cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5285/7963955c-9497-42ef-8802-84c14f27acfa
title: Spectral reflectance datasets, Multiscale Impacts of Cyanobacterial Crusts on Landscape Stability

description: Data consist of field spectral reflectance measurements and surface photographs of cyanobacterial soil crusts and other surficial materials in Diamantina National Park, Queensland. Data were collected as part of project NE/K011626/1 (associated with NE/K011464/1) Multiscale Impacts of Cyanobacterial Crusts on Landscape Stability. The reflectance data and associated surface photographs are of biological and physical soil crusts developed on claypan and sand dune surfaces alongside the Diamantina River (specifically on and around Lake Constance pan and Homestead pan. Data were collected and processed by Kevin White and Ian Davenport, using a Spectra Vista Hr1024i spectrometer with a spectralon reference panel. All data were processed using SVC Hr1024i PC Data acquisition software (version 1.6.7 Beta) to remove areas of spectral overlap. Photographs taken using a range of mobile device cameras. All field photographs are in JPEG (jpg) format. Data were collected for the purpose of assessing the ability to remotely sense presence/absence of cyanobacterial soil crusts for mapping purposes.
DOI: 10.21227/r6xp-zp41
title: mmWave measurement program

description: The ﬁfth-generation cellular networks (5G)has been proposed as a solution for the accelerating growth in data trafﬁc. As part of 5G, millimetre-wave (mmWave) is suggested as one of the potential spectrum candidates due to the vastly available bandwidth. Accordingly, both indoor and outdoor propagation measurements on mmWave have been widely conducted over the recent years. These ﬁeld measurements were heavily dependent on utilizing expensive channel-sounders and tools. In this paper, we propose an affordable and open-source test-bed solution for mmWave channel modeling covering 24 GHz and 77 GHz bands. The key contribution in the proposed test-bed is the use of costeffective mmWave Doppler radars, a speciﬁc methodology is developed for this purpose. The proposed test-bed is capable of resolving the received power at any given combination of angles-of-arrival (AoA) and angles-of-departure (AoD). In order to verify the functionality of the proposed test-bed, several measurement scenarios have been investigated in different indoor environments, the obtained propagation results using this testbed indicate a good consistency with the expected mmWave propagation characteristics. As the proposed test-bed is an open source and cost-effective, researchers and RF designers can easily conduct mmWave propagation measurements according to their particular needs.
DOI: 10.23725/6q2w-zw89
title: NWD119844.recab.cram

description: TOPMed: NWD119844 <br>HapMap_1000G: NA12878 <br>Seq Ctr: Baylor <br>File:  CRAM file
DOI: 10.25848/8ydb-mk41
title: 2016-2018 Readiness for Interprofessional Learnings Scale (RIPLS) Pre-test and Post-test Survey Results

description: This dataset contains the results of a Readiness for Interprofessional Learnings Scale (RIPLS) pre-test and post-test that was administered in association with a health professions course in inter-professional education (IPE). Between 2016 and 2018, 251 surveys were collected from medical and nursing students at the University of Miami who participated in a one-day course on inter-professional education. All 251 participant surveys were entered into the data file. 245 surveys were complete and used in the study analysis. The survey is comprised of demographic questions, followed by 19 pre-test and 19 post-test questions assessing student perceptions of IPE. The excel spreadsheet is organized with each participant’s demographic data, as well as their RIPLS responses, which fall on a Likert scale (1-5). Each participant row includes all collected data for that participant. No individual respondent can be identified using this data.
DOI: 10.5255/ukda-sn-8376-3
title: English Longitudinal Study of Ageing: Wave 8, 2016-2017, Sexual Self-Completion Data: Special Licence Access
DOI: 10.21227/sjsz-1r61
title: AITSteg: An Innovative Text Steganography Technique for Hidden Transmission of Text Message via Social Media

