Table 1: The sample of objects of the SiO monitoring presented in this paper and the time sampling achieved for each of them.
  coordinates v=1;2  
Name (type1) RA Dec   Av. sampling (days) Num. spectra Figures
  (1950) (1950)   v1;v2 v1;v2  
o Cet (M) 02 16 49.0 -03 12 13   29;41 125;86 5, 8
IK Tau (M) 03 50 43.6 +11 15 32   30;39 116;87 5, 10
TX Cam (M) 04 56 43.0 +56 06 48   31;45 121;66 20*
R Cnc (M) 08 13 48.6 +11 52 52   38;46 60;49 19*
X Hya (M) 09 33 06.7 -14 28 05   39;45 61;48  
R LMi (M) 09 42 35.0 +34 44 34   31;40 119;86 16*
R Leo (M) 09 44 52.2 +11 39 40   32;39 118;87 5, 14*
W Hya (M) 13 46 12.0 -28 07 06   30;38 121;87 18*
U Her (M) 16 23 35.0 +19 00 18   32;38 117;87 21*
R Aql (M) 19 03 57.7 +08 09 08   38;37 61;49 17*
$\chi$ Cyg (M) 19 48 38.4 +32 47 10   36;50 62;45  
R Aqr (M) 23 41 14.0 -15 33 42   32;39 118;85 5, 11*
R Cas (M) 23 55 52.0 +51 06 37   30;41 123;67 5, 15*
IRC+10011 (OH/IR) 01 03 48.0 +12 19 51   33;49 79;59 12*
OH 26.5+0.6 (OH/IR) 18 34 52.5 -05 26 37   40;47 58;48 13*
RT Vir (SR) 13 00 05.8 +05 27 14   31;41 108;64  
GY Aql (SR2) 19 47 25.0 -07 44 30   31;42 119;86 5, 9
VY CMa (SG) 07 20 55.0 -25 40 12   32;42 115;83 2*
VX Sgr (SG) 18 05 03.0 -22 13 55   31;41 117;63 3*
$\mu $ Cep (SG) 21 41 58.5 +58 33 01   34;42 78;61 4*
Orion IRc2 (SFR) 05 32 47.0 -05 24 23   30;41 122;92 1*

$\textstyle \parbox{13.5cm}{
Notes.- $^{1}$\space SG: Supergiant, SR: Semiregula...
...t a
Mira-type behavior. \\
$^{*}$\space These figures available only online.}$


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