Planet search with the Keck/NIRC2 vortex coronagraph in the Ms band for Vega

Author:

Ren Bin B.ORCID,Wallack Nicole L.,Hurt Spencer A.,Mawet Dimitri,Carter Aarynn L.ORCID,Echeverri Daniel,Llop-Sayson Jorge,Meshkat Tiffany,Oppenheimer RebeccaORCID,Aguilar JonathanORCID,Cady Eric,Choquet ÉlodieORCID,Ruane Garreth,Vasisht Gautam,Ygouf Marie

Abstract

Context. Gaps in circumstellar disks can signal the existence of planetary perturbers, making such systems preferred targets for direct imaging observations of exoplanets. Aims. Being one of the brightest and closest stars to the Sun, the photometric standard star Vega hosts a two-belt debris disk structure. Together with the fact that its planetary system is being viewed nearly face-on, Vega has been one of the prime targets for planet imaging efforts. Methods. Using the vector vortex coronagraph on Keck/NIRC2 in the Ms band at 4.67 μm, we report the planet detection limits from 1 au to 22 au for Vega with an on-target time of 1.8 h. Results. We reach a 3 MJupiter limit outward of 12 au, which is nearly an order of magnitude deeper than for other existing studies. Combining our observations with existing radial velocity studies, we can confidently rule out the existence of companions more than ~8 MJupiter from 22 au down to 0.1 au for Vega. Interior and exterior to ~4 au, this combined approach reaches planet detection limits down to ~2–3 MJupiter using radial velocity and direct imaging, respectively. Conclusions. By reaching multi-Jupiter mass detection limits, our results are expected to be complemented by the planet imaging of Vega in the upcoming observations using the James Webb Space Telescope to obtain a more holistic understanding of the planetary system configuration around Vega.

Funder

NASA ROSES XRP

European Research Council

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 1 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Vortex fiber nulling for exoplanet observations: implementation and first light;Journal of Astronomical Telescopes, Instruments, and Systems;2023-09-12

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