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# SN 2003en and 2003eq-eu were discovered at mag 23.2-25.5 # (cosmological). # SN 2003eo was discovered by the NEAT team. The reported brightest # mag is 20.2 on Mar. 27.14. SN2003ep 20021130.2 <190:C KAI SN2003ep 20030517.5 157:C KAI SN2003ep 20030528.5 163:C KAI SN2003ep 20030603.5 167:C KAI # SN 2003ep (21:21:07.34, +23:05:05.8 (J2000.0), offset = 4" due west) # is hosted by NGC7053, a spiral? (S?) galaxy. It embedded within the # central region, so probably the discovery was made by the image # subtraction. The expeced maximum of typical SN Ia is consistent # with the discovery magnitude. SN2003ev 20030409.4 <190:C KAI SN2003ev 20030601.3 185:C KAI SN2003ev 20030602.3 185:C KAI # SN 2003ev (13:10:31.80, -21:39:49.6 (J2000.0), offset = 2"E, 6"N) is # hosted by 2MASX J13103164-2139555, an apparently edge-on spiral # galaxy. In its neighbourhood, there are some galaxies with the # recession velocities are about 3000 km/s or 7000 km/s. If the # latter is near to that of the host galaxy, the expected maximum for # typical SN Ia is mag about 16.8. PSN2003-MCG+07-36-33 20030522.4 <190:C KAI PSN2003-MCG+07-36-33 20030601.4 186:C KAI PSN2003-MCG+07-36-33 20030602.4 183:C KAI PSN2003-MCG+07-36-33 20030603.4 181:C KAI # The object (17:44:07.72, +40:52:51.6 (J2000.0), offset = 10"W, 49"N) # is near to MCG +07-36-33, a possibly nearby spiral (S?) galaxy. The # appearance of the galaxy is rather small, and the new object seems # to be located too far from the center of the galaxy. And, if it # truely belongs to MCG +07-36-33, it is somewhat subluminous for SN # (M about -14.5). The spectroscopic type determination is urged. Sincerely Yours, Hitoshi Yamaoka, Kyushu Univ., Japan yamaoka@rc.kyushu-u.ac.jp
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