| MJD | V | * | Image | B | * | Image | R | * | Images | I | * | Images | 
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 56142.33 | 17.40± 0.06 | Tb |   | -- | - | - | -- | - | - | -- | - | - | 
| 56267.15 | -- | - | - | -- | - | - | 17.00± 0.05 | Tb |   | -- | - | - | 
| 56490.38 | 16.95± 0.04 | Tb |  | -- | - | - | -- | - | - | -- | - | - | 
| 56536.26 | 16.93± 0.05 | b |  | -- | - | - | 16.69± 0.06 | b |  | -- | - | - | 
| 56537.18 | 17.01± 0.04 | Ab |   | 17.07± 0.05 | Ab |   | 16.84± 0.03 | b |   | -- | - | - | 
| 56915.16 | 17.30± 0.04 | b |  | 17.34± 0.06 | b |  | 17.08± 0.05 | b |  | -- | - | - | 
| 57227.34 | 17.15± 0.04 | b |  | 17.19± 0.05 | b |  | 16.91± 0.04 | b |  | -- | - | - | 
| 57310.10 | 16.99± 0.03 | b |  | -- | - | - | -- | - | - | 16.77± 0.07 | b |  | 
| 57633.35 | 16.70± 0.05 | Ab |   | 16.81± 0.06 | Ab |   | 16.42± 0.05 | Ab |   | -- | - | - | 
| 57635.35 | 16.72± 0.05 | b |  | -- | - | - | -- | - | - | 16.31± 0.06 | b |  | 
| 57638.25 | 16.73± 0.04 | b |  | -- | - | - | -- | - | - | 16.31± 0.07 | b |  | 
| 57888.07 | 16.13± 0.04 | b |  | 16.21± 0.09 | b |  | 15.74± 0.04 | b |  | -- | - | - | 
| 57928.32 | 16.18± 0.04 | b |  | 16.31± 0.06 | b |  | 15.84± 0.06 | b |  | 15.71± 0.08 | b |  | 
| 57958.26 | 16.20± 0.06 | b |  | 16.33± 0.07 | b |  | -- | - | - | 15.75± 0.06 | b |  | 
| 57963.26 | 16.22± 0.06 | b |  | 16.33± 0.07 | b |  | -- | - | - | -- | - | - | 
| 57988.22 | 16.23± 0.07 | b |  | 16.36± 0.07 | b |  | -- | - | - | 15.84± 0.06 | b |  | 
| 58035.03 | 16.39± 0.04 | b |  | -- | - | - | 16.10± 0.04 | b |  | -- | - | - | 
| 58043.05 | 16.41± 0.05 | b |  | 16.53± 0.05 | b |  | 16.15± 0.04 | b |  | -- | - | - | 
| 58045.05 | 16.41± 0.05 | b |  | -- | - | - | -- | - | - | 15.92± 0.06 | b |  | 
| 58067.10 | 16.36± 0.04 | b |  | -- | - | - | -- | - | - | 15.96± 0.06 | b |  | 
| 58073.09 | 16.35± 0.06 | b |  | 16.47± 0.07 | b |  | -- | - | - | -- | - | - | 
| 58077.08 | 16.31± 0.07 | b |  | -- | - | - | -- | - | - | 15.91± 0.07 | b |  | 
| 58098.07 | 16.36± 0.06 | b |  | 16.46± 0.07 | b |  | -- | - | - | -- | - | - | 
| 58103.08 | 16.30± 0.05 | b |  | -- | - | - | -- | - | - | 15.86± 0.07 | b |  | 
| 58312.26 | 16.33± 0.06 | b |  | 16.48± 0.07 | b |  | 16.02± 0.06 | b |  | -- | - | - | 
| 58316.24 | 16.26± 0.06 | b |  | -- | - | - | -- | - | - | 15.82± 0.06 | b |  | 
| 58339.26 | 16.23± 0.07 | b |  | -- | - | - | -- | - | - | 15.80± 0.07 | b |  | 
| 58342.26 | 16.21± 0.04 | b |  | 16.35± 0.06 | b |  | -- | - | - | -- | - | - | 
| 58366.11 | 16.26± 0.04 | b |  | 16.39± 0.06 | b |  | -- | - | - | -- | - | - | 
| 58375.09 | 16.33± 0.04 | b |  | -- | - | - | 16.02± 0.04 | b |  | -- | - | - | 
| 58403.06 | 16.17± 0.03 | b |  | -- | - | - | -- | - | - | 15.67± 0.05 | b |  | 
| 58420.01 | 16.01± 0.06 | b |  | 16.14± 0.08 | b |  | -- | - | - | -- | - | - | 
| 58436.04 | 15.92± 0.04 | b |  | 16.05± 0.06 | b |  | 15.67± 0.04 | b |  | -- | - | - | 
| 58671.35 | 15.96± 0.03 | Ab |   | 16.14± 0.03 | b |  | 15.69± 0.04 | b |  | -- | - | - | 
| 58695.41 | 16.01± 0.03 | b |  | -- | - | - | 15.74± 0.04 | b |  | -- | - | - | 
| 58750.11 | 16.10± 0.03 | b |  | -- | - | - | -- | - | - | 15.68± 0.05 | b |  | 
