cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5061/dryad.3m8p1
title: Data from: Thresholds and gradients in a semi-arid grassland: long-term grazing treatments induce slow, continuous and reversible vegetation change

description: 1. Temporal changes in semi-arid ecosystems can include transitions
 between alternative stable states, involving thresholds and multiple
 domains of attraction, but can also include relatively continuous,
 symmetric and reversible shifts within a single stable state. Conceptual
 state-and-transition models (STMs) describe both types of ecosystem
 dynamics by including state transitions (plant community changes
 difficult-to-reverse without substantial input or effort) and phase shifts
 (easily reversible community changes) as consequences of management
 practices and environmental variability. Grazing management is purported
 to be the primary driver of state transitions in current STMs for North
 American grasslands, but there is limited empirical evidence from these
 grasslands showing that grazing can cause difficult-to-reverse transitions
 between alternate stable states. 2 .In a northern mixed-grass prairie in
 Wyoming, USA, we examined plant community responses to (i) long-term
 (33-year) grazing intensity treatments (none, light, moderate and heavy
 stocking rates) and (ii) 8 years of light or no grazing in pastures that
 were grazed heavily for the previous 25 years. 3. Long-term grazing
 treatments were associated with distinct, but not stable, plant
 communities. From year 22 to 33, heavier stocking rates decreased cover of
 dominant C3 grasses and increased cover of the dominant C4 grass Bouteloua
 gracilis. 4. Reversing stocking rates from heavy to light or no grazing
 resulted in reversal of changes induced by prior heavy stocking for
 dominant C3 grasses, but not for B. gracilis. For both groups, rates of
 change following grazing treatment reversals were consistent with rates of
 change during the initial years of the experiment (1982–1990). 5.
 Synthesis and applications. In a semi-arid rangeland with a long
 evolutionary history of grazing, different long-term grazing intensity
 treatments caused slow, continuous, and directional changes with important
 management implications, but did not appear to induce alternative stable
 states. For this and similar ecosystems, quantifying the time-scales and
 compositional gradients associated with key phase shifts may be more
 important than identifying thresholds between alternative stable states.
description: Absolute Basal Cover by
 SpeciesAnalyses reported in the
 paper are based on the basal cover data included in this file. A species
 list is included to link species codes with scientific
 names.Porensky_etal_2016_basal_absolute_cover.xlsx
DOI: 10.17182/hepdata.132661.v2/t1
title: "Table 1" of "Beam Energy Dependence of Fifth and Sixth-Order Net-proton Number Fluctuations in Au+Au Collisions at RHIC"

description: Event-by-event proton multiplicity distributions for 0-40$\%$, 0-5$\%$ and 50-60$\%$ Au+Au collisions at $\sqrt{s_{NN}} = 3 GeV. The distributions are not corrected for proton and antiproton detection efficiency.
description: No data abstract available.
DOI: 10.17182/hepdata.132661.v2/t2
title: "Table 2" of "Beam Energy Dependence of Fifth and Sixth-Order Net-proton Number Fluctuations in Au+Au Collisions at RHIC"

description: Proton factorial cumulants K4, K5 and K6 in 0-40$\%$ and 50-60$\%$ Au+Au collisions from $\sqrt{s_{NN}}$ = 3 - 200 GeV. At $\sqrt{s_{NN}}$ = 3 GeV, measurement is done with halfrapdity coverage (-0.5 $&lt;$ y $&lt;$ 0) while for rest of energies the rapidity coverage is (-0.5 $&lt;$ y $&lt;$ -0.5).
description: No data abstract available.
DOI: 10.17182/hepdata.132661.v2/t3
title: "Table 3" of "Beam Energy Dependence of Fifth and Sixth-Order Net-proton Number Fluctuations in Au+Au Collisions at RHIC"

