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          <element elementId="50">
            <name>Title</name>
            <description>A name given to the resource</description>
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              <elementText elementTextId="3139">
                <text>Faculty Publications</text>
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    <name>Article</name>
    <description>Faculty Publications -Articles</description>
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      <name>Dublin Core</name>
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          <name>Creator</name>
          <description>An entity primarily responsible for making the resource</description>
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              <text>Reshma, M.; Stalin, C.S.; Mandal, Amit Kumar; Kayal, Abhijit; Gudennavar, S.B.; Joseph, Prajwel</text>
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          <name>Title</name>
          <description>A name given to the resource</description>
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              <text>Detection of time delay between UV and X-ray variability in Mrk 1044 using AstroSat observations</text>
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          <name>Date</name>
          <description>A point or period of time associated with an event in the lifecycle of the resource</description>
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            <elementText elementTextId="208078">
              <text>01-01-2026</text>
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          <name>Source</name>
          <description>A related resource from which the described resource is derived</description>
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            <elementText elementTextId="208079">
              <text>Journal of High Energy Astrophysics;Volume;51;Issue;;Article No.;100552;</text>
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          <name>Identifier</name>
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              <text>&lt;a href="https://doi.org/10.1016/j.jheap.2026.100552" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.1016/j.jheap.2026.100552&lt;/a&gt; &lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/pages/publications/105027550161?origin=resultslist" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/pages/publications/105027550161?origin=resultslist&lt;/a&gt;</text>
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          <name>Coverage</name>
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              <text>Reshma M., Department of Physics and Electronics, CHRIST University, Karnataka, Bangalore, 560029, India; Stalin C.S., Indian Institute of Astrophysics, Block II, Koramangala, Karnataka, Bangalore, 560034, India; Mandal A.K., Center for Theoretical Physics of the Polish Academy of Sciences, Al. Lotnikow 32/46, 02-668 Warsaw, Poland; Kayal A., Indian Institute of Astrophysics, Block II, Koramangala, Karnataka, Bangalore, 560034, India; Gudennavar S.B., Department of Physics and Electronics, CHRIST University, Karnataka, Bangalore, 560029, India; Joseph P., Indian Institute of Astrophysics, Block II, Koramangala, Karnataka, Bangalore, 560034, India</text>
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              <text>Active galactic nuclei are known to exhibit flux variations across the entire electromagnetic spectrum. Among these, correlations between UV/optical and X-ray flux variations serve as a key diagnostics for understanding the physical connection between the accretion disk and the corona. In this work, we present the results of analysis of ultraviolet (UV) and X-ray flux variations in the narrow line Seyfert 1 galaxy Mrk 1044. Simultaneous observations in the far-UV band (FUV: 1300 - 1800  and the X-ray band (0.5 - 7 keV) obtained during 31 August - 8 September 2018 with the Ultraviolet Imaging Telescope and the Soft X-ray Telescope onboard AstroSat were used for this study. Significant flux variability was detected in both FUV and X-ray bands. The fractional root mean square variability amplitude ( F var) was found to be 0.036  0.001 in the FUV band and 0.384  0.004 in the X-ray band. To explore potential time lag between the two bands, cross-correlation analysis was performed using both the interpolated cross-correlation function (ICCF) and just another vehicle for estimating lags in nuclei (JAVELIN) methods. Results from both approaches are consistent within 2 ? uncertainty, indicating that X-ray variations lead the FUV variations, with measured lags of 2.25  0.05 days (ICCF) and 2.35?0.01+0.02 days (JAVELIN). This is the first detection of a time delay between UV and X-ray variations in Mrk 1044. The observed UV lag supports the disk reprocessing scenario, wherein X-ray emission from the corona irradiates the accretion disk, driving the observed UV variability.  2026 Elsevier B.V.</text>
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          <name>Subject</name>
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              <text>Active - galaxies; Galaxies; Galaxies - X-rays; Individual; Mrk 1044 - ultraviolet</text>
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          <name>Publisher</name>
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            <elementText elementTextId="208084">
              <text>Elsevier B.V.</text>
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              <text>ISSN: 22144048;</text>
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          <name>Language</name>
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            <elementText elementTextId="208086">
              <text>English</text>
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          <name>Type</name>
          <description>The nature or genre of the resource</description>
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              <text>Article</text>
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          <name>Rights</name>
          <description>Information about rights held in and over the resource</description>
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            <elementText elementTextId="208088">
              <text>Restricted Access; Hardcopy may be available in the library</text>
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          <name>Format</name>
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              <text>online</text>
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