| MJD | V | * | Image | B | * | Image | R | * | Images | I | * | Images | 
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 56140.37 | 16.29± 0.05 | b |  | -- | - | - | 16.09± 0.06 | b |  | -- | - | - | 
| 56599.17 | 16.49± 0.05 | b |  | 16.52± 0.06 | b |  | 16.19± 0.05 | b |  | -- | - | - | 
| 56976.16 | 16.28± 0.04 | b |  | 16.34± 0.06 | b |  | 16.01± 0.05 | b |  | -- | - | - | 
| 56982.22 | 16.32± 0.06 | b |  | 16.35± 0.06 | b |  | 16.03± 0.07 | b |  | -- | - | - | 
| 57038.13 | 16.34± 0.04 | b |  | 16.37± 0.05 | b |  | 16.07± 0.04 | b |  | -- | - | - | 
| 57310.13 | 15.84± 0.05 | b |  | 15.93± 0.07 | b |  | 15.54± 0.04 | b |  | -- | - | - | 
| 57328.19 | 15.88± 0.05 | b |  | 15.97± 0.07 | b |  | 15.62± 0.07 | b |  | -- | - | - | 
| 57335.18 | 15.92± 0.06 | b |  | -- | - | - | 15.63± 0.04 | b |  | -- | - | - | 
| 57401.10 | 15.94± 0.04 | b |  | 16.03± 0.05 | b |  | -- | - | - | -- | - | - | 
| 57406.10 | 15.93± 0.04 | b |  | 16.05± 0.03 | b |  | 15.66± 0.04 | b |  | 15.50± 0.07 | b |  | 
| 57634.37 | 15.89± 0.05 | Ab |   | 15.97± 0.08 | Ab |   | 15.65± 0.07 | Ab |   | 15.58± 0.06 | b |  | 
| 57638.43 | 15.89± 0.06 | b |  | -- | - | - | -- | - | - | 15.50± 0.10 | b |  | 
| 57687.13 | 15.75± 0.04 | b |  | 15.87± 0.06 | b |  | 15.52± 0.04 | b |  | 15.35± 0.06 | b |  | 
| 57964.33 | 16.11± 0.04 | b |  | 16.17± 0.07 | b |  | 15.85± 0.05 | b |  | 15.67± 0.06 | b |  | 
| 58045.16 | 16.06± 0.04 | Ab |   | 16.14± 0.07 | Ab |   | 15.84± 0.05 | Ab |   | -- | - | - | 
| 58073.20 | 16.09± 0.04 | b |  | 16.21± 0.06 | Ab |   | -- | - | - | -- | - | - | 
| 58103.16 | 16.17± 0.04 | Ab |   | -- | - | - | -- | - | - | 15.86± 0.06 | b |  | 
| 58108.11 | 16.11± 0.05 | b |  | 16.17± 0.08 | b |  | -- | - | - | 15.77± 0.07 | b |  | 
| 58312.39 | 16.12± 0.05 | b |  | 16.17± 0.07 | b |  | -- | - | - | -- | - | - | 
| 58317.37 | 16.13± 0.04 | b |  | 16.19± 0.07 | b |  | 15.90± 0.04 | b |  | -- | - | - | 
| 58341.34 | 15.95± 0.06 | b |  | -- | - | - | -- | - | - | 15.57± 0.07 | b |  | 
| 58342.40 | 16.00± 0.05 | b |  | 16.08± 0.07 | b |  | 15.79± 0.05 | b |  | -- | - | - | 
| 58375.14 | 16.09± 0.04 | b |  | -- | - | - | 15.84± 0.05 | b |  | -- | - | - | 
| 58420.10 | 16.03± 0.04 | b |  | 16.08± 0.06 | b |  | -- | - | - | 15.63± 0.06 | b |  | 
| 58433.00 | 15.98± 0.04 | b |  | -- | - | - | 15.74± 0.05 | b |  | 15.61± 0.06 | b |  | 
| 58672.39 | 16.20± 0.07 | b |  | -- | - | - | 15.95± 0.05 | b |  | 15.91± 0.07 | b |  | 
| 58695.36 | 16.19± 0.05 | b |  | 16.25± 0.05 | b |  | 15.97± 0.04 | b |  | -- | - | - | 
| 58784.12 | 16.21± 0.05 | b |  | 16.30± 0.05 | b |  | -- | - | - | -- | - | - | 
| 58812.22 | 16.15± 0.05 | b |  | -- | - | - | -- | - | - | 15.79± 0.05 | b |  | 
| 58902.07 | 16.20± 0.04 | b |  | -- | - | - | 15.98± 0.04 | b |  | -- | - | - | 
| 59059.38 | 16.44± 0.05 | b |  | 16.50± 0.05 | b |  | -- | - | - | -- | - | - | 
| 59081.26 | 16.46± 0.05 | b |  | -- | - | - | 16.22± 0.05 | b |  | -- | - | - | 
| 59084.34 | -- | - | - | -- | - | - | 16.24± 0.04 | Tb |  | -- | - | - | 
| 59161.07 | 16.66± 0.05 | b |  | 16.72± 0.06 | b |  | 16.39± 0.04 | b |  | -- | - | - | 
