| MJD | V | * | Image | B | * | Image | R | * | Images | I | * | Images | 
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 56140.37 | 17.23± 0.05 | - |  | -- | - | - | 17.13± 0.09 | - |  | -- | - | - | 
| 56599.17 | 17.23± 0.05 | - |  | 17.24± 0.06 | - |  | 17.09± 0.05 | - |  | -- | - | - | 
| 56976.16 | 17.18± 0.04 | - |  | 17.24± 0.06 | - |  | 17.07± 0.05 | - |  | -- | - | - | 
| 57038.13 | 17.16± 0.04 | - |  | 17.18± 0.05 | - |  | 17.06± 0.04 | - |  | -- | - | - | 
| 57310.13 | 17.29± 0.06 | - |  | 17.30± 0.07 | - |  | 17.22± 0.05 | - |  | -- | - | - | 
| 57335.18 | 17.30± 0.06 | - |  | -- | - | - | 17.18± 0.04 | - |  | -- | - | - | 
| 57401.10 | 17.30± 0.04 | - |  | 17.26± 0.06 | - |  | -- | - | - | -- | - | - | 
| 57634.34 | 17.32± 0.04 | - |  | 17.32± 0.07 | - |  | 17.24± 0.05 | - |  | 17.18± 0.06 | - |  | 
| 57687.13 | 17.29± 0.04 | - |  | 17.27± 0.06 | - |  | 17.18± 0.04 | - |  | 17.21± 0.07 | - |  | 
| 57964.35 | 17.24± 0.04 | A |   | 17.25± 0.06 | A |   | 17.11± 0.05 | A |   | 16.99± 0.06 | A |   | 
| 58045.16 | 17.40± 0.05 | A |   | 17.43± 0.07 | A |   | 17.29± 0.05 | A |   | -- | - | - | 
| 58073.19 | 17.24± 0.04 | A |   | 17.27± 0.06 | A |   | -- | - | - | -- | - | - | 
| 58103.16 | 17.25± 0.04 | A |   | -- | - | - | -- | - | - | 17.08± 0.07 | - |  | 
| 58108.11 | 17.18± 0.05 | - |  | 17.20± 0.08 | - |  | -- | - | - | 16.77± 0.09 | - |  | 
| 58312.39 | 17.05± 0.05 | - |  | 17.08± 0.07 | - |  | -- | - | - | -- | - | - | 
| 58316.38 | 17.16± 0.03 | - |  | 17.24± 0.05 | - |  | 17.02± 0.03 | - |  | 16.91± 0.05 | - |  | 
| 58317.37 | 17.16± 0.04 | - |  | 17.15± 0.07 | - |   | 17.03± 0.04 | - |   | -- | - | - | 
| 58341.34 | 17.24± 0.06 | - |  | -- | - | - | -- | - | - | 17.06± 0.07 | - |  | 
| 58342.38 | 17.27± 0.04 | A |   | 17.32± 0.07 | A |   | 17.17± 0.05 | A |   | 17.02± 0.06 | - |   | 
| 58375.14 | 17.34± 0.05 | - |  | -- | - | - | 17.21± 0.05 | - |  | -- | - | - | 
| 58420.08 | 17.21± 0.04 | A |   | 17.25± 0.06 | A |   | 17.13± 0.04 | - |  | 17.00± 0.07 | A |   | 
| 58433.00 | 17.25± 0.05 | - |  | -- | - | - | 17.13± 0.05 | - |  | 17.21± 0.07 | - |  | 
| 58672.39 | 17.35± 0.07 | - |  | -- | - | - | 17.27± 0.05 | - |  | 17.03± 0.10 | - |  | 
| 58695.36 | 17.18± 0.05 | - |  | 17.18± 0.05 | - |  | 17.06± 0.04 | - |  | -- | - | - | 
| 58784.12 | 17.20± 0.05 | - |  | 17.19± 0.05 | - |  | -- | - | - | -- | - | - | 
| 58812.22 | 17.20± 0.05 | - |  | -- | - | - | -- | - | - | 17.03± 0.05 | - |  | 
| 58902.07 | 17.21± 0.04 | - |  | -- | - | - | 17.12± 0.04 | - |  | -- | - | - | 
| 59059.38 | 17.15± 0.05 | - |  | 17.17± 0.06 | - |  | -- | - | - | -- | - | - | 
| 59081.30 | 17.20± 0.04 | A |   | 17.18± 0.06 | - |  | 17.09± 0.04 | A |   | -- | - | - | 
| 59084.34 | -- | - | - | -- | - | - | 17.07± 0.04 | T |  | -- | - | - | 
| 59161.07 | 17.20± 0.05 | - |  | 17.20± 0.06 | - |  | 17.08± 0.04 | - |  | -- | - | - | 
| 59171.09 | 17.22± 0.05 | - |  | -- | - | - | -- | - | - | 16.86± 0.06 | - |  | 