description: Proton factorial cumulants K4, K5 and K6 from UrQMD model (0-40$\%$ and 50-60$\%$ centrality) for Au+Au collisions from $\sqrt{s_{NN}}$ = 3 - 200 GeV. UrQMD calculation for 3 GeVis with rapidity coverage (-0.5 $&lt;$ y $&lt;$ 0) while for rest of energies the rapidity coverage is (-0.5 $&lt;$ y $&lt;$ -0.5). In addition, two-component model (0-40$\%$) calculations for facorial cumulants are also given.
description: No data abstract available.
DOI: 10.17182/hepdata.132661.v2/t4
title: "Table 4" of "Beam Energy Dependence of Fifth and Sixth-Order Net-proton Number Fluctuations in Au+Au Collisions at RHIC"

description: Net-proton cumulant ratios C4/C2, C5/C1, C6/C2 (0-40$\%$ and 50-60$\%$ centrality) and C3/C1 (0-40$\%$ centrality) in Au+Au collisions from $\sqrt{s_{NN}}$ = 3 - 200 GeV. At $\sqrt{s_{NN}}$ = 3 GeV, measurement is done for protons instead of net-protons, and with halfrapdity coverage (-0.5 $&lt;$ y $&lt;$ 0) while for rest of energies the rapidity coverage is (-0.5 $&lt;$ y $&lt;$ -0.5).
description: No data abstract available.
DOI: 10.17182/hepdata.132661.v2/t5
title: "Table 5" of "Beam Energy Dependence of Fifth and Sixth-Order Net-proton Number Fluctuations in Au+Au Collisions at RHIC"

description: Net-proton cumulant ratios C4/C2, C5/C1, C6/C2 (0-40$\%$ and 50-60$\%$ centrality) and C3/C1 (0-40$\%$ centrality) from UrQMD model in Au+Au collisions from $\sqrt{s_{NN}}$ = 3 -200 GeV. At $\sqrt{s_{NN}}$ = 3 GeV, UrQMD calculation is done for protons instead of net-protons, and with halfrapdity coverage (-0.5 $&lt;$ y $&lt;$ 0) while for rest of energies the rapidity coverage is (-0.5 $&lt;$ y $&lt;$ -0.5).
description: No data abstract available.
DOI: 10.17182/hepdata.132661.v2/t6
title: "Table 6" of "Beam Energy Dependence of Fifth and Sixth-Order Net-proton Number Fluctuations in Au+Au Collisions at RHIC"

description: Fifth-to-first (KS5/KS1) and sixth-to-second (KS6/KS2) order K-statistic ratios of net-proton distributions in Au+Au collisions at $\sqrt{s_{NN}}$ = 7.7 GeV for 0-40$\%$ and 50-60$\%$ centrality.
description: No data abstract available.
DOI: 10.17182/hepdata.132661.v2/t7
title: "Table 7" of "Beam Energy Dependence of Fifth and Sixth-Order Net-proton Number Fluctuations in Au+Au Collisions at RHIC"

description: Net-proton cumulant ratio C6/C2 and corresponding K-statistic ratio (0-40$\%$) in Au+Au collisions at $\sqrt{s_{NN}}$ = 7.7 GeV as a function of sample size. Uncertainties are only statistical.
description: No data abstract available.
DOI: 10.17182/hepdata.132661.v2/t8
title: "Table 8" of "Beam Energy Dependence of Fifth and Sixth-Order Net-proton Number Fluctuations in Au+Au Collisions at RHIC"

description: Cumulant ratios C4/C2, C5/C1, C6/C2 and C3/C1 of net-proton distributions measured with half rapdity coverage (-0.5 $&lt;$ y $&lt;$ 0) in 0-40$\%$ central Au+Au collisions for collider energies from $\sqrt{s_{NN}}$ = 7.7 - 54.4 GeV.
description: No data abstract available.
DOI: 10.5061/dryad.86gm0
title: Data from: Multicollinearity in spatial genetics: separating the wheat from the chaff using commonality analyses

