Stellar activity observed by the Kepler Space Telescope. The M dwarf of the Kepler-32 system with five orbiting planets

2013 ◽  
Vol 57 (10) ◽  
pp. 757-765 ◽  
Author(s):  
I. S. Savanov ◽  
E. S. Dmitrienko
2011 ◽  
Vol 55 (10) ◽  
pp. 890-895 ◽  
Author(s):  
I. S. Savanov ◽  
E. S. Dmitrienko

2012 ◽  
Vol 56 (2) ◽  
pp. 116-123 ◽  
Author(s):  
I. S. Savanov ◽  
E. S. Dmitrienko

2021 ◽  
Vol 161 (4) ◽  
pp. 172
Author(s):  
Serge B. Dieterich ◽  
Andrew Simler ◽  
Todd J. Henry ◽  
Wei-Chun Jao

2020 ◽  
Vol 498 (1) ◽  
pp. 33-43
Author(s):  
R Ridden-Harper ◽  
B E Tucker ◽  
M Gully-Santiago ◽  
G Barentsen ◽  
A Rest ◽  
...  

ABSTRACT The K2 mission of the Kepler Space Telescope offers a unique possibility to examine sources of both Galactic and extragalactic origin with high-cadence photometry. Alongside the multitude of supernovae and quasars detected within targeted galaxies, it is likely that Kepler has serendipitously observed many transients throughout K2. Such events will likely have occurred in background pixels, coincidentally surrounding science targets. Analysing the background pixels presents the possibility to conduct a high-cadence survey with areas of a few square degrees per campaign. We demonstrate the capacity to independently recover key K2 transients such as KSN 2015K and SN 2018oh. With this survey, we expect to detect numerous transients and determine the first comprehensive rates for transients with lifetimes of ≤1 d.


2014 ◽  
Vol 445 (3) ◽  
pp. 2810-2817 ◽  
Author(s):  
E. Plachy ◽  
J. M. Benkő ◽  
Z. Kolláth ◽  
L. Molnár ◽  
R. Szabó

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