cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5281/zenodo.3988971
title: Data for "Atomic structure of solute clusters in Al-Zn-Mg alloys"

description: This dataset contains the data used in the publication entitled "<strong>Atomic structure of solute clusters in Al-Zn-Mg alloys</strong>", published in Acta Materialia 17. December 2020. The data contained herein are: As-acquired transmission electron microscopy (TEM) images. Atom probe tomography data. All structural models used in density functional theory (DFT) calculations. Structures used for simulating scanning-TEM (STEM) images and nanobeam diffraction (NBD) patterns. The TEM images includes high angle annular dark field (HAADF) images and selected area diffraction patterns. These are given in .dm3/.dm4 files, and can be opened in e.g. the "Gatan Microscopy Suite" software. The images are also given as .tif images. The files are names after the "Figx_alloy_condition_xxx". "Figx" refers to the figure in the main article, "alloy" describes the alloy used and "condition" describes from what ageing condition. The uncorrected image series used for Fig. 6c (in the article) is included and requires the SmartAlign plugin in the Gatan Microscopy Suite to analyse the dataset. SmartAlign allows for correcting rigid and non-rigid distortions in the STEM images in order to reduce effect of specimen drift and scan noise during acquisition. The ATP data is given as a .xlsx file. The data here is the processed data after applying the maximum separation algorithm. The data here is used to produce Figs. 2b and 2c in the paper. <br> <br> The structures used in the DFT calculations are given here as .cif files. These are separated into "Single_clusters" and "Stacked_clusters" and named according to Tabs. 1 and 2 in the Supplementary material of the paper. The two structures used for simulating STEM-HAADF and NBD patterns are given in the folder "TEM_simulations". "Mg32Zn124D_94x94" was used for NBD and "Mg32Zn124D_X_Zn4" was used for HAADF-STEM. The stack used for Supplementary Fig. 7c is labeled "Mg32Zn124D_94x94_slab_1Allayerop.cif".
DOI: 10.6084/m9.figshare.12936857
title: Positive deviance for promoting dual-method contraceptive use among women in Uganda: a cluster randomized controlled trial (Dataset_PhaseII)

description: The data set comprised of baseline and follow-up data of 960 women from 20 health facilities in Mbarara District, Uganda/.
DOI: 10.6084/m9.figshare.12936857.v2
title: Positive deviance for promoting dual-method contraceptive use among women in Uganda: a cluster randomized controlled trial (Dataset_PhaseII)

description: The data set comprised of baseline and follow-up data of 960 women from 20 health facilities in Mbarara District, Uganda/.
DOI: 10.25919/hgcr-5p06
title: Parkes observations for project P895 semester 2020APRS_03

description: Since the year 2005, the Parkes Pulsar Timing Array (PPTA) project has been placing ever more stringent constraints on the amplitude of a gravitational wave background signal. Such upper bounds on the amplitude of the gravitational wave signal are currently dominated by a single pulsar: PSR J1909-3744. The upper bound with this pulsar alone already cuts into the range of tenable theoretical models. Further reducing the amplitude bound (by continued regular observations of this pulsar) will significantly narrow that range. The first evidence of gravitational waves in the pulsar data are likely to be observed in the timing for PSR J1909-3744, but with only a single pulsar we will not be able to make an unambiguous detection. However, knowledge of the likely signal strength (derived from this pulsar) will help to optimise the observing strategy for the detection of the gravitational wave signals with existing or future pulsar timing arrays.
DOI: 10.5281/zenodo.4362116
title: Porous RuOxNySz Electrodes for Microsupercapacitors and Microbatteries with Enhanced Areal Performance

description: Figures 1, 2, 3, 4 & 5
DOI: 10.5281/zenodo.4362115
title: Porous RuOxNySz Electrodes for Microsupercapacitors and Microbatteries with Enhanced Areal Performance

description: Figures 1, 2, 3, 4 & 5
DOI: 10.3886/e121361v2-72580
title: Depression, risk factors, and coping strategies in the context of social dislocations resulting from the second wave of COVID-19: A web survey in Japan
DOI: 10.6084/m9.figshare.12919013
title: Chemistry of Atmospheric Fine Particles during the COVID-19 Pandemic in a Megacity of Eastern China

description: COVID-19 observed and simulated data<br>
DOI: 10.6084/m9.figshare.12919013.v3
title: Chemistry of Atmospheric Fine Particles during the COVID-19 Pandemic in a Megacity of Eastern China

