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A search for transiting companions in the J1407 (V1400 Cen) system
- Source :
- Astronomy & Astrophysics, 652, 1-8
- Publication Year :
- 2021
- Publisher :
- arXiv, 2021.
-
Abstract
- In 2007, the young star 1SWASP J140747.93-394542.6 (V1400 Cen) underwent a complex series of deep eclipses over 56 days. This was attributed to the transit of a ring system filling a large fraction of the Hill sphere of an unseen substellar companion. Subsequent photometric monitoring has not found any other deep transits from this candidate ring system, but if there are more substellar companions and they are coplanar with the potential ring system, there is a chance that they will transit the star as well. This young star is active and the light curves show a 5% modulation in amplitude with a dominant rotation period of 3.2 days due to star spots rotating in and out of view. We model and remove the rotational modulation of the J1407 light curve and search for additional transit signatures of substellar companions orbiting around J1407. We combine the photometry of J1407 from several observatories, spanning a 19 year baseline. We remove the rotational modulation by modeling the variability as a periodic signal, whose periodicity changes slowly with time over several years due to the activity cycle of the star. A Transit Least Squares (TLS) analysis searches for any periodic transiting signals within the cleaned light curve. We identify an activity cycle of J1407 with a period of 5.4 years. A Transit Least Squares search does not find any plausible periodic eclipses in the light curve, from 1.2% amplitude at 5 days up to 1.9% at 20 days. This sensitivity is confirmed by injecting artificial transits into the light curve and determining the recovery fraction as a function of transit depth and orbital period. J1407 is confirmed as a young active star with an activity cycle consistent with a rapidly rotating solar mass star. With the rotational modulation removed, the TLS analysis rules out transiting companions with radii larger than about 1 Jupiter.<br />Comment: 8 pages, 9 figures, 3 tables, accepted for publication in Astronomy & Astrophysics. Reduced data and reduction scripts on github at https://github.com/StanBarmentloo/J1407_transit_search_activity
- Subjects :
- Stars: activity
Rotation period
010504 meteorology & atmospheric sciences
FOS: Physical sciences
Astrophysics
01 natural sciences
Planets and satellites: rings
Photometry (optics)
0103 physical sciences
Astrophysics::Solar and Stellar Astrophysics
Transit (astronomy)
010303 astronomy & astrophysics
Astrophysics::Galaxy Astrophysics
Solar and Stellar Astrophysics (astro-ph.SR)
0105 earth and related environmental sciences
Physics
Earth and Planetary Astrophysics (astro-ph.EP)
Solar mass
Starspot
Astronomy and Astrophysics
Planets and satellites: detection
Light curve
Dynamo
Exoplanet
Astrophysics - Solar and Stellar Astrophysics
Space and Planetary Science
Hill sphere
Astrophysics::Earth and Planetary Astrophysics
Astrophysics - Earth and Planetary Astrophysics
Subjects
Details
- Database :
- OpenAIRE
- Journal :
- Astronomy & Astrophysics, 652, 1-8
- Accession number :
- edsair.doi.dedup.....8c5dfa3d8d2b24ad8ed36e5ff5a61503
- Full Text :
- https://doi.org/10.48550/arxiv.2106.15902