cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5517/ccdc.csd.cc2gvljg
title: CCDC 2289676: Experimental Crystal Structure Determination

description: Related Article: Marvin Fresia, Alexandra Dierks, Peter G. Jones, Thomas Lindel|2023|Org.Biomol.Chem.|21|9065|doi:10.1039/D3OB01566A
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.cc2gymvx
title: CCDC 2292600: Experimental Crystal Structure Determination

description: Related Article: Jie Fan, Qinqin Yan, Huaqing Liu, Lijun Li, Zhong-Quan Liu, Zejiang Li|2023|New J.Chem.|47|20713|doi:10.1039/D3NJ04433E
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.cc2g230p
title: CCDC 2266131: Experimental Crystal Structure Determination

description: Related Article: Sonia Moreno, David Royo, Abdel G. El-Hachimi, María Rodríguez-Castillo, Miguel Monge, M. Elena Olmos, José M. López-de-Luzuriaga|2023|Dalton Trans.|52|17119|doi:10.1039/D3DT02000B
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: 10.5066/p943edyx
title: Geologic map of the Oxia Palus Quadrangle of Mars

description: The Oxia Palus quadrangle contains three distinct geologic provinces: (1) an elevated cratered plateau that occupies three-fourths of the quadrangle and is similar to much of the southern hemisphere of Mars; (2) the low, relatively featureless Chryse Planitia in the northwest corner; and (3) a complex province of chaotic terrain and immense channels or valleys that divides the plateau an determinates at Chryse Planitia. Generally, the oldest geologic units occur in the plateau province and the youngest in Chryse Planitia. Discovery by Mariner 9 of the channels, the four largest of which are given neames meaning Mars in Akkadian, Sumerian, Anglo-Saxon, and Greek (west to east), renews the possibility of water and therefore life on Mars. This possibility may be tested in July 1976 by a landing of the unmanned Viking spacecraft in Chryse Planitia at the mouths of the channels (lat 19.5 degrees N., long 34 degrees).
DOI: 10.5066/p9plwwof
title: Geologic map of the Phoenicis Lacus Quadrangle of Mars

description: The Phoenicis Lacus quadrangle (named Lake of the Phoenix by Schiaparelli, 1877) includes some of the largest geologic features recognized on the terrestrial planets. Arsia and Pavonis Montes, (South Spot and Middle Spot of Marine 9) rise 18 and 17 km, respectively, above the surrounding plateau to an elevation large volcanoes Ascraeus and Olympus Montes, located outside the quadrangle to the north, are also about 27 km in height, about three times as high as any volcano on Earth. The summit caldera of Arsia Mons, more than 100 km in diameter, is the largest known. Syria and Sinai Plana are part of the highest plateau of Mars, the Tharsis plateau; their relative elevation, 10 km, is twice that of the Tibetan Plateau, the highest plateau on Earth. Noctis Labyrinthus, the great system of fault valleys at the west end of Vallis Marineris which is located outside the quadrangle to the east, displays a more clearly developed system of faults than the largest continental fault system on Earth, the East Planitia; the difference in elevation between the volcanic peaks and the Amazonis low plains is greater than the relief from the top of the Andes to the bottom of the Peruvian trench. This great slope on Mars is similar to the continental shelf and slope that marks the transition between the continents and ocean basin floors on the Earth.
DOI: 10.5281/zenodo.10211681
title: Measurements of fault slip associated with the 2023 Superstition Hills Fault slow slip event

description: Creepmeter time series, global navigation satellite system (GNSS) measurements, line-of-sight Sentinel-1A interferograms with atmospheric corrections, and field measurements of slip along the Superstition Hills Fault in 2023 due to slow slip.
DOI: 10.5281/zenodo.10211682
title: Measurements of fault slip associated with the 2023 Superstition Hills Fault slow slip event

description: Creepmeter time series, global navigation satellite system (GNSS) measurements, line-of-sight Sentinel-1A interferograms with atmospheric corrections, and field measurements of slip along the Superstition Hills Fault in 2023 due to slow slip.
DOI: 10.5066/p974x5xt
title: Geologic map of the Coprates Quadrangle of Mars

