge LTER, Colorado

description: Martinelli snow field contour lines.  This dataset is part of the Martinelli grid geographic information system (GIS). Additional information concerning the Niwot Ridge LTER hierarchical GIS can be found in Walker et al. (1993).
DOI: 10.6073/pasta/6d7988d3ed445e914c47d4ef689db1ee
title: 1-meter elevation lattice grid, Martinelli Snowfield, Niwot Ridge LTER, Colorado

description: Resampled version of Martinelli snow field lattice grid (martlat) with finer resolution.  This dataset is part of the Martinelli grid geographic information system (GIS). Additional information concerning the Niwot Ridge LTER hierarchical GIS can be found in Walker et al. (1993).
DOI: 10.17632/dpc5sm8y8k.1
title: Housing preferences for a small and portable dwelling: Stated choice experiment

description: The online survey was opened for three weeks in June 2013 and it was distributed in the Netherlands through various channels. A total of 450 people were personally invited to complete the survey, and from the company that designed and produced the housing concept, the invitation was shared through newsletters (760 people), an internal social network (8000), and the company’s Twitter account (16,000). Overall, the questionnaire reached 625 respondents, of whom 280 (nearly 50%) completed the survey.
DOI: 10.25606/surf.578c6039-bae5e320
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (1024-022)

description: We present the results of the "Cosmogrid" cosmological N-body simulation suites based on the concordance LCDM model. The Cosmogrid simulation was performed in a 30 Mpc box with 2048³ particles. The mass of each particle is 1.28x10^5 Msun, which is sufficient to resolve ultra-faint dwarfs. We found that the halo mass function shows good agreement with the Sheth & Tormen fitting function down to ~10^7 Msun. We have analyzed the spherically averaged density profiles of the three most massive halos which are of galaxy group size and contain at least 170 million particles. The slopes of these density profiles become shallower than -1 at the inner most radius. We also find a clear correlation of halo concentration with mass. The mass dependence of the concentration parameter cannot be expressed by a single power law, however a simple model based on the Press-Schechter theory proposed by Navarro et al. gives reasonable agreement with this dependence. The spin parameter does not show a correlation with the halo mass. The probability distribution functions for both concentration and spin are well fitted by the log-normal distribution for halos with the masses larger than ~10^8 Msun. The subhalo abundance depends on the halo mass. Galaxy-sized halos have 50% more subhalos than ~10^11 Msun halos have. This is snapshot 022 of the 1024³ resolution collection.
DOI: 10.14457/cu.the.2002.239
title: ประชาสังคม เวทีสาธารณะ กับกระบวนการกลายเป็นประเด็นสาธารณะ ศึกษากรณี โครงการก่อสร้างโรงบำบัดน้ำเสียคลองด่าน จังหวัดสมุทรปราการ
DOI: 10.14457/cu.the.2003.514
title: การฟ้อนของชาวผู้ไทย : กรณีศึกษาหมู่บ้านโพน อำเภอคำม่วง จังหวัดกาฬสินธุ์
DOI: 10.14457/cu.the.2003.515
title: การนำเสนอปฏิบัติการทางเลือกของการเรียนการสอนตามสภาพจริง ในวิชาหลักสูตรและการสอนทั่วไป สำหรับนิสิตคณะศึกษาศาสตร์
DOI: 10.14457/cu.the.2003.516
title: ความเครียดในงาน และการจัดความเครียดของพยาบาลวิชาชีพและพยาบาลเทคนิค โรงพยาบาลสมเด็จพระปิ่นเกล้า พ.ศ.2546
DOI: 10.14457/cu.the.2003.517
title: ปัญหาที่พักอาศัยของนักศึกษามหาวิทยาลัย ที่มีสองวิทยาเขต กรณีศึกษา มหาวิทยาลัยกรุงเทพ วิทยาเขตรังสิต และวิทยาเขตกล้วยน้ำไท
DOI: 10.14457/cu.the.2003.518
title: การพัฒนาระบบระบายอากาศชนิดไหลในแนวดิ่งอย่างสม่ำเสมอ สำหรับอากาศที่มีฝุ่นฟุ้ง
DOI: 10.25606/surf.578c6039-011dade3
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (1024-024)

