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Home All issues Volume 565 (May 2014) A&A, 565 (2014) A127 Full HTML
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Table 3

Summary of our three years of monitoring with the Onsala telescope.

Source 08-12-12 09-03-17 09-08-13 09-11-07 10-01-08 10-12-06 11-03-06 11-04-22 11-05-18 11-06-15 11-10-30 11-12-09
IRC+10011 v1 9.6 3.6 2.9 3.0 3.1 1.9 1.6 1.5 2.1 5.3 6.1
v2 4.8 4.1 4.1 6.0 3.5 3.1 3.8 4.8 7.5 8.4
v3 2.6 <0.6 0.3 0.2 0.9 0.6 0.4 0.6 0.7 2.8 2.4
o Cet v1 13.8 2.0 34.8 45.6 39.3 12.9 3.1 3.1 3.5 27.7 19.3
v2 5.6 14.1 33.3 30.8 7.3 3.1 2.1 2.4 26.0 17.2
v3 <0.3 <0.6 <0.2 <0.2 <0.2 <0.15 <0.3 <0.2 <0.2 <0.2 <0.2
IK Tau v1 26.8 17.5 14.2 14.4 5.5 8.1 7.0 7.6 8.1 14.7 10.7
v2 16.7 13.3 16.5 6.7 5.2 6.0 8.0 7.6 14.8 9.5
v3 2.6 <0.4 <0.2 0.4 <0.2 0.15 0.5 0.9 1.7 2.2 0.9
U Ori v1 9.0 2.1 1.8 1.7 0.8 9.2 8.4 6.3 4.6 1.7 1.3
v2 2.5 1.0 2.1 5.0 11.7 9.9 6.3 4.0 1.1 0.7
v3 1.3 <0.6 <0.2 <0.2 <0.2 0.2 0.2 <0.2 <0.15 <0.15 <0.15
TX Cam v1 8.2 4.0 5.5 4.1 12.6 2.5 4.4 2.1 2.4 4.3 6.2 4.1
v2 1.5 7.9 15.5 4.4 6.0 5.7 6.3 6.2 10.4 6.3
v3 0.4 <0.15 <0.6 0.25 1.2 <0.1 <0.1 <0.1 <0.1 0.2 0.3 0.2
V Cam v1 1.5 1.2 1.0 1.4 1.6 0.7 0.5 0.5 0.7 0.6 0.7
v2 1.3 1.1 1.0 2.3 1.0 0.8 0.6 0.6 1.2 1.3
v3 <0.2 <0.2 <0.1 <0.15 <0.1 <0.1 <0.1 <0.1 <0.1 0.3 0.6
R Leo v1 2.3 30.2 40.4 28.0 8.3 20.4 25.9 25.7 24.0 19.1 19.0
v2 38.6 51.9 21.8 6.9 12.1 4.0 14.0 16.0 29.4 25.3
v3 0.4 5.6 4.4 <0.2 <0.1 0.7 <0.1 <0.1 0.2 <0.2 0.4
R LMi v1 8.1 10.8 2.2 4.9 7.7 4.6 4.0 3.1 3.6 2.9 2.0 3.0
v2 4.9 3.3 5.7 1.4 2.2 1.6 2.0 2.1 6.3 9.1
v3 0.7 1.1 <0.4 <0.15 0.2 <0.1 <0.1 <0.1 <0.1 <0.1 <0.1 <0.1
U Her v1 8.9 2.8 10.3 9.3 20.3 36.2 28.6 22.2 19.5 24.1 27.1
v2 5.6 14.2 13.4 21.2 36.5 28.3 22.1 20.2 23.1 23.7
v3 0.3 <0.4 1.8 3.4 4.7 6.0 3.3 1.2 <0.1 <0.1 <0.15
