cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25505/fiz.icsd.cc20czv7
title: CSD 1858569: Experimental Crystal Structure Determination

description: Related Article: Fabrice Dal Bo, Sergey M. Aksenov, Peter C. Burns|2019|J.Solid State Chem.|271|126|doi:10.1016/j.jssc.2018.12.044
description: An entry from the Inorganic Crystal Structure Database, the world’s repository for inorganic crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the joint CCDC and FIZ Karlsruhe Access Structures service and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.25505/fiz.icsd.cc21bdf7
title: CSD 1886828: Experimental Crystal Structure Determination

description: Related Article: A.T. Chemey, T.E. Albrecht-Schmitt|2019|Acta Crystallogr.,Sect.E:Cryst.Commun.|75|139|doi:10.1107/S2056989018018194
description: An entry from the Inorganic Crystal Structure Database, the world’s repository for inorganic crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the joint CCDC and FIZ Karlsruhe Access Structures service and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.25919/5c307b7bf36e9
title: Parkes observations for project P958 semester 2018OCTS_06

description: A major breakthrough in fast radio burst (FRB) astronomy was recently made when the repeating FRB 121102 was localized to sub-arcsecond precision. The bursts were found to originate in a bright radio nebula (hypothesized to be a young supernova remnant or pulsar wind nebulae) in a distant dwarf galaxy. These dwarf galaxies are also preferential hosts to superluminous supernova and long gamma-ray bursts, and it has been therefore suggested that the source of the repeating FRB could be a young highly magnetised neutron star. While an understanding of the repeating FRB is emerging, it is still unclear what relationship it has to the rest of the population.   Over the last year searches with the Australian Square Kilometre Array Pathfinder (ASKAP) have detected 26 bursts, and over the next six month will likely detect another 12 FRBs, which  will be localized to a few arcseconds.   Here we propose to search this population for repeats.  Our comprehensive sample and a dense monitoring campaign of well localised bursts, at a fluence limit more than 60 times lower than that of their detections, will either confirm the presence of additional repeating FRBs or the uniqueness of FRB 121102 amongst the population.
DOI: 10.5517/ccdc.csd.cc21dhnm
title: CCDC 1888850: Experimental Crystal Structure Determination

description: Related Article: Frank R. Fronczek|2019|CSD Communication|||
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5517/ccdc.csd.cc21dhpn
title: CCDC 1888851: Experimental Crystal Structure Determination

description: Related Article: Joshua B. Cox, Aoi Kimishima, and John L. Wood|2018|J.Am.Chem.Soc.|141|25|doi:10.1021/jacs.8b10212
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: 10.17632/3xvc5zwkg6.1
title: Data for: A reverse-transcription/RNase H based protocol for depletion of mosquito ribosomal RNA facilitates viral intrahost evolution analysis, transcriptomics and pathogen discovery.

description: Outputs from Multiqc and BBmap for data analysis.
DOI: 10.25919/5c30a22b1e777
title: Parkes observations for project P995 semester 2018OCTS_01

description: We propose to perform observations of the very young pulsar PSR B0540–69 in the Large Magellanic Cloud to detect pulsed flux from this traditionally radio-quiet source.  We are motivated to do so due to a relatively recent X-ray observation of a 36% change in its spin down rate, thought to be due to a state change in its magnetospheric processes.  There is reason to believe this may be accompanied by an increase in pulsed flux, as has been seen in intermittent pulsar behaviour, for example.  Additionally, PSR B0540–69 is known to emit giant pulses, one of only a small number of pulsars to do so.  With the new Ultra Wideband Low-frequency (UWL) receiver system, we will be able to conduct the highest sensitivity observations of this source yet achieved at radio wavelengths.  A successful detection of pulsed flux will provide important insight into the magnetospheric evolution and behaviour in this pulsar, and a better understanding of how its glitch behaviour may influence its emission.  Even without such a detection, we will be able to study the giant pulse behaviour of PSR B0540–69 with unprecedented sensitivity.
DOI: 10.25919/5c30a2b3e3cc5
title: Parkes observations for project P995 semester 2018OCTS_02

