Flexible GN&C architecture enables an innovative control solution to repurpose the Kepler Space Telescope

2016 ◽  
Author(s):  
Dustin Putnam ◽  
Doug Wiemer ◽  
Ian Gravseth
Keyword(s):  
Control Solution ◽  
Space Telescope ◽  
Kepler Space Telescope

scholarly journals K2: Background Survey – the search for undiscovered transients in Kepler/K2 data

2020 ◽  
Vol 498 (1) ◽  
pp. 33-43
Author(s):  
R Ridden-Harper ◽  
B E Tucker ◽  
M Gully-Santiago ◽  
G Barentsen ◽  
A Rest ◽  
...  
Keyword(s):  
Space Telescope ◽  
Unique Possibility ◽  
High Cadence ◽  
Kepler Space Telescope

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.

scholarly journals Non-linear dynamical analysis of the Blazhko effect with the Kepler space telescope: the case of V783 Cyg

2014 ◽  
Vol 445 (3) ◽  
pp. 2810-2817 ◽  
Author(s):  
E. Plachy ◽  
J. M. Benkő ◽  
Z. Kolláth ◽  
L. Molnár ◽  
R. Szabó
Keyword(s):  
Dynamical Analysis ◽  
Space Telescope ◽  
Non Linear ◽  
Blazhko Effect ◽  
Kepler Space Telescope

The Spots and Activity of Stars in the Beehive Cluster Observed by the Kepler Space Telescope (K2)

2018 ◽  
Vol 62 (5) ◽  
pp. 352-358
Author(s):  
I. S. Savanov ◽  
E. S. Kalinicheva ◽  
E. S. Dmitrienko
Keyword(s):  
Space Telescope ◽  
Kepler Space Telescope
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