Transmission spectroscopy of HAT-P-32b

DOI

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.

Identifier
DOI http://doi.org/10.26093/cds/vizier.35900100
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/590/A100
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/590/A100
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/590/A100
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/590/A100
Provenance
Creator Mallonn M.; Strassmeier K.G.
Publisher CDS
Publication Year 2016
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Natural Sciences; Observational Astronomy; Physics; Solar System Astronomy; Stellar Astronomy