description: We propose to perform observations of the very young pulsar PSR B0540–69 in the Large Magellanic Cloud to detect pulsed flux from this traditionally radio-quiet source.  We are motivated to do so due to a relatively recent X-ray observation of a 36% change in its spin down rate, thought to be due to a state change in its magnetospheric processes.  There is reason to believe this may be accompanied by an increase in pulsed flux, as has been seen in intermittent pulsar behaviour, for example.  Additionally, PSR B0540–69 is known to emit giant pulses, one of only a small number of pulsars to do so.  With the new Ultra Wideband Low-frequency (UWL) receiver system, we will be able to conduct the highest sensitivity observations of this source yet achieved at radio wavelengths.  A successful detection of pulsed flux will provide important insight into the magnetospheric evolution and behaviour in this pulsar, and a better understanding of how its glitch behaviour may influence its emission.  Even without such a detection, we will be able to study the giant pulse behaviour of PSR B0540–69 with unprecedented sensitivity.
DOI: 10.25919/5c30a343e10b9
title: Parkes observations for project P958 semester 2018OCTS_07

description: A major breakthrough in fast radio burst (FRB) astronomy was recently made when the repeating FRB 121102 was localized to sub-arcsecond precision. The bursts were found to originate in a bright radio nebula (hypothesized to be a young supernova remnant or pulsar wind nebulae) in a distant dwarf galaxy. These dwarf galaxies are also preferential hosts to superluminous supernova and long gamma-ray bursts, and it has been therefore suggested that the source of the repeating FRB could be a young highly magnetised neutron star. While an understanding of the repeating FRB is emerging, it is still unclear what relationship it has to the rest of the population.   Over the last year searches with the Australian Square Kilometre Array Pathfinder (ASKAP) have detected 26 bursts, and over the next six month will likely detect another 12 FRBs, which  will be localized to a few arcseconds.   Here we propose to search this population for repeats.  Our comprehensive sample and a dense monitoring campaign of well localised bursts, at a fluence limit more than 60 times lower than that of their detections, will either confirm the presence of additional repeating FRBs or the uniqueness of FRB 121102 amongst the population.
DOI: 10.5517/ccdc.csd.cc21dl02
title: CCDC 1888923: Experimental Crystal Structure Determination

description: Related Article: ZJ Quan|2019|CSD Communication|||
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5281/zenodo.2532054
title: Help wanted identifying hams in Swarm-E (e-POP) RRI data

description: In the spirit of making data from the Radio Receiver Instrument (RRI) onboard Swarm-E (formally known as e-POP) more accessible to the ham radio community via the Ham Radio Science Citizen Investigation (HamSCI), we have converted RRI's data into a ".raw" format so that it can be ingested into open source software such as Gqrx or GNU Radio.  We have done this for all RRI data related to the 2015, 2017, and 2018 ARRL Field Days.

We encourage everyone to help us identify hams in RRI's signal.  You can use the Gqrx tool discussed here, or you can use your own technique.  If you decode a ham's call sign, if you would like to share your technique, or if you have any comments or suggestion contact us and let us know! 

<strong>Data Rules of the Road</strong>

Please acknowledge the HamSCI project and Gareth Perry when using data from this archive in presentations and publications.

<strong>Swarm-E RRI</strong>

Swarm-E RRI is a digital radio receiver with 4 3-m monopole antennas.  In most cases, the monopoles are electronically configured into a crossed-diople configuration.  In this configuration, RRI records I/Q samples for the two dipoles.  RRI has a sampling rate of 62500.33933 Hz, and a ~40 kHz bandpass, and can be tuned to anywhere between 10 Hz and 18 MHz.  More information on Swarm-E RRI can be found in the Swarm-E RRI instrument paper or Gareth Perry's recent Radio Science article.

