cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.17632/mdtv54yy4n.1
title: Carbon emission data during the construction stage of ultra-high-rise office buildings (taking a ultra-high-rise office building in Guangzhou, China as an example)

description: The following research data are mainly used to support the current submitted paper: “Calculation and Analysis of Actual Carbon Emissions during the Building Construction Stage—An Example of Ultra-high-rise Office Building in Guangzhou, China.”
The relevant original data comes from the China Construction Fourth Engineering Division Co., Ltd. Science and Innovation Building project. This project is located in Guangzhou, Guangdong Province, China. The data records the carbon emissions of the Science and Innovation Building project during the construction phase. The data records the project’s carbon emissions from multiple perspectives, including carbon emissions from the production and transportation of building materials, carbon emissions from machinery used on the construction site, carbon emissions generated by related energy consumption during the construction process, and carbon reduction measures used in the project. In addition, relevant calculations are performed on the original data to facilitate research on carbon emissions from ultra-high-rise buildings.
The database mainly stores a total of 6 Excel documents containing the original data and calculated data mentioned above. And they have been categorized and named according to the categories.
DOI: 10.17632/thwpmt3px7.1
title: Structural Damage Detection Dataset: Dynamic Response of Coupled Substructures

description: This dataset contains dynamic response measurements for Structural Health Monitoring (SHM), focusing on the detection and identification of damage in assembly products. The data is derived from experiments involving two substructures (A and B) that can be dynamically coupled to form an assembly for which the damage is expected to occur in the joints connecting the substructures. The coupling configuration is illustrated in the attached image (Image.jpg). In addition to substructure measurements, the dataset includes measurements from four differently damaged assemblies:

- undamaged assembly,
- assembly with a 5 mm cut at location J_1,
- assembly with a 10 mm cut at location J_1, and
- assembly with a 10 mm cut at location J_2.

Locations J_1 and J_2 are shown in Image.jpg.

The data is stored in the data.h5 file and organized as follows:

- The main group is named 'data'.
 + Within 'data', there are six subgroups:
 * Groups 'A' and 'B' contain measurements for substructures A and B, respectively.
 * Four groups for the differently damaged assemblies ('assembly_undamaged', 'assembly_J1_1_4', 'assembly_J1_1_2', and 'assembly_J2_1_2').

 + Each subgroup contains measurements of impact force (in Newtons) and response in terms of acceleration (in units of standard gravity), organized as follows:

 * Groups are named 'r_e', where the number following 'r' denotes the response degree of freedom ID, and the number following 'e' indicates the excitation force application degree of freedom ID.
 * Each group contains two subgroups, 'response_data' and 'excitation_data', which hold the acceleration and force measurements, respectively.
 * 'response_data' and 'excitation_data' include up to four subgroups named numerically ('1', '2', etc.), representing repeated measurements, allowing for data averaging.

Details regarding the locations and directions of the excitation force application, the locations of the response measurements, and measurement units are stored as attributes of the 'response_data' and 'excitation_data' groups. Both, locations and directions for structures A and B are valid for the coordinate systems, displayed in Image_2.jpg. The coordinate system of the assembly coincides with the coordinate system of the substructure A in its first occurrence (on the left side of the assembly in Image.jpg). Attributes describing the damage state of each assembly group are stored within the respective assembly groups (i.e. groups 'assembly_undamaged', 'assembly_J1_1_4', 'assembly_J1_1_2', and 'assembly_J2_1_2').

Acquisition setup: each acceleration/force measurement was performed within 1s of sampling time with a sampling rate of 51.2 kS/s.

This dataset is valuable for researchers and practitioners in SHM, providing comprehensive data for developing and testing algorithms aimed at detecting structural damage based on the dynamic properties of the structure.
DOI: 10.15468/dl.24mdsf
title: Occurrence Download

description: A dataset containing 0 species occurrences available in GBIF matching the query:
{
 "Geometry" : [
 "POLYGON ((148.459334 -32.905979, 148.459334 -32.91047, 148.46158 -32.91047, 148.46158 -32.905979, 148.459334 -32.905979))"
 ]
}

 The dataset includes 0 records from 0 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0056800-240626123714530/datasets/export for details.
DOI: 10.17632/bdyyxdxf5b.1
title: Study of nasal heating function based on 40 cases of nasal cavity model

description: The heating condition of 40 nasal cavity models and their geometric parameters were analyzed and grouped
DOI: 10.17632/wsdxcgv8w3.1
title: NCHA Bioink characterisation

description: Data pertaining to characterisation of nanocellulose-hyaluronic acid bioinks
DOI: 10.15468/dl.qzratf
title: Occurrence Download

description: A dataset listing the 1703 species recorded in GBIF matching the query:
{
 "and" : [
 "GadmGid is BRA.25_1",
 "OccurrenceStatus is Present",
 "TaxonKey is Aves"
 ]
}

 The dataset's 1703 records were derived from 63 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0056789-240626123714530/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.15468/dl.3gve4p
title: Occurrence Download

description: A dataset containing 798048 species occurrences available in GBIF matching the query:
{
 "TaxonKey" : [
 "is Aquila chrysaetos (Linnaeus, 1758)"
 ]
}