description: With the popularity of smartphones and widespread use of high-speed Internet, social media has become a vital part of people’s daily life. Currently, text messages are used in many applications, such as mobile chatting, mobile banking, and mobile commerce. However, when we send a text message via short message service (SMS) or social media, the information contained in the text message transmits as a plain text, which exposes it to attacks. In some cases, this information may be confidential, such as banking credentials, secret missions, and confidential appointments; moreover, it is a major drawback to send such information via SMS or social media, as neither provides security before transmission. In this study, we propose a novel text steganography technique called AITSteg, which provides end-to-end security during the transmission of text messages via SMS or social media between end users. The AITSteg technique is evaluated by considering a trusted scenario. We then evaluate the efficiency of the proposed technique in terms of embedding capacity, invisibility, robustness, and security. The experiments confirm that the AITSteg is able to prevent various attacks, including man-in-the-middle attacks, message disclosure, and manipulation by readers. Moreover, we compare the experimental results with the existing techniques to show the superiority of the proposed technique. To the best of our knowledge, this is the first text steganography technique that provides end-to-end secure transmission of the text message using symmetric keys via social media.
DOI: 10.25919/5b7524e5172b4
title: Parkes observations for project P737 semester 2018APRS_10

description: Pulsar observations using the Parkes radio telescope have led to some of the most exciting astronomical results in the last few years.  The aim of this proposal is to carry out tests of the new backend instruments which cannot be carried out during standard maintenance periods. High precision pulsar timing experiments require cross-coupling in the feed to be measured.  This can only be done using observations of PSR J0437-4715 from rise-to-set.  We propose to undertake such observations and make the results available for any users of the telescope.  We will also use P737 to commission new receivers such as the UWB.
DOI: 10.23725/qzj6-rr18
title: NWD119844.recab.cram.crai

description: TOPMed: NWD119844 <br>HapMap_1000G: NA12878 <br>Seq Ctr: Baylor <br>File:  CRAI index file
DOI: 10.25919/5b7525fe2800b
title: Parkes observations for project P976 semester 2018APRS_03

description: Spider pulsars - black widows (BW) and redbacks (RB) - reside in incredibly tight orbits with low-mass stellar companions. The close proximity of the two orbiting bodies leads to heavy irradiation of the companion by the pulsar wind, causing material to be driven from its surface. This excess material is not gravitationally bound to the star, and the extent to which it reaches can only be constrained by observing the duration of eclipses of the radio pulsar emission that it causes. Little information about these systems is set in stone: the physical processes behind the eclipses, the dimensions, densities and magnetic properties of the eclipse medium, mass loss rates and subsequent evolution of the companions, are all unknown. Previous radio studies of a handful of spider systems have highlighted the importance of high-time resolution and large frequency coverage in constraining their properties. Measurement of the flux density, dispersion measure, rotation measure and depolarisation of the pulsars, as a function of the orbits, directly probes the eclipse process and properties of the medium causing it. All of these measurables are frequency dependent, thus with ultra-wideband observations we will have access to an unparalleled insight into spider pulsar systems. We plan to observe three eclipses for each of three BWs and two RBs in order to constrain variability between the two classes, multiple systems within each class, and the eclipses in an individual system. In addition, such observations will demonstrate and help to optimise the capabilities of the new UWL receiver.
DOI: 10.5281/zenodo.1346251
title: Dummy Upload For Arxiv:1506.09008 Supplementary Data

description: ###Preamble###

This upload contains initialization files and data for simulations reported in:<br>
https://arxiv.org/abs/1506.09008: Coarse-grained modelling of strong DNA bending II: Cyclization

The initialization files allow a user to repeat the reported simulations using the oxDNA model. oxDNA is available for download from:<br>
https://dna.physics.ox.ac.uk/index.php/Main_Page. <br>
The use and meaning of the input and output files are documented extensively on this wiki. 

This is only a practice upload, and so only a small part of the total material is included.

###Organisation### 

Simulations are organised by system type. Folder DXXCYY corresponds to simulation of a cyclization system with Nd = XX and Nbp=YY, with the meaning of these symbols given in the text referenced above. "_seq" indicates simulation of a specific sequence, as listed in Table S1 of the reference.

