| MJD | V | * | Image | B | * | Image | R | * | Images | I | * | Images | 
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 56140.37 | 18.40± 0.07 | T |  | -- | - | - | 17.86± 0.17 | - |  | -- | - | - | 
| 56599.17 | 18.35± 0.05 | - |  | 18.58± 0.07 | - |  | 17.90± 0.06 | - |  | -- | - | - | 
| 56976.16 | 18.52± 0.05 | - |  | 18.85± 0.08 | - |  | 17.91± 0.06 | - |  | -- | - | - | 
| 57038.13 | 18.37± 0.05 | - |  | 18.69± 0.06 | - |  | 17.81± 0.05 | - |  | -- | - | - | 
| 57310.13 | 18.34± 0.08 | - |  | 18.63± 0.08 | - |  | 17.79± 0.05 | - |  | -- | - | - | 
| 57335.18 | 18.42± 0.07 | - |  | -- | - | - | 17.89± 0.05 | - |  | -- | - | - | 
| 57401.10 | 18.64± 0.06 | - |  | 18.85± 0.07 | - |  | -- | - | - | -- | - | - | 
| 57634.34 | 18.51± 0.05 | - |  | 18.76± 0.08 | - |  | 17.91± 0.06 | - |  | 17.84± 0.07 | - |  | 
| 57687.13 | 18.54± 0.06 | - |  | 18.77± 0.08 | - |  | 17.88± 0.05 | - |  | 17.53± 0.07 | - |  | 
| 57964.33 | 18.45± 0.06 | - |  | 18.70± 0.08 | - |  | 17.78± 0.06 | - |  | 17.58± 0.07 | - |  | 
| 58045.18 | 18.22± 0.06 | - |  | 18.49± 0.09 | - |  | 17.71± 0.06 | - |  | -- | - | - | 
| 58073.20 | 18.35± 0.05 | - |  | 18.52± 0.07 | - |  | -- | - | - | -- | - | - | 
| 58103.18 | 18.41± 0.07 | T |  | -- | - | - | -- | - | - | -- | - | - | 
| 58108.11 | 18.40± 0.06 | - |  | 18.70± 0.10 | - |  | -- | - | - | 17.64± 0.12 | - |  | 
| 58312.39 | 18.46± 0.06 | - |  | 18.81± 0.15 | - |  | -- | - | - | -- | - | - | 
| 58317.37 | 18.52± 0.06 | - |  | 18.69± 0.08 | - |  | 17.87± 0.05 | - |  | -- | - | - | 
| 58341.34 | 18.55± 0.07 | - |  | -- | - | - | -- | - | - | 17.61± 0.07 | - |  | 
| 58342.40 | 18.48± 0.08 | - |  | 18.77± 0.12 | - |  | 17.93± 0.07 | - |  | -- | - | - | 
| 58375.14 | 18.66± 0.07 | - |  | -- | - | - | 17.94± 0.06 | - |  | -- | - | - | 
| 58420.10 | 18.57± 0.06 | - |  | 18.70± 0.08 | - |  | -- | - | - | 17.98± 0.10 | - |  | 
| 58433.00 | 18.47± 0.10 | - |  | -- | - | - | 17.86± 0.06 | - |  | 17.40± 0.08 | - |  | 
| 58672.39 | 18.52± 0.11 | - |  | -- | - | - | 17.97± 0.06 | - |  | 17.72± 0.17 | - |  | 
| 58695.36 | 18.55± 0.06 | - |  | 18.69± 0.06 | - |  | 17.91± 0.04 | - |  | -- | - | - | 
| 58784.12 | 18.49± 0.06 | - |  | 18.77± 0.06 | - |  | -- | - | - | -- | - | - | 
| 58812.22 | 18.49± 0.05 | - |  | -- | - | - | -- | - | - | 17.74± 0.07 | - |  | 
| 58902.07 | 18.51± 0.05 | - |  | -- | - | - | 17.97± 0.05 | - |  | -- | - | - | 
| 59059.38 | 18.43± 0.05 | - |  | 18.67± 0.06 | - |  | -- | - | - | -- | - | - | 
| 59081.30 | 18.47± 0.05 | A |   | 18.58± 0.06 | - |  | 17.85± 0.04 | A |   | -- | - | - | 
| 59084.34 | -- | - | - | -- | - | - | 17.92± 0.04 | T |  | -- | - | - | 
| 59161.07 | 18.55± 0.06 | - |  | 18.86± 0.08 | - |  | 17.97± 0.05 | - |  | -- | - | - | 
| 59171.09 | 18.55± 0.06 | T |  | -- | - | - | -- | - | - | > 15.91 | - |  | 
| 59227.08 | 18.42± 0.04 | - |  | 18.73± 0.05 | - |  | 17.80± 0.04 | - |  | -- | - | - | 