<strong>Data Format</strong>

Each data file contains raw 32 bit complex I/Q samples for a given RRI dipole at a given frequency.  The samples are interleaved, e.g., IQIQIQIQ... The data files do not contain any metadata.  Any information regarding the time, frequency, and corresponding RRI dipole is in the file name.  

<strong>Filename Format</strong>

The filename format gives information about the time and data of the recording, the tuned frequency, and which of RRI's dipoles the recording corresponds too.  For example, <em>gqrx_20150628_011614_3525000_62500_RRI_Dipole1 </em>contains data recorded on Dipole 1, starting at 01:16:14 UT on June 28, 2015, at 3525000 Hz (3.525 MHz), at a sampling rate of 62500 Hz (RRI's 62500.33933 Hz sampling rate).

<strong>Gqrx</strong>

We have opted to convert the data into the .raw format so that it can be ingested into Gqrx.  There are other ways of analyzing RRI's data; this is just one way which we felt was as easy first step.  We are open to posting about other techniques on the HamSCI site as well.  To help get started with Gqrx, we have developed a <em>How to play an RRI raw IQ file on Gqrx</em> page.
DOI: 10.5281/zenodo.2532410
title: Effects With and Effects Of Representation Control - wahlkarte02

description: Data and analysis script for lab study "wahlkarte02", conducted at Leibniz-Institut für Wissensmedien, Tübingen.

Immediate effects with and subsequent effects of representation control on time on task and proportion correct are inverstigated.

For more information see meta information and codebooks.
DOI: 10.5281/zenodo.2532411
title: Effects With and Effects Of Representation Control - wahlkarte02

description: Data and analysis script for lab study "wahlkarte02", conducted at Leibniz-Institut für Wissensmedien, Tübingen.

Immediate effects with and subsequent effects of representation control on time on task and proportion correct are inverstigated.

For more information see meta information and codebooks.
DOI: 10.5281/zenodo.2532053
title: Help wanted identifying hams in Swarm-E (e-POP) RRI data

description: In the spirit of making data from the Radio Receiver Instrument (RRI) onboard Swarm-E (formally known as e-POP) more accessible to the ham radio community via the Ham Radio Science Citizen Investigation (HamSCI), we have converted RRI's data into a ".raw" format so that it can be ingested into open source software such as Gqrx or GNU Radio.  We have done this for all RRI data related to the 2015, 2017, and 2018 ARRL Field Days.

We encourage everyone to help us identify hams in RRI's signal.  You can use the Gqrx tool discussed here, or you can use your own technique.  If you decode a ham's call sign, if you would like to share your technique, or if you have any comments or suggestion contact us and let us know! 

<strong>Data Rules of the Road</strong>

Please acknowledge the HamSCI project and Gareth Perry when using data from this archive in presentations and publications.

<strong>Swarm-E RRI</strong>

Swarm-E RRI is a digital radio receiver with 4 3-m monopole antennas.  In most cases, the monopoles are electronically configured into a crossed-diople configuration.  In this configuration, RRI records I/Q samples for the two dipoles.  RRI has a sampling rate of 62500.33933 Hz, and a ~40 kHz bandpass, and can be tuned to anywhere between 10 Hz and 18 MHz.  More information on Swarm-E RRI can be found in the Swarm-E RRI instrument paper or Gareth Perry's recent Radio Science article.

<strong>Data Format</strong>

Each data file contains raw 32 bit complex I/Q samples for a given RRI dipole at a given frequency.  The samples are interleaved, e.g., IQIQIQIQ... The data files do not contain any metadata.  Any information regarding the time, frequency, and corresponding RRI dipole is in the file name.  

<strong>Filename Format</strong>

The filename format gives information about the time and data of the recording, the tuned frequency, and which of RRI's dipoles the recording corresponds too.  For example, <em>gqrx_20150628_011614_3525000_62500_RRI_Dipole1 </em>contains data recorded on Dipole 1, starting at 01:16:14 UT on June 28, 2015, at 3525000 Hz (3.525 MHz), at a sampling rate of 62500 Hz (RRI's 62500.33933 Hz sampling rate).

