4.6 Article

ExoClock Project. II. A Large-scale Integrated Study with 180 Updated Exoplanet Ephemerides

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出版社

IOP Publishing Ltd
DOI: 10.3847/1538-4365/ac3a10

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资金

  1. European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program [758892]
  2. UKSA/STFC [ST/T001836/1, ST/V003380/1, ST/W00254X/1]
  3. Czech Astronomical Society
  4. NASA Award [NNX16AC65A]
  5. Paris Region fellowship program - Ile-de-France Region
  6. program for research and Horizon 2020 innovation under the Marie Sklodowska-Curie grant [945298]
  7. ASI [2018.22.HH.O]
  8. [CZ.02.1.01/0.0/0.0/16_026/0008390]
  9. [BK225/RAu-11/2021]
  10. [02/140/SDU/10-22-02]
  11. Marie Curie Actions (MSCA) [945298] Funding Source: Marie Curie Actions (MSCA)
  12. NASA [906274, NNX16AC65A] Funding Source: Federal RePORTER

向作者/读者索取更多资源

The ExoClock project monitors and updates the ephemerides of Ariel targets using observations from ground telescopes, midtime values from literature, and space instrument observations. The updated ephemerides have implications for future scheduling and have significantly improved precision.
The ExoClock project is an inclusive, integrated, and interactive platform that was developed to monitor the ephemerides of the Ariel targets to increase the mission efficiency. The project makes the best use of all available resources, i.e., observations from ground telescopes, midtime values from the literature, and finally, observations from space instruments. Currently, the ExoClock network includes 280 participants with telescopes capable of observing 85% of the currently known Ariel candidate targets. This work includes the results of similar to 1600 observations obtained up to 2020 December 31 from the ExoClock network. These data in combination with similar to 2350 midtime values collected from the literature are used to update the ephemerides of 180 planets. The analysis shows that 40% of the updated ephemerides will have an impact on future scheduling as either they have a significantly improved precision or they have revealed biases in the old ephemerides. With the new observations, the observing coverage and rate for half of the planets in the sample has been doubled or more. Finally, from a population perspective, we identify that the differences in the 2028 predictions between the old and the new ephemerides have an STD that is double what is expected from Gaussian uncertainties. These findings have implications for planning future observations, where we will need to account for drifts potentially greater than the prediction uncertainties. The updated ephemerides are open and accessible to the wider exoplanet community both from our Open Science Framework repository and our website.

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