cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.48370/ofd/qs7obv
title: Turzyca lisia (Carex vulpina L.), 6160

description: Herbarium
DOI: 10.15161/oar.it/73932
title: CovidStat project data

description: This record contains the daily updated data of the CovidStat project. CovidStat is a project carried out by the CovidStat Working Group at INFN, whose creation was promoted within the Italian National Institute of Nuclear Physics with the aim of making a statistical analysis of the data provided daily by the Civil Protection on the spread of the pandemic in Italy. CovidStat data can interactively be browsed at https://covid19.infn.it.
description: The software to process this Root TTree is in the related identifier. Be sure to use the right corresponding version, based on the data in which Root TTree was generated.
DOI: 10.5281/zenodo.5105713
title: Selective excitation enables encoding and measurement of multiple diffusion parameters in a single experiment

description: NMR spectra data for diffusion experiments. NMR pulse sequence compatible with Bruker spectrometers for the selective diffusion measurement.
DOI: 10.5281/zenodo.5105712
title: Selective excitation enables encoding and measurement of multiple diffusion parameters in a single experiment

description: NMR spectra data for diffusion experiments. NMR pulse sequence compatible with Bruker spectrometers for the selective diffusion measurement.
DOI: 10.5281/zenodo.4624106
title: High-resolution synthetic UV–submm images for simulated Milky Way-type galaxies from the Auriga project (Au 21-26)

description: We present redshift-zero synthetic observational data considering dust attenuation and dust emission for the thirty galaxies of the Auriga project, calculated with the SKIRT radiative transfer code. The set of thirty Auriga galaxies reproduce a wide range of present-day observables, in particular, disk-dominated galaxies with appropriate stellar masses, sizes, rotation curves, star formation rates, and metallicities. The post-processing procedure includes components for star-forming regions, stellar sources, and diffuse dust taking into account stochastic heating of dust grains. This allows us to obtain realistic high-resolution broadband images and fluxes from ultraviolet to sub-millimeter wavelengths. Please visit auriga.ugent.be for more information. This dataset contains images/SEDs for Auriga galaxies 21-26 i.e. 6/30 galaxies.
description: Visit www.auriga.ugent.be for further information. This project received funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme, grant agreement No. 683184 (Consolidator Grant LEGA-C). AUK, MB, DBA, and AT acknowledge the financial support of the Flemish Fund for Scientific Research (FWO-Vlaanderen), research projects G039216N and G030319N. IDL acknowledges support from ERC starting grant 851622 DustOrigin. LC is the recipient of an Australian Research Council Future Fellowship (FT180100066) funded by the Australian Government. The radiative transfer simulations carried out for this work used the Tier-2 facilities of the Flemish Supercomputer Center (https:// www.vscentrum.be/) located at the Ghent University.
DOI: 10.5281/zenodo.4624105
title: High-resolution synthetic UV–submm images for simulated Milky Way-type galaxies from the Auriga project (Au 21-26)

description: We present redshift-zero synthetic observational data considering dust attenuation and dust emission for the thirty galaxies of the Auriga project, calculated with the SKIRT radiative transfer code. The set of thirty Auriga galaxies reproduce a wide range of present-day observables, in particular, disk-dominated galaxies with appropriate stellar masses, sizes, rotation curves, star formation rates, and metallicities. The post-processing procedure includes components for star-forming regions, stellar sources, and diffuse dust taking into account stochastic heating of dust grains. This allows us to obtain realistic high-resolution broadband images and fluxes from ultraviolet to sub-millimeter wavelengths. Please visit auriga.ugent.be for more information. This dataset contains images/SEDs for Auriga galaxies 21-26 i.e. 6/30 galaxies.
description: Visit www.auriga.ugent.be for further information. This project received funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme, grant agreement No. 683184 (Consolidator Grant LEGA-C). AUK, MB, DBA, and AT acknowledge the financial support of the Flemish Fund for Scientific Research (FWO-Vlaanderen), research projects G039216N and G030319N. IDL acknowledges support from ERC starting grant 851622 DustOrigin. LC is the recipient of an Australian Research Council Future Fellowship (FT180100066) funded by the Australian Government. The radiative transfer simulations carried out for this work used the Tier-2 facilities of the Flemish Supercomputer Center (https:// www.vscentrum.be/) located at the Ghent University.
DOI: 10.5281/zenodo.4616351
title: High-resolution synthetic UV–submm images for simulated Milky Way-type galaxies from the Auriga project (Au 1-4)

