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Dataset results
19 results for “IOTA”
Supporting Data for Martian Dynamo Change at ~4.1 Ga: Evidence from the Magnetic Measurements of the Iota Crater
<p><a href="https://zenodo.org/api/records/14257490/draft/files/MAG_MAVEN_NIGHTTIME.txt/content" target="_blank" rel="noopener noreferrer">MAG_MAVEN_NIGHTTIME.txt</a> contains magnetic field from MAVEN nighttime tracks across the study area;</p> <p><a href="https://zenodo.org/uploads/14257490" target="_blank" rel="noopener noreferrer">TOPOGRAPHY_CRUST_AB.txt </a> contains the topography and crustal thickness data in Figure 2;</p> <p><a href="https://zenodo.org/api/records/14257490/draft/files/MAGNETIC_MODEL_CALCULATION.csv/content" target="_blank" rel="noopener noreferrer">MAGNETIC_MODEL_CALCULATION.csv</a> contains the <span>normalized circumferential averaged magnetic field upon the impact crater with different diameters and internal magnetizations, which are calculated randomly one hundred times in each case.</span></p>
MESA inlists for 'Revisiting the Red Giant Branch Hosts KOI-3886 and $\iota$ Draconis. Detailed Asteroseismic Modeling and Consolidated Stellar Parameters' by Campante et al.
<p>MESA inlists used in preparation of the paper 'Revisiting the Red Giant Branch Hosts KOI-3886 and $\iota$ Draconis. Detailed Asteroseismic Modeling and Consolidated Stellar Parameters' by Campante et al. Two folders are provided in the .zip file:</p> <ul> <li>TL_Pipeline — inlists (MESA release version 12115) used to build the grid of stellar models used in Sect. 4.1 of the paper.</li> <li>JO_Pipeline — inlists (MESA release version 12778) used to build both grids of stellar models used in Sect. 4.2 of the paper.</li> </ul>
Interactive Obesity Treatment Approach for Obesity Prevention in Adults With Early Serious Mental Illness: iOTA-SMI
ClinicalTrials.gov study NCT03980743. IPD Sharing: NO. Countries: 1. Publications: 1.
Iota-Carrageenan Nasal Spray in Common Cold
ClinicalTrials.gov study NCT01944631. IPD Sharing: Not stated. Countries: 1. Publications: 1.
Prophylaxis Covid-19 in Healthcare Agents by Intensive Treatment With Ivermectin and Iota-carrageenan
ClinicalTrials.gov study NCT04701710. IPD Sharing: NO. Countries: 1. Publications: 1.
IOTA Versus Pattern Recognition Method in Diagnosis of Ovarian Masses
ClinicalTrials.gov study NCT02800031. IPD Sharing: UNDECIDED. Countries: 1. Publications: 1.
Study to Investigate if Sucking a Coldamaris Lozenge Elutes Sufficient Iota-carrageenan to Inactivate Usual Common Cold Viruses
ClinicalTrials.gov study NCT04533906. IPD Sharing: UNDECIDED. Countries: 1. Publications: 1.
Interactive Obesity Treatment Approach (iOTA) for Obesity Prevention in Serious Mental Illness
ClinicalTrials.gov study NCT03695289. IPD Sharing: UNDECIDED. Countries: 1. Publications: 6.
Prospective Validation of the ADNEX Model for Discrimination Between Benign and Malignant Adnexal Masses in Pregnancy: International Ovarian Tumour Analysis in Pregnancy Study (p-IOTA)
ClinicalTrials.gov study NCT05974618. IPD Sharing: NO. Countries: 1. Publications: 47.
International Ovarian Tumour Analysis (IOTA) Phase 5
ClinicalTrials.gov study NCT01698632. IPD Sharing: Not stated. Countries: 1. Publications: 4.
Efficacy of a Nasal Spray Containing Iota-Carrageenan in the Prophylaxis of COVID-19 Disease in Health Personnel Dedicated to Patients Care With COVID-19 Disease
ClinicalTrials.gov study NCT04521322. IPD Sharing: Not stated. Countries: 1. Publications: 1.
Value of MRI in the Characterization of Ovarian Masses Unable to Classify With Ultrasound Using the International Ovarian Tumor Analysis (IOTA) Simple Rules
ClinicalTrials.gov study NCT02836275. IPD Sharing: Not stated. Countries: 1. Publications: 11.
IOTA LR2
Open the record for dataset details and reuse information.
Trophectoderm specific function of Atypical Protein Kinase C iota (PKCi) is essential for post-implantation mammalian development.
GEO Series GSE100285. Mus musculus. 2 samples. Type: Expression profiling by high throughput sequencing.
