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Latest Details
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Name
  GSC 02679-02690  
AAVSO UID
000-BLQ-351 (146 observations)  
Constellation
Cygnus Sequence
J2000.0
20 08 05.86 +34 04 53.3  (302.02442 +34.08147) Search nearby
B1950.0 20 06 10.47 +33 56 06.2
Proper motion
RA: -2.0 +/- 2.0 mas/yDec: -15.6 +/- 1.5 mas/ySource: UCAC4
Galactic coord. 71.450 +0.775
Other names

(Internal only)
2MASS J20080585+3404532 AKARI-IRC-V1 J2008058+340453 ASASSN-V J200805.89+340453.2
IRAS 20061+3355    
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Variability type
SR
Spectral type --
Mag. range
11.93 V (0.3)clear
Discoverer Josef Kalasek
Epoch
10 Aug 2012 (HJD 2456150) Ephemeris
Outburst --
Period 50 d
Rise/eclipse dur. --
Remarks
There are currently no remarks on file for this star. (Not logged in)  Add remark
References
There are currently no additional references filed for this star.
External Links
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Location    Go   
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Catalog Data
Information from selected catalogs obtained by cross-matching to 2 arc seconds using the CDS X-Match Service. These data may not be complete.
2MASS J = 5.83H = 4.76K = 4.33J - K = 1.50
AllWISE W1 = 4.16W2 = 3.87W3 = 4.03W4 = 3.74W1 - W2 = 0.29W3 - W4 = 0.29
APASS-DR9 B = 14.16V = 11.93g' = 12.94r' = 10.99i' = 9.05B - V = 2.23
Images
Please review Digitized Sky Survey Acknowledgment and Copyright.
Size 5' x 5' (297 x 298 pixels)
Center 20 08 05.86 +34 04 53.3 (J2000)
Source STScI
Survey

Red, all sky, 1.0 arcsec/pixel
  Negative
Supporting Documents
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2 GSC 02679-02690 first light curve Conner, David S 2015-04-26 15:28 UTC The variability of GSC 02679-02690 was first detected by Josef Kalasek, using images from the Bradford Robotic Telescope Cluster Camera (Tenerife) between 2012 July and 2013 December. The variability was confirmed by David Conner. This light curve combines our data for this star.
1 GSC 02679-02690 Conner, David S 2015-04-26 15:28 UTC A period search of our data for this star using Peranso/ANOVA suggested a fundamental period of approximately 50 days. This phase plot is the resulting curve using this period.
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Revision History
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1 Conner, David S 2015-04-27 22:16 UTC Initial submission.