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Table 1

Photometric datasets on WASP-33.

LC# Date [UT] N FIL Source LC# Date [UT] N FIL Source

01 2003–2007 2285 I HATNet 23X 2011-10-13 505 J Kitt Peak
02X 2010-03-03 275 z FLWO 24 2011-10-23 96 C LTremosa
03 2010-08-23 245 R KHose 25 2011-11-12 291 I Konkoly
04 2010-08-26 282 R FHormuth 26 2011-11-12 79 V GCorfini
05 2010-08-26 163 R RNaves 27 2011-11-14 907 V SDvorak
06 2010-09-17 220 R TScarmato 28X 2011-11-23 404 R JGaitan
07 2010-09-28 277 R EHerrero 29X 2011-11-23 127 R RNaves
08X 2010-10-11 598 B WDauberman 30 2011-11-24 446 I Konkoly
09X 2010-10-15 191 R RNaves 31X 2011-11-24 177 V RNaves
10 2010-10-20 434 R CLopresti 32 2011-12-01 888 I TDax
11 2010-10-20 138 R RNaves 33 2011-12-10 146 C FGarcia
12 2010-11-03 451 z Kitt Peak 34 2011-12-15 109 I JGaitan
13 2010-11-19 863 V SDvorak 35X 2011-12-20 149 V DGorshanov
14 2010-12-06 1254 C SShadick 36 2011-12-21 134 V RNaves
15 2010-12-25 440 C AMaurice 37 2011-12-27 230 C JLopesino
16 2011-01-05 437 C CWiedemair 38X 2012-01-01 113 V RNaves
17 2011-01-13 778 V SDvorak 39X 2012-01-01 420 C JLopesino
18 2011-01-16 238 C SGajdos 40 2012-01-09 316 I SShadick
19 2011-09-21 311 I SShadick 41 2012-01-12 130 V RNaves
20 2011-09-24 468 C LBrat 42 2012-01-20 534 I SShadick
21X 2011-10-05 196 R RNaves 43 2012-02-11 365 I SShadick
22 2011-10-13 310 Hα Kitt Peak

Notes. Header: LC#: light curve identification number used in this paper; Date: starting date of the observations; N: number of data points (may differ from those given at the ETD site, e.g., because of multiple items); FIL: filter used in the observation (“C” indicates that no filter was used); Source: observer or observatory name. Plots of these light curves are presented in the main body of the paper and in the Appendix. Light curves labeled by “X” are not used in the analysis presented in this paper. They exhibit the following peculiarities. #02: partial transit, difficulties in trend filtering; #08: the transit is deep; #09: deep and skewed transit; #21: deep and skewed transit; #23: near infrared “J” filter is used; #28: large oscillations, earlier and narrower transit (the difference appears to be 28 min!); #29: large oscillations, same night observation as that of #28 but no apparent severe shift in the transit center; #31: deep and skewed transit, is in conflict with the regular behavior observed on the same night (see #30); #35: deeper by >50% than the average transit; #38: deep blip after the ingress; #39: deep blip after the ingress (the same night event as #38).

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