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79 results for “Sources information”
Data from: Gaps, an elusive source of phylogenetic information
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Supplementary information for: Deterministic assembly of arrays of lithographically defined WS_2 and MoS_2 monolayer features directly from multilayer sources into van der Waals heterostructures
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Evidence Based Information Provision to Improve Decision Making After Oesophagogastric Cancer Diagnosis (SOURCE)
ClinicalTrials.gov study NCT04232735. IPD Sharing: NO. Countries: 1. Publications: 0.
Netizens' Perception of COVID-19 Information & Information Sources.
ClinicalTrials.gov study NCT04497441. IPD Sharing: UNDECIDED. Countries: 1. Publications: 0.
The Influence of Information Sources on Knowledge and Anxiety in Inflammatory Bowel Disease Patients
ClinicalTrials.gov study NCT01916161. IPD Sharing: Not stated. Countries: 1. Publications: 0.
Information Sources in Pulmonary Hypertension
ClinicalTrials.gov study NCT07207525. IPD Sharing: UNDECIDED. Countries: 1. Publications: 0.
The amniotic fluid transcriptome: a source of novel information about human fetal development
GEO Series GSE33168. Homo sapiens. 12 samples. Type: Expression profiling by array.
APPENDIX Individuals included in the genetic and/or skull morphology analyses are presented with source and locality information (reference to sites in Fig. 1 are given in parentheses when available). Voucher numbers are provided for individuals that were collected: AMNH — American Museum of Natural History, New York, NY, USA, BMNH — Natural History Museum, London, UK, FMNH — Field Museum, Chicago, IL, USA, HZM — Harrison Zoological Museum, Kent, UK, MCZ — Museum of Comparative Zoology, Harvard, MA, USA, MZB — Muzeum Zoologicum Bogoriense, Bogor, Indonesia, RMNH — National Museum of Natural History Naturalis, Leiden, Netherlands, SEN — Senckenberg Museum, Frankfurt, Germany, TK — tissue collection and TTU — specimen numbers; Texas Tech. University, Lubbock, TX, USA, and USNM — Smithsonian Institute, Washington D.C., USA. All specimens from peninsular Malaysia with THK or MBCRU field numbers were collected by A. Zubaid, and the specimens or duplicate wing punches were deposited at UKM (Universiti Kebangsaan Malaysia, Bangi, Selangor, Malaysia). The original taxonomy of type specimens (type) are listed. Haplotypes (Hap) are given for individuals of H. bicolor (=H. bicolor-131) and H. kunzi (=H. bicolor-142). GenBank accession numbers are given for one representative of each unique haplotype in A new species in the Hipposideros bicolor group (Chiroptera: Hipposideridae) from Peninsular Malaysia
APPENDIX Individuals included in the genetic and/or skull morphology analyses are presented with source and locality information (reference to sites in Fig. 1 are given in parentheses when available). Voucher numbers are provided for individuals that were collected: AMNH — American Museum of Natural History, New York, NY, USA, BMNH — Natural History Museum, London, UK, FMNH — Field Museum, Chicago, IL, USA, HZM — Harrison Zoological Museum, Kent, UK, MCZ — Museum of Comparative Zoology, Harvard, MA, USA, MZB — Muzeum Zoologicum Bogoriense, Bogor, Indonesia, RMNH — National Museum of Natural History Naturalis, Leiden, Netherlands, SEN — Senckenberg Museum, Frankfurt, Germany, TK — tissue collection and TTU — specimen numbers; Texas Tech. University, Lubbock, TX, USA, and USNM — Smithsonian Institute, Washington D.C., USA. All specimens from peninsular Malaysia with THK or MBCRU field numbers were collected by A. Zubaid, and the specimens or duplicate wing punches were deposited at UKM (Universiti Kebangsaan Malaysia, Bangi, Selangor, Malaysia). The original taxonomy of type specimens (type) are listed. Haplotypes (Hap) are given for individuals of H. bicolor (=H. bicolor-131) and H. kunzi (=H. bicolor-142). GenBank accession numbers are given for one representative of each unique haplotype
California Drinking Water Source Assessment Program – UC Davis Information Center for the Environment
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2MASS 6X Merged Extended Source Information Table
During the final months of 2MASS observatory operations, a campaign of targeted "long exposure" observations was carried out during times when no previously unscanned parts of the sky were available for the main survey. These observations used the same freeze-frame scanning technique employed for the survey, but with READ2-READ1 exposures six times longer than was used for normal survey observations (hence they are referred to as "6x" observations). The 2MASS 6x measurements were intended to probe ~1 magnitude deeper than the main survey in unconfused regions.Approximately 590 deg2 of sky distributed in 30 targeted regions were scanned at least once using the long exposures. Most of this area is concentrated in two large, comprehensive surveys of the Large and Small Magellanic Clouds, 383 deg2 and 127 deg2, respectively. Twenty-eight additional smaller fields were mapped in the 6x mode from both observatories, covering targets that include the Pleiades open cluster, galactic star formation complexes, M31, nearby galaxy clusters and the Lockman Hole. The merged source tables contain the mean positions magnitudes and uncertainties for sources detected multiple times in each of the 2MASS data sets. The merging was carried out using an autocorrelation of the respective databases to identify groups of extractions that are positionally associated with each other, all lying within a 1.5" radius circular region. A number of confirmation statistics are also provided in the tables that can be used to test for source motion and/or variability, and the general quality of the merge.
