Published data for transiting extrasolar planets


 

The data available here have been presented in my papers on transiting extrasolar planets. The data format is text files containing HJD or BJD (usually minus 2400000), differential magnitude and magnitude error. Note that the photometry presented here was obtained using telescope defocussing techniques.

Target Files N(data) Comments
HAT-P-5 Loiano (Gunn r filter)
Calar Alto (u,g,r,I filters)
311
204
Published by Southworth et al. (2012MNRAS.422.3099S).
HAT-P-13 Loiano (i filter)
Portalegre (I filter)
274
247
Published by Southworth et al. (2012MNRAS.420.2580S).
WASP-2 DK 1.5m (R filter)
Loiano (r filter)
Times of transit midpoint
211
63
28
Published by Southworth et al. (2010MNRAS.408.1680S).
WASP-4 DK 1.5m (R filter) 452 Published by Southworth et al. (2009MNRAS.399..287S).
Please note that the absolute values of the timestamps are wrong, but the relative values are reliable.
WASP-5 DK 1.5m (R filter) 181 Published by Southworth et al. (2009MNRAS.396.1023S).
Please note that the absolute values of the timestamps are wrong, but the relative values are reliable.
WASP-7 DK 1.5m (I filter) 217 Published by Southworth et al. (2011A+A...527A...8S).
WASP-15 GROND (griz passbands)
DK 1.5m (R filter)
229 g, 225 r, 228 i, 227 z, 92 R Published by Southworth et al. (2013MNRAS.434.1300S).
WASP-16 DK 1.5m (R filter) 355 Published by Southworth et al. (2013MNRAS.434.1300S).
WASP-17 DK 1.5m (R filter) 494 Published by Southworth et al. (2012MNRAS.426.1338S).
WASP-18 DK 1.5m (V filter) 629 Published by Southworth et al. (2009ApJ...707..167S).
Please note that the absolute values of the timestamps are wrong, but the relative values are reliable.
WASP-19 NTT 3.6m (Hellier)
NTT 3.6m (Tregloan-Reed)
NTT 3.6m (unpublished)
74
218
60
The data for the night of 2010/01/27 were published by Hellier et al. (2012MNRAS.426.1338S). The data for the nights of 2010/01/23 and 2010/01/24 were published by Tregloan-Reed et al. (2013MNRAS.428.3671T). One additional night's data (2010/01/28) is included here but has not been published because systematic noise makes it unreliable.
WASP-22 DK 1.5m and T82 674 (DK)
578 (T82)
Published by Southworth et al. (2016MNRAS.457.4205S).
WASP-24 DK 1.5m (R filter)
DK 1.5m (I filter)
347 (R)
422 (I)
Published by Southworth et al. (2014MNRAS.444..776S).
WASP-25 DK 1.5m (R filter) 384 Published by Southworth et al. (2014MNRAS.444..776S).
WASP-26 DK 1.5m (I filter) 891 Published by Southworth et al. (2014MNRAS.444..776S).
WASP-41 DK 1.5m and T82 628 (DK)
282 (T82)
Published by Southworth et al. (2016MNRAS.457.4205S).
WASP-42 DK 1.5m 468 Published by Southworth et al. (2016MNRAS.457.4205S).
WASP-50 NTT 3.6m (r filter) 251 Published by Tregloan-Reed & Southworth (2013MNRAS.431..966T).
WASP-55 DK 1.5m 540 Published by Southworth et al. (2016MNRAS.457.4205S).
WASP-57 all data (u, g, r, i, z, R, bb filters) 251 Published by Southworth et al. (2015MNRAS.454.3094S).
WASP-103 all data (r, I, g, r, i, z filters) 2190 Published by Southworth et al. (2015MNRAS.447..711S).

 

 

 

 

 

 

 


Last modified: 2016/03/02           John Southworth (Keele University, UK)