| MJD | V | * | Image | B | * | Image | R | * | Images | I | * | Images | 
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 56142.33 | 16.69± 0.06 | T |  | -- | - | - | -- | - | - | -- | - | - | 
| 56267.14 | -- | - | - | -- | - | - | 16.63± 0.05 | T |  | -- | - | - | 
| 56490.38 | 16.68± 0.04 | T |  | -- | - | - | -- | - | - | -- | - | - | 
| 56536.26 | 16.68± 0.05 | - |  | -- | - | - | 16.61± 0.06 | - |  | -- | - | - | 
| 56537.20 | 16.68± 0.05 | - |  | 16.67± 0.07 | - |  | -- | - | - | -- | - | - | 
| 56915.14 | 16.62± 0.03 | A |   | 16.61± 0.05 | A |   | 16.54± 0.04 | A |   | -- | - | - | 
| 57227.33 | 16.68± 0.04 | A |   | 16.67± 0.04 | A |   | 16.60± 0.04 | A |   | -- | - | - | 
| 57310.09 | 16.64± 0.03 | A |   | -- | - | - | -- | - | - | 16.44± 0.06 | A |   | 
| 57633.28 | 16.66± 0.04 | - |  | 16.64± 0.04 | - |  | 16.55± 0.04 | - |  | -- | - | - | 
| 57635.35 | 16.64± 0.05 | - |  | -- | - | - | -- | - | - | 16.49± 0.06 | - |  | 
| 57638.27 | 16.68± 0.05 | - |  | -- | - | - | -- | - | - | 16.55± 0.04 | - |  | 
| 57928.34 | 16.64± 0.04 | A |   | 16.62± 0.05 | A |   | 16.55± 0.05 | A |   | 16.43± 0.07 | A |   | 
| 57958.29 | 16.68± 0.04 | - |  | 16.68± 0.04 | - |  | -- | - | - | 16.56± 0.05 | - |  | 
| 57963.25 | 16.66± 0.06 | T |  | -- | - | - | -- | - | - | -- | - | - | 
| 58035.03 | 16.62± 0.04 | - |  | -- | - | - | 16.52± 0.04 | - |  | -- | - | - | 
| 58043.05 | 16.67± 0.04 | A |   | 16.66± 0.05 | A |   | 16.56± 0.04 | - |  | 16.58± 0.05 | - |  | 
| 58073.09 | 16.66± 0.06 | - |  | 16.59± 0.07 | - |  | -- | - | - | -- | - | - | 
| 58098.09 | 16.71± 0.04 | - |  | 16.70± 0.04 | - |  | 16.62± 0.03 | A |   | -- | - | - | 
| 58312.29 | 16.76± 0.04 | - |  | 16.78± 0.04 | - |  | 16.66± 0.04 | - |  | -- | - | - | 
| 58316.26 | 16.68± 0.04 | - |  | -- | - | - | -- | - | - | 16.54± 0.04 | - |  | 
| 58341.23 | 16.75± 0.05 | - |  | 16.77± 0.05 | - |  | -- | - | - | -- | - | - | 
| 58366.12 | 16.68± 0.03 | - |  | 16.70± 0.04 | - |  | -- | - | - | -- | - | - | 
| 58375.12 | 16.72± 0.04 | - |  | -- | - | - | 16.62± 0.03 | - |  | -- | - | - | 
| 58403.08 | 16.73± 0.04 | - |  | -- | - | - | -- | - | - | 16.62± 0.06 | - |  | 
| 58433.09 | 16.68± 0.06 | - |  | 16.65± 0.06 | - |  | 16.59± 0.06 | - |  | -- | - | - | 
| 58671.29 | 16.72± 0.07 | - |  | 16.78± 0.06 | - |  | -- | - | - | -- | - | - | 
| 58673.29 | 16.75± 0.08 | - |  | -- | - | - | 16.65± 0.07 | - |  | 16.58± 0.08 | - |  | 
| 58696.30 | 16.67± 0.07 | - |  | 16.67± 0.07 | - |  | 16.59± 0.08 | - |  | -- | - | - | 
| 58750.07 | 16.68± 0.07 | - |  | 16.70± 0.06 | - |  | -- | - | - | -- | - | - | 
| 58779.05 | 16.70± 0.06 | - |  | -- | - | - | 16.64± 0.03 | - |  | -- | - | - | 
| 58812.07 | 16.67± 0.08 | - |  | -- | - | - | 16.58± 0.08 | - |  | -- | - | - | 
| 59000.39 | 16.64± 0.07 | - |  | -- | - | - | 16.58± 0.10 | - |  | -- | - | - | 
| 59055.31 | 16.67± 0.07 | - |  | -- | - | - | 16.58± 0.08 | - |  | -- | - | - | 