description: Direct gradient analyses in spatial genetics provide unique opportunities
 to describe the inherent complexity of genetic variation in wildlife
 species and are the object of many methodological developments. However,
 multicollinearity among explanatory variables are a systemic issue in
 multivariate regression analyses and are likely to cause serious
 difficulties in properly interpreting results of direct gradient analyses,
 with the risk of erroneous conclusions, misdirected research and
 inefficient or counter-productive conservation measures. Using simulated
 datasets along with linear and logistic regressions on distance matrices,
 we illustrate how commonality analysis (CA), a detailed variance
 partitioning procedure that was recently introduced in the field of
 ecology, can be used to deal with non-independence among spatial
 predictors. By decomposing model fit indices into unique and common (or
 shared) variance components, CA allows identifying the location and
 magnitude of multicollinearity, revealing spurious correlations and thus
 thoroughly improving the interpretation of multivariate regressions.
 Despite a few inherent limitations, especially in the case of resistance
 model optimisation, this review highlights the great potential of CA to
 account for complex multicollinearity patterns in spatial genetics and
 identifies future applications and lines of research. We strongly urge
 spatial geneticists to systematically investigate commonalities when
 performing direct gradient analyses.
description: Data and R-scripts used
 to get results presented in the manuscript.Data were simulated
 using CDpop. R-scripts were used in R 3.1.0.Data and Scripts_Prunier et
 al_MEC.zip
DOI: 10.17182/hepdata.132661.v3/t1
title: "Table 1" of "Beam Energy Dependence of Fifth and Sixth-Order Net-proton Number Fluctuations in Au+Au Collisions at RHIC"

description: Event-by-event proton multiplicity distributions for 0-40$\%$, 0-5$\%$ and 50-60$\%$ Au+Au collisions at $\sqrt{s_{NN}} = 3 GeV. The distributions are not corrected for proton and antiproton detection efficiency.
description: No data abstract available.
DOI: 10.17182/hepdata.132661.v3/t2
title: "Table 2" of "Beam Energy Dependence of Fifth and Sixth-Order Net-proton Number Fluctuations in Au+Au Collisions at RHIC"

description: Proton factorial cumulants K4, K5 and K6 in 0-40$\%$ and 50-60$\%$ Au+Au collisions from $\sqrt{s_{NN}}$ = 3 - 200 GeV. At $\sqrt{s_{NN}}$ = 3 GeV, measurement is done with halfrapdity coverage (-0.5 $&lt;$ y $&lt;$ 0) while for rest of energies the rapidity coverage is (-0.5 $&lt;$ y $&lt;$ -0.5).
description: No data abstract available.
DOI: 10.17182/hepdata.132661.v3/t3
title: "Table 3" of "Beam Energy Dependence of Fifth and Sixth-Order Net-proton Number Fluctuations in Au+Au Collisions at RHIC"

description: Proton factorial cumulants K4, K5 and K6 from UrQMD model (0-40$\%$ and 50-60$\%$ centrality) for Au+Au collisions from $\sqrt{s_{NN}}$ = 3 - 200 GeV. UrQMD calculation for 3 GeVis with rapidity coverage (-0.5 $&lt;$ y $&lt;$ 0) while for rest of energies the rapidity coverage is (-0.5 $&lt;$ y $&lt;$ -0.5). In addition, two-component model (0-40$\%$) calculations for facorial cumulants are also given.
description: No data abstract available.
DOI: 10.17182/hepdata.132661.v3/t4
title: "Table 4" of "Beam Energy Dependence of Fifth and Sixth-Order Net-proton Number Fluctuations in Au+Au Collisions at RHIC"

description: Net-proton cumulant ratios C4/C2, C5/C1, C6/C2 (0-40$\%$ and 50-60$\%$ centrality) and C3/C1 (0-40$\%$ centrality) in Au+Au collisions from $\sqrt{s_{NN}}$ = 3 - 200 GeV. At $\sqrt{s_{NN}}$ = 3 GeV, measurement is done for protons instead of net-protons, and with halfrapdity coverage (-0.5 $&lt;$ y $&lt;$ 0) while for rest of energies the rapidity coverage is (-0.5 $&lt;$ y $&lt;$ -0.5).
description: No data abstract available.
DOI: 10.17182/hepdata.132661.v3/t5
title: "Table 5" of "Beam Energy Dependence of Fifth and Sixth-Order Net-proton Number Fluctuations in Au+Au Collisions at RHIC"

