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[vsnet-campaign-sn 709] SNe classifications

Dear SN watchers,

  IAUC 8225 informed the classifications of the recent three SNe by
the CfA group.  The spectra can be seen at:
http://cfa-www.harvard.edu/cfa/oir/Research/supernova/RecentSN.html .

SN 2003io:
In [vsnet-campaign-sn 704] (Oct. 3):
>SN2003io  20000107.0  <200:C Puc
>SN2003io  20030930.27  171C  Puc
># SN 2003io (2:17:26.87, +14:34:36.3 (J2000.0), offset = 11"E, 13"S)
># is hosted by UGC 1761, an irregular (Im) galaxy within a small group
># of galaxies.  The expected maximum for typical SN Ia is mag about
># 15.5. 

  It is a type II SN.

SN 2003iq:
In [vsnet-campaign-sn 705] (Oct. 9):
>SN2003iq  20031005.97  <175:CR  LLA
>SN2003iq  20031008.958  164:CR  LLA
>SN2003iq  20031009.60   160:R   BiS
>observers: BiS: Bisei Astronomical Observatory
># SN 2003iq (1:59:19.92, +17:59:41.8 (J2000.0), offset = 5"E, 46"S)
># appears in the same spiral (SA(s)b) galaxy NGC 772 as SN 2003hl.
># At the discovery, the new object is slightly brighter than SN
># 2003hl.  The expected maximum for typical SN Ia in this galaxy  
># is mag about 14.7.  Further observation and spectral classification
># is urged. 

  It is also a type II SN, with a very blue continuum (a young SN) and
relatively strong He line.

SN 2003is:
In [vsnet-campaign-sn 707] (Oct. 16):
>SN2003is  20031004.1 <195:C  KAI
>SN2003is  20031014.1  180:C  KAI
>SN2003is  20031015.1  180:C  KAI
># SN 2003is (19:21:08.00, +43:19:35.4 (J2000.0), offset = 4"W, 4"N) is
># hosted by MCG +07-40-3 = UGC 11430, a face-on spiral (SA(s)c galaxy.
># Because of a low Galactic latitude (b = 13o), there are many
># foreground stars around MCG +07-40-3; a mag 14 star is located about
># 25" NE of the center of the galaxy.  The expected maximum for
># typical SN Ia is mag about 16.3.

  It is a type Ic SN, probably somewhat (a few days) before maximum
light on Oct. 16.18 UT.

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