| MJD | V | * | Image | B | * | Image | R | * | Images | I | * | Images | 
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 56140.37 | 18.11± 0.06 | - |  | -- | - | - | 17.83± 0.18 | - |  | -- | - | - | 
| 56599.17 | 18.15± 0.06 | - |  | 18.17± 0.07 | - |  | 18.06± 0.06 | - |  | -- | - | - | 
| 56976.16 | 18.06± 0.05 | - |  | 18.24± 0.06 | - |  | 17.96± 0.06 | - |  | -- | - | - | 
| 57038.13 | 18.16± 0.05 | - |  | 18.15± 0.06 | - |  | 18.02± 0.05 | - |  | -- | - | - | 
| 57310.13 | 18.40± 0.08 | - |  | 18.42± 0.09 | - |  | 18.33± 0.06 | - |  | -- | - | - | 
| 57335.18 | 18.04± 0.06 | - |  | -- | - | - | 17.89± 0.05 | - |  | -- | - | - | 
| 57401.10 | 18.12± 0.05 | - |  | 18.15± 0.06 | - |  | -- | - | - | -- | - | - | 
| 57634.34 | 18.31± 0.05 | - |  | 18.36± 0.08 | - |  | 18.20± 0.06 | - |  | 18.26± 0.09 | - |  | 
| 57687.13 | 18.11± 0.05 | - |  | 18.23± 0.07 | - |  | 18.09± 0.05 | - |  | 18.44± 0.10 | - |  | 
| 57964.35 | 18.22± 0.05 | A |   | 18.22± 0.07 | A |   | 18.07± 0.06 | A |   | 18.22± 0.09 | A |   | 
| 58043.10 | 18.18± 0.05 | - |  | -- | - | - | 17.96± 0.05 | - |  | 18.08± 0.10 | - |  | 
| 58045.16 | 18.04± 0.05 | A |   | 18.07± 0.07 | A |   | 17.91± 0.06 | A |   | -- | - | - | 
| 58073.19 | 18.22± 0.05 | A |   | 18.24± 0.07 | A |   | -- | - | - | -- | - | - | 
| 58103.16 | 18.10± 0.05 | A |   | -- | - | - | -- | - | - | 17.70± 0.08 | - |  | 
| 58108.11 | 18.08± 0.06 | - |  | 18.13± 0.08 | - |  | -- | - | - | 18.28± 0.23 | - |  | 
| 58312.39 | 18.00± 0.05 | - |  | 18.06± 0.10 | - |  | -- | - | - | -- | - | - | 
| 58316.38 | 17.95± 0.04 | - |  | 18.02± 0.06 | - |  | 17.88± 0.04 | - |  | 17.97± 0.07 | - |  | 
| 58317.37 | 17.96± 0.05 | - |  | 18.03± 0.07 | - |   | 17.90± 0.05 | - |   | -- | - | - | 
| 58341.34 | 18.11± 0.07 | - |  | -- | - | - | -- | - | - | 17.84± 0.07 | - |  | 
| 58342.38 | 18.12± 0.06 | A |   | 18.15± 0.09 | A |   | 18.02± 0.06 | A |   | 18.09± 0.09 | - |   | 
| 58375.14 | 18.07± 0.05 | - |  | -- | - | - | 18.00± 0.06 | - |  | -- | - | - | 
| 58420.08 | 18.00± 0.05 | A |   | 18.04± 0.07 | A |   | 17.98± 0.05 | - |  | 17.59± 0.09 | A |   | 
| 58433.00 | 18.05± 0.07 | - |  | -- | - | - | 18.09± 0.06 | - |  | 17.94± 0.10 | - |  | 
| 58672.39 | 18.05± 0.09 | - |  | -- | - | - | 17.95± 0.06 | - |  | 18.04± 0.24 | - |  | 
| 58695.36 | 18.01± 0.05 | - |  | 18.03± 0.06 | - |  | 17.90± 0.04 | - |  | -- | - | - | 
| 58784.12 | 18.07± 0.06 | - |  | 18.11± 0.06 | - |  | -- | - | - | -- | - | - | 
| 58812.22 | 18.35± 0.05 | - |  | -- | - | - | -- | - | - | 18.39± 0.08 | - |  | 
| 58902.07 | 17.98± 0.04 | - |  | -- | - | - | 17.90± 0.05 | - |  | -- | - | - | 
| 59059.38 | 18.03± 0.05 | - |  | 18.01± 0.06 | - |  | -- | - | - | -- | - | - | 
| 59081.30 | 18.15± 0.05 | A |   | 18.18± 0.06 | - |  | 18.07± 0.04 | A |   | -- | - | - | 
| 59084.34 | -- | - | - | -- | - | - | 18.09± 0.04 | T |  | -- | - | - | 
| 59161.07 | 18.14± 0.06 | - |  | 18.20± 0.07 | - |  | 18.05± 0.05 | - |  | -- | - | - | 
| 59171.09 | 17.95± 0.05 | - |  | -- | - | - | -- | - | - | 18.16± 0.09 | - |  | 
| 59227.08 | 17.98± 0.04 | - |  | 18.10± 0.04 | - |  | 17.89± 0.04 | - |  | -- | - | - | 
| 59415.36 | 18.24± 0.07 | - |  | -- | - | - | 18.08± 0.06 | - |  | -- | - | - | 
| 59441.39 | 17.94± 0.05 | - |  | 17.96± 0.06 | - |  | -- | - | - | -- | - | - | 
