Airglow Data Obtained at Kiso Station, Tokyo Astronomical Observatory, The University of Tokyo (137.63 E, 35.79 N, altitude=1130m) Airglow intensities at zenith (3 degrees diameter): Observations have been made regularly on moonless clear nights. The reduction of data had been carried out by Photometry Division, Tokyo Astronomical Observatory, The University of Tokyo (1979-1988), and by Optical and Infrared Astronomy Division, National Astronomical Observatory of Japan (1988-1990). Files are named as KMyymm.txt where yy: year mm: month. Data Format example: 1980 1 21 KISO <= year,month,date (raw data value) 4358 5000 5300 OH53 OH53 NO. D H M 4358 5000 5300 RAYLEIGHS S10 S10 S10 RAY STD. ZERO 1 21 22 55 153 154 72 68.2 256.5 237.3 -19.2 -8.1 250 37 2 21 22 56 151 151 72 67.1 250.1 232.7 -17.4 -7.3 249 38 3 21 22 57 151 152 72 66.1 249.8 235.1 -14.7 -6.2 252 37 4 21 22 58 147 151 71 63.7 246.6 222.7 -23.9 -10.0 252 38 5 21 22 59 149 150 72 65.3 246.7 231.6 -15.1 -6.3 250 38 6 21 23 0 149 150 72 65.0 245.6 230.5 -15.1 -6.3 251 38 ........................................ NIGHT MEAN= 64.2 233.0 218.6 -14.5 -6.1 The date in the title line refers to the local date of the evening. The actual observations may be done after midnight, on the next day. (D, H, M) = date and time in JST (=UT+9) wavelength bands 4358 Angstrom (Hg from city light) 5000 Angstrom (background for reference) 5300 Angstrom (background for reference) 5577 Angstrom (O I) 5893 Angstrom (Na D) 6300 Angstrom (O I) STD = standard lamp ZERO = dark signal 1 Rayleigh = 10^6 photons cm^-2 sec-1 /column S10 = equivalent number of 10-th magnitude G0 stars per square degree 1 Rayleigh = 239 S10 at 5300 Angstrom