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1,477 results for “Cometes”
Hello Comet, shall we dance?, by Robert Barsa, Slovakia
<p>Third place in the 2021 IAU OAE Astrophotography Contest, category Comets.</p> <p>This beautiful and poetic image taken from Slovakia in July 2020 captures the comet C/2020 F3 (Neowise). The direction of the tails of the comet provides a clue as to the position of the Sun. In the past, the appearance of a comet in the skies could be accompanied by apprehension and even fear from those who did not know what these objects really are. Through careful observations and the applications of knowledge from physics, chemistry and geology, we now understand that comets are objects left over from the earliest days when the Solar System formed. The most distinctive features of a comet are the bluish ion (gas) tail, and whitish dust tail, which can extend for tens of millions of kilometres. These distinctive features, easily observable with the unaided eye together with an understanding of the science, are no longer cause for fear, rather they help us understand the history of our Solar System, and bring awe, joy and contemplation, as portrayed in this image.</p> <p>Credit: Robert Barsa/IAU OAE</p>
Spectroscopic identification of water emission from a main-belt comet: Supporting data and code
<p>Reduced data, source files, and code used in the analysis of JWST spectroscopy of comet 238P/Read, by Kelley et al. (2023, Nature 619, 720. 10.1038/s41586-023-06152-y).</p>
Comparative Outcomes Management With Electronic Data Technology (COMET) Study
ClinicalTrials.gov study NCT01461473. IPD Sharing: NO. Countries: 1. Publications: 2.
Study Evaluating the Safety and Efficacy of AR-15512 (COMET-3)
ClinicalTrials.gov study NCT05360966. IPD Sharing: NO. Countries: 1. Publications: 1.
COMET Example Directory
<p>The current directory includes example files needed for running the COMET package in R. The example dataset provided in this directory is from publicly available data from Cook et al (2020). If you would like to test our framework on your own dataset please format your input data in a similar fashion as the files in this directory. <br><br>Reference:<br>Cook, D. P., & Vanderhyden, B. C. (2020). Context specificity of the EMT transcriptional response. <i>Nature communications</i>, <i>11</i>(1), 2142.</p>
FIGURAS 53-56 in Novas Espécies De Cometes Audinet- Serville, 1828 (Coleoptera, Cerambycidae)
FIGURAS 53-56: Vista dorsal: 53, Cometes tumidicollis (Villiers, 1958), holótipo ♂; 54, C. flavipennis Buquet, 1851, holótipo; 55, C. peruvianus (Villiers, 1958), holótipo (?); 56, C. violaceicollis (Villiers, 1958), holótipo (?).
FIGURAS 46-52 in Novas Espécies De Cometes Audinet- Serville, 1828 (Coleoptera, Cerambycidae)
FIGURAS 46-52: Metafêmur: 46, Cometes solangeae sp. nov., parátipo ♀; 47, C. rileyi sp. nov., holótipo ♂; 48, C. zikani Melzer, 1926, paralectótipo ♀; 49, C. melzeri Santos-Silva & Martins, 2004, holótipo ♀; 50, C. monnei sp. nov., holótipo ♂; 51, idem, parátipo ♀; 52, C. acutipennis Buquet, 1851, ♂. Barra = 1,0 mm.
FIGURAS 13-18 in Novas Espécies De Cometes Audinet- Serville, 1828 (Coleoptera, Cerambycidae)
FIGURAS 13-18: Vista dorsal: 13, Cometes thomasi sp. nov., parátipo ♀, 10,6 mm; 14, C. turnbowi sp. nov., holótipo ♀, 9,0 mm; 15, C. hovorei sp. nov., holótipo ♂, 10,6 mm; 16, C. flavoviridis (Villiers, 1958), holótipo (?); 17, C. acutipennis Buquet, 1851, holótipo; 18, C. laetificus Bates, 1870, holótipo ♂.