description: We present redshift-zero synthetic observational data considering dust attenuation and dust emission for the thirty galaxies of the Auriga project, calculated with the SKIRT radiative transfer code. The set of thirty Auriga galaxies reproduce a wide range of present-day observables, in particular, disk-dominated galaxies with appropriate stellar masses, sizes, rotation curves, star formation rates, and metallicities. The post-processing procedure includes components for star-forming regions, stellar sources, and diffuse dust taking into account stochastic heating of dust grains. This allows us to obtain realistic high-resolution broadband images and fluxes from ultraviolet to sub-millimeter wavelengths. Please visit auriga.ugent.be for more information. This dataset contains images/SEDs for Auriga galaxies 1-4 i.e. 4/30 galaxies.
description: Visit www.auriga.ugent.be for further information. This project received funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme, grant agreement No. 683184 (Consolidator Grant LEGA-C). AUK, MB, DBA, and AT acknowledge the financial support of the Flemish Fund for Scientific Research (FWO-Vlaanderen), research projects G039216N and G030319N. IDL acknowledges support from ERC starting grant 851622 DustOrigin. LC is the recipient of an Australian Research Council Future Fellowship (FT180100066) funded by the Australian Government. The radiative transfer simulations carried out for this work used the Tier-2 facilities of the Flemish Supercomputer Center (https:// www.vscentrum.be/) located at the Ghent University.
DOI: 10.5281/zenodo.4616350
title: High-resolution synthetic UV–submm images for simulated Milky Way-type galaxies from the Auriga project (Au 1-4)

description: We present redshift-zero synthetic observational data considering dust attenuation and dust emission for the thirty galaxies of the Auriga project, calculated with the SKIRT radiative transfer code. The set of thirty Auriga galaxies reproduce a wide range of present-day observables, in particular, disk-dominated galaxies with appropriate stellar masses, sizes, rotation curves, star formation rates, and metallicities. The post-processing procedure includes components for star-forming regions, stellar sources, and diffuse dust taking into account stochastic heating of dust grains. This allows us to obtain realistic high-resolution broadband images and fluxes from ultraviolet to sub-millimeter wavelengths. Please visit auriga.ugent.be for more information. This dataset contains images/SEDs for Auriga galaxies 1-4 i.e. 4/30 galaxies.
description: Visit www.auriga.ugent.be for further information. This project received funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme, grant agreement No. 683184 (Consolidator Grant LEGA-C). AUK, MB, DBA, and AT acknowledge the financial support of the Flemish Fund for Scientific Research (FWO-Vlaanderen), research projects G039216N and G030319N. IDL acknowledges support from ERC starting grant 851622 DustOrigin. LC is the recipient of an Australian Research Council Future Fellowship (FT180100066) funded by the Australian Government. The radiative transfer simulations carried out for this work used the Tier-2 facilities of the Flemish Supercomputer Center (https:// www.vscentrum.be/) located at the Ghent University.
DOI: 10.5281/zenodo.4618346
title: High-resolution synthetic UV–submm images for simulated Milky Way-type galaxies from the Auriga project (Au 5-8)

description: We present redshift-zero synthetic observational data considering dust attenuation and dust emission for the thirty galaxies of the Auriga project, calculated with the SKIRT radiative transfer code. The set of thirty Auriga galaxies reproduce a wide range of present-day observables, in particular, disk-dominated galaxies with appropriate stellar masses, sizes, rotation curves, star formation rates, and metallicities. The post-processing procedure includes components for star-forming regions, stellar sources, and diffuse dust taking into account stochastic heating of dust grains. This allows us to obtain realistic high-resolution broadband images and fluxes from ultraviolet to sub-millimeter wavelengths. Please visit auriga.ugent.be for more information. This dataset contains images/SEDs for Auriga galaxies 5-8 i.e. 4/30 galaxies.
description: Visit www.auriga.ugent.be for further information. This project received funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme, grant agreement No. 683184 (Consolidator Grant LEGA-C). AUK, MB, DBA, and AT acknowledge the financial support of the Flemish Fund for Scientific Research (FWO-Vlaanderen), research projects G039216N and G030319N. IDL acknowledges support from ERC starting grant 851622 DustOrigin. LC is the recipient of an Australian Research Council Future Fellowship (FT180100066) funded by the Australian Government. The radiative transfer simulations carried out for this work used the Tier-2 facilities of the Flemish Supercomputer Center (https:// www.vscentrum.be/) located at the Ghent University.
DOI: 10.5281/zenodo.4618345
title: High-resolution synthetic UV–submm images for simulated Milky Way-type galaxies from the Auriga project (Au 5-8)