For each system, a "closed" and an "open" folder are present. These correspond to the two windows of umbrella sampling that were performed separately. 

###Content###

Within each folder are the necessary initialization files to run the simulations exactly as reported in the reference above, simply by calling oxDNA from within the folder, using "inputVMMC" as the input file.

Also included are output files for a single realisation of the simulation. 

Note that the results in the reference above were all obtained from 5 independent replicas, using different initial conditions and different seeds. These can be (statistically) recreated simply by drawing random starting configurations from the single available traj_hist file.  

<br>
description: {"references": ["R. M. Harrison et al.: Coarse-grained modelling of strong DNA bending II: Cyclization. arXiv:1506.09008"]}
DOI: 10.5281/zenodo.1346252
title: Dummy Upload For Arxiv:1506.09008 Supplementary Data

description: ###Preamble###

This upload contains initialization files and data for simulations reported in:<br>
https://arxiv.org/abs/1506.09008: Coarse-grained modelling of strong DNA bending II: Cyclization

The initialization files allow a user to repeat the reported simulations using the oxDNA model. oxDNA is available for download from:<br>
https://dna.physics.ox.ac.uk/index.php/Main_Page. <br>
The use and meaning of the input and output files are documented extensively on this wiki. 

This is only a practice upload, and so only a small part of the total material is included.

###Organisation### 

Simulations are organised by system type. Folder DXXCYY corresponds to simulation of a cyclization system with Nd = XX and Nbp=YY, with the meaning of these symbols given in the text referenced above. "_seq" indicates simulation of a specific sequence, as listed in Table S1 of the reference.

For each system, a "closed" and an "open" folder are present. These correspond to the two windows of umbrella sampling that were performed separately. 

###Content###

Within each folder are the necessary initialization files to run the simulations exactly as reported in the reference above, simply by calling oxDNA from within the folder, using "inputVMMC" as the input file.

Also included are output files for a single realisation of the simulation. 

Note that the results in the reference above were all obtained from 5 independent replicas, using different initial conditions and different seeds. These can be (statistically) recreated simply by drawing random starting configurations from the single available traj_hist file.  

<br>
description: {"references": ["R. M. Harrison et al.: Coarse-grained modelling of strong DNA bending II: Cyclization. arXiv:1506.09008"]}
DOI: 10.23725/37ka-sf55
title: NWD136397.recab.cram.crai

description: TOPMed: NWD136397 <br>HapMap_1000G: HG01110 <br>Seq Ctr: NYGC <br>File:  CRAI index file
DOI: 10.23725/hcsq-kp83
title: NWD136397.recab.cram

description: TOPMed: NWD136397 <br>HapMap_1000G: HG01110 <br>Seq Ctr: NYGC <br>File:  CRAM file
DOI: 10.25919/5b75286c54298
title: Parkes observations for project P595 semester 2018APRS_07

description: We propose to continue the PULSE@Parkes project in which high school students from Australia and around the World use the Parkes radio telescope in a remote observing model to observe and analyse pulsar data.  The data from some PULSE@Parkes observations are used to support the FERMI Gamma ray mission, other observations supplement the P456 Pulsar Timing Array project and the remainder were chosen in order to make a detailed analysis of pulsar timing irregularities and intermittency.
DOI: 10.5517/ccdc.csd.cc20g1k3
title: CCDC 1860544: Experimental Crystal Structure Determination

description: Related Article: J.G. Elsberg, N.G. Spiropulos, A.C. Colson, E.C. Brown|2018|Acta Crystallogr.,Sect.E:Cryst.Commun.|74|1259|doi:10.1107/S2056989018011246
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.cc20g2h2
title: CCDC 1860573: Experimental Crystal Structure Determination

description: Related Article: F.N. Rein, W. Chen, B.L. Scott, R.C. Rocha|2018|Acta Crystallogr.,Sect.E:Cryst.Commun.|74|1250|doi:10.1107/S2056989018011258
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.cc20gr3c
title: CCDC 1861212: Experimental Crystal Structure Determination

