cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5281/zenodo.7828250
title: Genome assemblies: Horizontal transfer of pOXA-48 from a hypervirulent Klebsiella pneumoniae ST23/KL57 to Serratia marcescens

description: Hypervirulent Klebsiella pneumonia isolates express a range of virulence factors, often encoded on virulence plasmids. Occasionally these hypervirulent lineages acquire antimicrobial resistance genes rendering them multidrug-resistant. We describe the nosocomial transmission of a hypervirulent K. pneumoniae ST23/KL57 isolate carrying an NDM-1 and OXA-48 beta-lactamase among COVID-19 patients in a Danish university hospital. Furthermore, we characterize the plasmid structure and describe a within-patient horizontal transfer of a plasmid carrying a blaOXA-48 gene from K. pneumoniae ST23/KL57 to a Serratia marcescens isolate.
DOI: 10.25502/xsf8-kz38/d
title: Baseline study data

description: The proposed project aims to drive increased production and consumption of OFSP among smallholder Farmers, thus improve food and nutrition security and livelihoods for women and children, especially improved diet diversity in Benue and Oyo state. The project also will build strong demand and capacity amongst stakeholders–from government to private sector, and farmer associations–to fully utilize OFSP and vine multiplication for improved nutrition and livelihood in the 2 selected states (Benue and Oyo) of Nigeria. The project will demonstrate, through the case of OFSP, how a bio-fortified crop can be profitably produced, marketed, and utilized in nutrition programming in the two selected states. 

In collaboration with GAIN and selected state Agriculture Development Program (ADPs), the project will specifically empower at least 560 Farmers (70 per LGA) in Benue and Oyo states to access, farm and market OFSP for improved livelihood while their households and community generally will be aware of OFSP nutrition and economic benefits for adoption and consumption. This will entail capacity building (training), setting up demonstration plots for training of farmers on Good Agronomic Practices (GAP), train 40 selected farmers (5 per LGA) on vine multiplication by 16 (2 per LGA) Training of Trainers (ToT) and facilitate market linkages for produce.  There will be a series of trainings on processing of OFSP roots into bio-available vitamin A-rich products as well as enriching indigenous food products with OFSP for both household consumption and income generation.
DOI: 10.4121/21915822
title: Data belonging to the paper: Leopard density and interspecific spatiotemporal interactions in a hyena-dominated landscape

description: Data belonging to the paper: Leopard density and interspecific spatiotemporal interactions in a hyena-dominated landscape by Sander Vissia, Julien Fattebert & Frank van Langevelde. The purpose of the data collection was to estimate leopard densities and spatio-temporal activity patterns of leopard and brown hyena and spotted hyena .<br>
DOI: 10.4121/21915822.v1
title: Data belonging to the paper: Leopard density and interspecific spatiotemporal interactions in a hyena-dominated landscape

description: Data belonging to the paper: Leopard density and interspecific spatiotemporal interactions in a hyena-dominated landscape by Sander Vissia, Julien Fattebert & Frank van Langevelde. The purpose of the data collection was to estimate leopard densities and spatio-temporal activity patterns of leopard and brown hyena and spotted hyena .<br>
DOI: 10.4121/21915768
title: Dataset used for the publication of the article: Co-occurrence of high densities of brown hyena and spotted hyena in central Tuli, Botswana

description: Dataset used for the publication of the article: Co-occurrence of high densities of brown hyena and spotted hyena in central Tuli, Botswana by S. Vissia, R. Wadhwa & F.van Langevelde.<br>The dataset includes the r script and datafiles for the secr-modelling to estimate the hyena densities and the r script and datafiles to calculate temporal overlap between the hyena species.
DOI: 10.4121/21915768.v1
title: Dataset used for the publication of the article: Co-occurrence of high densities of brown hyena and spotted hyena in central Tuli, Botswana