description: We present redshift-zero synthetic observational data considering dust attenuation and dust emission for the thirty galaxies of the Auriga project, calculated with the SKIRT radiative transfer code. The set of thirty Auriga galaxies reproduce a wide range of present-day observables, in particular, disk-dominated galaxies with appropriate stellar masses, sizes, rotation curves, star formation rates, and metallicities. The post-processing procedure includes components for star-forming regions, stellar sources, and diffuse dust taking into account stochastic heating of dust grains. This allows us to obtain realistic high-resolution broadband images and fluxes from ultraviolet to sub-millimeter wavelengths. Please visit auriga.ugent.be for more information. This dataset contains images/SEDs for Auriga galaxies 5-8 i.e. 4/30 galaxies.
description: Visit www.auriga.ugent.be for further information. This project received funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme, grant agreement No. 683184 (Consolidator Grant LEGA-C). AUK, MB, DBA, and AT acknowledge the financial support of the Flemish Fund for Scientific Research (FWO-Vlaanderen), research projects G039216N and G030319N. IDL acknowledges support from ERC starting grant 851622 DustOrigin. LC is the recipient of an Australian Research Council Future Fellowship (FT180100066) funded by the Australian Government. The radiative transfer simulations carried out for this work used the Tier-2 facilities of the Flemish Supercomputer Center (https:// www.vscentrum.be/) located at the Ghent University.
DOI: 10.5281/zenodo.4619608
title: High-resolution synthetic UV–submm images for simulated Milky Way-type galaxies from the Auriga project (Au 9-15)

description: We present redshift-zero synthetic observational data considering dust attenuation and dust emission for the thirty galaxies of the Auriga project, calculated with the SKIRT radiative transfer code. The set of thirty Auriga galaxies reproduce a wide range of present-day observables, in particular, disk-dominated galaxies with appropriate stellar masses, sizes, rotation curves, star formation rates, and metallicities. The post-processing procedure includes components for star-forming regions, stellar sources, and diffuse dust taking into account stochastic heating of dust grains. This allows us to obtain realistic high-resolution broadband images and fluxes from ultraviolet to sub-millimeter wavelengths. Please visit auriga.ugent.be for more information. This dataset contains images/SEDs for Auriga galaxies 9-15 i.e. 7/30 galaxies.
description: Visit www.auriga.ugent.be for further information. This project received funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme, grant agreement No. 683184 (Consolidator Grant LEGA-C). AUK, MB, DBA, and AT acknowledge the financial support of the Flemish Fund for Scientific Research (FWO-Vlaanderen), research projects G039216N and G030319N. IDL acknowledges support from ERC starting grant 851622 DustOrigin. LC is the recipient of an Australian Research Council Future Fellowship (FT180100066) funded by the Australian Government. The radiative transfer simulations carried out for this work used the Tier-2 facilities of the Flemish Supercomputer Center (https:// www.vscentrum.be/) located at the Ghent University.
DOI: 10.5281/zenodo.4619607
title: High-resolution synthetic UV–submm images for simulated Milky Way-type galaxies from the Auriga project (Au 9-15)

