cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25919/5c4a1219a18c3
title: Parkes observations for project P456 semester 2018OCTS_28

description: The Parkes Pulsar Timing Array (PPTA) project has three primary goals: (a) detection of gravitational waves from astronomical sources, (b) establishment of a pulsar timescale, and (c) improvement of our understanding of Solar-system dynamics. The PPTA is the oldest of three international pulsar timing groups. We have the smallest telescope and the smallest group, but the best measurements and the best results. Our bound on the strength of the incoherent gravitational wave background is the only bound which significantly constrains theoretical models. We have maintained our leading position because: we have the southern sky; we have a small but well-focussed group; we have the best-calibrated receivers; and we have been able to observe with an almost regular cadence of 15 to 20 days at three different wavelengths. With this proposal we aim to maintain our pre-eminent position in the field.

Unlike most observing proposals, this is a continuing proposal for which the observations will continue to improve bounds on ultra-low-frequency gravitational waves until they are finally detected. Continued Parkes observations will remain valuable at least until the first stage of the SKA is able to improve on our sensitivity and observing cadence. Even after the gravitational wave background is detected we will want to continue observations in support of the nascent field of gravitational wave astronomy!
DOI: 10.3886/e108221v1
title: Utilization and Quality: How the Quality of Care Influences Demand for Obstetric Care in Nigeria

description: This research examines the association between health facility quality, subjective perceptions, and utilization of obstetric care. We draw on unique survey data from Nigeria describing the quality of care at rural primary health care facilities and the utilization of obstetric care by households in the service areas of these facilities. Constructing a quality index using the detailed survey data, we show that facility quality is positively related to perceptions of quality and utilization. Disaggregating quality into structural, process and outcome dimensions, we find a consistently strong relationship only between utilization and structural measures of quality. The results suggest that efforts to improve quality may involve a trade-off between investing in dimensions that are more easily observed by households, which will influence utilization, and investing in dimensions that are more closely related to outcomes.
DOI: 10.18739/a2w08wg3r
title: Marine Mammal Watch, Northern Bering Sea and Chukchi Sea, August-September, 2017
DOI: 10.25919/5c4a1f2d5f280
title: Parkes observations for project P456 semester 2018OCTS_29

description: The Parkes Pulsar Timing Array (PPTA) project has three primary goals: (a) detection of gravitational waves from astronomical sources, (b) establishment of a pulsar timescale, and (c) improvement of our understanding of Solar-system dynamics. The PPTA is the oldest of three international pulsar timing groups. We have the smallest telescope and the smallest group, but the best measurements and the best results. Our bound on the strength of the incoherent gravitational wave background is the only bound which significantly constrains theoretical models. We have maintained our leading position because: we have the southern sky; we have a small but well-focussed group; we have the best-calibrated receivers; and we have been able to observe with an almost regular cadence of 15 to 20 days at three different wavelengths. With this proposal we aim to maintain our pre-eminent position in the field.

Unlike most observing proposals, this is a continuing proposal for which the observations will continue to improve bounds on ultra-low-frequency gravitational waves until they are finally detected. Continued Parkes observations will remain valuable at least until the first stage of the SKA is able to improve on our sensitivity and observing cadence. Even after the gravitational wave background is detected we will want to continue observations in support of the nascent field of gravitational wave astronomy!
DOI: 10.25919/5c4a2140ebaaa
title: Parkes observations for project P860 semester 2018OCTS_01

description: This is a request for observing time for the initial follow-up of pulsar discoveries from the low-latitude Galactic plane section of the HTRU survey (P630). We are in the final stages of our first pass processing with our periodicity search algorithm, and have already discovered 106 previously unknown pulsars. We expect that processing should be complete within the 2018OCTS semester. Extrapolation and population synthesis shows that the Galactic plane survey should result in a further 5 discoveries.

Interesting science can usually only be derived from a new pulsar after confirmation and a follow-up timing campaign is carried out. One year of initial timing is the minimum timespan required to fully characterise any newly-discovered pulsars, essential for deriving pulsar parameters such as the characteristic age, magnetic ?eld strength, spin-down rate, as well as to detect any unexpected behaviour of the pulsar which might result from emission instabilities.

