Unable to resolved from star J004406.24+420132.4 (4 magnitude fainter) about 1 arcsecond away. That contributes about -0.03 magnitudes in R and V and -0.06 magnitudes in B.
| MJD | V | * | Image | B | * | Image | R | * | Images | I | * | Images | 
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 56142.35 | 15.54± 0.03 | Tb |  | -- | - | - | -- | - | - | -- | - | - | 
| 56267.17 | -- | - | - | -- | - | - | 15.33± 0.04 | Tb |  | -- | - | - | 
| 56537.22 | 15.56± 0.03 | b |  | 16.02± 0.03 | b |  | 15.30± 0.04 | b |  | -- | - | - | 
| 56593.08 | 15.60± 0.03 | b |  | -- | - | - | 15.31± 0.03 | b |  | -- | - | - | 
| 57282.18 | 15.65± 0.03 | b |  | 16.12± 0.04 | b |  | 15.37± 0.04 | b |  | -- | - | - | 
| 57314.14 | 15.66± 0.03 | b |  | -- | - | - | -- | - | - | 15.09± 0.05 | b |  | 
| 57635.41 | 15.53± 0.07 | b |  | 15.98± 0.08 | b |  | 15.26± 0.07 | b |  | 14.97± 0.07 | b |  | 
| 57958.32 | 15.62± 0.06 | b |  | 16.11± 0.06 | b |  | -- | - | - | 15.08± 0.06 | b |  | 
| 57963.28 | 15.65± 0.06 | b |  | 16.09± 0.05 | b |  | 15.37± 0.06 | b |  | -- | - | - | 
| 58045.07 | 15.62± 0.04 | b |  | 16.06± 0.04 | b |  | 15.31± 0.05 | b |  | -- | - | - | 
| 58067.12 | 15.64± 0.05 | b |  | -- | - | - | -- | - | - | 15.09± 0.07 | b |  | 
| 58098.12 | 15.61± 0.06 | b |  | 16.09± 0.05 | b |  | -- | - | - | -- | - | - | 
| 58312.32 | 15.63± 0.05 | b |  | 16.08± 0.04 | b |  | 15.35± 0.05 | b |  | -- | - | - | 
| 58316.28 | 15.68± 0.04 | b |  | -- | - | - | -- | - | - | 15.11± 0.06 | b |  | 
| 58372.12 | -- | - | - | -- | - | - | -- | - | - | 15.04± 0.06 | Tb |  | 
| 58403.12 | 15.57± 0.04 | b |  | -- | - | - | 15.28± 0.06 | b |  | -- | - | - | 
| 58671.30 | 15.70± 0.03 | Tb |  | -- | - | - | -- | - | - | -- | - | - | 
| 58672.32 | 15.61± 0.04 | b |  | -- | - | - | 15.32± 0.05 | b |  | 15.01± 0.07 | b |  | 
| 58695.31 | 15.62± 0.04 | b |  | -- | - | - | 15.34± 0.04 | b |  | 15.05± 0.05 | b |  | 
| 58750.10 | 15.63± 0.03 | b |  | 16.06± 0.02 | b |  | -- | - | - | -- | - | - | 
| 58779.07 | 15.58± 0.03 | b |  | -- | - | - | 15.29± 0.04 | b |  | -- | - | - | 
| 58836.18 | 15.61± 0.03 | b |  | -- | - | - | -- | - | - | 15.05± 0.04 | b |  | 
| 59001.37 | 15.59± 0.04 | b |  | -- | - | - | 15.30± 0.05 | b |  | -- | - | - | 
| 59019.33 | 15.64± 0.05 | b |  | 16.09± 0.04 | b |  | -- | - | - | -- | - | - | 
| 59055.32 | 15.62± 0.04 | Ab |   | 16.06± 0.04 | b |  | 15.34± 0.03 | b |  | 15.05± 0.05 | Ab |   | 
| 59077.22 | 15.61± 0.04 | b |  | -- | - | - | 15.33± 0.04 | b |  | -- | - | - | 
| 59082.20 | 15.64± 0.03 | b |  | 16.10± 0.03 | b |  | 15.34± 0.02 | b |  | -- | - | - | 
| 59131.06 | 15.60± 0.03 | Ab |   | 16.02± 0.04 | b |  | 15.30± 0.03 | b |  | -- | - | - | 
| 59166.08 | 15.60± 0.03 | Ab |   | -- | - | - | -- | - | - | 15.03± 0.05 | Ab |   | 
| 59194.08 | 15.62± 0.03 | Ab |   | 16.07± 0.02 | b |  | 15.34± 0.04 | b |  | -- | - | - | 
| 59376.36 | 15.61± 0.05 | b |  | 16.09± 0.05 | b |  | -- | - | - | -- | - | - | 
