cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5517/ccdc.csd.cc2dftnb
title: CCDC 2217822: Experimental Crystal Structure Determination

description: Related Article: Rayan Chakraborty, Parikshit Kumar Rajput, Gokul M. Anilkumar, Shabnum Maqbool, Ranjan Das, Atikur Rahman, Pankaj Mandal, Angshuman Nag|2023|J.Am.Chem.Soc.|145|1378|doi:10.1021/jacs.2c12034
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.cc2dftpc
title: CCDC 2217823: Experimental Crystal Structure Determination

description: Related Article: Rayan Chakraborty, Parikshit Kumar Rajput, Gokul M. Anilkumar, Shabnum Maqbool, Ranjan Das, Atikur Rahman, Pankaj Mandal, Angshuman Nag|2023|J.Am.Chem.Soc.|145|1378|doi:10.1021/jacs.2c12034
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.cc2dftk7
title: CCDC 2217819: Experimental Crystal Structure Determination

description: Related Article: Rayan Chakraborty, Parikshit Kumar Rajput, Gokul M. Anilkumar, Shabnum Maqbool, Ranjan Das, Atikur Rahman, Pankaj Mandal, Angshuman Nag|2023|J.Am.Chem.Soc.|145|1378|doi:10.1021/jacs.2c12034
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: 10.7295/w9cil54880
title: CIL:54880, Homo sapiens, Induced pluripotent stem cell-derived human mesenchymal stem cells
DOI: 10.7295/w9cil54881
title: CIL:54881, Homo sapiens, Induced pluripotent stem cell-derived human mesenchymal stem cells
DOI: 10.7295/w9cil54882
title: CIL:54882, Homo sapiens, Induced pluripotent stem cell-derived human mesenchymal stem cells
DOI: 10.7295/w9cil54883
title: CIL:54883, Homo sapiens, Induced pluripotent stem cell-derived human mesenchymal stem cells
DOI: 10.7295/w9cil54884
title: CIL:54884, Homo sapiens, Induced pluripotent stem cell-derived human mesenchymal stem cells
DOI: 10.5281/zenodo.7549228
title: Roadmap to Reasoning in Microservice systems: A Rapid Review Dataset

description: It contains data retrieved from Scopus based on the following query: TITLE-ABS-KEY ( ( microservices OR microservice OR micro-service ) AND architecture AND ( ( reconstruction OR "Intermediate Representation" ) OR reasoning OR ( evolution AND changes ) ) AND ( technique OR solution OR model ) ) AND PUBYEAR &gt; 1959 AND PUBYEAR &lt; 2023 AND PUBYEAR &gt; 1959 AND PUBYEAR &lt; 2023 The filter process is applied by the authors to build a microservice systems reasoning roadmap.
DOI: 10.5281/zenodo.7549227
title: Roadmap to Reasoning in Microservice systems: A Rapid Review Dataset

description: It contains data retrieved from Scopus based on the following query: TITLE-ABS-KEY ( ( microservices OR microservice OR micro-service ) AND architecture AND ( ( reconstruction OR "Intermediate Representation" ) OR reasoning OR ( evolution AND changes ) ) AND ( technique OR solution OR model ) ) AND PUBYEAR &gt; 1959 AND PUBYEAR &lt; 2023 AND PUBYEAR &gt; 1959 AND PUBYEAR &lt; 2023 The filter process is applied by the authors to build a microservice systems reasoning roadmap.
DOI: 10.25919/r5fn-fn34
title: Parkes observations for project PX500 semester 2022OCTS_16

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: 10.6084/m9.figshare.21067703.v1
title: Mid-Devonian basaltic magmatism and associated sedimentation: the Ooloo Hill Formation, central-eastern South Australia

