cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5281/zenodo.2168018
title: Solar Eclipse 2017 recordings of the medium-wave AM broadcast band from Victoria, BC, Canada

description: recorded by Nick Hall-Patch,  VE7DXR

location recorded: 48.42735°N 123.32426°W

These data files are of the entire medium wave broadcast band (535-1705kHz) from 16:01:35UTC to 18:09:35UTC, recorded in Victoria, BC, Canada.  Data files are .wav format, but the archived files are .zip, with several .wav files packaged together in each .zip file

Antenna:   broadband delta loop antenna, 22-foot apex with a 40-foot base, oriented 110-290 degrees;  Wellbrook (https://www.wellbrook.uk.com/loopantennas/) ALA100 preamplifier

Receiver:  RFSpace (http://www.rfspace.com) NetSDR, 20dB attenuation, center frequency set at 1100kHz, recording 1300kHz wide passband, using RFSpace SpectraVue v.3.39 software (http://www.rfspace.com/RFSPACE/SpectraVue.html).
description: In the AM broadcast band (535-1705kHz), there are roughly two modes of broadcast station signal coverage, one of which occurs in the daytime, and the other at night.   During the day time, signals are propagated by ground wave and and not usually heard well beyond 150km from the transmitter.  However, at night, an absorptive region in the ionosphere, the D-layer, disappears, allowing signals to refract off higher regions of the ionosphere, and to be heard hundreds and even thousands, of kilometers away from the transmitter.   During the solar eclipse of 2017, signals were observed changing from daytime to nighttime mode and then back again as the moon's shadow moved across the continental USA.

   The radio stations in this band use amplitude modulation, which requires a strong stable carrier wave, well suited for observing changes in signal strength over a time period.

There are three missing periods in the data set due to operator error:    16:31:34- 16:32:30UT, 17:02:29-17:09:15UT, 17:39:13-17:39:36UT

File "VE7DXR-wideband_450_1750kHz_20170821_152909UT.wav" is a reference file recorded before any effects of the eclipse might have been felt.

Included in these files are an installation file for SpectraVue 3.39 ("spectravue339.exe") for playback of the .wav files, an .ini file to be used with SpectraVue after it has been installed ("NetSDR_playback.ini"), plus a reference file to assist in identifying signals ("canusa-Jan2019.pdf").    As well, there is set of instructions for installation and use of the software, including instructions for using SpectraVue to extract a time series of signal power for an individual radio station's signal ("using SpectraVue to create signal strength time series-VE7DXR.pdf").
Finally, referencing the article archived at http://hamsci.org/sites/default/files/publications/2019_am-eclipse2017_hall-patch.pdf , will give the user of these files an idea of how radio reception datasets from different locations can be used to compare the effects that the solar eclipse had on radio propagation.
DOI: 10.5281/zenodo.2168019
title: Solar Eclipse 2017 recordings of the medium-wave AM broadcast band from Victoria, BC, Canada

description: recorded by Nick Hall-Patch,  VE7DXR

location recorded: 48.42735°N 123.32426°W

These data files are of the entire medium wave broadcast band (535-1705kHz) from 16:01:35UTC to 18:09:35UTC, recorded in Victoria, BC, Canada.  Data files are .wav format, but the archived files are .zip, with several .wav files packaged together in each .zip file

Antenna:   broadband delta loop antenna, 22-foot apex with a 40-foot base, oriented 110-290 degrees;  Wellbrook (https://www.wellbrook.uk.com/loopantennas/) ALA100 preamplifier

Receiver:  RFSpace (http://www.rfspace.com) NetSDR, 20dB attenuation, center frequency set at 1100kHz, recording 1300kHz wide passband, using RFSpace SpectraVue v.3.39 software (http://www.rfspace.com/RFSPACE/SpectraVue.html).
description: In the AM broadcast band (535-1705kHz), there are roughly two modes of broadcast station signal coverage, one of which occurs in the daytime, and the other at night.   During the day time, signals are propagated by ground wave and and not usually heard well beyond 150km from the transmitter.  However, at night, an absorptive region in the ionosphere, the D-layer, disappears, allowing signals to refract off higher regions of the ionosphere, and to be heard hundreds and even thousands, of kilometers away from the transmitter.   During the solar eclipse of 2017, signals were observed changing from daytime to nighttime mode and then back again as the moon's shadow moved across the continental USA.