description: COVID-19 observed and simulated data<br>
DOI: 10.15161/oar.it/73348
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: 10.25919/xc86-ka87
title: Parkes observations for project P885 semester 2020APRS_22

description: We propose to observe the magnetars 1E 1547.0-5408 and PSR J1622-4950 approximately weekly, to track their rotation, flux density, and polarisation, as we have long been doing through this project. The revolutionary UWL capabilities promise new opportunities to disentangle still mysterious radio emission mechanisms in magnetars. This promise is supported by the recent follow up of XTE J1810-197, again a radio magnetar after 10 years dormant, for which our observations with the UWL receiver are providing unique and tantalizing measurements of its radio spectrum and polarisation.
DOI: 10.21258/1713744
title: Swiss national forest inventory - Result table No. 898491
DOI: 10.21258/1699411
title: Swiss national forest inventory - Result table No. 891921
DOI: 10.21258/1679019
title: Swiss national forest inventory - Result table No. 898083
DOI: 10.21258/1691269
title: Swiss national forest inventory - Result table No. 891833
DOI: 10.21258/1713107
title: Swiss national forest inventory - Result table No. 899068
DOI: 10.21258/1676670
title: Swiss national forest inventory - Result table No. 892000
DOI: 10.6084/m9.figshare.12901928
title: Breast cancer Qatar dataset RA-QA

description: RNASeq expression data and coded clinical annotation.
DOI: 10.21258/1696520
title: Swiss national forest inventory - Result table No. 892681
DOI: 10.21258/1705835
title: Swiss national forest inventory - Result table No. 891771
DOI: 10.21258/1719665
title: Swiss national forest inventory - Result table No. 898225
DOI: 10.21258/1688531
title: Swiss national forest inventory - Result table No. 891731
DOI: 10.5281/zenodo.4362098
title: Chang'e 5 RF recording at 8471.2 MHz with Allen Telescope Array after TEI-2 (Y polarization)

description: This dataset contains a recording of X-band telemetry signals from the Chinese lunar sample retrieve mission Chang'e 5 done on 2020-12-13, after the TEI-2 manoeuvre that ejected the spacecraft away from lunar orbit. The recording was done at Allen Telescope Array using antenna 2h in dual XY (linear) polarization. The hardware configuration was as follows: antenna 2h was connected to RFCB LO d, which was tuned to a frequency of 8475 MHz and used an output IF of 512 MHz. A USRP N321 was connected to the IF output of the RFCB and digitized both polarizations. The USRP used external 10 MHz reference and PPS coming from the observatory distribution system. The IQ sample rate of the USRP was 30.72 Msps and a GNU Radio flowgraph was used to channelize four frequencies from the spacecraft (8463.7, 8471.2, 8478.6 and 8486.2 MHz), using an IQ sample rate of 480 ksps for each channel. Only the 8471.2 MHz channel contains a signal from the spacecraft. The GNU Radio flowgraph stored the IQ data for each channel as 32-bit floats in the GNU Radio metatata file format, with detached headers. After recording, the data was converted 16-bit integers and SigMF format. This dataset contains the IQ data for the channel at 8471.2 MHz, which corresponds to the orbiter, in SigMF format. Each polarization is in a different file. The original metadata headers are also provided. This dataset contains the Y polarization. The X polarization can be found in "Chang'e 5 RF recording at 8471.2 MHz with Allen Telescope Array after TEI-2 (X polarization)".
DOI: 10.5281/zenodo.4362097
title: Chang'e 5 RF recording at 8471.2 MHz with Allen Telescope Array after TEI-2 (Y polarization)

description: This dataset contains a recording of X-band telemetry signals from the Chinese lunar sample retrieve mission Chang'e 5 done on 2020-12-13, after the TEI-2 manoeuvre that ejected the spacecraft away from lunar orbit. The recording was done at Allen Telescope Array using antenna 2h in dual XY (linear) polarization. The hardware configuration was as follows: antenna 2h was connected to RFCB LO d, which was tuned to a frequency of 8475 MHz and used an output IF of 512 MHz. A USRP N321 was connected to the IF output of the RFCB and digitized both polarizations. The USRP used external 10 MHz reference and PPS coming from the observatory distribution system. The IQ sample rate of the USRP was 30.72 Msps and a GNU Radio flowgraph was used to channelize four frequencies from the spacecraft (8463.7, 8471.2, 8478.6 and 8486.2 MHz), using an IQ sample rate of 480 ksps for each channel. Only the 8471.2 MHz channel contains a signal from the spacecraft. The GNU Radio flowgraph stored the IQ data for each channel as 32-bit floats in the GNU Radio metatata file format, with detached headers. After recording, the data was converted 16-bit integers and SigMF format. This dataset contains the IQ data for the channel at 8471.2 MHz, which corresponds to the orbiter, in SigMF format. Each polarization is in a different file. The original metadata headers are also provided. This dataset contains the Y polarization. The X polarization can be found in "Chang'e 5 RF recording at 8471.2 MHz with Allen Telescope Array after TEI-2 (X polarization)".
DOI: 10.5281/zenodo.4347577
title: Chang'e 5 RF recording at 8471.2 MHz with Allen Telescope Array after TEI-2 (X polarization)

