NGC 4151 ASCA-VSNET multiwavelength campaign: photometry guideline We recommend to use one or a few of the following comparison stars. (J2000.0) V B-V U-B spec name =============================================================== GSC3017.903 121043.76 +391925.3 9.83 0.59 -0.01 G0 GSC3017.1484 121031.35 +392641.2 11.47 1.00 0.80 sq1_2 GSC3017.1357 120955.95 +392825.7 11.22 1.02 0.83 sq1_5 GSC3017.1470 121012.41 +391934.3 12.58 0.65 0.22 sq1_4 GSC3017.1645 121038.53 +392029.3 12.79 1.22 1.40 sq1_3 For small telescopes with wide FOVs, the first comparison star would provide the best statistics and the suitable color. The second or third comparison star would be suitable for smaller FOVs. Some notes: (1) Please use the fixed aperture size to minimize the effect of galaxy comtamination. (2) PSF-fitting photometry might yield less contamination, but the nucleus is bright enough for usual aperture photometry. (3) Multicolor photometry is strongly encouraged. (4) Please make observations on as many possible nights in order to make sufficient zero-point adjustment between observers. Single-night observation is usually useless. (5) No dense time-series is necessary. However, several points during one night would help when correlating observations. (6) Report your observations in differential magnitudes to these comparison stars (or fully reduced magnitude), with UT, bands and other information. (7) The expected variation would be smaller than errors of visual observations. However, there was an occasion when the rise reported by visual observers coincides with the spectroscopic change in the broad line. According to the reports to VSNET, the source has been on a stready decline from the 1995 bright state. Regards, Taichi Kato VSNET Collaboration team