description: We present redshift-zero synthetic observational data considering dust attenuation and dust emission for the thirty galaxies of the Auriga project, calculated with the SKIRT radiative transfer code. The set of thirty Auriga galaxies reproduce a wide range of present-day observables, in particular, disk-dominated galaxies with appropriate stellar masses, sizes, rotation curves, star formation rates, and metallicities. The post-processing procedure includes components for star-forming regions, stellar sources, and diffuse dust taking into account stochastic heating of dust grains. This allows us to obtain realistic high-resolution broadband images and fluxes from ultraviolet to sub-millimeter wavelengths. Please visit auriga.ugent.be for more information. This dataset contains images/SEDs for Auriga galaxies 9-15 i.e. 7/30 galaxies.
description: Visit www.auriga.ugent.be for further information. This project received funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme, grant agreement No. 683184 (Consolidator Grant LEGA-C). AUK, MB, DBA, and AT acknowledge the financial support of the Flemish Fund for Scientific Research (FWO-Vlaanderen), research projects G039216N and G030319N. IDL acknowledges support from ERC starting grant 851622 DustOrigin. LC is the recipient of an Australian Research Council Future Fellowship (FT180100066) funded by the Australian Government. The radiative transfer simulations carried out for this work used the Tier-2 facilities of the Flemish Supercomputer Center (https:// www.vscentrum.be/) located at the Ghent University.
DOI: 10.5281/zenodo.4625218
title: High-resolution synthetic UV–submm images for simulated Milky Way-type galaxies from the Auriga project (Au 16-20)

description: We present redshift-zero synthetic observational data considering dust attenuation and dust emission for the thirty galaxies of the Auriga project, calculated with the SKIRT radiative transfer code. The set of thirty Auriga galaxies reproduce a wide range of present-day observables, in particular, disk-dominated galaxies with appropriate stellar masses, sizes, rotation curves, star formation rates, and metallicities. The post-processing procedure includes components for star-forming regions, stellar sources, and diffuse dust taking into account stochastic heating of dust grains. This allows us to obtain realistic high-resolution broadband images and fluxes from ultraviolet to sub-millimeter wavelengths. Please visit auriga.ugent.be for more information. This dataset contains images/SEDs for Auriga galaxies 16-20, i.e. 5/30 galaxies.
description: Visit www.auriga.ugent.be for further information. This project received funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme, grant agreement No. 683184 (Consolidator Grant LEGA-C). AUK, MB, DBA, and AT acknowledge the financial support of the Flemish Fund for Scientific Research (FWO-Vlaanderen), research projects G039216N and G030319N. IDL acknowledges support from ERC starting grant 851622 DustOrigin. LC is the recipient of an Australian Research Council Future Fellowship (FT180100066) funded by the Australian Government. The radiative transfer simulations carried out for this work used the Tier-2 facilities of the Flemish Supercomputer Center (https:// www.vscentrum.be/) located at the Ghent University.
DOI: 10.5281/zenodo.4625217
title: High-resolution synthetic UV–submm images for simulated Milky Way-type galaxies from the Auriga project (Au 16-20)

description: We present redshift-zero synthetic observational data considering dust attenuation and dust emission for the thirty galaxies of the Auriga project, calculated with the SKIRT radiative transfer code. The set of thirty Auriga galaxies reproduce a wide range of present-day observables, in particular, disk-dominated galaxies with appropriate stellar masses, sizes, rotation curves, star formation rates, and metallicities. The post-processing procedure includes components for star-forming regions, stellar sources, and diffuse dust taking into account stochastic heating of dust grains. This allows us to obtain realistic high-resolution broadband images and fluxes from ultraviolet to sub-millimeter wavelengths. Please visit auriga.ugent.be for more information. This dataset contains images/SEDs for Auriga galaxies 16-20, i.e. 5/30 galaxies.
description: Visit www.auriga.ugent.be for further information. This project received funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme, grant agreement No. 683184 (Consolidator Grant LEGA-C). AUK, MB, DBA, and AT acknowledge the financial support of the Flemish Fund for Scientific Research (FWO-Vlaanderen), research projects G039216N and G030319N. IDL acknowledges support from ERC starting grant 851622 DustOrigin. LC is the recipient of an Australian Research Council Future Fellowship (FT180100066) funded by the Australian Government. The radiative transfer simulations carried out for this work used the Tier-2 facilities of the Flemish Supercomputer Center (https:// www.vscentrum.be/) located at the Ghent University.
DOI: 10.5281/zenodo.4624122
title: High-resolution synthetic UV–submm images for simulated Milky Way-type galaxies from the Auriga project (Au 27-30)