description: This dataset contains a recording of X-band telemetry signals from the Chinese lunar sample retrieve mission Chang'e 5 done on 2020-12-13, after the TEI-2 manoeuvre that ejected the spacecraft away from lunar orbit. The recording was done at Allen Telescope Array using antenna 2h in dual XY (linear) polarization. The hardware configuration was as follows: antenna 2h was connected to RFCB LO d, which was tuned to a frequency of 8475 MHz and used an output IF of 512 MHz. A USRP N321 was connected to the IF output of the RFCB and digitized both polarizations. The USRP used external 10 MHz reference and PPS coming from the observatory distribution system. The IQ sample rate of the USRP was 30.72 Msps and a GNU Radio flowgraph was used to channelize four frequencies from the spacecraft (8463.7, 8471.2, 8478.6 and 8486.2 MHz), using an IQ sample rate of 480 ksps for each channel. Only the 8471.2 MHz channel contains a signal from the spacecraft. The GNU Radio flowgraph stored the IQ data for each channel as 32-bit floats in the GNU Radio metatata file format, with detached headers. After recording, the data was converted 16-bit integers and SigMF format. This dataset contains the IQ data for the channel at 8471.2 MHz, which corresponds to the orbiter, in SigMF format. Each polarization is in a different file. The original metadata headers are also provided. This dataset contains the X polarization. The Y polarization can be found in "Chang'e 5 RF recording at 8471.2 MHz with Allen Telescope Array after TEI-2 (Y polarization)".
DOI: 10.5281/zenodo.4347576
title: Chang'e 5 RF recording at 8471.2 MHz with Allen Telescope Array after TEI-2 (X polarization)

description: This dataset contains a recording of X-band telemetry signals from the Chinese lunar sample retrieve mission Chang'e 5 done on 2020-12-13, after the TEI-2 manoeuvre that ejected the spacecraft away from lunar orbit. The recording was done at Allen Telescope Array using antenna 2h in dual XY (linear) polarization. The hardware configuration was as follows: antenna 2h was connected to RFCB LO d, which was tuned to a frequency of 8475 MHz and used an output IF of 512 MHz. A USRP N321 was connected to the IF output of the RFCB and digitized both polarizations. The USRP used external 10 MHz reference and PPS coming from the observatory distribution system. The IQ sample rate of the USRP was 30.72 Msps and a GNU Radio flowgraph was used to channelize four frequencies from the spacecraft (8463.7, 8471.2, 8478.6 and 8486.2 MHz), using an IQ sample rate of 480 ksps for each channel. Only the 8471.2 MHz channel contains a signal from the spacecraft. The GNU Radio flowgraph stored the IQ data for each channel as 32-bit floats in the GNU Radio metatata file format, with detached headers. After recording, the data was converted 16-bit integers and SigMF format. This dataset contains the IQ data for the channel at 8471.2 MHz, which corresponds to the orbiter, in SigMF format. Each polarization is in a different file. The original metadata headers are also provided. This dataset contains the X polarization. The Y polarization can be found in "Chang'e 5 RF recording at 8471.2 MHz with Allen Telescope Array after TEI-2 (Y polarization)".
DOI: 10.5281/zenodo.4341911
title: Chang'e 5 RF recording at 8471.2 MHz with Allen Telescope Array between TEI-1 and TEI-2 (Y polarization)

