Re: IAUC draft

From: Tony Spadafora (ALSpadafora@lbl.gov)
Date: Tue Mar 18 2003 - 18:02:35 PST

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    Dear Mamoru,

    Regarding the SCP names, the first three lines should be:

    > M. Doi, Univ. of Tokyo, on behalf of the Supernova Cosmology
    > Project (cf. IAUC 7971, plus B. Lee and R. Vogel)
    > and the Subaru high-redshift supernova

    -Tony

    ps If there was anyone else new on SCP who was involved but not listed
    on IAUC 7764 plus 7971, they should please let me know)

    Mamoru Doi wrote:
    >
    > Dear all,
    >
    > Here is a revised draft for the IAUC for last fall run.
    > Based on discussions on LBNL-Japan meeting last week,
    > SuF02-81, 12, 83 were moved to the category "not confirmed
    > with spectroscopy". There may be still some. We also add
    > SuF02-05.
    >
    > Do we include HST follow-up information?
    >
    > Please give us any suggestions, comments,
    >
    > -Mamoru and Naoki
    >
    > ---------------------------------------------------------------------
    > M. Doi, Univ. of Tokyo, on behalf of the Supernova Cosmology
    > Project (cf. IAUC 7763 and 7764, plus V. Prasad, G. Sainton, E.
    > Smith, and A. Spadafora) and the Subaru high-redshift supernova
    > search group (N. Yasuda, N. Kashikawa, K. Motohara, T. Morokuma,
    > K.Sekiguchi, G. Kosugi, H. Furusawa, Y. Komiyama, T. Takata,
    > M. Ouchi, Y. Ohyama, and Subaru Observatory SXDS Project members),
    > reports the discovery of possible 29 supernovae found with Subaru
    > telescope +prime-focus Suprime-Cam in SDSS i' band. Reference
    > images were taken on Sep. 30 and Oct.1, 2002. The limiting magnitude
    > of reference images was about 26.6mag (S/N=5 for 2arcsec aperture).
    > We took search images on Nov. 3. The magnitude increase of the
    > SNe compared with the images in the reference are given in the
    > table below (photometric accuracy 0.1-0.2mag).
    >
    > Follow-up photometry was carried out with Suprime-Cam, and we
    > confirmed SN signals at least 3 epochs among 7
    > (Nov.3,6,10,28,30,Dec.7,8) for 30 SNe below.
    >
    > The supernova spectra were obtained at the Gemini telescope on
    > Nov. 6, 8, and 9; at the KeckII Telescope on Nov. 6, 7, 9, and 10;
    > at the Very Large Telescope on Nov. 7 - 10; and at the Subaru
    > telescope on Nov. 12. Redshifts were obtained for 19 SNe
    > using either the host galaxy spectrum or with template spectrum
    > fitting of SN.
    >
    > SCPname 2002 UT R.A. (J2000) Decl. i' z type host info.
    > SuF02-065 Nov. 3.3 02:17:34.53 -05:00:15.4 25.2 1.18 Ia 1.3" SSE
    > SuF02-060 Nov. 3.3 02:17:34.51 -04:53:46.6 24.5 1.063 Ia 0.0"
    > SuF02-007 Nov. 3.3 02:18:52.36 -05:01:13.2 24.8 1.18? Ia no host
    > SuF02-061 Nov. 3.3 02:17:22.73 -05:16:56.1 24.7 1.08? ? 0.0"
    > SuF02-017 Nov. 3.3 02:16:45.71 -05:09:51.2 25.0 1.0? Ia no host
    > SuF02-071 Nov. 3.3 02:17:08.63 -05:02:06.4 23.8 0.928 Ia 1.4" E
    > SuF02-037 Nov. 3.3 02:17:43.30 -04:30:56.7 24.6 0.926 Ia 0.4" E
    > SuF02-000 Nov. 3.3 02:17:42.54 -05:06:34.0 24.8 0.92 Ia? 0.5" NE
    > SuF02-005 Nov. 3.3 02:18:35.7 -04:31:11.0 24.6 0.863 ? 0.3" NE
    > SuF02-002 Nov. 3.3 02:17:12.24 -04:55:08.7 24.4 0.823 Ia? 0.3" NW
    > SuF02-021 Nov. 3.3 02:18:10.56 -04:40:20.6 24.6 0.69 Ia? 2.9" SSW
    > SuF02-055 Nov. 3.3 02:18:53.20 -04:32:59.2 23.7 0.66 Ia 0.6" N
    > SuF02-082 Nov. 3.3 02:18:40.73 -05:03:44.3 25.3 0.623 Ia? 1.1" NNW
    > SuF02-025 Nov. 3.3 02:16:23.93 -04:49:29.4 24.5 0.606 Ia 0.2" W
    > SuF02-077 Nov. 3.3 02:18:35.15 -04:26:38.9 25.1 0.59 Ia? 0.6" NW
    > SuF02-001 Nov. 3.3 02:17:00.05 -04:58:19.6 23.4 0.57 Ia 0.5" W
    > SuF02-019 Nov. 3.3 02:17:38.08 -05:08:46.8 24.5 0.505 Ia? 0.3" NW
    > SuF02-028 Nov. 3.3 02:16:56.37 -05:00:57.4 24.9 0.347? ? 1.5" SE
    > SuF02-059 Nov. 3.3 02:20:28.06 -04:58:50.3 25.7 0.269 Ia? 0.2" E
    >
    > SCPname 2002 UT R.A. (J2000) Decl. i' host info.
    > SuF02-081 Nov. 3.3 02:20:07.55 -05:08:27.2 25.1 0.0"
    > SuF02-012 Nov. 3.3 02:18:51.59 -04:47:24.8 25.1 0.2" N
    > SuF02-083 Nov. 3.3 02:18:06.22 -05:00:38.1 26.0 0.4" S
    > SuF02-034 Nov. 3.3 02:18:31.21 -05:01:24.4 25.6 0.2" N
    > SuF02-004 Nov. 3.3 02:18:09.01 -04:54:17.9 25.1 0.6" SE
    > SuF02-086 Nov. 3.3 02:17:16.18 -05:06:02.7 26.2 no host
    > SuF02-076 Nov. 3.3 02:16:26.37 -05:04:32.5 26.1 no host
    > SuF02-J01 Nov. 3.3 02:17:45.97 -04:36:46.2 25.2 0.2" W
    > SuF02-051 Nov. 3.3 02:17:27.48 -04:40:45.2 25.4 no host
    > SuF02-057 Nov. 3.3 02:20:13.92 -05:07:36.0 25.6 no host
    > SuF02-056 Nov. 3.3 02:20:00.03 -04:44:20.2 24.3 0.5" SE
    >
    > Mamoru Doi
    > Institute of Astronomy
    > School of Science
    > University of Tokyo
    > voice +81-422-34-5084
    > fax. +81-422-34-5041
    > doi@ioa.s.u-tokyo.ac.jp

    -- 
    Tony Spadafora                                ALSpadafora@lbl.gov 
    Physics Division                              Tel: (510) 495-2316 
    Lawrence Berkeley National Lab                FAX: (510) 486-6738 
    1 Cyclotron Road BLDG 50R5032
    Berkeley, CA 94720-8160
    


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