Dr John Taylor j.k.taylor@keele.ac.uk
High-precision photometry by telescope defocussing - VI. WASP-24, WASP-25 and WASP-26
Southworth, John; Hinse, T.C.; Burgdorf, M.; Calchi Novati, S.; Dominik, M.; Galianni, P.; Gerner, T.; Giannini, E.; Gu, S.-H.; Hundertmark, M.; Jørgensen, U.G.; Juncher, D.; Kerins, E.; Mancini, L.; Rabus, M.; Ricci, D.; Schäfer, S.; Skottfelt, J.; Tregloan-Reed, J.; Wang, X.-B.; Wertz, O.; Alsubai, K.A.; Andersen, J.M.; Bozza, V.; Bramich, D.M.; Browne, P.; Ciceri, S.; D'Ago, G.; Damerdji, Y.; Diehl, C.; Dodds, P.; Elyiv, A.; Fang, X.-S.; Finet, F.; Figuera Jaimes, R.; Hardis, S.; Harpsøe, K.; Jessen-Hansen, J.; Kains, N.; Kjeldsen, H.; Korhonen, H.; Liebig, C.; Lund, M.N.; Lundkvist, M.; Mathiasen, M.; Penny, M.T.; Popovas, A.; Prof., S.; Rahvar, S.; Sahu, K.; Scarpetta, G.; Schmidt, R.W.; Schönebeck, F.; Snodgrass, C.; Street, R.A.; Surdej, J.; Tsapras, Y.; Vilela, C.
Authors
T.C. Hinse
M. Burgdorf
S. Calchi Novati
M. Dominik
P. Galianni
T. Gerner
E. Giannini
S.-H. Gu
M. Hundertmark
U.G. Jørgensen
D. Juncher
E. Kerins
L. Mancini
M. Rabus
D. Ricci
S. Schäfer
J. Skottfelt
J. Tregloan-Reed
X.-B. Wang
O. Wertz
K.A. Alsubai
J.M. Andersen
V. Bozza
D.M. Bramich
P. Browne
S. Ciceri
G. D'Ago
Y. Damerdji
C. Diehl
P. Dodds
A. Elyiv
X.-S. Fang
F. Finet
R. Figuera Jaimes
S. Hardis
K. Harpsøe
J. Jessen-Hansen
N. Kains
H. Kjeldsen
H. Korhonen
C. Liebig
M.N. Lund
M. Lundkvist
M. Mathiasen
M.T. Penny
A. Popovas
S. Prof.
S. Rahvar
K. Sahu
G. Scarpetta
R.W. Schmidt
F. Schönebeck
C. Snodgrass
R.A. Street
J. Surdej
Y. Tsapras
C. Vilela
Abstract
We present time series photometric observations of 13 transits in the planetary systems WASP-24, WASP-25 and WASP-26. All three systems have orbital obliquity measurements, WASP-24 and WASP-26 have been observed with Spitzer, and WASP-25 was previously comparatively neglected. Our light curves were obtained using the telescope-defocussing method and have scatters of 0.5–1.2 mmag relative to their best-fitting geometric models. We use these data to measure the physical properties and orbital ephemerides of the systems to high precision, finding that our improved measurements are in good agreement with previous studies. High-resolution Lucky Imaging observations of all three targets show no evidence for faint stars close enough to contaminate our photometry. We confirm the eclipsing nature of the star closest to WASP-24 and present the detection of a detached eclipsing binary within 4.25 arcmin of WASP-26.
Citation
Southworth, J., Hinse, T., Burgdorf, M., Calchi Novati, S., Dominik, M., Galianni, P., …Vilela, C. (2014). High-precision photometry by telescope defocussing - VI. WASP-24, WASP-25 and WASP-26. Monthly Notices of the Royal Astronomical Society, 444(1), 776 -789. https://doi.org/10.1093/mnras/stu1492
Journal Article Type | Article |
---|---|
Acceptance Date | Jul 23, 2014 |
Online Publication Date | Aug 20, 2014 |
Publication Date | Oct 11, 2014 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Oxford University Press |
Peer Reviewed | Peer Reviewed |
Volume | 444 |
Issue | 1 |
Pages | 776 -789 |
DOI | https://doi.org/10.1093/mnras/stu1492 |
Keywords | stars: fundamental parameters, planetary systems, stars: individual: WASP-24, stars: individual: WASP-25, stars: individual: WASP-26 |
Publisher URL | http://dx.doi.org/10.1093/mnras/stu1492 |
Files
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