cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.6084/m9.figshare.25241488
title: official dataset for the article, entitled as "Soil tillage effect on the control of invasive Spartina anglica in a coastal wetland" in the publication of a journal of <i>Wetlands Ecology and Management</i>

description: <i>Spartina anglica</i>, an invasive marsh grass, was designated as a harmful marine organism in 2016 due to its ability to stabilize mudflats and reduce macrobenthic diversity. To control such invasive species, physical, chemical, or biological methods can be applied while chemical methods are prohibited by law due to ecological disruption. However, the preferred methods of soil tillage, cutting, and native plant restoration for managing <i>S. anglica</i> have rarely been analyzed. To compare the methods, we performed 9 treatments with four replicates, comprising control, different frequencies of clipping (once and twice) and tilling (once and twice), and different densities (50 and 100 seedling) of restoration of the native plants <i>Suaeda japonica</i> and <i>Phragmites australis</i>. To evaluate the severity of disturbance, we measured coverage, stem density, average plant height, and above-ground biomass for two years. We found <i>P. australis</i> and <i>S. japonica</i> did not successfully establish or survive due to niche differences and the inherent biological features of<i> Spartina</i>. However, physical removal had a stronger effect than interspecific interaction. Two cutting treatments in the early and the late growing season reduced plant height and biomass of <i>S. anglica</i> by 6% and 34%, respectively, compared with the control treatment at the rapid vegetative growth stage in the following year. We also found that two tillage treatments reduced biomass, plant cover, and stem density by 32%, 38%, and 83%, respectively, in the following year. In the study site, managing invasive species such as <i>S. anglica</i> is best achieved by physically destroying the plant using soil tillage while attempting to such as <i>S. anglica</i> demands complete physical destroy by several attempts of soil tillage while attempt to restore native species had marginal control effects.
DOI: 10.6073/pasta/3bb6080db763aec9b384fc60e4560164
title: Consumer Stocks: Physical Data from Everglades National Park (FCE), South Florida from February 1996 to April 2008

description: We hypothesize that standing crops of consumers reflect patterns of allochthonous nutrient transport along the estuarine interface at the Florida Coastal Everglades (FCE) LTER. Our goal is to investigate how variation in hydrology, water quality, and disturbance influence secondary production. This data set represents the physical data of the sampled plots.
DOI: 10.34740/kaggle/dsv/7651712
title: crypto-data-daily-updates
DOI: 10.6084/m9.figshare.3761562.v2857
title: Online Labour Index: Measuring the Online Gig Economy for Policy and Research

description: Data repository for the data underlying the Online Labour Index. See http://ilabour.oii.ox.ac.uk online-labour-index/ for details.
DOI: 10.34740/kaggle/dsv/7651713
title: Public Opinion Russia Ukraine War (Updated Daily)
DOI: 10.25430/researchdata.cab.unipd.it.00001202
title: Data for Periodic protected agriculture mapping at continental scales with Sentinel-2 imagery within the Google Earth Engine platform

description: The collection contains the script as a .txt file to run the classifier OPAC and its whole workflow in the Google Earth Engine platform.
DOI: 10.25919/6h78-s390
title: Parkes observations for project P1219 semester 2023OCTS_20

description: The magnetic field potentially regulates the process of star formation and the evolution of molecular clouds. It is inherently difficult to measure interstellar magnetic field strengths, with the measurement of Zeeman splitting a unique method to estimate the magnetic field strength along the line of sight directly. Despite the detection of Zeeman splitting in other mediums, there are as yet no Zeeman detections against compact background sources in quiescent molecular clouds or the cold neutral medium. Pulsars with extremely small solid angles and relatively high transverse velocities are ideal background sources to study the magnetic field in molecular clouds, providing a distinct signal to measure splitting against. There are four pulsars with OH absorption detections, namely PSR B1849+00, B1641-45, B1718-35, and B1749-28. We propose to utilize these four pulsars to explore the properties of the magnetic field and its variations within molecular clouds through both the Zeeman splitting of OH absorption and rotation measure estimations, between epochs. If a detection is confirmed, it will open a new window on the hard-to-measure magnetic fields in molecular clouds, independent of interpretation, thus shedding light on the physics of star formation and the interstellar medium.
DOI: 10.25919/6xyt-2708
title: Parkes observations for project P1219 semester 2023OCTS_19