   The radio stations in this band use amplitude modulation, which requires a strong stable carrier wave, well suited for observing changes in signal strength over a time period.

There are three missing periods in the data set due to operator error:    16:31:34- 16:32:30UT, 17:02:29-17:09:15UT, 17:39:13-17:39:36UT

File "VE7DXR-wideband_450_1750kHz_20170821_152909UT.wav" is a reference file recorded before any effects of the eclipse might have been felt.

Included in these files are an installation file for SpectraVue 3.39 ("spectravue339.exe") for playback of the .wav files, an .ini file to be used with SpectraVue after it has been installed ("NetSDR_playback.ini"), plus a reference file to assist in identifying signals ("canusa-Jan2019.pdf").    As well, there is set of instructions for installation and use of the software, including instructions for using SpectraVue to extract a time series of signal power for an individual radio station's signal ("using SpectraVue to create signal strength time series-VE7DXR.pdf").
Finally, referencing the article archived at http://hamsci.org/sites/default/files/publications/2019_am-eclipse2017_hall-patch.pdf , will give the user of these files an idea of how radio reception datasets from different locations can be used to compare the effects that the solar eclipse had on radio propagation.
DOI: 10.5281/zenodo.2554773
title: Binary black-hole simulation SXS:BBH:1405

description: Simulation of a black-hole binary system evolved by the SpEC code.
DOI: 10.5281/zenodo.2554774
title: Binary black-hole simulation SXS:BBH:1405

description: Simulation of a black-hole binary system evolved by the SpEC code.
DOI: 10.25919/5c5398d4036f1
title: Parkes observations for project PX500 semester 2018OCTS_48

description: This proposal relates to time purchased by the Chinese Academy of Sciences for Parkes follow-up confirmation and timing of FAST discoveries.  As the observing time has been purchased this proposal (and the related PX501) does not require TAC grading.  The primary reason for submitting a proposal is to ensure an outreach statement and that the proposal is entered into OPAL for the data archive to access. The Chinese team have two time requests. The time scheduled for the first, relating to this proposal, will be allocated in blocks of 24 hours and the data will become available in the data archive with an 18 month embargo period.  The second type of time will be scheduled in shorter blocks and the data archived with a 10 year embargo.
DOI: 10.25919/5c5398d41c84d
title: Parkes observations for project P958 semester 2018OCTS_24

description: A major breakthrough in fast radio burst (FRB) astronomy was recently made when the repeating FRB 121102 was localized to sub-arcsecond precision. The bursts were found to originate in a bright radio nebula (hypothesized to be a young supernova remnant or pulsar wind nebulae) in a distant dwarf galaxy. These dwarf galaxies are also preferential hosts to superluminous supernova and long gamma-ray bursts, and it has been therefore suggested that the source of the repeating FRB could be a young highly magnetised neutron star. While an understanding of the repeating FRB is emerging, it is still unclear what relationship it has to the rest of the population.   Over the last year searches with the Australian Square Kilometre Array Pathfinder (ASKAP) have detected 26 bursts, and over the next six month will likely detect another 12 FRBs, which  will be localized to a few arcseconds.   Here we propose to search this population for repeats.  Our comprehensive sample and a dense monitoring campaign of well localised bursts, at a fluence limit more than 60 times lower than that of their detections, will either confirm the presence of additional repeating FRBs or the uniqueness of FRB 121102 amongst the population.
DOI: 10.5281/zenodo.2554572
title: Binary black-hole simulation SXS:BBH:1401

description: Simulation of a black-hole binary system evolved by the SpEC code.
DOI: 10.5281/zenodo.2554573
title: Binary black-hole simulation SXS:BBH:1401

description: Simulation of a black-hole binary system evolved by the SpEC code.
DOI: 10.25345/c5z02z
title: MassIVE MSV000083387 - E. Coli Nissle wild type versus knockout strain
title: E. Coli Nissle wild type versus knockout strain grown in M-9 media.
DOI: 10.25912/5c53a22ae2810
title: Dataset of the Foot Disease in Inpatients Study
DOI: 10.17632/4tp4tdkfdb.1
title: Data for: A comparative adsorption study of benzophenone-3 onto synthesized lipophilic organosilicate, Laponite and montmorillonite

