A search for variability in exoplanet analogues and low-gravity brown dwarfs
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Issue Date
2018-11-22Author
Vos, Johanna M.
Biller, Beth A.
Bonavita, Mariangela
Eriksson, Simon
Liu, Michael C.
Best, William M. J.
Metchev, Stanimir
Radigan, Jacqueline
Allers, Katelyn N.
Janson, Markus
Buenzli, Esther
Dupuy, Trent J.
Bonnefoy, Mickaël
Manjavacas, Elena
Brandner, Wolfgang
Crossfield, Ian
Deacon, Niall
Henning, Thomas
Homeier, Derek
Kopytova, Taisiya
Schlieder, Joshua
Publisher
Royal Astronomical Society
Type
Article
Article Version
Scholarly/refereed, publisher version
Rights
Copyright 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society
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Show full item recordAbstract
We report the results of a J-band survey for photometric variability in a sample of young, low-gravity objects using the New Technology Telescope (NTT) and the United Kingdom Infrared Telescope (UKIRT). Surface gravity is a key parameter in the atmospheric properties of brown dwarfs and this is the first large survey that aims to test the gravity dependence of variability properties. We do a full analysis of the spectral signatures of youth and assess the group membership probability of each target using membership tools from the literature. This results in a 30 object sample of young low-gravity brown dwarfs. Since we are lacking in objects with spectral types later than L9, we focus our statistical analysis on the L0–L8.5 objects. We find that the variability occurrence rate of L0–L8.5 low-gravity brown dwarfs in this survey is 30+16−8 per cent. We reanalyse the results of Radigan (2014) and find that the field dwarfs with spectral types L0–L8.5 have a variability occurrence rate of 11+13−4 per cent. We determine a probability of 98 per cent that the samples are drawn from different distributions. This is the first quantitative indication that the low-gravity objects are more likely to be variable than the field dwarf population. Furthermore, we present follow-up JS and KS observations of the young, planetary-mass variable object PSO 318.5–22 over three consecutive nights. We find no evidence of phase shifts between the JS and KS bands and find higher JS amplitudes. We use the JS light curves to measure a rotational period of 8.45 ± 0.05 h for PSO 318.5–22.
Description
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2018 [The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
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Citation
Johanna M Vos, Beth A Biller, Mariangela Bonavita, Simon Eriksson, Michael C Liu, William M J Best, Stanimir Metchev, Jacqueline Radigan, Katelyn N Allers, Markus Janson, Esther Buenzli, Trent J Dupuy, Mickaël Bonnefoy, Elena Manjavacas, Wolfgang Brandner, Ian Crossfield, Niall Deacon, Thomas Henning, Derek Homeier, Taisiya Kopytova, Joshua Schlieder, A search for variability in exoplanet analogues and low-gravity brown dwarfs, Monthly Notices of the Royal Astronomical Society, Volume 483, Issue 1, February 2019, Pages 480–502, https://doi.org/10.1093/mnras/sty3123
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