description: The magnetic field potentially regulates the process of star formation and the evolution of molecular clouds. It is inherently difficult to measure interstellar magnetic field strengths, with the measurement of Zeeman splitting a unique method to estimate the magnetic field strength along the line of sight directly. Despite the detection of Zeeman splitting in other mediums, there are as yet no Zeeman detections against compact background sources in quiescent molecular clouds or the cold neutral medium. Pulsars with extremely small solid angles and relatively high transverse velocities are ideal background sources to study the magnetic field in molecular clouds, providing a distinct signal to measure splitting against. There are four pulsars with OH absorption detections, namely PSR B1849+00, B1641-45, B1718-35, and B1749-28. We propose to utilize these four pulsars to explore the properties of the magnetic field and its variations within molecular clouds through both the Zeeman splitting of OH absorption and rotation measure estimations, between epochs. If a detection is confirmed, it will open a new window on the hard-to-measure magnetic fields in molecular clouds, independent of interpretation, thus shedding light on the physics of star formation and the interstellar medium.
DOI: 10.25919/sqq9-sm68
title: Parkes observations for project P1219 semester 2023OCTS_18

description: The magnetic field potentially regulates the process of star formation and the evolution of molecular clouds. It is inherently difficult to measure interstellar magnetic field strengths, with the measurement of Zeeman splitting a unique method to estimate the magnetic field strength along the line of sight directly. Despite the detection of Zeeman splitting in other mediums, there are as yet no Zeeman detections against compact background sources in quiescent molecular clouds or the cold neutral medium. Pulsars with extremely small solid angles and relatively high transverse velocities are ideal background sources to study the magnetic field in molecular clouds, providing a distinct signal to measure splitting against. There are four pulsars with OH absorption detections, namely PSR B1849+00, B1641-45, B1718-35, and B1749-28. We propose to utilize these four pulsars to explore the properties of the magnetic field and its variations within molecular clouds through both the Zeeman splitting of OH absorption and rotation measure estimations, between epochs. If a detection is confirmed, it will open a new window on the hard-to-measure magnetic fields in molecular clouds, independent of interpretation, thus shedding light on the physics of star formation and the interstellar medium.
DOI: 10.25919/1q01-tq67
title: Parkes observations for project P630 semester 2009APRS_16

description: We propose to carry out the most ambitious and comprehensive all-sky survey for pulsars and transient sources to date. Using the 20cm multibeam and a new digital filterbank array this survey will create a petabyte digital record of the sky that can be data mined in the future and used to search for relativistic binary and millisecond pulsars, RRATs, and extragalactic radio bursts. The survey should discover 100s of new millisecond and normal pulsars and help define the lower limit to pulsar periods, test theories of relativistic gravity, find transients and provide pulsars for gravitational wave detection. With all the hardware in place, and our first new pulsar discovery made, we request a substantial time allocation this semester.
DOI: 10.5281/zenodo.10257484
title: Bare LIG_Universal VLS2.30DT_Clemson University

description: Bare LIG electrodes used as the main dataset in Qian et al manuscript
DOI: 10.5281/zenodo.10257485
title: Bare LIG_Universal VLS2.30DT_Clemson University

description: Bare LIG electrodes used as the main dataset in Qian et al manuscript
DOI: 10.5519/qd.t6trtdp4
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (5774467 records)
DOI: 10.5281/zenodo.10581569
title: E. coli aptasensr data_Qian et al (2023)

description: This dataset was developed in the biosensors lab (McLamore PI) as part of the SmartPath Center of Excllence. The data was a component of a collaboratiove project that led to a publication by Qian et al (2023). A link to the published manuscript in ACS Omega is below

