MJD | V | * | Image | B | * | Image | R | * | Images | I | * | Images |
---|---|---|---|---|---|---|---|---|---|---|---|---|
56599.13 | 16.67± 0.03 | - | 16.92± 0.04 | - | 16.48± 0.04 | - | -- | - | - | |||
56604.11 | 16.68± 0.03 | - | 16.98± 0.03 | - | 16.46± 0.05 | - | -- | - | - | |||
56930.16 | 16.67± 0.03 | - | 16.98± 0.04 | - | 16.46± 0.04 | - | -- | - | - | |||
56951.10 | 16.69± 0.04 | - | 17.00± 0.03 | - | 16.49± 0.05 | - | -- | - | - | |||
57307.14 | 16.66± 0.04 | A | 16.96± 0.03 | A | 16.47± 0.04 | A | -- | - | - | |||
57340.22 | 16.63± 0.06 | - | -- | - | - | -- | - | - | 16.21± 0.08 | - | ||
57634.30 | -- | - | - | 16.96± 0.04 | T | 16.46± 0.06 | T | -- | - | - | ||
57638.23 | 16.66± 0.05 | - | 16.96± 0.05 | - | 16.49± 0.07 | - | 16.28± 0.07 | - | ||||
57743.02 | 16.79± 0.04 | - | 17.06± 0.03 | - | 16.57± 0.02 | - | 16.36± 0.04 | - | ||||
57958.38 | 16.72± 0.03 | - | -- | - | - | 16.52± 0.04 | - | 16.30± 0.04 | - | |||
57963.33 | 16.67± 0.04 | A | 16.96± 0.03 | A | -- | - | - | 16.28± 0.07 | - | |||
57964.26 | 16.71± 0.04 | - | -- | - | - | 16.53± 0.04 | - | -- | - | - | ||
57988.31 | 16.76± 0.03 | - | 17.03± 0.04 | - | -- | - | - | 16.34± 0.04 | - | |||
58035.07 | 16.58± 0.06 | - | -- | - | - | 16.36± 0.07 | - | -- | - | - | ||
58045.10 | 16.73± 0.03 | - | 17.02± 0.04 | - | 16.53± 0.04 | - | -- | - | - | |||
58067.14 | 16.72± 0.03 | - | -- | - | - | -- | - | - | 16.30± 0.04 | - | ||
58073.12 | 16.75± 0.04 | - | 16.98± 0.05 | - | -- | - | - | -- | - | - | ||
58077.14 | 16.76± 0.04 | - | 17.01± 0.03 | - | -- | - | - | 16.37± 0.07 | - | |||
58098.18 | 16.71± 0.03 | - | -- | - | - | -- | - | - | 16.33± 0.04 | - | ||
58103.11 | 16.75± 0.03 | - | 17.02± 0.04 | - | -- | - | - | 16.27± 0.05 | - | |||
58316.31 | 16.71± 0.04 | A | 16.97± 0.04 | A | 16.50± 0.04 | A | -- | - | - | |||
58317.29 | 16.68± 0.04 | A | -- | - | - | -- | - | - | 16.27± 0.06 | A | ||
58339.32 | 16.68± 0.04 | - | 16.97± 0.04 | - | 16.48± 0.05 | - | -- | - | - | |||
58342.23 | 16.68± 0.03 | - | 17.02± 0.03 | - | -- | - | - | 16.29± 0.04 | - | |||
58372.15 | 16.70± 0.03 | A | -- | - | - | -- | - | - | 16.24± 0.05 | A | ||
58373.13 | 16.63± 0.04 | - | 16.95± 0.05 | - | -- | - | - | -- | - | - | ||
58403.14 | 16.66± 0.03 | - | 16.92± 0.03 | - | -- | - | - | -- | - | - | ||
58433.06 | 16.67± 0.03 | - | 16.98± 0.03 | - | 16.49± 0.03 | - | -- | - | - | |||
58672.33 | 16.70± 0.03 | A | 17.01± 0.03 | - | 16.45± 0.04 | - | 16.26± 0.05 | - | ||||
58695.25 | 16.68± 0.03 | A | 16.99± 0.04 | - | 16.51± 0.03 | - | 16.30± 0.04 | - | ||||
58757.06 | 16.71± 0.03 | - | -- | - | - | 16.50± 0.03 | - | -- | - | - | ||