This follow-up timing project is necessary for identifying any interesting pulsar systems discovered from the HTRU Galactic plane survey. Since all of the pulsars on the observing list here are being followed-up for the first time, they will produce completely new and exciting results. In addition, this timing project will enable a large-scale examination of the Galactic plane pulsar population, exploring the true boundaries of pulsar parameter space. Given the large number of discoveries expected and the long integration length required, this dedicated follow-up timing campaign is vital for achieving our science goals.
DOI: 10.25919/5c4a21ffb6283
title: Parkes observations for project P860 semester 2018OCTS_02

description: This is a request for observing time for the initial follow-up of pulsar discoveries from the low-latitude Galactic plane section of the HTRU survey (P630). We are in the final stages of our first pass processing with our periodicity search algorithm, and have already discovered 106 previously unknown pulsars. We expect that processing should be complete within the 2018OCTS semester. Extrapolation and population synthesis shows that the Galactic plane survey should result in a further 5 discoveries.

Interesting science can usually only be derived from a new pulsar after confirmation and a follow-up timing campaign is carried out. One year of initial timing is the minimum timespan required to fully characterise any newly-discovered pulsars, essential for deriving pulsar parameters such as the characteristic age, magnetic ?eld strength, spin-down rate, as well as to detect any unexpected behaviour of the pulsar which might result from emission instabilities.

This follow-up timing project is necessary for identifying any interesting pulsar systems discovered from the HTRU Galactic plane survey. Since all of the pulsars on the observing list here are being followed-up for the first time, they will produce completely new and exciting results. In addition, this timing project will enable a large-scale examination of the Galactic plane pulsar population, exploring the true boundaries of pulsar parameter space. Given the large number of discoveries expected and the long integration length required, this dedicated follow-up timing campaign is vital for achieving our science goals.
DOI: 10.5281/zenodo.2548898
title: Species abundance information improves sequence taxonomy classification accuracy - Qiita data

description: QIIME 2 Artifacts containing microbiome samples, organised by EMPO 3 classification.

Used to test q2-clawback.

Downloaded from Qiita. Draws from the following Qiita study ids:

11113[1], 11444, 1716, 10369[2], 990[3], 2080, 1713, 894, 1289, 1883, 1673, 1288, 10353, 2192[4], 10323, 678, 1773, 662, 1799, 864, 1481, 1024[5], 1064, 2182, 10934, 1674, 1795[6], 10273, 10283[7], 10422[8], 804, 10308, 1056[9], 2382[5], 1240, 889, 1041, 1717, 1222, 11149, 11669, 807[10], 10245, 1711, 1721, 910, 1001, 895, 550[11], 1747[12], 713[13], 755, 861, 958[14], 11161[15], 11154[16], 945, 723, 1715, 1714, 10798.

References<br>
1. Schulfer, A. F. et al. Nat Microbiol 3, 234–242 (2017).<br>
2. Ruhe, J. et al. Front Plant Sci 7 (2016).<br>
3. O'Brien, S. L. et al. Environ Microbiol 18, 2039–2051 (2016).<br>
4. Lax, S. et al. Science 345, 1048–1052 (2014).<br>
5. Zarraonaindia, I. et al. mBio 6 (2015).<br>
6. Navas-Molina, J. A. et al. in Methods Enzymol 371–444 (2013).<br>
7. Fang, X. et al. Front Microbiol 9 (2018).<br>
8. Tripathi, A. et al. mSystems 3 (2018).<br>
9. Delsuc, F. et al. Mol Ecol 23, 1301–1317 (2013).<br>
10. Gibbons, S. M. et al. PLoS ONE 9, e97435 (2014).<br>
11. Caporaso, J. G. et al. Genome Biol 12, R50 (2011).<br>
12. Hyde, E. R. et al. mSystems 1 (2016).<br>
13. Brazelton, W. J., Nelson, B. & Schrenk, M. O. Front Microbiol 2 (2012).<br>
14. Vitaglione, P. et al. Am J Clin Nutr 101, 251–261 (2014).<br>
15. Spirito, C. M., Marzilli, A. M. & Angenent, L. T. Environ Sci Technol 52, 13438–13447 (2018).<br>
16. Pham, V. T. H. et al. Sci Rep 7 (2017).
DOI: 10.5281/zenodo.2548899
title: Species abundance information improves sequence taxonomy classification accuracy - Qiita data

description: QIIME 2 Artifacts containing microbiome samples, organised by EMPO 3 classification.

