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<!DOCTYPE html PUBLIC "-//W3C//DTD XHTML 1.1 Strict//EN" "http://www.w3.org/TR/xhtml1/DTD/xhtml1-strict.dtd">
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<title>SPEX - Downloadable light curves</title>
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<h1><a href="index.html">DOWNLOADABLE LIGHT CURVES</a></h1>
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<p class="slogan">MTA CSFK Lendület Near-Field Cosmology Research Group</p>
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<li><a href="index.html">About Lendület</a></li>
<li><a href="TESS_en.html">About TESS</a></li>
<li><a href="kepler_en.html">About Kepler</a></li>
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<li><a class="current" href="data_en.html">Downloadable light curves</a>
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<li><a href="#KeplerBLRRL">Kepler Blazhko RR Lyrae</a></li>
<li><a href="#KeplernonBLRRL">Kepler non-Blazhko RR Lyrae</a></li>
<li><a href="#K2RRL">K2-E2 RR Lyrae</a></li>
<li><a href="#K2LEO">K2 LEO IV RR Lyrae</a></li>
<li><a href="#CoRoT">CoRoT RR Lyrae</a></li>
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<a name="KeplerBLRRL"><h2>Kepler Blazhko RR Lyrae light curves</h2></a>
<p>These 4-year long, detrended, cleaned, 'final' light curves were made from the
Kepler observations using tailor-made apertures to retain as much flux as possible. All of them belong to
Blazhko-modulated RRab stars.</p>
<h3>Download the light curves:</h3>
<p>
<a href="data/Blazhko_data.tar.bz2">All light curves tarred and bzipped</a>
<br><br>
Benkő et al. 2014, ApJS, 213, 31:
<ul>
<li><a href="data/table_kplr003864443.tailor-made.dat">KIC 3864443 (V2178 Cyg)</a></li>
<li><a href="data/table_kplr004484128.tailor-made.dat">KIC 4484128 (V808 Cyg)</a></li>
<li><a href="data/table_kplr005559631.tailor-made.dat">KIC 5559631 (V783 Cyg)</a></li>
<li><a href="data/table_kplr006183128.tailor-made.dat">KIC 6183128 (V354 Lyr)</a></li>
<li><a href="data/table_kplr006186029.tailor-made.dat">KIC 6186029 (V445 Lyr)</a></li>
<li><a href="data/table_kplr007257008.tailor-made.dat">KIC 7257008</a></li>
<li><a href="data/table_kplr007505345.tailor-made.dat">KIC 7505345 (V355 Lyr)</a></li>
<li><a href="data/table_kplr007671081.tailor-made.dat">KIC 7671081 (V450 Lyr)</a></li>
<li><a href="data/table_kplr009001926.tailor-made.dat">KIC 9001926 (V353 Lyr)</a></li>
<li><a href="data/table_kplr009578833.tailor-made.dat">KIC 9578833 (V366 Lyr)</a></li>
<li><a href="data/table_kplr009697825.tailor-made.dat">KIC 9697825 (V360 Lyr)</a></li>
<li><a href="data/table_kplr009973633.tailor-made.dat">KIC 9973633</a></li>
<li><a href="data/table_kplr010789273.tailor-made.dat">KIC 10789273 (V838 Cyg)</a></li>
<li><a href="data/table_kplr011125706.tailor-made.dat">KIC 11125706</a></li>
<li><a href="data/table_kplr012155928.tailor-made.dat">KIC 12155928 (V1104 Cyg)</a></li>
</ul>
Benkő & Szabó, 2015, ApJL, 809, L19:
<ul>
<li><a href="data/table_kplr007021124.tailor-made.dat">KIC 7021124</a></li>
<li><a href="data/table_kplr009508655.tailor-made.dat">KIC 9508655 (V350 Lyr)</a></li>
<li><a href="data/READ.ME">README file</a></li>
</ul>
</p>
<br>
<h3>Disclaimer</h3>
<p>If you download and use these data, please refer to this paper:<br>
<center>J. M. Benkő, E. Plachy, R. Szabó, L. Molnár, Z. Kolláth:<br>
<em><a href="http://arxiv.org/abs/1406.5864" target="_blank">Long Time-Scale Behaviour of the Blazhko Effect from rectified Kepler Data</a></em><br>
ApJS, 213, 31, 2014</center>
<br><br>
If you download and use V350 Lyr and KIC 7021124 data, please refer to this paper, as well:<br><br>
<center>J. M. Benkő, R. Szabó:<br>
<em><a href="http://adsabs.harvard.edu/abs/2015ApJ...809L..19B" target="_blank">The Blazhko effect and additional excited modes in RR Lyrae stars</a></em><br>
ApJL, 809, L19, 2015</center><br>