description: Dataset used for the publication of the article: Co-occurrence of high densities of brown hyena and spotted hyena in central Tuli, Botswana by S. Vissia, R. Wadhwa & F.van Langevelde.<br>The dataset includes the r script and datafiles for the secr-modelling to estimate the hyena densities and the r script and datafiles to calculate temporal overlap between the hyena species.
DOI: 10.4121/21915789
title: Dataset belonging to the paper: The effect of body size on co-occurrence patterns within an African carnivore guild

description: Dataset belonging to the paper: The effect of body size on co-occurrence patterns within an African carnivore guild. The purpose of the data collection was to determine spatial and temporal co-occurrence patterns of small, medium-sized and large carnivores.
DOI: 10.4121/21915789.v1
title: Dataset belonging to the paper: The effect of body size on co-occurrence patterns within an African carnivore guild

description: Dataset belonging to the paper: The effect of body size on co-occurrence patterns within an African carnivore guild. The purpose of the data collection was to determine spatial and temporal co-occurrence patterns of small, medium-sized and large carnivores.
DOI: 10.4121/21915834
title: Dataset belonging to the paper Seasonal variation in prey preference, diet partitioning and niche breadth in a rich large carnivore guild

description: Dataset belonging to the paper Seasonal variation in prey preference, diet partitioning and niche breadth in a rich large carnivore guild by Sander Vissia, Ariet Bouman, Francisca Virtuoso and Frank van Langevelde. The purpose of the data collection was to compare seasonal changes in prey preference, diet partitioning and niche breadth of four large carnivore species, namely leopard, spotted hyena, brown hyena and wild dog.
DOI: 10.4121/21915834.v1
title: Dataset belonging to the paper Seasonal variation in prey preference, diet partitioning and niche breadth in a rich large carnivore guild

description: Dataset belonging to the paper Seasonal variation in prey preference, diet partitioning and niche breadth in a rich large carnivore guild by Sander Vissia, Ariet Bouman, Francisca Virtuoso and Frank van Langevelde. The purpose of the data collection was to compare seasonal changes in prey preference, diet partitioning and niche breadth of four large carnivore species, namely leopard, spotted hyena, brown hyena and wild dog.
DOI: 10.25345/c5z02zk1n
title: MassIVE MSV000091714 - Tau immunoprecipitation from human neurons
title: Immunoprecipitation was performed on human neuron samples. Protein eluates were digested to peptides which were analyzed by DIA mass spectrometry. A spectral library was generated from all samples. Quantities in Tau-IP samples were compared to control-IP samples.
DOI: 10.57967/hf/0534
title: processed_scientific_papers
DOI: 10.35003/8hq9qc
title: Replication Data for: A New Tool to Account for Crater Obliteration Effects in Crater Size-Frequency Distribution Measurements

description: • Our new application applies crater measurement techniques to shapeﬁle geometries • The tool uses open software libraries and supports multicore and 64 bit data processing • Workarounds for geodesic measurements and polygon modiﬁcations were implemented
DOI: 10.35003/8hq9qc/7fvzw6
title: Figure04.ppt

description: Densely cratered reference area (blue) north of Malapert Massif on the lunar nearside at ~15°E, 70°S.
DOI: 10.35003/8hq9qc/qujru2
title: Figure05.ppt

description: Distortion of area measurements in Lambert azimuthal equal area projection with growing eccentricity of the reference body.
DOI: 10.35003/8hq9qc/8nonk8
title: Figure02.ppt

description: Application of geodesic polygon buffer by using geodesic measurements.
DOI: 10.35003/8hq9qc/b4homf
title: Figure03.ppt

description: Flow chart of CSFD measurements with CSFD Tools.
DOI: 10.35003/8hq9qc/tylufo
title: Figure01.ppt

description: Assignment of reference areas for four crater measurement techniques.
DOI: 10.23729/958d4b59-52f4-4d84-9306-5c21d244c7e3
title: Airborne laser scanning point clouds from Evo test site, ~0.7 pts/m2, 119 sample plots, 2014

