From: Ariel Goobar (ariel@physto.se)
Date: Wed Mar 19 2003 - 02:44:26 PST
Please add also the name of our new postdoc, Vallery Stanishev
among the new names. He worked with Gaston on the VLT spectral
reductions for the last run.
Ariel
On Tue, 18 Mar 2003, Tony Spadafora wrote:
> 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
>
>
-- ___________________________________________________________________ Ariel Goobar (www.physto.se/~ariel) Department of Physics, Stockholm University AlbaNova University Center, SE-106 91 Stockholm, SWEDEN tel: +46 8 55378659 fax: +46 8 55378601
This archive was generated by hypermail 2.1.4 : Wed Mar 19 2003 - 02:44:53 PST