[IAUC] CBET 762: 20061129 : SUPERNOVAE 2006oy-2006qm

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                                                  Electronic Telegram No. 762
Central Bureau for Astronomical Telegrams
INTERNATIONAL ASTRONOMICAL UNION
M.S. 18, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
IAUSUBS en CFA.HARVARD.EDU or FAX 617-495-7231 (subscriptions)
CBAT en CFA.HARVARD.EDU (science)
URL http://cfa-www.harvard.edu/iau/cbat.html


SUPERNOVAE 2006oy-2006qm
     Further to CBETs 611 and 745, B. Bassett, South African Astronomical
Observatory (SAAO); A. Becker, University of Washington (UW); H. Brewington,
Apache Point Observatory (APO); C. Choi, Seoul National University (SNU);
D. Cinabro, Wayne State University; F. DeJongh, Fermilab; J. Dembicky, APO;
D. L. DePoy, Ohio State University (OSU); B. Dilday, University of Chicago
(UC); M. Doi, University of Tokyo (UoT); J. Frieman, Fermilab and UC; P.
Garnavich, University of Notre Dame; M. Harvanek, APO; C. Hogan, UW; J.
Holtzman, New Mexico State University; M. Im, SNU; S. Jha, Stanford
University (SU); K. Konishi, UoT; J. Krzesinski, APO; H. Lampeitl, Space
Telescope Science Institute (STScI); R. Kessler, UC; B. Ketzeback, D. Long,
O. Malanushenko, and V. Malanushenko, APO; J. Marriner and D. McGinnis,
Fermilab; R. McMillan, APO; G. Miknaitis, Fermilab; T. Morokuma, UoT; R.
Nichol, University of Portsmouth (UP); K. Pan, APO; J. L. Prieto, OSU; M.
Richmond, Rochester Institute of Technology; A. Riess, STScI; R. Romani,
SU; M. Sako, University of Pennsylvania; G. Saurage, APO; D. Schneider,
Pennsylvania State University; M. Smith, UP; S. Snedden, APO; N. Takanashi
and K. Tokita, UoT; K. van der Heyden, SAAO; S. Watters, APO; C. Wheeler,
University of Texas; N. Yasuda, UoT; and C. Zheng, SU, on behalf of the
Sloan Digital Sky Survey II collaboration, report the discovery of
forty-one new supernovae on multiple g, r, and i images taken with the
SDSS 2.5-m telescope at APO by the SDSS observing team, with 34 of them
confirmed as type-Ia supernovae, one as a type-I supernova, one as a
probable type-Ia supernova, two as type-II events, one as a probable
type-II supernova, one as a probable type-Ib supernova, and one as a
probable type-Ic hypernova.
     Romani, Zheng, Sako, Wheeler, and Schneider, together with U. Hopp
(University of Munich) and W. Kollatschny (University of Goettingen),
report that spectroscopic observations with the Hobby Eberly Telescope
on Nov. 20-25 UT indicate that 2006oy, 2006pb, 2006pd, 2006ph, 2006pk,
2006pj, 2006pg, 2006pm, 2006pi, and 2006pl are type-Ia supernovae,
and 2006pa is a probable type-Ia supernova.
     M. Stritzinger and J. Sollerman, Dark Cosmology Center (DCC); A.
Goobar, University of Stockholm (US); and R. Nichol and M. Smith, UP,
report that observations by Stritzinger and G. Leloudas (DCC) with the
Nordic Optical Telescope on Nov. 23 indicate that 2006pn, 2006ps,
and 2006pr are type-Ia supernovae, 2006oz is a probable type-Ib event,
and 2006pu is a type-II supernova.
     R. J. Foley and A. V. Filippenko, University of California,
Berkeley, report that observations with the Keck I telescope (+ LRIS)
on Nov. 23 UT indicate that 2006pq, 2006pf, 2006pt, and 2006pz are
type-Ia supernovae.
     A. Aragon-Salamanca, University of Nottingham; M. Bremer,
University of Bristol; M. Turatto, University of Padova; A. Goobar,
US; R. Nichol, UP; J. Sollerman, University of Copenhagen; P.
Ruiz-Lapuente and F. Castander, University of Barcelona; A. Romer,
University of Sussex; C. Collins, Liverpool John Moores University; and
J. Lucey and A. Edge, University of Durham, report that spectroscopy
obtained by M. Smith (UP), L. Ostman (US), and J. Sollerman on Nov. 24
and 25 UT with the European Southern Observatory 3.6-m New Technology
Telescope shows that 2006py, 2006pe, 2006po, 2006qc, 2006qg, 2006qh,
and 2006qj are type-Ia supernovae, 2006qk is a probable type-Ic
hypernova, and 2006pc is a type-II supernova.
     Spectroscopic observations with the Subaru 8-m telescope by N.
Takanashi, Y. Ihara, T. Morokuma, K. Tokita, K. Konishi, and N. Yasuda
on Nov. 26 UT indicate that 2006pw, 2006qe, 2006pp, 2006qi, 2006ql,
2006qa, 2006qb, 2006pv, 2006qd, and 2006px are type-Ia supernovae,
2006qm is a type-I supernova, and 2006qf is a probable type-II
supernova.
     The discovery magnitudes tabulated below are all SDSS g
magnitudes.  Spectroscopic redshifts are given in the column labelled
"z".  Peak dates (all 2006) are approximate estimates from early fits
to the multi-band light curves or from the spectra.


