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Date: Thu, 13 May 93 16:32:27 +0900
From: nomoto@apsun1.astron.s.u-tokyo.ac.jp
>From srk@astro.isas.ac.jp Thu May 13 08:43:50 1993
From: Shri KULKARNI <srk@astro.isas.ac.jp>
Subject: 1993j
Dear Ken: Thanks very much for your preprint.
The high frequency data is somewhat confusing. The IRAM folks claim
results different from ours. I know which one to believe!
Here is a summary of our measurements (todate)
---------------------------------------------------------
Message 1/62 From Tony Phillips
May 12 '93 at 4:39 pm pdt
Return-Path: <jap@astro.caltech.edu>
Date: Wed, 12 May 93 16:39:23 PDT
To: srk@surya.caltech.edu
Subject: 1993j
Hi Shri,
Here are the latest flux measurements. As you can see, it not fading
yet.
--Tony
Date f(GHz) S(mJy) Beam(") Posn
---- ------ -------- -------- -----------------------
11/4/93 99.4 18 +/- 2 5.5 X 4.0 09:51:18.9 69:15:27
14/4/93 99.4 17 +/- 2 5.6 X 4.0 09:51:19.0 69:15:27
21/4/93 99.4 20 +/- 3 6.0 X 4.0 09:51:18.9 69:15:28
30/4/93 99.4 17 +/- 2 4.5 X 4.3 09:51:19.0 69:15:27
10/5/93 99.4 23 +/- 3 3.0 X 2.8 09:51:19.0 69:15:27
Date f(GHz) 1993j 3c273 0954+658 3c345
---- ------ -------- ------- -------- -------
11/4/93 99.4 18 mJy 22.1 Jy 1.9 Jy -
14/4/93 99.4 17 25.4 1.9 5.1 Jy
21/4/93 99.4 20 27.3 2.2 5.9
30/4/93 99.4 17 25.1 2.2 4.6
10/5/93 99.4 23 30.6 2.4 6.1
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