cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.17182/hepdata.147191.v1/t94
title: "fig7_bottom_left_0" of "Jet-hadron correlations with respect to the event plane in $\sqrt{s_{\mathrm{NN}}}$ = 200 GeV Au+Au collisions in STAR"

description: mid-plane/in-plane ratio of near-side yields associated charged hadrons for 20-40 GeV/c jets from 20-50% centrality collisions.
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.3pk73
title: Data from: Nested species interactions promote feasibility over stability during the assembly of a pollinator community

description: The foundational concepts behind the persistence of ecological communities
 have been based on two ecological properties: dynamical stability and
 feasibility. The former is typically regarded as the capacity of a
 community to return to an original equilibrium state after a perturbation
 in species abundances and is usually linked to the strength of
 interspecific interactions. The latter is the capacity to sustain positive
 abundances on all its constituent species and is linked to both
 interspecific interactions and species demographic characteristics. Over
 the last 40 years, theoretical research in ecology has emphasized the
 search for conditions leading to the dynamical stability of ecological
 communities, while the conditions leading to feasibility have been
 overlooked. However, thus far, we have no evidence of whether species
 interactions are more conditioned by the community's need to be
 stable or feasible. Here, we introduce novel quantitative methods and use
 empirical data to investigate the consequences of species interactions on
 the dynamical stability and feasibility of mutualistic communities. First,
 we demonstrate that the more nested the species interactions in a
 community are, the lower the mutualistic strength that the community can
 tolerate without losing dynamical stability. Second, we show that high
 feasibility in a community can be reached either with high mutualistic
 strength or with highly nested species interactions. Third, we find that
 during the assembly process of a seasonal pollinator community located at
 The Zackenberg Research Station (northeastern Greenland), a high
 feasibility is reached through the nested species interactions established
 between newcomer and resident species. Our findings imply that nested
 mutualistic communities promote feasibility over stability, which may
 suggest that the former can be key for community persistence.
description: Network_data_and_RcodeThe data file contains the network data and Rcode used in the study. The files Zackenberg_1996.xlsx and Zackenberg_1997.xlsx contain the daily pollinator-plant interaction matrices for 1996 and 1997, respectively. These matrices were used by the first time in: Olesen JM, Bascompte J, Elberling H, and Jordano P. (2008) Temporal dynamics in a pollinator network. Ecology 89, 1573-1582. The code to calculate the feasibility, stability, and nestedness of any given matrix is provided and commented in toolbox.R. We are also proving a commented example (example.R) to illustrate the application of this code as in the manuscript.
DOI: 10.17182/hepdata.147191.v1/t100
title: "fig7_bottom_right_2" of "Jet-hadron correlations with respect to the event plane in $\sqrt{s_{\mathrm{NN}}}$ = 200 GeV Au+Au collisions in STAR"

description: mid-plane/in-plane ($p_{T, assoc}$ inclusive) ratio of away-side yields associated charged hadrons for 20-40 GeV/c jets from 20-50% centrality collisions.
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/t92
title: "fig7_top_right_2" of "Jet-hadron correlations with respect to the event plane in $\sqrt{s_{\mathrm{NN}}}$ = 200 GeV Au+Au collisions in STAR"

description: mid-plane/in-plane ($p_{T, assoc}$ inclusive) ratio of away-side yields associated charged hadrons for 15-20 GeV/c jets from 20-50% centrality collisions.
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/t95
title: "fig7_bottom_left_1" of "Jet-hadron correlations with respect to the event plane in $\sqrt{s_{\mathrm{NN}}}$ = 200 GeV Au+Au collisions in STAR"

description: out-of-plane/in-plane ratio of near-side yields associated charged hadrons for 20-40 GeV/c jets from 20-50% centrality collisions.
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/t96
title: "fig7_bottom_left_2" of "Jet-hadron correlations with respect to the event plane in $\sqrt{s_{\mathrm{NN}}}$ = 200 GeV Au+Au collisions in STAR"

description: mid-plane/in-plane ($p_{T, assoc}$ inclusive) ratio of near-side yields associated charged hadrons for 20-40 GeV/c jets from 20-50% centrality collisions.
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/t97
title: "fig7_bottom_left_3" of "Jet-hadron correlations with respect to the event plane in $\sqrt{s_{\mathrm{NN}}}$ = 200 GeV Au+Au collisions in STAR"

