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Table 1:

Log of the VISIR observations of $\ell $ Car and RS Pup. MJD* is the modified Julian date of the start the exposures on the target minus 54 000, and $\phi $ the phase of the Cepheid. The Detector Integration Time (DIT) is given in milliseconds for one BURST image. $\theta $ is the seeing in the visible ( $\lambda=0.5~\mu$m) measured by the observatory DIMM sensor, in arcseconds, and AM is the airmass of the observation. The duration of each observation was 360 s on target.
# MJD* $\phi $ Star Filter DIT $\theta $ AM
a 609.953   HD 76110 PAH1 16 1.5 1.09
b 609.961   HD 76110 PAH2 8 1.4 1.11
c* 609.980 0.53 RS Pup PAH1 16 1.6 1.26
d 609.987 0.53 RS Pup PAH2 8 1.3 1.31
e 610.002 0.26 $\ell $ Car PAH1 16 1.5 1.34
f 610.009 0.26 $\ell $ Car PAH2 8 1.3 1.37
g 610.035   HD 89682 PAH1 16 1.6 1.26
h 610.042   HD 89682 PAH2 8 1.8 1.29
i 610.081   HD 98118 PAH1 16 1.7 1.31
j 610.089   HD 98118 PAH2 8 1.6 1.36
k 610.960   HD 76110 PAH1 16 0.7 1.11
l 610.967   HD 76110 SIC 20 0.9 1.13
m 610.979 0.29 $\ell $ Car PAH1 16 1.0 1.31
n 610.986 0.29 $\ell $ Car SIC 20 0.8 1.32
o 610.998 0.55 RS Pup PAH1 16 0.8 1.38
p* 611.005 0.55 RS Pup SIC 20 0.9 1.44
q 611.016   HD 89682 PAH1 16 0.6 1.23
r 611.024   HD 89682 SIC 20 0.9 1.24
s 611.073   HD 124294 PAH1 16 0.8 1.06
t 611.081   HD 124294 SIC 20 0.8 1.05

* Observations #c and #p suffer from low photometric SNR.


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