If you have any question, don't hesitate to contact the PI of the project, József Benkő: benko at konkoly.hu
</p>
<hr>
<br>
<a name="KeplernonBLRRL"><h2>Kepler non-Blazhko RR Lyrae light curves</h2></a>
<p>These 4-year long, detrended, cleaned, 'final' light curves were made from the
Kepler observations using tailor-made apertures to retain as much flux as possible. These ones belong to
non-modulated (non-Blazhko) RRab stars.</p>
<h3>Download the light curves:</h3>
<p>
<a href="data/nonBL.tar.bz2">All light curves tarred and bzipped</a>
<br><br>
Benkő MNRAS, 473, 412, 2018:
<ul>
<li><a href="data/table_kplr003733346.tailor-made.dat">KIC 3733346 (NR Lyr)</a></li>
<li><a href="data/table_kplr003866709.tailor-made.dat">KIC 3866709 (V715 Cyg)</a></li>
<li><a href="data/table_kplr005299596.tailor-made.dat">KIC 5299596 (V782 Cyg)</a></li>
<li><a href="data/table_kplr006070714.tailor-made.dat">KIC 6070714 (V784 Cyg)</a></li>
<li><a href="data/table_kplr006100702.tailor-made.dat">KIC 6100702 (ASAS 185038+4125.4)</a></li>
<li><a href="data/table_kplr006763132.tailor-made.dat">KIC 6763132 (NQ Lyr)</a></li>
<li><a href="data/table_kplr006936115.tailor-made.dat">KIC 6936115 (FN Lyr)</a></li>
<li><a href="data/table_kplr007030715.tailor-made.dat">KIC 7030715 (ASAS 192325+4231.7)</a></li>
<li><a href="data/table_kplr007176080.tailor-made.dat">KIC 7176080 (V349 Lyr)</a></li>
<li><a href="data/table_kplr007742534.tailor-made.dat">KIC 7742534 (V368 Lyr)</a></li>
<li><a href="data/table_kplr007988343.tailor-made.dat">KIC 7988343 (V1510 Cyg)</a></li>
<li><a href="data/table_kplr008344381.tailor-made.dat">KIC 8344381 (V346 Lyr)</a></li>
<li><a href="data/table_kplr009591503.tailor-made.dat">KIC 9591503 (V894 Cyg)</a></li>
<li><a href="data/table_kplr009658012.tailor-made.dat">KIC 9658012 </a></li>
<li><a href="data/table_kplr009717032.tailor-made.dat">KIC 9717032 </a></li>
<li><a href="data/table_kplr009947026.tailor-made.dat">KIC 9947026 (NSV 11924)</a></li>
<li><a href="data/table_kplr010136240.tailor-made.dat">KIC 10136240 (V1107 Cyg)</a></li>
<li><a href="data/table_kplr010136603.tailor-made.dat">KIC 10136603 (V839 Cyg)</a></li>
<li><a href="data/table_kplr011802860.tailor-made.dat">KIC 11802860 (AW Dra)</a></li>
<li><a href="data/READ.ME">README file</a></li>
</ul>
<br>
<h3>Disclaimer</h3>
<p>If you download and use these data, please refer to these papers:<br>
<center>J. M. Benkő:<br>
<em><a href="" target="_blank">On the connection between almost periodic functions and Blazhko light curves</a></em><br>
MNRAS, 473, 412, 2018</center>
<br><br>
<center>J. Nemec, R. Smolec, J. Benkő et al.:<br>
<em><a href="http://adsabs.harvard.edu/abs/2011MNRAS.417.1022N" target="_blank">Fourier analysis of non-Blazhko ab-type RR Lyrae stars observed with the Kepler space telescope</a></em><br>
MNRAS, 417, 1022, 2011</center>
If you have any questions, don't hesitate to contact the PI of the project, József Benkő: benko at konkoly.hu
</p>
<hr>
<br>
<a name="K2RRL"><h2>K2-E2 RR Lyrae:</h2></a>
<p>These 8.9-day long RR Lyrae data files were taken during the K2 Two-Wheel Concept Engineering Test (K2-E2). The detrended, cleaned, 'final' light curves belong to various RR Lyrae subtypes (Blazhko-modulated RRab stars, non-Blazhko stars, RRc, RRd).</p>
<h3>Download the data:</h3>
<ul>
<li><a href="data/k2-e2_light_curves.txt">33 K2-E2 RR Lyrae light curves</a></li>
<li><a href="data/k2-e2_rrlyrae_freqtable.txt">33 K2-E2 RR Lyrae frequency table</a></li>
<li><a href="data/CSS_RRd_table_1.txt">Basic parameters of confirmed RRd stars from CSS</a></li>
<li><a href="data/CSS_RRd_table_2.txt">Pulsation parameters of confirmed RRd stars from CSS</a></li>
</ul>
<h3>Disclaimer</h3>
<p>If you download and use these data, please refer to this paper:<br>
<center>L. Molnár, R. Szabó, P. A. Moskalik, et al.:<br>