description: out-of-plane/in-plane ($p_{T, assoc}$ inclusive) ratio of near-side yields associated charged hadrons for 20-40 GeV/c jets from 20-50% centrality collisions.
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/t98
title: "fig7_bottom_right_0" of "Jet-hadron correlations with respect to the event plane in $\sqrt{s_{\mathrm{NN}}}$ = 200 GeV Au+Au collisions in STAR"

description: mid-plane/in-plane ratio of away-side yields associated charged hadrons for 20-40 GeV/c jets from 20-50% centrality collisions.
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/t99
title: "fig7_bottom_right_1" of "Jet-hadron correlations with respect to the event plane in $\sqrt{s_{\mathrm{NN}}}$ = 200 GeV Au+Au collisions in STAR"

description: out-of-plane/in-plane ratio of away-side yields associated charged hadrons for 20-40 GeV/c jets from 20-50% centrality collisions.
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/t101
title: "fig7_bottom_right_3" of "Jet-hadron correlations with respect to the event plane in $\sqrt{s_{\mathrm{NN}}}$ = 200 GeV Au+Au collisions in STAR"

description: out-of-plane/in-plane ($p_{T, assoc}$ inclusive) ratio of away-side yields associated charged hadrons for 20-40 GeV/c jets from 20-50% centrality collisions.
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.388ds
title: Data from: Identification of chloroplast genome loci suitable for high-resolution phylogeographic studies of Colocasia esculenta (L.) Schott (Araceae) and closely related taxa

description: Recently, we reported the chloroplast genome-wide association of
 oligonucleotide repeats, indels and nucleotide substitutions in aroid
 chloroplast genomes. We hypothesized that the distribution of
 oligonucleotide repeat sequences in a single representative genome can be
 used to identify mutational hotspots and loci suitable for population
 genetic, phylogenetic and phylogeographic studies. Using information on
 the location of oligonucleotide repeats in the chloroplast genome of taro
 (Colocasia esculenta), we designed 30 primer pairs to amplify and sequence
 polymorphic loci. The primers have been tested in a range of
 intra-specific to intergeneric comparisons, including ten taro samples
 (Colocasia esculenta) from diverse geographical locations, four other
 Colocasia species (C. affinis, C. fallax, C. formosana, C. gigantea) and
 three other aroid genera (represented by Remusatia vivipara, Alocasia
 brisbanensis and Amorphophallus konjac). Multiple sequence alignments for
 the intra-specific comparison revealed nucleotide substitutions (point
 mutations) at all 30 loci and microsatellite polymorphisms at 14 loci. The
 primer pairs reported here reveal levels of genetic variation suitable for
 high-resolution phylogeographic and evolutionary studies of taro and other
 closely related aroids. Our results confirm that information on repeat
 distribution can be used to identify loci suitable for such studies, and
 we expect that this approach can be used in other plant groups.
description: Suppl_Material_Alignments_for_30_lociSequence alignments for all 30 loci are given as .phy format files. For intra-specific (Fig. 2a), inter-specific (Fig 2b) and inter-generic (Fig. 2c) comparison, representative taxa have been selected from these alignments. First three letters in an accession name indicate the species used, fourth and fifth letters show the country of collection according to the International Organization for Standardization (ISO), and the last two digits represent accession number.
DOI: 10.5061/dryad.r2s74q4
title: Data from: Foraging efficiency and size matching in a plant – pollinator community: the importance of sugar content and tongue length

description: A longstanding question in ecology is how species interactions are
 structured within communities. Although evolutionary theory predicts close
 size matching between floral nectar tube depth and pollinator proboscis
 length of interacting species, such size matching has seldom been shown
 and explained in multispecies assemblages. Here, we investigated the
 degree of size matching among Asteraceae and their pollinators and its
 relationship with foraging efficiency. The majority of pollinators,
 especially Hymenoptera, choose plant species on which they had high
 foraging efficiencies. When proboscides were shorter than nectar tubes,
 foraging efficiency rapidly decreased because of increased handling time.
 When proboscides were longer than nectar tubes, a decreased nectar reward
 rather than an increased handling time made shallow flowers more
 inefficient to visit. Altogether, this led to close size matching.
 Overall, our results show the importance of nectar reward and handling
 time as drivers of plant – pollinator network structure.
description: ELE_Interaction_probabilityRawdata interaction probabilityELE_Foraging_efficiencyRawdata handling time and sugar extraction rate