description: Net-proton cumulant ratios C4/C2, C5/C1, C6/C2 (0-40$\%$ and 50-60$\%$ centrality) and C3/C1 (0-40$\%$ centrality) from UrQMD model in Au+Au collisions from $\sqrt{s_{NN}}$ = 3 -200 GeV. At $\sqrt{s_{NN}}$ = 3 GeV, UrQMD calculation is done for protons instead of net-protons, and with halfrapdity coverage (-0.5 $&lt;$ y $&lt;$ 0) while for rest of energies the rapidity coverage is (-0.5 $&lt;$ y $&lt;$ -0.5).
description: No data abstract available.
DOI: 10.17182/hepdata.132661.v3/t6
title: "Table 6" of "Beam Energy Dependence of Fifth and Sixth-Order Net-proton Number Fluctuations in Au+Au Collisions at RHIC"

description: Fifth-to-first (KS5/KS1) and sixth-to-second (KS6/KS2) order K-statistic ratios of net-proton distributions in Au+Au collisions at $\sqrt{s_{NN}}$ = 7.7 GeV for 0-40$\%$ and 50-60$\%$ centrality.
description: No data abstract available.
DOI: 10.17182/hepdata.132661.v3/t7
title: "Table 7" of "Beam Energy Dependence of Fifth and Sixth-Order Net-proton Number Fluctuations in Au+Au Collisions at RHIC"

description: Net-proton cumulant ratio C6/C2 and corresponding K-statistic ratio (0-40$\%$) in Au+Au collisions at $\sqrt{s_{NN}}$ = 7.7 GeV as a function of sample size. Uncertainties are only statistical.
description: No data abstract available.
DOI: 10.15468/dl.fcru4c
title: Occurrence Download

description: A dataset containing 686 species occurrences available in GBIF matching the query:
{
 "and" : [
 "BasisOfRecord is one of (Machine Observation, Observation, Human Observation, Living Specimen, Occurrence evidence)",
 "HasCoordinate is true",
 "HasGeospatialIssue is false",
 "License is one of (CC0 1.0, CC-BY 4.0)",
 "OccurrenceStatus is Present",
 "TaxonKey is Amaranthus palmeri",
 "Year 2000-2026"
 ]
}

 The dataset includes 686 records from 18 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0000699-260126135527185/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.17182/hepdata.132661.v3/t8
title: "Table 8" of "Beam Energy Dependence of Fifth and Sixth-Order Net-proton Number Fluctuations in Au+Au Collisions at RHIC"

description: Cumulant ratios C4/C2, C5/C1, C6/C2 and C3/C1 of net-proton distributions measured with half rapdity coverage (-0.5 $&lt;$ y $&lt;$ 0) in 0-40$\%$ central Au+Au collisions for collider energies from $\sqrt{s_{NN}}$ = 7.7 - 54.4 GeV.
description: No data abstract available.
DOI: 10.17182/hepdata.132661.v3/t9
title: "Table 9" of "Beam Energy Dependence of Fifth and Sixth-Order Net-proton Number Fluctuations in Au+Au Collisions at RHIC"

description: Cumulant ratios C5/C1 of net-proton distributions measured in 40-50$\%$, 60-70$\%$, and 70-80$\%$ Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV. This is supplemental data and was not part of the original paper.
description: No data abstract available.
DOI: 10.17182/hepdata.147191.v1/t1
title: "fig1_0" of "Jet-hadron correlations with respect to the event plane in $\sqrt{s_{\mathrm{NN}}}$ = 200 GeV Au+Au collisions in STAR"