description: Airborne laser scanning point clouds acquired from the Evo study site on May 22, 2014 (most of the sample plots) and on September 8, 2014 (some of the sample plots) using a Leica ALS70-HA SN7202 laser scanner recording five returns (firs, 1-3 intermediate, last) with the following parameters: Flying altitude: 2500 m above the ground level Point density: ~0.7 pts/m2 Flying speed: 150 knots Pulse frequency: 105 kHz CRS: EUREF-FIN(ETRS89) The point clouds are provided in the LAS 1.2 file format separately for each sample plot (25-m radius around the sample plot center), identified by a four-digit number in the filename.
DOI: 10.23729/397dd90d-3643-4228-9768-b76ce0b6a9ac
title: Airborne laser scanning point clouds from Evo test site, ~6 pts/m2, 119 sample plots, Autumn 2014

description: Airborne laser scanning point clouds acquired from the Evo study site on September 5, 2014 in leaf-on conditions using a Leica ALS70-HA SN7202 laser scanner recording five returns (first, 1-3 intermediate, last) with the following parameters: Flying altitude: 900 m above the ground level Point density: ~6 pts/m2 Flying speed: 150 knots Pulse frequency: 240 kHz CRS: EUREF-FIN(ETRS89) The point clouds are provided in the LAS 1.2 file format separately for each sample plot (25-m radius around the sample plot center), identified by a four-digit number in the filename.
DOI: 10.23729/bda72e80-d8c5-4b58-a567-81a19c6a4213
title: Airborne laser scanning point clouds from Evo test site, ~15 pts/m2, 119 sample plots, summer 2009

description: Airborne laser scanning point clouds acquired from the Evo study site on June 25, 2009 in leaf-on conditions using a Leica ALS50-II SN058 laser scanner recording three returns (firs, intermediate, last) with the following parameters: Opening angle: 30 deg. Side overlap: 20% Flying altitude: 400 m above the ground level Flying speed: 80 knots Scan frequency: 52.2 Hz Pulse frequency: 150 kHz GNSS and IMU: Leica IPAS Pro v1.3 & Novatel GrafNav v7.8 CRS: EUREF-FIN(ETRS89) The point clouds feature a point density of ~15 pts/m2 with points classified into two categories: unclassified (1), ground (2). The point clouds are provided in the LAS 1.0 file format separately for each sample plot (25-m radius around the sample plot center), identified by a four-digit number in the filename.
DOI: 10.5517/ccdc.csd.cc2865j6
title: CCDC 2091307: Experimental Crystal Structure Determination

description: Related Article: Yang-Yi Liu, Zhi-Qiang Liu, Yu-Qing Wang, Ying Zhou, Yan Qin, Hui-Peng Lv, Peng-Fei Li, Xiao-Gang Chen, Xian-Jiang Song, Yong Ai|2023|Cryst.Growth Des.|23|2602|doi:10.1021/acs.cgd.2c01455
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.cc2865k7
title: CCDC 2091308: Experimental Crystal Structure Determination

description: Related Article: Yang-Yi Liu, Zhi-Qiang Liu, Yu-Qing Wang, Ying Zhou, Yan Qin, Hui-Peng Lv, Peng-Fei Li, Xiao-Gang Chen, Xian-Jiang Song, Yong Ai|2023|Cryst.Growth Des.|23|2602|doi:10.1021/acs.cgd.2c01455
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.cc2865l8
title: CCDC 2091309: Experimental Crystal Structure Determination

description: Related Article: Yang-Yi Liu, Zhi-Qiang Liu, Yu-Qing Wang, Ying Zhou, Yan Qin, Hui-Peng Lv, Peng-Fei Li, Xiao-Gang Chen, Xian-Jiang Song, Yong Ai|2023|Cryst.Growth Des.|23|2602|doi:10.1021/acs.cgd.2c01455
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.cc2bc06y
title: CCDC 2155529: Experimental Crystal Structure Determination

