J/ApJ/612/511ivo://CDS.VizieR/J/ApJ/612/511doi:10.26093/cds/vizier.16120511CDSLazio T.J.W.Farrell W.M.Dietrick J.Greenlees E.Hogan E.Jones C.,Hennig L.A.2017-12-06T07:37:59Z2005-06-17T16:50:50ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frmagnetic-fieldsradio-sourcessolar-system-planetsWe predict the radio flux densities of the extrasolar planets in the current census, making use of an empirical relation - the radiometric Bode's law - determined from the five "magnetic" planets in the solar system (the Earth and the four gas giants). Radio emission from these planets results from solar wind-powered electron currents depositing energy in the magnetic polar regions. We find that most of the known extrasolar planets should emit in the frequency range 10-1000 MHz and, under favorable circumstances, have typical flux densities as large as 1mJy. We also describe an initial, systematic effort to search for radio emission in low radio frequency images acquired with the Very Large Array (VLA). The limits set by the VLA images (~300mJy) are consistent with, but do not provide strong constraints on, the predictions of the model.2004ApJ...612..511Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/612/511CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/612/511https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/612/511http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/612/511https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/612/511https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/612/511http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/612/511GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/612/511/table1 (Exoplanet radio emission)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/612/511/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/612/511/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/612/511/table1?GETtext/xml+votable180.050000true269.147958-29.5392220.0055555555555555566/679 748 871 1597 2110 2472 4136 5009 5522 5718 6760 6831 7240 7746 8357 8843 9403 9843 11473 12030 12146 12644 12899 14416 14419 14466 14525 14548 15174 16213 16652 17341 17730 18496 18614 18748 18821 19904 19912 20145 21838 22036 22252 22590 22878 23013 23201 24019 24178 25939 26183 26575 26706 27018 27750 28130 28763 28821 29513 29541 30015 31374 32848 32930 33243 33630 33717 33923 34069 34905 34951 35079 35362 35442 36697 37461 37573 38545 39257 39280 39675 40101 40442 41446 41607 41724 42248 42333 42760 43012 43818 43911 44243 44398 45364 45865 46297 46306 46967 48105https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/612/511?format=asciiRadiodefaultJ/ApJ/612/511/table1Exoplanet radio emissionrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameStar name (1)charomegaPlanet's rotation rate relative to Jupiter's ratefloatlogPLog of the predicted powerlog(W)floatmuThe {mu} value (2)floatnuFrequencyMHzfloatlogS? Log of the predicted burst flux densitylog(Jy)floatnullableSimbadSimbad column added by the CDSchar_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.main_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.main