Richard Mathar
Oct27-04, 09:15 AM
<jabberwocky><div class="vbmenu_control"><a href="jabberwocky:;" onClick="newWindow=window.open('','usenetCode','toolbar=no, location=no,scrollbars=yes,resizable=yes,status=no ,width=650,height=400'); newWindow.document.write('<HTML><HEAD><TITLE>Usenet ASCII</TITLE></HEAD><BODY topmargin=0 leftmargin=0 BGCOLOR=#F1F1F1><table border=0 width=625><td bgcolor=midnightblue><font color=#F1F1F1>This Usenet message\'s original ASCII form: </font></td></tr><tr><td width=449><br><br><font face=courier><UL><PRE>hb> Date: Thu, 14 Oct 2004 13:56:59 +0200\nhb> From: Hans Boehringer <hxb@mpe.mpg.de>\nhb> To: sdss-general@astro.princeton.edu\nhb> Subject: Postdoctoral/graduate student position available\n\nPostdoctoral/graduate student position available\n-----------------------------------------------------------------\n\nThe MPE research group for galaxy clusters and cosmology in the theory\ndepartment of the Max-Planck-Institut for extraterrestrial physics is\ncarrying out observational and theoretical research on the\nastrophysics of galaxy clusters and the large-scale structure of the\nUniverse. Within\n\nthis program we are inviting applications for a three year graduate\nstudent or two year postdoc position for the topic:\n\nObservational study of the galaxy population and galaxy evolution in\ngalaxy clusters\n\nGalaxy clusters as the largest well defined building blocks of our\nUniverse are good laboratories to study galaxy evolution and ideal\ntracers of the large-scale structure of the Universe. To apply\nclusters for such studies we have to gain a precise understanding of\nthe galaxy cluster structure and the determination of cluster masses.\nFor this purpose we are leading a large international effort to\nimprove our characterization of galaxy clusters through the\ncombination of X-ray and optical observations. In addition we are\nusing X-ray surveys to construct representative, well characterized\nsamples of galaxy clusters for these studies.\n\nThe research planed for the advertised position will focus on the\noptical characterization of galaxy clusters and their galaxy\npopulation. The prime source of information is the Sloan Digital Sky\nSurvey (with privileged data access in the case of a graduate\nstudent), a large number of ESO Wide Field Imaging observations\nconducted by us, as well as future observations with the new ESO wide\nfield telescope VST. The data will partly also be combined with\ndetailed follow-up spectroscopy. At the core of the projects is an XMM\nLarge Programme combined with optical studies which will provide\nunprecedentedly precise information on the structure of a\nrepresentative sample of galaxy clusters. The main research goals are\nthe study of the variation of the galaxy population with the cluster\nmass, type, and environment, the variation of the mass-to-light ratio,\nthe characterization of the cluster structure and of cluster mergers,\nand the study of the correspondence of the X-ray and optical\nappearance of galaxy clusters. Such a survey also has a large\ndiscovery potential.\n\nThe graduate student position will be associated to the International\nMax-Planck Research School (http://www.imprs-astro.mpg.de/). The\npostdoc position is a two year fellowship position. The positions are\navailable now.\n\nFor more information and for applications contact:\n\nDr. Hans Boehringer\nMax-Planck-Institut fuer extraterrestrische Physik\nPostfach 1612\nD-85741 Garching\n\nE-mail: hxb@mpe.mpg.de\nTel.: +49 89 30000 3347\n\n[s.a.r. mod. note: reformatted to <80 characters per line. -- mjh]\n</UL></PRE></font></td></tr></table></BODY><HTML>');"> <IMG SRC=/images/buttons/ip.gif BORDER=0 ALIGN=CENTER ALT="View this Usenet post in original ASCII form"> View this Usenet post in original ASCII form </a></div><P></jabberwocky>hb> Date: Thu, 14 Oct 2004 13:56:59 +0200
hb> From: Hans Boehringer <hxb@mpe.mpg.de>
hb> To: sdss-general@astro.princeton.edu
hb> Subject: Postdoctoral/graduate student position available
Postdoctoral/graduate student position available
-----------------------------------------------------------------
The MPE research group for galaxy clusters and cosmology in the theory
department of the Max-Planck-Institut for extraterrestrial physics is
carrying out observational and theoretical research on the
astrophysics of galaxy clusters and the large-scale structure of the
Universe. Within
this program we are inviting applications for a three year graduate
student or two year postdoc position for the topic:
Observational study of the galaxy population and galaxy evolution in
galaxy clusters
Galaxy clusters as the largest well defined building blocks of our
Universe are good laboratories to study galaxy evolution and ideal
tracers of the large-scale structure of the Universe. To apply
clusters for such studies we have to gain a precise understanding of
the galaxy cluster structure and the determination of cluster masses.