Used to test q2-clawback.

Downloaded from Qiita. Draws from the following Qiita study ids:

11113[1], 11444, 1716, 10369[2], 990[3], 2080, 1713, 894, 1289, 1883, 1673, 1288, 10353, 2192[4], 10323, 678, 1773, 662, 1799, 864, 1481, 1024[5], 1064, 2182, 10934, 1674, 1795[6], 10273, 10283[7], 10422[8], 804, 10308, 1056[9], 2382[5], 1240, 889, 1041, 1717, 1222, 11149, 11669, 807[10], 10245, 1711, 1721, 910, 1001, 895, 550[11], 1747[12], 713[13], 755, 861, 958[14], 11161[15], 11154[16], 945, 723, 1715, 1714, 10798.

References<br>
1. Schulfer, A. F. et al. Nat Microbiol 3, 234–242 (2017).<br>
2. Ruhe, J. et al. Front Plant Sci 7 (2016).<br>
3. O'Brien, S. L. et al. Environ Microbiol 18, 2039–2051 (2016).<br>
4. Lax, S. et al. Science 345, 1048–1052 (2014).<br>
5. Zarraonaindia, I. et al. mBio 6 (2015).<br>
6. Navas-Molina, J. A. et al. in Methods Enzymol 371–444 (2013).<br>
7. Fang, X. et al. Front Microbiol 9 (2018).<br>
8. Tripathi, A. et al. mSystems 3 (2018).<br>
9. Delsuc, F. et al. Mol Ecol 23, 1301–1317 (2013).<br>
10. Gibbons, S. M. et al. PLoS ONE 9, e97435 (2014).<br>
11. Caporaso, J. G. et al. Genome Biol 12, R50 (2011).<br>
12. Hyde, E. R. et al. mSystems 1 (2016).<br>
13. Brazelton, W. J., Nelson, B. & Schrenk, M. O. Front Microbiol 2 (2012).<br>
14. Vitaglione, P. et al. Am J Clin Nutr 101, 251–261 (2014).<br>
15. Spirito, C. M., Marzilli, A. M. & Angenent, L. T. Environ Sci Technol 52, 13438–13447 (2018).<br>
16. Pham, V. T. H. et al. Sci Rep 7 (2017).
DOI: 10.25919/5c4a2d24ce774
title: Parkes observations for project P860 semester 2018OCTS_03

description: This is a request for observing time for the initial follow-up of pulsar discoveries from the low-latitude Galactic plane section of the HTRU survey (P630). We are in the final stages of our first pass processing with our periodicity search algorithm, and have already discovered 106 previously unknown pulsars. We expect that processing should be complete within the 2018OCTS semester. Extrapolation and population synthesis shows that the Galactic plane survey should result in a further 5 discoveries.

Interesting science can usually only be derived from a new pulsar after confirmation and a follow-up timing campaign is carried out. One year of initial timing is the minimum timespan required to fully characterise any newly-discovered pulsars, essential for deriving pulsar parameters such as the characteristic age, magnetic ?eld strength, spin-down rate, as well as to detect any unexpected behaviour of the pulsar which might result from emission instabilities.

This follow-up timing project is necessary for identifying any interesting pulsar systems discovered from the HTRU Galactic plane survey. Since all of the pulsars on the observing list here are being followed-up for the first time, they will produce completely new and exciting results. In addition, this timing project will enable a large-scale examination of the Galactic plane pulsar population, exploring the true boundaries of pulsar parameter space. Given the large number of discoveries expected and the long integration length required, this dedicated follow-up timing campaign is vital for achieving our science goals.
DOI: 10.5061/dryad.5db0168/1
title: Breeding adult data

description: This file includes the data collected on adult birds that were included in the study. The statistical analysis of these data is reported in Table 2 of the published article.
DOI: 10.5061/dryad.5db0168/2
title: Egg and clutch data

description: This file includes the data collected on egg and clutch characteristics that were included in the study. The statistical analysis of these data is reported in Table 3 and Table 4 of the published article.
DOI: 10.25919/5c4a34d43a577
title: Parkes observations for project P737 semester 2018OCTS_01

