Additional Doppler Monitoring Corroborates HAT-P-11c as a Planet Article Swipe
Samuel W. Yee
,
Erik A. Petigura
,
Howard Isaacson
,
Andrew W. Howard
,
Sarah Blunt
,
Paul A. Dalba
,
Fei Dai
,
Benjamin J. Fulton
,
Steven Giacalone
,
Stephen R. Kane
,
Molly Kosiarek
,
Teo Močnik
,
Malena Rice
,
Ryan A. Rubenzahl
,
Nicholas Saunders
,
Dakotah Tyler
,
Lauren M. Weiss
,
Jingwen Zhang
·
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.3847/2515-5172/ad675e
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.3847/2515-5172/ad675e
In 2010, Bakos and collaborators discovered a Neptune-sized planet transiting the K-dwarf HAT-P-11 every five days. Later in 2018, Yee and collaborators reported an additional Jovian-mass companion on a nine year orbit based on a decade of Doppler monitoring. The eccentric outer giant HAT-P-11c may be responsible for the peculiar polar orbit of the inner planet HAT-P-11b. However, Basilicata et al. recently suggested that the HAT-P-11c Doppler signal could be caused by stellar activity. In this research note, we extend the Yee et al. Doppler time series by six years. The combined data set spanning 17 yr covers nearly two orbits of the outer planet. Importantly, we observe two periastron passages of planet c and do not observe a coherent activity signature. Together with the previously reported astrometric acceleration of HAT-P-11 from Hipparcos and Gaia, we believe there is strong evidence for HAT-P-11c as a bona fide planet.
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- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.3847/2515-5172/ad675e
- OA Status
- hybrid
- Cited By
- 2
- References
- 16
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4401019970
All OpenAlex metadata
Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W4401019970Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.3847/2515-5172/ad675eDigital Object Identifier
- Title
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Additional Doppler Monitoring Corroborates HAT-P-11c as a PlanetWork title
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articleOpenAlex work type
- Language
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enPrimary language
- Publication year
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2024Year of publication
- Publication date
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2024-07-26Full publication date if available
- Authors
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Samuel W. Yee, Erik A. Petigura, Howard Isaacson, Andrew W. Howard, Sarah Blunt, Paul A. Dalba, Fei Dai, Benjamin J. Fulton, Steven Giacalone, Stephen R. Kane, Molly Kosiarek, Teo Močnik, Malena Rice, Ryan A. Rubenzahl, Nicholas Saunders, Dakotah Tyler, Lauren M. Weiss, Jingwen ZhangList of authors in order
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https://doi.org/10.3847/2515-5172/ad675ePublisher landing page
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YesWhether a free full text is available
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hybridOpen access status per OpenAlex
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https://doi.org/10.3847/2515-5172/ad675eDirect OA link when available
- Concepts
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Planet, Physics, Giant planet, Astronomy, Outer planets, Jupiter (rocket family), Jovian, Orbit (dynamics), Astrophysics, Doppler effect, Neptune, Exoplanet, Astrobiology, Planetary system, Spacecraft, Engineering, Saturn, Aerospace engineeringTop concepts (fields/topics) attached by OpenAlex
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2025: 1, 2024: 1Per-year citation counts (last 5 years)
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10Other works algorithmically related by OpenAlex
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| abstract_inverted_index.nearly | 99 |
| abstract_inverted_index.orbits | 101 |
| abstract_inverted_index.planet | 9, 56, 113 |
| abstract_inverted_index.series | 87 |
| abstract_inverted_index.signal | 68 |
| abstract_inverted_index.strong | 140 |
| abstract_inverted_index.years. | 90 |
| abstract_inverted_index.Doppler | 38, 67, 85 |
| abstract_inverted_index.K-dwarf | 12 |
| abstract_inverted_index.believe | 137 |
| abstract_inverted_index.observe | 108, 118 |
| abstract_inverted_index.planet. | 105, 148 |
| abstract_inverted_index.stellar | 73 |
| abstract_inverted_index.Abstract | 0 |
| abstract_inverted_index.HAT-P-11 | 13, 131 |
| abstract_inverted_index.However, | 58 |
| abstract_inverted_index.Together | 123 |
| abstract_inverted_index.activity | 121 |
| abstract_inverted_index.coherent | 120 |
| abstract_inverted_index.combined | 92 |
| abstract_inverted_index.evidence | 141 |
| abstract_inverted_index.passages | 111 |
| abstract_inverted_index.peculiar | 50 |
| abstract_inverted_index.recently | 62 |
| abstract_inverted_index.reported | 23, 127 |
| abstract_inverted_index.research | 77 |
| abstract_inverted_index.spanning | 95 |
| abstract_inverted_index.HAT-P-11c | 44, 66, 143 |
| abstract_inverted_index.Hipparcos | 133 |
| abstract_inverted_index.activity. | 74 |
| abstract_inverted_index.companion | 27 |
| abstract_inverted_index.eccentric | 41 |
| abstract_inverted_index.suggested | 63 |
| abstract_inverted_index.Basilicata | 59 |
| abstract_inverted_index.HAT-P-11b. | 57 |
| abstract_inverted_index.additional | 25 |
| abstract_inverted_index.discovered | 6 |
| abstract_inverted_index.periastron | 110 |
| abstract_inverted_index.previously | 126 |
| abstract_inverted_index.signature. | 122 |
| abstract_inverted_index.transiting | 10 |
| abstract_inverted_index.Jovian-mass | 26 |
| abstract_inverted_index.astrometric | 128 |
| abstract_inverted_index.monitoring. | 39 |
| abstract_inverted_index.responsible | 47 |
| abstract_inverted_index.Importantly, | 106 |
| abstract_inverted_index.acceleration | 129 |
| abstract_inverted_index.Neptune-sized | 8 |
| abstract_inverted_index.collaborators | 5, 22 |
| cited_by_percentile_year.max | 95 |
| cited_by_percentile_year.min | 90 |
| countries_distinct_count | 3 |
| institutions_distinct_count | 18 |
| citation_normalized_percentile.value | 0.76329779 |
| citation_normalized_percentile.is_in_top_1_percent | False |
| citation_normalized_percentile.is_in_top_10_percent | False |