130 LY HYDRAE (UGSU) Range: 14.0-18.5V Position: 13 31 53.89 -29 40 58.9 (J2000, from .dat file) Magnitude: V=18.530 B-V=-0.111 (Henden, single night) ID RA (2000) DEC X Y N V ERR B-V ERR a) Comparison star sequence 1 13 31 45.1 -29 42 55 -115 -116 3 11.096 0.166 0.228 0.014 2 13 31 51.5 -29 37 29 -32 210 3 11.918 0.020 0.601 0.006 3 13 32 15.0 -29 38 20 275 159 3 12.164 0.018 0.580 0.004 4 13 31 49.8 -29 39 51 -54 68 3 12.778 0.016 0.585 0.012 5 13 31 47.8 -29 43 26 -80 -147 3 13.086 0.019 0.635 0.005 6 13 32 10.3 -29 37 24 214 215 3 14.451 0.022 0.733 0.009 7 13 32 02.2 -29 39 36 108 83 3 14.833 0.014 0.773 0.005 8 13 31 49.0 -29 42 14 -64 -75 3 15.413 0.022 0.612 0.008 9 13 32 10.1 -29 42 48 211 -109 3 15.642 0.022 0.612 0.019 10 13 31 59.8 -29 41 21 77 -22 3 16.071 0.027 1.156 0.021 11 13 31 53.1 -29 41 44 -11 -45 3 17.269 0.049 0.663 0.048 12 13 31 45.5 -29 41 08 -110 -9 2 18.144 0.019 0.677 0.069 b) Wide-colour extension for CCD calibration 13 31 51.4 -29 43 44 -33 -165 3 17.195 0.041 0.400 0.053 13 31 34.9 -29 42 55 -248 -116 3 17.097 0.038 0.432 0.044 13 32 05.7 -29 36 11 154 288 3 14.786 0.013 1.224 0.010 Notes: 1. Star #1 is saturated, and is only accurate to about 0.2 magnitude. This star was also measured by Tycho-2 at V=11.02+/-0.09. This magnitude needs to be used with care. 2. Classified as NL in GCVS 4th edition (Kholopov, et al. 1985). However possible superhumps were detected by Vrielman during the April 1998 outburst, but they were not confirmed. Thus the reality of the SU UMa nature of this variable is still to be determined. Also known as Hya2 (Downes and Shara, 1993). 3. Varies at minimum between about V=17.7 and V=18.5. Bruce Sumner 14 April 1999 Revised 10 June 1999 Revised 5 December 2000