Resolved from J013416.71+303122.8 of comparable brightness 4 arcseconds NE.
| MJD | V | * | Image | B | * | Image | R | * | Images | I | * | Images | 
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 56140.37 | 17.16± 0.05 | - |  | -- | - | - | 16.91± 0.09 | - |  | -- | - | - | 
| 56599.17 | 17.27± 0.05 | - |  | 17.20± 0.06 | - |  | 17.13± 0.05 | - |  | -- | - | - | 
| 56976.16 | 17.13± 0.04 | - |  | 17.14± 0.06 | - |  | 16.99± 0.05 | - |  | -- | - | - | 
| 56982.22 | 17.07± 0.06 | - |  | 17.06± 0.06 | - |  | 16.96± 0.07 | - |  | -- | - | - | 
| 57038.13 | 17.24± 0.04 | - |  | 17.17± 0.05 | - |  | 17.12± 0.04 | - |  | -- | - | - | 
| 57310.13 | 17.05± 0.06 | X |  | 17.15± 0.07 | - |  | 17.10± 0.05 | - |  | -- | - | - | 
| 57328.19 | 17.26± 0.05 | - |  | 17.23± 0.07 | - |  | 17.12± 0.07 | - |  | -- | - | - | 
| 57335.18 | 17.22± 0.06 | - |  | -- | - | - | 17.15± 0.04 | - |  | -- | - | - | 
| 57401.10 | 17.26± 0.04 | - |  | 17.31± 0.06 | - |  | -- | - | - | -- | - | - | 
| 57406.10 | 17.30± 0.05 | - |  | 17.36± 0.06 | - |  | 17.17± 0.05 | - |  | 17.01± 0.08 | - |  | 
| 57634.37 | 17.26± 0.06 | A |   | 17.25± 0.08 | A |   | 17.15± 0.07 | A |   | 17.20± 0.06 | - |  | 
| 57638.43 | 17.30± 0.06 | - |  | -- | - | - | -- | - | - | 17.07± 0.10 | - |  | 
| 57687.13 | 17.25± 0.04 | - |  | 17.28± 0.06 | - |  | 17.11± 0.04 | - |  | 17.04± 0.07 | - |  | 
| 57964.33 | 17.35± 0.05 | - |  | 17.36± 0.07 | - |  | 17.25± 0.05 | - |  | 17.10± 0.07 | - |  | 
| 58045.18 | 17.33± 0.05 | - |  | 17.30± 0.07 | - |  | 17.29± 0.06 | - |  | -- | - | - | 
| 58073.20 | 17.35± 0.05 | - |  | 17.29± 0.07 | - |  | -- | - | - | -- | - | - | 
| 58103.18 | 17.24± 0.05 | T |  | -- | - | - | -- | - | - | -- | - | - | 
| 58108.11 | 17.17± 0.05 | - |  | 17.10± 0.08 | - |  | -- | - | - | 17.07± 0.09 | - |  | 
| 58312.39 | 17.14± 0.05 | - |  | 17.10± 0.07 | - |  | -- | - | - | -- | - | - | 
| 58317.37 | 17.17± 0.04 | - |  | 17.15± 0.07 | - |  | 17.07± 0.04 | - |  | -- | - | - | 
| 58341.34 | 17.16± 0.06 | - |  | -- | - | - | -- | - | - | 16.95± 0.07 | - |  | 
| 58342.40 | 17.24± 0.06 | - |  | 17.21± 0.07 | - |  | 17.18± 0.05 | - |  | -- | - | - | 
| 58375.14 | 17.25± 0.05 | - |  | -- | - | - | 17.16± 0.05 | - |  | -- | - | - | 
| 58420.10 | 17.38± 0.05 | - |  | 17.38± 0.06 | - |  | -- | - | - | 17.25± 0.08 | - |  | 
| 58433.00 | 17.17± 0.05 | - |  | -- | - | - | 17.04± 0.05 | - |  | 16.75± 0.06 | - |  | 
| 58672.39 | 17.14± 0.07 | - |  | -- | - | - | 17.00± 0.05 | - |  | 16.99± 0.12 | - |  | 
| 58695.36 | 17.13± 0.05 | - |  | 17.12± 0.05 | - |  | 17.02± 0.04 | - |  | -- | - | - | 
