From fidusz@freemail.c3.hu Sat Oct 31 17:11 JST 1998 Date: 31 Oct 1998 09:11:09 +0100 MIME-Version: 1.0 To: tkato@kusastro.kyoto-u.ac.jp Subject: UV Aur sequ From: Fidrich Robert <fidusz@freemail.c3.hu> Content-Type: text Content-Length: 814 Dear VSNET Folks, I have at least 3 different sequence for the UV Aur. The differecne beetven the magnitudes reaches 1 magn. Please could you tell me which sequence should one use for the future? Here at the HAA/VSS we used the AFOEV sequence that go down only to 95 os so. The BAA use the same sequence and added visual estimated mags for fainter stars as for as I know. Two years ago I've got the sequence (based on GSC) that VSNET observers use. The comparison beetween the sequence I know is listed below... star GSC number (BAA) (VSNET) VT or Vj -------------------------------------- A 2394.465 70 C 2394.790 82 94 85 D 2394.687 87 98 88 E 2394.102 91 95 G 2394.992 93 95 H 2394.1328 100 105 107 J 2394.113 104 105 106 K 2394.788 108 112 L 114 Regards, Robert