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          <element elementId="50">
            <name>Title</name>
            <description>A name given to the resource</description>
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                <text>Conference Papers</text>
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    <name>Conference Paper</name>
    <description>Faculty Publications- Conference Papers</description>
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      <name>Dublin Core</name>
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        <element elementId="50">
          <name>Title</name>
          <description>A name given to the resource</description>
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            <elementText elementTextId="186902">
              <text>REMAP: Determination of the inner edge of the dust torus in AGN by measuring time delays</text>
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          <name>Subject</name>
          <description>The topic of the resource</description>
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            <elementText elementTextId="186903">
              <text>Active; Galaxies; Quasars; Reverberation; Seyfert</text>
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        <element elementId="41">
          <name>Description</name>
          <description>An account of the resource</description>
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            <elementText elementTextId="186904">
              <text>Active galactic nuclei (AGN) are high luminosity sources powered by accretion of matter onto super-massive black holes (SMBHs) located at the centres of galaxies. According to the Unification model of AGN, the SMBH is surrounded by a broad emission line region (BLR) and a dusty torus. It is difficult to study the extent of the dusty torus as the central region of AGN is not resolvable using any conventional imaging techniques available today. Though, current IR interferometric techniques could in principle resolve the torus in nearby AGN, it is very expensive and limited to few bright and nearby AGN. A more feasible alternative to the interferometric technique to find the extent of the dusty torus in AGN is the technique of reverberation mapping (RM). REMAP (REverberation Mapping of AGN Program) is a long term photometric monitoring program being carried out using the 2 m Himalayan Chandra Telescope (HCT) operated by the Indian Institute of Astrophysics, Bangalore, aimed at measuring the torus size in many AGN using the technique of RM. It involves accumulation of suitably long and well sampled light curves in the optical and near-infrared bands to measure the time delays between the light curves in different wavebands. These delays are used to determine the radius of the inner edge of the dust torus. REMAP was initiated in the year 2016 and since then about one hour of observing time once every five days (weather permitting) has been allocated at the HCT. Our initial sample carefully selected for this program consists of a total of 8 sources observable using the HCT. REMAP has resulted in the determination of the extent of the inner edge of the dusty torus in one AGN namely H0507+164. Data accumulation for the second source is completed and observations on the third source are going on. We will outline the motivation of this observational program, the observational strategy that is followed, the analysis procedures adopted for this work and the results obtained from this program till now.  2019 Societe Royale des Sciences de Liege. All rights reserved.</text>
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          <name>Creator</name>
          <description>An entity primarily responsible for making the resource</description>
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            <elementText elementTextId="186905">
              <text>Mandal A.K.; Rakshit S.; Pal I.; Stalin C.S.; Sagar R.; Mathew B.</text>
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        <element elementId="48">
          <name>Source</name>
          <description>A related resource from which the described resource is derived</description>
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              <text>Bulletin de la Societe Royale des Sciences de Liege, Vol-88, pp. 158-165.</text>
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          <name>Publisher</name>
          <description>An entity responsible for making the resource available</description>
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            <elementText elementTextId="186907">
              <text>Societe Royale des Sciences de Liege</text>
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        <element elementId="40">
          <name>Date</name>
          <description>A point or period of time associated with an event in the lifecycle of the resource</description>
          <elementTextContainer>
            <elementText elementTextId="186908">
              <text>2019-01-01</text>
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        <element elementId="43">
          <name>Identifier</name>
          <description>An unambiguous reference to the resource within a given context</description>
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            <elementText elementTextId="186909">
              <text>&lt;a href="https://doi.org/10.25518/0037-9565.8788" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.25518/0037-9565.8788&lt;/a&gt;
&lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85099901158&amp;amp;doi=10.25518%2F0037-9565.8788&amp;amp;partnerID=40&amp;amp;md5=f1c87445e13495b797c6cf8c6c05d145" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/inward/record.uri?eid=2-s2.0-85099901158&amp;amp;doi=10.25518%2f0037-9565.8788&amp;amp;partnerID=40&amp;amp;md5=f1c87445e13495b797c6cf8c6c05d145&lt;/a&gt;</text>
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        <element elementId="47">
          <name>Rights</name>
          <description>Information about rights held in and over the resource</description>
          <elementTextContainer>
            <elementText elementTextId="186910">
              <text>All Open Access; Bronze Open Access; Green Open Access</text>
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        <element elementId="46">
          <name>Relation</name>
          <description>A related resource</description>
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            <elementText elementTextId="186911">
              <text>ISSN: 17835720; CODEN: BSRSA</text>
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          <name>Format</name>
          <description>The file format, physical medium, or dimensions of the resource</description>
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              <text>Online</text>
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          </elementTextContainer>
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        <element elementId="44">
          <name>Language</name>
          <description>A language of the resource</description>
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            <elementText elementTextId="186913">
              <text>English</text>
            </elementText>
          </elementTextContainer>
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        <element elementId="51">
          <name>Type</name>
          <description>The nature or genre of the resource</description>
          <elementTextContainer>
            <elementText elementTextId="186914">
              <text>Conference paper</text>
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          </elementTextContainer>
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          <name>Coverage</name>
          <description>The spatial or temporal topic of the resource, the spatial applicability of the resource, or the jurisdiction under which the resource is relevant</description>
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            <elementText elementTextId="186915">
              <text>Mandal A.K., Department of Physics and Electronics, CHRIST (Deemed to be University), Hosur Road, Bangalore, 560 029, India, Indian Institute of Astrophysics, Block II, Koramangala, Bangalore, 560 034, India; Rakshit S., Finnish Centre for Astronomy with ESO (FINCA), University of Turku, Vesilinnantie 5 Quantum, 20014, Finland; Pal I., Indian Institute of Astrophysics, Block II, Koramangala, Bangalore, 560 034, India; Stalin C.S., Indian Institute of Astrophysics, Block II, Koramangala, Bangalore, 560 034, India; Sagar R., Indian Institute of Astrophysics, Block II, Koramangala, Bangalore, 560 034, India; Mathew B., Department of Physics and Electronics, CHRIST (Deemed to be University), Hosur Road, Bangalore, 560 029, India</text>
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