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Details for Revision 1
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Name
  KID 06543674  
AAVSO UID
--  
Constellation
Cygnus Sequence
J2000.0
19 50 09.98 +41 57 03.2  (297.54158 +41.95089) Search nearby
B1950.0 19 48 29.49 +41 49 23.0
Galactic coord. 76.356 +7.878
Other names

(Internal only)
Please note that aliases shown in grey link to obsolete records.
2MASS J19500997+4157033 KIC 06543674 KIC 06543683
KID 06543682 KID 06543683  
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Variability type
EA
Spectral type --
Mag. range
13.483 - ? R
Discoverer --
Epoch
28 Jun 2009 (HJD 2455010.7355) Ephemeris
Outburst --
Period 2.39083 d
Rise/eclipse dur. --
Remarks
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1 Otero, Sebastian Alberto The entry KID 06543682 also shows the EA variability with almost the same amplitude but it is an artifact since the real star at that position (2MASS J19501051+4157057 at 19 50 10.51 +41 57 05.7, sep. 6".1) is almost 4 mag. fainter than the eclipsing binary.
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References
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1 R.W. Slawson et al., 2011, arXiv:1103.1659v1 [astro-ph.SR] 2011arXiv1103.1659S
2 R.W. Slawson et al., 2011, arXiv:1103.1659v1 [astro-ph.SR] (Light curve) 2011arXiv1103.1659S
3 A. Prsa et al., 2010, arXiv:1006.2815v1 [astro-ph.SR] 2010arXiv1006.2815P
4 A. Prsa et al., 2010, arXiv:1006.2815v1 [astro-ph.SR] (Light curve) 2010arXiv1006.2815P
5 Kepler data (MAST) --
External Links
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Supporting Documents
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1 Light curves Otero, Sebastian Alberto 2011-12-30 04:26 UTC Light curves of the three stars that have been identified as the eclipsing binary showing the effects of light contamination.
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Revision History
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3 Otero, Sebastian Alberto 2011-12-30 04:26 UTC Primary record creation. Amplitude and eclipse duration from Kepler data. V-magnitude derived from UCAC3 and CMC14. UCAC3 position.
2 Admin, VSX 2011-03-13 04:30 UTC Update from [2011arXiv1103.1659S].
1 Admin, VSX 2010-06-19 01:56 UTC Initial upload.

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