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: 10.5061/dryad.v2n78h0/1
title: Losing the trait without losing the signal 12sp data

description: 1. Mean Just-Noticeable-Differences (JNDs) of chromatic and achromatic ventral and dorsal conspicuousness of males and females for the 12 species; 2. Mean spectral reflectance of male and female ventral patches, male dorsal surfaces and habitat for each of the 12 species.
DOI: 10.25345/c53w59
title: MassIVE MSV000083360 - PProteomic analysis of enhanced cellular effects of electroporation and cisplatin in triple-negative breast cancer cells
title: We performed a comprehensive and label-free quantitative proteomic analysis of the human adenocarcinoma epithelial TNBC cells (MDA-MB-231) treated with Cisplatin (CsP) and Cisplatin with EP (EP+CsP). We identified hundreds of differentially expressed proteins that defines molecular mechanisms involved in cellular responses of MDA-MB-231 cells to ECT. The underlying dataset represents a valuable resource for mechanistic studies and for the validation of knowledge gained from this study in the future using animal models. The systemic data should build a foundation for a better understanding of the mechanisms of the cytotoxicity of the Cisplatin as a potent anticancer drug.
DOI: 10.25345/c5031x
title: MassIVE MSV000083361 - Proteomic profiles of gilts postnatal Proteome profiles of gilts postnatal vaginal development in lower reproductive tract vaginal swabs mirror histomorphic developmental changes in lower reproductive tract across
title: Healthy vaginal development depends on the expression and precise regulation of genes and proteins. We hypothesized that the porcine vagina continues to develop during the first two weeks of postnatal. Our objectives were to determine the differences in vaginal histomorphology between postnatal day (PND) 2 and 16 in suckling gilts, and to profile proteins collected from suckling gilts on PND 2 and PND 16 using vaginal swabs.    Hematoxylin and Eosin (H&E) stained posterior region sections showed increased numbers of epithelial layers and greater numbers of anucleated cells in apical layer between PND 2 and PND 16.  Shotgun proteomic analysis using LC-MS/MS detected 1554 high confidence proteins, with 881 differentially expressed proteins between PND 2 and 16. Signature of the most highly expressed proteins across both days supported that proteins captured on swabs were components of epithelial cells lining the lumen. One-third of proteins upregulated between PND 2 and 16 were categorized as secreted, including lipocalins.  Categories enriched by downregulated proteins included cell-cell adherens junction, translation and ER to Golgi vesicle-mediated transport, and likely reflected increased cornification of the stratified epithelium and mirrored changes in histomorphology of vagina. Findings support the porcine vagina continues to develop postnatal, and vaginal swabs are a means to study changes in the reproductive tract.
DOI: 10.6073/pasta/05ced379ab83f6f76024fa61f910613c
title: SBC LTER: Ocean: Currents and Biogeochemistry: Moored CTD and ADCP data from Purisima Mooring (PUR), ongoing since 1999

description: ADCP (Currents), CTD (Hydrography) and Optics data (Fluorescence, Beam
  Attenuation and Volume Scattering Function) were collected at La
  Purisima (site ID: PUR), north of Point Conception. Data have been
  interpolated to a 20 minute interval. ADCP data are binned at a 1.0
  meter interval, measured as height from the bottom to a maximum of 16
  bins. All bins may not be filled, and in some cases, data from bins
  technically above the surface are included. VSF data are available at
  angles, 100, 125 and 150 degrees. CTD parameters include Pressure,
  Temperature, Conductivity, Salinity, Density and Fluorescence. The CTD
  array is located approximately 4.5 meters from the surface, and there
  are additional temperature thermistors near the CTD array, at the
  bottom, and mid way between these two.
DOI: 10.5517/ccdc.csd.cc1j9v4t
title: CCDC 1409636: Experimental Crystal Structure Determination

