Return-Path: Received: from carignan.iap.fr ([unix socket]) by carignan (Cyrus v2.1.18-IPv6-Debian-2.1.18-1) with LMTP; Sun, 27 Apr 2008 23:45:20 +0200 X-Sieve: CMU Sieve 2.2 Return-path: Received: from mix.iap.fr ([194.57.221.39] helo=terapix.iap.fr) by carignan.iap.fr with esmtp (Exim 4.50) id 1JqEgL-0002MX-9E; Sun, 27 Apr 2008 23:45:13 +0200 Received: from petidomo by terapix.iap.fr with local (Exim 3.36 #1 (Debian)) id 1JqEh8-0005Ly-00; Sun, 27 Apr 2008 23:46:02 +0200 Received: from carignan.iap.fr ([194.167.0.147]) by terapix.iap.fr with esmtp (Exim 3.36 #1 (Debian)) id 1JqEh7-0005Lk-00 for ; Sun, 27 Apr 2008 23:46:01 +0200 Received: from vieuxpapes.iap.fr ([194.57.221.61]) by carignan.iap.fr with esmtp (Exim 4.50) id 1JqEgK-0002MS-Rn for teralist@iap.fr; Sun, 27 Apr 2008 23:45:12 +0200 Received: from ras75-2-82-224-50-75.fbx.proxad.net (ras75-2-82-224-50-75.fbx.proxad.net [82.224.50.75]) (using TLSv1 with cipher AES128-SHA (128/128 bits)) (No client certificate requested) by vieuxpapes.iap.fr (Postfix) with ESMTP id 98CE2A63 for ; Sun, 27 Apr 2008 23:45:12 +0200 (CEST) Message-Id: From: Henry Joy McCracken To: teralist@iap.fr Content-Type: text/plain; charset=US-ASCII; format=flowed; delsp=yes Content-Transfer-Encoding: 7bit Mime-Version: 1.0 (Apple Message framework v919.2) Subject: [teralist] bilan tardif hjmcc Date: Sun, 27 Apr 2008 23:45:09 +0200 Reply-To: teralist@iap.fr Precedence: list Sender: petidomo GRAND POSTIER X-Spam-Checker-Version: SpamAssassin 3.0.3 (2005-04-27) on cairanne.iap.fr X-Spam-Level: X-Spam-Status: No, score=-2.6 required=5.0 tests=AWL,BAYES_00 autolearn=ham version=3.0.3 bonsoir emmanuel, mea culpa et desole pour le retard-- un sortir imprevu au resto... - This week I was working on the astrometric and photometric solution of the WIRCAM d3-data and also trying to resolve problems related to cross talk. - Many mails were exchanged between loic, chris willot and myself over the origin of the black marks on the final d3 stacks. Loic thinks that the black marks come from incorrect crosstalk removal. He will supply to us images which have not been crosstalk corrected and then the stacks will be redone. - If the black marks are due to to persistence effects, then they should be less important with a larger number of images in the sky background stack. What are the optimal numbers of images to include in the sky background? To answer this question, QF has been run on 2000 Ks images BEFORE PROCESSING; the plots have yet to be made showing the background variation as a function of time. This should help us to quantify how rapidly the sky varies during each night. Then, potentially, we will re-do the sky subtraction with a larger number of sky frames. - With patrick, tests were made with the new script which computes the zero-points chip-by-chip. There are some important differences between the two scripts; it turns out that Herve's script uses a very small matching radius and consequently finds many smaller numbers of objects wrt to patrick's. Another question which is not yet resolved is what to do for the cases where there are very small numbers of stars in each detector. It seems the reason the solution is unstable for the d3- images is precisely because of the small numbers of matching stars in some D3 frames - PI data: Data from Mr. Hutchings should have been processed at the end of September (when the request was lodged: unfortunately this slipped under the carpet and was not processed; the pre-processed data has also been removed from CFHT, so loic will have to re-do this part of the processing. I think we have to be careful how the processing priorities are set.