description: We report composition and age data from a restricted &lt;370 km<sup>2</sup>, volcano-sedimentary basin beneath Mesozoic cover to the northwest of the Flinders Ranges, South Australia. This volcano-sedimentary basin comprises two components: a sedimentary sequence that includes shales, siltstones and sandstones, and a basalt–sedimentary member. Together, these components are defined as the Ooloo Hill Formation. Whole-rock K–Ar geochronology for five basalt samples yields a preferred mean K–Ar age of 392 ± 8 Ma. Two samples of detrital zircons from the sedimentary rock yield SHRIMP U–Pb maximum depositional ages of <i>ca</i> 527 and 510 Ma. These ages are significant, as they rule out a Neoproterozoic age for the sedimentary basin and demonstrate that this basin is not part of the Adelaide Superbasin. Lower eruptive sequences are calc-alkaline and mafic in composition (SiO<sub>2</sub> = 46.1–47.8 wt%, Na<sub>2</sub>O + K<sub>2</sub>O = 3.7–6.1 wt%, MgO = 6.85–8.37 wt%, Mg# = 57–65 and ε<sub>Nd(390 Ma)</sub> = 3.4–4.0) and may represent two small-scale melting events from compositionally distinct mantle reservoirs. The uppermost eruptive sequence is tholeiitic andesite (SiO<sub>2</sub> = 51.6 wt%, Na<sub>2</sub>O + K<sub>2</sub>O = 8.1 wt%, MgO = 2.2 wt%, Mg# = 27 and ε<sub>Nd(390 Ma)</sub> = 3.0) and displays geochemical affinity to the first two eruptive sequences, possibly representing a differentiated magma from a similar source region. Incompatible trace-element ratios and isotopic compositions suggest the source was a heterogeneous oceanic island basalt-like parent magma derived from partial melting of the asthenospheric mantle. We envisage decompressional melting was linked to large-scale tectonic processes inboard of the Tasman Orogen, with magma ascent facilitated by crustal faulting.KEY POINTSFirst record of a mid-Devonian intracontinental volcano-sedimentary basin in South Australia.Basalts have an oceanic island basalt-like mantle source that represents at least two small-scale melting events from compositionally distinct mantle reservoirs.A localised mid-Devonian backarc basin or transpressional/transtensional basin linked to intracontinental faulting formed inboard of the Tasman Orogen. First record of a mid-Devonian intracontinental volcano-sedimentary basin in South Australia. Basalts have an oceanic island basalt-like mantle source that represents at least two small-scale melting events from compositionally distinct mantle reservoirs. A localised mid-Devonian backarc basin or transpressional/transtensional basin linked to intracontinental faulting formed inboard of the Tasman Orogen.
DOI: 10.6084/m9.figshare.21078614
title: Genesis of the Wilsons Promontory batholith of southeast Victoria, Australia: heterogeneities in the Proterozoic basement

description: The monzogranites and syenogranites of the Early Devonian (Emsian), post-tectonic, high-level, S-type Wilsons Promontory batholith contain magmatic garnet and cordierite, in addition to biotite, as well as biotite–quartz pseudomorphs after early orthopyroxene. The batholith forms the southern tip of the Australian mainland and consists of four penecontemporaneous plutons, emplaced at shallow crustal depth, intruding Ordovician to Lower Devonian lower greenschist-facies, quartz-rich metaflysch rocks in the Bassian tectonic zone. The magmas were initially H<sub>2</sub>O-undersaturated and at <i>T</i> &gt; 800 °C, having been generated by partial melting of greywacke-dominated, Paleoproterozoic to Mesoproterozoic (<i>ca</i> 1.6 Ga) basement rocks in the Selwyn Block (the northern tip of the VanDieland microcontinent). However, the specific source rocks differ from those of the S-type granitic plutons in the neighbouring Melbourne tectonic zone. This probably reflects compositional variations within the Selwyn Block, which has been proposed to form the basement terrane beneath both the Melbourne and Bassian zones. The compositional zonation in the batholith is due to sequential intrusion of separate magma batches rather than <i>in situ</i> differentiation, and the main mechanism responsible for primary chemical variations in the rocks appears to have been peritectic assemblage entrainment. Some local differentiation also occurred, probably by filter pressing, to produce aplites and tourmaline-bearing pegmatites. Normal granitic rocks (<i>i.e.</i> not aplites or pegmatites) with SiO<sub>2</sub> &gt;76 wt% were not produced through differentiation of other granitic magmas in the batholith. At the global scale, this suggests that fractionation models for the origins of high-silica granitic and rhyolitic magmas may need revision.KEY POINTSS-type magmas of the Wilsons Promontory batholith were H<sub>2</sub>O-undersaturated and at <i>T</i> &gt; 800 °C.They were generated by partial melting of greywacke-dominated, Paleoproterozoic to Mesoproterozoic (<i>ca</i> 1.6 Ga) basement.The sources differ from those of the plutons in the Melbourne Zone, suggesting heterogeneity in the Selwyn Block.Most compositional variation is due to intrusion of separate magma batches and peritectic assemblage entrainment, not differentiation. S-type magmas of the Wilsons Promontory batholith were H<sub>2</sub>O-undersaturated and at <i>T</i> &gt; 800 °C. They were generated by partial melting of greywacke-dominated, Paleoproterozoic to Mesoproterozoic (<i>ca</i> 1.6 Ga) basement. The sources differ from those of the plutons in the Melbourne Zone, suggesting heterogeneity in the Selwyn Block. Most compositional variation is due to intrusion of separate magma batches and peritectic assemblage entrainment, not differentiation.
DOI: 10.6084/m9.figshare.21078614.v1
title: Genesis of the Wilsons Promontory batholith of southeast Victoria, Australia: heterogeneities in the Proterozoic basement

