Table 1
Spitzer light curves used in this work.
| Program | AOR | Start | IRAC band | N p | Baseline | BLISS | BLISS | β w | β r | |
| ID | ID | date | (μm) | model | N x | N y | ||||
|
|
||||||||||
| 542 | 39218176 | 2010 Apr. 26 | 3.6 | 101 |
|
0 | 0 | 0.92 | 1.06 | |
| 542 | 39217920 | 2010 Apr. 27 | 4.5 | 103 | p([xy] 2 + l2) | 0 | 0 | 0.85 | 1.20 | |
| 70148 | 40216832 | 2010 Oct. 16 | 3.6 | 110 |
|
0 | 0 | 0.93 | 1.56 | |
| 70148 | 40217088 | 2010 Oct. 17 | 4.5 | 109 |
|
0 | 0 | 0.85 | 1.33 | |
| 70148 | 40217344 | 2010 Oct. 25 | 3.6 | 109 |
|
0 | 0 | 0.66 | 1.15 | |
| 70148 | 40217600 | 2010 Oct. 27 | 4.5 | 109 |
|
0 | 0 | 1.04 | 1.05 | |
| 70148 | 40217856 | 2010 Oct. 28 | 3.6 | 110 | p([xy] 2 + l2) | 0 | 0 | 0.93 | 1.00 | |
| 70148 | 40211882 | 2010 Oct. 31 | 4.5 | 109 |
|
0 | 0 | 0.96 | 1.59 | |
| 70049 | 42045952 | 2011 Apr. 29 | 4.5 | 666 |
|
10 | 11 | 0.93 | 1.17 | |
| 70049 | 42046208 | 2011 Apr. 30 | 4.5 | 667 |
|
11 | 10 | 0.99 | 1.20 | |
| 70049 | 42046464 | 2011 May 1 | 4.5 | 597 |
|
9 | 9 | 0.98 | 1.37 | |
| 70049 | 42046720 | 2011 May 2 | 4.5 | 663 |
|
9 | 10 | 0.99 | 1.15 | |
| 70049 | 42046976 | 2011 May 3 | 4.5 | 667 |
|
10 | 9 | 0.96 | 1.40 | |
| 70049 | 42047232 | 2011 May 4 | 4.5 | 610 |
|
10 | 9 | 0.94 | 1.19 | |
| 70049 | 42047488 | 2011 May 5 | 4.5 | 665 |
|
9 | 10 | 0.92 | 1.17 | |
| 70049 | 42047744 | 2011 May 6 | 4.5 | 667 |
|
9 | 9 | 0.87 | 1.07 | |
| 70049 | 42048000 | 2011 May 7 | 4.5 | 472 |
|
8 | 8 | 0.93 | 1.74 | |
| 70049 | 42048256 | 2011 May 8 | 4.5 | 667 | p([xy] 2) | 10 | 9 | 0.94 | 1.03 | |
| 70049 | 42048512 | 2011 May 9 | 4.5 | 666 |
|
10 | 9 | 0.98 | 1.21 | |
| 70049 | 42048768 | 2011 May 10 | 4.5 | 667 |
|
10 | 10 | 0.98 | 1.81 | |
| 70049 | 42049280 | 2011 May 11 | 4.5 | 666 |
|
9 | 9 | 0.89 | 1.18 | |
| 70049 | 42049536 | 2010 May 12 | 4.5 | 112 |
|
0 | 0 | 0.91 | 1.16 | |
| 70049 | 42050048 | 2011 May 14 | 4.5 | 655 |
|
10 | 9 | 0.98 | 1.77 | |
| 70049 | 42050304 | 2011 May 15 | 4.5 | 667 |
|
10 | 10 | 0.95 | 1.16 | |
| 70049 | 42050560 | 2011 May 16 | 4.5 | 583 |
|
10 | 9 | 0.83 | 1.27 | |
| 70049 | 42050816 | 2011 May 17 | 4.5 | 667 |
|
11 | 10 | 0.90 | 1.45 | |
| 70049 | 42051072 | 2011 May 18 | 4.5 | 667 |
|
10 | 10 | 0.89 | 1.12 | |
| 70049 | 42051328 | 2011 May 19 | 4.5 | 639 |
|
10 | 9 | 0.89 | 1.67 | |
| 70049 | 44591872 | 2011 Nov. 6 | 3.6 | 660 |
|
11 | 10 | 0.89 | 1.54 | |
| 70049 | 44592128 | 2011 Nov. 7 | 3.6 | 443 |
|
7 | 8 | 0.82 | 1.29 | |
Notes. Each light curve corresponds to a specific Spitzer observing block (AOR). For each of them, the table gives the ID of the Spitzer program and of the AOR, the start date, the IRAC channel used, the number of measurements, the baseline function selected for our global modeling (see Sect. 3), the number of divisions in the x- and y-directions used for the BLISS pixel mapping (see Sect. 3), and the βw and βr error rescaling factors (see Sect. 3). For the baseline function, p(ϵN) denotes, respectively, a N-order polynomial function of the logarithm of time (ϵ = l), of the PSF x- and y-positions (ϵ = [xy]), and widths (ϵ = wx & wy).
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