description: Related Article: C.W. Padgett, W.E. Lynch, K. Sheriff, R. Dean, S. Zingales|2018|IUCrData|3|x181138|doi:10.1107/S2414314618011380
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: 10.23725/065g-c493
title: NWD146103.recab.cram

description: TOPMed: NWD146103 <br>HapMap_1000G: NA19238 <br>Seq Ctr: WashU <br>File:  CRAM file
DOI: 10.25919/5b75292fcb3e8
title: Parkes observations for project P885 semester 2018APRS_09

description: We propose to observe PSR J1622-4950 and 1E1547.0-5408 weekly, two
of three magnetars known to currently emit radio pulsations, to
track their rotation, flux density, and polarisation. Less frequently
we will monitor XTE J1810-197, which used to emit radio pulsations,
to be on the lookout for its revival - as just happened with PSR
J1622-4950, which turned on in April 2017 after more than 2 years dormant!
These observations yield a continuous record of torque, illuminating
the continued release of magnetic energy. Our broader aims are to
develop a better understanding of the dynamical behaviour of magnetar
magnetospheres, and to establish the conditions under which radio
emission takes place therein, in addition to characterising their
variable radio emission in order to place constraints on the emission
mechanisms, which in at least some respects differ from those of
ordinary pulsars.
DOI: 10.5281/zenodo.1346270
title: Turketwh/Prx_3-Mersvm_Data: First Release Of Prx 3-Mer Svm Data Set

description: First release of Prx 3-mer SVM data set to accompany manuscript submissions.
DOI: 10.5281/zenodo.1346271
title: Turketwh/Prx_3-Mersvm_Data: First Release Of Prx 3-Mer Svm Data Set

description: First release of Prx 3-mer SVM data set to accompany manuscript submissions.
DOI: 10.5517/ccdc.csd.cc1pgqhc
title: CCDC 1563283: Experimental Crystal Structure Determination

description: Related Article: S. Kansiz, N. Dege, V.A. Kalibabchuk|2018|Acta Crystallogr.,Sect.E:Cryst.Commun.|74|1263|doi:10.1107/S2056989018011489
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.cc20h6g6
title: CCDC 1861657: Experimental Crystal Structure Determination

description: Related Article: V.C. Ramani, R.D. Shah, M.M. Jotani, E.R.T. Tiekink|2018|Acta Crystallogr.,Sect.E:Cryst.Commun.|74|1254|doi:10.1107/S2056989018011477
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.cc20hp7g
title: CCDC 1862115: Experimental Crystal Structure Determination

description: Related Article: J.H. Lee, D. Koh|2018|IUCrData|3|x181152|doi:10.1107/S2414314618011525
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: 10.25919/5b75296c50cb0
title: Parkes observations for project P895 semester 2018APRS_03

description: Since the year 2005, the Parkes Pulsar Timing Array (PPTA) project has been placing ever more stringent constraints on the amplitude of a gravitational wave background signal.  Such upper bounds on the amplitude of the gravitational wave signal are currently dominated by a single pulsar: PSR J1909-3744.  The upper bound with this pulsar alone already cuts into the range of tenable theoretical models.  Further reducing the amplitude bound (by continued regular observations of this pulsar) will significantly narrow that range.  The first evidence of gravitational waves in the pulsar data are likely to be observed in the timing for PSR J1909-3744, but with only a single pulsar we will not be able to make an unambiguous detection.  However, knowledge of the likely signal strength (derived from this pulsar) will help to optimise the observing strategy for the detection of the gravitational wave signals with existing or future pulsar timing arrays.
DOI: 10.25919/5b752a24ce35c
title: Parkes observations for project P892 semester 2018APRS_08

description: SUPERBx looks at the highest Galactic latitudes in a search for pulsars and fast radio bursts (FRBs). We use optimised GPU codes and supercomputing to search for these, 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. Our pulsar discoveries are typically nearby scintillating sources, intermittent sources and those in interesting binary systems. Our FRB discoveries have discovery lags of ~1 second, rather than months/years and these feed rapid alerts to the world-wide follow-up community via a dedicated VOEvent format an Astronomer's Telegrams. The goal of this is to allow localisation of the discovered FRBs. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors and to exploit their many uses as tools for precision cosmology measurements.
DOI: 10.25919/5b752a6bd63a5
title: Parkes observations for project P885 semester 2018APRS_10