description: The monzogranites and syenogranites of the Early Devonian (Emsian), post-tectonic, high-level, S-type Wilsons Promontory batholith contain magmatic garnet and cordierite, in addition to biotite, as well as biotite–quartz pseudomorphs after early orthopyroxene. The batholith forms the southern tip of the Australian mainland and consists of four penecontemporaneous plutons, emplaced at shallow crustal depth, intruding Ordovician to Lower Devonian lower greenschist-facies, quartz-rich metaflysch rocks in the Bassian tectonic zone. The magmas were initially H<sub>2</sub>O-undersaturated and at <i>T</i> &gt; 800 °C, having been generated by partial melting of greywacke-dominated, Paleoproterozoic to Mesoproterozoic (<i>ca</i> 1.6 Ga) basement rocks in the Selwyn Block (the northern tip of the VanDieland microcontinent). However, the specific source rocks differ from those of the S-type granitic plutons in the neighbouring Melbourne tectonic zone. This probably reflects compositional variations within the Selwyn Block, which has been proposed to form the basement terrane beneath both the Melbourne and Bassian zones. The compositional zonation in the batholith is due to sequential intrusion of separate magma batches rather than <i>in situ</i> differentiation, and the main mechanism responsible for primary chemical variations in the rocks appears to have been peritectic assemblage entrainment. Some local differentiation also occurred, probably by filter pressing, to produce aplites and tourmaline-bearing pegmatites. Normal granitic rocks (<i>i.e.</i> not aplites or pegmatites) with SiO<sub>2</sub> &gt;76 wt% were not produced through differentiation of other granitic magmas in the batholith. At the global scale, this suggests that fractionation models for the origins of high-silica granitic and rhyolitic magmas may need revision.KEY POINTSS-type magmas of the Wilsons Promontory batholith were H<sub>2</sub>O-undersaturated and at <i>T</i> &gt; 800 °C.They were generated by partial melting of greywacke-dominated, Paleoproterozoic to Mesoproterozoic (<i>ca</i> 1.6 Ga) basement.The sources differ from those of the plutons in the Melbourne Zone, suggesting heterogeneity in the Selwyn Block.Most compositional variation is due to intrusion of separate magma batches and peritectic assemblage entrainment, not differentiation. S-type magmas of the Wilsons Promontory batholith were H<sub>2</sub>O-undersaturated and at <i>T</i> &gt; 800 °C. They were generated by partial melting of greywacke-dominated, Paleoproterozoic to Mesoproterozoic (<i>ca</i> 1.6 Ga) basement. The sources differ from those of the plutons in the Melbourne Zone, suggesting heterogeneity in the Selwyn Block. Most compositional variation is due to intrusion of separate magma batches and peritectic assemblage entrainment, not differentiation.
DOI: 10.6084/m9.figshare.20648375
title: Dating initial crystallisation of some Devonian plutons in central Victoria and geological implications

