cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.6084/m9.figshare.28685309
title: Supplementary Material for: Randomised Trial of Pharmacist Integration in Haemodialysis Teams: Effects on Phosphorus Control and Patient Outcomes

description: Background:
Despite the limited historical engagement of hospital pharmacists in managing blood phosphorus levels, their involvement in this aspect of care for hemodialysis patients remains an underexplored yet potentially promising and effective approach that warrants further investigation. 
Methods:
A prospective, randomized controlled clinical trial was conducted to compare a control group receiving standard care from doctors and nurses with a test group that, in addition to standard care, received medication education and health promotion interventions from pharmacists. This trial is registered at chictr.org.cn, ChiCTR2100044887 and is complete.
Results:
The test group demonstrated a significant reduction in blood phosphorus levels (P = 0.0056) and an improvement in blood calcium levels (P = 0.0238), whereas the control group showed no significant changes. The study also identified several potential high-risk factors for chronic kidney disease, including rural residence (72% of the patients), hypertension (84%), low educational attainment (84%), occupation as farmers or laborers (92%), and low to middle income levels (52%). Conversely, factors such as smoking, alcohol consumption, and marital status were not found to be significant risk factors. The impact of varying health promotion methodologies on biochemical indicators and blood pressure was minimal.
Conclusions:
The integration of pharmacists into the clinical team appeared to contribute to the reduction of blood phosphorus levels and healthcare expenditures, highlighting their pivotal role in the cost-effective, multidisciplinary management of hemodialysis patients. This finding underscores the significant economic and clinical importance of considering pharmacists as valuable members of the healthcare team in efforts to optimize patient outcomes.
DOI: 10.6084/m9.figshare.28749800
title: Supplementary Material for: Preoperatory Flot Regimen for Gastroesophageal Cancer and Renal Function: A New Onco-Nephrological Perspective.

description: (1) Background: The FLOT regimen, a combination of fluorouracil, leucovorin, oxaliplatin, and docetaxel, is a standard treatment for gastric and esophagogastric junction cancers, but concerns exist about its potential renal toxicity. The exact prevalence and severity of renal toxicity need to be well-documented, and this knowledge gap could impact the optimal use of the FLOT regimen in clinical practice. We aimed to evaluate the renal toxicity profile of the FLOT regimen with a specific focus on Acute Kidney Disease onset in a real-life setting and explore associated risk factors. (2) Methods: We conducted a multicenter retrospective study involving 96 patients treated with preoperatory FLOT. The incidence of acute kidney disease (AKD) and potential risk factors were identified. (3) Results: AKD occurred in three patients (incidence rate of 0.0122 cases/month of follow-up). Oral antidiabetic agents and prostate hypertrophy emerged as significant predictors of AKD. (4) Conclusion: Acute Kidney Disease is uncommon in patients treated with the preoperatory FLOT regimen. Our findings highlight the importance of diligent renal function monitoring and appropriate preventive strategies in patients undergoing FLOT treatment. These results encourage the conduction of further studies and clinical experiences in larger populations and patients with lower baseline eGFR.
DOI: 10.15482/usda.adc/27292860
title: Data from: A Comparative Life Cycle Assessment of Kraft-based and Hemp-based Polylactide (PLA) 3D Printed Part with Fused Filament Fabrication

description: [Note: Data file updated January 2025. In the sheet named KL PLA, "pure PLA" and "Hemp PLA" were changed to "Kraft lignin PLA."]<br>This study presents a comparative life cycle assessment (LCA) of hemp straw and kraft lignin as fillers for polylactic acid (PLA) 3D-printed tensile specimens to evaluate their relative environmental impacts. Both materials, as low-cost, renewable bio-based fillers, offer the potential to enhance the elongation properties of PLA, which is otherwise brittle, while reducing the overall environmental footprint of 3D-printed components. The analysis reveals that hemp straw performs slightly better than kraft lignin across most impact categories, making it a more favorable option for eco-conscious prosumers seeking sustainable filament alternatives. This research is motivated by the increasing demand for bio-based materials and the growth of the U.S. industrial hemp industry, alongside the broader trend of using sustainable filaments in additive manufacturing. The environmental impacts of hemp straw PLA and kraft lignin PLA were assessed using several life cycle impact assessment methods, including ReCiPe 2016 Endpoint (H), Cumulative Energy Demand (CED), and IPCC GWP100. The results show that kraft lignin PLA exhibited slightly higher environmental impacts, particularly in the Marine Eutrophication, Land Use, and Water Consumption categories. Pre-processing and filament production were the major process contributors to the overall environmental footprint. Sensitivity analysis confirmed that transportation distances of materials had minimal influence on the results. Overall, hemp straw PLA demonstrated marginally lower environmental impacts, suggesting it may be the more eco-friendly choice for 3D-printed tensile specimens. This study highlights the importance of further research to evaluate the impacts at larger production scales and in different application scenarios. Future work will explore the environmental performance of treated biomass for wider applications, including hemp fiber and hurd, as alternative fillers for 3D-printed components.
DOI: 10.15468/dl.a6qxtu
title: Occurrence Download

description: A dataset containing 181 species occurrences available in GBIF matching the query:
{
 "and" : [
 "Geometry POLYGON((-11.75934 44.10051,37.75934 44.10051,37.75934 63.89949,-11.75934 63.89949,-11.75934 44.10051))",
 "HasCoordinate is true",
 "HasGeospatialIssue is false",
 "OccurrenceStatus is Present",
 "TaxonKey is Rhagoletis batava Hering, 1958"
 ]
}

