From: Mamoru Doi (doi@ioa.s.u-tokyo.ac.jp)
Date: Tue Mar 18 2003 - 07:08:58 PST
Dear Chris,
Thank you very much for your quick suggestions.
>- VLT observations occurred on Nov. 7-11
>
>- If you wish to give more details, the VLT observations were done
>with FORS2 on Yepun (VLT-UT4)
>
>- The redshift of SuF02-065 is z=1.181 from the [OII] line.
>
>- The redshift of SuF02-017 from the VLT spectrum is probably z=1.03.
>Andy may want to confirm this.
I update the draft.
>- There appears to be some strange characters associated with the listing
>for SuF02-005
I hope I fixed this correctly. The characters must be blank in Japanese
fonts, and it is hard for me to see those characters with my PC.
Best regards,
-Mamoru
Ver.3
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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 with GMOS on Gemini-N on
Nov. 6, 8, and 9; with ESI on KeckII on Nov. 6, 7, 9,
and 10; with FORS2 on Yepun (VLT-UT4) on Nov. 7 - 11; and
with FOCAS on Subaru 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 1.181 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 1.03 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 02:18:35.70 -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
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