description: The Coprates quadrangle lies to the east of the Tharsis volcanic complex and the Noctis Labyrinthus tectonic complex. To the north are the plains of Lunae Planum, to the east the vast patches of chaotic terrain and the large sinuous channels that trend northward into Chryse Planitia. On the southwest is the Thaumasia Fossae region of tectonically deformed cratered terrain, to the southeast, the Argyre Basin, the best preserved of the ancient martian impact basins. The geology of the Corpates quadrangle is dominated by the Valles Marineris chasma system, which stretches in an east-southeast direction for about 2,500 km across the quadrangle. Its maximum width is about 600 km from the north rim of Ophir Chasma to the south rim of Melas Chasma. The terminus of Valles Marineris at the eastern edge of the map is about 500 km wide in the north-south direction. Individual segments of the chasma system are 100 to 150 km wide and 2 to 4 km deep.
DOI: 10.5066/p9ytj1mc
title: Geologic map of the Noachis Quadrangle of Mars

description: The Noachis quadrangle is in the ancient cratered highlands of Mars. Craters dominate the surface of the planet in this area; most are of impact origin, some are of volcanic origin, and some are of undetermined origin. Impact craters in the Noachis quadrangle are classified into four groups based on their morphologic characteristics, each group representing a relative age range. Where applicable, superposition relations support relative age determinations based on crater morphology.
DOI: 10.5281/zenodo.10215118
title: 3-Monochloropropandiol and Glycidyl Esters in Heat-Processed Oil-Based Food Products: Exposure and Risk
DOI: 10.5281/zenodo.10215119
title: 3-Monochloropropandiol and Glycidyl Esters in Heat-Processed Oil-Based Food Products: Exposure and Risk
DOI: 10.5066/p9xy9qc2
title: Geologic map of the Elysium Quadrangle of Mars
DOI: 10.6084/m9.figshare.24654024
title: AEM01654-23-Supplemental_Dataset_2

description: GWAS analyses output file
DOI: 10.6084/m9.figshare.24654024.v1
title: AEM01654-23-Supplemental_Dataset_2

description: GWAS analyses output file
DOI: 10.25952/qb79-km81
title: The School House System

description: The dataset consists of survey results, collected from secondary students within two secondary schools located in South-East Victoria. The survey consists of Likert-scale questions relating to engagement, connectedness and staff-student relationships both within a house context and a whole-school context.
description: The dataset consists of survey results, collected from secondary students within two secondary schools located in South-East Victoria. The survey consists of Likert-scale questions relating to engagement, connectedness and staff-student relationships both within a house context and a whole-school context.
DOI: 10.5066/p9cvi0wg
title: Geologic map of the Hellas Quadrangle of Mars

description: The area of MC-28 is centered at the east edge of the Hellas Planitia (Hellas basin and surrounding plains) within densely cratered terrain that covers more than half the surface of Mars (Carr, 1973). The deepest part of the basin lies 4-5 km below the surface of the cratered terrain (Hanel and others, 1972). An irregular band of mountain and knobby material about the eastern margin of the basin and broad bands of mantled rough material on the floor of the basin represent ejecta from this very old impact. The vast, gently sloping, featureless eastern and southern part of Hellas Planitia, shown on the Shaded Relief Map of Mars (U.S.G.S., Atlas of Mars, MM 25M IR, 1972), is probably the result of extensive volcanic flooding form shield volcanoes and from possible fissures in the north-east part of the quadrangle. Long, flat-floored sinuous channels originate in these volcanic terrains and course into the basin.
DOI: 10.5281/zenodo.10214950
title: Simulated gene expression datasets using SimulatorGRN

description: This record contains gene expression data simulated using SimulatorGRN that that were used for the evaluation of BoostDiff.
DOI: 10.5281/zenodo.8054802
title: Simulated gene expression datasets using SimulatorGRN

