Southworth, J and Tregloan-Reed, J and Andersen, MI and Novati, SC and Ciceri, S and Colque, JP and D'Ago, G and Dominik, M and Evans, DF and Gu, S-H and Herrera-Cordova, A and Hinse, TC and Jorgensen, UG and Juncher, D and Kuffmeier, M and Mancini, L and Peixinho, N and Popovas, A and Rabus, M and Skottfelt, J and Tronsgaard, R and Unda-Sanzana, E and Wang, X-B and Wertz, O and Alsubai, KA and Andersen, JM and Bozza, V and Bramich, DM and Burgdorf, M and Damerdji, Y and Diehl, C and Elyiv, A and Jaimes, RF and Haugbolle, T and Hundertmark, M and Kains, N and Kerins, E and Korhonen, H and Liebig, C and Mathiasen, M and Penny, MT and Rahvar, S and Scarpetta, G and Schmidt, RW and Snodgrass, C and Starkey, D and Surdej, J and Vilela, C and von Essen, C and Wang, Y (2016) High-precision photometry by telescope defocussing - VIII. WASP-22, WASP-41, WASP-42 and WASP-55. Monthly Notices of the Royal Astronomical Society, 457 (4). 4205 - 4217. ISSN 1365-2966

2016MNRAS.457.4205S.pdf - Published Version

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Item Type: Article
Additional Information: This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2016 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Uncontrolled Keywords: stars, fundamental parameters, WASP-22, WASP-41, WASP-42, WASP-55, planetary systems
Subjects: Q Science > QB Astronomy
Q Science > QC Physics
Divisions: Faculty of Natural Sciences > School of Physical and Geographical Sciences
Related URLs:
Depositing User: Symplectic
Date Deposited: 14 Jun 2016 09:36
Last Modified: 19 Oct 2017 13:11

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