| 58757.17 | 17.18± 0.05 | - |  | -- | - | - | 17.06± 0.05 | - |  | -- | - | - | 
| 58784.14 | 17.20± 0.05 | A |   | 17.17± 0.05 | - |  | -- | - | - | 16.91± 0.08 | - |  | 
| 58812.22 | 17.12± 0.05 | - |  | -- | - | - | -- | - | - | 16.94± 0.06 | - |  | 
| 58902.07 | 17.25± 0.04 | - |  | -- | - | - | 17.18± 0.04 | - |  | -- | - | - | 
| 59059.38 | 17.12± 0.05 | - |  | 17.14± 0.06 | - |  | -- | - | - | -- | - | - | 
| 59081.26 | 17.05± 0.05 | - |  | -- | - | - | 16.94± 0.05 | - |  | -- | - | - | 
| 59084.38 | -- | - | - | -- | - | - | 16.89± 0.07 | T |  | -- | - | - | 
| 59161.07 | 17.12± 0.05 | - |  | 17.13± 0.06 | - |  | 17.00± 0.04 | - |  | -- | - | - | 
| 59171.09 | 17.03± 0.05 | - |  | -- | - | - | -- | - | - | 16.83± 0.06 | - |  | 
| 59227.12 | 17.17± 0.04 | A |   | 17.12± 0.05 | A |   | 17.03± 0.04 | A |   | 16.96± 0.08 | - |  | 
| 59415.36 | 17.08± 0.05 | - |  | -- | - | - | 16.94± 0.04 | - |  | -- | - | - | 
| 59441.39 | 17.09± 0.05 | - |  | 17.09± 0.06 | - |  | -- | - | - | -- | - | - | 
| 59463.30 | 17.13± 0.05 | A |   | -- | - | - | -- | - | - | 16.93± 0.05 | - |  | 
| 59523.15 | 17.19± 0.04 | - |  | -- | - | - | 17.07± 0.04 | - |  | -- | - | - | 
| 59525.15 | 17.19± 0.04 | - |  | 17.19± 0.05 | - |  | -- | - | - | -- | - | - | 
| 59546.15 | 17.20± 0.04 | - |  | -- | - | - | -- | - | - | 16.95± 0.05 | - |  | 
| 59551.11 | 17.32± 0.05 | - |  | 17.31± 0.06 | - |  | -- | - | - | -- | - | - | 
| 59583.15 | 17.24± 0.04 | - |  | -- | - | - | 17.12± 0.05 | - |  | -- | - | - | 
| 59608.07 | 17.24± 0.04 | - |  | -- | - | - | -- | - | - | 16.89± 0.06 | - |  | 
| 59794.35 | 17.07± 0.04 | T |  | -- | - | - | -- | - | - | -- | - | - | 
| 59823.24 | 17.16± 0.04 | - |  | 17.18± 0.05 | - |  | -- | - | - | -- | - | - | 
| 59851.17 | 17.15± 0.05 | A |   | 17.15± 0.04 | - |  | 16.99± 0.05 | - |  | 16.92± 0.09 | - |  | 
| 59854.22 | 17.14± 0.05 | - |  | 17.11± 0.06 | - |  | -- | - | - | -- | - | - | 
| 59879.12 | 17.11± 0.10 | - |  | -- | - | - | -- | - | - | 16.93± 0.06 | A |   | 
| 59904.12 | 17.12± 0.04 | - |  | 17.14± 0.05 | - |  | 17.03± 0.04 | - |  | 16.89± 0.06 | - |  | 
| 59932.13 | 17.11± 0.06 | - |  | -- | - | - | 17.00± 0.05 | - |  | -- | - | - | 
| 60172.37 | 17.22± 0.04 | - |  | 17.22± 0.05 | - |  | -- | - | - | -- | - | - | 
| 60205.15 | 17.14± 0.05 | - |  | -- | - | - | 17.01± 0.05 | - |  | -- | - | - | 
| 60227.12 | 17.14± 0.05 | - |  | -- | - | - | -- | - | - | 16.86± 0.07 | - |  | 
| 60262.13 | 17.16± 0.04 | - |  | 17.20± 0.05 | - |  | 17.06± 0.05 | - |  | -- | - | - | 