FIGURAS 19-24 in Novas Espécies De Cometes Audinet- Serville, 1828 (Coleoptera, Cerambycidae)
FIGURAS 19-24: Cabeça e pronoto: 19, Cometes mariahelenae sp. nov., holótipo ♂; 20, C. solangeae sp. nov., parátipo ♀; 21, C. thomasi sp. nov., parátipo ♀; 22, C. hovorei sp. nov., holótipo ♂; 23, C. laetificus Bates, 1870, ♀; 24, C. rileyi sp. nov., holótipo ♂. Barra = 1,0 mm.
FIGURAS 7-12 in Novas Espécies De Cometes Audinet- Serville, 1828 (Coleoptera, Cerambycidae)
FIGURAS 7-12: Vista dorsal: 7, Cometes morrisi sp. nov., holótipo ♂, 8,7 mm; 8, idem, ♀ (espécime não incluído como tipo), 8,4 mm; 9, C. nearnsi sp. nov., parátipo ♂, 12,9 mm; 10, C. solangeae sp. nov., parátipo ♀, 12,0 mm; 11, C. rileyi sp. nov., holótipo ♂, 11,1 mm; 12, C. solisi sp. nov., parátipo ♀, 8,4 mm.
FIGURAS 25-35 in Novas Espécies De Cometes Audinet- Serville, 1828 (Coleoptera, Cerambycidae)
FIGURAS 25-35: Escapo: 25, Cometes monnei sp. nov., holótipo ♂; 26, idem, parátipo ♀; 27, C. zikani Melzer, 1926, paralectótipo ♀; 28, C. melzeri Santos-Silva & Martins, 2004, holótipo ♀; 29, C. hovorei sp. nov., holótipo ♂; 30, C. thomasi sp. nov., holótipo ♂; 31, idem, parátipo ♀; 32, C. laetificus Bates, 1870, ♀; 33, C. mariahelenae sp. nov., holótipo ♂; 34, idem, parátipo ♀; 35, C. solangeae sp. nov., parátipo ♀. Barra = 1,0 mm.
FIGURAS 1-6 in Novas Espécies De Cometes Audinet- Serville, 1828 (Coleoptera, Cerambycidae)
FIGURAS 1-6: 1, Cometes giesberti sp. nov., parátipo ♀, cabeça e pronoto. Vista dorsal: 2, C. giesberti sp. nov., holótipo ♀, 11,1 mm; 3, C. lingafelteri sp. nov., holótipo ♀, vista dorsal, 10,3 mm.; 4, C. mariahelenae sp. nov., holótipo ♂, 9,5 mm; 5, C. marcelae sp. nov., holótipo ♂, 8,5 mm; 6, C. monnei sp. nov., holótipo ♂, 10,0 mm.
FIGURAS 36-45 in Novas Espécies De Cometes Audinet- Serville, 1828 (Coleoptera, Cerambycidae)
FIGURAS 36-45: Élitro: 36, Cometes monnei sp. nov., holótipo ♂; 37, C. zikani Melzer, 1926, paralectótipo ♀; 38, C. melzeri Santos-Silva & Martins, 2004, holótipo ♀; 39, C. solisi sp. nov., parátipo ♀; 40, C. festivus Bates, 1885, ♀; 41, C. turnbowi sp. nov., holótipo ♀. Ápíce eli- tral: 42, C. marcelae sp. nov., holótipo ♂; 43, C. spinipennis (Villiers, 1958), ♀; 44, C. solisi sp. nov., parátipo ♀; 45, C. festivus Bates, 1885, ♀. Barra = 0,5 mm.