| 59379.35 | 15.60± 0.04 | b |  | -- | - | - | 15.30± 0.03 | b |  | -- | - | - | 
| 59409.39 | 15.64± 0.03 | Ab |   | 16.12± 0.06 | b |  | 15.34± 0.04 | b |  | -- | - | - | 
| 59442.28 | 15.61± 0.03 | Ab |   | 16.05± 0.04 | b |  | 15.32± 0.03 | b |  | 15.03± 0.05 | Ab |   | 
| 59467.15 | 15.60± 0.03 | Ab |   | 16.02± 0.03 | b |  | 15.32± 0.04 | b |  | -- | - | - | 
| 59522.07 | 15.62± 0.03 | b |  | 16.05± 0.04 | b |  | -- | - | - | -- | - | - | 
| 59546.08 | 15.58± 0.03 | Ab |   | 16.01± 0.03 | b |  | -- | - | - | 15.04± 0.05 | b |  | 
| 59583.08 | 15.61± 0.04 | Ab |   | -- | - | - | 15.36± 0.05 | b |  | 15.06± 0.04 | b |  | 
| 59753.33 | 15.61± 0.04 | Ab |   | 16.10± 0.04 | b |  | 15.35± 0.04 | b |  | -- | - | - | 
| 59816.18 | 15.59± 0.03 | Ab |   | 16.03± 0.03 | b |  | 15.30± 0.03 | b |  | -- | - | - | 
| 59848.07 | 15.60± 0.03 | Ab |   | 16.05± 0.04 | b |  | -- | - | - | 15.05± 0.03 | b |  | 
| 59851.07 | 15.63± 0.04 | b |  | -- | - | - | 15.35± 0.05 | b |  | 15.07± 0.07 | b |  | 
| 59854.14 | 15.61± 0.03 | b |  | 16.07± 0.03 | b |  | 15.33± 0.03 | b |  | -- | - | - | 
| 59879.07 | 15.60± 0.04 | b |  | 16.03± 0.04 | b |  | -- | - | - | -- | - | - | 
| 59905.22 | 15.60± 0.03 | b |  | 16.04± 0.04 | b |  | -- | - | - | 15.04± 0.05 | b |  | 
| 60147.30 | 15.59± 0.04 | Ab |   | 16.02± 0.03 | b |  | 15.28± 0.04 | b |  | -- | - | - | 
| 60152.39 | 15.57± 0.04 | b |  | 16.03± 0.04 | b |  | -- | - | - | -- | - | - | 
| 60172.29 | 15.59± 0.04 | Ab |   | -- | - | - | 15.30± 0.06 | Ab |   | 15.03± 0.06 | Ab |   | 
| 60202.14 | 15.63± 0.04 | Ab |   | 16.08± 0.04 | Ab |   | 15.38± 0.06 | Ab |   | -- | - | - | 
| 60251.05 | 15.56± 0.04 | Ab |   | 16.02± 0.03 | b |  | -- | - | - | 15.00± 0.05 | b |  | 
| 60290.08 | 15.56± 0.04 | b |  | -- | - | - | -- | - | - | 15.03± 0.06 | b |  | 
| 60292.09 | 15.54± 0.05 | b |  | -- | - | - | -- | - | - | 14.99± 0.08 | b |  | 
| 60533.24 | 15.57± 0.04 | b |  | -- | - | - | -- | - | - | 14.99± 0.06 | b |  | 
| 60555.18 | 15.57± 0.04 | b |  | 16.02± 0.03 | b |  | 15.29± 0.04 | b |  | -- | - | - | 
| 60556.13 | 15.56± 0.04 | b |  | 15.98± 0.04 | b |   | 15.27± 0.04 | b |   | -- | - | - | 
| 60594.03 | 15.59± 0.05 | b |  | -- | - | - | -- | - | - | 15.03± 0.07 | b |  | 
| 60595.05 | 15.66± 0.06 | b |  | 16.11± 0.05 | b |  | 15.39± 0.05 | b |  | -- | - | - | 
| 60651.06 | 15.61± 0.04 | b |  | 16.07± 0.04 | b |  | 15.31± 0.05 | 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 [0.18 mag] | B [0.15 mag] | R [0.13 mag] | |
|---|---|---|---|
| B [0.15 mag] | 0.78 (34) | ||
| R [0.13 mag] | 0.82 (33) | 0.77 (22) | |
| I [0.14 mag] | 0.86 (22) | 0.72 (8) | 0.88 (8) | 
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) | 0.62 | 1.41 | ||
| R (I|R) | 0.42 | 0.90 | -0.60 | 0.05 | |
| I (I|R) | 0.43 | 1.37 | 0.27 | 1.52 | 0.26 | 1.26 | 
By John C. Martin, University of Illinois Springfield Henry R. Barber Research Observatory
Generated on 2025-08-04 15:53:14 UT-5