description: This record contains gene expression data simulated using SimulatorGRN that that were used for the evaluation of BoostDiff.
DOI: 10.5281/zenodo.8054803
title: Simulated gene expression datasets using SimulatorGRN

description: This record contains gene expression data simulated using SimulatorGRN that that were used for the evaluation of BoostDiff.
DOI: 10.5066/p9bv7y5t
title: Geologic map of the Syrtis Major Quadrangle of Mars

description: The Syrtis Major quadrangle is located in the equatorial belt of Mars across the boundary between the cratered plateau region to the south and west and the northern lowland plains. The cratered plateau is part of the northern extension of cratered highlands, which generally stand at altitudes greater than 4 km. The southeastern part of the quadrangle is dominated by eastward-sloping plains on the floors of Sytris Major and Isidis Planitia. Total relief in the quadrangle is greater than 6 km over a latitudinal distance of 2,000 km, corresponding to a regional slope of 0.6 degree in an east-northeast direction.
DOI: 10.5281/zenodo.10215151
title: Data set for "Reconciling High-resolution Strain Rate of Continental China from GNSS Data with the Spherical Spline Interpolation"

description: Data set for "Reconciling High-resolution Strain Rate of Continental China from GNSS Data with the Spherical Spline Interpolation". And This database contains GNSS velocity and strain rate field data for mainland China obtained by the spherical spline method. Also, we include the sub-graph data for each graph of the manuscript "Reconciling High-resolution Strain Rate of Continental China from GNSS Data with the Spherical Spline Interpolation". We have detailed the meaning and format of each data in the "readme.txt", and a separate "readme.txt" is included in each zip.
DOI: 10.5281/zenodo.7735598
title: Data set for "Reconciling High-resolution Strain Rate of Continental China from GNSS Data with the Spherical Spline Interpolation"

description: Data set for "Reconciling High-resolution Strain Rate of Continental China from GNSS Data with the Spherical Spline Interpolation". And This database contains GNSS velocity and strain rate field data for mainland China obtained by the spherical spline method. Also, we include the sub-graph data for each graph of the manuscript "Reconciling High-resolution Strain Rate of Continental China from GNSS Data with the Spherical Spline Interpolation". We have detailed the meaning and format of each data in the "readme.txt", and a separate "readme.txt" is included in each zip.
DOI: 10.5281/zenodo.7735599
title: Data set for "Reconciling High-resolution Strain Rate of Continental China from GNSS Data with the Spherical Spline Interpolation"

description: Data set for "Reconciling High-resolution Strain Rate of Continental China from GNSS Data with the Spherical Spline Interpolation". This database contains unprocessed seismic mechanism (http://isc.ac.uk) and GNSS velocity field data (https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2019JB018774). And This database also contains strain rate field data for mainland China obtained by the spherical spline method. Also, we include the sub-graph data for each graph of the manuscript "Reconciling High-resolution Strain Rate of Continental China from GNSS Data with the Spherical Spline Interpolation". We have detailed the meaning and format of each data in the "readme.txt", and a separate "readme.txt" is included in each zip.
DOI: 10.5281/zenodo.7735806
title: Data set for "Reconciling High-resolution Strain Rate of Continental China from GNSS Data with the Spherical Spline Interpolation"

description: Data set for "Reconciling High-resolution Strain Rate of Continental China from GNSS Data with the Spherical Spline Interpolation". This database contains unprocessed seismic mechanism (http://isc.ac.uk) and GNSS velocity field data (https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2019JB018774). And This database also contains strain rate field data for mainland China obtained by the spherical spline method. Also, we include the sub-graph data for each graph of the manuscript "Reconciling High-resolution Strain Rate of Continental China from GNSS Data with the Spherical Spline Interpolation". We have detailed the meaning and format of each data in the "readme.txt", and a separate "readme.txt" is included in each zip.
DOI: 10.34740/kaggle/dsv/7077716
title: Daily Public Opinion on Israel-Palestine War
DOI: 10.5281/zenodo.10093009
title: Cross-correlation functions of Popocatépetl volcano (1999-2000, 2015-2016, and 2019-2020)

