cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5281/zenodo.4395190
title: Chang'e 5 RF recording at 8471.2 MHz with Allen Telescope Array on 2020-12-19 (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 2020-12-19, after the Earth flyby, in a direct trajectory to the Sun-Earth L1 Lagrange point. 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 and 8486.2 MHz channels contains signals 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, in SigMF format. Each polarization is in a different file. The original metadata headers are also provided. This dataset contains the X polarization. The X polarization can be found in "Chang'e 5 RF recording at 8471.2 MHz with Allen Telescope Array on 2020-12-19 (X polarization)".
DOI: 10.5281/zenodo.4395189
title: Chang'e 5 RF recording at 8471.2 MHz with Allen Telescope Array on 2020-12-19 (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 2020-12-19, after the Earth flyby, in a direct trajectory to the Sun-Earth L1 Lagrange point. 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 and 8486.2 MHz channels contains signals 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, in SigMF format. Each polarization is in a different file. The original metadata headers are also provided. This dataset contains the X polarization. The X polarization can be found in "Chang'e 5 RF recording at 8471.2 MHz with Allen Telescope Array on 2020-12-19 (X polarization)".
DOI: 10.5281/zenodo.4393318
title: Chang'e 5 RF recording at 8471.2 MHz with Allen Telescope Array on 2020-12-19 (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 2020-12-19, after the Earth flyby, in a direct trajectory to the Sun-Earth L1 Lagrange point. 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 and 8486.2 MHz channels contains signals 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, 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 on 2020-12-19 (Y polarization)".
DOI: 10.5281/zenodo.4393317
title: Chang'e 5 RF recording at 8471.2 MHz with Allen Telescope Array on 2020-12-19 (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 2020-12-19, after the Earth flyby, in a direct trajectory to the Sun-Earth L1 Lagrange point. 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 and 8486.2 MHz channels contains signals 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, 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 on 2020-12-19 (Y polarization)".
DOI: 10.5281/zenodo.4405179
title: Chang'e 5 RF recording at 8486.2 MHz with Allen Telescope Array on 2020-12-19 (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 2020-12-19, after the Earth flyby, in a direct trajectory to the Sun-Earth L1 Lagrange point. 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 and 8486.2 MHz channels contains signals 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 8486.2 MHz, 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 8486.2 MHz with Allen Telescope Array on 2020-12-19 (Y polarization)".
DOI: 10.5281/zenodo.4405178
title: Chang'e 5 RF recording at 8486.2 MHz with Allen Telescope Array on 2020-12-19 (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 2020-12-19, after the Earth flyby, in a direct trajectory to the Sun-Earth L1 Lagrange point. 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 and 8486.2 MHz channels contains signals 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 8486.2 MHz, 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 8486.2 MHz with Allen Telescope Array on 2020-12-19 (Y polarization)".
DOI: 10.5281/zenodo.4408773
title: Chang'e 5 RF recording at 8471.2 MHz with Allen Telescope Array on 2020-12-20

description: This dataset contains a recording of X-band telemetry signals from the Chinese lunar sample retrieve mission Chang'e 5 done on 2020-12-20, after the Earth flyby, in a direct trajectory to the Sun-Earth L1 Lagrange point. 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 and 8486.2 MHz channels contains signals 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, in SigMF format. Each polarization is in a different file. The original metadata headers are also provided. This dataset contains the both the X and Y polarizations.
DOI: 10.5281/zenodo.4408772
title: Chang'e 5 RF recording at 8471.2 MHz with Allen Telescope Array on 2020-12-20

description: This dataset contains a recording of X-band telemetry signals from the Chinese lunar sample retrieve mission Chang'e 5 done on 2020-12-20, after the Earth flyby, in a direct trajectory to the Sun-Earth L1 Lagrange point. 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 and 8486.2 MHz channels contains signals 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, in SigMF format. Each polarization is in a different file. The original metadata headers are also provided. This dataset contains the both the X and Y polarizations.
DOI: 10.5281/zenodo.4409595
title: Chang'e 5 RF recording at 8486.2 MHz with Allen Telescope Array on 2020-12-20

description: This dataset contains a recording of X-band telemetry signals from the Chinese lunar sample retrieve mission Chang'e 5 done on 2020-12-20, after the Earth flyby, in a direct trajectory to the Sun-Earth L1 Lagrange point. 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 and 8486.2 MHz channels contains signals 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 8486.2 MHz, in SigMF format. Each polarization is in a different file. The original metadata headers are also provided. This dataset contains the both the X and Y polarizations.
DOI: 10.5281/zenodo.4409594
title: Chang'e 5 RF recording at 8486.2 MHz with Allen Telescope Array on 2020-12-20