2MASS 6X Merged Point Source Information Table
During the final months of 2MASS observatory operations, a campaign of targeted "long exposure" observations was carried out during times when no previously unscanned parts of the sky were available for the main survey. These observations used the same freeze-frame scanning technique employed for the survey, but with READ2-READ1 exposures six times longer than was used for normal survey observations (hence they are referred to as "6x" observations). The 2MASS 6x measurements were intended to probe ~1 magnitude deeper than the main survey in unconfused regions.Approximately 590 deg2 of sky distributed in 30 targeted regions were scanned at least once using the long exposures. Most of this area is concentrated in two large, comprehensive surveys of the Large and Small Magellanic Clouds, 383 deg2 and 127 deg2, respectively. Twenty-eight additional smaller fields were mapped in the 6x mode from both observatories, covering targets that include the Pleiades open cluster, galactic star formation complexes, M31, nearby galaxy clusters and the Lockman Hole. The merged source tables contain the mean positions magnitudes and uncertainties for sources detected multiple times in each of the 2MASS data sets. The merging was carried out using an autocorrelation of the respective databases to identify groups of extractions that are positionally associated with each other, all lying within a 1.5" radius circular region. A number of confirmation statistics are also provided in the tables that can be used to test for source motion and/or variability, and the general quality of the merge.
2MASS Calibration Merged Extended Source Information Table
Photometric calibration for 2MASS was performed using observations of calibration fields made at regular intervals during each night of survey operations. Measurements of standard stars in the fields were used to derive the photometric zero point offsets as a function of time during each night. Atmospheric extinction coefficients were derived from 2MASS observations made over long periods.2MASS calibration fields, or tiles, are 1° long in declination and approximately 8.5' wide in right ascension. There are 35 regular survey calibration fields distributed at approximately two hour intervals in right ascension near declinations of approximately -30°, 0° and +30°. An additional five calibration fields were defined in and around the Large and Small Magellanic Clouds to support the deep observation (6x) campaign towards the end of survey operations.Over the course of the survey, the regular calibration fields were scanned between 562 and 3692 times in nominally photometric conditions. Equatorial fields were observed from both observatories, so were observed more frequently than those near ±30° which were observed with only one telescope. The special Magellanic Cloud calibration fields were observed 108 to 468 times between November 2000 and February 2001.The following table contains brief descriptions of the entries in the Survey, 6x and Calibration Merged Point Source Information Tables. The merged source tables contain the mean positions magnitudes and uncertainties for sources detected multiple times in each of the 2MASS data sets. The merging was carried out using an autocorrelation of the respective databases to identify groups of extractions that are positionally associated with each other, all lying within a 1.5" radius circular region. A number of confirmation statistics are also provided in the tables that can be used to test for source motion and/or variability, and the general quality of the merge.
2MASS Survey Merged Extended Source Information Table
The merged source tables contain the mean positions magnitudes and uncertainties for sources detected multiple times in each of the 2MASS data sets. The merging was carried out using an autocorrelation of the respective databases to identify groups of extractions that are positionally associated with each other, all lying within a 1.5" radius circular region. A number of confirmation statistics are also provided in the tables that can be used to test for source motion and/or variability, and the general quality of the merge.
2MASS LMC/SMC Calibration Merged Point Source Information Table
Photometric calibration for 2MASS was performed using observations of calibration fields made at regular intervals during each night of survey operations. Measurements of standard stars in the fields were used to derive the photometric zero point offsets as a function of time during each night. Atmospheric extinction coefficients were derived from 2MASS observations made over long periods.2MASS calibration fields, or tiles, are 1° long in declination and approximately 8.5' wide in right ascension. There are 35 regular survey calibration fields distributed at approximately two hour intervals in right ascension near declinations of approximately -30°, 0° and +30°. An additional five calibration fields were defined in and around the Large and Small Magellanic Clouds to support the deep observation (6x) campaign towards the end of survey operations.Over the course of the survey, the regular calibration fields were scanned between 562 and 3692 times in nominally photometric conditions. Equatorial fields were observed from both observatories, so were observed more frequently than those near ±30° which were observed with only one telescope. The special Magellanic Cloud calibration fields were observed 108 to 468 times between November 2000 and February 2001.The following table contains brief descriptions of the entries in the Survey, 6x and Calibration Merged Point Source Information Tables. The merged source tables contain the mean positions magnitudes and uncertainties for sources detected multiple times in each of the 2MASS data sets. The merging was carried out using an autocorrelation of the respective databases to identify groups of extractions that are positionally associated with each other, all lying within a 1.5" radius circular region. A number of confirmation statistics are also provided in the tables that can be used to test for source motion and/or variability, and the general quality of the merge.