58779.11 | 16.66± 0.03 | - | -- | - | - | 16.47± 0.03 | - | -- | - | - | ||
58784.02 | 16.64± 0.04 | - | 16.93± 0.04 | - | -- | - | - | -- | - | - | ||
58836.09 | 16.71± 0.02 | A | -- | - | - | 16.50± 0.03 | - | 16.25± 0.04 | - | |||
59001.40 | 16.78± 0.05 | T | -- | - | - | -- | - | - | -- | - | - | |
59019.39 | 16.80± 0.03 | - | 17.19± 0.06 | - | -- | - | - | -- | - | - | ||
59026.34 | 16.72± 0.04 | A | -- | - | - | 16.50± 0.05 | - | -- | - | - | ||
59059.28 | 16.73± 0.03 | A | 17.02± 0.03 | A | 16.55± 0.04 | - | 16.30± 0.06 | - | ||||
59081.20 | 16.75± 0.04 | - | -- | - | - | -- | - | - | 16.32± 0.07 | - | ||
59082.29 | 16.70± 0.04 | - | 17.00± 0.04 | - | 16.52± 0.05 | - | -- | - | - | |||
59131.15 | 16.73± 0.04 | A | 17.06± 0.04 | - | 16.53± 0.04 | - | -- | - | - | |||
59166.22 | 16.76± 0.03 | A | -- | - | - | -- | - | - | 16.36± 0.07 | A | ||
59194.17 | 16.74± 0.04 | A | 17.02± 0.03 | - | 16.54± 0.04 | - | -- | - | - | |||
59380.36 | 16.76± 0.05 | A | 17.01± 0.04 | - | 16.61± 0.06 | - | -- | - | - | |||
59415.32 | 16.74± 0.04 | - | -- | - | - | 16.55± 0.06 | - | -- | - | - | ||
59441.34 | 16.78± 0.03 | A | 17.09± 0.03 | - | -- | - | - | 16.33± 0.06 | A | |||
59463.12 | 16.78± 0.03 | - | -- | - | - | -- | - | - | 16.36± 0.06 | - | ||
59483.12 | 16.77± 0.03 | A | 17.05± 0.04 | - | 16.54± 0.04 | - | -- | - | - | |||
59523.05 | 16.73± 0.04 | A | 17.04± 0.04 | - | 16.51± 0.05 | - | 16.28± 0.06 | - | ||||
59548.10 | 16.76± 0.04 | A | 17.04± 0.04 | - | 16.56± 0.04 | - | 16.35± 0.06 | - | ||||
59759.37 | 16.80± 0.05 | - | 17.08± 0.05 | - | 16.59± 0.05 | - | -- | - | - | |||
59794.28 | 16.77± 0.03 | A | 17.02± 0.04 | - | -- | - | - | 16.41± 0.06 | - | |||
59823.20 | 16.71± 0.04 | - | -- | - | - | 16.50± 0.05 | - | -- | - | - | ||
59849.13 | 16.74± 0.03 | A | -- | - | - | -- | - | - | 16.38± 0.06 | A | ||
59903.06 | 16.80± 0.03 | - | 17.07± 0.03 | - | 16.59± 0.04 | - | -- | - | - | |||
59904.08 | 16.72± 0.03 | - | -- | - | - | 16.54± 0.04 | - | 16.36± 0.06 | - | |||
59932.06 | 16.74± 0.03 | A | 17.00± 0.03 | - | -- | - | - | 16.40± 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 [0.27 mag] | B [0.22 mag] | R [0.25 mag] | |
---|---|---|---|
B [0.27 mag] | 0.68 (36) | ||
R [0.25 mag] | 0.83 (33) | 0.54 (24) | |
I [0.20 mag] | 0.52 (27) | 0.06 (15) | 0.69 (10) |
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) | 1.63 | 0.81 | ||
R (I|R) | 1.08 | 1.09 | 0.34 | 0.08 | |
I (I|R) | 0.68 | 1.30 | 0.19 | 0.94 | 0.73 | 1.42 |
By John C. Martin, University of Illinois Springfield Henry R. Barber Research Observatory
Generated on 2023-08-14 14:15:12 UT-5