SN       Discov.       R.A. (2000.0) Decl.     Mag.    z    Estimated
         Date UT                                            Peak Date
2006oy   Oct. 12    20 53 58.30  - 0 21 36.2   22.4   0.20   Oct. 23
2006oz   Oct. 20    22 08 53.56  + 0 53 50.4   22.3    --    --
2006pa   Oct. 22     2 32 23.95  - 0 42 48.9   22.0   0.25   Nov. 3
2006pb   Oct. 23     0 46 43.55  - 1 01 58.5   21.9   0.17   Nov. 2
2006pc   Oct. 28     1 44 10.58  - 0 09 21.2   22.5   0.06   Nov. 6
2006pd   Nov.  8    23 31 46.12  - 0 40 05.0   21.1   0.19   Nov. 13
2006pe   Nov.  9     0 23 09.17  - 0 03 13.1   21.0   0.16   Nov. 18
2006pf   Nov.  9     1 41 45.13  - 0 11 20.9   22.5   0.4    Nov. 17
2006pg   Nov.  9     3 27 20.71  + 1 05 22.8   22.1   0.32   Nov. 11
2006ph   Nov.  9    21 34 33.48  - 0 53 09.0   21.3   0.24   Nov. 13
2006pi   Nov.  9    22 03 16.60  - 0 36 24.6   22.0   0.37   Nov. 17
2006pj   Nov.  9    22 37 18.35  + 0 44 17.3   22.2   0.31   Nov. 19
2006pk   Nov.  9    23 04 59.85  - 0 52 24.1   21.4   0.25   Nov. 18
2006pl   Nov. 11    21 54 26.92  + 0 35 18.7   21.9   0.2    Nov. 22
2006pm   Nov. 11    21 54 50.28  + 0 56 01.2   21.7   0.21   Nov. 19
2006pn   Nov. 13     3 49 02.85  - 0 31 58.0   21.6   0.13   Nov. 28
2006po   Nov. 13    20 23 15.17  - 0 50 54.6   21.4   0.18   Nov. 20
2006pp   Nov. 14     0 48 58.47  + 0 28 37.0   22.6   0.34   Nov. 25
2006pq   Nov. 14     1 25 07.05  - 1 13 08.2   22.2   0.2    Nov. 29
2006pr   Nov. 14     1 34 14.69  - 0 24 13.1   21.7   0.11   Nov. 26
2006ps   Nov. 14     1 43 45.30  - 1 06 42.9   22.2   0.1    Dec. 3
2006pt   Nov. 14     2 27 16.17  - 0 23 36.5   22.1   0.30   Nov. 19
2006pu   Nov. 14     2 42 53.82  + 0 53 34.3   21.5   0.15   Nov. 25
2006pv   Nov. 14     3 38 29.47  - 0 40 32.1   21.4   0.21   Nov. 22
2006pw   Nov. 14    22 46 26.96  + 1 09 02.9   22.6   0.33   Nov. 16
2006px   Nov. 14    23 33 17.10  + 0 57 40.0   22.3   0.28   Nov. 25
2006py   Nov. 15    22 41 42.05  - 0 08 12.9   21.3   0.06   Dec. 4
2006pz   Nov. 16     2 55 08.24  + 0 14 05.2   22.7   0.33   Oct. 29
2006qa   Nov. 16     3 01 09.73  - 0 01 34.5   23.0   0.40   Nov. 20
2006qb   Nov. 16     3 28 14.65  - 0 12 03.5   22.3   0.33   Nov. 12
2006qc   Nov. 16    20 51 19.84  - 0 57 08.4   22.6   0.2    Dec. 1
2006qd   Nov. 16    23 08 05.14  - 0 10 33.9   22.6   0.27   Nov. 25
2006qe   Nov. 16    23 12 19.98  - 0 32 03.9   22.8   0.39   Nov. 19
2006qf   Nov. 17     3 51 57.24  - 0 23 47.8   22.3   0.17   Nov. 22
2006qg   Nov. 18    21 54 18.09  + 0 26 49.2   22.0   0.23   Nov. 30
2006qh   Nov. 19    21 47 53.02  + 0 42 24.6   22.4   0.12   Nov. 29
2006qi   Nov. 20     1 50 19.56  + 0 53 05.6   22.2   0.19   Nov. 23
2006qj   Nov. 20    20 11 05.61  - 0 19 11.8   21.4   0.11   Nov. 27
2006qk   Nov. 22    22 25 32.38  + 0 09 15.1   21.4   0.06   Dec. 5
2006ql   Nov. 23     1 50 09.11  + 0 25 13.7   22.8   0.27   Nov. 26
2006qm   Nov. 23     2 42 24.07  - 0 47 47.5   22.6   0.14   Dec. 4


NOTE: These 'Central Bureau Electronic Telegrams' are sometimes
      superseded by text appearing later in the printed IAU Circulars.

                         (C) Copyright 2006 CBAT
2006 November 29                 (CBET 762)               Daniel W. E. Green


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