ExoClock Project. II. A Large-scale Integrated Study with 180 Updated Exoplanet Ephemerides
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F61389021%3A_____%2F22%3A00571808" target="_blank" >RIV/61389021:_____/22:00571808 - isvavai.cz</a>
Result on the web
<a href="https://arxiv.org/pdf/2110.13863.pdf" target="_blank" >https://arxiv.org/pdf/2110.13863.pdf</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.3847/1538-4365/ac3a10" target="_blank" >10.3847/1538-4365/ac3a10</a>
Alternative languages
Result language
angličtina
Original language name
ExoClock Project. II. A Large-scale Integrated Study with 180 Updated Exoplanet Ephemerides
Original language description
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.
Czech name
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Czech description
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Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
<a href="/en/project/EF16_026%2F0008390" target="_blank" >EF16_026/0008390: Partnership for excellence in superprecise optics</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2022
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Astrophysical Journal Supplement Series
ISSN
0067-0049
e-ISSN
1538-4365
Volume of the periodical
258
Issue of the periodical within the volume
2
Country of publishing house
GB - UNITED KINGDOM
Number of pages
47
Pages from-to
40
UT code for WoS article
000753167800001
EID of the result in the Scopus database
2-s2.0-85125866218