It appears to be the case that BU Her = GSC 2113-0870, and that the star is also IRAS 18483+2444. The USNO-A2.0 b-r color is ~3.0, so fairly red, confirming the general identity. Are you reporting that you actually observed an outburst by comparison to your own previous observations? If not, then I think you have been caught by the very high near-infrared sensitivity of the CCD chip, which will show cool stars such as BU Her as anomalously bright. The GCVS magnitude range is for blue light, so wil seem much fainter than an unfiltered CCD magnitude. I note that the red magnitude in USNO-A2.0 is 11.7, while the blue magnitude is 14.6. \Brian