description: Rather than being inherited as detrital grains, many of the rounded and/or embayed cores in zircon crystals from granitic rocks are probably antecrysts, formed early in the magmatic systems. Using laser-ablation, sector-field ICP-MS, we obtained internally consistent weighted-mean concordia ages of 375.3 ± 2.5 Ma and 376.9 ± 2.6 for early crystallisation of two samples from the previously undated Mount Disappointment pluton in the Melbourne Zone. Within uncertainty, our date of 376.4 ± 2.4 Ma for the Baringhup pluton of the Harcourt batholith is the same as the published and our new date for the Mount Alexander pluton, in the same batholith. Using the same techniques, we produced an improved date of 370.9 ± 6.5 Ma for the I-type Ercildoun Granite in the neighbouring Bendigo Zone of the Lachlan Fold Belt. We also obtained dates that confirm published ages for the Mount Bute Granite in the Stawell Zone, the Tynong pluton of the Tynong batholith in the Melbourne Zone and the Oberon pluton of the Wilsons Promontory batholith in the Bassian Zone. These dates confirm the Late Devonian (Fransian) age of most of this widespread plutonism, as well as the reported Emsian age of the Wilsons Promontory batholith. However, part of what has been mapped as the Mount Wombat pluton of the Strathbogie batholith could be significantly older than the rest. Many rounded or embayed cores in zircon crystals are antecrysts rather than inherited detrital grains. The Mount Disappointment pluton is confirmed as Late Devonian in age, at 375.2 ± 2.5 Ma. At 378.2 ± 2.0 Ma, the Baringhup pluton of the Harcourt batholith is the same age as the Mount Alexander pluton, in the same batholith. Part of the Mount Wombat pluton in the Strathbogie batholith may be older than the rest of the pluton.
DOI: 10.6084/m9.figshare.20648375.v1
title: Dating initial crystallisation of some Devonian plutons in central Victoria and geological implications

description: Rather than being inherited as detrital grains, many of the rounded and/or embayed cores in zircon crystals from granitic rocks are probably antecrysts, formed early in the magmatic systems. Using laser-ablation, sector-field ICP-MS, we obtained internally consistent weighted-mean concordia ages of 375.3 ± 2.5 Ma and 376.9 ± 2.6 for early crystallisation of two samples from the previously undated Mount Disappointment pluton in the Melbourne Zone. Within uncertainty, our date of 376.4 ± 2.4 Ma for the Baringhup pluton of the Harcourt batholith is the same as the published and our new date for the Mount Alexander pluton, in the same batholith. Using the same techniques, we produced an improved date of 370.9 ± 6.5 Ma for the I-type Ercildoun Granite in the neighbouring Bendigo Zone of the Lachlan Fold Belt. We also obtained dates that confirm published ages for the Mount Bute Granite in the Stawell Zone, the Tynong pluton of the Tynong batholith in the Melbourne Zone and the Oberon pluton of the Wilsons Promontory batholith in the Bassian Zone. These dates confirm the Late Devonian (Fransian) age of most of this widespread plutonism, as well as the reported Emsian age of the Wilsons Promontory batholith. However, part of what has been mapped as the Mount Wombat pluton of the Strathbogie batholith could be significantly older than the rest. Many rounded or embayed cores in zircon crystals are antecrysts rather than inherited detrital grains. The Mount Disappointment pluton is confirmed as Late Devonian in age, at 375.2 ± 2.5 Ma. At 378.2 ± 2.0 Ma, the Baringhup pluton of the Harcourt batholith is the same age as the Mount Alexander pluton, in the same batholith. Part of the Mount Wombat pluton in the Strathbogie batholith may be older than the rest of the pluton.
DOI: 10.6084/m9.figshare.21067703
title: Mid-Devonian basaltic magmatism and associated sedimentation: the Ooloo Hill Formation, central-eastern South Australia

