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Table · dataset · 2014

WASP-43 OSIRIS transmission spectroscopy

Listed in IVOA Registry (Virtual Observatory)

We used the Gran Telescopio Canarias (GTC) instrument OSIRIS to obtain long-slit spectra in the optical range 520-1040nm of the planetary host star WASP-43 and of a reference star during a full primary transit event.

Description

We integrated the stellar flux of both stars in different wavelength regions producing several light curves. We measure a mean planet-to-star radius ratio in the white light curve of 0.15988^+0.00133^_-0.00145_.

We present a tentative detection in the planet-to-star radius ratio around the NaI doublet ({lambda} 588.9, 589.5nm) when compared to the nearby continuum at the 2.9-sigma level. We find no significant excess of the measured planet-to-star radius ratio around the KI doublet ({lambda} 766.5nm, 769.9nm) when compared to the nearby continuum.

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Catalogue records · 2

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Stated by source
Optical
Inferred from text
Astronomical sciences 73%
Provenance · 1 source records, 9 field assertions
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IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/a+a/563/a4115 d agoJSON v1
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access_levelsource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[field].anzsrc:group:5101enrichment · IVOA Registrytaxonomy-embedding@1.1.0title+keywords+description (73%)
concepts[field].local:field:astronomymapping · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].ivoa_waveband:opticalsource · IVOA Registryconnector:ivoa_registry@1.0.0
descriptionsource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_description
license_textsource · IVOA Registryconnector:ivoa_registry@1.0.0
publication_datesource · IVOA Registryconnector:ivoa_registry@1.0.0
titlesource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_title
updated_datesource · IVOA Registryconnector:ivoa_registry@1.0.0