description: We present the results of the "Cosmogrid" cosmological N-body simulation suites based on the concordance LCDM model. The Cosmogrid simulation was performed in a 30 Mpc box with 2048³ particles. The mass of each particle is 1.28x10^5 Msun, which is sufficient to resolve ultra-faint dwarfs. We found that the halo mass function shows good agreement with the Sheth & Tormen fitting function down to ~10^7 Msun. We have analyzed the spherically averaged density profiles of the three most massive halos which are of galaxy group size and contain at least 170 million particles. The slopes of these density profiles become shallower than -1 at the inner most radius. We also find a clear correlation of halo concentration with mass. The mass dependence of the concentration parameter cannot be expressed by a single power law, however a simple model based on the Press-Schechter theory proposed by Navarro et al. gives reasonable agreement with this dependence. The spin parameter does not show a correlation with the halo mass. The probability distribution functions for both concentration and spin are well fitted by the log-normal distribution for halos with the masses larger than ~10^8 Msun. The subhalo abundance depends on the halo mass. Galaxy-sized halos have 50% more subhalos than ~10^11 Msun halos have. This is snapshot 024 of the 1024³ resolution collection.
DOI: 10.25606/surf.578c6039-63b96f74
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (1024-019)

description: We present the results of the "Cosmogrid" cosmological N-body simulation suites based on the concordance LCDM model. The Cosmogrid simulation was performed in a 30 Mpc box with 2048³ particles. The mass of each particle is 1.28x10^5 Msun, which is sufficient to resolve ultra-faint dwarfs. We found that the halo mass function shows good agreement with the Sheth & Tormen fitting function down to ~10^7 Msun. We have analyzed the spherically averaged density profiles of the three most massive halos which are of galaxy group size and contain at least 170 million particles. The slopes of these density profiles become shallower than -1 at the inner most radius. We also find a clear correlation of halo concentration with mass. The mass dependence of the concentration parameter cannot be expressed by a single power law, however a simple model based on the Press-Schechter theory proposed by Navarro et al. gives reasonable agreement with this dependence. The spin parameter does not show a correlation with the halo mass. The probability distribution functions for both concentration and spin are well fitted by the log-normal distribution for halos with the masses larger than ~10^8 Msun. The subhalo abundance depends on the halo mass. Galaxy-sized halos have 50% more subhalos than ~10^11 Msun halos have. This is snapshot 019 of the 1024³ resolution collection.
DOI: 10.25606/surf.578c6039-6dd3641a
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (1024-018)

description: We present the results of the "Cosmogrid" cosmological N-body simulation suites based on the concordance LCDM model. The Cosmogrid simulation was performed in a 30 Mpc box with 2048³ particles. The mass of each particle is 1.28x10^5 Msun, which is sufficient to resolve ultra-faint dwarfs. We found that the halo mass function shows good agreement with the Sheth & Tormen fitting function down to ~10^7 Msun. We have analyzed the spherically averaged density profiles of the three most massive halos which are of galaxy group size and contain at least 170 million particles. The slopes of these density profiles become shallower than -1 at the inner most radius. We also find a clear correlation of halo concentration with mass. The mass dependence of the concentration parameter cannot be expressed by a single power law, however a simple model based on the Press-Schechter theory proposed by Navarro et al. gives reasonable agreement with this dependence. The spin parameter does not show a correlation with the halo mass. The probability distribution functions for both concentration and spin are well fitted by the log-normal distribution for halos with the masses larger than ~10^8 Msun. The subhalo abundance depends on the halo mass. Galaxy-sized halos have 50% more subhalos than ~10^11 Msun halos have. This is snapshot 018 of the 1024³ resolution collection.
DOI: 10.25606/surf.578c6039-746207de
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (1024-017)

description: We present the results of the "Cosmogrid" cosmological N-body simulation suites based on the concordance LCDM model. The Cosmogrid simulation was performed in a 30 Mpc box with 2048³ particles. The mass of each particle is 1.28x10^5 Msun, which is sufficient to resolve ultra-faint dwarfs. We found that the halo mass function shows good agreement with the Sheth & Tormen fitting function down to ~10^7 Msun. We have analyzed the spherically averaged density profiles of the three most massive halos which are of galaxy group size and contain at least 170 million particles. The slopes of these density profiles become shallower than -1 at the inner most radius. We also find a clear correlation of halo concentration with mass. The mass dependence of the concentration parameter cannot be expressed by a single power law, however a simple model based on the Press-Schechter theory proposed by Navarro et al. gives reasonable agreement with this dependence. The spin parameter does not show a correlation with the halo mass. The probability distribution functions for both concentration and spin are well fitted by the log-normal distribution for halos with the masses larger than ~10^8 Msun. The subhalo abundance depends on the halo mass. Galaxy-sized halos have 50% more subhalos than ~10^11 Msun halos have. This is snapshot 017 of the 1024³ resolution collection.
DOI: 10.25606/surf.578c6039-8e34cd6b
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (1024-020)