| 59077.20 | 16.70± 0.07 | - |  | 16.68± 0.07 | - |  | 16.61± 0.07 | - |  | 16.56± 0.10 | - |  | 
| 59131.09 | 16.71± 0.07 | - |  | -- | - | - | 16.61± 0.07 | - |  | -- | - | - | 
| 59166.12 | 16.71± 0.07 | - |  | -- | - | - | -- | - | - | 16.55± 0.09 | - |  | 
| 59194.11 | 16.68± 0.07 | - |  | 16.66± 0.07 | - |  | -- | - | - | -- | - | - | 
| 59376.35 | 16.62± 0.07 | - |  | 16.66± 0.07 | - |  | -- | - | - | -- | - | - | 
| 59409.37 | 16.72± 0.07 | - |  | -- | - | - | 16.62± 0.07 | - |  | -- | - | - | 
| 59441.26 | 16.71± 0.07 | - |  | 16.72± 0.07 | - |  | -- | - | - | 16.65± 0.09 | - |  | 
| 59467.11 | 16.70± 0.07 | - |  | -- | - | - | 16.57± 0.06 | - |  | -- | - | - | 
| 59522.04 | 16.73± 0.07 | - |  | 16.72± 0.07 | - |  | -- | - | - | 16.53± 0.11 | - |  | 
| 59546.05 | 16.68± 0.07 | - |  | -- | - | - | 16.60± 0.07 | - |  | -- | - | - | 
| 59583.10 | 16.62± 0.07 | - |  | 16.63± 0.07 | - |  | -- | - | - | -- | - | - | 
| 59739.36 | 16.68± 0.07 | - |  | 16.70± 0.07 | - |  | 16.59± 0.07 | - |  | -- | - | - | 
| 59816.14 | 16.63± 0.06 | - |  | -- | - | - | -- | - | - | 16.39± 0.07 | - |  | 
| 59851.09 | 16.69± 0.07 | - |  | 16.68± 0.07 | - |  | 16.57± 0.07 | - |  | -- | - | - | 
| 59879.03 | 16.64± 0.07 | - |  | -- | - | - | -- | - | - | 16.60± 0.07 | - |  | 
| 59905.07 | 16.69± 0.07 | - |  | 16.67± 0.06 | - |  | 16.62± 0.07 | - |  | -- | - | - | 
| 60147.26 | 16.72± 0.07 | - |  | 16.69± 0.07 | - |  | -- | - | - | -- | - | - | 
| 60172.17 | 16.68± 0.07 | - |  | 16.68± 0.07 | - |  | 16.59± 0.06 | - |  | 16.43± 0.07 | - |  | 
| 60202.10 | 16.72± 0.06 | - |  | 16.69± 0.07 | - |  | -- | - | - | -- | - | - | 
| 60251.01 | 16.67± 0.08 | - |  | -- | - | - | -- | - | - | 16.56± 0.07 | - |  | 
| 60290.10 | 16.71± 0.07 | - |  | -- | - | - | 16.59± 0.07 | - |  | -- | - | - | 
| 60469.35 | 16.65± 0.06 | - |  | 16.63± 0.07 | - |  | -- | - | - | -- | - | - | 
| 60504.31 | 16.69± 0.07 | - |  | -- | - | - | 16.60± 0.06 | - |  | -- | - | - | 
| 60529.23 | 16.72± 0.07 | - |  | -- | - | - | -- | - | - | 16.52± 0.07 | - |  | 
| 60555.13 | 16.71± 0.06 | - |  | 16.69± 0.06 | - |  | 16.60± 0.05 | - |  | -- | - | - | 
| 60587.10 | 16.70± 0.06 | - |  | -- | - | - | -- | - | - | 16.53± 0.07 | - |  | 
| 60649.08 | 16.71± 0.07 | - |  | 16.70± 0.07 | - |  | 16.61± 0.07 | - |  | -- | - | - | 


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 [0.14 mag] | B [0.20 mag] | R [0.14 mag] | |
|---|---|---|---|
| B [0.20 mag] | 0.72 (31) | ||
| R [0.14 mag] | 0.73 (30) | 0.80 (16) | |
| I [0.25 mag] | 0.29 (19) | 0.28 (7) | 0.20 (5) | 
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) | 0.51 | 1.19 | ||
| R (I|R) | 0.46 | 0.96 | 0.56 | 0.31 | |
| I (I|R) | 0.40 | 0.65 | 0.26 | 0.49 | 0.15 | 0.55 | 
By John C. Martin, University of Illinois Springfield Henry R. Barber Research Observatory
Generated on 2025-08-04 15:53:14 UT-5