期刊
ASTROPHYSICAL JOURNAL
卷 696, 期 2, 页码 1355-1366出版社
IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/696/2/1355
关键词
planetary systems; stars: atmospheres; stars: individual (HD 209458); techniques: photometric
资金
- NSF [AST-0307493]
We present high-resolution High Resolution Echelle Spectrometer (HIRES)/Keck spectra of HD 209458, and a Monte Carlo variation on the basic method used by other workers, to look for the excess in-transit absorption in the NaD doublet at 5893 angstrom due to the extrasolar planet. The HIRES data, binned by bandpass, allow a direct comparison with previous results. We find >3 sigma results in most test bandpasses around the NaD doublet, including relative absorption of (-108.8 +/- 25.7) x 10(-5) in the narrow bandpass used by other workers. This is approximate to 4.7 times larger than the narrow results reported by Charbonneau et al. for HD 209458b. However, >2 sigma absorption is detected in some weak Fe I and Ni I lines that were tested for comparison, raising concern about the uncertainties introduced by continuum-fitting and terrestrial atmosphere subtraction.
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