description: We present redshift-zero synthetic observational data considering dust attenuation and dust emission for the thirty galaxies of the Auriga project, calculated with the SKIRT radiative transfer code. The set of thirty Auriga galaxies reproduce a wide range of present-day observables, in particular, disk-dominated galaxies with appropriate stellar masses, sizes, rotation curves, star formation rates, and metallicities. The post-processing procedure includes components for star-forming regions, stellar sources, and diffuse dust taking into account stochastic heating of dust grains. This allows us to obtain realistic high-resolution broadband images and fluxes from ultraviolet to sub-millimeter wavelengths. Please visit auriga.ugent.be for more information. This dataset contains images/SEDs for Auriga galaxies 27-30 i.e. 4/30 galaxies.
description: Visit www.auriga.ugent.be for further information. This project received funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme, grant agreement No. 683184 (Consolidator Grant LEGA-C). AUK, MB, DBA, and AT acknowledge the financial support of the Flemish Fund for Scientific Research (FWO-Vlaanderen), research projects G039216N and G030319N. IDL acknowledges support from ERC starting grant 851622 DustOrigin. LC is the recipient of an Australian Research Council Future Fellowship (FT180100066) funded by the Australian Government. The radiative transfer simulations carried out for this work used the Tier-2 facilities of the Flemish Supercomputer Center (https:// www.vscentrum.be/) located at the Ghent University.
DOI: 10.5281/zenodo.4624121
title: High-resolution synthetic UV–submm images for simulated Milky Way-type galaxies from the Auriga project (Au 27-30)

description: We present redshift-zero synthetic observational data considering dust attenuation and dust emission for the thirty galaxies of the Auriga project, calculated with the SKIRT radiative transfer code. The set of thirty Auriga galaxies reproduce a wide range of present-day observables, in particular, disk-dominated galaxies with appropriate stellar masses, sizes, rotation curves, star formation rates, and metallicities. The post-processing procedure includes components for star-forming regions, stellar sources, and diffuse dust taking into account stochastic heating of dust grains. This allows us to obtain realistic high-resolution broadband images and fluxes from ultraviolet to sub-millimeter wavelengths. Please visit auriga.ugent.be for more information. This dataset contains images/SEDs for Auriga galaxies 27-30 i.e. 4/30 galaxies.
description: Visit www.auriga.ugent.be for further information. This project received funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme, grant agreement No. 683184 (Consolidator Grant LEGA-C). AUK, MB, DBA, and AT acknowledge the financial support of the Flemish Fund for Scientific Research (FWO-Vlaanderen), research projects G039216N and G030319N. IDL acknowledges support from ERC starting grant 851622 DustOrigin. LC is the recipient of an Australian Research Council Future Fellowship (FT180100066) funded by the Australian Government. The radiative transfer simulations carried out for this work used the Tier-2 facilities of the Flemish Supercomputer Center (https:// www.vscentrum.be/) located at the Ghent University.
DOI: 10.48370/ofd/d2mwnx/ldiuhi
title: HMW_Carex_ovalis_Gooden._H_8831.jpg

description: :unav
DOI: 10.48370/ofd/d2mwnx
title: Turzyca zajęcza (Carex ovalis Gooden.), 8831

description: Herbarium
DOI: 10.6084/m9.figshare.14987031.v1
title: my_data.csv

description: Toy dataset with one response variable "y" and two covariates "x" and "z".<br>
DOI: 10.6084/m9.figshare.14987031
title: my_data.csv

description: Toy dataset with one response variable "y" and two covariates "x" and "z".<br>
DOI: 10.48370/ofd/4lembj/2quuys
title: HMW_Carex_ovalis_Gooden._H_6644.jpg

description: :unav
DOI: 10.48370/ofd/4lembj
title: Turzyca zajęcza (Carex ovalis Gooden.), 6644

description: Herbarium
DOI: 10.48370/ofd/iz3oru/fx83sp
title: HMW_Carex_ovalis_Gooden._H_4990.jpg

description: :unav
DOI: 10.48370/ofd/iz3oru
title: Turzyca zajęcza (Carex ovalis Gooden.), 4990

description: Herbarium
DOI: 10.48370/ofd/xnmd9p/qc9kle
title: HMW_Carex_ovalis_Gooden._H_2730.jpg

description: :unav
DOI: 10.6084/m9.figshare.14500386
title: Supplementary Material for: Quantitative MR-derived biomarkers as predictors of function and histotype in adenohypophyseal tumours

description: Medicine