 The dataset includes 798048 records from 788 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0056773-240626123714530/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.acisfj0914056p375313_001
title: Chandra X-ray Observatory Stack acisfJ0914056p375313_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.acisfj0958132p690240_001
title: Chandra X-ray Observatory Stack acisfJ0958132p690240_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.acisfj1046076m594306_001
title: Chandra X-ray Observatory Stack acisfJ1046076m594306_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.acisfj0912029p532023_001
title: Chandra X-ray Observatory Stack acisfJ0912029p532023_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.acisfj0914039p400616_001
title: Chandra X-ray Observatory Stack acisfJ0914039p400616_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.acisfj0955290p694334_001
title: Chandra X-ray Observatory Stack acisfJ0955290p694334_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.acisfj0958172m110546_001
title: Chandra X-ray Observatory Stack acisfJ0958172m110546_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.acisfj1045179p590438_001
title: Chandra X-ray Observatory Stack acisfJ1045179p590438_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.acisfj1000169m301516_001
title: Chandra X-ray Observatory Stack acisfJ1000169m301516_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.acisfj0958165p183912_001
title: Chandra X-ray Observatory Stack acisfJ0958165p183912_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.acisfj0916455p524009_001
title: Chandra X-ray Observatory Stack acisfJ0916455p524009_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.acisfj0914362p561257_001
title: Chandra X-ray Observatory Stack acisfJ0914362p561257_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.acisfj0957451p330857_002
title: Chandra X-ray Observatory Stack acisfJ0957451p330857_002

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.acisfj0958113p022636_001
title: Chandra X-ray Observatory Stack acisfJ0958113p022636_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.acisfj1001109p023517_001
title: Chandra X-ray Observatory Stack acisfJ1001109p023517_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.acisfj0918083m120446_001
title: Chandra X-ray Observatory Stack acisfJ0918083m120446_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.acisfj0958433p073956_001
title: Chandra X-ray Observatory Stack acisfJ0958433p073956_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.acisfj1046560p631245_001
title: Chandra X-ray Observatory Stack acisfJ1046560p631245_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.acisfj0918486p513058_001
title: Chandra X-ray Observatory Stack acisfJ0918486p513058_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.acisfj0959477p344919_001
title: Chandra X-ray Observatory Stack acisfJ0959477p344919_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.acisfj0957301p690253_001
title: Chandra X-ray Observatory Stack acisfJ0957301p690253_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.acisfj1000408p021313_001
title: Chandra X-ray Observatory Stack acisfJ1000408p021313_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.acisfj1000261p441047_001
title: Chandra X-ray Observatory Stack acisfJ1000261p441047_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.acisfj0958281p024145_001
title: Chandra X-ray Observatory Stack acisfJ0958281p024145_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.acisfj0958301m265519_001
title: Chandra X-ray Observatory Stack acisfJ0958301m265519_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.acisfj0958113p014325_001
title: Chandra X-ray Observatory Stack acisfJ0958113p014325_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.acisfj0959598p020826_001
title: Chandra X-ray Observatory Stack acisfJ0959598p020826_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.acisfj1023366p633525_001
title: Chandra X-ray Observatory Stack acisfJ1023366p633525_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.acisfj0918256p063723_001
title: Chandra X-ray Observatory Stack acisfJ0918256p063723_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.acisfj1001513p014945_001
title: Chandra X-ray Observatory Stack acisfJ1001513p014945_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.acisfj0917043p513635_001
title: Chandra X-ray Observatory Stack acisfJ0917043p513635_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.acisfj1023535m574549_001
title: Chandra X-ray Observatory Stack acisfJ1023535m574549_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.acisfj0959071p015528_001
title: Chandra X-ray Observatory Stack acisfJ0959071p015528_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.acisfj0959288p014527_001
title: Chandra X-ray Observatory Stack acisfJ0959288p014527_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.acisfj1028389p450028_001
title: Chandra X-ray Observatory Stack acisfJ1028389p450028_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.acisfj1024310p470907_001
title: Chandra X-ray Observatory Stack acisfJ1024310p470907_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.acisfj0958408p282754_001
title: Chandra X-ray Observatory Stack acisfJ0958408p282754_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.acisfj0959106p022125_001
title: Chandra X-ray Observatory Stack acisfJ0959106p022125_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.acisfj1000299p020542_001
title: Chandra X-ray Observatory Stack acisfJ1000299p020542_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.acisfj1003009p021722_001
title: Chandra X-ray Observatory Stack acisfJ1003009p021722_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.acisfj1049182p564042_001
title: Chandra X-ray Observatory Stack acisfJ1049182p564042_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.acisfj1000217p022329_001
title: Chandra X-ray Observatory Stack acisfJ1000217p022329_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.acisfj0918234m810001_001
title: Chandra X-ray Observatory Stack acisfJ0918234m810001_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.acisfj0959407p021841_001
title: Chandra X-ray Observatory Stack acisfJ0959407p021841_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.acisfj1024472m183826_001
title: Chandra X-ray Observatory Stack acisfJ1024472m183826_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.acisfj0958434p014024_001
title: Chandra X-ray Observatory Stack acisfJ0958434p014024_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".