description: Related Article: Tagir A. Yangirov, Akhnef A. Fatykhov, Elvira A. Sedova, Leonard M. Khalilov, Ekaterina S. Meshcheryakova, Sergey P. Ivanov, Sergey N. Salazkin, Vladimir A. Kraikin|2019|Tetrahedron|75|1282|doi:10.1016/j.tet.2019.01.043
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.cc1j9v9z
title: CCDC 1409641: Experimental Crystal Structure Determination

description: Related Article: Tagir A. Yangirov, Akhnef A. Fatykhov, Elvira A. Sedova, Leonard M. Khalilov, Ekaterina S. Meshcheryakova, Sergey P. Ivanov, Sergey N. Salazkin, Vladimir A. Kraikin|2019|Tetrahedron|75|1282|doi:10.1016/j.tet.2019.01.043
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: 10.6073/pasta/f7df24ad5fcafcf2138f8c1275d764f6
title: SBC LTER: Ocean: Currents and Biogeochemistry: Moored CTD and ADCP data from Santa Barbara Harbor Mooring (SBH), ongoing since 1999

description: CTD (Hydrography) data were collected at Santa Barbara Harbor (site
  ID: SBH). Data have been interpolated to a 20 minute interval. The CTD
  data for this site are harvested from SCCOOS
  (http://sccoos.org/) and
  processed in Matlab.
DOI: 10.17632/h59jynh6cn.1
title: Data for: Degradation of Tetra- and Trichloroethylene under Iron Reducing Conditions by Acidimicrobiaceae sp. A6

description: Data for figures
DOI: 10.5517/ccdc.csd.cc1pc9hv
title: CCDC 1559997: Experimental Crystal Structure Determination

description: Related Article: Chuan-Lei Zhang, Zi-Teng Liu, Heng Xu, He-Gen Zheng, Jing Ma, Jing Zhao|2019|Dalton Trans.|48|2285|doi:10.1039/C9DT00005D
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.cc1yw7cf
title: CCDC 1813635: Experimental Crystal Structure Determination

description: Related Article: Yaru Liu, Chang Liu, Xiao Zhang, Lan Liu, Chunyu Ge, Xinrui Zhuang, NanXi Zhang, Qingfeng Yang, Yong-Qing Huang, Zhengguo Zhang|2019|J.Solid State Chem.|272|1|doi:10.1016/j.jssc.2019.01.017
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.cc1zt712
title: CCDC 1841494: Experimental Crystal Structure Determination

description: Related Article: Rahman Bikas, Fatemeh Ajormal, Marzieh Emami, Joaquín Sanchiz, Nader Noshiranzadeh, Anna Kozakiewicz|2019|Polyhedron|162|20|doi:10.1016/j.poly.2019.01.035
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.cc1zt723
title: CCDC 1841495: Experimental Crystal Structure Determination

description: Related Article: Rahman Bikas, Fatemeh Ajormal, Marzieh Emami, Joaquín Sanchiz, Nader Noshiranzadeh, Anna Kozakiewicz|2019|Polyhedron|162|20|doi:10.1016/j.poly.2019.01.035
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.cc1zt734
title: CCDC 1841496: Experimental Crystal Structure Determination

description: Related Article: Rahman Bikas, Fatemeh Ajormal, Marzieh Emami, Joaquín Sanchiz, Nader Noshiranzadeh, Anna Kozakiewicz|2019|Polyhedron|162|20|doi:10.1016/j.poly.2019.01.035
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.cc1zt745
title: CCDC 1841497: Experimental Crystal Structure Determination

description: Related Article: Rahman Bikas, Fatemeh Ajormal, Marzieh Emami, Joaquín Sanchiz, Nader Noshiranzadeh, Anna Kozakiewicz|2019|Polyhedron|162|20|doi:10.1016/j.poly.2019.01.035
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.cc200s4z
title: CCDC 1847790: Experimental Crystal Structure Determination

description: Related Article: Ganapathy Ranjani, Rajagopal Nagarajan|2019|Org.Lett.|21|675|doi:10.1021/acs.orglett.8b03848
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.