description: The ZIP file contains the cross-correlations (CC) functions computed from ambient seismic noise of Popocatépetl's temporal and permanent seismic networks (e.g., 1999-2000, 2015-2016, and 2019-2020). The CC are organizated in two folders BM and PCC, the CC computed using Bensen method and Phase Weighting cross-correlation, respectevely.
Data in SAC format. All details about stations (name, latitude longitude, elevation) and data (sampling rate, starting and ending time, etc.) are in the HEADER of each file.
DOI: 10.5281/zenodo.10093010
title: Cross-correlation functions of Popocatépetl volcano (1999-2000, 2015-2016, and 2019-2020)

description: The ZIP file contains the cross-correlations (CC) functions computed from ambient seismic noise of Popocatépetl's temporal and permanent seismic networks (e.g., 1999-2000, 2015-2016, and 2019-2020). The CC are organizated in two folders BM and PCC, the CC computed using Bensen method and Phase Weighting cross-correlation, respectevely.
Data in SAC format. All details about stations (name, latitude longitude, elevation) and data (sampling rate, starting and ending time, etc.) are in the HEADER of each file.
DOI: 10.5066/p9lmxccn
title: Geologic map of the Arabia Quadrangle of Mars

description: The Arabia quadrangle is located in the northern hemisphere of Mars; it extends 30 degrees N. from the equator and 45 degrees E. from the prime meridian. It is within the area of unmantled terrain defined by Soberblom and others (1973) and the planet-encircling band of old cratered deposits shown on the preliminary geologic map of Mars (Carr and others, 1973). Crater density in the Arabia quadrangle is similar to the heavily cratered regions located south of the equator owing to inclination of the great circle division between heavily and less cratered Martian terrains (Soberblom and others (1974). None of the large prominent telescopically defined Martian surface markings dominate the Arabia quadrangle, although the northern tip of Meridiani Sinus projects slightly into the extreme southwest corner. The topographic map of Mars (U. S. Geol. Survey, 1976) indicates that elevations in the Araba quadrangle rise toward the northeast. The entire region lacks high relief.
DOI: 10.5066/p95d1lib
title: Geologic map of the Eridania Quadrangle of Mars

description: The Eridania quadrangle is located within the densely cratered terrain of the southern hemisphere of Mars, east of the large circular Hellas Basin. The area contains three distinct physiographic provinces that divide the quadrangle into latitudinal belts. The northern part of the quadrangle is dominated by cratered upland plateau, the central part by plains, the southern part by a mottled surface of rugged topography and a high density of craters subdued by erosion. In general, the oldest geologic units occur in the upland terrains, the youngest in the central lowlands.
DOI: 10.34740/kaggle/dsv/6983486
title: AZP v1
DOI: 10.5281/zenodo.10214979
title: Finding Candida auris in public metagenomic repositories

description: Candida auris is a newly emerged multidrug-resistant fungus capable of causing invasive infections with high mortality. Despite intense efforts to understand how this pathogen rapidly emerged and spread worldwide, its environmental reservoirs are poorly understood. Here, we present a collaborative effort between the U.S. Centers for Disease Control and Prevention, the National Center for Biotechnology Information, and GridRepublic (a volunteer computing platform) to identify C. auris sequences in publicly available metagenomic datasets. We developed the MetaNISH pipeline that uses SRPRISM to align sequences to a set of reference genomes and computes a score for each reference genome. We used MetaNISH to scan ~300,000 SRA metagenomic runs from 2010 onwards and identified five datasets containing C. auris reads. Finally, GridRepublic has implemented a prospective C. auris molecular monitoring system using MetaNISH and volunteer computing.
DOI: 10.5281/zenodo.10214980
title: Finding Candida auris in public metagenomic repositories

