Find link

language:

Find link is a tool written by Edward Betts.

searching for Transit-timing variation 20 found (78 total)

alternate case: transit-timing variation

GSC 03089-00929 (695 words) [view diff] no match in snippet view article find links to article

Umbäässa, orbiting this star by using the transit method. The transit timing variation analysis did not reveal any additional planets in the system as

Kepler-89 (486 words) [view diff] no match in snippet view article find links to article

Kento; et al. (2013). "Characterization of the KOI-94 System with Transit Timing Variation Analysis: Implication for the Planet-Planet Eclipse". The Astrophysical

WASP-32 (440 words) [view diff] no match in snippet view article find links to article

star in prograde direction in 2014. The follow-up study utilizing transit timing variation analysis, have failed to find any, therefore have excluded existence

HAT-P-26 (836 words) [view diff] no match in snippet view article find links to article

measured planetary temperature is equal to 563+58 −54 K. In 2019, a transit timing variation analysis of HAT-P-26b indicated the possible presence of a second

WASP-3 (381 words) [view diff] no match in snippet view article find links to article

Raetz; Ch.Ginski; Ch.Adam, C.Marka; M.Moualla; M.Mugrauer (2010). "Transit timing variation in exoplanet WASP-3b". Monthly Notices of the Royal Astronomical

WASP-10 (474 words) [view diff] no match in snippet view article find links to article

Krushevska, V.; Tachihara, K.; Takahashi, H.; Mugrauer, M. (2011). "Transit timing variation and activity in the WASP-10 planetary system★". Monthly Notices

WASP-12 (684 words) [view diff] no match in snippet view article find links to article

Collins, Karen A.; Kielkopf, John F.; Stassun, Keivan G. (2015). "TRANSIT TIMING VARIATION MEASUREMENTS OF WASP-12b AND QATAR-1b: NO EVIDENCE OF ADDITIONAL

HAT-P-36 (579 words) [view diff] no match in snippet view article find links to article

2012 by the HATNet Project using the transit method. A search for transit timing variation did not result in detection of additional planets in the system

GSC 03949-00967 (553 words) [view diff] no match in snippet view article find links to article

TrES-5 b: departure from a linear ephemeris instead of short-period transit timing variation". Astronomy & Astrophysics. 656. A88. arXiv:2110.14294. Bibcode:2021A&A

Kepler-84 (652 words) [view diff] no match in snippet view article find links to article

doi:10.3847/0004-6256/152/1/8, S2CID 119110229 Xie, Ji-Wei (2012), "Transit Timing Variation of Near-Resonance Planetary Pairs: Confirmation of 12 Multiple-Planet

Kepler-32 (715 words) [view diff] exact match in snippet view article find links to article

Kepler-32c with an orbital period of 8.7522 days. In April 2013, transit-timing variation analysis confirmed 3 other planets to be in the system. However

Kepler-25 (682 words) [view diff] exact match in snippet view article find links to article

of the planetary systems. These planets were confirmed through transit-timing variation method. A third planet was discovered through follow-up radial

K2-138 (1,317 words) [view diff] exact match in snippet view article find links to article

for K2-138 did not have a high enough signal-to-noise ratio for transit-timing variation (TTV) analysis. However, the Spitzer Space Telescope could be able

GJ 3470 b (1,316 words) [view diff] no match in snippet view article find links to article

7 June 2023. Awiphan, S.; Kerins, E.; et al. (December 2016). "Transit timing variation and transmission spectroscopy analyses of the hot Neptune GJ3470b"

TrES-3b (440 words) [view diff] no match in snippet view article find links to article

Vasilii; Ignatov, Vladimir; Vaňko, M.; Püsküllü, Ç. (2020). "Probing Transit Timing Variation and Its Possible Origin with 12 New Transits of TrES-3b". The Astronomical

XO-3b (1,182 words) [view diff] no match in snippet view article find links to article

PMID 15829958. S2CID 119496437. Yang, Fan; Wei, Xing (2022), "Transit Timing Variation of XO-3b: Evidence for Tidal Evolution of Hot Jupiter with High

GJ 3470 (1,480 words) [view diff] no match in snippet view article find links to article

16 July 2020. Awiphan, S.; Kerins, E.; et al. (December 2016). "Transit timing variation and transmission spectroscopy analyses of the hot Neptune GJ3470b"

WASP-52 (1,213 words) [view diff] no match in snippet view article find links to article

the star, the misalignment being 5.47+4.61 −4.21°. Search for transit timing variation did not result in detection of additional planets in system as

WASP-12b (1,924 words) [view diff] no match in snippet view article find links to article

Collins, Karen A; Kielkopf, John F; Stassun, Keivan G (2017). "Transit Timing Variation Measurements of WASP-12b and Qatar-1b: No Evidence for Additional

GJ 1214 (1,326 words) [view diff] no match in snippet view article find links to article

high-precision defocused transit observations and a search for evidence of transit timing variation". Astronomy & Astrophysics. 549: A10. arXiv:1207.3064. Bibcode:2013A&A