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<ri:Resource created="2023-04-27T09:12:38Z" 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>HATS-46 b EFOSC2 light curve</title><shortName>J/MNRAS/521/5636</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/521/5636</identifier><altIdentifier>doi:10.26093/cds/vizier.75215636</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ahrer E.</name></creator><creator><name>Wheatley P.J.</name></creator><creator><name>Gandhi S.</name></creator><creator><name>Kirk J.</name></creator><creator><name>King G.W.</name></creator><creator><name>Louden T.,Welbanks L.</name></creator><date role="Updated">2024-08-22T20:17:10Z</date><date role="Created">2023-04-27T09:12:38Z</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>multiple-stars</subject><subject>exoplanets</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><description>We have performed low-resolution ground-based spectroscopy of HATS-46 b in transmission, using the EFOSC2 instrument on the ESO New Technology Telescope (NTT). HATS-46 b is a highly inflated exoplanet that is a prime target for transmission spectroscopy, having a Jupiter-like radius (0.95R_Jup_) but a much lower mass (0.16M_Jup_). It orbits a G-type star with a 4.7d period, giving an equilibrium temperature of 1100K. We observed one transit of HATS-46 b with the NTT, with the time-series spectra covering a wavelength range of 3900-9000{AA} at a resolution (R) of ~380. We achieved a remarkably precise transmission spectrum of 1.03 x photon noise, with a median uncertainty of 357ppm for ~200{AA}-wide bins, despite the relative faintness of the host star with Vmag=13.6. The transmission spectrum does not show strong absorption features and retrievals favour a cloudy model, ruling out a clear atmosphere with 3.0{sigma} confidence. We also place a conservative upper limit on the sodium abundance under the alternative scenario of a clear atmosphere. This is the eighth planet in the LRG-BEASTS (Low-Resolution Ground-Based Exoplanet Atmosphere Survey using Transmission Spectroscopy) survey, which uses 4 m-class telescopes such as the NTT to obtain low-resolution transmission spectra of hot Jupiters with precisions of around one atmospheric scale height.</description><source format="bibcode">2023MNRAS.521.5636A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/521/5636</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/AJ/155/112">J/AJ/155/112 : Radial velocities + light curves for HATS-43 - HATS-46</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/MNRAS/521/5636</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/521/5636</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/521/5636</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/521/5636</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/521/5636</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/521/5636</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>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/521/5636/lc</name><description>Wavelength binned and white-light light curves of the transit of HATS-46b</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>Time</name><description>Time in MJD</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>FWL</name><description>Normalised white-light flux (3900-9000{AA})</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_FWL</name><description>Error in white-light flux (3900-9000{AA})</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>FWB01</name><description>Normalised flux in 300{AA}-wide bin centred on 4050{AA}</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_FWB01</name><description>Error in flux in 300{AA}-wide bin centred on 4050{AA}</description><ucd>stat.error</ucd><dataType 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xsi:type="vs:VOTableType">double</dataType></column><column><name>FWB17</name><description>Normalised flux in 200{AA}-wide bin centred on 7140{AA}</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_FWB17</name><description>Error in flux in 200{AA}-wide bin centred on 7140{AA}</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>FWB18</name><description>Normalised flux in 200{AA}-wide bin centred on 7340{AA}</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_FWB18</name><description>Error in flux in 200{AA}-wide bin centred on 7340{AA}</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>FWB19</name><description>Normalised flux in 209{AA}-wide bin centred on 7544{AA}</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_FWB19</name><description>Error in flux in 209{AA}-wide bin centred on 7544{AA}</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>FWB20</name><description>Normalised flux in 100{AA}-wide bin centred on 7699{AA}</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_FWB20</name><description>Error in flux in 100{AA}-wide bin centred on 7699{AA}</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>FWB21</name><description>Normalised flux in 201{AA}-wide bin centred on 7849{AA}</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_FWB21</name><description>Error in flux in 201{AA}-wide bin centred on 7849{AA}</description><ucd>stat.error</ucd><dataType 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