From: Tony Spadafora (ALSpadafora@lbl.gov)
Date: Fri Jun 07 2002 - 18:43:56 PDT
SCP colleagues:
The SCP executive committee proposed we prepare three separate IAU
circulars for SNe discovered at Subaru, at CTIO, and at CFHT. We will
try to submit them together and with a uniform style so that it will be
clear that they are part of common SCP campaign.
Naoki has (already!) prepared the data for the Subaru candidates - see
below. Rob will prepare the CTIO candidates and Reynald is asking Julien
to prepare the CFHT ones.
For questions arising from the analyis of spectrum (confidence in ID, z,
etc.) we've asked Andy Howell, who has been tracking this on the spectra
web page, to coordinate all the comments from the spectroscopy analysis
folks (there will be lots, no doubt.)
I will try to coordinate common information and format for all three.
I've set up a page:
http://panisse.lbl.gov/collab/papers/IAUC_2002A/
to keep current drafts and any relevant information (e.g. last years circulars.)
Last year, Dan Green allowed us to list the full author list. This time,
we would refer to last year's and list only new people. It should go
much quicker this time.
-Tony
-------- Original Message --------
Subject: Re: preparing IAU ciruclars for current SCP run
Date: Fri, 07 Jun 2002 17:26:41 +0900
From: Naoki Yasuda <naoki.yasuda@nao.ac.jp>
...
The following is the quick list of spectroscopically confirmed SNe found
by Subaru.
Please let me know missing information to be included in IAUC.
SNe found by Suprime-Cam/Subaru
SCPname Date Time (UT) Exp(sec) R.A. (J2000) Decl. mag SN
type Observation
----------------------------------------------------------------------------------------------------------
S02-000 2002-04-09 11:11-12:12 2880 14:03:54.08 +04:59:49.0 i'=23.36 Ia
at z=0.278 FORS2
S02-001 2002-04-09 11:11-12:12 2880 14:03:56.42 +05:23:16.5 Ic=24.57 ??
at z=1.42 FORS2
S02-002 2002-04-09 11:11-12:12 2880 14:04:18.16 +05:19:25.6 i'=24.72 Ia
at z=1.086 FORS2 ISSAC HST(HIZN1)
S02-016 2002-04-09 11:11-12:12 2880 14:04:00.13 +04:59:50.6 i'=24.83 Ia
at z=0.561 Keck
S02-027 2002-04-09 12:16-13:19 2880 13:58:31.78 +05:27:08.3 i'=24.13 ??
at z=0.9 GMOS ISSAC
S02-032 2002-04-09 13:21-14:23 2880 14:03:39.82 +05:46:50.6 i'=23.99 Ia
at z=1.08 FOCAS HST(LOZN2)
S02-035 2002-04-09 11:11-12:12 2880 14:02:41.15 +05:19:27.4 i'=25.50 ??
at z=1.37 Keck
S02-049 2002-04-09 10:05-11:08 2880 14:00:23.29 +05:45:41.9 i'=24.19 Ia
at z=0.88 GMOS HST(LOZN1)
S02-064 2002-05-09 05:56-07:09 2640 13:25:46.62 +27:34:21.1 i'=22.44 Ia
at z=0.56 / GMOS
Ic
at z=0.33
S02-075 2002-05-07 10:41-14:00 6960 13:24:25.92 +27:44:33.9 i'=23.74 Ia
at z=0.79 FORS2 GMOS HST(LOZN3)
S02-064's reference is taken on 2002-04-09.
S02-075's reference is taken on 2002-04-12.
Others' references are taken on 2002-03-19.
--- Naoki Yasuda @ National Astronomical Observatory of Japan e-mail: naoki.yasuda@nao.ac.jp -- Tony Spadafora ALSpadafora@lbl.gov Physics Division Tel: (510) 495-2316 Lawrence Berkeley National Lab FAX: (510) 486-6738 1 Cyclotron Rd., MS 50-232 Berkeley, CA 94720, USA
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