https://pubs.acs.org/doi/full/10.1021/acsomega.3c05797
DOI: 10.5281/zenodo.10581570
title: E. coli aptasensr data_Qian et al (2023)

description: This dataset was developed in the biosensors lab (McLamore PI) as part of the SmartPath Center of Excllence. The data was a component of a collaboratiove project that led to a publication by Qian et al (2023). A link to the published manuscript in ACS Omega is below

https://pubs.acs.org/doi/full/10.1021/acsomega.3c05797
DOI: 10.25919/smqt-ne98
title: Parkes observations for project P1219 semester 2023OCTS_21

description: The magnetic field potentially regulates the process of star formation and the evolution of molecular clouds. It is inherently difficult to measure interstellar magnetic field strengths, with the measurement of Zeeman splitting a unique method to estimate the magnetic field strength along the line of sight directly. Despite the detection of Zeeman splitting in other mediums, there are as yet no Zeeman detections against compact background sources in quiescent molecular clouds or the cold neutral medium. Pulsars with extremely small solid angles and relatively high transverse velocities are ideal background sources to study the magnetic field in molecular clouds, providing a distinct signal to measure splitting against. There are four pulsars with OH absorption detections, namely PSR B1849+00, B1641-45, B1718-35, and B1749-28. We propose to utilize these four pulsars to explore the properties of the magnetic field and its variations within molecular clouds through both the Zeeman splitting of OH absorption and rotation measure estimations, between epochs. If a detection is confirmed, it will open a new window on the hard-to-measure magnetic fields in molecular clouds, independent of interpretation, thus shedding light on the physics of star formation and the interstellar medium.
DOI: 10.25919/whe4-3s93
title: Parkes pulsar observations with undefined project IDs for 2023OCTS_22

description: Parkes pulsar observations with undefined project IDs for 2023OCTS. This collection contains observations from project IDs PX114 and PX127.
DOI: 10.6084/m9.figshare.20915780
title: Understanding the diversity and phylogenetic placements of New Zealand amphipods within a global context

description: Amphipods are an ecologically diverse group of crustaceans. Due to the limited number of fossil data and common morphological homoplasy, molecular data can be very useful to understand their evolutionary relationships and history. However, despite their global distribution and an increasing number of phylogenetic studies, molecular data from the Southern Hemisphere is considerably limited. Here, I report multigene data (18S, 28S, and COI) of New Zealand endemic freshwater families as well as some other marine taxa. Also, I report two new species/genera that have not been described yet. Phylogenetic analyses were conducted including major amphipod groups to understand phylogenetic placements of New Zealand amphipods. Based on the ML and Bayesian trees, <i>Paracallipe</i>, <i>Paraleptamphopus</i>, and the two unknown species belong to the eusiroids/iphimedioids clade; <i>Parorchestia</i> and a talitrid species clearly belong to talitroids; <i>Paracorophium</i> and <i>Monocorophium</i> were placed within corophiids; <i>Themisto</i> belongs to physosomatans; <i>Josephosella</i> was closely related to other hadzoids. The present study suggests that the Southern and Northern Hemisphere freshwater amphipods are likely to have originated from different marine ancestors. Molecular data from other regions in the Southern Hemisphere will be highly valuable for understanding the phylogeographic histories of amphipods that have shaped the current diversity and distribution.
DOI: 10.6084/m9.figshare.20478736
title: Factors influencing cyanobacteria blooms: review of the historical monitoring data to assess management options for Lake Horowhenua