| 59415.36 | 18.38± 0.07 | - |  | -- | - | - | 17.93± 0.05 | - |  | -- | - | - | 
| 59441.39 | 18.38± 0.06 | - |  | 18.62± 0.06 | T |  | -- | - | - | -- | - | - | 
| 59463.30 | 18.16± 0.07 | A |   | -- | - | - | -- | - | - | 17.41± 0.05 | - |  | 
| 59523.15 | 18.38± 0.04 | - |  | -- | - | - | 17.82± 0.04 | - |  | -- | - | - | 
| 59525.15 | 18.29± 0.05 | - |  | 18.56± 0.05 | - |  | -- | - | - | -- | - | - | 
| 59546.15 | 18.41± 0.04 | - |  | -- | - | - | -- | - | - | 17.78± 0.05 | - |  | 
| 59551.11 | 18.38± 0.06 | - |  | 18.62± 0.07 | - |  | -- | - | - | -- | - | - | 
| 59583.15 | 18.45± 0.05 | - |  | -- | - | - | 17.87± 0.05 | - |  | -- | - | - | 
| 59608.07 | 18.43± 0.05 | - |  | -- | - | - | -- | - | - | 17.39± 0.07 | - |  | 
| 59794.35 | 18.41± 0.05 | T |  | -- | - | - | -- | - | - | -- | - | - | 
| 59823.24 | 18.35± 0.05 | - |  | 18.68± 0.06 | - |  | -- | - | - | -- | - | - | 
| 59851.13 | 18.45± 0.06 | - |  | -- | - | - | 17.85± 0.05 | - |  | -- | - | - | 
| 59854.22 | 18.44± 0.05 | - |  | 18.62± 0.06 | - |  | -- | - | - | -- | - | - | 
| 59879.12 | 18.34± 0.06 | - |  | -- | - | - | -- | - | - | 17.86± 0.09 | A |   | 
| 59904.12 | 18.39± 0.05 | - |  | 18.68± 0.06 | - |  | 17.76± 0.05 | - |  | 17.64± 0.07 | - |  | 
| 59932.13 | 18.20± 0.06 | - |  | -- | - | - | 17.68± 0.06 | - |  | -- | - | - | 
| 60172.37 | 18.32± 0.04 | - |  | 18.59± 0.05 | - |  | -- | - | - | -- | - | - | 
| 60205.15 | 18.09± 0.06 | - |  | -- | - | - | 17.63± 0.05 | - |  | -- | - | - | 
| 60227.12 | 18.03± 0.06 | - |  | -- | - | - | -- | - | - | 17.20± 0.07 | - |  | 
| 60262.13 | 18.23± 0.05 | - |  | 18.52± 0.06 | - |  | 17.71± 0.05 | - |  | -- | - | - | 
| 60290.15 | 18.21± 0.05 | - |  | 18.47± 0.06 | - |  | -- | - | - | 17.40± 0.07 | - |  | 
| 60292.18 | 18.28± 0.04 | - |  | -- | - | - | 17.77± 0.05 | - |  | -- | - | - | 
| 60342.08 | 18.42± 0.05 | - |  | -- | - | - | 17.86± 0.05 | - |  | -- | - | - | 
| 60504.38 | 18.13± 0.05 | - |  | 18.43± 0.06 | - |  | 17.63± 0.05 | - |  | -- | - | - | 
| 60529.36 | 18.15± 0.05 | - |  | -- | - | - | -- | - | - | 17.45± 0.07 | - |  | 
| 60556.24 | 18.31± 0.05 | - |  | 18.63± 0.06 | - |  | 17.78± 0.05 | - |  | -- | - | - | 
| 60594.10 | 18.41± 0.08 | - |  | -- | - | - | -- | - | - | 17.50± 0.08 | - |  | 
| 60612.14 | 18.35± 0.06 | - |  | -- | - | - | 17.84± 0.06 | - |  | -- | - | - | 
| 60651.14 | 18.29± 0.05 | - |  | 18.56± 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 [0.62 mag] | B [0.43 mag] | R [0.34 mag] | |
|---|---|---|---|
| B [0.43 mag] | 0.72 (33) | ||
| R [0.34 mag] | 0.77 (33) | 0.63 (18) | |
| I [0.78 mag] | 0.40 (18) | 0.30 (7) | 0.14 (6) | 
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) | 2.93 | 0.75 | ||
| R (I|R) | 3.42 | 1.25 | 0.68 | 0.08 | |
| I (I|R) | 4.76 | 0.92 | 2.25 | 0.68 | 0.66 | 0.83 | 
By John C. Martin, University of Illinois Springfield Henry R. Barber Research Observatory
Generated on 2025-08-04 15:53:14 UT-5