description: This dataset contains a recording of X-band telemetry signals from the Chinese lunar sample retrieve mission Chang'e 5 done on 2020-12-12, between the TEI-1 (trans-Earth injection 1) manoeuvre that moved the spacecraft to an elliptical lunar orbit and the TEI-2 manoeuvre that ejected the spacecraft away from lunar orbit. The recording was done at Allen Telescope Array using antenna 2h in dual XY (linear) polarization. The hardware configuration was as follows: antenna 2h was connected to RFCB LO d, which was tuned to a frequency of 8475 MHz and used an output IF of 512 MHz. A USRP N321 was connected to the IF output of the RFCB and digitized both polarizations. The USRP used external 10 MHz reference and PPS coming from the observatory distribution system. The IQ sample rate of the USRP was 30.72 Msps and a GNU Radio flowgraph was used to channelize four frequencies from the spacecraft (8463.7, 8471.2, 8478.6 and 8486.2 MHz), using an IQ sample rate of 480 ksps for each channel. Only the 8471.2 MHz channel contains a signal from the spacecraft. The GNU Radio flowgraph stored the IQ data for each channel as 32-bit floats in the GNU Radio metatata file format, with detached headers. After recording, the data was converted 16-bit integers and SigMF format. This dataset contains the IQ data for the channel at 8471.2 MHz, which corresponds to the orbiter, in SigMF format. Each polarization is in a different file. The original metadata headers are also provided. This dataset contains the Y polarization. The X polarization can be found in "Chang'e 5 RF recording at 8471.2 MHz with Allen Telescope Array between TEI-1 and TEI-2 (X polarization)".
DOI: 10.5281/zenodo.4341910
title: Chang'e 5 RF recording at 8471.2 MHz with Allen Telescope Array between TEI-1 and TEI-2 (Y polarization)

description: This dataset contains a recording of X-band telemetry signals from the Chinese lunar sample retrieve mission Chang'e 5 done on 2020-12-12, between the TEI-1 (trans-Earth injection 1) manoeuvre that moved the spacecraft to an elliptical lunar orbit and the TEI-2 manoeuvre that ejected the spacecraft away from lunar orbit. The recording was done at Allen Telescope Array using antenna 2h in dual XY (linear) polarization. The hardware configuration was as follows: antenna 2h was connected to RFCB LO d, which was tuned to a frequency of 8475 MHz and used an output IF of 512 MHz. A USRP N321 was connected to the IF output of the RFCB and digitized both polarizations. The USRP used external 10 MHz reference and PPS coming from the observatory distribution system. The IQ sample rate of the USRP was 30.72 Msps and a GNU Radio flowgraph was used to channelize four frequencies from the spacecraft (8463.7, 8471.2, 8478.6 and 8486.2 MHz), using an IQ sample rate of 480 ksps for each channel. Only the 8471.2 MHz channel contains a signal from the spacecraft. The GNU Radio flowgraph stored the IQ data for each channel as 32-bit floats in the GNU Radio metatata file format, with detached headers. After recording, the data was converted 16-bit integers and SigMF format. This dataset contains the IQ data for the channel at 8471.2 MHz, which corresponds to the orbiter, in SigMF format. Each polarization is in a different file. The original metadata headers are also provided. This dataset contains the Y polarization. The X polarization can be found in "Chang'e 5 RF recording at 8471.2 MHz with Allen Telescope Array between TEI-1 and TEI-2 (X polarization)".
DOI: 10.5281/zenodo.4331733
title: Chang'e 5 RF recording at 8471.2 MHz with Allen Telescope Array between TEI-1 and TEI-2 (X polarization)

description: This dataset contains a recording of X-band telemetry signals from the Chinese lunar sample retrieve mission Chang'e 5 done on 2020-12-12, between the TEI-1 (trans-Earth injection 1) manoeuvre that moved the spacecraft to an elliptical lunar orbit and the TEI-2 manoeuvre that ejected the spacecraft away from lunar orbit. The recording was done at Allen Telescope Array using antenna 2h in dual XY (linear) polarization. The hardware configuration was as follows: antenna 2h was connected to RFCB LO d, which was tuned to a frequency of 8475 MHz and used an output IF of 512 MHz. A USRP N321 was connected to the IF output of the RFCB and digitized both polarizations. The USRP used external 10 MHz reference and PPS coming from the observatory distribution system. The IQ sample rate of the USRP was 30.72 Msps and a GNU Radio flowgraph was used to channelize four frequencies from the spacecraft (8463.7, 8471.2, 8478.6 and 8486.2 MHz), using an IQ sample rate of 480 ksps for each channel. Only the 8471.2 MHz channel contains a signal from the spacecraft. The GNU Radio flowgraph stored the IQ data for each channel as 32-bit floats in the GNU Radio metatata file format, with detached headers. After recording, the data was converted 16-bit integers and SigMF format. This dataset contains the IQ data for the channel at 8471.2 MHz, which corresponds to the orbiter, in SigMF format. Each polarization is in a different file. The original metadata headers are also provided. This dataset contains the X polarization. The Y polarization can be found in "Chang'e 5 RF recording at 8471.2 MHz with Allen Telescope Array between TEI-1 and TEI-2 (Y polarization)".
DOI: 10.5281/zenodo.4331732
title: Chang'e 5 RF recording at 8471.2 MHz with Allen Telescope Array between TEI-1 and TEI-2 (X polarization)

