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Circular No. 8640
Central Bureau for Astronomical Telegrams
INTERNATIONAL ASTRONOMICAL UNION
Mailstop 18, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
IAUSUBS@CFA.HARVARD.EDU or FAX 617-495-7231 (subscriptions)
CBAT@CFA.HARVARD.EDU (science)
URL http://cfa-www.harvard.edu/iau/cbat.html ISSN 0081-0304
Phone 617-495-7440/7244/7444 (for emergency use only)
SUPERNOVAE 2005lb-2005lq
CBET 315 contains information for sixteen newly discovered
supernovae found on multiple g, r, and i images taken with the SDSS
2.5-m telescope and reported by J. Frieman on behalf of the Sloan
Digital Sky Survey II collaboration; all of the new objects are
type-Ia supernovae except for 2005lb and 2005lc (type-II events)
and 2005lm (probable type-II event). Fourteen of the supernovae
were discovered at mag g > 20; the other two are tabulated below:
SN Date UT R.A. (2000.0) Decl. Mag. z
2005lb Sept. 10 22 54 50.05 - 0 15 09.0 18.0 0.03
2005lc Sept. 10 3 02 11.18 - 1 09 59.4 18.8 0.01
V1663 AQUILAE
R. C. Puetter, University of California at San Diego; R. J.
Rudy, D. K. Lynch, S. Mazuk, and C. C. Venturini, The Aerospace
Corporation; R. B. Perry, Langley Research Center, NASA; and B.
Walp, Lick Observatory, report 0.47- to 2.5-micron spectroscopy of
V1663 Aql (cf. IAUC 8540, 8544) with the Lick 3.0-m telescope (+
VNIRIS) at Nov. 14.160 UT. The optical spectrum was largely
nebular, showing [O III], [N II], H_alpha, and weak He I 587.6-nm,
He I 706.5-nm, and [O I]. Weak neutral lines of O I and C I were
present. The spectrum showed coronal-line emission of [S VIII],
[S IX], strong [Si VI] and [Si VII], weak [Ca VIII], and the
unidentified novae lines. The emission lines were flat-topped with
minor structure, and their FWHM and FWZI were 2000 km/s and 2600
km/s, respectively. Based on the O I lines, which are about
equally produced by Lyman_beta and continuum fluorescence, the
reddening is possibly as large as 2 magnitudes in E(B-V).
COMETS C/2005 S12 AND C/2005 S13 (SOHO)
Two additional Kreutz sungrazing comets have been found on
SOHO website images (cf. IAUC 8638), their first available
positions given below. C/2005 S12 was stellar in C3 images,
reaching mag 7.0 at 11.1 solar radii on Sept. 26.431. S/2005 S13
was tiny, stellar, and too faint for photometry in C3 images, and
both objects were faint and diffuse in C2 images.
Comet 2005 UT R.A.(2000)Decl. Inst. F MPEC
C/2005 S12 Sep. 26.154 11 53.8 - 2 05 C3/2 HS 2005-X11
C/2005 S13 29.821 12 05.8 - 3 41 C3/2 BZ 2005-X11
(C) Copyright 2005 CBAT
2005 December 5 (8640) Daniel W. E. Green
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