description: Related Article: Zhihui Zhang, Ningjin Zhang, Liang Zhang|2022|CSD Communication|||
description: Related Article: Zhi-Hui Zhang, Qi Zhou, Zhiming Li, Ningjin Zhang, LiangZhang|2022|Chem (Cell Press)|9|847|doi:10.1016/j.chempr.2022.11.009
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: 10.35003/t9yaqe
title: Replication Data for: Mineralogy of volatile-rich clasts in brecciated meteorites

description: Meteoritic breccias are valuable samples as they can contain rare materials from the early solar system as clasts. Volatile-rich, CI- and CM-like clasts may represent parent body lithologies, which cannot be found as individual meteorites in today's meteorite collections. In order to reveal a better knowledge about the presence and chemical characteristics and variability of volatile (water-bearing) materials in the early solar system these clasts play an important role. Such materials may have been available as the volatile component during the accretion of terrestrial planets. To understand the distribution of volatile-rich materials in the solar system, we studied CI- and CM-like clasts in brecciated meteorites including polymict ureilites, HEDs, CR, CB, CH, and ordinary chondrites. CI-like clasts occur throughout all of the mentioned meteorite groups, whereas the CM-like clasts have only been identified in HEDs and ordinary chondrites. The abundance of volatile-rich clasts in general decreases in the order CH &gt; CR &gt; ureilites &gt; HEDs &gt; CB &gt; OC &gt; R. The mineralogy of CI-like clasts is similar to CI chondrites, but their compositions of phyllosilicates differ. The mineralogy of CM-like clasts clearly links them to CM chondrites. They must have been delivered to the HED parent body by low-velocity impacts after differentiation and volcanism, as there is no evidence for high shock and heating processes. Additionally, we propose that CI-like clasts in the CR, CB, and CH chondrites are a primary component of the appropriate parent bodies (accretionary breccias). Conversely, the CI-like clasts in polymict ureilites and HEDs represent an infall as (micro)meteorites or as low-velocity impactors, which happened after the accretion and differentiation of the appropriate parent bodies.
DOI: 10.35003/t9yaqe/db8p0o
title: trr170_paper39_tables_S4_S5_S6.tab

description: :unav
DOI: 10.35003/t9yaqe/oudfyd
title: trr170_paper39_tables_S7_S8.tab

description: :unav
DOI: 10.35003/t9yaqe/83esjq
title: trr170_paper39_tables_S1_S2_S3.tab

description: :unav
DOI: 10.35003/t9yaqe/q4eqea
title: trr170_paper39_table_S9.tab

description: :unav
DOI: 10.35003/t9yaqe/h3ppvd
title: fig_4_trr39.ppt

description: Fe-deficit of sulfides (Fe1−xS) in CI- and CM-like clasts and from C2 chondrites Bells, Essebi, and Tagish Lake. Sulfides in CM-like clasts tend to have a lower Fe deficit compared to those in CI-like clasts and C2 chondrites, which span the whole range.
DOI: 10.35003/t9yaqe/y4m8zu
title: fig_10_trr39.ppt

description: Volatile-rich, CI-like clast DaG999-08 found in a polymict ureilite.
DOI: 10.35003/t9yaqe/edd77j
title: fig_6_trr39.ppt

description: a) Volatile-rich, CI-like clast DaG 164-01 from a polymict ureilite is characterized by framboidal as well as irregularly shaped grains of magnetite, lath-shaped pyrrhotite, and accessory phosphate grains all embedded into a fine-grained phyllosilicate-rich matrix. ...
DOI: 10.35003/t9yaqe/avcxoh
title: fig_12_trr39.ppt

