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The year-long flux variations in Boyajian's star are asymmetric or aperiodic
Michael Hippke, Daniel Angerhausen, 2018.
What it's used for here
ApJL 854, L11. Cross-calibrates ASAS-SN, ASAS, Kepler, Gaia, SuperWASP and amateur photometry 2006-2017 to the millimagnitude level; the roughly 4 per cent year-long variations cannot be cyclic with a period under 10 years.
Our copy
Research copy, for editors and curators. The work is the publisher's, so readers are sent to it. We keep this copy so the citation can be checked if the page changes or goes.
arxiv.org · fetched 30 Oct 2026
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Cite it
Michael Hippke, & Daniel Angerhausen (2018). The year-long flux variations in Boyajian's star are asymmetric or aperiodic. https://doi.org/10.3847/2041-8213/aaab44
@article{hippke2018yearlong,
author = {Michael Hippke} and {Daniel Angerhausen},
title = {The year-long flux variations in Boyajian's star are asymmetric or aperiodic},
year = {2018},
doi = {10.3847/2041-8213/aaab44},
url = {https://arxiv.org/abs/1710.05000}
}TY - JOUR TI - The year-long flux variations in Boyajian's star are asymmetric or aperiodic AU - Michael Hippke AU - Daniel Angerhausen PY - 2018 DO - 10.3847/2041-8213/aaab44 UR - https://arxiv.org/abs/1710.05000 ER -
and . “The year-long flux variations in Boyajian's star are asymmetric or aperiodic.” 2018. https://doi.org/10.3847/2041-8213/aaab44.