期刊
ASTROPHYSICAL JOURNAL
卷 832, 期 2, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.3847/0004-637X/832/2/191
关键词
planets and satellites: atmospheres; stars: individual (WASP-39); techniques: photometric; techniques: spectroscopic
资金
- ESO program [096.C-0765(E)]
- European Research Council under the European Union Seventh Framework Program (FP7) ERC [336792]
- Royal Society
- French Agence Nationale de la Recherche (ANR) [ANR-12-BS05-0012]
- [617119]
- STFC [ST/M003515/1, ST/L000709/1] Funding Source: UKRI
- Science and Technology Facilities Council [ST/L000709/1, ST/M003515/1] Funding Source: researchfish
We present transmission spectroscopy of the warm Saturn-mass exoplanet WASP-39b made with the Very. Large. Telescope. FOcal Reducer. and. Spectrograph. (FORS2) across the wavelength range 411-810 nm. The transit depth is measured with a typical precision of 240 parts per million (ppm) in wavelength bins of 10 nm on a V = 12.1 mag star. We detect the sodium absorption feature (3.2 sigma) and find evidence of potassium. The ground-based transmission spectrum is consistent with Hubble Space Telescope (HST) optical spectroscopy, supporting the interpretation that WASP-39b has a largely clear atmosphere. Our results demonstrate the great potential of the recently upgraded FORS2 spectrograph for optical transmission spectroscopy, with which we obtained HST-quality light curves from the ground.
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