Possible Nova in Sgr: Haseda's observation K. Haseda (Aichi, Japan) just reported the following photographic estimates (with f400mm lens and T-Max400(120)). The notation follows that by Kanatsu. Haseda's observation clearly indicates that the variable shows recurring maxima consistent with the Mira-type classification. (Haseda reported that the brightenings of the object has been noticed several times in the past; the detection has not been reported because of a presumed assumption that the object is identical with V4006 Sgr). Photographic magnitude estimates by VSOLJ members object YYYYMMDD(UT) mag code GSC6850.4355 20000313.813 104p Had.VSOLJ GSC6850.4355 20000822.513 <124p Had.VSOLJ GSC6850.4355 20010319.788 <106p Had.VSOLJ GSC6850.4355 20010922.469 106p Had.VSOLJ GSC6850.4355 20020223.000 <134p Had.VSOLJ GSC6850.4355 20020319.826 <134p Had.VSOLJ GSC6850.4355 20020412.793 <134p Had.VSOLJ GSC6850.4355 20020502.648 126p Had.VSOLJ GSC6850.4355 20020511.688 <124p Had.VSOLJ GSC6850.4355 20020521.640 <134p Had.VSOLJ GSC6850.4355 20020609.643 <124p Had.VSOLJ GSC6850.4355 20020710.648 105p Had.VSOLJ GSC6850.4355 20020714.560 106p Had.VSOLJ GSC6850.4355 20020731.524 106p Had.VSOLJ GSC6850.4355 20020805.556 110p Had.VSOLJ GSC6850.4355 20020809.558 114p Had.VSOLJ GSC6850.4355 20020813.535 114p Had.VSOLJ GSC6850.4355 20020827.540 115p Had.VSOLJ Regards, Taichi Kato
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