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The impact of photospheric brightness field on exoplanetary transit timings and the TTV excess of HD 189733 b. / Baluev, Roman V.
в: Monthly Notices of the Royal Astronomical Society, Том 509, № 1, 01.01.2022, стр. 1048-1061.Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
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TY - JOUR
T1 - The impact of photospheric brightness field on exoplanetary transit timings and the TTV excess of HD 189733 b
AU - Baluev, Roman V.
PY - 2022/1/1
Y1 - 2022/1/1
N2 - We consider the issue of excessive TTV noise observed for the exoplanet HD 189733 b. Trying to explain it through the host star photospheric activity, we model the stellar surface brightness as a random field, then characterize statistical properties of the resulting transit signal perturbation and compute individual corrections to transit timings uncertainties. We find that possible effect of the photospheric brightness field can explain only a minor portion (∼10 s) of the observed (∼70 s) TTV excess of HD 189733, suggesting that the rest should be attributed to other sources. Regarding the photospheric pattern, we place an upper limit of ∼0.01 on the combination ϵcellrcell, where ϵcell is the relative magnitude of brightness variations, and rcell is the geometric cellularity scale (relative to star radius).
AB - We consider the issue of excessive TTV noise observed for the exoplanet HD 189733 b. Trying to explain it through the host star photospheric activity, we model the stellar surface brightness as a random field, then characterize statistical properties of the resulting transit signal perturbation and compute individual corrections to transit timings uncertainties. We find that possible effect of the photospheric brightness field can explain only a minor portion (∼10 s) of the observed (∼70 s) TTV excess of HD 189733, suggesting that the rest should be attributed to other sources. Regarding the photospheric pattern, we place an upper limit of ∼0.01 on the combination ϵcellrcell, where ϵcell is the relative magnitude of brightness variations, and rcell is the geometric cellularity scale (relative to star radius).
KW - HD 189733
KW - activity
KW - data analysis
KW - individual
KW - methods
KW - photometric
KW - planetary systems
KW - stars
KW - statistical
KW - techniques
KW - I.
KW - CONFIRMATION
KW - GRANULATION
KW - STELLAR ACTIVITY
KW - methods: statistical
KW - WASP-12
KW - RADIAL-VELOCITY
KW - stars: activity
KW - ANALYSIS TOOL
KW - PLANETS
KW - methods: data analysis
KW - techniques: photometric
KW - TIME
KW - PARAMETERS
KW - stars: individual: HD 189733
UR - https://www.mendeley.com/catalogue/697dddf4-a89e-3285-93d8-7f01a44e117c/
UR - http://www.scopus.com/inward/record.url?scp=85121266432&partnerID=8YFLogxK
U2 - 10.1093/mnras/stab3073
DO - 10.1093/mnras/stab3073
M3 - Article
VL - 509
SP - 1048
EP - 1061
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
SN - 0035-8711
IS - 1
ER -
ID: 87339560