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6 results for “Dwarf Novae”

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zenodo40/100

Reproduction package for the paper "Near-ultraviolet detections of four dwarf nova candidates in the globular cluster 47 Tucanae"

<p>This is a basic reproduction package for the paper &quot;Near-ultraviolet detections of four dwarf nova candidates in the globular cluster 47 Tucanae&quot; by <a href="https://www.aanda.org/articles/aa/abs/2020/02/aa37043-19/aa37043-19.html">Modiano et al. (2020)</a>. It aims to provide the most important data products to check and reproduce the main results of the paper.</p>

opencc-by-4.0Mar 2020View details →
zenodo40/100

Gravity modes on rapidly rotating accreting white dwarfs and their variation after dwarf novae

<p>MESA (r10398) inlist files and Gyre (5.2) files used in preparation of the paper &quot;Gravity modes on rapidly rotating accreting white dwarfs and their variation after dwarf novae&quot;. More details for specific files are given in README.txt.&nbsp;</p>

opencc-by-4.0Apr 2023View details →
zenodo36/100

Datasets for article "Transient behavior of three SU UMa-type dwarf novae; AR Pic, QW Ser and V521 Peg"

<p>Datasets for the article &quot;Transient behavior of three SU UMa-type dwarf novae; AR Pic, QW Ser and V521 Peg&quot;</p> <p>&nbsp;</p>

opencc-by-4.0Apr 2022View details →
zenodo36/100

Hydrogen Burning on Accreting White Dwarfs: Stability, Recurrent Novae, and the Post-nova Supersoft Phase

<p>MESA inlists associated with&nbsp;<a href="https://ui.adsabs.harvard.edu/?#abs/2013ApJ...777..136W">Hydrogen Burning on Accreting White Dwarfs: Stability, Recurrent Novae, and the Post-nova Supersoft Phase</a></p>

opencc-by-4.0Mar 2019View details →
zenodo32/100

Unveiling the nature of two dwarf novae: CRTS J080846.2+313106 and V416 Dra

<p>The observed spectra of two dwarf novae, CRTS J080846.2+313106 and V416 Dra, have been uploaded.&nbsp;</p>

opencc-by-4.0Jul 2024View details →
nasa20/100

Outburst Catalog of Dwarf Novae-type and Other Cataclysmic Variables

This outburst catalog contains a wide variety of observational properties for 722 dwarf nova-type (DN) cataclysmic variables (CVs) and 309 CVs of other types from the Catalina Real-time Transient Survey (CRTS). In particular, it includes the apparent outburst and quiescent V-band magnitudes, duty cycles, limits on the recurrence time, upper- and lower-limits on the distance and absolute quiescent magnitudes, color information, orbital parameters, and X-ray counterparts. These properties were determined by means of a classification script presented in the reference paper. The DNs in the catalog show a correlation between the outburst duty cycle and the orbital period (and outburst recurrence time), as well as between the quiescent absolute magnitude and the orbital period (and duty cycle). This is the largest sample of dwarf nova properties collected to date (2016). Besides serving as a useful reference for individual systems and a means of selecting objects for targeted studies, it will prove valuable for statistical studies that aim to shed light on the formation and evolution of cataclysmic variables. The CRTS identifies transients in the data from the Catalina Sky Survey (Larson et al. 1998, BAAS, 30, 1037; 2003, BAAS, 35, 982), a photometric survey that searches for Potentially Hazardous Asteroids and Near Earth Objects. Three sub-surveys constitute the Catalina Sky Survey, namely the original CSS (Catalina Schmidt Survey), the MLS (Mt Lemmon Survey) based in Arizona, and the SSS (Siding Spring Survey) in Australia, which ended on 2014 July 5. The field of view and typical limiting magnitude for each survey (at ~30 s integrations) are 8.2 degrees and V~19.5 mag for the CSS, 1.1 degrees and V~21.5 mag for the MLS, and 4 degrees and V~19 mag for the SSS. Together, these surveys cover 30, 000 deg&lt;sup&gt;2&lt;/sup&gt; between -70 and +70 degrees Declination (see Drake et al. 2014, MNRAS, 441, 1186 for more details). The entire zone within 15 Degrees of the Galactic Plane is avoided due to overcrowding, as are the Magellanic Clouds. The properties of the cataclysmic variables in this catalog are derived from the long-term optical light curves from the CRTS, as well as magnitudes, fluxes and orbital parameters from the SDSS, 2MASS, UKIDSS, ROSAT, Chandra, XMM and WISE catalogs, and from the Catalog of Cataclysmic Binaries, Low-Mass X-Ray Binaries and Related Objects (RKCat: Ritter and Kolb 2003, A&amp;A, 404, 301, available at the HEASARC as the RITTERCV, RITTERLMXB and RITTERRBIN tables). This table was created by the HEASARC in October 2017 based on the &lt;a href="https://cdsarc.cds.unistra.fr/ftp/cats/J/MNRAS/456/4441"&gt;CDS catalog J/MNRAS/456/4441&lt;/a&gt; file catalog.dat. . This is a service provided by NASA HEASARC .

restrictednotspecifiedApr 2025View details →

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electrophysiologyopenPublished Dandiset metadata and archive endpoints are available through the production DANDI API.
Last verified 2026-04-30Open record

International Brain Laboratory public data

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ibl
behavioral-neuroscienceopenPublic sessions can be searched and loaded from the IBL public data server through ONE.
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neuroscienceopenPublished datasets are available on demand over the internet.
Last verified 2026-04-29Open record