description: We report composition and age data from a restricted &lt;370 km<sup>2</sup>, volcano-sedimentary basin beneath Mesozoic cover to the northwest of the Flinders Ranges, South Australia. This volcano-sedimentary basin comprises two components: a sedimentary sequence that includes shales, siltstones and sandstones, and a basalt–sedimentary member. Together, these components are defined as the Ooloo Hill Formation. Whole-rock K–Ar geochronology for five basalt samples yields a preferred mean K–Ar age of 392 ± 8 Ma. Two samples of detrital zircons from the sedimentary rock yield SHRIMP U–Pb maximum depositional ages of <i>ca</i> 527 and 510 Ma. These ages are significant, as they rule out a Neoproterozoic age for the sedimentary basin and demonstrate that this basin is not part of the Adelaide Superbasin. Lower eruptive sequences are calc-alkaline and mafic in composition (SiO<sub>2</sub> = 46.1–47.8 wt%, Na<sub>2</sub>O + K<sub>2</sub>O = 3.7–6.1 wt%, MgO = 6.85–8.37 wt%, Mg# = 57–65 and ε<sub>Nd(390 Ma)</sub> = 3.4–4.0) and may represent two small-scale melting events from compositionally distinct mantle reservoirs. The uppermost eruptive sequence is tholeiitic andesite (SiO<sub>2</sub> = 51.6 wt%, Na<sub>2</sub>O + K<sub>2</sub>O = 8.1 wt%, MgO = 2.2 wt%, Mg# = 27 and ε<sub>Nd(390 Ma)</sub> = 3.0) and displays geochemical affinity to the first two eruptive sequences, possibly representing a differentiated magma from a similar source region. Incompatible trace-element ratios and isotopic compositions suggest the source was a heterogeneous oceanic island basalt-like parent magma derived from partial melting of the asthenospheric mantle. We envisage decompressional melting was linked to large-scale tectonic processes inboard of the Tasman Orogen, with magma ascent facilitated by crustal faulting.KEY POINTSFirst record of a mid-Devonian intracontinental volcano-sedimentary basin in South Australia.Basalts have an oceanic island basalt-like mantle source that represents at least two small-scale melting events from compositionally distinct mantle reservoirs.A localised mid-Devonian backarc basin or transpressional/transtensional basin linked to intracontinental faulting formed inboard of the Tasman Orogen. First record of a mid-Devonian intracontinental volcano-sedimentary basin in South Australia. Basalts have an oceanic island basalt-like mantle source that represents at least two small-scale melting events from compositionally distinct mantle reservoirs. A localised mid-Devonian backarc basin or transpressional/transtensional basin linked to intracontinental faulting formed inboard of the Tasman Orogen.
DOI: 10.6084/m9.figshare.20506826
title: The early–middle Silurian Delite monzogranite and quartz syenite, East Kunlun Orogenic Belt, NW China: petrogenesis and implications for tectonic evolution of the Proto‑Tethys

description: The tectonic evolution of the Proto‑Tethys in the East Kunlun Orogenic Belt (EKOB) is controversial. Herein, new petrological, whole-rock geochemical, zircon U–Pb geochronological and zircon Lu–Hf isotopic data for early Paleozoic intrusive rocks in the Delite region are reported. LA-ICP-MS zircon U–Pb isotopic data show that the Delite monzogranite and quartz syenite were formed at 437.0 ± 2.9 Ma and 424.8 ± 2.2 Ma, respectively. The Delite monzogranite contains high SiO<sub>2</sub>, Al<sub>2</sub>O<sub>3</sub> and K<sub>2</sub>O and A/CNK ratios, but low MgO and Mg# values (33–38). This study considers that the monzogranite is a typical S-type granite and originated from partial melting of ancient crustal clastic material (metagreywacke) in a syn-collision setting. The quartz syenite is K-rich and Mg-poor, with low Mg# values (36–41), exhibiting geochemical signatures of an alkalic syenite derived from partial melting of basaltic lower crust in a post-collision setting. Combining with the previous work, we suggest that in the middle part of the EKOB the Proto-Tethys closed at <i>ca</i> 437 Ma with a post-collisional setting after <i>ca</i> 427 Ma. KEY POINTSZircons LA-ICP-MS U–Pb isotopic data indicate that the Delite monzogranite and quartz syenite were formed at 437.0 ± 2.9 Ma and 424.8 ± 2.2 Ma, respectively.The Delite monzogranite was formed in a syn-collision setting. The Delite quartz syenite was related to the post-collision setting.It is suggested that the Proto-Tethys closed at <i>ca</i> 437 Ma in the middle part of the EKOB, and the post-collisional setting was after <i>ca</i> 427 Ma in the EKOB. Zircons LA-ICP-MS U–Pb isotopic data indicate that the Delite monzogranite and quartz syenite were formed at 437.0 ± 2.9 Ma and 424.8 ± 2.2 Ma, respectively. The Delite monzogranite was formed in a syn-collision setting. The Delite quartz syenite was related to the post-collision setting. It is suggested that the Proto-Tethys closed at <i>ca</i> 437 Ma in the middle part of the EKOB, and the post-collisional setting was after <i>ca</i> 427 Ma in the EKOB.