New Haseda variable (HadV95) Katsumi Haseda (Aichi, Japan) reports the discovery of a new variable star (HadV95). HadV95 = GSC6790.500 154639.42 -295251.9 (2000.0) 13.62 0 = USNO0600.10735586 154639.417 -295251.85 (2000.0) 11.0 14.4 = 2MASS 154639.473 -295252.34 (2000.0) 7.631 6.726 6.357 = IRAS15435-2943 154333.8 -294335 (1950.0) F12=0.83 F25=0.40 F60=0.40L F100=9.12L VAR=77 LRS=-1 possibly II: variable star with 'young' O-rich circumstellar shell or VII: variable star with more evolved C-rich circumstellar shell or VIa: non-variable star with relatively cold dust at large distance, may be carbon-rich = 154639.1 -295250 (2000.0) FSC15435-2943 0.771 0.414 0.574L 4.119L = 154639.3 -295251 (2000.0) IRAS15435-2943 0.795 0.412 0.400L 8.851L 77% = 154639.3 -295251 (2000.0) SSC15435-2943 0.795 0.412 0.400L 8.851L HadV95 SR: 12.8-14.4p Photographic magnitude estimates by VSOLJ members object YYYYMMDD(UT) mag code HadV95 19960326.776 141p Had.VSOLJ HadV95 19990221.799 128p Had.VSOLJ HadV95 19990222.815 129p Had.VSOLJ HadV95 20000114.833 132p Had.VSOLJ HadV95 20000211.819 128p Had.VSOLJ HadV95 20010201.847 128p Had.VSOLJ HadV95 20010304.797 131p Had.VSOLJ HadV95 20010511.658 144p Had.VSOLJ HadV95 20010626.583 129p Had.VSOLJ HadV95 20010713.556 129p Had.VSOLJ Observer's code: Had: K. Haseda (Aichi, Japan) Instruments: 10cm F4.0 twin patrol camera +T-Max400(120)