Observations
| Object(s) | Instrument(s) | Date(s) | Aim(s) | Results |
| κ1 Ceti (young active nearby solar-like star, G5 class) | LOFAR (dynamic radio spectra in the 115-190 MHz range) + AZT-11 (optical photometry) | 5-7 October 2018 | Search for flares and/or CMEs | |
| AT Mic (a system of active red dwarfs, M4.5+M4.5 class) | AstroSat (X-ray observations in the range from 0.3 to 150 keV + UV/EUV observations) | Not set yet (October 2018 – September 2019) | Search for flares | |
| EV Lac (active red dwarf, M4 class) AD Leo (active red dwarf, M3.5 class) CN Leo (active red dwarf, M6 class) DG CVn (active red dwarf, M4 class) YZ CMi (active red dwarf, M4 class) 61 Cyg (a system of active K dwarfs, K5+K7 class) |
RATAN-600 (radio observations in the 3-30 GHz range) | 1-17 August 2018, 16-29 November 2018 |
Search for flares |
Targets of interest
|
Spectral class |
Objects |
|
M4-M7 |
1. EV Lac 2. AD Leo 3. DG CVn 4. YZ CMi |
|
M0-M3 |
1. HD 95735 2. AU Mic 3. FK Aqr 4. YY Gem |
|
K4-K8 |
(one or two targets depending on the field of view) 2. CC Eri 3. BY Dra 4. EQ Vir |
|
K0-K3 |
1. eps Eri 2. 70 Oph 3. V538 Aur 4. LQ Hya |
|
G0-G9 |
1. ksi Boo 2. kap01 Cet 3. pi01 UMa 4. EK Dra |
The selection criteria were:
1. High activity, to ensure the high probability of the flare detection. (It is increases with the decrease of the star's temperature).
2. Possible close proximity to the Earth.
3. "Normal" stars: trying to exclude the interacting binaries and T Tauris.