description: This dataset contains a recording of X-band telemetry signals from the Chinese lunar sample retrieve mission Chang'e 5 done on 2020-12-20, after the Earth flyby, in a direct trajectory to the Sun-Earth L1 Lagrange point. 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 and 8486.2 MHz channels contains signals 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 8486.2 MHz, in SigMF format. Each polarization is in a different file. The original metadata headers are also provided. This dataset contains the both the X and Y polarizations.
DOI: 10.6084/m9.figshare.13514170
title: Proposition of PhD topics from T. J.-Y. Derrien

description: I list here PhD topics I could propose to undertake in near future. <br>
DOI: 10.25646/7803
title: Tagesdaten-CSV aus dem DIVI-Intensivregister

description: Die Tagesdaten-CSV entspricht einem Auszug der Daten des DIVI-Intensivregisters. Die Datei enthält eine Aggregation der aktuellsten Meldungen pro Landkreis. Es werden die aktuell gemeldeten Anzahlen der COVID-19 Intensivfälle sowie die gemeldeten intensivmedizinischen Behandlungskapazitäten angezeigt. Die Tagesdaten-CSV liefert dabei ausschließlich einen Blick auf die Daten gemäß dem Stand des betrachteten Tages. Die Daten sind im situationsbedingten Kontext aufbereitet, damit sind verschiedene Tagesdaten-CSVs u.U. nicht direkt miteinander vergleichbar. Die aktuellsten Meldungen werden im gewählten Betrachtungszeitfenster über alle Meldebereiche und Standorte aufsummiert. Weitere Informationen sind zu finden unter https://www.intensivregister.de/#/faq
DOI: 10.34740/kaggle/dsv/1805702
title: US counties COVID 19 dataset
DOI: 10.6084/m9.figshare.13514191.v1
title: codenet_dataset.pkl

description: Codenet dataset
DOI: 10.6084/m9.figshare.13514191
title: codenet_dataset.pkl

description: Codenet dataset
DOI: 10.5281/zenodo.4409744
title: Linked Ogham Ontology

description: Linked Ogham Ontology @ http://ontology.ogham.link
DOI: 10.5281/zenodo.4130691
title: Data and code for paper "Reciprocal interactions between tumour cell populations enhance growth and reduce radiation sensitivity in prostate cancer."

description: This repository contains raw data and code for the manuscript with DOI: 10.1038/s42003-020-01529-5.
DOI: 10.15468/v9unvr
title: Three new species of Marcepania Ja?oszy?ski (Coleoptera: Staphylinidae Scydmaeninae)

description: This dataset contains the digitized treatments in Plazi based on the original journal article Ja?oszy?ski, Pawe? (2020): Three new species of Marcepania Ja?oszy?ski (Coleoptera: Staphylinidae Scydmaeninae). Zootaxa 4852 (2): 223-230, DOI: https://doi.org/10.11646/zootaxa.4852.2.7
DOI: 10.15468/79dzmm
title: Two new species of the genus Zaitzevia Champion, 1923 from China (Coleoptera Elmidae: Macronychini)

description: This dataset contains the digitized treatments in Plazi based on the original journal article Jiang, Ri-Xin, Wang, Shuo (2020): Two new species of the genus Zaitzevia Champion, 1923 from China (Coleoptera Elmidae: Macronychini). Zootaxa 4852 (2): 231-238, DOI: https://doi.org/10.11646/zootaxa.4852.2.9
DOI: 10.15468/dz7xne
title: A new species of Marphysa (Annelida: Eunicida: Eunicidae) from India, with notes on previously described or reported species from the region

description: This dataset contains the digitized treatments in Plazi based on the original journal article Hutchings, Pat, Lavesque, Nicolas, Priscilla, Lyndsay, Daffe, Guillemine, Malathi, E., Glasby, Christopher J. (2020): A new species of Marphysa (Annelida: Eunicida: Eunicidae) from India, with notes on previously described or reported species from the region. Zootaxa 4852 (3): 285-308, DOI: https://doi.org/10.11646/zootaxa.4852.3.2
DOI: 10.25919/cb2c-4f35
title: Parkes observations for project P1088 semester 2020OCTS_02