description: Event-plane resolution, second-order harmonic relative to the event plane, $R_{2}(\Psi_{2})$, respectively.
description: Angular distributions of charged particles relative to jet axes are studied in $\sqrt{s_{NN}} = 200$ GeV Au+Au collisions as a function of the jet orientation with respect to the event plane. This differential study tests the expected path-length dependence of energy loss experienced by a hard-scattered parton as it traverses the hot and dense medium formed in heavy-ion collisions. A second-order event plane is used in the analysis as an experimental estimate of the reaction plane formed by the collision impact parameter and the beam direction. Charged-particle jets with $15 &lt; p_{T, jet} &lt;$ 20 and $20 &lt; p_{T, jet} &lt;$ 40 GeV\c were reconstructed with the anti-$k_T$ algorithm with radius parameter setting of $R=0.4$ in the 20-50% centrality bin to maximize the initial-state eccentricity of the interaction region. The reaction plane fit method is implemented to remove the flow-modulated background with better precision than prior methods. Yields and widths of jet-associated charged-hadron distributions are extracted in three angular bins between the jet axis and the event plane. The event-plane (EP) dependence is further quantified by ratios of the associated yields in different EP bins. No dependence on orientation of the jet axis with respect to the event plane is seen within the uncertainties in the kinematic regime studied. This finding is consistent with a similar experimental observation by ALICE in $\sqrt{s_{NN}} = 2.76$ TeV Pb+Pb collision data.
DOI: 10.17182/hepdata.147191.v1/t2
title: "fig1_1" of "Jet-hadron correlations with respect to the event plane in $\sqrt{s_{\mathrm{NN}}}$ = 200 GeV Au+Au collisions in STAR"

description: Event-plane resolution, second-order harmonic relative to the event plane, $R_{4}(\Psi_{2})$, respectively.
description: Angular distributions of charged particles relative to jet axes are studied in $\sqrt{s_{NN}} = 200$ GeV Au+Au collisions as a function of the jet orientation with respect to the event plane. This differential study tests the expected path-length dependence of energy loss experienced by a hard-scattered parton as it traverses the hot and dense medium formed in heavy-ion collisions. A second-order event plane is used in the analysis as an experimental estimate of the reaction plane formed by the collision impact parameter and the beam direction. Charged-particle jets with $15 &lt; p_{T, jet} &lt;$ 20 and $20 &lt; p_{T, jet} &lt;$ 40 GeV\c were reconstructed with the anti-$k_T$ algorithm with radius parameter setting of $R=0.4$ in the 20-50% centrality bin to maximize the initial-state eccentricity of the interaction region. The reaction plane fit method is implemented to remove the flow-modulated background with better precision than prior methods. Yields and widths of jet-associated charged-hadron distributions are extracted in three angular bins between the jet axis and the event plane. The event-plane (EP) dependence is further quantified by ratios of the associated yields in different EP bins. No dependence on orientation of the jet axis with respect to the event plane is seen within the uncertainties in the kinematic regime studied. This finding is consistent with a similar experimental observation by ALICE in $\sqrt{s_{NN}} = 2.76$ TeV Pb+Pb collision data.
DOI: 10.17182/hepdata.147191.v1/t3
title: "fig4_0" of "Jet-hadron correlations with respect to the event plane in $\sqrt{s_{\mathrm{NN}}}$ = 200 GeV Au+Au collisions in STAR"

description: $p_{T, jet}$ resolution for $15 &lt; p_{T, jet}^{GEN} &lt; 20$ GeV/c $R=0.4$ full jets. Jets are measured from all angles relative to the event plane in the 20-50% most central events.
description: Angular distributions of charged particles relative to jet axes are studied in $\sqrt{s_{NN}} = 200$ GeV Au+Au collisions as a function of the jet orientation with respect to the event plane. This differential study tests the expected path-length dependence of energy loss experienced by a hard-scattered parton as it traverses the hot and dense medium formed in heavy-ion collisions. A second-order event plane is used in the analysis as an experimental estimate of the reaction plane formed by the collision impact parameter and the beam direction. Charged-particle jets with $15 &lt; p_{T, jet} &lt;$ 20 and $20 &lt; p_{T, jet} &lt;$ 40 GeV\c were reconstructed with the anti-$k_T$ algorithm with radius parameter setting of $R=0.4$ in the 20-50% centrality bin to maximize the initial-state eccentricity of the interaction region. The reaction plane fit method is implemented to remove the flow-modulated background with better precision than prior methods. Yields and widths of jet-associated charged-hadron distributions are extracted in three angular bins between the jet axis and the event plane. The event-plane (EP) dependence is further quantified by ratios of the associated yields in different EP bins. No dependence on orientation of the jet axis with respect to the event plane is seen within the uncertainties in the kinematic regime studied. This finding is consistent with a similar experimental observation by ALICE in $\sqrt{s_{NN}} = 2.76$ TeV Pb+Pb collision data.
DOI: 10.5061/dryad.r3408
title: Data from: Neglecting the call of the wild: captive frogs like the sound of their own voice

