What it's used for here
arXiv:2607.20643 (July 2026). Models the symmetric 1.1 per cent dip in TESS Sector 15 (September 2019) as a planetary transit and combines it with archival and new radial velocities: a 2.3-sigma companion of about 9 Jupiter masses and 1.7 Jupiter radii with a period of at least about 1030 days, in several allowed period windows. Independently recovered in this department's TESS search.
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arxiv.org · fetched 30 Oct 2026
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Cited by on this site 2 records
Cite it
Cristina Madurga-Favieres, & et al. (2026). Evidence for a giant companion orbiting Tabby's star. https://arxiv.org/abs/2607.20643
@article{madurga2026evidence,
author = {Cristina Madurga-Favieres} and {et al.},
title = {Evidence for a giant companion orbiting Tabby's star},
year = {2026},
url = {https://arxiv.org/abs/2607.20643}
}TY - GEN TI - Evidence for a giant companion orbiting Tabby's star AU - Cristina Madurga-Favieres AU - et al. PY - 2026 UR - https://arxiv.org/abs/2607.20643 ER -
and . “Evidence for a giant companion orbiting Tabby's star.” 2026.