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<ri:Resource created="2008-01-09T12:36:11Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>NGC4395 light curves</title><shortName>J/ApJ/632/799</shortName><identifier>ivo://CDS.VizieR/J/ApJ/632/799</identifier><altIdentifier>doi:10.26093/cds/vizier.16320799</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Peterson B.M.</name></creator><creator><name>Bentz M.C.</name></creator><creator><name>Desroches L.-B.</name></creator><creator><name>Filippenko A.V.</name></creator><creator><name>Ho L.C.,Kaspi S.</name></creator><creator><name>Laor A.</name></creator><creator><name>Maoz D.</name></creator><creator><name>Moran E.C.</name></creator><creator><name>Pogge R.W.</name></creator><creator><name>Quillen A.C.</name></creator><date role="Updated">2017-07-11T13:09:19Z</date><date role="Created">2008-01-09T12:36:11Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>active-galactic-nuclei</subject><subject>seyfert-galaxies</subject><subject>ultraviolet-astronomy</subject><description>A reverberation-mapping program on NGC 4395, the least luminous known Seyfert 1 galaxy, undertaken with the Space Telescope Imaging Spectrograph on the Hubble Space Telescope yields a measurement of the mass of the central black hole M_BH_=(3.6+/-1.1)x10^5^M_{sun}_. The observations consist of two visits of five orbits each, in 2004 April and July. During each of these visits, the UV continuum varied by at least 10% (rms), and only C IV {lambda}1549 showed corresponding variations large enough to reliably determine the emission-line lag, which was measured to be of order 1-hr for both visits.</description><source format="bibcode">2005ApJ...632..799P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/632/799</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/98/477">J/ApJS/98/477 : Optical spectral atlas of Seyfert nuclei (Ho+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/112/315">J/ApJS/112/315 : Spectroscopic parameters of Seyfert nuclei (Ho+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/133/77">J/ApJS/133/77 : VLA radio continuum survey of Seyfert galaxies (Ho+, 2001)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/632/799</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/632/799</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/632/799</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/632/799</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/632/799</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/632/799</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>UV</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/632/799/data</name><description>Light curves for visits 2 and 3</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>T</name><description>Simbad column added by the CDS</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>HJD</name><description>Julian Date of observation</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F1350</name><description>1350{AA} flux (1)</description><unit>1e-16W.m**-2.nm**-1</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F1350</name><description>Uncertainty in F1350 (1)</description><unit>1e-16W.m**-2.nm**-1</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FCIV</name><description>C IV (1549{AA}) integrated line flux (2)</description><unit>fW.m**-2</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_FCIV</name><description>Uncertainty in FCIV (2)</description><unit>fW.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>