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Name
  USNO-B1.0 1053-0243135  
AAVSO UID
000-BKW-427 (No observations)  
Constellation
Serpens Sequence
J2000.0
15 23 01.27 +15 23 04.7  (230.75529 +15.38464) Search nearby
B1950.0 15 20 41.83 +15 33 43.2
Proper motion
RA: -5.2 +/- 3.2 mas/yDec: -10.0 +/- 4.0 mas/ySource: UCAC4
Galactic coord. 22.332 +52.951
Other names

(Internal only)
2MASS J15230127+1523045 ASASSN-V J152301.27+152304.7 CSS_J152301.3+152304
UCAC4 527-057728 WISE J152301.26+152304.5  
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Variability type
DSCT
Spectral type --
Mag. range
15.51 - 15.61 CV
Discoverer Stefan Hümmerich
Epoch
24 May 2012 (HJD 2456071.9846) Ephemeris
Outburst --
Period 0.047988 d  (69.103 min)
Rise/eclipse dur. 48%  (33.2 min)
Remarks
Some references may be clicked to view in new window. Roll over index number to view submission details.
1 Hümmerich, Stefan Type, amplitude, period and epoch were derived from CRTS data. UCAC4 position. J-K= 0.13 (2MASS).
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References
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1 Drake, A.J. et al. First Results from the Catalina Real-time Transient
Survey 2009, ApJ, 696, 870		 2009ApJ...696..870D
External Links
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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 = 15.04H = 14.90K = 14.91J - K = 0.12
AllWISE W1 = 14.74W2 = 14.87W1 - W2 = -0.13
APASS-DR9 B = 15.94V = 15.66g' = 15.69r' = 15.69i' = 15.52B - V = 0.27
GALEX-DR5 FUV = 20.73NUV = 17.92FUV - NUV = 2.81
SDSS-DR12 u = 16.74g = 15.66r = 15.62i = 15.64z = 15.68u - g = 1.08r - i = -0.02
Images
Please review Digitized Sky Survey Acknowledgment and Copyright.
Size 5' x 5' (297 x 298 pixels)
Center 15 23 01.27 +15 23 04.7 (J2000)
Source STScI
Survey

Red, all sky, 1.0 arcsec/pixel
  Negative
Supporting Documents
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1 USNO-B1.0 1053-0243135 - light curve and phase plot Hümmerich, Stefan 2013-02-21 23:02 UTC USNO-B1.0 1053-0243135 - light curve and phase plot
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Revision History
Currently approved revision is checked. Click revision number to view details of that revision.
1 Hümmerich, Stefan 2013-02-22 06:25 UTC Initial submission.

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