<em><a href="http://arxiv.org/abs/1507.04714" target="_blank">An RR Lyrae family portrait: 33 stars observed in Pisces with K2-E2</a></em><br>
MNRAS, 452, 4283, 2015</center><br>
If you have any question, please contact László Molnár: lmolnar at konkoly.hu
</p>
<hr>
<br>
<a name="K2LEO"><h2>K2 RR Lyrae light curves in Leo IV dwarf galaxy</h2></a>
<p>Leo IV fell into the field-of-view of the first scientific campaign (C1) of the K2 mission and was observed between May 30 and August 21, 2014. The datafile contains 82-day long raw and processed light curves of 3 RR Lyrae belonging to the galaxy. For more information please see the Molnár et al. paper below.</p>
<h3>Download the data</h3>
<ul>
<li><a href="data/molnar_k2-leo4-rrlyr_data.txt">Raw and processed K2 RR Lyrae light curves in Leo IV</a></li>
</ul>
<h3>Disclaimer</h3>
<p>If you download and use these data, please refer to this paper:<br>
<center>L. Molnár, A. Pál, E. Plachy, V. Ripepi, M. I. Moretti, R. Szabó, L. Kiss:<br>
<em><a href="http://arxiv.org/abs/1508.05587" target="_blank">Pushing the limits, episode 2: K2 observations of extragalactic RR Lyrae stars in the dwarf galaxy Leo IV</a></em><br>
ApJ, 812, 2, 2015</center><br>
If you have any question, please contact László Molnár: lmolnar at konkoly.hu
</p>
<hr>
<br>
<a name="CoRoT"><h2>CoRoT RR Lyrae light curves from LRa03 to LRc10</h2></a>
<p>We found new RR Lyrae stars in later CoRoT observing runs. For details please see
Benkő et al. (2016).</p>
<h3>Download the data</h3>
<ul>
<li><a href="data/CoRoT_RR_data.tar.bz2">Processed CoRoT RR Lyrae light curves</a></li>
</ul>
<h3>Disclaimer</h3>
<p>If you download and use these data, please refer to this paper:<br>
<center>J. M. Benkő, R. Szabó, A. Derekas, Á. Sódor:<br>
<em><a href="http://arxiv.org/abs/1608.06418" target="_blank">Finest light curve details, physical parameters, and period fluctuations of CoRoT RR Lyrae stars</a></em><br>
MNRAS, 463, 1769, 2016</center><br>
If you have any question, please contact Jozsef Benkő: benko at konkoly.hu
</p>
<hr>
<br>
<a name="K2_MB_ast"><h2>Main-belt asteroids from the K2 Mission</h2></a>
<p>We studied main-belt asteroids with K2 in the M35 and Neptun/Nereid fields. For details please see
Szabó et al. (2016).</p>
<h3>Download the data</h3>
<ul>
<li><a href="data/M35_all_phot.dat">Photometric data of asteroids in the M35 field</a></li>
<li><a href="data/Nereid_all_phot.dat">Photometric data of asteroids in the Neptune/Nereid field</a></li>
<li><a href="data/M35_asteroids.dat">Rotational parameters of asteroids in the M35 field</a></li>
<li><a href="data/Nereid_asteroids.dat">Rotational parameters of asteroids in the Neptune/Nereid field</a></li>
</ul>
<h3>Disclaimer</h3>
<p>If you download and use these data, please refer to this paper:<br>
<center>R. Szabó, A. Pál, K. Sárneczky et al.:<br>
<em><a href="http://arxiv.org/abs/1609.02759" target="_blank">Uninterrupted optical light curves of main-belt asteroids from the K2 mission</a></em><br>
Astronomy and Astrophysics, 596, A40, 2016</center><br>
If you have any question, please contact Róbert Szabó: rszabo at konkoly.hu
</p>
<hr>
<br>
<p>We also studied main-belt asteroids with K2 in the Uranus field in Campaign 8. For details please see
Molnár et al. (2018).</p>
<h3>Download the data</h3>
<ul>
<li><a href="data/uranusfield-asteroids-photometry.txt">Photometric data of asteroids in the K2 Uranus field</a></li>
</ul>
<h3>Disclaimer</h3>
<p>If you download and use these data, please refer to this paper:<br>
<center>L. Molnár, A. Pál, K. Sárneczky et al.:<br>
<em><a href="http://arxiv.org/abs/1706.06056" target="_blank">Main-belt asteroids in the K2 Uranus field</a></em><br>
ApJS 234, 37, 2018</center><br>
If you have any question, please contact László Molnár: lmolnar at konkoly.hu
</p>
</div>
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<h3>© 2020 R. Szabó, A. Bódi, P. Szabó</h3>
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