For this purpose we are leading a large international effort to
improve our characterization of galaxy clusters through the
combination of X-ray and optical observations. In addition we are
using X-ray surveys to construct representative, well characterized
samples of galaxy clusters for these studies.
The research planed for the advertised position will focus on the
optical characterization of galaxy clusters and their galaxy
population. The prime source of information is the Sloan Digital Sky
Survey (with privileged data access in the case of a graduate
student), a large number of ESO Wide Field Imaging observations
conducted by us, as well as future observations with the new ESO wide
field telescope VST. The data will partly also be combined with
detailed follow-up spectroscopy. At the core of the projects is an XMM
Large Programme combined with optical studies which will provide
unprecedentedly precise information on the structure of a
representative sample of galaxy clusters. The main research goals are
the study of the variation of the galaxy population with the cluster
mass, type, and environment, the variation of the mass-to-light ratio,
the characterization of the cluster structure and of cluster mergers,
and the study of the correspondence of the X-ray and optical
appearance of galaxy clusters. Such a survey also has a large
discovery potential.
The graduate student position will be associated to the International
Max-Planck Research School (http://www.imprs-astro.mpg.de/). The
postdoc position is a two year fellowship position. The positions are
available now.
For more information and for applications contact:
Dr. Hans Boehringer
Max-Planck-Institut fuer extraterrestrische Physik
Postfach 1612
D-85741 Garching
E-mail: hxb@mpe.mpg.de
Tel.: +49 89 30000 3347
[s.a.r. mod. note: reformatted to <80 characters per line. -- mjh]
hb> From: Hans Boehringer <hxb@mpe.mpg.de>
hb> To: sdss-general@astro.princeton.edu
hb> Subject: Postdoctoral/graduate student position available
Postdoctoral/graduate student position available
-----------------------------------------------------------------
The MPE research group for galaxy clusters and cosmology in the theory
department of the Max-Planck-Institut for extraterrestrial physics is
carrying out observational and theoretical research on the
astrophysics of galaxy clusters and the large-scale structure of the
Universe. Within
this program we are inviting applications for a three year graduate
student or two year postdoc position for the topic:
Observational study of the galaxy population and galaxy evolution in
galaxy clusters
Galaxy clusters as the largest well defined building blocks of our
Universe are good laboratories to study galaxy evolution and ideal
tracers of the large-scale structure of the Universe. To apply
clusters for such studies we have to gain a precise understanding of
the galaxy cluster structure and the determination of cluster masses.
For this purpose we are leading a large international effort to
improve our characterization of galaxy clusters through the
combination of X-ray and optical observations. In addition we are
using X-ray surveys to construct representative, well characterized
samples of galaxy clusters for these studies.
The research planed for the advertised position will focus on the
optical characterization of galaxy clusters and their galaxy
population. The prime source of information is the Sloan Digital Sky
Survey (with privileged data access in the case of a graduate
student), a large number of ESO Wide Field Imaging observations
conducted by us, as well as future observations with the new ESO wide
field telescope VST. The data will partly also be combined with
detailed follow-up spectroscopy. At the core of the projects is an XMM
Large Programme combined with optical studies which will provide
unprecedentedly precise information on the structure of a
representative sample of galaxy clusters. The main research goals are
the study of the variation of the galaxy population with the cluster
mass, type, and environment, the variation of the mass-to-light ratio,
the characterization of the cluster structure and of cluster mergers,
and the study of the correspondence of the X-ray and optical
appearance of galaxy clusters. Such a survey also has a large
discovery potential.
The graduate student position will be associated to the International
Max-Planck Research School (http://www.imprs-astro.mpg.de/). The
postdoc position is a two year fellowship position. The positions are
available now.
For more information and for applications contact:
Dr. Hans Boehringer
Max-Planck-Institut fuer extraterrestrische Physik
Postfach 1612
D-85741 Garching
E-mail: hxb@mpe.mpg.de
Tel.: +49 89 30000 3347
[s.a.r. mod. note: reformatted to <80 characters per line. -- mjh]