Prospective RegIstration Of the peRformance of the IoTa ADNEX Model in Dutch gYnaecological Practice
ClinicalTrials.gov study NCT06103916. IPD Sharing: UNDECIDED. Countries: 1. Publications: 0.
IOTA Ultrasound Criteria and Serum CA 125 for Ovarian Malignancy Detection
ClinicalTrials.gov study NCT06977334. IPD Sharing: Not stated. Countries: 1. Publications: 0.
Efficacy and Safety of Iota-Carrageenan Eye Drops (NCX-4240)
ClinicalTrials.gov study NCT03009799. IPD Sharing: UNDECIDED. Countries: 1. Publications: 0.
Masses in Young Patients - International Ovarian Tumour Analysis (MY-IOTA)
ClinicalTrials.gov study NCT06693596. IPD Sharing: Not stated. Countries: 1. Publications: 0.
Lynds 1641 and iota Ori Region XMM-Newton X-Ray Point Source Catalog
This table contains results from an XMM-Newton and Spitzer survey of the part of the Orion A cloud south of the Orion Nebula, the 'Survey of Orion A with XMM-Newton and Spitzer (SOXS)'. The goal of SOXS is to detect the relatively bright X-ray sources in the Orion A cloud and complete the census of more evolved YSOs in this region. These stars represent a sample of cloud members chosen with minimal a priori bias toward their IR properties. This XMM-Newton survey includes the Lynds 1641 (L1641) dark cloud, a region of the Orion A cloud with very few massive stars and hence a relatively low ambient UV flux, and the region around the O9 III star iota Orionis. In addition to proprietary data, the authors used archival XMM data of the Orion Nebula Cluster (ONC) to extend their analysis to a major fraction of the Orion A cloud. They have detected 1060 X-ray sources with more than 4.5-sigma significance in L1641 and the iota Ori region. About 94% of the sources have Two Micron All Sky Survey (2MASS) and Spitzer counterparts, 204 and 23 being Class II and Class I or protostar objects, respectively. In addition, the authors have identified 489 X-ray sources as counterparts to Class III candidates, given they are bright in X-rays and appear as normal photospheres at mid-IR wavelengths. The remaining 205 X-ray sources are likely distant active galactic nuclei (AGN) or other galactic sources not related to Orion A. The authors find that Class III candidates appear more concentrated in two main clusters in L1641. The first cluster of Class III stars is found toward the northern part of L1641, concentrated around iota Ori. The stars in this cluster are more evolved than those in the Orion Nebula. The authors estimate a distance of 300-320 pc for this cluster showing that it is in the foreground of the Orion A cloud. Another cluster rich in Class III stars is located in L1641 South and appears to be a slightly older cluster embedded in the Orion A cloud. Furthermore, other evolved Class III stars are found north of the ONC toward NGC 1977. The SOXS survey is composed of seven specifically proposed ~ 50 ks XMM-Newton fields, south of the ONC, to which the authors added four archival fields in the same region. The archival fields are centered on iota Orionis, V380 Ori, and V883 Ori, respectively (see Fig. 1 and Table 1 of the reference paper for more details of the X-ray observations). This HEASARC table contains the contents of Table 2 (1060 X-ray detected sources in the fields S1 - S10 listed in Table 1 of the reference paper), Table 3 (best-fit spectral parameters for the 232 brightest of these X-ray sources) and Table 4 (list of 1041 IR counterparts to the X-ray sources) from the reference paper. Some X-ray sources have no identified counterparts (16 of them in fact lie outside of the FOV of the Spitzer observations), most have a single counterpart, and a small number have 2 or even 3 IR counterparts within the 5 arcseconds matching radius used. For X-ray sources with more than 1 IR counterpart, we have added entries for the additional counterparts (71 in total), repeating the X-ray information in such cases. Thus, this HEASARC table contains 1131 (1060 + 71) entries corresponding to the 1060 X-ray source detections. To make its contents easier to visualize, the HEASARC has added a a parameter ir_match which lists the counterpart number for the entry: If there is no identified IR counterpart, ir_match is set to 0, for the first listed IR counterpart to 1, for the second and third, to 2 and 3, respectively. Thus, if the user wants to reduce the table back to a pure list of X-ray sources and their primary IR counterparts, they should search the table selecting ir_match < 2. This table was created by the HEASARC in August 2013 based on the electronic versions of Tables 2 and 3 from the original reference paper (2013ApJ...768...99P) and Table 4 from the erratum (2013ApJ...773...80P), which were all obtained from the ApJ web site. This is a service provided by NASA HEASARC .
ScienceDex guides
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Allen Brain Atlas
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International Brain Laboratory public data
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OpenNeuro
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