| 60290.19 | 17.22± 0.05 | A |   | 17.23± 0.05 | A |   | -- | - | - | 17.00± 0.08 | A |   | 
| 60292.18 | 17.16± 0.04 | - |  | -- | - | - | 17.08± 0.05 | - |  | -- | - | - | 
| 60342.08 | 17.18± 0.04 | - |  | -- | - | - | 17.06± 0.05 | - |  | -- | - | - | 
| 60504.38 | 17.18± 0.04 | - |  | 17.16± 0.05 | - |  | 17.03± 0.05 | - |  | -- | - | - | 
| 60529.38 | 17.23± 0.05 | A |   | 17.25± 0.07 | - |  | 17.13± 0.05 | - |  | 17.02± 0.06 | - |  | 
| 60556.24 | 17.16± 0.04 | - |  | 17.15± 0.05 | - |  | 17.02± 0.04 | - |  | -- | - | - | 
| 60592.14 | 17.23± 0.07 | - |  | 17.49± 0.05 | X |  | 17.11± 0.05 | - |  | -- | - | - | 
| 60594.10 | 17.07± 0.06 | - |  | -- | - | - | -- | - | - | 16.89± 0.07 | - |  | 
| 60612.14 | 17.11± 0.05 | - |  | -- | - | - | 16.99± 0.06 | - |  | -- | - | - | 
| 60651.14 | 17.11± 0.04 | - |  | 17.12± 0.05 | - |  | -- | - | - | -- | - | - | 


If the brightness variation is true variability then there should be a correlation between brightness changes recorded in different filter bands. The following table are the R-squared linear correlation factors calculated for the pairs of bands. The number in parentheses next to the R-squared value is the number of elements used to calculate the correlation factor. The number in square brackets next to the band is the range of magnitudes measured.
| V [0.35 mag] | B [0.32 mag] | R [0.39 mag] | |
|---|---|---|---|
| B [0.32 mag] | 0.85 (36) | ||
| R [0.39 mag] | 0.86 (38) | 0.73 (22) | |
| I [0.50 mag] | 0.53 (24) | 0.37 (12) | 0.45 (10) | 
The plots below are provided to check the values in the table above and also to show any non-linear correlations


Welch & Stetson (1993, AJ, 105, 1813) present a method for varible star detection in CCD images from automated surveys. Data from two bands are compared and two statistics are calculated: R and I.
The I-statistic has an expectation value of zero for stars that are NOT variable. A larger non-zero I-value indicates a higher likelihood that the star is variable. The R statistic indicates how the color of the star changes as the variable grows brighter with R = 1.0 being no change in color.
R and I values have only been calculated if there are more than four (4) matched measurements of brightness in each band.
| V (I|R) | B (I|R) | R (I|R) | |
|---|---|---|---|
| B (I|R) | 2.02 | 0.81 | ||
| R (I|R) | 2.17 | 0.89 | 1.59 | 0.44 | |
| I (I|R) | 1.92 | 1.13 | 1.53 | 1.18 | 1.87 | 1.07 | 
By John C. Martin, University of Illinois Springfield Henry R. Barber Research Observatory
Generated on 2025-08-04 15:53:14 UT-5