description: In this study, the adsorption of a hydrophobic molecule, benzophenone-3 (BZ-3) was investigated onto three adsorbents: synthesized lipophilic organosilicate (OSL), Laponite (Lap) and montmorillonite (Mt). A comparative study for all adsorbents with batch adsorption experiments was achieved to determine the optimal conditions. The effects of the main experimental parameters were determined such as solvent, pH, temperature, initial concentration of BZ-3 and contact time. The adsorption capacity was evaluated by means of HPLC analysis equipped with UV detection and the adsorbent - BZ-3 complexes were characterized by means of Dynamic Light Scattering (DLS) analysis and Attenuated Total Reflectance - Fourier Transform InfraRed (ATR - FTIR) spectroscopy. Finally, the adsorption isotherm equilibrium was described according to Langmuir, Freundlich and Temkin models. The results showed that optimal value of the adsorbed BZ-3 for all adsorbents was found at pH 10, at 38 °C, with BZ-3 concentration of 2.5 g/L during 24 h of contact time. The results obtained showed a promising capacity of the OSL to adsorb BZ-3 (340 mg of BZ-3/g of adsorbent) compared to Lap (137 mg/g) and Mt (192.3 mg/g). Langmuir model fitted the best with OSL and Mt adsorption while Freundlich model fitted the best with Lap adsorption.
DOI: 10.5063/f12z13r6
title: Global Ocean Health Index 2018 assessment

description: Scores from the 2018 global Ocean Health Index (OHI) assessment and accompanying data and models. The global Ocean Health Index assesses ocean health for 220 coastal countries and territories and has been conducted yearly since 2012. The Index describes how well we are sustainably managing 10 goals which represent the full suite of benefits that people want and need from the ocean. These goals include: artisanal fishing opportunity, biodiversity, carbon storage, clean waters, coastal livelihoods and economies, coastal protection, food provision, natural products, sense of place, and tourism and recreation. Each goal is given a score ranging from 0 to 100, and the full suite of goal scores are then averaged to obtain an overall index score for each region. Please see our website for additional resources and information (http://ohi-science.org/).
DOI: 10.5281/zenodo.2554434
title: Binary black-hole simulation SXS:BBH:1395

description: Simulation of a black-hole binary system evolved by the SpEC code.
DOI: 10.5281/zenodo.2554435
title: Binary black-hole simulation SXS:BBH:1395

description: Simulation of a black-hole binary system evolved by the SpEC code.
DOI: 10.5517/ccdc.csd.cc1ppnqr
title: CCDC 1569955: Experimental Crystal Structure Determination

description: Related Article: Bing Liu, Wenbo Li, Hai-Hong Wu, Junliang Zhang|2019|Org.Chem.Front.|6|694|doi:10.1039/C8QO01404C
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5281/zenodo.2554181
title: Some atmospheric model fields shown in paper titled "E3SMv0-HiLAT: A Modified Climate System Model Targeted for the Study of High Latitude Processes

description: These files contain 2-D fields of atmospheric T and P maps, as climatologies averaged over years 234-253 of the E3SMv0-HiLAT model preindustrial simulation, and from the CESM Large Ensemble control simulation (LENS), the basis for two of the plots in our manuscript that is, as of January 2019, in review at JAMES.  All of these data files are binary, written sequentially, 288 x 192.  Also included are some PowerPoint-generated pdf images of the two fields.
description: This page only provides the fields shown in figures 4 and 5 of the manuscript. A more complete set of climatological atmospheric fields are posted under this page: https://doi.org/10.5281/zenodo.2557890