<strong>Gqrx</strong>

We have opted to convert the data into the .raw format so that it can be ingested into Gqrx.  There are other ways of analyzing RRI's data; this is just one way which we felt was as easy first step.  We are open to posting about other techniques on the HamSCI site as well.  To help get started with Gqrx, we have developed a <em>How to play an RRI raw IQ file on Gqrx</em> page.
DOI: 10.5281/zenodo.2532420
title: Effects With and Effects Of Representation Control - wahlkarte05

description: Data and analysis script for lab study "wahlkarte05", conducted at Leibniz-Institut für Wissensmedien, Tübingen.

Immediate effects with and subsequent effects of representation control on time on task and proportion correct are inverstigated with a fully crossed experimental design. We also differentiated between reproduction and near transfer.

For more information see meta information and codebooks.
DOI: 10.25345/c56c86
title: MassIVE MSV000083300 - GNPS - Bacteriophage Subject 1
title: untargeted metabolomics. analysis of skin, feces, saliva, and nasal samples collected using swabs from a subject, subject 1, with bacterial infection treated using bacteriophage.
DOI: 10.5281/zenodo.2532419
title: Effects With and Effects Of Representation Control - wahlkarte05

description: Data and analysis script for lab study "wahlkarte05", conducted at Leibniz-Institut für Wissensmedien, Tübingen.

Immediate effects with and subsequent effects of representation control on time on task and proportion correct are inverstigated with a fully crossed experimental design. We also differentiated between reproduction and near transfer.

For more information see meta information and codebooks.
DOI: 10.5281/zenodo.2532423
title: Effects With and Effects Of Representation Control - wahlkarte03

description: Data and analysis script for lab study "wahlkarte03", conducted at Leibniz-Institut für Wissensmedien, Tübingen.

Immediate effects with and subsequent effects of different types of representation control on time on task and proportion correct are inverstigated. We compared three types of representation control: 1)Active representation control: Participants adjusted visualization layout (displayed information and information organization) by using check boxes 2)Modeling: Participants adjusted visualization layout with one click, individual steps were shown  3) Short-circuit: Participants adjusted visualization layout with one click, individual steps were not shown

For more information see meta information and codebooks.
DOI: 10.5281/zenodo.2532424
title: Effects With and Effects Of Representation Control - wahlkarte03

description: Data and analysis script for lab study "wahlkarte03", conducted at Leibniz-Institut für Wissensmedien, Tübingen.

Immediate effects with and subsequent effects of different types of representation control on time on task and proportion correct are inverstigated. We compared three types of representation control: 1)Active representation control: Participants adjusted visualization layout (displayed information and information organization) by using check boxes 2)Modeling: Participants adjusted visualization layout with one click, individual steps were shown  3) Short-circuit: Participants adjusted visualization layout with one click, individual steps were not shown

For more information see meta information and codebooks.
DOI: 10.5281/zenodo.2532497
title: Hemiptera-Phytoplasma-Plant dataset

description: This is a database of Hemiptera-Phytoplasma-Plant (HPP) biological interactions worldwide. The database contains 1860 records of plant-phytoplasma pairwise associations, and 968 records of insect-phytoplasma pairwise associations. Priority is given to the first record of association between a 16Sr phytoplasma subgroup and a host (plant or insect vector) reported for each country.
DOI: 10.17632/63t8dt3mc9.1
title: Data for: A Spin Glass State in Ba3TiRu2O9