description: Factors influencing cyanobacterial blooms in Lake Horowhenua, Aotearoa/New Zealand, have been deduced from over 40 yrs routine monitoring data, detailed studies and high frequency (15-min interval) data from an in-lake monitoring buoy. Lake Horowhenua is currently hypertrophic but flips between a winter clear-water, macrophyte dominated phase (<i>Potamogeton crispus),</i> and a turbid phytoplankton dominated phase with substantial cyanobacterial (<i>Microcystis sp.</i>) blooms from mid-summer to autumn. Nitrogen for growth comes from agriculture and horticulture via groundwater and spring-fed streams. Phosphorus is released from the sediment when the weed beds die back. These nutrients stimulate the growth of <i>Microcystis sp.</i>, until the water temperature falls below 15°C. <i>Microcystis sp</i> can raise the pH to over 10, which releases P from the sediment, sustaining its growth. High pH transforms non-toxic ammonium-N released from the sediment to toxic unionised NH<sub>3</sub>, which may contribute to fish kills in summer/autumn. Management strategies cannot use P-inactivation agents for cultural reasons and eradicating the macrophyte beds by spraying would cause the lake to permanently flip to a turbid state. Management of the macrophyte beds with a weed harvester is being trialled to allow a gradual replacement of <i>P. crispus</i> with indigenous species from the seed bank in the sediment.
DOI: 10.6084/m9.figshare.20478736.v1
title: Factors influencing cyanobacteria blooms: review of the historical monitoring data to assess management options for Lake Horowhenua

description: Factors influencing cyanobacterial blooms in Lake Horowhenua, Aotearoa/New Zealand, have been deduced from over 40 yrs routine monitoring data, detailed studies and high frequency (15-min interval) data from an in-lake monitoring buoy. Lake Horowhenua is currently hypertrophic but flips between a winter clear-water, macrophyte dominated phase (<i>Potamogeton crispus),</i> and a turbid phytoplankton dominated phase with substantial cyanobacterial (<i>Microcystis sp.</i>) blooms from mid-summer to autumn. Nitrogen for growth comes from agriculture and horticulture via groundwater and spring-fed streams. Phosphorus is released from the sediment when the weed beds die back. These nutrients stimulate the growth of <i>Microcystis sp.</i>, until the water temperature falls below 15°C. <i>Microcystis sp</i> can raise the pH to over 10, which releases P from the sediment, sustaining its growth. High pH transforms non-toxic ammonium-N released from the sediment to toxic unionised NH<sub>3</sub>, which may contribute to fish kills in summer/autumn. Management strategies cannot use P-inactivation agents for cultural reasons and eradicating the macrophyte beds by spraying would cause the lake to permanently flip to a turbid state. Management of the macrophyte beds with a weed harvester is being trialled to allow a gradual replacement of <i>P. crispus</i> with indigenous species from the seed bank in the sediment.
DOI: 10.6084/m9.figshare.20915780.v1
title: Understanding the diversity and phylogenetic placements of New Zealand amphipods within a global context

description: Amphipods are an ecologically diverse group of crustaceans. Due to the limited number of fossil data and common morphological homoplasy, molecular data can be very useful to understand their evolutionary relationships and history. However, despite their global distribution and an increasing number of phylogenetic studies, molecular data from the Southern Hemisphere is considerably limited. Here, I report multigene data (18S, 28S, and COI) of New Zealand endemic freshwater families as well as some other marine taxa. Also, I report two new species/genera that have not been described yet. Phylogenetic analyses were conducted including major amphipod groups to understand phylogenetic placements of New Zealand amphipods. Based on the ML and Bayesian trees, <i>Paracallipe</i>, <i>Paraleptamphopus</i>, and the two unknown species belong to the eusiroids/iphimedioids clade; <i>Parorchestia</i> and a talitrid species clearly belong to talitroids; <i>Paracorophium</i> and <i>Monocorophium</i> were placed within corophiids; <i>Themisto</i> belongs to physosomatans; <i>Josephosella</i> was closely related to other hadzoids. The present study suggests that the Southern and Northern Hemisphere freshwater amphipods are likely to have originated from different marine ancestors. Molecular data from other regions in the Southern Hemisphere will be highly valuable for understanding the phylogeographic histories of amphipods that have shaped the current diversity and distribution.
DOI: 10.5281/zenodo.10628850
title: Calibration-Independent Certification of a Quantum Frequency Converter