description: Number of identified CI- and CM-like clasts in each meteorite group.
DOI: 10.35003/fy0b6e
title: Replication Data for: Hydrogen isotopic composition of CI- and CM-like clasts from meteorite breccias – Sampling unknown sources of carbonaceous chondrite materials

description: Volatile-rich, CI- and CM-like clasts occur in different brecciated achondrite and chondrite groups. The CI-like clasts in HEDs, polymict ureilites, as well as ordinary, CR, and CB chondrites have a similar mineralogy, indicating a similar alteration history. However, when viewed in detail, their mineral chemistry shows some minor differences between the clasts from different meteorite groups. For CM-like clasts found in HED meteorites, the clasts are, based on their mineralogy, clearly fragments of CM chondrites. To be able to decipher whether CI- (or CM-)like clasts from different meteorite groups are related to certain meteorite classes known to contain volatiles, we obtained D/H ratios of several clasts from the meteorite groups mentioned above and compared them with those of CI and CM chondrites as well as to unique carbonaceous chondrites such as Bells, Essebi, and Tagish Lake. Considering the δD-values, CM-like clasts in HEDs span a similar range compared to bulk values of CM chondrites, further indicating that CM-like clasts are fragments of CM chondrites. For CI-like clasts a clear distinction can be made: While CI-like clasts in HEDs and ordinary chondrites show a very similar range in their δD-signatures compared to “common” CI chondrites, meaning that these clasts are likely related to CI chondrites, the CI-like clasts in polymict ureilites are enriched in D up to 3000‰; a similarly high enrichment is found for the CI-like clasts in CR chondrites. Thus, although the CI-like clasts in ureilites and CR chondrites likely experienced similar alteration histories as the CI-like clasts found in the other meteorite types, these clasts probably formed in a different region than the CI chondrites and, thus, are more accurately referred to as C1 clasts. Overall, the existence and isotopic signatures of the C1 clasts in several meteorite groups proves the existence of additional primitive, volatile-rich material in the (early) Solar System besides the matter we study as the CI, CM, and CR chondrites. This material was distributed throughout the Solar System very early and might have played an important role for the volatile inventory of the terrestrial planets.
DOI: 10.35003/t9yaqe/ly0tnh
title: fig_2_trr39.ppt

description: CM-like clasts in HEDs. White squares show detail images.
DOI: 10.35003/t9yaqe/oqyjxo
title: fig_7_trr39.ppt

description: Composition and abundance of olivine and pyroxene grains in CI-like clasts.
DOI: 10.35003/fy0b6e/0pwayh
title: Table_1_trr80.tab

description: List of samples and the analyzed clast types.
DOI: 10.35003/t9yaqe/wdsvrv
title: fig_13_trr39.ppt

description: Comparison of a CM-like clast from the howardite MAC 02666 and the CM chondrite LON 94101.
DOI: 10.35003/fy0b6e/fkizup
title: Table_3_trr80.tab

description: dD values and D/H, C/H, and Si/H ratios of all analyzed areas sorted by meteorite groups and clast types. C/H and Si/H ratios are subject to systematic uncertainties due to possible matrix effects of at least a factor of 2.
DOI: 10.35003/fy0b6e/ssjt2f
title: Table_2_trr80.tab

description: Typical characteristics of CM- and CI-like clasts from various host meteorites. For more details of CI- and CM-like clasts, we refer to Patzek et al. (2018a).
DOI: 10.35003/t9yaqe/esgjkm
title: fig_8_trr39.ppt

description: a) CI-like clast in the CH3 chondrite Acfer 182-01. The clast is heavily fragmented and contains some grains of Fo-rich olivine. b) ...
DOI: 10.35003/fy0b6e/etygav
title: Patzek-et-al-2019-DH-Research-data-R2_supplement.tab

description: :unav
DOI: 10.35003/t9yaqe/2mbsdi
title: maps.13175.pdf

description: M. Patzek et al. MAPS 2018
DOI: 10.35003/t9yaqe/elecqf
title: fig_1_trr39.ppt