description: The magnetic properties of Ba3TiRu2O9 , whose crystal structure is based on stacked triangular planar lattices of MO6 dimers and single MO6 octahedra, are reported. The system is magnetically disturbed by a substantial amount of Ti/Ru chemical disorder. The Weiss temperature and effective magnetic moment were found to be -29.5 K and 1.82 μB/f.u. respectively, and a bifurcation in the zero field cooled and field cooled magnetic susceptibility is observed below 4.7 K, suggesting that this is a compositionally-disordered spin-glass system. The material is a semiconductor with an activation energy for charge transport of approximately 0.14 eV.
DOI: 10.17632/y93xpftdp8.1
title: Data for: Influence of dipole interaction radius and dilution on phase transition in kagome artificial spin ice

description: Wang-Landau modeling data of kagome artificial spin ice with dipole interaction cutoff radius (8 and 14 nearest neighbors). Also Wang-Landau modeling data of diluted kagome artificial spin ice with dipole interaction cutoff radius (14 nearest neighbors).
DOI: 10.3886/e107961v1
title: The iSP Study: Promotion of Self-Efficacy in Junior High Students

description: A growing body of correlational research finds a relationship between self-efficacy—beliefs in one’s capabilities—and academic success. But few studies have investigated whether self-efficacy is causally related to academic success. We hypothesized that an experience of success would promote self-efficacy in junior high school students and would lead to academic improvements. To induce an experience of success, we secretly presented easy anagrams to target students (41 males and 43 females; 12–13 years old) who then outperformed their classmates (116 males and 115 females). We assessed students’ self-efficacy and academic achievement scores before and after the anagram tasks. We found that the success-induced students raised their self-efficacy, and this elevated self-efficacy persisted for as long as one year. Moreover, success-induced males eventually showed significant improvement in their academic achievement. These results provide a real-world experimental enactment of Bandura’s self-efficacy theory and have implications for the practices of educational practitioners.
description: Response Rates: We randomly sampled a total of 84 students (41 males, 43 females) for Success condition and 231 students (116 males, 115  females)  for Control condition in a randomized controlled treatment experiment. We deleted case-wise the participants failing to attend one or more assessing periods. Finally, we analyzed the complete  assessment  data of 267 students (72  in  the Success  condition  and  195  in  the  Control  condition).
description: Presence of Common Scales: An original scale for task specific self-efficacy. We  defined  self-efficacy  procedurally  in  this study as a student’s rating in response to this specific question: “How well can you perform in the letter rearrangement game?”  Students  indicated  their  answer  on  a  five-pointscale,  ranging  from  1  (very  badly)  to  5  (very  well).
description: cognitive assessment test~~on-site questionnaire~~
description: Seventh-graders of a junior high school in Nagano, Japan.Smallest Geographic Unit: Seventh-grade students of a junior high school in Japan
description: A randomized clustered sampling
DOI: 10.5517/ccdc.csd.cc1n8h4k
title: CCDC 1527498: Experimental Crystal Structure Determination

description: Related Article: Faiza Asghar, Bhajan Lal, Amin Badshah, Ian S. Butler, Muhammad Nawaz Tahir|2019|Inorg.Chim.Acta|488|8|doi:10.1016/j.ica.2018.12.052
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.cc1pzrm1
title: CCDC 1578694: Experimental Crystal Structure Determination

description: Related Article: Zeineb Ouerghi, Heinz Gornitzka, Ersin Temel, Imen Dridi, Riadh Kefi|2019|J.Mol.Struct.|1181|338|doi:10.1016/j.molstruc.2018.12.108
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.cc1z181b
title: CCDC 1818461: Experimental Crystal Structure Determination

description: Related Article: Meng-Cheng Zhang, Dong-Chao Wang, Ming-Sheng Xie, Gui-Rong Qu, Hai-Ming Guo, Shu-Li You|2019|Chem Cell mPress|5|156|doi:10.1016/j.chempr.2018.10.003
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.cc1z182c
title: CCDC 1818462: Experimental Crystal Structure Determination

description: Related Article: Meng-Cheng Zhang, Dong-Chao Wang, Ming-Sheng Xie, Gui-Rong Qu, Hai-Ming Guo, Shu-Li You|2019|Chem Cell mPress|5|156|doi:10.1016/j.chempr.2018.10.003
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.