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<ri:Resource created="2022-05-05T10:02:54Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" 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/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd 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>Light curve &amp; radial velocity of 4 giants planets</title><shortName>J/AJ/163/125</shortName><identifier>ivo://CDS.VizieR/J/AJ/163/125</identifier><altIdentifier>doi:10.26093/cds/vizier.51630125</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Jordan A.</name></creator><creator><name>Hartman J.D.</name></creator><creator><name>Bayliss D.</name></creator><creator><name>Bakos G.A.</name></creator><creator><name>Brahm R.</name></creator><creator><name>Bryant E.M.,Csubry Z.</name></creator><creator><name>Henning T.</name></creator><creator><name>Hobson M.</name></creator><creator><name>Mancini L.</name></creator><creator><name>Penev K.</name></creator><creator><name>Rabus M.</name></creator><creator><name>Suc V.,de Val-Borro M.</name></creator><creator><name>Wallace J.</name></creator><creator><name>Barkaoui K.</name></creator><creator><name>Ciardi D.R.</name></creator><creator><name>Collins K.A.,Esparza-Borges E.</name></creator><creator><name>Furlan E.</name></creator><creator><name>Gan T.</name></creator><creator><name>Benkhaldoun Z.</name></creator><creator><name>Ghachoui M.,Gillon M.</name></creator><creator><name>Howell S.</name></creator><creator><name>Jehin E.</name></creator><creator><name>Fukui A.</name></creator><creator><name>Kawauchi K.</name></creator><creator><name>Livingston J.H.,Luque R.</name></creator><creator><name>Matson R.</name></creator><creator><name>Matthews E.C.</name></creator><creator><name>Osborn H.P.</name></creator><creator><name>Murgas F.</name></creator><creator><name>Narita N.,Palle E.</name></creator><creator><name>Parvianen H.</name></creator><creator><name>Waalkes W.C.</name></creator><date role="Updated">2022-09-30T22:14:52Z</date><date role="Created">2022-05-05T10:02:54Z</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>dwarf-stars</subject><subject>exoplanets</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>spectroscopy</subject><subject>radial-velocity</subject><description>The relative rarity of giant planets around low-mass stars compared with solar-type stars is a key prediction from the core-accretion planet formation theory. In this paper we report on the discovery of four gas giant planets that transit low-mass late K and early M dwarfs. The planets HATS-74Ab (TOI737b), HATS-75b (TOI552b), HATS-76b (TOI555b), and HATS-77b (TOI730b) were all discovered from the HATSouth photometric survey and follow-up using TESS and other photometric facilities. We use the new ESPRESSO facility at the VLT to confirm systems and measure their masses. We find that these planets have masses of 1.46{+/-}0.14M_J_, 0.491{+/-}0.039M_J_, 2.629{+/-}0.089M_J_, and 1.374_-0.074_^+0.100^M_J_, respectively, and radii of 1.032{+/-}0.021R_J_, 0.884{+/-}0.013R_J_, 1.079{+/-}0.031R_J_, and 1.165{+/-}0.021R_J_, respectively. The planets all orbit close to their host stars with orbital periods ranging from 1.7319days to 3.0876days. With further work, we aim to test core-accretion theory by using these and further discoveries to quantify the occurrence rate of giant planets around low-mass host stars.</description><source format="bibcode">2022AJ....163..125J</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/163/125</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>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/II/346">II/346 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IV/38">IV/38 : TESS Input Catalog - v8.0 (TIC-8) (Stassun+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/415/1153">J/A+A/415/1153 : [Fe/H] for 98 extra-solar planet-host stars (Santos+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/622/1102">J/ApJ/622/1102 : The planet-metallicity correlation. 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