activity
19992026
most citedThe WASP Project and the SuperWASP Cameras

1.2k citations · 17.1k across the 247 of their papers we have counts for

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Showing 2022Show all

12 papers · 1 filter

astro-ph.EP2022★ 19 cited

Limb darkening measurements from TESS and Kepler light curves of transiting exoplanets

P. F. L. Maxted

Inaccurate limb-darkening models can be a significant source of error in the analysis of the light curves for transiting exoplanet and eclipsing binary star systems. To test the ac…

astro-ph.EP2022★ 8 cited

Discovery of TOI-1260d and the characterisation of the multi-planet system

Kristine W. F. Lam, J. Cabrera, M. J. Hooton +83

We report the discovery of a third planet transiting the star TOI-1260, previously known to host two transiting sub-Neptune planets with orbital periods of 3.127 and 7.493 days, re…

astro-ph.SR2022★ 8 cited

Fundamental effective temperature measurements for eclipsing binary stars -- II. The detached F-type eclipsing binary CPD-54 810

N. J. Miller, P. F. L. Maxted, D. Graczyk +2

CPD-54 810 is a double-lined detached eclipsing binary containing two mid-F type dwarfs on an eccentric 26-day orbit. We perform a combined analysis of the extensive photometry obt…

astro-ph.SR2022

Revised Temperatures For Two Benchmark M-dwarfs -- Outliers No More

David V. Martin, Tayt Armitage, Alison Duck +7

Well-characterised M-dwarfs are rare, particularly with respect to effective temperature. In this letter we re-analyse two benchmark M-dwarfs in eclipsing binaries from Kepler/K2:…

astro-ph.EP2022★ 29 cited

TOI-836: A super-Earth and mini-Neptune transiting a nearby K-dwarf

Faith Hawthorn, Daniel Bayliss, Thomas G. Wilson +137

We present the discovery of two exoplanets transiting TOI-836 (TIC 440887364) using data from TESS Sector 11 and Sector 38. TOI-836 is a bright ( mag), high proper motion…

astro-ph.SR2022★ 8 cited

Surface brightness-colour relations of dwarf stars from detached eclipsing binaries -- I. Calibrating sample

D. Graczyk, G. Pietrzyński, C. Galan +19

Surface brightness -- colour relations (SBCRs) are very useful tools for predicting the angular diameters of stars. They offer the possibility to calculate very precise spectrophot…