description: Acoustic communication is highly influential in the expression of social
 behavior by anuran amphibians, transmitting information about the
 individual’s physical condition and motivation. We studied the phonotactic
 (approach movements) responses of wild and captive male golden mantella
 frogs to conspecific wild and captive playback calls to determine the
 impact of captivity on social behaviour mediated by vocalisations. Calls
 were recorded from one wild and two captive populations. Phonotaxis
 experiments were then conducted by attracting M. aurantiaca males across a
 PVC grid on the forest floor or enclosure floor to a speaker. For each
 playback, the following parameters were recorded to define the accuracy of
 phonotaxis: (1) number of jumps; (2) jump angles; (3) jump distances; (4)
 path straightness. During this experiment we observed that wild frogs had
 a similar behavioural (phonotaxis) response to calls independent of their
 source while frogs from Chester Zoo had a significantly stronger response
 to calls of other conspecifics held separately at Chester Zoo. The lack of
 appropriate phonotaxis response by captive bred frogs to the calls of wild
 conspecifics could have serious negative conservation implications, if the
 captive bred individuals were released back to the wild.
description: Phonotaxis_dataParamenters for phonotaxis responses of captive and wild golden mantellas to a playback experiment using 3 different calls.Tabela_ChesterCallingCall parameters from chester zoo golden mantella captive colonyTabela_MitsinjoCallingCall parameters of vocalization of Mitisnjo breeding center golden matella captive colonyTabela_MangabeCallingCall parameters from wild golden mantella populations from MangabeTI_MadagascarTonic immobility response and morphometric data of golden mantellas frogs from Madagascar
DOI: 10.17182/hepdata.147191.v1/t4
title: "fig4_1" of "Jet-hadron correlations with respect to the event plane in $\sqrt{s_{\mathrm{NN}}}$ = 200 GeV Au+Au collisions in STAR"

description: $p_{T, jet}$ resolution for $20 &lt; p_{T, jet}^{GEN} &lt; 40$ GeV/c $R=0.4$ full jets. Jets are measured from all angles relative to the event plane in the 20-50% most central events.
description: Angular distributions of charged particles relative to jet axes are studied in $\sqrt{s_{NN}} = 200$ GeV Au+Au collisions as a function of the jet orientation with respect to the event plane. This differential study tests the expected path-length dependence of energy loss experienced by a hard-scattered parton as it traverses the hot and dense medium formed in heavy-ion collisions. A second-order event plane is used in the analysis as an experimental estimate of the reaction plane formed by the collision impact parameter and the beam direction. Charged-particle jets with $15 &lt; p_{T, jet} &lt;$ 20 and $20 &lt; p_{T, jet} &lt;$ 40 GeV\c were reconstructed with the anti-$k_T$ algorithm with radius parameter setting of $R=0.4$ in the 20-50% centrality bin to maximize the initial-state eccentricity of the interaction region. The reaction plane fit method is implemented to remove the flow-modulated background with better precision than prior methods. Yields and widths of jet-associated charged-hadron distributions are extracted in three angular bins between the jet axis and the event plane. The event-plane (EP) dependence is further quantified by ratios of the associated yields in different EP bins. No dependence on orientation of the jet axis with respect to the event plane is seen within the uncertainties in the kinematic regime studied. This finding is consistent with a similar experimental observation by ALICE in $\sqrt{s_{NN}} = 2.76$ TeV Pb+Pb collision data.