RR Aql v1 1.8 2.8 1.4 1.6 0.9 1.5 1.6 1.6 1.5 0.8 0.7
v2 2.2 0.5 1.2 0.7 1.2 2.0 1.7 1.6 0.6 0.7
v3 <0.2 <0.6 <0.2 0.2 <0.2 <0.2 <0.2 <0.2 <0.2 <0.2 <0.15
μ Cep v1 <0.6 2.26 1.4 1.0 1.5 1.6 1.4 1.3 1.3 1.1 0.6
v2 2.4 1.4 1.1 1.1 0.8 0.7 0.8 1.0 0.9 0.7
v3 <0.2 <0.15 0.2 0.2 <0.1 <0.1 0.1 <0.1 <0.1 <0.1 <0.1
R Cas v1 6.8 31.2 8.7 5.4 6.0 4.4 8.8 17.0 19.6 26.9 26.2 15.9
v2 11.1 11.2 17.1 2.8 6.5 18.6 29.1 31.1 22.8 19.5
v3 1.3 4.6 <0.5 <0.15 <0.15 <0.1 <0.1 0.2 1.0 1.8 2.6 1.2
Y Cas v1 2.8 1.7 0.7 0.9 0.9 1.1 1.2 1.7 2.7 2.9 2.1
v2 1.3 0.9 1.1 0.8 1.0 1.8 1.9 1.7 1.9 1.2
v3 <0.2 <0.4 <0.15 0.1 <0.1 0.1 0.2 0.3 0.3 0.2 <0.1
W And v1 0.6 0.6 0.2 0.4 1.3 0.2 0.14 0.2 0.3 0.6 0.4
v2 0.7 0.5 0.4 1.3 0.3 <0.1 0.2 0.2 0.5 0.5
v3 0.4 <0.4 <0.15 <0.2 <0.1 <0.1 <0.1 <0.1 <0.1 <0.1 <0.1
R Cnc v1 2.8 3.1 3.2 1.2 2.5 0.8 1.7 1.7 1.6 2.7 1.6
v2 7.2 6.1 3.3 1.1 1.0 1.3 0.8 0.6 0.9 1.2
v3 <0.2 <0.5 <0.2 <0.2 <0.1 <0.1 <0.15 <0.1 <0.15 <0.15 <0.2
RU Her v1 <0.5 1.7 3.9 5.6 1.6 1.6 1.9 1.5 1.7 0.3 0.3
v2 4.2 6.7 5.9 1.7 1.3 1.1 0.8 0.9 0.3 0.3
v3 <0.2 <0.5 1.4 1.1 <0.4 <0.1 <0.1 <0.1 <0.1 <0.1 <0.1
GY Aql v1 <0.1 2.0 0.7 <0.2 6.6 3.7 2.9 2.3 2.6 5.8 10.2
v2 2.5 1.7 0.9 5.5 3.1 2.3 2.5 2.4 6.1 5.5
v3 <0.3 <0.5 <0.2 <0.2 <0.15 <0.12 <0.2 <0.2 <0.2 0.3 0.4
R Aql v1 l0.2 6.4 3.7 1.3 1.6 1.4 2.6 5.1 6.6 7.3 5.0
v2 11.2 2.6 0.9 3.8 5.9 10.7 7.5 6.6 5.8 4.5
v3 <0.2 <0.5 <0.2 <0.2 0.6 0.2 <0.2 <0.15 <0.1 <0.1 <0.15
χ Cyg v1 2.1 <0.5 0.5 2.9 3.2 5.2 5.1 5.2 4.9 1.5 1.3
v2 <0.5 0.4 0.8 <0.1 0.16 <0.15 0.2 0.2 0.5 1.5
v3 <0.2 <0.5 <0.15 <0.15 <0.2 <0.1 <0.15 <0.1 0.1 <0.1 <0.1

Notes. For each epoch (date format YY-MM-DD), we indicate the peak flux or, in the case of no detection, the upper limit. Bold face values are the closest observations in time to our VLBA observations.

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