| 59227.08 | 17.13± 0.04 | - |  | 17.15± 0.04 | - |  | 17.03± 0.04 | - |  | -- | - | - | 
| 59415.36 | 17.22± 0.05 | - |  | -- | - | - | 17.09± 0.04 | - |  | -- | - | - | 
| 59441.39 | 17.20± 0.05 | - |  | 17.21± 0.06 | - |  | -- | - | - | -- | - | - | 
| 59463.30 | 17.28± 0.05 | A |   | -- | - | - | -- | - | - | 17.06± 0.05 | - |  | 
| 59523.15 | 17.15± 0.04 | - |  | -- | - | - | 17.05± 0.04 | - |  | -- | - | - | 
| 59525.15 | 17.23± 0.04 | - |  | 17.25± 0.05 | - |  | -- | - | - | -- | - | - | 
| 59546.15 | 17.33± 0.04 | - |  | -- | - | - | -- | - | - | 17.03± 0.05 | - |  | 
| 59551.11 | 17.37± 0.04 | - |  | 17.45± 0.05 | - |  | -- | - | - | -- | - | - | 
| 59583.15 | 17.22± 0.04 | - |  | -- | - | - | 17.09± 0.04 | - |  | -- | - | - | 
| 59608.07 | 17.24± 0.04 | - |  | -- | - | - | -- | - | - | 17.17± 0.06 | - |  | 
| 59794.35 | 17.10± 0.04 | T |  | -- | - | - | -- | - | - | -- | - | - | 
| 59823.24 | 17.12± 0.04 | - |  | 17.19± 0.05 | - |  | -- | - | - | -- | - | - | 
| 59851.13 | 17.29± 0.04 | - |  | -- | - | - | 17.15± 0.04 | - |  | -- | - | - | 
| 59854.22 | 17.29± 0.04 | - |  | 17.33± 0.06 | - |  | -- | - | - | -- | - | - | 
| 59879.12 | 17.17± 0.04 | - |  | -- | - | - | -- | - | - | 17.02± 0.06 | A |   | 
| 59904.12 | 17.12± 0.04 | - |  | 17.16± 0.05 | - |  | 17.01± 0.04 | - |  | 16.90± 0.06 | - |  | 
| 59932.13 | 17.20± 0.06 | - |  | -- | - | - | 17.05± 0.05 | - |  | -- | - | - | 
| 60172.37 | 17.13± 0.04 | - |  | 17.16± 0.04 | - |  | -- | - | - | -- | - | - | 
| 60205.15 | 17.09± 0.05 | - |  | -- | - | - | 16.95± 0.05 | - |  | -- | - | - | 
| 60227.12 | 17.04± 0.05 | - |  | -- | - | - | -- | - | - | 16.97± 0.06 | - |  | 
| 60262.13 | 17.17± 0.04 | - |  | 17.20± 0.05 | - |  | 17.06± 0.04 | - |  | -- | - | - | 
| 60290.15 | 17.22± 0.04 | - |  | 17.27± 0.05 | - |  | -- | - | - | 17.16± 0.07 | - |  | 
| 60292.18 | 17.23± 0.04 | - |  | -- | - | - | 17.10± 0.05 | - |  | -- | - | - | 
| 60342.08 | 17.13± 0.04 | - |  | -- | - | - | 17.01± 0.05 | - |  | -- | - | - | 
| 60504.38 | 17.21± 0.04 | - |  | 17.21± 0.05 | - |  | 17.08± 0.05 | - |  | -- | - | - | 
| 60529.36 | 17.29± 0.05 | - |  | -- | - | - | -- | - | - | 17.08± 0.06 | - |  | 
| 60556.24 | 17.07± 0.04 | - |  | 17.10± 0.05 | - |  | 16.95± 0.04 | - |  | -- | - | - | 
| 60594.10 | 17.34± 0.06 | - |  | -- | - | - | -- | - | - | 17.07± 0.07 | - |  | 
| 60612.14 | 17.24± 0.05 | - |  | -- | - | - | 17.13± 0.06 | - |  | -- | - | - | 
| 60651.14 | 17.17± 0.04 | - |  | 17.17± 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 [0.36 mag] | B [0.37 mag] | R [0.34 mag] | |
|---|---|---|---|
| B [0.37 mag] | 0.88 (34) | ||
| R [0.34 mag] | 0.94 (35) | 0.85 (20) | |
| I [0.45 mag] | 0.25 (22) | 0.47 (9) | 0.38 (9) | 
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) | 2.22 | 0.79 | ||
| R (I|R) | 2.63 | 0.95 | 1.70 | 0.33 | |
| I (I|R) | 1.54 | 0.98 | 1.26 | 0.37 | 2.70 | 1.00 | 
By John C. Martin, University of Illinois Springfield Henry R. Barber Research Observatory
Generated on 2025-08-04 15:53:14 UT-5