For a full list of the 16 authors involved please see the title page of the manuscript.
DOI: 10.5281/zenodo.2554182
title: Some atmospheric model fields shown in paper titled "E3SMv0-HiLAT: A Modified Climate System Model Targeted for the Study of High Latitude Processes

description: These files contain 2-D fields of atmospheric T and P maps, as climatologies averaged over years 234-253 of the E3SMv0-HiLAT model preindustrial simulation, and from the CESM Large Ensemble control simulation (LENS), the basis for two of the plots in our manuscript that is, as of January 2019, in review at JAMES.  All of these data files are binary, written sequentially, 288 x 192.  Also included are some PowerPoint-generated pdf images of the two fields.
description: This page only provides the fields shown in figures 4 and 5 of the manuscript. A more complete set of climatological atmospheric fields are posted under this page: https://doi.org/10.5281/zenodo.2557890

For a full list of the 16 authors involved please see the title page of the manuscript.
DOI: 10.5517/ccdc.csd.cc1pt2bx
title: CCDC 1573229: Experimental Crystal Structure Determination

description: Related Article: Jun-Jie Wang, Pan-Pan Si, Jie Yang, Shan-Shan Zhao, Pan-Pan Li, Bo Li, Si-Yin Wang, Ming Lu, Su-Xin Yu|2019|Polyhedron|162|255|doi:10.1016/j.poly.2019.01.045
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5281/zenodo.2554174
title: 0.3 ms of asymmetric GM1:POPC/POPC (24:76/97) bilayer

description: Lollipop-like GM1. Fourth 25 microseconds of total 300 microseconds.
DOI: 10.5517/ccdc.csd.cc1z3bkz
title: CCDC 1820461: Experimental Crystal Structure Determination

description: Related Article: Phillip S. Grant, Margaret A. Brimble, Daniel P. Furkert|2018|Chem.Asian J.|14|1128|doi:10.1002/asia.201800903
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5517/ccdc.csd.cc1z3bl0
title: CCDC 1820462: Experimental Crystal Structure Determination

description: Related Article: Phillip S. Grant, Margaret A. Brimble, Daniel P. Furkert|2018|Chem.Asian J.|14|1128|doi:10.1002/asia.201800903
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5517/ccdc.csd.cc1z455g
title: CCDC 1821255: Experimental Crystal Structure Determination

description: Related Article: Jinzhong Gu, Min Wen, Yan Cai, Zifa Shi, Aliaksandr S. Arol, Marina V. Kirillova, Alexander M. Kirillov|2019|Inorg.Chem.|58|2403|doi:10.1021/acs.inorgchem.8b02926
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5517/ccdc.csd.cc1z457j
title: CCDC 1821257: Experimental Crystal Structure Determination

description: Related Article: Jinzhong Gu, Min Wen, Yan Cai, Zifa Shi, Aliaksandr S. Arol, Marina V. Kirillova, Alexander M. Kirillov|2019|Inorg.Chem.|58|2403|doi:10.1021/acs.inorgchem.8b02926
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5281/zenodo.2554195
title: Dataset: Climate experts' views on geoengineering depend on their beliefs about climate change impacts

description: This is the dataset and corresponding do-files to reproduce the main results from the Paper "Climate experts’ views on geoengineering depend on their beliefs about climate change impacts" and from the Supplemenatary Information. This fith versions incorporates additional work done after journal review.
DOI: 10.5281/zenodo.2554196
title: Dataset: Climate Experts' views on geoengineering

description: This is the dataset and corresponding do-files to reproduce the main results from the Paper "How climate experts' views on geoengineering depend on their beliefs about climate change impacts" and the Supplemenatary Information
DOI: 10.5517/ccdc.csd.cc1z7q1z
title: CCDC 1824661: Experimental Crystal Structure Determination

description: Related Article: Santosh Kumar, Raj Pal Sharma, Paloth Venugopalan, Valeria Ferretti, Michel Tarpin, Stéphanie Sayen, Emmanuel Guillon|2019|Inorg.Chim.Acta|488|260|doi:10.1016/j.ica.2019.01.020
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5517/ccdc.csd.cc1z7q20
title: CCDC 1824662: Experimental Crystal Structure Determination

description: Related Article: Santosh Kumar, Raj Pal Sharma, Paloth Venugopalan, Valeria Ferretti, Michel Tarpin, Stéphanie Sayen, Emmanuel Guillon|2019|Inorg.Chim.Acta|488|260|doi:10.1016/j.ica.2019.01.020
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5281/zenodo.2554193
title: Main dataset 'Environmental specificity in Drosophila-bacteria symbiosis affects host developmental plasticity'

