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dc.contributor.authorPardo Carrión, Juan Ramón-
dc.contributor.authorSerabyn, Eugene-
dc.contributor.authorWiedner, Martina C.-
dc.contributor.authorMoreno, Raphael.-
dc.contributor.authorOrton, Glenn-
dc.date.accessioned2019-08-16T12:01:00Z-
dc.date.available2019-08-16T12:01:00Z-
dc.date.issued2017-07-01-
dc.identifierdoi: 10.1016/j.icarus.2017.02.019-
dc.identifierissn: 0019-1035-
dc.identifier.citationIcarus 290: 150-155 (2017)-
dc.identifier.urihttp://hdl.handle.net/10261/188371-
dc.description.abstractOne of the legacies of the now retired Caltech Submillimeter Observatory (CSO) is presented in this paper. We measured for the first time the emission of the giant planets Jupiter and Saturn across the 0.3 to 1.3  mm wavelength range using a Fourier Transform Spectrometer mounted on the 10.4 m dish of the CSO at Mauna Kea, Hawaii, 4100 m above sea level. A careful calibration, including the evaluation of the antenna performance over such a wide wavelength range and the removal of the Earth's atmosphere effects, has allowed the detection of broad absorption lines on those planets’ atmospheres. The calibrated data allowed us to verify the predictions of standard models for both planets in this spectral region, and to confirm the absolute radiometry in the case of Jupiter. Besides their physical interest, the results are also important as both planets are calibration references in the current era of operating ground-based and space-borne submillimeter instruments.-
dc.description.sponsorshipWe would like nevertheless to thank the NSF for supporting the operations of the CSO at the time the measurements were achieved by grants ATM-9616766, AST-9615025 and AST-9980846. J.R. Pardo acknowledges support in the final part of this work by the Union’s Seventh Framework Programme (FP/2007-2013)/ERC Grant Agreement n. 610256 (NANOCOSMOS).-
dc.publisherElsevier-
dc.relationinfo:eu-repo/grantAgreement/EC/FP7/610256-
dc.rightsclosedAccess-
dc.subjectRadio continuum and lines: planetary atmospheres-
dc.subjectPlanets: Jupiter and Saturn-
dc.subjectCalibration: millimeter and submillimeter wavelengths-
dc.titleGround-based measurements of the 1.3 to 0.3 mm spectrum of Jupiter and Saturn, and their detailed calibration-
dc.typeartículo-
dc.relation.publisherversionhttps://doi.org/10.1016/j.icarus.2017.02.019-
dc.date.updated2019-08-16T12:01:00Z-
dc.language.rfc3066eng-
dc.contributor.funderNational Science Foundation (US)-
dc.contributor.funderEuropean Commission-
dc.relation.csic-
dc.identifier.funderhttp://dx.doi.org/10.13039/100000001es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100000780es_ES
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