description: We propose to observe PSR J1622-4950 and 1E1547.0-5408 weekly, two
of three magnetars known to currently emit radio pulsations, to
track their rotation, flux density, and polarisation. Less frequently
we will monitor XTE J1810-197, which used to emit radio pulsations,
to be on the lookout for its revival - as just happened with PSR
J1622-4950, which turned on in April 2017 after more than 2 years dormant!
These observations yield a continuous record of torque, illuminating
the continued release of magnetic energy. Our broader aims are to
develop a better understanding of the dynamical behaviour of magnetar
magnetospheres, and to establish the conditions under which radio
emission takes place therein, in addition to characterising their
variable radio emission in order to place constraints on the emission
mechanisms, which in at least some respects differ from those of
ordinary pulsars.
DOI: 10.3886/e100462v3-7783
title: Replication Files for "College Party Culture and Sexual Assault"

description: This project includes the National Incident Based Reporting System data samples used in the following publication.<br><br>Lindo, Jason M., Peter M. Siminski, and Isaac D. Swensen. Forthcoming. College Party Culture and Sexual Assault. American Economic Journal: Applied Economics.<br><br><br><br><br>
DOI: 10.5281/zenodo.1346214
title: Cross-Tissue Eqtl Enrichment Of Associations In Schizophrenia

description: non-CNS data used in the study.

the original data these were generated from have been deposited in the European Genome-phenome Archive (EGA) under accession EGAS00001000805.

complete files (all associations):<br>
org/blood_cis_all.gz (whole blood)<br>
org/fat_cis_all.gz (adipose)<br>
org/lcl_all_cis.gz (LCLs)<br>
org/skin_cis_all.gz (epidermal)

e-gene files (best association per gene at FDR &lt; 0.01):<br>
org/eQTL.B.Peer50.FDR01 (whole blood)<br>
org/eQTL.F.Peer50.FDR01 (adipose)<br>
org/eQTL.L.Peer50.FDR01 (LCLs)<br>
org/eQTL.S.Peer50.FDR01 (epidermal)

control variants (2m template) bed files:<br>
fakeQTL_tw_blood.bed<br>
fakeQTL_tw_fat.bed<br>
fakeQTL_tw_lcl.bed<br>
fakeQTL_tw_skin.bed

control variants (2m template) rs names:<br>
fakeQTL_tw_blood.mrk<br>
fakeQTL_tw_fat.mrk<br>
fakeQTL_tw_lcl.mrk<br>
fakeQTL_tw_skin.mrk

control variants (9m template) R data files:<br>
fakeQTL9m_tw_blood.RData<br>
fakeQTL9m_tw_fat.RData<br>
fakeQTL9m_tw_lcl.RData<br>
fakeQTL9m_tw_skin.RData

control variants (9m template) matlab files:<br>
fakeQTL9m_tw_blood.mat<br>
fakeQTL9m_tw_fat.mat<br>
fakeQTL9m_tw_lcl.mat<br>
fakeQTL9m_tw_skin.mat

 

if you use these data, please cite the data sources:

Genetic interactions affecting human gene expression identified by variance association mapping. Brown, A.A., Buil, A., Viñuela, A., Lappalainen, T., Zheng, H.-F., Richards, J.B., Small, K.S., Spector, T.D., Dermitzakis, E.T. and Durbin, R. (2014). eLife 2014;3:e01381 doi: 10.7554/eLife.01381

Gene-gene and gene-environment interactions detected by transcriptome sequence analysis in twins. Buil, A., Brown, A.A., Lappalainen, T., Vinuela, A., Davies, M.N., Zheng, H.-F., Richards, J.B., Glass, D., Small, K.S., Durbin, R. et al. (2015) Nat Genet, 47, 88-91.