description: We present the results of the "Cosmogrid" cosmological N-body simulation suites based on the concordance LCDM model. The Cosmogrid simulation was performed in a 30 Mpc box with 2048³ particles. The mass of each particle is 1.28x10^5 Msun, which is sufficient to resolve ultra-faint dwarfs. We found that the halo mass function shows good agreement with the Sheth & Tormen fitting function down to ~10^7 Msun. We have analyzed the spherically averaged density profiles of the three most massive halos which are of galaxy group size and contain at least 170 million particles. The slopes of these density profiles become shallower than -1 at the inner most radius. We also find a clear correlation of halo concentration with mass. The mass dependence of the concentration parameter cannot be expressed by a single power law, however a simple model based on the Press-Schechter theory proposed by Navarro et al. gives reasonable agreement with this dependence. The spin parameter does not show a correlation with the halo mass. The probability distribution functions for both concentration and spin are well fitted by the log-normal distribution for halos with the masses larger than ~10^8 Msun. The subhalo abundance depends on the halo mass. Galaxy-sized halos have 50% more subhalos than ~10^11 Msun halos have. This is snapshot 020 of the 1024³ resolution collection.
DOI: 10.14457/cu.the.2003.519
title: การสื่อความหมายด้วยภาพถ่ายและข้อความในเอกสารแนะนำตัวผู้สมัครสมาชิกวุฒิสภา เขตกรุงเทพมหานคร พ.ศ.2543
DOI: 10.14457/cu.the.2003.520
title: ความสัมพันธ์ระหว่างค่ากำลังรับแรงเฉือนกับค่าความหนืดของดินเหนียว
DOI: 10.14457/cu.the.2003.521
title: การปรับเปลี่ยนอัตลักษณ์ความเป็นจีนของชาวไทยเชื้อสายจีน ในบริบทขององค์กรประชาสังคมของกลุ่มชาติพันธุ์จีน : ศึกษากรณีองค์กรในจังหวัดอุบลราชธานี
DOI: 10.25345/c57p6v
title: MassIVE MSV000083476 - PLZF and DDX5 interacting proteins in spermatogonia
title: DDX5 or PLZF co-immunoprecipitation in lysates from cultured undifferentiated spermatogonia followed by analysis by mass spectrometry.
DOI: 10.5281/zenodo.2576583
title: Contextual maritime data set (RDF triples)

description: This data set is the RDF conversion w.r.t. the datAcron ontology, of the contextual maritime data available at https://zenodo.org/record/1167595 . It has been generated by the RDF-Gen method on the data sets describing sea ports (World Port Index, Ports of Brittany, SeaDataNet fishing ports) and protected regions (fishing areas, fishing interdiction, Natura2000).
DOI: 10.5281/zenodo.2576584
title: Contextual maritime data set (RDF triples)

description: This data set is the RDF conversion w.r.t. the datAcron ontology, of the contextual maritime data available at https://zenodo.org/record/1167595 . It has been generated by the RDF-Gen method on the data sets describing sea ports (World Port Index, Ports of Brittany, SeaDataNet fishing ports) and protected regions (fishing areas, fishing interdiction, Natura2000).
DOI: 10.3886/e108486v1-10603
title: Do pro-social students care more for the environment?

description: This
study uses pro-social and pro-environment attitudes as indicators of social and
environmental sustainability to empirically examine the relationship between
the two pillars of sustainability. Self reported survey responses of undergraduate
students of University of Utah are used for conducting a two-stage quantile
regression analysis wherein social support serves as an instrument for
identifying pro-social attitude for estimating the relationship between
pro-social and pro-environment attitudes. The estimates show that students who receive
more social support tend to be more pro-social, and more pro-social students
are more pro-environment. These results reiterate that universities can enhance
sustainability education by adopting a more holistic approach wherein social
and environmental sustainability are cointegrated. Additionally, by strengthening
their role as a vital source of social support for students, universities can further
enhance the synergistic relationship between pro-social and pro-environment
attitudes of university students.