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datasets available to search
ShareScore release 0.9.0
Dataset results
75 results for “Neptune”
Tubulointerstitium RNAseq Voom Transformed Transcriptome from the Neptune Cohort
GEO Series GSE219185. Homo sapiens. 220 samples. Type: Expression profiling by high throughput sequencing.
The Influence of Stellar Contamination on the Interpretation of Near-Infrared Transmission Spectra of Sub-Neptune Worlds around M-Dwarfs
<p>Supplementary Figures displaying posterior probability distributions of all simulation scenarios discussed in <em><strong>The Influence of Stellar Contamination on the Interpretation of Near-Infrared Transmission Spectra of Sub-Neptune Worlds around M-dwarfs. </strong></em></p> <p>Arxiv link to the paper: https://arxiv.org/abs/1912.04389</p> <p>The directory structure is as follows: </p> <p>1) 30ppm_JWST_NIRISS_BIAS: Cases with varying levels of stellar contamination and varying planetary atmospheric scenarios (clear/cloudy/high-metallicity) over the JWST NIRISS-like bandpass with 30ppm spectro-photometric precision. Here we show that there is a bias incurred in the retrieval results when fitting with a model not accounting for the stellar contamination correction.</p> <p>2) 30ppm_JWST_NIRCAM_BIAS: Case of 14% spot and 63% faculae over the JWST-NIRCam like bandpass with 30ppm precision for a cloudy atmosphere planet.</p> <p>3) JWST_NIRISS_VARY_PRECISION: Cases with varying levels of stellar contamination for a high-metallicity+cloudy planetary atmosphere exploring different JWST precisions from 15-120ppm. Here we show that the bias incurred when retrieving with the uncorrected atmosphere model persists over our grid of JWST sensitivities with increasing levels of stellar contamination. However, this bias is not noteworthy for spot-covering fractions below 1%. </p> <p>4) 30ppm_JWST_NIRISS_NO_IMPROVEMENT_WITH_JOINT_RETRIEVAL_OF_STELLAR_SPECTRUM: Case of 12% spot covering fraction with a high-metallicity+cloudy planetary atmosphere (with 30ppm precision over NIRISS-like bandpass) shows no improvement in the precision of planetary temperature, metallicity, and carbon-to-oxygen ratio despite acquiring improved constraints on the stellar contamination parameters directly from the disk-integrated spectrum of the star. </p> <p>5) 30ppm_JWST_NIRISS_STELLAR_MODEL_DIFF_BIAS: Case of 12% spot covering fraction with a high-metallicity+cloudy planetary atmosphere (with 30ppm precision on the NIRISS-like bandpass range) incorporating "realistic" stellar contamination with a different stellar model. Here we show that there is a bias that arises in the retrievals due to generational stellar model differences (also mimicking stellar model-data differences in our example case) despite including the correction for stellar contamination. Our work suggests that planetary parameter retrievals, despite correcting for stellar contamination are heavily dependent on an accurate characterization of the stellar photosphere. </p> <p>*** In addition to the supplementary figures in the above mentioned directories, you can also access a high-resolution version of Figure 10 from the paper, accompanied by the full retrieval corner plot illustrating bias induced due to stellar model differences. </p> <p>*These figures have made use of the pygtc plotting routine for displaying posterior probability distribution corner plots (Bocquet et al, (2016), pygtc: beautiful parameter covariance plots (aka. Giant Triangle Confusograms), Journal of Open Source Software, 1(6), 46, doi:10.21105/joss.00046)</p>
Data sets for "Fluid-like elastic response of superionic NH3 in Uranus and Neptune" by Kimura and Murakami
<p>This is the source data of Brillouin spectra shown in Fig. 1 for the article "Fluid-like elastic response of superionic NH3 in Uranus and Neptune" by Kimura and Murakami.</p>
FIGURE 2 in NSB (Neptune Sandbox Berlin): An expanded and improved database of marine planktonic microfossil data and deep-sea stratigraphy
FIGURE 2. Current architecture of the NSB database.
FIGURE 11 in NSB (Neptune Sandbox Berlin): An expanded and improved database of marine planktonic microfossil data and deep-sea stratigraphy
FIGURE 11. Age model selection in NSB_ADP_wx.
Safety and Efficacy of Peripheral, Cobalt-chromium Sirolimus Eluting Stent (PERS) Versus Cobalt-chromium Stent (Neptune C)
ClinicalTrials.gov study NCT04323033. IPD Sharing: NO. Countries: 1. Publications: 0.
Natural History, Epidemiology and Pathogenesis of Severe HPV-Related Diseases (Neptune)
ClinicalTrials.gov study NCT05026138. IPD Sharing: Not stated. Countries: 1. Publications: 0.
Neptune Krill Oil (NKO™) in Early Stage Alzheimer's Disease (MNEMOSYNE)
ClinicalTrials.gov study NCT00867828. IPD Sharing: Not stated. Countries: 1. Publications: 0.
Brain Stimulation for Improving Cognition in Chronic Stroke (NEPTUNE)
ClinicalTrials.gov study NCT04655963. IPD Sharing: NO. Countries: 1. Publications: 0.
Integrative genomics identifies novel associations with APOL1 risk genotype in African American NEPTUNE subjects [glomerulus]
GEO Series GSE68125. Homo sapiens. 44 samples. Type: Expression profiling by array.
Tubulointerstitial transcriptome data in the Neptune Cohort
GEO Series GSE133288. Homo sapiens. 244 samples. Type: Expression profiling by array.