2MASS LMC/SMC Calibration Merged Extended Source Information Table
Photometric calibration for 2MASS was performed using observations of calibration fields made at regular intervals during each night of survey operations. Measurements of standard stars in the fields were used to derive the photometric zero point offsets as a function of time during each night. Atmospheric extinction coefficients were derived from 2MASS observations made over long periods.2MASS calibration fields, or tiles, are 1° long in declination and approximately 8.5' wide in right ascension. There are 35 regular survey calibration fields distributed at approximately two hour intervals in right ascension near declinations of approximately -30°, 0° and +30°. An additional five calibration fields were defined in and around the Large and Small Magellanic Clouds to support the deep observation (6x) campaign towards the end of survey operations.Over the course of the survey, the regular calibration fields were scanned between 562 and 3692 times in nominally photometric conditions. Equatorial fields were observed from both observatories, so were observed more frequently than those near ±30° which were observed with only one telescope. The special Magellanic Cloud calibration fields were observed 108 to 468 times between November 2000 and February 2001.The following table contains brief descriptions of the entries in the Survey, 6x and Calibration Merged Point Source Information Tables. The merged source tables contain the mean positions magnitudes and uncertainties for sources detected multiple times in each of the 2MASS data sets. The merging was carried out using an autocorrelation of the respective databases to identify groups of extractions that are positionally associated with each other, all lying within a 1.5" radius circular region. A number of confirmation statistics are also provided in the tables that can be used to test for source motion and/or variability, and the general quality of the merge.
2MASS Calibration Merged Point Source Information Table
Photometric calibration for 2MASS was performed using observations of calibration fields made at regular intervals during each night of survey operations. Measurements of standard stars in the fields were used to derive the photometric zero point offsets as a function of time during each night. Atmospheric extinction coefficients were derived from 2MASS observations made over long periods.2MASS calibration fields, or tiles, are 1° long in declination and approximately 8.5' wide in right ascension. There are 35 regular survey calibration fields distributed at approximately two hour intervals in right ascension near declinations of approximately -30°, 0° and +30°. An additional five calibration fields were defined in and around the Large and Small Magellanic Clouds to support the deep observation (6x) campaign towards the end of survey operations.Over the course of the survey, the regular calibration fields were scanned between 562 and 3692 times in nominally photometric conditions. Equatorial fields were observed from both observatories, so were observed more frequently than those near ±30° which were observed with only one telescope. The special Magellanic Cloud calibration fields were observed 108 to 468 times between November 2000 and February 2001.The following table contains brief descriptions of the entries in the Survey, 6x and Calibration Merged Point Source Information Tables. The merged source tables contain the mean positions magnitudes and uncertainties for sources detected multiple times in each of the 2MASS data sets. The merging was carried out using an autocorrelation of the respective databases to identify groups of extractions that are positionally associated with each other, all lying within a 1.5" radius circular region. A number of confirmation statistics are also provided in the tables that can be used to test for source motion and/or variability, and the general quality of the merge.
2MASS Survey Merged Point Source Information Table
The merged source tables contain the mean positions magnitudes and uncertainties for sources detected multiple times in each of the 2MASS data sets. The merging was carried out using an autocorrelation of the respective databases to identify groups of extractions that are positionally associated with each other, all lying within a 1.5" radius circular region. A number of confirmation statistics are also provided in the tables that can be used to test for source motion and/or variability, and the general quality of the merge.
DATASET - In search of an effective source use pattern for writing argumentative and informative synthesis texts
<p>This SPSS file contains the data corresponding to the study as published in the article <em>In search of an effective source use pattern for writing argumentative and informative synthesis texts </em>(Vandermeulen, Van den Broek, Van Steendam, & Rijlaarsdam, 2019). </p> <p> </p>
Source Data of Supplementary Information
<p>Supplementary Information Source Data of Photoluminescence Mechanism of Carbon Dots: Triggering High-colour-purity Red Fluorescence Emission through Edge Amino Protonation</p>
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Allen Brain Atlas
Allen Brain Atlas is an Allen Institute collection of brain map atlases, datasets, APIs, and analysis tools covering mouse, human, and non-human primate brain resources.
Annotated Behaviour and Observability Dataset (ABODe)
ABODe is a University of Edinburgh DataShare dataset for behavior classification in group-housed mice using home-cage video, identities, bounding boxes, ground-plate positions, and annotator labels.
DANDI Archive for NWB datasets
DANDI is a BRAIN Initiative archive for publishing and sharing neurophysiology data, including electrophysiology, optophysiology, and behavioral data packaged as NWB and related standards.
International Brain Laboratory public data
The International Brain Laboratory public data releases expose standardized mouse decision-making experiments, including Neuropixels recordings, widefield calcium imaging, behavior, and session metadata accessed through the ONE API.
OpenNeuro
OpenNeuro is a free, open platform for sharing neuroimaging datasets, with public search, dataset pages, and download paths for web, S3, DataLad, and the OpenNeuro CLI.