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3 results for “K Dwarfs”

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zenodo36/100

GCM simulations of Earth-like M- and K-dwarf planets

<p>Simulations are described in papers:</p> <ul> <li> <div>Lobo, A. H., Shields, A. L., Palubski, I. Z., &amp; Wolf, E. (2023). <strong>Terminator Habitability: The Case for Limited Water Availability on M-dwarf Planets</strong>. <em>The Astrophysical Journal</em>, <em>945</em>(2), 161. https://doi.org/10.3847/1538-4357/aca970</div> </li> <li>Lobo, A. H., Shields, A. L., (in press, 2024). <strong>Climate Regimes Across the Habitable Zone: a Comparison of Synchronous Rocky M- and K-dwarf Planets</strong>. <em>The Astrophysical Journal.&nbsp;</em></li> </ul> <p>&nbsp;</p>

opencc-by-4.0Aug 2024View details →
zenodo24/100

From solar to stellar flare characteristics. On a new peak size distribution for G-, K-, and M-dwarf star flares

<p>This dataset contains additional material for the research paper &quot;From solar to stellar flare characteristics. On a new peak size distribution for G-, K-, and M-dwarf star flares&quot;, Astron. Astrophys., 2018.</p> <p>Based on the flare list available at http://156.17.94.1/sphinx_l1_catalogue/SphinX_cat_main.html, here peak X-ray flare intensities of&nbsp; Q- to C-class flares measured by the SphinX instrument (see, e.g., Kotov, 2011; Sylvester et al., 2011, 2012; Gburek et al., 2011a,b, 2013; Gryciuk et al., 2017) during the solar minimum of <strong>2009</strong> and their corresponding GOES E &gt; 10 MeV peak proton fluxes are given.</p> <p><br> Column 1: Month<br> Column 2: Day<br> Column 3: X-ray flux peak hour<br> Column 4: X-ray flux peak minute<br> Column 5: X-ray flare peak intensity (W/m<sup>2</sup>)<br> Column 5: GOES E &gt; 10 MeV peak proton flux (pfu)<br> Column 6: Flare location (according to the SphinX-database)</p>

opencc-by-4.0Nov 2018View details →
nasa20/100

ROSAT All-Sky Survey: A-K Dwarfs/Subgiants

This catalog presents X-ray data for all the main-sequence and subgiant stars of spectral types A, F, G, and K and luminosity classes IV and V listed in the Bright Star Catalogue (also known as the HR Catalogue) that have been detected as X-ray sources in the ROSAT All-Sky Survey (RASS). A number of stars in the appropriate spectral type range that do not have assigned luminosity classes have also been included. The catalogue contains 980 such HR stars detected as X-ray sources out of a total of 3054 stars in the HR Catalogue that satisfy the selection criteris, implying an average detection rate of 32%. In addition to the measured ROSAT PSPC count rates, source detection parameters, hardness ratios, and X-ray fluxes, X-ray luminosities derived from Hipparcos parallaxes are also listed. This database was created at the HEASARC in February 1999 based on the ADC/&lt;a href="https://cdsarc.cds.unistra.fr/ftp/cats/J/A+AS/132/155"&gt;CDS Catalog J/A+AS/132/155&lt;/a&gt;. This is a service provided by NASA HEASARC .

restrictednotspecifiedApr 2025View details →

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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.

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Last verified 2026-04-29Open record

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