| 58779.03 | 16.23± 0.03 | b |  | 16.36± 0.03 | b |  | -- | - | - | -- | - | - | 
| 58812.16 | 16.32± 0.03 | b |  | -- | - | - | 16.06± 0.03 | b |  | -- | - | - | 
| 59000.37 | 16.64± 0.06 | b |  | -- | - | - | 16.32± 0.04 | b |  | -- | - | - | 
| 59055.29 | 16.79± 0.06 | b |  | 16.90± 0.06 | b |  | -- | - | - | -- | - | - | 
| 59077.25 | 16.67± 0.07 | b |  | -- | - | - | 16.32± 0.05 | b |  | 16.20± 0.06 | b |  | 
| 59131.11 | 16.61± 0.05 | b |  | 16.73± 0.05 | b |  | -- | - | - | -- | - | - | 
| 59166.14 | 16.44± 0.05 | b |  | -- | - | - | -- | - | - | 15.98± 0.06 | b |  | 
| 59194.12 | 16.31± 0.03 | b |  | -- | - | - | 15.99± 0.05 | b |  | -- | - | - | 
| 59376.38 | 15.97± 0.07 | b |  | 16.15± 0.06 | b |  | -- | - | - | -- | - | - | 
| 59409.33 | 15.86± 0.05 | Ab |   | -- | - | - | 15.55± 0.05 | b |  | -- | - | - | 
| 59442.36 | 15.85± 0.06 | b |  | 16.04± 0.07 | b |  | -- | - | - | 15.34± 0.05 | b |  | 
| 59467.13 | 15.88± 0.06 | b |  | -- | - | - | 15.62± 0.03 | b |  | -- | - | - | 
| 59522.10 | 16.09± 0.04 | b |  | 16.26± 0.05 | b |  | -- | - | - | -- | - | - | 
| 59546.13 | 16.25± 0.03 | b |  | -- | - | - | -- | - | - | 15.77± 0.06 | b |  | 
| 59583.12 | 16.01± 0.05 | b |  | -- | - | - | 15.76± 0.04 | b |  | -- | - | - | 
| 59739.38 | 16.28± 0.05 | b |  | 16.44± 0.06 | b |  | 16.00± 0.05 | b |  | -- | - | - | 
| 59816.16 | 15.96± 0.06 | b |  | -- | - | - | 15.71± 0.04 | b |  | -- | - | - | 
| 59848.09 | 15.89± 0.04 | b |  | -- | - | - | -- | - | - | 15.43± 0.05 | b |  | 
| 59879.05 | 15.93± 0.05 | b |  | 16.09± 0.06 | b |  | -- | - | - | -- | - | - | 
| 59905.10 | 15.97± 0.03 | b |  | -- | - | - | 15.68± 0.03 | b |  | 15.50± 0.04 | b |  | 
| 60147.27 | 15.97± 0.07 | b |  | -- | - | - | 15.70± 0.07 | b |  | -- | - | - | 
| 60172.21 | 15.92± 0.07 | b |  | -- | - | - | -- | - | - | 15.48± 0.10 | b |  | 
| 60201.09 | 15.91± 0.07 | b |  | -- | - | - | 15.66± 0.07 | b |  | -- | - | - | 
| 60251.03 | 15.95± 0.06 | b |  | 16.09± 0.07 | b |  | -- | - | - | -- | - | - | 
| 60290.06 | 15.79± 0.07 | b |  | -- | - | - | -- | - | - | 15.36± 0.09 | b |  | 
| 60469.38 | 16.09± 0.07 | b |  | -- | - | - | 15.82± 0.08 | b |  | -- | - | - | 
| 60504.34 | 16.10± 0.07 | b |  | 16.26± 0.08 | b |  | -- | - | - | -- | - | - | 
| 60533.25 | 16.12± 0.07 | Tb |  | -- | - | - | -- | - | - | -- | - | - | 
| 60555.16 | 16.14± 0.06 | b |  | -- | - | - | 15.85± 0.07 | b |  | 15.68± 0.09 | b |  | 
| 60594.07 | 16.29± 0.07 | b |  | 16.46± 0.07 | b |  | 16.01± 0.07 | b |  | -- | - | - | 
| 60651.11 | 16.18± 0.06 | b |  | -- | - | - | -- | - | - | 15.73± 0.09 | 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 [1.61 mag] | B [1.30 mag] | R [1.53 mag] | |
|---|---|---|---|
| B [1.30 mag] | 1.00 (29) | ||
| R [1.53 mag] | 0.99 (29) | 0.99 (12) | |
| I [1.43 mag] | 0.98 (24) | 0.98 (4) | 1.00 (4) | 
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) | 53.00 | 0.73 | ||
| R (I|R) | 87.16 | 0.96 | 85.01 | 0.53 | |
| I (I|R) | 34.61 | 1.28 | --- | --- | --- | ---- | 
By John C. Martin, University of Illinois Springfield Henry R. Barber Research Observatory
Generated on 2025-08-04 15:53:14 UT-5