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Latest Details
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Name
  NSVS 3434304  
AAVSO UID
000-BLR-147 (No observations)  
Constellation
Cepheus Sequence
J2000.0
22 13 04.90 +56 04 21.5  (333.27043 +56.07264) Search nearby
B1950.0 22 11 15.97 +55 49 28.0
Proper motion
RA: 5.3 +/- 5.6 mas/yDec: 3.0 +/- 5.7 mas/ySource: UCAC4
Galactic coord. 102.096 -0.255
Other names

(Internal only)
2MASS J22130490+5604213 ASASSN-V J221304.82+560421.4 IRAS 22112+5549
MSX6C G102.0960-00.2549 UCAC4 731-081678 URAT1 731-399917
USNO-B1.0 1460-0397716 ZTF J221304.90+560421.5  
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Variability type
SR
Spectral type --
Mag. range
14.218 (0.483) g
Discoverer Ivan Sergey, Dubrovki Sergei, Astrobloknot Team
Epoch
25 Sep 2018 (HJD 2458386.8798) Ephemeris
Outburst --
Period 474.4164069 d
Rise/eclipse dur. --
Remarks
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1 2020arXiv200508662C Epoch of minimum given.
2 Sergey, Ivan Possible Period 70 d. J-K = 1.5. NSVS magnitudes in the table are for the blend of the variable with GSC 03973-00299 (V= 13.1; sep. 21") and GSC 03973-00326 (V= 13.6; sep. 42").
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References
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1 ZTF Catalog of Periodic Variable Stars (online data) 2020arXiv200508662C
2 Chen, X.; et al., 2020, The Zwicky Transient Facility Catalog of Periodic
Variable Stars
2020arXiv200508662C
3 Northern Sky Variability Survey, Wozniak, P.R., et al., 2004 2004AJ....127.2436W
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 = 6.99H = 5.86K = 5.49J - K = 1.50
AllWISE W1 = 5.33W2 = 5.15W3 = 4.64W4 = 4.05W1 - W2 = 0.18W3 - W4 = 0.59
APASS-DR9 i' = 10.19
Images
Please review Digitized Sky Survey Acknowledgment and Copyright.
Size 5' x 5' (297 x 298 pixels)
Center 22 13 04.90 +56 04 21.5 (J2000)
Source STScI
Survey

Red, all sky, 1.0 arcsec/pixel
  Negative
Supporting Documents
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1 Photometric curve Sergey, Ivan 2015-07-10 11:00 UTC
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Revision History
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2 Otero, Sebastian Alberto 2021-10-26 10:21 UTC Update from 2020arXiv200508662C. Gaia EDR3 position.
1 Sergey, Ivan 2015-07-10 21:57 UTC Initial submission.