Catalog Service: Transmission spectroscopy of HAT-P-32b
Description
We obtained low-resolution, multi-object spectra of the planet host star HAT-P-32 and multiple comparison stars during a transit event of HAT-P-32b. The spectral flux was binned in 62 narrow channels from 3300 to 10000{AA} and used to create differential photometric light curves. These light curves were analysed for a wavelength dependence of the effective planetary radius.
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Publisher: CDSivo://CDS[Pub. ID]
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This resource was registered on: 2016 May 25 13:22:48ZThis resource description was last updated on: 2021 Oct 21 00:00:00Z
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This is service that does not comply with any IVOA standard but instead provides access to special capabilities specific to this resource.
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Developed with the support of the National Science Foundation under Cooperative Agreement AST0122449 with the Johns Hopkins University The NAVO project is a member of the International Virtual Observatory Alliance
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