description: This upload contains the data set for the manuscript titled "Calibration-Independent Certification of a Quantum Frequency Converter". Notes describing the added data set are uploaded alongside. Please see the Arxiv version https://arxiv.org/abs/2304.09517 for plots.
DOI: 10.5281/zenodo.10628851
title: Calibration-Independent Certification of a Quantum Frequency Converter

description: This upload contains the data set for the manuscript titled "Calibration-Independent Certification of a Quantum Frequency Converter". Notes describing the added data set are uploaded alongside. Please see the Arxiv version https://arxiv.org/abs/2304.09517 for plots.
DOI: 10.25345/c5xk8520r
title: MassIVE MSV000094112 - Analysis of Synaptic Palmitoylated Proteins in a CLN1 Mouse Model
title: Palmitoylation is a lipid modification that is critical for protein trafficking. Conversely, depalmitoylation detaches palmitic acid from modified proteins in the cytosol or endolysosome to regulate their recycling and degradation. The balance between these two opposing mechanisms controls proteostasis. While the role of palmitoylation is well-established in neuronal differentiation and synaptic plasticity, depalmitoylation is far less understood. Here, we study a lysosomal depalmitoylating enzyme, palmitoyl-protein thioesterase 1 (PPT1), which is associated with the devastating neurodegenerative disease infantile neuronal ceroid lipofuscinosis (CLN1).
DOI: 10.5281/zenodo.10414530
title: Hindcasting small mammal assemblages

description: These data and code are associated with:

xxx (submitted). Hindcasting long-term data unveils the influence of a changing climate on small mammal communities.
DOI: 10.5281/zenodo.10414531
title: Hindcasting small mammal assemblages

description: These data and code are associated with:

xxx (submitted). Hindcasting long-term data unveils the influence of a changing climate on small mammal communities.
DOI: 10.5281/zenodo.10676790
title: Bottle Data HOT, Station WHOTS 52

description: This dataset contains CTD data and data from water samples collected at discrete depths via Niskin bottles mounted on the CTD rosette at HOT (Hawaii Ocean Time Series) station WHOTS 52. WHOTS 52 includes a surface mooring outfitted for meteorological and oceanographic measurements, the location of which alternates between the eastern (WHOTS 50) and southern (WHOTS 52) edges of ALOHA.  These sites are in collaboration with Woods Hole Oceanographic Institution. Time is in a separate column from date and is in GMT. 

(https://www.soest.hawaii.edu/whots/)

(https://hahana.soest.hawaii.edu/hot/intro.html)
DOI: 10.5281/zenodo.10676791
title: Bottle Data HOT, Station WHOTS 52

description: This dataset contains CTD data and data from water samples collected at discrete depths via Niskin bottles mounted on the CTD rosette at HOT (Hawaii Ocean Time Series) station WHOTS 52. WHOTS 52 includes a surface mooring outfitted for meteorological and oceanographic measurements, the location of which alternates between the eastern (WHOTS 50) and southern (WHOTS 52) edges of ALOHA.  These sites are in collaboration with Woods Hole Oceanographic Institution. Time is in a separate column from date and is in GMT. 

(https://www.soest.hawaii.edu/whots/)

(https://hahana.soest.hawaii.edu/hot/intro.html)
DOI: 10.25505/fiz.icsd.cc2h89mq
title: CSD 2301893: Experimental Crystal Structure Determination

description: Related Article: Jason Lively and Aaron Celestian|2024|ICSD Communication|||
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.cc2h8bfk
title: CSD 2301918: Experimental Crystal Structure Determination

description: Related Article: Jason Lively and Aaron Celestian|2024|ICSD Communication|||
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.cc2h8bgl
title: CSD 2301919: Experimental Crystal Structure Determination

description: Related Article: Jason Lively and Aaron Celestian|2024|ICSD Communication|||
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.cc2h8bhm
title: CSD 2301920: Experimental Crystal Structure Determination

description: Related Article: Jason Lively and Aaron Celestian|2024|ICSD Communication|||
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.