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SN2003ee 20020405.20 <216C PAL SN2003ee 20030209.51 <210C PAL SN2003ee 20030303.58 178C PAL SN2003ee 20030327.32 165C PAL SN2003ee 20030328.20 165C PAL SN2003ee 20030328.24 165C PAL SN2003ee 20030407.34 165C PAL SN2003ee 20030410.13 165C PAL SN2003ee 20030411.22 166C PAL SN2003ee 20030421.223 16.628B LCO SN2003ee 20030421.223 16.548V LCO SN2003ee 20030421.223 16.383I LCO # SN 2003ee (11:33:24.50, -09:59:26.4 (J2000.0), offset = 1"E, 1"S) is # hosted by an anonymous compact blue galaxy. The spectrum taken at # the Las Campanas Observatory on May 5.10 UT suggests that it is a # type IIn supernova with a blue continuum, at z = 0.021. The # observed brightness is comparable to the expected maximum of SN Ia, # and it remains blue a month or more from the explosion, which # suggest that this SN is somewhat peculiar. SN 2003dq: In [vsnet-campaign-sn 605] (Apr. 15) >SN2003dq 20020402.27 <218C PAL >SN2003dq 20030324.16 <215C PAL >SN2003dq 20030325.24 <213C PAL >SN2003dq 20030409.42 190C PAL >SN2003dq 20030410.15 189C PAL > ># SN 2003dq (11:04:45.44, +15:26:49.4 (J2000.0), offset = 2" due ># south) is hosted by a dim (mag 19) spiral galaxy MAPS-NGP ># O_432-0786358, which is an eastern component of a pair of galaxies. The Las Campanas spectrum on May 5.06 UT shows that it is type II SN several weeks after explosion. SN 2003dt: In [vsnet-campaign-sn 618] (May 6) > It turned out to be type Ia SN several weeks after maximum on May > 5.45. The Las Campanas spectrum taken on May 5.35 suggests that it is about 3 months past maximum. SN(?) 2003ec: In [vsnet-campaign-sn 615] (May 4) >SN2003ec 20030502.801 164V LuO >SN2003ec 20030503.662 164V LuO > ># SN 2003ec (15:46:16.67, +2:24:48.7, offset = 4"E, 7"S) is hosted by ># NGC 5990, a spiral ((R')Sa pec?) galaxy. The expected maximum for ># typical SN Ia is mag about 15.6. K. Itagaki reported that this object can be clearly seen on his CCD images taken on 2001 May 13 and 2002 May 3, which suggests that it is a foreground star. The Las Campanas spectrum of this object on May 5.33 UT shows a featureless blue continuum. In the DSS 2 blue image this object emerged from the glow of the host galaxy, though it is buried in DSS red images. Sincerely Yours, Hitoshi Yamaoka, Kyushu Univ., Japan yamaoka@rc.kyushu-u.ac.jp
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