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- Date: Fri, 27 Feb 2009 10:59:56 -0500
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This message was created automatically by mail delivery software (Exim). See http://uit.tufts.edu/?pid=548 for more information. A message that you sent could not be delivered to all of its recipients. The following address(es) failed: depatment cosmos phy tufts edu SMTP error from remote mail server after RCPT TO:<depatment cosmos phy tufts edu>: host cosmos.phy.tufts.edu [130.64.83.16]: 550 unknown user ------ This is a copy of the message, including all the headers. ------ Return-path: <gayle grant tufts edu> Received: from webmail02.usg.tufts.edu ([130.64.1.34]:41510 helo=localhost) by beech.usg.tufts.edu with esmtp (Exim 4.60) (envelope-from <gayle grant tufts edu>) id 1Ld57u-00071t-dr for depatment cosmos phy tufts edu; Fri, 27 Feb 2009 10:59:50 -0500 Received: from host-130-64-83-119.medford.tufts.edu (host-130-64-83-119.medford.tufts.edu [130.64.83.119]) by webmail.tufts.edu (Horde MIME library) with HTTP; Fri, 27 Feb 2009 10:59:50 -0500 Message-ID: <20090227105950 32pnecg6eos4kwoo webmail tufts edu> Date: Fri, 27 Feb 2009 10:59:50 -0500 From: Gayle Grant <gayle grant tufts edu> To: depatment cosmos phy tufts edu Subject: Events for today Friday 2/27/09 MIME-Version: 1.0 Content-Type: text/plain; charset=ISO-8859-1; format="flowed" Content-Disposition: inline Content-Transfer-Encoding: quoted-printable User-Agent: Internet Messaging Program (IMP) H3 (4.0.5) X-Remote-Browser: Mozilla/4.0 (compatible; MSIE 6.0; Windows NT 5.1; AskBar 3.00; SV1; GTB5; .NET CLR 1.1.4322; InfoPath.1) X-Originating-IP: 130.64.83.119 Good morning: Events for today, February 27, 2009 Robinson 251 Noon Informal lunch with Dr. Danilo Marchesini. All students are encouraged to attend. Pizza and soda will be available. Friday February 27, 2009 3:00 pm Nelson Auditorium, Anderson 112 Please note refreshments will be served in Robinson 251(Knipp Library)at 2:= 30. TUFTS UNIVERSITY Special Physics and Astronomy Colloquium =93The Universe at z=3D2-4: New Insights into Galaxy Formation and Evolutio= n=94 Danilo Marchesini Yale University In the past five years, our understanding of the galaxy population at redshift z=3D2-4 has improved significantly. As the redshift range z=3D2-4 represents a key epoch in the buildup and evolution of galaxies, studies of the properties of galaxies at these redshifts provide important clues on the physical processes at work during galaxy formation and evolution. I will summarize our current knowledge of the galaxy population at z=3D2-4, as well as discuss these results in the context of the latest generations of galaxy formation models. I will conclude by presenting the most relevant open issues and how these will be addressed by ongoing projects and future facilities. **Please note room change Refreshments served in Knipp Library, Robinson 251, at 2:30 pm
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