description: Composition and abundance of olivine and pyroxene grains in CM-like clasts.
DOI: 10.35003/fy0b6e/wbruau
title: Figure S1.jpg

description: :unav
DOI: 10.35003/t9yaqe/ctdnoj
title: fig_15_trr39.ppt

description: a, b) Essebi showing magnetite framboids, olivine, and pyroxene grains of different sizes and composition (mostly Mg-rich).
DOI: 10.35003/fy0b6e/8iwbtk
title: Figure 8.png

description: Ranges of dD values of individual measurement spots (colored bars) and weighted averages (symbols within colored bars) for samples from this study.
DOI: 10.35003/fy0b6e/jph5xl
title: Figure 7.png

description: The dD signatures of areas in CM-like clasts obtained in this study and the range of literature data of similar clasts and bulk CM chondrites. T
DOI: 10.35003/t9yaqe/cqejz6
title: fig_14_trr39.ppt

description: a) Unique carbonaceous chondrite clast 09 within the polymict eucrite NWA 7542.
DOI: 10.35003/fy0b6e/xxwt65
title: Figure 2.jpg

description: (a) CI-like clast in the polymict eucrite NWA 7542, which is dominated by phyllosilicate matrix and magnetite grains.
DOI: 10.35003/t9yaqe/h56tid
title: fig_5_trr39.ppt

description: Ternary diagram showing the composition of various carbonates from CI-like clasts in polymict ureilites (green), ordinary chondrites (black), and CM-like clasts in HEDs (red).
DOI: 10.35003/fy0b6e/hmd3nq
title: Figure 9.png

description: The dD signatures of areas in Bells, Essebi, Tagish Lake, and CI-like clasts from ureilites compared to literature data.
DOI: 10.35003/t9yaqe/j17m9o
title: fig_11_trr39.ppt

description: White squares indicate detail images.
DOI: 10.35003/t9yaqe/kqhu3c
title: fig_16_trr39.ppt

description: CI-like lithology in the Kaidun section 56-01 with abundant grains of magnetite, lath-shaped pyrrhotite and large portions of fine-grained phyllosilicate-rich matrix.
DOI: 10.35003/fy0b6e/otdtol
title: Figure 5.jpg

description: D/H vs. Si/H and D/H vs. C/H ratios of 1.25 1.25 mm2 -sized areas in CI-like clasts in ureilites (EET 83309, DaG 319, and DaG 999) and CR chondrites (Al Rais and Renazzo), and in the matrix of Renazzo and Ivuna.
DOI: 10.35003/t9yaqe/4v2xaw
title: fig_3_trr39.ppt

description: Atomic Mg-Fe-Si ternary diagrams showing defocused electron beam analyses of matrix portions.
DOI: 10.35003/fy0b6e/9wprft
title: Figure 1.jpg

description: (a) CM-like clast (no. 11) within the polymict eucrite NWA 7542 contains chondrules or mineral fragments of Mg-rich olivine and pyroxene, which are surrounded by fine-grained rims.
DOI: 10.35003/fy0b6e/bltc3u
title: Figure 6.jpg

description: (a) The H and C ion images of this area in Bells are well correlated.
DOI: 10.35003/t9yaqe/w0qfu9
title: fig_9_trr39.ppt

description: a) BSE image of a sulfide grain with “flame-like” exsolution lamellae of pentlandite from a clast in the polymict ureilite DaG 976. Co (b) and Ni (d) positively correlate within the lamellae.
DOI: 10.35003/fy0b6e/eekgk9
title: Figure 4.png

description: dD values of single analyses carried out on different clasts.
DOI: 10.35003/fy0b6e/earvpu
title: Figure 3.png

description: dD values of five CM-like clasts in the HED meteorites NWA 7542 (diamond), Saricicek (triangle), and EET 87513 (circles) range from 220 to +340‰.