SIMBAD references

2014MNRAS.441..304S - Mon. Not. R. Astron. Soc., 441, 304-315 (2014/June-2)

Transit timing analysis in the HAT-P-32 system.

SEELIGER M., DIMITROV D., KJURKCHIEVA D., MALLONN M., FERNANDEZ M., KITZE M., CASANOVA V., MACIEJEWSKI G., OHLERT J.M., SCHMIDT J.G., PANNICKE A., PUCHALSKI D., GOGUS E., GUVER T., BILIR S., AK T., HOHLE M.M., SCHMIDT T.O.B., ERRMANN R., JENSEN E., COHEN D., MARSCHALL L., SARAL G., BERNT I., DERMAN E., GALAN C. and NEUHAUSER R.

Abstract (from CDS):

We present the results of 45 transit observations obtained for the transiting exoplanet HAT-P-32b. The transits have been observed using several telescopes mainly throughout the YETI (Young Exoplanet Transit Initiative) network. In 25 cases, complete transit light curves with a timing precision better than 1.4min have been obtained. These light curves have been used to refine the system properties, namely inclination i, planet-to-star radius ratio Rp/Rs, and the ratio between the semimajor axis and the stellar radius a/Rs. First analyses by Hartman et al. suggests the existence of a second planet in the system, thus we tried to find an additional body using the transit timing variation (TTV) technique. Taking also the literature data points into account, we can explain all mid-transit times by refining the linear ephemeris by 21ms. Thus, we can exclude TTV amplitudes of more than ∼ 1.5min.

Abstract Copyright: © 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2014)

Journal keyword(s): planets and satellites: individual: HAT-P-32b - stars: individual: HAT-P-32 - planetary systems

Simbad objects: 10

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2021.01.27-03:28:22

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