description: Main dataset from the manuscript 'Environmental specificity in <em>Drosophila</em>-bacteria symbiosis affects host developmental plasticity' (2019)
DOI: 10.5281/zenodo.2554194
title: Main dataset 'Environmental specificity in Drosophila-bacteria symbiosis affects host developmental plasticity'

description: Main dataset from the manuscript 'Environmental specificity in <em>Drosophila</em>-bacteria symbiosis affects host developmental plasticity' (2019)
DOI: 10.5517/ccdc.csd.cc1z7q31
title: CCDC 1824663: Experimental Crystal Structure Determination

description: Related Article: Santosh Kumar, Raj Pal Sharma, Paloth Venugopalan, Valeria Ferretti, Michel Tarpin, Stéphanie Sayen, Emmanuel Guillon|2019|Inorg.Chim.Acta|488|260|doi:10.1016/j.ica.2019.01.020
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.7281/t1/4aj8y1/ddf6ot
title: Turnbull2018_20171022_proxydata.tab

description: Tabular file in .csv format containing an anonymized version of the data used to create all tables and figures in this publication.
DOI: 10.7281/t1/4aj8y1/vympw9
title: Turnbull2018_Deidentified booklet data codebook.pdf

description: A codebook to guide users of the datasets in Turnbull2018_20171022_proxydata.csv
DOI: 10.5281/zenodo.2541937
title: Data for the publication  "The global aerosol-climate model ECHAM6.3-HAM2.3 – Part 2: Cloud evaluation, aerosol radiative forcing and climate sensitivity"

description: This repository contains the data for the paper:

"Neubauer, D., Ferrachat, S., Siegenthaler-Le Drian, C., Stier, P. Partridge, D. G., Tegen, I., Bey, I., Stanelle, T., Kokkola, H., and Lohmann, U.: The global aerosol-climate model ECHAM6.3-HAM2.3 – Part 2: Cloud evaluation, aerosol radiative forcing and climate sensitivity, submitted to Geosci. Mod. Dev. Discuss, 2019."

Each tar-file contains the data (or instructions how to obtain the data) to reproduce a figure or table in our paper.

Note that the scripts to plot this data are to be found in the accompanying package (http://dx.doi.org/10.5281/zenodo.2553892)
DOI: 10.5517/ccdc.csd.cc1zbnhg
title: CCDC 1827496: Experimental Crystal Structure Determination

description: Related Article: C. Ounally, M. Essid, G. Bruno, S. Abid, G. Faggio, Z. Aloui|2019|J.Mol.Struct.|1183|52|doi:10.1016/j.molstruc.2018.12.092
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5281/zenodo.2541936
title: Data for the publication "The global aerosol-climate model ECHAM6.3-HAM2.3 – Part 2: Cloud evaluation, aerosol radiative forcing and climate sensitivity"

description: This repository contains the data for the paper: "Neubauer, D., Ferrachat, S., Siegenthaler-Le Drian, C., Stier, P. Partridge, D. G., Tegen, I., Bey, I., Stanelle, T., Kokkola, H., and Lohmann, U.: The global aerosol-climate model ECHAM6.3-HAM2.3 – Part 2: Cloud evaluation, aerosol radiative forcing and climate sensitivity, Geosci. Mod. Dev., https://doi.org/10.5194/gmd-2018-307, 2019." Each tar-file contains the data (or instructions how to obtain the data) to reproduce a figure or table in our paper. Note that the scripts to plot this data are to be found in the accompanying package (http://dx.doi.org/10.5281/zenodo.2553891)
DOI: 10.17632/fyj56dcdcg.1
title: Data for: The evolution of a new class of CO2 absorbents: aromatic amines

description: Tabulated data of reaction enthalpy and entropy from literature.
DOI: 10.18739/a2s46h57s
title: Siberian boreal forest energy balance (ViPER (Vegetation Impacts on Permafrost) project), Cherskiy, Sakha Republic, Russia, 2016 - 2017
DOI: 10.5281/zenodo.2554485
title: Binary black-hole simulation SXS:BBH:1396

description: Simulation of a black-hole binary system evolved by the SpEC code.