[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]

[vsnet-campaign-sn 518] SN observations from IAUC 8031

SN2002jo  20020905.0  <185C  Dim
SN2002jo  20021211.20  164C  Dim
SN2002jo  20021211.23  164C  Dim
SN2002jo  20021212.21  163C  Dim

# NGC 5708, a host galaxy of SN 2002jo (14:38:16.42, +40:27:14.0
# (J2000.0), offset = 1"E, 10"S), is a late spiral (Sdm:) galaxy.
# There is a foreground star (mag about 13) about 36" SSE of the
# nucleus, so the SN is located on the way to this star from the
# nucleus.  The expected maximum for typical SN Ia is mag about 14.5
# when unreddened within the host galaxy.  The UCB team took a
# spectrum of it on Dec. 12 UT, which revealed that it is a reddened
# SN Ia about 3 weeks after maximum.

SN2002jp  20020514.2  <185C  KAI
SN2002jp  20021123.5   169C  KAI
SN2002jp  20021207.5   167C  KAI
SN2002jp  20021210.5   171:C SCH
SN2002jp  20021211.5   172C  KAI

# NGC 3313, a host galaxy of SN 2002jp (10:37:26.50, -25:21:35.2
# (J2000.0), offset = 14"E, 146"S), is a barred-spiral (SB(r)b) galaxy
# with a ring structure.  The SN is located well outside of the spiral
# arm.  There is a bright (rmag about 12-13) foreground star 5" NNW of
# the nucleus of NGC 3313.  The UCB team also took a spectrum of this
# SN as above, and revealed that it is a type Ic SN about 2 weeks
# after maximum.

VSNET Home Page

Return to Daisaku Nogami