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    <name>Article</name>
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          <name>Title</name>
          <description>A name given to the resource</description>
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              <text>A Search for X-Ray/UV Correlation in the Reflection-dominated Seyfert 1 Galaxy Markarian 1044</text>
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              <text>Correlated variability between coronal X-rays and disk optical/UV photons provides a very useful diagnostic of the interplay between the different regions around an active galactic nucleus (AGN) and how they interact. AGNs that reveal strong X-ray reflection in their spectra should normally exhibit optical/UV to X-ray correlation consistent with reprocessingwhereas the optical/UV emission lags behind the X-rays. While such correlated delay has been seen in some sources, it has been absent in others. Mrk 1044 is one such source that has been known to reveal strong X-ray reflection in its spectra. In our analysis of three long XMM-Newton and several Swift observations of the source, we found no strong evidence for correlation between its UV and X-ray lightcurves both on short and long timescales. Among other plausible causes for the nondetection, we posit that higher X-ray variability rather than UV and strong general relativistic effects close to the black hole may also be responsible. We also present results from the spectral analysis based on XMM-Newton and NuSTAR observations, which show the strong soft X-ray excess and iron K? line in the 0.3-50 keV spectrum that can be described by relativistic reflection.  2023. The Author(s). Published by the American Astronomical Society.</text>
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          <name>Creator</name>
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              <text>Barua S.; Adegoke O.K.; Misra R.; Pawar P.; Jithesh V.; Medhi B.J.</text>
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              <text>Astrophysical Journal, Vol-958, No. 1</text>
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          <name>Publisher</name>
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              <text>Institute of Physics</text>
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          <name>Date</name>
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              <text>2023-01-01</text>
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              <text>&lt;a href="https://doi.org/10.3847/1538-4357/acf464" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.3847/1538-4357/acf464&lt;/a&gt;
&lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85177564288&amp;amp;doi=10.3847%2F1538-4357%2Facf464&amp;amp;partnerID=40&amp;amp;md5=dd9ede5dbbc138f21eb469de7d2554a6" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/inward/record.uri?eid=2-s2.0-85177564288&amp;amp;doi=10.3847%2f1538-4357%2facf464&amp;amp;partnerID=40&amp;amp;md5=dd9ede5dbbc138f21eb469de7d2554a6&lt;/a&gt;</text>
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          <name>Rights</name>
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              <text>All Open Access; Gold Open Access; Green Open Access</text>
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              <text>ISSN: 0004637X</text>
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              <text>Online</text>
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          <name>Language</name>
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              <text>English</text>
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              <text>Barua S., Department of Physics, Gauhati University, Jalukbari Assam, Guwahati, 781014, India; Adegoke O.K., Cahill Center for Astronomy and Astrophysics, California Institute of Technology, Pasadena, 91125, CA, United States; Misra R., Inter-University Centre for Astronomy and Astrophysics (IUCAA), PB No. 4, Ganeshkhind, Pune, 411007, India; Pawar P., Inter-University Centre for Astronomy and Astrophysics (IUCAA), PB No. 4, Ganeshkhind, Pune, 411007, India, Department of Physics, Deogiri College, Maharashtra, Aurangabad, 431005, India; Jithesh V., Department of Physics and Electronics, CHRIST (Deemed to be University), Hosur Main Road, Bengaluru, 560029, India; Medhi B.J., Department of Physics, Gauhati University, Jalukbari Assam, Guwahati, 781014, India</text>
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