Integrative genomics identifies novel associations with APOL1 risk genotype in African American NEPTUNE subjects
GEO Series GSE68127. Homo sapiens. 99 samples. Type: Expression profiling by array.
Programm des SC Neptun
<u>Source</u>: Europeana <br><u>4DCity URL</u>: <a href="https://4dcity.org/imgupload/1652096302.8843.jpg">https://4dcity.org/imgupload/1652096302.8843.jpg</a> <br><u>Original Image URL</u>: <a href="https://api.europeana.eu/thumbnail/v2/url.json?uri=https%3A%2F%2Fwww.stadtmuseum.leipzig.de%2FDE-MUS-853418%2Fmedien%2FwmMedium%3DSM006857&type=IMAGE">https://api.europeana.eu/thumbnail/v2/url.json?uri=https%3A%2F%2Fwww.stadtmuseum.leipzig.de%2FDE-MUS-853418%2Fmedien%2FwmMedium%3DSM006857&type=IMAGE</a> <br><br><u>Image-Metadata:</u><br>Filename: 1652096302.8843.jpg<br>Image Dimensions: 220x350<br>Megapixels: 0.08 MP<br>Filesize: 27.73 KB<br>
Walking to Neptune
<u>Source</u>: Flickr <br><u>4DCity URL</u>: <a href="https://4dcity.org/imgupload/1677512389.7033.jpg">https://4dcity.org/imgupload/1677512389.7033.jpg</a> <br><u>Original Image URL</u>: <a href="https://live.staticflickr.com/65535/50775944841_bfbbaf183c_m.jpg">https://live.staticflickr.com/65535/50775944841_bfbbaf183c_m.jpg</a>
Dyrham Park - Statue of Neptune
Source: Objaverse 1.0 / Sketchfab
Combination of ETV, TQ-A3334 and TQ-B2450 for CHB (Neptune Study)
ClinicalTrials.gov study NCT04202653. IPD Sharing: Not stated. Countries: 0. Publications: 0.
VG2 LECP 3.2 MINUTE NEPTUNE FAR ENCOUNTER STEP DATA
This far encounter step data set consists of the counting rate and flux data for electrons and ions from the Low Energy Charged Particle (LECP) experiment on Voyager 2 while the spacecraft was within the vicinity of Neptune. This instrument measures the intensities of in-situ charged particles ( >13 keV electrons and >24 keV ions) with various levels of discrimination based on energy range and mass species. A subset of almost 100 LECP channels are included in this data set. The LECP data are globally calibrated to the extent possible. Particles include electrons, protons, alpha particles, and light, medium, and heavy nuclei particles. The far encounter data are 3.2 minute rate and flux measurements within 1/8 of the LECP instrumental motor rotation period (the angular scanning periods, or step period).
VG2 LECP 0.4S HIGH RESOLUTION NEPTUNE FAR ENCOUNTER DATA
This far encounter data set consists of electron and ion counting rate data from the Low Energy Charged Particle (LECP) experiment on Voyager 2 while the spacecraft was within the vicinity of Neptune. This instrument measures the intensities of in-situ charged particles ( >13 keV electrons and >24 keV ions) with various levels of discrimination based on energy range and mass species. A subset of almost 100 LECP channels are included in this data set. The LECP data are globally calibrated to the extent possible. Particles include electrons, protons, alpha particles, and light, medium, and heavy nuclei particles. The far encounter data are 0.4 second rate measurements within 1/8 of the LECP instrumental motor rotation period (the angular scanning periods, or step period).
VG2 LECP 12.8 MINUTE NEPTUNE FAR ENCOUNTER STEP DATA
This far encounter step data set consists of the counting rate and flux data for electrons and ions from the Low Energy Charged Particle (LECP) experiment on Voyager 2 while the spacecraft was within the vicinity of Neptune. This instrument measures the intensities of in-situ charged particles ( >13 keV electrons and >24 keV ions) with various levels of discrimination based on energy range and mass species. A subset of almost 100 LECP channels are included in this data set. The LECP data are globally calibrated to the extent possible. During Neptune far encounter, the entire LEPT (Low Energy Particle Telescope) and part of the LEMPA (Low Energy Magnetospheric Particle Analyzer) subsystems were turned on for data collection. Particles include electrons, protons, alpha particles, and light, medium, and heavy nuclei particles. The far encounter data are 12.8 minute rate and flux measurements within 1/8 of the LECP instrumental motor rotation period (the angular scanning periods, or step period).
VG2 LECP 12.8 MINUTE NEPTUNE FAR ENCOUNTER STEP DATA
This far encounter step data set consists of the counting rate and flux data for electrons and ions from the Low Energy Charged Particle (LECP) experiment on Voyager 2 while the spacecraft was within the vicinity of Neptune. This instrument measures the intensities of in-situ charged particles ( >13 keV electrons and >24 keV ions) with various levels of discrimination based on energy range and mass species. A subset of almost 100 LECP channels are included in this data set. The LECP data are globally calibrated to the extent possible. During Neptune far encounter, the entire LEPT (Low Energy Particle Telescope) and part of the LEMPA (Low Energy Magnetospheric Particle Analyzer) subsystems were turned on for data collection. Particles include electrons, protons, alpha particles, and light, medium, and heavy nuclei particles. The far encounter data are 12.8 minute rate and flux measurements within 1/8 of the LECP instrumental motor rotation period (the angular scanning periods, or step period).
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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.