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<ri:Resource created="2020-07-01T10:13:41Z" 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>Transmission Spectroscopy Metric of exoplanets</title><shortName>J/AJ/159/239</shortName><identifier>ivo://CDS.VizieR/J/AJ/159/239</identifier><altIdentifier>doi:10.26093/cds/vizier.51590239</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Guo X.</name></creator><creator><name>Crossfield I.J.M.</name></creator><creator><name>Dragomir D.</name></creator><creator><name>Kosiarek M.R.</name></creator><creator><name>Lothringer J.,Mikal-Evans T.</name></creator><creator><name>Rosenthal L.</name></creator><creator><name>Benneke B.</name></creator><creator><name>Knutson H.A.</name></creator><creator><name>Dalba P.A.,Kempton E.M.R.</name></creator><creator><name>Henry G.W.</name></creator><creator><name>McCullough P.R.</name></creator><creator><name>Barman T.</name></creator><creator><name>Blunt S.,Chontos A.</name></creator><creator><name>Fortney J.</name></creator><creator><name>Fulton B.J.</name></creator><creator><name>Hirsch L.</name></creator><creator><name>Howard A.W.</name></creator><creator><name>Isaacson H.,Matthews J.</name></creator><creator><name>Mocnik T.</name></creator><creator><name>Morley C.</name></creator><creator><name>Petigura E.A.</name></creator><creator><name>Weiss L.M.</name></creator><date role="Updated">2020-11-26T11:25:38Z</date><date role="Created">2020-07-01T10:13:41Z</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>exoplanets</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><subject>radial-velocity</subject><subject>stellar-radii</subject><subject>infrared-photometry</subject><subject>effective-temperature</subject><description>Recent years have seen increasing interest in the characterization of sub-Neptune-sized planets because of their prevalence in the Galaxy, contrasted with their absence in our solar system. HD97658 is one of the brightest stars hosting a planet of this kind, and we present the transmission spectrum of this planet by combining four Hubble Space Telescope transits, 12 Spitzer/IRAC transits, and eight Microvariability and Oscillations of Stars Telescope (MOST) transits of this system. Our transmission spectrum has a higher signal-to-noise ratio than those from previous works, and the result suggests that the slight increase in transit depth from wavelength 1.1-1.7{mu}m reported in previous works on the transmission spectrum of this planet is likely systematic. Nonetheless, our atmospheric modeling results are inconclusive, as no model provides an excellent match to our data. Nonetheless, we find that atmospheres with high C/O ratios (C/O~&gt;0.8) and metallicities of ~&gt;100 solar metallicity are favored. We combine the mid-transit times from all of the new Spitzer and MOST observations and obtain an updated orbital period of P=9.489295{+/-}0.000005, with a best-fit transit time center at T0=2456361.80690{+/-}0.00038(BJD). No transit timing variations are found in this system. We also present new measurements of the stellar rotation period (34{+/-}2days) and stellar activity cycle (9.6yr) of the host star HD97658. Finally, we calculate and rank the Transmission Spectroscopy Metric of all confirmed planets cooler than 1000K and with sizes between 1R_{Earth}_ and 4R_{Earth}_. We find that at least a third of small planets cooler than 1000K can be well characterized using James Webb Space Telescope, and of those, HD97658b is ranked fifth, meaning that it remains a high-priority target for atmospheric characterization.</description><source format="bibcode">2020AJ....159..239G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/159/239</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/B/hst">B/hst : HST Archived Exposures Catalog (STScI, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia 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of HD 97658 (Van Grootel+,2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/150/169">J/AJ/150/169 : Radial velocities of HD 6434 (Hinkel+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/848/34">J/ApJ/848/34 : CATalog of Stellar Unified Properties (Hinkel+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/153/191">J/AJ/153/191 : Transiting planet GJ 1132 (Southworth+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/155/66">J/AJ/155/66 : Stroemgren photometric observations GJ436b (Lothringer+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/631/A90">J/A+A/631/A90 : K2-138 HARPS radial velocities (Lopez+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/157/33">J/AJ/157/33 : Radial velocity exploration of {sigma} Eridani (Mawet+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/157/192">J/AJ/157/192 : Radial velocities and transit times 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>BJD</name><description>[2450463/2458560] Barycentric Julian Date, TDB system</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RVel</name><description>[-20.58/14.62] Radial Velocity</description><unit>m/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_RVel</name><description>[0.91/7.78] Uncertainty in RVel</description><unit>m/s</unit><ucd>stat.error;spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SHK</name><description>[0.149/0.379] Stellar activity indicator, Calcium H &amp; K lines (1)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Inst</name><description>Instrument used (2)</description><ucd>instr.setup</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column></table><table><name>J/AJ/159/239/table11</name><description>Transmission Spectroscopy Metric of confirmed planets with R_{Earth}_&lt;R_planet_&lt;4R_{Earth}_, and cooler than 1000K</description><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>Name</name><description>Planet name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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