 The dataset includes 181 records from 10 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0015036-250402121839773/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.25574/csc2.stk.acisfj1454274p160546_001
title: Chandra X-ray Observatory Stack acisfJ1454274p160546_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1401431m113929_001
title: Chandra X-ray Observatory Stack acisfJ1401431m113929_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1450205p235449_001
title: Chandra X-ray Observatory Stack acisfJ1450205p235449_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1358365p372532_001
title: Chandra X-ray Observatory Stack acisfJ1358365p372532_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1350398p350211_001
title: Chandra X-ray Observatory Stack acisfJ1350398p350211_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1453331p311420_001
title: Chandra X-ray Observatory Stack acisfJ1453331p311420_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1349489p270439_001
title: Chandra X-ray Observatory Stack acisfJ1349489p270439_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1453317p215255_001
title: Chandra X-ray Observatory Stack acisfJ1453317p215255_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1432589p340232_001
title: Chandra X-ray Observatory Stack acisfJ1432589p340232_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1403267m060117_001
title: Chandra X-ray Observatory Stack acisfJ1403267m060117_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1449208p631625_001
title: Chandra X-ray Observatory Stack acisfJ1449208p631625_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1402479p491021_001
title: Chandra X-ray Observatory Stack acisfJ1402479p491021_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1504433p043536_001
title: Chandra X-ray Observatory Stack acisfJ1504433p043536_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1357164m093229_001
title: Chandra X-ray Observatory Stack acisfJ1357164m093229_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1450508p050653_001
title: Chandra X-ray Observatory Stack acisfJ1450508p050653_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1449080p090129_001
title: Chandra X-ray Observatory Stack acisfJ1449080p090129_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1359147p275844_001
title: Chandra X-ray Observatory Stack acisfJ1359147p275844_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1350515p261644_001
title: Chandra X-ray Observatory Stack acisfJ1350515p261644_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1406122p222752_001
title: Chandra X-ray Observatory Stack acisfJ1406122p222752_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1432586p323846_001
title: Chandra X-ray Observatory Stack acisfJ1432586p323846_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1458364p472702_001
title: Chandra X-ray Observatory Stack acisfJ1458364p472702_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1451480m151148_001
title: Chandra X-ray Observatory Stack acisfJ1451480m151148_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1353591p334600_001
title: Chandra X-ray Observatory Stack acisfJ1353591p334600_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1403389m335636_001
title: Chandra X-ray Observatory Stack acisfJ1403389m335636_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1505256p020558_001
title: Chandra X-ray Observatory Stack acisfJ1505256p020558_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1357445m395848_001
title: Chandra X-ray Observatory Stack acisfJ1357445m395848_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1458371m314155_001
title: Chandra X-ray Observatory Stack acisfJ1458371m314155_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1432586p330312_001
title: Chandra X-ray Observatory Stack acisfJ1432586p330312_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1501006p010032_001
title: Chandra X-ray Observatory Stack acisfJ1501006p010032_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1438265p034207_001
title: Chandra X-ray Observatory Stack acisfJ1438265p034207_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1440057m001743_001
title: Chandra X-ray Observatory Stack acisfJ1440057m001743_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1434190p344324_001
title: Chandra X-ray Observatory Stack acisfJ1434190p344324_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1403297p462749_001
title: Chandra X-ray Observatory Stack acisfJ1403297p462749_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1452122p430128_001
title: Chandra X-ray Observatory Stack acisfJ1452122p430128_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1452581p335149_001
title: Chandra X-ray Observatory Stack acisfJ1452581p335149_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1458248m002609_001
title: Chandra X-ray Observatory Stack acisfJ1458248m002609_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1500280p212316_001
title: Chandra X-ray Observatory Stack acisfJ1500280p212316_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1458568m313525_001
title: Chandra X-ray Observatory Stack acisfJ1458568m313525_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1402502p263106_001
title: Chandra X-ray Observatory Stack acisfJ1402502p263106_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1459101p714052_001
title: Chandra X-ray Observatory Stack acisfJ1459101p714052_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1408516p020555_001
title: Chandra X-ray Observatory Stack acisfJ1408516p020555_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1501069p225001_001
title: Chandra X-ray Observatory Stack acisfJ1501069p225001_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1455480p570512_001
title: Chandra X-ray Observatory Stack acisfJ1455480p570512_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1539477p431223_001
title: Chandra X-ray Observatory Stack acisfJ1539477p431223_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1354237m010223_001
title: Chandra X-ray Observatory Stack acisfJ1354237m010223_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1400178p010515_001
title: Chandra X-ray Observatory Stack acisfJ1400178p010515_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".