description: Candida auris is a newly emerged multidrug-resistant fungus capable of causing invasive infections with high mortality. Despite intense efforts to understand how this pathogen rapidly emerged and spread worldwide, its environmental reservoirs are poorly understood. Here, we present a collaborative effort between the U.S. Centers for Disease Control and Prevention, the National Center for Biotechnology Information, and GridRepublic (a volunteer computing platform) to identify C. auris sequences in publicly available metagenomic datasets. We developed the MetaNISH pipeline that uses SRPRISM to align sequences to a set of reference genomes and computes a score for each reference genome. We used MetaNISH to scan ~300,000 SRA metagenomic runs from 2010 onwards and identified five datasets containing C. auris reads. Finally, GridRepublic has implemented a prospective C. auris molecular monitoring system using MetaNISH and volunteer computing.
DOI: 10.5517/ccdc.csd.cc2dy93s
title: CCDC 2232685: Experimental Crystal Structure Determination

description: Related Article: Yingzhu Sun, Changjiang Yu, Wanping Qian, Hongtao Zhang, Lijuan Jiao, Jiazhu Li, Minghua Liu, Erhong Hao|2023|Chem.Commun.|59|13986|doi:10.1039/D3CC04727J
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.cc2dy94t
title: CCDC 2232686: Experimental Crystal Structure Determination

description: Related Article: Yingzhu Sun, Changjiang Yu, Wanping Qian, Hongtao Zhang, Lijuan Jiao, Jiazhu Li, Minghua Liu, Erhong Hao|2023|Chem.Commun.|59|13986|doi:10.1039/D3CC04727J
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.cc2h5jw3
title: CCDC 2299235: Experimental Crystal Structure Determination

description: Related Article: A.A. Gaydamaka, S.V. Rashchenko, A.I. Semerikova, E.S. Smirnova, A.G. Ivanova, S.G. Arkhipov, B.A. Zakharov, N.E. Bogdanov, E.V. Boldyreva|2023|Acta Crystallogr.,Sect.B:Struct.Sci.,Cryst.Eng. and Mat.|79|495|doi:10.1107/S2052520623008740
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.cc2h5jx4
title: CCDC 2299236: Experimental Crystal Structure Determination

description: Related Article: A.A. Gaydamaka, S.V. Rashchenko, A.I. Semerikova, E.S. Smirnova, A.G. Ivanova, S.G. Arkhipov, B.A. Zakharov, N.E. Bogdanov, E.V. Boldyreva|2023|Acta Crystallogr.,Sect.B:Struct.Sci.,Cryst.Eng. and Mat.|79|495|doi:10.1107/S2052520623008740
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.cc2h5jy5
title: CCDC 2299237: Experimental Crystal Structure Determination

description: Related Article: A.A. Gaydamaka, S.V. Rashchenko, A.I. Semerikova, E.S. Smirnova, A.G. Ivanova, S.G. Arkhipov, B.A. Zakharov, N.E. Bogdanov, E.V. Boldyreva|2023|Acta Crystallogr.,Sect.B:Struct.Sci.,Cryst.Eng. and Mat.|79|495|doi:10.1107/S2052520623008740
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.cc2h5jz6
title: CCDC 2299238: Experimental Crystal Structure Determination

description: Related Article: A.A. Gaydamaka, S.V. Rashchenko, A.I. Semerikova, E.S. Smirnova, A.G. Ivanova, S.G. Arkhipov, B.A. Zakharov, N.E. Bogdanov, E.V. Boldyreva|2023|Acta Crystallogr.,Sect.B:Struct.Sci.,Cryst.Eng. and Mat.|79|495|doi:10.1107/S2052520623008740
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.cc2h5k08
title: CCDC 2299239: Experimental Crystal Structure Determination

description: Related Article: A.A. Gaydamaka, S.V. Rashchenko, A.I. Semerikova, E.S. Smirnova, A.G. Ivanova, S.G. Arkhipov, B.A. Zakharov, N.E. Bogdanov, E.V. Boldyreva|2023|Acta Crystallogr.,Sect.B:Struct.Sci.,Cryst.Eng. and Mat.|79|495|doi:10.1107/S2052520623008740
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.