Comet fading begins beyond Saturn
<p>The discovery probability of long-period comets (LPCs) passing near the Sun is highest during their first passage and then declines, or fades, during subsequent return passages. Comet fading is largely attributed to devolatilization and fragmentation via thermal processing within 2-3 AU of the Sun (1 AU being the Earth-Sun distance). Here our numerical simulations show that comet observing campaigns miss vast numbers of LPCs making returning passages through the Saturn region (near 10 AU) because these comets fade during prior, even more distant passages exterior to Saturn and thus elude detection. Consequently, comet properties significantly evolve at solar distances much larger than previously considered, and this offers new insights into the physical and dynamical properties of LPCs, both near and far from Earth.</p>
replication_Comet
<p>This is the replication package for the paper titled "Generalized Mutant Schemata with Closed Maps Metaprograms"</p>
EM27/SUN network data CoMet 2018 Poland Silesia
<p>EM27/SUN network data sampled during the CoMet 2018 measurement campaign in the upper Silesian coal basin in Poland.</p> <p>The data set contains the raw interferograms recorded for all four sites. </p>
Other common names: East African Grammomys, Rwenzori Grammomys, Rwenzori Thicket Rat Taxonomy. Thamnomys ibeanus Osgood, 1910, Molo, Kenya. Grammomys ibeanus was previously includ-ed in G. cometes, but molecular data show it to be closer to G. macmillani. Monotypic. Distribution. Occurs quite widely in E Africa associated with mountains of the Rift Valley system and the Eastern Arc, including S South Sudan, E Uganda, Kenya, Tanzania, Malawi, and Mozambique. in Muridae
Other common names: East African Grammomys, Rwenzori Grammomys, Rwenzori Thicket Rat Taxonomy. Thamnomys ibeanus Osgood, 1910, Molo, Kenya. Grammomys ibeanus was previously includ-ed in G. cometes, but molecular data show it to be closer to G. macmillani. Monotypic. Distribution. Occurs quite widely in E Africa associated with mountains of the Rift Valley system and the Eastern Arc, including S South Sudan, E Uganda, Kenya, Tanzania, Malawi, and Mozambique.
Silver Comet - Training 02 - Stolt3D
Crew Training 02 of the Stolt3D expedition - our second model, this time of the Silver Comet training wreck at Dutch Springs! * Photographers: Mike & Larry * Safety: Chuck & Bill * Instructor: Christopher * Support: Olga & Meredith This model focuses on alignment target integration, mesh-hole-filling, depth filtering (to eliminate specular noise from particulates), and fine-tuning our swim patterns & team dynamics. (The *next* model posted here will use chunking/alignment-merges to integrate data from multiple divers & different cameras for a single site, and will also have the stern deck geometry fixed.) Source: * ~530 images (Mike) * ~300 images (Larry) Mezzanine: * 25MM polygon * 16k tex Hardware used to process this model: * 24x Xeon, 2.67 GHz * 192 GB DDR3 ECC RAM (68 GB used) * 2TB block storage (38 GB used) * RTX 3070 GPU * RTX 2070 Super GPU For more updates, toolchain, and (soon) Stolt Dagali results, check out our project at **[scuba.tech/stolt3d](https://www.scuba.tech/stolt3d)**! Source: Objaverse 1.0 / Sketchfab
FIGURAS 21-26 in Variação do colorido elitral, nova espécie e novos registros em Cometes Audinet-Serville, 1828 (Coleoptera, Cerambycidae, Disteniinae)
FIGURAS 21-26: Vista dorsal: 21, C. quadrimaculatus (Villiers, 1958), ♂, 8,3 mm; 22, C. spinipennis (Villiers, 1958), ♀, 9,7 mm; 23, C. eximius Bates, 1872, ♂, 10,0 mm; 24, C. festivus Bates, 1885, ♀, 14,0 mm; 25, C. birai sp. nov., holótipo ♀, 15,4 mm; 26, C. birai sp. nov. (fêmea não incluída como tipo).
FIGURAS 15-19 in Variação do colorido elitral, nova espécie e novos registros em Cometes Audinet-Serville, 1828 (Coleoptera, Cerambycidae, Disteniinae)
FIGURAS 15-19: Cometes birai sp. nov., holótipo ♀: 15, escapo; 18, ápice elitral; 19, metafêmur. C. acutipennis Buquet, 1851, ♂: 16, escapo; 17, ápice elitral. Barra = 1 mm.
ScienceDex guides
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These curated guides explain access requirements, typical timelines, costs, and reuse considerations for widely used research datasets.
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.