| 59463.30 | 18.24± 0.08 | A |   | -- | - | - | -- | - | - | 18.21± 0.07 | - |  | 
| 59523.15 | 18.19± 0.04 | - |  | -- | - | - | 18.08± 0.04 | - |  | -- | - | - | 
| 59525.14 | 18.21± 0.04 | A |   | 18.22± 0.05 | - |  | 18.06± 0.06 | - |  | -- | - | - | 
| 59546.15 | 18.00± 0.04 | - |  | -- | - | - | -- | - | - | 17.99± 0.06 | - |  | 
| 59551.11 | 17.94± 0.05 | - |  | 18.07± 0.06 | - |  | -- | - | - | -- | - | - | 
| 59583.15 | 18.20± 0.04 | - |  | -- | - | - | 18.08± 0.05 | - |  | -- | - | - | 
| 59608.07 | 18.08± 0.05 | - |  | -- | - | - | -- | - | - | 18.00± 0.09 | - |  | 
| 59794.35 | 18.21± 0.05 | T |  | -- | - | - | -- | - | - | -- | - | - | 
| 59823.24 | 18.00± 0.05 | - |  | 18.02± 0.05 | - |  | -- | - | - | -- | - | - | 
| 59851.13 | 18.09± 0.05 | - |  | -- | - | - | 18.11± 0.05 | - |  | -- | - | - | 
| 59854.19 | 18.15± 0.05 | A |   | 18.22± 0.07 | A |   | 18.04± 0.06 | - |  | -- | - | - | 
| 59879.12 | 18.04± 0.05 | - |  | -- | - | - | -- | - | - | 17.60± 0.07 | A |   | 
| 59904.12 | 18.19± 0.05 | - |  | 18.20± 0.05 | - |  | 18.05± 0.05 | - |  | 18.16± 0.08 | - |  | 
| 59932.13 | 17.99± 0.06 | - |  | -- | - | - | 17.86± 0.06 | - |  | -- | - | - | 
| 60172.37 | 18.20± 0.04 | - |  | 18.22± 0.05 | - |  | -- | - | - | -- | - | - | 
| 60205.15 | 17.99± 0.06 | - |  | -- | - | - | 17.89± 0.05 | - |  | -- | - | - | 
| 60227.12 | 18.22± 0.06 | - |  | -- | - | - | -- | - | - | 18.52± 0.13 | - |  | 
| 60262.13 | 18.15± 0.05 | - |  | 18.18± 0.05 | - |  | 18.06± 0.05 | - |  | -- | - | - | 
| 60290.14 | 18.06± 0.05 | A |   | 18.11± 0.06 | A |   | 17.87± 0.06 | - |  | 18.18± 0.09 | - |  | 
| 60290.14 | 18.07± 0.04 | A |   | 18.10± 0.06 | A |   | 17.86± 0.06 | - |  | 18.17± 0.09 | - |  | 
| 60292.18 | 18.11± 0.04 | - |  | -- | - | - | 17.98± 0.05 | - |  | -- | - | - | 
| 60342.09 | 18.07± 0.04 | A |   | -- | - | - | 17.96± 0.05 | - |  | 17.81± 0.08 | - |  | 
| 60504.38 | 18.03± 0.05 | - |  | 18.10± 0.05 | - |  | 17.97± 0.06 | - |  | -- | - | - | 
| 60506.38 | 18.03± 0.05 | - |  | -- | - | - | 17.86± 0.05 | - |  | 17.82± 0.09 | - |  | 
| 60529.37 | 18.06± 0.05 | A |   | 18.11± 0.06 | - |  | -- | - | - | 17.98± 0.07 | - |  | 
| 60556.25 | 18.07± 0.04 | A |   | 18.10± 0.05 | - |  | 17.97± 0.05 | - |  | 17.86± 0.08 | - |  | 
| 60564.22 | 17.95± 0.04 | - |  | 18.03± 0.08 | - |  | 17.83± 0.06 | - |  | -- | - | - | 
| 60595.13 | 18.21± 0.06 | - |  | 18.15± 0.08 | - |  | 18.01± 0.07 | - |  | -- | - | - | 
| 60594.10 | 18.20± 0.07 | - | -- | - | - | -- | - | - | 17.76± 0.09 | - | ||
| 60612.14 | 18.18± 0.05 | - |  | -- | - | - | 18.08± 0.06 | - |  | -- | - | - | 
| 60651.15 | 18.29± 0.05 | A |   | 18.33± 0.05 | - |  | 18.10± 0.06 | - |  | -- | - | - | 


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 [0.46 mag] | B [0.46 mag] | R [0.50 mag] | |
|---|---|---|---|
| B [0.46 mag] | 0.85 (38) | ||
| R [0.50 mag] | 0.69 (44) | 0.79 (27) | |
| I [0.92 mag] | 0.26 (27) | 0.43 (12) | 0.15 (15) | 
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) | 3.02 | 0.71 | ||
| R (I|R) | 3.11 | 1.06 | 2.80 | 0.39 | |
| I (I|R) | 2.84 | 0.67 | 2.29 | 0.55 | 1.72 | 0.74 | 
By John C. Martin, University of Illinois Springfield Henry R. Barber Research Observatory
Generated on 2025-08-04 15:53:14 UT-5