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# SN 2003df is dim (mag > 20) one discovered from NEAT images. The # host galaxy is 2MASX J12073149+2657279 (mag about 18). SN2003dg 20030324.4 <200:C KAI SN2003dg 20030408.4 193:C KAI SN2003dg 20030409.4 191:C KAI # SN 2003dg (11:57:31.97, -01:15:13.6 (J2000.0), offset = 2"E, 3"S) is # hosted by UGC 6934, an edge-on spiral (SA(r)cd: sp0) galaxy. The # expected maximum for typical SN Ia is mag about 16.1. # The SN component which has been emerged from the afterglow of GRB # 030329 is assigned as SN 2003dh. The brightness of SN component # itself is estimated as below mag 20, besides the afterglow persists # at mag 19. SN2003di 20020222.53 <206C PAL SN2003di 20020401.41 <205C PAL SN2003di 20030204.58 178C PAL SN2003di 20030204.60 178C PAL SN2003di 20030211.60 171C PAL SN2003di 20030224.64 172C PAL SN2003di 20030307.54 179C PAL SN2003di 20030314.40 180C PAL SN2003di 20030325.39 184C PAL SN2003di 20030408.15 192C PAL # SN 2003di (12:00:24.08, +11:58:26.5 (J2000.0), offset = 17"E, 11"N) # is hosted by a small galaxy near MCG +02-31-010 = CGCG 069-017. If # the host galaxy is at the same distance as MCG +02-31-010, the # maximum magnitude is consistent with the expected maximum for SN Ia. Sincerely Yours, Hitoshi Yamaoka, Kyushu Univ., Japan yamaoka@rc.kyushu-u.ac.jp
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