description: We propose a targeted pulsar survey of twelve candidate sources that display interplanetary scintillation or linear polarisation in lower frequency observations using the Murchison Widefield Array (MWA). Known pulsars have been detected using these characteristics. We request 12 hours of Parkes observations using the UWL receiver and back-end to conduct a sensitive and thorough pulsar search using novel techniques. Targeted searches for pulsars using imaging surveys have been revived in recent years due to the availability of new sensitive, broadband, widefield surveys using SKA precursors/pathfinders, and have already resulted in pulsar discoveries. Discovering new pulsars provides prospects for many science cases because pulsars provide powerful probes of the ISM and fundamental physics either individually or as a population.
DOI: 10.15468/ky4p74
title: Ampelisca Kr?yer, 1842 (Amphipoda: Ampeliscidae) in the Persian Gulf and the Gulf of Oman

description: This dataset contains the digitized treatments in Plazi based on the original journal article Momtazi, Farzaneh (2020): Ampelisca Kr?yer, 1842 (Amphipoda: Ampeliscidae) in the Persian Gulf and the Gulf of Oman. Zootaxa 4852 (3): 333-349, DOI: https://doi.org/10.11646/zootaxa.4852.3.5
DOI: 10.15468/zrqs8k
title: A new species of Cnemaspis Strauch (Squamata: Gekkonidae) of the C. siamensis group from Tenasserim Mountains, Thailand

description: This dataset contains the digitized treatments in Plazi based on the original journal article Grismer, L. Lee, Yushchenko, Platon V., Pawangkhanant, Parinya, Nazarov, Roman A., Naiduangchan, Mali, Suwannapoom, Chatmongkon, Poyarkov, Nikolay A. (2020): A new species of Cnemaspis Strauch (Squamata: Gekkonidae) of the C. siamensis group from Tenasserim Mountains, Thailand. Zootaxa 4852 (5): 547-564, DOI: https://doi.org/10.11646/zootaxa.4852.5.3
DOI: 10.25384/sage.24055837.v1
title: sj-xlsx-4-jop-10.1177_02698811231191103 – Supplemental material for Fluoxetine rescues the depressive-like behaviour induced by reserpine and the altered emotional behaviour induced by nicotine withdrawal in zebrafish: Involvement of tyrosine hydroxylase

description: Supplemental material, sj-xlsx-4-jop-10.1177_02698811231191103 for Fluoxetine rescues the depressive-like behaviour induced by reserpine and the altered emotional behaviour induced by nicotine withdrawal in zebrafish: Involvement of tyrosine hydroxylase by Daniela Braida, Luisa Ponzoni, Ilaria Dellarole, Stefano Morara and Mariaelvina Sala in Journal of Psychopharmacology
DOI: 10.25384/sage.20072540.v1
title: sj-spv-2-hpq-10.1177_13591053221103421 – Relationships between experiencing anti-fat microaggressions, body appreciation, and perceived physical and mental health

description: sj-spv-2-hpq-10.1177_13591053221103421 for Relationships between experiencing anti-fat microaggressions, body appreciation, and perceived physical and mental health by Elizabeth A O’Neill, Kate Trout and Virginia Ramseyer Winter in Journal of Health Psychology
DOI: 10.25384/sage.22361675
title: sj-fasta-2-dhj-10.1177_20552076231165963 - Supplemental material for iDHU-Ensem: Identification of dihydrouridine sites through ensemble learning models

description: Supplemental material, sj-fasta-2-dhj-10.1177_20552076231165963 for iDHU-Ensem: Identification of dihydrouridine sites through ensemble learning models by Muhammad Taseer Suleman, Fahad Alturise and Tamim Alkhalifah, Yaser Daanial Khan in Digital Health
DOI: 10.25384/sage.24055915.v1
title: Supplemental Material - How Electoral Cycles Shape the Implementation of Public Works Programs: Evidence From India

description: Supplemental Material for How Electoral Cycles Shape the Implementation of Public Works Programs: Evidence From India by Anjali Thomas and Jonathan Darsey in Political Research Quarterly.
DOI: 10.25384/sage.22361675.v1
title: sj-fasta-2-dhj-10.1177_20552076231165963 - Supplemental material for iDHU-Ensem: Identification of dihydrouridine sites through ensemble learning models

description: Supplemental material, sj-fasta-2-dhj-10.1177_20552076231165963 for iDHU-Ensem: Identification of dihydrouridine sites through ensemble learning models by Muhammad Taseer Suleman, Fahad Alturise and Tamim Alkhalifah, Yaser Daanial Khan in Digital Health
DOI: 10.25384/sage.24055919
title: Supplemental Material - Social Imagery and Judicial Legitimacy: Evidence From Evangelical Christians

description: Supplemental Material for Social Imagery and Judicial Legitimacy: Evidence From Evangelical Christians by Alex Badas and Eric R. Schmidt in Political Research Quarterly