description: This dataset contains a recording of X-band telemetry signals from the Chinese lunar sample retrieve mission Chang'e 5 done on 2020-12-12, between the TEI-1 (trans-Earth injection 1) manoeuvre that moved the spacecraft to an elliptical lunar orbit and the TEI-2 manoeuvre that ejected the spacecraft away from lunar orbit. The recording was done at Allen Telescope Array using antenna 2h in dual XY (linear) polarization. The hardware configuration was as follows: antenna 2h was connected to RFCB LO d, which was tuned to a frequency of 8475 MHz and used an output IF of 512 MHz. A USRP N321 was connected to the IF output of the RFCB and digitized both polarizations. The USRP used external 10 MHz reference and PPS coming from the observatory distribution system. The IQ sample rate of the USRP was 30.72 Msps and a GNU Radio flowgraph was used to channelize four frequencies from the spacecraft (8463.7, 8471.2, 8478.6 and 8486.2 MHz), using an IQ sample rate of 480 ksps for each channel. Only the 8471.2 MHz channel contains a signal from the spacecraft. The GNU Radio flowgraph stored the IQ data for each channel as 32-bit floats in the GNU Radio metatata file format, with detached headers. After recording, the data was converted 16-bit integers and SigMF format. This dataset contains the IQ data for the channel at 8471.2 MHz, which corresponds to the orbiter, in SigMF format. Each polarization is in a different file. The original metadata headers are also provided. This dataset contains the X polarization. The Y polarization can be found in "Chang'e 5 RF recording at 8471.2 MHz with Allen Telescope Array between TEI-1 and TEI-2 (Y polarization)".
DOI: 10.21258/1709464
title: Swiss national forest inventory - Result table No. 892967
DOI: 10.21258/1697988
title: Swiss national forest inventory - Result table No. 891686
DOI: 10.21258/1678401
title: Swiss national forest inventory - Result table No. 897580
DOI: 10.21258/1703204
title: Swiss national forest inventory - Result table No. 891789
DOI: 10.21258/1683508
title: Swiss national forest inventory - Result table No. 891687
DOI: 10.21258/1696306
title: Swiss national forest inventory - Result table No. 897191
DOI: 10.21258/1688333
title: Swiss national forest inventory - Result table No. 899376
DOI: 10.21258/1695369
title: Swiss national forest inventory - Result table No. 898178
DOI: 10.21258/1691664
title: Swiss national forest inventory - Result table No. 898187
DOI: 10.21258/1697309
title: Swiss national forest inventory - Result table No. 898541
DOI: 10.21258/1693256
title: Swiss national forest inventory - Result table No. 891800
DOI: 10.21258/1713729
title: Swiss national forest inventory - Result table No. 902056
DOI: 10.21258/1682969
title: Swiss national forest inventory - Result table No. 899148
DOI: 10.21258/1713209
title: Swiss national forest inventory - Result table No. 902071
DOI: 10.21258/1713054
title: Swiss national forest inventory - Result table No. 897718
DOI: 10.21258/1687029
title: Swiss national forest inventory - Result table No. 891847
DOI: 10.21258/1691251
title: Swiss national forest inventory - Result table No. 891998
DOI: 10.21258/1702694
title: Swiss national forest inventory - Result table No. 898725
DOI: 10.21258/1714889
title: Swiss national forest inventory - Result table No. 892007
DOI: 10.21258/1702810
title: Swiss national forest inventory - Result table No. 902281
DOI: 10.21258/1690328
title: Swiss national forest inventory - Result table No. 891693
DOI: 10.6084/m9.figshare.13415867
title: E. coli 1D2 nanopore sequencing reads

description: Set of 1D<sup>2</sup> <i>E. coli</i> reads used for testing PoreOver (https://github.com/jordisr/poreover) in "Pair consensus decoding improves accuracy of neural network basecallers for nanopore sequencing" Silvestre-Ryan and Holmes (2020).<br><br>Files:- ecoli-74e17dd3: <i>E. coli</i> reference genome- read_pairs.txt: list of 1D<sup>2</sup> read pairs- reads/: directory of FAST5 files<br><br>This data was originally generated by Oxford Nanopore Technologies and is shared with permission. Sequencing was done with R9.4 pore chemistry in October 2018 and accuracy may not be representative of the current platform.<br>