| 59171.09 | 16.64± 0.05 | b |  | -- | - | - | -- | - | - | 16.33± 0.06 | b |  | 
| 59227.08 | 16.78± 0.04 | b |  | 16.80± 0.04 | b |  | 16.50± 0.04 | b |  | -- | - | - | 
| 59415.36 | 16.75± 0.04 | b |  | -- | - | - | 16.51± 0.04 | b |  | -- | - | - | 
| 59441.39 | 16.80± 0.05 | b |  | 16.80± 0.06 | b |  | -- | - | - | -- | - | - | 
| 59463.30 | 16.76± 0.04 | Ab |   | -- | - | - | -- | - | - | 16.57± 0.05 | b |  | 
| 59523.15 | 16.78± 0.04 | b |  | -- | - | - | 16.56± 0.04 | b |  | -- | - | - | 
| 59525.15 | 16.75± 0.04 | b |  | 16.75± 0.05 | b |  | -- | - | - | -- | - | - | 
| 59546.15 | 16.79± 0.04 | b |  | -- | - | - | -- | - | - | 16.60± 0.05 | b |  | 
| 59551.11 | 16.78± 0.04 | b |  | 16.77± 0.05 | b |  | -- | - | - | -- | - | - | 
| 59583.15 | 16.76± 0.04 | b |  | -- | - | - | 16.54± 0.04 | b |  | -- | - | - | 
| 59608.07 | 16.76± 0.04 | b |  | -- | - | - | -- | - | - | 16.60± 0.05 | b |  | 
| 59794.35 | 16.49± 0.04 | Tb |  | -- | - | - | -- | - | - | -- | - | - | 
| 59823.24 | 16.51± 0.04 | b |  | 16.53± 0.04 | b |  | -- | - | - | -- | - | - | 
| 59851.13 | 16.53± 0.04 | b |  | -- | - | - | 16.31± 0.04 | b |  | -- | - | - | 
| 59854.22 | 16.55± 0.04 | b |  | 16.58± 0.05 | b |  | -- | - | - | -- | - | - | 
| 59879.12 | 16.51± 0.04 | b |  | -- | - | - | -- | - | - | 16.25± 0.06 | Ab |   | 
| 59904.12 | 16.52± 0.04 | b |  | 16.56± 0.05 | b |  | 16.30± 0.04 | b |  | 16.28± 0.06 | b |  | 
| 59932.13 | 16.52± 0.05 | b |  | -- | - | - | 16.31± 0.05 | b |  | -- | - | - | 
| 60172.37 | 16.55± 0.04 | b |  | 16.58± 0.04 | b |  | -- | - | - | -- | - | - | 
| 60205.15 | 16.50± 0.04 | b |  | -- | - | - | 16.29± 0.04 | b |  | -- | - | - | 
| 60227.12 | 16.50± 0.04 | b |  | -- | - | - | -- | - | - | 16.23± 0.05 | b |  | 
| 60262.13 | 16.52± 0.04 | b |  | 16.55± 0.04 | b |  | 16.32± 0.04 | b |  | -- | - | - | 
| 60290.15 | 16.50± 0.04 | b |  | 16.54± 0.05 | b |  | -- | - | - | 16.26± 0.06 | b |  | 
| 60292.18 | 16.52± 0.04 | b |  | -- | - | - | 16.30± 0.05 | b |  | -- | - | - | 
| 60342.08 | 16.47± 0.04 | b |  | -- | - | - | 16.27± 0.05 | b |  | -- | - | - | 
| 60504.38 | 16.54± 0.04 | b |  | 16.60± 0.04 | b |  | 16.32± 0.05 | b |  | -- | - | - | 
| 60529.36 | 16.55± 0.04 | b |  | -- | - | - | -- | - | - | 16.30± 0.06 | b |  | 
| 60556.24 | 16.51± 0.04 | b |  | 16.55± 0.05 | b |  | 16.31± 0.04 | b |  | -- | - | - | 
| 60594.10 | 16.54± 0.05 | b |  | -- | - | - | -- | - | - | 16.28± 0.06 | b |  | 
| 60612.14 | 16.50± 0.05 | b |  | -- | - | - | 16.32± 0.05 | b |  | -- | - | - | 
| 60651.14 | 16.50± 0.04 | b |  | 16.53± 0.05 | b |  | -- | - | - | -- | - | - | 


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 [1.05 mag] | B [0.94 mag] | R [1.04 mag] | |
|---|---|---|---|
| B [0.94 mag] | 1.00 (35) | ||
| R [1.04 mag] | 0.99 (36) | 0.99 (20) | |
| I [1.25 mag] | 0.99 (22) | 0.97 (8) | 0.98 (7) | 
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) | 34.71 | 0.74 | ||
| R (I|R) | 45.25 | 1.01 | 34.80 | 0.58 | |
| I (I|R) | 50.42 | 1.07 | 27.44 | 0.86 | 29.43 | 1.12 | 
By John C. Martin, University of Illinois Springfield Henry R. Barber Research Observatory
Generated on 2025-08-04 15:53:14 UT-5